Web2 apr. 2015 · $\begingroup$ The phrase "sitting just outside the body's atmosphere" has no meaning on Earth as the atmosphere doesn't have a hard boundary. Drag is a major consideration for satellites even as high as the International Space Station, at over 400 km of altitude. But yes, you could theoretically orbit a body with no atmosphere just above … Web13 okt. 2016 · The orbits of all large planets are rather close to circles: that of Earth, for instance, has e=0.0167 (3) The mean anomaly M, an angle growing at a steady rate, …
How to Calculate Orbital Period - Kerbal Space Program Forums
WebConvert the moon’s orbital period into years and its distance from Jupiter into AU and put them into this formula to calculate M, which is approximately the mass of Jupiter (in … Web27 okt. 2015 · It's given by Kepler's second law: A line joining a planet and the Sun sweeps out equal areas during equal intervals of time. The swept area is proportional to the distance times the orbital velocity: d A = d t ∗ v ∗ r / 2 = c o n s t. This makes the product of velocity and distance from the sun a constant. Is this what you are asking for? top edge rusher in nfl
5.6: Kepler’s Laws - Physics LibreTexts
WebA measure of distance often used in the equation to calculate orbital periods is the AU (astronomical unit) which is the distance between the Earth and our Sun. The distance of … Web6 feb. 2024 · By observing the time between transits, we know the orbital period. Kepler's Third law can be used to determine the orbital radius of the planet if the mass of the … Web26 mrt. 2016 · Add the 420 kilometers to Earth's radius to calculate the total distance between the International Space Station's and Earth's centers, and then convert to meters: Now substitute that into the orbital equation, and you find the International Space Station's orbital period (in units of seconds): Finally, convert to hours: About This Article top edge rushers