Academy Newspaper Saturday 17th January 1874
Mr. Marth, in a letter to Mr. Lassell published in the
Astronomical Society’s Notices, has pointed out the favourable chances that
observers may have during the present apparition of Uranus of contributing
something towards the decisive settlement of the question respecting the
existence of Sir William Herschel's additional satellites of the Georgium
Sidus. The geocentric place of Uranus in the heavens is now only some twenty
seconds south of that in which it appeared in 1790 at a three-days’ later date,
so that the planet in its retrograde course passed on Thursday night (Jan. 15),
and will pass on the night of February 6 the same stars which it passed on the
evenings of January 18 and February 9, in 1790. Some of these stars were then
supposed to be additional satellites. It seems certainly desirable that the
opportunity for recovering these little stars, and also for ascertaining the
effect of the neighbourhood of the planet upon their visibility, should not be
allowed to slip away unused. It will be remembered that Sir W. Herschel
announced the discovery of six satellites to Uranus, two only of which, viz.,
the second and fourth, have been confirmed by subsequent observations. Two
inner satellites revolving within the first of Sir W, Herschel’s have been
observed by Mr. Lassell (who named them Ariel and Umbriel) at Malta, to which
place he transferred his large reflector on account of the great clearness of
the atmosphere there, and by others. The existence of four of Sir W. Herschel’s
satellites is therefore very uncertain, and it is to these that Mr. Marth
refers.



.jpg)

.jpg)


