Massive bodies and escape speed Gravity bends the path of light


Seeing black holes Observed properties of black holes


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Seeing black holes

Observed properties of black holes

  • Luminosity
  • Orientation
  • Jets

Gravitational energy

  • Black holes generate energy from matter falling into them.

Rotating black holes

  • For non-rotating black holes:
  • - event horizon is at the Schwarzschild radius
  • - inner edge of the disk is at 3 Schwarzschild radii
  • For maximally rotating black holes:
  • - event horizon is at ½ Schwarzschild radius
  • - inner edge of the disk is at ½ Schwarzschild radius
  • Schwarzschild radius = 3 km (M/MSun)

Luminosity

  • Gravitational energy is converted to kinetic energy as particles fall towards BH
  • Efficiency of generators:
    • Chemical burning < 0.000001%
    • Nuclear burning < 1%
    • Non-rotating black hole = 6%
    • Rotating black hole = 42%

Eddington Luminosity

  • Limit on the brightness of a black hole

Eddington Luminosity

Black holes shine brightest in X-rays

  • Why?

Luminosity of a ‘Black Body’ Radiator

  • For the spherical object, the total power radiated = the total luminosity is:
  • L = 4R2T4
  • T = temperature
  •  = Stephan-Boltzman constant
  • = 5.6710-8 W/m2 ·K4
  • R = radius

Luminosity Law

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  • 2
  • If star A is 2 times as hot as star B, and the same radius, then it will be 24 = 16 times as luminous.

Black holes shine brightest in X-rays

  • Take BH of one solar mass
  • Event horizon is 3 km or 1/200,000 of Sun’s radius
  • Luminosity can be 30,000 time the Sun’s luminosity

Black holes shine brightest in X-rays

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  • 2
  • TA = 6000  5700 K = 30,000,000 K

A object’s color depends on its surface temperature

  • Wavelength of peak radiation:
    • Wien Law max = 2.9 x 106 / T(K) [nm]

Electromagnetic spectrum

  • Black holes are so hot that they mainly produce X-rays

Review Questions

  • What are the two facts which caused Einstein to invent the special theory of relativity?
  • What are two key consequences of special relativity for how we observe moving objects?
  • What effect does gravity have on spacetime?
  • How do astronomers search for black holes?
  • How are black holes actually simpler than any other objects in astronomy?

Review Questions

  • What are fundamental versus observed properties of black holes?
  • What is the efficiency of a BH for conversion of matter to energy?
  • What is the maximum luminosity for a BH of a given mass?
  • At what wavelength range do stellar mass black holes produce most of their radiation?

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