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词条 Alpha Chamaeleontis
释义

  1. References

{{Starbox begin
| name = α Chamaeleontis
}}{{Starbox observe
| epoch = J2000.0
| equinox = J2000.0 (ICRS)
| constell = Chamaeleon
| ra = {{RA|08|18|31.55319}}
| dec = {{DEC|−76|55|10.9964}}
| appmag_v = 4.06[3]
}}{{Starbox character
| class = {{nowrap|F5 V Fe-0.8}}[4]
| b-v = +0.40[3]
| u-b = −0.04[3]
| r-i =
| variable =
}}{{Starbox astrometry
| radial_v =
| prop_mo_ra = −0.13
| prop_mo_dec = +6.89
| parallax = 51.12
| p_error = 0.12
| parallax_footnote =
| absmag_v = +2.59[10]
}}{{Starbox detail
| mass = 1.42[11]
| radius =
| luminosity = 7.64[12]
| temperature = {{Val|6776|230|fmt=commas}}[11]
| gravity = {{Val|4.28|0.14}}[11]
| metal_fe = −0.26[4]
| rotational_velocity = 0[16]
| rotation =
| age_gyr = 1.8[11]
}}{{Starbox catalog
| names = α Cha, CPD−76° 507, Gliese 305, HD 71243, HIP 40702, HR 3318, SAO 256496.[18]
}}{{Starbox reference
| Simbad=alf+Cha
}}{{starbox end}}

Alpha Chamaeleontis, Latinized from α Chamaeleontis, is a solitary[19] star in the southern circumpolar constellation of Chamaeleon. It has an apparent visual magnitude of 4.06[3] and thus is bright enough to be seen with the naked eye. With an annual parallax shift of 51.12 mas, it is located 63.8 light years from the Sun.

This is an F-type main sequence star with a stellar classification of {{nowrap|F5 V Fe−0.8}},[4] where 'Fe−0.8' indicates an anomalously low abundance of iron. It has an estimated 1.4 times the mass of the Sun,[11] and radiates 7.64[12] times the solar luminosity from its outer atmosphere at an effective temperature of 6,776 K.[11] The star is around 1.8[11] billion years old with a projected rotational velocity that is too low to be measured.[16] The star has been examined for an infrared excess that would suggest the presence of an orbiting debris disk, but none was found.[28]

References

1. ^{{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=. }}
2. ^{{citation | last1=Eggleton | first1=P. P. | last2=Tokovinin | first2=A. A. | title=A catalogue of multiplicity among bright stellar systems | journal=Monthly Notices of the Royal Astronomical Society | volume=389 | issue=2 | pages=869–879 | date=September 2008 | doi=10.1111/j.1365-2966.2008.13596.x | bibcode=2008MNRAS.389..869E | arxiv=0806.2878 | postscript=. }}
3. ^{{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 | issue=1 | pages=343–57 | date=2012 | bibcode=2012MNRAS.427..343M | arxiv=1208.2037 | doi=10.1111/j.1365-2966.2012.21873.x | postscript=. }}
4. ^{{citation | title=The Collisional Evolution of Debris Disks | display-authors=1 | last1=Gáspár | first1=András | last2=Rieke | first2=George H. | last3=Balog | first3=Zoltán | journal=The Astrophysical Journal | volume=768 | issue=1 | id=25 | pages=29 | date=May 2013 | doi=10.1088/0004-637X/768/1/25 | bibcode=2013ApJ...768...25G | arxiv=1211.1415 | postscript=. }}
5. ^{{citation | last1=David | first1=Trevor J. | last2=Hillenbrand | first2=Lynne A. | title=The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets | journal=The Astrophysical Journal | volume=804 | issue=2 | pages=146 | year=2015 | bibcode=2015ApJ...804..146D | doi=10.1088/0004-637X/804/2/146 | arxiv=1501.03154 | postscript=. }}
6. ^{{citation | last1=Gray | first1=R. O. | last2=Corbally | first2=C. J. | last3=Garrison | first3=R. F. | last4=McFadden | first4=M. T. | last5=Bubar | first5=E. J. | last6=McGahee | first6=C. E. | last7=O'Donoghue | first7=A. A. | last8=Knox | first8=E. R. | title=Contributions to the Nearby Stars (NStars) Project: spectroscopy of stars earlier than M0 within 40 pc-The Southern Sample | journal=The Astronomical Journal | display-authors=1 | volume=132 | issue=1 | pages=161–70 | date=2006 | doi=10.1086/504637 | bibcode=2006AJ....132..161G | arxiv=astro-ph/0603770 | postscript=. }}
7. ^{{citation | last1=Uesugi | first1=Akira | last2=Fukuda | first2=Ichiro | title=Catalogue of rotational velocities of the stars | journal=Contributions from the Institute of Astrophysics and Kwasan Observatory | date=1970 | publisher=University of Kyoto | bibcode=1970crvs.book.....U | postscript=. }}
8. ^{{citation | last1=Mermilliod | first1=J.-C. | title=Compilation of Eggen's UBV data, transformed to UBV (unpublished) | publisher=SIMBAD | postscript=. | date=1986 | bibcode=1986EgUBV........0M }}
9. ^{{cite simbad | title=alf Cha | accessdate=2016-12-10 | postscript=. }}
[1][2][3][4][5][6][7][8][9]
}}{{Stars of Chamaeleon|state=collapsed}}

8 : F-type main-sequence stars|Chamaeleon (constellation)|Bayer objects|Durchmusterung objects|Henry Draper Catalogue objects|Hipparcos objects|HR objects|Gliese and GJ objects

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