Tuesday 24 January 2017

TEST BANK 21ST CENTURY ASTRONOMY THE SOLAR SYSTEM 5TH EDITION BY KAY

TEST BANK 21ST CENTURY ASTRONOMY THE SOLAR SYSTEM 5TH EDITION BY KAY



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Chapter 5: Light
Learning Objectives
Define the bold-faced vocabulary terms within the chapter.
Multiple Choice: 10, 11, 12, 13, 35
Short Answer: 5.1 Light Brings Us the News of the Universe
Summarize the electromagnetic properties of light.
Multiple Choice: 1, 2, 3, 4, 5, 23, 25
Short Answer: Explain how and when light acts like a wave, and when it acts like a particle.
Multiple Choice: 15, 16, 17
Relate color, wavelength, and energy of photons.
Multiple Choice: 6, 7, 8, 14, 18, 19, 24
Short Answer: List the names and wavelength ranges of the electromagnetic spectrum.
Multiple Choice: 9, 20, 21, 22
5.2 The Quantum View of Matter Explains Spectral Lines
Illustrate the processes of atomic absorption and emission of light.
Multiple Choice: 27, 28, 29, 38
Short AnswerRelate spectral features to changes in energy state of an atom.
Multiple Choice: 26, 30, 31, 32, 33, 34, 36, 37, 39
Short Answer: 5.3 The Doppler Shift Indicates Motion Toward or Away from Us
Explain why radial motion produces a Doppler shift.
Multiple Choice: 40, 41, 42, 43, 46
Short Answer:
5.4 Temperature Determines the Spectrum of Light That an Object Emits
Summarize what it means for a system to be in equilibrium.
Multiple Choice: 44
Relate temperature to the rate of thermal motions.
Multiple Choice: 45, 52
Short Answer: Illustrate the relationship between flux and luminosity.
Multiple Choice: 53
Characterize how blackbody spectra describe the luminosity, temperature, and color of an object.
Multiple Choice: 47, 48, 49, 50, 51, 54, 55, 56
Short Answer: 5.5 The Brightness of Light Depends on Its Luminosity and Distance
Use the inverse square law to relate luminosity, brightness, and distance.
Multiple Choice: 57, 58, 59
Short Answer: Working It Out 5.2
Use the Doppler equation to relate radial velocity with shifts in the wavelengths of spectral lines.
Multiple Choice: 60, 61, 62
Working It Out 5.3
Use the Stefan-Boltzmann law to relate temperature, flux, and luminosity of a blackbody.
Short Answer: Use Wien’s law to relate the temperature and peak wavelength of blackbody emission.
Multiple Choice: 63, 64, 65
Short Answer: Working It Out 5.4
Calculate a planet’s temperature based on its parent star and albedo.
Multiple Choice: 66, 67, 68, 69, 70
Short Answer: MULTIPLE CHOICE
1.      The speed of light was first determined by which scientist?
a.       Galileo
b.      Newton
c.       Kepler
d.      Rømer
e.       Einstein
2.      The speed of light in a vacuum is
a.       300,000 m/s.
b.      300,000 mph.
c.       300,000 km/s.
d.      300,000,000 mph.
e.       infinite.




3.      What is the difference between visible light and X-rays?
a.       Speed; X-rays go faster than visible light.
b.      Speed; X-rays go slower than visible light.
c.       Wavelength; X-rays have a shorter wavelength than visible light.
d.      Wavelength; X-rays have a longer wavelength than visible light.
e.       X-rays are made up of particles, whereas visible light is made up of waves.
4.      How does the speed of light traveling through a medium (such as air or glass) compare to the speed of light in a vacuum?
a.       It is the same as the speed of light in a vacuum.
b.      It is always less than the speed of light in a vacuum.
c.       It is always greater than the speed of light in a vacuum.
d.      Sometimes it is greater than the speed of light in a vacuum and sometimes it is less, depending on the medium.
e.       Light can’t travel through a medium; it only can go through a vacuum.
5.      A light-year is a unit that is used to measure
a.       time.
b.      wavelength.
c.       speed.
d.      energy.
e.       distance.
6.      Which formula denotes how the speed of light is related to its wavelength and frequency?
a.       c = λf
b.      c = λ/f
c.       c = f/λ
d.      c = 1/λf
e.       There is no relationship between wavelength and frequency.
7.      The color of visible light is determined by its
a.       speed.
b.      wavelength.
c.       mass.
d.      distance from you.
e.       size.
8.      How do the wavelength and frequency of red light compare to the wavelength and frequency of blue light?
a.       Red light has a longer wavelength and higher frequency than blue light.
b.      Red light has a longer wavelength and lower frequency than blue light.
c.       Red light has a shorter wavelength and higher frequency than blue light.
d.      Red light has a shorter wavelength and lower frequency than blue light.




9.      What wavelengths of light can the human eye see?
a.       3.8 µm to 7.5 µm
b.      3.8 nm to 7.5 nm
c.       380 cm to 750 cm
d.      380 nm to 750 nm
e.       3.8 m to 7.5 m
10.      What does amplitude reveal about light?
a.       wavelength
b.      frequency
c.       speed
d.      brightness
11.      The unit Hertz is a measure of what quantity?
a.       wavelength
b.      frequency
c.       speed
d.      brightness

12.      When talking about a wave, what does the term “medium” refer to?
a.       the size of an object
b.      the substance through which the wave travels
c.       the brightness level
d.      the vacuum
13.      A nanometer is a measure of which quantity?
a.       wavelength
b.      frequency
c.       speed
d.      brightness



14.      Which of the following photons carries the smallest amount of energy?
a.       a blue photon of the visible spectrum, whose wavelength is 450 nm
b.      an infrared photon, whose wavelength is 105 m
c.       a red photon in the visible spectrum, whose wavelength is 700 nm
d.      a microwave photon, whose wavelength is 102 m
e.       an ultraviolet photon, whose wavelength is 300 nm

15.      Einstein showed that the _________ could be explained if photons carried quantized amounts of energy.
a.       warping of space and time
b.      Heisenberg uncertainty principle
c.       photoelectric effect
d.      theory of special relativity
e.       Bohr model of the atom
16.      Light has aspects of
a.       only a wave.
b.      only a particle.
c.       both a particle and a wave.
d.      neither a particle nor a wave.
17.      Saying that something is quantized means that it
a.       is a wave.
b.      is a particle.
c.       travels at the speed of light.
d.      can only have discrete quantities.
e.       is smaller than an atom.
18.      A red photon has a wavelength of 650 nm. An ultraviolet photon has a wavelength of 250 nm. The energy of an ultraviolet photon is _________ the energy of a red photon.
a.       2.6 times larger than
b.      6.8 times larger than
c.       2.6 times smaller than
d.      6.8 times smaller than
e.       the same as
19.      Light with a wavelength of 600 nm has a frequency of
a.       2 × 105 Hz
b.      5 × 107 Hz
c.       2 × 1010 Hz
d.      5 × 1012 Hz
e.       5 × 1014 Hz
20.      Which of the following lists different types of electromagnetic radiation in order from the shortest wavelength to the longest wavelength?
a.       radio waves, infrared, visible, ultraviolet, X-rays
b.      gamma rays, ultraviolet, visible, infrared, radio waves
c.       gamma rays, X-rays, infrared, visible, ultraviolet
d.      X-rays, infrared, visible, ultraviolet, radio waves
e.       radio waves, ultraviolet, visible, infrared, gamma rays

21.      As wavelength increases, the energy of a photon _________ and its frequency _________.
a.       increases; decreases
b.      increases; increases
c.       decreases; decreases
d.      decreases; increases
22.      If the frequency of a beam of light were to increase, its period would _________ and its wavelength would _________.
a.       decrease; increase
b.      increase; decrease
c.       increase; increase
d.      decrease; decrease
e.       stay the same; stay the same
23.      The fact that the speed of light is constant as it travels through a vacuum means that
a.       photons with longer wavelengths have lower frequencies.
b.      radio wave photons have shorter wavelengths than gamma ray photons.
c.       X-rays can be transmitted through the atmosphere around the world.
d.      ultraviolet photons have less energy than visible photons.
24.      If the wavelength of a beam of light were to double, how would that affect its frequency?
a.       The frequency would be four times higher.
b.      The frequency would be two times higher.
c.       The frequency would be two times lower.
d.      The frequency would be four times lower.
e.       There is no relationship between wavelength and frequency.
25.      If the Sun instantaneously stopped giving off light, what would happen on the day-side of Earth?
a.       It would immediately get dark.
b.      It would get dark 8.3 minutes later.
c.       It would get dark 27 minutes later.
d.      It would get dark 1 hour later.
e.       It would get dark 24 hours later.
26.      When an electron moves from a higher energy level in an atom to a lower energy level,
a.       the atom is ionized.
b.      a continuous spectrum is emitted.
c.       a photon is emitted.
d.      a photon is absorbed.
e.       the electron loses mass.
27.      If you observe an isolated hot cloud of gas, you will see
a.       an absorption spectrum.
b.      a continuous spectrum.
c.       an emission spectrum.
d.      a rainbow spectrum.
e.       a dark spectrum.

28.      Which of these objects would emit an absorption spectrum?
a.       an incandescent lightbulb
b.      a fluorescent lightbulb
c.       an isolated hot gas cloud
d.      a hot, solid object
e.       a thin, cool gas cloud that lies in front of a hotter blackbody
29.      If you observe a star, you will see
a.       an absorption spectrum.
b.      a continuous spectrum.
c.       an emission spectrum.
d.      a rainbow spectrum.
e.       a dark spectrum.
30.      In the energy level diagram shown in the figure below, the electron is excited to the E4 energy level. If the electron transitions to an energy level giving off a photon, which level would produce a photon with the largest energy?
a.       E1
b.      E2
c.       E3
d.      E4
e.       E5
31.      In the energy level diagram shown in the figure below, the electron is excited to the E4 energy level. If the electron transitions to an energy level giving off a photon, which level would produce a photon with the largest frequency?
a.       E1
b.      E2
c.       E3
d.      E4
e.       E5
32.      In the energy level diagram shown in the figure below, the electron is excited to the E4 energy level. If the electron transitions to an energy level giving off a photon, which level would produce a photon with the largest wavelength?
a.       E1
b.      E2
c.       E3
d.      E4
e.       E5







33.      In the energy level diagram shown in the figure below, the electron is excited to the E2 energy level. If the atom absorbs a photon with the exact frequency to move the electron to another energy level, which energy level would correspond to the largest frequency difference?
a.       E1
b.      E2
c.       E3
d.      E4
e.       E5
34.      In the energy level diagram shown in the figure below, the electron is excited to the E2 energy level. If the atom absorbs a photon with the exact wavelength to move the electron to another energy level, which energy level would correspond to the largest wavelength difference?
a.       E1
b.      E2
c.       E3
d.      E4
e.       E5
35.      Astronomers measure the amount of various elements in other stars and most commonly compare them to which of the following when studying the composition of a star?
a.       solar abundance
b.      big bang abundance
c.       terrestrial abundance
d.      water
36.      In the figure below, you see a stellar spectrum. The dip in the data near 650 nm corresponds most closely with which of the following?
a.       sodium emission
b.      sodium absorption
c.       hydrogen emission
d.      hydrogen absorption
e.       iron absorption
37.      Why is a neutral iron atom a different element than a neutral carbon atom?
a.       A carbon atom has fewer neutrons in its nucleus than an iron atom.
b.      An iron atom has more protons in its nucleus than a carbon atom.
c.       An iron atom has more electrons than a carbon atom.
d.      A carbon atom is bigger than an iron atom.
38.      In the quantum mechanical view of the atom, electrons are often depicted as
a.       a cloud that is centered on the nucleus.
b.      a particle orbiting the nucleus.
c.       free to orbit at any distance from the nucleus.
d.      a particle inside the nucleus.
39.      The n = 5 electronic energy level in a hydrogen atom is 1.5 × 1019 J higher than the n = 3 level. If an electron moves from the n = 5 level to the n = 3 level, then a photon of wavelength
a.       1.3 nm, which is in the ultraviolet region, is emitted.
b.      1.3 nm, which is in the ultraviolet region, is absorbed.
c.       1,300 nm, which is in the infrared region, is absorbed.
d.      1,300 nm, which is in the infrared region, is emitted.
e.       No light will be absorbed or emitted.
40.      The Doppler shift can be used to determine the _________ of an object.
a.       energy
b.      temperature
c.       radial velocity
d.      color
e.       three-dimensional velocity
41.      A spaceship is traveling toward Earth while giving off a constant radio signal with a wavelength of 1 meter (m). What will the signal look like to people on Earth?
a.       a signal with a wavelength less than 1 m
b.      a signal with a wavelength more than 1 m
c.       a signal moving faster than the speed of light
d.      a signal moving slower than the speed of light
e.       a signal with a wavelength of 1 m, moving the normal speed of light
42.      Which of these stars would have the biggest redshift?
a.       a star moving at low speed toward you
b.      a star moving at high speed toward you
c.       a star moving at low speed away from you
d.      a star moving at high speed away from you
e.       a star that is not moving away from you or toward you
43.      A spaceship is traveling from planet B on the left, toward planet A on the right. The spaceship is traveling at a speed of 15,000 km/s to the left while it sends out a signal with a wavelength of 4 m. If astronomers living on planets A and B measure the radio waves coming from the spaceship, what wavelengths will they measure?
a.       Planet A measures 6 m, and planet B measures 2 m.
b.      Planet A measures 2 m, and planet B measures 6 m.
c.       Planet A measures 4.2 m, and planet B measures 3.8 m.
d.      Planet A measures 3.8 m, and planet B measures 4.2 m.
e.       Both Planet A and planet B measure 4 m.
44.      What does it mean to say that an object is in thermal equilibrium?
a.       It isn’t absorbing any energy.
b.      It isn’t radiating any energy.
c.       It is radiating more energy than it is absorbing.
d.      It is absorbing more energy than it is radiating.
e.       It is absorbing the same amount of energy that it is radiating.
45.      The Kelvin temperature scale is used in astronomy because
a.       at 0 K an object has absolutely zero energy.
b.      water freezes at 0 K.
c.       water boils at 100 K.
d.      hydrogen freezes at 0 K.
e.       the highest temperature possible is 1000 K.
46.      You observe the spectrum of two stars. Star A has an emission line from a known element at 600 nm. Star B has emission lines from the same atom, but the emission line is occurring at 650 nm. One possible explanation for this observation is: that star A is
a.       cooler than star B.
b.      farther away from us than star B.
c.       moving toward us faster than star B.
d.      made of different elements than star B.
e.       larger than star B.
47.      In the figure below, which blackbody spectrum corresponds to the object with the highest temperature?
a.       A
b.      B
c.       C
d.      D
e.       E
48.      In the figure below, which blackbody spectrum corresponds to the object that would appear the most red to the human eye?
a.       A
b.      B
c.       C
d.      D
e.       E
49.      In the figure below, which blackbody spectrum corresponds to the object that would appear white to the human eye?
a.       A
b.      B
c.       C
d.      D
e.       E
50.      As a blackbody’s temperature increases, it also becomes _________ and _________.
a.       more luminous; redder
b.      more luminous; bluer
c.       less luminous; redder
d.      less luminous; bluer
e.       more luminous; stays the same color
51.      Compare two blackbody objects, one at 200 K and one at 400 K. How much larger is the flux from the 400 K object compared to the flux from the 200 K object?
a.       2 times larger
b.      4 times larger
c.       8 times larger
d.      16 times larger
e.       They have the same flux.
52.      At what temperature does water freeze?
a.       0 K
b.      32 K
c.       100 K
d.      273 K
e.       373 K
53.      You observe a red star and a blue star and are able to determine that they are the same size. Which star has a higher surface temperature, and which star is more luminous?
a.       The red star has a higher surface temperature and more luminous.
b.      The red star has a higher surface temperature, and the blue star is more luminous.
c.       The blue star has a higher surface temperature and more luminous.
d.      The blue star has a higher surface temperature, and the red star is more luminous.
e.       They have the same luminosities and temperatures.
54.      At what peak wavelength does your body radiate the most given that your temperature is approximately that of Earth, which is 300 K?
a.       105 m
b.      103 m
c.       102 m
d.      10 m
e.       1,000 m
55.      Why do some stars in the sky appear blue, whereas other stars appear red?
a.       The red stars have higher surface temperatures than the blue stars.
b.      The blue stars have higher surface temperatures than the red stars.
c.       The blue stars are closer to us than the red stars.
d.      The red stars are closer to us than the blue stars.
e.       The blue stars are moving toward us, while red stars are moving away from us.
56.      Consider an incandescent lightbulb. If you wanted to turn a 10-W lightbulb into a 100-W lightbulb, how would you change the temperature of the filament inside the bulb?
a.       Raise its temperature by a factor of 3.2.
b.      Raise its temperature by a factor of 1.8.
c.       Raise its temperature by a factor of 10.
d.      Lower its temperature by a factor of 2.6.
e.       Lower its temperature by a factor of 5.4.
57.      Star A and star B appear equally bright in the sky. Star A is twice as far away from Earth as star B. How do the luminosities of stars A and B compare?
a.       Star A is twice as luminous as star B.
b.      Star B is twice as luminous as star A.
c.       Star A is four times as luminous as star B.
d.      Star B is four times as luminous as star A.
e.       Stars A and B have the same luminosity.
58.      Star C and star D have the same luminosity. Star C is twice as far away from Earth as star D. How do the brightnesses of stars C and D compare?
a.       Star C appears four times as bright as star D.
b.      Star C appears twice as bright as star D.
c.       Star D appears twice as bright as star C.
d.      Star D appears four times as bright as star C.
e.       Stars C and D appear equally bright.
59.      The average red giant in the night sky is about 1,000 times more luminous than the average main-sequence star. If both kinds of stars have about the same brightness, how much farther away are the red giants compared to the main-sequence stars?
a.       32 times farther
b.      1,000 times farther
c.       65 times farther
d.      5.6 times farther
e.       The red giants and main-sequence stars have approximately the same distances.
60.      You are driving on the freeway when a police officer records a shift of 7 nm when he or she your speed with a radar gun that operates at a wavelength of 0.1 m. How fast were you going?
a.       43 mph
b.      83 mph
c.       21 mph
d.      65 mph
e.       47 mph
61.      You record the spectrum of a star and find that a calcium absorption line has an observed wavelength of 394.0 nm. This calcium absorption line has a rest wavelength is 393.3 nm. What is the radial velocity of this star?
a.       5,000 km/s
b.      500 km/s
c.       50 km/s
d.      5 km/s
e.       0.5 km/s


62.      If you find that the hydrogen alpha line in a star’s spectrum occurs at a wavelength of 656.45 nm, what is the star’s radial velocity? Note that the rest wavelength of this line is 656.30 nm.
a.       150 km/s away from you
b.      150 km/s toward you
c.       350 km/s toward you
d.      70 km/s away from you
e.       70 km/s toward you
.
63.      If Jupiter has a temperature of 165 K, at what wavelength does its spectrum peak? Use the electromagnetic spectrum in the figure below to answer this question.
a.       18 nm—orange visible wavelengths
b.      1,800 mm—microwave wavelengths
c.       1,800 nm—infrared wavelengths
d.      18,000 nm—ultraviolet wavelengths
e.       18,000 nm—infrared wavelengths
64.      If the typical temperature of a red giant is 3000 K, at what wavelength is its radiation the brightest? Use the electromagnetic spectrum in the figure below to help you answer this question.
a.       1 µm—infrared wavelengths
b.      1 µm—red visible wavelengths
c.       20 µm—infrared wavelengths
d.      20 µm—red visible wavelengths
e.       700 µm—red visible wavelengths
65.      If a star has a peak wavelength of 290 nm, what is its surface temperature?
a.       1000 K
b.      2000 K
c.       5000 K
d.      10,000 K
e.       100,000 K
66.      A black car left in the sunlight becomes hotter than a white car left in the sunlight under the same conditions because
a.       the white car absorbs more sunlight than the black car.
b.      the white car reflects more sunlight than the black car.
c.       the black car absorbs only blue photons and reflects red photons, whereas the white car absorbs only red photons and reflects blue photons.
d.      the atoms in the black car are smaller than the atoms in the white car.]



67.      Which of the following factors does not directly influence the temperature of a planet?
a.       the luminosity of the Sun
b.      the distance of the planet from the Sun
c.       the albedo of the planet
d.      the size of the planet
e.       the atmosphere of the planet
68.      An asteroid with an albedo of 0.1 and a comet with an albedo of 0.6 are orbiting at roughly the same distance from the Sun. How do their temperatures compare?
a.       They both have the same temperature.
b.      The comet is hotter than the asteroid.
c.       The asteroid is hotter than the comet.
d.      You must know their sizes to compare their temperatures.
e.       You must know their compositions to compare their temperatures.
69.      Which of these planets would be expected to have the highest average temperature?
a.       a light-colored planet close to the Sun
b.      a dark-colored planet close to the Sun
c.       a light-colored planet far from the Sun
d.      a dark-colored planet far from the Sun
e.       There is not enough information to know which would be hotter.
70.      If Saturn has a semimajor axis of 10 astronomical units (AU) and an albedo of 0.7. If Saturn were to emit the same amount of energy as it absorbs from the Sun, what is Saturn’s expected temperature?
a.       130 K
b.      15 K
c.       35 K
d.      170 K
e.       65 K
SHORT ANSWER
1.      Compare and contrast the wavelengths, frequencies, speeds, and energies of red and blue photons.
2.      How is the energy of a photon related to its, frequency, wavelength, and speed?
3.      What is the intensity of light, and how does it depend on wavelength?
4.      What is an electromagnetic wave?
5.      The first five energy levels of hydrogen are E1 = 0 eV, E2 = 10.2 eV, E3 = 12.1 eV, E4 = 12.7 eV, and E5 = 13.1 eV. If the electron is in the n = 4 level, what energies can a single emitted photon have?
6.      Explain what the term “ground state” means.
7.      Explain how continuous, emission, and absorption spectra are produced.
8.      How are atoms excited, and why do they become de-excited?
9.      Explain how an emission line is formed, and why it is unique to a given element.
10.      The difference in energy between the n = 2 and n = 1 electronic energy levels in the hydrogen atom is 1.6 × 1018 J. If an electron moves from the n = 1 level to the n = 2 level, will a photon be emitted or absorbed? What will its energy be, and what type of electromagnetic radiation is it? Use the electromagnetic spectrum shown in the figure below to answer this question.
Describe, in your own words, why electrons cannot orbit the nucleus like the planets orbit Why do we see black lines in an absorption spectrum if the absorbed photons are (almost) instantaneously reemitted by the atoms in the cloud?
11.      For a star that lies in the plane of Earth’s orbit around the Sun, how does the observed wavelength of the hydrogen absorption line at 656.28 nm in its spectrum change in wavelength (if at all) with the time of year?
12.      A spaceship approaches Earth at 0.9 times the speed of light and shines a powerful searchlight onto Earth. How fast will the photons from this searchlight be moving when they hit Earth?
13.      If you are standing in a fixed location, you may notice that the pitch of a passing train’s whistle changes. What produces this effect?
14.      Suppose you observe a star emitting a certain emission line of helium at 584.8 nm. The rest wavelength of this line is 587.6 nm. How fast is the star moving? Is it moving toward you or away from you?
15.      Imagine a satellite is orbiting a planet. This satellite gives off radio waves with a constant wavelength of 1 m. An observer on Earth then measures the signal from the satellite when it is directly between Earth and the planet. How does the wavelength received compare to the wavelength that the satellite gave off?
16.      Explain what is meant when someone says “thermal motions.”
17.      Sketch two blackbody curves, one for a hot blue object and the second for a cooler red object. Be sure to label your axes.
18.      How does temperature relate to the speed of gas particles?
19.      Name four physical properties of an object that we can determine by analyzing the radiation that it emits, and briefly describe how these properties are determined. Cite the names of any laws that apply.
20.      Imagine you observed three different stars: a red star, a blue star, and a yellow star. You are able to determine that each of these stars has the same radius. Answer each question below and explain how you know.
A: Which star has the highest surface temperature?
B: Which star is the most luminous?
C: Which star is the brightest?
21.      If you were driving down a deserted country road and you saw a light in the distance, what would you need to measure or know about it in order to calculate how far away it was?
22.      Imagine you see a street lamp that is 100 m away from you and is 10,000 times more luminous than a firefly. How close would you have to be to the firefly to make it look as bright as the street lamp?
23.      How much would you have to change the temperature of an object if you wanted to increase its flux by a factor of 100?
24.      If you want a blackbody’s peak wavelength to be cut in half, by how much do you need to increase its temperature?
25.      What two factors control a planet’s surface temperature if it has no atmosphere, and no internal source of heat?
26.      How can the average temperature of Earth stay approximately constant even though Earth is always getting energy from the Sun?
27.      Astronomers have now found a large number of exoplanets, which are planets that orbit around stars other than the Sun. Imagine astronomers found a planet identical to Earth orbiting a star that had the same radius as the Sun, but with a temperature that is twice the temperature of the Sun. How far would this new planet need to be away from its star to have the same average temperature as Earth?
28.      What would you expect the temperature of a comet to be if its distance was 100 AU from the Sun? Assume that it is very icy and reflective so that its albedo is equal to 0.6. Does it matter what the radius of the comet is?



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