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Nearby stars catalogue

2MASSI J1424187-351432

Star 2MASSI J1424187-351432

Red dwarf 2MASSI J1424187-351432 is located 63 light years away from the Sun. It is a single star of spectral class M6.5, that has typically about 25 % of solar mass. For now, there are no known exoplanets in this star system.

Sun distance
63 light years

2MASSI J1424187-351432

Red dwarf, High proper motion star

Spectral class: M6.5

Location +

Right ascension: 14h 24m 18.698s

Declination: -35° 14' 33.964'' (southern hemisphere)

Parallax: 51.739

Sun distance: 63.039 ly | 19.3 pc

Basic characteristic

Mass: 10 % M Sun

(estimate)

Size: 10 % 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 2MASSI J1424187-351432

       2MASSI J1424187-351432 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
Gaia DR3 6119528334597735296

External sources

Simbad database (2MASSI J1424187-351432)

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

Gaia database (Gaia DR3 6119528334597735296)

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

Theta Centauri	1.3 M☉	5.8 ly
CD-36 9107	-	6.2 ly
SIPS J1426-2946	-	6.2 ly
SIPS J1452-3458	-	7.5 ly
SIPS J1430-3114	-	7.6 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.