The pair orbit each other with an estimated
period of 616 years, a
semimajor axis of 1.5
arc seconds, and an
eccentricity of 0.1.[7] Both components are
evolved, yellow-white hued,
F-typegiant stars. The primary, component A, has a visual magnitude of 6.23[2] and a
stellar classification of F4 III.[2] The companion, component B, is magnitude 6.29[2] and of class F3 III.[2] Their composite
spectrum is classified as F2V.[3] The mass ratio is 0.782, meaning the secondary is only 78.2% as massive as the primary.[12] An 18th magnitude companion star lies 73.4 arc seconds distant along a
position angle of 243°, as of 1998.[13]
^
abHouk, Nancy (1979), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 3, Ann Arbor, Michigan: Dept. of Astronomy, University of Michigan,
Bibcode:
1982mcts.book.....H.
^
abHurly, P. R. (1975), "Combined-light UBV Photometry of 103 Bright Southern Visual Doubles", Monthly Notes of the Astronomical Society of Southern Africa, 34: 7,
Bibcode:
1975MNSSA..34....7H.
The pair orbit each other with an estimated
period of 616 years, a
semimajor axis of 1.5
arc seconds, and an
eccentricity of 0.1.[7] Both components are
evolved, yellow-white hued,
F-typegiant stars. The primary, component A, has a visual magnitude of 6.23[2] and a
stellar classification of F4 III.[2] The companion, component B, is magnitude 6.29[2] and of class F3 III.[2] Their composite
spectrum is classified as F2V.[3] The mass ratio is 0.782, meaning the secondary is only 78.2% as massive as the primary.[12] An 18th magnitude companion star lies 73.4 arc seconds distant along a
position angle of 243°, as of 1998.[13]
^
abHouk, Nancy (1979), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 3, Ann Arbor, Michigan: Dept. of Astronomy, University of Michigan,
Bibcode:
1982mcts.book.....H.
^
abHurly, P. R. (1975), "Combined-light UBV Photometry of 103 Bright Southern Visual Doubles", Monthly Notes of the Astronomical Society of Southern Africa, 34: 7,
Bibcode:
1975MNSSA..34....7H.