OGLE-2007-BLG-368Lb
| Exoplanet | List of exoplanets | |
|---|---|---|
| Parent star | ||
| Star | OGLE-2007-BLG-368L | |
| Constellation | Scorpius | |
| Right ascension | (α) | 17h 56m 25.96s |
| Declination | (δ) | –32° 14′ 14.7″ |
| Distance | 19230 ly (5900 pc) | |
| Spectral type | K5V? | |
| Observed separation | ||
| Projected separation | (d) | 3.3 ± 1.4 AU |
| Physical characteristics | ||
| Mass | (m) | 0.0694 MJ (22.1 M⊕) |
| Discovery information | ||
| Discovery date | December 8, 2009 | |
| Discoverer(s) | Sumi et al. | |
| Discovery method | Gravitational microlensing | |
| Discovery site | Mount John University Observatory,  | |
| Discovery status | Published | |
| Database references | ||
| Extrasolar Planets Encyclopaedia | data | |
| SIMBAD | data | |
| Exoplanet Archive | data | |
| Open Exoplanet Catalogue | data | |
OGLE-2007-BLG-368Lb is an extrasolar planet located approximately 19,230 light-years away in the constellation of Scorpius, orbiting the star OGLE-2007-BLG-368L. This planet was detected on December 8, 2009 by the gravitational microlensing by Sumi. It has mass 6.94% of Jupiter (i.e. 22 times that of Earth) and is located 3.3 AU from the star when observed. Based on those properties it would classify as a Cold Neptune. It is the second Cold Neptune to be observed, the first being OGLE-2005-BLG-169Lb.[1] This planet is most likely be similar to Uranus and Neptune in the solar system in terms of atmospheric and internal properties.
References
- ↑ Sumi, T.; et al. (2010). "A Cold Neptune-Mass Planet OGLE-2007-BLG-368Lb: Cold Neptunes Are Common". The Astrophysical Journal. 710 (2): 1641–1653. arXiv:0912.1171. Bibcode:2010ApJ...710.1641S. doi:10.1088/0004-637X/710/2/1641.
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