Carbon in the Universe

Author:

Henning Th.1,Salama F.1

Affiliation:

1. Th. Henning is at the Astrophysikalisches Institut und Universitäts-Sternwarte, Schillergäβchen 2-3, D-07745 Jena, Germany. F. Salama is at NASA Ames Research Center Space Science Division, Moffet Field, CA 94035–1000, USA.

Abstract

Carbon is a major player in the evolutionary scheme of the universe because of its abundance and its ability to form complex species. It is also a key element in the evolution of prebiotic molecules. The different forms of cosmic carbon are reviewed ranging from carbon atoms and carbon-bearing molecules to complex, solid-state, carbonaceous structures. The current state of knowledge is assessed on the observational and laboratory fronts. Fundamental astrophysical implications are examined as well as the impact of these studies on the hitherto poorly understood physical and chemical properties of carbon materials in space.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference113 articles.

1. As reported by the Astrochemistry Working Group of Division VI (Interstellar Matter) of the International Astronomical Union (www.strw.leidenuniv.nl/ iau34/links.html).

2. CI is used to denote neutral atomic C (C) CII to denote singly ionized C (C + ) CIII to denote doubly ionized C (C 2+ ) and so forth.

3. The solar mass M ⊙ is equal to 1.989 10 30 kg.

4. Synthesis of the Elements in Stars

5. 4 He(α ) 8 Be(α ) 12 C * ( γ γ) 12 C.

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