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© 2017 Pearson Education, Inc. © 2017 Pearson Education, Inc.

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Question 1 Which of these is NOT a form of electromagnetic radiation Gamma rays Infrared Sound Visible light Radio 2017 Pearson Education Inc Question 1 Which of these is NOT a form of ID: 624721

education pearson question 2017 pearson education 2017 question light lines temperature spectral waves star

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Slide1

© 2017 Pearson Education, Inc.Slide2

Question

1

Which of these is NOT a form of electromagnetic radiation?Gamma raysInfraredSoundVisible lightRadio

© 2017 Pearson Education, Inc.Slide3

Question 1

Which of these is NOT a form of

electromagnetic radiation?Gamma raysInfraredSoundVisible lightRadio

Explanation: Sound comes

from pressure waves; all

others are types of electro-magnetic radiation of different wavelengths.

© 2017 Pearson Education, Inc.Slide4

Question 2

The distance between successive wave crests defines the _____ of a wave.

wavelengthfrequencyperiodamplitudeenergy

© 2017 Pearson Education, Inc.Slide5

Question 2

The distance between successive wave crests defines the _____ of a wave.

wavelengthfrequencyperiodamplitudeenergyExplanation: Light can range from short-wavelength

gamma

rays to long-wavelength radio waves

.© 2017 Pearson Education, Inc.Slide6

Question 3

The frequency at which a star’s intensity is greatest depends directly on its

radius.mass.magnetic field.temperature.direction of motion.

© 2017 Pearson Education, Inc.Slide7

Question 3

The frequency at which a star’s intensity is greatest depends directly on its

radius.mass.magnetic field.temperature.direction of motion.Explanation: Wien’s law means that

hotter stars produce much more

high-frequency light.

© 2017 Pearson Education, Inc.Slide8

Question 4

Rigel

appears as a bright bluish star, whereas Betelgeuse appears as a bright reddish star.Rigel is _____ Betelgeuse.cooler than the same temperature as older than

hotter than

more massive than

© 2017 Pearson Education, Inc.

The constellation ORION

Betelgeuse

RigelSlide9

Question 4

Rigel

appears as a bright bluish star, whereas Betelgeuse appears as a bright reddish star.Rigel is _____ Betelgeuse.cooler than the same temperature as older than

hotter than

more massive than

Explanation: Hotter

stars look

bluer

in color;

cooler

stars look redder

.

© 2017 Pearson Education, Inc.

The constellation ORION

Betelgeuse

RigelSlide10

Question 5

If a light source is

approaching you, you will observe thatits spectral lines are redshifted.the light is much brighter.its spectral lines are shorter in wavelength.the amplitude of its waves has increased.its photons have increased in speed.

© 2017 Pearson Education, Inc.Slide11

Question 5

If a light source is

approaching

you, you will observe that

its spectral lines are redshifted.

the light is much brighter.

its spectral lines are shorter in wavelength.

the amplitude of its waves has increased.

its photons have increased in speed.

Explanation: The Doppler shift explains that wavelengths from sources approaching us are

blueshifted

.

© 2017 Pearson Education, Inc.Slide12

Question 6

The wavelengths of

emission lines produced by an elementdepend on its temperature. are identical to its absorption lines. depend on its density.are different from its absorption lines.

depend on its intensity.

© 2017 Pearson Education, Inc.Slide13

Question 6

The wavelengths of

emission lines produced by an elementdepend on its temperature. are identical to its absorption lines. depend on its density.are different from its absorption lines.

depend on its intensity.

Explanation: Elements

absorb or emit the same wavelengths of light

based on their electron energy levels.

© 2017 Pearson Education, Inc.Slide14

Question 7

Analyzing a star’s spectral lines can tell us about all of these EXCEPT its

composition.surface temperature.transverse (side-to-side) motion.rotation.density.

© 2017 Pearson Education, Inc.Slide15

Question 7

Analyzing a star’s spectral lines can tell us about all of these EXCEPT its

composition.surface temperature.transverse (side-to-side) motion.

rotation.

density

Explanation: Only motion toward

or away from us influences a star’s spectral lines. Spectra can also tell us about a star’s magnetic field.

© 2017 Pearson Education, Inc.Slide16

Question

8

What types of electromagnetic radiation from space reach the surface of Earth? radio waves and microwaves X-rays and ultraviolet light infrared and gamma rays

visible light and radio waves

visible and ultraviolet light

© 2017 Pearson Education, Inc.Slide17

Question 8

What types of

electromagnetic radiation from space reach the surface of Earth? radio waves and microwaves X-rays and ultraviolet light infrared and gamma raysvisible light and radio wavesvisible and ultraviolet light

Explanation: Earth’s

atmosphere allows

radio waves and visible

light to reach the ground.

© 2017 Pearson Education, Inc.Slide18

Question 9

Which of the following has a fundamentally different nature than the other four?

Proton Electron Neutron Atomic nucleusPhoton

© 2017 Pearson Education, Inc.Slide19

Question 9

Which of the following has a fundamentally different nature than the other four?

Proton Electron

Neutron

Atomic nucleus

PhotonExplanation: Photons are packages of light energy. Protons, neutrons, and

electrons are particles of matter within an atomic nucleus.

© 2017 Pearson Education, Inc.