Astronomy and Space

Kepler-35

Kepler-35 is a binary star system in the constellation of Cygnus. These stars, called Kepler-35A and Kepler-35B have masses of 89% and 81% solar masses respectively, and both are assumed to be of spectral class G. They are separated by 0.176 AU, and complete an eccentric orbit around a common center of mass every 20.73 days.

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See also

• ▸Bonnie Buratti
• ▸Casbah of Algiers
• ▸Fermi Gamma-ray Space Telescope

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