Star HD 125072
Subgiant HD 125072 is located 39 light years away from the Sun.
It is a single star of spectral class K3IV, that has 81 % of solar mass.
For now, there are no known exoplanets in this star system.
More about HD 125072
Nearby star HD 125072 is approximately 80 % of the size of Sun and temperature on its surface is around 4867 K (4594 °C), which is about 84 % of Sun's temperature.
HD 125072 can be found in southern celestial hemisphere, you cannot see it with naked eye, but you can observe this star with basic telescope.
Other designations of this star
CD−58°5564, GJ 542, Gliese 542, HD 125072, HIC 69972, HIP 69972, SAO 241627, LHS 2892, LTT 5625, Gaia EDR3 5866992641380992256
External sources
Simbad database (HD 125072)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
Class of stars Subgiant
A subgiant is a term used to describe a luminous star that is typically running out of hydrogen for nuclear fusion and is thus departing from the main sequence. These stars are classified as Yerkes luminosity class IV.
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Right ascension: 14h 19m 3.882s
Declination: -59° 22' 57.507'' (southern hemisphere)
Parallax: 84.603
Sun distance: 38.551 ly | 11.8 pc
Temperature: 4867 K | 0.84 T Sun
Age: 9.98 billions years | 2.17 Sun
Luminosity: 0.347 L Sun
Apparent magnitude (V): 6.7
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