Pre-Phase A Report - Lisa - Nasa
Pre-Phase A Report - Lisa - Nasa
Pre-Phase A Report - Lisa - Nasa
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Chapter 7<br />
Spacecraft Design<br />
7.1 System configuration<br />
7.1.1 Spacecraft<br />
The spacecraft configuration is shown in Figure 7.1 . It consists of a cylinder with a<br />
height of 480 mm and a diameter of 1800 mm. It supports a Y-shaped tubular structure,<br />
the payload thermal shield, which serves to reduce the effects of changes in the solar<br />
luminosity on the optical assemblies contained in the two arms of the Y. A top lid across<br />
the cylinder (not shown in Figure 7.1) prevents sunlight from striking the payload thermal<br />
shield. The spacecraft equipment is mounted on the inside wall of the structural cylinder.<br />
Extending out from the structural cylinder is a sun shield that keeps sunlight off the<br />
cylinder wall. The main solar panels are mounted on this sun shield.<br />
The spacecraft structural cylinder and the payload thermal shield are made of a graphiteepoxy<br />
composite chosen for its low coefficient of thermal expansion. The payload thermal<br />
shield is gold-coated and suspended by stressed fiberglass bands from the spacecraft cylinder<br />
to thermally isolate it from the spacecraft. The optical assemblies are in turn thermally<br />
isolated from the payload thermal shield. On the outside of the spacecraft cylinder the<br />
FEEP (Field Emission Electric Propulsion) thruster blocks are mounted in six clusters of<br />
four thrusters each.<br />
Outside of the payload thermal shield, pointing parallel to the arms, star trackers are<br />
mounted on the lower side of the solar panel rim. For redundancy, a total of 4 star<br />
trackers are used. In addition Fine Sun Sensors and Sun Acquisition Sensors are mounted<br />
on the spacecraft.<br />
Two steerable 30 cm diameter high-gain X-band antennas are mounted via suitable interface<br />
structures on the outside of the spacecraft, far enough inside the central cylinder<br />
diameter to avoid interference problems during separation. The antennas, used during the<br />
operational phase, provide the necessary 2π coverage in azimuth. Low- and medium-gain<br />
antennas are mounted on short booms at the lower side of the structural cylinder.<br />
In the operational heliocentric orbit the spacecraft nominal orientation is such that the<br />
YZ-plane coincides with the plane of the interferometer. Thus the spacecraft X-axes<br />
make an angle of 30◦ with the Sun direction. The angle between the X-axis and the Earth<br />
Corrected version 2.08 143 3-3-1999 9:33