by A giant star called VVV-WIT-08 exhibited a smooth, eclipse-like drop in brightness to a depth of 97% in 2012; minimum brightness occurred in April 2012 and the total event duration was a few hundred days, according to an analysis of data from the VISTA Variables in the Via Lactea survey (VVV), a project using the British-built VISTA telescope in Chile and operated by ESO.
VVV-WIT-08 is a giant star located more than 25,000 light-years away in the constellation of Sagittarius.
It may belong to a new class of ‘blinking’ binary system, where a giant star — 100 times larger than the Sun — is eclipsed once every few decades by an as-yet unseen orbital companion.
The companion, which may be another star or a planet, is surrounded by an opaque disk, which covers the giant star, causing it to disappear and reappear in the sky.
Source
VVV-WIT-08 is a giant star located more than 25,000 light-years away in the constellation of Sagittarius.
It may belong to a new class of ‘blinking’ binary system, where a giant star — 100 times larger than the Sun — is eclipsed once every few decades by an as-yet unseen orbital companion.
The companion, which may be another star or a planet, is surrounded by an opaque disk, which covers the giant star, causing it to disappear and reappear in the sky.
Source
