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Nearby stars catalogue

MCC 869

Star MCC 869

Orange star MCC 869 is located 87 light years away from the Sun. It is a single star of spectral class K8, that has typically about 70 % of solar mass. For now, there are no known exoplanets in this star system.

Sun distance
87 light years

MCC 869

Orange star, High proper motion star

Spectral class: K8

Location +

Right ascension: 23h 53m 20.023s

Declination: 59° 56' 42.97'' (northern hemisphere)

Parallax: 37.418

Sun distance: 87.166 ly | 26.7 pc

Basic characteristic

Photometry

Apparent magnitude (V): 10.6

Absolute magnitude (V): 8.4

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

More about MCC 869

       MCC 869 can be found in northern celestial hemisphere, you cannot see it with naked eye, but you can observe this star with basic telescope. The star is easily observable from Northern America, Europe and Asia.

Other designations of this star
Gaia DR3 2011565220332867584

External sources

Simbad database (MCC 869)

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

Gaia database (Gaia DR3 2011565220332867584)

Archive from the Gaia mission

Closest stars

LSPM J0006+5942	-	3.8 ly
PM J00104+6212	-	4.8 ly
Gaia EDR3 2012238465045216896	-	5.1 ly
Gaia EDR3 2012238465046622848	-	5.8 ly
Ross 310	-	6.2 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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