L'étude des objets géocroiseurs (NEO ou Near Earth Objects) s'est considérablement développée sous de multiples aspects sous l'impulsion notable des recherches concernant les risques de collision avec la Terre. Les observations jouent dans ce contexte un rôle primordial. Cet article s'attache à souligner leur importance pour accroître notre connaissance de ces objets et la nécessité d'en organiser des coordinations spécifiques. Il développe les objectifs de ces observations, explicite des méthodes pour réaliser la détection de nouveaux objets, discute de leur suivi et de l'archivage des données, donne des informations sur leur utilisation pour améliorer la connaissance de leurs orbites et sur l'influence du choix des théories planétaires prises en compte dans le modèle.
The study of NEOs (Near Earth Objects) has considerably been developed in several ways under the huge impulse of the research on the risks of an hazardous collision with the Earth. In this context observations play a very important role. This article attempts to underline their importance in improving our knowledge of these objects and the necessity of organizing dedicated programs. It develops the objectives of these observations, describes methods to perform the detection of new objects, discusses their follow-up and the necessity of finding using archives. It also gives information about the fit of the observations in order to improve the knowledge of the orbits of NEO and about the effect of the planetary theories taken into account in the model.
Mot clés : Astéroïdes, NEO, Objets géocroiseurs, Surveillance, Suivi, Observations
William Thuillot 1 ; Jérémie Vaubaillon 1 ; Hans Scholl 2 ; François Colas 1 ; P. Rocher 1 ; Mirel Birlan 1 ; Jean-Eudes Arlot 1
@article{CRPHYS_2005__6_3_327_0, author = {William Thuillot and J\'er\'emie Vaubaillon and Hans Scholl and Fran\c{c}ois Colas and P. Rocher and Mirel Birlan and Jean-Eudes Arlot}, title = {Relevance of the {NEO} dedicated observing programs}, journal = {Comptes Rendus. Physique}, pages = {327--335}, publisher = {Elsevier}, volume = {6}, number = {3}, year = {2005}, doi = {10.1016/j.crhy.2005.01.002}, language = {en}, }
TY - JOUR AU - William Thuillot AU - Jérémie Vaubaillon AU - Hans Scholl AU - François Colas AU - P. Rocher AU - Mirel Birlan AU - Jean-Eudes Arlot TI - Relevance of the NEO dedicated observing programs JO - Comptes Rendus. Physique PY - 2005 SP - 327 EP - 335 VL - 6 IS - 3 PB - Elsevier DO - 10.1016/j.crhy.2005.01.002 LA - en ID - CRPHYS_2005__6_3_327_0 ER -
%0 Journal Article %A William Thuillot %A Jérémie Vaubaillon %A Hans Scholl %A François Colas %A P. Rocher %A Mirel Birlan %A Jean-Eudes Arlot %T Relevance of the NEO dedicated observing programs %J Comptes Rendus. Physique %D 2005 %P 327-335 %V 6 %N 3 %I Elsevier %R 10.1016/j.crhy.2005.01.002 %G en %F CRPHYS_2005__6_3_327_0
William Thuillot; Jérémie Vaubaillon; Hans Scholl; François Colas; P. Rocher; Mirel Birlan; Jean-Eudes Arlot. Relevance of the NEO dedicated observing programs. Comptes Rendus. Physique, Volume 6 (2005) no. 3, pp. 327-335. doi : 10.1016/j.crhy.2005.01.002. https://comptes-rendus.academie-sciences.fr/physique/articles/10.1016/j.crhy.2005.01.002/
[1] Bull. Am. Astron. Soc., 33 (2001), p. 1116
[2] Bull. Am. Astron. Soc., 34 (2002), p. 1315
[3] Bull. Am. Astron. Soc., 32 (2000), p. 1023
[4] , Imaging Technology and Telescopes, Proc. SPIE, vol. 4091, 2000, p. 225
(J.W. Bilbro; J.B. Breckinridge; R.A. Carreras; S.R. Czyzak; M.J. Eckart; R.F. Fiete; P.S. Idell, eds.)[5] R.S. McMillan, Solar system research with the spacewatch 1.8-m telescope, Lunar and Planetary Lab. Technical Report, University of Arizona, Tucson, 2001
[6] Bull. Am. Astron. Soc., 32 (2000), p. 1018
[7] S. Larson, E. Beshore, R. Hill, E. Christensen, D. McLean, S. Kolar, R. McNaught, G. Garradd, American Astronomical Society, DPS Meeting 35, 2003, 36.04
[8] Mem. Soc. Astron. Italiana, 73 (2002), p. 636
[9] Proceedings of Asteroids, Comets, Meteors – ACM 2002, ESA SP-500, Noordwijk (B. Warmbein, ed.), 2002, p. 801
[10] , Survey and Other Telescope Technologies and Discoveries, Proc. SPIE, vol. 4836, 2002, p. 83
(J.A. Tyson; S. Wolff, eds.)[11] Dynamics, Ephemerides, and Astrometry of the Solar System, Proc. of the 172nd Symposium of the International Astronomical Union, held in Paris, France, 38 July 1995 (S. Ferraz-Mello; B. Morando; J.-E. Arlot, eds.), 1996, p. 153
[12] Astron. Astrophys., 417 (2004), pp. 1165-1171
[13] Celest. Mech. Dyn. Astron., 80 (2001), pp. 205-213
[14] Astron. Astrophys., 384 (2002), pp. 322-328
[15] An efficient integrator that uses Gauss–Radau spacings (A. Carusi; G. Valsecchi, eds.), Dynamical of Comets: Their Origin and Evolution, Reidel, Dordrecht, 1985, pp. 185-202
[16] Icarus, 117 (1995), pp. 71-89 (and 38 coauthors)
[17] Icarus, 123 (1996), pp. 227-244 (and 37 coauthors)
[18] Science, 263 (1994), pp. 940-943
[19] Icarus, 151 (2001) no. 2, pp. 139-149
[20] Astron. Astrophys., 397 (2003), pp. 325-328
[21] Icarus, 170 (2004) no. 2, pp. 259-294
[22] Icarus, 170 (2004) no. 2, pp. 295-311
[23] Icarus, 166 (2003) no. 1, pp. 116-130
[24] Astron. Nachr., 325 (2004) no. 6–8, pp. 571-573
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