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(55637) 2002 UX25 and Orbital resonance

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

Difference between (55637) 2002 UX25 and Orbital resonance

(55637) 2002 UX25 vs. Orbital resonance

is a possible dwarf planet that orbits the Sun in the Kuiper belt beyond Neptune. 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 (55637) 2002 UX25 and Orbital resonance

(55637) 2002 UX25 and Orbital resonance have 9 things in common (in Unionpedia): Apsis, Astronomical unit, Dwarf planet, Jet Propulsion Laboratory, Kuiper belt, List of possible dwarf planets, Michael E. Brown, Neptune, Tethys (moon).

Apsis

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

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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.

(55637) 2002 UX25 and Astronomical unit · Astronomical unit and Orbital resonance · See more »

Dwarf planet

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

(55637) 2002 UX25 and Dwarf planet · Dwarf planet and Orbital resonance · See more »

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.

(55637) 2002 UX25 and Jet Propulsion Laboratory · Jet Propulsion Laboratory and Orbital resonance · See more »

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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List of possible dwarf planets

It is estimated that there may be 200 dwarf planets in the Kuiper belt of the outer Solar System and possibly more than 10,000 in the region beyond.

(55637) 2002 UX25 and List of possible dwarf planets · List of possible dwarf planets and Orbital resonance · See more »

Michael E. Brown

Michael E. Brown (born June 5, 1965) is an American astronomer, who has been professor of planetary astronomy at the California Institute of Technology (Caltech) since 2003.

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Neptune

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

(55637) 2002 UX25 and Neptune · Neptune and Orbital resonance · See more »

Tethys (moon)

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

(55637) 2002 UX25 and Tethys (moon) · Orbital resonance and Tethys (moon) · See more »

The list above answers the following questions

(55637) 2002 UX25 and Orbital resonance Comparison

(55637) 2002 UX25 has 37 relations, while Orbital resonance has 188. As they have in common 9, the Jaccard index is 4.00% = 9 / (37 + 188).

References

This article shows the relationship between (55637) 2002 UX25 and Orbital resonance. To access each article from which the information was extracted, please visit:

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