Astronomy:Kepler-1704b

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Short description: Eccentric super-Jupiter orbiting Kepler-1704
Kepler-1704b
Discovery
Discovered byPaul A. Dalba et al. [1]
Discovery date2021
Designations
KOI-375.01
Orbital characteristics
Periastron0.16
Apoastron3.9
2.026+0.024
−0.031
AU
Eccentricity0.921+0.010
−0.015
Orbital period988.8811177±0.0009114[2]
Inclination89.01+0.59
−0.27
°
Physical characteristics
Mean radius10.81 R[2]
Mass4.15 ± 0.29 MJ
Physics253.8+3.7
−4.1
K[1]

Kepler-1704b is a super-Jupiter on a highly eccentric orbit around the star Kepler-1704. It has a mass of 4.51 ||J}}}}}}. The planet's distance from its star varies from 0.16 to 3.9 AU. It is a failed hot Jupiter, been scattered from its birth orbit to orbit with periastron just above tidal circularization distance.[1]

Characteristics

Kepler-1704b is much more massive than Jupiter, at 4.51 MJ.[1] The high planetary mass makes Kepler-1704b a super-Jupiter. Kepler-1704b goes on a highly eccentric 2.7 year-long (988.88 days) orbit around its star as well as transiting.[1] The extreme eccentricity yields a temperature difference of up to 700 K.[1]

Star

The star, Kepler-1704, is a G2, 5745-kelvin star 825 parsecs (2,690 ly) from Earth and the sun. It has a mass of 1.131 M, a radius of 1.697 R, and a luminosity of 2.83 L. The high radius for the star's mass hints that Kepler-1704 is not a main-sequence star.[3]

See also

References

  1. 1.0 1.1 1.2 1.3 1.4 1.5 Dalba, Paul A.; Kane, Stephen R.; Li, Zhexing; Macdougall, Mason G.; Rosenthal, Lee J.; Cherubim, Collin; Isaacson, Howard; Thorngren, Daniel P. et al. (2021-07-14). "Giant Outer Transiting Exoplanet Mass (GOT 'EM) Survey. II. Discovery of a Failed Hot Jupiter on a 2.7 Yr, Highly Eccentric Orbit". The Astronomical Journal 162 (4): 154. doi:10.3847/1538-3881/ac134b. Bibcode2021AJ....162..154D. 
  2. 2.0 2.1 "Kepler Objects of Interest". https://exoplanetarchive.ipac.caltech.edu/cgi-bin/TblView/nph-tblView?app=ExoTbls&config=cumulative. 
  3. Dalba, Paul A.; Kane, Stephen R.; Li, Zhexing; Macdougall, Mason G.; Rosenthal, Lee J.; Cherubim, Collin; Isaacson, Howard; Thorngren, Daniel P. et al. (2021). "Giant Outer Transiting Exoplanet Mass (GOT 'EM) Survey. II. Discovery of a Failed Hot Jupiter on a 2.7 Yr, Highly Eccentric Orbit". The Astronomical Journal 162 (4): 154. doi:10.3847/1538-3881/ac134b. Bibcode2021AJ....162..154D.