The orbital movements of planets in our solar system can be modeled by elliptical equations. Discuss the shapes of the path of the Moon around the Earth and the Earth around the Sun.

2.2°  

step-by-step explanation:

let θ = the angle of elevation.

tanθ =77/2020

tanθ = 0.038 12

      θ = tan⁻¹0.038 12

      θ = 2.2°

answer: 270

step-by-step explanation:

you have to times 200 by 1.35 to get your answer

inch

step-by-step explanation:

yard and mile are too big.