The _______________ is the amount of energy needed to pull an electron completely away from the nucleus.
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Q50: A(n) _ is an atom that has
Q51: The position of an absorption or emission
Q52: An atom can only have orbits of
Q53: The _ temperature scale is used in
Q54: During the first year of its operation,
Q56: An object that is a perfect absorber
Q57: A star like the Sun emits a(n)
Q58: Absorption lines are produced by _.
A) atoms
Q59: The Doppler effect is useful in measuring
Q60: What physical situation is necessary to create
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