Dwarf Planet Ceres | 13 Aug 2020

Why in News

As per the data collected by NASA’s Dawn spacecraft, dwarf planet Ceres reportedly has salty water underground.

• Dawn (2007-18) was a mission to the two most massive bodies in the main asteroid belt - Vesta and Ceres.

Key Points

• Latest Findings:
  
  • The scientists have given Ceres the status of an “ocean world” as it has a big reservoir of salty water underneath its frigid surface.
    
    • This has led to an increased interest of scientists that the dwarf planet was maybe habitable or has the potential to be.
    • Ocean Worlds is a term for ‘Water in the Solar System and Beyond’.
  • The salty water originated in a brine reservoir spread hundreds of miles and about 40 km beneath the surface of the Ceres.
  • Further, there is an evidence that Ceres remains geologically active with cryovolcanism - volcanoes oozing icy material.
    
    • Instead of molten rock, cryovolcanoes or salty-mud volcanoes release frigid, salty water sometimes mixed with mud.
• Subsurface Oceans on other Celestial Bodies: Jupiter’s moon Europa, Saturn’s moon Enceladus, Neptune’s moon Triton, and the dwarf planet Pluto.
  
  • This provides scientists a means to understand the history of the solar system.
• Ceres:
  
  • It is the largest object in the asteroid belt between Mars and Jupiter.
    
    • It was the first member of the asteroid belt to be discovered when Giuseppe Piazzi spotted it in 1801.
  • It is the only dwarf planet located in the inner solar system (includes planets Mercury, Venus, Earth and Mars).
    
    • Scientists classified it as a dwarf planet in 2006.
  • It has a diameter of about 950 km, which is more than one-fourth of Earth’s moon.
    • It takes 1,682 Earth days, or 4.6 Earth years, to make one trip around the sun.
    • It completes one rotation around its axis every 9 hours.
  • It does not have any moon or rings.
  • It has a 92 km wide crater named Occator located in its northern hemisphere.

Source: IE