Supernova shockwave video captured for the first time by scientists

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The shockwave generated by the explosion of an ageing giant star has been observed by an international team of astronomers for the first time.

A supernova occurs when a star collapses in on itself. Astronomers have theorised a shockwave was part of this process. The shockwave was observed when a red giant exploded.

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The star was 270 times the radius of our Sun and 750 million light years away.

Astronomers see supernova shockwave for first time, supernova shockwave video, supernova shockwave video animation, supernova shockwave animation, supernova shockwave video nasa, supernova shockwave seen for first time by scientists,

Astronomers see supernova shockwave for first time, supernova shockwave video, supernova shockwave video animation, supernova shockwave animation, supernova shockwave video nasa, supernova shockwave seen for first time by scientists,

The discovery, accepted for publishing in the Astrophysical Journal, will help scientists understand the life cycle of stars, said study co-author Brad Tucker of the Australian National University.

Astronomers see supernova shockwave for first time, supernova shockwave video, supernova shockwave video animation, supernova shockwave animation, supernova shockwave video nasa, supernova shockwave seen for first time by scientists,

Astronomers see supernova shockwave for first time, supernova shockwave video, supernova shockwave video animation, supernova shockwave animation, supernova shockwave video nasa, supernova shockwave seen for first time by scientists,

This is the first time we are seeing this in the normal visible colours, and we now know it happens.

Astronomers see supernova shockwave for first time, supernova shockwave video, supernova shockwave video animation, supernova shockwave animation, supernova shockwave video nasa, supernova shockwave seen for first time by scientists,

Here the insane video:

Shock Breakout and Early Light Curves of Type II-P Supernovae Observed with Kepler; P. M. Garnavich, B. E. Tucker, A. Rest, E. J. Shaya, R. P. Olling, D. Kasen, A. Villar. arXiv.org

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