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Ceres (dwarf planet) and Orbital resonance

Shortcuts: Differences, Similarities, Jaccard Similarity Coefficient, References.

Difference between Ceres (dwarf planet) and Orbital resonance

Ceres (dwarf planet) vs. Orbital resonance

Ceres (minor-planet designation: 1 Ceres) is the largest object in the asteroid belt that lies between the orbits of Mars and Jupiter, slightly closer to Mars' orbit. In celestial mechanics, an orbital resonance occurs when orbiting bodies exert a regular, periodic gravitational influence on each other, usually because their orbital periods are related by a ratio of small integers.

Similarities between Ceres (dwarf planet) and Orbital resonance

Ceres (dwarf planet) and Orbital resonance have 41 things in common (in Unionpedia): Apsis, Asteroid, Asteroid belt, Astronomical unit, Astronomy & Astrophysics, Axial tilt, Callisto (moon), Clearing the neighbourhood, Conjunction (astronomy), Definition of planet, Dwarf planet, Earth, Ecliptic, Enceladus, Europa (moon), Haumea, Jet Propulsion Laboratory, Jupiter, Kuiper belt, Mars, Mercury (planet), Monthly Notices of the Royal Astronomical Society, Orbital eccentricity, Orbital inclination, Orbital period, Osculating orbit, Planetesimal, Pluto, Proper orbital elements, Rhea (moon), ..., Saturn, Science (journal), Semi-major and semi-minor axes, Solar System, Tethys (moon), The Planetary Society, Titius–Bode law, Trojan (astronomy), Uranus, Venus, 2 Pallas. Expand index (11 more) »

Apsis

An apsis (ἁψίς; plural apsides, Greek: ἁψῖδες) is an extreme point in the orbit of an object.

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Asteroid

Asteroids are minor planets, especially those of the inner Solar System.

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Asteroid belt

The asteroid belt is the circumstellar disc in the Solar System located roughly between the orbits of the planets Mars and Jupiter.

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Astronomical unit

The astronomical unit (symbol: au, ua, or AU) is a unit of length, roughly the distance from Earth to the Sun.

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Astronomy & Astrophysics

Astronomy & Astrophysics is a peer-reviewed scientific journal covering theoretical, observational, and instrumental astronomy and astrophysics.

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Axial tilt

In astronomy, axial tilt, also known as obliquity, is the angle between an object's rotational axis and its orbital axis, or, equivalently, the angle between its equatorial plane and orbital plane.

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Callisto (moon)

Callisto (Jupiter IV) is the second-largest moon of Jupiter, after Ganymede.

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Clearing the neighbourhood

"Clearing the neighbourhood around its orbit" is a criterion for a celestial body to be considered a planet in the Solar System.

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Conjunction (astronomy)

In astronomy, a conjunction occurs when two astronomical objects or spacecraft have either the same right ascension or the same ecliptic longitude, usually as observed from Earth.

Ceres (dwarf planet) and Conjunction (astronomy) · Conjunction (astronomy) and Orbital resonance · See more »

Definition of planet

The definition of planet, since the word was coined by the ancient Greeks, has included within its scope a wide range of celestial bodies.

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Dwarf planet

A dwarf planet is a planetary-mass object that is neither a planet nor a natural satellite.

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Earth

Earth is the third planet from the Sun and the only astronomical object known to harbor life.

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Ecliptic

The ecliptic is the circular path on the celestial sphere that the Sun follows over the course of a year; it is the basis of the ecliptic coordinate system.

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Enceladus

Enceladus is the sixth-largest moon of Saturn.

Ceres (dwarf planet) and Enceladus · Enceladus and Orbital resonance · See more »

Europa (moon)

Europa or as Ευρώπη (Jupiter II) is the smallest of the four Galilean moons orbiting Jupiter, and the sixth-closest to the planet.

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Haumea

Haumea, minor-planet designation 136108 Haumea, is a dwarf planet located beyond Neptune's orbit.

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Jet Propulsion Laboratory

The Jet Propulsion Laboratory (JPL) is a federally funded research and development center and NASA field center in Pasadena, California, United States, with large portions of the campus in La Cañada Flintridge, California.

Ceres (dwarf planet) and Jet Propulsion Laboratory · Jet Propulsion Laboratory and Orbital resonance · See more »

Jupiter

Jupiter is the fifth planet from the Sun and the largest in the Solar System.

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Kuiper belt

The Kuiper belt, occasionally called the Edgeworth–Kuiper belt, is a circumstellar disc in the outer Solar System, extending from the orbit of Neptune (at 30 AU) to approximately 50 AU from the Sun.

Ceres (dwarf planet) and Kuiper belt · Kuiper belt and Orbital resonance · See more »

Mars

Mars is the fourth planet from the Sun and the second-smallest planet in the Solar System after Mercury.

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Mercury (planet)

Mercury is the smallest and innermost planet in the Solar System.

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Monthly Notices of the Royal Astronomical Society

Monthly Notices of the Royal Astronomical Society (MNRAS) is a peer-reviewed scientific journal covering research in astronomy and astrophysics.

Ceres (dwarf planet) and Monthly Notices of the Royal Astronomical Society · Monthly Notices of the Royal Astronomical Society and Orbital resonance · See more »

Orbital eccentricity

The orbital eccentricity of an astronomical object is a parameter that determines the amount by which its orbit around another body deviates from a perfect circle.

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Orbital inclination

Orbital inclination measures the tilt of an object's orbit around a celestial body.

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Orbital period

The orbital period is the time a given astronomical object takes to complete one orbit around another object, and applies in astronomy usually to planets or asteroids orbiting the Sun, moons orbiting planets, exoplanets orbiting other stars, or binary stars.

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Osculating orbit

In astronomy, and in particular in astrodynamics, the osculating orbit of an object in space at a given moment in time is the gravitational Kepler orbit (i.e. ellipse or other conic) that it would have about its central body if perturbations were not present.

Ceres (dwarf planet) and Osculating orbit · Orbital resonance and Osculating orbit · See more »

Planetesimal

Planetesimals are solid objects thought to exist in protoplanetary disks and in debris disks.

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Pluto

Pluto (minor planet designation: 134340 Pluto) is a dwarf planet in the Kuiper belt, a ring of bodies beyond Neptune.

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Proper orbital elements

The proper orbital elements of an orbit are constants of motion of an object in space that remain practically unchanged over an astronomically long timescale.

Ceres (dwarf planet) and Proper orbital elements · Orbital resonance and Proper orbital elements · See more »

Rhea (moon)

Rhea (Ῥέᾱ) is the second-largest moon of Saturn and the ninth-largest moon in the Solar System.

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Saturn

Saturn is the sixth planet from the Sun and the second-largest in the Solar System, after Jupiter.

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Science (journal)

Science, also widely referred to as Science Magazine, is the peer-reviewed academic journal of the American Association for the Advancement of Science (AAAS) and one of the world's top academic journals.

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Semi-major and semi-minor axes

In geometry, the major axis of an ellipse is its longest diameter: a line segment that runs through the center and both foci, with ends at the widest points of the perimeter.

Ceres (dwarf planet) and Semi-major and semi-minor axes · Orbital resonance and Semi-major and semi-minor axes · See more »

Solar System

The Solar SystemCapitalization of the name varies.

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Tethys (moon)

Tethys (or Saturn III) is a mid-sized moon of Saturn about across.

Ceres (dwarf planet) and Tethys (moon) · Orbital resonance and Tethys (moon) · See more »

The Planetary Society

The Planetary Society is an American internationally active, non-governmental, nonprofit foundation.

Ceres (dwarf planet) and The Planetary Society · Orbital resonance and The Planetary Society · See more »

Titius–Bode law

The Titius–Bode law (sometimes termed just Bode's law) is a hypothesis that the bodies in some orbital systems, including the Sun's, orbit at semi-major axes in a function of planetary sequence.

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Trojan (astronomy)

In astronomy, a trojan is a minor planet or moon that shares the orbit of a planet or larger moon, wherein the trojan remains in the same, stable position relative to the larger object.

Ceres (dwarf planet) and Trojan (astronomy) · Orbital resonance and Trojan (astronomy) · See more »

Uranus

Uranus is the seventh planet from the Sun.

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Venus

Venus is the second planet from the Sun, orbiting it every 224.7 Earth days.

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2 Pallas

Pallas, minor-planet designation 2 Pallas, is the second asteroid to have been discovered (after Ceres), and is one of the largest asteroids in the Solar System.

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The list above answers the following questions

Ceres (dwarf planet) and Orbital resonance Comparison

Ceres (dwarf planet) has 219 relations, while Orbital resonance has 188. As they have in common 41, the Jaccard index is 10.07% = 41 / (219 + 188).

References

This article shows the relationship between Ceres (dwarf planet) and Orbital resonance. To access each article from which the information was extracted, please visit:

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