Faster access than browser!Similarities between Planets beyond Neptune and Pluto
Planets beyond Neptune and Pluto have 62 things in common (in Unionpedia): Alan Stern, Apparent magnitude, Apparent retrograde motion, Apsis, Argument of periapsis, Asteroid, Astronomical unit, Blink comparator, Charon (moon), Classical mechanics, Clearing the neighbourhood, Clyde Tombaugh, Comet, Dwarf planet, E. Myles Standish, Earth, Ecliptic, Ernest William Brown, Europa (moon), Flagstaff, Arizona, Ganymede (moon), Gerard Kuiper, Giant planet, Harvard College Observatory, IAU definition of planet, Icarus (journal), International Astronomical Union, Io (moon), James W. Christy, Jupiter, ..., Kuiper belt, Lowell Observatory, Mars, Methane, Michael E. Brown, NASA, Neptune, New Horizons, Orbital eccentricity, Orbital inclination, Percival Lowell, Perturbation (astronomy), Planet, Planets beyond Neptune, Plutino, Precovery, Retrograde and prograde motion, Robert Sutton Harrington, Saturn, Scientific American, Semi-major and semi-minor axes, Solar System, The New York Times, Thomas Jefferson Jackson See, Trans-Neptunian object, Triton (moon), University of Hawaii, Uranus, Urbain Le Verrier, Vesto Slipher, Voyager 2, William Henry Pickering. Expand index (32 more) »
Alan Stern
Sol Alan Stern (born November 22, 1957) is an American engineer and planetary scientist.
Alan Stern and Planets beyond Neptune · Alan Stern and Pluto ·
Apparent magnitude
The apparent magnitude of a celestial object is a number that is a measure of its brightness as seen by an observer on Earth.
Apparent magnitude and Planets beyond Neptune · Apparent magnitude and Pluto ·
Apparent retrograde motion
Apparent retrograde motion is the apparent motion of a planet in a direction opposite to that of other bodies within its system, as observed from a particular vantage point.
Apparent retrograde motion and Planets beyond Neptune · Apparent retrograde motion and Pluto ·
Apsis
An apsis (ἁψίς; plural apsides, Greek: ἁψῖδες) is an extreme point in the orbit of an object.
Apsis and Planets beyond Neptune · Apsis and Pluto ·
Argument of periapsis
The argument of periapsis (also called argument of perifocus or argument of pericenter), symbolized as ω, is one of the orbital elements of an orbiting body.
Argument of periapsis and Planets beyond Neptune · Argument of periapsis and Pluto ·
Asteroid
Asteroids are minor planets, especially those of the inner Solar System.
Asteroid and Planets beyond Neptune · Asteroid and Pluto ·
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 Planets beyond Neptune · Astronomical unit and Pluto ·
Blink comparator
A blink comparator was a viewing apparatus used by astronomers to find differences between two photographs of the night sky.
Blink comparator and Planets beyond Neptune · Blink comparator and Pluto ·
Charon (moon)
Charon, also known as (134340) Pluto I, is the largest of the five known natural satellites of the dwarf planet Pluto.
Charon (moon) and Planets beyond Neptune · Charon (moon) and Pluto ·
Classical mechanics
Classical mechanics describes the motion of macroscopic objects, from projectiles to parts of machinery, and astronomical objects, such as spacecraft, planets, stars and galaxies.
Classical mechanics and Planets beyond Neptune · Classical mechanics and Pluto ·
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 Planets beyond Neptune · Clearing the neighbourhood and Pluto ·
Clyde Tombaugh
Clyde William Tombaugh (February 4, 1906January 17, 1997) was an American astronomer.
Clyde Tombaugh and Planets beyond Neptune · Clyde Tombaugh and Pluto ·
Comet
A comet is an icy small Solar System body that, when passing close to the Sun, warms and begins to release gases, a process called outgassing.
Comet and Planets beyond Neptune · Comet and Pluto ·
Dwarf planet
A dwarf planet is a planetary-mass object that is neither a planet nor a natural satellite.
Dwarf planet and Planets beyond Neptune · Dwarf planet and Pluto ·
E. Myles Standish
Erland Myles Standish, Jr. (born March 5, 1939) is a mathematical astronomer and a former professor at Yale University.
E. Myles Standish and Planets beyond Neptune · E. Myles Standish and Pluto ·
Earth
Earth is the third planet from the Sun and the only astronomical object known to harbor life.
Earth and Planets beyond Neptune · Earth and Pluto ·
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 Planets beyond Neptune · Ecliptic and Pluto ·
Ernest William Brown
Ernest William Brown FRS (29 November 1866 – 22 July 1938) was an English mathematician and astronomer, who spent the majority of his career working in the United States and became a naturalised American citizen in 1923.
Ernest William Brown and Planets beyond Neptune · Ernest William Brown and Pluto ·
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 Planets beyond Neptune · Europa (moon) and Pluto ·
Flagstaff, Arizona
Flagstaff is a city in and the county seat of Coconino County in northern Arizona, in the southwestern United States.
Flagstaff, Arizona and Planets beyond Neptune · Flagstaff, Arizona and Pluto ·
Ganymede (moon)
Ganymede (Jupiter III) is the largest and most massive moon of Jupiter and in the Solar System.
Ganymede (moon) and Planets beyond Neptune · Ganymede (moon) and Pluto ·
Gerard Kuiper
Gerard Peter Kuiper (born Gerrit Pieter Kuiper; December 7, 1905 – December 23, 1973) was a Dutch–American astronomer, planetary scientist, selenographer, author and professor.
Gerard Kuiper and Planets beyond Neptune · Gerard Kuiper and Pluto ·
Giant planet
A giant planet is any massive planet.
Giant planet and Planets beyond Neptune · Giant planet and Pluto ·
Harvard College Observatory
The Harvard College Observatory (HCO) is an institution managing a complex of buildings and multiple instruments used for astronomical research by the Harvard University Department of Astronomy.
Harvard College Observatory and Planets beyond Neptune · Harvard College Observatory and Pluto ·
IAU definition of planet
The International Astronomical Union (IAU) defined in August 2006 that, in the Solar System, a planet is a celestial body which.
IAU definition of planet and Planets beyond Neptune · IAU definition of planet and Pluto ·
Icarus (journal)
Icarus is a scientific journal dedicated to the field of planetary science.
Icarus (journal) and Planets beyond Neptune · Icarus (journal) and Pluto ·
International Astronomical Union
The International Astronomical Union (IAU; Union astronomique internationale, UAI) is an international association of professional astronomers, at the PhD level and beyond, active in professional research and education in astronomy.
International Astronomical Union and Planets beyond Neptune · International Astronomical Union and Pluto ·
Io (moon)
Io (Jupiter I) is the innermost of the four Galilean moons of the planet Jupiter.
Io (moon) and Planets beyond Neptune · Io (moon) and Pluto ·
James W. Christy
James Walter "Jim" Christy (born September 15, 1938) is an American astronomer.
James W. Christy and Planets beyond Neptune · James W. Christy and Pluto ·
Jupiter
Jupiter is the fifth planet from the Sun and the largest in the Solar System.
Jupiter and Planets beyond Neptune · Jupiter and Pluto ·
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 Planets beyond Neptune · Kuiper belt and Pluto ·
Lowell Observatory
Lowell Observatory is an astronomical observatory in Flagstaff, Arizona, United States.
Lowell Observatory and Planets beyond Neptune · Lowell Observatory and Pluto ·
Mars
Mars is the fourth planet from the Sun and the second-smallest planet in the Solar System after Mercury.
Mars and Planets beyond Neptune · Mars and Pluto ·
Methane
Methane is a chemical compound with the chemical formula (one atom of carbon and four atoms of hydrogen).
Methane and Planets beyond Neptune · Methane and Pluto ·
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.
Michael E. Brown and Planets beyond Neptune · Michael E. Brown and Pluto ·
NASA
The National Aeronautics and Space Administration (NASA) is an independent agency of the executive branch of the United States federal government responsible for the civilian space program, as well as aeronautics and aerospace research.
NASA and Planets beyond Neptune · NASA and Pluto ·
Neptune
Neptune is the eighth and farthest known planet from the Sun in the Solar System.
Neptune and Planets beyond Neptune · Neptune and Pluto ·
New Horizons
New Horizons is an interplanetary space probe that was launched as a part of NASA's New Frontiers program.
New Horizons and Planets beyond Neptune · New Horizons and Pluto ·
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 Planets beyond Neptune · Orbital eccentricity and Pluto ·
Orbital inclination
Orbital inclination measures the tilt of an object's orbit around a celestial body.
Orbital inclination and Planets beyond Neptune · Orbital inclination and Pluto ·
Percival Lowell
Percival Lawrence Lowell (March 13, 1855 – November 12, 1916) was an American businessman, author, mathematician, and astronomer who fueled speculation that there were canals on Mars.
Percival Lowell and Planets beyond Neptune · Percival Lowell and Pluto ·
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.
Perturbation (astronomy) and Planets beyond Neptune · Perturbation (astronomy) and Pluto ·
Planet
A planet is an astronomical body orbiting a star or stellar remnant that is massive enough to be rounded by its own gravity, is not massive enough to cause thermonuclear fusion, and has cleared its neighbouring region of planetesimals.
Planet and Planets beyond Neptune · Planet and Pluto ·
Planets beyond Neptune
Following the discovery of the planet Neptune in 1846, there was considerable speculation that another planet might exist beyond its orbit.
Planets beyond Neptune and Planets beyond Neptune · Planets beyond Neptune and Pluto ·
Plutino
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.
Planets beyond Neptune and Plutino · Plutino and Pluto ·
Precovery
In astronomy, precovery (short for pre-discovery recovery) is the process of finding the image of an object in old archived images or photographic plates for the purpose of calculating a more accurate orbit.
Planets beyond Neptune and Precovery · Pluto and Precovery ·
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).
Planets beyond Neptune and Retrograde and prograde motion · Pluto and Retrograde and prograde motion ·
Robert Sutton Harrington
Robert Sutton Harrington (October 21, 1942 – January 23, 1993) was an American astronomer who worked at the United States Naval Observatory (USNO).
Planets beyond Neptune and Robert Sutton Harrington · Pluto and Robert Sutton Harrington ·
Saturn
Saturn is the sixth planet from the Sun and the second-largest in the Solar System, after Jupiter.
Planets beyond Neptune and Saturn · Pluto and Saturn ·
Scientific American
Scientific American (informally abbreviated SciAm) is an American popular science magazine.
Planets beyond Neptune and Scientific American · Pluto and Scientific American ·
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.
Planets beyond Neptune and Semi-major and semi-minor axes · Pluto and Semi-major and semi-minor axes ·
Solar System
The Solar SystemCapitalization of the name varies.
Planets beyond Neptune and Solar System · Pluto and Solar System ·
The New York Times
The New York Times (sometimes abbreviated as The NYT or The Times) is an American newspaper based in New York City with worldwide influence and readership.
Planets beyond Neptune and The New York Times · Pluto and The New York Times ·
Thomas Jefferson Jackson See
Thomas Jefferson Jackson (T. J. J.) See (February 19, 1866 – July 4, 1962) was an American astronomer whose promulgated theories in astronomy and physics were eventually disproven.
Planets beyond Neptune and Thomas Jefferson Jackson See · Pluto and Thomas Jefferson Jackson See ·
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).
Planets beyond Neptune and Trans-Neptunian object · Pluto and Trans-Neptunian object ·
Triton (moon)
Triton is the largest natural satellite of the planet Neptune, and the first Neptunian moon to be discovered.
Planets beyond Neptune and Triton (moon) · Pluto and Triton (moon) ·
University of Hawaii
The University of Hawaiʻi system (formally the University of Hawaiʻi and popularly known as UH) is a public, co-educational college and university system that confers associate, bachelor's, master's, and doctoral degrees through three university campuses, seven community college campuses, an employment training center, three university centers, four education centers and various other research facilities distributed across six islands throughout the State of Hawaii in the United States.
Planets beyond Neptune and University of Hawaii · Pluto and University of Hawaii ·
Uranus
Uranus is the seventh planet from the Sun.
Planets beyond Neptune and Uranus · Pluto and Uranus ·
Urbain Le Verrier
Urbain Jean Joseph Le Verrier (11 March 1811 – 23 September 1877) was a French mathematician who specialized in celestial mechanics and is best known for predicting the existence and position of Neptune using only mathematics.
Planets beyond Neptune and Urbain Le Verrier · Pluto and Urbain Le Verrier ·
Vesto Slipher
Vesto Melvin Slipher (November 11, 1875 – November 8, 1969) was an American astronomer who performed the first measurements of radial velocities for galaxies, providing the empirical basis for the expansion of the universe.
Planets beyond Neptune and Vesto Slipher · Pluto and Vesto Slipher ·
Voyager 2
Voyager 2 is a space probe launched by NASA on August 20, 1977, to study the outer planets.
Planets beyond Neptune and Voyager 2 · Pluto and Voyager 2 ·
William Henry Pickering
William Henry Pickering (February 15, 1858 – January 16, 1938) was an American astronomer.
Planets beyond Neptune and William Henry Pickering · Pluto and William Henry Pickering ·
The list above answers the following questions
- What Planets beyond Neptune and Pluto have in common
- What are the similarities between Planets beyond Neptune and Pluto
Planets beyond Neptune and Pluto Comparison
Planets beyond Neptune has 155 relations, while Pluto has 244. As they have in common 62, the Jaccard index is 15.54% = 62 / (155 + 244).
References
This article shows the relationship between Planets beyond Neptune and Pluto. To access each article from which the information was extracted, please visit:
