Draft:AB Doradus c

AB Doradus C is the third component of the Trio of stars at make up the AB Doradus system in the constellation of the same system. This system is located approximately 48 Light-year from Earth. AB Doradus C is known as a Red dwarf, a type of star with low mass and low Temperature. Its mass is estimated to be about 0.2 Solar mass, and it has very weak radiant Energy compared to the sun.

AB Doradus C is a member of a trio also formed by the stars AB DoradusAB dorsus is located in the constellation of the dolphin ​ A and B. These three stars are gravitationally bound together and orbit around a common center of gravity. This system was studied as an example of a young star cluster because AB Doradus A is a young Star with an age of around 75 to 120 1,000,000 Year.

AB Doradus C has been observed using a variety of astronomical methods, including spectroscopy and photometry, allowing astronomers to study its properties and characteristics. Its low mass and temperature place it among M type objects, which are the coolest and darkest stars.

AB Doradus C research has broader implications for the study of stellar evolution and star system formation. It can provide important information about the formation of planet and other bodies in the universe, because these processes are closely related to young Star system like AB Doradus ​