inclination of an orbit
inclinación orbital
orbital inclination oor Galisies
orbital inclination
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Inclinación orbital
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angle between a reference plane and the plane of an orbit
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Its orbital eccentricity is negligible, and its orbital inclination is about 1°.
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Haumea has an orbital period of 284 Earth years, a perihelion of 35 AU, and an orbital inclination of 28°.
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Kiviuq is believed to be in Kozai resonance, cyclically reducing its orbital inclination while increasing the eccentricity and vice versa.
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As Poynting–Robertson drag causes particles to slowly drift towards Jupiter, their orbital inclinations are excited while passing through it.
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These surveys eventually covered the location of Haumea, with its high orbital inclination and current position far from the ecliptic.
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The orbital inclination of satellites such as this one is limited by the Kozai effect, discovered by Yoshihide Kozai in 1962.
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One piece of evidence for such a past resonance is Miranda's unusually high orbital inclination (4.34°) for a body so close to the planet.
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The large thickness of the halo can be attributed to the excitation of orbital inclinations and eccentricities of dust particles by the electromagnetic forces in the Jovian magnetosphere.
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With an orbital inclination of 34.8°, Pallas's orbit is unusually highly inclined to the plane of the asteroid belt, and its orbital eccentricity is nearly as large as that of Pluto, making Pallas relatively inaccessible to spacecraft.
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By plotting the mean orbital motion, inclination and eccentricity of a set of asteroids, he discovered several distinct groupings.
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It probably escaped detection during the earlier surveys due to its relatively high orbital inclination, and the fact that it was at its farthest distance from the ecliptic at the time of its discovery, in the northern constellation of Coma Berenices.
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This is thought to be due to Haumea's weak 7:12 orbital resonance with Neptune gradually modifying its initial orbit over the course of a billion years, through the Kozai effect, which allows the exchange of an orbit's inclination for increased eccentricity.
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Miranda probably escaped from its resonance with Umbriel via a secondary resonance, and the mechanism of this escape is believed to explain why its orbital inclination is more than 10 times those of the other regular Uranian moons (see Uranus' natural satellites).
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Sinope orbits Jupiter on a high-eccentricity and high-inclination retrograde orbit.
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Ananke orbits Jupiter on a high-eccentricity and high-inclination retrograde orbit.
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The outer moons of the giant planets tend to be small and have eccentric orbits with arbitrary inclinations.
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Halimede has the second most eccentric and third most inclined orbit around Neptune.
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Braille has an unusually inclined orbit, and belongs to the somewhat rare class of asteroids known as Mars-crossing asteroids.
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In 2004, astrometric measurements with the Fine Guidance Sensors on the Hubble Space Telescope suggest that the planet's orbit is inclined by around 53° with respect to the plane of the sky.
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Its orbit is retrograde, moderately inclined and eccentric.
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The elliptical orbit of Neptune is inclined 1.77° compared to that of Earth.
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Its orbit is highly inclined and moderately eccentric, despite being at the same distance from the Sun as the central part of the asteroid belt.
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Skoll is about 6 kilometres in diameter (assuming an albedo of 0.04) and orbits Saturn at an average distance of 17.6 Gm (million km) in 869 days, following a highly eccentric and moderately inclined orbit.
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The remainder of the moons consist of an unknown number of small irregular moons with elliptical and inclined orbits, which are thought to be captured asteroids or fragments of captured asteroids.
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Evidence of tilted circumbinary discs can be seen through warped geometry within circumstellar discs, precession of protostellar jets, and inclined orbits of circumplanetary objects (as seen in the eclipsing binary TY CrA).
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