Fig. I.]

54. The continual changing of the Moon’s phases or shapes demonstrates

that she shines not by any light of her own: for if she did, being

globular, we should always see her with a round full Orb like the Sun.

Her Orbit is represented in the Scheme by the little circle _m_, upon

the Earth’s Orbit ⊕: but it is drawn fifty times too large in proportion

to the Earth’s; and yet is almost too small to be seen in the Diagram.

[Sidenote: One half of her always enlightened.]

55. The Moon has scarce any difference of seasons; her Axis being almost

perpendicular to the Ecliptic. What is very singular, one half of her

has no darkness at all; the Earth constantly affording it a strong light

in the Sun’s absence; while the other half has a fortnight’s darkness

and a fortnight’s light by turns.

[Sidenote: Our Earth is her Moon.]

56. Our Earth is a Moon to the Moon, waxing and waneing regularly, but

appearing thirteen times as big, and affording her thirteen times as

much light, as she does to us. When she changes to us, the Earth appears

full to her; and when she is in her first quarter to us, the Earth is in

it’s third quarter to her; and _vice versâ_.

57. But from one half of the Moon, the Earth is never seen at all: from

the middle of the other half, it is always seen over head; turning round

almost thirty times as quick as the Moon does. From the line which

limits our view of the Moon, or all round what we call her edges, only

one half of the Earth’s side next her is seen; the other half being hid

below the Horizon. To her, the Earth seems to be the biggest Body in the

Universe; for it appears thirteen times as big as she does to us.

[Sidenote: A Proof of the Moon’s having no Atmosphere;]

58. The Moon has no such Atmosphere, or body of air surrounding her as

we have: for if she had, we could never see her edge so well defined as

it appears; but there would be a sort of a mist or haziness round her,

which would make the Stars look fainter, when they were seen through it.

But observation proves, that the Stars which disappear behind the Moon

retain their full lustre until they seem to touch her very edge, and

then vanish in a moment. This has been often observed by Astronomers,

but particularly by CASSINI[13] of the Star γ in the breast of Virgo,

which appears single and round to the bare eye; but through a refracting

Telescope of 16 feet appears to be two Stars so near together, that the

distance between them seems to be but equal to one of their apparent

diameters. The Moon was observed to pass over them on the 21st of

_April_ 1720, _N. S._ and as her dark edge drew near to them, it caused

no change in their colour or Situation. At 25 min. 14 sec. past 12 at

night, the most westerly of these Stars was hid by the dark edge of the

Moon; and in 30 seconds afterward, the most easterly Star was hid: each

of them disappearing behind the Moon in an instant, without any

preceding diminution of magnitude or brightness; which by no means could

have been the case if there were an Atmosphere round the Moon; for then,

one of the Stars falling obliquely into it before the other, ought by

refraction to have suffered some change in its colour, or in it’s

distance from the other Star which was not yet entered into the

Atmosphere. But no such alteration could be perceived though the

observation was performed with the utmost attention to that particular;

and was very proper to have made such a discovery. The faint light,

which has been seen all around the Moon, in total Eclipses of the Sun,

has been observed, during the time of darkness, to have it’s center

coincident with the center of the Sun; and is therefore much more likely

to arise from the Atmosphere of the Sun than from that of the Moon; for

if it were the latter, it’s center would have gone along with the

Moon’s.

[Sidenote: Nor Seas.

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