A lthough activ e geologic processes, such as plate tectonics and erosion, hav e destroy ed or altered most of the v ery early rock record on Earth, other objects in the solar sy stem, such as lunar rocks, asteroids, and meteorites, hav e changed little ov er billions of y ears. Study ing these objects can prov ide information about Earth’s formation and early history .
Standard detail
ESS1.C(b)
Depth 3Parent ID: 2FB8018CF02E403E8DB062D3503E3D02Standard set: Earth and Space Sciences
Original statement
Quick facts
- Statement code
- ESS1.C(b)
- List ID
- b
- Standard ID
- 8CB423B719D042659790CC423863C1E4
- Subject
- Earth and Space Sciences
- Grades
- 09, 10, 11, 12
- Ancestor IDs
- 2FB8018CF02E403E8DB062D3503E3D025E6D83FA89D24D4EB16092761F18408CAD94F02B4D584A45B043D56891759C26
- Source document
- NGSS
- License
- CC BY 4.0 US