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Star 111 Tauri B

Orange star 111 Tauri B is located 47 light years away from the Sun. It is a single star of spectral class K4V, that has typically about 70 % of solar mass. For now, there are no known exoplanets in this star system.
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Sun distance
47 light years

111 Tauri B

Orange star, High proper motion star
Spectral class: K4V

Basic characteristic

icon weight
Mass: 70 % M Sun
| 775.2 M Jupiter
 (estimate)
+
Star mass
The mass of the star 111 Tauri B is unknown. Based on its other characteristics, it is estimated to be about 70 % of the Sun's mass.

The mass of a star is the total amount of matter it contains. It is one of the most important properties of a star, as it determines almost everything about how the star lives, changes, and dies. In astronomy, star mass is usually measured in solar masses (M☉) — where 1 solar mass is equal to the mass of our Sun... icon More about Star mass in StellarGuide
radius icon
Size: 70 % R Sun
| 7.1 R Jupiter
(estimate)
+
Star size
Radius of the star 111 Tauri B is not known. Its estimated value based on other similar stars is about 70 % solar radii.

The size of a star refers to its radius — the distance from its center to its surface. Star size is usually measured in solar radii (R☉), where 1 solar radius equals approximately 696,000 kilometers. Depending on their type and life stage, stars can be much smaller or larger than the Sun... icon More about Star size in StellarGuide
temperature iconTemperature: 4700 K
 (estimate)
+
Star temperature
Surface temperature of 111 Tauri B is estimated to be 4660 K, which is 81 % of the temperature on the surface of the Sun.

The temperature of a star refers to the temperature at its surface, also called the photosphere. It is measured in kelvins (K), the standard unit for temperature in astronomy. A star’s temperature tells us a lot about its physical properties and where it stands in its evolutionary stage... icon More about Star temperature in StellarGuide

Photometry

Magnitude iconApparent magnitude (V): 7.9
Magnitude iconAbsolute magnitude (V): 7.1
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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111 Tauri B system structure

111 Tauri A
111 Tauri B

More about 111 Tauri B

       111 Tauri B can be found in northern celestial hemisphere, you cannot see it with naked eye, but you can observe this star with basic telescope. The star is easily observable from Northern America, Europe and Asia. 
Other designations of this star
Gaia EDR3 3394298532176344960
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External sources
icon study
_empty
Scientific study, Accepted: 29. 12. 2026
icon study
A Sample of Thick-Disk Stars Hosting Hot Jupiters
Scientific study, Accepted: 16. 10. 2026
icon study
A Spatial Map of the Atmospheric Limb of a Hot Jupiter
Scientific study, Accepted: 14. 10. 2026
simbad icon
Simbad database (* 111 Tau B)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
gaia icon
Gaia database (Gaia EDR3 3394298532176344960)
Archive from the Gaia mission

Frequently Asked Questions

How far is the 111 Tauri B system from the Sun?

The 111 Tauri B system is 47 light years or 14.5 parsecs from the Sun.

What galaxy is the 111 Tauri B star in?

The 111 Tauri B is in the Milky Way galaxy just like the Sun.

How many stars are in the 111 Tauri B system?

The 111 Tauri B is a single star, there are no other known stars in the system.

What type of star is the 111 Tauri B?

The star 111 Tauri B is a Orange star star.

What temperature is the 111 Tauri B?

The primary in the 111 Tauri B system has an effective temperature of K ( °C). Find out more about the temperature of stars in Stellar guide
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Estimated values
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Stellar Catalog brings the stars from our galaxy to you. Discover their position, physical properties and whether there are any exoplanets or disks orbiting them. The data in Stellar Catalog come from respectable sources like Gaia space telescope, or SIMBAD database.

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