CHAPTER XI.

OUT OF OFFICE (1842-3).

All being thus decided, and my last duty performed, I saw no reason to

delay any longer that relaxation of which I now stood much in need, and

during the next month the entries in my Journal are comparatively few.

While I was resting my friends were at work:—

“_November 9th, 1842._—Matthew informs me that Lord Brougham

had a long conversation with Sir James Graham, on the 7th

instant, on the subject of my treatment, in the course of

which he (Lord B.) told Sir James Graham that in his opinion

the Government was making a great practical mistake, and

intimated that I must of course defend myself, and that he,

from his long acquaintance with myself and opinion of the plan,

should feel bound to take up the cudgels on my behalf in the

House of Lords. That Sir James Graham appeared also to think

that a mistake had been made, and promised to speak to some

other members of the Cabinet on the subject. Lord Brougham

subsequently wrote to Sir James Graham a letter to be laid

before Peel.”

To give to the public such a knowledge of facts as would enable it to

do justice either to my plan or myself, it was obviously important to

publish that correspondence with the Treasury in which I had again and

again urged improvement, and in which my application had been as often

either neglected or evaded; in which, also, I had received notice of my

dismissal, had deprecated this step, and had been informed of persistence

in the intention, with such show of reason as had been vouchsafed me.

Being aware, however, that such publication was likely to be the subject

of attack, I was careful, before venturing on it, to ascertain my right

to make it; and this I knew must depend upon precedent and require

reference to authority:—

“_November 26th._—Matthew applied to Earl Spencer[335] for his

opinion.”

The following is his lordship’s letter:—

“Longford, November 25th, 1842.

“MY DEAR SIR,—As the correspondence you sent me looked rather

alarming as to bulk, I delayed reading it till I had the

opportunity of a journey. I took this opportunity yesterday.

“I can see no public grounds why your brother should not

publish it if he thinks fit. As a question of personal prudence

I think the thing more doubtful, but I think your letter

only goes to his _right_ to publish it. I have no business,

therefore, to say anything more than that I think he has a

right to publish it.

“You know, however, that I sometimes have done more than answer

a question put to me simply, and I will do so now by adding to

my answer that if I was in his place I would not publish it....

“Yours most truly,

“SPENCER.

“M. D. HILL, Esq.”

“_November 29th._—To-day the Merchants’ Committee [which had

applied for an interview early in August] has seen Sir Robert

Peel. They strongly urged the necessity for completing the

measure—their want of confidence in the Post Office—their

confidence in me, and the great satisfaction it would be to

the public to see me restored to office. Peel satisfied the

deputation that he was sincerely desirous of carrying out the

measure, and Goulburn, who was present, assured them that,

whatever might have been the feeling originally entertained

by the Post Office, all there were now earnest friends of

the measure! (It did not occur to the Committee to inquire

where, then, lay the danger of ‘collision.’) Peel invited the

Committee to send in a statement of those parts of the plan

which they still wished to see carried into effect; but he

stated that a return from the Post Office showed that, _with

the exception of about £100,000 per annum, the net revenue

was obtained from foreign and colonial letters_.[336] This

statement, which he made in an early stage of the conversation,

threw the Committee quite aback; for though I had prepared

them, as I thought, to distrust all information derived from

the Post Office, their want of familiarity with the subject,

and the confident manner with which the statement was made,

caused them to believe it.”

The Committee at my suggestion subsequently applied for a copy of this

return, but it was prudently withheld; and, with equal prudence, no

reason was assigned for the refusal. Of this return, however, more will

appear by-and-by. Meantime, the question of publishing the correspondence

remaining still undecided, I sought further advice. On December 4th I

received the following letter from Mr. Baring:—

“Brighton, Dec. 3rd, 1842.

“DEAR SIR,—I hope to be at Lee on Tuesday, and shall be at your

service on Wednesday morning. But if you are not afraid of a

bad dinner, which you probably will get the first day of our

return, you had better come down on Tuesday, dine and sleep at

Lee, and we will talk over the matter on Wednesday.

“Yours very truly,

“F. T. BARING.”

After careful perusal and reperusal of the correspondence, Mr. Baring,

in the course of several conversations, pronounced my line of conduct

very judicious, and the conduct of Government very shabby. He said it

was absurd to expect that the Post Office would satisfactorily carry

into effect the remaining parts of my plan, and that consequently my

dismissal was most unfair towards the measure. He added that, even

without reference to my plan, my retention as a permanent officer would

be useful as a check upon the proceedings of the Post Office; and that

such retention would be in conformity with the system of Treasury

management, which consists in having an officer to check each subordinate

department. He assured me that it was never his intention that my

services should cease as a matter of course at the expiration of the

year mentioned in his last letter, the fair interpretation of which was

that he considered it advantageous to continue my services indefinitely,

but that as he was then leaving office, and as there were rumours of

an intention on the part of the next Government to abandon my plan, he

did not feel justified in giving me a claim for more than one year’s

salary. These opinions he would be prepared to state in Parliament. He

thought it probable that Lord Lowther’s jealousy was the cause of the

mischief, and that that jealousy was excited by my opposition to his

plan of registration, which, he remarked, if carried into effect would

have created an uproar throughout the country. He was of opinion that I

had a right to publish the correspondence, but feared that by so doing

I should bar the door against other employment, to which he regarded me

as having a claim, that otherwise would probably be recognised even by

the Government then in power; so that he was rather averse to my taking

any step before the meeting of Parliament. I replied that, although I,

of course, should be glad to obtain other employment under Government,

my chief anxiety was to satisfy the public that I had not misled them by

holding out expectations which could not be realized, and that, although

I would carefully consider his kind advice, my present inclination was to

sacrifice all other considerations to the accomplishment of this object;

on which he remarked that, if I were not satisfied with the discussion

in Parliament, I could still publish the correspondence. He expressed

an opinion that it would not be practicable to bring before Parliament

copies of my Reports, or those of the Post Office, to the Treasury,

inasmuch as such Reports being considered confidential, the rule is to

refuse their production. This was a serious disappointment, as I had

depended mainly on the publication of these Reports as a means of showing

the manner in which my duties had been discharged, and the nature of the

opposition of the Post Office.

“_Same day._—Matthew has seen Lord Spencer. His view coincides

almost exactly with Mr. Baring’s, differing only (if I have

understood Mr. B. rightly) in thinking that the late, as well

as the present, Government would disapprove of any appeal to

the public, except through Parliament.”

As Mr. Warburton concurred in disapproving immediate publication, I

yielded to the advice of so many influential friends, though my own

opinion was still strongly in favour of the prompter course. Meanwhile

there came in from various members of Parliament and many other friends

letters of sympathy and support; among others, the following kind and

characteristic one from Mr. Cobden:—

“Newcastle-on-Tyne, 20th January, 1843.

“MY DEAR SIR,—The men of the League are your devoted servants

in every way that can be useful to you. Colonel Thompson,

Bright, and I, have _blessed you_ not a few times in the course

of our agitating tour.... I go back to Manchester to-morrow,

after a very gratifying tour in Scotland. ‘The heather’s on

fire.’

“Believe me,

“Yours very truly,

“R. COBDEN.

“R. HILL, Esq.”

This was followed, within a week, by a second letter, in which it

will be seen that the warmth of his feelings led him into very strong

expressions. These I do not suppress, as every one can make for them the

allowance due to time, circumstance, and a generous nature:—

“Manchester, 26th January, 1843.

“MY DEAR SIR,—I have read over the correspondence, and, so

far as success in placing the Government in the wrong goes,

you will be pronounced triumphant by all who will read it.

But nothing is more true than the remark in your brother’s

excellent letter, that the force of public opinion cannot

be brought to bear upon the authorities to compel them to

work out details. So far as your object in that direction is

concerned, your correspondence will, I suspect, be nugatory. If

your object be to justify yourself in the eyes of the public,

_that_, I submit, is supererogatory. You cannot stand better

than you do with the impartial British public. You will get no

further facilities from Tory functionaries. They hate the whole

thing _with a diabolical hatred_. And well they may. It is a

terrible engine for upsetting monopoly and corruption: witness

our League operations, the _spawn of your penny postage_! Now,

let me deal frankly and concisely with you. I want to see

you remunerated for the work you have done. The labourer is

worthy of his hire. The country is in your debt. An organized

plan is alone necessary to insure you a national subscription

of a sum of money sufficient to reimburse you for time,

trouble, and annoyance incurred and expended in your great

social revolution.... A public subscription—a really national

one—would give you power and independence, and when the next

change of Government takes place you would be in the ascendant.

Until then I expect no hearty co-operation in carrying out

your details. We must be content, in the meantime, to prevent

the Tories from robbing us of any substantial part of the

principle, and I think we have bulldogs enough in the House

now to prevent that. I should like to have some talk with you

about this matter. Meantime, excuse my plainness, and don’t

suspect me of wishing to make you a _sordid_ patriot. You see

what an effect the £50,000 League Fund is producing: a similar

demonstration in favour of the author of Postage Reform, and

a seat in Parliament in prospective, would have a like effect

upon the enemy.

“Believe me,

“Yours truly,

“R. COBDEN.

“ROWLAND HILL, Esq.”

Very different, but no less characteristic of the writer, is the

following letter, received some months later, from Thomas Hood:—

“17, Elm Tree Road, St. John’s Wood,

1st May.

“MY DEAR SIR,

* * * * *

“I have seen so many instances of folly and ingratitude similar

to those you have met with, that it would never surprise me

to hear of the railway people some day, finding their trains

running on so well, proposing to discharge the engines.

* * * * *

“I am, my dear Sir,

“Yours very truly,

“THOMAS HOOD.

“R. HILL, Esq.”

Meanwhile, I felt nowise daunted by late events, but rather filled with

fresh zeal; for although I never willingly entered into a conflict, yet

when one was forced upon me, or stood between me and what I deemed right,

I was by no means backward at the work.

One of my earliest moves after leaving office was towards personal and

domestic economy. While I was in receipt of a large salary, and had my

attention fully occupied, and indeed my powers heavily taxed, I had

allowed my expenditure to obtain dimensions unsuitable to my present

condition. Of course I intended to seek new occupation, but this would

require time; and, meanwhile, I felt that if I would act independently

I must make myself independent of circumstances. I therefore entered at

once upon a course of vigorous retrenchment, and partly by my efforts,

but much more by the zealous and most efficient co-operation of my

dear wife, our expenditure was soon brought within very narrow limits.

Without any change of house or diminution in number of servants, our

disbursements were soon reduced by one-half, and it was only in the first

year after the change that my expenditure exceeded my income. I may add

that it never had exceeded it before, and that it never exceeded it again.

As the parliamentary session approached, however, I had to turn my

attention more and more to the work of preparation for the duty which

I expected it to bring. I therefore put my papers in the most perfect

order—a proceeding which has greatly facilitated the writing of this part

of my narrative.

Sir Thomas Wilde having very kindly undertaken to lay my case before

Parliament, I could not but feel some anxiety as to the view that might

be taken of this course by Mr. Wallace, who had himself acted as leader

in earlier days. I therefore wrote to him on the subject as delicately

as I could, and a fortnight afterwards, when he came to town for the

parliamentary session, I called upon him with some feeling of anxiety. I

quote from my Journal:—

“He behaves nobly, as he always has done, fully acquiescing in

the arrangement with regard to Sir Thomas Wilde, and expressing

his own readiness to follow Sir Thomas’s lead.”

Meanwhile, however, my attention was called to considerations of a

somewhat different character:—

“_February 8th._—Met Mr. Stephen, of the Colonial Office, in

Piccadilly, and at his request walked with him to the Colonial

Office. On the way he urged me to apply to the Government

for employment, saying that he felt sure my claim would be

acknowledged—intimating that I might expect such an appointment

as a Commissionership of Customs. I replied, that such a step

would be considered as a tacit engagement on my part not

to bring my case before the public; that other friends had

recommended a similar course, under the impression that the

complimentary expressions in the letters from the Treasury

were intended by Government to suggest it, but that, after

mature deliberation, I had decided not to do anything which

should prevent my making known to the public the true causes

of the small amount of revenue actually obtained, as compared

with my anticipations, and justifying my conduct throughout.

Mr. Stephen rejoined that he did not doubt I might stipulate

to do all this, providing that I refrained from attacking the

Government, and yet obtain lucrative and honourable employment.

To this I said I of course could not object, and he recommended

that two of the leading merchants or bankers in the city, of

opposite politics, should make the application on my behalf.

I promised to consider the suggestion, but requested that he

would, in the meantime, read the correspondence, a copy of

which I sent him the same afternoon.

“_February 11th._—Prepared a memorandum ... called on Mr.

Stephen, read it to him, and left it with him; he expressing

a desire to reconsider the matter, with a view, perhaps, of

making such inquiries of Goulburn, with whom he is intimate,

as would enable him to judge of the probable success of such

an application as he had suggested. I desired that he would do

whatever he thought best, clearly understanding, however, that

I was no party to anything of the kind.

“_February 15th._—Mr. Stephen writes that he has ascertained

that nothing can be done unless I submit to be gagged, and not

very much even then; so the whole ends in smoke.

“_Same day._—Wrote to Mr. Stephen thanking him for his

kindness, which, from the very unreserved manner in which he

spoke of the Government, I feel very strongly; but of course

declining to apply to Government.”[337]

About three weeks later, Mr. Goulburn, in reply to an application made

by Mr. Hutt, on behalf of Sir Thomas Wilde, for the production of my

correspondence with the Treasury, refused to give more than a few

letters, withholding those of chief importance;[338] and though, on

being pressed, he somewhat enlarged the grant, it still remained very

imperfect. Unsatisfactory, however, as was this concession, motion was

made accordingly:—

“_March 29th._—My correspondence with the Treasury. The

printed copies were delivered this morning. By the omission

of all the letters urging progress in the plan, Goulburn’s

notice of dismissal is brought into juxtaposition with a

minute of December 24th, 1841 (of which I never heard till

now), confirming the extension of my engagement for one year

from September 14th, 1841, and made to appear as the natural

sequence of such minute, instead of being, as it was in fact,

the answer to my complaints of no progress, and of Post Office

interference to prevent my journey to Newcastle. The whole

thing is cunningly done, and it shows that the five weeks taken

to prepare the correspondence have not been lost. The case is

so much damaged, however, that I have determined to give the

papers a very limited circulation, and to press on Wilde to

consent to the publication of the whole. Sir Robert Peel, in

his letter[339] to me, admits that ‘important improvements’

still remain to be effected; but in the printed copy the word

‘important’ is dropped.”[340]

To my surprise, the strength of my case, grievously impaired as it was by

this maiming of the correspondence, was nevertheless recognised in one of

the journals regularly supporting the Government:—

“_March 30th._—The _Morning Herald_ gives the correspondence

with Sir Robert Peel, and has a leader, sneering, of course,

at penny postage, but expressing an opinion that I have been

unjustly treated, and ought to have a place or a pension.”

This is the last entry in my Journal for the present. On the one hand,

I became so engrossed in preparation for the coming conflict—a conflict

which seemed to me as one almost of life and death—that I had no time to

spare save for pressing demands; while, on the other hand, the motive to

record was greatly weakened since my exclusion from the Treasury. For

the history of the following three years and a-half, my dependence is on

documents, parliamentary or otherwise, produced during the period (all

of which I have carefully preserved), and on such recollections as are

suggested by their perusal.

On April 10th a petition for inquiring into the state of the Post

Office, prepared by myself and in my own name, was presented to the

House of Commons by Mr. Baring; and on the following night Mr. Hawes

gave notice that Sir Thomas Wilde would call the attention of the House

to the same soon after the Easter holidays—a notice, however, which from

various causes had to be repeated several times before being acted

upon. Of this petition, which appears at length in the Report of the

Committee,[341] I will merely mention here that, after reference to my

appointment and subsequent dismissal, after statements as to the very

incomplete introduction of my plan, evidence as to the hopelessness of

its completion being effected by the Post Office, and representations as

to the vast interests at stake, I concluded by expressing my desire “to

submit the truth of the foregoing allegations to the severest scrutiny,”

and by petitioning for the necessary inquiry.

This petition was presently backed by another from eight members[342]

of the Mercantile Committee, so often mentioned before, in which, after

briefly adverting to the beneficial effect of the improvement already

made, the petitioners, expressing an earnest desire for the completion of

the plan, prayed for inquiry with a view to that end.

I now felt that the time was come when my friends should be put in full

possession of the facts of the case; and, consequently, having printed

all of the correspondence which had been applied for in Parliament,

that withheld as well as that granted, I sent copies, marked “strictly

confidential,” to the members of the Mercantile Committee, and some

others of my friends, prefacing it with an introduction, in which I

justified the proceeding—first, by the declaration of the Chancellor

of the Exchequer, that his denial was made on the ground that the part

which had been withheld was unnecessary, no allegation being made as

to inconvenience to the public service, and, secondly, by the high

authority which I had for saying that I had a right, looking to the

nature of the correspondence itself, to official usage, and all other

circumstances, to place the whole before the public. This step, taken

on April 13th, was on the 19th condemned in the House of Commons by

the Chancellor of the Exchequer, Mr. Goulburn, but defended by the

ex-Chancellor of the Exchequer, Mr. Baring.

It was not until May 1st that I obtained a copy of the return upon which

Sir Robert Peel, in the preceding November, based his injurious and

erroneous statement that the inland post yielded but £100,000 a-year to

the revenue. This return was now laid before Parliament on the motion

of Sir George Clerk. In consequence I addressed a letter to the daily

papers, in which I expressed myself as follows:—

“I have no hesitation in stating that the return, whether

considered in regard to its general results or to the division

of revenue under the two heads, is utterly fallacious.”

I concluded by promising to give in due time a full exposure of the

fallacy—a promise afterwards fulfilled.[343]

In the short period during which this return was under my consideration,

an incident occurred which must be mentioned, because, besides giving

additional evidence of Post Office incompetency, it excited some surprise

and not a little amusement. The Overland Route to India being now

established, a notice was issued by the Post Office, that persons wishing

to send letters by that route to Australia must address them to “an agent

in India,” who in turn must pay the postage onward, as otherwise the

letters would not be forwarded. To the unreasonableness of expecting

that every one writing by that route to Australia should have an agent

planted half-way, was added such vagueness of expression as would have

rendered the injunction very misleading; “India” being put for “Bombay,”

where alone, according to Post Office arrangement, the postage could be

paid. The absurdity of the proceeding was so manifest that within a week

from its appearance the notice was withdrawn.

In this short period, also, Mr. Ashurst, acting for the Mercantile

Committee, issued a circular to mayors of towns and other representative

persons, recommending that petitions should be sent up praying for the

complete execution of my plan; the recommendation being accompanied with

a statement showing, in the most pithy manner, the chief estimates as

to number of letters and average of postage under the old rates, made

severally by the Post Office authorities, the Parliamentary Committee,

and myself, previously to the adoption of the plan, and comparing them

with actual results.

About this time Mr. Baring had moved for a return, to show how far

the instructions, issued by the Treasury more than a year and a-half

ago,[344] for the extension of rural distribution, had been carried into

effect by the Post Office. Of course he had, ere this, learnt from me

that its operation had been suspended by the Treasury; but now, in the

return called for, this essential fact was suppressed, the whole answer

being as follows:—

“No definite arrangements have yet been made by the Post Office

in conformity with the Minutes of the Lords of the Treasury,

dated the 13th and 27th days of August, 1841, relating to the

Post Office distribution in the rural districts of the United

Kingdom.

“W. L. MABERLY.

“General Post Office, 8th April, 1843.”

The motion, so important to me, and, as I thought, and still think, to

the cause of postal reform, seemed in danger of lapsing to the end of

the session, not coming on until June 27th. The House was far from full,

but the number present was considerable. I obtained a seat for myself

and my brother Arthur under the gallery, sitting on the opposition side

of the House, that I might the more readily supply my friends with any

information that might be required during the progress of the debate.

Colonel Maberly, likewise under the gallery, was, I suppose for the

like reason, on the Government side of the House. The debate occupies

forty-seven pages in “Hansard;”[345] but keen as was the interest with

which my brother and I listened to every word, I shall not trouble the

reader of the present day with more than a brief abstract.

The motion of which Sir Thomas Wilde had given notice was for a Select

Committee, “To inquire into the progress which had been made in carrying

into effect the recommendations of Mr. Rowland Hill for Post Office

improvement; and whether the further carrying into effect of such

recommendations or any of them will be beneficial to the country.”[346]

Sir Thomas Wilde, after adverting to the deliberate adoption of my plan

by Parliament, and this in a time of commercial depression, with the

knowledge that its adoption was expected to produce a small permanent and

a large immediate reduction of revenue, pointed out that my plan had

been presented as a whole, no part being recommended unless accompanied

with the remainder. After referring to the authoritative condemnation

of the old system, to my appointment, to the acknowledged value of my

services, to the opposition of the Post Office, to the hopelessness

of expecting the completion of my plan from that department, or even

from the Treasury, unless aided by one able and ready to deal with the

fallacies with which resistance was defended; after having pointed out

the unfairness of the experiment on which my plan had been judged, and,

in fine, given a history of the progress (and non-progress) of postal

reform during the time I was at the Treasury, and of my dismissal

therefrom, he concluded by moving the resolution of which he had given

notice.[347]

The Chancellor of the Exchequer, while repeating some of the allegations

made in his letter to me, endeavoured to inculpate the late Government,

and to throw upon them the responsibility of my dismissal, condemned

my divulging the correspondence as a breach of confidence, greatly

overstated the power committed to me during his tenure of office, spoke

of much having been accomplished since I left the Treasury, enumerating

for this purpose some measures adopted on my recommendation while I was

still there, and others hastily resolved on since the presentation of my

petition, no one of which, however, was yet carried into execution.

He attempted to defend the opposition to the reduction of the

registration-fee by greatly overstating the amount of money-order

business, extolled Lord Lowther, absurdly attributing to him the

origination of penny postage,[348] though he had voted against it

in committee;[349] asserted that the Post Office did not pay its own

expenses;[350] but ended by saying that he had no objection to a limited

inquiry, and by proposing, as an amendment to Sir Thomas Wilde’s motion,

the following:—

“That a Select Committee be appointed to inquire into the

measures adopted for the general introduction of the system

of penny postage, and for the facilitating the conveyance of

letters throughout the country.”[351]

Mr. F. Baring (late Chancellor of the Exchequer) saw no objection to the

amendment, and hoped that Sir Thomas Wilde would allow it to be carried

in lieu of his own motion. He touched upon the unfair use made of the

term “penny postage,” a term by no means including the whole plan, for

the purpose of limiting my engagement; and remarked that in renewing

this engagement for one year he had not meant to restrict it to that

period, but had merely refrained from acting discourteously towards his

successor, while “all along of opinion that the services of Mr. Hill

at the Treasury would be required for a much longer period than one

year.”[352] He continued as follows (and I hope that I may be pardoned

for making the quotation):—

“He also thought it was only common justice to say that, at the

period when it was determined to carry out this plan, he had

not the slightest personal knowledge of Mr. Rowland Hill....

He had expected that a person who had been long engaged in

the preparation of an extensive system of this kind would

not carry out the change with that coolness and judgment that

was requisite; and he had expected that he should have great

difficulties to contend with in inducing Mr. Hill to adopt

any alteration in his plan that might appear requisite. He

found quite the contrary of this, and that Mr. Hill, with the

greatest readiness, adopted any suggestions that were made to

him; so that instead of difficulties, he found every facility

in carrying the plan into effect. True, Mr. Hill gave his

reasons for the opinion that he had adopted, or for the course

that he recommended; but if any of his suggestions were not

adopted, he always found Mr. Hill most ready to give way to the

course which he suggested.”[353]

He admitted that—

“No absolute bargain had been broken with Mr. Rowland Hill,

still he could not help expressing his sincere regret that,

after three years’ exertions, which were characterized by the

utmost zeal and intelligence, he should be allowed to retire

from the public service in the way in which he had. He repeated

that, although no bargain had been broken, still, if zeal,

intelligence, and ability, and the rendering important public

services, entitled any one to claim consideration, Mr. Hill had

a most powerful case.”[354]

Towards the close of his speech he dealt as follows with Mr. Goulburn’s

statement as to the extent of the money-order operations:—

“The calculation which the right hon. gentleman had made, as to

the amount of money transmitted through the Money-Order Office,

was a most extraordinary one. The right hon. gentleman stated

the amount to be eight millions, whereas he should have said

four millions; the right hon. gentleman had made the slight

mistake of doubling the amount by calculating the money which

was paid in, and adding to it the same money when paid out.

According to the right hon. gentleman’s mode of calculating, to

arrive at the quantity of water which passes through a pipe,

you must add the water which enters at one end to the same

water when it passes out at the other end, and the quantity so

added together will give the result desired.”[355]

He rejoiced that a Committee was to be appointed, and he observed, in

conclusion:—

“That if ever there was a measure in reference to which the

people had a right to ascertain whether it was carried into

effect fully and fairly, it was this.”[356]

Sir Robert Peel—

“Had never felt a doubt as to the great social advantages

of lowering the duty on letters; the only doubt was as to

its financial effect: in all other respects the result of

any inquiry would show that, whatever might have been the

loss to the revenue, much advantage had been derived in what

concerned the encouragement of industry, and the promotion of

communication between the humbler classes of the community.”

After observing that “it was, therefore, no dissatisfaction with Mr.

Hill’s conduct, no indifference to his services, that led him and his

right hon. friend to take the course they had taken,”[357] he said, in

reference to my original appointment—

“It appeared to him that, had it been deemed necessary to

retain Mr. Hill’s services, and had it been conceived that the

Post Office authorities were hostile to the plan, prejudiced

against its principle and its details, and indisposed to lend

themselves with zeal and cordiality to carrying it out, the

plan should have been, not to retain Mr. Hill in control over

the Post Office (yet unconnected with it), but to have at once

made him Secretary of the Post Office. That department would

thus have been no longer in a position continually to obstruct,

as the complaint was, the due execution of the plan; but Mr.

Hill himself, the person so deeply anxious for the success of

the scheme, would have the immediate control of it.”[358]

He also spoke of Colonel Maberly in terms of general esteem, and denied

that he had failed in cordial co-operation with me, speaking likewise

in high terms of Lord Lowther, and maintaining (contrary to fact) that

he had voted in committee for all Mr. Warburton’s resolutions,[359] and

was a decided friend to Mr. Hill’s system.[360] He acquiesced in the

appointment of a Committee, and “would assure them (the House) that,

while he continued in office, he would lend all his weight, influence,

and authority to insure full justice to the new system.”[361]

Sir Thomas Wilde declared himself satisfied with the amendment, which was

agreed to without a division.[362]

The indirect effect of the modification demanded by Ministers in Sir

Thomas Wilde’s motion was to take the nomination of the Committee out

of the hands of the mover, and to give it to Government—the natural

consequence being that the majority was made to consist of Government

supporters. Of the thirteen gentlemen selected, six only were of the

Liberal party; amongst these, however, were some of my best friends. Of

course, in securing a majority, Government also obtained the appointment

of the Chairman, and the choice fell upon Sir George Clerk. Upon this

choice no further comment can be required than a simple statement of the

position. I had appealed against a decision of the Treasury, a Court

was constituted to try the case, and of this Court the Secretary of

the Treasury was President. Lord Brougham used to tell of an amusing

occurrence, I think at York, at the time when he was on the Northern

Circuit. When the list of the jury was calling over, preparatory to

trying a certain case, the judge, remarking identity of name between one

of the jurors and the plaintiff in the suit, and inquiring, “I suppose,

Mr. Thomson, you are no relation to the plaintiff in this cause?” was

answered, “Please you, my Lord, I _is_ the plaintiff.” The interloper

was of course discharged, and a severe rebuke was given to the officer

of the court by whom so improper a selection had been made. Looking at

my own case, however, the parallel would have been more complete had

he been retained, and made, at least, foreman of the jury. However, to

have obtained a Committee at all was a very great gain; for though the

bias to be naturally expected from its composition did not fail to show

itself in the course of the proceedings, still opportunity was thus given

for that full and plain statement of facts which, I felt sure, would

suffice to set me right with the public; and, in justice to the Committee

generally, I must say that my opportunity for making such statements was

fairly given. I had, indeed, some browbeating to endure (even beyond what

appears in the Report, as may be seen by the letter given below),[363]

but with this the Committee generally did not appear to sympathize;

indeed, I have reason to believe that it tended rather to injure than to

benefit the cause which it was meant to advance.

APPENDICES.

APPENDIX A.

[See p. 57.]

ROYAL ASTRONOMICAL SOCIETY.

[_For my Biography, written, chiefly from my dictation, in

June, 1874._]

Although a member of the Astronomical Society for more than half a

century, and, with the exception of two out of about 430, the oldest now

living, I have never contributed to the Society’s transactions.

Yet from boyhood I have been very much attached to astronomical pursuits.

My father was well informed on the subject, and eventually, though

several years later than myself, became a member of the Society.[364] He

had long possessed a reflecting telescope, capable of showing Jupiter’s

Moons and Belts, and Saturn’s Rings, though not, according to my

recollection, any of the moons, even the rings appearing not severally

but as one. He had also a Hadley’s Quadrant, an artificial horizon, and a

tolerably good clock, and he regularly took in the “Nautical Almanac.”

By means of this simple apparatus, he not only regulated the clock, but

determined the latitude and even the longitude of our house, or rather of

the playground, at Hill Top.

In these occupations I was invariably his assistant; and it was in this

manner and with the aid of his lectures that I gradually acquired, even

while a boy, a taste for Astronomy, and, for my age, no inconsiderable

knowledge of the subject.

My father (like myself in youth and early manhood) was a great walker,

and we frequently journeyed together. When I was only nine years of age,

I walked with him, for the most part after dark, from Birmingham to

Stourbridge, a distance of twelve miles, with occasional lifts—no doubt

according to usage—on his back. I recollect that it was a brilliant

starlight night, and the names of the constellations and of the brighter

single stars, their apparent motions and the distinction between the

so-called fixed stars and planets, formed then, as on many other similar

occasions, never-failing subjects of interesting conversation, and to me

of instruction. On the way we passed by the side of a small pool, and,

the air being still, the surface of the water gave a perfect reflection

of the stars. I have a vivid recollection, after an interval of nearly

seventy years, of the fear with which I looked into what appeared to me

a vast abyss, and of my clinging to my father to protect me from falling

into it.

The remarkable comet of 1811—remarkable from the length of time it

continued in sight—interested me greatly. I was then fifteen years of

age. I examined it frequently with our telescope, got much information

from my father and from such books as were accessible to me; and before

the comet had disappeared was, I believe, tolerably familiar with what

was then known of cometary astronomy.

As already stated in the “Prefatory Memoir,” the teaching of a subject

was with me concurrent, or nearly so, with the learning. I soon began to

lecture on Astronomy, first to the boys of our school, and afterwards to

a literary and scientific association of which I was a member.

With a view to these lectures, availing myself of the “Transactions

of the Royal Society” (taken in by one of the Birmingham libraries to

which we subscribed), I read, I believe without exception, all the

contributions of Sir William Herschel, then incomparably the first of

living English astronomers. My reverence for the man led me to contrive,

on the occasion of my second visit to London (1815), to go round by

Slough, in order that I might obtain a glimpse—as the coach passed—of

his great telescope, which I knew could be seen over the tops of the

neighbouring buildings.

In the “Prefatory Memoir” I have already spoken of my teaching

navigation, of the planispheres which I constructed for my father’s

lectures upon electricity, of my trigonometrical survey, of my visit

to Captain Kater and the Greenwich Observatory, and of my Vernier

pendulums—all more or less intimately connected with my pursuit of

Astronomy. Nor must I omit mention of a popular explanation of the

transit of Mercury in May, 1832, which I wrote for the “Penny Magazine.”

(See Vol. I., p. 82.)

I may also mention, as a fact worth recording, that in 1817 (I believe)

the celebrated mathematician, M. Biot, passed through Birmingham on his

return from the Shetland Isles, where he had been engaged in measuring

an arc of the meridian.[365] My father was invited to dine with him, I

think at the house of Mr. Tertius Galton; and afterwards both he and I,

among others, were invited to meet him at the rooms of the Philosophical

Institution. Very few obeyed this second summons, perhaps because the day

fixed upon was Sunday. He showed us in action a small instrument for the

polarization of light—a subject of which my father and I, and I think the

others, were up to that time profoundly ignorant. The only individual

with whom M. Biot appeared to be previously acquainted was an emigré, Dr.

De Lys, a leading physician of Birmingham, whose father, the Marquis De

Lys, had been guillotined during the Reign of Terror. In the evening we

met again at a coach office in the Market Place, to bid farewell to M.

Biot on his departure for London, when he caused some tittering, and put

poor Dr. De Lys to the blush by publicly kissing him, in French fashion,

on both cheeks.

To return to the Astronomical Society. My attendance at its meetings, so

long as I continued to live near Birmingham, was necessarily rare. On

my removal to the neighbourhood of London it became more frequent, but

even then my time was so fully occupied with more pressing duties that

my attendance remained very irregular, and it totally ceased several

years ago. I have, however, invariably read the “Monthly Notices” of the

Society’s proceedings, and have thus benefited more, perhaps, than by

mere attendance.

Still, as already stated, I have never contributed to the Society’s

transactions, the truth being that up to the time of my becoming disabled

for steady application to any difficult subject, my mind was so entirely

engrossed with my official duties, that the little leisure I could obtain

was necessarily devoted to recruiting my health.

Nevertheless, as already shown,[366] I have attempted something to

promote my favourite science. The following is an instance of the kind:—

VARIABLE STARS.

On the 16th January, 1865, I addressed the following letter to my late

excellent friend, Admiral Smyth:—

“MY DEAR ADMIRAL,—I have just completed the perusal of your

very interesting volume on ‘The Colours of Double Stars,’

kindly presented to me by Dr. Lee in your name and his; and I

thank you for the gratification it has afforded me.

“What you say on the subject of variable stars has called to

my recollection an idea which first occurred to me shortly

after the discovery of the periodicity of the increase and

decrease in the number and frequency of solar spots. I am

aware that such increase and decrease is not continuous, and

that the variation is not such as materially to affect the

Sun’s brightness. Still, in point of fact, is not our own Sun

a variable star—however slightly—with a period, tolerably well

defined, of about eleven years? And may not the more marked

character of other variable stars be owing to similar causes to

those which produce the spots in our sun, acting with greater

regularity and intensity?

“If you think it deserving attention, pray favour me with your

opinion of my theory. Possibly it may have been suggested

previously, but if so, I am not aware of the fact.

“I remain, my dear Admiral, yours faithfully,

“ROWLAND HILL.

“Admiral Smyth, F.R.S., &c., &c., &c.”

Shortly afterwards I received a very friendly letter from Mrs. Smyth, the

tenor of which will be sufficiently understood from what follows:—

“Hampstead, 20th January, 1865.

“DEAR MRS. SMYTH,—Many thanks for your letter. Pray don’t let

the Admiral withdraw himself from his present work. My theory

can wait, or I may find an opportunity of consulting some other

authority.

“Our kindest regards.

“Very truly yours,

“ROWLAND HILL.”

I accordingly, on the 14th February following, addressed a letter—similar

to the one to Admiral Smyth—to my friend, Mr. Warren De La Rue, then

President—as Admiral Smyth had once been—of the Astronomical Society;

but although Mr. De La Rue took much trouble to ascertain whether my

theory had, as he thought, been suggested before, it was not till long

afterwards that he was able to give any definite information on the

subject.

In a letter of July 9th, 1866, Mr. De La Rue drew my attention to a

paper by Mr. Balfour Stewart in the Transactions of the Royal Society of

Edinburgh, which, in the opinion of Mr. De La Rue, “gives a very explicit

enunciation” of the theory.

On referring to the paper in question (Vol. XXIII, part iii.), I found

that it was read on the 18th April, 1864, and the following is an extract

from a memorandum which I made on the subject:—“Indirectly, by showing

a probable connexion between the maxima and minima of Sun-spots and the

rotation of Jupiter about the Sun, and by suggesting that the periodic

variations of the stars is caused by the rotation of large planets

about them, Mr. Balfour Stewart has, I think, forestalled me.” Perhaps,

however, I may be justified in doubting whether the enunciation here

given is very explicit.

Before proceeding, it is necessary to digress for a moment. When a boy

I was fond of reading books of elementary science. I occasionally met

with statements which puzzled me—which appeared to me to be wrong—but

assuming, as children do, the infallibility of the author—or perhaps I

should say of a printed book—I naturally came to the conclusion that my

own understanding was in fault, and became greatly disheartened. After

awhile—I forget on what occasion—I applied for solution of the puzzle to

my father, who, possessing a large amount of general information, was

well qualified to advise. To my great delight, he assured me that I was

right and the author wrong. My unqualified faith in printed statements

was now, of course, at an end; and a habit was gradually formed of

mentally criticising almost everything I read—a habit which, however

useful in early life, is, as I have found in old age, a cause of much

waste of thinking power when the amount is so reduced as to render

economy of essential importance.

Still, through the greater part of my life this habit of reading

critically, combined as it was with the power of rapid calculation, has

been of great use to me, especially in my contests with the Post Office,

and, after I had joined the Department, in the revision of the thousands

of Reports, Returns, and Minutes prepared by other officers.

In general literature, if the author attempt to deal with science, the

chance of a blunder appears to be great. Even Lord Macaulay could not

always do so with safety, as appears from the following passage:—“In

America the Spanish territories [in 1698] spread from the equator

northward and southward _through all the signs of the Zodiac_ far into

the temperate zone.”[367] What can be the meaning of the words which I

have marked for Italics?

Mrs. Oliphant, too, whose admirable stories I never miss reading, says,

in one of her latest, “there was a new moon making her way _upwards_ in

the pale sky.”[368]

There is no writer to whom I feel more grateful than to Miss Edgeworth.

When a boy I read her delightful stories with the greatest possible

interest, and I feel sure that they had considerable influence in the

formation of my character. Unfortunately, however, they are frequently

disfigured by scientific errors. Thus, in her admirable story of “The

Good Aunt,” the following passage occurs: “My dearest Aunt,” cried he

[Charles], stopping her hand, as she was giving her diamond ear-rings to

Mr. Carat—“stay, my dearest aunt, one instant, till I have seen whether

this is a good day for selling diamonds.”

“O, my dear young gentleman, no day in the Jewish calendar more proper

for de purchase,” said the Jew.

“For the purchase! yes,” said Charles, “but for the sale?”

“My love,” said his aunt, “surely you are not so foolish as to think

there are lucky and unlucky days.”

“No, I don’t mean anything about lucky and unlucky days,” said Charles,

running up to consult the barometer; “but what I mean is not foolish

indeed; in some book I’ve read that the dealers in diamonds buy them

when the air is light, and sell them when it is heavy, if they can,

because their scales are so nice that they vary with the change in the

atmosphere.”

Now, as the metallic weights are of greater specific gravity than the

diamonds, the interests of the dealers—so far as they are affected by

change of atmosphere—must be to buy when the air is _heavy_ and sell

when it is _light_. An increase of density in the air would, of course,

reduce the gravity of both diamonds and weights, but not equally: the

diamonds, being the more bulky, would lose gravity more than the weights,

and consequently would weigh less. If it were possible that the air

should increase in density till it became as heavy, bulk for bulk, as the

diamonds, they would float therein, or, in other words, weigh nothing at

all.

I well remember when, as a boy, I first read this admirable story, how

much I was puzzled by the mistake in question.

An error, occasionally met with in novels, is as follows. A wonderful

marksman has to exhibit his powers, which he does thus:—He throws into

the air two birds—or perhaps inanimate objects—as two apples; then,

_waiting till both are in a line with himself_, sends his arrow or bullet

through both. A slight consideration will show that, in a vast majority

of cases, no amount of waiting would suffice.

Another prevailing error is, that a person simply standing by the side of

a pool can see his own reflection from the surface—Narcissus must have

found some support which enabled him to lean over the fountain.

But it is in books especially intended to teach elementary science that

such errors are most to be regretted.

A few years since I purchased for some of my grandchildren the eighth

edition of “The Seasons,” by Mrs. Marcet. It is an admirable work,

highly interesting and useful; but before placing it in the hands of my

grandchildren, I thought it necessary to read it myself—a very pleasing

task, by-the-by—and to correct any errors I might find. As examples, I

may mention that in Volume I. snow is described as frozen rain; that

in Volume IV. _both_ stones in a flour-mill are said to revolve; and

that the description in the same volume of a marine steam engine is very

incorrect.

Again, few books are better calculated to interest boys than Dr. Parris’s

“Philosophy in Sport,” but when, in the year 1829, I bought a copy for

the School-Library at Bruce Castle, I found it necessary, before placing

it there, to make numerous corrections to which I drew the attention

of the author, who, in a letter dated March 18th, 1829, still in my

possession, thanks me for my communication, and admits some of the

errors, though not all.

As a specimen of the admitted errors, I give the following:—“Mr. Seymour

now informed his young pupils that he had an experiment to exhibit,

which would further illustrate, in a very pleasing manner, the truth of

the doctrine of _vis inertiæ_. He accordingly inverted a wine-glass,

and placed a shilling on its foot; and having pushed it suddenly along

the table, _the coin flew off towards the operator, or in a direction

opposite to that in which the glass was moving_.”[369]

My correction is as follows: “The coin would fall nearly in a

perpendicular direction, but inclined a little _towards_ the direction in

which the glass was moving, owing to the friction between the glass and

coin.”

As a specimen of the non-admitted errors, I give the following: “He

had ignorantly fired a quantity of oxygen and hydrogen gases in a tin

vessel; the consequence of the combustion was the immediate formation of

a _vacuum_; and what happened? Why, the pressure of the external air,

not being any longer balanced by elastic matter in the interior of the

apparatus, crushed it with violence, as any other enormous weight might

have done; and so ended the accident, which report magnified into a most

awful catastrophe.”[370]

My correction is as follows: “The first effect of the combustion was to

_expand_ the air in the vessel, and this _expansion_ it was that caused

the accident.”

On which the author, after quoting my correction, replies, “Now you will

allow me to say that here you have fallen into an error; I am perfectly

correct in saying that the accident arose from the external pressure

of the atmosphere; for remember that the vessel contained a mixture of

oxygen and hydrogen gases, which, by combustion, immediately combined

and formed water, leaving an almost perfect vacuum in the interior.”

If any one entertain a doubt as to which of us is correct, I would

suggest his filling a small bladder with the proper mixture of oxygen and

hydrogen, and exploding it by electrical means; as I did nearly sixty

years ago. The bladder will be destroyed; but, according to Dr. Parris’s

view, it should simply collapse.

But even men of unquestionable scientific knowledge are not always

correct. The late Professor Phillips, in his able and interesting

Address as President of the British Association in 1865, after noticing

Foucault’s recent admeasurement of the velocity of light, proceeded as

follows:—“By this experiment the velocity of light appears to be less,

sensibly less, than was previously admitted; and this conclusion is of

the highest interest. For, as by assuming too long a radius for the orbit

of Jupiter, the calculated rate of light-movement was too great; so now,

by employing the more exact rate and the same measures of time, we can

correct the estimated distance of Jupiter and all the other planets from

the Sun.”[371]

Professor Phillips’s great forte was geology, not astronomy. To any one

familiar with the means by which Römer determined the velocity of light,

it is unnecessary to point out that, although his observations were

made on the satellites of Jupiter, the radius of Jupiter’s orbit has

nothing to do with the problem. The only material facts are, first, the

_difference_ between the maximum and minimum distance of Jupiter from the

earth,—that is to say (disregarding eccentricity) the diameter of the

earth’s orbit; and, secondly, the effect which this varying distance has

on the times at which the eclipses apparently take place. This effect

Römer found to extend to about 16 minutes—and he thence concluded that

light occupied 16 minutes in travelling across the earth’s orbit.

With the view of rendering the above intelligible to those not familiar

with the subject, I offer the following illustration:—Suppose it to be

known that about a certain hour a gun will be fired at a remote spot,

the direction of which, but not the distance, is known, and that two

persons (A. and B.) arrange to avail themselves of the opportunity for

ascertaining, approximately, the velocity of sound; then, each being

furnished with a good watch marking seconds, A. places himself at a

certain spot, and B. at a known distance—say a mile—from A., and in a

direction opposite to that of the gun, so that B.’s distance from the gun

shall be a mile greater than A.’s—the actual distance in either case is

unimportant.

Each now records the exact moment at which he hears the report; and if

the gun be fired repeatedly, several such records are made, in order to

give a more accurate result.

A. and B. then meet and compare notes. They, of course, find that A.’s

time is in each instance earlier than B.’s. The average of the several

differences would be about 4¾ seconds—showing that sound travels a mile

in that time.[372]

The mode of procedure here described is, of course, not that actually

adopted for determining the velocity of sound, but it is a practicable

mode, and is selected because it is analogous to that adopted by Römer

for determining the velocity of light.

A copy of Professor Phillips’s Address was sent to me immediately after

its delivery, and, on my detecting the error, I endeavoured to induce a

friend of his, deservedly eminent as a practical astronomer, to draw the

Professor’s attention thereto, with a view to its correction before the

publication of the permanent report of the Society’s proceedings; but,

unfortunately, the attempt did not succeed.

In another similar case, however, as appears by the following

correspondence between the Astronomer Royal and myself, I was more

successful:—

“Hampstead, N.W.

“1868—June 17.[373]

“MY DEAR SIR,—Pray accept my thanks for the copy of your

Report. It came while I was at Brighton; but, since my return

home, I have read it with great interest. I felt it a great

privation not to be able to attend the Visitation.

“Will you allow me to request your attention to what appear

to me to be serious errors in the recent annual Address of

the President of the Astronomical Society? They will be found

in the last paragraph of page 119 of the ‘Monthly Notices’

for February. To save you trouble, I have extracted the part

in question, and have underlined the words which I think

erroneous. ‘At the present time the Earth is about three

millions of miles nearer to the Sun in our northerly winter

than in our summer; our coldest month is about 60° Fh. colder

than our hottest, and our winter lasts for about eight days

_longer_ than our summer. M. Leverrier has calculated that

200,000 years ago the Earth approached the Sun by upwards of

ten millions of miles nearer in winter than in summer: the

winters were then nearly a month _longer_ than the summers, and

in the latitude of London there was a difference of about 112°

Fh. between the hottest and the coldest periods of the year.’

“If you find that I am right, perhaps you will have the

kindness to draw Mr. Pritchard’s attention to the errors, with

a view to their correction before the Address is printed in

the ‘Transactions.’ I would write to Mr. Pritchard myself, but

that, as I could not speak with authority, I might give offence.

“I have watched the subsequent monthly numbers in the

expectation of finding a correction, but none has appeared.

“Faithfully yours,

“ROWLAND HILL.

“The Astronomer Royal, &c., &c., &c.”

The Astronomer Royal promptly replied as follows:—

“Royal Observatory, Greenwich, London, S.E.

“1868—June 18.

“MY DEAR SIR,—I will duly bring before Mr. Pritchard the

substance of your note of yesterday.

“The two clauses which you have cited are, on the face of them,

erroneous; and in the first the fault clearly is in the word

_longer_. In the second, the fault may be in the word _nearer_.

For, during the period through which the great eccentricity

prevails, the semi-revolution in the precession of the

equinoxes may have reversed the seasons.

“It would seem that Mr. Pritchard has had in view the table in

‘Lyell’s Principles of Geology,’ Vol. I., p. 293. In the notes

continued on p. 294, the references are to the case of winter

in aphelion.

“The subject is a thorny one, but well worth your attention.

“I am, my dear Sir, yours very truly,

“G. B. AIRY

“Sir Rowland Hill, K.C.B., &c., &c., &c.”

I am not aware how the passage in question stands in the Society’s

Transactions.[374]

The following narrative seems to show that in a progressive science like

Astronomy even the highest authority is not infallible.

Some sixty years ago, my attention having been accidentally drawn to a

tide-mill for grinding corn, I began to consider what was the source of

the power employed, and came to the conclusion that it was the momentum

of the earth’s revolution on its axis. The next question I asked myself

was—could such power be diverted, in however slight a degree, without

drawing, as it were, on the stock? Further consideration showed me that

the draught required for grinding the corn was trifling in comparison

with that employed in grinding the pebbles on every seashore upon the

earth’s surface; and, consequently, that the drain on the earth’s

momentum might suffice in the course of ages to effect an appreciable

retardation in the earth’s diurnal revolution.

I now, as usual in case of difficulty, applied to my father. He could

detect no fault in my reasoning, but informed me that Laplace had

demonstrated in his great work (“_La Mécanique Céleste_”) that the time

occupied in the earth’s diurnal revolution is absolutely invariable. Of

course both my father and I accepted the authority as unquestionable; but

I never could fully satisfy my mind on the subject, and for the greater

part of my life it was a standing puzzle.

It may be stated briefly that Laplace’s demonstration appears to

have rested mainly on the fact that his Lunar Tables, if employed in

calculating backwards certain eclipses of the Sun which happened about

2,000 years ago, give results agreeing so nearly with the ancient records

as altogether to exclude the possibility of any appreciable increase in

the length of the sidereal day during that long period.

But in the year 1866 Professor Adams (really the first discoverer of

the planet Neptune) received the Gold Medal of the Astronomical Society

for, among other recent claims, the discovery of an error in the data

on which Laplace constructed his Lunar Tables which vitiates the above

demonstration.

The details of this important discovery—and the co-operation therein of

M. Delaunay—were fully and ably stated by Mr. Warren De La Rue, then

President of the Society, on the presentation of the Medal.[375] And the

position of the question two years later is concisely stated as follows

by the Rev. Charles Pritchard, in an Addendum to his address as President

in 1868:—“_At present_, then, the case stands thus,—the Lunar Tables,

if calculated on the principles of gravitation alone, as expounded by

Messrs. Adams and Delaunay, and as confirmed by other mathematicians,

will not exactly represent the moon’s true place at intervals separated

by 2,000 years, provided the length of the day is assumed to be uniform

and unaltered during the whole of the intervening period. There are

grounds, however, for at least suspecting that, owing to the effects

of tidal action, the diurnal rotation is, and has been, in a state of

extremely minute retardation; but the mathematical difficulties of the

case, owing greatly to the interposition of terrestrial continents,

are so great that no definite quantitative results have hitherto been

attainable. The solution of the difficulty is one of those questions

which are reserved for the Astronomy of the future.”[376]

I need not say that this confirmation of the truth of my early conjecture

proved highly gratifying. I have only to add that the increase during

the last 2,000 years in the length of the sidereal day is generally

estimated at about the eightieth part of a second; but the estimate has,

I apprehend, no better foundation than this—namely, that since the recent

correction in the Lunar Tables an assumed increase to the extent in

question has become necessary in order to make the backward calculation

of the ancient eclipses agree with the records as to time.

I have found it very difficult at my age (little less than fourscore),

and with my mental powers seriously impaired, to deal, however

imperfectly, with a subject so abstruse as that now under consideration;

and I think it by no means improbable that there may be some error in my

statement of facts or in my argument thereon.

All that I can say is that I have done my best to render intelligible to

ordinary readers an important advance in modern Astronomy—interesting in

itself, irrespective of its remote and accidental connection with my own

biography.

The following very gratifying letter from the Astronomer Royal may

perhaps be appropriately given here. It is in reply to my congratulations

when, in recognition of his great public services, he was made a K.C.B.:—

“Flamsteed House, Greenwich Park, London, S.E.

“1872—June 22.

“MY DEAR SIR,—I could scarcely have had a more gratifying

letter in reference to the public compliment just paid to me

from any one than that from yourself. I can truly say that it

has been my secret pride to do what can be done by a person

in my position for public service; and whose recognition of

this can be more grateful than that of one who—by efforts in a

similar strain, but on an infinitely larger scale—has almost

changed the face of the civilized world?

“My wife (I am hesitating between two titles, not knowing

which is at the present moment correct, but being quite sure

of that which I have written) begs me to convey to you her

acknowledgment of your kind message.

“I am, my dear Sir, very truly yours,

“G. B. AIRY.”

APPENDIX B.

[See p. 71.]

“PREFACE TO THE LAWS OF THE SOCIETY FOR LITERARY AND SCIENTIFIC

IMPROVEMENT.

“In presenting to the public ‘The Laws and Regulations of the Society

for Literary and Scientific Improvement,’ its members feel it their duty

briefly to state the motives which influenced them in the formation of

such an establishment, and to explain their reasons for occasionally

deviating in the construction of their Laws from the systems which are

generally adopted for the governance of similar bodies.

“The experience of almost every one who has passed the time usually

devoted to education, but who still feels desirous of improvement, must

have convinced him of the difficulty of regularly devoting his leisure

hours to the object he has in view, from the want of constantly acting

motives, and the absence of regulations which can enforce the observance

of stated times. However strong the resolutions he has made, and whatever

may be his conviction of the necessity of adhering to them, trivial

engagements which might easily be avoided, will furnish him, from time to

time, with excuses to himself for his neglect of study: thus may he spend

year after year, constantly wishing for improvement, but as constantly

neglecting the means of it, and old age may come upon him before he has

accomplished the object of his desires; then will he look back with

regret on the many opportunities he has lost, and acknowledge in despair

that the time is gone by.

“Under these impressions, a few individuals who are desirous of extending

their literary and scientific knowledge, have endeavoured to establish a

society for that purpose; convinced that by so doing they have provided

most powerful motives for mental improvement.

“It has been thought highly desirable, that every member of the society

should be, as nearly as possible, upon an equality, that all may feel

alike interested in the success of the whole. In order to accomplish this

important object, every regular auditor is expected, according to the

rules of the society, to deliver a lecture in his turn. Thus, instead of

the society being divided into two parties, one consisting of lecturers,

the other of critics, every member feels himself called upon to listen to

the others with candour and attention, as he is aware that the time will

come when he shall require the same consideration from them. It will be

observed also, on a perusal of the laws, that each lecture is followed

by a discussion. Thus care is insured on the part of the lecturer that

he shall not attempt a subject which he has not well studied; and an

opportunity is given to every member to obtain an explanation of anything

advanced, which he may not have understood, or to express his opinions on

the questions that may arise, and, by these means, correct or confirm his

own ideas. But the principal advantage of a discussion is, that it calls

forth the individual exertion of every member, by inviting each to take a

part in the general instruction, and thus affording constant inducements

to private reading and study.

“In a town so populous as Birmingham, and which for superiority in art is

dependent on the discoveries of science, it cannot be doubted that many

individuals may be found who are desirous of intellectual advancement.

For such persons ‘The Society for Literary and Scientific Improvement’

was established; and they are respectfully and earnestly invited to lend

their assistance towards the promotion of its objects. The society cannot

promise that they shall meet with any considerable talent or learning

among its members; but in mixing with their equals, with young men of

similar tastes and similar pursuits, they may hope to find in a generous

emulation most powerful motives for application and perseverance.

“The details of management of a society like this, may, on a superficial

view, appear of little importance; those, however, who have had

opportunities of closer examination, will, it is presumed, agree with

the members of this Institution, in considering an attention to such

particulars as necessary, not only to the well-being, but to the

permanent existence of an association, for whatever purpose it may be

formed.

“With views like these, the ‘Society for Literary and Scientific

Improvement’ have been anxious to establish a mode of electing the

Committee, that should secure (as nearly as possible), an accurate

representation of the whole body; not only because it appeared reasonable

that the members would feel interested in the welfare of the Institution,

in proportion as the arrangements and regulations met their own views and

wishes, but because experience proves that, owing to imperfect methods of

choosing those who are to direct the affairs of a society, the whole sway

sometimes gets into the hands of a small party, and is exercised, perhaps

unconsciously, in a way that renders many persons indifferent, and

alienates others, until all becomes listlessness, decay, and dissolution.

“Men of worth and talent, of every denomination in religion and

politics, will be welcome members of the society; and to prevent any

unpleasant collision of opinions, it has been thought advisable to

exclude altogether the discussion of subjects which have reference to

peculiarities in religious belief, or to the political speculations of

the day; the important questions which respect the wealth of nations,

however, as they have no connexion with passing politics, are considered

as among the proper objects for the society’s attention.

“Such gentlemen as may feel desirous of improving their minds by engaging

in establishments of a nature similar to this, but who, on account of

their residing at a distance from any large town, have not hitherto

had the opportunity, will, it is hoped, be induced by the regulations

respecting corresponding members, to join the society; and they may

depend upon meeting with every attention, whenever the Committee shall be

favoured with their communications.”

APPENDIX C.

[See p. 93.]

CUBE ROOTS.

The mode of extracting the roots of _exact cubes_ which I taught the

boys, and which was probably that adopted by Zerah Colbourn, will be

best shown by an example. Suppose the question to be, What is the cube

root of 596,947,688? This looks like a formidable array of figures, and

a schoolboy, resorting to the usual mode of extracting the root, would

fill his slate with figures, and perhaps occupy an hour in the process.

Zerah Colbourn or my class would have solved the question in a minute,

and without making any figures at all. My class would have proceeded as

follows: They would first fix in their memories the number of millions

(596) and the last figure of the cube (8), disregarding all other

figures. Then, knowing the cubes of all numbers from 1 to 12 inclusive,

they would at once see that the first or left-hand figure of the root

must be 8; and deducting the cube of 8 (512) from 596, they would obtain

a remainder of 84. This they would compare with the difference between

the cube of 8 (512) and the cube of 9 (729), that is to say, with 217;

and seeing that it was nearly four-tenths of such difference, they would

conclude that the second figure of the root was 4. The third or last

figure of the root would require no calculation, the terminal figure of

an _exact_ cube always indicating the terminal figure of its root—thus

8 gives 2. The cube root, therefore, is 842. In this process there is

some risk of error as regards the second figure of the root, especially

when the third figure is large; but with practice an expert calculator

is able to pay due regard to that and certain other qualifications which

I could not explain without making this note unduly long. As already

stated, Zerah Colbourn did occasionally blunder in the second figure; and

this circumstance assisted me in discovering the above process, which I

have little doubt is the one he followed. If, instead of an exact cube,

another number of nine figures be taken, the determination of the third

figure of the root, instead of being the easiest, becomes by far the most

difficult part of the calculation.

[This part of the explanation was written by Sir Rowland Hill, as a note

to the Prefatory Memoir, before the year 1871. What follows was added in

1875.]

Rule for extracting the roots of imperfect cubes divisible into three

periods:—

1. Find first and second figures as described above.

2. Deduct cube of first figure from the first period (of the number whose

root is to be extracted), modified, if necessary, as hereafter described.

3. Then multiply the number (expressed by both figures) by each figure in

succession, and by 3.

4. Deduct the product (or the significant figures thereof—see example),

from the remainder obtained as above. (See 2).

5. Divide the remainder _now_ obtained by the square of the number

expressed by both figures (see 3), multiplied by 3—dropping insignificant

figures (see example),—and the quotient will be the last figure (or 3rd

figure) of the root.

I can confidently affirm from experience that there is nothing in the

above calculations too difficult for those who, possessing a natural

aptitude, are thoroughly well practised in mental arithmetic. I doubt,

however, whether the mode just described be exactly that which we

followed; our actual mode, looking at the results as described above

(which is in exact accordance with my Journal), must, I think, have been

more facile; but as it is fully fifty years since I gave any thought to

the subject, and as, in the eightieth year of my age, I find my brain

unequal to further investigation, I must be contented with the result at

which I have arrived.

It must be remarked, however, that cases will arise when some

modification of the process will be necessary. As, for instance, when

the first period of the cube is comparatively light, it may be necessary

to include therein one or more figures of the second period treated as

decimals; indeed, if the first period consist of a single figure, it

will be better to incorporate it with the second period, and treat both

together as one period,[377] relative magnitude in the first period

dealt with being important as a means of securing accuracy in the last

figure of the root. But expert calculators soon learn to adopt necessary

modifications, and by the “give-and-take” process to bring out the

correct result. Indeed, I find it recorded in my Journal that “small

errors will sometimes arise which, under unfavourable circumstances,

will occasionally amount to a unit.” These observations it must be

understood to apply only to the extraction of the roots of imperfect

cubes, which Zerah Colbourn invariably refused to attempt. When the cube

is perfect, the last figure of the root, as shown in the text, requires

no calculation at all.

_Example._

What is the cube root of 596,947,687?

[NOTE.—This is the number treated above, except that in the

unit’s place 7 is substituted for 8, in order to render the

number an imperfect cube; so slight a change, however—though

rendering it necessary to _calculate_ the last figure of the

root,—will still leave the root as before.]

Following the rule, we find the first and second figures of the

root in the manner described above. They are 8 and 4.

We next calculate the third or last figure of the root.

As the first figure of the second period of the cube is so

large, it will be unsafe to disregard it. Call the first

period, therefore, 596·9; all other figures may be neglected.

596·9 mill.

(2) 8³ = 512 ”

-----

84·9 ”

(3) deduct 84 x 8 x 4 x 3 = (roughly) 80·6 ”

-----

(5) divide by 84² x 3 = (88 x 80 x 3)[378] = 2·1 4·3

-----

2

Quotient—2, which is the third or last figure of the root.

[NOTE.—I have not encumbered the above figures with the ciphers

which should accompany them, as, to the expert calculator, this

will be needless.]

The root, therefore, is 842.

It is stated in the text that my pupils could extract the cube roots

of numbers ranging as high as 2,000,000,000. In the ordinary mode this

number would be divided, as above, into four periods; but my pupils

treated the 2,000 as one period, the approximate root of which is of

course 12, the cube of 12 being 1,728.

APPENDIX D.

[See p. 202.]

VERNIER PENDULUM.

Bruce Castle, Tottenham,

June 7th, 1832.

_To the Council of the Royal Astronomical Society._

GENTLEMEN,—In troubling you with the following sketch of an improvement

in astronomical clocks, I have a two-fold object. First, to obtain the

loan of the necessary instruments, should you consider the plan worth

prosecuting; and, secondly, to avail myself of the suggestions of such

members of the Society as are more experienced than myself in the minute

details of practical astronomy. The objects of the proposed improvement

are: To supply an apparatus capable of measuring time to a small fraction

of a second, and to make the determination of the exact time a matter

of calm and deliberate inquiry, and thus to avoid the errors which must

frequently arise from the hurry attending the present method.

In order to accomplish these objects, I propose to make use of the

principle of the Vernier, by suspending in front of the clock an

additional pendulum somewhat shorter than that of the clock, and so

placed that the coincidence of the two when vertical may be determined by

means similar to those used by Captain Kater; this additional or Vernier

pendulum to be put in motion at the instant of observation by means of

a trigger under the command of the observer at the telescope, and its

vibrations reckoned till a coincidence takes place between it and the

clock pendulum. This pendulum may have a maintaining power and an index

to save the trouble of counting. When at rest, the Vernier pendulum must

of course be raised to the extent of its oscillation.

The results of experiments commenced with very imperfect instruments

about two years and a-half ago, and continued at intervals to the present

time, appear to be as follows:—

When a Vernier pendulum, vibrating once in ·9 second, or 10 times in 9

seconds, is employed, its coincidences with the seconds pendulum of the

clock may be determined to a single vibration with the greatest ease by

the unassisted eye, and thus, of course, tenths of a second are readily

estimated.

When a Vernier pendulum vibrating once in ·99 second, or 100 times in 99

seconds, is employed, its coincidences with the seconds pendulum of the

clock may also be determined to a single vibration, but not without the

aid of a telescope. By these means hundredths of a second are measured

without much difficulty.

In order to avoid the inconvenience of having to suspend sometimes one

pendulum and sometimes the other, and also to escape the loss of time

which, if the hundredths pendulum were constantly used, would arise when

the observer wished to estimate tenths of a second only, I propose to

adopt the following arrangement:—To employ a single Vernier pendulum of

such a length as to vibrate once in 8·99 second, or a thousand times in

899 seconds. This pendulum differs so slightly from the tenths pendulum

(making ten vibrations in 8·99 seconds, instead of 9 seconds), that

for estimating tenths of a second it is practically the same, while

it affords the means of measuring hundredths of a second also. Its

operation will be best understood by an example:—Suppose the interval to

be measured by means of the Vernier to be ·24 second. At the second and

third vibrations of the Vernier pendulum after its release there would be

approximate coincidences between it and the clock pendulum, showing the

fraction of time to be between two-tenths and three-tenths of a second.

The coincidence at the second vibration would, however, be somewhat

nearer than that at the third. At the twelfth vibration there would be

another approximate coincidence somewhat closer than the first. At the

twenty-second vibration there would be a yet closer coincidence. At the

thirty-second one closer still, and at the forty-second vibration the

coincidence would be the most accurate of the series. Thus it appears

that the tenths of a second may be known by counting single vibrations

of the Vernier pendulum till a coincidence of some kind occurs, and that

the hundredths of a second may be determined by counting the decades of

vibrations, or all the coincidences after the first, until the most exact

coincidence arises.

By the use of the Vernier pendulum, when connected with an index, all

chance of error in reading the clock will, it is conceived, be avoided.

Having touched the trigger at the moment of observation, the observer

has, as it were, registered the time, and he may examine the clock at his

leisure, for it is manifest that a comparison of the index of the Vernier

pendulum with that of the clock will at any time determine the moment

of observation. It will also be seen that, should the observer omit to

notice the first coincidence of the pendulums, no inconvenience except

delay will arise, because the same coincidences will occur in a regular

series as long as the pendulums continue in motion.

There are a few provisions necessary for extreme accuracy which, in this

hasty sketch, it would be out of place to notice. I will just mention,

however, that the apparatus contains within itself the means of measuring

what may be called _the mean error of the observer_, or the average

interval which, as regards the particular individual, elapses between the

instant of observation and the release of the Vernier pendulum.

To subject the plan which I have here attempted hastily to describe to a

rigid trial will require instruments of much greater accuracy than those

which I can command, and if the Society possess a good clock not now in

use, I shall feel extremely obliged if I can obtain the loan of it. An

additional pendulum the requisite length, is not, I presume, to be found

among the Society’s instruments.

I have the honour to be, Gentlemen,

Your obedient servant,

ROWLAND HILL.

APPENDIX E.

[See p. 205.]

COACH COMPANY.

Two (or more) principal offices to be established in convenient places

for business—say, _one near the Bank, and one near the Regent Circus,

Piccadilly_; these offices to communicate with each other by means of

omnibuses.

_Coaches and omnibuses to radiate from these offices to all parts of the

environs of London._

A country office to be established at the extremity of each route.

The town to be divided into small districts, and the country into

larger, each with a house for the receipt and distribution of _parcels_.

(Shopkeepers who have goods to distribute in the neighbourhood may

undertake this). These stations to be, as far as practicable, on the

routes of the coaches.

The principal and the country offices to be receiving and distributing

houses, each for its own district.

Each coach in coming from the country to collect parcels from the

stations on its route, bringing them to its principal office. On going

out, to carry parcels for distribution from the principal office to the

same stations. Thus every parcel will pass through one or other of the

principal offices. (Exceptions can be made, if desirable, with respect

to parcels which would otherwise pass twice over the ground, viz., those

received at stations between the principal office and the place of their

destination; but the first arrangement would be by far the most simple).

Stations not on a coach route must transfer parcels to the nearest

stations which are on a route, and receive parcels from the same. [Qy. A

small extra charge].

Places to be booked at any station for any coach; a memorandum being

transmitted to the principal office concerned, with the parcels.

In some cases the passengers themselves may be so transmitted.

The omnibuses passing between the principal offices to carry passengers

and parcels from each for the other. Thus every coach will practically

start from both principal offices.

Coaches to depart from each principal office all at the same time. Say,

for all principal places, once every hour, from —— in the morning till ——

at night.

Coaches to arrive at each principal office all at the same time, say a

few minutes before the time of departure, the interval being sufficient

to transfer passengers and parcels.

The periods of departure and arrival at one office to differ by

half-an-hour from the corresponding periods at the other, so as to allow

just time enough (calculated at half-an-hour), for a transfer by the

omnibuses from one office to the other. Thus the coaches from one office

will start at the beginning and from the other in the middle of each hour.

Horses to be kept and changed at the country offices, or at stations

about the middle of each route. The latter arrangement will make the

stage shorter, and will bring the horse stations more immediately under

central revision. It will also require a less number of horse stations,

as in many cases one station will serve for two or more roads branching

out from each other. (At least one pair of horses must be kept at the

extreme station).

Supernumerary coaches and horses to be kept at the central offices for

use on any road on which there may be a temporary demand.

Each coachman to pay a certain rent, and with certain deductions to

receive the payments for passengers and parcels, but to have no control

as to the sum to be charged, the hour of starting, &c.

The masters of the stations to be remunerated by a certain sum (to be

paid by the coachman) for each passenger booked, and for each parcel

received or distributed.

Contracts to be made in all possible cases. Thus the coachmaker may

supply coaches at —— each per annum, or at —— per mile travelled.

The keepers of the horse stations may contract each for the supply of

horses required at his station at —— per mile.

In disposing of the shares, a preference to be given to those who would

make frequent use of the coaches, especially to those who travel to

London daily, as their influence would materially promote the interests

of the concern.

A personal right to go to or from town daily, by the same coach, to be

sold for a period, say a week, at a considerably reduced rate, or a month

at a still lower rate.

Proprietors to be entitled to similar privileges at five per cent. less

than others.

Transferable tickets, giving the holder a right to travel by any coach in

either direction on a particular road, to be sold (say twenty at a time)

at a slightly reduced rate.

All the carriages to be painted alike, and so as readily to distinguish

them from those not belonging to the Company.

An establishment on an extensive scale, such as is described in the

foregoing sketch, would possess many decided advantages over the little

independent establishments now existing. It would be more economically

managed; the necessary publicity would be more easily given to its

arrangements; the responsibility of the servants would be more efficient;

and the extent and permanence of the undertaking would justify the most

watchful attention to exact punctuality, to a proper speed, to the safety

and comfort of the passengers, and, in short, to all circumstances

conducive to a high reputation with the public.

_Economy._—This would manifestly result from the great division of

labour, and the wholesale demand for every article of expenditure. Also

from the power of transferring coaches from any road on which there was

less to one on which there was more travelling than usual.

The system of contracts and sub-contracts could not be introduced with

advantage into a small concern.

_Publicity._—The readiness with which the arrangements could be described

would tend greatly to their publicity. Thus, it would be easily said and

easily remembered, that from a certain office coaches depart every hour,

and from a certain other office at the half-hour, to all the principal

places within the limits of the threepenny post. This statement, with a

list of the places, fares, &c., would be placarded at every station, and

on every coach and omnibus.

_Responsibility._—An active and intelligent superintendent, well

acquainted with the means of holding others to responsibility, should

devote his whole time to the undertaking, visiting the various stations

periodically to see that all arrangements are observed, to settle the

accounts, &c.

He should require accurate reports to be made, showing at all times the

actual state of affairs, and the improvement or deterioration in each

department The most exact rules should be laid down and enforced for the

conduct of each class of servants. These rules should be placarded in the

coaches, at the stations, &c.

Enquiries as to the conduct of all concerned should be made frequently of

the proprietors who use the coaches daily, and every possible attention

paid to the well-founded complaints of passengers generally. A till might

be placed in each carriage, with an inscription requesting passengers

having cause to complain to put a statement of such complaint, with _name

and address_, into the till, which should be opened at the central office

at least once in each day.

_Punctuality and Speed._—The proper time of starting and that of passing

each station should be inscribed conspicuously on each coach, as well as

at each station. The actual time kept should be recorded at each extreme

station and at the horse station, and fines levied on the coachman for

deviation beyond certain limits. The allowance of time for the journey

should be such as to require the coachman to drive steadily but rapidly,

with no stoppage beyond a very short one (say a minute) at each station,

and a little more for taking up and putting down passengers on the road.

The coach should never wait nor turn out of the direct road between the

extreme stations. To save time, the passengers, in the omnibuses at

least, should be requested to pay as they go on. At the inferior stations

a signal might be established to show whether the coach need stop or not.

_Safety of Passengers._—Coaches of the safest construction, steady

horses, and temperate coachmen, only should be employed; and whenever

an accident occurs from whatever cause, a heavy fine should be levied

on the coachman, allowing him the right to recover the whole or part of

the penalty of the coach-contractor or horse-contractor, according to

circumstances. No galloping should be allowed.

The coach-contractor should be required to station a man at each central

office to examine each coach every time it comes in.

_Comfort of Passengers._—Some protection from wet and cold to be provided

for the outside passengers. Means of ascending and descending to be

improved. A convenient room at each station for those waiting. The

stations should _not_ be taverns; but coffee and some other refreshments

may be provided—there being no obligation, however, to call for anything.

The room should contain a map of London, directory, &c.

The arrangements of the Company would be capable of gradual and

almost indefinite extension. Thus they might take in towns more and

more distant, or they might comprehend hackney-coaches, cabriolets,

and omnibuses to all parts of London. The machinery required for the

distribution of parcels might be applied to that of the periodic

publications; and a contract might be entered into, advantageous to the

public as well as to the Company, for the collection, carriage, and

distribution of the twopenny and threepenny post letters.

This distribution might easily take place _each hour_, the letters being

carried by the coaches. No guards would be required, as the bags might be

put into a boot, of which keys should be kept at the post-offices only.

APPENDIX F.

[See p. 230.]

[The following letter to _The Scotsman_ was written by Mr. John Forster,

late Member for Berwick. In a marginal note Sir R. Hill has written, “I

vouch for its accuracy.”]

“SIR ROWLAND HILL AND THE PRINTING PRESS.

“London, February 12, 1872.

“SIR,—In your interesting article on the ‘Walter Press’ it was

stated that the idea of a Rotatory Machine printing newspapers

on a continuous sheet of paper was not novel; that Sir Rowland

Hill had worked at it many years before, as had other persons

in America. As to most of your readers this mention of a

benefactor of theirs in another way as a mechanical inventor

was no doubt something new and curious, it may be interesting

to them to learn what Sir Rowland Hill’s share of merit in

this matter was. I send with this a copy of the specification

of his patent for letter-press printing machines, taken out in

1835 (No. 6762, printed by the Patent Office in 1857), and an

account of it given in the ‘Repertory of Patent Inventions,’

No. 35. By these it will be seen that the most important

achievements of modern printing were effected by Sir Rowland

Hill thirty-seven years ago. His machine was to print either

with stereotype-plates or movable type (the difficulty of

fastening the last securely to cylinders revolving at great

speed was met by special contrivances); was itself to keep the

printing surfaces inked; to print a continuous roll of paper,

of any length, and both sides, while passing once through the

apparatus; to cut up the roll into sheets; and means were

contrived of performing those operations on two rolls at once,

so that at one revolution of the printing cylinders two copies

could be struck off. Such a machine was actually constructed

(at an expense of about £2,000), and was frequently shown at

work at No. 44, Chancery Lane, as many persons must remember.

Though driven by hand, it could produce at the rate of seven or

eight thousand impressions in an hour. One great difficulty of

most printing machines is that of securing perfect _register_

(the exact coincidence of the printing on opposite sides of the

paper). This was anticipated and met by the patent. The one

thing the inventor failed to do was to overcome the resistance

the collectors of the stamp duty presented to this printing on

a continuous roll, and to the affixing of the stamps to the

newspapers at the proper intervals during their passage through

the machine. Many years afterwards they allowed this to be done

by machinery contrived by Mr. Edwin Hill (who had assisted his

brother in the preparation of the printing machine), which was

affixed to the presses of the _Times_ and other papers, and

which itself registered, for the security of the revenue, the

number of impressions made. In 1835, the task of satisfying

the Treasury that this could be done with safety to it was too

formidable to be overcome,—at least it was not overcome. Sir

Rowland Hill’s attention was soon afterwards absorbed by his

plans of postal reform; and no one can regret this, seeing

what work he did in the Post Office, which probably no one

but himself could have done so well; while if the fourteen

years of his patent passed unprofitably to the inventor, other

hands have carried to extraordinary perfection the scheme of

a printing machine. Of course the Americans and the ‘Walter

Press’ have greatly advanced on ‘Hill’s Machine’ of 1835;

especially by the preparation of stereotype plates for this

particular service. In his specification, Sir Rowland Hill made

due mention of his predecessors, recording that an imitation of

the process of printing calico by cylinders revolving rapidly

was proposed for letter-press printing as early as 1790, by

Mr. William Nicholson, and that this was applied to stereotype

plates bent to a cylindrical surface by Mr. Edward Cowper in

1816. But the first practical scheme of newspaper printing on

a continuous roll of paper by revolving cylinders was produced

and set to work by Rowland Hill in 1835.

“I am, &c.,

“J. F.

“The Editor, _The Scotsman_.”

[Two years later Sir Rowland Hill wrote the following letter to the

_Journal of the Society of Arts_:]—

“TYPE-PRINTING MACHINERY

“SIR,—In the interesting paper ‘On Type-printing Machinery,’ by

the Rev. Arthur Rigg, which appeared in your _Journal_ of the

13th inst., there are certain errors affecting myself which I

request permission to correct.

“It is stated that rotating cylinders and continuous rolls

of paper were principles first introduced into type-printing

machinery by Mr. Nicholson in 1790, and further on it is

asserted, in reference no doubt to the printing machine which I

invented in 1835, that I ‘revived a proposal of Nicholson’s.’

“Now, so far from Mr. Nicholson proposing to print from types

on continuous rolls of paper, a reference to the specification

of his invention (A.D. 1790, No. 1,748) will show that,

excluding his proposals for calico and wall-paper printing,

which have nothing to do with type-printing machinery, he

invariably speaks of printing on sheets of paper; indeed, the

means of producing continuous rolls of paper were not invented

till several years later. Again, it will be seen that the means

he proposes for attaching the types to his cylinder, the real

difficulty to be overcome, are clearly insufficient for the

purpose; indeed, as stated in the specification of my patent

(A.D. 1835, No. 6,762), which was drawn by the late Mr. Farey—a

man thoroughly conversant with the subject—‘on account of

deficiencies and imperfections in the machinery described in

that specification [Mr. Nicholson’s] the same has never been

practised or brought into use.’

“Towards the close of his paper, Mr. Rigg seems to imply that

hitherto all schemes for fixing moveable types on a cylinder

have failed. I can only say that in my machine this difficulty

was entirely overcome. Indeed, in a letter which appeared in

the _Mechanics’ Magazine_ of November 12th, 1836 (when the

subject was before the public), I was enabled to state that

‘in the opinion of many eminent printers who have seen my

machine the end in view has been fully accomplished, for while

any portion of type may be detached from the cylinder with a

facility even greater than that with which a similar change

can be made in an ordinary form, each letter can be so firmly

locked in its place that there is no danger whatever of its

being loosened by centrifugal force or by any other cause.’

“While upon this subject, I may as well add that a comparison

of my specification with that of the ‘Walter Press’ (A.D. 1866,

No. 3,222) will show that, except as regards the apparatus for

cutting and distributing the printed sheets, and excepting

further that the ‘Walter Press’ is only adapted for printing

from stereotype plates, while mine would not only print from

stereotype plates, but, what was far more difficult, from

moveable types also, the two machines are almost identical. I

gladly admit, however, that the enormous difficulty of bringing

a complex machine into practical use—a difficulty familiar to

every inventor—has been most successfully overcome by Messrs.

Calverley and MacDonald, the patentees of the ‘Walter Press.’

“I am, &c.,

“ROWLAND HILL.

“Hampstead, February 26, 1874.”

APPENDIX G.

[See p. 260.]

EXTRACT FROM THE “GREENOCK ADVERTISER,” OF FRIDAY, MARCH 8th, 1850.

_Testimonial to_ ROBERT WALLACE, Esq., _late M.P. for

Greenock_. _The Pioneer of Postage Reform._

The Life of Sir Rowland Hill and the History of Penny Postage, Vol. 1 (of 2) · 第 11 / 12 章