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Asteroid

An asteroid (minor planet or planetoid) is a relatively small "planet-like" object which orbits within a solar system; generally less than 1km in diameter. They are believed to be remnants of the protoplanetary discs; which were not incorporated into planets during the system's formation. Most asteroids will align themselves within an asteroid belt and some have moons; asteroids (like most celestial objects) tend to have elliptical orbits. "Small" asteroids (generally fragments from collisions) which are approximately boulder-sized or less, are known as "meteoroids". Asteroids composed largely of ice are known as comets. Some asteroids are the remains of old comets that have had most of their ice driven away by close proximitiy to the Sun, leaving behind only the heavier mineral components.

More than 9000 asteroids have been discovered within the Earth system. The largest asteroid in Earth's inner solar system is Ceres, with a diameter of 900-1000km. Two other large asteroids are Pallas and Vesta; both have diameters of ~500km.

A large group of asteroids have orbits between the orbits of Mars and Jupiter, roughly 2 to 4 AU, in a region known as the Main belt. These couldn't form a planet due to the gravitational influence of Jupiter. Jupiter's gravitational influence also results in Kirkwood gaps in the asteroid belt, orbits cleared by orbital resonance.

Another important group are the Trojans; they are in the orbit of Jupiter, on two Lagrangian points. Similar sets of asteriods appear to lie in the trojan points in almost all planetary orbits.

Another group exists within the Kuiper belt. The Kuiper belt is the source of about half of the comets that come to the inner solar system. Some of these are not much smaller than Pluto and Charon -- the largest found so far is Quaoar, thought to be around 1250 km in diameter, the same size as (or even slightly larger than) Charon - and some astronomers expect that we shall one day find some Trans-Neptunian objects bigger than Pluto.

The Centaurs orbit the Sun, between the orbits of the giant planets. The first of these to be discovered was 2060 Chiron in 1977. These are generally supposed to be asteroids or comets that were ejected from their proper orbits.

Up until 1998, asteroids were discovered by a four-step process. First, a region of the sky was photographed by a wide-field telescope. Pairs of photographs were taken, typically one hour apart. Multiple pairs may be taken over a series of days. Second, the two films of the same region were viewed under a stereoscope[?]. Any body in orbit around the sun would move slightly between the pair of films. Under the stereoscope, the image of the body would appear to float slightly above the background of stars. Third, once a moving body was identified, its location would be measured precisely using a digitizing microscope. The location would be measured relative to known star locations.

These first three steps do not constitute asteroid discovery: the observer has only found an apparition[?]. The final step of discovery was to send the locations and time of observations to Brian Marsden[?] of the Minor Planets Center[?]. Dr. Marsden has computer programs that compute whether an apparition tied together previous apparitions into a single orbit. If so, then the observer of the final apparition is declared a discoverer, and the discoverer got the honor of naming the asteroid (subject to the approval of the International Astronomical Union).

Since 1998, a large majority of the asteroids have been discovered with automated systems that comprise CCD cameras and computers directly connected to telescopes. A list of teams using such automated systems include[1] (http://neo.jpl.nasa.gov/programs):

The LINEAR system alone has discovered 157,920 asteroids as of April, 2002 [2] (http://www.ll.mit.edu/LINEAR). Between all of the automated systems, 2298 near-Earth asteroids have been discovered [3] (http://neo.jpl.nasa.gov/missions/stats).

There is increasing interest in identifying asteroids whose orbit crosses the Earth's, and that could, given enough time, collide with the earth. The two most important groups of near-Earth asteroids are the Amors, and the Atens. Various asteroid deflection strategies have been proposed.

The first "nearby" photos, of an asteroid, were taken by the Galileo spacecraft of Gaspra and Ida (1991), while NEAR Shoemaker landed on Eros(2001).

When the orbit of an asteroid is confirmed, it is given a number, and later it may also be given a name (e.g. 1 Ceres). The first few are named after figures from Graeco-Roman mythology, but as such names started to run out, others were also used - famous people, the names of the discover's wives, even television characters. A few groups have names with a common theme - for instance Centaurs are all named after legendary Centaurs, and Trojans after heroes from the Trojan War. The Centaurs are of special interest; many of them are massive comets, such as Chiron.

Asteroids are classified into spectral types by their optical spectrum, which corresponds to the composition of the asteroid's surface material. Note that the proportion of known asteroids falling into the various spectral types does not necessarily reflect the proportion of all asteroids that are of that type; some types are easier to detect than others, biasing the totals.

• C-type asteroids[?] - 75% of known asteroids. The C stands for "carbonaceous." They are extremely dark (albedo 0.03), similar to carbonaceous chondrite[?] meteorites. These asteroids have approximately the same chemical composition as the Sun, minus hydrogen, helium and other volatiles. The spectra of these asteroids have relatively blue colors and are fairly flat and featureless.
• S-type asteroids[?] - This type of asteroids represents about 17% of known asteroids. The S stands for silicaceous. They are relatively bright objects (albedo .10-.22). They have a metallic composition (mainly nickel, iron and magnesium-silicates). The spectra of this class are reddish and similar to those of stony-iron meteorites.
• M-type asteroids[?] - This class includes most of the rest of the asteroids. The M stands for metallic; they are bright asteroids (albedo .10-.18), made of pure nickel-iron.

There are also a number of rarer asteroid types, the number of types continuing to grow as more asteroids are studied.

The largest asteroids:

NumberName Diameter (km)Date DiscoveredDiscoverer
1Ceres 1003January 1, 1801 Piazzi, G.
2Pallas 608March 28, 1802 Olbers, H. W.
4Vesta 538March 29, 1807 Olbers, H. W.
10Hygeia[?] 450April 12, 1849 de Gasparis, A.
31Euphrosyne[?] 370September 1, 1854 Ferguson, J.
704Interamnia[?] 350October 2, 1910 Cerulli, V.
511Davida[?] 323May 30, 1903 Dugan, R. S.
65Cybele 309March 8, 1861 Tempel, E. W.
52Europa 289February 4, 1858 Goldschmidt, H.
451Patienta[?] 276December 4, 1899 Charlois, A.
15Eunomia[?] 272July 29, 1851 de Gasparis, A.
16Psyche 250March 17, 1851 de Gasparis, A.
48Doris[?] 250September 19, 1857 Goldschmidt, H.
92Undina[?] 250July 7, 1867 Peters, C. H. F.
324Bamberga[?] 246February 25, 1892 Palisa, J.
3Juno 2401804K. Harding
24Themis 234April 5, 1853 de Gasparis, A.
95Arethusa[?] 230November 23, 1867 Luther, R.

Other noteworthy asteroids:

NumberNameDiameter (km)Year DiscoveredComment
243 Ida 56 x 24 x 21 September 29, 1884 Visited by Galileo probe
Dactyl 1.4 1991 Moon of 243 Ida
253 Mathilde 66 x 48 x 46 November 12, 1885 Visited by NEAR Shoemaker
433 Eros 13 x 13 x 33 August 13, 1898 Visited by NEAR Shoemaker
624 Hektor[?] February 10, 1907 Largest Jovian Trojan asteroid discovered
951 Gaspra 19 x 12 x 11 July 30, 1916 Visited by Galileo probe
2060 Chiron 170 1977 First Centaur to be discovered
4593 Reipurth March 16, 1980 discovered by Claes-Ingvar Lagerkvist[?]
3753 Cruithne 5 October 10, 1986 Unusual Earth-associated orbit
4179 Toutatis 4.5 x 2.4 x 1.9 January 4, 1989 Will approach Earth closely in 2004
4769 Castalia 1.8 x 0.8 August 9, 1989 First asteroid to be imaged
5261Eureka[?] June 20, 1990 First Martian Trojan asteroid (L5 point) discovered
2002 AA29[?] 0.1 January 9, 2002 Unusual Earth-associated orbit

Public domain picture from NASA

Solar system:
Sun - Mercury - Venus - Earth - Mars - Asteroids - Jupiter - Saturn - Uranus - Neptune - Pluto - Comets

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