COLLECTION NAME:
NASA Planetary Photo Journal Collection
Record
Title:
Luminous Blue Variable: Destined To Be a Supernova?
Original Caption Released with Image:
Click on the image for full resolution Poster Version of Diagram 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 that exploded in 1987 in the Large Magellanic Cloud, and was the nearest supernova 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 on Spitzer 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.
Image Credit:
NASA/JPL-Caltech/UC Berkeley
Produced By:
California Institute of Technology
Mission:
Spitzer Space Telescope (SST)
Spacecraft:
Spitzer Space Telescope (SST)
Instrument:
Infrared Array Camera (IRAC)
Product Size:
720 samples x 720 lines
facet_what:
Earth
facet_where:
California
facet_when:
1987
facet_when_year:
1987
Image #:
PIA09119
UID:
SPD-PHOTJ-PIA09119
