CoRoT 2005 Events
2005 Events
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The CoRoT telescope, flying on a polar orbit at 896 km, has been designed to filter the thermal perturbations coming from the Earth environment (day/night cycling during periods with eclipses). Thus, these thermal tests, beyond the basic objective of technical qualification, were crucial to characterize in details the behavior of the instrument and check the overall thermal modelling. As a result of this campaign of measurements in the SIMLES chamber, at Intespace, we are now able to show the excellent thermal performances of the instrument, and in particular thoses of the most critical sub-systems: the afocal telescope, the camera and the upper part of the equipment bay hosting the analogical electronics. These tests also allowed to verify, in vacuum and at -40° C (focal unit regulation temperature), the optical performances and the detector radiometry (noises in the image spots). | |||
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The conference with written press, radio and television took place in the Intespace clean rooms, round the CoRoT payload in progress of being functionnally tested. Annie Baglin, P.I of the mission, was among us to answer journalists' questions. On November 17, the CNES project team went on with this communication event, receiving a delegation of members of Parliament, invited to visit the Toulouse Space Center. | |||
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The 2nd CoRoT Workshop in Brazil, held in Ubatuba and organized by the University of Sao Paulo, was the opportunity of fruitful exchanges between researchers preparing the CoRoT mission in Europe and Brazil. Many subjects were discussed : rotation and magnetic field effects inside stars, simulation of stellar activity in light curves, observation of young cluster (PMS stars), dynamics of extrasolar planetary systems, migration and metallicity... | |||
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After delivery of the baffle and a series of optical tests, the CoRoT instrument was integrated in the clean rooms of the Toulouse Space Center, from 16.08 to 08.09.2005. The operations performed by the CNES integration team consisted in setting the camera inside the telescope, then in assembling the optical part with the equipment bay, which is a very touchy operation. The following activities were to put in place the focal unit radiator, the MLI sheets and the probes for the environment tests to be made in the next few weeks. The instrument was transferred to Intespace on 9 September 2005. | |||
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This one-week technical trip to Baïkonour (Kazakhstan) allowed the satellite teams from CNES and Alcatel to better know the Starsem facilities which will be used for the CoRoT launch campaign. Among the reviewed subjects : An-124 aircraft offloading, campaign scenario, safety for satellite fueling operations, remote monitoring, launch pad activity. The launch fo CoRoT is foreseen summertime 2006, by a SOYUZ 2-1B rocket. | |||
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During last Paris Air Show, CNES President Yannick d'Escatha and AEB President Sergio Mauricio Gaudenzi signed the agreement establishing the participation of Brazil in CoRoT. The agreement adresses the reception of the scientific telemetry data by the Alcantara earth terminal and the implication of Brazilian researchers and engineers in the development of the user ground segment. Observatories in Brazil will also contribute to the scientific program of joint ground observations. In return, the astronomers community in Brazil will have a privileged access to the CoRoT data through several Co-Investigators. | |||
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This scientific workshop, organized by CNES with the Midi-Pyrénées Observatory, was the opportunity to bring together more than 120 researchers coming from the CoRoT community.
Three new thematic groups have been created: DAT (asteroseismology data analysis), Binary Systems, ACROCoRoT (convection, rotation, surface activity). Fifteen months before expected launch date (summertime 2006), this workshop gave the chance to every participant to see the CoRoT telescope, being integrated in our clean rooms, and also to visit the satellite control center. | |||
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In order to improve and secure the reception of CoRoT scientific telemetry data, the project team starts discussions with the Vienna Observatory on the possibility to share the ground station (3-meter dish antenna) developped and used since July 2003 for MOST telemetry data reception. | |||
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In the night of the 13th April 2005, the CoRoT telescope, being integrated in the CST clean rooms, was pointed toward the sky and performed a first set of pictures in the vicinity of the Polaris star. The analysis of these images will make it possible to check some optical parameters (geometry and photometry), but the pictures, acquired at room temperature and with air turbulence, are yet a bit far from the instrument final performances, expected in space. | |||
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Agenda
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These successful tests mark the final qualification of the baffle, after correction (under CSL responsability) of several mechanical anomalies seen during a first series of tests in August 2004. In particular, the feet to fix it to the upper telescope plate have been modified. | |||
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Agenda
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