Black Hole Questions • What happens to space-time near a ... · solar, Black hole 3.3 ≤M ≤5.5...
Transcript of Black Hole Questions • What happens to space-time near a ... · solar, Black hole 3.3 ≤M ≤5.5...
• 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
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
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
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
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
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
Viewgraph
The Event Horizon
Are black holes sucking everything into the Universe into them?—No talking to neighbors on this one.
A)YesB)No
Concept Question
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
Fig. 18.12
Fig. 18.13
Time slows downThere are strong
gravitational gradients
Strange Things that Happen Near the Event Horizon
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