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0:00.0 | This is the BBC. |
0:02.0 | Thanks for downloading this episode of In Our Time. |
0:05.0 | There's a reading list to go with it on our website and you can get news about our programs |
0:09.0 | if you follow us on Twitter at BBC In Our Time. |
0:12.0 | I hope you enjoyed the programs. |
0:14.0 | Hello, there are enough protons in the sun for it to last a thousand billion years |
0:18.0 | and it's only about halfway through them, so that's a relief. |
0:22.0 | The properties of protons there, as on Earth and throughout the Universe, |
0:26.0 | are those that make chemistry biology and life itself possible. |
0:29.0 | They've existed since the split second after the Big Bang |
0:32.0 | and are found in a nuclei of all elements. |
0:35.0 | Hydrogen, by far the most abundant element in the Universe, |
0:38.0 | is a single proton with one electron. |
0:41.0 | Stripped electrons, those protons can be accelerated to smash other nuclei |
0:46.0 | to reveal more of the secrets of particle physics |
0:48.0 | and they can be used in the treatment of some cancers. |
0:51.0 | And while much is known about protons, much remains to be discovered. |
0:55.0 | We'd be to discuss the proton, Frank Close, Professor Emeritus of Physics at the University of Oxford, |
1:01.0 | Simon Jolli, lecturer in high energy physics at the University of Scotland, |
1:05.0 | and Helen Heath, reader in physics at the University of Bristol. |
1:09.0 | Frank Close, what's the proton? |
1:12.0 | Well, proton is one of the seeds of atoms. |
... |
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