Astronomy:HD 69830 b

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Short description: Neptunian-sized exoplanet orbiting HD 69830
HD 69830 b
HD 69830 b (Celestia).jpg
Discovery
Discovered byC. Lovis et al.[1]
Discovery dateMay 18, 2006
Radial velocity
Orbital characteristics
0.0764 ± 0.0017 AU (11,430,000 ± 250,000 km)[2]
Eccentricity0.128±0.028[2]
Orbital period8.66897±0.00028 d[2]
astron|astron|helion}}2,453,496.8 ± 0.06
340 ± 26
Semi-amplitude3.4±0.1 m/s[2]
StarHD 69830
Physical characteristics
Mass≥10.1+0.38
−0.37
 M
[2]
Physics~804 K


HD 69830 b is a Neptune-mass or super-Earth-mass exoplanet orbiting the star HD 69830. It is at least 10 times more massive than Earth. It also orbits very close to its parent star and takes 82/3 days to complete an orbit.

Based on theoretical modeling in the 2006 discovery paper, this is likely to be a rocky planet, not a gas giant.[1] However, other work has found that if it had formed as a gas giant, it would have stayed that way,[3] and it is now understood that planets this massive are rarely rocky.[4]

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.[5]

References

  1. 1.0 1.1 Lovis, Christophe et al. (2006). "An extrasolar planetary system with three Neptune-mass planets". Nature 441 (7091): 305–309. doi:10.1038/nature04828. PMID 16710412. Bibcode2006Natur.441..305L. http://obswww.unige.ch/~pernier/publications-www/articles-pdf-ps/2006Natur.441..305L.pdf. Retrieved 2013-11-22. 
  2. 2.0 2.1 2.2 2.3 2.4 Laliotis, Katherine 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. doi:10.3847/1538-3881/acc067. Bibcode2023AJ....165..176L. 
  3. H. Lammer (2007). "The impact of nonthermal loss processes on planet masses from Neptunes to Jupiters". Geophysical Research Abstracts 9 (7850). http://www.cosis.net/abstracts/EGU2007/07850/EGU2007-J-07850.pdf?PHPSESSID=1eb3a7a98603083dda25d18001ea2a33. 
  4. Chen, Jingjing; Kipping, David (2017). "Probabilistic Forecasting of the Masses and Radii of Other Worlds". The Astrophysical Journal 834 (1): 17. doi:10.3847/1538-4357/834/1/17. Bibcode2017ApJ...834...17C. 
  5. Jackson, Brian; Richard Greenberg; Rory Barnes (2008). "Tidal Heating of Extra-Solar Planets". Astrophysical Journal 681 (2): 1631. doi:10.1086/587641. Bibcode2008ApJ...681.1631J. 

Coordinates: Sky map 08h 18m 23.9s, −12° 37′ 55.8″