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ESA Document - Emits - ESA

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s<br />

Z (m)<br />

x 10<br />

-1<br />

4<br />

0<br />

1<br />

2<br />

3<br />

4<br />

Impulsive Hohmann Transfer<br />

Applied Delta V<br />

Station Keeping<br />

Forced Motion<br />

Station Keeping<br />

Forced Motion<br />

Free Drift<br />

Trajectory in CRF (height vs. X)<br />

-16 -14 -12 -10 -8 -6 -4 -2 0 2<br />

x 10 4<br />

5<br />

X (m)<br />

Figure 4-110: Intermediate rendezvous<br />

HMM<br />

Assessment Study<br />

Report: CDF-20(A)<br />

February 2004<br />

page 374 of 422<br />

4.5.2.4.2 Terminal rendezvous<br />

Next, the crew commands a forced approach to the next hold point located at 100 meters in front<br />

of the target and also in V-bar. This new hold point will be the base of a station keeping<br />

manoeuvre that will allow the crew to check again the status of the subsystem and the<br />

availability of the docking port, etc.<br />

Finally, a new forced approach is commanded and the MAV reaches the docking port of the<br />

Orbiter that establishes the structural latching of all required elements.<br />

4.5.2.4.3 Transfer of crew and dedocking<br />

Finally the structural latching occurs. The crew is transferred from the MAV to the orbiter. After<br />

that the MAV is ejected. Then there is a check out of all orbiter subsystems. Once this is done,<br />

the departure to Earth can begin.<br />

4.5.2.5 Baseline design<br />

The MAV final stage is a three-axis stabilised spacecraft.<br />

The attitude determination main sensors are the star tracker (STR) and the inertial measurement<br />

unit (IMU). During Sun acquisition and safe modes, Sun acquisitions sensor and Earth infrared<br />

sensors are principally used. The two STRs that will be operated in parallel for some phases of<br />

the mission.

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