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中性子星のライフサイクル
1,372,686 views |
デイビッド・ラニー |
TED-Ed
• November 2018
Read transcript
百年ごとに銀河系のどこかで大質量星が燃料を使い果たします。その構造を支える十分なエネルギーを作れないため、重力崩壊により超新星爆発を起こします。そのような恒星の終焉は、宇宙で最も密度の高い天体の１つとして知られる中性子星の誕生です。デイビッド・ラニーが中性子星とは一体何なのかを探求します。 講師: デイビッド・ラニー 監督: JodyPrody このビデオの教材 : https://ed.ted.com/lessons/the-life-cycle-of-a-neutron-star-david-lunney
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