Earth and Space Science
| Energy
in the Earth System: Students will recognize
that earth systems have sources of energy that influence
crustal plate movements and climate. |
Academic Expectations: 2.2 Patterns
of Change, 2.3 Systems, 2.4 Scale and Models, 2.5 Constancy,
and 2.6 Change Over Time |
Core Content
|
Sample Demonstrators, Skills, Activities
|
| SC-H-2.1.1
Earth systems have sources of energy that are internal and
external to the Earth. The Sun is the major external
source of energy. Two primary sources of internal energy
are the decay of radioactive isotopes and the gravitational
energy from Earth’s original formation. |
- Describe the energy sources that cause the motion of the
earth’s crust, ocean currents, and weather systems.
- Design an investigation to analyze the relationships
among the variables that affect various motions within
earth systems.
- Discuss the effects on earth systems when variables that
affect energy transfers are changed.
- Predict the effects on the earth when one or more energy
sources change or disappear.
|
| SC-H-2.1.2
The outward transfer of Earth’s internal heat drives
convection circulation in the mantle. This causes the
crustal plates to move on the face of the Earth. |
- Analyze the evidence to support the existence of a
single large continent early in the earth’s history.
- Evaluate the relationship among various properties of
geological plates and how the properties affect the
existence and behavior of the plates.
- Evaluate how the properties of crustal plates affect
their behavior.
- Analyze the behaviors of crustal plates and how they
affect natural and social systems.
|
| SC-H-2.1.3
Heating of Earth’s surface and atmosphere by the Sun
drives convection within the atmosphere and oceans, producing
winds and ocean currents. |
- Compare and contrast convection, conduction, and
radiation and how they affect global climatic patterns.
- Analyze how the transfer of energy on the Earth’s
surface affects global systems.
- Evaluate the affects on global systems of changes in
position of the earth relative to the sun.
- List the factors that influence energy transfers at or
near the earth’s surface.
|
| SC-H-2.1.4
Global climate is determined by energy transfer from the
Sun at and near Earth’s surface. Dynamic processes such as
cloud cover and the Earth’s rotation and static conditions
such as the position of mountain ranges and oceans influence
this energy transfer. |
- Describe the relationship between latitude and average
temperature; explain the mechanism behind this trend.
- Explain why weather systems rotate in the opposite
direction in each hemisphere.
- Explain why windward slopes often have more
precipitation than leeward slopes.
- Account for the more moderate temperatures in England
than at similar latitudes in Asia.
|
| Content Area: Earth
and Space Science |
Level: High School |
| Subtopic:
Energy in the Earth System; Students will recognize that Earth
systems have sources of energy that influence crustal plate
movements and climate. |
| Core
Content: SC-H-2.1.1, SC-H-2.1.2 |
New crustal material is forming at the mid-Atlantic
ridge causing the Atlantic Ocean to widen.
- Discuss the effect of this Atlantic widening on other crustal
plates.
- Describe the energy source that drives these plate movements.
Open Response 2.1 Scoring Guide
| Score |
Description |
| 4 |
- Student points out that spreading of the Atlantic
seafloor will increase pressure on plate boundaries
elsewhere in the world. This can cause continental
crust to buckle, forming mountain ranges. Oceanic
crust will subduct and melt, causing volcanic activity and
the formation of islands. The appearance of new
crustal material on the seafloor leads to the destruction
of crustal material elsewhere.
- ·
Student discusses convection currents driven by heat in
the Earth’s core. Material wells up from the
mantle to the crust, moves across the surface and
ultimately subducts back into the mantle. This
convection process is part of the natural cooling of the
planet. The heat in the Earth’s core comes from
gravitational pressure and radioactive decay.
|
| 3 |
- Student explains the main idea detailed above.
- Student exhibits understanding of plate tectonics and
convection currents.
|
| 2 |
- Student correctly responds to one of the two bullets.
-OR-
- Student provides a partially correct response on both
bullets.
- Student exhibits some confusion regarding plate
tectonics and convection currents.
|
| 1 |
- Student response contains serious errors or
misconceptions.
- Student exhibits limited or no understanding of plate
tectonics and convection currents.
|
| 0 |
- No response or response is totally incorrect or
irrelevant.
|
Earth and Space Science
| Geochemical
Cycles: Students will recognize the Earth is a
stable system in which elements move through the system using
the Earth’s internal and external sources of energy.
Academic Expectations: 2.2 Patterns
of Change, 2.3 Systems, 2.4 Scale and Models, 2.5 Constancy,
and 2.6 Change Over Time |
Core Content
|
Sample Demonstrators, Skills, Activities
|
| SC-H-2.2.1
Earth is a system containing essentially a fixed amount of
each stable chemical atom or element. Each element can
exist in several different reservoirs. Each element on
Earth moves among reservoirs in the solid Earth, oceans,
atmosphere, and organisms as part of geochemical cycles. |
- List several different places where the same element can
be found on Earth.
- Explain how conservation of matter applies to closed
cycles in Earth systems. Examples may include
carbon, nitrogen, water, and phosphorus cycles.
|
| SC-H-2.2.2
Movement of matter between reservoirs is driven by Earth’s
internal and external sources of energy. These movements
are often accompanied by a change in physical and chemical
properties of the matter. Carbon, for example, occurs in
carbonate rocks such as limestone, in the atmosphere as carbon
dioxide gas, in water as dissolved carbon dioxide, and in all
organisms as complex molecules that control the chemistry of
life. |
- Explain how solar and geothermal energy sources drive
cycles in Earth systems.
- Examples may include carbon, nitrogen, water, and
phosphorus cycles.
|
Open Response 2.2
| Content Area: Earth
and Space Science |
Level: High School |
| Subtopic:
Geochemical Cycles; Students will recognize the Earth is a
stable system in which elements move through the system using
the Earth’s internal and external sources of energy. |
| Core
Content: SC-H-2.2.1, SC-H-2.2.2 |
The hydrologic cycle describes how water moves
between the atmosphere, surface and ground water, polar ice caps,
the oceans, and even through organisms.
- Briefly describe the how water moves between these different
locations. Include the energy source responsible for the
transport.
- Given that water is conserved, discuss the implications of
melting a significant portion of the polar ice caps.
Open Response 2.2 Scoring Guide
| Score |
Description |
| 4 |
- Student describes the principle ways in which water
moves from place to place and the energy source
responsible. These include:
- evaporation caused by solar heating
- precipitation caused by air cooling and water
condensing
- downhill flow and groundwater seepage caused by the
force of gravity
- snow compressing into ice caused by the weight of
snow above it
- transpiration and respiration by living organisms
- Students should point out the energy source behind the
entire cycle is ultimately the sun.
- Student describes several implications of melting polar
ice caps. These include:
- rising ocean levels and decreased salinity
- increased river flow and accompanying erosion
- formation of large lakes such as the Great Lakes
- formation of large reservoirs of ground water like
those found in the midwest
|
| 3 |
- Student explains the basic components of the hydrologic
cycle and recognizes the sun as the ultimate energy
source.
- Student also correctly describes several implications of
polar melting.
|
| 2 |
- Student correctly responds to one of the two bullets.
-OR-
- Student provides a partially correct response on both
bullets.
- Student exhibits some confusion regarding the hydrologic
cycle.
|
| 1 |
- Student response contains serious errors or
misconceptions.
- Student exhibits limited or no understanding of
the hydrologic cycle.
|
| 0 |
- No response or response is totally incorrect or
irrelevant.
|
Earth and Space Science
| The
Formation and Ongoing Changes of the Earth System:
Students will understand the timeline involved with the
formation of the solar system and the methods used to measure
geologic time. |
| Academic
Expectations: 2.2 Patterns of Change, 2.3
Systems, 2.4 Scale and Models, 2.5 Constancy, and 2.6 Change
Over Time |
Core Content
|
Sample Demonstrators, Skills, Activities
|
| SC-H-2.3.1
The Sun, Earth, and the rest of the solar system formed
approximately 4.6 billion years ago from a nebular cloud of
dust and gas. |
- Describe different theories, and list the evidence for
each theory, of how the solar system was formed.
- Identify critical factors that affect a particular
theory of how the solar system was formed.
|
| SC-H-2.3.2
Techniques used to estimate geological time include using
radioactive dating, observing rock sequences, and comparing
fossils to correlate the rock sequences at various locations. |
- Use various dating techniques to illustrate how living
and nonliving systems have changed over time.
- Use the fossil record to estimate geological time or
periods.
- Cite evidence to support the theory that geological
processes have remained constant over time.
- Analyze factors that would support theories concerning
changes resulting from a single, global, catastrophic
event.
- Formulate a conclusion from collected data that
demonstrates how a particular change could occur.
- Theorize how a break in a rock sequence could be used as
evidence for a catastrophic event.
|
| SC-H-2.3.3
Interactions among the solid Earth, the oceans, the
atmosphere, and living things have resulted in the ongoing
development of a changing Earth system. Earthquakes and
volcanic eruptions can be observed on a human time scale, but
many processes, such as mountain building and plate movements,
take place over hundreds of millions of years. |
- List obvious natural changes to the Earth’s surface
that have occurred during the last century.
- Account for the fact that rocks from Mt. Everest contain
fossils of extinct organisms.
|
| SC-H-2.3.4
Evidence for one-celled forms of life, the bacteria,
extends back more than 3.5 billion years. The changes in
life over time caused dramatic changes in the composition of
the Earth’s atmosphere, which did not originally contain
oxygen. |
- Present in graphical form the evidence for the existence
of one-celled forms of life.
- Describe the chemical and biological processes that
would contribute to the production of oxygen and other
gases in the Earth’s atmosphere.
|
Open Response 2.3
| Content Area: Earth
and Space Science |
Level: High School |
| Subtopic:
The Formation and Ongoing Changes of the Earth System;
Students will understand the timeline involved with the
formation of the solar system and the methods used to measure
geologic time. |
| Core
Content: SC-H-2.3.2 |

- Look at the above picture and place the following events in
order from oldest to youngest.
- final deposition of sandstone layer
- final deposition of limestone layer
- final deposition of siltstone layer
- earthquake along normal fault
- formation of granitic dike
- deposition of soil layer
- Explain how you came up with the above sequence.
Open Response 2.3 Scoring Guide
| Score |
Description |
| 4 |
- Student correctly identifies the sequence as follows:
- Final deposition of limestone layer
- Final deposition of siltston layer
- Earthquake along normal fault
- Final deposition of sandstone layer
- Formation of granitic dike
- Deposition of soil layer
- Student should apply the basic rules of relative dating
to determine the sequence. The layers should be laid
down chronologically with the oldest on the bottom, thus
the limestone formed before the siltstone, which preceeded
the sandstone with the soil forming last. The fact
that the earthquake moves the entire limestone and
siltstone layer indicates it occurred following their
formation. The sandstone layer had started forming
prior to the quake as it shows slippage but finished
forming after the quake as it levels out. (Note:
Student may correctly place sandstone layer before
earthquake in the sequence. If so, the student
should specify an erosion event that leveled the sandstone
layer after the quake.) The dike formed after the
quake because it has not been displaced along the
fault. Also, the dike spreads out when it reaches
the surface thus the sandstone layer had finished
forming. The formation of the soil layer is the
final event as it appears above the dike.
|
| 3 |
- Student correctly identifies the basic sequence and
provides reasonable explanation.
- One event may be out of order.
- Student exhibits understanding of relative dating
techniques.
|
| 2 |
- Student mixes the sequence or provides an incomplete
explanation.
- Student exhibits some confusion regarding relative
dating.
|
| 1 |
- Student mixes the sequence and provides little or no
correct explanation of reasoning.
- Student exhibits limited or no understanding of relative
dating.
|
| 0 |
- No response or response is totally incorrect or
irrelevant.
|
Science Behind the Question:
By looking at a cross section of rocks, an order of
events can be determined. Layers of rock are younger than ones
below them and older than ones above. Earthquakes are younger
than layers they move and older than ones they do not.
Earth and Space
Science
|
|
| Academic
Expectations: 2.2 Patterns of Change, 2.3
Systems, 2.4 Scale and Models, 2.5 Constancy, and 2.6 Change
Over Time |
Core Content
|
Sample
Demonstrators, Skills, Activities
|
| SC-H-2.4.1
The big bang theory and observational measurements that
support it place the origin of the universe at a time between
10 and 20 billion years ago, when the universe began in a hot
dense state. According to this theory, the universe has
been expanding since then. |
- Identify the evidence which supports the “Big Bang”
theory of the formation of the universe.
- Discuss various factors or evidence which may not
support the “Big Bang” theory.
- Describe different methods for determining the age of
the universe.
|
| SC-H-2.4.2
Early in the history of the universe, the first atoms to
form were mainly hydrogen and helium. Over time, these
elements clump together by gravitational attraction to form
trillions of stars. |
- Describe the forces that cause the elements present in
space to form a sun, galaxy, or nebula.
- Discuss the sequence of events within a star which
produce elements heavier than hydrogen and helium.
- Describe different methods for determining the elemental
make-up of stars.
|
| SC-H-2.4.3
Stars have life cycles of birth through death that are
analogous to those of living organisms. During their
lifetimes, stars generate energy from nuclear fusion reactions
that create successively heavier chemical elements. Some
stars explode at the end of their lives, and the heavy
elements they have created are blasted out into space to form
the next generation of stars and planets. |
- Use models to demonstrate how elements are created
during the process of fission and fusion.
- Demonstrate how energy can be “created” during the
process of fission and fusion.
- Analyze the loss of mass and the gain of energy which
occurs in a nuclear reaction.
|
Open Response 2.4
| Content Area: Earth
and Space Science |
Level: High School |
| Subtopic:
The Formation and Ongoing Changes of the Universe; Students
will understand current theories regarding the formation of
the universe, its time line, and the life cycle of stars. |
| Core
Content: SC-H-2.4.2, SC-H-2.4.3 |
The force of gravity tries to compress stars while
radiation pressure from nuclear fussion reactions tries to prevent
the compression.
- Describe how the gravitational pressure at the star’s core
leads to nuclear fussion reactions.
- Compare the reaction rates for low mass stars to those of high
mass stars. Explain the cause of this trend.
Open Response 2.4 Scoring Guide
| Score |
Description |
| 4 |
- Student correctly identifies the connection between
gravitational pressure and nuclear fusion reactions.
Student explains the connection with the following
sequence: gravitational pressure increases the temperature
in the star’s core, which leads to greater kinetic
energy for the protons, which leads to the protons getting
closer together before repelling each other during
collisions. As the pressure continues to rise, the
protons continue to get closer until they reach the point
where the strong and weak nuclear forces bind the protons
together in a nuclear fusion reaction. This releases
radiation that pushes out and energy which raises the
temperature. The star reaches stable equilibrium
where the gravitational pressure pushing in is balanced by
the radiation pressure pushing out.
- Student correctly identifies that high mass stars will
have greater reaction rates than low mass stars.
Student explains that high mass stars have a greater
gravitational pressure in the core. This requires a
higher radiation pressure for the star to maintain
equilibrium. Increasing the reaction rate can only
generate higher radiation pressure. Students may
also point out that high mass stars consume material
faster and thus are shorter lived than low mass stars.
|
| 3 |
- Student correctly identifies the basic sequence that
ties gravitational pressure to nuclear fussion reactions
and connection between mass and reaction rate.
- Student exhibits understanding of the relationship
between gravitational pressure and radiation pressure.
|
| 2 |
- Student correctly responds to one of the two bullets.
-OR-
- Student provides a partially correct response on both
bullets.
- Student has some confusion on the relationship between
gravitational pressure and radiation pressure.
|
| 1 |
- Student response contains serious errors or
misconceptions.
- Student exhibits limited or no understanding of the
relationship between gravitational pressure and radiation
pressure.
|
| 0 |
- No response or response is totally incorrect or
irrelevant.
|
Science Behind the Question:
Stars are dynamic. Gravitational forces continually
try to crush the the star. Temperatures and pressures at the
core of the star get so large that nuclear fussion takes place. This
releases radiation that holds the gravitational collapse at bay.
|