The Gravitational Wave Hunt Heads to Space

By Nathaniel Scharping | March 8, 2016 4:24 pm
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An artist’s rendering of LISA Pathfinder floating in space. (Credit: ESA–C.Carreau)

As scientists announced the discovery of gravitational waves for the first time last month, an even more sensitive experiment was already underway.

Scientists officially took the hunt for gravitational waves to outer space when the LISA Pathfinder mission launched in December 2015. LISA is a floating experiment parked nearly one million miles away from Earth, at the exact point where the gravitational pull of the Earth is matched by that of the sun. LISA Pathfinder officially started the science portion of its mission Monday, and will test whether it’s possible to build a hyper-sensitive, space-based gravitational wave detector. The success of the LISA experiment hinges on getting two small gold-platinum cubes to float perfectly still about 16 inches apart in the vacuum of space.

Over the next six months, researchers will put the spacecraft and cubes through a battery of tests to understand the ways different forces could disturb the test cubes’ perfect free fall. The idea is to eliminate all the noise, except the noise generated by a passing gravitational wave.

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LISA’s journey to its final destination, almost a million miles away from Earth, toward the Sun. Credit: ESA/ATG medialab

First Steps

LISA is not meant to find gravitational waves, however. The current mission is meant only as a proof-of-concept, and to tease out design flaws and test the equipment aboard the spacecraft in preparation for the next phase of the mission, called eLISA. That mission is set to launch in 2034, and the experiment will consist of a “mother” and two “daughter” satellites arranged in an L-shape and connected by lasers, much like LIGO and other detectors here on Earth.

However, instead of arms spaced 4 kilometers apart like LIGO’s, eLISA’s laser arms will be separated by 1 million kilometers. If each eLISA satellite can remain perfectly still, it will enable scientists to detect gravitational waves at much lower frequencies, such as those created by binary supermassive black holes, ultra-compact binaries and small black holes falling into supermassive black holes. LISA Pathfinder will prove whether this is possible.

Gravitational waves require us to observe something nearly beyond perception — the waves that LIGO recorded squeezed its 4-kilometer-long arms by about 1/10,000th the diameter of a proton. One of the biggest problems LIGO had to overcome was the presence of unwanted vibrations caused by everything from tiny earthquakes to traffic noise, all of which could throw off the measurements. By taking the gravitational wave hunt into space, researchers hope to stay far away from any possible perturbations.

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An illustration of the LISA experiment. The two gold cubes are each monitored by a laser interferometer which precisely tracks their position. (Credit: ESA/ATG medialab)

Tracking Every Variable

The LISA spacecraft was launched on Dec. 2, 2015, and officially began operations on March 1 with a weeklong commissioning period, followed by the commencement of scientific experiments on Monday. Over the next six months, scientists will perform a variety of experiments on the masses and the spacecraft itself to test LISA Pathfinder’s measuring equipment and account for all possible sources that could disturb the cubes. 

One experiment will raise the temperature inside the high vacuum environment of their housing, heating the few gas molecules that are left inside, to measure if this has any effect on the cubes. The team will also apply increasingly stronger magnetic and electric forces to assess the amount of force that is needed to divert them from free fall. The researchers say that their equipment should provide measurements accurate up to .01 nanometers, or a millionth of a millionth of a meter.

The data gathered will help construct a model that will eliminate all other sources of motion except for gravity.

The era of gravitational wave astronomy is officially underway, and things are only going to get more interesting.

CATEGORIZED UNDER: Space & Physics, top posts
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  • http://www.mazepath.com/uncleal/qz4.htm Uncle Al

    two small gold-platinum cubes
    “In LISA Pathfinder, the test masses consist of a 1.96 kg cube of gold:platinum mono-phasic alloy of dimension 46 mm on a side. The alloy is formed from 73% gold and 27% platinum, chosen as this material can have an extremely low magnetic susceptibility χm ~10^(-5) and high density ~20 g/cm^(-3). The combination of both greatly reduces the effect of external forces on the test mass.”

    (3.92 kg)(32.1507 troy oz/kg)(0.73)(1263.25 USD/oz Au) = $116,222
    (3.92 kg)(32.1507 troy oz/kg)(0.27)(984.086 USD/oz Pt) = $33,486.8
    $(USD) 149,709 of metal in two test masses, 08 March 2016. Small?

    If each eLISA satellite can remain perfectly still” is both incorrect (they are in orbit vs. the fixed stars) and irrelevant. The test centers of mass must be in mutual unperturbed vacuum free fall unless a gravitational wave propagates past. Solar wind and coronal mass ejections will differentially affect the refractive index of the intervening “vacuum” re laser ranging. Are three satellites sufficient to trilaterate the source?

  • Erik Bosma

    I’m not anywhere close to being a Luddite but I just wonder if all this is worth it That’s a lot of money to prove a theory which has already been proven over and over again. And I’m curious at the accuracy they profess. A tiny fraction of the width of a proton. Same with all these Mars missions. It’s pretty obvious that planet is dead and we can’t live on it.

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