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4 Final Report - Emits - ESA

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4 <strong>Final</strong><br />

<strong>Report</strong><br />

Oculus, whereas MWI 100-100/100 has a bigger rotor and different motor design.<br />

Prototype MBW<br />

Figure 4.4-1: MBW characteristics and photography of the prototype MBW (courtesy of RCT)<br />

The microvibration levels generated by the prototype MBW wheels have been characterised in 2007<br />

by EADS Astrium GmbH in the frame of the DLR study “High Precision Attitude Control of Earth<br />

Observation Satellites”. The results of this study show that the MBW disturbance levels are lower by a<br />

factor of 10 to 240 (depending on frequency and wheel rotation rate) than typical BBW levels.<br />

However, it shall be noted that the comparison is supposing hard-mounted wheels, whereas a BBW<br />

mounted on an elastomeric suspension would be the actual competitor for a high accuracy pointing<br />

mission. Moreover, microvibrations is analysed at the source, whereas its impact on LoS at PLM level,<br />

largely dependent on structure transmission is the relevant parameter. It is undoubted that the<br />

microvibrations will be lower, but the above ratios shall not be taken as granted.<br />

The MBW appear in all cases as a good candidate for the Geo-Oculus mission, due to its inherent low<br />

microvibration content. The low maturity level (TRL ~4) and the associated development and technical<br />

risks shall also be accounted for. The pre-development needs to be actively pursued to reach TRL 5 at<br />

the beginning of phase C/D.<br />

4.4.2.3 Ball Bearing Wheel (BBW) option<br />

A second option is to use standard ball bearing wheels mounted on elastomeric mounts developed for<br />

LEO observation missions. This option has been analysed in 2007 in the frame of the CNES study<br />

“Constraints for High resolution observation on GEO”. A microvibration analysis was performed for<br />

three different structural transmissions, without elastomeric suspension, with a 15 Hz suspension, and<br />

with a 30 Hz one. Microvibration levels measured on 8 flight models of Pleiades BBW (18 Nms Teldix<br />

RSI) are used as input to the structural model, typical of a GEO spacecraft equipped with an optical<br />

payload for Earth observation. The results are post-processed so that to show the peak-to-peak<br />

variation of the LoS over an integration time of 70 ms. The results of this study are therefore directly<br />

relevant for Geo-Oculus.<br />

Doc. No: GOC-ASG-RP-002 Page 4-45<br />

Issue: 2<br />

Date: 13.05.2009 Astrium GmbH

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