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TU Corvi
TUCrvLightCurve.png
A light curve for TU Corvi, plotted from TESS data [1]
Observation data
Epoch J2000       Equinox J2000
Constellation Corvus
Right ascension 12h 35m 58.79603s [2]
Declination −20° 31′ 38.9160″ [2]
Apparent magnitude (V) 6.20 [3]
Characteristics
Spectral type F0 V [4]
B−V color index 0.34±0.01 [3]
Variable type δ Sct [5] [6]
Astrometry
Radial velocity (Rv)−2.0±4.3 [7] km/s
Proper motion (μ) RA: +30.202 [2]  mas/ yr
Dec.: −51.280 [2]  mas/ yr
Parallax (π)13.2558 ± 0.3343  mas [2]
Distance246 ± 6  ly
(75 ± 2  pc)
Absolute magnitude (MV)2.08 [3]
Details
Mass1.45 [8]  M
Radius2.7 [2]  R
Luminosity12.6+1.2
−1.1
[8]  L
Surface gravity (log g)3.93±0.14 [8]  cgs
Temperature7,132±242 [8]  K
Metallicity [Fe/H]−0.07±0.07 [9]  dex
Rotational velocity (v sin i)103 [10] km/s
Age786 [8]  Myr
Other designations
TU Crv, BD−19°3521, HD 109585, HIP 61496, HR 4797, SAO 180937 [11]
Database references
SIMBAD data

TU Corvi is a yellow-white hued star in the southern constellation of Corvus. It is a dimly visible to the naked eye with an apparent visual magnitude of 6.20. [3] The distance to this star can be estimated from its annual parallax shift of 13.3  mas, yielding a range of about 246  light years. Based upon measured changes in its proper motion, it may be a close binary system. [12]

This is an F-type main-sequence star with a stellar classification of F0 V. [4] Previously it had been classed as F0 III, [13] matching an evolved giant star. It is a Delta Scuti variable, varying by an amplitude of 0.025 in B magnitude with a period of 118 minutes. [5] [6] At the age of 786 [8] million years, it has a high rate of spin with a projected rotational velocity of 103 km/s. [10] The star has 1.45 times the mass of the Sun and is radiating 12.6 times the Sun's luminosity from its photosphere at an effective temperature of 7,132 K. [8]

References

  1. ^ "MAST: Barbara A. Mikulski Archive for Space Telescopes". Space Telescope Science Institute. Retrieved 8 December 2021.
  2. ^ a b c d e f Vallenari, A.; et al. (Gaia Collaboration) (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. arXiv: 2208.00211. doi: 10.1051/0004-6361/202243940. Gaia DR3 record for this source at VizieR.
  3. ^ a b c d Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331. arXiv: 1108.4971. Bibcode: 2012AstL...38..331A. doi: 10.1134/S1063773712050015. S2CID  119257644.
  4. ^ a b Houk, Nancy; Smith-Moore, M. (1978). Michigan catalogue of two-dimensional spectral types for the HD stars. Vol. 4. Ann Arbor: Dept. of Astronomy, University of Michigan. Bibcode: 1988mcts.book.....H.
  5. ^ a b 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. Bibcode: 2017ARep...61...80S. doi: 10.1134/S1063772917010085. S2CID  125853869.
  6. ^ a b Watson, Christopher (4 January 2010). "TU Corvi". The International Variable Star Index. American Association of Variable Star Observers. Retrieved 21 July 2015.
  7. ^ de Bruijne, J. H. J.; Eilers, A.-C. (October 2012). "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project". Astronomy & Astrophysics. 546: 14. arXiv: 1208.3048. Bibcode: 2012A&A...546A..61D. doi: 10.1051/0004-6361/201219219. S2CID  59451347. A61.
  8. ^ a b c d e f g David, Trevor J.; Hillenbrand, Lynne A. (2015). "The Ages of Early-type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets". The Astrophysical Journal. 804 (2): 146. arXiv: 1501.03154. Bibcode: 2015ApJ...804..146D. doi: 10.1088/0004-637X/804/2/146. S2CID  33401607.
  9. ^ Gáspár, András; et al. (August 2016), "The Correlation between Metallicity and Debris Disk Mass", The Astrophysical Journal, 826 (2): 14, arXiv: 1604.07403, Bibcode: 2016ApJ...826..171G, doi: 10.3847/0004-637X/826/2/171, S2CID  119241004, 171
  10. ^ a b Zorec, J.; Royer, F. (2012). "Rotational velocities of A-type stars. IV. Evolution of rotational velocities". Astronomy & Astrophysics. 537: A120. arXiv: 1201.2052. Bibcode: 2012A&A...537A.120Z. doi: 10.1051/0004-6361/201117691. S2CID  55586789.
  11. ^ "TU Crv". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 30 August 2018.
  12. ^ Mason, Brian D.; et al. (1999). "Speckle Interferometry of New and Problem HIPPARCOS Binaries". The Astronomical Journal. 117 (4): 1890. Bibcode: 1999AJ....117.1890M. doi: 10.1086/300823.
  13. ^ Cowley, A.; et al. (April 1969). "A study of the bright A stars. I. A catalogue of spectral classifications". Astronomical Journal. 74: 375–406. Bibcode: 1969AJ.....74..375C. doi: 10.1086/110819.