Planetary science

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Apollo15DunaTisza
Magnetosphere rendition
Jupiter

Planetary science is a branch of astronomy that involves the study of planets, moons, and planetary systems (in particular those of the Solar System) and the processes that form them. It combines elements from physics, chemistry, geology, atmospheric science, and biology to understand the fundamental properties and evolution of planets, both in our own and other star systems. Planetary scientists study a wide range of topics including the formation and history of planets, their geology and geophysics, their atmospheres and climates, the possibility of life beyond Earth, and the potential for human space exploration and colonization.

History[edit | edit source]

The field of planetary science has its roots in ancient astronomy, but it began to develop as a modern science with the advent of telescopic observation and space exploration. The 20th century saw significant advances with the launch of the first artificial satellite, Sputnik, and subsequent space missions to the Moon, Mars, Venus, and beyond. These missions provided invaluable data about other worlds in our Solar System, leading to new theories and models about planetary formation and evolution.

Sub-disciplines[edit | edit source]

Planetary science is a broad field that encompasses several sub-disciplines, including but not limited to:

  • Comparative Planetology: Comparing and contrasting the properties of various planets to understand their formation and evolution.
  • Planetary Geology: Studying the solid bodies of the Solar System, including planets, moons, and asteroids, to understand their composition, structure, and history.
  • Planetary Atmospheres: Investigating the composition, structure, dynamics, and weather patterns of planetary atmospheres.
  • Astrobiology: The study of the origin, evolution, distribution, and future of life in the universe, with a particular focus on the potential for life on other planets.
  • Planetary Astronomy: Observing planets, moons, and other celestial bodies to gather data on their orbits, size, shape, and other physical characteristics.

Key Concepts[edit | edit source]

Some of the key concepts in planetary science include:

  • Planetary Differentiation: The process by which a planet forms from a homogenous body into a stratified state, with a core, mantle, and crust.
  • Impact Cratering: The formation of craters on the surface of planets and moons due to collisions with other celestial bodies.
  • Volcanism: The eruption of molten rock (magma) from a planet's interior to its surface.
  • Tectonics: The study of the structure and motion of a planet's surface.
  • Hydrology: In the context of planetary science, the study of the distribution and movement of water (in all its forms) on, above, and below the surface of planets.

Future Directions[edit | edit source]

The future of planetary science is likely to be driven by ongoing and future space missions, including both manned and unmanned explorations. Missions like NASA's Mars 2020 rover and the European Space Agency's JUpiter ICy moons Explorer (JUICE) mission are set to explore other planets and moons in greater detail than ever before. Additionally, advancements in telescope technology and interstellar travel concepts may one day allow scientists to study planets in other star systems, or exoplanets, up close.

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Contributors: Prab R. Tumpati, MD