Beta Capricorni, also known as Dabih, is a binary star system located in the constellation of Capricornus. It is approximately 328 light-years away from Earth and consists of two stars: a bright giant and a smaller companion star. Dabih is notable for its distinct yellow hue, which is characteristic of its spectral type. The primary star in the system is classified as a G-type giant, while the secondary star is a K-type main-sequence star. Together, they form a visually appealing pair in the night sky, making Beta Capricorni a popular target for amateur astronomers and stargazers.