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Specific orbital energy
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problem, the specific orbital energy ε {\displaystyle \varepsilon } (or vis-viva energy) of two orbiting bodies is the constant sum of their mutual potentialTransfer orbit (124 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill sphereElliptic orbit (2,715 words) [view diff] no match in snippet view article find links to article
of one body traveling along an elliptic orbit can be computed from the vis-viva equation as: v = μ ( 2 r − 1 a ) {\displaystyle v={\sqrt {\mu \left({2Peter Schilling (989 words) [view diff] case mismatch in snippet view article find links to article
songs, both the originals and new live versions and his newest album ‘Vis Viva’ on his YouTube channel. On March 24, 2024, a petition was initiated toOrbital speed (1,399 words) [view diff] no match in snippet view article find links to article
semi-major axis of the elliptical orbit. This expression is called the vis-viva equation. For the Earth at perihelion, the value is: 1.327 × 10 20 mOrbital decay (1,984 words) [view diff] no match in snippet view article find links to article
potential energies, in an unperturbed two-body orbit. By substituting the vis-viva equation into the kinetic energy component, the orbital energy of a circularList of equations (103 words) [view diff] no match in snippet view article find links to article
Mass–energy equivalence equation Primitive equations Relativistic wave equations Vis-viva equation Vorticity equation Wave equation Chemical equation (aka molecularArgument of periapsis (564 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill sphereHyperbolic trajectory (1,722 words) [view diff] no match in snippet view article find links to article
body traveling along a hyperbolic trajectory can be computed from the vis-viva equation as: v = μ ( 2 r + 1 a ) {\displaystyle v={\sqrt {\mu \left({2Mean anomaly (1,324 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill sphereOrbital mechanics (5,821 words) [view diff] no match in snippet view article find links to article
) of a body traveling along an elliptic orbit can be computed from the Vis-viva equation as: v = μ ( 2 r − 1 a ) {\displaystyle v={\sqrt {\mu \left({2Bi-elliptic transfer (2,054 words) [view diff] no match in snippet view article find links to article
The three required changes in velocity can be obtained directly from the vis-viva equation v 2 = μ ( 2 r − 1 a ) , {\displaystyle v^{2}=\mu \left({\fracMass ratio (464 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill spherePayload fraction (202 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill sphereOrbit insertion (672 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill sphereOrbital inclination (1,465 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill spherePropellant mass fraction (736 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill sphereDialectics of Nature (594 words) [view diff] exact match in snippet view article find links to article
still more incompletely applied. Words such as 'force', 'motion', and 'vis viva' were used where we should now speak of energy". Some then controversialOrbital node (936 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill sphereLissajous orbit (766 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill sphereTrue anomaly (1,107 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill sphereParabolic trajectory (1,090 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill sphereCircular orbit (1,276 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill sphereHydrodynamica (283 words) [view diff] exact match in snippet view article find links to article
the nature of hydrodynamic pressure and discovered the role of loss of vis viva in fluid flow, which would later be known as the Bernoulli principle. TheHohmann transfer orbit (3,662 words) [view diff] no match in snippet view article find links to article
{GMm}{r}}={\frac {-GMm}{2a}}.} Solving this equation for velocity results in the vis-viva equation, v 2 = μ ( 2 r − 1 a ) , {\displaystyle v^{2}=\mu \left({\fracOrbital period (2,059 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill sphereCelestial mechanics (2,194 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill sphereAzimuth (1,767 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill sphereRadial trajectory (1,439 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill sphereAerospace engineering (2,424 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill sphereBarycenter (astronomy) (1,521 words) [view diff] no match in snippet view article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill sphereDynamical friction (1,573 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill spherePerturbation (astronomy) (2,360 words) [view diff] no match in snippet view article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill sphereOrbital eccentricity (2,683 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill sphereTisserand's criterion (857 words) [view diff] no match in snippet view article find links to article
mass μ2, as a function of the distance and semi-major axis alone using vis-viva equation ( ξ ˙ 2 + η ˙ 2 + ζ ˙ 2 ) = v 2 = μ ( 2 r − 1 a ) {\displaystyle2005 HC4 (316 words) [view diff] no match in snippet view article find links to article
Objects – Dynamic Site. Retrieved 7 March 2014. As calculated with the vis-viva-equation : v 2 = G M ( 2 r − 1 a ) {\displaystyle v^{2}=GM\left({2 \overSphere of influence (astrodynamics) (1,386 words) [view diff] no match in snippet view article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill sphereSurface gravity (2,928 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill sphereSemi-major and semi-minor axes (2,365 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill sphereJames Jurin (1,364 words) [view diff] exact match in snippet view article find links to article
in defending Newton and attacking Gottfried Leibniz in the debate over vis viva, opposing the views of Benjamin Robins and Pietro Antonio Michelotti. JurinDaniel Bernoulli (1,847 words) [view diff] exact match in snippet view article find links to article
Pacey, A. J.; Fisher, S. J. (December 1967). "Daniel Bernoulli and the vis viva of compressed air". British Journal for the History of Science. 3 (4):Orbital maneuver (2,123 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill sphereOberth effect (1,968 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill sphereApsis (3,898 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill sphereEscape velocity (3,642 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill sphereKelvin's minimum energy theorem (564 words) [view diff] no match in snippet view article find links to article
proving the theorem. Thomson, W. (1849). Notes on hydrodynamics. V. On the vis-viva of a liquid in motion. Camb. Dubl. Math. J, 4, 90-94. Kelvin, W. T. B.Thomas L. Hankins (720 words) [view diff] exact match in snippet view article find links to article
Hankins, Thomas L. (1965). "Eighteenth-Century Attempts to Resolve the Vis viva Controversy". Isis. 56 (3): 281–297. doi:10.1086/349997. S2CID 143682504Indicator diagram (839 words) [view diff] exact match in snippet view article find links to article
ISBN 0-435-54150-1. Pacey, A.J. & Fisher, S.J. (1967) "Daniel Bernoulli and the vis viva of compressed air", The British Journal for the History of Science 3 (4)Kepler's equation (3,434 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill sphereLyapunov stability (3,765 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill sphereHill sphere (2,934 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill sphereTsiolkovsky rocket equation (4,342 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill sphereLagrange point (5,703 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill sphereGravity assist (5,021 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill sphereTwo-body problem (2,229 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill sphereWork (physics) (7,933 words) [view diff] exact match in snippet view article
correspondence of Descartes (PDF). p. 50. Iltis, C. (1971). "Leibniz and the vis viva controversy" (PDF). Isis. 62 (1): 21–35 (specifically p. 24). doi:10.1086/350705History of centrifugal and centripetal forces (2,949 words) [view diff] exact match in snippet view article find links to article
reference frame rotating with the planet. Leibniz introduced the notions of vis viva (kinetic energy) and action, which eventually found full expression inKepler's laws of planetary motion (8,294 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill sphereKepler's laws of planetary motion (8,294 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill spherePotentiality and actuality (6,501 words) [view diff] exact match in snippet view article find links to article
He preferred to refer to it as an entelecheia or 'living force' (Latin vis viva), but what he defined is today called kinetic energy, and was seen by LeibnizForce (11,784 words) [view diff] exact match in snippet view article find links to article
The product of a point mass and the square of its velocity was named vis viva (live force) by Leibniz. The modern concept of force corresponds to Newton'sN-body problem (8,605 words) [view diff] no match in snippet view article find links to article
Orbital period Orbital velocity Surface gravity Specific orbital energy Vis-viva equation Celestial mechanics Gravitational influences Barycenter Hill sphereMary Terrall (776 words) [view diff] exact match in snippet view article find links to article
Language?". Isis. Retrieved 21 September 2023. Terrall, Mary (2004). "Vis viva revisited". History of Science. Retrieved 21 September 2023. Lilti, Antoine