This page uses candidate pages for queue until Many Websites prove it existed by Google Chrome.
Kepler-1972 edit
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Lyra[1] |
Right ascension | 19h 13m 34.8691s |
Declination | 19° 11′ 54.011″ |
Apparent magnitude (V) | 10.063 |
Characteristics | |
Evolutionary stage | main-sequence star |
Spectral type | G1V |
Astrometry | |
Radial velocity (Rv) | 17.13 km/s |
Proper motion (μ) | RA: −3.723 mas/yr Dec.: −13.766 mas/yr |
Parallax (π) | 9.4499 ± 0.0158 mas |
Distance | 345.1 ± 0.6 ly (105.8 ± 0.2 pc) |
Details | |
Mass | 1.18 M☉ |
Radius | 1.12 R☉ |
Surface gravity (log g) | 11.1438 cgs |
Temperature | 5,818 K |
Rotation | 11.12 days |
Rotational velocity (v sin i) | 5.04 km/s |
Age | ~5 Gyr |
Other designations | |
KOI-3184 | |
Database references | |
SIMBAD | data |
Kepler-1972 or KOI-3184 is a G-Type main sequence Sun-like star located 923 light years away from Earth in Lyra Constellation. The discovery by A. Leleu with transmit method and published in Cornell University
Characteristics edit
Mass, gravity and radius edit
According to Cornell University, its solar mass is 1.18, the solar radius is 1.12 and its gravity is roughly 4.46 cgs[1]
Temperature edit
Its spectral class is classified as G1V, it would be assumed for its temperature is 5,818 Kelvin[1]
Planetary System edit
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.[1]
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 |