Earth Science Mid-term
Steady state theory
neither a beginning nor an end to the universe (matter is constantly destroyed and remade)
Contraction-expansion theory
someday, the universe will contract and expand again
light year
the distance light travels in one year
stars are made of -
hydrogen and helium
stars have a -
finite life span
the mass of a star controls its -
evolution
hydrogen -
burns first
helium -
burns last
parallex
used to measure the distance of stars from earth
hydrogen to helium -
fusion
helium to hydrogen -
fission
polaris -
North star
alpha centaur -
closest star to Earth
Nebula -
dust and gases
bright stars -
top
dim stars -
bottom
red shift
stars moving away
blue shift
stars moving towards
sun -
main sequence star; 70% hydrogen, 28% helium
apparent magnitude -
brightness from earth
Absolute magnitude -
brightness if all stars were the same distance
star nebula theory
the solar system condensed from a cloud of dust and gas
asteroid belt is located between -
Mars and Jupiter
Comets
tail always pointed away from the sun
Kuiper belt
beyond Neptune where comets originate
Meteoroid
small, solid particle
Meteor
streaks of light produced by a solid particle
Meteorite
a meteoroid that passes through earth's atmosphere and hits earth's surface
Inner planets -
Mercury, Venus, Earth and Mars
Outer planets -
Jupiter, Saturn, Uranus ans Neptune
Trophosphere -
layer closest to the ground; temperature drops with altitude; contains all weather
Stratosphere -
three layer oxygen atoms bonded together; protect earth from ultra violet radiation
Mesosphere -
temperature decreases with altitude; meteors burn up
Thermosphere -
largest and outermost layer; contains isosphere( bounces radio waves back to earth
Stage 1 of the atmosphere -
mostly hydrogen and helium; earth's surface was molten; no oxygen present
Stage 2 of the atmosphere -
formation of moon occurs; volcanoes result in carbon; oceans form, carbon dioxide leaves the atmosphere
Photosynthesis -
cynobacteria consumed carbon dioxide and released oxygen
Modern atmosphere -
1% trace gas; 21% oxygen; 78% nitrogen
Insolation -
the amount of solar radiation reaching a given area
ITCZ -
inter-tropical convergence zone; influenced by the sun's radiation; warm air rises
STHP -
sub-tropical high pressure belt; influences the distribution of deserts; cold air sinking
SPLP
sub-polar low pressure belt; warm air rises
PH -
polar high; high to low always
Wind flow -
forces that drive surface winds
Coriolis force -
the influence of the earth's rotation
cP
dry and cold
mP
moist and cold
mT
moist and warm
cT
dry and warm
warm front -
warm air; low pressure system; brings rain
cold front -
cold air sinking; high pressure system; good weather
stationary front -
slow moving
occluded front -
balance each other out ( warm and cold front)
dry line -
dry air
cyclone -
low pressure; tropical storm; counter clockwise; warm air rises
anti-cyclone -
high pressure; clear weather; clockwise; cooling air
sling psychrometer -
measures relative humidity
anemometer -
wind speed
ocean uses -
fresh water. petroleum, minerals, food
sea ice formation -
needle-like crystals become slush
iceberg formation -
icebergs break off of glaciers
shelf ice -
plate-like icebergs
wind power -
uneven solar heating generates winds
surface currents -
wind driven; primarily horizontal
deep currents -
differences in density caused by differences in temperature and salinity
Eutrophication -
fertilizer carried by run-off causes algae blooms; causes dead zones in oceans
sedimentation -
too much sediment stops sunlight from reaching plants; carried from land to water through storm drains
ocean acidification
excess carbon dioxide dissolved into ocean by waves; animals' shells are thinner
carbonates -
organisms that make their own carbonate shells; build-up of material such as limestone and dolomite
estuary -
a semi-enclosed area where fresh water and salt water mix
salinity -
higher salinity closer to oceans; lower salinity in rivers
higher salinity during droughts; lower salinity after rainfall
Tsunami -
waves generated by sudden movements of the seafloor
tides -
waves generated by the gravitational pull of the moon
wind driven waves -
created by the transfer of wind energy to the ocean surface
density driven waves -
located at the pycnocline (area in which water density increases at a rapid pace
geologic driven waves -
created by sudden movements of the seafloor; mostly occur in the Pacific ocean
tidal range -
the difference in height between high tides and low tides
sonar -
works by transmitting sound waves towards the ocean bottom
continental margin -
the zone of transition between ocean basin floor
continental shelf -
the gently sloping submerged surface extending from the shoreline
continental slope -
the steep gradient that leads to the deep ocean floor
turbidity current -
the downslope movement of dense, sediment-laden water
continental rise -
the gently sloping surface at the base of the continental slope
ocean basin floor -
the area of the deep ocean floor between the continental margin and the oceanic ridge
abyssal plain -
the very level area of the deep ocean floor
seamount -
an isolated volcanic peak that rises at least 1000 meters above the deep ocean floor
seafloor spreading -
the process by which plate tectonics produces at new oceanic ridges
hydrothermal vents -
form along mid-ocean ridges; where mineral rich water escapes through cracks in the oceanic crust
terrigenous sediments -
consist primarily of mineral grains that were eroded from continental rocks
biogenous sediments
consists of shells and skeleton marine animals
calcareous ooze
a thick, common biogenous sediment produced by dissolving calcium carbonate shells
siliceous ooze
biogenous sediment composed of silica-based shells of single-celled animals
hydrogenous sediment -
consists of minerals that crystallize directly from ocean water through various chemical reactions
gas hydrates -
compact chemical structures made of water and natural gas
manganese nodules -
hard lumps of manganese and other metals
thermocline -
the layer of ocean water between about 300 meters and 100 meters
relative humidity
is a ratio of the air's actual water-vapor content compared with the amount of water vapor
dew point -
the temperature to which a parcel of air would need to be cooled to reach saturation
cirrus -
clouds that are high, white, and thin
cumulus -
clouds that consist of rounded individual cloud masses
stratus -
clouds best described as sheets or layers that cover much or all of the sky
solar eclipse -
occur when the moon moves in a line directly between earth and the sun
lunar eclipse -
occur when the moon passes through the earth's shadow
red giant -
a large, cool star of high luminosity; occupies the upper right portion of the HR diagram
supergiant -
a very large, very bright red giant star
protostar -
a collapsing cloud of gas and dust destined to become a star
supernova -
an exploding massive star that increases in brightness many thousands of times
white dwarf -
a star that has exhausted most or all of its nuclear fuel and has collapsed
spiral galaxies -
about 30% of all galaxies; diameters of 20,000 to 125,000 light years
elliptical galaxies -
about 60% of galaxies; range in shape from round to oval