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Nearby stars catalogue

LP 830-14

Star LP 830-14

White dwarf LP 830-14 is located 60 light years away from the Sun. It is a single star of spectral class DC, 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
60 light years

LP 830-14

White dwarf

Spectral class: DC

Location +

Right ascension: 2h 35m 21.673s

Declination: -24° 0' 56.837'' (southern hemisphere)

Parallax: 54.147

Sun distance: 60.235 ly | 18.5 pc

Basic characteristic

Temperature: 6900 K

(estimate)

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

LP 830-14 system structure


	LP 830-14

More about LP 830-14

       LP 830-14 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 DR3 5125186299678747008

External sources

Simbad database (LP 830-14)

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

Gaia database (Gaia DR3 5125186299678747008)

Archive from the Gaia mission

Frequently Asked Questions

How far is the LP 830-14 system from the Sun?

The LP 830-14 system is 60 light years or 18.5 parsecs from the Sun.

What galaxy is the LP 830-14 star in?

The LP 830-14 is in the Milky Way galaxy just like the Sun.

How many stars are in the LP 830-14 system?

The LP 830-14 is a single star, there are no other known stars in the system.

What type of star is the LP 830-14?

The star LP 830-14 is a White dwarf star.

What temperature is the LP 830-14?

The primary in the LP 830-14 system has an effective temperature of K ( °C). Find out more about the temperature of stars in Stellar guide

Closest stars

HD 15468	-	5.5 ly
LP 829-41	-	5.8 ly
L 657-32	-	6 ly
Gaia DR3 5131300889999108608	-	6.2 ly
LEHPM 2421	-	6.6 ly

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About Stellar Catalog

Working with real data

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.

Fresh and validated

Stellar Catalog is continuously updated with new information from research papers. Stellar and planetary data are validated by automatic processes as well as humans.