Beta Corvi or β Corvi, officially named Kraz (/ ˈkræz /), [9] is the second-brightest star in the southern constellation of Corvus with an apparent visual magnitude of 2.647. [2]

Nov 9, 2020 · Kraz, Beta Corvi (β Crv), is a yellow bright giant located in the constellation Corvus. With an apparent magnitude of 2.647, it is the second brightest star in Corvus, after Gienah. It …

The four brightest stars, Gamma, Delta, Epsilon, and Beta Corvi, form a distinctive quadrilateral or cross -shape in the night sky. With an apparent magnitude of 2.59, Gamma Corvi—also known …

Beta Corvi, or Kraz, is a yellow-white G-type bright giant 140 light years distant from Earth. The star’s visual magnitude varies between 2.60 and 2.66. Beta Corvi is the second brightest star …

Kraz, also designated as β Corvi (beta Corvi), is a variable bright giant star of spectral class G5 in the constellation of Corvus. Kraz visual magnitude is 2.65.

Jul 12, 2016 · Although Corvus has no bright stars, its four brightest stars form a distinctive asterism known as THE SAIL (SPICA’S SPANKER), which is made up of Delta, Gamma, …

Kraz, also known as Beta Corvi, is the second brightest star in Corvus and has a visual magnitude that varies between 2.60 and 2.66. It is a yellow-white G-type bright giant that is located 140 …

Beta Corvi (Kraz) – This magnitude 2.66, yellow-orange giant, variable star is the second brightest star in Corvus and, is the southeastern star in the Sail asterism. It’s an eruptive variable …

Beta Corvi is a green dwarf star located at 033.3 : 981.2 in the Corvi constellation. The star system contains seven planets and a single moon. The Precursors visited here several times, …

This pattern is made up of four primary stars: Gamma, Delta, Epsilon, and Beta Corvi, which have apparent magnitudes ranging from 2.59 to 3.10, making them easily visible to the naked eye …