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• Recently, the Space Variable Objects Monitor (SVOM) satellite jointly developed by China and France was launched into orbit from the Xichang Satellite Launch Center in Sichuan province.

About Space Variable Objects Monitor (SVOM) Satellite

• It is the first astronomy satellite jointly developed by China and France.
• In 2018, the two countries had together developed and launched an oceanographic satellite.

  

• It is the most powerful satellite yet for studying gamma-ray bursts (GRBs) — they result from some of the universe’s most explosive events such as the birth of black holes and neutron star collisions.
• Once found, the satellite will measure and study their electromagnetic radiation properties.
• It will also use the bursts to unlock mysteries regarding the evolution of the universe, and gravitational waves (scientists have observed that both gravitational waves and GRBs originate from the collision of neutron stars).
• The SVOM satellite is capable of searching for kilonovas as well.
• The 930-kg satellite consists of four payloads — two developed by the French and two by the Chinese.
  • The French have built the ECLAIRs and MXT telescopes, which will detect and capture the GRBs.
  • The Gamma Ray Burst Monitor (GRB), built by the Chinese, will measure the spectrum of GRBs.
  • The Visible Telescope (VT), also developed by the Chinese, will detect and observe visible emissions produced immediately after a GRB.

What are gamma-ray bursts ?

• GRBs are bursts of highly energetic gamma rays, which last from less than a second to several minutes.
• They are known to occur in distant realms of the universe, and “can erupt with a quintillion (a 10 followed by 18 zeros) times the luminosity of the Sun”.
• There are two types of GRBs, short GRBs and long GRBs. Short GRBs are a result of the collision of either two neutron stars or a neutron star and a black hole, resulting in a black hole.
• They last for less than two seconds. Sometimes, short GRBs are followed by kilonovas — blasts of electromagnetic radiation (or light) that are produced by the radioactive decay of chemical elements.
• The decay can lead to the generation of heavier elements like gold, silver, and platinum.
• Long GRBs are produced due to the explosive deaths of massive stars.
• These can last for two seconds or longer.
• Scientists observe GRBs as they carry information pertaining to violent events such as the end of life of massive stars, the formation of black holes in distant galaxies, and how they shape the universe.

Source: IE

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