In a 1951 publication, Atlas Coeli (
Skalnate Pleso Atlas of the Heavens) by Czech astronomer
Antonín Bečvář, it bore the name Kraz, whose origin and meaning remain unknown.[12][13][14] In 2016, the IAU organized a
Working Group on Star Names (WGSN)[15] to catalog and standardize proper names for stars. The WGSN approved the name Kraz for this star on 1 June 2018 and it is now so included in the List of IAU-approved Star Names.[11]
In Chinese, 軫宿 (Zhěn Sù), meaning Chariot (asterism), refers to an
asterism consisting of Beta,
Gamma,
Epsilon and
Delta Corvi.[16] Consequently, Beta Corvi itself is known as 軫宿四 (Zhěn Sù sì, English: the Fourth Star of Chariot).[17]
Properties
Beta Corvi has about 3.7 times the
Sun's mass and is roughly 206 million years old,[3] which is old enough for a star of this mass to consume the hydrogen at its core and evolve away from the
main sequence. The
stellar classification is G5 II,[3] with the luminosity class of 'II' indicating this is a
bright giant. The
effective temperature of the star's outer envelope is about 5,100 K,[3] which produces a yellow hue common to
G-type stars.[18]
The measured
angular diameter of this star is 3.30 ± 0.17
mas.[7] At an estimated distance of 146
light-years (45
parsecs),[1] this yields a physical size of about 16 times the
radius of the Sun.[13][19] Because of the star's mass and radius, it is emitting about 164 times the
luminosity of the Sun.[8] The abundance of elements other than hydrogen or helium, what astronomers term
metallicity, is similar to the proportions in the
Sun.[6]
^
abcdGutierrez-Moreno, Adelina; et al. (1966). "A System of photometric standards". Publications of the Department of Astronomy University of Chile. Publicaciones Universidad de Chile, Department de Astronomy. 1: 1–17.
Bibcode:
1966PDAUC...1....1G.
^
abHR 4786, database entry, The Bright Star Catalogue, 5th Revised Ed. (Preliminary Version), D. Hoffleit and W. H. Warren, Jr.,
CDS ID
V/50. Accessed on line September 9, 2008.
^Evans, D. S. (June 20–24, 1966). Batten, Alan Henry; Heard, John Frederick (eds.). "The Revision of the General Catalogue of Radial Velocities". Determination of Radial Velocities and their Applications, Proceedings from IAU Symposium no. 30. University of Toronto:
International Astronomical Union. 30: 57.
Bibcode:
1967IAUS...30...57E.
^
abRichichi, A.; Percheron, I.; Khristoforova, M. (February 2005), "CHARM2: An updated Catalog of High Angular Resolution Measurements", Astronomy and Astrophysics, 431 (2): 773–777,
Bibcode:
2005A&A...431..773R,
doi:10.1051/0004-6361:20042039
^
abMallik, Sushma V. (December 1999), "Lithium abundance and mass", Astronomy and Astrophysics, 352: 495–507,
Bibcode:
1999A&A...352..495M
^Bernacca, P. L.; Perinotto, M. (1970). "A catalogue of stellar rotational velocities". Contributi Osservatorio Astronomico di Padova in Asiago. 239 (1): 1.
Bibcode:
1970CoAsi.239....1B.
^Kunitzch, Paul; Smart, Tim (2006) [1986]. A Dictionary of Modern Star Names: A Short Guide to 254 Star Names and Their Derivations. Cambridge, Massachusetts: Sky Publishing Corporation. p. 62.
ISBN978-1-931559-44-7.
^Kukarkin, B. V.; et al. (1981), "Nachrichtenblatt der Vereinigung der Sternfreunde e.V. (Catalogue of suspected variable stars)", Nachrichtenblatt der Vereinigung der Sternfreunde, Moscow: Academy of Sciences USSR Shternberg,
Bibcode:
1981NVS...C......0K