Astronomy 101 FINAL EXAM – Flashcards

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Which planets can be seen high overhead at night?
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Mercury, Venus, Mars, Jupiter, and Saturn can be seen with the "naked" eye
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Besides the moon, which planets exibit a full set of phases?
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Mercury and Venus have a full set of phases in additon to Earth's Moon.
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Should there be another planet [not dwarf] between Mars and Jupiter?
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Not enough material[=~4%Earth's Moon] to form another planet. Jupiter gravity=movement and jostling of material, made it impossible for formation of another planet.
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Moon vs. Mercury
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Average density of Moon is 3.3 g/cm3 • Mare- dark flat lowlands with few impact craters and formed when lava flowed in to the low areas of the moon about 3.1-3.8 billion years • Highlands - bright, mountainous, cratered regions that are the result of countless meteorite impacts and formed about 4.2 - 3.9 Billion years ago • No tectonic activity • Moon-quakes caused by gravitational interactions with the Earth and not by tectonic activity • Little interior heat • Transient atmosphere produced by evaporation of surface material • Weak magnetic field
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Mercury vs. Moon
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• Experiences huge temperature extremes because it has no atmosphere, a slow rotation and its close proximity to the sun •surface gravity is ~ 2x the Moon's • Crater Walls are less steep because of the higher Gravity • Smaller pattern of ejected material because of the higher Gravity • Lacks the large maria seen on the Moon
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What are planetary rings composed of?
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dust particles, astroids hitting moons= debris
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Which planets have moons bigger than Mercury?
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Jupiter-Ganymede, Saturn-Titan
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Which planets rotate seemingly opposite from Earth?
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Venus, Uranus
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What evidence suggests that Mars had liquid water on its surface?
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ancient river deltas, outflow channels, and dry riverbeds, and spherical rocks from salt drip.
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Where is all the water on Mars now?
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escaped into space via UV rays, underneath perma frost, at the polar ice caps
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How do volcanoes grow so big on other planets?
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If a planet doesn't have plate techtonics then the terrestrial portion of that planet adjusted over the magma hot just continues to grow.
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Which planets rip apart there moons?
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as moons cross the threshold they explode
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Why are these moons ripped up by their adjacent planet?
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they pass the rouche limit
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Why was Pluto demoted to dwarf planet?
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The discovery of Eris
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Chemical compositions of Jovian planets?
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liquid & gaseous
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Chemical composition of terrestrial planets?
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rocky & metallic
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What are the unique features of Uranus?
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• Diameter: 4x Earth • Mass: 14.5x Earth • Orbit: 20x further from Sun than Earth • Relatively featureless atmosphere • Methane gives the atmosphere its blue color • The axis is tilted by 97° • Rings & Moons orbit around the equator of Uranus
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How does one determine high pressure/low pressure systems on other worlds?
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Hurricanes are low pressure systems: rotate counter-clockwise in the N. Hemisphere and clockwise in the S. Hemisphere • High pressure systems rotate the opposite sense
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What is the most distant planet or plutoid from the Sun?
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furthest planet=Neptune CPME
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As of 2012, how many moons orbit each planet/& dwarf planet?
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...
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Which worlds have active volcanoes or geysers?
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Earth, Mars, Triton, Enceladus, and Titan
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Why are Mercury and Venus so hot, and Mars so cool?
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Venus=96%CO2=runaway greenhouse effect, Mercury= no atmosphere, side facing Sun is searing hot, the side pointing away=dead cold, and slow rotation. Mars
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What was Voyager II's mission, what is it doing now?
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designated officially to study just the planetary systems of Jupiter and Saturn then possibly hit Neptune and Uranus, not is likely to be travelling through the heliosheath and into interstellar space soon
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Planets that have tilts similar to Earth are?
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Mars=25°, Saturn 26°, Neptune 29.6°
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Why do some planets have huge atmospher's and others have little to none?
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the bigger the mass the higher the gravity= the more atmosphere it can hold onto
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What types of gases can Mars hold in it's atmosphere?
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1% of Earth's (trace amounts of oxygen), CO2 migrates seasonally from the N. Polar cap to the S. Polar cap
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Terrestrial planets vs. Jovian planets
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Small/Low Mass, Rocky/Metallic, High Density, Thin Atmosphere
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Jovian planets vs. Terrestrial Planets
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Big & massive, gaseous/ liquid, low density, thick atmosphere, many moons and rings • All Jovian planets have Hydrogen and Helium rich atmospheres • Atmospheric composition more similar to the Sun than the Earth
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What is a solar day?
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24h; time between successive passes of the Sun
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What is a sidereal day?
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23h56min; time between successive passes of a given star
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Which planets have long sidereal days?
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Venus' sidereal period is 243.02 days[solar day 1/2x] Mercury's sidereal period is 58.6467 days. [nights 2x longer than year]
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Billions of years ago the Moon was alot closer to Earth. How did this effect the tides and day length?
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meaning that each day/night cycle was shorter, and tides would also have been higher [possible couple hundred meters high]
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Why do some moons have spherical shapes and other not?
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a Moon's mass must be big enough so that the force of gravity shapes the moon into a sphere.
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What are the Galilean moons?
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Io, Europa, Ganymede, and Callisto
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M,V,E,M,c,J,S,U,N,p,h,m,e
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order of planets, dwwarf planets, plutoids
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How would the sunset look on the surface of Mercury?
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just a big freakin yellow Sun against a background of black, atmosphere=1%of Earth's
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How would the sunset look on the surface of Venus?
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Cloudy, dark, Raining sulfuric rain
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How would the sunset look on the surface of Mars?
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appear blue because dust scatters, and reflects Sun's light towards me [ie. in space= appear red because blue scatters away from me], Sun would have a halo
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Important moons of Saturn:
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Titan, Enceladus, Mimas, Hyperion
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Titan:
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Saturnian, 2nd largest, Only moon with a dense atmosphere - Atmosphere: Nitrogen (90%), no Oxygen - Methane clouds rains down methane on surface
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Enceladus:
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Saturnian, "tiger stripe", cracks=water geyser venting from South Polar Region and forms the E-ring [shoots 100+ mi. into space], N.Hemisphere=preserved, surface covered in water ice
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Mimas:
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Saturnian, "death star", is causing a gap in Saturn's Ring through a gravitation resonance [2:1] [like kicking on the swing at just the right time]
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Hyperion:
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Saturnian, "sponge-like'' Not enough mass to shape itself into a sphere, abnormal craters, covered with sharp edges
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How do the atmopheres of the Jovian planets differ from eachother?
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Jupiter: 90% hydrogen, 10% helium Saturn:hydrogen and helium, ++sulfur=yellow color,nitrogen and oxygen Uranus: blue methane, reflects blue& absorbs other colours Neptune: blue methan, clouds=crystalized methane
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Planet criteria:
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Orbits around the Sun • Sufficient mass for its self-gravity to shape itself into a sphere (or ellipsoid) • Cleared its neighborhood around its orbit
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Dwarf Planet criteria:
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Orbits around the Sun • Sufficient mass for its self-gravity to shape itself into a sphere (or ellipsoid) • Not cleared its neighborhood around its orbit • Not a moon
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Plutoid Criteria:
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Orbits around the Sun • Sufficient mass for its self-gravity to shape itself into a sphere • Not cleared its neighborhood around its orbit • Not a moon • Orbits beyond the orbit of Neptune
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If the Earth's axis was no longer tilted, then how would Earth be affected?
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no more seasons
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Roche Limit
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minimum radius at which a moon may orbit a planet without being ripped apart
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Saturn: Possible Ring Origin
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an object came too close to this planet and was torn apart by gravity, creating rings
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Saturn's Ring Characteristics
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Rings are very thin: 30 feet thick (on average) Rings are composed of icy dust particles that orbit around this planet's equator
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Saturn
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Jovian, Diameter: 9.5x Earth Mass: 95x Earth Orbit: 10x further from Sun than Earth -thick upper atmosphere=cannot see below it
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Kuiper Belt
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Disk region between 30 - 1000 AU that harbors about 100 million comets
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Oort Cloud - Sph
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erical shell between 10,000 - 100,000 AU containing up to a trillion comets
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Venus
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Diameter: 95% of Earth's, Mass: 82% of Earth's, Orbit: 28% closer to Sun Solar Day = 117 Earth days Axis: tilted by 177° (rotating backwards)
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Mars
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• Diameter: 50% of Earth's • Mass: 10% of Earth's • Orbit: 52% further from Sun
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Mercury
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• Diameter: 38% of Earth's • Mass: 6% of Earth's • Orbit: 61% closer to Sun
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Planetary Atmospheres
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• The more massive the planet the larger the gravity and the more gas it can hold in its atmosphere • The speed of the gases will determine if the planet's gravity can hold the gas in its atmosphere • Higher the temperature, the faster the gas velocity
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Neptune
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• Diameter: 3.9x Earth • Mass: 17x Earth • Orbit: 30x further from Sun than Earth • Methane in the upper atmosphere gives its blue color, White clouds of crystal methane found high in the atmosphere • Great Dark Spot is a high pressure storm system
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Saturn
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• Diameter: 9.5x Earth • Mass: 95x Earth • Orbit: 10x further from Sun than Earth
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Jupiter
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• Diameter: 11.2x Earth • Mass: 318x Earth • Orbit: 5x further from Sun than Earth Galilean Moons: Io, Europa, Ganymede, Callisto
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Solar System Formation
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from the collapse of a rotating cloud ~10000 AU in size (Solar Nebula) composition of a planet depends on the type of material that condenses into a solid at the planet's location, frostlines
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Outside the frost line
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rocks, metals and hydrogen compounds like water, methane and ammonia condense to form a solid material, Jovian planets form
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Inside frost line
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rocks and metals condense to form a solid material , the Terrestrial planets form
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Jupiter Great Red Spot
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High pressure Storm system that has lasted over 300 years, Rotates with period of 6 days, Can fit 2-3 Earths across Storm,
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Moons further away from Jupiter
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experience less gravitational heating: less active surface, more cratered, older surface
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low pressure systems
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rotate counter-clockwise in the N. Hemisphere and clockwise in the S. Hemisphere [hurricanes]
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high pressure systems
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rotate clockwise in the N. Hemispher and counter-clockwise in the S. Hemisphere [Jupiters Eye]
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Jupiter's Interior
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The lower the depth, the higher the temperature and pressure, Hydrogen gas turns liquid at 1000 km in depth, Liquid hydrogen turns liquid metallic at 20,000 km in depth
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Runaway Greenhouse Effect
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caused by the concentration of CO2 in the atmosphere
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Venus' interior
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is very hot like the Earth, but does not possess a magnetic field of its very slow rotation of 243 days
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Venus' atmosphere
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Atmosphere: 85x Earth's, 96.5% CO2, Temperature: 870° F, without CO2 the temperature would drop to about 150° F
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Venus' surface
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highlands & lowlands, active geological processes
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Mar's seasons
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caused by the axial tilt and distance from the Sun, last twice as long as on Earth CO2 migrates from the N. Polar cap to the S. Polar cap
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Mar's surface
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rocks rich in iron and silicon (iron reacts with O2 to form rust (rusty red)
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Mar's atmosphere:
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1% of Earth's (trace amounts of oxygen), Temperature: -211° to 80° F (Average: - 50° F)
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Mercury's surface
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surface gravity is ~ 2x the Moon's, crater walls are less steep because of the higher Gravity=Smaller pattern of ejected material, lacks the large maria seen on the Moon
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Mercury's atmosphere
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Experiences huge temperature extremes because it has no atmosphere, a slow rotation and its close proximity to the sun
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Triton
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Neptunean's, the only major moon to orbit its planet in retrograde motion (captured Kuiper belt object)
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Io
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Jupiters, blue geyser, volcanically active, no impact craters,
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Europa
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Jupiters, "q-ball", water/ice, cracks caused by Jupiters gravity
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Ganymede
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largest moon in the solar system, old regions=dark-many impact craters, youg=light-few craters, bright area=rich in water/ice
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Callisto
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Jupiters, "black with star pattern", +++preserved craters, cool, furthest from Jupiter,
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