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supernova

"One of the most energetic explosive events known is a supernova. These occur at the end of a star's lifetime, when its nuclear fuel is exhausted and it is no longer supported by the release of nuclear energy. If the star is particularly massive, then its core will collapse and in so doing will release a huge amount of energy. This will cause a blast wave that ejects the star's envelope into interstellar space. The result of the collapse may be, in some cases, a rapidly rotating neutron star that can be observed many years later as a radio pulsar." What this means is that when a star explodes it releases so much radiation and all this releases more energy that the sun would in its life span. This process could last up to a few weeks to a few months.


[1]

Speedy deletion nomination of Wanna see?

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Thank you for experimenting with Wikipedia. Your test worked, and the page that you created has been or soon will be deleted. Please use the sandbox for any other tests you want to do. Take a look at the welcome page if you would like to learn more about contributing to our encyclopedia.

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  1. ^ Tyler, Pat. [heasarc.nasa.gov/docs/snr.html "Supernova"]. astronomer. Pat Tyler. Retrieved October 19, 2011. {{ cite web}}: Check |url= value ( help)
From Wikipedia, the free encyclopedia

Welcome!

Hello, Youcantrustme420, and welcome to Wikipedia! Thank you for your contributions. I hope you like the place and decide to stay. Here are some pages that you might find helpful:

I hope you enjoy editing here and being a Wikipedian! Please sign your messages on discussion pages using four tildes (~~~~); this will automatically insert your username and the date. If you need help, check out Wikipedia:Questions, ask me on my talk page, or ask your question on this page and then place {{help me}} before the question. Again, welcome! -- Mayur (talkEmail) 16:26, 14 October 2011 (UTC) reply

supernova

"One of the most energetic explosive events known is a supernova. These occur at the end of a star's lifetime, when its nuclear fuel is exhausted and it is no longer supported by the release of nuclear energy. If the star is particularly massive, then its core will collapse and in so doing will release a huge amount of energy. This will cause a blast wave that ejects the star's envelope into interstellar space. The result of the collapse may be, in some cases, a rapidly rotating neutron star that can be observed many years later as a radio pulsar." What this means is that when a star explodes it releases so much radiation and all this releases more energy that the sun would in its life span. This process could last up to a few weeks to a few months.


[1]

Speedy deletion nomination of Wanna see?

If this is the first article that you have created, you may want to read the guide to writing your first article.

You may want to consider using the Article Wizard to help you create articles.

Thank you for experimenting with Wikipedia. Your test worked, and the page that you created has been or soon will be deleted. Please use the sandbox for any other tests you want to do. Take a look at the welcome page if you would like to learn more about contributing to our encyclopedia.

If you think that this notice was placed here in error, contest the deletion by clicking on the button labelled "Click here to contest this speedy deletion". Doing so will take you to the talk page where you will find a pre-formatted place for you to explain why you believe the page should not be deleted. You can also visit the page's talk page directly to give your reasons, but be aware that once tagged for speedy deletion, if the page meets the criterion, it may be deleted without delay. Please do not remove the speedy deletion tag yourself, but don't hesitate to add information to the page that would render it more in conformance with Wikipedia's policies and guidelines. If the page is deleted, you can contact one of these administrators to request that the administrator userfy the page or email a copy to you. France3470 (talk) 14:24, 20 October 2011 (UTC) reply

  1. ^ Tyler, Pat. [heasarc.nasa.gov/docs/snr.html "Supernova"]. astronomer. Pat Tyler. Retrieved October 19, 2011. {{ cite web}}: Check |url= value ( help)

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