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LISA Pathfinder set for launch site

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Posted September 2, 2015

LISA Pathfinder, ESA’s demonstrator for spaceborne observations of gravitational waves, is ready to leave for Europe’s Spaceport in Kourou, French Guiana.

LISA Pathfinder launch composite at IABG’s space test centre in Ottobrunn, near Munich, Germany, on 31 August 2015, before it departs to the launch site. Copyright ESA–P. Sebirot, 2015

LISA Pathfinder launch composite at IABG’s space test centre in Ottobrunn, near Munich, Germany, on 31 August 2015, before it departs to the launch site. Copyright ESA–P. Sebirot, 2015

Scheduled for launch on a Vega rocket later this year, the spacecraft was on display today at IABG’s test centre in Ottobrunn, near Munich, Germany, where final integration and extensive tests were performed over the past few months.

This was the last chance for scientists, engineers and members of the media to see LISA Pathfinder before it is packed for shipping.

“This is an extremely challenging mission that will pave the way for future space-based projects to observe gravitational waves, opening a new window to explore the cosmos,” said Paul McNamara, ESA’s project scientist.

Gravitational waves are ripples in the fabric of spacetime produced by accelerating massive bodies, such as a pair of orbiting black holes. Predicted by Albert Einstein’s general theory of relativity in 1915, they are expected to be ubiquitous in the Universe, but have not been directly detected to date.

This exploded view shows the LISA Pathfinder spacecraft in its entirety. The solar array provides power to the payload and support systems, and shields its sensitive payload from the Sun. Beneath the array is the white- and gold-hued science module, which carries the payload with the test masses and their electrode housings, the optical bench interferometer, and vacuum enclosure. All of these components fit neatly within the central cylinder, which in turn slots into the centre of the science module. The science module also contains support systems for LISA Pathfinder’s scientific experiments, and carries micronewton thrusters on its outer panels to adjust the position of the spacecraft. The propulsion module at the bottom of the exploded view will help LISA Pathfinder reach its final orbital location. Copyright ESA/ATG medialab

This exploded view shows the LISA Pathfinder spacecraft in its entirety. The solar array provides power to the payload and support systems, and shields its sensitive payload from the Sun. Beneath the array is the white- and gold-hued science module, which carries the payload with the test masses and their electrode housings, the optical bench interferometer, and vacuum enclosure. All of these components fit neatly within the central cylinder, which in turn slots into the centre of the science module. The science module also contains support systems for LISA Pathfinder’s scientific experiments, and carries micronewton thrusters on its outer panels to adjust the position of the spacecraft. The propulsion module at the bottom of the exploded view will help LISA Pathfinder reach its final orbital location. Copyright ESA/ATG medialab

While ground-based searches for these elusive messengers of gravity have been under way for the past few decades, a gravitational-wave observatory in space would open up new possibilities in this quest.

LISA Pathfinder will test the fundamental technologies and instrumentation needed for such an observatory, demonstrating them for the first time in space.

“Gravitational waves are an entirely fresh and different way to study the Universe, providing an important complement to the well-established approach of astronomy, based on observing the light emitted by celestial bodies,” says Paul.

LISA Pathfinder’s journey from launch to its final destination, around the L1 Sun–Earth Lagrangian point some 1.5 million km away from Earth towards the sun. Vega, designed to take small payloads into low orbit, will place LISA Pathfinder into an elliptical orbit, with a perigee (closest approach) of 200 km, apogee (furthest approach) of 1540 km, and angled about 6.5º to the equator. Then, when Vega’s final stage is jettisoned, LISA Pathfinder will continue under its own power, beginning a series of six apogee-raising manoeuvres powered by its own propulsion system. These manoeuvres will be completed two weeks after launch. After this, LISA Pathfinder will cruise towards its final orbiting location. A month after its final burn, it will jettison its propulsion module and continue its journey before settling into an orbit around the L1 Sun–Earth Lagrangian point. The entire journey, from launch to arrival at the operational orbit around L1 will take about eight weeks. Copyright ESA/ATG medialab

LISA Pathfinder’s journey from launch to its final destination, around the L1 Sun–Earth Lagrangian point some 1.5 million km away from Earth towards the sun. Vega, designed to take small payloads into low orbit, will place LISA Pathfinder into an elliptical orbit, with a perigee (closest approach) of 200 km, apogee (furthest approach) of 1540 km, and angled about 6.5º to the equator. Then, when Vega’s final stage is jettisoned, LISA Pathfinder will continue under its own power, beginning a series of six apogee-raising manoeuvres powered by its own propulsion system. These manoeuvres will be completed two weeks after launch. After this, LISA Pathfinder will cruise towards its final orbiting location. A month after its final burn, it will jettison its propulsion module and continue its journey before settling into an orbit around the L1 Sun–Earth Lagrangian point. The entire journey, from launch to arrival at the operational orbit around L1 will take about eight weeks. Copyright ESA/ATG medialab

Among the anticipated sources of gravitational waves are supernova explosions and double black holes. These objects are thought to be associated with overwhelmingly powerful events. For example, the energy released in gravitational waves during the last few minutes of the merging of just one pair of supermassive black holes is comparable to the total energy emitted as light by all stars and galaxies across the cosmos over the same time.

Scientists are also looking forward to discovering even more, unexpected cosmic sources once they are able to ‘listen’ to the Universe on this new channel.

“But we’re not quite there yet, and this is where LISA Pathfinder steps in,” says César García Marirrodriga, ESA’s project manager.

Gravitational waves are ripples in the fabric of spacetime produced by accelerating massive bodies to Albert Einstein’s general theory of relativity. In general relativity, gravity manifests itself as massive objects bending the structure of spacetime. In addition, something else happens if the gravitational field varies, for example when two massive objects orbit each other. The motion of massive bodies through spacetime perturbs its very fabric, imprinting a signal that travels away as a disturbance to the structure of spacetime itself: gravitational waves. The animation visualises the effect of these oscillations, which consist of sequential stretches and compressions of spacetime, rhythmically increasing and reducing the distance between particles as a wave propagates through the surroundings. It is thought that gravitational waves are abundant across the Universe, typically produced by powerful sources such as supernova explosions and pairs of orbiting black holes. However, despite the attempts of ground-based experiments to detect them directly, gravitational waves so far remain elusive. Copyright ESA–C.Carreau

Despite the enormous energy release in gravitational waves produced by these mighty cosmic events, they should only cause tiny perturbations to the fabric of spacetime. Instruments built to detect them must be capable of making exquisitely precise measurements of extremely small changes in distance between two reference objects.

Typically, for a space-based gravitational wave observatory, this will mean seeing the distance between two ‘test masses’ separated by around a million kilometres changing by about a millionth of a millionth of a metre.

This requires extraordinary measurement techniques using lasers, with the test masses flying freely in space, each shielded by a surrounding spacecraft from all extraneous influences, such as the solar wind.

LISA Pathfinder will test those crucial underlying technologies in a single spacecraft, with the two test masses separated by only 38 cm. The aim is to prove that the masses can fly through space, untouched but shielded by the spacecraft, and maintain their relative positions to the precision needed to realise a full-up gravitational wave observatory later.

“The extreme precision of measurements and control required in this domain pose a great technical challenge,” says Cesar.

“In fact, everything was a challenge in this brand-new class of missions: from the innovative instrumentation, to the new modelling of self-gravitation within the spacecraft, and the very complex integration tests of the spacecraft.

“The industrial and scientific teams that undertook these daunting tasks have done an extraordinary job, and now the mission is ready for launch.”

After ascent on the Vega rocket, LISA Pathfinder will enter an elliptical orbit around Earth, where it will use its own propulsion system to raise the high point of its orbit.

Eventually, after about eight weeks, the spacecraft will reach its operational orbit around the Lagrange point L1, 1.5 million km from Earth towards the Sun.

There, LISA Pathfinder will begin six months of demonstrating the technology for future gravitational-wave observatories in space.

“We’ve made great progress with LISA Pathfinder in the past decade and are very excited to be so close to operating this incredible physics laboratory in space,” concludes Paul.

Source: ESA

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