Collection of labs in Earth Science including topics such as mapping, rocks and minerals, weathering, earthquakes, plate tectonics, meteorology, earth's history and astronomy.


  • Science > General

Education Levels:

  • Grade 6
  • Grade 7
  • Grade 8
  • Grade 9
  • Grade 10


collections Labs Earth Science mapping rocks minerals weathering earthquakes plate tectonics meteorology earth's history astronomy



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Creative Commons Attribution 3.0


Update Standards?

SCI.9-12.E.1.1.1: Science

use eccentricity, rate, gradient, standard error of measurement, and density in context

SCI.9-12.E.1.2.1: Science

determine the relationships among: velocity, slope, sediment size, channel shape, and volume of a stream

SCI.9-12.E.1.2.2: Science

understand the relationships among: the planets' distance from the Sun, gravitational force, period of revolution, and speed of revolution

SCI.9-12.E.1.3.1: Science

in a field, use isolines to determine a source of pollution

SCI.9-12.E.1.1.1: Science

show how our observation of celestial motions supports the idea of stars moving around a stationary Earth (the geocentric model), but further investigation has led scientists to understand that most of these changes are a result of Earth's motion around the Sun (the heliocentric model)

SCI.9-12.E.1.2.1: Science

test sediment properties and the rate of deposition

SCI.9-12.E.1.3.1: Science

determine the changing length of a shadow based on the motion of the Sun

SCI.9-12.E.1.1.1: Science

after experimenting with conduction of heat (using calorimeters and aluminum bars), make recommendations to create a more efficient system of heat transfer

SCI.9-12.E.1.1.2: Science

determine patterns of topography and drainage around your school and design solutions to effectively deal with runoff

SCI.9-12.E.2.1.1: Science

analyze weather maps to predict future weather events

SCI.9-12.E.2.1.2: Science

use library or electronic references to obtain information to support a laboratory conclusion

SCI.9-12.E.2.2.1: Science

obtain printed or electronic materials which exemplify miscommunication and/or misconceptions of current commonly accepted scientific knowledge

SCI.9-12.E.2.3.1: Science

discuss how early warning systems can protect society and the environment from natural disasters such as hurricanes, tornadoes, earthquakes, tsunamis, floods, and volcanoes

SCI.9-12.E.6.1.1: Science

analyze a depositional-erosional system of a stream

SCI.9-12.E.6.2.1: Science

draw a simple contour map of a model landform

SCI.9-12.E.6.2.2: Science

design a 3-D landscape model from a contour map

SCI.9-12.E.6.2.3: Science

construct and interpret a profile based on an isoline map

SCI.9-12.E.6.2.4: Science

use flowcharts to identify rocks and minerals

SCI.9-12.E.6.5.1: Science

graph and interpret the nature of cyclic change such as sunspots, tides, and atmospheric carbon dioxide

SCI.9-12.E.6.5.2: Science

based on present data of plate movement, determine past and future positions of land masses

SCI.9-12.E.6.5.3: Science

using given weather data, identify the interface between air masses, such as cold fronts, warm fronts, and stationary fronts

SCI.9-12.E.7.2.1: Science

collect, collate, and process data concerning potential natural disasters (tornadoes, thunderstorms, blizzards, earthquakes, tsunamis, floods, volcanic eruptions, asteroid impacts, etc.) in an area and develop an emergency action plan

SCI.9-12.E.7.2.2: Science

using a topographic map, determine the safest and most efficient route for rescue purposes

SCI.9-12.E.4.1.1.a.1: Science

These motions explain such phenomena as the day, the year, seasons, phases of the moon, eclipses, and tides.

SCI.9-12.E.4.1.1.a.2: Science

Gravity influences the motions of celestial objects. The force of gravity between two objects in the universe depends on their masses and the distance between them.

SCI.9-12.E.4.1.1.b.1: Science

The orbit of each planet is an ellipse with the Sun located at one of the foci.

SCI.9-12.E.4.1.1.b.2: Science

Earth is orbited by one moon and many artificial satellites.

SCI.9-12.E.4.1.1.c: Science

Earth's coordinate system of latitude and longitude, with the equator and prime meridian as reference lines, is based upon Earth's rotation and our observation of the Sun and stars.

SCI.9-12.E.4.1.1.d: Science

Earth rotates on an imaginary axis at a rate of 15 degrees per hour. To people on Earth, this turning of the planet makes it seem as though the Sun, the moon, and the stars are moving around Earth once a day. Rotation provides a basis for our system of local time; meridians of longitude are the basis for time zones.

SCI.9-12.E.4.1.1.e: Science

The Foucault pendulum and the Coriolis effect provide evidence of Earth's rotation.

SCI.9-12.E.4.1.1.f.1: Science

Earth revolves around the Sun with its rotational axis tilted at 23.5 degrees to a line perpendicular to the plane of its orbit, with the North Pole aligned with Polaris.

SCI.9-12.E.4.1.1.f.2: Science

During Earth's one-year period of revolution, the tilt of its axis results in changes in the angle of incidence of the Sun's rays at a given latitude; these changes cause variation in the heating of the surface. This produces seasonal variation in weather.

SCI.9-12.E.4.1.1.g: Science

Seasonal changes in the apparent positions of constellations provide evidence of Earth's revolution.

SCI.9-12.E.4.1.1.h: Science

The Sun's apparent path through the sky varies with latitude and season.

SCI.9-12.E.4.1.1.i: Science

Approximately 70 percent of Earth's surface is covered by a relatively thin layer of water, which responds to the gravitational attraction of the moon and the Sun with a daily cycle of high and low tides.

SCI.9-12.E.4.1.2.a.1: Science

cosmic background radiation

SCI.9-12.E.4.1.2.a.2: Science

a red-shift (the Doppler effect) in the light from very distant galaxies.

SCI.9-12.E.4.1.2.b.1: Science

The stars differ from each other in size, temperature, and age.

SCI.9-12.E.4.1.2.b.2: Science

Our Sun is a medium-sized star within a spiral galaxy of stars known as the Milky Way. Our galaxy contains billions of stars, and the universe contains billions of such galaxies.

SCI.9-12.E.4.1.2.c.1: Science

The characteristics of the planets of the solar system are affected by each planet's location in relationship to the Sun.

SCI.9-12.E.4.1.2.c.2: Science

The terrestrial planets are small, rocky, and dense. The Jovian planets are large, gaseous, and of low density.

SCI.9-12.E.4.1.2.d.1: Science

Impact events have been correlated with mass extinction and global climatic change.

SCI.9-12.E.4.1.2.d.2: Science

Impact craters can be identified in Earth's crust.

SCI.9-12.E.4.1.2.e: Science

Earth's early atmosphere formed as a result of the outgassing of water vapor, carbon dioxide, nitrogen, and lesser amounts of other gases from its interior.

SCI.9-12.E.4.1.2.f: Science

Earth's oceans formed as a result of precipitation over millions of years. The presence of an early ocean is indicated by sedimentary rocks of marine origin, dating back about four billion years.

SCI.9-12.E.4.1.2.g.1: Science

Water is returned from the atmosphere to Earth's surface by precipitation. Water returns to the atmosphere by evaporation or transpiration from plants. A portion of the precipitation becomes runoff over the land or infiltrates into the ground to become stored in the soil or groundwater below the water table. Soil capillarity influences these processes.

SCI.9-12.E.4.1.2.g.2: Science

The amount of precipitation that seeps into the ground or runs off is influenced by climate, slope of the land, soil, rock type, vegetation, land use, and degree of saturation.

SCI.9-12.E.4.1.2.g.3: Science

Porosity, permeability, and water retention affect runoff and infiltration.

SCI.9-12.E.4.1.2.h: Science

The evolution of life caused dramatic changes in the composition of Earth's atmosphere. Free oxygen did not form in the atmosphere until oxygen-producing organisms evolved.

SCI.9-12.E.4.1.2.i.1: Science

Fossil evidence indicates that a wide variety of life-forms has existed in the past and that most of these forms have become extinct.

SCI.9-12.E.4.1.2.i.2: Science

Human existence has been very brief compared to the expanse of geologic time.

SCI.9-12.E.4.1.2.j.1: Science

The characteristics of rocks indicate the processes by which they formed and the environments in which these processes took place.

SCI.9-12.E.4.1.2.j.2: Science

Fossils preserved in rocks provide information about past environmental conditions.

SCI.9-12.E.4.1.2.j.3: Science

Geologists have divided Earth history into time units based upon the fossil record.

SCI.9-12.E.4.1.2.j.4: Science

Age relationships among bodies of rocks can be determined using principles of original horizontality, superposition, inclusions, cross-cutting relationships, contact metamorphism, and unconformities. The presence of volcanic ash layers, index fossils, and meteoritic debris can provide additional information.

SCI.9-12.E.4.1.2.j.5: Science

The regular rate of nuclear decay (half-life time period) of radioactive isotopes allows geologists to determine the absolute age of materials found in some rocks.

SCI.9-12.E.4.2.1.a: Science

Earth systems have internal and external sources of energy, both of which create heat.

SCI.9-12.E.4.2.1.b: Science

The transfer of heat energy within the atmosphere, the hydrosphere, and Earth's interior results in the formation of regions of different densities. These density differences result in motion.

SCI.9-12.E.4.2.1.c: Science

Weather patterns become evident when weather variables are observed, measured, and recorded. These variables include air temperature, air pressure, moisture (relative humidity and dewpoint), precipitation (rain, snow, hail, sleet, etc.), wind speed and direction, and cloud cover.

SCI.9-12.E.4.2.1.d: Science

Weather variables are measured using instruments such as thermometers, barometers, psychrometers, precipitation gauges, anemometers, and wind vanes.

SCI.9-12.E.4.2.1.e.1: Science

temperature and humidity affect air pressure and probability of precipitation

SCI.9-12.E.4.2.1.e.2: Science

air pressure gradient controls wind velocity

SCI.9-12.E.4.2.1.f: Science

Air temperature, dewpoint, cloud formation, and precipitation are affected by the expansion and contraction of air due to vertical atmospheric movement.

SCI.9-12.E.4.2.1.g: Science

Weather variables can be represented in a variety of formats including radar and satellite images, weather maps (including station models, isobars, and fronts), atmospheric cross-sections, and computer models.

SCI.9-12.E.4.2.1.h: Science

Atmospheric moisture, temperature and pressure distributions; jet streams, wind; air masses and frontal boundaries; and the movement of cyclonic systems and associated tornadoes, thunderstorms, and hurricanes occur in observable patterns. Loss of property, personal injury, and loss of life can be reduced by effective emergency preparedness.

SCI.9-12.E.4.2.1.i: Science

Seasonal changes can be explained using concepts of density and heat energy. These changes include the shifting of global temperature zones, the shifting of planetary wind and ocean current patterns, the occurrence of monsoons, hurricanes, flooding, and severe weather.

SCI.9-12.E.4.2.1.j.1: Science

Analysis of seismic waves allows the determination of the location of earthquake epicenters, and the measurement of earthquake magnitude; this analysis leads to the inference that Earth's interior is composed of layers that differ in composition and states of matter.

SCI.9-12.E.4.2.1.k: Science

The outward transfer of Earth's internal heat drives convective circulation in the mantle that moves the lithospheric plates comprising Earth's surface.

SCI.9-12.E.4.2.1.l.1: Science

These plate boundaries are the sites of most earthquakes, volcanoes, and young mountain ranges.

SCI.9-12.E.4.2.1.l.2: Science

Compared to continental crust, ocean crust is thinner and denser. New ocean crust continues to form at mid-ocean ridges.

SCI.9-12.E.4.2.1.l.3: Science

Earthquakes and volcanoes present geologic hazards to humans. Loss of property, personal injury, and loss of life can be reduced by effective emergency preparedness.

SCI.9-12.E.4.2.1.m: Science

Many processes of the rock cycle are consequences of plate dynamics. These include the production of magma (and subsequent igneous rock formation and contact metamorphism) at both subduction and rifting regions, regional metamorphism within subduction zones, and the creation of major depositional basins through down-warping of the crust.

SCI.9-12.E.4.2.1.n: Science

Many of Earth's surface features such as mid-ocean ridges/rifts, trenches/subduction zones/island arcs, mountain ranges (folded, faulted, and volcanic), hot spots, and the magnetic and age patterns in surface bedrock are a consequence of forces associated with plate motion and interaction.

SCI.9-12.E.4.2.1.o: Science

Plate motions have resulted in global changes in geography, climate, and the patterns of organic evolution.

SCI.9-12.E.4.2.1.p: Science

Landforms are the result of the interaction of tectonic forces and the processes of weathering, erosion, and deposition.

SCI.9-12.E.4.2.1.q: Science

Topographic maps represent landforms through the use of contour lines that are isolines connecting points of equal elevation. Gradients and profiles can be determined from changes in elevation over a given distance.

SCI.9-12.E.4.2.1.r: Science

Climate variations, structure, and characteristics of bedrock influence the development of landscape features including mountains, plateaus, plains, valleys, ridges, escarpments, and stream drainage patterns.

SCI.9-12.E.4.2.1.s: Science

Weathering is the physical and chemical breakdown of rocks at or near Earth's surface. Soils are the result of weathering and biological activity over long periods of time.

SCI.9-12.E.4.2.1.t: Science

Natural agents of erosion, generally driven by gravity, remove, transport, and deposit weathered rock particles. Each agent of erosion produces distinctive changes in the material that it transports and creates characteristic surface features and landscapes. In certain erosional situations, loss of property, personal injury, and loss of life can be reduced by effective emergency preparedness.

SCI.9-12.E.4.2.1.u.1: Science

Streams (running water): Gradient, discharge, and channel shape influence a stream's velocity and the erosion and deposition of sediments. Sediments transported by streams tend to become rounded as a result of abrasion. Stream features include V-shaped valleys, deltas, flood plains, and meanders. A watershed is the area drained by a stream and its tributaries.

SCI.9-12.E.4.2.1.u.2: Science

Glaciers (moving ice): Glacial erosional processes include the formation of U-shaped valleys, parallel scratches, and grooves in bedrock. Glacial features include moraines, drumlins, kettle lakes, finger lakes, and outwash plains.

SCI.9-12.E.4.2.1.u.3: Science

Wave Action: Erosion and deposition cause changes in shoreline features, including beaches, sandbars, and barrier islands. Wave action rounds sediments as a result of abrasion. Waves approaching a shoreline move sand parallel to the shore within the zone of breaking waves.

SCI.9-12.E.4.2.1.u.4: Science

Wind: Erosion of sediments by wind is most common in arid climates and along shorelines. Wind-generated features include dunes and sand-blasted bedrock.

SCI.9-12.E.4.2.1.u.5: Science

Mass Movement: Earth materials move downslope under the influence of gravity.

SCI.9-12.E.4.2.1.v: Science

Patterns of deposition result from a loss of energy within the transporting system and are influenced by the size, shape, and density of the transported particles. Sediment deposits may be sorted or unsorted.

SCI.9-12.E.4.2.1.w: Science

Sediments of inorganic and organic origin often accumulate in depositional environments. Sedimentary rocks form when sediments are compacted and/or cemented after burial or as the result of chemical precipitation from seawater.

SCI.9-12.E.4.2.2.a.1: Science

the intensity caused by differences in atmospheric transparency and angle of incidence which vary with time of day, latitude, and season

SCI.9-12.E.4.2.2.a.2: Science

characteristics of the materials absorbing the energy such as color, texture, transparency, state of matter, and specific heat

SCI.9-12.E.4.2.2.a.3: Science

duration, which varies with seasons and latitude.

SCI.9-12.E.4.2.2.b.1: Science

Heating of Earth's surface and atmosphere by the Sun drives convection within the atmosphere and oceans, producing winds and ocean currents.

SCI.9-12.E.4.2.2.c: Science

A location's climate is influenced by latitude, proximity to large bodies of water, ocean currents, prevailing winds, vegetative cover, elevation, and mountain ranges.

SCI.9-12.E.4.2.2.d.1: Science

natural events such as El Nino and volcanic eruptions

SCI.9-12.E.4.2.2.d.2: Science

human influences including deforestation, urbanization, and the production of greenhouse gases such as carbon dioxide and methane.
Curriki Rating
On a scale of 0 to 3
On a scale of 0 to 3

This resource was reviewed using the Curriki Review rubric and received an overall Curriki Review System rating of 2.4, as of 2016-08-02.

Component Ratings:

Standards Alignment: 3
Subject Matter: 3
Support Steaching: 2
Assessments Quality: 2
Deeper Learning: 2

Reviewer Comments:

Support Steaching: Some activities and lesson plans need more detail for instructional implementation.

Not Rated Yet.

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