Black Hole Questions • What happens to space-time near a ... · solar, Black hole 3.3 ≤M ≤5.5...

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• What happens to space-time near a black hole? • Why are black holes black? • What observational evidence do we have for black holes? Black Hole Questions

Transcript of Black Hole Questions • What happens to space-time near a ... · solar, Black hole 3.3 ≤M ≤5.5...

Page 1: Black Hole Questions • What happens to space-time near a ... · solar, Black hole 3.3 ≤M ≤5.5 M solar •Variable X-ray emission (radius ≤300 km) Observational Evidence for

• What happens to space-time near a black hole?

• Why are black holes black?• What observational evidence

do we have for black holes?

Black Hole Questions

Page 2: Black Hole Questions • What happens to space-time near a ... · solar, Black hole 3.3 ≤M ≤5.5 M solar •Variable X-ray emission (radius ≤300 km) Observational Evidence for

Few SolarMasses

>106

Solar Masses

Core-collapse supernovae: for M > 3Msolar neutron degeneracy pressure cannot support a star against gravity

Supermassive black holes that form in the centers of galaxies as they form

Black Holes: Formation

Page 3: Black Hole Questions • What happens to space-time near a ... · solar, Black hole 3.3 ≤M ≤5.5 M solar •Variable X-ray emission (radius ≤300 km) Observational Evidence for

Newton (1687)

F = GM1M2/R2

Einstein

Special Relativity (1905) -Relates space and time in a 4-dimensional spacetime (nothing can move faster than the speed of light)

General Relativity (1915)-Gravity is the curvature of space by mass⇒Even light is bent by gravity!

What if M1=0?

A New Theory of Gravity

Page 4: Black Hole Questions • What happens to space-time near a ... · solar, Black hole 3.3 ≤M ≤5.5 M solar •Variable X-ray emission (radius ≤300 km) Observational Evidence for

Spacetime around the Sun Spacetime around a 1Msolarwhite dwarf

Fig.

S3-

15A

Fig.

S3-

15B

Spacetimearound the Sun compressed to a black hole

The Curvature of Space

Page 5: Black Hole Questions • What happens to space-time near a ... · solar, Black hole 3.3 ≤M ≤5.5 M solar •Variable X-ray emission (radius ≤300 km) Observational Evidence for

What would happen to the Earth’s orbit if the Sun were replaced with a 1 Msolar black hole?

A)The Earth would spiral into the black hole.B)NothingC)The Earth would escape from the solar

system.

Concept Question

Page 6: Black Hole Questions • What happens to space-time near a ... · solar, Black hole 3.3 ≤M ≤5.5 M solar •Variable X-ray emission (radius ≤300 km) Observational Evidence for

What would happen to the Earth’s orbit if the Sun were replaced with a 1 Msolar black hole?

A)The Earth would spiral into the black hole.B)NothingC)The Earth would escape from the solar

system.

Concept Question

Page 7: Black Hole Questions • What happens to space-time near a ... · solar, Black hole 3.3 ≤M ≤5.5 M solar •Variable X-ray emission (radius ≤300 km) Observational Evidence for

Viewgraph

The Event Horizon

Page 8: Black Hole Questions • What happens to space-time near a ... · solar, Black hole 3.3 ≤M ≤5.5 M solar •Variable X-ray emission (radius ≤300 km) Observational Evidence for

Are black holes sucking everything into the Universe into them?—No talking to neighbors on this one.

A)YesB)No

Concept Question

Page 9: Black Hole Questions • What happens to space-time near a ... · solar, Black hole 3.3 ≤M ≤5.5 M solar •Variable X-ray emission (radius ≤300 km) Observational Evidence for

Are black holes sucking everything into the Universe into them?—No talking to neighbors on this one.

A)YesB)No!—This is a popular

misconception

Concept Question

Page 10: Black Hole Questions • What happens to space-time near a ... · solar, Black hole 3.3 ≤M ≤5.5 M solar •Variable X-ray emission (radius ≤300 km) Observational Evidence for

Fig. 18.12

Fig. 18.13

Time slows downThere are strong

gravitational gradients

Strange Things that Happen Near the Event Horizon

Page 11: Black Hole Questions • What happens to space-time near a ... · solar, Black hole 3.3 ≤M ≤5.5 M solar •Variable X-ray emission (radius ≤300 km) Observational Evidence for

Cygnus X-1

Fig.

18.

14A

Fig.

18.

03

•Discovered in the 1970s by UHURU•2 kpc distant•Companion 8.5 ≤ M ≤ 20 Msolar, Black hole 3.3 ≤ M ≤ 5.5 Msolar•Variable X-ray emission (radius ≤ 300 km)

Observational Evidence for Solar-Mass-Scale Black Holes