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Encyclopedia > 85 Io
85 Io
Discovery
Discovered by: C. H. F. Peters
Discovery date: September 19, 1865
Orbital characteristics
Epoch March 6, 2006 (JD 2453800.5)
Aphelion 473.341 Gm (3.164 AU)
Perihelion: 320.334 Gm (2.141 AU)
Semi-major axis: 396.837 Gm (2.652 AU)
Eccentricity: 0.193
Orbital period: 1578.081 d (4.32 a)
Avg. orbital speed: 18.12 km/s
Mean anomaly: 206.947°
Inclination: 11.967°
Longitude of ascending node: 203.440°
Argument of perihelion: 122.293°
Physical characteristics
Dimensions: 180×160×160 km[1][4]
Mass: ~3.4×1018 (estimate)
Mean density: ~1.4 g/cm³ (estimate)[5]
Equatorial surface gravity: ~0.028 m/s² (estimate)
Escape velocity: ~0.07 km/s (estimate)
Rotation period: 0.2864 d (6.875 h) [2]
Albedo: 0.067 [3]
Temperature: ~172 K
max: 272K (-2° C)
Spectral type: C-type asteroid
Absolute magnitude: 7.61

85 Io (eye'-oh) is a large, dark Main belt asteroid of the C spectral class. It is probably a primitive body composed of carbonates. Like 70 Panopaea it orbits within the Eunomia asteroid family but it is not related to the shattered parent body. Christian Heinrich Friedrich Peters (September 19, 1813 – July 18, 1890) was an American astronomer, and one of the first to discover asteroids. ... is the 262nd day of the year (263rd in leap years) in the Gregorian calendar. ... 1865 (MDCCCLXV) is a common year starting on Sunday. ... Two bodies with a slight difference in mass orbiting around a common barycenter. ... In astronomy, an epoch is a moment in time for which celestial coordinates or orbital elements are specified. ... is the 65th day of the year (66th in leap years) in the Gregorian calendar. ... Year 2006 (MMVI) was a common year starting on Sunday of the Gregorian calendar. ... “JDN” redirects here. ... A diagram of Keplerian orbital elements. ... A diagram of Keplerian orbital elements. ... The semi-major axis of an ellipse In geometry, the term semi-major axis (also semimajor axis) is used to describe the dimensions of ellipses and hyperbolae. ... Look up giga- in Wiktionary, the free dictionary. ... This article is about the unit of length. ... The astronomical unit (AU or au or a. ... (This page refers to eccitricity in astrodynamics. ... The orbital period is the time it takes a planet (or another object) to make one full orbit. ... Look up day in Wiktionary, the free dictionary. ... 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. ... This article is about the unit of time. ... 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. ... For the science fiction novella by William Shunn, see Inclination (novella). ... This article describes the unit of angle. ... The Longitude of the ascending node (☊, also noted Ω) is one of the orbital elements used to specify the orbit of an object in space. ... The argument of periapsis (ω) is the orbital element describing the angle between an orbiting bodys ascending node (the point where the body crosses the plane of reference from South to North) and its periapsis (the point of closest approach to the central body), measured in the orbital plane and... This article or section is in need of attention from an expert on the subject. ... For other uses, see Density (disambiguation). ... 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. ... The surface gravity of a Killing horizon is the acceleration, as exerted at infinity, needed to keep an object at the horizon. ... Space Shuttle Atlantis launches on mission STS-71. ... In astronomy, a rotation period is the time an astronomical object takes to complete one revolution around its rotation axis relative to the background stars. ... The hour (symbol: h) is a unit of time. ... Albedo is the ratio of reflected to incident electromagnetic radiation. ... For other uses, see Temperature (disambiguation). ... For other uses, see Kelvin (disambiguation). ... Celsius is, or relates to, the Celsius temperature scale (previously known as the centigrade scale). ... C-type asteroids are carbonaceous asteroids. ... In astronomy, absolute magnitude is the apparent magnitude, m, an object would have if it were at a standard luminosity distance away from us, in the absence of interstellar extinction. ... The asteroid belt is a region of the solar system falling roughly between the planets Mars and Jupiter where the greatest concentration of asteroid orbits can be found. ... 253 Mathilde, a C-type asteroid. ... C-type asteroids are carbonaceous asteroids. ... In organic chemistry, a carbonate is a salt of carbonic acid. ... 70 Panopaea is a large main belt asteroid. ... The Eunomia family is a group of several hundred asteroids that share similar orbital and spectral properties. ...


Io is a retrograde rotator, with its pole pointing towards one of ecliptic coordinates (β, λ) = (-45°, 105°) or (-15°, 295°) with a 10° uncertainty[1]. This gives an axial tilt of about 125° or 115°, respectively. Its shape is quite regular. Prograde motion is the motion of a planetary body in a direction similar to that of other bodies within its system, and is sometimes called direct motion, especially in astrology. ... The ecliptic coordinate system is a celestial coordinate system that uses the ecliptic for its fundamental plane. ... In astronomy, axial tilt is the inclination angle of a planets rotational axis in relation to a perpendicular to its orbital plane. ...


It was discovered by C. H. F. Peters on September 19, 1865 and named after Io, a lover of Zeus in Greek mythology. Christian Heinrich Friedrich Peters (September 19, 1813 – July 18, 1890) was an American astronomer, and one of the first to discover asteroids. ... is the 262nd day of the year (263rd in leap years) in the Gregorian calendar. ... 1865 (MDCCCLXV) is a common year starting on Sunday. ... Hermes, Io (as cow) and Argus, black-figure amphora, 540–530 BC, Staatliche Antikensammlungen (Inv. ... For other uses, see Zeus (disambiguation). ... The bust of Zeus found at Otricoli (Sala Rotonda, Museo Pio-Clementino, Vatican) Greek mythology is the body of stories belonging to the Ancient Greeks concerning their gods and heroes, the nature of the world and the origins and significance of their own cult and ritual practices. ...


An Ionian diameter of 178 kilometres was measured from an occultation of a star on December 10, 1995 [4]. “km” redirects here. ... In this July, 1997 still frame captured from video, the bright star Aldebaran has just reappeared on the dark limb of the waning crescent moon in this predawn occultation. ... STAR is an acronym for: Organizations Society of Ticket Agents and Retailers], the self-regulatory body for the entertainment ticket industry in the UK. Society for Telescopy, Astronomy, and Radio, a non-profit New Jersey astronomy club. ... is the 344th day of the year (345th in leap years) in the Gregorian calendar. ... Year 1995 (MCMXCV) was a common year starting on Sunday (link will display full 1995 Gregorian calendar). ...


Io is also the name of the volcanic satellite of Jupiter. With a two-digit number and a two-letter name, 85 Io has the shortest designation of all minor planets. Atmosphere Surface pressure: trace Composition: 90% sulfur dioxide Io (eye-oe, IPA: , Greek Ῑώ) is the innermost of the four Galilean moons of Jupiter and, with a diameter of 3,642 kilometers, is the fourth largest moon in the Solar System. ... This article is about volcanoes in geology. ... A natural satellite is an object that orbits a planet or other body larger than itself and which is not man-made. ... Atmospheric characteristics Atmospheric pressure 70 kPa Hydrogen ~86% Helium ~14% Methane 0. ...


External links

  • shape model deduced from lightcurve

References

  1. J. Torppa et al Shapes and rotational properties of thirty asteroids from photometric data, Icarus, Vol. 164, p. 346 (2003).
  2. PDS lightcurve data
  3. Supplemental IRAS Minor Planet Survey
  4. A. Erikson Photometric observations and modelling of the asteroid 85 Io in conjunction with data from an occultation event during the 1995-96 apparition, Planetary and Space Science, Vol. 47, p. 327 (1999).
  5. G. A. Krasinsky et al Hidden Mass in the Asteroid Belt, Icarus, Vol. 158, p. 98 (2002).
Minor planets
Previous minor planet 85 Io Next minor planet
List of asteroids          Pronunciation

  Results from FactBites:
 
Io - Wikipedia, the free encyclopedia (231 words)
In Greek mythology, Io (IPA [ˈaɪoʊ] or [ˈiːoʊ]) was the daughter of Inachus, a river god.
Io programming language, a prototype-oriented programming language made by Steve Dekorte.
The related I/O is a common abbreviation of Input/output, and is also facetiously taken to mean "Ignorant Operator".
85 Io - definition of 85 Io in Encyclopedia (122 words)
85 Io is a large and dark-colored Main belt asteroid.
Peters on September 19, 1865 and named after Io, a lover of Zeus in Greek mythology.
A diameter of 178 kilometres was measured from an occultation of a star on December 10, 1995.
  More results at FactBites »


 
 

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