Physics and chemistry on the surface of cosmic dust grains: a laboratory view
Dust grains play a central role in the physics and chemistry of cosmic environments. They influence the optical and thermal properties of the medium due to their interaction with stellar radiation; provide surfaces for the chemical reactions that are responsible for the synthesis of a significant fr...
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| Published in | International reviews in physical chemistry Vol. 40; no. 2; pp. 299 - 364 |
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| Main Authors | , |
| Format | Journal Article |
| Language | English |
| Published |
Abingdon
Taylor & Francis
03.04.2021
Taylor & Francis Ltd |
| Subjects | |
| Online Access | Get full text |
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| Abstract | Dust grains play a central role in the physics and chemistry of cosmic environments. They influence the optical and thermal properties of the medium due to their interaction with stellar radiation; provide surfaces for the chemical reactions that are responsible for the synthesis of a significant fraction of key astronomical molecules; and they are building blocks of pebbles, comets, asteroids, planetesimals, and planets. In this paper, we review experimental studies of physical and chemical processes, such as adsorption, desorption, diffusion and reactions forming molecules, on the surface of reliable cosmic dust grain analogues as related to processes in diffuse, translucent, and dense interstellar clouds, protostellar envelopes, planet-forming disks, and planetary atmospheres. The information that such experiments reveal should be flexible enough to be used in many different environments. In addition, we provide a forward look discussing new ideas, experimental approaches, and research directions. |
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| AbstractList | Dust grains play a central role in the physics and chemistry of cosmic environments. They influence the optical and thermal properties of the medium due to their interaction with stellar radiation; provide surfaces for the chemical reactions that are responsible for the synthesis of a significant fraction of key astronomical molecules; and they are building blocks of pebbles, comets, asteroids, planetesimals, and planets. In this paper, we review experimental studies of physical and chemical processes, such as adsorption, desorption, diffusion and reactions forming molecules, on the surface of reliable cosmic dust grain analogues as related to processes in diffuse, translucent, and dense interstellar clouds, protostellar envelopes, planet-forming disks, and planetary atmospheres. The information that such experiments reveal should be flexible enough to be used in many different environments. In addition, we provide a forward look discussing new ideas, experimental approaches, and research directions. |
| Author | McCoustra, Martin Potapov, Alexey |
| Author_xml | – sequence: 1 givenname: Alexey surname: Potapov fullname: Potapov, Alexey email: alexey.potapov@uni-jena.de – sequence: 2 givenname: Martin surname: McCoustra fullname: McCoustra, Martin organization: Heriot-Watt University |
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| Snippet | Dust grains play a central role in the physics and chemistry of cosmic environments. They influence the optical and thermal properties of the medium due to... |
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| SubjectTerms | Accretion disks Celestial bodies Chemical reactions Comets Cosmic dust Interstellar matter Optical properties Planet formation Planetary atmospheres Protostars Star formation Stellar radiation Thermodynamic properties |
| Title | Physics and chemistry on the surface of cosmic dust grains: a laboratory view |
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