Encyclopedia of Astrobiology

Living Edition
| Editors: Muriel Gargaud, William M. Irvine, Ricardo Amils, Henderson James Cleaves, Daniele Pinti, José Cernicharo Quintanilla, Michel Viso

Volatile

Living reference work entry
DOI: https://doi.org/10.1007/978-3-642-27833-4_1669-3

Definition

In planetary science, volatiles are chemical elements and compounds with low boiling points typically associated with a planet’s or Moon’s crust and/or atmosphere. Some examples include nitrogen (N or N2), water, carbon dioxide, ammonia, hydrogen (H or H2), methane, and sulfur dioxide. These compounds or elements, in the solid state, are often significant components of the crusts of moons and planets. Planetary scientists often classify volatiles with exceptionally low melting points, such as hydrogen and helium, as gases, while those volatiles with melting points above about 100 K are classified as ices. Here, the terms “gas” and “ice” can apply to compounds that may be solids, liquids, or gases. Thus, Jupiter and Saturn are referred to as “gas giants,” and Uranus and Neptune are referred to as “ice giants,” even though the majority of the “gas” and “ice” in their interiors is liquid. The Earth’s Moon has a very low volatile content. Its crust contains oxygen chemically...

Keywords

Melting Point Chemical Element Boiling Point Sulfur Dioxide Negligible Amount 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.
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Copyright information

© Springer-Verlag Berlin Heidelberg 2014

Authors and Affiliations

  1. 1.Earth-Life Science Institute (ELSI)Tokyo Institute of TechnologyMeguro-kuJapan
  2. 2.Institute for Advanced StudyPrincetonUSA
  3. 3.Blue Marble Space Institute of ScienceWashingtonUSA
  4. 4.Center for Chemical EvolutionGeorgia Institute of TechnologyAtlantaUSA