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Hubble Telescope View of a Supernova Remnant.

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Hubble telescope Supernova Remnant.
supernova remnant E0102. Image credit: Hubble.

This Hubble Space Telescope photograph contains a supernova remnant located in the Small Magellanic Cloud - it's bluish haze at the centre of the photo. The remnant is known as E0102, and it's about 50 light-years away from the edge of a massive star forming region called N 76. The light from the supernova itself would have reached us about 2,000 years ago.

Reminiscent of a U.S. July 4 Independence Day celebration, here is a NASA Hubble Space Telescope image of a cosmic explosion that is quite similar to fireworks on Earth. In the nearby galaxy, the Small Magellanic Cloud, a massive star has exploded as a supernova, and begun to dissipate its interior into a spectacular display of colorful filaments.

The supernova remnant (SNR), known as “E0102″ for short, is the greenish-blue shell of debris just below the center of the Hubble image. Its name is derived from its cataloged placement (or coordinates) in the celestial sphere. More formally known as 1E0102.2-7219, it is located almost 50 light-years away from the edge of the massive star-forming region, N 76, also known as Henize 1956 in the Small Magellanic Cloud. This delicate structure, glowing a multitude of lavenders and peach hues, resides in the upper right of the image.

Determined to be only about 2,000 years old, E0102 is relatively young on astronomical scales and is just beginning its interactions with the nearby interstellar medium. Young supernova remnants like E0102 allow Astronomers to examine material from the cores of massive stars directly. This in turn gives insight on how stars form, their composition, and the chemical enrichment of the surrounding area. As well, young remnants are a great learning tool to better understand the physics of supernova explosions.

E0102 was observed in 2003 with the Hubble Advanced Camera for Surveys. Four filters that isolate light from blue, visible, and infrared wavelengths and Hydrogen emission were combined with oxygen emission images of the SNR taken with the Wide Field Planetary Camera 2 in 1995.

The Small Magellanic Cloud is a nearby dwarf Galaxy to our own Milky Way. It is visible in the Southern Hemisphere, in the direction of the constellation Tucana, and lies roughly 210,000 light-years distant.

Original Source: Hubble News Release

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