Neutron Stars & Black Holes

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Last updated 9:27 PM on 10/16/26
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15 Terms

1
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What is a neutron star?

An extremely dense stellar remnant formed when the core of a massive star collapses.

2
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What are neutron stars mainly made of?

Matter consisting largely of neutrons.

3
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Why is a neutron star extremely dense?

A large amount of mass is compressed into a very small volume.

4
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How does a neutron star form?

The core of a massive star collapses during a supernova, leaving a compact remnant.

5
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What is a black hole?

A region of space where gravity is so strong that light cannot escape from within its event horizon.

6
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How can a stellar-mass black hole form?

A sufficiently massive stellar core collapses under gravity.

7
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What is an event horizon?

The boundary beyond which light cannot escape from a black hole.

8
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Why can light not escape from inside a black hole's event horizon?

The curvature of spacetime is such that all future paths remain within the black hole.

9
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Can a black hole be observed directly using light emitted from inside it?

No, light from inside the event horizon cannot escape.

10
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How can scientists detect the presence of a black hole?

By observing its gravitational effects on nearby matter and radiation from surrounding material.

11
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What happens to nearby objects under the gravitational influence of a black hole?

Their motion is affected by its gravitational field.

12
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Does a black hole attract distant objects more strongly than any other object of the same mass?

No, at the same distance, its gravitational effect is the same as that of another object with equal mass.

13
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What is the difference between a white dwarf and a neutron star?

A neutron star is generally much denser and forms from a more massive stellar core.

14
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What is the difference between a neutron star and a black hole?

A neutron star has a physical surface, whereas a black hole has an event horizon.

15
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Why don't all stars become black holes?

Only stars with sufficiently massive collapsing cores can form stellar-mass black holes.