Astronomy:Kepler-36

From HandWiki
(Redirected from Astronomy:Kepler-36c)
Short description: Star in the constellation Cygnus
Kepler-36
Observation data
Equinox J2000.0]] (ICRS)
Constellation Cygnus
Right ascension  19h 25m 00.0431s[1]
Declination +49° 13′ 54.631″[1]
Apparent magnitude (V) 11.9
Characteristics
Spectral type G1IV
Astrometry
Proper motion (μ) RA: 0.970±0.041[1] mas/yr
Dec.: −8.073±0.043[1] mas/yr
Parallax (π)1.8654 ± 0.0215[1] mas
Distance1,750 ± 20 ly
(536 ± 6 pc)
Details
Mass1.071±0.043[2] M
Radius1.626±0.019[2] R
Surface gravity (log g)4.1±0.1[3] cgs
Temperature5911±66[2] K
Metallicity [Fe/H]−0.2±0.06[2] dex
Rotation17.20±0.2[2]
Rotational velocity (v sin i)4.9±1.0[2] km/s
Other designations
Gaia DR2 2129931456691176576, KOI-277, KIC 11401755, 2MASS J19250004+4913545[4]
Database references
SIMBADdata
KICdata

Kepler-36 is a star in the constellation of Cygnus with two known planets. It has an anomalously large radius, meaning that it is a subgiant.

Planetary system

On June 21, 2012, the discovery of two planets orbiting the star was announced. The planets, a super-Earth and a "mini-Neptune", are unusual in that they have very close orbits; their semi-major axes differ by only 0.013 AU. The outer planet orbits only 11% further than the inner one. Coupled with masses significantly higher than Earth, their gravitational influence to each other is significant, meaning that their interaction causes extreme transit timing variations for both. Kepler-36b and c have estimated densities of 6.8 and 0.86 g/cm3, respectively.[2] The two planets are close to a 7:6 orbital resonance.[2] The large difference in densities, despite the close proximity of the planets' orbits, is likely due to the large difference in mass.[5] The innermost and less massive planet likely lost most, or all, of the hydrogen/helium envelope acquired during formation.

The Kepler-36 planetary system[2][3]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b 3.83+0.11
−0.10
 M
0.1153 13.86821±0.00049 <0.04 90.0° 1.498+0.061
−0.049
 R
c 7.13±0.18 M 0.1283 16.21865±0.00010 <0.04 90.0° 3.679+0.096
−0.091
 R

References

  1. 1.0 1.1 1.2 1.3 1.4 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.
  2. 2.0 2.1 2.2 2.3 2.4 2.5 2.6 2.7 2.8 Carter, J. A. et al. (2012). "Kepler-36: A Pair of Planets with Neighboring Orbits and Dissimilar Densities". Science 337 (6094): 556–559. doi:10.1126/science.1223269. PMID 22722249. Bibcode2012Sci...337..556C. 
  3. 3.0 3.1 Vissapragada, Shreyas et al. (2020). "Diffuser-assisted Infrared Transit Photometry for Four Dynamically Interacting Kepler Systems". The Astronomical Journal 159 (3): 108. doi:10.3847/1538-3881/ab65c8. Bibcode2020AJ....159..108V. 
  4. "Kepler-36". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=Kepler-36. 
  5. Bodenheimer, P.; Stevenson, D.; Lissauer, J.; D'Angelo, G. (2018). "New Formation Models for the Kepler-36 System". The Astrophysical Journal 868 (2): id. 138 (17 pp.). doi:10.3847/1538-4357/aae928. Bibcode2018ApJ...868..138B. 

External links