Solar system exam 3

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103 Terms

1
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Keplers 1st law of planetary motion

each planet moves in an elliptical orbit with the sun at one focus of the ellipse

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what is inertia?

resistance in changes in motion

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Because radio waves have very ______ wavelengths, radio telescopes generally have ______ resolution

long, bad

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which law does eccentricity relate to

kepler’s 1st law

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the further away a planet is, the (more/less) eccentric the ellipse is? The closer they are, the (more/less) eccentric the ellipse is? An ellipse whose focal points are both at the center is a _______.

more, less, circle

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Keplers second law of planetary motion

the lines from the sun to any planet sweeps out equal areas of space in equal time intervals

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At what point in their orbits do objects move the fastest?

closer to the perihelion, when they are closer to the sun

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at what point in their orbits do objects move the slowest?

closer to the aphelion, when they are farther from the sun

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kepplers 3rd law of planetary motion

P2=a3

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for kepplers 3rd law, if a is smaller then P is______. If a is larger then P is _____.

smaller, larger

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what is the semi major axis? what is major axis?

distance from far side of orbit to center, distance from one side of orbit to the other

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what did galileo observe about the moon?

not perfect, there’s blemishes and craters

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proof of heliocentric model

possible for venus to be found on the other side of the sun from the earth. in this case, a full range of moon phases can be observed

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what did galileo do (what was his experiment and what did he learn?)

drop 2 objects off side of leaning tower and learned that objects fall at the same rate

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newtons first law

an object in motion stays in motion unless acted upon by an opposing force (law of inertia)

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Newtons second law

F=ma

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Newton’s third law

every action exerts an equal and opposite reaction

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what does your weight depend on?

your mass, planets mass, distance

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The gravitational acceleration all objects feel towards earth depends only on….

properties of the earth

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Newton’s law of universal gravitation

gravitational force depends on the mass of both objects and every object exerts a force on every other object

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Determining weight on another planet

Use the gravity equation to calculate your weight on that planet

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apparent weightlessness

If an object moves fast enough, it can escape earth’s gravitational pull and be in a constant free fall around the earth, causing an orbit

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newton’s modified version of Kepler’s 3rd law

(m1+m2)P²=a³

24
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Tidal force relationship

F=m/r³

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what causes tides

differences in gravitational forces across an object of size

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For tides, the side closer to the object feels a _________ force while the side farther feels a ______ force. As a result, compared to the average force on the earth, the closer side is being pulled _____ while the farther side is being pulled _____. This causes the closer side to ______ _____ the object while the farther side ____ _____ ___ the object.

greater, lesser, more, less, bulge towards, bulge away from

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The tidal strength of the sun is only ______ as strong as the tidal force of the moon

1/2

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how many high tides are there a day? how many low tides are there a day?

2 high, 2 low

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how often do high tides occur? When do low tides occur

every 12 hours, in between high tides

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Since moon moves around the Earth over time, we actually experience 2 high tides every…

24 hours and 50 minutes

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what are spring tides?

when the sun and moon exert tidal forces in the same direction, we experience our highest high tides and our lowest low tides

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what are neap tides?

when the sun and moon exert tidal forces in opposite directions, we experience our lowest high tides and our highest low tides

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during what moon phases do spring tides occur

new or full

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during what moon phases do neap tides occur

1st and 3rd quater

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how often do spring tides occur? how often do neap tides occur?

twice a month

36
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What is light also known as?

electromagnetic radiation

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what is electromagnetic radiation composed of?

oscillating electric and magnetic fields that oscillate perpendicular to the travel of motion

38
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what is wavelength

the length over which the wave repeats its pattern

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what is frequency?

how often the wave repeats itself

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what is a photon

light particle

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what is the energy of a photon?

E=hf

42
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what is the visible light range?

400nm-750nm

43
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order of e&m spectrum from longest wavelength to shortest wavelength

radio, micro, infared, visible, ultraviolet, x-rays, gamma

44
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what is spectroscopy

the study of light by spreading it out to see the various wavelengths being emitted

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what is a continous spectra?

from hot, dense objects

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what is an emission spectra?

emitted from excited, low density gases

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what is an absorption spectra?

continuous emission passes through low-density gases, which absorb their favorite wavelengths and let everything else pass through

48
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how do astronomers restrict observations for spectroscopic observations?

they restrict their observations to narrow slits

49
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what is a blackbody object?

objects that absorb any radiation which hits them, then re-radiate the absorbed energy

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what is blackbody radiation?

the spectrum of energy given off by a blackbody object

51
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stefan-boltzmann law

the hotter the object the higher the intensity, the more it radiates energy

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wien’s law formula (type the word wavelength for lambda)

wavelength~1/T

53
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Wein’s law states

The hotter the object, the shorter its peak wavelength

54
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in an electron shell, its orbital level is equal to its

energy levels

55
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when an electron jumps up, it _________ energy. When an electron jumps down, it _____ energy

absorbs, releases

56
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what is ionization?

when the electron completely frees itself from the magnetic pull of the nucleus

57
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discrete energy levels

an electron at a particular distance from the nucleaus will have a particular amount of energy

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what does the number of protons in an atom tell us?

what element it is

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what does the number of neutrons in an atom tell us?

what isotope the element is

60
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shorter wavelength= ______ electron jump, longer wavelength= _______ electron jump

larger, smaller

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what are the 4 reasons why the movement of electrons around the nucleus cause an atom to absorb/emit energy?

opposites attract, discrete levels, descrete energy levels, ionization

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what do the dips in sprecal lines represent on the solar spectrum

absorption lines

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what type of spectra does the sun give off

absorption spectra

64
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radial vs. transverse motion, which one does the doppler effect give you?

radial is towards and away from us, transverse is across our line of sight, radial

65
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the faster the radial motion, the ________ the doppler shift

greater

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how do astronomers detect a doppler shift?

look at spectrum of the light being emitted from objects in space

67
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what is a reflecting telescopes

use mirrors to focus light onto an image

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what is a refracting telescope?

use lenses to focus light onto an image

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what is chromatic aberration?

different colors focus at different points on a telescope

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why is a larger telescope better?

the larger the opening, the more light it will gather in a given amount of time

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what is angular resolution?

ability to observe two closely spaced objects as 2 different objects

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what two factors effect angular resolution? what is the formula?

size of telescope and wavelength of light angle=wavelength/diameter

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she larger the telescope, the ______ the angular resolution. The shorter the wavelength, the _______ the angular resolution

better, better

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is a small or large angular resolution better?

smaller

75
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opaque

blocks or prevents the passage of a specified form of radiation

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transparent

allows the passage of a specified form of radiation

77
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seeing

a measurement of the sharpness of a telescopic image

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what is a CCD?

collection of cells on a computer chip that collect light and convert it into electric harge

79
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what produces good seeing? what produces poor seeing?

a calm atmosphere, a turbelent atmosphere

80
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what wavelengths is the earth’s atmosphere transparent to?

visual and radio wavelengths

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what wavelengths is the earth partially opaque to?

ultraviolet and infared

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what wavelengths is the earth completely opaque to?

x-rays and gamma rays

83
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A comet, with a highly elliptical orbit, will spend most of its time
A. moving away from the Sun.
B. moving towards the Sun.
C. far away from the Sun.
D. very close to the Sun.

C. far away from the sun

84
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Planets closer to the Sun than Earth take _____ to complete one orbit.
A. more time
B. less time
C. the same amount of time

B. less time

85
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The Earth takes one year to orbit once around the Sun (the Earth’s period equals one year). A fictional planet orbits twice as far away from the Sun as Earth. How long does it take this fictional planet to orbit once around the Sun (i.e., what is the planet’s period)?
A. less than half a year
B. exactly half a year
C. exactly one year
D. exactly two years
E. greater than two years

E. greater than two years

86
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When dropped from the same height, when will a lead weight hit the ground compared to a less
dense wood ball?
A. much sooner
B. much later
C. the same time

A. much sooner

87
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A man pushes on a box, but it remains at rest.
What is the net force acting on the box? (the man is to the right of the box pushing to the left)
A. The net force is to the left.
B. The net force is to the right.
C. The net force is zero.

A. The net force is to the left

88
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When the tablecloth is pulled out from underneath the place setting, why does the place setting not
move?
A. Gravity pulls down on it forcefully enough to keep it in place.
B. While the tablecloth exerts a force on the place setting, the place setting also exerts a force on the tablecloth, and the two forces cancel out.
C. The place setting is not heavy enough to move.
D. Since no force is exerted on the place setting, it does not move.

B. While the tablecloth exerts a force on the place setting, the place setting also exerts a force on the tablecloth, and the two forces cancel out.

89
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If there is a spring tide today, approximately how long will it be until there is another spring tide?
A. one week
B. two weeks
C. one month
D. two months
E. six months

B. two weeks

90
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<p><span style="font-size: calc(var(--scale-factor)*24.05px)">Below are two stove-top burners, their colors indicate how hot </span><span style="font-size: calc(var(--scale-factor)*24.02px)">they are. You place identical pots of water on each burner at the </span><span style="font-size: calc(var(--scale-factor)*24.05px)">same time (the pots being as large as the bigger burner). In each case, which burner will boil the water quicker? If you cannot tell, choose option (c)</span></p>

Below are two stove-top burners, their colors indicate how hot they are. You place identical pots of water on each burner at the same time (the pots being as large as the bigger burner). In each case, which burner will boil the water quicker? If you cannot tell, choose option (c)

A

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<p><span style="font-size: calc(var(--scale-factor)*24.05px)">Below are two stove-top burners, their colors indicate how hot </span><span style="font-size: calc(var(--scale-factor)*24.02px)">they are. You place identical pots of water on each burner at the </span><span style="font-size: calc(var(--scale-factor)*24.05px)">same time (the pots being as large as the bigger burner). In each case, which burner will boil the water quicker? If you cannot tell, choose option (c)</span></p>

Below are two stove-top burners, their colors indicate how hot they are. You place identical pots of water on each burner at the same time (the pots being as large as the bigger burner). In each case, which burner will boil the water quicker? If you cannot tell, choose option (c)

b

92
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<p><span style="font-size: calc(var(--scale-factor)*24.05px)">Below are two stove-top burners, their colors indicate how hot </span><span style="font-size: calc(var(--scale-factor)*24.02px)">they are. You place identical pots of water on each burner at the </span><span style="font-size: calc(var(--scale-factor)*24.05px)">same time (the pots being as large as the bigger burner). In each case, which burner will boil the water quicker? If you cannot tell, choose option (c)</span></p>

Below are two stove-top burners, their colors indicate how hot they are. You place identical pots of water on each burner at the same time (the pots being as large as the bigger burner). In each case, which burner will boil the water quicker? If you cannot tell, choose option (c)

a

93
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The Sun is a hot dense source, surrounded by a low-density atmosphere. What type of spectrum do we observe from the Sun?
A. a continuous spectrum
B. an emission spectrum
C. an absorption spectrum
D. a Hydrogen spectrum
E. a diffuse spectrum

C. an absorption spectrum

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If you excite hydrogen gas in a glass tube by running an electric current through it, the three strongest lines in its emission spectrum will have wavelengths of 656 nm, 486 nm, and 434 nm. Suppose this gas tube was moving away from you really quickly while you were measuring the wavelengths of these three emission lines. What wavelengths might you observe?

A. 668 nm, 496 nm, 442 nm
B. 644 nm, 476 nm, 426 nm
C. 656 nm, 486 nm, 434 nm
D. 656 nm, 496 nm, 426 nm
E. 668 nm, 476 nm, 442 nm

A. 668 nm, 496 nm, 442 nm

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<p><span style="font-size: calc(var(--scale-factor)*20.30px)">The figure below shows the motion of five distant stars (A - E) relative to a stationary observer (telescope). The speed and direction of each star is </span><span style="font-size: calc(var(--scale-factor)*20.27px)">indicated by the length and direction of the arrows shown. </span><span style="font-size: calc(var(--scale-factor)*20.30px)">Rank the Doppler shift of the light observed from each star (A – E) from </span><span style="font-size: calc(var(--scale-factor)*20.27px)">greatest “blueshift”, through no shift, to greatest “redshift”.</span><span><br></span><span style="font-size: calc(var(--scale-factor)*18.05px)">A. </span><span style="font-size: calc(var(--scale-factor)*24.05px)">B &lt; D &lt; C &lt; E &lt; A</span><span><br></span><span style="font-size: calc(var(--scale-factor)*18.02px)">B. </span><span style="font-size: calc(var(--scale-factor)*24.05px)">A &lt; B &lt; D &lt; C &lt; E</span><span><br></span><span style="font-size: calc(var(--scale-factor)*18.05px)">C. </span><span style="font-size: calc(var(--scale-factor)*24.05px)">D &lt; C &lt; E &lt; B &lt; A</span><span><br></span><span style="font-size: calc(var(--scale-factor)*18.02px)">D. </span><span style="font-size: calc(var(--scale-factor)*24.05px)">E &lt; D &lt; B &lt; C &lt; A</span><span><br></span><span style="font-size: calc(var(--scale-factor)*18.05px)">E. </span><span style="font-size: calc(var(--scale-factor)*24.05px)">A = B = C = D = E</span></p>

The figure below shows the motion of five distant stars (A - E) relative to a stationary observer (telescope). The speed and direction of each star is indicated by the length and direction of the arrows shown. Rank the Doppler shift of the light observed from each star (A – E) from greatest “blueshift”, through no shift, to greatest “redshift”.
A. B < D < C < E < A
B. A < B < D < C < E
C. D < C < E < B < A
D. E < D < B < C < A
E. A = B = C = D = E

D. E < D < B < C < A

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<p><span style="font-size: calc(var(--scale-factor)*20.27px)">The first spectra shown below is of an element as it appears in a laboratory here on </span><span style="font-size: calc(var(--scale-factor)*20.30px)">Earth. In addition, the spectra of five stars (A - E) as seen from Earth are shown. Rank the size of the Doppler shift (from largest to smallest) for the light from each star (A – E).</span><span><br></span><span style="font-size: calc(var(--scale-factor)*18.05px)">A. </span><span style="font-size: calc(var(--scale-factor)*24.05px)">C &gt; B &gt; A &gt; D &gt; E</span><span><br></span><span style="font-size: calc(var(--scale-factor)*18.02px)">B. </span><span style="font-size: calc(var(--scale-factor)*24.05px)">C &gt; A &gt; E &gt; D &gt; B</span><span><br></span><span style="font-size: calc(var(--scale-factor)*18.05px)">C. </span><span style="font-size: calc(var(--scale-factor)*24.05px)">E &gt; D &gt; A &gt; B &gt; C</span><span><br></span><span style="font-size: calc(var(--scale-factor)*18.02px)">D. </span><span style="font-size: calc(var(--scale-factor)*24.05px)">B &gt; D &gt; E &gt; A &gt; C</span></p>

The first spectra shown below is of an element as it appears in a laboratory here on Earth. In addition, the spectra of five stars (A - E) as seen from Earth are shown. Rank the size of the Doppler shift (from largest to smallest) for the light from each star (A – E).
A. C > B > A > D > E
B. C > A > E > D > B
C. E > D > A > B > C
D. B > D > E > A > C

A. C > B > A > D > E

97
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Compared to a 5-m telescope, a 10-m telescope gathers _____ light in the same amount of time.
A. the same amount of
B. twice as much
C. four times as much
D. eight times as much

C. four times as much

98
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<p><span style="font-size: calc(var(--scale-factor)*27.80px)">Below are two images of the same pair of stars. Both were observed over the same wavelength range for the same amount of time. One was taken with the 1-m telescope while the other was taken with the 2-m telescope. Which image was taken with the 2-m telescope?</span><span><br></span><span style="font-size: calc(var(--scale-factor)*18.02px)">A. </span><span style="font-size: calc(var(--scale-factor)*24.05px)">Image 1</span><span><br></span><span style="font-size: calc(var(--scale-factor)*18.05px)">B. </span><span style="font-size: calc(var(--scale-factor)*24.05px)">Image 2</span><span><br></span><span style="font-size: calc(var(--scale-factor)*18.02px)">C. </span><span style="font-size: calc(var(--scale-factor)*24.05px)">There is insufficient information</span></p>

Below are two images of the same pair of stars. Both were observed over the same wavelength range for the same amount of time. One was taken with the 1-m telescope while the other was taken with the 2-m telescope. Which image was taken with the 2-m telescope?
A. Image 1
B. Image 2
C. There is insufficient information

A. image 1

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<p><span style="font-size: calc(var(--scale-factor)*26.30px)">Below are two images of the same pair of stars. Both were observed with the same telescope for the same amount of time. One was observed with a red filter while the other was observed with a blue filter. Which image was taken with the red filter? (Note: The stars give off the same amount of light in both colors.)</span><span><br></span><span style="font-size: calc(var(--scale-factor)*18.05px)">A. </span><span style="font-size: calc(var(--scale-factor)*24.05px)">Image 3</span><span><br></span><span style="font-size: calc(var(--scale-factor)*18.02px)">B. </span><span style="font-size: calc(var(--scale-factor)*24.05px)">Image 4</span><span><br></span><span style="font-size: calc(var(--scale-factor)*18.05px)">C. </span><span style="font-size: calc(var(--scale-factor)*24.05px)">There is insufficient information.</span></p>

Below are two images of the same pair of stars. Both were observed with the same telescope for the same amount of time. One was observed with a red filter while the other was observed with a blue filter. Which image was taken with the red filter? (Note: The stars give off the same amount of light in both colors.)
A. Image 3
B. Image 4
C. There is insufficient information.

B. image 4

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Most ground based telescope observe in the visible and radio wavelengths because
A. People are best suited to see in the visible wavelengths and hear in the radio wavelengths.
B. It is easiest to build telescopes which observe at these wavelengths.
C. All of the really cool objects emit light at these wavelengths.
D. Most other wavelengths cannot penetrate through the Earth’s atmosphere.
E. The Earth radiates too much energy in the other wavelengths, interfering with their detection.

D. Most other wavelengths cannot penetrate through the Earth’s atmosphere.