Luminous Blue Variable HD 168625: Destined To Be a Supernova?
Sig07 003

Credit: NASA/JPL-Caltech/N. Smith (UC Berkeley)

Artwork • January 9th, 2007 • sig07-003


A Luminous Blue Variable star (inset) in our galaxy, named HD168625, surrounded by a bipolar nebula that is similar to the one around SN1987A. SN1987A was a supernova in the Large Magellanic Cloud that was first seen on Earth in 1987, and was the nearest supernova detected in about 400 years.

The diagram explains the bipolar nebula around HD168625, which has a geometry that makes it a near twin of the famous nebula around SN1987A. Rings near the equator are sometimes seen around stars that shed mass from their surfaces, but the larger rings above the poles are very rare. Tipped toward Earth and illuminated by the star, the rings look like ellipses in images taken with NASA's Spitzer Space Telescope.

The image was taken in 2004 by the Infrared Array Camera (IRAC) on NASA's Spitzer Space Telescope at wavelengths between 3.6 and 8 microns. The massive star at the center, which lies within the constellation Sagittarius, is about 7,200 light-years from Earth.

About the Object

Star > Type > Variable
Star > Evolutionary Stage > Blue Supergiant
Star > Evolutionary Stage > Supernova
Star > Circumstellar Material > Outflow
Nebula > Type > Supernova Remnant
7,176 Light Years