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BD+79 38
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Star BD+79 38

Orange star BD+79 38 is located 79 light years away from the Sun. It is a single star of spectral class K5V, that has typically about 70 % of solar mass. For now, there are no known exoplanets in this star system.
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Sun distance
79 light years
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BD+79 38

Orange star, High proper motion star
Spectral class: K5V

Location +

Ascension iconRight ascension: 1h 21m 32.669s
Declination iconDeclination: 80° 9' 5.201'' (northern hemisphere)
Parallax iconParallax: 41.068
Distance iconSun distance: 79.419 ly | 24.4 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
| 743.8 M Jupiter
 (estimate)
+
Star mass
The mass of the star BD+79 38 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: 70 % R Sun
| 7.2 R Jupiter
(estimate)
+
Star size
Radius of the star BD+79 38 is not known. Its estimated value based on other similar stars is about 70 % 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
temperature iconTemperature: 4400 K
 (estimate)
+
Star temperature
Surface temperature of BD+79 38 is estimated to be 4434 K, which is 76 % of the temperature on the surface of the Sun.

The temperature of a star refers to the temperature at its surface, also called the photosphere. It is measured in kelvins (K), the standard unit for temperature in astronomy. A star’s temperature tells us a lot about its physical properties and where it stands in its evolutionary stage... icon More about Star temperature in StellarGuide

Photometry

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
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BD+79 38 system structure

 BD+79 38

More about BD+79 38

Nearby star BD+79 38 is a main sequence star that fuses hydrogen atoms into helium. 
       BD+79 38 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 EDR3 565471721996476160
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External sources
simbad icon
Simbad database (BD+79 38)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
gaia icon
Gaia database (Gaia EDR3 565471721996476160)
Archive from the Gaia mission

Frequently Asked Questions

How far is the BD+79 38 system from the Sun?

The BD+79 38 system is 79 light years or 24.4 parsecs from the Sun.

What galaxy is the BD+79 38 star in?

The BD+79 38 is in the Milky Way galaxy just like the Sun.

How many stars are in the BD+79 38 system?

The BD+79 38 is a single star, there are no other known stars in the system.

What type of star is the BD+79 38?

The star BD+79 38 is a Orange star star.

What temperature is the BD+79 38?

The primary in the BD+79 38 system has an effective temperature of K ( °C). Find out more about the temperature of stars in Stellar guide
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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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