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
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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
But before you do so, I should like you to notice, by the way, what
Galileo says about the Pythagorean and Copernican system of the
universe. For he points to my _Mystery of the Universe_,[26] published
fourteen years ago, in which I took the dimensions of the Planetary
orbits according to the astronomy of Copernicus, who makes the sun
immovable in the centre, and the earth movable both round the sun and
upon its own axis; and I showed that the differences of their orbits
corresponded to the five regular Pythagorean figures, which had been
already distributed by their author among the elements of the world,
though the attempt was admirable rather than happy or legitimate, and
for which figures’ sake Euclid wrote the whole of his Geometry. Now,
in that _Mystery_ you may find a sort of combination of Astronomy
and Euclid’s Geometry, and through this combination a most thorough
completion and finishing of them both; and this was the reason why I
waited with intense longing to see what sort of an argument Galileo
would produce in favour of the Pythagorean system of the universe.
After this explanation, Galileo’s letter about this argument was as
follows:—
[26] Kepler, in his _Mystery of the Universe_, endeavoured to
connect the orbits of the planets with the five regular solids,
thus: If in a sphere (i.) a cube be inscribed, and in the cube
a sphere (ii.); and in that sphere a tetrahedron, and in the
tetrahedron a sphere (iii.); and in that sphere a dodecahedron,
and in the dodecahedron a sphere (iv.); and in that sphere an
icosahedron, and in the icosahedron a sphere (v.); and in that
sphere an octahedron, and in the octahedron a sphere (vi.),
the diameters of these six spheres will be proportional to the
diameters of the orbits of Saturn, Jupiter, Mars, the Earth, Venus,
and Mercury respectively; or, as Kepler expresses it, the common
centre of these spheres represents the position of the Sun, and the
six spheres represent the spheres of the planets.
By these considerations, however, Kepler was led to enunciate
his third law, that the squares of the periodic times of planets
are proportional to the cubes of their mean distances from the
sun.—KEPLER, _Prodromus Dissertationum Mathematicarum continens
Mysterium Cosmographicum, etc._ (Tübingen, 1596.)
“Illustrissimo e Reverendissimo Signore mio colendissimo.
Public-domain text, read in full here on John Shaqi.
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