Alpha Chamaeleontis
Voorkoms
| Alpha Chamaeleontis
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| Alpha Chamaeleontis se posisie (in die rooi sirkel). | ||||
| Sterrebeeld | Kameleon | |||
| Spektraaltipe | F5 V Fe-0.8[1] | |||
| Soort | Hoofreeksster | |||
| Waarnemingsdata (Epog J2000) | ||||
| Regte klimming | 08h 18m 31.55319s[2] | |||
| Deklinasie | -76° 55′ 10.9964″[2] | |||
| Skynmagnitude (m) | 4,06[3] | |||
| Absolute magnitude (M) | +2,59[4] | |||
| B-V-kleurindeks | +0,40[3] | |||
| U-B-kleurindeks | -0,04[3] | |||
| Besonderhede | ||||
| Massa (M☉) | 1,42[5] | |||
| Ligsterkte (L☉) | 7,64[6] | |||
| Ouderdom (jaar) | 1,8 miljard[5] | |||
| Temperatuur (K) | 6 776[5] | |||
| Rotasiespoed (km/s) | 0[7] | |||
| Metaalinhoud [Fe/H] | -0,26[1] | |||
| Ander name | ||||
| α Cha, CPD−76° 507, Gliese 305, HD 71243, HIP 40702, HR 3318, SAO 256496 | ||||
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Alpha Chamaeleontis (afgekort as α Cha) is die helderste ster in die suidelike sirkumpolêre sterrebeeld Kameleon (Chamaeleon). Dit het ’n skynbare magnitude van 4,06[3] en kan dus met die blote oog gesien word. Dit is 63,8 ligjare van die Son af.
α Cha is ’n F-tipe hoofreeksster met ’n klassifikasie van F5 V Fe-0,8,[1] waar "Fe-0,8" ’n onreëlmatige lae voorkoms van yster aandui. Sy massa is 1,4 keer dié van die Son[5] en sy ligsterkte 7,64 keer[6] die Son s’n. Sy effektiewe temperatuur is 6 776 K.[5] Die ster is sowat 1,8 miljard jaar oud[5] en het ’n rotasiespoed wat te laag is om te meet.[7]
Verwysings
[wysig | wysig bron]- 1 2 3 Gray, R. O.; et al. (2006), "Contributions to the Nearby Stars (NStars) Project: spectroscopy of stars earlier than M0 within 40 pc-The Southern Sample", The Astronomical Journal, 132 (1): 161-70, arXiv:astro-ph/0603770, Bibcode:2006AJ....132..161G, doi:10.1086/504637.
- 1 2 van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653-664, arXiv:0708.1752, Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357.
- 1 2 3 4 Mermilliod, J.-C. (1986), Compilation of Eggen's UBV data, transformed to UBV (unpublished), SIMBAD, Bibcode:1986EgUBV........0M.
- ↑ 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.
- 1 2 3 4 5 6 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.
- 1 2 McDonald, I.; et al. (2012), "Fundamental Parameters and Infrared Excesses of Hipparcos Stars", Monthly Notices of the Royal Astronomical Society, 427 (1): 343-57, arXiv:1208.2037, Bibcode:2012MNRAS.427..343M, doi:10.1111/j.1365-2966.2012.21873.x.
- 1 2 Uesugi, Akira; Fukuda, Ichiro (1970), "Catalogue of rotational velocities of the stars", Contributions from the Institute of Astrophysics and Kwasan Observatory, University of Kyoto, Bibcode:1970crvs.book.....U.
Eksterne skakels
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Hierdie artikel is vertaal uit die Engelse Wikipedia