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Encyclopedia > 516 Amherstia
516 Amherstia
Discovery A
Discoverer Raymond Smith Dugan
Discovery date September 20, 1903
Alternate
designations
1903 MG; 1938 YO B
Category Main belt
Orbital elements C
Epoch October 22, 2004 (JD 2453300.5)
Eccentricity (e) 0.273
Semi-major axis (a) 401.045 Gm (2.681 AU)
Perihelion (q) 291.483 Gm (1.948 AU)
Aphelion (Q) 510.608 Gm (3.413 AU)
Orbital period (P) 1603.247 d (4.39 a)
Mean orbital speed 17.85 km/s
Inclination (i) 12.956°
Longitude of the
ascending node
(Ω)
328.912°
Argument of
perihelion
(ω)
258.439°
Mean anomaly (M) 139.799°
Physical characteristics D
Dimensions 73.1 km
Mass 4.1×1017 kg
Density 2.0 g/cm³
Surface gravity 0.0204 m/s²
Escape velocity 0.0386 km/s
Rotation period 0.312 d 1
Spectral class M-type asteroid
Absolute magnitude 8.27
Albedo 0.163–0.173 2
Mean surface
temperature
~167 K

516 Amherstia was the 8th asteroid discovered by Raymond Smith Dugan, and was named after Amherst College, his alma mater. Amherstia is a large M-type asteroid, with an estimated diameter of 73 km. It follows an eccentric orbit between Jupiter and Mars, with an orbital period of 4.39 years. Raymond Smith Dugan (May 30, 1878 – August 31, 1940) was an American astronomer and a graduate of Amherst College in Massachusetts (1899). ... September 20 is the 263rd day of the year (264th in leap years). ... 1903 (MCMIII) was a common year starting on Thursday (see link for calendar). ... 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 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. ... In astronomy, an epoch is a moment in time for which celestial coordinates or orbital elements are specified. ... October 22 is the 295th day of the year (296th in leap years) in the Gregorian Calendar, with 70 days remaining. ... 2004 (MMIV) was a leap year starting on Thursday 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 (Commonwealth English) or meter (American English) (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. ... A day (symbol: d) is a unit of time equal to 24 hours. ... 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. ... Look up Second in Wiktionary, the free dictionary 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, arc degree, or arcdegree), 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. ... For the majority of numbered asteroids, almost nothing is known apart from a few physical parameters. ... 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 a force of attraction that acts between bodies that have mass. ... 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. ... M-type asteroids are metallic asteroids; they are moderately bright (albedo . ... In astronomy, absolute magnitude is the apparent magnitude, m, an object would have if it were at a standard luminosity distance away from us. ... 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. ... Raymond Smith Dugan (May 30, 1878 – August 31, 1940) was an American astronomer and a graduate of Amherst College in Massachusetts (1899). ... Amherst College is an independent liberal arts college in Amherst, Massachusetts, USA. It is the third oldest college in Massachusetts. ... Alma mater is Latin for El Sahddai. It was used in ancient Rome as a title for the Father God, and in Medieval Christianity for the Holy Emmanuel. ... M-type asteroids are metallic asteroids; they are moderately bright (albedo . ... Atmospheric characteristics Atmospheric pressure 70 kPa Hydrogen ~86% Helium ~14% Methane 0. ... Mars is the fourth planet from the Sun in the solar system, named after the Roman god of war (the counterpart of the Greek Ares), on account of its blood red color as viewed in the night sky. ...

… | Previous minor planet | 516 Amherstia | Next minor planet | … 515 Athalia 515 Athalia is a minor planet orbiting the Sun. ... 517 Edith 517 Edith is a minor planet orbiting the Sun. ...



The minor planetsedit
Vulcanoids | Main belt | Groups and families | Near-Earth asteroids | 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:
 
516 Amherstia: Information from Answers.com (163 words)
516 Amherstia was the 8th asteroid discovered by Raymond Smith Dugan, and was named after Amherst College, his alma mater.
Amherstia is a large M-type asteroid, with an estimated diameter of 73 km.
It follows an eccentric orbit between Jupiter and Mars, with an orbital period of 4.39 years.
October 2004 meeting report (680 words)
Also discussed was the report form, which could be completed and returned to Jan Manek of the European Asteroidal Occultation Network (see http://www.euraster.net/).
John gave an in-depth account of some of the work already carried out by the occultation team set up at Armagh Observatory in the autumn of 2001, including the first successful event observed on the island of Ireland on 14 January 2002 when (516) Amherstia occulted the star HIP 36335.
Descriptions were made of planetary occultations of stars and the valuable information that they can yield.
  More results at FactBites »


 
 

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