Small Bodies

Facts about Selected Asteroids

Sources: NSSDC and Nine Planets

On January 1st 1801, Giuseppe Piazzi discovered an object he thought was a new comet. But after its orbit was better determined it was clear that it was not a comet but more like a small planet. Piazzi named it Ceres, after the Sicilian goddess of grain. Three other small bodies were discovered in the next few years (Pallas, Vesta, and Juno). By the end of the 19th century, several hundred were known.

Several hundred thousand asteroids have been discovered and given provisional designations so far. Thousands more are discovered each year. There are undoubtedly hundreds of thousands more that are too small to be seen from the Earth. There are 26 known asteroids larger than 200 km in diameter. Our census of the largest ones is now fairly complete: we probably know 99% of the asteroids larger than 100 km in diameter. Of those in the 10 to 100 km range we have cataloged about half. But we know very few of the smaller ones; there are probably considerably more than a million asteroids in the 1 km range.

The total mass of all the asteroids is less than that of the Moon.

[Gaspra] The image is a false color view of the asteroid 951 Gaspra taken by the Galileo spacecraft.

14 comets and asteroids have so far been explored by spacecraft:

In future, the Rosetta spacecraft will visit Comet Churyumov-Gerasmenko, and Dawn will orbit asteroids Vesta and Ceres.

Information on Selected Asteroids

Below is a table of information on selected asteroids, and at the bottom of the page are comments on the asteroids. All of the values for mass and many of the diameter values are only rough estimates. The links are to pages on the NSSDC site.

   Asteroid         Diameter      ~Mass    Rotation    Orbital   Spectral   Semimajor     Orbital        Orbital       Number
Number and Name       (km)       1015 kg     Period     Period     Class       Axis      Eccentricity   Inclination    and Name
---------------     --------     -------   --------    -------   --------   ---------    ------------   -----------    -------- 
   1 Ceres         960 x 932     870,000   9.075 hrs   4.60 yrs      C       2.766 AU       0.0779       10.58 deg      1 Ceres
   2 Pallas     570 x 525 x 482  318,000   7.811 hrs   4.61 yrs      U       2.776 AU       0.2309       34.85 deg      2 Pallas
   3 Juno             240         20,000   7.210 hrs   4.36 yrs      S       2.669 AU       0.2579       12.97 deg      3 Juno
   4 Vesta            530        300,000   5.342 hrs   3.63 yrs      U       2.361 AU       0.0903        7.13 deg      4 Vesta 
  45 Eugenia          214          6,100   5.699 hrs   4.49 yrs     FC       2.721 AU       0.083         6.61 deg     45 Eugenia
 140 Siwa             110                 18.5   hrs   4.52 yrs              2.732 AU       0.2009        1.97 deg    140 Siwa
 243 Ida            58 x 23        100     4.633 hrs   4.84 yrs      S       2.861 AU       0.0451        1.14 deg    243 Ida
 253 Mathilde     66 x 48 x 46    103.3  417.7   hrs   4.31 yrs      C       2.646 AU       0.2660        6.71 deg    253 Mathilde                                  
 433 Eros         33 x 13 x 13      7.2    5.270 hrs   1.76 yrs      S       1.458 AU       0.2230       10.83 deg    433 Eros
 951 Gaspra       19 x 12 x 11      10     7.042 hrs   3.29 yrs      S       2.209 AU       0.1738        4.10 deg    951 Gaspra
1566 Icarus           1.4         0.001    2.273 hrs   1.12 yrs      U       1.078 AU       0.8268       22.86 deg   1566 Icarus            
1620 Geographos       2.0         0.004    5.222 hrs   1.39 yrs      S       1.246 AU       0.3354       13.34 deg   1620 Geographos 
1862 Apollo           1.6         0.002    3.063 hrs   1.81 yrs      S       1.471 AU       0.5600        6.36 deg   1862 Apollo
2060 Chiron           180         4000     5.9   hrs   50.7 yrs      B      13.633 AU       0.3801        6.94 deg   2060 Chiron
2530 Shipka                                            5.25 yrs              3.019 AU       0.1237       10.10 deg   2530 Shipka
2703 Rodari                                            3.25 yrs              2.194 AU       0.0572        6.04 deg   2703 Rodari
3352 McAuliffe       2 - 5                             2.57 yrs              1.879 AU       0.3686        4.77 deg   3352 McAuliffe
3840 Mimistrobell                                      3.38 yrs              2.249 AU       0.0831        3.92 deg   3840 Mimistrobell
4179 Toutatis   4.6 x 2.4 x 1.9   0.05   130.    hrs   3.98 yrs      S       2.512 AU       0.6339        0.47 deg   4179 Toutatis
4660 Nereus             2                              1.82 yrs              1.490 AU       0.3603        1.42 deg   4660 Nereus
4769 Castalia      1.8 x 0.8      0.0005               1.10 yrs              1.063 AU       0.4831        8.89 deg   4769 Castalia  
4979 Otawara         18.9                              3.19 yrs              2.168 AU       0.1170        0.41 deg   4979 Otawara
9969 Braille       2.2 x 1.0                           3.58 yrs              2.341 AU       0.4336       29.0  deg        1992 KD

1 Ceres - The largest and first discovered asteroid, by G. Piazzi on January 1, 1801. Ceres comprises over one-third the 2.3 x 1021 kg estimated total mass of all the asteroids.
2 Pallas - The 2nd largest asteroid and second asteroid discovered, by H. Olbers in 1802.
3 Juno - The 3rd asteroid discovered, by K. Harding in 1804.
4 Vesta - The 3rd largest asteroid, Vesta appears to have a basaltic crust overlying an olivine mantle, indicating differentiation has occurred. Imaged by the Hubble Space Telescope in 1995.
45 Eugenia - Believed to have a small satellite S/1998 (45) 1 in near circular 4.7 day orbit as reported in IAU Circular #7129
140 Siwa - Scheduled for July 2008 flyby by the Rosetta spacecraft on its way to Comet P/Wirtanen
243 Ida - Imaged by Galileo on 28 August 1993. These images showed a small satellite, subsequently named Dactyl, in orbit about Ida.
253 Mathilde - Target of NEAR mission flyby on 27 June 1997 en route to 433 Eros.
433 Eros - Near-Earth asteroid scheduled to be studied by the NEAR mission, which flew by Eros in February 1999 and will go into orbit in February 2000.
951 Gaspra - Imaged by Galileo on 29 Oct 1991.
1566 Icarus - Highly eccentric Earth-crossing orbit.
1620 Geographos - Scheduled to be visited by Clementine before a computer malfunction cut the mission short.
1862 Apollo - Earth-crossing asteroid.
2060 Chiron - Asteroid/Comet (95P/Chiron) in chaotic eccentric orbit near Saturn and Uranus. 14 February 1996 perihelion was the subject of the Chiron Perihelion Campaign.
2530 Shipka - Originally scheduled for October, 2008 flyby by the Rosetta spacecraft on its way to Comet P/Wirtanen
2703 Rodari - Originally scheduled for May, 2008 flyby by the Rosetta spacecraft on its way to Comet P/Wirtanen
3352 McAuliffe - Amor (Mars-crossing) asteroid originally scheduled for 1999 flyby by the New Millenium Deep Space 1 spacecraft.
3840 Mimistrobell - Originally scheduled for September, 2006 flyby by the Rosetta spacecraft on its way to Comet P/Wirtanen.
4179 Toutatis - Double object, probably in contact, one 2.5 km and one 1.5 km diameter (estimated), imaged by Arecibo and Goldstone radar. Close approach to Earth of this object (about 1.5 million km) will occur on 29 September 2004.
4660 Nereus - Near-Earth asteroid, target of ISAS (Japan) Muses-C sample-return mission and NEAP rendezvous.
4769 Castalia - Double-lobed near-Earth asteroid, each lobe about .75 km diameter. Imaged by Arecibo radar.
4979 Otawara - Scheduled for July 2006 flyby by the Rosetta spacecraft on its way to Comet P/Wirtanen.
9969 Braille - Near-Earth asteroid target of 28 July 1999 flyby by the Deep Space 1 spacecraft. (Also known as 1992 KD)

New masses calculated for 3 largest asteroids - U.S. Naval Observatory press release, 7 January 1998


Links
This page is a composite of information authored by Dr. David R. Williams, NSSDC, dwilliam@nssdc.gsfc.nasa.gov, 7th October 1999 and by Bill Arnett, Nine Planets, 15th March 2004. The status of the Stardust, Deep Impact and Hyabusa missions has been updated. The page was compiled by Michael Gallagher on 14th September 2005