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Efficient Modelling of Small Bodies' Gravitational Potential for Autonomous Approach

Learn advanced techniques in asteroid modelling for autonomous approach, including gravitational potential and shape modeling. Join the training school at Rome's Tor Vergata University to enhance your skills. Supervised by experts Prof. Phil Palmer and Prof. Mark Roberts from Surrey Space Centre, University of Surrey, UK.

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Efficient Modelling of Small Bodies' Gravitational Potential for Autonomous Approach

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  1. Efficient modelling of small bodies gravitational potential forautonomous approach ESR: Andrea Turconi Supervisors: Prof. Phil Palmer, Prof. Mark Roberts Surrey Space Centre, University of Surrey, UK First Astronet-II Training School Rome "Tor Vergata" University – 14th-17th January 2013

  2. Personal Background First Astronet-II Training SchoolRome “Tor Vergata” University – Jan. 14th-17th, 2013

  3. Personal Background First Astronet-II Training SchoolRome “Tor Vergata” University – Jan. 14th-17th, 2013

  4. Asteroid modelling for autonomous approach • ~ 1 month early operations phase • Pics + Doppler & Ranging • Shape model • Spherical Harmonics Coefficients • Commands to S/C(delay) First Astronet-II Training SchoolRome “Tor Vergata” University – Jan. 14th-17th, 2013

  5. Asteroid modelling for autonomous approach Eros spheres modelElisabetHerrera Sucarrat,Phil Palmer,Mark Roberts(2012) • How to generate and use such a model in-situ? • How to mitigate inaccuracies? Potential and ZVC of a rotating system of cotangent spheresAndrea Turconi (2012) First Astronet-II Training SchoolRome “Tor Vergata” University – Jan. 14th-17th, 2013

  6. Thank you for your attention! Any questions?

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