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Nearby stars catalogue

DENIS J081231.6-244442

Star DENIS J081231.6-244442

Brown dwarf DENIS J081231.6-244442 is located 69 light years away from the Sun. It is a single star of spectral class L1.5, that has typically about 4 % of solar mass. For now, there are no known exoplanets in this star system.

Sun distance
69 light years

DENIS J081231.6-244442

Brown dwarf

Spectral class: L1.5

Location +

Right ascension: 8h 12m 31.881s

Declination: -24° 44' 44.726'' (southern hemisphere)

Parallax: 47.479

Sun distance: 68.695 ly | 21.1 pc

Basic characteristic

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 DENIS J081231.6-244442

       DENIS J081231.6-244442 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 EDR3 5697787766170389888

External sources

Simbad database (DENIS J081231.6-244442)

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

Gaia database (Gaia EDR3 5697787766170389888)

Archive from the Gaia mission

Class of stars Brown dwarf

Brown dwarfs are not really stars, because there is no thermonuclear fusion in their core. These objects are smaller and cooler than stars, but too massive to be considered planets.

Closest stars

2MASS J0805+4812	-	3 ly
Gaia EDR3 5695019333334724992	-	4.7 ly
Gaia EDR3 5601266725623628416	-	4.9 ly
Rho Puppis	1.9 M☉	5.4 ly
Gaia EDR3 5693178647798942336	-	5.8 ly

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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.