HD 69830 b
Exoplanet | List of exoplanets | |
---|---|---|
Parent star | ||
Star | HD 69830 | |
Constellation | Puppis | |
Right ascension | (α) | 08h 18m 23.947s[1] |
Declination | (δ) | −12° 37′ 55.81″[1] |
Apparent magnitude | (mV) | 5.95 |
Distance | 40.7 ± 0.2[1] ly (12.49 ± 0.05[1] pc) | |
Spectral type | G8V | |
Mass | (m) | 0.86 ± 0.03 M☉ |
Radius | (r) | 0.89 R☉ |
Temperature | (T) | 5385 ± 20 K |
Metallicity | [Fe/H] | −0.05 ± 0.02 |
Age | 5.1–6.1 Gyr | |
Orbital elements | ||
Semi-major axis | (a) | 0.0785 AU |
Eccentricity | (e) | 0.1 ± 0.04 |
Orbital period | (P) | 8.667 ± 0.003 d |
Argument of periastron |
(ω) | 340 ± 26° |
Time of periastron | (T0) | 2,453,496.8 ± 0.06 JD |
Semi-amplitude | (K) | 3.51 ± 0.15 m/s |
Physical characteristics | ||
Minimum mass | (m sin i) | 0.033 MJ |
Temperature | (T) | ~804 |
Discovery information | ||
Discovery date | May 18, 2006 | |
Discoverer(s) | Lovis et al.[2] | |
Discovery method | Radial velocity | |
Discovery status | Published[2] | |
Database references | ||
Extrasolar Planets Encyclopaedia | data | |
SIMBAD | data | |
Exoplanet Archive | data | |
Open Exoplanet Catalogue | data |
HD 69830 b is a Neptune-mass or super-Earth-mass exoplanet orbiting the star HD 69830. It is 10 times more massive than Earth. It also orbits very close to its parent star and takes 82/3 days to complete an orbit.
This is likely to be a rocky planet, not a gas giant.[2] If it had formed as a gas giant, it would have stayed that way.[3]
If HD 69830 b is a terrestrial planet, models predict that tidal heating would produce a heat flux at the surface of about 55 W/m2. This is 20 times that of Io.[4]
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
- 1 2 3 Lovis, Christophe; et al. (2006). "An extrasolar planetary system with three Neptune-mass planets" (PDF). Nature. 441 (7091): 305–309. arXiv:astro-ph/0703024. Bibcode:2006Natur.441..305L. doi:10.1038/nature04828. PMID 16710412.
- ↑ H. Lammer; et al. (2007). "The impact of nonthermal loss processes on planet masses from Neptunes to Jupiters" (PDF). Geophysical Research Abstracts. 9 (07850).
- ↑ Jackson, Brian; Richard Greenberg; Rory Barnes (2008). "Tidal Heating of Extra-Solar Planets". Astrophysical Journal. 681 (2): 1631. arXiv:0803.0026. Bibcode:2008ApJ...681.1631J. doi:10.1086/587641.
Coordinates:
This article is issued from
Wikipedia.
The text is licensed under Creative Commons - Attribution - Sharealike.
Additional terms may apply for the media files.