A well -
known eclipsing binary makes up part of Algol, a multiple - star system in the constellation Perseus.
Not exact matches
The newly discovered system,
known only by its astronomical catalogue number TYC 2505 -672-1, sets a new record for both the longest duration stellar
eclipse and the longest period between
eclipses in a
binary system.
That is just what happens in a newly discovered system,
known only by its astronomical catalogue number TYC 2505 -672-1, setting a new record for both the longest duration stellar
eclipse and the longest period between
eclipses in a
binary star system.
Theta1 B, also
known as BM Orionis, is another
eclipsing binary, spectral type B2 - B3, with a period of 6.471 days and a magnitude range of 7.90 to 8.65.
Theta1 Orionis A, also
known as V1016, is an
eclipsing binary with a period of 65.432 days and a magnitude range of 6.72 to 7.65.