V4046 Sagittarii
Double star V4046 Sagittarii |
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Observation dates equinox : J2000.0 , epoch : J2000.0 |
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AladinLite | |||||||||||
Constellation | Sagittarius | ||||||||||
Right ascension | 18 h 14 m 10 s | ||||||||||
declination | -32 ° 47 ′ 34 ″ | ||||||||||
Apparent brightness | 10.5 mag | ||||||||||
Astrometry | |||||||||||
distance | approx. 240 ly (approx. 70 pc ) |
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orbit | |||||||||||
period | 2.42 d | ||||||||||
Individual data | |||||||||||
Names | A; B. | ||||||||||
Age | approx. 12 million | ||||||||||
Other names and catalog entries |
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V4046 Sagittarii , or V4046 Sgr for short , is a spectroscopic binary star system in the constellation Sagittarius, about 240 light years away . The components belong to the spectral classes K5 and K7 and have almost identical masses of around 0.9 solar masses each; they are only a few solar radii apart. Their age is about 12 million years. In June 2009, a sub-millimeter array radio telescope was able to detect a protoplanetary disk surrounding the stars . This was the first discovery of such a disk in a binary star system and V4046 Sgr is the oldest star system so far in which such a disk has been detected.
Individual evidence
- ↑ Radio Telescope Images Reveal Planet-Forming Disk Orbiting Twin Suns. Harvard-Smithsonian Center for Astrophysics , June 10, 2009, accessed June 14, 2009 .