AK Pictoris is a star system in the constellationPictor. Its combined apparent magnitude is 6.182.[3] Based on the system's parallax, it is located 69 light-years (21.3 parsecs) away.[2] AK Pictoris is a member of the AB Doradus moving group,[10] a group of stars with similar motions that are thought to be associated.
AK Pictoris is a binary star. Its two stars orbit each other every 217.6 years, separated by 2.004″.[4] The primary star is a G-type star[5] with similar properties to the Sun. The secondary star is a K-type star.[5] The primary star is a young BY Draconis variable,[7] a class of variable stars that derive their variability from stellar rotation. It is also known to host a debris disk, inferred from its infrared excess.[10]
^Johnson, H. L. (1966). "UBVRIJKL Photometry of the Bright Stars". Communications of the Lunar and Planetary Laboratory. 4: 99. Bibcode:1966CoLPL...4...99J.
^ abSamus', N. N.; Goranskii, V. P.; Durlevich, O. V.; Zharova, A. V.; Kazarovets, E. V.; Kireeva, N. N.; Pastukhova, E. N.; Williams, D. B.; Hazen, M. L. (2003). "An Electronic Version of the Second Volume of the General Catalogue of Variable Stars with Improved Coordinates". Astronomy Letters. 29 (7): 468. Bibcode:2003AstL...29..468S. doi:10.1134/1.1589864. S2CID16299532.