Ch. 22 solar system

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21 Terms

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nebular theory

  • explains formation of solar system

  • sun and planets formed from solar nebula (rotating cloud of gas and dust(

  • solar neb contracted/formed hot protosun

  • planetesimals formed

  • planetesimals becme protoplanets

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terrestrial / earth like planets

  • mercury, venus, earth, mars

  • small, dense, rocky

  • large cores of iron and nickel

  • low escape velocities

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jovial / jupiter like planets

  • jupiter, saturn, uranus, neptune

  • large, low, gaseous

  • thick atmosphers of hydrogen, helium, methane, ammonia

  • high escape velocities

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impact craters

  • collisions with massive objects

  • common in early formation of solar system

  • have central peak and ejecta lands in or near center

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maria - lunar surface

  • dark regions

  • smooth lowlands

  • originated from asteroid impacts and basaltic lava flooding surface

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highlands - lunar surface

  • bring, densely cratered regions

  • make up back side of moon

  • older than maria

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lunar regolith

  • layer of gray, unconsolidated debris 2-20 m thick

  • igneous rock, breccia, glass beads and lunar dust from few billion years of meteoric bombardment

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mercury

  • 1st planet from sun

  • no atmosphere

  • cratered highlands

  • vast and smooth

  • dense

  • revolves quick, rotates slow

  • low escape velocity

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venus

  • 2nd planet from sun

  • 900F

  • similar to earth in size and density

  • thick clouds

    • no visible light

    • 97% carbon dioxide

    • pressure 90x earth

    • rains sulfuric acid

  • surface mapped by radar satellites

  • rotates opposite direction around sun

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mars

  • 4th planet - red planet

  • 1% as dense as earth

  • mostly co2

  • -193F

  • polar caps of frozen water and thin layer of frozen co2

  • dust storms of 170mph

  • large volcanos and canyons

  • tectonically dead

  • rock outcrops and crossbedding (suggests sand dunes)

  • “stream drainage” patterns

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jupiter

  • 5th planet

  • largest planet

  • banded appearance generated by wind

  • great red spot

    • southern hemis

    • counterclockwise rotating - cyclonic storm

  • 28 moons

    • 4 largest are lo, eurpa, ganymede, callisto

    • discovered by galileo

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saturn

  • 6th planet

  • bands of clouds and storms like jupiter

  • intense lightening

  • 93% hydrogen and 3% helium by volume

  • rings

    • small particles of water ice and rocky debris that orbit planet (moonlets)

    • debris possibly ejected from moons

    • discovered by galileo in 1610

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uranus

  • 7th planet

  • twins with neptune

  • rotates on its side

  • rings

  • large moons w/ varied terrains

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neptune

  • 8th planet

  • dynamic atmosphere

  • one of windiest places in solar system

  • greak dark spot

  • white, cirrus-like clouds above main cloud deck

  • triton is largest stellite and has ice lavas

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asteroids

  • leftover plantesimals from formation of solar system

  • most like between mars and jupiter in asteroid belt

  • small bodies - largest (ceres) is 620 miles in diameter

  • some have eccentric orbits

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comets

  • large dirty snowballs

  • made of frozen gases and rocky and metallic materials

  • frozen gases vaorize when near sun

    • produces glowing head caled coma

    • some develop tail that points away from sun bc radiation pressure and solar wind

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meteoroids

meteors but in space

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meteors

  • meteoroids when they enter earth’s atmospher

  • shower occurs when earth encounters sawm of meteoroids associated w/ a comet’s path

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meteorites

  • when found on earth

  • classified by composition

    • stony-irons - mixtures

    • carbonaceous chondrites

      • rare and made of simple amino acids and other organic material

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dwarf planets

  • includes pluto

  • not the only objects occupy their area of space

  • in kuiper belt - brand of icy objects found beyond orbit of neptune

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pluto

  • not naturally visible

  • discovered in 1930

  • dwarf planet

  • moon (charon) discovered in 1978

  • -210C