30 Arietis Bb
| Exoplanet | List of exoplanets | |
|---|---|---|
| Parent star | ||
| Star | 30 Arietis B | |
| Constellation | Aries | |
| Right ascension | (α) | 02h 36m 57.74s[1] |
| Declination | (δ) | +24° 38′ 53.0″[1] |
| Apparent magnitude | (mV) | 7.09 |
| Distance | 133 ± 3[1] ly (41 ± 1[1] pc) | |
| Spectral type | F6V | |
| Mass | (m) | 1.13 ± 0.08 M☉ |
| Radius | (r) | 1.13 ± 0.13 R☉ |
| Temperature | (T) | 6424 ± 180 K |
| Metallicity | [Fe/H] | 0.07 ± 0.2 |
| Age | 0.91 ± 0.03 Gyr | |
| Orbital elements | ||
| Semi-major axis | (a) | 0.995 ± 0.012 AU (148.9 ± 1.8 Gm) |
| Periastron | (q) | 0.708 AU (105.9 Gm) |
| Apastron | (Q) | 1.283 AU (191.9 Gm) |
| Eccentricity | (e) | 0.289 ± 0.092 |
| Orbital period | (P) | 335.1 ± 2.5 d (0.917 ± 0.007 y) |
| Orbital speed | (υ) | 32.3 km/s |
| Argument of periastron |
(ω) | 307 ± 18° |
| Time of periastron | (T0) | 2454538 ± 20 JD |
| Semi-amplitude | (K) | 270 m/s |
| Physical characteristics | ||
| Minimum mass | (m sin i) | 9.88 ± 0.94 MJ |
| Temperature | (T) | 300 |
| Discovery information | ||
| Discovery date | November 27, 2009 | |
| Discoverer(s) | Guenther et al. | |
| Discovery method | Radial velocity | |
| Discovery site | Karl Schwarzschild Observatory | |
| Discovery status | Published | |
| Database references | ||
| Extrasolar Planets Encyclopaedia | data | |
| SIMBAD | data | |
| Exoplanet Archive | data | |
| Open Exoplanet Catalogue | data | |
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 129 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.[2]
Overview
The exoplanet 30 Arietis Bb has a minimum mass of nearly 10 times that of Jupiter.[3] Because inclination is not identified, its true mass is unknown. Meanwhile, this planet orbits only 0.995 AU (or 700,000 km) closer to the star than Earth to the Sun, but its orbital eccentricity is much higher compared to Earth. At periastron, the planet’s closest distance to the star is 0.708 AU, which is slightly closer to the star than Venus to the Sun. At apastron, the planet’s farthest distance to the star is 1.283 AU, which is more than halfway between the orbits of Earth and Mars.[2]
References
- 1 2 3 4 van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. Vizier catalog entry for A Vizier catalog entry for B
- 1 2 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
- ↑ "30 Ari B b | New World Atlas - Exoplanet Exploration: Planets Beyond our Solar System". Exoplanet Exploration: Planets Beyond our Solar System. Retrieved 2018-07-30.
- Jean Schneider (2011). "Notes for Planet 30 Ari B b". Extrasolar Planets Encyclopaedia. Retrieved 3 October 2011.
