User:Kepler-1229b/sandbox/HD1273

HD 1273 is a G2V spectroscopic binary star located 75.1 light years away, in the constellation of Phoenix. In 1972, Cathpole proposed an astrometric orbit to explain the discrepancy between the trigonometric and spectroscopic parallax of HD 1273.

The star also receives the names of Gl 13, Hip 1349 and CD-53 36 A. As of December 2020, no exoplanets have been discovered around this Sun-like star. With an apparent magnitude of 6.852, the star is visible to the naked eye according to the Astronomical Magnitude Scale.