Frequencies of Occultations of Stars by Planets, Satellites, and Asteroids

Science  10 Mar 1972:
Vol. 175, Issue 4026, pp. 1108-1112
DOI: 10.1126/science.175.4026.1108


Calculations show that several occultations of stars by the large satellites of the outer planets, Pluto, and the large asteroids could be observed each decade with existing equipment at Earth-based telescopes. A systematic program of occultation predictions and observations is urged in order to improve our knowledge about the atmospheres, sizes, shapes, topography, and positions of these poorly understood bodies, in support of forthcoming spacecraft missions to the outer solar system.