Radiation and Spectroscopy Test Review Flashcards

1
Q

The number of waves passing the observer per second is:

A

The frequency in Hertz

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2
Q

Both sound waves and electromagnetic radiation:

A

Transfer energy

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3
Q

What does the phenomenon of diffraction demonstrate?

A

The wave nature of light

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4
Q

What does the phenomenon of interference demonstrate?

A

The particle nature of the photon

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5
Q

Which of these is constant for ALL types of electromagnetic radiation in a vacuum?

A

Velocity

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6
Q

Electromagnetic radiation:

A

Can behave both as a wave and as a particle

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7
Q

Of all the forms of electromagnetic radiation, the one with the lowest frequency is:

A

Radio Waves

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8
Q

The two forms of electromagnetic radiation that penetrate the atmosphere best are:

A

Visible and Radio Waves

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9
Q

Colors appear different to us because of their photons’ different:

A

Frequencies

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10
Q

Which type of radiation can be observed well from Earth’s surface?

A

Visible

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11
Q

The wavelength at which a blackbody radiates most depends on its:

A

Temperature

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12
Q

Star A and Star B have the same temperature, but Star A is 5 times bigger than Star B. Which statement below is correct?

A

Star A and B have the same color, but Star A is brighter.

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13
Q

What is spectroscopy?

A

An analysis of the way in which atoms absorb and emit light.

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14
Q

Typical stellar spectra appear as:

A

A rainbow, but with some dark lines mixed in

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15
Q

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

A

Kirchhoff

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16
Q

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

A

Helium

17
Q

An incandescent light (glowing tungsten filament) produces:

A

A continuous spectrum, with the peak giving the temperature of the filament.

18
Q

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

A

Atom

19
Q

In Bohr’s model of the atom, electrons:

A

only make transitions between orbitals of specific energies.

20
Q

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

21
Q

Why are molecular lines more complex than elemental spectral lines?

A

Molecules can vibrate and rotate as well.

22
Q

Spectral lines are often referred to as the stars’ “fingerprints” because:

A

All of these are correct

23
Q

The observed spectral lines of a star are all shifted towards the red end of the spectrum. Which statement is true?

A

This is an example of the Doppler effect.

24
Q

The broadening of spectral lines can be caused by:

A

Density of the hot medium; thermal motion of the hot atoms; rotation of the star.

25
Q

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

A

Its temperature; its radial motion; its chemical composition