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Star HD 38382

Yellow-White star HD 38382 is located 85 light years away from the Sun. It is a single star of spectral class F8.5V, that has typically about 130 % of solar mass. For now, there are no known exoplanets in this star system.
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Nearby stars catalogue
Sun distance
85 light years

HD 38382

Spectral class: F8.5V

Location +

Ascension iconRight ascension: 5h 44m 28.380s
Declination iconDeclination: -20° 7' 35.067'' (southern hemisphere)
Parallax iconParallax: 38.225
Distance iconSun distance: 85.325 ly | 26.2 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: 100 % M Sun
| 1016.1 M Jupiter
 (estimate)
+
Star mass
The mass of the star HD 38382 is unknown. Based on its other characteristics, it is estimated to be about 100 % 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: 100 % R Sun
| 10.2 R Jupiter
(estimate)
+
Star size
Radius of the star HD 38382 is not known. Its estimated value based on other similar stars is about 100 % 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): 6.3
Magnitude iconAbsolute magnitude (V): 4.2
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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HD 38382 system structure

HD 38382

More about HD 38382

Nearby star HD 38382 is a main sequence star that fuses hydrogen atoms into helium.
       HD 38382 can be found in southern celestial hemisphere, you cannot see it with naked eye, but you can observe this star with basic telescope. The star is also observable from Northern America, Europe and Asia. 
Other designations of this star
HR 1980, HIP 27075, SAO 170756, Gaia DR3 2966790170574625408
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External sources
simbad icon
Simbad database (HD 38382)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
gaia icon
Gaia database (Gaia DR3 2966790170574625408)
Archive from the Gaia mission

Frequently Asked Questions

How far is the HD 38382 system from the Sun?

The HD 38382 system is 85 light years or 26.2 parsecs from the Sun.

What galaxy is the HD 38382 star in?

The HD 38382 is in the Milky Way galaxy just like the Sun.

How many stars are in the HD 38382 system?

The HD 38382 is a single star, there are no other known stars in the system.

What type of star is the HD 38382?

The star HD 38382 is a Yellow-White star star.

What temperature is the HD 38382?

The primary in the HD 38382 system has an effective temperature of K ( °C). Find out more about the temperature of stars in Stellar guide
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HD 37065
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HD 39071
- 9 ly
3D map of stellar neighborhood
List of all nearby stars
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exoplanet iconAbout Stellar Catalog

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icon 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
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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