The world's most sophisticated science machines: LIGO

February 11, 2016
LIGO co-founders Kip Thorne (R), and Rainer Weiss (L), speak about gravitational waves during a press conference at the National
LIGO co-founders Kip Thorne (R), and Rainer Weiss (L), speak about gravitational waves during a press conference at the National Press Club in Washington, DC, February 11, 2016

The machines that gave scientists their first-ever glimpse at gravitational waves are the most advanced detectors ever built for sensing tiny vibrations in the universe.

The two US-based underground detectors are known as the Laser Interferometer Gravitational-wave Observatory, or LIGO for short.

One is located in Hanford, Washington; the other 1,800 miles (3,000 kilometers) away in Livingston, Louisiana.

Construction began in 1999, and observations were taken from 2001 to 2007.

Then they underwent a major upgrade to make them 10 times more powerful.

The advanced LIGO detectors became fully operational for the first time in September 2015.

In this case of this discovery, made on September 14, 2015, the detector in Louisiana first picked up the signal of a gravitational wave, originating 1.3 billion years ago in the southern sky.

Such waves are a measure of strain in space, an effect of the motion of large masses that stretches the fabric of space-time—which is a way of viewing space and time as a single, interweaved continuum.

The detector in Washington picked up the same signal 7.1 milliseconds later, allowing scientists to confirm the finding was real and not just a glitch.

The ultra-sophisticated tools work by using huge laser interferometers—each about 2.5 miles (four kilometers) long—which are buried beneath the ground to allow the most precise measurements.

The L-shaped instruments track using the physics of laser light and space.

They do not rely on light in the skies like a telescope does.

Rather, they sense the vibrations in space, an advantage which allows them to uncover the properties of black holes.

A picture shows part of the Virgo detector for gravitational waves that is located within the European Gravitational Observatory
A picture shows part of the Virgo detector for gravitational waves that is located within the European Gravitational Observatory, on February 9, 2016 between Cascina and Pisa in Tuscany
"As a gravitational wave propagates through space it stretches space-time," said David Shoemaker, leader of the Advanced LIGO project at the Massachusetts Institute of Technology (MIT).

The detector, in short, "is just a big device for changing strain in space into an electrical signal."

One way to imagine the curvature of and time is to imagine a ball falling on a trampoline.

The trampoline bows downward first, stretching the fabric vertically and shortening the sides.

Then as the ball bounces upward again, the horizontal movement of the fabric expands again.

The instrument acts like a transducer, changing that strain into changes in light—and then into an electronic signal so scientists can digitize it and analyze it.

The LIGO detectors contain two very long arms that contain optical instruments for bending light, and are positioned like the letter L.

"The light from the laser has to travel in a vacuum so that it is not disturbed by all the air fluctuations," said Shoemaker, noting that LIGO contains the "biggest high vacuum system in the world,"—measuring 1.2 meters (yards) by 2.5 miles (four kilometers) long.

If one arm shortens, and the other lengthens, scientists know they are seeing a gravitational wave.

On September 14, "we saw just that signal, the shortening of one arm, the lengthening of the other arm, and then a millisecond later, the opposite effect," said Shoemaker.

The LIGO teams at MIT and Caltech have worked in collaboration with a French-Italian partnership to build another advanced detector, known as VIRGO, which should come online later this year in Italy.

Explore further: Announcement Thursday on Einstein's gravitational waves

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3 / 5 (2) Feb 11, 2016
If gravity waves even existed how would you determine what is due to the moon, the planets, the sun, any other body. Also the resolution is ambiguous. But I ramble, first, the speed of light, i.e. the wave front moving from A to B is not constant.

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