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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
terrestrial / earth like planets
mercury, venus, earth, mars
small, dense, rocky
large cores of iron and nickel
low escape velocities
jovial / jupiter like planets
jupiter, saturn, uranus, neptune
large, low, gaseous
thick atmosphers of hydrogen, helium, methane, ammonia
high escape velocities
impact craters
collisions with massive objects
common in early formation of solar system
have central peak and ejecta lands in or near center
maria - lunar surface
dark regions
smooth lowlands
originated from asteroid impacts and basaltic lava flooding surface
highlands - lunar surface
bring, densely cratered regions
make up back side of moon
older than maria
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
mercury
1st planet from sun
no atmosphere
cratered highlands
vast and smooth
dense
revolves quick, rotates slow
low escape velocity
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
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
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
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
uranus
7th planet
twins with neptune
rotates on its side
rings
large moons w/ varied terrains
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
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
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
meteoroids
meteors but in space
meteors
meteoroids when they enter earth’s atmospher
shower occurs when earth encounters sawm of meteoroids associated w/ a comet’s path
meteorites
when found on earth
classified by composition
stony-irons - mixtures
carbonaceous chondrites
rare and made of simple amino acids and other organic material
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
pluto
not naturally visible
discovered in 1930
dwarf planet
moon (charon) discovered in 1978
-210C