Question

@experimentX

Answer 1

Let's start with Keplers laws

Answer 2

Let's see what I remember without looking at my cheat sheet

Answer 3

Something about
\[T^2=R^3\]

Answer 4

seems like I forgot Kepler laws ... let's see

Answer 5

The period of an object orbital around the sun is proportional to the radius?

Answer 6

whose radius? or perhaps some distance? The distance between that object and the sun?

Answer 7

http://en.wikipedia.org/wiki/Kepler's_laws_of_planetary_motion
ellipse ... semi major axis.

Answer 8

no cheating haha

Answer 9

:P

Answer 10

draw it with me

Answer 11

Let's see what I remember about the semi major axis.......

Answer 12

\[\LARGE (\frac{T_1}{T_2})^2=(\frac{R_1}{R_2})^3\]

Answer 13

\[\LARGE \frac{dA}{dT}=\frac{L}{2M}\]

Answer 14

why do we have two semi major axis?

Answer 15

what ratio is that?

Answer 16

it doesn't matter which side you take ... lol