Zeta Crateris: Perbedaan antara revisi
Tampilan
Konten dihapus Konten ditambahkan
k Bot: perubahan kosmetika |
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* [http://seds.lpl.arizona.edu/messier/xtra/ngc/uma-cl.html] Arizona University website |
* [http://seds.lpl.arizona.edu/messier/xtra/ngc/uma-cl.html] Arizona University website |
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* [http://www.kencroswell.com/DescendantsOfTheDipper.html] [[Ken Croswell]]'s astronomy website. |
* [http://www.kencroswell.com/DescendantsOfTheDipper.html] [[Ken Croswell]]'s astronomy website. |
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*LeDrew, Glenn (1998). [http://ottawa.rasc.ca/observers/an9803p4.html "AstroNotes: The Ursa Major Moving Cluster"]. Retrieved July 28, 2005. |
* LeDrew, Glenn (1998). [http://ottawa.rasc.ca/observers/an9803p4.html "AstroNotes: The Ursa Major Moving Cluster"]. Retrieved July 28, 2005. |
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* [http://www.ucm.es/info/Astrof/invest/actividad/skg/skg.html Stellar kinematic groups, Superclusters, Moving Groups] - D. Montes, UCM |
* [http://www.ucm.es/info/Astrof/invest/actividad/skg/skg.html Stellar kinematic groups, Superclusters, Moving Groups] - D. Montes, UCM |
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* [http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003AJ....125.1980K&db_key=AST&data_type=HTML&format=&high=41b4ade78800742] J.R.King et al. 2003 Astronomical Journal paper classifying group members based on Hipparcos data. |
* [http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003AJ....125.1980K&db_key=AST&data_type=HTML&format=&high=41b4ade78800742] J.R.King et al. 2003 Astronomical Journal paper classifying group members based on Hipparcos data. |
Revisi per 24 Maret 2010 02.31
Zeta Crateris (ζ Crt / ζ Crateris) adalah salah satu bintang pada rasi Crater . Bintang ini memiliki magnitudo 4.71 dan merupakan bintang dengan kelas G8III. Bintang ini berada pada jarak 350 tahun cahaya dari Bumi.
Etimologi
Nama lainnya untuk bintang ini adalah :
nama lain | asal bahasa | arti |
---|---|---|
翼宿三 / Yì Su sān | China | bintang ketiga pada rasi Sayap[1] |
Selain rasi Crater, bintang ini juga merupakan anggota dari berbagai rasi, asterisma atau kelompok berikut :
nama rasi / asterisma / kelompok | asal | arti | anggota lainnya |
---|---|---|---|
翼 / Yì | China | Sayap | α Crt, γ Crt, λ Crt, ν Hya, η Crt, δ Crt, ι Crt, κ Crt, ε Crt, HD 95678, θ Crt, GC16178 |
Sirius Supercluster | HD 13594, 5 Aql, δ Aqr, 32 Aqr, β Aur, 45 Boo, χ Cet, α CMa, 6 CMi, δ Col, 29 Com, α CrB, υ CrB, HD 209515, HD 184960, δ Del, 59 Dra, HD 129798, β Eri, ζ Eri, HD 157740, υ1 Hya, HD 109799, 21 LMi, ζ Leo, τ Leo, γ Lep, RR Lyn, α Oph , HD 65810, HD 178428, HD 165185, β Ser, HD 26923, HD 111456, ζ TrA, 37 UMa, β UMa, γ UMa, δ UMa, ε UMa, 78 UMa, ζ UMa, 80 UMa, o Vir, α Vol.[2][3] | ||
Ursa Major Moving Group[4] | (core star antara lain) : 37 UMa, β UMa, γ UMa, δ UMa, ε UMa, 78 UMa, ζ UMa, 80 UMa
stream star : δ Aqr, β Aur, ζ Boo, 18 Boo, χ Cet A, 29 Com, α CrB, 59 Dra, 21 LMi, γ Lep, 16 Lyr, γ Mic, χ1 Ori, 89 Psc, β Ser, ω Ser, τ6 Ser, 6 Sex, 66 Tau, ζ TrA, π1 UMa, 41 Vir |
Referensi
- ^ salah satu rasi bintang menurut bangsa Cina
- ^ Eggen, Olin J. (1992). "The Sirius supercluster in the FK5". Astronomical Journal. 104 (4): 1493–1504. doi:10.1086/116334. Diakses tanggal 2007-11-22.
- ^ http://articles.adsabs.harvard.edu/full/1983AJ.....88..642E
- ^ bintang ini termasuk stream star
Pranala luar
- [1] Arizona University website
- [2] Ken Croswell's astronomy website.
- LeDrew, Glenn (1998). "AstroNotes: The Ursa Major Moving Cluster". Retrieved July 28, 2005.
- Stellar kinematic groups, Superclusters, Moving Groups - D. Montes, UCM
- [3] J.R.King et al. 2003 Astronomical Journal paper classifying group members based on Hipparcos data.