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Star Gliese 3877

Red dwarf Gliese 3877 is located 23 light years away from the Sun. It is a single flare star of spectral class M7.0Ve, that has 8 % of solar mass. For now, there are no known exoplanets in this star system.
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Sun distance
23 light years

Gliese 3877

Red dwarf, flare star
Spectral class: M7.0Ve

Location +

Ascension iconRight ascension: 14h 56m 37.676s
Declination iconDeclination: -28° 10' 2.115'' (southern hemisphere)
Parallax iconParallax: 141.789
Distance iconSun distance: 23.003 ly | 7.1 pc
Star position
The position of a star tells us where it appears in the sky, similar to how we use coordinates like latitude and longitude on Earth. In astronomy, the three main coordinates are right ascension, declination and distance. .. icon More about Star position in StellarGuide

Basic characteristic

icon weight
Mass: 8 % M Sun
| 84 M Jupiter
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Star mass
Mass of the star Gliese 3877 is 0.08 solar masses (or 83.8 Jupiter 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: 10.7 % R Sun
| 1.1 R Jupiter
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Star size
Radius of the star Gliese 3877 is 0.107 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: 2800 K
 (estimate)
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Star temperature
Surface temperature of Gliese 3877 is estimated to be 2830 K, which is 48 % 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): 17.1
Magnitude iconAbsolute magnitude (V): 17.9
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 3877 system structure

Gliese 3877

More about Gliese 3877

Nearby star Gliese 3877 is a main sequence star that fuses hydrogen atoms into helium.
       Gliese 3877 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
LHS 3003, LP 914-54, NLTT 38829, PLX 3372.03, 2MASS J14563831-2809473, 2MUCD 11264, Gaia DR2 6224387727748521344, Gaia EDR3 6224387727748521344
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External sources
simbad icon
Simbad database (LP 914-54)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
gaia icon
Gaia database (Gaia EDR3 6224387727748521344)
Archive from the Gaia mission

Frequently Asked Questions

How far is the Gliese 3877 system from the Sun?

The Gliese 3877 system is 23 light years or 7.1 parsecs from the Sun.

What galaxy is the Gliese 3877 star in?

The Gliese 3877 is in the Milky Way galaxy just like the Sun.

How many stars are in the Gliese 3877 system?

The Gliese 3877 is a single star, there are no other known stars in the system.

What type of star is the Gliese 3877?

The star Gliese 3877 is a Red dwarf star.

What temperature is the Gliese 3877?

The primary in the Gliese 3877 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.
Closest stars

33 G. Librae
0.8 M☉ 4.5 ly

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0.07 M☉ 5.1 ly

WISE 1541-2250
0.01 M☉ 5.5 ly

Gliese 588
0.46 M☉ 6.6 ly

Gliese 555
0.29 M☉ 6.7 ly
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