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Draft:Kepler-1972

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Kepler-1972
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Lyra
Right ascension 19h 13m 34.8691s
Declination 19° 11′ 54.011″
Characteristics
Astrometry
Proper motion (μ) RA: −3.723 mas/yr
Dec.: −13.766 mas/yr
Details
Mass1.18 M
Radius1.12 R
Temperature5,818 K
Rotation11.12 days
Rotational velocity (v sin i)5.04 km/s
Age~5 Gyr
Other designations
KOI-3184
Database references
SIMBADdata

Kepler-1972 or KOI-3184 is a G-type main sequence Sun-like star located 923 light years away from Earth in the constellation of Lyra.

Characteristics

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Mass, gravity and radius

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Its solar mass is 1.18, the solar radius is 1.12 and its gravity is roughly 4.46 cgs[clarification needed].

Temperature

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Its spectral class is classified as G1V, it would be assumed for its temperature is 5,818 Kelvin.[1]

Planetary system

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Kepler-1972 has 2 exoplanets orbiting it. These planets are suspected since 2022, for their same mass and radius and their temperature is higher due to their being closest to its host star. The discovery by A. Leleu with transmit method.[1]

The Kepler-1972 planetary system
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b 0.0064±0.0019 MJ 7.54425±0.00054 0 0.072±0.004 RJ
c 0.0066±0.0020 MJ 11.3295±0.0011 0 0.078±0.005 RJ

References

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  1. ^ a b Leleu, A.; Delisle, J. -B.; Mardling, R.; Udry, S.; Chatel, G.; Alibert, Y.; Eggenberger, P. (2022). "Alleviating the transit timing variation bias in transit surveys. II. RIVERS: Twin resonant Earth-sized planets around Kepler-1972 recovered from a Kepler false positive". Astronomy and Astrophysics. 661: A141. arXiv:2201.11459. Bibcode:2022A&A...661A.141L. doi:10.1051/0004-6361/202142822.

Category:Planetary systems with one confirmed planet Category:G-type main-sequence stars 110113 061820 Category:Durchmusterung objects Category:Lyra 0755