The sidereal messenger of Galileo Galilei : $b and a part of the preface to Kepler's Dioptrics containing the original account of Galileo's astronomical discoveries — John Shaqi
The sidereal messenger of Galileo Galilei : $b and a part of the preface to Kepler's Dioptrics containing the original account of Galileo's astronomical discoveriesGalilei, Galileo
History
The sidereal messenger of Galileo Galilei : $b and a part of the preface to Kepler's Dioptrics containing the original account of Galileo's astronomical discoveries
Galilei, Galileo
Astronomy -- Early works to 1800; Jupiter (Planet) -- Satellites
Again, to assert that this sort of light is imparted to the Moon by the
planet Venus is so childish as to be undeserving of an answer; for who
is so ignorant as not to understand that at conjunction and within an
angular distance of 60° it is quite impossible for the part of the Moon
turned away from the Sun to be seen by the planet Venus?
But that this light is derived from the Sun penetrating with its light
the solid mass of the Moon, and rendering it luminous, is equally
untenable. For then this light would never lessen, since the hemisphere
of the Moon is always illumined by the Sun, except at the moment of
a lunar eclipse, yet really it quickly decreases while the Moon is
drawing near to the end of her first quarter, and when she has passed
her first quarter it becomes quite dull. Since, therefore, this
kind of secondary brightness is not inherent and the Moon’s own, nor
borrowed from any of the stars, nor from the Sun, and since there now
remains in the whole universe no other body whatever except the Earth,
what, pray, must we conclude? What must we assert? Shall we assert that
the body of the Moon, or some other dark and sunless orb, receives
light from the Earth? Why should it not be the Moon? And most certainly
it is. The Earth, with fair and grateful exchange, pays back to the
Moon an illumination like that which it receives from the Moon nearly
the whole time during the darkest gloom of night. Let me explain the
matter more clearly. At conjunction, when the Moon occupies a position
between the Sun and the Earth, the Moon is illuminated by the Sun’s
rays on her half towards the Sun which is turned away from the Earth,
and the other half, with which she regards the Earth, is covered with
darkness, and so in no degree illumines the Earth’s surface. When the
Moon has slightly separated from the Sun, straightway she is partly
illumined on the half directed towards us; she turns towards us a
slender silvery crescent, and slightly illumines the Earth; the Sun’s
illumination increases upon the Moon as she approaches her first
quarter, and the reflexion of that light increases on the Earth; the
brightness in the Moon next extends beyond the semicircle, and our
nights grow brighter; at length the entire face of the Moon looking
towards the Earth is irradiated with the most intense brightness by
the Sun, which happens when the Sun and Moon are on opposite sides of
the Earth; then far and wide the surface of the Earth shines with the
flood of moonlight; after this the Moon, now waning, sends out less
powerful beams, and the Earth is illumined less powerfully; at length
the Moon draws near her first position of conjunction with the Sun, and
forthwith black night invades the Earth. In such a cycle the moonlight
gives us each month alternations of brighter and fainter illumination.
But the benefit of her light to the Earth is balanced and repaid by the
benefit of the light of the Earth to her; for while the Moon is found
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