LISA Pathfinder arrives at its worksite

January 25, 2016
LISA Pathfinder, ESA's mission to test technology for future gravitational-wave observatories in space, depicted after the separation of the propulsion module.  LISA Pathfinder launched on 3 December 2015, and used its propulsion module to raise its orbit six times and embark on the path to its operational orbit. After releasing the propulsion module on 22 January, the science module will enter its final orbit around the first Sun–Earth Lagrangian point L1, 1.5 million km from Earth in the direction of the Sun. Credit: ESA

After a six-week journey, LISA Pathfinder arrived at its destination today, an orbit around a point of balance in space where it will soon start testing technologies crucial for exploring the gravitational Universe.

LISA Pathfinder is testing the key elements that could be used for a future mission to detect gravitational waves – ripples in spacetime predicted by Albert Einstein in his General Theory of Relativity.

To this end, it will release two test masses into near-perfect free fall and measure their motion with unprecedented accuracy.

LISA Pathfinder was launched on 3 December 2015 and arrived today in its orbit around 'L1', the first libration point of the Sun-Earth system, a virtual point in space some 1.5 million km from Earth towards the Sun.

LISA Pathfinder's arrival came after a final thruster burn using the spacecraft's hard-working propulsion module on 20 January. The small, 64-second firing was designed to slightly change its speed and just barely tip the craft onto its new orbit about L1.

Since launch, the propulsion module raised the orbit around Earth six times, the last of which kicked it towards L1.

"We had planned two burns to get us into final orbit at L1, but only one was needed," says Ian Harrison, Spacecraft Operations Manager at ESA's ESOC operations centre in Darmstadt, Germany.

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The journey and final orbit of LISA Pathfinder, ESA’s technology demonstration mission that will pave the way for future gravitational-wave observatories in space. LISA Pathfinder is scheduled for launch on 2 December 2015 on a Vega rocket from Europe’s Spaceport in French Guiana. Vega will place the spacecraft into an elliptical orbit, with a perigee (closest approach to Earth) of 200 km, apogee (furthest point) of 1540 km, with the path angled at 6.5º to the equator. Then, once Vega’s final stage is jettisoned, LISA Pathfinder will continue under its own power, beginning a series of six apogee-raising manoeuvres over the next two weeks. The last burn will set LISA Pathfinder on its way towards its final orbiting location. The cruise will last about six weeks, and the propulsion module will be discarded along the way four weeks in. Eventually, the spacecraft will circle the L1 Sun–Earth Lagrangian point. There, LISA Pathfinder will begin its six months of demonstrating key technologies for space-based observation of gravitational waves. Credit: ESA/ATG medialab

Separation after arrival 1.5 million km away

The propulsion module separated from the science section at 11:30 GMT (12:30 CET) today after the combination was set spinning for stability.

"Heat and vibration from the regular, hot thrusters on the propulsion module would cause too much disturbance during the spacecraft's delicate technology demonstration mission," notes Ian. "Primary propulsion during the rest of the mission will be provided by cold-gas microthrusters to keep us at L1."

These small thrusters were used in the hours after separation to kill the spin and stabilise the spacecraft.

Today's operations were monitored by the mission control and science teams at ESOC in real time via the Agency's deep-space station at Malargüe, Argentina.

During this evening, the craft will be slowly turned to point towards Earth and, around midnight, establish a full communications link via ESA's New Norcia ground station, Australia.

Next week, LISA Pathfinder's trajectory will be fine-tuned with a series of three microthruster bursts, taking it onto its final orbit, a 500 000 × 800 000 km around L1.

L1 was chosen because it is a quiet place in space, far away from large bodies such as Earth and is ideal for communications.

Preparing to test future technology

Preparing the spacecraft's systems and payload for work has already begun, with the full platform, the thrusters and the Disturbance Reduction System having already been checked.

Last week, the laser that will measure the most precise free-fall ever obtained in space was switched on and tested.

Next month, the two identical test cubes will be released in two steps. First, the launch lock fingers on the eight corners of each cube will be retracted on 3 February. Then, other mechanisms that secure the cubes will be released on 15 and 16 February.

This will enable the craft to begin, on 1 March, demonstrating that we can measure the separation of target masses with the extremely high accuracy required to measure from space in the future.

The relative motion of the two cubes will be measured by laser to within a staggering a billionth of a millimetre.

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