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The element first found in the Sun's spectrum,then on Earth 30 years later,is:


A) hydrogen.
B) helium.
C) solarium.
D) technetium.
E) aluminum.

F) All of the above
G) C) and D)

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A low density gas must be hot in order to produce an absorption line.

A) True
B) False

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Because the changes in energy levels happen in discrete steps,we refer to these as ________ leaps.

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What information about an astronomical object can be determined by observing its spectrum?


A) its temperature
B) its radial motion
C) its chemical composition
D) whether it has a strong magnetic field
E) All of the above

F) B) and E)
G) C) and E)

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The spectral lines of each element are distinctive to that element,whether we are looking at emission or absorption lines.

A) True
B) False

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An emission spectrum can be used to identify a(n) :


A) proton.
B) electron.
C) neutron.
D) atom.
E) neutrino.

F) C) and D)
G) A) and B)

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Define absorption lines.

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When light from a continuous source,such...

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Which of these is the classic continuous spectrum?


A) sunlight
B) a rainbow
C) a neon light
D) a fluorescent light
E) a glowing nebula, such as M-42

F) A) and E)
G) C) and D)

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If we increased the pressure in the gas of a blackbody,how will the spectral lines be affected?

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The lines will broad...

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All wavelengths of light travel at the same speed in a vacuum,and carry the same energy per photon.

A) True
B) False

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Why is spectroscopy important to astronomers?

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Virtually all the information we receive...

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According to the Zeeman effect,the splitting of a sunspot's spectral lines is due to:


A) their rapid rotation.
B) temperature variations.
C) their magnetic fields.
D) their radial velocity.
E) a Doppler shift.

F) B) and E)
G) B) and C)

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C

All Lyman emission lines are transitions from the excited state to ________ state.

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ground

A hydrogen atom consists of an electron and a(n) :


A) proton.
B) ion.
C) neutrino.
D) neutron.
E) lepton.

F) All of the above
G) A) and B)

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The longer the wavelength of the photon,the ________ the energy it carries.

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How many blue photons (frequency of 6.50 ร— 10ยนโด hz)per second would be required to carry 1 Watt (1 Watt = 1 Joule per second)of energy?

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Using E = hf and h = 6.63 ร— 10...

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The colors of a neon light arise because it is a(n)________ spectrum.

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emission (or bright line)

The three laws dealing with the creation of various spectra are due to:


A) Newton.
B) Fraunhofer.
C) Kirchhoff.
D) Bohr.
E) Einstein.

F) B) and E)
G) A) and E)

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The radial velocity of a star's motion in space can also broaden its spectral lines.

A) True
B) False

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A heavy neutral atom,such as iron,produces many spectral lines compared to light elements like hydrogen and helium.Why?


A) Because of the larger number of electrons and corresponding energy levels, more transitions are possible.
B) Because of the larger number of electrons, there are many ionization levels possible.
C) Because of the larger number protons, the amount of force holding the electrons to the atom can vary between different iron atoms.
D) Because of the atom's larger size, it will be hit by more photons in a beam of light.

E) C) and D)
F) None of the above

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