Potato radius

The potato radius is the size at which an asteroid is massive[1] enough that gravity begins to make it rounder.[2] The potato radius defines hydrostatic equilibrium and is used to separate dwarf planets from small solar system bodies.[3][4] Charles Lineweaver and Marc Norman at the Australian National University in Canberra first proposed, an objective definition of a planet, that separates potato-like objects from spherical ones.[5][6][7]

See also

References

  1. ^ Hall, Ian. "What Makes Earth A Planet, Not A Potato?". The Average Scientist .co.uk. Retrieved 1 August 2025.
  2. ^ "Potato radius". BBC Sky at Night Magazine. The Sky at Night, BBC. 9 January 2025. Retrieved 1 August 2025.
  3. ^ Caplan, M. E. (November 2015). "Calculating the Potato Radius of Asteroids using the Height of Mt. Everest". arXiv e-prints. Astrophysics Data System: arXiv:1511.04297. arXiv:1511.04297.
  4. ^
  5. ^ "Picking Planets from Potatoes". phys.org. Astrobiology Magazine. April 26, 2010. Retrieved 1 August 2025.
  6. ^ "'Potato Radius' To Define Dwarf Planets". MIT Technology Review. Emerging Technology from the arXiv. Retrieved 1 August 2025.
  7. ^ Nerlich, Steve (April 17, 2010). "Astronomy Without A Telescope โ€“ One Potato, Two Potato". Universe Today. Retrieved 1 August 2025.