Faster access than browser!Similarities between (225088) 2007 OR10 and Eris (dwarf planet)
(225088) 2007 OR10 and Eris (dwarf planet) have 27 things in common (in Unionpedia): Albedo, Astronomical unit, Ceres (dwarf planet), David L. Rabinowitz, Deep Ecliptic Survey, Degree (angle), Dwarf planet, Haumea, Julian day, Julian year (astronomy), Kuiper belt, List of Solar System objects most distant from the Sun in 2015, Makemake, Michael E. Brown, Minor-planet moon, Natural satellite, Palomar Observatory, Perihelion and aphelion, Pluto, Precovery, Scattered disc, Solar System, Sun, Trans-Neptunian object, 50000 Quaoar, 90377 Sedna, 90482 Orcus.
Albedo
Albedo (albedo, meaning "whiteness") is the measure of the diffuse reflection of solar radiation out of the total solar radiation received by an astronomical body (e.g. a planet like Earth).
(225088) 2007 OR10 and Albedo · Albedo and Eris (dwarf planet) ·
Astronomical unit
The astronomical unit (symbol: au, ua, or AU) is a unit of length, roughly the distance from Earth to the Sun.
(225088) 2007 OR10 and Astronomical unit · Astronomical unit and Eris (dwarf 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.
(225088) 2007 OR10 and Ceres (dwarf planet) · Ceres (dwarf planet) and Eris (dwarf planet) ·
David L. Rabinowitz
David Lincoln Rabinowitz (born 1960) is an American astronomer, discoverer of minor planets and researcher at Yale University.
(225088) 2007 OR10 and David L. Rabinowitz · David L. Rabinowitz and Eris (dwarf planet) ·
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).
(225088) 2007 OR10 and Deep Ecliptic Survey · Deep Ecliptic Survey and Eris (dwarf planet) ·
Degree (angle)
A degree (in full, a degree of arc, arc degree, or arcdegree), usually denoted by ° (the degree symbol), is a measurement of a plane angle, defined so that a full rotation is 360 degrees.
(225088) 2007 OR10 and Degree (angle) · Degree (angle) and Eris (dwarf planet) ·
Dwarf planet
A dwarf planet is a planetary-mass object that is neither a planet nor a natural satellite.
(225088) 2007 OR10 and Dwarf planet · Dwarf planet and Eris (dwarf planet) ·
Haumea
Haumea, minor-planet designation 136108 Haumea, is a dwarf planet located beyond Neptune's orbit.
(225088) 2007 OR10 and Haumea · Eris (dwarf planet) and Haumea ·
Julian day
Julian day is the continuous count of days since the beginning of the Julian Period and is used primarily by astronomers.
(225088) 2007 OR10 and Julian day · Eris (dwarf planet) and Julian day ·
Julian year (astronomy)
In astronomy, a Julian year (symbol: a) is a unit of measurement of time defined as exactly 365.25 days of SI seconds each.
(225088) 2007 OR10 and Julian year (astronomy) · Eris (dwarf planet) and Julian year (astronomy) ·
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.
(225088) 2007 OR10 and Kuiper belt · Eris (dwarf planet) and Kuiper belt ·
List of Solar System objects most distant from the Sun in 2015
This is a list of Solar System objects most distant from the Sun discovered by December of 2015. The objects are sorted by their approximate heliocentric distance from the Sun in December 2015 (as opposed to those with the greatest calculated aphelion in their orbit).
(225088) 2007 OR10 and List of Solar System objects most distant from the Sun in 2015 · Eris (dwarf planet) and List of Solar System objects most distant from the Sun in 2015 ·
Makemake
Makemake (minor-planet designation 136472 Makemake) is a dwarf planet and perhaps the largest Kuiper belt object in the classical population, with a diameter approximately two thirds that of Pluto.
(225088) 2007 OR10 and Makemake · Eris (dwarf planet) and Makemake ·
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.
(225088) 2007 OR10 and Michael E. Brown · Eris (dwarf planet) and Michael E. Brown ·
Minor-planet moon
A minor-planet moon is an astronomical object that orbits a minor planet as its natural satellite.
(225088) 2007 OR10 and Minor-planet moon · Eris (dwarf planet) and Minor-planet moon ·
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).
(225088) 2007 OR10 and Natural satellite · Eris (dwarf planet) and Natural satellite ·
Palomar Observatory
Palomar Observatory is an astronomical observatory located in San Diego County, California, United States, southeast of Los Angeles, California, in the Palomar Mountain Range.
(225088) 2007 OR10 and Palomar Observatory · Eris (dwarf planet) and Palomar Observatory ·
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.
(225088) 2007 OR10 and Perihelion and aphelion · Eris (dwarf planet) and Perihelion and aphelion ·
Pluto
Pluto (minor planet designation: 134340 Pluto) is a dwarf planet in the Kuiper belt, a ring of bodies beyond Neptune.
(225088) 2007 OR10 and Pluto · Eris (dwarf planet) 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.
(225088) 2007 OR10 and Precovery · Eris (dwarf planet) and Precovery ·
Scattered disc
The scattered disc (or scattered disk) is a distant circumstellar disc in the Solar System that is sparsely populated by icy small solar system bodies, and are a subset of the broader family of trans-Neptunian objects.
(225088) 2007 OR10 and Scattered disc · Eris (dwarf planet) and Scattered disc ·
Solar System
The Solar SystemCapitalization of the name varies.
(225088) 2007 OR10 and Solar System · Eris (dwarf planet) and Solar System ·
Sun
The Sun is the star at the center of the Solar System.
(225088) 2007 OR10 and Sun · Eris (dwarf planet) and Sun ·
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).
(225088) 2007 OR10 and Trans-Neptunian object · Eris (dwarf planet) and Trans-Neptunian object ·
50000 Quaoar
50000 Quaoar, provisional designation, is a non-resonant trans-Neptunian object (cubewano) and possibly a dwarf planet in the Kuiper belt, located in the outermost region of the Solar System.
(225088) 2007 OR10 and 50000 Quaoar · 50000 Quaoar and Eris (dwarf planet) ·
90377 Sedna
90377 Sedna is a large minor planet in the outer reaches of the Solar System that was,, at a distance of about 86 astronomical units (AU) from the Sun, about three times as far as Neptune.
(225088) 2007 OR10 and 90377 Sedna · 90377 Sedna and Eris (dwarf planet) ·
90482 Orcus
90482 Orcus, provisional designation, is a trans-Neptunian object from the Kuiper belt with a large moon, Vanth.
(225088) 2007 OR10 and 90482 Orcus · 90482 Orcus and Eris (dwarf planet) ·
The list above answers the following questions
- What (225088) 2007 OR10 and Eris (dwarf planet) have in common
- What are the similarities between (225088) 2007 OR10 and Eris (dwarf planet)
(225088) 2007 OR10 and Eris (dwarf planet) Comparison
(225088) 2007 OR10 has 47 relations, while Eris (dwarf planet) has 131. As they have in common 27, the Jaccard index is 15.17% = 27 / (47 + 131).
References
This article shows the relationship between (225088) 2007 OR10 and Eris (dwarf planet). To access each article from which the information was extracted, please visit:
