Star TIC 241249532
Red dwarf TIC 241249532 is located 1028 light years away from the Sun.
It is a single star, that has 45 % of solar mass.
For now, there are no known exoplanets in this star system.
Frequently Asked Questions
How far is the TIC 241249532 system from the Sun?
The TIC 241249532 system is 1028 light years or 315.2 parsecs from the Sun.
What galaxy is the TIC 241249532 star in?
The TIC 241249532 is in the Milky Way galaxy just like the Sun.
How many stars are in the TIC 241249532 system?
The TIC 241249532 is a single star, there are no other known stars in the system.
What type of star is the TIC 241249532?
The star TIC 241249532 is a Red dwarf star.
What temperature is the TIC 241249532?
The primary in the TIC 241249532 system has an effective temperature of K ( °C). Find out more about the temperature of stars in
Stellar guide
Class of stars Red dwarf
Red dwarfs are small, cool stars with surface temperatures of about 2,000–3,800 K, much cooler than the Sun. They usually have 8–50% of the Sun’s mass and shine very faintly, sometimes at just a tiny fraction of the Sun’s brightness. Classified mainly as spectral type M, they are the most common stars in the Milky Way, making up roughly 70–75% of its stellar population.
They fuse hydrogen slowly through the proton–proton chain and are fully convective, which allows them to use their fuel very efficiently. As a result, red dwarfs can live for tens of billions to trillions of years—far longer than the Sun. Many exoplanets orbit red dwarfs, including some in close habitable zones, though strong stellar activity can affect planetary environments.
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More about Star mass in StellarGuide
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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.
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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