AP Columbae

AP Columbae

A visual band light curve for AP Columbae, adapted from Clements et al. (2017)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Columba
Right ascension 06h 04m 52.14866s
Declination −34° 33 35.7744
Apparent magnitude (V) 12.96±0.01
Characteristics
Spectral type M5
V−R color index 1.47±0.03
R−I color index 1.89±0.03
Variable type Flare star
Astrometry
Radial velocity (Rv)23.91±0.49 km/s
Proper motion (μ) RA: +25.787 mas/yr
Dec.: +343.018 mas/yr
Parallax (π)115.3982±0.0298 mas
Distance28.264 ± 0.007 ly
(8.666 ± 0.002 pc)
Absolute magnitude (MV)13.34
Details
Mass0.265±0.008 M
Radius0.291±0.009 R
Luminosity (visual, LV)0.00641±0.00019 L
Habitable zone inner limit0.083 AU
Habitable zone outer limit0.165 AU
Temperature3,077±102 K
Rotation11±1 km/s
Age12–50 Myr
Other designations
2MASS J06045215-3433360, GSC 07079-01500, LTT 2449, L 523-55
Database references
SIMBADdata

AP Columbae is a pre-main-sequence star in the constellation of Columba. It is a small red dwarf with about one-quarter of the radius and mass of the Sun, but less than 1% of its luminosity. This star is located at around 28 ly (8.7 pc) from Earth based on measurements by the Gaia spacecraft, It is closest young star to the Earth, estimated to be 12 and 50 million years old. The Solar System for comparison is 4.5 billion years old.