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Gaia EDR3 4271449399422291712
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Star Gaia EDR3 4271449399422291712

Binary star Gaia EDR3 4271449399422291712 is located 58 light years away from the Sun. It consists of 2 red dwarf stars. For now, there are no known exoplanets in this star system.
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Sun distance
58 light years
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Gaia EDR3 4271449399422291712

Red dwarf

Location +

Ascension iconRight ascension: 18h 20m 56.625s
Declination iconDeclination: -1° 3' 14.246'' (equatorial region)
Parallax iconParallax: 56.265
Distance iconSun distance: 57.968 ly | 17.8 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: 40 % M Sun
| 366.6 M Jupiter
 (estimate)
+
Star mass
The mass of the star Gaia EDR3 4271449399422291712 is unknown. Based on its other characteristics, it is estimated to be about 40 % 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: 40 % R Sun
| 4 R Jupiter
(estimate)
+
Star size
Radius of the star Gaia EDR3 4271449399422291712 is not known. Its estimated value based on other similar stars is about 40 % 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: 3400 K
 (estimate)
+
Star temperature
Surface temperature of Gaia EDR3 4271449399422291712 is estimated to be 3433 K, which is 59 % 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 iconAbsolute magnitude (V): -1.3
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

Gaia EDR3 4271449399415019904

Red dwarf

Basic characteristic

icon weight
Mass: 30 % M Sun
| 303.8 M Jupiter
 (estimate)
+
Star mass
The mass of the star Gaia EDR3 4271449399415019904 is unknown. Based on its other characteristics, it is estimated to be about 30 % 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: 30 % R Sun
| 3.3 R Jupiter
(estimate)
+
Star size
Radius of the star Gaia EDR3 4271449399415019904 is not known. Its estimated value based on other similar stars is about 30 % 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: 3300 K
 (estimate)
+
Star temperature
Surface temperature of Gaia EDR3 4271449399415019904 is estimated to be 3341 K, which is 57 % 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 iconAbsolute magnitude (V): -1.3
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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Gaia EDR3 4271449399422291712 system structure

 Gaia EDR3 4271449399422291712
Gaia EDR3 4271449399415019904

More about Gaia EDR3 4271449399422291712

       Gaia EDR3 4271449399422291712 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 4271449399422291712
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External sources
gaia icon
Gaia database (Gaia EDR3 4271449399415019904)
Archive from the Gaia mission

Frequently Asked Questions

How far is the Gaia EDR3 4271449399422291712 system from the Sun?

The Gaia EDR3 4271449399422291712 system is 58 light years or 17.8 parsecs from the Sun.

What galaxy is the Gaia EDR3 4271449399422291712 star in?

The Gaia EDR3 4271449399422291712 is in the Milky Way galaxy just like the Sun.

How many stars are in the Gaia EDR3 4271449399422291712 system?

The Gaia EDR3 4271449399422291712 system contains 2 stars.

What type of star is the Gaia EDR3 4271449399422291712?

The primary in the Gaia EDR3 4271449399422291712 system is a Red dwarf star.

What temperature is the Gaia EDR3 4271449399422291712?

The primary in the Gaia EDR3 4271449399422291712 system has an effective temperature of K ( °C). Find out more about the temperature of stars in Stellar guide
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30. 10. 2026
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The early architecture of planetary systems may be set at birth: a study of Sun-like stars found similar rates of star-planet misalignment across different stages of development. Other findings trace how water and carbon dioxide ice fade around young stars, why white-dwarf debris resists breaking into tiny pieces, and why a reported planet around Gliese 48 remains unconfirmed.
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