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Nearby stars catalogue

LP 898-100

Star LP 898-100

White dwarf LP 898-100 is located 84 light years away from the Sun. It is a single star of spectral class DA9, 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
84 light years

LP 898-100

White dwarf

Spectral class: DA9

Location +

Right ascension: 0h 36m 15.393s

Declination: -41° 57' 31.053'' (southern hemisphere)

Parallax: 38.788

Sun distance: 84.088 ly | 25.8 pc

Basic characteristic

Temperature: 5000 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 898-100 system structure


	LP 898-100

More about LP 898-100

       LP 898-100 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 4993117773313626496

External sources

Simbad database (LP 898-100)

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

Gaia database (Gaia DR3 4993117773313626496)

Archive from the Gaia mission

Frequently Asked Questions

How far is the LP 898-100 system from the Sun?

The LP 898-100 system is 84 light years or 25.8 parsecs from the Sun.

What galaxy is the LP 898-100 star in?

The LP 898-100 is in the Milky Way galaxy just like the Sun.

How many stars are in the LP 898-100 system?

The LP 898-100 is a single star, there are no other known stars in the system.

What type of star is the LP 898-100?

The star LP 898-100 is a White dwarf star.

What temperature is the LP 898-100?

The primary in the LP 898-100 system has an effective temperature of K ( °C). Find out more about the temperature of stars in Stellar guide

Closest stars

Alpha Phoenicis	1.6 M☉	3.6 ly
Koenigstuhl 1	0.1 M☉	5.4 ly
UCAC4 237-000303	-	5.8 ly
G 267-127	-	6 ly
Kappa Phoenicis	1.7 M☉	6.9 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.

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