Use a model to predict how variations in the flow of energy through radiation, conduction, and convection into and out of Earth’s systems could contribute to global atmospheric processes and climatic effects.
Standard detail
ESS.ESS2.13
Depth 1Parent ID: 2F399A5C35CF433091C1AEEA54CD639DStandard set: Earth and Space Science
Original statement
Quick facts
- Statement code
- ESS.ESS2.13
- List ID
- 13
- Standard ID
- 18063E3083EB4CF6B031F18900B464CC
- Subject
- Science (2022-)
- Grades
- 09, 10, 11, 12
- Ancestor IDs
- 2F399A5C35CF433091C1AEEA54CD639D
- Source document
- Tennessee Academic Standards for Science
- License
- CC BY 4.0 US