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You entered: E0102-72
![Остаток сверхновой E0102-72 на радиоволнах и в рентгеновских лучах](https://images.astronet.ru/pubd/2006/11/07/0001217372/e0102multi_chandra_big.preview.jpg)
14.04.2000
Not all stars form a big Q after they explode. The shape of supernova remnant E0102-72, however, is giving astronomers a clue about how tremendous explosions disperse elements and interact with surrounded gas. The above image is a composite of three different photographs in three different types of light.
![Остаток сверхновой E0102 72](https://images.astronet.ru/pubd/2009/09/07/0001236016/e0102_composite900.preview.jpg)
5.09.2009
The expanding debris cloud from the explosion of a massive star is captured in this multiwavelength composite, combining x-ray and optical images from the Chandra and Hubble telescopes. Identified as E0102-72, the supernova remnant lies about 190,000 light-years away in our neighboring galaxy, the Small Magellanic Cloud.
![Горячий остаток сверхновой в ММО в рентгеновских лучах](https://images.astronet.ru/pubd/2006/11/11/0001217614/e0102_csx.preview.jpg)
9.12.1999
The Q-shaped cloud seen in this false-color X-ray image from the orbiting Chandra Observatory is big ... about 40 light-years across. It's hot too, as its X-ray glow is produced by multi-million degree gas.
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