Star OT Serpentis
Red dwarf OT Serpentis is located 37 light years away from the Sun.
It is a single star of spectral class M1.0V, that has 55 % of solar mass.
For now, there are no known exoplanets in this star system.
More about OT Serpentis
Nearby star OT Serpentis is a main sequence star that fuses hydrogen atoms into helium. It is approximately 50 % of the size of Sun and temperature on its surface is around 3134 K (2861 °C), which is about 54 % of Sun's temperature.
OT Serpentis can be found in northern celestial hemisphere, you cannot see it with naked eye, but you can observe this star with basic telescope. The star is easily observable from Northern America, Europe and Asia.
Other designations of this star
BD+21 2763, GJ 9520, Gliese 9520, HIC 75187, HIP 75187, 2MASS J15215291+2058394, RBS 1489, TIC 355793860, TYC 1493-378-1, USNO-B1.0 1109-00243006, V* OT Ser, Gaia EDR3 1214160733157163008
External sources
Simbad database (V* OT Ser)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
Class of stars Red dwarf
Red dwarfs are small reddish stars, that are by far the most common type of star in solar neighborhood. Their mass is usually between 10 and 50 % of solar mass.
stars
exoplanets
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Right ascension: 15h 21m 53.034s
Declination: 20° 58' 41.96'' (northern hemisphere)
Parallax: 87.325
Sun distance: 37.35 ly | 11.5 pc
Temperature: 3134 K | 0.54 T Sun
Apparent magnitude (V): 10
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