Miranda Moon Facts

 Miranda Moon Facts 


Miranda is the littlest of the adjusted satellites of Uranus. It additionally circles the nearest of the five bigger moons. It is named after one of the characters in Shakespeares play, "The Storm". It was additionally highlighted in Arthur C. Clark's book "2001: A Space Odyssey".

Miranda Diagrams

Realities about Miranda

  •     Miranda was found in 1948 by cosmologist Gerard Kuiper. The Kuiper Belt of the external nearby planet group is named for him.
  •     Miranda is made generally of ice with a rough material nearer to its middle.
  •     No two surface regions on Miranda are indistinguishable. Its geography goes from precipices to holes, and structural highlights.
  •     Verona Rupes is the biggest precipice in the planetary group. It ascends approximately 20 kilometers over the encompassing scene. It might have shaped when the surface blamed and broke, making a piece of it drop.
  •     Miranda's surface has a few structural locales that seem as though raceways called coronae. One of them has a "mark" molded highlight in the middle.
  •     Miranda is quite possibly of the littlest body in the planetary group to be self-adjusted under its own gravity.
  •     Miranda has encountered land movement that was reasonable brought about by flowing warming when this little moon was in orbital reverberation with its neighbor Umbriel.
  •     The Explorer 2 shuttle is the main mission to fly close to the point of imaging Miranda. There could be no different missions to Miranda arranged right now.

 

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