Kepler’s laws describe common features of the motions of orbiting objects, including their elliptical paths around the sun. O rbits may change due to the grav itational effects from, or collisions with, other objects in the solar sy stem.
Standard detail
ESS1.B(a)
Depth 3Parent ID: 836505B0C19A4EB0B73AB0826197168AStandard set: Earth and Space Sciences
Original statement
Quick facts
- Statement code
- ESS1.B(a)
- List ID
- a
- Standard ID
- DAC2229215FA4E0FA8E2F1BA8169EAFD
- Subject
- Earth and Space Sciences
- Grades
- 09, 10, 11, 12
- Ancestor IDs
- 836505B0C19A4EB0B73AB0826197168A5E6D83FA89D24D4EB16092761F18408CAD94F02B4D584A45B043D56891759C26
- Source document
- NGSS
- License
- CC BY 4.0 US