Astronomy with an Opera-glass: A Popular Introduction to the Study of the Starry Heavens with the Simplest of Optical InstrumentsServiss, Garrett Putman
Science
Astronomy with an Opera-glass: A Popular Introduction to the Study of the Starry Heavens with the Simplest of Optical Instruments
Serviss, Garrett Putman
Astronomy
The reader should not expect to be able to see the nebulae in the
Pleiades with an opera-glass. I have thought it proper to mention these
singular objects only in order that he might be in possession of the
principal and most curious facts about those interesting stars.[C]
[Footnote C: The Henry Brothers have continued the photographic work
described above, and their later achievements are even more interesting
and wonderful. They have found that there are many nebulous masses
involved in the group of the Pleiades, and have photographed them. One
of the most amazing phenomena in their great photograph of the Pleiades
is a long wisp or streak of nebulous matter, along which eight or nine
stars are strung in a manner which irresistibly suggests an intimate
connection between the stars and the nebula. This recalls the recent
(August, 1888) discovery made by Prof. Holden, with the great Lick
telescope, concerning the structure of the celebrated ring nebula in
Lyra, which, it appears, is composed of concentric ovals of stars and
nebulous stuff, so arranged that we must believe they are intimately
associated in a most wonderful community.]
Orion will next command our attention. You will find the constellation
in Map No. 19:
"Eastward beyond the region of the Bull
Stands great Orion; whoso kens not him in cloudless night
Gleaming aloft, shall cast his eyes in vain
To find a brighter sign in all the heaven."
To the naked eye, to the opera-glass, and to the telescope, Orion is
alike a mine of wonders. This great constellation embraces almost every
variety of interesting phenomena that the heavens contain. Here we have
the grandest of the nebulae, some of the largest and most beautifully
colored stars, star-streams, star-clusters, nebulous stars, variable
stars. I have already mentioned the positions of the principal stars in
the imaginary figure of the great hunter. I may add that his upraised
arm and club are represented by the stars seen in the map above Alpha
([alpha]) or Betelgeuse, one of which is marked Nu ([nu]), and another,
in the knob of the club, Chi ([chi]). I have also, in speaking of
Aldebaran, described the contrast in the colors of Betelgeuse and Beta
([beta]) or Rigel. Betelgeuse, it may be remarked, is slightly variable.
Sometimes it appears brighter than Rigel, and sometimes less brilliant.
It is interesting to note that, according to Secchi's division of the
stars into types, based upon their spectra, Betelgeuse falls into the
third order, which seems to represent a type of suns in which the
process of cooling, and the formation of an absorptive envelope or
shell, have gone on so far that we may regard them as approaching the
point of extinction. Rigel, on the other hand, belongs to the first
order or type which represents suns that are probably both hotter and
younger in the order of development. So, then, we may look upon the two
chief stars of this great constellation as representing two stages of
cosmical existence.
Public-domain text, read in full here on John Shaqi.
Reviews
Reviews
No reviews yet
Be the first to share your thoughts on this work.
Elsewhere in the archive
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account