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Kepler-25c

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Kepler-25c
Discovery[1]
Discovered bySteffen et al.
Discovery siteKepler Space Observatory
Discovery date2012
Transits, and transit-timing variations
Designations
KOI-244.01[2]
Orbital characteristics[3][1]
0.110 AU
Eccentricity0.0061+0.0049
−0.0041
12.7207±0.0001 d
Inclination92.764+0.042
−0.039
 º
StarKepler-25
Physical characteristics[3]
5.217+0.070
−0.065
 R🜨
Mass≥15.2+1.3
−1.6
 M🜨
Mean density
0.588+0.053
−0.061
 g/cm3

Kepler-25c is an exoplanet orbiting the star Kepler-25, located in the constellation Lyra.[4] The planet was first detected as a candidate extrasolar planet by the Kepler space telescope in 2011.[5] It was confirmed, in 2012, by Jason Steffen and collaborators using transit-timing variations obtained by the Kepler Space Telescope.[1] It orbits its parent star at only 0.110 astronomical units away, and at its distance it completes an orbit once every 12.7 days.[1]

References

  1. ^ a b c d Steffen, Jason H.; et al. (2012). "Transit timing observations from Kepler - III. Confirmation of four multiple planet systems by a Fourier-domain study of anticorrelated transit timing variations". Monthly Notices of the Royal Astronomical Society. 421 (3): 2342–2354. arXiv:1201.5412. Bibcode:2012MNRAS.421.2342S. doi:10.1111/j.1365-2966.2012.20467.x.
  2. ^ "Kepler-25b". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-10-05.
  3. ^ a b Mills, Sean M.; et al. (2019). "Long-period Giant Companions to Three Compact, Multiplanet Systems". The Astronomical Journal. 157 (4). 145. arXiv:1903.07186. Bibcode:2019AJ....157..145M. doi:10.3847/1538-3881/ab0899. S2CID 119197547.{{cite journal}}: CS1 maint: unflagged free DOI (link)
  4. ^ Roman, Nancy G. (1987). "Identification of a Constellation From a Position". Publications of the Astronomical Society of the Pacific. 99 (617): 695–699. Bibcode:1987PASP...99..695R. doi:10.1086/132034. Vizier query form
  5. ^ Borucki, William J.; et al. (2011). "Characteristics of Planetary Candidates Observed by Kepler. II. Analysis of the First Four Months of Data". The Astrophysical Journal. 736 (1). 19. arXiv:1102.0541. Bibcode:2011ApJ...736...19B. doi:10.1088/0004-637X/736/1/19.