CHAPTER XX

VOLCANOES OF THE LOWER OLD RED SANDSTONE OF "LAKE

CALEDONIA"--_continued_

The Southern Chain--The Pentland Volcano--The Biggar Centre--The

Duneaton Centre--The Ayrshire Volcanoes.

We have now to note the leading features of the groups of volcanic

rocks distributed along the southern line of vents already described.

At least four different centres of eruption may be observed on that

line. Their mutual limits are, on the whole, better seen than those of

the northern line, for from the north-eastern to the south-western end

of the volcanic belt the Old Red Sandstone and rocks of older date are

almost continuously exposed at the surface. The encroaching areas of

Carboniferous formations in Lanarkshire and Ayrshire interrupt but do

not entirely conceal the volcanic tracts.

II. THE SOUTHERN CHAIN OF VOLCANOES IN "LAKE CALEDONIA"

5. _The Pentland Volcano_

Beginning at the north-east end of the line we first come upon

the classic area of the Pentland Hills, for the study of which

the geologist is prepared by the admirable description of Charles

Maclaren,[363] and the earlier geognostical papers of Jameson.[364]

The area mapped in detail is represented in Sheet 32 of the Geological

Survey of Scotland, published in 1859, and described in the Memoir

accompanying that sheet.

[Footnote 363: _A Sketch of the Geology of Fife and the Lothians_,

1839. The detailed descriptions in this work are accompanied with a

map and two plates of sections. In the map all the volcanic rocks are

represented by one colour. In the sections the bedding of the rocks

is shown, and an indication is given of the succession of their chief

varieties.]

[Footnote 364: See specially _Mem. Wernerian Soc._ vol. ii.; also

MacKnight in vol. i. The account of the Pentland Hills by Hay

Cunningham in vol. vii. (1838) is clear but brief.]

When in these early days I surveyed this ground I found it extremely

difficult to understand. Being then myself but a beginner in geology,

and the study of old volcanic rocks not having yet advanced much beyond

its elementary stage, I failed to disentangle the puzzle. Not until

after more than twenty years, largely spent in the investigation of

volcanic rocks elsewhere, had I an opportunity of resurveying the

ground and bringing to its renewed study a wider knowledge of the

subject. A new edition of the map was issued in 1892, and I shall here

embody in my summary the chief results obtained in the course of this

revision.

The most obvious features in the Pentland area are the marked

development of the volcanic rocks at the north end of the chain,

their rapid diminution and disappearance towards the south-west, the

abrupt truncation of the bedded masses by the line of craggy declivity

which forms the northern termination of the hills, and lastly, the

continuation of the volcanic series northward in a totally different

form in the lower eminences of the Braid Hills.

The length of the whole volcanic tract is about eleven miles; its

breadth at the widest northern part is four miles, but from that

maximum it dwindles southwards and dies out in seven miles. Its western

side is in large measure flanked by the unconformable overlap of the

Upper Old Red Sandstone and Lower Carboniferous formations, though

in some places the base of the volcanic series is seen. The eastern

boundary is chiefly formed by a large fault which brings down the

Carboniferous rocks against the volcanic ridge. At the northern end,

this ridge plunges unconformably under the Upper Old Red Sandstone of

the southern outskirts of Edinburgh.

The bedded aspect of the truncated end of the Pentland chain, as seen

from the north, has been already alluded to (p. 281). The rocks dip to

the south-east, hence the lower members of the series are to be found

along the north-west side of the hills.

[Illustration: Fig. 86.--Section across the north end of the Pentland

Hills, from Warklaw Hill to Pentland Mains. Length about five miles.

1. Upper Silurian grits and shales, not seen where the line of

section crosses; 2 2. Andesites and diabases in numerous

interstratified sheets; 2 _s_. Intercalated sandstones and

conglomerates; 3. Felsitic tuffs and breccias and orthophyre

sheets; _n_, Volcanic neck; 4. Lower Carboniferous strata

lying unconformably on and overlapping the volcanic series;

5. Calciferous Sandstones and Carboniferous Limestone series

brought down against the volcanic series by a fault (_f_).

]

It will be noticed from the Geological Survey map that the volcanic

rocks of the main body of the Pentland Hills are arranged in

alternations of somewhat basic and more acid bands. The most basic

sheets are some amygdaloidal diabases at the bottom of the whole

series which make their appearance in Warklaw Hill (Fig. 86). The

greater number of the dark lavas are varieties of andesite, sometimes

tolerably compact, sometimes highly cellular and amygdaloidal. But

interstratified with these are thick sheets of what used to be

called "claystone," a term which here comprised decayed felsites

(orthophyres), and also felsitic tuffs and breccias. The remarkably

acid nature of some of these rocks has been already pointed out.

The total thickness of the volcanic series at the north end of the

hills is about 7000 feet, but as neither the top nor the bottom is

there visible, it may be considerably greater. At these maximum

dimensions the rocks form the high scarped front of the Pentland Hills,

which rises into so prominent a feature in the southern landscape of

Edinburgh. A series of transverse sections across the chain from north

to south will illustrate its structure and history. These I shall here

describe, reserving for subsequent consideration the great vent of the

Braid Hills.

A section taken through the north end of the chain, where the maximum

depth of volcanic material is exposed, presents the arrangement

represented in Fig. 86. It will be seen that the base of the series is

here concealed by the unconformable overlap of the Lower Carboniferous

rocks on the west side, while the top is cut off by the great fault

which on the east side brings down the Midlothian Coal-field.

[Illustration: Fig. 87.--View of the lava-escarpments of Warklaw Hill,

Pentland chain, from the north-west.]

The Lower Carboniferous conglomerates (4) creep over the edge and up

the slopes of the volcanic series of the Pentland Hills. They contain

abundant pebbles of the lavas, and were evidently laid down along a

shore from which the Pentland rocks rose steeply into land. Though

the actual base of the lavas is not seen here, two miles further to

the south highly-inclined Upper Silurian shales and mudstones are

found emerging unconformably from under the volcanic pile, and similar

strata probably underlie Warklaw Hill as indicated in the figure.

The Upper Silurian strata pass up into a lower group of the Lower

Old Red Sandstone, which has also been covered unconformably by the

volcanic series. In these underlying deposits we have evidence of the

pre-volcanic accumulations of the lake, which were broken up and tilted

at the beginning of the volcanic eruptions.

The lowest lavas, consisting of well-marked beds of diabase (2),

present their escarpments to the north-west and dip into the rising

ground, as sketched in Fig. 87. Their characters have been already

noticed in the general petrography of the Old Red Sandstone volcanic

rocks. Dark solid compact portions of them pass rapidly into coarsely

cellular slag, especially along the upper and under parts of the

several sheets. No tuff has been noticed between these basic flows, but

here and there thin lenticular layers of sandstone, lying in hollows

of the lava-sheets, are connected with vertical or highly-inclined

ramifying veins of similar material, with the plains of stratification

passing across the breadth of the veins. These features are an

exact reproduction of those above described in Forfarshire and

Kincardineshire. The amygdales consist of chalcedony, crystallized

quartz and calcite.

Torduff Hill, which rises to the east of Warklaw, consists of a mass of

coarse volcanic breccia or agglomerate (_n_), markedly felsitic in its

materials. It probably forms a neck marking a small volcanic vent, like

some others at the north end of the chain to be afterwards referred to.

In the lower part of Capelaw Hill, the next eminence in an easterly

direction, bedded andesites, with an intercalated band of sandstone and

conglomerate (2_s_), appear and pass under rocks of so decomposing a

kind that no good sections of them are to be found. The hill is covered

with grass, but among the rubbish of the screes pieces of felsite-like

rocks and breccias may be observed. Some of these blocks show an

alternation of layers of felsitic breccia with a fine felsite-like

material which may be a tuff. These rocks, conspicuous by the light

colours of their screes, alternate further up with other dark andesitic

lavas, and run south-westward for about five miles.

Beyond Capelaw Hill, upon a band of these pale rocks, comes a thick

group of sheets of dark andesite, which form the main mass of Allermuir

Hill. They are well seen from the south side and likewise from the

north, dipping towards the south-east at angles of from 35° to 40°, and

weathering along the crest of the hills into a succession of scars and

slopes which show the bedded character of the lavas.

At Caerketton Hill another band of pale material forms the conspicuous

craggy face so familiar in the aspect of the Pentland Hills as seen

from Edinburgh. This band consists of pale felsitic breccia, and

amorphous, compact, much-decayed rock, regarding which it is difficult

to decide whether it should be considered as a fine felsitic tuff,

or as a decomposed felsite. The band is better seen when traced

southwards. The light colour of its screes makes it easily followed by

the eye even from a distance along the hill-tops and declivities.

On the next hill to the south-west, known as Castlelaw Hill, this pale

band of rock is exposed in a few crags and quarries, and its debris,

protruding through the scanty herbage, slips down the slopes. On its

north side the screes display the same felsitic breccias and compact,

decayed felsitic rocks, occasionally showing a structure like the

flow-structure of rhyolite. The breccia which projects in blocks from

the summit of the hill has been quarried immediately below the crest on

the south side, where it overlies a thin intercalated band of a dull,

much-decomposed porphyry.

The breccias are composed almost entirely of thoroughly acid

rock-fragments, as may be judged from the percentage of silica shown

to occur in them. These fragments vary from the finest lapilli up to

angular pieces several inches long. They not infrequently display a

fine and extremely beautiful flow-structure. It is thus quite certain

that there are acid breccias intercalated among the more basic lavas

of the northern Pentlands, and that among the constituents of these

breccias are fragments of felsite or perhaps even lithoid rhyolite.

We may therefore be prepared to find that actual outflows of

felsitic lava accompanied the discharge of these highly-siliceous

tuffs. Unfortunately the manner in which the rocks decay and conceal

themselves under their own debris makes it difficult to separate the

undoubtedly fragmental bands from those which may be true lavas. But an

occasional opening, and here and there a scattered loose block, serve

to indicate that the two groups of rock certainly do coexist in this

pale band, which can be followed through the chain for upwards of six

miles until it is cut off by the eastern boundary fault.

At the south-west end of Castlelaw Hill, where a quarry has been

opened above the Kirk Burn, blocks of felsite may be observed showing

flow-structure on a large scale. The bands of varied devitrification

are sometimes a quarter of an inch broad, and weather out in lighter

and darker tints. Some of them have retained their felsitic texture

better than others, which have become more thoroughly kaolinized. That

these are not deceptive layers of different texture in fine tuffs is

made quite clear by some characteristic rhyolitic structures. The

bands are not quite parallel, but, on the contrary, are developed

lenticularly, and may be observed to be occasionally puckered, and to

be even bent back and folded over as in ordinary rhyolites. There is no

contortion to be observed among the stratified tuffs of the hills. This

irregularity in the layers is obviously original, and can only be due

to the flow of a moving lava.

On the east side of Castlelaw Hill, as shown in Fig. 86, dull reddish

andesites overlie the pale belt of felsitic rocks. Their lower bands

are marked by the presence of well-formed crystals of a dark green

mica. Their central and higher portions consist of porphyrites of the

prevalent type, both compact and vesicular. These lavas continue as far

as any rock can be seen. Beyond the boundary fault, the Burdiehouse

Limestone and oil-shales of the Lower Carboniferous series are met

with, inclined at high angles against the hills. It is impossible to

say how much of the volcanic series has here been removed from sight by

the dislocation.

If now we move three miles further to the south-west and take a second

section across the Pentland Hills, it will be found to expose the

arrangement of rocks represented in Fig. 88. At the western end the

Upper Old Red Sandstones (4) and Lower Carboniferous series (5) are

seen lying unconformably on the upturned edges of the Upper Silurian

shales (1). North Black Hill consists of a large intrusive sheet of

pale felsite (F) that has broken through the Silurian strata and has

in places thrust itself between them and the conglomerates of the

Lower Old Red Sandstone which lie unconformably upon them. In the

neighbouring Logan Burn, at the bottom of the Habbie's Howe Waterfall,

the felsite can be seen injected into the conglomerate. The felsitic

sill of North Black Hill runs for a mile and a half along the western

base of the volcanic series, and has a breadth of about half a mile. It

is the only important intrusive mass in the Pentland Hills.

[Illustration: Fig. 88.--Section across the Pentland Hills through

North Black Hill and Scald Law (length about three miles).]

To the south of the Silurian shales that lie against the southern

flank of North Black Hill, pale felsitic tuffs (3) occur, which are a

continuation of those already referred to as running southwards from

Capelaw Hill. Above them a series of andesites (2), with intercalated

bands of tuff, sandstone and conglomerate (2_s_), occupy the bottom

of the Logan valley and part of the slopes on both sides. In the

thickest band of tuffs, which is well-exposed along the road by the

side of the Loganlee Reservoir, a group of well-bedded strata occurs

from less than an inch to a foot or more in thickness. Generally

they are pale in colour, and are made up of white felsitic detritus,

but with a sprinkling of dull purplish-red fragments, and occasional

larger rounded pieces of different andesites. Some of the rocks might

be called felspathic sandstones. Other bands in the group are dark

purplish-red in tint, and consist mainly of andesitic debris, with

a dusting of white felsitic grains and fragments. There would thus

seem to have been showers both of felsitic and of andesitic ashes and

lapilli.

The dark lavas that overlie the tuffs are likewise well displayed

along the same road-section. They vary rapidly from extremely compact

homogeneous dark blue rocks, that weather with a greenish crust, to

coarse, slaggy masses and amygdaloids.

[Illustration: Fig. 89.--Section from the valley of the Gutterford Burn

through Green Law and Braid Law to Eight-Mile Burn.]

These more basic lavas are a continuation of those of Allermuir Hill,

and, as at that locality, they plunge here also under the same band

of white tuffs, breccias and felsites (3), which has been referred to

as stretching southward from Caerketton Crags. This band must here

be at least 500 feet thick. It forms Scald Law (1898 feet) and the

surrounding summits, and thus occupies the highest elevations in the

Pentland chain. It dips beneath the uppermost group of andesites,

which, as before, are here truncated by the eastern fault (_f_), the

Calciferous Sandstones and Carboniferous Limestone series (6) being

thrown against them.

A third section (Fig. 89), taken two miles still further south, shows a

remarkable attenuation of the volcanic series, and the appearance of a

thick group of conglomerates (2) lying conformably below that series,

but resting on the upturned edges of the upper Silurian shales (1). The

thick Allermuir porphyrites are here reduced to a few thin beds (3)

intercalated among the conglomerates and sandstones, amidst which the

whole volcanic series dies out southward. A detailed section of the

rocks exposed on the western front of Braid Law shows the following

succession:--

White felsitic rocks of Braid Law (4 in Fig. 89).

Coarse conglomerate passing down into sandstone. About 20 feet

visible.

Dark andesite, 4 feet.

Parting of yellow felspathic grit, 8 or 10 inches.

Andesite, 10 feet.

Hard felspathic grit, 6 feet.

Dark green amygdaloidal andesite, 2 feet.

Yellow felspathic sandstone and grit, 2 feet.

Dark green amygdaloidal andesite, 6 feet.

Felspathic grit and red and brown sandstone, 4 feet.

Dark andesite, perhaps 6 or 8 feet.

Great conglomerate with alternating courses of sandstone, rapidly

increasing in thickness southwards.

Above these dwindling representatives of the northern andesitic lavas

comes the continuation of the white band of tuffs and breccias of

Caerketton and Scald Law (4), which in turn dips under the highest

group of andesites. The Carboniferous strata (5) are brought in by the

fault (_f_). In little more than two miles beyond this line of section

the volcanic series disappears, and the Old Red Sandstone for a brief

space consists only of sedimentary deposits.

Besides the remarkable alternation of basic and acid ejections, there

is a further notable feature in the geology of the Pentland Hills.

This volcanic centre presents us with one of the most remarkable vents

anywhere to be seen among the volcanic rocks of Britain. The full

significance of this feature may best be perceived if we advance along

the hills from their south-western end. As has now been made clear, the

volcanic materials which begin about the line of the North Esk near

Carlops rapidly augment in thickness until, in a distance of not more

than seven miles, they attain a thickness of about 7000 feet, and then

form the great scarped front of the hills that look over Edinburgh. But

at the base of that wall their continuity abruptly ceases. The lower

ground, which extends thence to the southern suburbs of Edinburgh, and

includes the group of the Braid Hills, is occupied by another and more

complex group of rocks in which the parallelism and persistence so

marked in the Pentland chain entirely disappear.

This abrupt truncation of the bedded lavas and tuffs marks

approximately the southern margin of a large vent from which at

least some, if not most, of these rocks were probably ejected. The

size of this vent cannot be precisely ascertained on account of the

unconformable overspread of Lower Carboniferous strata. But that it

must have been a large and important volcanic orifice may be inferred

from the fact that the visible area of the materials that fill it up

measures two miles from north-east to south-west, and a mile and a

half from south-east to north-west, thus including a space of rather

more than two square miles. Its original limits towards the north and

south can be traced by help of the bedded lavas that partially surround

it, but on the two other sides they are concealed by the younger

formations. We shall probably not over-estimate the original area of

the vent if we state it at about four square miles.

[Illustration: Fig. 90.--Section across the north end of the Pentland

Hills, and the southern edge of the Braid Hill vent. Length about two

miles.

1 1. Andesites; 2. Fine tuffs, etc., of the Braid Hill vent; 3 3 3.

Agglomerate in lateral necks with felsitic intrusions (4).]

The materials that now fill this important orifice consist mainly of

"claystones," like those of the Pentland series--dull rocks, meagre to

the touch, varying in texture from the rough porous aspect of a sinter

through stages of increasing firmness till they become almost felsitic,

and ranging in colour from a dark purple-red, through shades of lilac

and yellow, to nearly white, but often strikingly mottled. A more or

less laminar structure is often to be observed among them, indicating

a dip in various directions (but especially towards the north) and at

considerable angles. Throughout this exceedingly fine-grained material,

lines of small lapilli may occasionally be detected, also bands of

breccia, consisting of broken-up tuff of the same character, and of

fine "hornstone" and felsite, with delicate flow-structure. Exhibiting

on the whole so little structure, this tract may be regarded as

consisting largely of fine volcanic dust derived from the explosion of

felsitic or orthophyric lavas. Some portions indeed are not improbably

composed of decayed felsites, like those which present so many

difficulties to the geologist who would try to trace their course among

the other lavas and tuffs of the Pentland chain. Various veins, dykes

and small bosses of felsite, andesite and even more basic material,

such as fine dolerite, have been intruded into the general body of the

mass.

On the outskirts of the main vent some subordinate necks may be

observed (3, 3 in Fig. 90), perhaps, like Torduff Hill, already

noticed (Fig. 86), marking lateral eruptions from the flanks of the

great cone. Three of these occur in a line more than half a mile long,

possibly indicating a fissure on the side of the old volcano, running

in a south-westerly direction from the southern edge of the vent. The

smallest of them measures about 500 feet in diameter; the largest is

oblong in shape, its shorter diameter being about 500 feet, and its

longer about 1000 feet. The materials that fill these lateral vents are

coarse agglomerates, traversed by veins and irregular intrusions of a

fine horny or flinty felsite.

From the acid character of most of the rocks that now fill the wide

vent of the Braid Hills it may be inferred that at least the last

eruptions from it consisted chiefly of acid tuffs and lavas. The upper

portion of the volcanic series being everywhere concealed, there are no

means left to verify this inference from an examination of the ejected

material. It may be remarked, however, that the pale yellow sandstones

which lie on the east side of the fault and are exposed in the Lyne

Water above West Linton are in great measure composed of fine felsitic

material.[365] They certainly belong to a higher horizon than the most

southerly lavas of the Pentland Hills, and if they have not derived

their volcanic detritus from the Biggar volcanic area, it may be

assumed that they obtained it from the vent of the Braid Hills. In any

case they show that after the lavas of the southern end of the Pentland

Hills were buried, acid volcanic detritus continued to be abundantly

distributed over this part of the floor of Lake Caledonia.

[Footnote 365: Explanation to Sheet 24 of the Geological Survey of

Scotland, pp. 10, 12.]

6. _The Biggar Centre_[366]

[Footnote 366: This area is included in Sheets 23 and 24 of the

Geological Survey of Scotland. It was mapped and described by myself.

(Explanations of Sheets 23 and 24.) Various parts of it have been

referred to by earlier writers, particularly Maclaren, _Geology of

Fife_, etc., p. 176.]

Another distinct group of volcanoes had its centre about 25 miles

south-westward from the Braid vent, and on the same line as those of

the Pentland Hills. In no part of the basin can the isolation of the

different volcanic clusters be so impressively observed as in the

area to the south-west of these hills. On the one hand, the lavas and

tuffs from the Braid vent die out, and on the other, as we follow the

conglomerates south-westwards, a new volcanic series immediately makes

its appearance.

The space between the last extremity of the Pentland lavas and the

beginning of the Biggar series does not exceed some 500 yards. It will

be remembered that the lower half of the Pentland volcanic series dies

out long before it reaches the southern end of the hills, and that it

is by lavas on the horizon of some of the dark andesites of Allermuir

Hill that the volcanic band is finally prolonged to its extreme

southern limit. The most northerly extension of the Biggar lavas lies

somewhere on the same general platform. But whereas, at the north

end of the Pentland chain, the volcanic sheets rest on the edges of

the Upper Silurian shales, at the south end, several hundred feet of

coarse conglomerate and sandstone intervene between the Silurian shales

and the porphyrites. So rapidly does the bulk of these sedimentary

formations increase that in the course of two miles they must be 3000

feet in thickness below the most northerly of the Biggar lavas just

referred to. But after that point, when they cross the Lyne Water,

they begin to be more and more interstratified with thin sheets of

andesite. These lavas, the beginning of the Biggar series, soon number

nine or ten distinct bands, and so quickly do they usurp the place of

the sedimentary materials that in a distance of not more than twelve

miles they form, where traversed by the river Clyde, the whole breadth

of the visible tract of Old Red Sandstone, to the exclusion of the

conglomerates.

Unfortunately, soon after the lavas make their appearance at the

north end they are in great measure overlapped unconformably by the

red sandstones at the base of the Carboniferous system, but where the

Medwin Water has cut through this covering, they can be seen here and

there underneath on their southerly course.

A section through the northern end of the Biggar series, where the

successive lavas are dying out northwards among the conglomerates,

shows the structure given in Fig. 91. The sedimentary strata consist

largely of debris of andesite, and the lavas include dark red or purple

andesites and also pale felsites, both having the same characters as

those of the Pentland Hills.

[Illustration: Fig. 91.--Section across the northern end of the Biggar

volcanic group, from Fadden Hill to beyond Mendick Hill.

1. Conglomerates and sandstones; 2. Lavas, the lowest being an

olivine-diabase or basalt, the main mass being andesites; 3. Felsites

and tuffs; 4. Upper Old Red Sandstone. _f_, Fault.]

In one important respect the volcanic series in the northern part of

the Biggar area differs from that of the Pentland Hills, for whereas

the uppermost parts of the latter are concealed by faults which bring

down the Carboniferous strata against the base of the hills, the lavas

at the north end of the Biggar district pass conformably under a thick

group of Lower Old Red conglomerates and sandstones. We thus learn

that here the volcanic eruptions ceased long before the close of the

deposition of the Lower Old Red Sandstone. The overlying sedimentary

series is disposed in a long synclinal trough, corresponding in

direction with the general north-easterly strike of the volcanic rocks

which reappear from under the sandstones and conglomerates along its

south-eastern border, where they are abruptly truncated by the fault

(_f_, Fig. 92), which brings them against the flanks of the Silurian

Uplands. It is interesting to note that by this dislocation the lavas

of the Lower Old Red Sandstone are placed almost in immediate contact

with those of the Lower Silurian series, which appear here on the

crests of numerous anticlinal folds that are obliquely cut off by the

fault.

There is yet another feature of interest in the northern part of

the Biggar volcanic centre. While the lowest visible lava is an

olivine-diabase not unlike parts of the Warklaw group of the Pentland

Hills, those which occur above it are partly andesites and partly

orthoclase-felsites. The latter form, among the hills near Dolphinton,

an important group which reaches its greatest development in the Black

Mount (1689 feet). These rocks cover a breadth of more than a mile of

ground, and probably attain a thickness of not less than 2000 feet.

They so closely resemble in their general characters the corresponding

rocks of the Pentland Hills that a brief description of them may

suffice. As in that chain of hills, they are so prone to decomposition

that they are in large part concealed under a covering of their own

debris and of herbage, though their fragments form abundant screes, and

numerous projecting knobs of rock suffice to show the main features of

the lavas and their accompaniments.

The felsites weather into pale yellow and greyish "claystones," but

where fresher sections can be procured they often show darker tints of

lilac and purple. They are close-grained, sometimes flinty, generally

porphyritic with scattered highly-kaolinized white felspars, but

without quartz, often presenting beautiful flow-structure, and not

infrequently showing a brecciated appearance, which in the usual

weathered blocks is hardly to be distinguished from the breccia of

interstratified tuffs.

A locality where some of these features may be satisfactorily examined

is a dry ravine in the farm of Bank, on the south-east side of the

Black Mount. Here the felsite possesses such a perfectly developed

flow-structure as to split into slabs which, dipping S.E. at about 25°,

might deceive the observer into the belief that it is a sedimentary

rock. A fresh fracture shows the laminæ of flow, many of which are

as thin as sheets of paper, to be lilac in colour, some of the more

decomposed layers assuming tints of grey. The felspars and micas are

arranged with their long axes parallel to the lines of flow. The rock

is not vesicular, but it breaks up here and there into the brecciated

condition just referred to. Below the sheet which displays the most

perfect flow-structure, what is probably a true volcanic breccia makes

its appearance. It consists of angular fragments of a similar lilac

felsite, of all sizes up to pieces two or three inches in length,

cemented in a matrix of the same material stained reddish-brown. In

this breccia the stones show little or no flow-structure.

Above the group of felsites and felsitic breccias, grey andesites make

their appearance, like some of those in the Pentland Hills. They are

sometimes extraordinarily vesicular, the vesicles in the body of the

rock being filled with calcite, agate, etc. Such lavas must have been

originally sheets of rough slag. The elongated steam-vesicles have been

partly filled up with micaceous sand and fine red mud that were washed

into crannies of the lava in direct communication with the overlying

water. It is evident that in the northern part of the Biggar centre the

succession of volcanic events followed closely the order observable in

the Pentland Hills, but on a feebler scale. We may suppose that the

lower diabases and andesites are the equivalents of those of Warklaw

and Allermuir, that the felsites and breccias were contemporaneous

with those of Capelaw, Caerketton and Castlelaw, and that the last

andesites made their appearance together with those which form the

highest lavas of the Pentland chain.

[Illustration: Fig. 92.--Section across the southern part of the Biggar

volcanic group from Covington to Culter.

1. Lower Silurian strata; 2. Lower Old Red Sandstone (pre-volcanic

group); 3. Andesite lavas with intercalated sandstones and

conglomerates; 4. Felsite neck. _f_, The boundary-fault on northern

edge of Southern Uplands.]

A section across the southern end of the Biggar volcanic belt shows

less diversity of structure (Fig. 92). The lavas (3) are there found

to flatten out and to spread unconformably over the older part of the

Lower Old Red Sandstone (2), which, as already stated, passes down

into the Upper Silurian shales. A few intercalations of conglomerate,

mainly made up of volcanic detritus, are here and there to be detected

among these lavas. But the chocolate sandstones and conglomerates that

lie unconformably below them contain no such detritus, for they belong

to the pre-volcanic part of the history of Lake Caledonia, and were

here locally upraised, perhaps as an accompaniment of the terrestrial

disturbances that preceded or attended the first outburst of volcanic

energy. Followed south-westwards, the stratigraphical break in the

Lower Old Red Sandstone disappears, and, as will be shown in the

account of the Duneaton centre, a continuous succession can there be

traced from the Upper Silurian shales up into the volcanic series.

An interesting feature in this district is the felsitic boss of

Quothquan already alluded to (p. 288) as rising up through the

andesites, and possibly marking one of the vents of the district. It is

one of a number of felsitic intrusions in this neighbourhood, of which

the most important is Tinto.

[Illustration: Fig. 93.--Section from Thankerton Moor across Tinto to

Lamington.

1_a_. Lower Silurian; 1. Upper Silurian strata; 2. Lower Old Red

Sandstone with two marked bands of conglomerate; 3. Lower Old

Sandstone (pre-volcanic chocolate sandstones); 4. Andesite lavas

with sandstones, conglomerates and tuffs lying unconformably

on No. 3; 5. Felsite sill of Tinto with the smaller sill of

the Pap Craig (6). _f_, Fault bounding the Silurian uplands on

the north. A small patch of the unconformable Lower Old Red

conglomerate is seen on the south side of the fault.

]

A third section taken across Tinto, from Thankerton Moor on the north

side to Lamington on the south, will serve further to illustrate the

great unconformability in the Lower Old Red Sandstone of this district,

and to show the relation of the largest felsitic intrusion to the

surrounding rocks (Fig. 93). The conglomerates and sandstones that

appear on the south slopes of Tinto lie near the base of the Old Red

Sandstone, and if we could bore among the overlying andesites we should

probably meet with the Upper Silurian shales among or conformably

beneath the red passage-beds, as in the Lesmahagow district.

The andesitic lavas creep over the upturned denuded edges of these

strata and sweep round the flanks of Tinto. This conspicuous hill

reaches a height of 2335 feet above the sea, and consists of the

felsitic rocks already described (p. 278). Seen from many points of

view it rises as a graceful cone, distinguished from all the other

eminences around it by the pinkish colour of its screes. In reality it

forms a continuous ridge which runs in an east and west direction for

about five and a half miles, with a breadth of about a mile. Some part

at least, and possibly the whole of this oblong mass, is in the form

of a sill or laccolite which dips towards the north. Conglomerates and

sandstones plunge under it on the southern side, and similar sandstones

overlie it on the north. If there be a neck in this mass, as one might

infer from the shape of the hill, its precise limits are concealed. The

rock does not break through the andesites, and may belong to an earlier

period of eruptivity than the lavas immediately around it. There were

other, though smaller, vents in the immediate neighbourhood. Besides

the cone of Quothquan just referred to, another may be marked by the

felsite boss which overlooks the village of Douglas, four miles to the

south-west of the Tinto ridge, while a third rises into a low rounded

hill close to the village of Symington.

The lavas spread out again to the south-west of Tinto in a group of

hills, until they are interrupted by a fault which brings in the

Douglas coal-field.[367] This dislocation abruptly terminates the

Biggar volcanic band in a south-westerly direction, after extending for

a length of 26 miles, with a breadth of sometimes as much as five miles.

[Footnote 367: See Explanation to Sheet 23 of the Geological Survey of

Scotland (1873), p. 15. This ground was mapped and described by Mr. B.

N. Peach.]

7. _The Duneaton Centre_

Among the high bleak muirlands on the confines of the three counties of

Lanark, Ayr and Dumfries, traversed by the Duneaton Water, a distinct

volcanic area may be traced.[368] Its boundaries, however, cannot be

satisfactorily fixed. It is overspread with Carboniferous rocks both

to the north-east and south-west, so that its rocks are only visible

along a strip about seven miles long and two miles broad. On the

north-western side its lower members are seen lying interstratified

among the sandstones and conglomerates which thence pass down

conformably into the Upper Silurian series (Fig. 94). But although we

thus get below the volcanic series we meet with no vents or sills among

the lower rocks. On the south-east side the highest lavas and tuffs are

overlain by some 5000 feet of red sandstones and conglomerates (2, 3),

which completely bury all traces of the volcanic history.

[Footnote 368: This area was mapped by Mr. B. N. Peach in Sheet 15

of the Geological Survey of Scotland, and is described by him in the

accompanying Memoir.]

The volcanic series in this limited district reaches an estimated

thickness of 4000 feet, built up of purple and green slaggy

andesites, dark heavy diabases (melaphyres) and tuffs, with abundant

interstratification of sandstone, especially towards the base. One of

its chief features of interest is the manner in which it exhibits,

better, perhaps, than can be found in any of the other volcanic areas,

the frequent and rapid alternations of lavas and tuffs with sandstone

and conglomerate. In this part of the region the volcanic discharges

were obviously frequent and intermittent, while at the same time the

transport and deposition of sediment were continuous. This sediment

consisted largely, indeed, of volcanic detritus mixed with ordinary

sand and silt. That these conditions of sedimentation were not wholly

inimical to animal life is shown by the occasional occurrence of

worm-burrows in the ashy sandstones.[369]

[Footnote 369: Memoir on Sheet 15 Geol. Surv. Scotland (1871), p. 22.]

[Illustration: Fig. 94.--Section across the Duneaton volcanic district

from the head of the Duneaton Water to Kirklea Hill.

1. Silurian strata; 2. Lower Old Red Sandstone and conglomerate; 3.

Coarse conglomerate; 4. Andesite-lavas; 5. Stratified tuffs; 6. Spango

granite; 7. Upper Old Red Sandstone.]

The thick accumulation of sandstones and conglomerates above the main

mass of lavas has been derived almost wholly from the waste of the

volcanic rocks (3). Blocks of andesite, well rounded and often from

six to twelve inches in diameter, may be seen in the remarkable band

of coarse conglomerate which runs as a nearly continuous ridge from

the Nith to the Clyde--a distance of more than twenty miles. Nothing

impresses the geologist more, as he wanders over this district,

than the evidence of the prodigious waste which the volcanic series

underwent before it was finally buried. Some part of the detritus may

have been supplied, indeed, by occasional discharges of fragmental

matter, as has already been suggested in the case of the Ochil and

Montrose conglomerates. But the nature of the pebbles in these masses

of ancient shingle shows them to be not bombs, but pieces worn away

from sheets of lava.

That the lavas underlie these piles of detritus and extend southwards

even up to the very edge of the Silurian Uplands is shown by the

rise of a number of successive beds from under the trough into which

the conglomerate has been thrown. These lavas, however, are almost

immediately cut off by the great boundary fault (_f_) which flanks the

Silurian territory. That they are not met with now to the south-east

of the dislocation, where they must once have lain, is an evidence of

the great denudation which the district has undergone. Fig. 94, which

gives a section across the broadest part of the area, from the edge

of the Muirkirk coal-field to the Silurian uplands, shows the general

structure of the ground.

No satisfactory evidence regarding the position of any of the vents of

the period has been met with in this district. The rocks to the south

of the boundary-fault are older than the Old Red Sandstone, and as

they must have been for some distance overspread by the conglomerates,

sandstones and volcanic series, we might hope to find somewhere among

them traces of necks or bosses. The only mass of eruptive rock in that

part of the district is the tract of Spango granite which has been

already referred to in connection with the subject of the vents and

granite protrusions of Old Red Sandstone time. This mass, about four

miles long and two miles broad, rises through Silurian strata, and

by means of the boundary fault is brought against the higher group

of conglomerates and sandstones. The Silurian shales and sandstones

around the granite have undergone contact-metamorphism, becoming highly

micaceous and schistose. The ascent of this granite must have taken

place between the upheaval and contortion of the Upper Silurian strata,

and the deposition of the higher parts of the Lower Old Red Sandstone

of this region. Its date might thus come within the limits of the

volcanic period. But one must frankly own that there is no positive

evidence to connect its production with the volcanic history.

8. _The Ayrshire Group of Vents_

The original limits of the volcanic districts in the remaining portion

of the Old Red Sandstone area on the mainland of Scotland, from

the valley of the Nith to the Firth of Clyde, can only be vaguely

indicated.[370] There is a difficulty in ascertaining the south-western

termination of the Duneaton area, and in deciding whether the lavas and

tuffs of Corsincone in Nithsdale should be assigned to that district or

be placed with those further to the south-west. Between Corsincone and

the next visible volcanic rocks of the Lower Old Red Sandstone there

intervenes a space of six miles, along which, owing to the effect of

the great fault that flanks the north-western margin of the Southern

Uplands, the Carboniferous Limestone and even the Coal-measures are

brought against the Silurian formations, every intermediate series of

rocks being there cut out. It may therefore be, on the whole, better to

include all the volcanic rocks on the left side of the Nith as part of

the Duneaton series. There will still remain a tract of five miles of

blank intermediate ground before we enter upon the volcanic rocks of

Ayrshire.

[Footnote 370: The mapping of the Old Red Sandstone volcanic areas of

Ayrshire for the Geological Survey was thus distributed:--The district

east of Dalmellington was surveyed by Mr. B. N. Peach, that between

Dalmellington and Straiton by Prof. James Geikie, and all from the line

of the Girvan Valley south of Straiton westward to the sea by myself.

The ground is embraced in Sheets 8, 13 and 14 of the Map of Scotland,

and is described in accompanying Explanations.]

Owing to complicated faults, extensive unconformable overlaps of

the Carboniferous formations, and enormous denudation, the volcanic

tracts of Old Red Sandstone age in Ayrshire have been reduced to mere

scattered patches, the true relations of which are not always easily

discoverable. One of these isolated areas flanks the Silurian Uplands

as a belt from a mile to a mile and a half in breadth and about six

miles long, but with its limits everywhere defined by faults. A second

much more diversified district extends for about ten miles to the

south-west of Dalmellington. It too forms a belt, averaging about four

miles in breadth, but presenting a singularly complicated geological

structure. Owing to faults, curvatures and denudation, the volcanic

rocks have there been isolated into a number of detached portions,

between some of which the older parts of the Old Red Sandstone, and

even the Silurian rocks, have been laid bare, while between others the

ground is overspread with Carboniferous strata. A third unbroken area

forms the Brown Carrick Hills, south of the town of Ayr, and is of

special interest from the fact that its rocks have been exposed along

a range of sea-cliffs and of beach-sections for a distance of nearly

four miles. Other detached tracts of volcanic rocks are displayed on

the shore at Turnberry and Port Garrick, on the hills between Mochrum

and the vale of the Girvan, and on the low ground between Dalrymple and

Kirkmichael.

The isolation of these various outliers and separated districts is

probably not entirely due to the effects of subsequent geological

revolutions. More probably some of the areas were always independent

of each other, and their igneous rocks were discharged from distinct

volcanic centres. We may conjecture that one of these centres lay

somewhere in the neighbourhood of New Cumnock, for the lavas between

that town and Dalmellington appear to diminish in thickness and number

as they are traced south-westward. Another vent, or more probably a

group of vents, may have stood on the site of the present hills to the

right and left of the Girvan Valley, south of the village of Straiton.

A third probably rose somewhere between Dailly and Crosshill, and

poured out the lavas of the ridges between Maybole and the Dailly

coal-field. The important centre of eruption that produced the thick

and extensive lavas of the Brown Carrick Hills may be concealed under

these hills, or may have stood somewhere to the west of Maybole. Still

another vent, perhaps now under the sea, appears to be indicated by the

porphyrites of the coast-section between Turnberry and Culzean Bay.

Owing to the complicated structure of the ground, several important

points in the history of the Old Red Sandstone of this region have not

been established beyond dispute. In particular, the unconformability

which undoubtedly exists in that system in the south-west of Ayrshire

has not been traced far enough eastwards to determine whether it

affects the volcanic belt east of Dalmellington, or whether the

break took place before or after the eruption of that belt. West of

Dalmellington it clearly separates a higher group of sandstones,

conglomerates and volcanic rocks from everything older than themselves.

The structure is similar to that in the Pentland Hills, a marked

disturbance having taken place here as well as there after a

considerable portion of the Lower Old Red Sandstone had been deposited.

These earlier strata were upraised, and on their denuded ends another

group of sandstones and conglomerates was laid down, followed by an

extensive eruption of volcanic materials.

It is the upper unconformable series that requires to be considered

here, as it includes all the volcanic rocks of the Old Red Sandstone

lying to the west of the meridian of Dalmellington. The position of

these rocks on their underlying conglomerates is admirably exposed

among the hills between the valleys of the Doon and the Girvan, as well

as on Bennan Hill to the south of Straiton. The andesites rise in a

craggy escarpment crowning long green slopes that more or less conceal

the conglomerates and sandstones below.

Along the coast-sections the structure of the volcanic rocks may be

most advantageously studied. The shore from the Heads of Ayr to Culzean

Castle affords a fine series of exposures, where every feature in

the succession of the lavas may be observed. Still more instructive,

perhaps, is the mile and a half of beach between Turnberry Bay and

Douglaston, of which I shall here give a condensed account, for

comparison with the coast-sections of Kincardineshire and Forfarshire

already described.

The special feature of this part of the Ayrshire coast-line is the

number of distinct andesite sheets which can be discriminated by means

of the thin layers of sandstone and sandy tuff that intervene between

them. In the short space of a mile and a half somewhere about thirty

sheets can be recognized, each marking a separate outflow of lava.

It was in this section that I first observed the sandstone-veinings

which have been described in previous pages, and nowhere are they more

clearly developed. Almost every successive stream of andesite has been

more or less fissured in cooling, and its rents and irregular cavernous

hollows have been filled with fine sand silted in from above. The

connection may often be observed between these sandstone partitions or

patches and the bed of the same material, which overspread the surface

of the lava at the time that the fissures were being filled up.

[Illustration: Fig. 95.--Cavernous spaces in andesite, filled in with

sandstone, John o' Groat's Port, Turnberry, Ayrshire.]

The andesites of the Turnberry shore are of the usual dark purplish-red

to green colours, more or less compact in the centre and vesicular

towards the top and bottom. They display with great clearness the large

empty spaces that were apt to be formed in such viscous slaggy lavas as

they moved along the lake-bottom. These spaces, afterwards filled with

fine sand, now appear as irregular enclosures of hard green sandstone

embedded in the andesite. The example shown in Fig. 95 may be seen in

one of the lavas at John o' Groat's Port.

[Illustration: Fig. 96.--Section of andesites, Turnberry Castle,

Ayrshire.]

From the arrangement of the veins of sandstone it is evident that

irregularly divergent, but often more or less stellate, fissures opened

in the lavas as they cooled. Sometimes, indeed, the molten rock appears

to have broken up into a shattered mass of fragments, as must often

have happened when lavas were poured over the lake-floor. What may be

an instance of this effect is to be seen on the cliff under the walls

of Turnberry Castle, whence the annexed sketch (Fig. 96) was taken. The

lower andesite (_a_) is highly amygdaloidal towards the top, and is

traversed in all directions with irregular veins and nests of sandstone

which can be traced upward to the bed (_b_), consisting of sandstone,

but so full of lumps or slags of amygdaloidal andesite that one is here

and there puzzled whether to regard it as a sedimentary deposit, or as

the upper layer of clinkers of a lava-stream strewn with sand. Above

this fragmentary layer lies another bed of andesite (_c_) of a coarsely

amygdaloidal structure, which encloses patches of the underlying

sandstone. It passes upward, in a space of from four to six feet, into

a mass of angular scoriaceous fragments (_d_) of all sizes up to blocks

18 inches in length cemented in a vein-stuff of calcite, chalcedony and

quartz. This brecciated structure ascends for about 13 or 14 feet, and

is then succeeded by a greenish compact andesite (_e_), which further

north becomes amygdaloidal and much veined with sandstone, passing into

a breccia of lava fragments and sandstone.

[Illustration: Fig. 97.--Lenticular form of a brecciated andesite

(shown in Fig. 96), Turnberry, Ayrshire.]

[Illustration: Map III.]

MAP OF THE VOLCANIC DISTRICTS OF THE LOWER OLD RED SANDSTONE

OF "LAKE CALEDONIA" IN CENTRAL SCOTLAND & NORTH EAST IRELAND

The remarkable brecciated band (_d_) in this cliff, though 13 or 14 feet

in the centre, immediately thins out on either side, until in the

course of a few yards it completely disappears and allows the lavas

_c_ and _e_ to come together, as shown in Fig. 97. We may suppose that

this section reveals the structure of the terminal portion of a highly

viscous lava which was shattered into fragments as it moved along under

water.

No clear evidence of the sites of any of the volcanic vents has yet

been detected in the Old Red Sandstone of Ayrshire. Possibly some

of the numerous felsitic bosses to the south-west of Dalmellington

may partly mark their positions. But the sills connected with the

volcanic series are well exposed in the 12 miles of hilly ground

between Dalmellington and Barr. Two groups of intrusive sheets may

there be seen. The most numerous consist of pale or dark-pink felsite,

often full of crystals of mica. They form prominent hills, such as

Turgeny, Knockskae and Garleffin Fell. The second group comprises

various diabase-sheets which have been intruded near the base of the

red sandstones and conglomerates, over a distance of seven miles on

the north side of the Stinchar Valley above Barr. They attain their

greatest development on Jedburgh Hill, where they form a series of

successive sills, the largest of which unite northwards into one thick

mass and die out southward among the sandstones and conglomerates.

The Ancient Volcanoes of Great Britain, Volume 1 (of 2) · 第 7 / 11 章