Spectral Analysis

Spectral Analysis

11th - 12th Grade

10 Qs

quiz-placeholder

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Spectral Analysis

Spectral Analysis

Assessment

Quiz

Mathematics

11th - 12th Grade

Practice Problem

Hard

CCSS
HSA.SSE.A.1, HSA.REI.D.10, HSF.IF.B.4

+2

Standards-aligned

Created by

Charles Martinez

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10 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Can an atom emit light if the electrons are all in the ground state?

yes

no

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What type of spectrum is produced by a hot low density gas, such as a neon sign?

Continuous Spectrum

Emission Spectrum

Absorption Spectrum

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What type of spectrum is produced by white light passing through a cold dark cloud?

Continuous spectrum

Emission Spectrum

Absorption Spectrum

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What types of spectra are produced by stars?

Continuous Spectrum

Emission Spectrum

Absorption Spectrum

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Media Image

The spectral curve on the graph below illustrates the energy output versus wavelength of an unknown star. Assume that the left end of each spectrum corresponds to shorter blue wavelengths. Which absorption spectra belongs to this unknown star?

a

b

c

d

Tags

CCSS.HSA.REI.D.10

CCSS.HSF.IF.B.4

CCSS.HSF.IF.C.7

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Media Image

The three spectral curves shown below illustrate the energy output versus wavelength for three unknown stars A, B, and C. Which of the stars has the highest temperature? Look carefully at the peaks!

A

B

C

Tags

CCSS.HSA.SSE.A.1

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

If star P is hotter than Star Q, which of the following statements is true about the dark line absorption spectra for two stars?

There will be more absorption lines at the blue end of the spectrum for the hotter star.

There will be more absorption lines at the red end of the spectrum for the hotter star.

There will be more lines in the absorption spectrum for the hotter star.

There will be fewer lines in the absorption spectrum of the hotter star.

None of the above can be concluded.

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