How Comets Work
Two major questions regarding comets have been up to now far from any solution. (i) How is it possible that water-ice sublimation from the nucleus surface does not lead to an insulating crust, stopping every gas and dust ejection within a few days? (ii) How is it possible that the gas flow crossing...
Gespeichert in:
Veröffentlicht in: | Astrophysical journal. Letters 2019-07, Vol.879 (1), p.L8 |
---|---|
Hauptverfasser: | , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext bestellen |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | |
---|---|
container_issue | 1 |
container_start_page | L8 |
container_title | Astrophysical journal. Letters |
container_volume | 879 |
creator | Fulle, M. Blum, J. Rotundi, A. |
description | Two major questions regarding comets have been up to now far from any solution. (i) How is it possible that water-ice sublimation from the nucleus surface does not lead to an insulating crust, stopping every gas and dust ejection within a few days? (ii) How is it possible that the gas flow crossing the refractory surface crust ejects dust particles bonded by tensile strengths larger than tens of Pa when the perihelion gas pressure at the nucleus-coma interface is less than one Pa? We have developed a simple but rigorous analytical model, assuming that the cometary nucleus consists of agglomerates of ice and dust ("clusters"). As soon as the clusters become exposed to sunlight, gas diffusion from their inside leads to their dehydration. We find that (i) the gas diffusing from the interior to the surface of a sunlit cluster has a steep density gradient at the cluster surface, which blasts the cluster into particles of sizes larger than or equal to those actually observed by Rosetta dust instruments; (ii) the heat-conduction and diffusion timescales are much shorter than the dehydration timescale, ensuring that the described process prevents any dumping of the nucleus activity driven by water-ice sublimation from 4 au inbound to 4 au outbound; and (iii) the clusters are in fact cm-sized pebbles, so that a cometary nucleus made of pebbles is confirmed to be the only one consistent with cometary gas and dust activity, a process unexplained until now. |
doi_str_mv | 10.3847/2041-8213/ab2898 |
format | Article |
fullrecord | <record><control><sourceid>proquest_O3W</sourceid><recordid>TN_cdi_iop_journals_10_3847_2041_8213_ab2898</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2365649235</sourcerecordid><originalsourceid>FETCH-LOGICAL-c380t-b4be81719c4532a0e92e9bf7b047b251e2debfdd861aa8463823843f95f27f83</originalsourceid><addsrcrecordid>eNp1j01LxDAQhoMouK7i1eOCeLNuvtpMjlLUFQpeFjwOSZvA1l1Tky7iv7elsl70NMPwzDvzEHLF6J0AqZacSpYBZ2JpLAcNR2R2GB0fepqfkrOUWko5LRjMyOUqfC7KsHN9WryG-HZOTrzZJnfxU-dk_fiwLldZ9fL0XN5XWS2A9pmV1gFTTNcyF9xQp7nT1itLpbI8Z443zvqmgYIZA7IQwIcvhde558qDmJPrKbaL4WPvUo9t2Mf34SJyUeSF1FzkA0Unqo4hpeg8dnGzM_ELGcXRGkctHBVxsh5WbqaVTeh-M03XbhGURoYVYNf4gbv9g_s39hsM5WHU</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2365649235</pqid></control><display><type>article</type><title>How Comets Work</title><source>IOP Publishing Free Content</source><creator>Fulle, M. ; Blum, J. ; Rotundi, A.</creator><creatorcontrib>Fulle, M. ; Blum, J. ; Rotundi, A.</creatorcontrib><description>Two major questions regarding comets have been up to now far from any solution. (i) How is it possible that water-ice sublimation from the nucleus surface does not lead to an insulating crust, stopping every gas and dust ejection within a few days? (ii) How is it possible that the gas flow crossing the refractory surface crust ejects dust particles bonded by tensile strengths larger than tens of Pa when the perihelion gas pressure at the nucleus-coma interface is less than one Pa? We have developed a simple but rigorous analytical model, assuming that the cometary nucleus consists of agglomerates of ice and dust ("clusters"). As soon as the clusters become exposed to sunlight, gas diffusion from their inside leads to their dehydration. We find that (i) the gas diffusing from the interior to the surface of a sunlit cluster has a steep density gradient at the cluster surface, which blasts the cluster into particles of sizes larger than or equal to those actually observed by Rosetta dust instruments; (ii) the heat-conduction and diffusion timescales are much shorter than the dehydration timescale, ensuring that the described process prevents any dumping of the nucleus activity driven by water-ice sublimation from 4 au inbound to 4 au outbound; and (iii) the clusters are in fact cm-sized pebbles, so that a cometary nucleus made of pebbles is confirmed to be the only one consistent with cometary gas and dust activity, a process unexplained until now.</description><identifier>ISSN: 2041-8205</identifier><identifier>EISSN: 2041-8213</identifier><identifier>DOI: 10.3847/2041-8213/ab2898</identifier><language>eng</language><publisher>Austin: The American Astronomical Society</publisher><subject>Agglomerates ; Bonding strength ; Clusters ; Comet nuclei ; Comets ; comets: general ; comets: individual (67P/Churyumov-Gerasimenko) ; Conduction heating ; Dehydration ; Density gradients ; Diffusion ; Dumping ; Dust ; Dust particles ; Gas flow ; Gas pressure ; Gaseous diffusion ; Ice ; Perihelions ; space vehicles: instruments ; Sublimation</subject><ispartof>Astrophysical journal. Letters, 2019-07, Vol.879 (1), p.L8</ispartof><rights>2019. The American Astronomical Society. All rights reserved.</rights><rights>Copyright IOP Publishing Jul 01, 2019</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c380t-b4be81719c4532a0e92e9bf7b047b251e2debfdd861aa8463823843f95f27f83</citedby><cites>FETCH-LOGICAL-c380t-b4be81719c4532a0e92e9bf7b047b251e2debfdd861aa8463823843f95f27f83</cites><orcidid>0000-0001-8435-5287</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://iopscience.iop.org/article/10.3847/2041-8213/ab2898/pdf$$EPDF$$P50$$Giop$$H</linktopdf><link.rule.ids>314,776,780,27901,27902,38845,38867,53815,53842</link.rule.ids><linktorsrc>$$Uhttps://iopscience.iop.org/article/10.3847/2041-8213/ab2898$$EView_record_in_IOP_Publishing$$FView_record_in_$$GIOP_Publishing</linktorsrc></links><search><creatorcontrib>Fulle, M.</creatorcontrib><creatorcontrib>Blum, J.</creatorcontrib><creatorcontrib>Rotundi, A.</creatorcontrib><title>How Comets Work</title><title>Astrophysical journal. Letters</title><addtitle>APJL</addtitle><addtitle>Astrophys. J. Lett</addtitle><description>Two major questions regarding comets have been up to now far from any solution. (i) How is it possible that water-ice sublimation from the nucleus surface does not lead to an insulating crust, stopping every gas and dust ejection within a few days? (ii) How is it possible that the gas flow crossing the refractory surface crust ejects dust particles bonded by tensile strengths larger than tens of Pa when the perihelion gas pressure at the nucleus-coma interface is less than one Pa? We have developed a simple but rigorous analytical model, assuming that the cometary nucleus consists of agglomerates of ice and dust ("clusters"). As soon as the clusters become exposed to sunlight, gas diffusion from their inside leads to their dehydration. We find that (i) the gas diffusing from the interior to the surface of a sunlit cluster has a steep density gradient at the cluster surface, which blasts the cluster into particles of sizes larger than or equal to those actually observed by Rosetta dust instruments; (ii) the heat-conduction and diffusion timescales are much shorter than the dehydration timescale, ensuring that the described process prevents any dumping of the nucleus activity driven by water-ice sublimation from 4 au inbound to 4 au outbound; and (iii) the clusters are in fact cm-sized pebbles, so that a cometary nucleus made of pebbles is confirmed to be the only one consistent with cometary gas and dust activity, a process unexplained until now.</description><subject>Agglomerates</subject><subject>Bonding strength</subject><subject>Clusters</subject><subject>Comet nuclei</subject><subject>Comets</subject><subject>comets: general</subject><subject>comets: individual (67P/Churyumov-Gerasimenko)</subject><subject>Conduction heating</subject><subject>Dehydration</subject><subject>Density gradients</subject><subject>Diffusion</subject><subject>Dumping</subject><subject>Dust</subject><subject>Dust particles</subject><subject>Gas flow</subject><subject>Gas pressure</subject><subject>Gaseous diffusion</subject><subject>Ice</subject><subject>Perihelions</subject><subject>space vehicles: instruments</subject><subject>Sublimation</subject><issn>2041-8205</issn><issn>2041-8213</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2019</creationdate><recordtype>article</recordtype><recordid>eNp1j01LxDAQhoMouK7i1eOCeLNuvtpMjlLUFQpeFjwOSZvA1l1Tky7iv7elsl70NMPwzDvzEHLF6J0AqZacSpYBZ2JpLAcNR2R2GB0fepqfkrOUWko5LRjMyOUqfC7KsHN9WryG-HZOTrzZJnfxU-dk_fiwLldZ9fL0XN5XWS2A9pmV1gFTTNcyF9xQp7nT1itLpbI8Z443zvqmgYIZA7IQwIcvhde558qDmJPrKbaL4WPvUo9t2Mf34SJyUeSF1FzkA0Unqo4hpeg8dnGzM_ELGcXRGkctHBVxsh5WbqaVTeh-M03XbhGURoYVYNf4gbv9g_s39hsM5WHU</recordid><startdate>20190701</startdate><enddate>20190701</enddate><creator>Fulle, M.</creator><creator>Blum, J.</creator><creator>Rotundi, A.</creator><general>The American Astronomical Society</general><general>IOP Publishing</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>8FD</scope><scope>H8D</scope><scope>KL.</scope><scope>L7M</scope><orcidid>https://orcid.org/0000-0001-8435-5287</orcidid></search><sort><creationdate>20190701</creationdate><title>How Comets Work</title><author>Fulle, M. ; Blum, J. ; Rotundi, A.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c380t-b4be81719c4532a0e92e9bf7b047b251e2debfdd861aa8463823843f95f27f83</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2019</creationdate><topic>Agglomerates</topic><topic>Bonding strength</topic><topic>Clusters</topic><topic>Comet nuclei</topic><topic>Comets</topic><topic>comets: general</topic><topic>comets: individual (67P/Churyumov-Gerasimenko)</topic><topic>Conduction heating</topic><topic>Dehydration</topic><topic>Density gradients</topic><topic>Diffusion</topic><topic>Dumping</topic><topic>Dust</topic><topic>Dust particles</topic><topic>Gas flow</topic><topic>Gas pressure</topic><topic>Gaseous diffusion</topic><topic>Ice</topic><topic>Perihelions</topic><topic>space vehicles: instruments</topic><topic>Sublimation</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Fulle, M.</creatorcontrib><creatorcontrib>Blum, J.</creatorcontrib><creatorcontrib>Rotundi, A.</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Astrophysical journal. Letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Fulle, M.</au><au>Blum, J.</au><au>Rotundi, A.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>How Comets Work</atitle><jtitle>Astrophysical journal. Letters</jtitle><stitle>APJL</stitle><addtitle>Astrophys. J. Lett</addtitle><date>2019-07-01</date><risdate>2019</risdate><volume>879</volume><issue>1</issue><spage>L8</spage><pages>L8-</pages><issn>2041-8205</issn><eissn>2041-8213</eissn><abstract>Two major questions regarding comets have been up to now far from any solution. (i) How is it possible that water-ice sublimation from the nucleus surface does not lead to an insulating crust, stopping every gas and dust ejection within a few days? (ii) How is it possible that the gas flow crossing the refractory surface crust ejects dust particles bonded by tensile strengths larger than tens of Pa when the perihelion gas pressure at the nucleus-coma interface is less than one Pa? We have developed a simple but rigorous analytical model, assuming that the cometary nucleus consists of agglomerates of ice and dust ("clusters"). As soon as the clusters become exposed to sunlight, gas diffusion from their inside leads to their dehydration. We find that (i) the gas diffusing from the interior to the surface of a sunlit cluster has a steep density gradient at the cluster surface, which blasts the cluster into particles of sizes larger than or equal to those actually observed by Rosetta dust instruments; (ii) the heat-conduction and diffusion timescales are much shorter than the dehydration timescale, ensuring that the described process prevents any dumping of the nucleus activity driven by water-ice sublimation from 4 au inbound to 4 au outbound; and (iii) the clusters are in fact cm-sized pebbles, so that a cometary nucleus made of pebbles is confirmed to be the only one consistent with cometary gas and dust activity, a process unexplained until now.</abstract><cop>Austin</cop><pub>The American Astronomical Society</pub><doi>10.3847/2041-8213/ab2898</doi><tpages>3</tpages><orcidid>https://orcid.org/0000-0001-8435-5287</orcidid><oa>free_for_read</oa></addata></record> |
fulltext | fulltext_linktorsrc |
identifier | ISSN: 2041-8205 |
ispartof | Astrophysical journal. Letters, 2019-07, Vol.879 (1), p.L8 |
issn | 2041-8205 2041-8213 |
language | eng |
recordid | cdi_iop_journals_10_3847_2041_8213_ab2898 |
source | IOP Publishing Free Content |
subjects | Agglomerates Bonding strength Clusters Comet nuclei Comets comets: general comets: individual (67P/Churyumov-Gerasimenko) Conduction heating Dehydration Density gradients Diffusion Dumping Dust Dust particles Gas flow Gas pressure Gaseous diffusion Ice Perihelions space vehicles: instruments Sublimation |
title | How Comets Work |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-09T12%3A31%3A51IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_O3W&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=How%20Comets%20Work&rft.jtitle=Astrophysical%20journal.%20Letters&rft.au=Fulle,%20M.&rft.date=2019-07-01&rft.volume=879&rft.issue=1&rft.spage=L8&rft.pages=L8-&rft.issn=2041-8205&rft.eissn=2041-8213&rft_id=info:doi/10.3847/2041-8213/ab2898&rft_dat=%3Cproquest_O3W%3E2365649235%3C/proquest_O3W%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2365649235&rft_id=info:pmid/&rfr_iscdi=true |