4 Final Report - Emits - ESA
4 Final Report - Emits - ESA
4 Final Report - Emits - ESA
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4 <strong>Final</strong><br />
<strong>Report</strong><br />
Alternative solutions which have been investigated are:<br />
• geostationary orbit with limited station keeping,<br />
• inclined geosynchronous orbit,<br />
• Molniya orbit (highly elliptical inclined orbit).<br />
The appealing features of these alternatives are on one hand potential propellant savings for station<br />
keeping and on the other hand improved viewing conditions over Europe.<br />
The maximum propellant saving may be achieved for a geostationary orbit with 7.5 deg inclination and<br />
0 deg initial right angle of ascending node. This orbit is rather stable such that no orbit corrections are<br />
needed. However, as it is the case for all inclined geosynchronous orbits, the orbit trace projected onto<br />
the Earth surface is a figure of eight which the satellite passes through once per orbit. This yields that<br />
the satellite is half an orbit over Northern latitudes (with better viewing conditions over Europe) and the<br />
other half orbit it is over Southern latitudes. If no corrections of the orbital plane are performed, the<br />
local time of the equator crossing will change over the year. This means that the satellite is at the most<br />
Northern position e.g. at 12:00 at a certain day of the year but half a year later this position is achieved<br />
at midnight. Hence, the good viewing conditions at daytime are achieved for a certain part of the year<br />
only and become even worse for the other part of the year. Since this feature is a significant constraint<br />
for the mission flexibility, all alternatives with inclined orbits have currently been dropped.<br />
Orbit determination performance<br />
The achievable precision for the position of the spacecraft is important since it contributes to the<br />
overall pointing budget which is rather stringent. The preferred solution with the best performance is a<br />
ranging technique based on 2 or 3 ground stations and using a spread spectrum method for the<br />
ranging signal. The orbit determination accuracy is 100 m to 150 m (3σ) along track and 10 m to 20 m<br />
(3σ) across track. The interesting feature is that this technology shows the same performance right<br />
after a manoeuvre when using 3 ground stations. Moreover, this technique is routinely used by SES<br />
Astra which gives strong evidence that it can be successfully applied to Geo-Oculus.<br />
The following alternative technologies have also been investigated:<br />
• single ground station ranging + line of sight measurements,<br />
• dual ranging,<br />
• DARTS,<br />
• short baseline interferometry,<br />
• long baseline interferometry,<br />
• optical telescope,<br />
• use of landmarks,<br />
• GPS.<br />
The GPS option is currently being investigated for geostationary orbits. It may provide a similar<br />
nominal performance as the ground based spread spectrum method but a significant degradation is<br />
expected for a couple of hours after a manoeuvre. All performance data for above listed options are<br />
found in [RD 7].<br />
Orbit transfer and launcher<br />
A geostationary transfer orbit strategy is suggested as baseline. The initial elliptical orbit provided<br />
by the launcher is changed to the final circular orbit with a liquid apogee engine installed in the<br />
spacecraft. The achievable maximum mass of the spacecraft in the final orbit is slightly higher<br />
Page 4-28 Doc. No: GOC-ASG-RP-002<br />
Issue: 2<br />
Astrium GmbH Date: 13.05.2009