Faster access than browser!Similarities between Orbital resonance and Planet
Orbital resonance and Planet have 57 things in common (in Unionpedia): Apsis, Asteroid, Asteroid belt, Astronomical unit, Astronomy & Astrophysics, Axial tilt, Callisto (moon), Ceres (dwarf planet), Clearing the neighbourhood, Definition of planet, Dione (moon), Dwarf planet, Earth, Ecliptic, Europa (moon), Exoplanet, Extrasolar Planets Encyclopaedia, Galilean moons, Ganymede (moon), Gravity, Iapetus (moon), Io (moon), Jupiter, Kuiper belt, Mars, Mercury (planet), Monthly Notices of the Royal Astronomical Society, Moons of Saturn, Moons of Uranus, Natural satellite, ..., Nature (journal), Neptune, Orbit, Orbital eccentricity, Orbital inclination, Orbital node, Orbital period, Perihelion and aphelion, Planetesimal, Pluto, Retrograde and prograde motion, Rhea (moon), Ring system, Rings of Saturn, Saturn, Semi-major and semi-minor axes, Solar System, Springer Science+Business Media, Super-Earth, Tethys (moon), Tidal force, Tidal locking, Titan (moon), Transit of Venus, Uranus, Venus, 2 Pallas. Expand index (27 more) »
Apsis
An apsis (ἁψίς; plural apsides, Greek: ἁψῖδες) is an extreme point in the orbit of an object.
Apsis and Orbital resonance · Apsis and Planet ·
Asteroid
Asteroids are minor planets, especially those of the inner Solar System.
Asteroid and Orbital resonance · Asteroid and Planet ·
Asteroid belt
The asteroid belt is the circumstellar disc in the Solar System located roughly between the orbits of the planets Mars and Jupiter.
Asteroid belt and Orbital resonance · Asteroid belt and Planet ·
Astronomical unit
The astronomical unit (symbol: au, ua, or AU) is a unit of length, roughly the distance from Earth to the Sun.
Astronomical unit and Orbital resonance · Astronomical unit and Planet ·
Astronomy & Astrophysics
Astronomy & Astrophysics is a peer-reviewed scientific journal covering theoretical, observational, and instrumental astronomy and astrophysics.
Astronomy & Astrophysics and Orbital resonance · Astronomy & Astrophysics and Planet ·
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.
Axial tilt and Orbital resonance · Axial tilt and Planet ·
Callisto (moon)
Callisto (Jupiter IV) is the second-largest moon of Jupiter, after Ganymede.
Callisto (moon) and Orbital resonance · Callisto (moon) and Planet ·
Ceres (dwarf planet)
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.
Ceres (dwarf planet) and Orbital resonance · Ceres (dwarf planet) and Planet ·
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.
Clearing the neighbourhood and Orbital resonance · Clearing the neighbourhood and Planet ·
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.
Definition of planet and Orbital resonance · Definition of planet and Planet ·
Dione (moon)
Dione (Διώνη) is a moon of Saturn.
Dione (moon) and Orbital resonance · Dione (moon) and Planet ·
Dwarf planet
A dwarf planet is a planetary-mass object that is neither a planet nor a natural satellite.
Dwarf planet and Orbital resonance · Dwarf planet and Planet ·
Earth
Earth is the third planet from the Sun and the only astronomical object known to harbor life.
Earth and Orbital resonance · Earth and Planet ·
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.
Ecliptic and Orbital resonance · Ecliptic and Planet ·
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.
Europa (moon) and Orbital resonance · Europa (moon) and Planet ·
Exoplanet
An exoplanet or extrasolar planet is a planet outside our solar system.
Exoplanet and Orbital resonance · Exoplanet and Planet ·
Extrasolar Planets Encyclopaedia
The Extrasolar Planets Encyclopaedia is an astronomy website, founded in Paris, France at the Meudon Observatory by Jean Schneider in February 1995, which maintains a database of all the currently known and candidate extrasolar planets, with individual pages for each planet and a full list interactive catalog spreadsheet.
Extrasolar Planets Encyclopaedia and Orbital resonance · Extrasolar Planets Encyclopaedia and Planet ·
Galilean moons
The Galilean moons are the four largest moons of Jupiter—Io, Europa, Ganymede, and Callisto.
Galilean moons and Orbital resonance · Galilean moons and Planet ·
Ganymede (moon)
Ganymede (Jupiter III) is the largest and most massive moon of Jupiter and in the Solar System.
Ganymede (moon) and Orbital resonance · Ganymede (moon) and Planet ·
Gravity
Gravity, or gravitation, is a natural phenomenon by which all things with mass or energy—including planets, stars, galaxies, and even light—are brought toward (or gravitate toward) one another.
Gravity and Orbital resonance · Gravity and Planet ·
Iapetus (moon)
Iapetus (Ιαπετός), or occasionally Japetus, is the third-largest natural satellite of Saturn, eleventh-largest in the Solar System, and the largest body in the Solar System known not to be in hydrostatic equilibrium.
Iapetus (moon) and Orbital resonance · Iapetus (moon) and Planet ·
Io (moon)
Io (Jupiter I) is the innermost of the four Galilean moons of the planet Jupiter.
Io (moon) and Orbital resonance · Io (moon) and Planet ·
Jupiter
Jupiter is the fifth planet from the Sun and the largest in the Solar System.
Jupiter and Orbital resonance · Jupiter and Planet ·
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.
Kuiper belt and Orbital resonance · Kuiper belt and Planet ·
Mars
Mars is the fourth planet from the Sun and the second-smallest planet in the Solar System after Mercury.
Mars and Orbital resonance · Mars and Planet ·
Mercury (planet)
Mercury is the smallest and innermost planet in the Solar System.
Mercury (planet) and Orbital resonance · Mercury (planet) and Planet ·
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.
Monthly Notices of the Royal Astronomical Society and Orbital resonance · Monthly Notices of the Royal Astronomical Society and Planet ·
Moons of Saturn
The moons of Saturn are numerous and diverse, ranging from tiny moonlets less than 1 kilometer across to the enormous Titan, which is larger than the planet Mercury.
Moons of Saturn and Orbital resonance · Moons of Saturn and Planet ·
Moons of Uranus
Uranus is the seventh planet of the Solar System; it has 27 known moons, all of which are named after characters from the works of William Shakespeare and Alexander Pope.
Moons of Uranus and Orbital resonance · Moons of Uranus and Planet ·
Natural satellite
A natural satellite or moon is, in the most common usage, an astronomical body that orbits a planet or minor planet (or sometimes another small Solar System body).
Natural satellite and Orbital resonance · Natural satellite and Planet ·
Nature (journal)
Nature is a British multidisciplinary scientific journal, first published on 4 November 1869.
Nature (journal) and Orbital resonance · Nature (journal) and Planet ·
Neptune
Neptune is the eighth and farthest known planet from the Sun in the Solar System.
Neptune and Orbital resonance · Neptune and Planet ·
Orbit
In physics, an orbit is the gravitationally curved trajectory of an object, such as the trajectory of a planet around a star or a natural satellite around a planet.
Orbit and Orbital resonance · Orbit and Planet ·
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.
Orbital eccentricity and Orbital resonance · Orbital eccentricity and Planet ·
Orbital inclination
Orbital inclination measures the tilt of an object's orbit around a celestial body.
Orbital inclination and Orbital resonance · Orbital inclination and Planet ·
Orbital node
An orbital node is either of the two points where an orbit intersects a plane of reference to which it is inclined.
Orbital node and Orbital resonance · Orbital node and Planet ·
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.
Orbital period and Orbital resonance · Orbital period and Planet ·
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.
Orbital resonance and Perihelion and aphelion · Perihelion and aphelion and Planet ·
Planetesimal
Planetesimals are solid objects thought to exist in protoplanetary disks and in debris disks.
Orbital resonance and Planetesimal · Planet and Planetesimal ·
Pluto
Pluto (minor planet designation: 134340 Pluto) is a dwarf planet in the Kuiper belt, a ring of bodies beyond Neptune.
Orbital resonance and Pluto · Planet and Pluto ·
Retrograde and prograde motion
Retrograde motion in astronomy is, in general, orbital or rotational motion of an object in the direction opposite the rotation of its primary, that is the central object (right figure).
Orbital resonance and Retrograde and prograde motion · Planet and Retrograde and prograde motion ·
Rhea (moon)
Rhea (Ῥέᾱ) is the second-largest moon of Saturn and the ninth-largest moon in the Solar System.
Orbital resonance and Rhea (moon) · Planet and Rhea (moon) ·
Ring system
A ring system is a disc or ring orbiting an astronomical object that is composed of solid material such as dust and moonlets, and is a common component of satellite systems around giant planets.
Orbital resonance and Ring system · Planet and Ring system ·
Rings of Saturn
The rings of Saturn are the most extensive ring system of any planet in the Solar System.
Orbital resonance and Rings of Saturn · Planet and Rings of Saturn ·
Saturn
Saturn is the sixth planet from the Sun and the second-largest in the Solar System, after Jupiter.
Orbital resonance and Saturn · Planet and Saturn ·
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.
Orbital resonance and Semi-major and semi-minor axes · Planet and Semi-major and semi-minor axes ·
Solar System
The Solar SystemCapitalization of the name varies.
Orbital resonance and Solar System · Planet and Solar System ·
Springer Science+Business Media
Springer Science+Business Media or Springer, part of Springer Nature since 2015, is a global publishing company that publishes books, e-books and peer-reviewed journals in science, humanities, technical and medical (STM) publishing.
Orbital resonance and Springer Science+Business Media · Planet and Springer Science+Business Media ·
Super-Earth
A super-Earth is an extrasolar planet with a mass higher than Earth's, but substantially below the masses of the Solar System's ice giants, Uranus and Neptune, which have masses of 15 and 17 times Earth's, respectively.
Orbital resonance and Super-Earth · Planet and Super-Earth ·
Tethys (moon)
Tethys (or Saturn III) is a mid-sized moon of Saturn about across.
Orbital resonance and Tethys (moon) · Planet and Tethys (moon) ·
Tidal force
The tidal force is an apparent force that stretches a body towards the center of mass of another body due to a gradient (difference in strength) in gravitational field from the other body; it is responsible for the diverse phenomena, including tides, tidal locking, breaking apart of celestial bodies and formation of ring systems within Roche limit, and in extreme cases, spaghettification of objects.
Orbital resonance and Tidal force · Planet and Tidal force ·
Tidal locking
Tidal locking (also called gravitational locking or captured rotation) occurs when the long-term interaction between a pair of co-orbiting astronomical bodies drives the rotation rate of at least one of them into the state where there is no more net transfer of angular momentum between this body (e.g. a planet) and its orbit around the second body (e.g. a star); this condition of "no net transfer" must be satisfied over the course of one orbit around the second body.
Orbital resonance and Tidal locking · Planet and Tidal locking ·
Titan (moon)
Titan is the largest moon of Saturn.
Orbital resonance and Titan (moon) · Planet and Titan (moon) ·
Transit of Venus
A transit of Venus across the Sun takes place when the planet Venus passes directly between the Sun and a superior planet, becoming visible against (and hence obscuring a small portion of) the solar disk.
Orbital resonance and Transit of Venus · Planet and Transit of Venus ·
Uranus
Uranus is the seventh planet from the Sun.
Orbital resonance and Uranus · Planet and Uranus ·
Venus
Venus is the second planet from the Sun, orbiting it every 224.7 Earth days.
Orbital resonance and Venus · Planet and Venus ·
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.
The list above answers the following questions
- What Orbital resonance and Planet have in common
- What are the similarities between Orbital resonance and Planet
Orbital resonance and Planet Comparison
Orbital resonance has 188 relations, while Planet has 397. As they have in common 57, the Jaccard index is 9.74% = 57 / (188 + 397).
References
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