Star PM J12368-0159

Red dwarf PM J12368-0159 is located 92 light years away from the Sun. It is a single star of spectral class M3.5V, that has typically about 25 % of solar mass. For now, there are no known exoplanets in this star system.

PM J12368-0159

Red dwarf, High proper motion star

Spectral class: M3.5V

Location

Right ascension: 12h 36m 51.97s

Declination: -1° 59' 1.988'' (equatorial region)

Parallax: 35.354

Sun distance: 92.255 ly | 28.3 pc

Basic characteristic

Mass: 30 % M Sun (estimate)

Size: 30 % R Sun (estimate)

Photometry

Apparent magnitude (V): 13.6

Absolute magnitude (V): 11.3

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 PM J12368-0159

Nearby star PM J12368-0159 is a main sequence star that fuses hydrogen atoms into helium.

       PM J12368-0159 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 3683234524210341376

External sources

Simbad database (PM J12368-0159)

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

Gaia database (Gaia DR3 3683234524210341376)

Archive from the Gaia mission

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.

Closest stars

G 13-47	-	3.9 ly
HD 112943	-	9.9 ly
LSPM J1252+0252	-	10.5 ly
G 13-39	-	12.3 ly
LP 554-55	-	13.3 ly

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