Jupiter's Moons





the only body in the solar system known to have active volcanos other than the Earth is:

A titan.

B callisto.

C Io.

D triton.



the Galilean satellite with the smoothest surface is

A Io

B Europa

C Ganymede

D callisto



the Galilean satellite with the highest average density is

A Io

B Europa

C Ganymede

D callisto



Jupiter's rings were discovered by

A spacecraft photography

B momentary occultation of starlight as the planet moved in front of a star

C visual observations by Galileo

D direct ground-based photography



the largest satellite (moon) in our planetary system is

A phobos, one moon of Mars

B titan, a moon of Saturn

C Ganymede, a moon of Jupiter

D the Earth's moon



of the Galilean moons of Jupiter, callisto has a surface that is the most heavily cratered. this fact implies that, compared to the others, callisto has the

A highest bulk density.

B most ice on its surface.

C most evolved surface.

D least evolved surface.

E strongest magnetic field.



the most geologically active object in the planetary system at the present time is

A Mars

B Earth

C the Earth's moon

D Io, the innermost large satellite of Jupiter



the Galilean satellites have densities that are:

A about like that of solid rock.

B about like that of Earth.

C less than that of water.

D greater than that of any of the Jovian planets.



the Galilean satellite furthest from Jupiter is

A Io

B Europa

C Ganymede

D callisto



Io appears more active than the other Galilean satellites of Jupiter. this activity may arise from

A stronger heating of Io due to tidal friction.

B the radiation close to Jupiter.

C Io's smaller density.

D Jupiter's magnetic field.



the Galilean satellite with the largest diameter is

A Io

B Europa

C Ganymede

D callisto



Io, one of the major Jupiter moons, is undergoing extensive volcanic activity associated with interior heating which is caused by

A solar radiation and heat falling on the surface

B the effect of Jupiter's van allen particles

C original heat, caused by gravitational condensation at the moon's formation

D tidal distortion and internal friction because of flexing



the energy for the volcanic activity on Io results from

A radioactive substances with it.

B chemical reactions.

C tidal action.

D energy radiated from Jupiter and the sun.

E both (a) and (b) above.



Jupiter's moon Io has no observable impact craters because

A volcanic activity has covered them over.

B its proximity to Jupiter prevents large impacts.

C the surface is molten and meteorites sink into it.

D a thick atmosphere keeps us from seeing the surface.



which chemical or chemicals appear to play a prominent role in the "volcanoes" of Io?

A sulfur

B h2o

C methane and ammonia

D molten lava



the major chemical constituent of the layers of material continuously being deposited upon the surface of Io, the moon of Jupiter, by "volcanic" activity is

A water

B silicate dust and rock

C hydrogen

D sulfur



the main source of heat which produces Io's volcanic activity is

A the solar wind

B the Jupiter-Io tidal force

C Jupiter's rapid rotation rate

D radioactivity



which of these has an icy surface with few impact craters that is covered by intersecting lines that look like cracks?

A Io

B Europa

C Ganymede

D callisto



which of these is the darkest of Jupiter's big moons, and yet has a surface which is saturated by impact craters?

A Io

B Europa

C Ganymede

D callisto



the source of intense heating in the interior of Jupiter's moon Io, causing continuous and intense volcanic activity, is

A solar UV and visible radiation

B frictional heating as the solar wind impacts upon the moon surface

C tidal flexing and distortion, caused by Jupiter and the other large moons

D heat released by continuous shrinkage after creation, transforming potential gravitational energy to heat



of the 4 Galilean satellites, the surface of ______ is currently the most active as evidenced by ______.

A callisto, cratering.

B Ganymede, fracturing.

C Europa, thawing and freezing of water.

D Io, volcanic activity.



which of these has the surface which has been least altered since its formation?

A Io

B Europa

C Ganymede

D callisto



the "volcanoes" on Jupiter's Galilean moon Io cover the surface of the moo with an annual layer of sulfur-laden material which is estimated to have what thickness?

A 1 meter

B about a millimeter

C 10 meters

D 10 centimeters



which of the Galilean satellites shows the oldest surface?

A Io

B Ganymede

C callisto

D Europa



which gas is thought to be responsible for the tremendous eruptions of material from Jupiter's innermost Galilean moon, Io, by providing the propulsive forces?

A sulfur in vapor form

B steam, or heated water vapor

C carbon dioxide, co2

D sulfur dioxide, so2



we can guess that Europa is active because we see

A lava flows.

B volcanic ridges and faults.

C no impact features.

D lobate scarps.



the radio bursts coming from Jupiter are now thought to be caused by a complex interaction between Jupiter's magnetic field and

A the red spot

B Io and its plasma torus

C the small inner satellites, including amalthea

D Jupiter's narrow ring



the satellite Io is interesting since it is the only body other than Earth known to exhibit

A a mainly nitrogen atmosphere

B oceans of liquid water

C current volcanic activity

D primitive life



compared to our moon, the Galilean moons of Jupiter tend to have

A a smaller mass.

B a lower density.

C smaller radii

D far fewer impact craters.



the material ejected by Io's volcanoes consists mostly of

A hydrogen

B helium

C sulfur

D iron



the Galilean satellite with many active volcanoes is

A Io

B Europa

C Ganymede

D callisto



the Galilean satellite showing the largest number of craters is

A Io

B Europa

C callisto

D Ganymede



which solar system body is believed to have deep oceans of liquid water under a surface of solid ice

A Io

B titan

C triton

D Europa



the Galilean moons farther from Jupiter have ________ density and a ________ proportion of water.

A lower, greater

B greater, greater

C lower, lower

D greater, lower

E there is no such pattern of density and proportion of water.



which of these has an icy surface with few impact craters and is covered b intersecting lines that look like cracks?

A Io

B Europa

C Ganymede

D callisto



the surfaces of some moons of Jupiter and Saturn are heavily cratered. we infer that these surface regions are

A regions of volcanic activity.

B relatively old.

C relatively young.

D highland regions.

E lowland regions.



the surface of Europa, one of the Galilean moons of Jupiter, appears to be covered with

A dark areas of older crust separated by lighter, grooved terrain

B many ancient craters and maria

C a smooth layer of ice, crossed by many cracks

D rugged mountain ranges and ancient volcanoes



we think four of the outer satellites of Jupiter were probably captured because:

A they are chemically different than the other satellites of the system.

B they orbit in the retrograde direction and that cannot be easily accounted for in other ways.

C they do not have atmospheres like the other satellites.

D they are exceedingly small and have prograde orbits.



the volcanism on Io is believed to be driven by

A sulfur dioxide and sulfur.

B carbon dioxide and dry ice.

C water vapor and carbon dioxide.

D none of these.



callisto and Ganymede, moons of Jupiter, have very shallow craters because

A they have dusty surfaces and solid cores

B no large bodies impacted them due to Jupiter's magnetic bow wave

C they have icy surfaces

D they are formed of metallic hydrogen and resist impact craters



the densities of the four Galilean satellites suggest that

A they are captured asteroids.

B they have been modified by collisions.

C the inner satellites were warmer than the outer satellites at formation.

D they formed long after Jupiter.



the required heating of the large Galilean moon, Io, of Jupiter, in order to produce volcanic activity is probably caused by

A original heat of formation

B nuclear fission within its interior

C radioactive elements in its surface

D distortion of its shape by gravitational forces from Jupiter and its other moons



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