Zsigmondy is a crater that exists on an astronomical body that orbits which planet ?
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Zsigmondy (crater) Zsigmondy is a lunar crater located beyond the northwestern limb on the far side of the Moon. Attached to the southeastern rim of the crater is the crater Omar Khayyam, which lies within the much larger Poczobutt. Farther to the east, along the north rim of Poczobutt, is Smoluchowski.
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Moon The Moon is an astronomical body that orbits planet Earth, being Earth's only permanent natural satellite. It is the fifth-largest natural satellite in the Solar System, and the largest among planetary satellites relative to the size of the planet that it orbits (its primary). Following Jupiter's satellite Io, the Moon is second-densest satellite among those whose densities are known.
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Barycenter The barycenter (or barycentre; from the Ancient Greek βαρύς "heavy" + κέντρον "centre") is the center of mass of two or more bodies that are orbiting each other, which is the point around which they both orbit. It is an important concept in fields such as astronomy and astrophysics. The distance from a body's center of mass to the barycenter can be calculated as a simple two-body problem.
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Garni (crater) Garni is an impact crater on Mars, in which, according to NASA, there is evidence of liquid water. In the press release of its finding on 28 September 2015, NASA considered it "the latest of many breakthroughs" in their Mars exploration. NASA and the US Geological Survey named the crater after the Armenian village of Garni. The naming was approved and adopted by the International Astronomical Union (IAU) on April 24, 2015.
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Copernican period The Copernican Period in the lunar geologic timescale runs from approximately 1.1 billion years ago to the present day. The base of the Copernican period is defined by impact craters that possess bright optically immature ray systems. The crater Copernicus is a prominent example of rayed crater, but it does not mark the base of the Copernican period.
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2098 Zyskin 2098 Zyskin, provisional designation 1972 QE, is a vestoid asteroid from the inner regions of the asteroid belt, approximately 10 kilometers in diameter. It was discovered by Russian–Ukrainian astronomer Lyudmila Zhuravleva at the Crimean Astrophysical Observatory in Nauchnyj on 18 August 1972. The asteroid was named for surgeon Lev Zyskin
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Moons (disambiguation) Moons are celestial bodies that orbit planets or smaller bodies.
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Eddie (crater) Eddie Crater is a crater in the Elysium quadrangle of Mars at 12.3° north latitude and 217.9° west longitude. It is 89 km in diameter and was named after Lindsay Eddie, a South African astronomer (1845–1913).
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Einstein (crater) Einstein is a large lunar crater that lies along the western limb of the Moon, making it difficult to observe from the Earth. The visibility of this formation is affected by libration effects, but even under the best conditions not much detail can be observed except from lunar orbit. Nearby craters of note include Moseley just to the north, Dalton along the eastern rim, Vasco da Gama just to the southeast, and Bohr to the south-southeast. The formation Vallis Bohr is visible to the south.
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Planetary geology Planetary geology, alternatively known as astrogeology or exogeology, is a planetary science discipline concerned with the geology of the celestial bodies such as the planets and their moons, asteroids, comets, and meteorites. Although the geo- prefix typically indicates topics of or relating to the Earth, planetary geology is named as such for historical and convenience reasons; applying geological science to other planetary bodies. Due to the types of investigations involved, it is also closely linked with Earth-based geology.
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(225088) 2007 OR10 (225088) 2007 OR is a trans-Neptunian object (TNO) orbiting the Sun in the scattered disc, approximately 1500 kilometers in diameter. It is the third-largest known body in the Solar System beyond the orbit of Neptune, and continues to be the largest known body in the Solar System without a name. According to estimates as of May 2016, it is slightly larger than Makemake or Haumea , and is hence almost certainly a dwarf planet. It has one known moon.
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Non-inclined orbit A non-inclined orbit is an orbit coplanar with a plane of reference. The orbital inclination is 0° for prograde orbits, and π (180°) for retrograde ones. If the plane of reference is a massive spheroid body's equatorial plane, these orbits are called equatorial; if the plane of reference is the ecliptic plane, they are called ecliptic.
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Kepler-11 Kepler-11 is a Sun-like star slightly larger than the Sun in the constellation Cygnus, located some 2,000 light years from Earth. It is located within the field of vision of the Kepler spacecraft, the satellite that NASA's Kepler Mission uses to detect planets that may be transiting their stars. Announced on February 2, 2011, the star system is among the most compact and flattest systems yet discovered. It is the first discovered case of a star system with six transiting planets. All discovered planets are larger than Earth, with the larger ones being about Neptune's size.
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Cézanne (crater) Cézanne is a crater on Mercury. It has a diameter of 75 kilometers. Its name was adopted by the International Astronomical Union in 1985. Cézanne is named for the French artist Paul Cézanne, who lived from 1839 to 1936.
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Minor planet A minor planet is an astronomical object in direct orbit around the Sun that is neither a planet nor exclusively classified as a comet. Minor planets can be dwarf planets, asteroids, trojans, centaurs, Kuiper belt objects, and other trans-Neptunian objects. As of 2017, the orbits of 734,274 minor planets were archived at the Minor Planet Center, 496,815 of which had received permanent numbers ).
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Astronomical object An astronomical object or celestial object is a naturally occurring physical entity, association, or structure that exists in the observable universe. In astronomy, the terms "object" and "body" are often used interchangeably. However, an astronomical body or celestial body is a single, tightly bound contiguous entity, while an astronomical or celestial "object" is a complex, less cohesively bound structure, that may consist of multiple bodies or even other objects with substructures.
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2010 RF43 2010 RF is a trans-Neptunian object of the scattered disc orbiting in the outermost regions of the Solar System, approximately 600 kilometers in diameter. With an absolute magnitude of 3.7, it was first observed on 9 September 2010, by astronomers at the La Silla Observatory in northern Chile. Astronomer Mike Brown lists it as highly likely a dwarf planet.
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Gravity well A gravity well or gravitational well is a conceptual model of the gravitational field surrounding a body in space – the more massive the body, the deeper and more extensive the gravity well associated with it. The Sun is very massive, relative to other bodies in the Solar System, so the corresponding gravity well that surrounds it appears "deep" and far-reaching. The gravity wells of asteroids and small moons, conversely, are often depicted as very shallow. Anything on the surface of a planet or moon is considered to be at the bottom of that celestial body's gravity well, and so escaping the effects of gravity from such a planet or moon (to enter outer space) is sometimes called "climbing out of the gravity well". The deeper a gravity well is, the more energy any space-bound "climber" must use to escape it.
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Crater of eternal darkness A crater of eternal darkness is a point on a body within the Solar System which is always in darkness. Such a crater must have a low altitude, and be on a body with very small axial tilt.
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Rayya (crater) Rayya is an impact crater on the southern hemisphere of Saturn's moon Enceladus. Rayya was first observed in "Cassini" images during that mission's March 2005 flyby of Enceladus. It is located at 32.5° South Latitude, 178.4° West Longitude, and is 9 kilometers across. "Cassini" observed numerous criss-crossing sets of fractures cutting across Rayya, forming canyons several hundred meters deep along the crater's rim.
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Osculating orbit In astronomy, and in particular in astrodynamics, the osculating orbit of an object in space at a given moment in time is the gravitational Kepler orbit (i.e. ellipse or other conic) that it "would have" about its central body if perturbations were not present. That is, it is the orbit that coincides with the current orbital state vectors (position and velocity).
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Ariadne (crater) Ariadne Crater is a crater on Venus. Its central peak serves as the prime meridian of the planet, a status formerly held by Eve Crater until relocated.