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Questions tagged [celestial-mechanics]

Celestial Mechanics is the branch of astronomy devoted to the study of the motion of the celestial bodies on the basis of the laws of gravitation.

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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, $$T = 2π/ω ...
Sirshendu Gayen's user avatar
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1 answer
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By analyzing the motion of Venus using NASA JPL Horizons ephemeris data (10-year span, 1-hour sampling), I found that the variation of orbital velocity $\Delta v(t)$ appears to closely follow a ...
TemiZion's user avatar
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In this paper the gravitational potential between a point mass and an extended rigid body is $$ U = -\mathbb{G}m_1\int_B \frac{\mathrm{d}^3 \mathbf{Q}'\rho(\mathbf{Q}')}{|\mathbf{r} + \mathrm{C}\...
jeffreygorwinkle's user avatar
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1 answer
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The potential due to a rigid body will be approximated using a Lagrange polynomial expansion as $$ U(x,y,z)=-\frac{\mathbb{G}Mm_p}{r} - \frac{\mathbb{G}m_p(I_1 + I_2 + I_3)}{2r^3} + \frac{3\mathbb{G}...
jeffreygorwinkle's user avatar
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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
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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
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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
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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 ...
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It is claimed that the moon stabilizes the Earth's axial tilt, but Mars and Venus (and Mercury, too) are rocky planets without large moons. Why are their axes stable?
Michael Stachowsky's user avatar
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Imagine a space probe that starts around Earth at time $t=0$ with velocity $\vec{V_0}$ (sun reference frame) and goes into an elliptical orbit around the sun such that after (almost) exactly one year ...
darksun's user avatar
12 votes
6 answers
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I read that pretty much all orbiting planets have some initial spin. My question is, if we were able to cancel that initial spin and make the planet or ,let's say, for convince's sake, an artificial ...
TheLostInUnknown's user avatar
12 votes
9 answers
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Spring tides occur during syzygy of the Earth, Sun and Moon. During a new moon, when the sun and moon are both pulling harder on the near side of the earth than the far side, this makes perfect sense, ...
Buff's user avatar
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The direct perturbation term in celestial mechanics can be written as: $$ \mathcal{H}_{\rm D} = - G\frac{m_1 m_2}{|\vec{r}_2 - \vec{r}_1|} = -G\frac{m_1 m_2}{r_2} \sum_{k=0}^{\infty} \binom{-1/2}{k} B^...
RKerr's user avatar
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I'm reading Bahcall & Wolf (1976) [ApJ 209, 214. Star distribution around a massive black h0le in a globular cluster]. As usual, they skip lots of derivations, and I'm having trouble getting from $...
Valentín Peña Donaire's user avatar
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Books such as Moulton focus on the classical perturbation theory famously developed by Lagrange and Laplace, while more modern books seem to use canonical perturbation theory. I can't currently see ...
timur's user avatar
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