The
stellar classification of this star is K3 IIIa,[3] where the
luminosity class of III indicates that this is an
evolvedgiant star that has exhausted the supply of hydrogen at its
core. It has expanded to around 56 times the radius of the Sun and radiates approximately 919 times the
Sun's luminosity from its
photosphere at an
effective temperature of 4,237 K.[5] Photometry measurements during the
Hipparcos mission indicate that this star is undergoing periodic variability by 0.0034 magnitudes over an 11.07941 day cycle.[10]
^
abcdWielen, 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.
^
abJohnson, H. L.; et al. (1966), "UBVRIJKL photometry of the bright stars", Communications of the Lunar and Planetary Laboratory, 4 (99): 99,
Bibcode:
1966CoLPL...4...99J.
^Streicher, Magda (June 2010), "Antlia, the Machine Pneumatique", Monthly Notes of the Astronomical Society of South Africa, 69 (5 and 6): 107–112,
Bibcode:
2010MNSSA..69..107S.