HAT-P-12

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HAT-P-12
Observation data
Epoch J2000      Equinox J2000
Constellation Canes Venatici[1]
Right ascension 13h 57m 33.4669s[2]
Declination +43° 29′ 36.6025″[2]
Apparent magnitude (V) 12.84
Characteristics
Spectral type K5[3]
Apparent magnitude (J) 10.794 ±0.023[4]
Apparent magnitude (H) 10.236 ±0.022[4]
Apparent magnitude (K) 10.108 ±0.016[4]
Astrometry
Radial velocity (Rv)−40.4589±0.0023[5] km/s
Proper motion (μ) RA: −134.791±0.030[2] mas/yr
Dec.: −44.294±0.035[2] mas/yr
Parallax (π)6.9763 ± 0.0220[2] mas
Distance468 ± 1 ly
(143.3 ± 0.5 pc)
Absolute magnitude (MV)12.35 ± 0.23
Details[6]
Mass0.719±0.016 M
Radius0.7084±0.0095 R
Luminosity0.21+0.02
−0.01
[3] 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[3]
Age2.5 ± 2.0[3] Gyr
Other designations
Gaia DR2 1499514786891168640, GSC 03033-00706, 2MASS J13573347+4329367, SDSS J135733.42+432936.5[4]
Database references
SIMBADdata
Exoplanet Archivedata
Extrasolar Planets
Encyclopaedia
data
Data sources:
Hipparcos Catalogue,
CCDM (2002),
Bright Star Catalogue (5th rev. ed.)

HAT-P-12 is a magnitude 13 Metal-Poor K Dwarf star approximately 468 light years away in the constellation Canes Venatici.[3][2]

Planetary system[]

In 2009 an exoplanet, HAT-P-12b, was discovered by the HATNet Project orbiting this star. The planet was discovered using the transit method and confirmed by follow up radial velocity measurements.[3] Transit-timing variations suggest the possible presence of additional non-transiting planets in the system.[7]

The HAT-P-12 planetary system[3]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b 0.211 ± 0.012 MJ 0.0384 ± 0.0003 3.2130598 ± 0.000006 0 0.95+2.85
−0.02
 RJ
[7] (unconfirmed) 0.218 MJ 8.853 0.15499 73.5°

See also[]

  • List of extrasolar planets

References[]

  1. ^ Roman, Nancy G. (1987). "Identification of a Constellation From a Position". Publications of the Astronomical Society of the Pacific. 99 (617): 695–699. Bibcode:1987PASP...99..695R. doi:10.1086/132034.Vizier query form
  2. ^ a b c d e f Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
  3. ^ a b c d e f g Hartman, J. D.; et al. (2009). "HAT-P-12b: A Low-density sub-Saturn mass planet transiting a metal-poor K dwarf". The Astrophysical Journal. 706 (1): 785–796. arXiv:0904.4704. Bibcode:2009ApJ...706..785H. doi:10.1088/0004-637X/706/1/785. S2CID 14540643.
  4. ^ a b c d "HAT-P-12". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-12-19.
  5. ^ Mancini, L.; et al. (2018). "The GAPS programme with HARPS-N at TNG. XVI. Measurement of the Rossiter-McLaughlin effect of transiting planetary systems HAT-P-3, HAT-P-12, HAT-P-22, WASP-39, and WASP-60". Astronomy and Astrophysics. 613. Table C.2. arXiv:1802.03859. Bibcode:2018A&A...613A..41M. doi:10.1051/0004-6361/201732234.
  6. ^ Wang, Xian-Yu; et al. (1 July 2021). "Transiting Exoplanet Monitoring Project (TEMP). VI. The Homogeneous Refinement of System Parameters for 39 Transiting Hot Jupiters with 127 New Light Curves". The Astrophysical Journal Supplement Series. 255 (1). 15. arXiv:2105.14851. Bibcode:2021ApJS..255...15W. doi:10.3847/1538-4365/ac0835.
  7. ^ a b Sariya, Devesh P.; Jiang, Ing-Guey; Su, Li-Hsin; Yeh, Li-Chin; Chang, Tze-En; Moskvin, V. V.; Shlyapnikov, A. A.; Ignatov, V.; Mkrtichian, David; Griv, Evgeny; Mannaday, Vineet Kumar; Thakur, Parijat; Sahu, D. K.; Chand, Swadesh; Bisht, D.; Sun, Zhao; Ji, Jianghui (2021), "Non-sinusoidal transit timing variations for the exoplanet HAT-P-12b", Research in Astronomy and Astrophysics, 21 (4): 097, arXiv:2012.08820, doi:10.1088/1674-4527/21/4/97, S2CID 229188086

External links[]

Coordinates: Sky map 13h 57m 33s, +43° 29′ 37″

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