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词条 HD 75710
释义

  1. References

{{Starbox begin
| name = HD 75710
}}{{Starbox observe
| epoch = J2000
| constell = Vela
| ra = {{RA|08|49|47.63746}}[1]
| dec = {{DEC|−45|18|28.3346}}[1]
| appmag_v = 4.94[3]
}}{{Starbox character
| class = A2 III[4]
| b-v = {{Val|+0.043|0.003}}[3]
}}{{Starbox astrometry
| radial_v = {{Val|+5.0|7.4}}[6]
| prop_mo_ra = −11.490[1]
| prop_mo_dec = +13.450[1]
| parallax = 2.7107
| p_error = 0.1660
| parallax_footnote = [1]
| absmag_v = −2.71[3]
}}{{Starbox detail
| source =
| mass =
| radius =
| luminosity = 914.04[11]
| gravity =
| temperature = 8,150[11]
| metal_fe =
| rotational_velocity = 110[13]
| age_myr =
}}{{Starbox catalog
| names={{odlist | B=g Vel | CD=−44° 4861 | CPD−44° 3126 | FK5=2698 | HD=75710 | HIP=43347 | HR=3520 | SAO=220540 | GC=12204 | PPM=313660 }}
}}{{Starbox reference
| Simbad = HD+75710
}}{{Starbox end}}

HD 75710 is a single[15] star in the constellation of Vela. It has an apparent visual magnitude of approximately 4.94,[3] which is bright enough to be faintly visible to the naked eye. Based upon an annual parallax shift of {{Val|2.7|ul=mas}},[1] it is located about 1,200 light years from the Sun.

The stellar classification of this star is A2 III,[4] suggesting it is in the giant star stage of its stellar evolution. It has a high rate of spin with a projected rotational velocity of 110 km/s, which is giving the star an oblate shape with an equatorial bulge that is 7% larger than the polar radius.[13] HD 75710 is radiating 914 times the Sun's luminosity from its photosphere at an effective temperature of 8,150 K.[11]

References

1. ^{{cite DR2}}
2. ^{{citation | title=XHIP: An extended hipparcos compilation | last1=Anderson | first1=E. | last2=Francis | first2=Ch. | journal=Astronomy Letters | volume=38 | issue=5 | pages=331 | year=2012 | bibcode=2012AstL...38..331A | doi=10.1134/S1063773712050015 | arxiv=1108.4971 | postscript=. }}
3. ^{{citation | last1=Houk | first1=Nancy | title=Michigan catalogue of two-dimensional spectral types for the HD stars | volume=2 | publication-place=Ann Arbor | publisher=Dept. of Astronomy, University of Michigan | year=1978 | bibcode=1978mcts.book.....H | postscript=. }}
4. ^{{citation | title=A catalogue of multiplicity among bright stellar systems | last1=Eggleton | first1=P. P. | last2=Tokovinin | first2=A. A. | journal=Monthly Notices of the Royal Astronomical Society | volume=389 | issue=2 | pages=869 | date=2008 | doi=10.1111/j.1365-2966.2008.13596.x | arxiv=0806.2878 | bibcode=2008MNRAS.389..869E | postscript=. }}
5. ^{{citation | title=Interferometric observations of rapidly rotating stars | last1=Belle | first1=G. T. | journal=The Astronomy and Astrophysics Review | volume=20| page=51 | year=2012 | doi=10.1007/s00159-012-0051-2 | bibcode=2012A&ARv..20...51V | arxiv=1204.2572 | postscript=. }}
6. ^{{citation | last1=de Bruijne | first1=J. H. J. | last2=Eilers | first2=A.-C. | title=Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project | journal=Astronomy & Astrophysics | volume=546 | id=A61 | pages=14 | date=October 2012 | doi=10.1051/0004-6361/201219219 | bibcode=2012A&A...546A..61D | arxiv=1208.3048 | postscript=. }}
7. ^{{citation | display-authors=1 | last1=McDonald | first1=I. | last2=Zijlstra | first2=A. A. | last3=Boyer | first3=M. L. | title=Fundamental parameters and infrared excesses of Hipparcos stars | journal=Monthly Notices of the Royal Astronomical Society | volume=427 | pages=343 | year=2012 | doi=10.1111/j.1365-2966.2012.21873.x | bibcode=2012MNRAS.427..343M | arxiv=1208.2037 | postscript=. }}
[1][2][3][4][5][6][7]
}}{{Stars of Vela}}

7 : A-type giants|Vela (constellation)|Bayer objects|Durchmusterung objects|Henry Draper Catalogue objects|Hipparcos objects|HR objects

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