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meetings - Space Flight Mechanics Committee

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Venus in 2010, but now it is on the way to re-encounter Venus in 2015. However, due to a<br />

malfunction of the propulsion system, AKATSUKI can be only injected into the orbit much<br />

higher than that originally planned. It causes a couple of issues to be considered in its orbit<br />

design, one of which is the long eclipse on the orbit around Venus. Introduced in this paper<br />

is an orbit design strategy to avoid the long eclipse under this situation.<br />

10:45 AAS Observations planning optimization for BepiColombo’s Mercury rotation<br />

13-387 experiment<br />

Alessandra Palli, University of Bologna; Rachele Meriggiola, University of Rome;<br />

Luciano Iess, University of Rome; Paolo Tortora, University of Bologna<br />

The identification of an observation planning ensuring the fulfillment of the scientific<br />

objectives is fundamental in the frame of Mercury’s rotation experiment to be carried out by<br />

ESA’s BepiColombo mission. The observables are represented by image pairs of the same<br />

landmark on Mercury’s surface, captured at two different epochs via the on-board high<br />

resolution camera. An end-to-end software simulator was implemented, including the<br />

optimization module, to reproduce the expected experiment performance in real operations.<br />

The accuracy returned by the rotational parameters estimation module represents the figure<br />

of merit of each solution and drives the<br />

11:05 AAS The Trajectory Control Strategies of Akatsuki for Venus Orbit Reinsertion<br />

13-388 Chikako Hirose, Japan Aerospace Exploration Agency<br />

The Japanese Venus explorer "Akatsuki (PLANET-C)", which now rotates about the Sun,<br />

will approach to Venus again in 2015. For the Venus orbit re-insertion, several trajectory<br />

strategies were devised. In this paper, we introduce the difficulties we faced in redesigning<br />

the trajectory of Akatsuki after the failure of the first Venus Orbit Insertion (VOI) in 2010<br />

and report some newly devised trajectory control strategies including Gravity Brake<br />

Method, which will make the most of the solar perturbations to conduct the Venus orbit<br />

insertion for the second time.<br />

Page 78<br />

23 rd AAS / AIAA <strong>Space</strong> <strong>Flight</strong> <strong>Mechanics</strong> Meeting

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