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Star HD 128020

Yellow-White star HD 128020 is located 91 light years away from the Sun. It is a single star of spectral class F8.5VFe-0.6, 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
91 light years

HD 128020

Yellow-White star, High proper motion star
Spectral class: F8.5VFe-0.6

Location +

Ascension iconRight ascension: 14h 37m 45.276s
Declination iconDeclination: -67° 55' 59.730'' (southern hemisphere)
Parallax iconParallax: 36.019
Distance iconSun distance: 90.551 ly | 27.8 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: 100 % M Sun
| 1016.1 M Jupiter
 (estimate)
+
Star mass
The mass of the star HD 128020 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 128020 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
Magnitude iconAbsolute magnitude (V): 3.8
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 128020 system structure

HD 128020

More about HD 128020

Nearby star HD 128020 is a main sequence star that fuses hydrogen atoms into helium.
       HD 128020 can be found in southern celestial hemisphere, you cannot see it with naked eye, but you can observe this star with basic telescope. 
Other designations of this star
Gaia DR3 5848156426657892480
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External sources
simbad icon
Simbad database (HD 128020)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
gaia icon
Gaia database (Gaia DR3 5848156426657892480)
Archive from the Gaia mission

Frequently Asked Questions

How far is the HD 128020 system from the Sun?

The HD 128020 system is 91 light years or 27.8 parsecs from the Sun.

What galaxy is the HD 128020 star in?

The HD 128020 is in the Milky Way galaxy just like the Sun.

How many stars are in the HD 128020 system?

The HD 128020 is a single star, there are no other known stars in the system.

What type of star is the HD 128020?

The star HD 128020 is a Yellow-White star star.

What temperature is the HD 128020?

The primary in the HD 128020 system has an effective temperature of K ( °C). Find out more about the temperature of stars in Stellar guide
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stellar brief logoStellar Brief

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24. 10. 2026
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The changing light of blue supergiant HD 74371 points to a dramatic turn in its life: the star appears to be moving blueward after a red-supergiant phase. Other fresh findings reveal helium escaping from an exoplanet, infrared rhythms on WASP 121, shifting radio and X-ray emissions from young V1298 Tauri, and clouds across WASP-43 b.
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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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