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Ross 47

Coordinates: Sky map 05h 42m 09.26772s, +12° 29′ 21.6225″
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Ross 47
Observation data
Epoch J1950.0      Equinox J1950.0
Constellation Orion
Right ascension 05h 42m 09.26772s[1]
Declination +12° 29′ 21.6225″[1]
Apparent magnitude (V) +11.509[2]
Characteristics
Spectral type M4.0Vn
U−B color index +14.264
B−V color index +13.130
Variable type BY Dra[2]
Astrometry
Radial velocity (Rv)105.83 ± 0.18 km/s
Proper motion (μ) RA: 2000.53[1] mas/yr
Dec.: −1569.63[1] mas/yr
Parallax (π)172.6762 ± 0.0286 mas[3]
Distance18.888 ± 0.003 ly
(5.7912 ± 0.0010 pc)
Absolute magnitude (MV)+12.75
Details[4]
Mass0.35 M
Radius0.17 R
Luminosity0.00069 L
Temperature3026±100 K
Metallicity [Fe/H]-0.19±0.17 dex
Other designations
V1352 Ori, Gaia DR2 3340477717172813568, GJ 213, HIP 26857, Ci 20 344, G 102-22, LFT 425, LHS 31, LTT 11704, NLTT 15489, Ross 47, TYC 722-455-1, 2MASS J05420897+1229252[2]
Database references
SIMBADdata
Ross 47 is located in the constellation Orion
Ross 47 is located in the constellation Orion
Ross 47
Location of Ross 47 in the constellation Orion

Ross 47 is a flare star of spectral type M4 located in the constellation Orion, 19 light-years from Earth.[1]

References

  1. ^ a b c d e van Leeuwen, F.; et al. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. S2CID 18759600.
  2. ^ a b c "Ross 47". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 16 February 2021.
  3. ^ Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv:2012.01533. Bibcode:2021A&A...649A...1G. doi:10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
  4. ^ Antoniadis-Karnavas, A.; Sousa, S. G.; Delgado-Mena, E.; Santos, N. C.; Teixeira, G. D. C.; Neves, V. (2020), "ODUSSEAS: A machine learning tool to derive effective temperature and metallicity for M dwarf stars", Astronomy & Astrophysics, 636: A9, arXiv:2002.09367, Bibcode:2020A&A...636A...9A, doi:10.1051/0004-6361/201937194, S2CID 211252698