Not exact matches
Located 1,350 light - years away, the Orion
Nebula is a relatively nearby laboratory for studying the star formation process across a wide range, from opulent giant stars to diminutive red dwarf stars and elusive,
faint brown dwarfs.
The multitude of
fainter water - rich, free - floating brown dwarfs and planets within the Orion
nebula are all new discoveries.
The most likely explanations involve radiation or outflows from an active galactic nucleus (AGN) that
is strongly obscured by dust so that only a
faint source can
be seen associated with the
nebula.
«It
's extremely bright, and it
's probably larger than the Slug
Nebula, but there
's nothing else visible except the
faint smudge of a galaxy.
4 Long before we had the Hubble Telescope, astronomers
were puzzled about the nature of
nebulae: odd,
faint stars that sometimes looked like spirals.
Barnard's Loop
is a huge semicircular
nebula that almost surrounds the entire constellation - this
nebula is very
faint though and it
is only easily detected on long - exposure photographs.
While the bright part of the
nebula is of about 65 arc seconds in diameter (more accurately, the «cork»
is about 42x87», the «wings» 157x87»), this
nebula is surrounded by a
faint halo covering a region of 290 arc seconds in diameter (Millikan, 1974); this material
was probably ejected in the form of stellar winds from the central star when it
was still in the Red Giant phase of evolution.
Planetary
Nebula Messier 76 (M76, NGC 650/651)
is one of the
faintest Messier Objects, and one of only four planetary
nebulae in Messier's catalog, situated in the Eastern part of constellation Perseus.
The glowing apparition
is known to amateur astronomers as the «Little Ghost
Nebula,» because it appears as a small, ghostly cloud surrounding the
faint, dying central star.
There
are many other (
fainter)
nebulae surrounding the Orion
nebula and there
are many stars forming in this region.
left - to - right in our image); this
is similar to our view of another,
fainter Messier planetary
nebula, M76, which
is called the Little Dumbbell.
IC 4701
is also a fairly large (but much
fainter) emission
nebula in this region.
This planetary
nebula is certainly the most impressive object of its kind in the sky, as the angular diameter of the luminous body
is nearly 6 arc minutes, with a
faint halo extensing out to over 15», half the apparent diameter of the Moon (Millikan 1974).
(March 24, 1781) «
Nebula in the great Bear [Ursa Major], near Beta: It
is difficulat to see, reports M. Méchain, especially when one illuminates the micrometer wires: its light
is faint, without a star.
To the left of the Eta Carinae
nebula is a second much
fainter (and possibly more distant)
nebula around NGC 3503.
In the very neighborhood, to the north, there
are also
fainter reflection
nebulae, partially reflecting the light of the Great
Nebula.
Already under fairly good conditions, the
nebula itself can
be glimpsed with the naked eye as a
faint nebulosity around this star.
Messier included the object in his catalogue with the following description: «Very
faint nebula, discovered in Sagittarius; its center
is brilliant & it contains no star, seen with an achromatic telescope of 3.5 feet [FL].