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COSMOS, VOL. II - World eBook Library

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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).

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