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Nearby stars catalogue

SIPS J0938-2748

Star SIPS J0938-2748

Red dwarf SIPS J0938-2748 is located 92 light years away from the Sun. It is a single star of spectral class M7.5, that has typically about 25 % of solar mass. For now, there are no known exoplanets in this star system.

Sun distance
92 light years

SIPS J0938-2748

Red dwarf, Low-mass star

Spectral class: M7.5

Location +

Right ascension: 9h 38m 39.745s

Declination: -27° 48' 21.245'' (southern hemisphere)

Parallax: 35.322

Sun distance: 92.338 ly | 28.3 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 SIPS J0938-2748

       SIPS J0938-2748 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 5657734928392398976

External sources

Simbad database (SIPS J0938-2748)

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

Gaia database (Gaia DR3 5657734928392398976)

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

PM J09268-3157	-	7.9 ly
LP 903-6	-	8 ly
SCR J0936-3237	-	8.3 ly
2MASS J09365490-3346212	-	9.6 ly
SIPS J0923-2727	-	10 ly

3D map of stellar neighborhood
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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.