1mo ago

Why does stuff move in a parabola on earth but in an ellipse in space?

So of course both of these are slight simplifications, but what is the connection between the two? If the earth is basically a circle, is an ellipse just a parabola stretched around a circle? Is a parabola just an approximation of a tiny part of an ellipse? How high do you have to be before you change your calculations of a trajectory?

The Math ain't mathing.

21 comments

When you throw something on earth and calculate it as a parabola, that's based on the approximation that the force of gravity is constant across the trajectory. It's actually a tiny bit weaker 20 feet up than at ground level, but the difference is so small that you can ignore it. The trajectory in a constant gravational field is parabolic.
When something is high enough that you're doing orbital calculations, you have to take the inverse square law into account. The elliptical orbit is a consequence of the gravitational force being inversely proportional to the square of the distance. It doesn't apply if the force is constant.
You can also say, look at a small segment of the pointy part of a very skinny ellipse, and it will look approximately like a parabola.
- Great explanation!
Geometry!
https://en.m.wikipedia.org/wiki/Conic_section
They are similar and related but not quite the same thing. It does come down to whether it is orbiting or returning to a 'flat' plane, and while an eclipse isn't quite the same thing as two parabolas put together, that isn't too far off.
You can think of a parabola as a segment of an ellipse, yes.
But remember: A stable orbit forms an ellipse. An unstable one doesn't. And throwing an object from the surface of a planet is, sans incredible math or even more incredible luck, going to be unstable.
- I don't think that's true. Any of it, really.
  A parabola has a constant second derivative, while a (half) ellipse has one that diverges to infinity in finite time (since it goes vertical). I can't really prove that no ellipse section is parabolic, off the top of my head, but that's strongly suggestive of it.
  Every two-body Newtonian orbit in a vacuum is stable, or an escape trajectory. It was either Newton himself or a contemporary that established that.
  
  First paragraph: I see what you're saying and I think you're right.
  Second paragraph: Even if you're right on this, and offhand I'm really not convinced you are because it seems like that neglects the possibility of collision, launching anything from the surface of a planet is a three-or-more body problem, featuring 1) the planet, 2) the star it's orbiting, 3) the launch body, and optionally a number of moons. But that's, ah, getting away from OP's question.
If something is moving in an elliptical orbit, and you are observing it from a fixed point in space, it will appear elliptical.
If something is moving in an elliptical orbit, and you are observing it from a body that is itself also moving in an elliptical orbit, it will appear parabolic.
It’s a parabola because the rest of the ellipse is in the ground.
They move in ellipses on earth as well, but it's cut short by hitting the ground. Also, air resistance affects the trajectory so that anything thrown/shot will eventually return.
Source: Thousands of hours in KSP
- KSP is such a great game. Such a shame what happened to KSP2 but that was doomed from the start.
  
  Yeah, KSP2 was botched on so many levels, primarily by Take2.
  Looking forward to seeing what comes out of KSA, though. With many of the old devs and modders of KSP1 on board it looks like they have a good start.
Lots of answers touched the correct answer, which is that in reality things don't follow parabolas on earth, a parabola is just close enough to the actual thing the object is doing to be indistinguishable. In reality everything follows elliptical orbits, but the top of an ellipsis with a Major axis of 6378 km and a few meters in the minor axis looks the same as a parabola, especially when you don't see the full orbit because the object hits the ground. If you were to throw a rock and suddenly the entire earth besides that rock collapsed to a single point, your rock will orbit earth in an elliptical orbit.
Are you familiar with the difference between polar (r, theta) coordinates and cartesian (x,y) coordinates? Parabolas are the solution to gravity that is uniform no matter where you sample. It assumes that gravity points in the same direction with the same magnitude no matter where you are. In this model, gravitational acceleration is always 9.81 m/s^2 in the -y direction. That is a reasonable simplification for things that are at the human scale constrained to near the earth's surface. Deviations from air resistance will matter far more than errors stemming from that assumption anyway.
Conic sections are the solutions to gravity that is between two objects where the force is along the line between the center of mass of both objects and the strength is inversely proportional to the square of separation. Now you need polar cpordinates and the direction of gravity changes as things move around. This works pretty well for orbits around the earth and orbits around the sun, because the earth is so much more massive than sattelites that orbit it, and the sun is so much more massive than things that orbit it. If you need really precise orbit trajectories, ellipses aren't truly accurate either. You need to account for all the orbiting bodies in the system. The 3-body problem famously doesn't have purely analytical solutions, and you need to resort to numerical methods to calculate trajectories.
So both solutions come from simplified mathematical models. Despite being simplifications, their predictive power is actually very goood. However, like you are intuiting, it's important to know when those simplifying assumptions lead to errors that start to become important. It's hard to come up with a particular threshold for when you need to switch from one model to another, because it really depends on how much accuracy your application needs.
Basically, it's an ellipse on Earth too. Just one that's nearly a parabola. Because of approximately constant gravity and an approximately (approximately!) flat Earth, like the current top commenter said.
Only stable orbits are elliptical. Many objects follow parabolic and hyperbolic trajectories in space. Eventually, many intersect with other objects. As time passes, objects that are not in stable (or semi-stable) orbits become less common through attrition.

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