Gravitational Lensing as Evidence

Science

Einstein's general relativity predicts that mass bends light. Astronomers have turned this effect into a powerful tool to map the invisible — using the distortion of distant galaxies to weigh dark matter halos that emit no light at all.

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11
Questions
5–10 min
Time
Q1 Question 1 of 11

What is gravitational lensing?

Q2 Question 2 of 11

Which physical theory predicts that massive objects bend light?

Q3 Question 3 of 11

What is an Einstein ring?

Q4 Question 4 of 11

What is the difference between strong gravitational lensing and weak gravitational lensing?

Q5 Question 5 of 11

Why is gravitational lensing useful for detecting dark matter?

Q6 Question 6 of 11

What is the Bullet Cluster?

Q7 Question 7 of 11

Why does the hot gas in the Bullet Cluster slow down during the collision while the dark matter does not?

Q8 Question 8 of 11

How do astronomers detect the dark matter in the Bullet Cluster?

Q9 Question 9 of 11

What do lensing maps of galaxy clusters consistently show about their mass distribution?

Q10 Question 10 of 11

Why is the Bullet Cluster considered the most direct observational evidence for dark matter?

Q11 Question 11 of 11

Which space telescopes have been specifically designed to perform weak gravitational lensing surveys to study dark matter?