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Gaia EDR3 1819588325493424256
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Star Gaia EDR3 1819588325493424256

Little is known about object Gaia EDR3 1819588325493424256. Based on its low brightness and position it seems to be a brown dwarf or a very low-mass star.
Sun distance
66 light years
galaxy map

Gaia EDR3 1819588325493424256

Brown dwarf

Location +

Ascension iconRight ascension: 19h 52m 27.358s
Declination iconDeclination: 15° 32' 19.270'' (equatorial region)
Parallax iconParallax: 49.388
Distance iconSun distance: 66.040 ly | 20.2 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
| 83.8 M Jupiter
 (estimate)
+
Star mass
The estimated mass of the star Gaia EDR3 1819588325493424256 is about 8 % of the Sun's mass, or approximately 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 % R Sun
| 1.1 R Jupiter
(estimate)
+
Star size
Radius of the star Gaia EDR3 1819588325493424256 is not known. Its estimated value based on other similar stars is about 10 % 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: 1700 K
 (estimate)
+
Star temperature
Surface temperature of Gaia EDR3 1819588325493424256 is estimated to be 1715 K, which is 29 % 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): -1.5
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 1819588325493424256 system structure

 Gaia EDR3 1819588325493424256

More about Gaia EDR3 1819588325493424256

       Gaia EDR3 1819588325493424256 can be found in northern 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 1819588325493424256
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External sources
gaia icon
Gaia database (Gaia EDR3 1819588325493424256)
Archive from the Gaia mission

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News from this star system

Frequently Asked Questions stardetail

How far is the Gaia EDR3 1819588325493424256 system from the Sun?

The Gaia EDR3 1819588325493424256 system is 66 light years or 20.2 parsecs from the Sun.

What galaxy is the Gaia EDR3 1819588325493424256 star in?

The Gaia EDR3 1819588325493424256 is in the Milky Way galaxy just like the Sun.

How many stars are in the Gaia EDR3 1819588325493424256 system?

The Gaia EDR3 1819588325493424256 is a single star, there are no other known stars in the system.

What type of star is the Gaia EDR3 1819588325493424256?

The star Gaia EDR3 1819588325493424256 is a Brown dwarf star.

What temperature is the Gaia EDR3 1819588325493424256?

The primary in the Gaia EDR3 1819588325493424256 system has an effective temperature of K ( °C). Find out more about the temperature of stars in Stellar guide
Class of stars Brown dwarf
Brown dwarfs are not really stars, because there is no thermonuclear fusion in their core. These objects are smaller and cooler than stars, but too massive to be considered planets.
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 - 4.2 ly

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 0.82 M☉ 5.3 ly

G 143-35
 - 5.3 ly
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