Term
| Physical Properties of Jupiter |
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Definition
mass 2x the mass of all other planets combined
no solid surface
differential rotation |
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Term
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Definition
bright zones and dark belts
Great Red Spot
mostly H but some He
small amounts of methane, ammonia, and water vapor |
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Term
| Jupiter's Internal Structure |
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Definition
radiates more energy than it recieves from sun because interior is still cooling from formation
central core is metallic hydrogen and helium and is rocky
outer core is molecular hydrogen and helium |
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Term
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Definition
surrounder by huge magnetic belts
about 300 km across, extends beyond Saturn's orbit
20,000x Earth's magnetosphere |
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Term
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Definition
Io
Europa
Ganymede
Callisto |
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Term
Physical Properties of Io
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Definition
iron, iron/ sulfide core
rocky mantle
many volcanoes
particles from eruption form Plasma Torus
youngest surface in solar system
no craters
sulfur and sulfonic compounds |
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Term
| Physical Properties of Europa |
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Definition
iron, iron/sulfide core
ice crust with possible water underneath
tidal forces cause ice to crack forming an ice jumble on the surface
almost no craters
crater: Pwyll |
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Term
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Definition
| discovered 1st asteroid in 1801 |
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Term
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Definition
| discovered Jupiter's moons |
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Term
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Definition
| 1st saw Jupiter's Great Red Spot |
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Definition
| credited with beginning meteor science |
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Term
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Definition
| theorized that Saturn's rings were made of particles |
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Definition
| started the search that led to the discovery of Pluto |
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Definition
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Definition
| used doppler effects to prove Maxwell's theory |
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Term
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Definition
| discovered Uranus in 1781 |
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Term
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Definition
| discovered rings of Saturn in 1977 |
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Term
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Definition
| predicted Neptune's location in 1845 |
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Term
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Definition
| found Neptune after calculations were published |
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Term
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Definition
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Definition
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Term
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Definition
| proposed Oort Cloud in 1950 |
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Term
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Definition
| discovered Pluto's moon Charon in 1978 |
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Term
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Definition
| dirty snowball model of comet |
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Term
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Definition
discovered Jupiter's Rings
carried message to ETs
The Grande Tour
found that Saturn's rings have spokes
discovered more of Saturn's moons
only mission to reach as far as Uranus
found 6 small Neptune moons
found that Neptune's rings were complete but thicker in some parts |
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Term
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Definition
discovered that rings form from the crashing of inner satellites
saw Aurora on Neptune
visited asteroids Gaspra and Ida |
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Term
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Definition
first craft to leave carrying message to ETs
passed close by Saturn |
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Term
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Definition
| visited asteroid Mathilde |
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Term
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Definition
| found new explanation for Lapelus |
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Term
| Physical Properties of Asteroids |
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Definition
small
eccentric orbits
rocky |
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Term
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Definition
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Term
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Definition
C-type: carbonaceous, dark
S-type: silicate (rocky)
M-type: metallic (iron and nickel) |
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Term
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Definition
asteroids with orbits so eccentric
they cross Earth's orbit |
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Term
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Definition
| orbit at L4 and L5 Lagrangian Points on Jupiter's orbit |
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Term
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Definition
| if a meteor reaches the Earth's surface |
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Term
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Definition
| bright flashes of light from micrometeoroids hitting the atmosphere |
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Term
| Where is the Kuiper Belt? |
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Definition
| just beyond Neptune's orbit |
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Term
| Where do most comets reside? |
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Definition
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Term
| Physical Properties of Meteoroids |
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Definition
less than 100 m in diameter
most rock, some iron
usually between 4.4 and 4.6 billion years old |
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Term
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Definition
| less common and have periods shorter than 200 years |
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Term
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Definition
| have periods of 100s, 1000s or even millions of years |
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Term
| Physical Properties of Comet |
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Definition
nucleus
coma of gas and dust (most visible part)
dust tail and ion tail
very eccentric orbits
icy |
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Term
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Definition
| the gradual disintegration of a comet as it reaches the sun, it leaves a meteor swarm and if the Earth's orbit encounters this swarm we see a meteor shower |
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Term
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Definition
Whipple
a comet is composed of dust grains, rocks, and frozen gases |
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Term
| Where is the asteroid belt? |
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Definition
| between the orbits of Mars and Jupiter |
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Term
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Definition
| gaps in the asteroid belt caused by resonance with Jupiter |
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Term
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Definition
iron: found most often but compose only 6% of all meteorites
stone: most common
stony irons |
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Term
| Physical Properties of Ganymede |
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Definition
iron, iron sulfide core
rocky mantle
icy crust
surface features indicate plate activity
dark areas that resemble maria but are just dirty ice
craters indicate old surface
largest moon in SS
larger than Pluto or Mercury
history similar to Earth's moon but has ice instead of rock |
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Term
| Physical Properties of Callisto |
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Definition
no plate activity
most heavily crated surface in SS
Vahalla impact basin with possible ocean inside
similar to Ganymede |
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Term
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Definition
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Term
| Medium Sized Moons of Saturn |
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Definition
Rhea (largest)
Dione and Tethyes
Mimas
Enceladus
Lapetus
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Term
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Definition
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Term
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Definition
almost as big as Ganymede
thicker and denser atmosphere than Earth
atmosphere is Nitrogen
methane and ethane lakes and rivers
orange haze due to organic molecules |
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Term
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Definition
relatively flat and cratered surface
craters and wisps but no large craters |
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Term
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Definition
similar to Tethyes
icy and cratered surface
craters, wisps, and rays |
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Term
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Definition
similar to Dione
icy and cratered surface
large crater and canyon |
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Term
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Definition
closest moon to Saturn
has crater covering 1/3 of its surface
has giant canyon opposite crater |
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Term
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Definition
orbits close to Mimas
very shiny, indicates it may be covered with ice
recent activity and internal heating |
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Term
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Definition
2 faced
leading side very dark
trailing side very bright |
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Term
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Definition
hamburger shaped
same size as Mimas |
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Term
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Definition
captured asteroid
retrograde motion |
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Term
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Definition
Ariel
Umbriel
Titania
Oberon
Miranda |
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Term
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Definition
youngest surface in SS
tectonic activity
few large craters
global fractures/ fault lines |
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Term
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Definition
darker
uniform surface covered with craters
unexplained bright ring feature |
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Term
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Definition
few large craters
many young scarps
some fresh material
trenches |
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Term
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Definition
many large craters
high mountain scarps
dark patches in crater floor |
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Term
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Definition
part of surface has undulating cratered plains
part with regions of scarps that show up as dark bands
global faults
chevron feature
racetrack feature
most unusual of the moons |
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Term
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Definition
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Term
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Definition
large
normal orbit
retrograde motion
ice volcanoes
nitrogen atmosphere
weird terrain in different hemispheres
flooded ice plains
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Term
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Definition
small
very eccentric orbit
prograde motion
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Term
| Describe Belts of Jupiter |
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Definition
made of dark aluminum hydrosulfide
dark
sinking |
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Term
| Describe Zones of Jupiter |
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Definition
white ammonia clouds
cooler
rising
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Term
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Definition
coriolis forces
anticyclonic storm (high pressure center with low pressure surrounding)
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Term
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Definition
Gossamer ring, main ring, halo
can be viewed from Earth using special telescope
forms from collisions of inner satellites
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Term
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Definition
less dense than water
flattened due to rapid and differential rotation
prominent but then rings
77% H, 22% He
no solid surface
95x Earth's mass |
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Term
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Definition
differential rotation rates
belts and zones like Jupiter but much less bright
similar to Jupiter's but pressure is lower
three cloud layers, thicker than Jupiters
mostly H some He (less than Jupiter's)
wind patterns similar to Jupiter's but with zonal flow
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Term
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Definition
similar to Jupiters
rick/ice core
inner core metallic H
outer core molecular H
radiates more energy than it gets from sun due to interior still cooling
H and He not well mixed
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Term
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Definition
strong magnetosphere but only 5% of Jupiter's
creates Auroras |
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Term
| What does helium do on Saturn? |
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Definition
| forms droplets and then falls to cool surface |
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Term
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Definition
so large and complex that telescopes can see them
composition of particles is water/ice mixture
all rings inside roche limit
radial spikes form and then dissipate
cassini division caused by resonance with other particles and Saturn's moon
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Term
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Definition
| closest distance to a planet that a moon would survive |
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Term
| What is the strangest ring of Saturn? |
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Definition
F Ring
outer most ring
appears to have kinks and braids
oddities caused by its 2 shepard moons |
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Term
| Formation of Saturns Rings |
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Definition
too active to have been there since beginning of SS
either the result of a catastrophic event or are continually replenished |
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Term
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Definition
| similar to Jupiter but with much less storms |
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Term
| Are Saturn's rings in its equatorial plane? |
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Definition
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Term
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Definition
mass 14.5x Earth's
similar to Neptune
axis of rotation lies in its plane of orbit (very odd, causes extreme seasonal variation) |
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Term
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Definition
similar to Uranus
mass 17.7x Earth's |
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Term
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Definition
outer atmosphere similar to Jupiter and Saturn
cold enough to freeze ammonia
mainly methane (gives it its blue color)
internal heat source
band structure more visible
storms similar to those on Jupiter but much fewer |
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Term
| Magnetospheres of Uranus and Neptune |
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Definition
substantial magnetic field but at a large angle to their rotation axis
magnetic fields are not produced by dynamos like other planets |
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Term
| Interior of Uranus and Neptune |
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Definition
rocky core surrounded by a type of slush then surrounded by molecular hydrogen
Neptune has internal heat source
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Term
| Ring System of Uranus and Neptune |
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Definition
both have very faint ring systems only recently observed
2 shepard moons keep epsilon ring from fusing
Neptune has 5 rings |
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Term
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Definition
eccentric
inclined to the plane of the ecliptic
crosses Neptune's orbit
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Term
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Definition
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Term
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Definition
high level of photochemical haze (cant see surface)
dark polar cap
brightening in mid latitudes
atmospheric movements indicate something is happening in interior
interior rotates slower than atm |
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Term
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Definition
9 rings found from ground based observation
epsilon ring is largest and most easily seen
very narrow
little dust in rings
consist of particles several cm across |
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Term
| What is the only shuttle to reach distances as far as Uranus? |
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Definition
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Term
| Has Neptune made a complete revolution since its finding? |
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Definition
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Term
| Atmosphere and Internal Structure of Neptune |
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Definition
had Great Dark Spot that disappeared in 1994
scooter=bright feature below great dark spot
interior similar to Uranus
blue due to Methane
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Term
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Definition
strangely off center like Uranus'
probably caused by some form of ice that can conduct
Aurora seen by Galileo Spacecraft |
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Term
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Definition
| Nitrogen and methane detected so far |
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Term
| Surface and Interior of Pluto |
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Definition
mapping of surface using lunar occulations
interior thought to be similar to icy moons like Ganymede
no evidence of a magnetic field |
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Term
| Possible Origins of Pluto |
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Definition
escaped moon from Neptune
Kuiper Belt asteroid
possible victim of violence in early SS |
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Term
| Is the ion or dust tail of a comet straighter? |
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Definition
| ion tail is straighter than dust tail |
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Term
| Where does the tail of a comet always point? |
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Definition
| away from the sun due to solar winds |
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Term
| Have objects been observed in the Oort Cloud? |
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Definition
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Term
| What defines a meteoroid? |
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Definition
| being less than 100 m in diameter |
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Term
| Larger meteorides are usually... |
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Definition
| loners from the asteroid belt and have caused most of the craters in the SS |
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Term
| What do most meteoroids carry? |
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Definition
| valueable info about the early stages of the SS bc they are so old |
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Term
| Total mass of all the asteroids is.. |
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Definition
less than that of the moon
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Term
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Definition
| icy and usually orbit far from the sun |
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Term
| What happens to comets as they begin to reach the sun? |
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Definition
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Term
| When are meteors more like comets and when are they more like asteroids? |
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Definition
more like comets when they burn up in the atmosphere
more like asteroids when they hit Earth |
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Term
| Comets are only bright when... |
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Definition
| they get close to the sun |
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Term
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Definition
a few km on average
loses 1% of mass as it orbits around the sun
rotates |
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Term
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Definition
maximum at perihelon
ion tail goes straight back
dust tail curves due to radiation pressure |
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Term
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Definition
hydrogen cloud
bright due to reflecting sunlight and fluorescent gases
can be up to 100,000 km across |
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