Astronomy:TT Corvi

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Short description: Variable star in the constellation Corvus
TT Corvi
Observation data
Equinox J2000.0]] (ICRS)
Constellation Corvus[1]
Right ascension  12h 23m 18.867s[2]
Declination −11° 48′ 43.63″[2]
Apparent magnitude (V) 6.47 to 6.57[3]
Characteristics
Evolutionary stage AGB[4]
Spectral type M3III[3]
Variable type semiregular[3]
Astrometry
Radial velocity (Rv)−0.17±0.15[2] km/s
Proper motion (μ) RA: −51.390[2] mas/yr
Dec.: −10.877[2] mas/yr
Parallax (π)3.2721 ± 0.0484[2] mas
Distance1,000 ± 10 ly
(306 ± 5 pc)
Absolute magnitude (MV)−0.75[1]
Details
Mass1.7[2] M☉
Radius80[5] R☉
Luminosity859[2] L☉
Surface gravity (log g)1.39[6] cgs
Temperature3,606[5] K
Age287[6] Myr
Other designations
TT Crv, HD 107814, HIP 60421[4]
Database references
SIMBADdata
A visual band light curve for TT Corvi, plotted from ASAS data[7]

TT Corvi (TT Crv) is a semiregular variable star in the constellation Corvus. It is a red giant of spectral type M3III and average apparent magnitude 6.48 around 923 light years distant.[8] It shines with a luminosity approximately 993 times that of the Sun and has a surface temperature of 3,630 K.[9]

References

  1. ↑ 1.0 1.1 Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters 38 (5): 331. doi:10.1134/S1063773712050015. Bibcode: 2012AstL...38..331A  XHIP record for this object at VizieR.
  2. ↑ 2.0 2.1 2.2 2.3 2.4 2.5 2.6 2.7 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940  Gaia DR3 record for this source at VizieR.
  3. ↑ 3.0 3.1 3.2 Samus', N. N.; Kazarovets, E. V.; Durlevich, O. V.; Kireeva, N. N.; Pastukhova, E. N. (2017). "General catalogue of variable stars: Version GCVS 5.1". Astronomy Reports 61 (1): 80. doi:10.1134/S1063772917010085. Bibcode: 2017ARep...61...80S. 
  4. ↑ 4.0 4.1 "TT Corvi". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=TT+Corvi. 
  5. ↑ 5.0 5.1 Stassun, Keivan G. et al. (2019). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal 158 (4): 138. doi:10.3847/1538-3881/ab3467. Bibcode: 2019AJ....158..138S. 
  6. ↑ 6.0 6.1 Kordopatis, G.; Schultheis, M.; McMillan, P. J.; Palicio, P. A.; De Laverny, P.; Recio-Blanco, A.; Creevey, O.; Álvarez, M. A. et al. (2023). "Stellar ages, masses, extinctions, and orbital parameters based on spectroscopic parameters of Gaia DR3". Astronomy and Astrophysics 669: A104. doi:10.1051/0004-6361/202244283. Bibcode: 2023A&A...669A.104K. 
  7. ↑ "ASAS All Star Catalogue". The All Sky Automated Survey. http://www.astrouw.edu.pl/asas/?page=aasc. 
  8. ↑ Tabur, V.; Bedding, T. R. (2009). "Long-term photometry and periods for 261 nearby pulsating M giants". Monthly Notices of the Royal Astronomical Society 400 (4): 1945–61. doi:10.1111/j.1365-2966.2009.15588.x. Bibcode: 2009MNRAS.400.1945T. 
  9. ↑ McDonald, I.; Zijlstra, A. A.; Boyer, M. L. (2012). "Fundamental Parameters and Infrared Excesses of Hipparcos Stars". Monthly Notices of the Royal Astronomical Society 427 (1): 343–57. doi:10.1111/j.1365-2966.2012.21873.x. Bibcode: 2012MNRAS.427..343M.