Star LP 847-48
Red dwarf LP 847-48 is located 36 light years away from the Sun.
It is a single star of spectral class M3V, that has typically about 25 % of solar mass.
For now, there are no known exoplanets in this star system.
More about LP 847-48
Nearby star LP 847-48 is a main sequence star that fuses hydrogen atoms into helium. It is approximately 40 % of the size of Sun and temperature on its surface is around 3354 K (3081 °C), which is about 58 % of Sun's temperature.
LP 847-48 can be found in southern celestial hemisphere, however it is too dim to be seen with the naked eye or even a small telescope.
Other designations of this star
HIC 48659, HIP 48659, NLTT 22957, 2MASS J09552387-2715405, TIC 22147322, TYC 6612-5-1, Gaia EDR3 5657274198660921472
External sources
Simbad database (LP 847-48)
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: 9h 55m 23.742s
Declination: -27° 15' 43.234'' (southern hemisphere)
Parallax: 91.737
Sun distance: 35.553 ly | 10.9 pc
Temperature: 3354 K | 0.58 T Sun
Apparent magnitude (V): 12.1
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