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RING FOUND BEYOND DWARF PLANET'S ROCHE LIMIT: WHY THIS MATTERS

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RING FOUND BEYOND DWARF PLANET'S ROCHE LIMIT: WHY THIS MATTERS

  • As per a new study, astronomers have found a ring around a dwarf planet, located in the Kuiper Belt at the solar system’s edge, called Quaoar.
  • The ring, however, is positioned much further away from the planet than is usual and defies theoretical explanations.
  • According to the study, the ring lies far away from the Roche limit — a mathematically determined distance beyond which rings aren’t supposed to exist.

About the dwarf planet Quaoar

  • With an estimated radius of 555 km, Quaoar is roughly half the size of Pluto and orbits beyond Neptune.
  • It also has a moon of its own, which is known as Weywot.
  • It is too small & distant to be observed directly, so the ring was detected with the help of a phenomenon called stellar occultation.

Stellar occultation

  • It occurs when, as seen from Earth, a bright star passes behind a planet.
  • It allows astronomers to observe the sharp silhouette of the planet for a brief period of time.
  • The rare phenomenon is used by researchers to analyse a planet’s atmosphere & determine if it has a ring around it.
  • In 1977, scientists discovered the Uranian ring system with the help of stellar occultation.
  • During 2018 - 2021, the dwarf planet passed in front of four stars, helping researchers observe the shadow of the eclipses.

Roche limit

  • The Earth’s gravity pulls on the moon.
  • However, one side of the moon is closer to the planet and hence, the pull is stronger on the side facing the Earth.
  • The result is the so-called tidal force, which either stretches or compresses the moon from all sides.
  • What helps the moon keep it together is its own gravity. It counteracts the effect of the tidal force.
  • But if you bring the moon closer to the Earth, the tidal force will overcome the satellite’s gravity and then disintegrate it, turning the moon into a ring.
  • The minimum distance at which this happens is known as the Roche limit.
  • It is named after the French astronomer Édouard Roche, who discovered the limit in 1848.
  • It is applicable to any planet and the celestial bodies around it.
  • Eg, Saturn. The rings that you see around the planet are within the Roche limit and therefore, there are no moons in that area.

Prelims Takeaway

  • Dwarf planet
  • Stellar occultation
  • Roche limit
  • Exoplanets

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