Lesson Info
- 30-45 minm
- 102
- 0
Lesson Resources
None AvailableAlignment Documents
None AvailableTechnical Details
Latest browser version supported
Chrome
FireFox
Device support
Android Phone / Tablet
iPad / iPhone
Mac
PC
Chromebook
Languages
English
Lesson Description
From the blue planet we live on to the rocky red planet of Mars and beyond to the gas and ice giants in the outer reaches of the Universe, the planets of our Solar System differ greatly in mass, size, and composition. In this lesson, you'll unlock the secrets of Solar System formation through simulations and real-world data.
Central Question
How did the Solar System form and what effect did it have on the formation of Earth and the other planets?
Instructional Objective
Explain how condensation temperatures of the elements influence the properties of the planets in our Solar System.
Topics
Learning Outcomes
- Determine the relationship between distance from the Sun and condensation temperature in the early Solar System
- Apply the relationship between distance from the Sun and condensation temperature to determine the composition of planets at a variety of distances from the Sun.
- Identify the location of the frost line and its relationship to planetary composition.
- Explain why giant planets could be found inside the frost line of a sample exoplanetary system.
Prerequisites
- Gravity
- Density
- Condensation
- Solar System Arrangement
Teach with This Lesson
There are three ways to teach with this lesson. Select the option that best fits the needs of you and your learners.
Do you want to
- open this lesson?
- preview this lesson?
- use this lesson with your learners?
Do you want to
- enroll your learners in the lesson?
- collect data on your learners?
- monitor your learners’ progress?
- integrate the lesson into your pre-existing online course?
Do you want to
- customize the lesson for your learners?
- enroll your learners in the customized version?
- share your customized version with the infiniscope Teaching Network?
