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Star Gliese 685

Red dwarf Gliese 685 is located 47 light years away from the Sun. It is a single star of spectral class M0.5V C, that has 55 % of solar mass. There is at least one exoplanet in this system.
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Sun distance
47 light years

Gliese 685

Red dwarf, High proper motion star
Spectral class: M0.5V C

Basic characteristic

icon weight
Mass: 55 % M Sun
| 576 M Jupiter
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Star mass
Mass of the star Gliese 685 is 0.55 solar masses.

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: 54 % R Sun
| 5.4 R Jupiter
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Star size
Radius of the star Gliese 685 is 0.54 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 icon
Temperature: 3893 K | 0.67 T Sun
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Star temperature
Surface temperature of Gliese 685 is 3893 K, which is 67 % 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): 10
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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Gliese 685 system structure

26 Draconis A
26 Draconis B
Gliese 685
Gliese 685 b 0.13 AU 9 M⊕ 24.2 days

More about Gliese 685

Gliese 685 is approximately 50 % of the size of Sun and temperature on its surface is around 3893 K (3620 °C), which is about 67 % of Sun's temperature.
       Gliese 685 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
GJ 685, LHS 3306, AC +62 26749, G 226-66, G 227-9, G 240-61, HIC 86087, HIP 86087, LFT 1361, LTT 15224, NLTT 45156, 2MASS J17353445+6140540, TIC 219780306, TYC 4199-693-1, WDS J17350+6153C, WISEA J173534.84+614048.3, Gaia EDR3 1439069444391326208
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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 (G 226-66)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
gaia icon
Gaia database (Gaia EDR3 1439069444391326208)
Archive from the Gaia mission

Frequently Asked Questions

How far is the Gliese 685 system from the Sun?

The Gliese 685 system is 47 light years or 14.3 parsecs from the Sun.

What galaxy is the Gliese 685 star in?

The Gliese 685 is in the Milky Way galaxy just like the Sun.

How many stars are in the Gliese 685 system?

The Gliese 685 is a single star, there are no other known stars in the system.

What type of star is the Gliese 685?

The star Gliese 685 is a Red dwarf star.

What temperature is star Gliese 685?

The star Gliese 685 has an effective temperature of 3893 K. 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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