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V509 Cassiopeiae

Star V509 Cassiopeiae

Yellow hypergiant V509 Cassiopeiae is located 15696 light years away from the Sun. It is a single star of spectral class G0Ia0, that has 1100 % of solar mass. For now, there are no known exoplanets in this star system.

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Nearby stars catalogue

Sun distance
15696 light years

V509 Cassiopeiae

Yellow hypergiant

Spectral class: G0Ia0

Location +

Right ascension: 23h 0m 5.100s

Declination: 56° 56' 43.000'' (northern hemisphere)

Parallax: 0.208

Sun distance: 15,695.660 ly | 4,812.3 pc

Basic characteristic

Mass: 1100 % M Sun

Size: 500 R Sun

(estimate)

Temperature: 6000 K | 1.04 T Sun

Luminosity: 269000 L Sun

V509 Cassiopeiae system structure


	V509 Cassiopeiae

More about V509 Cassiopeiae

Star V509 Cassiopeiae is is much bigger than the Sun and temperature on its surface is around 6000 K (5727 °C), which is about 104 % of Sun's temperature.

       V509 Cassiopeiae can be found in northern celestial hemisphere.

Other designations of this star
HR 8752, HD 217476, FK5 3839, HIC 113561, HIP 113561, SAO 35039, AAVSO 2255+56

Frequently Asked Questions

How far is the V509 Cassiopeiae system from the Sun?

The V509 Cassiopeiae system is 15696 light years or 4,812.3 parsecs from the Sun.

What galaxy is the V509 Cassiopeiae star in?

The V509 Cassiopeiae is in the Milky Way galaxy just like the Sun.

How many stars are in the V509 Cassiopeiae system?

The V509 Cassiopeiae is a single star, there are no other known stars in the system.

What type of star is the V509 Cassiopeiae?

The star V509 Cassiopeiae is a Yellow hypergiant star.

What temperature is star V509 Cassiopeiae?

The star V509 Cassiopeiae has an effective temperature of 6000 K. Find out more about the temperature of stars in Stellar guide

About Stellar Catalog

Working with real data

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

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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