Mars Express Mission Controllers Ready for NASA Phoenix Landing 20 May 2008

Mars Express Mission Controllers Ready for NASA Phoenix Landing 20 May 2008

Mars Express mission controllers ready for NASA Phoenix landing 20 May 2008 Operations Centre, Darmstadt, Germany. The Mars Express team will monitor the event from the Dedicated Control Room at ESOC. Effective reuse of on-board lander communications system Mission controllers will use the MELACOM (Mars Express Lander Communications) system to point towards Phoenix during EDL; the radio instrument was originally intended for communications with the Beagle 2 lander. Artist's impression of parachute deployment during Phoenix's descent to Mars. Credits: NASA - JPL Mars Express will perform a high-speed slew as MELACOM tracks Phoenix, rotating about one axis at a speed some two to three times faster than normal; this action has already been tested and ESA's Mars Express mission control team are confirmed. The orbit phasing of Mars Express was ready to monitor Phoenix's critical entry, descent already adjusted at the end of 2007 to provide and landing onto the Martian surface on 26 May visibility to Phoenix. 2008. Data recording is scheduled to begin at 23:21 UTC, The Mars Express mission control team have and run for 26 minutes, until 23:47 UTC. completed major preparations for supporting the entry, descent and landing (EDL) phase of NASA's "Our MELACOM data will enable NASA to confirm Phoenix mission to the Red Planet. On 25 May, the Phoenix lander's descent characteristics, Mars Express will point towards Phoenix's planned including speed and acceleration through the Mars entry trajectory and record signals broadcast from atmosphere," says Peter Schmitz, Deputy the lander as it plunges through the Martian Spacecraft Operations Manager and project lead atmosphere. for Mars Express Phoenix support activities. The recorded data will serve as a useful and MELACOM data will be downloaded to Earth via potentially crucial back-up to compare Phoenix's NASA's Deep Space terminals DSS-15 and planned and actual descent profiles. Landing is DSS-25. After a 15-minute, 20-second light-speed planned for 23:38 UTC, 25 May, which is 01:38 travel time, ESOC will receive the data transmitted CEST, 26 May. from Mars Express, i.e. at 00:40 UTC ( 02:40 CEST). Recorded data will subsequently be "We have tested a specially designed slew for our downloaded two more times to ensure no loss of spacecraft, and scheduled a series of data packets. downloads immediately after Phoenix's landing; NASA will receive our recorded data about one The ESA spacecraft will also fly over Phoenix's hour later," says Michel Denis, Spacecraft intended landing zone, beginning at 06:12 UTC Operations Manager at ESOC, ESA's Space (08:12 CEST) on 26 May and will again monitor 1 / 2 signals transmitted up from the surface. In the following week, Mars Express will monitor Phoenix using MELACOM 14 more times; at least one of these will be used to demonstrate and confirm that the ESA spacecraft can be used as a data relay station for NASA, receiving data from the surface and transmitting test commands to the lander. This capability has already been trialed between Mars Express and NASA's Mars Exploration Rovers (MER), now operating on the surface. In the days leading up to the Phoenix landing, NASA and ESA ground stations also cooperated to perform highly sophisticated 'delta-DOR' (delta - Differential One-way Range) interferometry measurements. This enabled a precise determination of whether Phoenix was on track to meet the planned entry point. This is the first time that ESA has been requested to operationally support NASA with the delta-DOR equipment installed at the Agency's two deep- space tracking stations, in Cebreros, Spain, and New Norcia, Australia. Source: European Space Agency APA citation: Mars Express mission controllers ready for NASA Phoenix landing (2008, May 20) retrieved 25 September 2021 from https://phys.org/news/2008-05-mars-mission-ready-nasa- phoenix.html This document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, no part may be reproduced without the written permission. The content is provided for information purposes only. 2 / 2 Powered by TCPDF (www.tcpdf.org).

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