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Nearby stars catalogue

EGGR 485

Star EGGR 485

White dwarf EGGR 485 is located 64 light years away from the Sun. It is a single star of spectral class DC10, that has typically about 60 % of solar mass. For now, there are no known exoplanets in this star system.

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Nearby stars catalogue

Sun distance
64 light years

EGGR 485

White dwarf

Spectral class: DC10

Location +

Right ascension: 7h 0m 52.117s

Declination: 31° 57' 34.301'' (northern hemisphere)

Parallax: 50.970

Sun distance: 63.989 ly | 19.6 pc

Photometry

Absolute magnitude (V): -1.5

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

EGGR 485 system structure


	EGGR 485

More about EGGR 485

       EGGR 485 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 890661253803216896

External sources

Simbad database (EGGR 485)

Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)

Gaia database (Gaia DR3 890661253803216896)

Archive from the Gaia mission

Frequently Asked Questions

How far is the EGGR 485 system from the Sun?

The EGGR 485 system is 64 light years or 19.6 parsecs from the Sun.

What galaxy is the EGGR 485 star in?

The EGGR 485 is in the Milky Way galaxy just like the Sun.

How many stars are in the EGGR 485 system?

The EGGR 485 is a single star, there are no other known stars in the system.

What type of star is the EGGR 485?

The star EGGR 485 is a White dwarf star.

What temperature is the EGGR 485?

The primary in the EGGR 485 system has an effective temperature of K ( °C). Find out more about the temperature of stars in Stellar guide

Closest stars

HD 266611	-	2.9 ly
HD 52711	1 M☉	3.7 ly
BD+33 1505	-	6.3 ly
G 103-41	-	6.4 ly
UCAC4 601-033776	-	8.3 ly

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About Stellar Catalog

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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.

Estimated values

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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