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Earth in the Solar System

  • Grade 6
  • Science
  • MS-ESS1
  • Earth & Space Science
  • Free lesson

Aligned to MS-ESS1 — Next Generation Science Standards.

What this lesson teaches

Gravity holds the solar system together, keeping planets orbiting the sun and moons orbiting planets. Earth's tilt and orbit cause seasons; the moon's orbit causes its phases.

Worked examples

Example 1

Earth orbits the sun once a year; because Earth is tilted, the hemisphere leaning toward the sun has summer while the other has winter.

Example 2

The Moon takes about 27 days to orbit Earth while Earth takes 365 to orbit the Sun — two separate clocks running at once.

Example 3

Seasons are not caused by distance. Earth is actually closest to the Sun in early January, during the northern winter; the tilt is what does it.

Practice questions

  1. What force keeps planets in orbit?
  2. Explain why we have seasons.
  3. Why does the moon appear to change shape over a month?

Watch the lesson

Every lesson comes with a video taught in English and Spanish — the same video the QR code in the printed workbook opens.

▶ Watch this lesson

En español

La Tierra en el Sistema Solar

La gravedad mantiene unido al Sistema Solar, haciendo que los planetas orbiten alrededor del sol y las lunas orbiten alrededor de los planetas. La inclinación y la órbita de la Tierra causan las estaciones del año; la órbita de la Luna causa sus fases.

Ejemplo 1: La Tierra orbita alrededor del sol una vez al año; debido a que la Tierra está inclinada, el hemisferio que se inclina hacia el sol tiene verano mientras el otro tiene invierno.

Ejemplo 2: La Luna tarda unos 27 días en orbitar la Tierra mientras la Tierra tarda 365 en orbitar el Sol — dos relojes distintos funcionando a la vez.

Ejemplo 3: Las estaciones no las causa la distancia. La Tierra está de hecho más cerca del Sol a principios de enero, durante el invierno del norte; lo que las causa es la inclinación.

More Earth & Space Science lessons

Why the Moon Has PhasesMS-ESS1-1The Solar System to ScaleMS-ESS1-3Reading Earth's History in Rock LayersMS-ESS1-4The Rock CycleMS-ESS2-1Weathering, Erosion, and DepositionMS-ESS2-2Plate Tectonics: Evidence the Continents MovedMS-ESS2-3

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