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Star WASP-188 B

Red dwarf WASP-188 B is located 2281 light years away from the Sun. It is a single star, that has typically about 25 % of solar mass. For now, there are no known exoplanets in this star system.
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Sun distance
2281 light years

WASP-188 B

Location +

Distance iconDistance from the primary: 1215 AU

Photometry

Magnitude iconAbsolute magnitude (V): -9.2
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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WASP-188 B system structure

WASP-188 A
WASP-188 A b 0.07 AU 458.7 M⊕ 14.8 R⊕ 5.7 days
WASP-188 B 1215 AU

More about WASP-188 B

       WASP-188 B can be found in northern celestial hemisphere. 
Other designations of this star
Gaia DR3 2095929373136748928
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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
gaia icon
Gaia database (Gaia DR3 2095929373136748928)
Archive from the Gaia mission

Frequently Asked Questions

How far is the WASP-188 B system from the Sun?

The WASP-188 B system is 2281 light years or 699.3 parsecs from the Sun.

What galaxy is the WASP-188 B star in?

The WASP-188 B is in the Milky Way galaxy just like the Sun.

How many stars are in the WASP-188 B system?

The WASP-188 B is a single star, there are no other known stars in the system.

What type of star is the WASP-188 B?

The star WASP-188 B is a Red dwarf star.

What temperature is the WASP-188 B?

The primary in the WASP-188 B system has an effective temperature of K ( °C). Find out more about the temperature of stars in Stellar guide
Class of stars Red dwarf
Red dwarfs are small, cool stars with surface temperatures of about 2,000–3,800 K, much cooler than the Sun. They usually have 8–50% of the Sun’s mass and shine very faintly, sometimes at just a tiny fraction of the Sun’s brightness. Classified mainly as spectral type M, they are the most common stars in the Milky Way, making up roughly 70–75% of its stellar population.

They fuse hydrogen slowly through the proton–proton chain and are fully convective, which allows them to use their fuel very efficiently. As a result, red dwarfs can live for tens of billions to trillions of years—far longer than the Sun. Many exoplanets orbit red dwarfs, including some in close habitable zones, though strong stellar activity can affect planetary environments.
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