Lecture 7:Spectroscopy & Astrophysics Flashcards

1)properties of blackbody radiation 2)Wein's and Stefan Boltzmann's laws 3)Kirchhoff’s laws and properties (emission/ absorption lines) of spectra 4)Doppler effect of light

1
Q

List the type of rays in order starting from lowest wavelength to highest wavelength

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2
Q

Thermal energy comes from kinetic energy of its internal particles. The greater its thermal energy, the hotter the object is

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3
Q

A blackbody is an ideal object that does not reflect any light and thus emits electromagnetic radiation in all wavelengths entirely as a result of its
temperature

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4
Q

Blackbody radiation: it refers to the light emitted by a blackbody

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5
Q

Wein’s law: The blackbody radiation consists of a continuous spectrum that peaks at a certain wavelength (or frequency

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6
Q

Peak of blackbody radiation = wavelength of maximum emission =>
wavelength at which the object looks brightest (gives colours to objects)

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7
Q

Stefan-Boltzmann’s law: The higher an object’s temperature, the more intensely the object emits electromagnetic radiation at all wavelengths and
the shorter the wavelength at which it emits most strongly

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8
Q

Explain Kirchoff’s three laws to do with the line spectrum of objects.

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9
Q

Explain the Lyman, Balmer, Paschen series of electron transitions

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10
Q

What is doppler effect?
When is blue shift seen when is red shift seen?

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