In
Chinese, 軫宿 (Zhěn Sù), meaning Chariot (asterism), refers to an asterism consisting of ε Corvi,
γ Corvi,
δ Corvi and
β Corvi.[11] Consequently, ε Corvi itself is known as 軫宿二 (Zhěn Sù èr, English: the Second Star of Chariot.).[12]
Epsilon Corvi is a
red giant with a
stellar classification of K2 III, having consumed the hydrogen at its core and
evolved away from the
main sequence. It has about three times the Sun's mass.[6] The
interferometry-measured
angular diameter of this star is about 4.99
mas,[13] which, at its estimated distance, equates to a physical radius of about 52 times the
radius of the Sun.[7] The
effective temperature of the outer envelope is 4320 K,[8] giving it an orange hue that is characteristic of a K-type star.[14] Around 4 times as massive as the Sun, it spent much of its life as a main sequence star of spectral type B5V.[15]
^
abcdCelis S., L. (October 1975), "Photoelectric photometry of late-type variable stars", Astronomy and Astrophysics Supplement Series, 22: 9–17,
Bibcode:
1975A&AS...22....9C
^Houk, Nancy (1979), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 4, Ann Arbor, Michigan: Dept. of Astronomy, University of Michigan,
Bibcode:
1988mcts.book.....H
^Wielen, R.; et al. (1999), "Sixth Catalogue of Fundamental Stars (FK6). Part I. Basic fundamental stars with direct solutions", Veroeffentlichungen des Astronomischen Rechen-Instituts Heidelberg, Astronomisches Rechen-Institut Heidelberg, 35 (35): 1,
Bibcode:
1999VeARI..35....1W