Hubble Captures the Supernova Remnant 1E 0102.2-7219
Featured in this Hubble image is an expanding, gaseous corpse — a supernova remnant — known as 1E 0102.2-7219. It is the remnant of a star that exploded long ago in the Small Magellanic Cloud, a satellite galaxy of our Milky Way located roughly 200 000 light-years away.
Because the gaseous knots in this supernova remnant are moving at different speeds and directions from the supernova explosion, those moving toward Earth are colored blue in this composition and the ones moving away are shown in red. This new Hubble image shows these ribbons of gas speeding away from the explosion site at an average speed of 3.2 million kilometers per hour. At that speed, you could travel to the Moon and back in 15 minutes.
Credit:NASA, ESA, and J. Banovetz and D. Milisavljevic (Purdue University)
About the Image
Id: | heic2102a |
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Type: | Observation |
Release date: | 15 January 2021, 10:00 |
Related releases: | heic2102 |
Size: | 2160 x 1294 px |
About the Object
Name: | 1E 0102.2-7219 |
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Type: | Milky Way : Nebula : Type : Supernova Remnant |
Constellation: | Tucana |
Category: | Nebulae |
Wallpapers
Coordinates
Position (RA): | 1 4 0.25 |
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Position (Dec): | -72° 2' 3.51" |
Field of view: | 1.41 x 0.85 arcminutes |
Orientation: | North is 3.2° left of vertical |
Colours & filters
Band | Wavelength | Telescope |
---|---|---|
Optical b | 467 nm |
Hubble Space Telescope
WFC3 |
Optical z(H-beta) | 492 nm |
Hubble Space Telescope
WFC3 |
Optical OIII | 502 nm |
Hubble Space Telescope
WFC3 |
Optical H-alpha + NII | 657 nm |
Hubble Space Telescope
WFC3 |
Optical z(H-alpha + NII) | 665 nm |
Hubble Space Telescope
WFC3 |
Optical z(OIII) | 508 nm |
Hubble Space Telescope
WFC3 |
Optical SII | 673 nm |
Hubble Space Telescope
WFC3 |