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Questions tagged [orbital-motion]

The path a body takes while moving through space under the influence of the gravitational forces of other bodies

1 vote
1 answer
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Angular momentum $L$ of a particle in central force is a constant of motion. So for circular orbit, $$L =mωr^2 = constant.$$ This implies $$ω ∝ 1/r^2,$$ hence the time period of revolution, $$T = 2π/ω ...
Sirshendu Gayen's user avatar
-1 votes
0 answers
30 views

I am working on orbit uncertainty propagation, where the initial position and velocity define the uncertainty. I want to construct an orbit that is determined by Delaunay variables. Now I just know ...
Zhangshu Cheng's user avatar
0 votes
0 answers
62 views

I am working on orbital uncertainty propagation where the initial uncertainty is given in Cartesian coordinates ( 𝑟 , 𝑣 ) (r,v), either as a covariance matrix or as bounded (non-statistical) ...
Zhangshu Cheng's user avatar
2 votes
1 answer
77 views

By analyzing the motion of Venus using NASA JPL Horizons ephemeris data (10-year span, 1-hour sampling), I found that the variation of orbital velocity $\Delta v(t)$ appears to closely follow a ...
TemiZion's user avatar
2 votes
1 answer
242 views

A solid ring cannot orbit a mass at its center because it is in unstable equilibrium, and a slight perturbation would cause it to drift. An object obviously can orbit. You can also take a portion of a ...
Ariel's user avatar
  • 121
3 votes
1 answer
69 views

In general I would like to know how to minimise fuel mass spent for an orbiting body that continuously jettisons its mass (i.e. ion thruster) so as to perform efficient transfer maneuver in ...
lodzki's user avatar
  • 43
0 votes
0 answers
40 views

In several comets, including the interstellar comet 3I/ATLAS, a non-gravitational acceleration is observed, i.e., a net thrust not fully accounted for by gravity. While outgassing is known to produce ...
John Stamoutsos's user avatar
1 vote
1 answer
117 views

The Klein–Gordon equation with a position-dependent effective mass, $$ \frac{\partial^2 E}{\partial t^2} = c^2 \nabla^2 E - \chi(x)^2 E, $$ describes a scalar field whose local propagation speed ...
slaphshot33324's user avatar
1 vote
0 answers
76 views

I would like to understand the derivation of the orbit equation. I am following the derivation at https://orbital-mechanics.space/the-orbit-equation/the-orbit-equation.html which is largely ...
Ana's user avatar
  • 111
4 votes
4 answers
508 views

When presented with the two-body problems, we usually start from Newton's 2nd equations for the two bodies: $$ \begin{split} m_1 \mathbf{\ddot{r}}_1 &= f(r) \mathbf{\hat{r}}, \\ m_2 \mathbf{\ddot{...
cosimoNigro's user avatar
2 votes
1 answer
227 views

For a non-spinning (Schwarzschild) black hole: The event horizon (Schwarzschild radius) is at: $$r = \frac{2GM}{c^2}$$ Inside this radius, not even light can escape. Outside that, there is the ...
Swarnim Khosla's user avatar
0 votes
1 answer
135 views

Is general relativity required to calculate to orbits of Pluto's moons? How to calculate of orbits of the Pluto's moons?
user382965's user avatar
1 vote
0 answers
43 views

One of my daydreams is a non rotating sky hook anchored on Phobos. I was wondering how to calculate the Coriolis Force induced by ascending or descending elevator cars. Wikipedia tells me: Coriolis ...
HopDavid's user avatar
  • 535
0 votes
0 answers
48 views

I am creating a program that calculates orbital mechanics. And one option I want is the ability to use as a starting point the current positions of the Solar System. So is there a site that can I use ...
0 votes
1 answer
76 views

Background Consider I'm studying the orbit of planets using the Schwarzschild metric is given by: $$ ds^2 = -\left(1 - \frac{2GM}{c^2 r}\right) c^2 dt^2 + \left(1 - \frac{2GM}{c^2 r}\right)^{-1} dr^2 +...
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