Abstract
DURING its reconnaissance of the asteroid 243 Ida, the Galileo spacecraft returned images of a second object, 1993(243)1 Dactyl1— the first confirmed satellite of an asteroid. Sufficient data were obtained on the motion of Dactyl to determine its orbit as a function of Ida's mass. Here we apply statistical and dynamical arguments to constrain the range of possible orbits, and hence the mass of Ida. Combined with the volume of Ida2, this yields a bulk density of 2.6 ± 0.5 g cm−3. Allowing for the uncertainty in the porosity of Ida, this density range is consistent with a bulk chon-dritic composition, and argues against some (but not all) classes of meteoritic igneous rock types that have been suggested as compositionally representative of S-type asteroids like Ida.
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References
Belton, M. J. S. & Carlson, R. IAU Circ. No. 5948 (1994).
Thomas, P. et al. (abstr.) Bull. Am. Astr. Soc. 26, 1155 (1994).
Belton, M. J. S. et al. Science 265, 1543–1547 (1994).
Binzel, R. P. et al. Icarus 105, 310–325 (1993).
Davies, M. E. et al. (abstr.) Bull. Am. Astr. Soc. 26, 1154–1155 (1994).
Roy, A. E. Orbital Motion 3rd edn 170 (Hilger, Bristol, 1988).
Hamilton, D. P. & Burns, J. A. Icarus 96, 43–64 (1992).
Chauvineau, B., Farinella, P. & Mignard, F. Icarus 105, 370–384 (1993).
Scheeres, D. J. Icarus 110, 225–238 (1994).
Scheeres, D. J., Ostro, S. J., Hudson, R. S. & Werner, R. A. (abstr.) Bull. Am. Astr. Soc. 26, 1166–1167 (1994).
McCord, T. B. & Chapman, C. R. Astrophys. J. 195, 553–562 (1975).
Leake, M., Gradie, J. & Morrison, D. Meteoritics 13, 101–120 (1978).
Feierberg, M. A., Larson, H. P. & Chapman, C. R. Astrophys. J. 257, 361–372 (1982).
Sears, D. W. G. & Dodd, R. T. in Meteorites and the Early Solar System (eds Kerridge, J. F. & Mathews, M. S.) 3–31 (Univ. Arizona Press, Tucson, 1988).
Gaffey, M. J. Icarus 60, 83–114 (1984).
Clarke, B. E., Fanale, F. P. & Salisbury, J. W. Icarus 97, 288–297 (1992).
Fanale, F. P., Clark, B. E. & Bell, J. F. J. geophys. Res. 97, 20863–20874 (1992).
Bell, J. F. & Keil, K. Proc. lunar planet. Sci. Conf. 18, 573–580 (1988).
Bell, J. F., Davis, D. R., Hartmann, W. K. & Gaffey, M. J. in Asteroids II (eds Binzel, R. P. et al.) 921–948 (Univ. Arizona Press, Tucson, 1989).
Gaffey, M. J., Burbine, T. H. & Binzel, R. P. Meteoritics 28, 161–187 (1993).
Gaffey, M. J. et al. Icarus 106, 573–602 (1993).
Lipschutz, M. E., Gaffey, M. J. & Pellas, P. in Asteroids II (eds Binzel, R. P. et al.) 740–777 (Univ. Arizona Press, Tucson, 1989).
Wasson, J. T. Meteorites 175–176 (Springer, New York, 1974).
Carrier, W. D., Olhoeft, G. R. & Mendell, W. in Lunar Source Book (eds Heiken, G. et al.) 475–594 (Cambridge Univ. Press, 1991).
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Belton, M., Chapman, C., Thomas, P. et al. Bulk density of asteroid 243 Ida from the orbit of its satellite Dactyl. Nature 374, 785–788 (1995). https://doi.org/10.1038/374785a0
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DOI: https://doi.org/10.1038/374785a0
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