Star LHS 475
Red dwarf LHS 475 is located 41 light years away from the Sun.
It is a single star of spectral class M3.5V, that has 26 % of solar mass.
There is at least one exoplanet in this system.
More about LHS 475
Nearby star LHS 475 is a main sequence star that fuses hydrogen atoms into helium. It is approximately 30 % of the size of Sun and temperature on its surface is around 3312 K (3039 °C), which is about 57 % of Sun's temperature.
LHS 475 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
L 22-69, GJ 4102, Gliese 4102, LFT 1458, 2MASS J19205439-8233170, TIC 369327947, TOI-910, WISEA J192056.23-823329.0, Gaia EDR3 6347643496607835520
External sources
Simbad database (L 22-69)
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.
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Right ascension: 19h 20m 57.203s
Declination: -82° 33' 35.853'' (southern hemisphere)
Parallax: 80.113
Sun distance: 40.712 ly | 12.5 pc
Temperature: 3312 K | 0.57 T Sun
Luminosity: 0.0087 L Sun
Apparent magnitude (V): 12.7
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12. 01 2023
Exoplanets
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