Intergalactic Planetary

Evidence

We learned how to use different aspects of planets to calculate others, such as using the distance to the sun and obliquity to orbit of a planet to calculate surface temperature.

We used equations we were already familiarized with by rearranging them to find new aspects. For example, in order to find the orbital period, you can use the equation for velocity, V=d/t, and implement the values for orbital speed and and distance from the sun.

Using the values we were given for each planet, we had to find the orbital period and force of gravity.

We were given the distance from the sun, the radius of the planet, and the mass of the planet.

We use the equations, 2πr^2/v, and G(m1m2)/d^2 to find out more about these two unknown planets and Earth.

I think the key to this project was simply collaboration. The task was sort of simple but it would've been really hard to to do alone. As you can tell from the different hand writings on the evidence, my partner and I divided and conquered. The reason why was because while I had a better understand of the literal equations, my partner was more knowledgable about the thinking behind the math. So in order to complete the project we had to work separately in order to compile our finished work together so they coincided into one whole project.