Mu Canis Majoris: Perbedaan antara revisi

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
Deklinasi	−14° 02′ 36,3520″
Magnitudo tampak (V)	5,12 (5,27 + 7,32)
Ciri-ciri
Kelas spektrum	K2/3 III + B9/A0 V
Astrometri
Kecepatan radial (Rv)	18,1±0,1 km/s
Gerak diri (μ)	RA: −1,59 mdb/thn ; Dek.: + 6,33 mdb/thn
Paralaks (π)	2,62±0,58 mdb
Jarak	sekitar 1.200 tc ; (sekitar 380 pc)
Magnitudo mutlak (MV)	−2,22
Detail
μ CMa A
Gravitasi permukaan (log g)	2489
Suhu	4441 K
Kecepatan rotasi (v sin i)	≤ 5 km/s
μ CMa B
Massa	14,7±0,3 M☉
Usia	11,6±0,5 megatahun
Penamaan lain
	μ CMa, 18 CMa, BD−13° 1741, HIP 33345, HR 2593, SAO 152123
Referensi basis data
SIMBAD	data

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Sebaris

Revisi terkini sejak 23 Mei 2018 21.25

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

^ ^a ^b ^c ^d ^e ^f van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv:0708.1752 , Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357.
^ ^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:0806.2878 , Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x.
^ 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.
^ 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:1208.3048 , Bibcode:2012A&A...546A..61D, doi:10.1051/0004-6361/201219219, A61.
^ 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.
^ ^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:1208.2037 , Bibcode:2012MNRAS.427..343M, doi:10.1111/j.1365-2966.2012.21873.x.
^ Eaton, J. A. (May 1990), "Rotational Velocities of G and K Giants", Information Bulletin on Variable Stars, 3460: 1, Bibcode:1990IBVS.3460....1E.
^ ^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:1007.4883 , Bibcode:2011MNRAS.410..190T, doi:10.1111/j.1365-2966.2010.17434.x.
^ http://www.atlascoelestis.com/alsufi%2038.htm

Artikel bertopik bintang ini adalah sebuah rintisan. Anda dapat membantu Wikipedia dengan mengembangkannya.

[vanLeeuwen2007-1] ^ ^a ^b ^c ^d ^e ^f van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv:0708.1752 , Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357.

[Eggleton2008-2] 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:0806.2878 , Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x.

[houk1978-3] 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.

[deBruijne2012-4] 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:1208.3048 , Bibcode:2012A&A...546A..61D, doi:10.1051/0004-6361/201219219, A61.

[ginestat2002-5] 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.

[McDonald2012-6] 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.

[Eaton1990-7] Eaton, J. A. (May 1990), "Rotational Velocities of G and K Giants", Information Bulletin on Variable Stars, 3460: 1, Bibcode:1990IBVS.3460....1E.

[Tetzlaff2011-8] 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:1007.4883 , Bibcode:2011MNRAS.410..190T, doi:10.1111/j.1365-2966.2010.17434.x.

[9] ttp://www.atlascoelestis.com/alsufi%2038.htm

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@@ Baris 1: / Baris 1: @@
+{{Starbox begin
-'''Nu Canis Majoris''' (μ CMa / μ Canis Majoris) adalah salah satu bintang di rasi [[Canis Major]].
+ | name = Mu Canis Majoris
+}}
+{{Starbox image
+ | image=
+{{Location mark
+|image=Canis Major constellation map.svg|alt=|float=center|width=250
+|label=|position=right
+|mark=Red circle.svg|mark_width=8|mark_link=μ CMa
+|x=272|y=294
+}}
+ |caption=Lokasi μ Canis Majoris (dilingkari)
+}}
+{{Starbox observe
+ | epoch = [[J2000.0]]
+ | equinox = [[J2000.0]] ([[International Celestial Reference System|ICRS]])
+ | constell = [[Canis Major]]
+ | ra = {{RA|06|56|06,64589}}<ref name=vanLeeuwen2007/>
+ | dec = {{DEC|−14|02|36,3520}}<ref name=vanLeeuwen2007/>
+ | appmag_v = 5,12 {{nowrap|(5,27 + 7,32)}}<ref name=Eggleton2008/>
+}}
+{{Starbox character
+ | class = {{nowrap|K2/3 III + B9/A0 V}}<ref name=houk1978/>
+ | b-v =
+ | u-b =
+ | variable =
+}}
+{{Starbox astrometry
+ | radial_v = {{Val|18.1|0.1}}<ref name=deBruijne2012/>
+ | prop_mo_ra = −1,59<ref name=vanLeeuwen2007/>
+ | prop_mo_dec = + 6,33<ref name=vanLeeuwen2007/>
+ | parallax = 2.62
+ | p_error = 0.58
+ | parallax_footnote = <ref name=vanLeeuwen2007/>
+ | absmag_v = −2,22<ref name=ginestat2002/>
+}}
+{{Starbox detail
+ | source =
+ | component1 = μ CMa A
+ | mass =
+ | radius =
+ | luminosity =
+ | temperature = 4441<ref name=McDonald2012/>
+ | gravity = 2489<ref name=McDonald2012/>
+ | metal_fe =
+ | rotational_velocity = ≤ 5<ref name=Eaton1990/>
+ | age_gyr =
+ | component2 = μ CMa B
+ | mass2 = {{Val|14.7|0.3}}<ref name=Tetzlaff2011/>
+ | age_myr2 = {{Val|11.6|0.5}}<ref name=Tetzlaff2011/>
+}}
+{{Starbox catalog
+ | names      = μ&nbsp;CMa, 18&nbsp;CMa, BD−13°&nbsp;1741, HIP 33345, HR 2593, SAO 152123
+}}
+{{Starbox reference
+ | Simbad = mu.+CMa
+}}
+{{Starbox end}}
+'''Mu Canis Majoris''' ('''μ CMa''' / '''μ Canis Majoris''') adalah salah satu bintang di rasi [[Canis Major]].
-μ Canis Majoris adalah bintang ber[[magnitudo]] +5.00.  Bintang ini berada pada jarak 908 [[tahun cahaya]] dari [[Bumi]].
+μ Canis Majoris memiliki [[magnitudo tampak]] 5,12.<ref name=Eggleton2008/> Bintang ini berada pada jarak 1200 [[tahun cahaya]] dari [[Matahari]].<ref name=vanLeeuwen2007/>
-==Etimologi==
+== Etimologi ==
 Bintang ini memiliki nama tradisional '''Isis''' yang merupakan nama salah satu dewi [[Mesir Kuno]].
@@ Baris 9: / Baris 67: @@
 == Referensi ==
-{{reflist}}
+{{reflist|refs=
+<ref name=vanLeeuwen2007>{{citation
-{{astronomi-stub}}
+ | title=Validation of the new Hipparcos reduction
+ | last1=van Leeuwen | first1=F.
+ | journal=Astronomy and Astrophysics
+ | volume=474 | issue=2 | pages=653–664 | date=2007
+ | arxiv=0708.1752 | bibcode=2007A&A...474..653V
+ | doi=10.1051/0004-6361:20078357 | postscript=. }}</ref>
+<ref name=Eggleton2008>{{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=. }}</ref>
+<ref name=McDonald2012>{{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 | doi=10.1111/j.1365-2966.2012.21873.x
+ | arxiv=1208.2037 | postscript=. }}</ref>
+<ref name=Eaton1990>{{citation
+ | title=Rotational Velocities of G and K Giants
+ | journal=Information Bulletin on Variable Stars
+ | last1=Eaton | first1=J. A.
+ | volume=3460 | page=1 | date=May 1990
+ | bibcode=1990IBVS.3460....1E | postscript=. }}</ref>
+<ref name=ginestat2002>{{citation
+ | title=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
+ | journal=The Astrophysical Journal Supplement Series
+ | last1=Ginestet | first1=N. | last2=Carquillat | first2=J. M.
+ | volume=143 | issue=2 | pages=513 | year=2002 | postscript=.
+ | bibcode=2002ApJS..143..513G | doi=10.1086/342942 }}</ref>
+<ref name=deBruijne2012>{{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=. }}</ref>
+<ref name=Tetzlaff2011>{{citation
+ | display-authors=1 | last1=Tetzlaff | first1=N.
+ | last2=Neuhäuser | first2=R. | last3=Hohle | first3=M. M.
+ | title=A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun
+ | journal=[[Monthly Notices of the Royal Astronomical Society]]
+ | volume=410 | issue=1 | pages=190–200 | date=January 2011
+ | doi=10.1111/j.1365-2966.2010.17434.x | bibcode=2011MNRAS.410..190T
+ | arxiv=1007.4883 | postscript=. }}</ref>
+<ref name=houk1978>{{citation
+ | last1=Houk | first1=Nancy | last2=Smith-Moore | first2=M.
+ | title=Michigan catalogue of two-dimensional spectral types for the HD stars
+ | volume=4 | publication-place=Ann Arbor | year=1978
+ | publisher=Dept. of Astronomy, University of Michigan
+ | bibcode=1988MSS...C04....0H | postscript=. }}</ref>
+}}
+{{bintang-stub}}
 [[Kategori:Rasi bintang Canis Major]]

Data pengamatan Epos J2000.0 Ekuinoks J2000.0 (ICRS)
Lokasi μ Canis Majoris (dilingkari)
Rasi bintang	Canis Major
Asensio rekta	06^j 56^m 06,64589^d^[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 (R_v)	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
Jarak	sekitar 1.200 tc (sekitar 380 pc)
Magnitudo mutlak (M_V)	−2,22^[5]

Detail
μ CMa A
Gravitasi permukaan (log g)	2489^[6]
Suhu	4441^[6] K
Kecepatan rotasi (v sin i)	≤ 5^[7] km/s
μ CMa B
Massa	14,7±0,3^[8] M_☉
Usia	11,6±0,5^[8] megatahun
Penamaan lain
μ CMa, 18 CMa, BD−13° 1741, HIP 33345, HR 2593, SAO 152123
Referensi basis data
SIMBAD	data