ESA - LISA Mission patch.
7 March 2011
A key technical challenge of the joint ESA–NASA LISA mission has been solved: how to maintain precise pointing of a laser beam across five million km of space.
The next-decade Laser Interferometer Space Antenna (LISA) mission will look for ripples in spacetime – their existence predicted by Albert Einstein – known as gravitational waves. A trio of identical spacecraft will fly five million km apart in an equilateral triangle formation, linked by laser beams.
LISA satellite connected by lasers
A precision-measuring method called interferometry can combine these laser beams to identify the slightest movement between free-floating metallic cubes within each spacecraft.
Motion within a set frequency range will be scrutinised to search out gravitational waves emitted by massive black holes and similarly energetic cosmic objects.
“Our research set out to solve one of LISA’s most challenging elements,” said Lucio Scolamiero, overseeing some of the LISA technology studies for ESA.
Three LISA spacecraft
“How do we maintain the optical pathways between the spacecraft and therefore the measurement chain between them?”
Owing to the finite speed of light, it will take 16 seconds for each laser beam to cover the five million km to its receiving spacecraft.
LISA must steer the laser beam to compensate for the orbital movement of each spacecraft during this time.
In the process, the steering mirror has to remain stable down to the subatomic scale: any motion would be misinterpreted as a gravitational wave.
“That this could be achieved at all was by no means certain: to begin with, we didn’t even have available means to measure the performance of such a system,” Lucio added.
TNO-developed pointing system
“But we received two promising proposals and decided to pursue both of them.”
The two designs were developed independently by separate industrial groups: TNO in the Netherlands and RUAG and CSEM in Switzerland.
“ESA doesn’t duplicate technology development but does sometimes pursue complementary approaches,” Lucio explained.
RUAG & CSEM pointing system
“If one proves inadequate then we have another as backup.”
The two palm-sized designs share some elements. Both use capacitance-based sensors to measure mirror angle errors needing correction. Electrodes are spaced a very short distance apart; any shift in this distance causes a change in the electric charge running between them.
Test setup
The motor to make the adjustment is based on piezoelectric ceramics similar to those found in quartz watches, which convert electric signals into movement.
These ceramics are sliced up for precision performance. TNO’s design uses ‘piezo-stacks’ while RUAG–CSEM’s employs a ‘piezo-leg’ reproducing ‘walking’ motion.
To steer the mirror, both approaches reject ball-bearing components in favour of ‘flexural hinges’. Metallic blades around 0.1 mm thick are carefully shaped using a precision manufacturing technique.
The Albert Einstein Institute in Hannover, Germany, developed an ultra-stable measuring system to validate device performance. They used laser-based interferometry – the same technique LISA will rely on – with the experiment performed inside a vacuum chamber and mounted on a bench of ZERODUR glass, all-but immune to temperature-driven distortion.
“Both developments are fully compliant to our extreme performance requirements,” Lucio concluded. A decision on which version to fly will be taken later during LISA's implementation phase.
A single-satellite precursor, LISA Pathfinder, will be launched in 2013 to flight-validate key technologies for the full LISA mission, a large-mission candidate in ESA's Cosmic Vision programme.
Related links:
TNO: http://www.tno.nl/index.cfm?Taal=2
RUAG: http://www.ruag.com/
CSEM: http://www.csem.ch/
Albert Einstein Institute, Hannover: http://www.aei.mpg.de/hannover-en/66-contemporaryIssues/home/index.html
Images, Text, Credits: ESA / AEI/ MildeMarketing / Exozet / TNO / RUAG / CSEM / Albert Einstein Institute.
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