COSMOS, VOL. II - World eBook Library
COSMOS, VOL. II - World eBook Library COSMOS, VOL. II - World eBook Library
DISCOVERIES IN THE CELESTIAL SPACES. 705 tern," the perceptible evidence of the translatatory motion of the earth. Galileo had also early perceived (September 1612), the importance of the occupations of Jupiter's satellites for geographical determinations of longitude on land. He proposed this method, first to the Spanish court in 1616, and afterwards to the States General of Holland, with a view of its being applied to nautical purposes,* little aware, as it would appear, of the insuperable difficulties presented to its practical application on the unstable element. He wished to go himself, or to send his son Vicenzio, to Spain, with a hundred telescopes, which he would prepare. He required as a recompense " una croce di San Jago," and an annual payment of 4000 scudi, a small sum, he says, considering that hopes had been given to him, in the house of Cardinal Borgia, of receiving 6000 ducats annually. The discovery of the secondary planets of Jupiter was soon followed by the observations of the so-called triple form of Sciturn as a planeta, tergeminus. As early as November * Galilei, Opere, t. ii. (Longitudine per via de' Pianeti Mcdicei) pp. 435--506; Nelli, Vita vol. ii. pp. 656-688; Venturi, Memorie e Leitere di G. Galilei, P. i. p. 177. As early as 1612, or scarcely two years after the discovery of Jupiter's satellites, Galileo boasted, somewhat prematurely indeed, of having completed tables of those secondary satellites "to within 1' of time." A long diplomatic correspondence was carried on with the Spanish ambassador in 1616, and with the Dutch ambassador in 1636, but without leading to the desired object. The telescopes were to magnify from forty to fifty times. In order more easily to find the satellites when the ship is in motion, and (as he believed) to keep them in the field, he invented, in 1617 (Nelli, vol. ii. p. 663), the binocular telescope, which has generally been ascribed to the Capucine monk, Schyrleus de Rheita, who had much experience in optical matters, and who endeavoured to construct telescopes magnifying four thousand times. Galileo made experiments with his binocular (which he also called a celatone or testiera), in the harbour of Leghorn, while the ship was violently moved by a strong wind. He also caused a contrivance to be prepared in the arsenal at Pisa, by which the observer of the satellites might be protected from all motion, by seating himself in a kind of boat, floating in another boat filled with water or with oil (Lettera al Picchena de' 22 Marzo, 1617; Nelli, Vita, vol. i. p. 281; Galilei, Opere, t. ii. p. 473 ; Lettera a Lorenzo Realio del 5 Giugno, 1637). The proof which Galileo (Opere, t. ii. p. 454) brought forward of the advantage to the naval service of his method over Morin's method of lunar distances is very striking. 2z
706 COSMOS. 1610, Galileo informed Kepler that "Saturn consisted of three stars, which were in mutual contact with one another." In this observation lay the germ of the discovery of Saturn's ring. Hevelius, in 1656, described the variations in its form, the unequal opening of the handles (anse), and their occasional total disappearance. The merit of having given a scientific explanation of all the phenomena of Saturn's ring belongs, however, to the acute observer Huygens, who, in 1655, in accordance with the suspicious custom of the age, and like Galileo, concealed his discovery in an anagram of eighty- eight letters. Dominicus Cassini was the first who observed the black stripe on the ring, and, in 1684, he recognised that it is divided into at least two concentric rings. I have here collected together what has been learnt during a century regarding the most wonderful and least anticipated of all the forms occurring in the heavenly regions, a form which has led to ingenious conjectures regarding the original mode of formation of the secondary and primary planets. The spots upon the sun were first observed through tele- scopes by Johann Fabricius of East Friesland, and by Galileo (at Padua or Venice as is asserted) ; in the publication of the discovery, in June 1611, Fabricius incontestibly preceded Galileo by one year, since his first letter to the Burgomaster, Marcus Welser, is dated the 4th of May, 1612. The earliest observations of Fabricius were made, according to Arago's careful researches in March 1611,* and, according to Sir David Brewster, even as early as towards the close of the year 1610 ; while Christopher Scheiner did not carry his own observations back to an earlier period than April 1611, and it is probable that he did not seriously occupy himself with the solar spots until the October of the same year. Concerning Galileo we * See Arago, in the Annuaire for 1842, pp. 460-476 (Decouvertes des taches Solaires et de la Rotation du Soleil). Brewster (Martyrs of Science, pp. 36 and 39), places the first observation of Galileo in October or November 1610. Compare Nelli, Vita, vol. i. pp. 324-384; Galilei, Opere, t. i. p. lix.; t. ii. pp. 85-200 ; t. iv. p. 53. On Harriot's observations, see Eigaud, pp. 32 and 38. The Jesuit Scheiner, who was summoned from Gratz to Rome, has been accused of striving to revenge himself on Galileo, on account of the literary contest regarding the discovery of the solar spots, by getting it whispered to Pope Urban VIIL, through another Jesuit, Grassi, that he (the Pope), in the DialogU delle Scienze Nuove, was represented as the foolish and ignorant Simplicio (Nelli, vol. ii. p. 515).
- Page 309 and 310: 654 COSMOS, heavenly bodies, in the
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- Page 339 and 340: 684 COSMOS. Waisselrode of Allen, b
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- Page 357 and 358: 702 COSMOS. he first directed towar
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- Page 385 and 386: 730 COSMOS. Men had now discovered
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706 <strong>COSMOS</strong>.<br />
1610, Galileo informed Kepler that "Saturn consisted of three<br />
stars, which were in mutual contact with one another." In<br />
this observation lay the germ of the discovery of Saturn's<br />
ring. Hevelius, in 1656, described the variations in its form,<br />
the unequal opening of the handles (anse), and their occasional<br />
total disappearance. The merit of having given a<br />
scientific explanation of all the phenomena of Saturn's ring<br />
belongs, however, to the acute observer Huygens, who, in<br />
1655, in accordance with the suspicious custom of the age,<br />
and like Galileo, concealed his discovery in an anagram of<br />
eighty- eight letters. Dominicus Cassini was the first who<br />
observed the black stripe on the ring, and, in 1684, he recognised<br />
that it is divided into at least two concentric rings. I<br />
have here collected together what has been learnt during a<br />
century regarding the most wonderful and least anticipated of<br />
all the forms occurring in the heavenly regions, a form which<br />
has led to ingenious conjectures regarding the original mode<br />
of formation of the secondary and primary planets.<br />
The spots upon the sun were first observed through tele-<br />
scopes by Johann Fabricius of East Friesland, and by Galileo<br />
(at Padua or Venice as is asserted) ; in the publication of the<br />
discovery, in June 1611, Fabricius incontestibly preceded<br />
Galileo by one year, since his first letter to the Burgomaster,<br />
Marcus Welser, is dated the 4th of May, 1612. The earliest<br />
observations of Fabricius were made, according to Arago's<br />
careful researches in March 1611,* and, according to Sir David<br />
Brewster, even as early as towards the close of the year 1610 ;<br />
while Christopher Scheiner did not carry his own observations<br />
back to an earlier period than April 1611, and it is probable<br />
that he did not seriously occupy himself with the solar spots<br />
until the October of the same year. Concerning Galileo we<br />
* See Arago, in the Annuaire for 1842, pp. 460-476 (Decouvertes<br />
des taches Solaires et de la Rotation du Soleil). Brewster (Martyrs<br />
of Science, pp. 36 and 39), places the first observation of Galileo in<br />
October or November 1610. Compare Nelli, Vita, vol. i. pp. 324-384;<br />
Galilei, Opere, t. i. p. lix.; t. ii. pp. 85-200 ; t. iv. p. 53. On Harriot's<br />
observations, see Eigaud, pp. 32 and 38. The Jesuit Scheiner, who was<br />
summoned from Gratz to Rome, has been accused of striving to revenge<br />
himself on Galileo, on account of the literary contest regarding the discovery<br />
of the solar spots, by getting it whispered to Pope Urban V<strong>II</strong>L,<br />
through another Jesuit, Grassi, that he (the Pope), in the DialogU delle<br />
Scienze Nuove, was represented as the foolish and ignorant Simplicio<br />
(Nelli, vol. ii. p. 515).