OGLE-2007-BLG-349(AB)b
Exoplanet | List of exoplanets | |
---|---|---|
| ||
Parent star | ||
Star | OGLE-2007-BLG-349 | |
Constellation | Sagittarius | |
Right ascension | (α) | 18h 05m 24s |
Declination | (δ) | –26° 25′ 19″ |
Apparent magnitude | (mV) | 24.73[1] |
Distance | ~8,000[2] ly (2760 ± 380[1] pc) | |
Spectral type | M / M[1] | |
Mass | (m) | A: 0.41 (± 0.07)[1] M☉ B: 0.30 (± 0.07)[1] M☉ |
Physical characteristics | ||
Mass | (m) | 80 (± 13)[1] M⊕ |
Observed separation | ||
Projected separation | (d) | +0.43 −0.34 2.59[1] AU |
Discovery information | ||
Discovery date | 22 September 2016 | |
Discoverer(s) | Hubble Space Telescope | |
Discovery method | Gravitational microlensing | |
Discovery status | Published | |
Other designations | ||
OGLE-2007-BLG-349(AB)c | ||
Database references | ||
Extrasolar Planets Encyclopaedia | data | |
SIMBAD | data | |
Exoplanet Archive | data | |
Open Exoplanet Catalogue | data |
OGLE-2007-BLG-349(AB)b[note 1] is a circumbinary extrasolar planet about 8,000 light-years away in the constellation of Sagittarius.[2] It is the first circumbinary exoplanet to be discovered using the microlensing method of detecting exoplanets.[1]
Characteristics
Mass and orbit
OGLE-2007-BLG-349L(AB)b is a super-Neptune, an exoplanet that has a mass and radius larger than that of Neptune. It has a mass of around 80 M⊕.[1] This is somewhat close to the mass of Saturn, so OGLE-2007-BLG-349L(AB)b can also be considered a gas giant. It orbits at a distance of around 2.9 AU in a circumbinary orbit, meaning it orbits around two stars.
Host star
The planet orbits in a circumbinary (M-type) binary star system named OGLE-2007-BLG-349L. They orbit around each other roughly every 9 days.[1] The stars have masses of 0.41 and 0.30 M☉, respectively. The age of the system, radii and temperatures of the stars are not known. In comparison, the Sun is 4.6 billion years old[3] and has a surface temperature of 5778 K.[4]
The star's apparent magnitude, or how bright it appears from Earth's perspective, is 14.3. Therefore, it is too dim to be seen with the naked eye.
See also
- Optical Gravitational Lensing Experiment or OGLE
- 47 Ursae Majoris b
- OGLE-2005-BLG-390Lb
- OGLE-2006-BLG-109Lb
Notes
- ↑ The paper incorrectly refers to the planet as planet "c", however, this is probably just an error and should not be confused with the "B" star. Alternatively it can be used to differ from the secondary star.
References
- 1 2 3 4 5 6 7 8 9 10 http://hubblesite.org/pubinfo/pdf/2016/32/pdf.pdf
- 1 2 https://exoplanets.nasa.gov/news/1389/hubble-finds-planet-orbiting-pair-of-stars-8000-light-years-away/
- ↑ Fraser Cain (16 September 2008). "How Old is the Sun?". Universe Today. Retrieved 19 February 2011.
- ↑ Fraser Cain (15 September 2008). "Temperature of the Sun". Universe Today. Retrieved 19 February 2011.
Coordinates: 18h 05m 24s, −26° 25′ 19″