5: Radiation and Spectra Flashcards

(35 cards)

1
Q

general term for waves (including light waves) that emit outward from a source

A

radiation

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2
Q

in physics, describes the action of forces that one object exerts on other distant objects

A

field

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3
Q

nonexistent substance said to fill all of space, proposed by nineteenth-century scientists to explain movement of electromagnetic waves

A

aether

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4
Q

number of cycles in a wave per second

A

hertz (Hz)

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5
Q

a series or pattern of dark lines superimposed on a continuous spectrum

A

absorption spectrum

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6
Q

an idealized object that absorbs all electromagnetic energy that falls onto it

A

blackbody

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7
Q

a spectrum of light composed of radiation of a continuous range of wavelengths or colors, rather than only certain discrete wavelengths

A

continuous spectrum

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8
Q

separation of different wavelengths of white light through refraction of different amounts

A

dispersion

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9
Q

the apparent change in wavelength or frequency of the radiation from a source due to its relative motion away from or toward the observer

A

Doppler effect

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10
Q

radiation consisting of waves propagated through regularly varying electric and magnetic fields and traveling at the speed of light

A

electromagnetic radiation

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11
Q

the whole array or family of electromagnetic waves, from radio to gamma rays

A

electromagnetic spectrum

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12
Q

a series or pattern of bright lines superimposed on a continuous spectrum

A

emission spectrum

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13
Q

the amount of energy passing through a unit area (for example, 1 square meter) per second - watts per square meter

A

energy flux

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14
Q

a particular amount of energy possessed by an atom or ion above the energy it possesses in its least energetic state; also used to refer to the states of energy an electron can have in an atom

A

energy level

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15
Q

the process of giving an atom or an ion an amount of energy greater than it has in its lowest energy (ground) state

A

excitation

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16
Q

the number of waves that cross a given point per unit time (in radiation)

17
Q

photons (of electromagnetic radiation) of energy with wavelengths no longer than 0.01 nanometer; the most energetic form of electromagnetic radiation

18
Q

the lowest energy state of an atom

19
Q

electromagnetic radiation of wavelength 103–106 nanometers; longer than the longest (red) wavelengths that can be perceived by the eye, but shorter than radio wavelengths

20
Q

(for light) the amount of energy (light) flowing through a given area in a given time decreases in proportion to the square of the distance from the source of energy or light

A

inverse square law

21
Q

an atom that has become electrically charged by the addition or loss of one or more electrons

22
Q

the process by which an atom gains or loses electrons

23
Q

any of two or more forms of the same element whose atoms have the same number of protons but different numbers of neutrons

24
Q

electromagnetic radiation of wavelengths from 1 millimeter to 1 meter; longer than infrared but shorter than radio waves

25
the massive part of an atom, composed mostly of protons and neutrons, and about which the electrons revolve
nucleus (of an atom)
26
a discrete unit (or “packet”) of electromagnetic energy
photon
27
motion toward or away from the observer; the component of relative velocity that lies in the line of sight
radial velocity
28
all electromagnetic waves longer than microwaves, including radar waves and AM radio waves
radio waves
29
an instrument for obtaining a spectrum; in astronomy, usually attached to a telescope to record the spectrum of a star, galaxy, or other astronomical object
spectrometer
30
a formula from which the rate at which a blackbody radiates energy can be computed; the total rate of energy emission from a unit area of a blackbody is proportional to the fourth power of its absolute temperature: F = σT4
Stefan-Boltzmann law
31
electromagnetic radiation of wavelengths 10 to 400 nanometers; shorter than the shortest visible wavelengths
ultraviolet
32
electromagnetic radiation with wavelengths of roughly 400–700 nanometers; visible to the human eye
visible light
33
the distance from crest to crest or trough to trough in a wave
wavelength
34
formula that relates the temperature of a blackbody to the wavelength at which it emits the greatest intensity of radiation
Wien's law
35
electromagnetic radiation with wavelengths between 0.01 nanometer and 20 nanometers; intermediate between those of ultraviolet radiation and gamma rays
X-rays