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Star BD+45 598

Yellow star BD+45 598 is located 239 light years away from the Sun. It is a single star, that has typically about 90 % of solar mass. For now, there are no known exoplanets in this star system.
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Sun distance
239 light years

BD+45 598

Location +

Ascension iconRight ascension: 2h 21m 13.153s
Declination iconDeclination: 46° 0' 6.433'' (northern hemisphere)
Parallax iconParallax: 13.648
Distance iconSun distance: 238.977 ly | 73.3 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: 110 % M Sun
| 1152.3 M Jupiter
 (estimate)
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Star mass
The mass of the star BD+45 598 is unknown. Based on its other characteristics, it is estimated to be about 110 % 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: 120 % R Sun
| 12.2 R Jupiter
(estimate)
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Star size
Radius of the star BD+45 598 is not known. Its estimated value based on other similar stars is about 120 % 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: 6000 K
 (estimate)
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Star temperature
Surface temperature of BD+45 598 is estimated to be 5966 K, which is 104 % 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+45 598 system structure

BD+45 598

More about BD+45 598

       BD+45 598 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 DR3 353635070145291008
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External sources

Frequently Asked Questions

How far is the BD+45 598 system from the Sun?

The BD+45 598 system is 239 light years or 73.3 parsecs from the Sun.

What galaxy is the BD+45 598 star in?

The BD+45 598 is in the Milky Way galaxy just like the Sun.

How many stars are in the BD+45 598 system?

The BD+45 598 is a single star, there are no other known stars in the system.

What type of star is the BD+45 598?

The star BD+45 598 is a Yellow star star.

What temperature is the BD+45 598?

The primary in the BD+45 598 system has an effective temperature of K ( °C). Find out more about the temperature of stars in Stellar guide
Class of stars Yellow star
Sun-like stars belong mainly to spectral type G and are commonly called yellow dwarfs. They have surface temperatures of roughly 5,300–6,000 K (about 5,000–5,700 °C), giving them a slightly yellow-white appearance. With masses typically between about 0.8 and 1.1 times that of the Sun, they sit between hotter, more massive white stars and cooler orange and red stars on the main sequence. The Sun itself is a standard G2V star and serves as the benchmark for understanding the structure and behavior of this stellar class.

These stars generate energy by fusing hydrogen into helium in their cores through the proton–proton chain. Their total lifetimes on the main sequence are around 10 billion years, during which their brightness slowly increases. After exhausting hydrogen in their cores, Sun-like stars expand into red giants, shed their outer layers to form planetary nebulae, and eventually leave behind dense white dwarfs. Many known exoplanet systems orbit Sun-like stars, making them key targets in the search for potentially habitable worlds.
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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
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