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Gaia DR3 1833091840095015680

Star Gaia DR3 1833091840095015680

Little is known about object Gaia DR3 1833091840095015680. Based on its low brightness and position it seems to be a brown dwarf or a very low-mass star.

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Nearby stars catalogue

Sun distance
93 light years

Gaia DR3 1833091840095015680

Unknown star type

Location +

Right ascension: 20h 3m 6.310s

Declination: 22° 59' 53.170'' (northern hemisphere)

Parallax: 35.229

Sun distance: 92.583 ly | 28.4 pc

Photometry

Absolute stellar magnitude in different parts of the electromagnetic spectrum from infrared (K band) to ultraviolet (U band).

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 DR3 1833091840095015680 system structure


	Gaia DR3 1833091840095015680

More about Gaia DR3 1833091840095015680

       Gaia DR3 1833091840095015680 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 DR3 1833091840095015680

External sources

Gaia database (Gaia DR3 1833091840095015680)

Archive from the Gaia mission

Frequently Asked Questions

How far is the Gaia DR3 1833091840095015680 system from the Sun?

The Gaia DR3 1833091840095015680 system is 93 light years or 28.4 parsecs from the Sun.

What galaxy is the Gaia DR3 1833091840095015680 star in?

The Gaia DR3 1833091840095015680 is in the Milky Way galaxy just like the Sun.

How many stars are in the Gaia DR3 1833091840095015680 system?

The Gaia DR3 1833091840095015680 is a single star, there are no other known stars in the system.

What type of star is the Gaia DR3 1833091840095015680?

The primary in the Gaia DR3 1833091840095015680 system is a star.

What temperature is the Gaia DR3 1833091840095015680?

The primary in the Gaia DR3 1833091840095015680 system has an effective temperature of K ( °C). Find out more about the temperature of stars in Stellar guide

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Data in Stellar Catalog come from trusted scientific sources. Primary source is Gaia space telescope mapping the stars in Milky Way. Other sources include research papers, Simbad catalog and Exoplanet.eu database.

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Objects listed in the Stellar Catalog often have values that are estimates. These estimates are determined using their known characteristics, such as spectral type, brightness across different wavelengths, distance from a star, and other factors.

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