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Classical Kuiper belt object and Plutino

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

Difference between Classical Kuiper belt object and Plutino

Classical Kuiper belt object vs. Plutino

A classical Kuiper belt object, also called a cubewano ("QB1-o"), is a low-eccentricity Kuiper belt object (KBO) that orbits beyond Neptune and is not controlled by an orbital resonance with Neptune. In astronomy, the plutinos are a dynamical group of trans-Neptunian objects in the outermost region of the Solar System that orbit in 2:3 mean-motion resonance with Neptune.

Similarities between Classical Kuiper belt object and Plutino

Classical Kuiper belt object and Plutino have 12 things in common (in Unionpedia): Deep Ecliptic Survey, Ecliptic, Kuiper belt, Neptune, Orbital eccentricity, Orbital inclination, Orbital resonance, Perihelion and aphelion, Perturbation (astronomy), Pluto, Resonant trans-Neptunian object, Trans-Neptunian object.

Deep Ecliptic Survey

The Deep Ecliptic Survey (DES) is a project to find Kuiper belt objects (KBOs), using the facilities of the National Optical Astronomy Observatory (NOAO).

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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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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.

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Neptune

Neptune is the eighth and farthest known planet from the Sun in the Solar System.

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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 resonance

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.

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Perihelion and aphelion

The perihelion of any orbit of a celestial body about the Sun is the point where the body comes nearest to the Sun.

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Perturbation (astronomy)

In astronomy, perturbation is the complex motion of a massive body subject to forces other than the gravitational attraction of a single other massive body.

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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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Resonant trans-Neptunian object

In astronomy, a resonant trans-Neptunian object is a trans-Neptunian object (TNO) in mean-motion orbital resonance with Neptune.

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Trans-Neptunian object

A trans-Neptunian object (TNO, also written transneptunian object) is any minor planet in the Solar System that orbits the Sun at a greater average distance (semi-major axis) than Neptune, 30 astronomical units (AU).

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The list above answers the following questions

Classical Kuiper belt object and Plutino Comparison

Classical Kuiper belt object has 53 relations, while Plutino has 33. As they have in common 12, the Jaccard index is 13.95% = 12 / (53 + 33).

References

This article shows the relationship between Classical Kuiper belt object and Plutino. To access each article from which the information was extracted, please visit:

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