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Star Ross 193 B

White dwarf Ross 193 B is located 53 light years away from the Sun. It is a single star of spectral class DC10, that has typically about 60 % of solar mass. For now, there are no known exoplanets in this star system.
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Sun distance
53 light years

Ross 193 B

Spectral class: DC10

Photometry

Magnitude iconApparent magnitude (V): 16.7
Magnitude iconAbsolute magnitude (V): 15.6
Absolute stellar magnitude in different parts of the electromagnetic spectrum from infrared (K band) to ultraviolet (U band).
5
10
15
20
25
30
35
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
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Ross 193 B system structure

Ross 193 A
Ross 193 B

More about Ross 193 B

       Ross 193 B 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 6913810483611035776
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External sources
icon study
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Scientific study, Accepted: 29. 12. 2026
icon study
A Spatial Map of the Atmospheric Limb of a Hot Jupiter
Scientific study, Accepted: 14. 10. 2026
simbad icon
Simbad database (Ross 193B)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
gaia icon
Gaia database (Gaia EDR3 6913810483611035776)
Archive from the Gaia mission

Frequently Asked Questions

How far is the Ross 193 B system from the Sun?

The Ross 193 B system is 53 light years or 16.2 parsecs from the Sun.

What galaxy is the Ross 193 B star in?

The Ross 193 B is in the Milky Way galaxy just like the Sun.

How many stars are in the Ross 193 B system?

The Ross 193 B is a single star, there are no other known stars in the system.

What type of star is the Ross 193 B?

The star Ross 193 B is a White dwarf star.

What temperature is the Ross 193 B?

The primary in the Ross 193 B system has an effective temperature of K ( °C). Find out more about the temperature of stars in Stellar guide
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