Star Ross 154
Red dwarf Ross 154 is located 10 light years away from the Sun.
It is a single flare star of spectral class M3.5 V, that has 17 % of solar mass.
For now, there are no known exoplanets in this star system.
More about Ross 154
Nearby star Ross 154 is a main sequence star that fuses hydrogen atoms into helium. It is approximately 20 % of the size of Sun and temperature on its surface is around 3293 K (3020 °C), which is about 57 % of Sun's temperature.
Ross 154 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
Gliese 729, GJ 729, V1216 Sgr, CD−23° 14742, GCTP 4338, HIP 92403, LHS 3414, V1216 Sagittarii, Ross 154, Gaia EDR3 4075141768785646848
External sources
Simbad database (Ross 154)
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
studies
Right ascension: 18h 49m 50.117s
Declination: -23° 50' 13.551'' (southern hemisphere)
Parallax: 336.027
Sun distance: 9.706 ly | 3 pc
Temperature: 3293 K | 0.57 T Sun
Age: 0.8 billions years | 0.17 Sun
Luminosity: 0.0038 L Sun
Apparent magnitude (V): 10.4
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