SGR 1900+14
From Wikipedia, the free encyclopedia
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| Observation data Epoch J2000 |
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| Constellation (pronunciation) |
Aquila |
| Right ascension | 19h 07m 16.85s |
| Declination | +09° 18' 50.4"' |
| Characteristics | |
| U-B color index | ? |
| B-V color index | ? |
| Variable type | None |
| Astrometry | |
| Distance | 20 kly (6.1 kpc) |
| Details | |
| Mass | ? M☉ |
| Radius | ? R☉ |
| Luminosity | ? L☉ |
| Temperature | ? K |
| Metallicity | ? |
| Rotation | ? |
| Age | ? years |
| Other designations | |
SGR 1900+14, is located in the constellation of Aquila about 20,000 light-years away. It is an example of an intensely magnetic star, known as a magnetar, which is thought to arise from a fairly recent supernova explosion; only four are known to exist for certain within our Milky Way Galaxy. Could be a possible super-magnetic quark star.
NASA’s Spitzer Space Telescope detected a mysterious ring around SGR 1900+14 at two narrow infrared frequencies in 2005 and 2007. The 2007 Spitzer image showed no discernable change in the ring after two years. The ring measures seven light-years across. The origin of the ring is currently unknown and is the subject of an article in the May 29, 2008 issue of the journal Nature. [1]

