M9

M9 = NGC6333 ( 17h 19.2m -18°31´, 7.9 mag. )
This smallest of Ophiuchus globular clusters was found by Messier on May 28, 1764.

M9 (globular cluster)
M10 (globular cluster)
M12 (globular cluster)
M14 (globular cluster)
M19 (globular cluster)
M62 (globular cluster)
M107 (globular cluster) ...

M9 (globular cluster)
M10 (globular cluster)
M12 (globular cluster)
M14 (globular cluster)
M19 (globular cluster)
M62 (globular cluster)
M107 (globular cluster) ...

M9 is a globular cluster of stars located within the constellation of Ophiuchus. It is located at the edge of a dark patch of dark nebulosity. This cluster is about 26,000 light-years from us and has a diameter of about 70 light-years.

M9 Pistol
The M9 pistol, formally Pistol, Semiautomatic, 9mm, M9, is a 9x19mm Parabellum pistol of the Military of the United States adopted in the 1980s....
which is issued to the majority of combat and support units.

M9 (NGC 6333) is the smallest of this group, unresolved except in large instruments.
The cluster is found 3.5 degrees SE of eta Ophiuchi. It is considered to be about 26,000 light years away.

8 Teide 1 in the Pleiades appears to have a mass and a spectral type M9 (Rebolo et al. 1995). A second candidate was identified by methane absorption lines in Gliese 229B, a faint object orbiting the M1 star Gliese 229 in the constellation Lepus, 18.

Previously thought to be a very dim red dwarf star (M9.0 V) on its detection more than 25 years ago, Luyten Palomar (LP) 944-20 was detemined to be a brown dwarf in 1998 when Chris G.

Ophiuchus contains several star clusters, such as IC 4665, NGC 6633, M9, M10, M12, M14, M19, M62, and M107, as well as the nebula IC 4603-4604. The unusual galaxy merger remnant NGC 6240 is also in Ophiuchus.

5 to M9.5. The spectrum of an M star shows lines belonging to molecules and all neutral metals but hydrogen lines are usually absent. Titanium oxide can be strong in M stars, usually dominating by about M5.

LPVs, of which thousands are known, are among the biggest of all stars, exceeded only by high mass supergiants. R Leo is a deep class M (M8) giant, whose class also varies, between M7 and M9, ...

M9.0V
18.50
20.02
03h 39m 35s
âˆ'35° 25′ 41″
0.201″
16.19
TNotes : The light year distances for the nearest star systems taken from parallax data determined by the Research Consortium on Nearby Stars (or RECONS).

See also: Star, Sky, Light, Constellation, Planet