Show Summary Details

Quick Reference

The star Alpha Virginis, magnitude 1.0. It is a spectroscopic binary consisting of a pair of B-type stars elongated by gravity so that the received light varies every 4 days as the pair orbit each other, although the amplitude is less than 0.1 mag. In addition, the primary is a variable of the Beta Cephei class, with a period of 0.17 days. Spica lies 250 l.y. away.

Subjects: Astronomy and Astrophysics.

Reference entries

Users without a subscription are not able to see the full content. Please, subscribe or login to access all content.