An O-type star in the constellation Aurgia which is also one of the best known runaway
stars. It is one of three stars, the others being Mu Columbae and 53
Arietis, which are moving rapidly on divergent paths from a common point
in space near where the Trapezium in Orion presently lies. Approximately 2.7 million years ago an event occurred that
violently ejected these three stars: it may have been a supernova explosion or, alternately, a close encounter between two massive binary
|AE Aurigae (center right) amid the Flaming Star Nebula,
which it illuminates. Image by the KPNO 0.9-meter telescope. Credit:
T. A. Rector & B. A. Wolpa, NOAO, AURA, NSF
Although intrinsically very luminous, AE Aurigae lies close to the limit
of naked-eye visibility in our skies. Its apparent faintness is due to a
combination of its great distance and the fact that a significant fraction
of its light is absorbed by interstellar dust. As its name implies, it is
also a variable star.
AE Aurigae is presently passing through an unrelated interstellar cloud
of gas and dust that it is illuminating and giving rise to the so-called Flaming Star Nebula.
||1,460 ± 480 light-years
||R.A. 05h 16m 18.2s,
Dec. +34° 18' 43"
|HR 1712, HD 34078,
BD+34°980, HIP 24575,
SAO 57816, GC 6429,