Saturday, 14 March 2026

Measuring the Earth

Proposition 2: The surface of any fluid at rest is the surface of a sphere whose centre is the same as that of the earth.
— Archimedes (287 – 212 BCE), demonstrating that the Greeks knew the world’s shape.

It so happens that the earth and the universe have the same centre, for the heavy bodies do move also towards the centre of the earth, yet only incidentally, because it has its centre at the centre of the universe. As evidence that they move also towards the centre of the earth, we see that weights moving towards the earth do not move in parallel lines but always at the same angles to it: therefore they are moving towards the same centre, namely that of the earth. It is now clear that the earth must be at the centre and immobile … From these conclusions it is clear that the earth does not move …
— Aristotle (384 – 322 BCE), showing how you can reach a wrong conclusion from the right facts.

But this is not found to be the case; and therefore the alleged cause is not the true one. Let us then examine into the natural cause. The surface of every liquid body, when at rest, is spherical and concentric with that of the earth; and, if the liquid be not at rest, it moves until it attains such a surface. If then we take two vessels and pour water into each, and, after filling the siphon and closing its extremities with the fingers, insert one leg into one vessel plunging it beneath the water, and the other into the other, all the water will be continuous, for each of the liquids in the vessels communicates with that in the siphon … as soon as the water is continuous it must inevitably flow into the lower vessel through the channel of communication, until either all the water in both vessels stands at the same height, or one of the vessels is emptied.
— Hero of Alexandria (1st century CE), on the siphon.

If the extent of the Atlantic Ocean were not an obstacle, we might easily pass by sea from Iberia to India, keeping in the same parallel.
— Eratosthenes (c. 275 – 194 BCE).

These men made a statement which I myself do not believe, though others may, to the effect that as they sailed on a westerly course round the southern end of Libya [Africa], they had the sun on their right — to the northward of them. This is how Libya was first discovered to be surrounded by sea …
— Herodotus (c. 480 BCE – 425 BCE), The Histories, Book 4, Penguin Classics, 284.

To be sure, the great majority of writers agree that the earth is at rest in the centre of the universe, so that they consider it unbelievable and even ridiculous to suppose to the contrary. Yet, when one weighs the matter carefully, he will see that this question is not yet disposed of, and for that reason is by no means to be considered unimportant. Every change of position which is observed is due either to the motion of the observer, or of the observed object, or to motions in different directions of both …Now the earth is the place from which we observe the revolution of the heavens and where it is displayed to our eyes. Therefore, if the earth should possess any motion, [it] would be noticeable in everything that is situated outside of it, but in the opposite direction, just as if everything were travelling past the earth. And of this nature is, above all, the daily revolution. For this motion seems to embrace the whole world, in fact, everything that is outside the earth, with the single exception of the earth itself … This opinion was actually held by the Pythagoreans Heracleides and Ekphantus and the Syracusean Nicetas (as told by Cicero) in that they assumed the earth to be rotating in the centre of the universe …

If therefore, one should maintain that the earth is not in the centre of the universe, but that the difference between the two is not great enough to be measurable on the sphere of the fixed stars, but on the other hand noticeable and recognisable on the orbits of the sun and the planets; and if further he were of the opinion that the motions of the latter for this reason appear irregular, just as if they [revolved around] another centre than that of the earth such a person might, perhaps, have assigned the true reason for such apparently irregular motions. For since the planets appear now nearer, now more distant from the earth, this betrays necessarily that the earth is not at the centre of these circular orbits.
— Nicolas Copernicus (1473 – 1543), de Revolutionibus Orbium Caelestium.

This world is more wonderful than convenient
— Henry David Thoreau (1817 – 1862), Commencement oration, Harvard, 1837.

Can anyone be so foolish as to believe that there are men whose feet are higher than their heads, or places where things may be hanging downwards, trees growing backwards, or rain falling upwards? Where is the marvel of the hanging gardens of Babylon if we are to allow of a hanging world of the Antipodes?
— Lucius Caelius Firmianus Lactantius (4th century), quoted by Daniel Boorstin, The Discoverers.

‘Belief in Antipodes’ became another stock charge against heretics prepared for burning. Some few compromising spirits tried to accept a spherical earth for geographic reasons, while still denying the existence of Antipodean inhabitants for theological reasons. But their numbers did not multiply.
— Daniel Boorstin, The Discoverers, Dent, 1984, 108.

The apparatus is very simple; it consists of a wooden arm, 6 feet long, made so as to unite great strength with little weight [it was a truss structure]. This arm is suspended in an horizontal position, by a slender wire 40 inches long, and to each extremity is hung a leaden ball, about 2 inches in diameter; and the whole is inclosed in a narrow wooden case, to defend it from the wind.

As no more force is required to make this arm turn round on its centre than what is necessary to twist the suspending wire, it is plain, that if the wire is sufficiently slender, the most minute force, such as the attraction of a leaden weight a few inches in diameter, will be sufficient to draw the arm sensibly aside. The weights which Mr. Michell intended to use were 8 inches in diameter. One of these was to be placed on one side of the case, opposite to one of the balls, and as near as it could conveniently be done, and the other on the other side, opposite to the other ball, so that the attraction of both these weights would conspire in drawing the arm aside; and, when its position, as affected by the weights, was ascertained, the weights were to be removed to the other side of the case, so as to draw the arm the contrary way, and the position of the arm was to be again determined; and, consequently, half the difference of these positions would show how much the arm was drawn aside by the attraction of the weights.

In order to determine from hence the density of the earth, it is necessary to ascertain what force is required to draw the arm aside through a given space. This Mr. Michell intended to do, by putting the arm in motion, and observing the time of its vibrations, from which it may easily be computed.
— Henry Cavendish (1731 – 1810), Scientific Papers, published 1921.

I have made here [in San Domingo] a simple pendulum of steel which I have made as invariant as possible. It has a bob of [12 kilograms], about [12 centimetres] in diameter and [3 centimetres] deep. To keep it swinging true, I have put on the rod a crossbar of iron to serve as an axis, at right-angles to the rod. The instrument is mounted on a tempered steel knife-edge on two steel springs. These two springs are mounted on a copper plate in which there is a hole for the rod. The plate rests on a stool [1.5 metres] high, and is levelled by three screws …
— Pierre Bouguer (1698 – 1758), letter from Bouguer to René de Réaumur in 1735.

We used the barometer that we set up to study the balance between the weight of the mercury and the air in all the accessible parts of the atmosphere. We saw how many feet we had to rise or descend to make the mercury change height by one line. It is then necessary to find the specific weight of air that balances other bodies. In this way, I have found by comparison with copper that on the top of Pichincha, there is a loss from unity of 1/11 000. Now it follows that the weight of my simple pendulum also loses 1/11 000 part of its weight. This loss produces a similar reduction in the restoring force, and naturally, I found the pendulum to be slow by 1/11 000. To correct this loss, it was necessary to adjust the pendulum’s length by 4/100 of a line …
— Pierre Bouguer (1698 – 1758), ‘Memoirs Sur le Pendule’, Memoire de Physique, IV, pp. B-33, B-34.

Since the discovery by Richer of the shortening of the pendulum near the Equator, several observers have reported results from different places and at different times. It would have been useless to repeat these measures if we could not improve on the accuracy of the first observers; but if the accuracy of a set of measures is to be judged, it seems to me necessary that the methods of operation should be described. I have never feared to present to the Académie the details of my experiments, showing the care taken, and the degree of accuracy; I still say that this is the minimum acceptable in the circumstances to let the reader do the same.
— Charles Marie de La Condamine (1701 – 1774), Memoires de l’Academie Royale des Sciences, 1735, reprinted in Memoires sur le Pendule, no date, 4.

In this country, night and day were of more even length than in either Greenland or Iceland: on the shortest day of the year, the sun was already up by 9 a.m., and did not set until after 3 p.m.
Grænlendinga Saga, chapter 3, Penguin Classics, 56.

‘My guide … Where is now the ice?
How standeth he in posture thus revers’d?
And how from eve to morn in space so brief
Hath the sun made his transit?’ He in few
Thus answering spake; ‘Thou deem’st thou art still
On th’ other side of the centre, where I grasp’d
Th’ abhorred worm, that boreth through the world.
This wast on th’ other side, so long as I
Descended; when I turn’d, thou didst o’erpass
That point, to which from ev’ry part is dragg’d
All heavy substance. Thou art now arriv’d
Under the hemisphere oppos’d to that,
Which the great continent doth overspread …
— Dante Alighieri (c. 1265 – 1321), The Divine Comedy: Hell, canto XXXIV, 95-108, translated by Henry Cary, 1814, and travelling down through a spherical earth.

It is now evident that this earth really moves though to us it seems stationary. In fact, it is only by reference to something fixed that we detect the movement of anything. How would a person know that a ship was in movement, if, from the ship in the middle of the river, the banks were invisible to him and he was ignorant of the fact that water flows? Therein we have the reason why every man, whether he be on the earth, in the sun or on another planet, always has the impression that all other things are in movement whilst he himself is in a sort of immovable centre; he will certainly always choose poles which will vary accordingly as his place of existence is the sun, the moon, Mars, etc.
— Nicolas Cusanus (Nicholas Krebs of Cusa) (1401 – 1464).


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