Scientists turn to the moon to catch spacetime’s faintest music | Current Affairs | Vision IAS

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Scientists turn to the moon to catch spacetime’s faintest music

2 min read

Gravitational Waves and their Detection

Gravitational waves, predicted by Albert Einstein in 1916, are oscillations in spacetime caused by massive cosmic events like merging black holes. These waves travel at the speed of light, subtly stretching and compressing spacetime. Initially, these waves were considered mathematical constructs but were first detected in 2015 by the Laser Interferometer Gravitational-wave Observatory (LIGO) in the US.

Detection Mechanisms

  • LIGO uses interferometers with laser beams to detect these waves by measuring changes in light reflection caused by gravitational influences.
  • Gravitational waves can alter distances as minute as less than an atom’s diameter.
  • The observatories can detect waves from events up to 7 billion light-years away.

Advancements in Gravitational Wave Detection

Moon-Based Detection: LILA

  • The Laser Interferometer Lunar Antenna (LILA) is an upcoming project to detect sub-hertz frequency gravitational waves on the moon.
  • The moon offers ideal conditions with low seismic noise and a natural vacuum, necessitating less infrastructure.
  • LILA's phases include the initial LILA Pioneer, leveraging American and Indian lunar missions, followed by LILA Horizon, requiring astronaut involvement.

Other Proposed Projects

  • Space-based projects like the Laser Interferometer Space Antenna (LISA) aim to detect low-frequency gravitational waves using satellites.
  • Future projects include DECIGO and TianGo, focused on decihertz frequency detection.
  • India is preparing for LIGO-India, expected to enhance gravitational-wave astronomy in the country.

Exploring the Gravitational-Wave Spectrum

Current ground-based observatories and projects like SKA focus on specific frequency ranges, but the decihertz range remains largely unexplored. This range could reveal insights into intermediate-mass black holes and the early universe. By monitoring pulsars and their frequency changes, astronomers can potentially use the Milky Way as a gravitational-wave detector.

In essence, gravitational-wave astronomy is expanding rapidly and promises to unveil the mysteries of the cosmos, allowing us to observe the universe from its very formation.

  • Tags :
  • Gravitational Wave Detection
  • Laser Interferometer Lunar Antenna (LILA)
  • Laser Interferometer Gravitational-wave Observatory (LIGO)
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