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Encyclopedia > 230 Athamantis
230 Athamantis
Discovery A
Discoverer K. de Ball
Discovery date September 3, 1882
Alternate
designations
1949 WG B
Category Main belt
Orbital elements C
Epoch 30 January 2005 (JD 2453400.5)
Eccentricity (e) 0.062
Semi-major axis (a) 356.347 Gm (2.382 AU)
Perihelion (q) 334.395 Gm (2.235 AU)
Aphelion (Q) 378.299 Gm (2.529 AU)
Orbital period (P) 1342.801 d (3.68 a)
Mean orbital speed 19.3 km/s
Inclination (i) 9.435°
Longitude of the
ascending node
(Ω)
239.979°
Argument of
perihelion
(ω)
138.926°
Mean anomaly (M) 70.608°
Physical characteristics D
Dimensions 109.0 km
Mass unknown
Density unknown
Surface gravity unknown
Escape velocity unknown
Rotation period 24.0055 h
Spectral class S
Absolute magnitude 7.35
Albedo 0.181
Mean surface
temperature
unknown

230 Athamantis is a fairly large Main belt asteroid. It is classified as a S-type asteroid and is probably composed of a mixture of silicates and metals. Leo Anton Karl de Ball (November 23, 1853 – December 12, 1916) was a German-Austrian astronomer. ... September 3 is the 246th day of the year (247th in leap years). ... 1882 was a common year starting on Sunday (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... Image of the main asteroid belt between the orbits of Mars and Jupiter. ... In astronomy, an epoch is a moment in time for which celestial coordinates or orbital elements are specified. ... January 30 is the 30th day of the year in the Gregorian Calendar. ... 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 (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. ... Density (symbol: ρ - Greek: rho) is a measure of mass per unit of volume. ... 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. ... The hour (symbol: h) is a unit of time. ... Asteroids are assigned a type based on spectral shape, color, and sometimes albedo. ... Approximately 17% of all known asteroids are of an S-type (for stony) composition. ... 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. ... Image of the main asteroid belt between the orbits of Mars and Jupiter. ... An asteroid is a small, solid object in our Solar System, orbiting the Sun. ... Approximately 17% of all known asteroids are of an S-type (for stony) composition. ... In chemistry, a silicate is a compound consisting of silicon and oxygen (SixOy), one or more metals, and possibly hydrogen. ... Hot metal work from a blacksmith In chemistry, a metal (Greek: Metallon) is an element that readily forms ions (cations) and has metallic bonds, and metals are sometimes described as a lattice of positive ions (cations) in a cloud of electrons. ...


It was discovered by K. de Ball on September 3, 1882 in Bothkamp. It was his only asteroid discovery. Leo Anton Karl de Ball (November 23, 1853 – December 12, 1916) was a German-Austrian astronomer. ... September 3 is the 246th day of the year (247th in leap years). ... 1882 was a common year starting on Sunday (see link for calendar). ...


It was named after Athamantis, daughter of Athamas the mythical Greek king of Orchomenus. In Greek mythology, Helle figured prominently in the story of Jason and the Argonauts. ... The king of Orchomenus in Greek mythology, Athamas (rich harvest) was married first to the goddess Nephele with whom he had the twins Phrixus and Helle. ... ... Orchomenus is an ancient city of Boeotia in Greece, which was the setting for many early Greek Myths. ...


Aspects

Stationary, than retrograde Opposition Distance to earth Brightness Stationary, than prograde Conjunction to sun
30th October 2004 14th December 2004 1,32763 AE 11,0 mag 27th January 2005 22nd August 2005
27th February 2006 17th April 2006 1,53161 AE 10,6 mag 1st Juni 2006 18th December 2006
12th July 2007 31st August 2007 1,28545 AE 10,1 mag 9th October 2007 15th May 2008
7th December 2008 26th January 2009 1,45007 AE 10,5 mag 11th March 2009 1st October 2009
8th April 2010 25th May 2010 1,47035 AE 10,3 mag 12th July 2010 29th January 2011
7th September 2011 22nd October 2011 1,24895 AE 9,9 mag 29th November 2011 4th July 2012
13th January 2013 6th March 2013 1,52998 AE 10,7 mag 18th April 2013 6th November 2013
19th May 2014 7th July 2014 1,38156 AE 10,3 mag 22nd August 2014 19th March 2015
25th October 2015 9th December 2015 1,31409 AE 10,0 mag 23th January 2016 17th August 2016
22nd February 2017 12th April 2017 1,53556 AE 10,6 mag 26th May 2017 13th December 2017
6th July 2018 24th August 2018 1,29432 AE 10,2 mag 3th October 2018 10th May 2019
3th December 2019 22nd January 2020 1,43642 AE 10,4 mag 6th March 2020 26th September 2020

References

… | Previous minor planet | 230 Athamantis | Next minor planet | … 229 Adelinda is a large, dark outer Main belt asteroid. ... 231 Vindobona is a large Main belt asteroid. ...



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:
 
Athamantis, discovery date (646 words)
Athamantis also catalogued with number 230 is a small asteroid that it orbits between the Mars orbits and Jupiter that I could locate with the small telescope which I have, refractor of 90mm.
Athamantis has an orbital period of 3,68 years and a period of rotation on its axis of 23,99 hours.
Therefore, the date of discovery and identification of the asteroid Athamantis or 230 it was November 1
  More results at FactBites »


 
 

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