195666666

195666666 is a notable astronomical object, specifically a star located in the constellation of Cygnus. It is classified as a main-sequence star, which means it is in the stable phase of its life cycle, converting hydrogen into helium in its core. The star is approximately 1.2 times the mass of the Sun and has a surface temperature of around 5800 Kelvin, which places it in the spectral class G2V, similar to our Sun.

195666666 is approximately 250 light-years away from Earth. Its luminosity is about 1.5 times that of the Sun, indicating it is slightly more luminous than our star. The star is part of a binary system, with a companion star that orbits it at a distance of about 100 astronomical units. The companion star is a red dwarf, much smaller and cooler than 195666666.

The star 195666666 is of particular interest to astronomers due to its similarity to the Sun. Studying this star can provide insights into the evolution and characteristics of stars similar to our own. Additionally, the binary nature of the system offers opportunities to study the interactions between stars in close orbits.