HD 142245

HD 142245
Observation data
Epoch J2000      Equinox J2000
Constellation Serpens
Right ascension 15h 52m 56.2803s[1]
Declination +15° 25′ 50.5399″[1]
Apparent magnitude (V) 7.45
Characteristics
Evolutionary stage subgiant
Spectral type K0IV+M1[2]
Astrometry
Radial velocity (Rv)6.92 km/s
Proper motion (μ) RA: -57.477 mas/yr
Dec.: -21.764 mas/yr
Parallax (π)10.2562 ± 0.0411 mas[3]
Distance318 ± 1 ly
(97.5 ± 0.4 pc)
Orbit
PrimaryHD 142245 A
CompanionHD 142245 BC
Semi-major axis (a)2.5"
(237 AU[4])
Details[5]
HD 142245 A
Mass1.52±0.05[2] M☉
Radius4.8±0.1[6] R☉
Luminosity11.4[6] L☉
Surface gravity (log g)3.21±0.14 cgs
Temperature4838±36[7] K
Metallicity0.20±0.02[7]
Age2.855±0.514 Gyr
HD 142245 BC
Mass0.56[4] M☉
Other designations
BD+15 2925, Gaia DR2 1193193836691820032, HD 142245, HIP 77783, TYC 1496-1841-1, 2MASS J15525629+1525507[1]
Database references
SIMBADdata

HD 142245 is a hierarchical triple star system about 318 light-years away.

The primary subgiant star HD 142245 A belongs to the spectral class of K0. Its age is much younger than Sun`s at 2.855±0.514 billion years.[7] The primary star is slightly enriched by heavy elements, having 160% of solar abundance.[7]

In 2014, the co-moving binary stellar companion HD 142245 BC was detected. It consists of pair of red dwarf stars with composite spectral class M1, orbiting each other on 4 AU orbit.[4]

No other stellar companions were found at projected separations from 5.48 to 153.34 AU around HD 142245 A.[2]

  1. ^ a b c Cite error: The named reference SIMBAD was invoked but never defined (see the help page).
  2. ^ a b c Wittrock, Justin M.; Kane, Stephen R.; Horch, Elliott P.; Howell, Steve B.; Ciardi, David R.; Everett, Mark E. (2017), "Exclusion of Stellar Companions to Exoplanet Host Stars", The Astronomical Journal, 154 (5): 184, arXiv:1709.05315, Bibcode:2017AJ....154..184W, doi:10.3847/1538-3881/aa8d69, S2CID 55789971
  3. ^ Cite error: The named reference GaiaDR2 was invoked but never defined (see the help page).
  4. ^ a b c M. Mugrauer, C. Ginski, "High-contrast imaging search for stellar and substellar companions of exoplanet host stars", 2014
  5. ^ Sousa, S. G.; Adibekyan, V.; Delgado-Mena, E.; Santos, N. C.; Andreasen, D. T.; Ferreira, A. C. S.; Tsantaki, M.; Barros, S. C. C.; Demangeon, O.; Israelian, G.; Faria, J. P.; Figueira, P.; Mortier, A.; Brandao, I.; Montalto, M.; Rojas-Ayala, B.; Santerne, A. (2018), "SWEET-Cat updated New homogenous spectroscopic parameters", Astronomy & Astrophysics, A58: 620, arXiv:1810.08108, Bibcode:2018A&A...620A..58S, doi:10.1051/0004-6361/201833350, S2CID 119374557
  6. ^ a b Bonfanti, A.; Ortolani, S.; Piotto, G.; Nascimbeni, V. (2015), "Revising the ages of planet-hosting stars", Astronomy & Astrophysics, 575: A18, arXiv:1411.4302, Bibcode:2015A&A...575A..18B, doi:10.1051/0004-6361/201424951, S2CID 54555839
  7. ^ a b c d Ghezzi, Luan; Montet, Benjamin T.; Johnson, John Asher (2018), "Retired a Stars Revisited: An Updated Giant Planet Occurrence Rate as a Function of Stellar Metallicity and Mass", The Astrophysical Journal, 860 (2): 109, arXiv:1804.09082, Bibcode:2018ApJ...860..109G, doi:10.3847/1538-4357/aac37c, S2CID 118969017