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Mu Canis Majoris

Mu Canis Majoris

Lokasi μ Canis Majoris (dilingkari)
Data pengamatan
Epos J2000.0      Ekuinoks J2000.0 (ICRS)
Rasi bintang Canis Major
Asensio rekta  06j 56m 06,64589d[1]
Deklinasi  −14° 02′ 36,3520″[1]
Magnitudo tampak (V) 5,12 (5,27 + 7,32)[2]
Ciri-ciri
Kelas spektrum K2/3 III + B9/A0 V[3]
Astrometri
Kecepatan radial (Rv)18,1±0,1[4] km/s
Gerak diri (μ) RA: −1,59[1] mdb/thn
Dek.: + 6,33[1] mdb/thn
Paralaks (π)2,62±0,58[1] mdb
Jaraksekitar 1.200 tc
(sekitar 380 pc)
Magnitudo mutlak (MV)−2,22[5]
Detail
μ CMa A
Gravitasi permukaan (log g)2489[6]
Suhu4441[6] K
Kecepatan rotasi (v sin i)≤ 5[7] km/s
μ CMa B
Massa14,7±0,3[8] M
Usia11,6±0,5[8] megatahun
Penamaan lain
μ CMa, 18 CMa, BD−13° 1741, HIP 33345, HR 2593, SAO 152123
Referensi basis data
SIMBADdata

Mu Canis Majoris (μ CMa / μ Canis Majoris) adalah salah satu bintang di rasi Canis Major.

μ Canis Majoris memiliki magnitudo tampak 5,12.[2] Bintang ini berada pada jarak 1200 tahun cahaya dari Matahari.[1]

Etimologi

Bintang ini memiliki nama tradisional Isis yang merupakan nama salah satu dewi Mesir Kuno.

Pada Almagest, bintang ini disebut sebagai quae in capite, berarti "yang berada di kepala (sang anjing besar)".[9]

Referensi

  1. ^ a b c d e f van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv:0708.1752alt=Dapat diakses gratis, Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357. 
  2. ^ a b Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society, 389 (2): 869–879, arXiv:0806.2878alt=Dapat diakses gratis, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x. 
  3. ^ Houk, Nancy; Smith-Moore, M. (1978), Michigan catalogue of two-dimensional spectral types for the HD stars, 4, Ann Arbor: Dept. of Astronomy, University of Michigan, Bibcode:1988MSS...C04....0H. 
  4. ^ 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:1208.3048alt=Dapat diakses gratis, Bibcode:2012A&A...546A..61D, doi:10.1051/0004-6361/201219219, A61. 
  5. ^ Ginestet, N.; Carquillat, J. M. (2002), "Spectral Classification of the Hot Components of a Large Sample of Stars with Composite Spectra, and Implication for the Absolute Magnitudes of the Cool Supergiant Components", The Astrophysical Journal Supplement Series, 143 (2): 513, Bibcode:2002ApJS..143..513G, doi:10.1086/342942. 
  6. ^ a b 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:1208.2037alt=Dapat diakses gratis, Bibcode:2012MNRAS.427..343M, doi:10.1111/j.1365-2966.2012.21873.x. 
  7. ^ Eaton, J. A. (May 1990), "Rotational Velocities of G and K Giants", Information Bulletin on Variable Stars, 3460: 1, Bibcode:1990IBVS.3460....1E. 
  8. ^ a b Tetzlaff, N.; et al. (January 2011), "A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun", Monthly Notices of the Royal Astronomical Society, 410 (1): 190–200, arXiv:1007.4883alt=Dapat diakses gratis, Bibcode:2011MNRAS.410..190T, doi:10.1111/j.1365-2966.2010.17434.x. 
  9. ^ http://www.atlascoelestis.com/alsufi%2038.htm
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