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| metal_fe = –0.09<ref name=aj135_1_209/>
| rotational_velocity = 18<ref name="HR1"/>
| age_gyr =
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{{Starbox catalog
{{Starbox end}}
Ang '''Beta Ceti''' (β Cet, β Ceti) ay ang pinakamaliwanag na [[bituin]] sa [[konstelasyon]] ng [[Cetus]]. Kahit na mayroon itong [[pagtatanda ni Bayer]] na "beta", ito ang talagang mas maliwanag kaysa sa [[Alpha Ceti]]. May tradisyunal na pangalan itong'''Deneb Kaitos''' at '''Diphda'''. Madaling makita ang naranghang higanteng ito dahil sa lokasyon nito sa madilim na
==Talababa==
<ref name="HR1">{{cite web | title=Bright Star Catalogue, 5th Revised Ed. (Hoffleit+, 1991) | work=[[VizieR]] | publisher=[[Centre de Données astronomiques de Strasbourg]] | url=http://vizier.u-strasbg.fr/viz-bin/VizieR-S?HR%206695 | accessdate=2010-09-30 }}</ref>
<ref name=sagesser_jordan2005>{{cite conference | last1=Sägesser | first1=S. N. | last2=Jordan | first2=C. | title=Emission measures for the single giant β Ceti | booktitle=Proceedings of the 13th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun, held 5-9 July, 2004 in Hamburg, Germany | editor1-first=F. | editor1-last=Favata | editor2-first=G. A. J. | editor2-last=Hussain | editor3-first=B. | editor3-last=Battrick | publisher=European Space Agency | page=931 | month=March | year=2005 | bibcode=2005ESASP.560..931S }}</ref>
<ref name=chandra>{{cite web | date=
<ref name=aaa343_222>{{citation | last1=Elgarøy | first1=Øystein | last2=Engvold | first2=Oddbjørn | last3=Lund | first3=Niels | title=The Wilson-Bappu effect of the MgII K line - dependence on stellar temperature, activity and metallicity | journal=Astronomy and Astrophysics | volume=343 | pages=222–228 | month=March | year=1999 | bibcode=1999A&A...343..222E }}</ref>
[[Kategorya:Mga bagay ni Bayer|Ceti, Beta]]
[[Kategorya:Cetus (konstelasyon)]]
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