Kepler-46

Kepler-46

Artist's conception of the Kepler-46 system showing the two planets. Planet b transits its star, the same method by which it was detected.
Observation data
Epoch J2000      Equinox J2000
Constellation Lyra
Right ascension 19h 17m 04.4930s[1]
Declination 42° 36′ 15.041″[1]
Characteristics
Apparent magnitude (J) 13.814[2]
Apparent magnitude (H) 13.436[2]
Apparent magnitude (K) 13.347[2]
Astrometry
Proper motion (μ) RA: 3.101(24) mas/yr[1]
Dec.: 0.864(27) mas/yr[1]
Parallax (π)1.2963 ± 0.0225 mas[1]
Distance2,520 ± 40 ly
(770 ± 10 pc)
Absolute bolometric
magnitude
 (Mbol)
5.18 (predicted)[note 1]
Details
Mass0.902+0.040
−0.038
[3] M
Radius0.938+0.038
−0.039
[3] R
Temperature5155±150[3] K
Metallicity [Fe/H]0.41±0.10[3][note 2] dex
Rotation27.859±0.075 days[4]
Age9.7+3.7
−3.5
[3] Gyr
Other designations
Gaia DR2 2102700131386216576, KOI-872, KIC 7109675, 2MASS J19170449+4236150[2]
Database references
SIMBADdata
KICdata

Kepler-46, previously designated KOI-872, is a star located in the constellation Lyra. Observed since 2009 by the Kepler space observatory, it has since been found to possess a planetary system consisting of at least three planets and while it has a similar mass to the Sun (90%) it is significantly older at ten billion years.[3]

Kepler-46 b (previously KOI-872.01), was the first planet discovered in the system. It was found through detailed analysis of Kepler space observatory data. An additional planet, Kepler-46 c, was discovered by an outside group using Kepler public data through analysis of transit timing variations. While only one additional planet was confirmed by the analysis, the study revealed the potential existence of an unconfirmed planet KOI-872.03 (KOI-872 d).[5] Validation by the multiplicity method confirmed the existence of this planet which was then renamed Kepler-46d.

  1. ^ a b c d Cite error: The named reference Gaia DR3 was invoked but never defined (see the help page).
  2. ^ a b c d "Kepler-46". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved May 16, 2012.
  3. ^ a b c d e f Cite error: The named reference Saad-Olivera2017 was invoked but never defined (see the help page).
  4. ^ Cite error: The named reference McQuillan2013 was invoked but never defined (see the help page).
  5. ^ Cite error: The named reference Nesvorny2012 was invoked but never defined (see the help page).


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