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Stellar Catalog
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MCC 435
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Star MCC 435

Orange star MCC 435 is located 84 light years away from the Sun. It is a single star of spectral class K7V, that has typically about 70 % of solar mass. For now, there are no known exoplanets in this star system.
Sun distance
84 light years

MCC 435

Orange star, High proper motion star
Spectral class: K7V

Location +

Ascension iconRight ascension: 4h 12m 41.868s
Declination iconDeclination: 70° 12' 6.168'' (northern hemisphere)
Parallax iconParallax: 38.709
Distance iconSun distance: 84.259 ly | 25.8 pc
Star position
The position of a star tells us where it appears in the sky, similar to how we use coordinates like latitude and longitude on Earth. In astronomy, the three main coordinates are right ascension, declination and distance. .. icon More about Star position in StellarGuide

Basic characteristic

icon weight
Mass: 70 % M Sun
| 680.9 M Jupiter
 (estimate)
+
Star mass
The mass of the star MCC 435 is unknown. Based on its other characteristics, it is estimated to be about 70 % of the Sun’s mass.

The mass of a star is the total amount of matter it contains. It is one of the most important properties of a star, as it determines almost everything about how the star lives, changes, and dies. In astronomy, star mass is usually measured in solar masses (M☉) — where 1 solar mass is equal to the mass of our Sun... icon More about Star mass in StellarGuide
radius icon
Size: 60 % R Sun
| 6.4 R Jupiter
(estimate)
+
Star size
Radius of the star MCC 435 is not known. Its estimated value based on other similar stars is about 60 % solar radii.

The size of a star refers to its radius — the distance from its center to its surface. Star size is usually measured in solar radii (R☉), where 1 solar radius equals approximately 696,000 kilometers. Depending on their type and life stage, stars can be much smaller or larger than the Sun... icon More about Star size in StellarGuide

Photometry

Magnitude iconApparent magnitude (V): 9.7
Magnitude iconAbsolute magnitude (V): 7.6
Absolute stellar magnitude in different parts of the electromagnetic spectrum from infrared (K band) to ultraviolet (U band).
5
10
15
20
25
30
35
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 435
Nearby star MCC 435 is a main sequence star that fuses hydrogen atoms into helium.
       MCC 435 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 494177257749671936
External sources
simbad icon
Simbad database (MCC 435)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
gaia icon
Gaia database (Gaia DR3 494177257749671936)
Archive from the Gaia mission
Closest stars

PM J04302+7049
- 2.4 ly

LP 32-204
- 4.8 ly

HD 30163
- 5.1 ly

G 221-21
- 5.2 ly

G 221-20
- 5.2 ly
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Estimated values
icon 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 brings the stars from our galaxy to you. Discover their position, physical properties and whether there are any exoplanets or disks orbiting them. The data in Stellar Catalog come from respectable sources like Gaia space telescope, or SIMBAD database.
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