Skip to main content
  • Conference proceedings
  • © 1975

Satellite Dynamics

Symposium São Paulo/Brazil June 19–21, 1974

Part of the book series: IUTAM Symposia (IUTAM)

Buy it now

Buying options

eBook USD 84.99
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book USD 109.99
Price excludes VAT (USA)
  • Compact, lightweight edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info

Tax calculation will be finalised at checkout

Other ways to access

This is a preview of subscription content, log in via an institution to check for access.

Table of contents (20 papers)

  1. Front Matter

    Pages I-VIII
  2. Third Session Thursday, June 20, 1974, Morning

    1. Orbit Determination in the Presence of Atmospheric Drag Errors

      • B. D. Tapley, A. R. Neto, B. E. Schutz
      Pages 154-169
  3. Fourth Session Thursday, June 20, 1974, Afternoon

    1. Literal Algebra for Satellite Dynamics

      • E. M. Gaposchkin
      Pages 170-179
  4. Fifth Session Friday, June 21, 1974, Morning

    1. The Rotational Motion of a Satellite and Atmospheric Density Determination

      • V. V. Beletskii, V. M. Grigorevsky, S. Ya. Kolesnik
      Pages 233-279
  5. Sixth Session Friday, June 21, 1974, Afternoon

    1. Optimal Impulsive Interplanetary Transfers

      • Jean-Paul Gravier, Christian Marchal, Robert Dudley Culp
      Pages 342-369

About this book

This volume includes original papers presented at the 4th Symposium on Satellite Dynamics held at the XII Annual Plenary Meeting of COSPAR. At a time where it might be thought that very few problems were left un­ solved in celestial mechanics, we discover that new and more challenging questions must be answered. The pre­ cision of observations reaches the centimeter level and physical phenomena which had been disregarded come into play. We need a better treatment of atmospheric drag, radiation forces, and a better knowledge of the earth's gravitational field. Time has to be precisely defined as well as reference systems, including improved values for precision and nutation. The question of resonances introduced by nonzonal harmonics was to be carefully in­ vestigated. Numerical integration techniques must be optimized and means of controlling their errors improved. Analytical techniques must be made appropriate for com­ puter processing. Presently existing methods of solu­ tions of differential equations of interest to celestial mechanics are getting cumbersome as all these new facts come to light. It is clear that entirely new and more effective methods are necessary. These methods must, among other requirements, take into account the essential nonlinear character of the equations. Finally, the mo­ tion about the center of mass of a satellite is becoming an essential need for the thorough understanding and de­ scription of the orbital motion.

Editors and Affiliations

  • Instituto Astronomico e Geofisico, São Paulo, Brazil

    Girgio E. O. Giacaglia

  • COSPAR Editorial Office, Northwood, England

    A. C. Stickland

Bibliographic Information

Buy it now

Buying options

eBook USD 84.99
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book USD 109.99
Price excludes VAT (USA)
  • Compact, lightweight edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info

Tax calculation will be finalised at checkout

Other ways to access