Stellar distances are determined by stellar parallax, which is the angular shift of stars caused by changes in the observer's position. Our solar system is part of the Milky Way galaxy, which is approximately 100,000 light years across. The basic physical stellar quantities are luminosity, temperature, chemical composition, size, and mass. A light year is approximately 9.46 x 10^12 km, and a parsec is defined as the distance where a star's parallax is 1 arcsecond, which equals 3.1 x 10^16 m or 206,263 AU. The closest stars to our solar system are Proxima Centauri and Barnard's Star.