Deck 23: Thermal Radiation
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Deck 23: Thermal Radiation
1
By definition this ideal object absorbs all energy that hits it:
A) Blackbody
B) Thermal Body
C) Nuclear Body
D) Chemical Body
A) Blackbody
B) Thermal Body
C) Nuclear Body
D) Chemical Body
Blackbody
2
The total light output of an object is called ____.
A) Wien's law
B) Stefan's Law
C) Blackbody Law
D) luminosity
A) Wien's law
B) Stefan's Law
C) Blackbody Law
D) luminosity
luminosity
3
The temperature of a body and its color (peak wavelength) is called _____.
A) Stefan's Boltzman Law
B) Wien's law
C) Blackbody law
D) Planck's law
A) Stefan's Boltzman Law
B) Wien's law
C) Blackbody law
D) Planck's law
Wien's law
4
The Sun radiates most strongly at a wavelength of about 550 nm. A star that radiated most strongly at 400 nm would be
A) hotter than the Sun.
B) cooler than the Sun.
C) the same temperature as the Sun.
D) hotter or cooler, depending on its color.
A) hotter than the Sun.
B) cooler than the Sun.
C) the same temperature as the Sun.
D) hotter or cooler, depending on its color.
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5
_________ is the vibration of the atoms.
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6
_________ is the temperature scale that starts at zero.
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7
The luminosity of a hot body rises rapidly as its temperature increases.
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8
The hotter the body, the longer waves it emits.
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