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Standards that all students are expected to achieve in the
course of their studies are unmarked. Standards that all students
should have the opportunity to learn are marked with an asterisk
(*).
Earth's Place in the Universe
- Astronomy and planetary exploration reveal the solar system's
structure, scale, and change over time. As a basis for
understanding this concept:
- Students know how the differences and similarities
among the sun, the terrestrial planets, and the gas planets may
have been established during the formation of the solar system.
- Students know the evidence from Earth and moon
rocks indicates that the solar system was formed from a nebular
cloud of dust and gas approximately 4.6 billion years ago.
- Students know the evidence from geological studies
of Earth and other planets suggest that the early Earth was very
different from Earth today.
- Students know the evidence indicating that the
planets are much closer to Earth than the stars are.
- Students know the Sun is a typical star and is
powered by nuclear reactions, primarily the fusion of hydrogen
to form helium.
- Students know the evidence for the dramatic effects
that asteroid impacts have had in shaping the surface of planets
and their moons and in mass extinctions of life on Earth.
- * Students know the evidence for the existence of
planets orbiting other stars.
- Earth-based and space-based astronomy reveal the structure,
scale, and changes in stars, galaxies, and the universe over time.
As a basis for understanding this concept:
- Students know the solar system is located in an
outer edge of the disc-shaped Milky Way galaxy, which spans
100,000 light years.
- Students know galaxies are made of billions of
stars and comprise most of the visible mass of the universe.
- Students know the evidence indicating that all
elements with an atomic number greater than that of lithium have
been formed by nuclear fusion in stars.
- Students know that stars differ in their life
cycles and that visual, radio, and X-ray telescopes may be used
to collect data that reveal those differences.
- * Students know accelerators boost subatomic
particles to energy levels that simulate conditions in the stars
and in the early history of the universe before stars formed.
- * Students know the evidence indicating that the
color, brightness, and evolution of a star are determined by a
balance between gravitational collapse and nuclear fusion.
- * Students know how the red-shift from distant
galaxies and the cosmic background radiation provide evidence
for the "big bang" model that suggests that the universe has
been expanding for 10 to 20 billion years.
Dynamic Earth Processes
- Plate tectonics operating over geologic time has changed the
patterns of land, sea, and mountains on Earth's surface. As the
basis for understanding this concept:
- Students know features of the ocean floor (magnetic
patterns, age, and sea-floor topography) provide evidence of
plate tectonics.
- Students know the principal structures that form at
the three different kinds of plate boundaries.
- Students know how to explain the properties of
rocks based on the physical and chemical conditions in which
they formed, including plate tectonic processes.
- Students know why and how earthquakes occur and the
scales used to measure their intensity and magnitude.
- Students know there are two kinds of volcanoes: one
kind with violent eruptions producing steep slopes and the other
kind with voluminous lava flows producing gentle slopes.
- * Students know the explanation for the location
and properties of volcanoes that are due to hot spots and the
explanation for those that are due to subduction.
Energy in the Earth System
- Energy enters the Earth system primarily as solar radiation
and eventually escapes as heat. As a basis for understanding this
concept:
- Students know the relative amount of incoming solar
energy compared with Earth's internal energy and the energy used
by society.
- Students know the fate of incoming solar radiation
in terms of reflection, absorption, and photosynthesis.
- Students know the different atmospheric gases that
absorb the Earth's thermal radiation and the mechanism and
significance of the greenhouse effect.
- * Students know the differing greenhouse conditions
on Earth, Mars, and Venus; the origins of those conditions; and
the climatic consequences of each.
- Heating of Earth's surface and atmosphere by the sun drives
convection within the atmosphere and oceans, producing winds and
ocean currents. As a basis for understanding this concept:
- Students know how differential heating of Earth
results in circulation patterns in the atmosphere and oceans
that globally distribute the heat.
- Students know the relationship between the rotation
of Earth and the circular motions of ocean currents and air in
pressure centers.
- Students know the origin and effects of temperature
inversions.
- Students know properties of ocean water, such as
temperature and salinity, can be used to explain the layered
structure of the oceans, the generation of horizontal and
vertical ocean currents, and the geographic distribution of
marine organisms.
- Students know rain forests and deserts on Earth are
distributed in bands at specific latitudes.
- * Students know the interaction of wind patterns,
ocean currents, and mountain ranges results in the global
pattern of latitudinal bands of rain forests and deserts.
- * Students know features of the ENSO (El Niņo
southern oscillation) cycle in terms of sea-surface and air
temperature variations across the Pacific and some climatic
results of this cycle.
- Climate is the long-term average of a region's weather and
depends on many factors. As a basis for understanding this
concept:
- Students know weather (in the short run) and
climate (in the long run) involve the transfer of energy into
and out of the atmosphere.
- Students know the effects on climate of latitude,
elevation, topography, and proximity to large bodies of water
and cold or warm ocean currents.
- Students know how Earth's climate has changed over
time, corresponding to changes in Earth's geography, atmospheric
composition, and other factors, such as solar radiation and
plate movement.
- * Students know how computer models are used to
predict the effects of the increase in greenhouse gases on
climate for the planet as a whole and for specific regions.
Biogeochemical Cycles
- Each element on Earth moves among reservoirs, which exist in
the solid earth, in oceans, in the atmosphere, and within and
among organisms as part of biogeochemical cycles. As a basis for
understanding this concept
- Students know the carbon cycle of photosynthesis and
respiration and the nitrogen cycle.
- Students know the global carbon cycle: the different
physical and chemical forms of carbon in the atmosphere, oceans,
biomass, fossil fuels, and the movement of carbon among these
reservoirs.
- Students know the movement of matter among reservoirs is
driven by Earth's internal and external sources of energy.
- * Students know the relative residence times and flow
characteristics of carbon in and out of its different
reservoirs.
Structure and Composition of the Atmosphere
- Life has changed Earth's atmosphere, and changes in the
atmosphere affect conditions for life. As a basis for
understanding this concept:
- Students know the thermal structure and chemical composition
of the atmosphere.
- Students know how the composition of Earth's atmosphere has
evolved over geologic time and know the effect of outgassing,
the variations of carbon dioxide concentration, and the origin
of atmospheric oxygen.
- Students know the location of the ozone layer in the upper
atmosphere, its role in absorbing ultraviolet radiation, and the
way in which this layer varies both naturally and in response to
human activities.
California Geology
- The geology of California underlies the state's wealth of
natural resources as well as its natural hazards. As a basis for
understanding this concept:
- Students know the resources of major economic importance in
California and their relation to California's geology.
- Students know the principal natural hazards in different
California regions and the geologic basis of those hazards.
- Students know the importance of water to society, the
origins of California 's fresh water, and the relationship
between supply and need.
- * Students know how to analyze published geologic hazard
maps of California and know how to use the map's information to
identify evidence of geologic events of the past and predict
geologic changes in the future.
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