Liftoff for LISA Pathfinder

Major step towards a gravitational wave observatory in space on 100th anniversary of Einstein's General Relativity

December 03, 2015

The LISA Pathfinder satellite mission lifted off earlier today on a Vega rocket from the European spaceport in Kourou, French Guiana, on its way to demonstrate technology for observing gravitational waves from space. “This mission is one large step towards a spaceborne gravitational wave detector. 96 percent of the Universe cannot be observed with existing astronomical methods. A future mission like eLISA will detect gravitational waves from space, for example from supermassive black hole binaries, and open a new window to the gravitational Universe,” says Prof. Dr. Karsten Danzmann, director at the Albert Einstein Institute and professor at Leibniz Universität Hannover.

The LISA Pathfinder (LPF) launch coincides almost perfectly with the 100th anniversary of the publication of Albert Einstein's theory of general relativity, published on 2 December 1915. The theory predicts the existence of gravitational waves, tiny ripples in space-time propagating at the speed of light, which so far have not been directly observed.

LPF will test the entirely new technologies required for to observe gravitational waves from space. At its core is a pair of free-floating, identical 46 mm gold–platinum cubes separated by 38 cm, which will be isolated from all external and internal forces acting on them except one: gravity.

“LISA Pathfinder will put these test masses in the best free-fall ever produced in space and monitor their relative positions to unprecedented precision,” says Karsten Danzmann, who also is the Co-Principal Investigator for the LISA Pathfinder Technology Package, the scientific heart of the satellite. “This will lay the foundations for future gravitational-wave observatories in space such as eLISA.”

Liftoff from Kourou
The Vega launcher lifted off at 4:04 GMT (5:04 CET). About seven minutes later, after separation of the first three stages, the first ignition of Vega’s upper stage propelled LPF into a low orbit, followed by another ignition about one hour and forty minutes into the flight.

The spacecraft separated from the upper stage at 5:49 GMT (6:49 CET). Controllers at ESA’s operations centre in Darmstadt, Germany then established control.

LPF is now in an elliptical orbit, its closest point to Earth at around 200 km and farthest point at around 1500 km. On December 6, a series of six thruster burns will commence, which will lift the apogee of the elliptical orbit higher and higher over the next five days.

Towards the Lagrange point
Finally, LPF will leave orbit around Earth entirely and drift on a transfer orbit towards the so-called Lagrangian point L1 – around 1.5 million kilometres away from Earth towards the Sun. LPF is expected to reach its operational orbit about 10 weeks after launch, on 13 February. After final checks, it will begin its six-month scientific mission on 1 March.

En route to the final orbit, the two test masses will be released from the locking mechanisms that hold them during launch and cruise. Once in orbit around L1, the final mechanisms will be unlocked and the test masses will no longer be in mechanical contact with the spacecraft.

Precise laser measurements
A laser interferometer will measure the position and orientation of the two test masses relative to the spacecraft and to each other with a precision of approximately 10 picometers (one hundred millionth of a millimetre). The construction of the precise optical measurement system was lead by the Max Planck Institute for Gravitational Physics (Albert Einstein Institute) in Hannover.

“The technology now flying on LISA Pathfinder is the result of more than a decade of scientific and engineering devolepment. It is very rewarding to see the satellite on its way into space,” says Dr. Jens Reiche the LISA Pathfinder National Project Manager at the Albert Einstein Institute in Hannover.

Data analysis in Hannover
The main scientific mission of LPF begins on March 1, 2016 and will last for at least six months. “The satellite is a complex spaceborn laboratory with which we will conduct several dense series of experiments to measure the near-perfect free fall,” says Dr. Martin Hewitson, responsible for the data analysis software developed at the Albert Einstein Institute in Hannover. These experiments will determine all non-gravitational parasitic accelerations, identify important sources of disturbances and further minimize those if necessary.

The Max Planck Institute for Gravitational Physics in Hannover is one of the leading partners in the development of the data analysis software which plays a central role in extracting the crucial information from the measurement data. For this purpose the institute has set up an operations control room in Hannover. Since an immediate data analysis is required for the configuration of follow-up experiments, scientist from the institute will also take part in the around-the-clock shifts in the European Space Operations Centre (ESOC) in Darmstadt, Germany.

LPF is an ESA mission, with the European space industry under the overall integration responsibility of Airbus DS and research institutions from France, Germany, Italy, the Netherlands, Spain, Switzerland and Great Britain as well as NASA participating.

LPF is funded through the German Aerospace Center (Deutsches Zentrum für Luft- und Raumfahrt; DLR) by the Federal Ministry for Economic Affairs and Energy based on a resolution of the German Bundestag.

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