Psi Capricorni: Perbedaan antara revisi
Konten dihapus Konten ditambahkan
Rescuing 1 sources and tagging 0 as dead.) #IABot (v2.0.8 |
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| names=psi Cap, 16 Capricorni, 16 Cap, [[Henry L. Giclas catalogue|Gl]] 805, [[Harvard Revised catalogue|HR]] 7936, [[Cordoba Durchmusterung|CD]] −25°15018, [[Henry Draper catalogue|HD]] 197692, [[General Catalogue of Trigonometric Parallaxes|GCTP]] 4947.00, [[Smithsonian Astrophysical Observatory Star Catalog|SAO]] 189664, [[Fifth Fundamental Catalogue|FK5]] 779, GC 28929, [[Hipparcos catalogue|HIP]] 102485. }}
{{Starbox end}}
'''Psi Capricorni (ψ Cap / ψ Capricorni)''' adalah salah satu [[bintang]] pada [[rasi bintang]] [[Capricornus]]. ψ Capricorni merupakan [[bintang katai]] kuning tipe F (''yellow-white F-type main sequence dwarf'') dengan [[magnitudo]] 4.13. [[bintang]] ini berada pada jarak 48 [[tahun cahaya]] dari [[Bumi]].
== Etimologi ==
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| Yue|| [[China]] || kapak perang<ref>http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Capricornus*.html</ref>
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| Quae sub genu dextro (Almagest)|| [[Bahasa Latin|Latin]] || yang berarti di lutut kanan (sang kambing laut)<ref>http://www.atlascoelestis.com/alsufi%2031.htm</ref>
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== Pranala luar ==
* {{cite web | url = http://simbad.u-strasbg.fr/sim-id.pl?protocol=html&Ident=HD+197692 | title = HD 197692 -- Star | publisher = SIMBAD: Centre de Données astronomiques de Strasbourg | language = English | accessdate = 2006-08-16 }}
* {{cite web | date = 1998-03-04 | url = http://www.ari.uni-heidelberg.de/datenbanken/aricns/cnspages/4c01688.htm | title = 4C01688 | publisher = ARICNS | language = English | accessdate = 2006-08-16 | archive-date = 2011-06-07 | archive-url = https://web.archive.org/web/20110607164839/http://www.ari.uni-heidelberg.de/datenbanken/aricns/cnspages/4c01688.htm | dead-url = yes }}
* {{cite web | url = http://www.alcyone.de/SIT/bsc/HR7936.html | title = ψ Capricorni | publisher = Alcyone ephemeris | language = English | accessdate = 2006-08-16 }}
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[[Kategori:Rasi bintang Capricornus]]
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