CHAPTER II

THE WISE MEN OF ALEXANDRIA

WHEN Alexander the Great overcame the Egyptians, he sailed

along the African coast past the mouths of the river Nile until he came

to a place which seemed to him suitable for building a great city. It

was a strip of land on the sea-shore with a great lake behind it and

an island in front. “Here,” said the mighty conqueror, “shall be my

capital city, to be called Alexandria after my name.” So he sent for

his great architect Dinocrates, and told him to plan the streets and

palaces of the new royal city. Thousands of slaves were soon set to

work. The streets were made straight and wide, and canals were dug to

join the lake to the open sea and to the Nile, so that great merchant

vessels would find shelter from the storms.

The island was joined to the city by a causeway a mile long, and a

lighthouse 400 feet high was built on the island. The lighthouse was

in the shape of a round tower. On the top of the tower a bright fire

was kept constantly burning, so that the smoke by day and the flame by

night should guide ships safely into the harbour. This tower was the

first lighthouse ever built, and is said to have cost a quarter of a

million pounds (£250,000).

Within fifty years of its foundation Alexandria became one of the

foremost centres of commerce. The second of the Egyptian kings founded

the famous Library of Alexandria, and thus secured for the city a place

in the front rank of learning, which it kept for six hundred years.

Many of the great works of Greek writers were saved from destruction

by being preserved in Alexandria. The third king compelled every

stranger who passed through Alexandria with a book in his possession to

leave a copy of it at the Library. He also built a Museum, which was an

institution closely resembling what we should now call a University.

It had dwelling-rooms for professors, it had lecture halls, and a

great dining-room. The University grew and flourished, and attracted

clever young men from all the shores of the Mediterranean Sea. One of

these students was Euclid, who wrote the books on Geometry. There were

also poets, critics, and historians. Many books from all nations were

translated into Greek, including the Old Testament, at which seventy

scribes are said to have worked.

It was an Alexandrian astronomer named Aristarchus, who about 270 B.C.

first determined the distance of the sun from the earth in comparison

with that of the moon. He knew that the moon was a round ball, and

that its various shapes or phases were produced by the sun shining

upon it at different angles. He carefully watched the growing sickle

of the moon from day to day, waiting for the time when the moon should

appear to be exactly a half-circle. When this is the case an imaginary

line drawn from the eye of the observer to the centre of the moon is

at right angles to a similar line drawn from the centre of the moon

to the sun, as shown in the picture (Fig. 6). At the instant when the

sun’s light was seen to be shining squarely on the moon, that is just

before sunset, Aristarchus pointed one leg of an instrument like a

pair of compasses to the moon, and the other leg to the sun. The angle

between the two directions was found to be not quite a right angle. It

measured, in fact, 87 degrees (Fig. 6), whereas a right angle contains

90 degrees.

[Illustration: Fig. 6.--Comparing the Distances of the Sun and Moon.]

Now, if a triangle be drawn like that in Fig. 6, in which the angle

at M is a right angle, and that at E is 87 degrees, this triangle

illustrates the results of the observations. The moon’s distance is

represented in the triangle by the line EM, and the sun’s distance by

SM. It does not matter how large or small the triangle is drawn; for,

if the lines are inclined at the proper angles, the line SM will always

be the same number of times longer than EM.

Aristarchus concluded from his observations that the sun was eighteen

or nineteen times farther away than the moon. In reality, it is about

four hundred times that distance, but considering that the ancients

had very imperfect instruments, and that it is almost impossible to

decide the exact instant when the moon is just half-full, it is not

remarkable that the result obtained was far too small. As the result

of other observations, Aristarchus found that 720 suns, placed edge to

edge, would just circle the sky, and this is very close to the truth.

Men of science honour him for his ingenious methods of measuring the

sun’s distance and size, and for his painstaking observations, though

the results were not perfect.

Another famous astronomer of Alexandria, who was also the custodian of

the Library, was the first to measure the size of the earth. He was in

the habit of sailing up the Nile, and found that the farther he sailed

the more new stars appeared in the south, while the northern stars

disappeared gradually. This fact convinced him that the earth, like the

moon, is a round globe, and he thought that if he could go very much

farther in the same direction towards the south, he would eventually

circle the earth, and arrive at Alexandria again from the north. But

to measure the circle of the earth it was not necessary to travel

all round it. It was sufficient to find the fraction of the circle

traversed by travelling a certain distance, and this could be done by

measuring how much higher the southern stars appeared in the sky after

travelling a certain distance. Since the stars are very much farther

away than the sun, the difference in their height could not be due to

the distance travelled, but only to the roundness of the earth.

The astronomer sailed from Alexandria as far as the Falls of Aswan, and

carefully measured the distance he had travelled, which he found to be

520 miles. He found that at midday the sun stood about 7 degrees higher

in the sky at Aswan than at Alexandria. This angle was just about

1-50th of a whole circle. The astronomer concluded that if he continued

to travel south for fifty times that distance he would travel round the

globe, and in doing so he would cover the distance of 26,000 miles. The

real circumference of the earth is 23,700 miles, so that the learned

Alexandrian was not far wrong. But he would have been even more correct

had he known that Aswan is not really due south of Alexandria, but a

little east of south. This made his line too long.

The name of this great astronomer was Eratosthenes. His end was a sad

one. He lost the sight of his eyes and his powers of observation.

He starved himself to death, saying that life without the means of

pursuing his studies was not worth living.

Another remarkable man who lived in those days at Alexandria was Heron.

He was employed at the Museum, lecturing on Mechanics, Optics, and

the principles of Surveying.

[Illustration: Fig. 7.--Heron’s Steam-Engine.]

He invented a number of contrivances and machines which were the wonder

of his age. The people of Babylon had invented clocks driven by water.

[Illustration: Fig. 8.--The Jumping Ball.]

Heron improved these by letting the water drop through a small hole

bored in a precious stone of great hardness, so that the water should

not be able to enlarge the hole and to make the clock run faster. The

water dropped into a vessel containing a little boat. The boat had a

mast which was graduated, so that as the water rose, one graduation

after another appeared above the edge of the vessel.

These graduations indicated the hours. He also made the boat turn a

wheel, which at each hour caused a number of balls to fall into a

silver goblet. The number of balls indicated the number of hours, so

that the clock struck the hour very much like our clocks of to-day.

Heron is famous for having invented a kind of steam-engine, consisting

of a hollow ball with two nozzles pointed in opposite direction (Fig.

7). The steam passed into the ball through the arms by which it was

suspended, and the steam hitting against the air outside caused the

ball to spin round. In another form of the apparatus (Fig. 8) a ball

was kept jumping up and down by the steam issuing from a vertical pipe.

Heron found that when a narrow tube is put into water, and the upper

end is stopped with the finger while still under water, then on lifting

the tube out of the water with the stopped end uppermost, the water

does not flow out at the open end below until the finger is removed.

He, therefore, constructed a vessel (Fig. 9) which became known as the

“Vestal’s Goblet”; it was filled by plunging it into water, stopping

the upper opening with the finger, and lifting it out. The water

escaped in a spray through the small holes below on removing the finger.

[Illustration: Fig. 9.--The Vestal’s Goblet.]

[Illustration: Fig. 10.--The Double Goblet.]

In another form of the instrument there were two compartments which

were filled in the same manner with wine and water respectively. It was

a custom among the Greeks to mix wine with water, and offer the same

mixture to the gods in the temples.

Heron also made a self-feeding wick for oil lamps, which were then in

common use. The oil was burnt in an open vessel (Fig. 11), and as it

burnt away the wick was consumed also, but Heron made the oil itself

turn up the wick. He made a plate of wood float on the oil; as the oil

burnt away the plate of wood gradually sank, and in doing so it moved a

cog wheel. The cog wheel in turning moved a straight rack, or toothed

bar of wood, at the end of which the wick was fastened. In this way

the wick was moved on as the oil was consumed, and the lamp was kept

steadily burning.

The most important instrument which Heron improved was the Surveyor’s

Level. Egypt depends for its fertility upon the floods of the Nile, as

there is very little rain in Egypt.

[Illustration: Fig. 11.--Heron’s Self-Feeding Wick for Lamps.]

From the oldest times the Egyptians had to see that they could

distribute the land after the flood in the same way as it was

distributed before, each man getting his own land back. This was found

to be very difficult, as many landmarks were destroyed by the flood.

The art of Surveying was practised at a very early date in Egypt, and

there is no doubt that the science of Geometry was born in Egypt,

as it was necessary in order to be able to determine the extent and

boundaries of land.

[Illustration: Fig. 12.--Modern form of Heron’s Level.]

An important problem in connection with Surveying was to find when

two points are on the same level. This is done nowadays with a

spirit-level if the points are close together, or with an instrument

called a theodolite if the points are far apart. But a theodolite

requires a telescope, and the Alexandrians lived long before the

telescope was invented. Heron, however, got over the difficulty by

constructing a long box filled with water and provided with openings,

in the form of a cross, at each end. Above the crosses were glass tubes

communicating with each other, in which the water was kept at the same

level, and when that was the case the two crosses were exactly at the

same level, and any object seen through both crosses together was at

the same level as the crosses themselves. Heron probably used rods very

similar to the black and white rods used by surveyors at the present

day for measuring distances and levels.

Heron also invented a mechanical stone crusher, an organ driven by

water power, a counting machine to show the distance travelled by a

ship or a chariot, and an arrangement of mirrors which he called a

spy-glass.

Many of the works of Heron have been preserved to us. They are

written in Greek, which was the language used in Alexandria since its

foundation. Heron was always careful to make his reasoning quite clear

to his pupils, and he insisted that they must not believe anything

without proof.

“It is necessary,” he said, “that those who wish to become acquainted

with mechanical art should know what causes are at work in every

motion. It is important that nothing should be put before students

without proof, and that nothing should remain doubtful for them. In our

presentation every problem is to find a solution. We therefore recall

various principles taught by the ancients which are connected with our

subject.”

Wonders of physical science · 第 2 / 17 章