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N132D:
NASA Space Observatories Glimpse Faint Afterglow of Nearby Stellar Explosion

N132D
Credit: X-ray: NASA/SAO/CXC; Optical: NASA, ESA, Hubble Heritage Team (STScI/AURA)
JPEG (783 kb), Tiff (23.1 MB), PS (3.8 MB)
This beautiful image shows a glowing horseshoe-shaped cloud of hot gas against a backdrop of thousands of stars in the Large Magellanic Cloud, a nearby galaxy. Observations with Chandra (X-ray/blue) and Hubble (optical/pink & purple) were used to make this composite image of N132D, a supernova remnant that was produced by the explosion of a massive star.

The explosion sent shock waves rumbling through interstellar space at speeds of several million miles per hour. These shock waves, analogous to the sonic boom produced by supersonic motion of an airplane, produce sudden, large changes in pressure, and temperature behind the waves.

Chandra X-ray of N132D
Note the change in orientation
The X-ray glow in this image is produced primarily by shock wave heating of interstellar gas to temperatures of about 10 million degrees Celsius. The horseshoe shape may have been caused by the uneven distribution of interstellar gas around the site of the explosion.

Deep within the remnant, the Hubble optical image reveals a smaller, bright crescent-shaped cloud of emission from hydrogen gas, and faint purple wisps that correspond to regions rich in oxygen atoms. These wisps provide evidence of the manufacture of oxygen and other elements such as carbon by nuclear reactions in the core of the pre-supernova star. These and other heavy elements are dispersed by the explosion and millions of years later could be incorporated into new generations of stars and their accompanying planets.

The star that exploded as a supernova to produce N132D was probably more than 20 times as massive as the Sun. Most of the stars in this image are less massive and will not go out with a bang. By comparison with N132D, they will go quietly into the night as they eventually fade away to become white dwarf stars.

Fast Facts for N132D:
Credit  X-ray: NASA/SAO/CXC; Optical: NASA, ESA, Hubble Heritage Team (STScI/AURA)
Scale  Image is 3.2 arcmin across.
Category  Supernovas & Supernova Remnants
Coordinates (J2000)  RA 05h 25m 01s.40 | Dec -69º 38' 31"
Constellation  Dorado
Observation Dates  July 20, 2000
Observation Time  20.2 hours
Obs. ID  1828
Orientation  See the annotated image
Color Code  X-ray: Blue; Optical: Pink & Purple
Instrument  ACIS
Distance Estimate  About 160,000 light years
Release Date  October 04, 2005

More Information on N132D:
Press Room: N132D Press Release
More Images of N132D
N132D Handout: html | pdf
Zoom in on N132D (flash)
Powerpoint and PDF
Download image for your desktop
Related Chandra Images:
Photo Album: DEM L71 (12 Mar 03)
Photo Album: N132D (22 May 02)
Photo Album: N132D (01 Sep 99)
More Information on Supernovas & Supernova Remnants :
X-ray Astronomy Field Guide: Supernovas & Supernova Remnants
Questions and Answers: Supernova Remnants and Neutron Stars
Chandra Images: Supernovas & Supernova Remnants
Related Links:
Optical Image: Hubble Space Telescope


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