What is the LIGO-India project for which the Centre has approved Rs 2,600 crore? Where will it come up and when will it start operating? Why is it important? Here are all your questions answered
Last month, the Union Cabinet cleared Rs 2,600 crore for the Laser Interferometer Gravitational-Wave Observatory (LIGO) project that will come up in Hingoli, Maharashtra, some 590 km east of Mumbai. The project, which the Centre had approved in principle seven years ago, will be jointly funded by the departments of science and technology and atomic energy besides infrastructural support from the US.
The observatory will work in tandem with four similar facilities around the world — two in the US, one in Italy, and one in Japan — and is expected to start functioning by 2030. So, what is the LIGO-India project and why is it important? Here is all you need to know about this mega project.
What is LIGO?
Laser Interferometer Gravitational-Wave Observatory or LIGO is a global network of laboratories that can detect gravitational waves, which are tiny ripples in the fabric of space and time. LIGOs have detectors designed to look for these tiny cosmic ripples. For instance, the LIGO detectors can pick up a change of distance that is several times smaller than a proton.
So far, there are four such facilities in the world. There are two LIGOs in Washington State and Louisiana in the US. The one in Italy is called Virgo. The fourth one, named Kamioka Gravitational-Wave Detector (KAGRA), is in Japan.
What causes gravitational waves?
Gravitational waves are caused by some of the most violent events in the universe involving massive objects in motion, such as merging neutron stars or black holes, or exploding stars. Albert Einstein has first predicted the existence of gravitational waves soon after formulating the theory of General Relativity in 1915. Gravitational waves can help expand our understanding of the universe.
When LIGO made history
LIGO detected gravitational waves for the first time in 2015. Two black holes, 29 and 36 times the mass of the sun, merged 1.3 billion years ago to produce those waves. The scientists involved in the project — Rainer Weiss, Barry C Barish, and Kip S Thorne — won the Nobel Prize in Physics in 2017.
The detection confirmed Einstein’s theory that space and time are not distinct entities but are woven together in a fabric-like structure that curves, stretches, and even warps, because of gravity waves created by massive objects moving at high speeds. Since then, LIGO and its partner observatory Advanced Virgo (the facility in Italy) have detected more than 50 such signals.
Why have several gravitational wave detectors?
When a LIGO detector picks up a signal, scientists need to confirm that the source is indeed an event in space and not something on Earth, like an earthquake, traffic, or similar. One of the ways to rule out any errors is by looking for similar signals from all the detectors spread worldwide. With all the detectors working in tandem, scientists can nail down the sources of gravitational waves. India will add the fifth observatory to this elite network.
About LIGO-India
LIGO-India was first approved in 2016. Four Indian institutes — including the DCSEM, the Raja Ramanna Centre for Advanced Technology, and the Institute for Plasma Research of the Atomic Energy Department, and the Inter-University Centre for Astronomy and Astrophysics — are part of the project, along with the California Institute of Technology (Caltech) and the Massachusetts Institute of Technology (MIT), which together operate the US-based LIGO detectors. The US National Science Foundation is also part of the project.
After the consideration of several locations, Hingoli was chosen as the project site. Around 174 acres have been earmarked for the facility. The US will reportedly provide infrastructure worth about $60 million, including hardware, technical data, and training.
How the observatory works
The LIGO detectors comprise two 4-km-long L-shaped interferometers, which are essentially vacuum chambers about 4 ft in diameter with mirrors at the end. Light rays are released simultaneously in both chambers. The rays split into two beams traveling back and forth down the arms. The light should return at the same time in both chambers. However, if a gravitational wave passes through, there is a change in the length — smaller than one-ten-thousandth the diameter of a proton — which the LIGO detectors can pick up.