Collection of games 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 Games Earth Science mapping rocks minerals weathering earthquakes plate tectonics meteorology earth's history astronomy



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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.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.
Curriki Rating
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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: 2
Support Steaching: 2
Interactivity Quality: 3
Deeper Learning: 2

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