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
What now, dear reader, shall we make out of our telescope? Shall we
make a Mercury’s magic-wand to cross the liquid ether with, and, like
Lucian,[28] lead a colony to the uninhabited evening star, allured by
the sweetness of the place? or shall we make it a Cupid’s arrow, which,
entering by our eyes, has pierced our inmost mind, and fired us with
a love of Venus? For what language is too strong for the marvellous
beauty of this orb, if, having no light of its own, it can attain
simply by the borrowed light of the sun to such splendour, as Jupiter
has not, nor the moon, though enjoying a proximity to the sun as close
as Venus; for if the moon’s light be compared with the light of Venus,
it will be seen to be certainly greater on account of the apparent
magnitude of the moon, but, in comparison with the light of Venus,
dull, dead, and leaden. O truly golden Venus! Will any one doubt any
more that the whole orb of Venus is wrought most smoothly out of pure
unalloyed gold, since its surface, when only placed in the sunlight,
reflects a splendour so intense! And here let me add my experiments
about the alteration of the light of Venus on blinking the eye, which
I have examined in the part of my Astronomy which treats of Optics.
Reasoning will be able to conclude nothing else but this, that the orb
of Venus turns on its own axis with an exceedingly swift rotation,
displaying one after another different parts of its surface which are
more or less capable of retaining the sun’s light.[29]
[28] Lucian, _Ver. Hist._ i. 12.
[29] The first scientific determination of the period of the
rotation of Venus was made by Dominique Cassini in 1666, from
observations of spots on the planet, and concluded to be about 24
hours; but in 1726 Bianchini deduced a period of 24 d. 8 h. from
similar observations. The true period is considered to be 23 h. 21
m., determined by Schroeter by a series of observations lasting
from 1788 to 1793 on the periodicity of the deformation of the
horns of Venus.—(ARAGO, _Astronomie Populaire_, 1854.)
Kepler’s statements can only be regarded as anticipations of
phenomena not yet actually observed.
But enough of my own conclusions. Let us now hear as an epilogue
Galileo’s conclusions built up out of all the observations which he
has made with his telescope, and announced from time to time. Thus he
writes once more:—
[Sidenote: Galileo’s conclusions with regard to the inherent nature of
the brightness of the stars.]
“Illustrissimo e Reverendissimo Signore mio colendissimo.
Public-domain text, read in full here on John Shaqi.
Reviews
Reviews
No reviews yet
Be the first to share your thoughts on this work.
Elsewhere in the archive
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account