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A chamber for studying planetary environments and its applications to astrobiology
Identificadores del recurso
Measurement Science and Technology 17(8): 2274 (2006)
0957-0233
https://iopscience.iop.org/article/10.1088/0957-0233/17/8/031
http://hdl.handle.net/20.500.12666/931
10.1088/0957-0233/17/8/031
1361-6501
Procedència
(DIGITAL.INTA)

Fitxa

Títol:
A chamber for studying planetary environments and its applications to astrobiology
Descripció:
Citation E Mateo-Martí et al 2006 Meas. Sci. Technol. 17 2274
We have built a versatile environmental simulation chamber capable of reproducing atmospheric compositions and surface temperatures for most of the planetary objects. It has been especially developed to make feasible in situ irradiation and characterization of the sample under study. The total pressure in the chamber can range from 5 to 5 × 10−9 mbar. The required atmospheric composition is regulated via a residual gas analyser with ca ppm precision. Temperatures can be set from 4 K to 325 K. The sample under study can be irradiated with ion and electron sources, a deuterium ultraviolet (UV) lamp and a noble-gas discharge UV lamp. One of the main technological challenges of this device is to provide the user the possibility of performing ion and electron irradiation at a total pressure of 0.5 mbar. This is attained by means of an efficient differential pumping system. The in situ analysis techniques implemented are UV spectroscopy and infrared spectroscopy (IR). This machine is especially suitable for following the chemical changes induced in a particular sample by irradiation in a controlled environment. Therefore, it can be used in different disciplines such as planetary geology, astrobiology, environmental chemistry, materials science and for instrumentation testing.
"Work carried out at CAB was supported by the European Union, Instituto Nacional de T´ecnica Aerospacial, Ministeriode Educación y Ciencia (MEC) and Comunidad de Madrid."
Peerreview
Idioma:
English
Autor/Productor:
Mateo Martí, Eva
Prieto Ballesteros, O.
Sobrado, J. M.
Gómez Elvira, J.
Martín Gago, J. A.
Editor:
IOP Science Publishing
Otros colaboradores/productores:
Instituto Nacional de Técnica Aeroespacial (INTA)
Comunidad de Madrid
Drets:
IOP Publishing
info:eu-repo/semantics/restrictedAccess
Data:
2024-02-09T13:06:07Z
2006-07-13
Tipo de recurso:
info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
Format:
application/pdf

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            17. <mods:abstract>We have built a versatile environmental simulation chamber capable of reproducing atmospheric compositions and surface temperatures for most of the planetary objects. It has been especially developed to make feasible in situ irradiation and characterization of the sample under study. The total pressure in the chamber can range from 5 to 5 × 10−9 mbar. The required atmospheric composition is regulated via a residual gas analyser with ca ppm precision. Temperatures can be set from 4 K to 325 K. The sample under study can be irradiated with ion and electron sources, a deuterium ultraviolet (UV) lamp and a noble-gas discharge UV lamp. One of the main technological challenges of this device is to provide the user the possibility of performing ion and electron irradiation at a total pressure of 0.5 mbar. This is attained by means of an efficient differential pumping system. The in situ analysis techniques implemented are UV spectroscopy and infrared spectroscopy (IR). This machine is especially suitable for following the chemical changes induced in a particular sample by irradiation in a controlled environment. Therefore, it can be used in different disciplines such as planetary geology, astrobiology, environmental chemistry, materials science and for instrumentation testing.</mods:abstract>

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