Encyclopedia of Astrobiology

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

Molecules in Space

Living reference work entry
DOI: https://doi.org/10.1007/978-3-642-27833-4_1834-12

Definition

In this entry, by “molecules” we refer to all types of (generally chemically) bound species consisting of two or more atoms. They may be chemically saturated as well as unsaturated, may contain unpaired electrons (i.e., are radicals), or may be charged positively (cations) or negatively (anions). Space refers here to all regions outside the solar system. On occasion, we restrict the discussion only to the interstellar medium and circumstellar envelopes in the Milky Way, thus excluding stellar atmospheres as well as extragalactic sources. Molecules in space usually, but not exclusively, refer to those in the gas phase.

Overview

The spectra produced by molecules in space are used to characterize the physical and chemical properties of certain media in space. For example, certain atomic and molecular absorption lines in the visible region observed in stellar atmospheres are used to classify the stars. Atomic and molecular lines play an important role in star formation, as they...

Keywords

Astrochemistry Circumstellar envelope Interstellar medium Ion Molecule Radio astronomy Rotational spectroscopy 
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References and Further Reading

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Copyright information

© Springer-Verlag Berlin Heidelberg 2014

Authors and Affiliations

  1. 1.I. Physikalisches InstitutUniversität zu KölnKölnGermany