TU Corvi
{{Short description|Star in the constellation Corvus}}
{{Starbox begin
| name = TU Corvi
}}
{{Starbox image
| image = 250px
| caption = A light curve for TU Corvi, plotted from TESS data
}}
{{Starbox observe
| epoch = J2000
| constell = Corvus
| dec = {{DEC|-20|31|38.9160}}
}}
{{Starbox character
| type =
| u-b =
| variable = δ Sct
}}
{{Starbox astrometry
| parallax = 13.2558
| p_error = 0.3343
}}
{{Starbox detail
| source =
| luminosity = {{Val|12.6|1.2|1.1}}
| temperature = {{Val|7132|242|fmt=commas}}
| metal_fe = {{Val|−0.07|0.07}}
}}
{{Starbox catalog
| names={{odlist | V=TU Crv | BD=−19°3521 | HD=109585 | HIP=61496 | HR=4797 | SAO=180937 | AAVSO=1230-19 }}
}}
{{Starbox reference
| Simbad = V*+TU+Crv
}}
{{Starbox end}}
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. The distance to this star can be estimated from its annual parallax shift of {{Val|13.3|ul=mas}}, yielding a range of about 246 light years. Based upon measured changes in its proper motion, it may be a close binary system.
This is an F-type main-sequence star with a stellar classification of F0 V. Previously it had been classed as F0 III, 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. At the age of 786 million years, it has a high rate of spin with a projected rotational velocity of 103 km/s. 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.
References
{{reflist|refs=
{{cite simbad | title=TU Crv | access-date=30 August 2018 }}
{{cite Gaia DR3|3515324014724705664}}
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| url=https://mast.stsci.edu/portal/Mashup/Clients/Mast/Portal.html
| publisher=Space Telescope Science Institute |access-date=8 December 2021}}
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| doi=10.3847/0004-637X/826/2/171 | bibcode=2016ApJ...826..171G | arxiv=1604.07403 | s2cid=119241004 | doi-access=free }}
| title=TU Corvi | last1=Watson | first1=Christopher
| date=4 January 2010 | work=The International Variable Star Index
| publisher=American Association of Variable Star Observers
| url=http://www.aavso.org/vsx/index.php?view=detail.top&oid=10698
| accessdate=21 July 2015 }}
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| doi=10.1088/0004-637X/804/2/146
| arxiv=1501.03154 | bibcode=2015ApJ...804..146D | s2cid=33401607 }}
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| volume=537 | pages=A120 | year=2012
| bibcode=2012A&A...537A.120Z |arxiv=1201.2052
| doi=10.1051/0004-6361/201117691 | s2cid=55586789
}}
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| doi=10.1051/0004-6361/201219219
| bibcode=2012A&A...546A..61D | arxiv=1208.3048 | s2cid=59451347 }}
| title=General catalogue of variable stars: Version GCVS 5.1
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| volume=61 | issue=1 | pages=80 | year=2017
| doi=10.1134/S1063772917010085 | bibcode=2017ARep...61...80S | s2cid=125853869 }}
| title=Speckle Interferometry of New and Problem HIPPARCOS Binaries
| journal=The Astronomical Journal | display-authors=1
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| volume=117 | issue=4 | pages=1890 | year=1999
| doi=10.1086/300823 | bibcode=1999AJ....117.1890M | doi-access=free }}
{{cite journal | display-authors=1
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| title=A study of the bright A stars. I. A catalogue of spectral classifications
| journal=Astronomical Journal
| volume=74 | pages=375–406 | date=April 1969
| doi=10.1086/110819 | bibcode=1969AJ.....74..375C }}
}}
{{Stars of Corvus}}
Category:F-type main-sequence stars
Category:Delta Scuti variables
Category:Corvus (constellation)