CH 04

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19 Terms

1
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What identifies whether an atom carries a charge as an ion or is neutral?

The number of electrons.

2
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What identifies the type of element?

The number of protons.

3
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What is expected in a spectrum of a star observed from above Earth's atmosphere compared to ground-based observation?

It would show slightly fewer absorption lines.

4
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What type of spectrum would sunlight reflected from Saturn's moon Titan be expected to be?

Absorption spectrum.

5
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If the temperature of neon gas is increased, what happens to the emission spectrum?

We would observe fewer red lines and more blue lines.

6
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What can be inferred about a star with many red and blue absorption lines compared to one with many blue absorption lines?

It is cooler than the other star.

7
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What are the basic components of a simple spectroscope?

A slit, a mirror, a detector, a prism, and an eyepiece or screen.

8
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What additional components are used in spectrographs for modern astronomical observations?

A telescope, a dispersing device, and a detector.

9
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What defines an atom that has been ionized?

It has different numbers of protons and electrons.

10
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How many different photons can be emitted as a hydrogen atom in the third excited state falls to the ground state?

Up to 4 different photons.

11
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Compared to a transition from the first excited state to the ground state, what is the energy of a photon emitted from the third excited state to the second excited state?

Lower energy.

12
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Compared to complex atoms like neon, how many excited states does simple hydrogen have?

Fewer excited states.

13
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What can astronomers determine from analyzing starlight?

The star's motion, composition, and temperature.

14
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What is the characteristic of absorption lines in the hottest stars?

They are thin and distinct.

15
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What is the characteristic of absorption lines in the fastest spinning stars compared to slowly rotating stars?

They are broad and fuzzy.

16
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What happens if most electrons of a star's abundant element are not in a condition to absorb light?

The element may not produce strong lines.

17
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What determines the properties of a star observed from its spectrum?

Composition, temperature, and motion.

18
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What happens to a star's hydrogen lines if it is very hot?

The lines of hydrogen are weak due to ionization.

19
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What does the temperature of a star help determine about its appearance?

The color of the star's glow (hotter stars appear bluer, cooler stars appear redder).