Star TOI-260
Red dwarf TOI-260 is located 66 light years away from the Sun.
It is a single star of spectral class M0V, that has 55 % of solar mass.
There is at least one exoplanet in this system.
More about TOI-260
Nearby star TOI-260 is a main sequence star that fuses hydrogen atoms into helium. It is approximately 60 % of the size of Sun and temperature on its surface is around 4050 K (3777 °C), which is about 70 % of Sun's temperature.
TOI-260 can be found in southern celestial hemisphere, you cannot see it with naked eye, but you can observe this star with basic telescope. The star is also observable from Northern America, Europe and Asia.
Other designations of this star
BD-10 47, G 158-59, Gliese 1008, GJ 1008, HIC 1532, HIP 1532, LTT 156, NLTT 988, 2MASS J00190556-0957530, TIC 37749396, WISEA J001905.53-095756.6, Gaia EDR3 2428162410789155328
External sources
Simbad database (BD-10 47)
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
en
Right ascension: 0h 19m 5.524s
Declination: -9° 57' 58.293'' (equatorial region)
Parallax: 49.476
Sun distance: 65.922 ly | 20.2 pc
Temperature: 4050 K | 0.7 T Sun
Age: 15.9 billions years | 3.46 Sun
Apparent magnitude (V): 9.9
česky
espaňol
deutsch
francais
X (twitter)
facebook