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Note: each asteroid is given a unique sequential identifying number after its orbit is precisely determined. Prior to this, asteroids are known only by their systematic name or Provisional Designation , such as "1950 DA". LARGEST KNOWN ASTEROIDS The number of bodies grows rapidly as the size decreases. For example, there are estimated to be another twelve asteroids with diameters between 200 and 224 km. The inner main belt (defined as the region interior to the 3:1 Kirkwood Gap at 2.50 AU) has few large asteroids. Only 4 Vesta and 9 Metis qualify for the above list. For a listing by mass see Here . RETROGRADE AND HIGH-INCLINATION ASTEROIDS Asteroids with orbital inclinations greater than 90° orbit in a Retrograde direction. There are only eight (as of August 2004 ) retrograde asteroids known, only two of which are numbered. This makes them the rarest group of all. High-inclination asteroids are either Mars-crossers (probably in the process of being ejected from the solar system) or Damocloid s. OTHER NOTEWORTHY MINOR PLANETS SPACECRAFT TARGETS ASTEROIDS WITH THE SAME OR SIMILAR NAMES AS MOONS NUMBERED ASTEROIDS THAT ARE ALSO COMETS Note there are a quite a few other cases where a non-numbered asteroid with only a systematic designation (such as ) turned out to be a comet. The above table lists only numbered asteroids that are also comets. ASTEROIDS THAT WERE MISNAMED AND RENAMED In earlier times, before the modern numbering and naming rules were in effect, asteroids were sometimes given numbers and names before their orbits were precisely known. And in a few cases duplicate names were given to the same object (with modern use of computers to calculate and compare orbits with old recorded positions, this type of error no longer occurs). This led to a few cases where asteroids had to be renamed. {Link without Title}
RECORD-SETTING CLOSE APPROACHES BY ASTEROIDS TO EARTH Only asteroids that break a previous record are included. Note that Near-earth Object detection technology drastically improved around the turn of the century, so objects being detected today (in 2004 ) would have been missed only a decade earlier. Some of these bodies may be too small to technically qualify as asteroids; by some definitions, an asteroid must be at least 50 meters in diameter. ''See also'': Closest Approaches to the Earth by Minor Planets EXCEPTIONALLY SLOW-ROTATING OBJECTS Rotation Period s have been determined for only a small fraction of asteroids (from Light Curve s or from radar studies). Most asteroids have rotation periods of less than 24 hours; however, 288 Glauke has a rotation period of about 50 days. ''See also'': Minor Planet Lightcurve Parameters SEE ALSO
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BOOKS ''Dictionary of Minor Planet Names, 5th ed.: Prepared on Behalf of Commission 20 Under the Auspices of the International Astronomical Union'', Lutz D. Schmadel , ISBN 3540002383 |