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HD 152564
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Star HD 152564

White-Blue star HD 152564 is located 625 light years away from the Sun. It is a single star of spectral class Ap/Bp, that has typically about 190 % of solar mass. For now, there are no known exoplanets in this star system.
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Sun distance
625 light years
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HD 152564

White-Blue star
Spectral class: Ap/Bp

Location +

Ascension iconRight ascension: 16h 59m 33.923s
Declination iconDeclination: -69° 16' 5.585'' (southern hemisphere)
Parallax iconParallax: 5.221
Distance iconSun distance: 624.710 ly | 191.5 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: 240 % M Sun
| 2461.8 M Jupiter
 (estimate)
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Star mass
The mass of the star HD 152564 is unknown. Based on its other characteristics, it is estimated to be about 240 % 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: 210 % R Sun
| 21.3 R Jupiter
(estimate)
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Star size
Radius of the star HD 152564 is not known. Its estimated value based on other similar stars is about 210 % 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 icon
Temperature: 11950 K | 2.07 T Sun
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Star temperature
Surface temperature of HD 152564 is 11950 K, which is 207 % 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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HD 152564 system structure

 HD 152564

More about HD 152564

Star HD 152564 is a main sequence star that fuses hydrogen atoms into helium. It is is approximately 2 times bigger than the Sun and temperature on its surface is around 11950 K (11677 °C), which is about 207 % of Sun's temperature.
       HD 152564 can be found in southern celestial hemisphere, and it is possible to see it with naked eye.
Other designations of this star
TYC 9275-3003-1, HR 6276, HIP 83150, Gaia DR3 5808183303451658112
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External sources
icon study
On the surface distribution of chromium in Ap star HD 152564
Scientific study, Accepted: 20. 08. 2024
gaia icon
Gaia database (Gaia DR3 5808183303451658112)
Archive from the Gaia mission

Frequently Asked Questions

How far is the HD 152564 system from the Sun?

The HD 152564 system is 625 light years or 191.5 parsecs from the Sun.

What galaxy is the HD 152564 star in?

The HD 152564 is in the Milky Way galaxy just like the Sun.

How many stars are in the HD 152564 system?

The HD 152564 is a single star, there are no other known stars in the system.

What type of star is the HD 152564?

The star HD 152564 is a White-Blue star star.

What temperature is star HD 152564?

The star HD 152564 has an effective temperature of 11950 K. Find out more about the temperature of stars in Stellar guide
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Working with real data
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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icon Stellar Catalog is continuously updated with new information from research papers. Stellar and planetary data are validated by automatic processes as well as humans.
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