Develop and use a model to show how unequal heating of the Earth's systems causes patterns of atmospheric and oceanic circulation that determine regional climates. Emphasize how warm water and air move from the equator toward the poles.
In this unit, students analyze the phenomenon of our sun as the primary source of energy on Earth. In this lesson, students explore how the sun’s uneven heating of the planet drives weather phenomena and climate phenomena, which result from complex interactions within Earth’s systems. This page is an extract from parts of this lesson.
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In this unit, students focus on the phenomena of Earth’s ice as they model how glaciers shape Earth’s surface. In this lesson, they investigate how scientists use ice cores to reconstruct Earth’s past climates and environments. This page is a high-level extract of this lesson.
In this unit, students explore the science phenomena of matter, energy, and heat transfer to explore weather and climate. In this lesson they investigate how the sun powers the global water cycle, which in turn has very local impacts that affect regional climates around the world. This page is a high-level extract of this lesson.
In this unit, students investigate the relationship between the water cycle, ocean salinity, weather, and climate. In this lesson, students explore ocean salinity and analyze how ocean density is related to its molecular structure. This page highlights key components of this lesson.
In this unit, students build on their scientific knowledge about matter, energy, and heat transfer to explore science phenomena related to weather and climate. They investigate how the sun powers the global water cycle, which in turn has very local impacts that affect the phenomena of regional climates around the world. This page showcases all the parts of this lesson.
