Astronomy:HAT-P-6b

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Short description: Extrasolar planet in the Andromeda constellation
HAT-P-6b / Nachtwacht
Exoplanet Comparison HAT-P-6 b.png
Size comparison of HAT-P-6b with Jupiter.
Discovery
Discovered byNoyes et al.
Discovery dateOctober 15, 2007
transit
Orbital characteristics
0.05239+0.00080
−0.00082
AU[1]
Eccentricity<0.044[1]
Orbital period3.852985±0.000005[2] d
Inclination166±10 °[3]
StarHAT-P-6
Physical characteristics
Mean radius1.33 ± 0.06 |♃|J}}}}}}[2]
Mass1.106+0.039
−0.040
[1] ||J}}}}}}
Mean density583 kg/m3 (983 lb/cu yd)[1]


HAT-P-6b is a transiting extrasolar planet discovered by Noyes et al. on October 15, 2007.[2] It is located approximately 910 light-years away[4] in the constellation of Andromeda, orbiting the star HAT-P-6. This hot Jupiter planet orbits with a semi-major axis of about 7.832 gigameters, and takes 92 hours, 28 minutes, 17 seconds and 9 deciseconds to orbit the star.[2] It has true mass of 5.7% greater than Jupiter and a radius 33% greater than Jupiter, corresponding to a density of 0.583 g/cm3, which is less than water.[1]

The planet HAT-P-6b is named Nachtwacht. The name was selected in the NameExoWorlds campaign by the Netherlands, during the 100th anniversary of the IAU, after Rembrandt's painting The Night Watch.[5][6]

The sky projected angle between stellar and orbital axis is roughly 166°, making it one of the few planets that is in a retrograde orbit around its parent star.[3] Observations made by Spitzer Space Telescope shows that the planet atmosphere has a weak temperature inversion, or no inversion at all, depending on how strong is the stellar chromospheric activity.[7]

Artist's impression of Hat-P-6b orbiting its host star with an aurora on its south pole.

References

  1. 1.0 1.1 1.2 1.3 1.4 Bonomo, A. S. et al. (2017). "The GAPS Programme with HARPS-N at TNG . XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets". Astronomy and Astrophysics 602: A107. doi:10.1051/0004-6361/201629882. Bibcode2017A&A...602A.107B. 
  2. 2.0 2.1 2.2 2.3 Noyes, R. W. et al. (2008). "HAT-P-6b: A Hot Jupiter Transiting a Bright F Star". The Astrophysical Journal Letters 673 (1): L79–L82. doi:10.1086/527358. Bibcode2008ApJ...673L..79N. 
  3. 3.0 3.1 Hébrard, Guillaume; Ehrenreich, David; Bouchy, François; Delfosse, Xavier; Moutou, Claire; Arnold, Luc; Boisse, Isabelle; Bonfils, Xavier et al. (2011). "The retrograde orbit of the HAT-P-6b exoplanet". Astronomy and Astrophysics 527: L11. doi:10.1051/0004-6361/201016331. Bibcode2011A&A...527L..11H. 
  4. Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode2018A&A...616A...1G.  Gaia DR2 record for this source at VizieR.
  5. "Approved names" (in en). http://www.nameexoworlds.iau.org/final-results. 
  6. "International Astronomical Union | IAU". https://www.iau.org/news/pressreleases/detail/iau1912/. 
  7. Todorov, Kamen O.; Deming, Drake; Knutson, Heather A.; Burrows, Adam; Sada, Pedro V.; Cowan, Nicolas B.; Agol, Eric; Desert, Jean-Michel et al. (2012). "Warm Spitzer Observations of Three Hot Exoplanets: XO-4b, HAT-P-6b, and HAT-P-8b". The Astrophysical Journal 746 (1): 111. doi:10.1088/0004-637X/746/1/111. Bibcode2012ApJ...746..111T. 

External links

Coordinates: Sky map 23h 39m 05.8061s, +42° 27′ 57.513″