Light from our Universe Flashcards

1
Q

Radiation from the Universe

A

Energetic sub-atomic particles or wave traveling outward from a source

Particle with mass
- Cosmic rays

Radiation with no mass

  • Light: electromagnetic (EM)
  • Gravitational waves
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2
Q

Light as Observed

A

Carrying energy: Sunlight warms up the Earth

Travel at a constant speed

Can be absorbed/emitted

Travel at a straight line

  • can bend when going into water
  • can reflect/diffract/interfere
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3
Q

Light as EM Wave

A

Travel at v= c in vacuum

Carrying Energy

Frequency: 𝜐= c/𝝀

Used to describe low-energy radio, infrared radiation

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4
Q

Light as Particle - Photons

A

Carry quantized amount of energy

  • E=h𝜐
  • Higher frequency photons carry more energies

Can interact like particles

  • elastic collision
  • reflection/refraction

Used to describe higher energy radiations
- X-rays, gamma-rays

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5
Q

Propagation of light

A

Energy per unit area decreases as the square of the distance from the source

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6
Q

Spectral Lines

A

a dark or bright line in an otherwise uniform and continuous spectrum, resulting from emission or absorption of light in a narrow frequency range, compared with the nearby frequencies

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7
Q

Emission Lines

A

a bright line in the emission spectrum

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8
Q

Absrobtion Lines

A

dark lines, or lines of reduced intensity, on a continuous spectrum

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9
Q

Radiation Mechanisms Exploited in Astronomy

A

Neutral Hydrogen 21-cm Line

Blackbody Radiation

Synchrotron Radiation

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10
Q

Neutral Hydrogen 21-cm Line

A

Hydrogen is the most abundant element in the interstellar medium

Lie in microwave radio frequency, can penetrate interstellar dust which are opaque to visible light

Exceptionally sensitive tracer of tidal interactions between galaxies

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11
Q

Blackbody Radiation

A

thermal radiation

From an object that absorbs all radiations falling on it or from an object with thermal equilibrium with its environment
- e.g., cosmic microwave background

Dependent solely on the temperature of the emitter

Distinct spectrum: β€œhot stars are blue, cold stars are red”

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12
Q

Synchrotron Radiation

A

non-thermal radiation

From relativistic charged particles, usually electrons, spiralling/accelerating in magnetic field

Each radiate in a range of wavelength

Synchrotron radiation is a sum of radiations of many electrons

Radio synchrotron radiation can be found in places with magnetic fields and electrons
- Pulsars, supernovae, and jets in active galaxy or near the black holes

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