Major Atmospheric Cherenkov Experiment (MACE) Observatory

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Major Atmospheric Cherenkov Experiment (MACE) Observatory
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Major Atmospheric Cherenkov Experiment (MACE) Observatory

Context:MACE

Recently the Secretary of the Department of Atomic Energy (DAE) and Chairman of the Atomic Energy Commission, inaugurated the MACE Observatory in Hanle, Ladakh

 

Cherenkov experiments involve the study of Cherenkov radiation, a phenomenon that occurs when charged particles, such as electrons or protons, travel through a dielectric medium (like water) at speeds exceeding the speed of light in that medium. This results in the emission of a characteristic blue light, similar to a sonic boom produced by an object travelling faster than sound.

 

More on News:

  • This state-of-the-art facility is the largest imaging Cherenkov telescope in Asia and holds the distinction of being the highest of its kind globally, situated at an altitude of approximately 4,300 metres.
  • This inauguration was part of the DAE’s Platinum Jubilee celebrations.

 

Key Highlights:

  • Indigenous Development: Built by the Bhabha Atomic Research Centre (BARC) in collaboration with the Electronics Corporation of India Ltd (ECIL) and other Indian industry partners.
  • Research Focus: MACE is set to position India at the forefront of global cosmic ray research by enabling the study of high-energy gamma rays.
  • Construction Features: Lightweight yet strong design with high-temperature endurance.
    • Ultra-fast backend electronics optimised for low-power and cold-temperature operations, with nanosecond digitisation capabilities.
  • Observation Capabilities: MACE can capture gamma-ray flares from sources up to 200 million light-years away.
  • Hanle’s Unique Conditions: The area’s extremely low light pollution provides ideal conditions for gamma-ray observations
    • Its geographical position allows MACE to monitor cosmic sources that are not visible from other locations worldwide.

 

Gamma Ray Detection: Gamma rays do not reach the Earth’s surface due to atmospheric absorption but generate high-energy particles that emit Cherenkov radiation. MACE captures this radiation using its mirrors and cameras, tracing it back to its cosmic source.

 

Future Aspirations:

  • Scientific Impact: MACE will enhance India’s capacity to study high-energy phenomena like supernovae and black holes, complementing global observatories.
  • International Collaboration: Aims to foster partnerships and strengthen India’s position in the global scientific community.
  • Inspiration for Future Generations: Encourages exploration of new frontiers in astrophysics among students and young scientists.

 

Conclusion:

The inauguration of the MACE observatory marks a significant advancement for India in the field of astrophysics and cosmic-ray research, enhancing its capabilities to explore the mysteries of the universe.

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The Source’s Authority and Ownership of the Article is Claimed By THE STUDY IAS BY MANIKANT SINGH

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