16 June 2015
The Core Assembly of the LISA Technology Package (in the centre) was constructed by Airbus Defence and Space, and was integrated into the LISA Pathfinder by IABG in Munich.
Airbus Defence & Space.
The Core Assembly of the LISA Technology Package (in the middle) during integration by Airbus Defence and Space in Friedrichshafen.
Before LISA Pathfinder can launch into space, the payload must first be thoroughly tested. During the vibration tests, the LTP Core Assembly was checked to ensure that it will be able to withstand the violent accelerations of the rocket launch without sustaining damage.
LISA Pathfinder will test in space the technology that be used for the eLISA Gravitational Wave Observatory. The eLISA space observatory will consist of three spacecraft – a mother craft and two daughter craft. They will be positioned in a near-equilateral triangle formation, with each side measuring approximately two million kilometres. The entire triangle will rotate and follow Earth on its orbit around the Sun at distances ranging between 10 and 25 million kilometres. The spacecraft are connected by laser beams – a feat of unprecedented technical precision. The observatory will be able to ‘hear’ any gravitational waves that pass through their alignment in a frequency range of between 0.1 millihertz and 0.1 hertz.
After more than 10 years of intense development, Airbus in Friedrichshafen has completed the main component that will be at the heart of the highly sensitive payload of the LISA Pathfinder mission – the LISA Technology Package (LTP) Core Assembly. The German Aerospace Center (Deutsches Zentrum für Luft- und Raumfahrt; DLR) is supporting LISA Pathfinder within the framework of the European Space Agency (ESA) Science Programme. The mission, to be launched in October this year, is designed to validate important technologies whose function and performance capabilities cannot be tested here on Earth, or where only partial testing would be possible on the ground. This mission will pave the way for the Evolved Laser Interferometer Space Antenna (eLISA) gravitational wave observatory that, after its scheduled launch in 2034, will track down the highest-energy and most violent astrophysical events unfolding across the Universe.
Tuning into the 'sound' of the universe
If a stone is dropped in water, oscillations spread in waves across the surface of the water from the point of impact. Like stones falling into water, substantial masses that move through space extremely quickly and with rapidly changing acceleration also produce waves. These propagate through space and inevitably announce their presence as very small oscillations in space-time. These gravitational waves – predicted by the German physicist Albert Einstein in his Theory of General Relativity as far back as 1916 – allow us to 'listen to the sound' of the Universe, opening a new and unobstructed window to observe exotic celestial objects.
Among these are supernovae, close binary star systems consisting of white dwarfs, collisions between neutron stars and pulsars or black hole collisions during galaxy mergers. In the core of galaxies, objects such as white dwarfs, neutron stars or black holes, may travel towards the super massive black hole at the centre; if they get close enough, they will start to spiral in as their orbits shrink as a result of the loss of energy and angular momentum carried away by gravitational waves (extreme-mass-ratio inspirals). Gravitational waves from the time immediately after the Big Bang can reveal more about the origin of the Universe. However, Einstein was somewhat doubtful that gravitational waves would ever be detected, as their effects are extremely small; it has not been possible to measure them so far. But today – almost 100 years after Einstein's prediction, mankind is on the verge of making their 'extremely quiet' oscillations 'audible'. It is expected that proof will be furnished in the coming years – initially using ground-based systems, and subsequently with eLISA out in space.
LISA Pathfinder prepares the way for eLISA
The eLISA space observatory will consist of three spacecraft – a mother craft and two daughter craft. They will be positioned in a near-equilateral triangle formation, with each side measuring approximately two million kilometres. The entire triangle will rotate and follow Earth on its orbit around the Sun at distances ranging between 10 and 25 million kilometres. The spacecraft are connected by laser beams – a feat of unprecedented technical precision. The observatory will be able to 'hear' any gravitational waves that pass through their alignment in a frequency range of between 0.1 millihertz and 0.1 hertz. The necessary technology requires initial testing in space, as the mission is extremely complex and involves components that cannot be tested adequately on the ground.
LISA Pathfinder will handle this task. The components used in the scientific payload – the LTP – were developed by several European countries and put together to form a composite payload by Airbus Defence & Space in Friedrichshafen. DLR played a key role in the development of the payload within the framework of the ESA Science Programme. Here, the German contribution received a substantial boost from a grant awarded by the DLR Space Administration to the Max Planck Institute for Gravitational Physics (Albert Einstein Institute) in Hannover.
Highly sensitive measurement system
The LTP control electronics in the LISA Pathfinder orbiter have been installed and tested, and the final and most important unit in the payload, the LTP Core Assembly, will follow shortly. Its construction is now complete, and the unit has been sent from Friedrichshafen to IABG in Munich for integration into the spacecraft and final testing.
During the mission, two identical cube-shaped test masses, each weighing two kilograms, will be suspended in their own LTP vacuum vessel, almost free of internal and external disturbances, hence demonstrating free flight in space. A special gold-platinum alloy has been used for the masses, ensuring that magnetic forces do not have any effect. Using ultraviolet radiation, a contactless discharge system prevents any electrostatic charging of the masses. The caging and venting mechanism – responsible for protecting the test masses from intense vibrations during launch, releasing them in a highly controlled setting, and capturing them as necessary – is a particular challenge in this context. The laser interferometer will measure the position and orientation of the two test masses relative to the spacecraft and to each other at a precision of approximately one hundred millionth of a millimetre. In addition, there are other, less precise, sensors that also help determine their positions. A Drag-Free Attitude Control System (DFACS) uses the measurement data to control the spacecraft and to ensure it always remains centred on the test masses. Cold gas micronewton thrusters developed for the Gaia astrometry mission, which have the capability of delivering propulsion in extremely fine and uniform amounts, will control the position of the spacecraft.
The mission is scheduled for launch in October 2015. A one-year period of operation in an orbit around L1, approximately 1.5 million kilometres from Earth towards the Sun, will follow after launch. The Lagrangian points, named after Joseph-Louis Lagrange, are positions in which a gravitational state of equilibrium occurs, meaning that (in ideal cases), a spacecraft can 'linger' there.
Last modified:18/06/2015 08:18:09