Les tailles, formes et propriétés de surface ou sous surface des géocroiseurs sont encore mal connues, dans la mesure où leur détermination repose sur l'exploration locale. Ces objets irréguliers (essentiellement des astéroïdes, mais aussi des noyaux cométaires inactifs) ont des tailles allant de quelques kilomètres à quelques mètres, avec environ un millier d'entre eux dépassant le kilomètre. Les surfaces semblent assez rugueuses et sont couvertes, au moins partiellement, de régolites.
The sizes, shapes, and surface or subsurface properties of Near Earth Objects (mostly asteroids, also inactive comet nuclei) are still poorly known, since any accurate determination requires in situ missions. It may nevertheless be estimated that the sizes of these irregular bodies range from a few tens of kilometres to a few tens of meters, with possibly about 1000 NEOs with sizes greater than 1 km. Their surfaces are estimated to be quite rough, and at least partially covered with regolith.
Mots clés : Astéroïdes, Comètes, Géocroiseurs, Taille, Forme, Propriétés physiques de surface
A. Chantal Levasseur-Regourd 1 ; Marcello Fulchignoni 2 ; Marco Delbó 3 ; Richard P. Binzel 4
@article{CRPHYS_2005__6_3_313_0, author = {A. Chantal Levasseur-Regourd and Marcello Fulchignoni and Marco Delb\'o and Richard P. Binzel}, title = {NEO sizes, shapes and surface physical properties}, journal = {Comptes Rendus. Physique}, pages = {313--320}, publisher = {Elsevier}, volume = {6}, number = {3}, year = {2005}, doi = {10.1016/j.crhy.2005.01.003}, language = {en}, }
TY - JOUR AU - A. Chantal Levasseur-Regourd AU - Marcello Fulchignoni AU - Marco Delbó AU - Richard P. Binzel TI - NEO sizes, shapes and surface physical properties JO - Comptes Rendus. Physique PY - 2005 SP - 313 EP - 320 VL - 6 IS - 3 PB - Elsevier DO - 10.1016/j.crhy.2005.01.003 LA - en ID - CRPHYS_2005__6_3_313_0 ER -
A. Chantal Levasseur-Regourd; Marcello Fulchignoni; Marco Delbó; Richard P. Binzel. NEO sizes, shapes and surface physical properties. Comptes Rendus. Physique, Volume 6 (2005) no. 3, pp. 313-320. doi : 10.1016/j.crhy.2005.01.003. https://comptes-rendus.academie-sciences.fr/physique/articles/10.1016/j.crhy.2005.01.003/
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