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Crash Course: High Mass Stars
Introduction Imagine a star so massive, it's like a cosmic nuclear reactor, fusing hydrogen into helium at an incredible rate. But what happens when these stars run out of fuel? Let's find out.
The Core Idea High mass stars are incredibly massive stars that live fast and die young. They're born with more than 8 times the mass of our sun, and they burn through their fuel in a mere 10 million years or so. When they exhaust their fuel, they collapse under their own gravity, leading to a massive explosion known as a supernova.
Key Facts & Figures
Thought Bubble Imagine you're standing on the surface of a high mass star, watching as it burns through its fuel at an incredible rate. The surface temperature is a scorching 50,000 degrees Celsius, and the star is fusing hydrogen into helium at a rate of 100 million tons per second. As you look out into space, you see the star's intense radiation and powerful winds shaping the surrounding gas and dust into a beautiful nebula. But as the star exhausts its fuel, it begins to collapse under its own gravity, leading to a massive explosion that will be seen from millions of light-years away.
Why This Matters
Crash Course Recap
Quiz Yourself
Answer: a) 10 million years
Answer: b) It collapses under its own gravity
Answer: a) VY Canis Majoris
Answer: a) The creation of heavy elements
Answer: a) They are responsible for creating many of the heavy elements found in the universe.
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