Kepler's 2nd law: Difference between revisions

Kepler's 2nd law (edit)

132 bytes added , 19 February 2023

no edit summary

6,480

edits

@@ Line 3: / Line 3: @@
 ''''' Kepler's laws of planetary motion''''' 1609-1619
-: $$\frac{d\theta}{dt} \propto \frac{1}{r^2}$$
+A line joining a planet and the Sun sweeps out equal areas during equal intervals of time.
+: <math>\frac{d\theta}{dt} \propto \frac{1}{r^2}</math>
 == Resources: ==
@@ Line 10: / Line 12: @@
 == Discussion: ==
+[[Category:Pages for Merging]]