Loading…

Electrostatic precipitation of dust in the Martian atmosphere: Implications for the utilization of resources during future manned exploration missions

Future human missions to Mars will require the utilization of local resources for oxygen, fuel, and water. The In Situ Resource Utilization (ISRU) project is an active research endeavor at NASA to develop technologies that can enable cost effective ways to live off the land. The extraction of oxygen...

Full description

Saved in:
Bibliographic Details
Published in:Journal of physics. Conference series 2011-12, Vol.327 (1), p.12048-14
Main Authors: Calle, C I, Thompson, S M, Cox, N D, Johansen, M R, Williams, B S, Hogue, M D, Clements, J S
Format: Article
Language:English
Subjects:
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by cdi_FETCH-LOGICAL-c430t-9e04905c4d1179ad05fa993d4fa3a4b205178de80016438bc48cdd4007a4dc3d3
cites cdi_FETCH-LOGICAL-c430t-9e04905c4d1179ad05fa993d4fa3a4b205178de80016438bc48cdd4007a4dc3d3
container_end_page 14
container_issue 1
container_start_page 12048
container_title Journal of physics. Conference series
container_volume 327
creator Calle, C I
Thompson, S M
Cox, N D
Johansen, M R
Williams, B S
Hogue, M D
Clements, J S
description Future human missions to Mars will require the utilization of local resources for oxygen, fuel, and water. The In Situ Resource Utilization (ISRU) project is an active research endeavor at NASA to develop technologies that can enable cost effective ways to live off the land. The extraction of oxygen from the Martian atmosphere, composed primarily of carbon dioxide, is one of the most important goals of the Mars ISRU project. The main obstacle is the relatively large amount of dust present in the Martian atmosphere. This dust must be efficiently removed from atmospheric gas intakes for ISRU processing chambers. A common technique to achieve this removal on earth is by electrostatic precipitation, where large electrostatic fields are established in a localized region to charge, precipitate and collect dust particles. This technique is difficult to adapt to the Martian environment, with an atmospheric pressure of about one-hundredth of the terrestrial atmosphere. At these low pressures, the corona discharges required to implant an electrostatic charge to the particles to be collected is extremely difficult to sustain and the corona easily transitions to a glow/streamer discharge, which is unsuitable for particle charging. In this paper, we report on our successful efforts to establish a stable corona under Martian simulated conditions. We also present results on dust collecting efficiencies with an electrostatic precipitator prototype that could be effectively used on a future mission to the red planet.
doi_str_mv 10.1088/1742-6596/327/1/012048
format article
fullrecord <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_1753538086</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1753538086</sourcerecordid><originalsourceid>FETCH-LOGICAL-c430t-9e04905c4d1179ad05fa993d4fa3a4b205178de80016438bc48cdd4007a4dc3d3</originalsourceid><addsrcrecordid>eNpdkc9KxDAQh4souK6-ggS8eFl30qRt6k3Ef7DiRc8hJlPN0jY1SUF9EJ_X1JVFzCUZ8vFjZr4sO6ZwRkGIJa14viiLulyyvFrSJdAcuNjJZtuP3T_v_ewghDUAS6eaZV9XLeroXYgqWk0Gj9oOdipcT1xDzBgisT2Jr0julY9W9UTFzoXhFT2ek7tuaK3-wQNpnP8Bx2hb-7nN8Bjc6DWGlOZt_0KaMY4eSaf6Hg3B96F1fkN3NoQp6jDba1Qb8Oj3nmdP11ePl7eL1cPN3eXFaqE5g7ioEXgNheaG0qpWBopG1TUzvFFM8eccCloJgwKAlpyJZ82FNoYDVIobzQybZ6eb3MG7txFDlKkDjW2renRjkLQqWMEEiDKhJ__QdZqqT93JvKhqXnIoaaLKDaXTToPHRg7edsp_SApy0iUnE3IyIZMuSeVGF_sGbPaL8A</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2579464061</pqid></control><display><type>article</type><title>Electrostatic precipitation of dust in the Martian atmosphere: Implications for the utilization of resources during future manned exploration missions</title><source>Full-Text Journals in Chemistry (Open access)</source><source>Publicly Available Content (ProQuest)</source><creator>Calle, C I ; Thompson, S M ; Cox, N D ; Johansen, M R ; Williams, B S ; Hogue, M D ; Clements, J S</creator><creatorcontrib>Calle, C I ; Thompson, S M ; Cox, N D ; Johansen, M R ; Williams, B S ; Hogue, M D ; Clements, J S</creatorcontrib><description>Future human missions to Mars will require the utilization of local resources for oxygen, fuel, and water. The In Situ Resource Utilization (ISRU) project is an active research endeavor at NASA to develop technologies that can enable cost effective ways to live off the land. The extraction of oxygen from the Martian atmosphere, composed primarily of carbon dioxide, is one of the most important goals of the Mars ISRU project. The main obstacle is the relatively large amount of dust present in the Martian atmosphere. This dust must be efficiently removed from atmospheric gas intakes for ISRU processing chambers. A common technique to achieve this removal on earth is by electrostatic precipitation, where large electrostatic fields are established in a localized region to charge, precipitate and collect dust particles. This technique is difficult to adapt to the Martian environment, with an atmospheric pressure of about one-hundredth of the terrestrial atmosphere. At these low pressures, the corona discharges required to implant an electrostatic charge to the particles to be collected is extremely difficult to sustain and the corona easily transitions to a glow/streamer discharge, which is unsuitable for particle charging. In this paper, we report on our successful efforts to establish a stable corona under Martian simulated conditions. We also present results on dust collecting efficiencies with an electrostatic precipitator prototype that could be effectively used on a future mission to the red planet.</description><identifier>ISSN: 1742-6596</identifier><identifier>ISSN: 1742-6588</identifier><identifier>EISSN: 1742-6596</identifier><identifier>DOI: 10.1088/1742-6596/327/1/012048</identifier><language>eng</language><publisher>Bristol: IOP Publishing</publisher><subject>Atmosphere ; Barometric pressure ; Carbon dioxide ; Coronas ; Discharge ; Dust ; Dust control ; Electric fields ; Electrostatic charge ; Electrostatic precipitation ; Electrostatic precipitator dust ; Electrostatic precipitators ; In situ resources utilization ; Manned Mars missions ; Mars ; Mars atmosphere ; Mars dust ; Mars environment ; Particle charging ; Physics ; Precipitators ; Streamer gas discharge ; Utilization</subject><ispartof>Journal of physics. Conference series, 2011-12, Vol.327 (1), p.12048-14</ispartof><rights>Copyright IOP Publishing Dec 2011</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c430t-9e04905c4d1179ad05fa993d4fa3a4b205178de80016438bc48cdd4007a4dc3d3</citedby><cites>FETCH-LOGICAL-c430t-9e04905c4d1179ad05fa993d4fa3a4b205178de80016438bc48cdd4007a4dc3d3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://www.proquest.com/docview/2579464061?pq-origsite=primo$$EHTML$$P50$$Gproquest$$Hfree_for_read</linktohtml><link.rule.ids>314,780,784,25753,27924,27925,37012,37013,44590</link.rule.ids></links><search><creatorcontrib>Calle, C I</creatorcontrib><creatorcontrib>Thompson, S M</creatorcontrib><creatorcontrib>Cox, N D</creatorcontrib><creatorcontrib>Johansen, M R</creatorcontrib><creatorcontrib>Williams, B S</creatorcontrib><creatorcontrib>Hogue, M D</creatorcontrib><creatorcontrib>Clements, J S</creatorcontrib><title>Electrostatic precipitation of dust in the Martian atmosphere: Implications for the utilization of resources during future manned exploration missions</title><title>Journal of physics. Conference series</title><description>Future human missions to Mars will require the utilization of local resources for oxygen, fuel, and water. The In Situ Resource Utilization (ISRU) project is an active research endeavor at NASA to develop technologies that can enable cost effective ways to live off the land. The extraction of oxygen from the Martian atmosphere, composed primarily of carbon dioxide, is one of the most important goals of the Mars ISRU project. The main obstacle is the relatively large amount of dust present in the Martian atmosphere. This dust must be efficiently removed from atmospheric gas intakes for ISRU processing chambers. A common technique to achieve this removal on earth is by electrostatic precipitation, where large electrostatic fields are established in a localized region to charge, precipitate and collect dust particles. This technique is difficult to adapt to the Martian environment, with an atmospheric pressure of about one-hundredth of the terrestrial atmosphere. At these low pressures, the corona discharges required to implant an electrostatic charge to the particles to be collected is extremely difficult to sustain and the corona easily transitions to a glow/streamer discharge, which is unsuitable for particle charging. In this paper, we report on our successful efforts to establish a stable corona under Martian simulated conditions. We also present results on dust collecting efficiencies with an electrostatic precipitator prototype that could be effectively used on a future mission to the red planet.</description><subject>Atmosphere</subject><subject>Barometric pressure</subject><subject>Carbon dioxide</subject><subject>Coronas</subject><subject>Discharge</subject><subject>Dust</subject><subject>Dust control</subject><subject>Electric fields</subject><subject>Electrostatic charge</subject><subject>Electrostatic precipitation</subject><subject>Electrostatic precipitator dust</subject><subject>Electrostatic precipitators</subject><subject>In situ resources utilization</subject><subject>Manned Mars missions</subject><subject>Mars</subject><subject>Mars atmosphere</subject><subject>Mars dust</subject><subject>Mars environment</subject><subject>Particle charging</subject><subject>Physics</subject><subject>Precipitators</subject><subject>Streamer gas discharge</subject><subject>Utilization</subject><issn>1742-6596</issn><issn>1742-6588</issn><issn>1742-6596</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2011</creationdate><recordtype>article</recordtype><sourceid>PIMPY</sourceid><recordid>eNpdkc9KxDAQh4souK6-ggS8eFl30qRt6k3Ef7DiRc8hJlPN0jY1SUF9EJ_X1JVFzCUZ8vFjZr4sO6ZwRkGIJa14viiLulyyvFrSJdAcuNjJZtuP3T_v_ewghDUAS6eaZV9XLeroXYgqWk0Gj9oOdipcT1xDzBgisT2Jr0julY9W9UTFzoXhFT2ek7tuaK3-wQNpnP8Bx2hb-7nN8Bjc6DWGlOZt_0KaMY4eSaf6Hg3B96F1fkN3NoQp6jDba1Qb8Oj3nmdP11ePl7eL1cPN3eXFaqE5g7ioEXgNheaG0qpWBopG1TUzvFFM8eccCloJgwKAlpyJZ82FNoYDVIobzQybZ6eb3MG7txFDlKkDjW2renRjkLQqWMEEiDKhJ__QdZqqT93JvKhqXnIoaaLKDaXTToPHRg7edsp_SApy0iUnE3IyIZMuSeVGF_sGbPaL8A</recordid><startdate>20111206</startdate><enddate>20111206</enddate><creator>Calle, C I</creator><creator>Thompson, S M</creator><creator>Cox, N D</creator><creator>Johansen, M R</creator><creator>Williams, B S</creator><creator>Hogue, M D</creator><creator>Clements, J S</creator><general>IOP Publishing</general><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>H8D</scope><scope>HCIFZ</scope><scope>L7M</scope><scope>P5Z</scope><scope>P62</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>7U5</scope><scope>8BQ</scope><scope>JG9</scope></search><sort><creationdate>20111206</creationdate><title>Electrostatic precipitation of dust in the Martian atmosphere: Implications for the utilization of resources during future manned exploration missions</title><author>Calle, C I ; Thompson, S M ; Cox, N D ; Johansen, M R ; Williams, B S ; Hogue, M D ; Clements, J S</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c430t-9e04905c4d1179ad05fa993d4fa3a4b205178de80016438bc48cdd4007a4dc3d3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2011</creationdate><topic>Atmosphere</topic><topic>Barometric pressure</topic><topic>Carbon dioxide</topic><topic>Coronas</topic><topic>Discharge</topic><topic>Dust</topic><topic>Dust control</topic><topic>Electric fields</topic><topic>Electrostatic charge</topic><topic>Electrostatic precipitation</topic><topic>Electrostatic precipitator dust</topic><topic>Electrostatic precipitators</topic><topic>In situ resources utilization</topic><topic>Manned Mars missions</topic><topic>Mars</topic><topic>Mars atmosphere</topic><topic>Mars dust</topic><topic>Mars environment</topic><topic>Particle charging</topic><topic>Physics</topic><topic>Precipitators</topic><topic>Streamer gas discharge</topic><topic>Utilization</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Calle, C I</creatorcontrib><creatorcontrib>Thompson, S M</creatorcontrib><creatorcontrib>Cox, N D</creatorcontrib><creatorcontrib>Johansen, M R</creatorcontrib><creatorcontrib>Williams, B S</creatorcontrib><creatorcontrib>Hogue, M D</creatorcontrib><creatorcontrib>Clements, J S</creatorcontrib><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</collection><collection>Advanced Technologies &amp; Aerospace Collection</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central</collection><collection>Aerospace Database</collection><collection>SciTech Premium Collection (Proquest) (PQ_SDU_P3)</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>ProQuest Advanced Technologies &amp; Aerospace Database</collection><collection>ProQuest Advanced Technologies &amp; Aerospace Collection</collection><collection>Publicly Available Content (ProQuest)</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>METADEX</collection><collection>Materials Research Database</collection><jtitle>Journal of physics. Conference series</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Calle, C I</au><au>Thompson, S M</au><au>Cox, N D</au><au>Johansen, M R</au><au>Williams, B S</au><au>Hogue, M D</au><au>Clements, J S</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Electrostatic precipitation of dust in the Martian atmosphere: Implications for the utilization of resources during future manned exploration missions</atitle><jtitle>Journal of physics. Conference series</jtitle><date>2011-12-06</date><risdate>2011</risdate><volume>327</volume><issue>1</issue><spage>12048</spage><epage>14</epage><pages>12048-14</pages><issn>1742-6596</issn><issn>1742-6588</issn><eissn>1742-6596</eissn><abstract>Future human missions to Mars will require the utilization of local resources for oxygen, fuel, and water. The In Situ Resource Utilization (ISRU) project is an active research endeavor at NASA to develop technologies that can enable cost effective ways to live off the land. The extraction of oxygen from the Martian atmosphere, composed primarily of carbon dioxide, is one of the most important goals of the Mars ISRU project. The main obstacle is the relatively large amount of dust present in the Martian atmosphere. This dust must be efficiently removed from atmospheric gas intakes for ISRU processing chambers. A common technique to achieve this removal on earth is by electrostatic precipitation, where large electrostatic fields are established in a localized region to charge, precipitate and collect dust particles. This technique is difficult to adapt to the Martian environment, with an atmospheric pressure of about one-hundredth of the terrestrial atmosphere. At these low pressures, the corona discharges required to implant an electrostatic charge to the particles to be collected is extremely difficult to sustain and the corona easily transitions to a glow/streamer discharge, which is unsuitable for particle charging. In this paper, we report on our successful efforts to establish a stable corona under Martian simulated conditions. We also present results on dust collecting efficiencies with an electrostatic precipitator prototype that could be effectively used on a future mission to the red planet.</abstract><cop>Bristol</cop><pub>IOP Publishing</pub><doi>10.1088/1742-6596/327/1/012048</doi><tpages>14</tpages><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier ISSN: 1742-6596
ispartof Journal of physics. Conference series, 2011-12, Vol.327 (1), p.12048-14
issn 1742-6596
1742-6588
1742-6596
language eng
recordid cdi_proquest_miscellaneous_1753538086
source Full-Text Journals in Chemistry (Open access); Publicly Available Content (ProQuest)
subjects Atmosphere
Barometric pressure
Carbon dioxide
Coronas
Discharge
Dust
Dust control
Electric fields
Electrostatic charge
Electrostatic precipitation
Electrostatic precipitator dust
Electrostatic precipitators
In situ resources utilization
Manned Mars missions
Mars
Mars atmosphere
Mars dust
Mars environment
Particle charging
Physics
Precipitators
Streamer gas discharge
Utilization
title Electrostatic precipitation of dust in the Martian atmosphere: Implications for the utilization of resources during future manned exploration missions
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-07T20%3A37%3A57IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Electrostatic%20precipitation%20of%20dust%20in%20the%20Martian%20atmosphere:%20Implications%20for%20the%20utilization%20of%20resources%20during%20future%20manned%20exploration%20missions&rft.jtitle=Journal%20of%20physics.%20Conference%20series&rft.au=Calle,%20C%20I&rft.date=2011-12-06&rft.volume=327&rft.issue=1&rft.spage=12048&rft.epage=14&rft.pages=12048-14&rft.issn=1742-6596&rft.eissn=1742-6596&rft_id=info:doi/10.1088/1742-6596/327/1/012048&rft_dat=%3Cproquest_cross%3E1753538086%3C/proquest_cross%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c430t-9e04905c4d1179ad05fa993d4fa3a4b205178de80016438bc48cdd4007a4dc3d3%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=2579464061&rft_id=info:pmid/&rfr_iscdi=true