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| ==Overview== | ==Overview== | ||
| The exoplanet 30 Arietis Bb has a ] of nearly 10 times that of ].<ref>{{cite web |url=http://exoplanet.eu/planet.php?p1=30+Ari+B&p2=b |title=Notes for Planet 30 Ari B b |author=Jean Schneider |year=2011 |website= |publisher=] |accessdate=3 October 2011}}</ref> |
The exoplanet 30 Arietis Bb has a ] of nearly 10 times that of ].<ref>{{cite web |url=http://exoplanet.eu/planet.php?p1=30+Ari+B&p2=b |title=Notes for Planet 30 Ari B b |author=Jean Schneider |year=2011 |website= |publisher=] |accessdate=3 October 2011}}</ref> In 2020, after the inclination of the planetary orbit was measured to be just 4.14{{±|0.96|0.90}}°, the "planet" was found to fall in the mass range of the red dwarf star.<ref name=Kiefer2020>{{citation|arxiv=2009.14164|title=Determining the true mass of radial-velocity exoplanets with Gaia 9 planet candidates in the brown-dwarf/stellar regime and 27 confirmed planets|year=2020}}</ref> | ||
| ==References== | ==References== | ||
Revision as of 00:54, 26 October 2020
Extrasolar planet| Discovery | |
|---|---|
| Discovered by | Guenther et al. |
| Discovery site | Karl Schwarzschild Observatory |
| Discovery date | November 27, 2009 |
| Detection method | Radial velocity |
| Orbital characteristics | |
| Semi-major axis | 0.995 ± 0.012 AU (148,800,000 ± 1,800,000 km) |
| Eccentricity | 0.289 ± 0.092 |
| Orbital period (sidereal) | 335.1 ± 2.5 d 0.917 ± 0.007 y |
30 Arietis Bb (sometimes abbreviated 30 Ari Bb) is an extrasolar planet which orbits the F-type main sequence star 30 Arietis B, located in a quadruple star system approximately 146 light years away in the constellation Aries. The gas giant planet was discovered by on Friday, November 27, 2009 by using precise radial velocity method from echelle spectrograph installed in Alfred-Jensch telescope in Karl Schwarzschild Observatory.
Overview
The exoplanet 30 Arietis Bb has a minimum mass of nearly 10 times that of Jupiter. In 2020, after the inclination of the planetary orbit was measured to be just 4.14
−0.90°, the "planet" was found to fall in the mass range of the red dwarf star.
References
- Guenther, E. W.; et al. (2009). "A substellar component orbiting the F-star 30 Arietis B". Astronomy and Astrophysics. 507 (3): 1659–1665. arXiv:0912.4619. Bibcode:2009A&A...507.1659G. doi:10.1051/0004-6361/200912112.
- Jean Schneider (2011). "Notes for Planet 30 Ari B b". Extrasolar Planets Encyclopaedia. Retrieved 3 October 2011.
- Determining the true mass of radial-velocity exoplanets with Gaia 9 planet candidates in the brown-dwarf/stellar regime and 27 confirmed planets, 2020, arXiv:2009.14164
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