Relevance of the NEO dedicated observing programs

Abstract 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. To cite this article: W. Thuillot et al., C. R. Physique 6 (2005).

[1]  Richard P. Binzel,et al.  Photometric Observations and Modeling of Asteroid 1620 Geographos , 1996 .

[2]  Richard P. Binzel,et al.  Spectral Properties of Near-Earth Objects: Palomar and IRTF Results for 48 Objects Including Spacecraft Targets (9969) Braille and (10302) 1989 ML , 2001 .

[3]  E. M. Standish,et al.  An approximation to the errors in the planetary ephemerides of the Astronomical Almanac , 2004 .

[4]  Mirel Birlan,et al.  Solar system observations by remote observing technique: useful experience for robotic telescope strategies , 2004 .

[5]  J. Anthony Tyson,et al.  Survey and Other Telescope Technologies and Discoveries , 2002 .

[6]  Richard P. Binzel,et al.  Keck observations of near-Earth asteroids in the thermal infrared , 2003 .

[7]  Richard P. Binzel,et al.  Observed spectral properties of near-Earth objects: results for population distribution, source regions, and space weathering processes , 2004 .

[8]  Budi Dermawan,et al.  Thermal observations of MUSES-C mission target (25143) 1998 SF$_\mathsf{36}$ , 2003 .

[9]  P. Bretagnon,et al.  Analytical Planetary solution VSOP2000 , 2001 .

[10]  Elisabetta Dotto,et al.  The lightcurve of 4179 Toutatis: Evidence for complex rotation. , 1995 .

[11]  Richard P. Binzel,et al.  Bias-corrected population, size distribution, and impact hazard for the near-Earth objects , 2004 .

[12]  E. M. Standish,et al.  Accuracy limit of modern ephemerides imposed by the uncertainties in asteroid masses , 2002 .

[13]  R. S. Hudson,et al.  Shape of Asteroid 4769 Castalia (1989 PB) from Inversion of Radar Images , 1994, Science.

[14]  E. Everhart An efficient integrator that uses Gauss-Radau spacings , 1985 .