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Observations of the planet Saturn with the twenty-foot Equatoreal at Valletta

โœ Scribed by W. Lassell


Publisher
John Wiley and Sons
Year
1855
Tongue
English
Weight
595 KB
Volume
39
Category
Article
ISSN
0004-6337

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โœฆ Synopsis


Observations of the planet Saturn with the twcuty-foot Equatoren1 at Valletta.

(Die Zeichnungen werden nachgeliefert).

1852 Oct. 5, Power 330. The planet instantly struck me b y its beauty and sharpiiess, though still far from the meridian.

After some conteniplation I felt persuaded that I never s a w the planet s o well. The exterior bright ring (A) presented evidently a s t r i 11 e d appearance, most strongly in the middle, yet not concentrated iuto a n y single indisputable line. The inferiority of brightness of' A, airiounted to contrast with the inner bright ririg B. The obscure ring C, far better seen than I have ever seen it before, extending precisely half way from the inner edge of B to the plaiiet's IiniIi; of' urtiforni brightness and without iiny trace of a division. The exterior boundary of C was very hard, u p to the inner edge of B, but I could riot assert tliiit there w a s any division there.

The shape of the shatlow of the hall upon the ring i s a ng u l a r , a s Oct. 5 drawn, and there is a spot upon the southfolloming portion o f the ring 80 close to the ball, a s to b e almost iiiidistiiiguishable whether it was on the ball or ring.


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โœ M. R. Dolman ๐Ÿ“‚ Article ๐Ÿ“… 1865 ๐Ÿ› John Wiley and Sons ๐ŸŒ English โš– 77 KB ๐Ÿ‘ 2 views

The letters in the colunin ,,OI~s." are the initials of Sirnow, Mc Clure and Houyh. These observations have been iiiade Iiy the Chronographic method, 1 5 wires being eniployecl for AR, with the exception of 1864 Dec. 14, when only 5 wires were used. The Declinations are corrected for parallax.