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Related Concept Videos

Conditions on Early Earth02:06

Conditions on Early Earth

Around 4 billion years ago, oceans began to condense on earth while volcanic eruptions released nitrogen, carbon dioxide, methane, ammonia, and hydrogen into the primordial atmosphere. However, organisms with the characteristics of life were not initially present on earth. Scientists have used experimentation to determine how organisms evolved that could grow, reproduce, and maintain an internal environment.
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Acceleration due to Gravity on Other Planets

The gravitational acceleration of an object near the Earth's surface is called the acceleration due to gravity. It can be measured by conducting simple experiments on Earth. However, such an experiment is impossible to conduct on the surface of other planets.
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Investigating Europa's Habitability with the Europa Clipper.

Steven D Vance1, Kathleen L Craft2, Everett Shock3

  • 1Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA USA.

Space Science Reviews
|December 4, 2023
PubMed
Summary

The Europa Clipper mission investigates Jupiter's moon Europa's habitability by characterizing its ice shell, ocean, composition, and geology. This comprehensive study aims to understand the conditions necessary for life on this ocean world.

Keywords:
EuropaHabitabilityIceJupiterOcean worlds

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Area of Science:

  • Planetary Science
  • Astrobiology
  • Ocean Worlds

Background:

  • Europa's habitability is a complex system driven by physical and chemical processes.
  • Characterizing habitability requires a collaborative, integrated system approach.

Purpose of the Study:

  • To explore Europa as an integrated system for a complete picture of its habitability.
  • To characterize the ice shell, ocean, composition, and geology of Europa.

Main Methods:

  • Europa Clipper mission's three primary science objectives.
  • Investigating surface-ice-ocean exchange, non-ice materials, carbon compounds, and geological features.
  • Assessing thermal anomalies, plumes, geodetic and radiation measurements, and reconnaissance for future missions.

Main Results:

  • The mission aims to characterize the heterogeneity and properties of Europa's ice shell and ocean.
  • It will analyze Europa's surface and atmospheric composition, including carbon-containing compounds.
  • Geological characterization will focus on surface features and areas of high scientific interest.

Conclusions:

  • Synthesizing mission data with remote observations will constrain Europa's habitability.
  • The Habitability Assessment Board (HAB) guides the complex task of habitability assessment.
  • The Europa Clipper mission is poised to significantly advance our understanding of potential habitability beyond Earth.