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HD 69830 c

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Neptunian-sized planet orbiting HD 69830
HD 69830 c
HD 69830 c
Discovery
Discovered byC. Lovis et al.
Discovery dateMay 18, 2006
Detection methodRadial velocity
Orbital characteristics
Semi-major axis0.181 ± 0.004 AU (27,080,000 ± 600,000 km)
Eccentricity0.03±0.027
Orbital period (sidereal)31.6158±0.0051 d
Time of periastron2,453,469.6 ± 2.8
Argument of periastron221 ± 35
Semi-amplitude2.6±0.1 m/s
StarHD 69830
Physical characteristics
Mass≥12.09+0.55
−0.54 M🜨
Temperature~522 K

HD 69830 c is an exoplanet orbiting HD 69830. It is the second-closest planet in its system and has a minimum mass 12 times that of Earth. Based on theoretical modeling in the 2006 discovery paper, it is likely to be a rocky planet, not a gas giant. However, other work has found that if it had formed as a gas giant, it would have stayed that way, and it is now understood that planets this massive are rarely rocky.

References

  1. ^ 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. S2CID 4343578. Archived from the original (PDF) on 2016-03-03. Retrieved 2013-11-22.
  2. ^ Laliotis, Katherine; Burt, Jennifer A.; et al. (February 2023). "Doppler Constraints on Planetary Companions to Nearby Sun-like Stars: An Archival Radial Velocity Survey of Southern Targets for Proposed NASA Direct Imaging Missions". The Astronomical Journal. 165 (4): 176. arXiv:2302.10310. Bibcode:2023AJ....165..176L. doi:10.3847/1538-3881/acc067.
  3. H. Lammer; et al. (2007). "The impact of nonthermal loss processes on planet masses from Neptunes to Jupiters" (PDF). Geophysical Research Abstracts. 9 (7850).
  4. Chen, Jingjing; Kipping, David (2017). "Probabilistic Forecasting of the Masses and Radii of Other Worlds". The Astrophysical Journal. 834 (1): 17. arXiv:1603.08614. Bibcode:2017ApJ...834...17C. doi:10.3847/1538-4357/834/1/17. S2CID 119114880.


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