Timeline for Conservation of angular momentum in a planetary system
Current License: CC BY-SA 3.0
Post Revisions
13 events
| when toggle format | what | by | license | comment | |
|---|---|---|---|---|---|
| Oct 31, 2016 at 11:57 | history | protected | rob♦ | ||
| Oct 31, 2016 at 11:50 | answer | added | FearlessVirgo | timeline score: 0 | |
| Oct 31, 2016 at 8:26 | answer | added | Tamang Abhisek | timeline score: 0 | |
| Apr 7, 2015 at 14:21 | vote | accept | CommunityBot | ||
| Apr 7, 2015 at 14:18 | vote | accept | CommunityBot | ||
| Apr 7, 2015 at 14:21 | |||||
| Apr 7, 2015 at 13:34 | comment | added | Sanchises | Note that, although the sun is often depicted as stationary, it is not! Perhaps your understanding will get better if you consider two equal masses rotating around each other in an elliptical orbit. | |
| Apr 7, 2015 at 13:18 | answer | added | RE60K | timeline score: 8 | |
| Apr 7, 2015 at 13:16 | comment | added | ACuriousMind♦ | Equations are "physics logic". Don't discriminate against formulae! | |
| Apr 7, 2015 at 13:12 | history | edited | Emilio Pisanty | CC BY-SA 3.0 |
Formatting fixes.
|
| Apr 7, 2015 at 13:09 | review | Close votes | |||
| Apr 7, 2015 at 17:28 | |||||
| Apr 7, 2015 at 12:48 | history | edited | Qmechanic♦ | CC BY-SA 3.0 |
deleted 12 characters in body; edited tags
|
| Apr 7, 2015 at 12:45 | answer | added | image357 | timeline score: 4 | |
| Apr 7, 2015 at 12:20 | history | asked | user74370 | CC BY-SA 3.0 |