File:Planets and dwarf planets' tilt and rotation speed.webm
Jump to navigation
Jump to search
Planets_and_dwarf_planets'_tilt_and_rotation_speed.webm (file size: 10.64 MB, MIME type: video/webm)
Summary
| Description |
English: Anyway in this video... to roughly explain the tilts: we think they started out roughly the same in tilt, so either by huge impacts, tidal forces or planetary migration the tilts have been changed. The reason why larger planets tend to spin faster is because they took on more of the Sun-orbiting mass, adding the mass's orbital motion to their spin in the process |
| Date | |
| Source | YouTube: https://www.youtube.com/watch?v=WX6PRDqfLNc – View/save archived versions on archive.org and archive.today |
| Author | Dr. James O'Donoghue under YouTube alias "Interplanetary" |
Licensing
.svg){kind=icon}
This video, screenshot or audio excerpt was originally uploaded on YouTube under a CC BY license.
Their website states: "YouTube allows users to mark their videos with a Creative Commons CC BY license."
To the uploader: You must provide a link (URL) to the original file and the authorship information if available.
This file is licensed under the Creative Commons Attribution 3.0 Unported license.
Attribution:
James O'Donoghue
- You are free:
- to share – to copy, distribute and transmit the work
- to remix – to adapt the work
- Under the following conditions:
- attribution – You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use.
File history
Click on a date/time to view the file as it appeared at that time.
| Date/Time | Dimensions | User | Comment | |
|---|---|---|---|---|
| current | 16:13, 16 May 2023 | (10.64 MB) | wikimediacommons>CactiStaccingCrane | Uploaded a work by Dr. James O'Donoghue under YouTube alias "Interplanetary" from https://www.youtube.com/watch?v=WX6PRDqfLNc with UploadWizard |
File usage
The following page uses this file: