Earth and Sun

Canvas not supported; please update your browser.

What keeps the Earth moving in its approximately circular path around the Sun? It's a combination of the 30 km/s speed of the Earth and the gravitational force exerted on the Earth by the Sun.

This simulation shows five different Earths, with initial speeds of 80%, 100%, 120%, 141.42%, and 150% of the real Earth's speed. This results in four different orbital shapes - two elliptical orbits, a circular orbit, a parabolic trajectory, and a hyperbolic trajectory.

Simulation first posted on 7-13-2016. Written by Andrew Duffy

Creative Commons License
This work by Andrew Duffy is licensed under a Creative Commons Attribution-ShareAlike 4.0 International License.
This simulation can be found in the collection at http://physics.bu.edu/~duffy/classroom.html. Creative Commons License
This work by Andrew Duffy is licensed under a Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International License.
This simulation can be found in the collection at http://physics.bu.edu/~duffy/classroom.html.

The counter has been running on this page since 8-10-2018. The number of people accessing the page since then is: