LISA Pathfinder: Time called on Europe's gravity probe

The European Space Agency (Esa) has turned off one of its most successful ever missions.

LISA Pathfinder was sent into orbit in 2015 to prove key technologies that could be used on some future project to detect gravitational waves - the ripples that disturb space-time whenever black holes collide.

The satellite spectacularly surpassed the objectives set for it.

And that success led directly to the selection in June of the LISA mission.

This billion-euro venture, which is envisaged as a trio of satellites, is expected to launch between 2030 and 2034.

It will incorporate many of Pathfinder's systems, including its all-important laser interferometer instrumentation that we now know has the means necessary to catch gravitational waves (GW) in space.

"LISA Pathfinder has shown that LISA is feasible at full sensitivity, more than we could hope for," said principal investigator Stefano Vitale.

"I think it has been a stepping stone for GW astronomy, and an incredibly rewarding experience for all the team involved. Thank you, and stay tuned on LISA!" he told BBC News.

Prof Vitale was invited to send the final "kill commands" to Pathfinder, which has been conducting its measurement demonstration 1.5 million km from Earth in the sunward direction.

The commands, despatched from Esa's mission control centre in Darmstadt, Germany, tricked Pathfinder to reboot itself on to software that had already been corrupted.

It meant the gravity probe was locked down, unable to run its subsystems including its transmitter.

"The only way you could recover the spacecraft would be to go up there and attach an umbilical and restart from another computer," explained Pathfinder's spacecraft operations manager, Ian Harrison.

The kill procedure, more properly known as "passivating" the satellite, ensures there is no hazard to future missions through a collision or interference of radio communications.

The Darmstadt team in April had already fired the thrusters on Pathfinder to move it away from its station - a popular location for many Sun-studying missions.

It should now drift harmlessly around our star.

"There's a very, very small chance it could return to the Earth-Moon system; it's so remote but you can't actually say it's zero," said Ian Harrison.

"The mission analysis actually looked at the planetary positions 500 years into the future."

  • Gravitational waves are a prediction of the Theory of General Relativity
  • It took decades to develop the technology to directly detect them
  • They are ripples in the fabric of space-time generated by violent events
  • Accelerating masses will produce waves that propagate at the speed of light
  • Detectable sources ought to include merging black holes and neutron stars
  • LIGO fires lasers into long, L-shaped tunnels; the waves disturb the light
  • LISA will fire lasers between three spacecraft separated by 2.5 million km
  • Detecting the waves opens up the Universe to completely new investigations

Gravitational waves are the big thing in science right now.

Ground-based laboratories in the US have recently begun detecting them from coalescing objects that are 20-30 times the mass of our Sun.

But by sending an observatory into space, scientists would expect to discover sources that are millions of times bigger still, and to sense their activity all the way out to the edge of the observable Universe.

It should significantly advance our understanding of gravity and how it works; and perhaps even highlight some chinks in Einstein's so-far flawless equations.

LISA will detect gravitational waves by bouncing laser light between three spacecraft flying in a triangle formation, where the sides of the triangle are 2.5 million km long. The light beams will be measuring the precise positions of small, free-floating blocks inside the satellites.

When gravitational waves pass through the triangle, the distance between blocks of the different spacecraft should change by tiny amounts - just fractions of the width of an atom.
Share on Google Plus

About SuperNova

This is a short description in the author block about the author. You edit it by entering text in the "Biographical Info" field in the user admin panel.


Post a Comment