LIGO and Virgo: The machines that unlock the universe’s mysteries2 min read . Updated: 17 Oct 2017, 07:57 PM IST
LIGO, Virgo that gave scientists first-ever glimpse of gravitational waves resulting from a collision of neutron stars are the most advanced detectors ever built for sensing tiny vibrations in the universe
Washington: The three machines that gave scientists their first-ever glimpse of gravitational waves resulting from a collision of neutron stars are the most advanced detectors ever built for sensing tiny vibrations in the universe.
The LIGO and Virgo detectors have previously picked up the “chirp" of black holes merging in the distant universe, sending out ripples in the fabric of space and time.
The detection of these gravitational waves for the first time in 2015 confirmed Albert Einstein’s century old theory of general relativity.
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.
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.
The third underground detector is near Pisa, Italy, and is known as Virgo.
Built a quarter century ago by a French-Italian partnership, the Virgo detector ended its initial round of observations in 2011 and then underwent an upgrade.
Advanced Virgo came online in April of this year, and made its first observation of gravitational waves on 14 August, marking the fourth such event that scientists have observed since 2015.
Virgo is less sensitive than LIGO, but having three detectors helps scientists zero in on the area of the universe where a cosmic event is happening, and measure the distance with greater accuracy.
“A smaller search area enables follow-up observations with telescopes and satellites for cosmic events that produce gravitational waves and emissions of light, such as the collision of neutron stars," said Georgia Tech professor Laura Cadonati.
These huge laser interferometers -- each about 2.5 miles (four kilometers) long -- are buried beneath the ground to allow the most precise measurements.
The L-shaped instruments track gravitational waves 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 and neutron stars.
“As a gravitational wave propagates through space it stretches space-time," explained 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 space 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 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.
The detectors contain two very long arms that contain optical instruments for bending light, and are positioned like the letter L.
If one arm shortens, and the other lengthens, scientists know they are seeing a gravitational wave.