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Star HD 175225

Subgiant HD 175225 is located 87 light years away from the Sun. It is a single star of spectral class G9IVa, that has typically about 300 % of solar mass. For now, there are no known exoplanets in this star system.
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Sun distance
87 light years

HD 175225

Subgiant, High proper motion star
Spectral class: G9IVa

Location +

Ascension iconRight ascension: 18h 51m 34.897s
Declination iconDeclination: 52° 58' 34.210'' (northern hemisphere)
Parallax iconParallax: 37.687
Distance iconSun distance: 86.543 ly | 26.5 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: 100 % M Sun
| 1058 M Jupiter
 (estimate)
+
Star mass
The mass of the star HD 175225 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: 160 % R Sun
| 16 R Jupiter
(estimate)
+
Star size
Radius of the star HD 175225 is not known. Its estimated value based on other similar stars is about 160 % 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: 5400 K
 (estimate)
+
Star temperature
Surface temperature of HD 175225 is estimated to be 5417 K, which is 93 % 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 175225 system structure

HD 175225

More about HD 175225

       HD 175225 can be found in northern celestial hemisphere, and it is possible to see it with naked eye. The star is easily observable from Northern America, Europe and Asia. 
Other designations of this star
Gaia DR3 2146204847257954944
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External sources
simbad icon
Simbad database (HD 175225)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
gaia icon
Gaia database (Gaia DR3 2146204847257954944)
Archive from the Gaia mission

Frequently Asked Questions

How far is the HD 175225 system from the Sun?

The HD 175225 system is 87 light years or 26.5 parsecs from the Sun.

What galaxy is the HD 175225 star in?

The HD 175225 is in the Milky Way galaxy just like the Sun.

How many stars are in the HD 175225 system?

The HD 175225 is a single star, there are no other known stars in the system.

What type of star is the HD 175225?

The star HD 175225 is a Subgiant star.

What temperature is the HD 175225?

The primary in the HD 175225 system has an effective temperature of K ( °C). Find out more about the temperature of stars in Stellar guide
Class of stars Subgiant
A subgiant is a term used to describe a luminous star that is typically running out of hydrogen for nuclear fusion and is thus departing from the main sequence. These stars are classified as Yerkes luminosity class IV.
Possible companions

LP 141-7
- 0.4 ly
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exoplanet iconAbout Stellar Catalog

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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.
Fresh and validated
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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