Astronomy Unit 1 Flashcards

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1
Q

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

A

absorption spectrum

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2
Q

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

A

blackbody

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3
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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4
Q

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

A

dispersion

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5
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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6
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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7
Q

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

A

electromagnetic spectrum

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8
Q

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

A

emission spectrum

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9
Q

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

A

energy flux

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10
Q

a particular level, or 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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11
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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12
Q

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

A

frequency

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13
Q

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

A

gamma rays

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14
Q

he lowest energy state of an atom

A

ground state

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15
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 wavelength

A

infrared

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16
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

17
Q

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

A

ion

18
Q

the process by which an atom gains or loses electrons

A

ionization

19
Q

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

A

isotope

20
Q

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

A

microwave

21
Q

the massive part of an atom, composed mostly of protons and neutrons, and about
which the electrons revolve

A

nucleus

22
Q

a discrete unit (or “packet”) of electromagnetic energy

A

photon

23
Q

motion toward or away from the observer; the component of relative velocity that lies in the
line of sight

A

radical velocity

24
Q

all electromagnetic waves longer than microwaves, including radar waves and AM radio waves

A

radio waves

25
Q

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

A

spectrometer

26
Q

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 itsnabsolute temperature: F = σT4

A

Stefan-Boltzmann law

27
Q

electromagnetic radiation of wavelengths 10 to 400 nanometers; shorter than the shortest visible
wavelengths

A

ultraviolet

28
Q

electromagnetic radiation with wavelengths of roughly 400–700 nanometers; visible to the human
eye

A

visible light

29
Q

the distance from crest to crest or trough to trough in a wave

A

wavelength

30
Q

formula that relates the temperature of a blackbody to the wavelength at which it emits the
greatest intensity of radiadion

A

Wien’s law

31
Q

electromagnetic radiation with wavelengths between 0.01 nanometer and 20 nanometers;
intermediate between those of ultraviolet radiation and gamma rays

A

x-rays