Gamma Phoenicis adalah bintang kelas G8III yang berada di rasi Phoenix. Bintang ini berada pada jarak 198 tahun cahaya dari Bumi. Bintang ini bermagnitudo 3.32.
Etimologi
Nama tradisional bintang ini adalah Al Rial V atau Al Rial al Khamsaa,[10] yang berarti "burung unta kecil kelima" dalam bahasa Arab. Nama lainnya untuk bintang ini adalah:
↑Keenan, P.; McNeil, R. (October 1989). "The Perkins catalog of revised MK types for the cooler stars". Astrophysical Journal Supplement Series. 71: 245–266. Bibcode:1989ApJS...71..245K. doi:10.1086/191373.
12Mermilliod, J. C. (2006). "VizieR Online Data Catalog: Homogeneous Means in the UBV System (Mermilliod 1991)". VizieR On-line Data Catalog: II/168. Originally published in: Institut d'Astronomie. 2168. Bibcode:2006yCat.2168....0M.Vizier catalog entryDiarsipkan 2018-12-14 di Wayback Machine.
↑Samus, N. N.; Durlevich, O. V.; etal. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/gcvs. Originally published in: 2009yCat....102025S. 1. Bibcode:2009yCat....102025S.
↑"Gam Phe". The International Variable Star Index. AAVSO – American Association of Variable Star Observers. Diakses tanggal 29 January 2018.
↑Evans, D. S. (1967). "The Revision of the General Catalogue of Radial Velocities". Determination of Radial Velocities and their Applications. 30: 57. Bibcode:1967IAUS...30...57E.
12"Salinan arsip". Diarsipkan dari asli tanggal 2023-07-28. Diakses tanggal 2009-10-19.
↑This is the photocentric semi-major axis, from the motion shown by the observed "star" relative to distant objects, and in practice relative to the barycentre. This is always smaller than the orbital semi-major axis, dramatically smaller when the primary star is much more massive than the secondary or when it is not much brighter.
