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Wednesday, December 12, 2012

quiz : Astronomy

1.

Rank the five terrestrial worlds in order of size from smallest to largest:
Student ResponseValueCorrect Answer
Student Response Moon, Mercury, Mars, Venus, Earth.100%Student Response  
Mercury, Venus, Earth, Moon, Mars.
Mercury, Moon, Venus, Earth, Mars.
Moon, Mercury, Venus, Earth, Mars.
Mercury, Moon, Mars, Earth, Venus.
Score:1.83/1.83

2.

The planet's orbital period is:
Student ResponseValueCorrect Answer
the time its magnetic field takes to spin once.
Student Response the time it takes to return to the same location in the sky, relative to the Sun.100%Student Response  
the time it takes it to rotate and have the same face toward us again.
the time it takes for it to retrograde back to the same position as we pass it.
the time it takes for a satellite to orbit it.
Score:1.83/1.83

3.

How do the densities of the jovian and terrestrial planets compare?
Student ResponseValueCorrect Answer
The closer a planet lies to the Sun, the less its density.
Made from the same solar nebula, they are all similar.
More massive jovians all have high densities, compared to the tiny terrestrials.
Student Response All terrestrials are more dense than any of the jovians.100%Student Response  
No real pattern here; densities vary greatly and are very individual to each world.
Score:1.83/1.83

4.

The Kuiper Belt is found where in the solar system?
Student ResponseValueCorrect Answer
sixty degrees ahead or behind Jupiter
between the orbits of Jupiter and Uranus
between the orbits of Mars and Jupiter
Student Response beyond the orbit of Neptune100%Student Response  
among the orbits of the terrestrial planets
Score:1.83/1.83

5.

In composition and density, the asteroids most resemble:
Student ResponseValueCorrect Answer
Kuiper Belt objects like Pluto.
comets.
Student Response pieces of terrestrial planets.100%Student Response  
jovian moons.
the Sun.
Score:1.83/1.83

6.

A meteorite is
Student ResponseValueCorrect Answer
Student Response an irregularly shaped body, mostly found orbiting between Mars and Jupiter.0%
an icy body with a long tail extending from it.
a streak of light in the atmosphere.
a chunk of space debris that has struck the ground.Student Response  
a chunk of space debris orbiting the Earth.
Score:0/1.83

7.

The Kuiper Belt is an "outer asteroid belt" consisting of what types of solar system
bodies?
Student ResponseValueCorrect Answer
terrestrial planets
Student Response icy cometlike bodies100%Student Response  
meteoroids
asteroids
jovian planets
Score:1.83/1.83

8.

The jovian planets
Student ResponseValueCorrect Answer
Student Response all have rings around their equators.100%Student Response  
are all much more dense than any of the terrestrials planets.
all spin slower than the earth.
all lie less than 5 AU from the Sun.
have satellite systems with less than 4 moons.
Score:1.83/1.83

9.

Masses of the planets are easiest to determine if:
Student ResponseValueCorrect Answer
they are dense and easily deflect the path of passing spacecraft.
Student Response they have natural satellites whose motions can be precisely measured.100%Student Response  
they move rapidly and their periods are easily measured.
they are terrestrial and the extra size of the planet's disk can be measured.
they are jovian and their oblateness can be found.
Score:1.83/1.83

10.

From center to surface, which of the following correctly lists the interior layers of a terrestrial world?
Student ResponseValueCorrect Answer
Student Response core, mantle, crust100%Student Response  
core, crust, lithosphere
mantle, core, crust
mantle, crust, core
Score:1.83/1.83

11.

Which of the terrestrial worlds has the strongest magnetic field?
Student ResponseValueCorrect Answer
Mars
Venus
the Moon
Student Response Earth100%Student Response  
Mercury
Score:1.83/1.83

12.

Which of the following most likely explains why Venus does not have a strong magnetic field?
Student ResponseValueCorrect Answer
It has too thick an atmosphere.
Student Response Its rotation is too slow.100%Student Response  
It is too close to the Sun.
It does not have a metallic core.
It is too large.
Score:1.83/1.83

13.

There are no auroras on Venus because it
Student ResponseValueCorrect Answer
is too hot.
lacks atmospheric oxygen.
Student Response lacks a strong magnetic field.100%Student Response  
lacks strong winds.
Score:1.83/1.83

14.

What process has shaped Earth's surface more than any other?
Student ResponseValueCorrect Answer
impact cratering
acid rain
volcanism
wind erosion
Student Response plate tectonics100%Student Response  
Score:1.83/1.83

15.

Which of the following worlds has the most substantial atmosphere?
Student ResponseValueCorrect Answer
Mercury
Mars
Student Response Venus100%Student Response  
the Moon
Earth
Score:1.83/1.83

16.

Valles Marineris is a(n)
Student ResponseValueCorrect Answer
huge series of cliffs on Mercury.
extensive plain on Mars.
large canyon on Venus.
Student Response large canyon on Mars.100%Student Response  
large valley on the Moon.
Score:1.83/1.83

17.

Which of the following show evidence of ancient river beds?
Student ResponseValueCorrect Answer
the Moon
Student Response Mars100%Student Response  
Mercury
Venus
all of the above
Score:1.83/1.83

18.

What gas is the primary constituent of our atmosphere?
Student ResponseValueCorrect Answer
carbon dioxide
hydrogen
Student Response nitrogen100%Student Response  
oxygen
helium
Score:1.83/1.83

19.

Which statement about seismic waves is FALSE?
Student ResponseValueCorrect Answer
P waves travel faster, so the gap between their arrival times gives the source's distance.
S waves are blocked by the fluid outer core and cannot be observed on the other side of the planet from the epicenter.
Student Response Only P waves can be detected in the shadow zone.100%Student Response  
Close to the epicenter, both S and P waves can be recorded.
Both S and P waves can be detected by seismographs.
Score:1.83/1.83

20.

When strong solar winds are displaced poleward by our magnetic fields, we get
Student ResponseValueCorrect Answer
Student Response intense auroral displays.100%Student Response  
droughts and dust bowls in the American West.
the Van Allen radiation belts.
hurricanes in the tropics.
sunspots.
Score:1.83/1.83

21.

The region around Earth where the magnetic field traps charged particles is the:
Student ResponseValueCorrect Answer
aurora borealis and aurstralis.
Student Response Van Allen Radiation Belts.100%Student Response  
exosphere.
corona.
ozone layer.
Score:1.83/1.83

22.

We determine the structure of the Earth's core using
Student ResponseValueCorrect Answer
deep mine shafts.
magnetic resonance imaging.
radar and sonar.
Student Response seismic wave data.100%Student Response  
satellite imaging.
Score:1.83/1.83

23.

The Dynamo Theory holds that:
Student ResponseValueCorrect Answer
lightning plays a major role in generating our magnetic fields.
the Earth's core, like Mercury's, is now a solid, rigid bar magnet.
any other planet of similar density will also have a strong magnetic field.
Student Response magnetic fields are generated by rapidly spinning, fluid magnetic interiors.100%Student Response  
the Earth's magnetic field must switch polarities every few million years.
Score:1.83/1.83

24.

The principal greenhouse gases in our present atmosphere are:
Student ResponseValueCorrect Answer
Student Response water vapor and carbon dioxide.100%Student Response  
hydrogen sulfide and carbon disulfide.
hydrogen and helium.
methane and ammonia.
sulfuric acid vapor and carbon dioxide.
Score:1.83/1.83

25.

The Greenhouse Effect works by trapping
Student ResponseValueCorrect Answer
outgoing ultraviolet radiation from the Earth.
incoming ultraviolet radiation from the Sun.
incoming infrared radiation from the Sun.
Student Response the heat from the Sun in Earth's atmosphere.0%
outgoing infrared radiation from the Earth.Student Response  
Score:0/1.83

26.

At what phase are the tides least noticeable?
Student ResponseValueCorrect Answer
new Moon
waxing crescent
waning gibbous
First quarterStudent Response  
Student Response full Moon0%
Score:0/1.83

27.

What is true of spring tides?
Student ResponseValueCorrect Answer
The difference between low and high tides would be smallest.
The Moon's phase will be first quarter.
There would be one high and one low tide each day.
The third quarter Moon would be high overhead at dawn.
Student Response The difference between low and high tides would be greatest.100%Student Response  
Score:1.83/1.83

28.

In size, Mercury is intermediate between:
Student ResponseValueCorrect Answer
Student Response the Moon and Mars.100%Student Response  
Pluto and the Moon.
Ceres and Pluto.
Earth and Venus.
Mars and Earth.
Score:1.83/1.83

29.

One of the effects of Mercury's very slow spin is
Student ResponseValueCorrect Answer
large variations in the size of its polar cap.
wind patterns that are slow, but global in size.
tectonic activity.
Student Response extreme variations in its surface temperature.100%Student Response  
an intensely powerful magnetic field.
Score:1.83/1.83

30.

All of the statements below are true. Which one gives the primary reason why the surface of Venus today is some 450°C hotter than the surface of Earth?
Student ResponseValueCorrect Answer
Student Response Venus has a much stronger greenhouse effect than Earth.100%Student Response  
Venus has a much higher reflectivity than Earth.
Venus has a higher atmospheric pressure than Earth.
Venus is only about 73% as far from the Sun as Earth.
Score:1.83/1.83

31.

Why is the sky blue (on Earth)?
Student ResponseValueCorrect Answer
Because molecules scatter red light more effectively than blue light.
No one knows – this is one of the great mysteries of science.
Because the Sun emits mostly blue light.
Student Response Because molecules scatter blue light more effectively than red light.100%Student Response  
Because deep space is blue in color.
Score:1.83/1.83

32.

The lunar highlands are:
Student ResponseValueCorrect Answer
formed by plate tectonics, like the Earth's Himalayas.
brighter than the mare, since they are covered with reflective glass from the rays.
formed by volcanic eruptions, much like our Andes.
made of lighter colored, younger rocks than the mare.
Student Response more rugged, heavily cratered , and older than the lunar mare.100%Student Response  
Score:1.83/1.83

33.

What did radar astronomers find in the polar regions of Mercury?
Student ResponseValueCorrect Answer
auroral displays much like Earth's
polar caps of dry ice that vary seasonally, much like Mars
Student Response water ice that never melts in the deep craters100%Student Response  
rift valleys
large mare basins, such as near our Moon's south pole
Score:1.83/1.83

34.

How does Mercury's rotation relate to the Sun?
Student ResponseValueCorrect Answer
Student Response Its rotation rate is 2/3 as long as its year, due to tidal resonances.100%Student Response  
Its day is the same length as its year.
It does not spin at all, being tidal stopped by the solar tides.
It always keeps one face tidally locked toward the Sun, as our Moon does with us.
Its year is much shorter, only 88 days, than its slow rotation of 243 days on its axis.
Score:1.83/1.83

35.

What is true of the Moon's orbital and rotational periods?
Student ResponseValueCorrect Answer
Student Response They are equal.100%Student Response  
The rotational period varies with the Moon's phase.
The rotational period is longer.
The orbital period is greatest at full moon.
The orbital period is longer.
Score:1.83/1.83

36.

Which of these features is attributed to the shrinking of Mercury's core?
Student ResponseValueCorrect Answer
rays
rilles
Student Response scarps100%Student Response  
craters
mare
Score:1.83/1.83

37.

Mercury's surface most resembles which of these?
Student ResponseValueCorrect Answer
Venus' polar regions
the lunar mare
Mars' deserts
Student Response the lunar far side100%Student Response  
the earth's deserts
Score:1.83/1.83

38.

Which of these theories seems to best explain the Moon's origin?
Student ResponseValueCorrect Answer
Student Response Impact Theory100%Student Response  
Fusion Theory
Coformation Theory
Capture Theory
Fission Theory
Score:1.83/1.83

39.

Venus orbits the Sun in 225 days. How long does it take to rotate on its axis?
Student ResponseValueCorrect Answer
225 days, so it keeps the same face toward the Sun
36 days, for reasons unknown
450 days, exactly at 2:1 spin-orbit resonance
Student Response 243 days, even though the Earth's tidal pull is not involved100%Student Response  
24 hours, 36 minutes, very similar to Earth and Mars
Score:1.83/1.83

40.

Through radar observations it was found that Venus'
Student ResponseValueCorrect Answer
Student Response rotation on its axis is retrograde.100%Student Response  
atmosphere is changing rapidly.
orbital period is 243 days.
orbit around the Sun is speeding up.
orbit around the Sun is in the clockwise sense.
Score:1.83/1.83

41.

Earth and Venus are often called sister planets; in which ways are they most alike?
Student ResponseValueCorrect Answer
surface temperature and pressure
atmospheric composition and density
polar caps and rusty red deserts
Student Response size, density, and surface gravity100%Student Response  
cloud composition and meteorology
Score:1.83/1.83

42.

The surface of Venus can be observed with:
Student ResponseValueCorrect Answer
Student Response radar observations from Arecibo.100%Student Response  
the Mt. Wilson 100" telescope.
most amateur telescopes.
the Hubble Space Telescope.
All of these have provided detailed observations about the surface of our sister planet.
Score:1.83/1.83

43.

Maxwell Mons on Venus is a huge:
Student ResponseValueCorrect Answer
impact crater larger than Texas.
Student Response shield volcano.100%Student Response  
tectonic mountain chain, like the Himalayas.
rift valley.
ocean basin larger than the Pacific Ocean.
Score:1.83/1.83

44.

The largest volcanic structures on Venus are called:
Student ResponseValueCorrect Answer
Student Response coronae.100%Student Response  
cinder cones.
calderas.
crater cones.
shield volcanoes.
Score:1.83/1.83

45.

What is the result of the Greenhouse effect on the surface environment of Venus?
Student ResponseValueCorrect Answer
It has reduced the surface temperature by about 30 degrees Celsius.
Student Response It has raised the surface temperature by hundreds of degrees Celsius100%Student Response  
It causes the surface temperature of Venus to become hotter than the Sun.
Its effect is about the same as on Earth.
It has little or no effect.
Score:1.8/1.8

46.

What is the main constituent of the atmosphere of Venus?
Student ResponseValueCorrect Answer
Student Response carbon dioxide100%Student Response  
oxygen
hydrogen
nitrogen
sulfuric acid
Score:1.8/1.8

47.

The highest peak on Venus is called:
Student ResponseValueCorrect Answer
Student Response Maxwell.100%Student Response  
Gula.
Shif.
Lakshmi.
Cleopatra.
Score:1.8/1.8

48.

The absence of a magnetic field on Venus probably stems from its:
Student ResponseValueCorrect Answer
high surface temperatures.
lower density than Earth, suggesting an absence of an iron core.
extremely thick atmosphere.
Student Response slow rotation.100%Student Response  
nearness to the Sun.
Score:1.8/1.8

49.

Which is the correct size order, from smallest to largest?
Student ResponseValueCorrect Answer
Venus, Mars, Earth
Student Response Mercury, Mars, Venus100%Student Response  
The Moon, Earth, Mars
Mercury, the Moon, Mars
Mercury, Venus, Mars
Score:1.8/1.8

50.

How long is a day on Mars?
Student ResponseValueCorrect Answer
9 hours, 55 minutes
243 Earth days
23 hours, 56 minutes
Student Response 24 hours, 36 minutes100%Student Response  
about 4.2 Earth days
Score:1.82/1.82

51.

The most prominent feature of Mars observable from Earth is
Student ResponseValueCorrect Answer
Student Response its bright polar caps.100%Student Response  
the prominent feature, Valles Marineris.
its two prominent moons.
the large volcano Olympus Mons.
its thick atmosphere.
Score:1.83/1.83

52.

Most of the dark regions on Mars visible from Earth are
Student ResponseValueCorrect Answer
Student Response volcanic planes like the lunar maria.100%Student Response  
features like the Valles Marineris.
lava flows from active volcanoes.
the seasonal growth of vegetation on the planet.
mountainous regions.
Score:1.83/1.83

53.

Valles Marineris is the most striking example of a(n)
Student ResponseValueCorrect Answer
impact crater.
oceanic trench.
Student Response rift valley.100%Student Response  
scarp.
shield volcano.
Score:1.8/1.8

54.

Why is Mars red?
Student ResponseValueCorrect Answer
Dust storms on the planet have blasted the planet so fiercely that the rocks have reddened.
The ancient volcanoes poured out vast plains of molten sulfur, much as on Io, which has now solidified and preserved the reddish color.
Sulfuric acid rain etched a reddish color into iron-rich surface rocks.
Student Response The iron in the surface rocks have been oxidized over time.100%Student Response  
Mercuric oxide is abundant and has a red tint.
Score:1.8/1.8

55.

How many moons does Mars have?
Student ResponseValueCorrect Answer
none
one
Student Response two100%Student Response  
three
four
Score:1.8/1.8

56.

The main constituent of the martian atmosphere is
Student ResponseValueCorrect Answer
Student Response carbon dioxide.100%Student Response  
helium.
methane.
hydrogen.
nitrogen.
Score:1.8/1.8

57.

The largest shield volcano yet discovered is:
Student ResponseValueCorrect Answer
Prometheus on Io.
Kilimanjaro on Earth.
Student Response Olympus Mons on Mars.100%Student Response  
Maxwell Mons on Venus.
Caloris on Mercury.
Score:1.8/1.8

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