Major Atmospheric Cherenkov Experiment (MACE) Telescope

The Major Atmospheric Cherenkov Experiment (MACE) telescope is a state-of-the-art ground-based gamma-ray telescope inaugurated in Hanle, Ladakh, on October 4.

The telescope is located at around 4.3 km above sea level. It is the highest imaging Cherenkov telescope in the world.

  • It boasts of a 21-metre-wide dish, the largest of its kind in Asia and second-largest in the world.
  • The facility was built by the Bhabha Atomic Research Centre, the Tata Institute of Fundamental Research, the Electronics Corporation of India Ltd., and the Indian Institute of Astrophysics.
  • MACE’s main goal is to study gamma rays with more than 20 billion eV of energy.
  • The telescope can examine high-energy gamma rays emitted from near black holes beyond the Milky Way and which are digesting large volumes of matter.
  • Other potential astrophysical targets include gamma-ray pulsars, blazars, and gamma-ray bursts.
  • Light comes in a wide range of wavelengths but humans can only see a small portion.
  • In the electromagnetic spectrum, gamma rays have the shortest wavelength and the highest energy, with each light-particle possessing more than 100,000 electron volts.
  • Gamma rays are produced by exotic energetic objects in the cosmos, including rapidly spinning pulsars, supernova explosions, hot whirlpools of matter around black holes, and gamma-ray bursts.
  • Because of their high energy, gamma rays are a health hazard. They can damage living cells and may even trigger deleterious mutations in DNA.
  • The earth’s atmosphere blocks gamma rays from reaching the ground. Thus, astronomers who want to study objects that emit gamma rays prefer using space observatories.
  • When a gamma ray from a cosmic source enters the atmosphere, it interacts with molecules in the air to produce a copious shower of electron-positron pairs.
  • As these charged particles travel through the atmosphere at speeds greater than the speed of light in air, they emit a faint blue light, called Cherenkov radiation.
  • This radiation has wavelengths typical of violet and blue light of the visible spectrum and of the ultraviolet wavelength range.

(Source: The Hindu)

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