HAT-P-12

HAT-P-12 is a magnitude 13 low-metallicity K dwarf star approximately 463 light years away in the constellation Canes Venatici, which hosts one known exoplanet.

HAT-P-12 / Komondor
Observation data
Epoch J2000      Equinox J2000
Constellation Canes Venatici
Right ascension 13h 57m 33.4669s
Declination +43° 29 36.602
Apparent magnitude (V) 12.84
Characteristics
Spectral type K5
Apparent magnitude (J) 10.794 ±0.023
Apparent magnitude (H) 10.236 ±0.022
Apparent magnitude (K) 10.108 ±0.016
Variable type planetary transit
Astrometry
Radial velocity (Rv)−40.4589±0.0023 km/s
Proper motion (μ) RA: −134.793(8) mas/yr
Dec.: −44.229(11) mas/yr
Parallax (π)7.0448 ± 0.0105 mas
Distance463.0 ± 0.7 ly
(141.9 ± 0.2 pc)
Absolute magnitude (MV)12.35 ± 0.23
Details
Mass0.719±0.016 M
Radius0.7084±0.0095 R
Luminosity0.21+0.02
0.01
 L
Surface gravity (log g)4.594±0.013 cgs
Temperature4710±49 K
Metallicity [Fe/H]−0.24+0.055
0.062
 dex
Rotation0.5 ± 0.4 kms−1
Age2.5 ± 2.0 Gyr
Other designations
Komondor, HAT-P-12, Gaia DR3 1499514786891168640, GSC 03033-00706, 2MASS J13573347+4329367, SDSS J135733.42+432936.5
Database references
SIMBADdata
Exoplanet Archivedata
Data sources:
Hipparcos Catalogue,
CCDM (2002),
Bright Star Catalogue (5th rev. ed.)
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