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Contents

   



(Top)
 


1 Physical properties  





2 See also  





3 References  





4 External links  














HAT-P-5b






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Coordinates: Sky map18h17m37.299s, +36° 37 16.88
 

From Wikipedia, the free encyclopedia
 


This is an old revision of this page, as edited by JJMC89 bot III (talk | contribs)at12:28, 14 May 2023 (Moving Category:Lyra (constellation)toCategory:Lyra per Wikipedia:Categories for discussion/Speedy). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.
(diff)  Previous revision | Latest revision (diff) | Newer revision  (diff)

HAT-P-5b
Size comparison of HAT-P-5b with Jupiter.
Discovery
Discovered byBakos et al.
Discovery dateOctober 9, 2007

Detection method

transit
Orbital characteristics

Semi-major axis

0.04075 ± 0.00076 AU (6,096,000 ± 114,000 km)
Eccentricity0

Orbital period (sidereal)

2.788491 ± 2.5e-5 d
Inclination86.75 ± 0.44
StarHAT-P-5
Physical characteristics

Mean radius

1.204±0.017 RJ[1]
Mass0.989±0.053 MJ[1]

Mean density

660 ± 110 kg/m3 (1,110 ± 190 lb/cu yd)
Temperature1485+109
−118
[2]

HAT-P-5b is a transiting extrasolar planet located approximately 1000 light-years away in the constellationofLyra, orbiting the star HAT-P-5. It is a hot Jupiter with a mass 6% greater than Jupiter and a radius 26% greater than Jupiter, corresponding to a density of 0.66 g/cm3, which is less than water. This planet was found by Bakos et al. on October 9, 2007.[3]

The planet HAT-P-5b is named Kráľomoc. The name was selected in the NameExoWorlds campaign by Slovakia, during the 100th anniversary of the IAU. Kráľomoc is an ancient Slovak term for the planet Jupiter.[4][5]

Physical properties

The measured temperature on the planetary dayside is 1485+109
−118
K.[2]

See also

References

  1. ^ a b Wang, Xian-Yu; et al. (1 July 2021). "Transiting Exoplanet Monitoring Project (TEMP). VI. The Homogeneous Refinement of System Parameters for 39 Transiting Hot Jupiters with 127 New Light Curves". The Astrophysical Journal Supplement Series. 255 (1). 15. arXiv:2105.14851. Bibcode:2021ApJS..255...15W. doi:10.3847/1538-4365/ac0835. S2CID 235253975.{{cite journal}}: CS1 maint: unflagged free DOI (link)
  • ^ a b Wallack, Nicole L.; Knutson, Heather A.; Deming, Drake (2021), "Trends in Spitzer Secondary Eclipses", The Astronomical Journal, 162 (1): 36, arXiv:2103.15833, Bibcode:2021AJ....162...36W, doi:10.3847/1538-3881/abdbb2, S2CID 232417602{{citation}}: CS1 maint: unflagged free DOI (link)
  • ^ Bakos, G. Á.; et al. (2007). "HAT-P-5b: A Jupiter-like Hot Jupiter Transiting a Bright Star". The Astrophysical Journal Letters. 671 (2): L173–L176. arXiv:0710.1841. Bibcode:2007ApJ...671L.173B. doi:10.1086/525022. S2CID 15514048.
  • ^ "Approved names". NameExoworlds. Retrieved 2020-01-02.
  • ^ "International Astronomical Union | IAU". www.iau.org. Retrieved 2020-01-02.
  • External links

    Media related to HAT-P-5 b at Wikimedia Commons



  • t
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  • Retrieved from "https://en.wikipedia.org/w/index.php?title=HAT-P-5b&oldid=1154749615"

    Categories: 
    Exoplanets discovered by HATNet
    Hot Jupiters
    Transiting exoplanets
    Exoplanets discovered in 2007
    Giant planets
    Lyra
    Exoplanets with proper names
    Exoplanet stubs
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    This page was last edited on 14 May 2023, at 12:28 (UTC).

    This version of the page has been revised. Besides normal editing, the reason for revision may have been that this version contains factual inaccuracies, vandalism, or material not compatible with the Creative Commons Attribution-ShareAlike License.



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