Polaris
is a trinary system, consisting of a large yellow Cepheid
variable (a UMi A), distantly (about 2700 AU or 380 billion
km) orbited by a bright yellow dwarf (a UMi B). Polaris
B can be seen with even a modest telescope and was first
noticed by William Herschel in 1780. In 1929, it was discovered
by examining the spectrum of Polaris A that it had another
very close dwarf companion (variously a UMi P, a UMi a
or a UMi Ab). In January 2006, NASA released images from
the Hubble telescope, directly showing all three members
of the Polaris trinary system. The nearer dwarf star is
in an orbit of only 20 AU (3 billion km) from Polaris
A, explaining why its light is swamped by its close and
much brighter companion. |