Nuclear Fusion: The Sun's Engine

Science

The Sun converts 4 million tonnes of mass into pure energy every single second. Discover how Einstein's famous equation E=mc squared explains the Sun's incredible power and how nuclear fusion keeps the Sun shining.

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10
Questions
5–10 min
Time
Q1 Question 1 of 10

What is nuclear fusion?

Q2 Question 2 of 10

What is produced when the Sun fuses hydrogen nuclei in its core?

Q3 Question 3 of 10

What does Einstein's equation E=mc squared tell us about mass and energy?

Q4 Question 4 of 10

The Sun converts about 600 million tonnes of hydrogen into helium every second. Yet the Sun has hardly changed over billions of years. Why?

Q5 Question 5 of 10

Of the 600 million tonnes of hydrogen the Sun fuses per second, how much becomes pure energy?

Q6 Question 6 of 10

What prevents the Sun from collapsing under its own gravity?

Q7 Question 7 of 10

Why does nuclear fusion require such extreme temperatures and pressures to occur?

Q8 Question 8 of 10

Nuclear fusion in the Sun produces neutrinos. Why were solar neutrinos a mystery to scientists for decades?

Q9 Question 9 of 10

Why is nuclear fusion considered a potential clean energy source for Earth?

Q10 Question 10 of 10

How does the proton-proton chain in the Sun differ from the nuclear fission used in today's nuclear power plants?