Black Holes Flashcards

1
Q

What is a black hole?

A

A black hole is a region of space-time in which gravity is so strong that nothing - not even light - can escape it.

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2
Q

What is escape velocity?

A

The speed necessary for an object to completely escape the gravity of a large body.
V esc = the square root of 2GM/R

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3
Q

What happens to the escape velocity from an object if your shrink it?

A

TBA

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4
Q

Would light be able to escape Earth’s surface if you could shrink it to less than 1 cm?

A

No

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5
Q

What is the event horizon?

A

The “surface” of a black hole that is given by the radius at which the escape velocity is equal to the speed of light.
V esc = c
Nothing can escape from within the event horizon because nothing can go faster than light.

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6
Q

What is the Schwarzschild radius?

A

Radius of the event horizon:
Rs = 2GM/c(squared)
or in kilometers:
Rs = 3 times M (solar masses)

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7
Q

What is the radius of the event horizon of a 3 Msun black hole?

A

Rs = 3 x M
3 x 3 = 9
Answer: 9 kim

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8
Q

Out galaxy has a supermassive black hole in its center with a mass of about 4 million Msun. How big is the radius of the event horizon?

A

Rs = 3 x M
(Radius of the event horizon equation)

3 x 14 million = 12 million

Answer: 12 million

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9
Q

Singularity

A

The place at the center of a black hole where, in principle, gravity crushes all matter into an indefinitely tiny and dense point.

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10
Q

How can we detect black holes?

A

Black holes’ gravitational effects can be detected. They are easiest to find if they are in close binaries (stellar-mass black holes) or if they are in the center of a galaxy (supermassive black holes)..

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11
Q

What are stellar-mass black holes?

A

Small black holes approximately 3 to 10+ solar masses. They can form through supernovae, neutron stars or white dwarfs that accrete mass beyond 3 solar masses, and neutron stars that merge.

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