Serpens south

Globular cluster


caption = A cluster of new stars called Serpens South. Courtesy of NASA/ESA
name = Serpens South
type = Emission
epoch = J2000.0
ra = RA|18|30|5.00
dec = DEC|2|02|30.00
dist_ly = 260 parsec (848 ly)
appmag_v = n/a
size_v = 14.4×20.3arcmins
constellation = Serpens
radius_ly = 3.5×5 ly
absmag_v = n/a
notes =
names =

The Serpens South star cluster is a relatively dense group of 50 young stars, 35 of which are protostars just beginning to form. The cluster is situated in the southern portion of the Serpens cloud, located approximately 848 light-years away from Earth.

The cluster was uncovered by NASA's Spitzer Space Telescope in the southern portion of the Serpens cloud. The discovery was possible due to the infrared observation capabilities of the SST because at visible wavelengths the stars are completely obscured by interstellar dust in the Serpens cloud.

The stars of the cluster were dubbed "siblings" by the team of astronomers led by Dr. Robert Gutermuth, of the Harvard-Smithsonian Center for Astrophysics, because they were able to determine that the newly discovered stars belonged to the Serpens star-forming cloud [ [http://www.spitzer.caltech.edu/Media/happenings/20070808/ Stellar Sbilings in Serpens south] ] , which also hosts the famous and massive Serpens star cluster (Messier 5).

The discovery of Serpens South is a direct result of the Gould's Belt Legacy project, which aims to study all prominent star-forming regions within about 1,600 light-years of Earth. These regions together form a ring of molecular clouds and associated young stars known as the Gould’s Belt and was first described by astronomer Benjamin Gould in 1879. Astronomers working on the project are trying to determine how members of large large stellar families are related [ [http://www.physorg.com/news105801659.html Two Telescopes Combine to Probe Young 'Family' of Stars] ] [ [http://www.cfa.harvard.edu/gouldbelt/ Mission statement - Gould's Belt Survey] ] .

This region of the Serpens constellation is similar to Messier 16 or the Eagle Nebula, another star forming region in Serpens which is observable in visible wavelengths. The Eagle Nebula was famously photographed by the Hubble Space Telescope.

External links

* [http://www.spitzer.caltech.edu/spitzer/index.shtml The Spitzer Space Telescope]
* [http://cfa-www.harvard.edu/ The Harvard-Smithsonian Center for Astrophysics homepage]
* [http://www.cfa.harvard.edu/gouldbelt/ The Gould's Belt Survey]

References