stars

exoplanets

studies

Nearby stars catalogue

Ross 24

Star Ross 24

Red dwarf Ross 24 is located 92 light years away from the Sun. It is a single star of spectral class M1.0Ve, that has typically about 25 % of solar mass. For now, there are no known exoplanets in this star system.

Sun distance
92 light years

Ross 24

Red dwarf, High proper motion star

Spectral class: M1.0Ve

Location +

Right ascension: 3h 58m 36.931s

Declination: 52° 1' 21.658'' (northern hemisphere)

Parallax: 35.485

Sun distance: 91.913 ly | 28.2 pc

Basic characteristic

Mass: 50 % M Sun

(estimate)

Size: 50 % R Sun

(estimate)

Photometry

Absolute stellar magnitude in different parts of the electromagnetic spectrum from infrared (K band) to ultraviolet (U band).

K
2.1

H
1.6

J
1.2

Grp
0.8

I
0.8

G
0.6

V
0.5

Gbp
0.5

B
0.4

U
0.3

More about Ross 24

Nearby star Ross 24 is a main sequence star that fuses hydrogen atoms into helium.

       Ross 24 can be found in northern celestial hemisphere, however it is too dim to be seen with the naked eye or even a small telescope.

Other designations of this star
Gaia DR3 251688283301485824

External sources

Simbad database (Ross 24)

Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)

Gaia database (Gaia DR3 251688283301485824)

Archive from the Gaia mission

Class of stars Red dwarf

Red dwarfs are small, relatively cool, reddish stars. They are by far the most common type of star in the solar neighborhood. Their mass typically ranges from about 8% to 50% of the Sun's mass.

Closest stars

Gaia DR3 251476382498509952	-	3.7 ly
LSPM J0347+5424	-	4.8 ly
UCAC4 735-033510	-	8 ly
Ross 25	-	10.1 ly
LSR J0401+5131	-	10.1 ly

3D map of stellar neighborhood
List of all nearby stars

About Stellar Catalog

Working with real data

Data in Stellar Catalog come from trusted scientific sources. Primary source is Gaia space telescope mapping the stars in Milky Way. Other sources include research papers, Simbad catalog and Exoplanet.eu database.

Estimated values

Objects listed in the Stellar Catalog often have values that are estimates. These estimates are determined using their known characteristics, such as spectral type, brightness across different wavelengths, distance from a star, and other factors.

Fresh and validated

Stellar Catalog is continuously updated with new information from research papers. Stellar and planetary data are validated by automatic processes as well as humans.