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Encyclopedia > 1866 Sisyphus
1866 Sisyphus
Discovery A
Discoverer Paul Wild
Discovery date Dec 5, 1972
Alternate
designations
1972 XA B
Category Apollo asteroid
Orbital elements C D
Epoch Dec 1, 2005 (JD 2453705.5)
Eccentricity (e) 0.539
Semi-major axis (a) 283.343 Gm (1.8940 AU)
Perihelion (q) 130.751 Gm (0.874 AU)
Aphelion (Q) 435.936 Gm (2.914 AU)
Orbital period (P) 952.094 d (2.61 a)
Mean orbital speed  ? km/s
Inclination (i) 41.181°
Longitude of the
ascending node
(Ω)
63.600°
Argument of
perihelion
(ω)
293.033°
Mean anomaly (M) 261.365°
Physical characteristics
Dimensions 8.5 km
Mass  ?? kg
Density  ? g/cm³
Surface gravity  ? m/s²
Escape velocity  ? km/s
Rotation period .1 d
Spectral class  ?
Absolute magnitude  ?
Albedo .160
Mean surface
temperature
~? K

1866 Sisyphus (sis'-ə-fəs) is an Apollo asteroid which, at approximately 10 km in diameter, is the largest of the Earth-crossing asteroids. It is comparable in size to the Chicxulub object whose impact killed off the dinosaurs. There are various people named Paul Wild, including two astronomers: Prof. ... December 5 is the 339th day (340th in leap years) of the year in the Gregorian calendar. ... 1972 (MCMLXXII) was a leap year that started on a Saturday. ... The provisional designation of comets and asteroids are similar to each other: they both follow a pattern set in 1925 by the Minor Planet Center of the IAU. Historical designations At first, astronomers strove to assign symbols to the minor planets: 1 Ceres a stylized sickle 2 Pallas a lozenge... Minor planets, or planetoids are minor bodies of the Solar system orbiting the Sun (or of other planetary systems orbiting other stars) that are larger than meteoroids (the largest of which might be taken to be around 10 meters or so across) but smaller than major planets (Mercury having a... The Apollo asteroid 25143 Itokawa. ... In astronomy, an epoch is a moment in time for which celestial coordinates or orbital elements are specified. ... 2005 (MMV) is a common year starting on Saturday of the Gregorian calendar. ... The Julian day or Julian day number (JDN) is the number of days that have elapsed since 12 noon Greenwich Mean Time (UT or TT) on Monday, January 1, 4713 BC in the proleptic Julian calendar . ... In astrodynamics, under standard assumptions any orbit must be of conic section shape. ... In geometry, the semi-major axis (also semimajor axis) a applies to ellipses and hyperbolas. ... Giga (symbol: G) is a prefix in the SI system of units denoting 109, or 1 000 000 000. ... The metre (or meter) (symbol: m) is the SI base unit of length. ... The astronomical unit (AU or au or a. ... This article is about several astronomical terms (apogee & perigee, aphelion & perihelion, generic equivalents based on apsis, and related but rarer terms. ... This article is about several astronomical terms (apogee & perigee, aphelion & perihelion, generic equivalents based on apsis, and related but rarer terms. ... The orbital period is the time it takes a planet (or another object) to make one full orbit. ... See also Day (language) A day (symbol: d) is a unit of time. ... In astronomy, a Julian year is a unit of time defined as exactly 365. ... The orbital speed of a body, generally a planet, a natural satellite, an artificial satellite, or a multiple star, is the speed at which it orbits around the barycenter of a system, usually around a more massive body. ... The second (symbol: s) is the SI base unit of time. ... Inclination is one of the six orbital parameters describing the shape and orientation of a celestial orbit and is the angular distance of the orbital plane from the plane of the reference (usually planets equator or the ecliptic), stated in degrees. ... A degree (in full, a degree of arc), usually symbolized °, is a measurement of plane angle, representing 1/360 of a full rotation. ... The Longitude of the ascending node () is one of the orbital elements used to specify the orbit of an object in space. ... The argument of the perihelion is one of the orbital elements describing the orbit of a planet. ... In the study of orbital dynamics the mean anomaly is a measure of time, specific to the orbiting body p, which is a multiple of 2π radians at and only at periapsis. ... Mass is a property of physical objects that, roughly speaking, measures the amount of matter they contain. ... The international prototype, made of platinum-iridium, which is kept at the BIPM under conditions specified by the 1st CGPM in 1889. ... Density (symbol: ρ - Greek: rho) is a measure of mass per unit of volume. ... A cubic centimetre (cm3) is an SI derived unit of volume, equal to the volume of a cube with side length of 1 centi metre. ... Gravity is the force of attraction between massive particles. ... In physics, for a given gravitational field and a given position, the escape velocity is the minimum speed an object without propulsion, at that position, needs to have to move away indefinitely from the source of the field, as opposed to falling back or staying in an orbit within a... In astronomy, a rotation period is the time an astronomical object takes to complete one revolution around its rotation axis. ... Asteroids are assigned a type based on spectral shape, color, and sometimes albedo. ... In astronomy, absolute magnitude is the apparent magnitude, m, an object would have if it were at a standardized distance away. ... The albedo is a measure of reflectivity of a surface or body. ... Temperature is the physical property of a system which underlies the common notions of hot and cold; the material with the higher temperature is said to be hotter. ... The kelvin (symbol: K) is the SI unit of temperature, and is one of the seven SI base units. ... The Apollo asteroid 25143 Itokawa. ... An Earth-crosser asteroid is a Near-Earth asteroid whose orbit crosses that of Earth. ... Radar topography reveals the 180 kilometer (112 mile) wide ring of the crater (image courtesy NASA/JPL-Caltech) Chicxulub Crater is an ancient impact crater buried underneath the Yucatan peninsula, with its center located approximately underneath the town of Chicxulub, Yucatán, Mexico. ... The Cretaceous-Tertiary (K-T or KT) extinction event, also known as the KT boundary, was a period of massive extinction of species, about 65. ... Orders Saurischia    Sauropodomorpha    Theropoda Ornithischia Dinosaurs are animals that dominated the terrestrial ecosystem for over 100 million years. ...


Sisyphus was discovered in 1972 by Paul Wild, and named after the Sisyphus of Greek mythology. 1972 (MCMLXXII) was a leap year that started on a Saturday. ... Prof. ... Sisyphus (also Sísyphos or Sisuphos), in Greek mythology, was the son of Aeolus and Enarete, husband of Merope, and King/Founder of Ephyra (Corinth). ... Greek mythology comprises the collected narratives of Greek gods, goddesses, heroes, and heroines, originally created and spread within an oral-poetic tradition. ...



The minor planetsedit
Vulcanoids | Main belt | Groups and families | Near-Earth objects | Jupiter Trojans
Centaurs | Damocloids | Comets | Trans-Neptunians (Kuiper belt · Scattered disc · Oort cloud)
For other objects and regions, see: Binary asteroids, Asteroid moons and the Solar system
For a complete listing, see: List of asteroids. For pronunciation, see: Pronunciation of asteroid names.

  Results from FactBites:
 
Existentialism (5281 words)
In Greek mythology, Sisyphus, who had once deceived the gods and cheated death, was condemned for eternity to roll a stone up a hill.
Sisyphus is stuck in an eternally pointless task.
We are no different from Sisyphus; and if his punishment makes the afterlife a hell for him, we are already living in that hell.
  More results at FactBites »


 

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