stars

exoplanets

studies

Nearby stars catalogue

SIPS J1943-6125

Star SIPS J1943-6125

Little is known about object SIPS J1943-6125. Based on its low brightness and position it seems to be a very low-mass star or maybe a massive brown dwarf.

Sun distance
83 light years

SIPS J1943-6125

Red dwarf, High proper motion star

Location +

Right ascension: 19h 43m 33.093s

Declination: -61° 25' 53.931'' (southern hemisphere)

Parallax: 39.272

Sun distance: 83.051 ly | 25.5 pc

Basic characteristic

Mass: 8 % M Sun

| 83.8 M Jupiter

(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 SIPS J1943-6125

       SIPS J1943-6125 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 6442331445127207808

External sources

Simbad database (SIPS J1943-6125)

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

Gaia database (Gaia EDR3 6442331445127207808)

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

L 160-102	-	2.7 ly
SCR J1940-6330	-	4.7 ly
UPM J1926-5838	-	5 ly
Gaia DR3 6442402569783360128	-	5.8 ly
UCAC4 165-206398	-	6.9 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.