Electrical Heating of Meteorite Parent Bodies and Planets by Dynamo Induction from a Pre-main Sequence T Tauri "Solar Wind"
SEVERAL lines of evidence suggest that the time interval of early heating in the solar system was short in comparison with the total age of solid matter. The fast heating process has been attributed to radiogenic matter of short half life. Urey was the first to point out the possible significance of...
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| Veröffentlicht in: | Nature (London) 1968-01, Vol.219 (5157), p.924-926 |
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| creator | SONETT, C. P COLBURN, D. S SCHWARTZ, K |
| description | SEVERAL lines of evidence suggest that the time interval of early heating in the solar system was short in comparison with the total age of solid matter. The fast heating process has been attributed to radiogenic matter of short half life. Urey was the first to point out the possible significance of
26
Al in this respect
1
, but certain difficulties eventually led him to question this hypothesis
2
. Interest was again aroused with Reynolds's discovery
3,4
of radiogenic daughter
129
Xe and, together with
244
Pu fission tracks
5
, this attests to the presence of short-lived sources of radiogenic heat in the protosolar nebula. Fish, Goles and Anders have studied the hypothesis of extinct radionuclide heating in great detail and have provided specific estimates of the required nuclide concentration for melting and differentiation
6
. |
| doi_str_mv | 10.1038/219924a0 |
| format | Article |
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26
Al in this respect
1
, but certain difficulties eventually led him to question this hypothesis
2
. Interest was again aroused with Reynolds's discovery
3,4
of radiogenic daughter
129
Xe and, together with
244
Pu fission tracks
5
, this attests to the presence of short-lived sources of radiogenic heat in the protosolar nebula. Fish, Goles and Anders have studied the hypothesis of extinct radionuclide heating in great detail and have provided specific estimates of the required nuclide concentration for melting and differentiation
6
.</description><identifier>ISSN: 0028-0836</identifier><identifier>EISSN: 1476-4687</identifier><identifier>DOI: 10.1038/219924a0</identifier><language>eng</language><publisher>London: Nature Publishing Group UK</publisher><subject>HEATING ; Humanities and Social Sciences ; INDUCTION ; letter ; METEORITES ; multidisciplinary ; N32150 --Physics--Astrophysics--Solar Phenomena ; PLANETS ; PLANETS/heating by dynamo induction from pre-main sequence T Tauri solar wind, (T) ; RADIATIONS ; Science ; Science (multidisciplinary) ; SOLAR WIND ; SOLAR WIND/effects on heating of planets and meteorite parent bodies by dynamo induction ; STARS ; STELLAR EVOLUTION ; SUN METEORITES/heating by dynamo induction from pre-main sequence T Tauri solar wind, (T) ; SUN/solar wind emission from pre- main sequence T Tauri phase of, (T)</subject><ispartof>Nature (London), 1968-01, Vol.219 (5157), p.924-926</ispartof><rights>Springer Nature Limited 1968</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-a332t-4524c2695e8a53f6d4ffea43843fea679b89f0520e23280d06e2e091034feb813</citedby><cites>FETCH-LOGICAL-a332t-4524c2695e8a53f6d4ffea43843fea679b89f0520e23280d06e2e091034feb813</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,885,2727,27924,27925</link.rule.ids><backlink>$$Uhttps://www.osti.gov/biblio/4484418$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>SONETT, C. P</creatorcontrib><creatorcontrib>COLBURN, D. S</creatorcontrib><creatorcontrib>SCHWARTZ, K</creatorcontrib><creatorcontrib>Ames Research Center, Moffett Field, Calif</creatorcontrib><title>Electrical Heating of Meteorite Parent Bodies and Planets by Dynamo Induction from a Pre-main Sequence T Tauri "Solar Wind"</title><title>Nature (London)</title><addtitle>Nature</addtitle><description>SEVERAL lines of evidence suggest that the time interval of early heating in the solar system was short in comparison with the total age of solid matter. The fast heating process has been attributed to radiogenic matter of short half life. Urey was the first to point out the possible significance of
26
Al in this respect
1
, but certain difficulties eventually led him to question this hypothesis
2
. Interest was again aroused with Reynolds's discovery
3,4
of radiogenic daughter
129
Xe and, together with
244
Pu fission tracks
5
, this attests to the presence of short-lived sources of radiogenic heat in the protosolar nebula. Fish, Goles and Anders have studied the hypothesis of extinct radionuclide heating in great detail and have provided specific estimates of the required nuclide concentration for melting and differentiation
6
.</description><subject>HEATING</subject><subject>Humanities and Social Sciences</subject><subject>INDUCTION</subject><subject>letter</subject><subject>METEORITES</subject><subject>multidisciplinary</subject><subject>N32150 --Physics--Astrophysics--Solar Phenomena</subject><subject>PLANETS</subject><subject>PLANETS/heating by dynamo induction from pre-main sequence T Tauri solar wind, (T)</subject><subject>RADIATIONS</subject><subject>Science</subject><subject>Science (multidisciplinary)</subject><subject>SOLAR WIND</subject><subject>SOLAR WIND/effects on heating of planets and meteorite parent bodies by dynamo induction</subject><subject>STARS</subject><subject>STELLAR EVOLUTION</subject><subject>SUN METEORITES/heating by dynamo induction from pre-main sequence T Tauri solar wind, (T)</subject><subject>SUN/solar wind emission from pre- main sequence T Tauri phase of, (T)</subject><issn>0028-0836</issn><issn>1476-4687</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1968</creationdate><recordtype>article</recordtype><recordid>eNpt0M1qGzEUBWBRGojrBPIE4eJVu5hGI2nGmmWbn8bgEEMcshyuNVeJwlhKJM3C9OUzxa1XXZ3Nx4FzGDsr-feSS30hyqYRCvknNinVvC5Ureef2YRzoQuuZX3MvqT0yjmvyrmasN_XPZkcncEebgmz888QLNxRphBdJlhhJJ_hZ-gcJUDfwapHTznBZgdXO4_bAAvfDSa74MHGsAWEVaRii87DA70P5A3BGtY4RAezh9BjhCfnu9kJO7LYJzr9m1P2eHO9vrwtlve_Fpc_lgVKKXKhKqGMqJuKNFbS1p2yllBJreSY9bzZ6MbySnASUmje8ZoE8WZ8Q1na6FJO2WzfG1J2bTLjLPNigvfj8lYprVSpR_R1j0wMKUWy7Vt0W4y7tuTtn2fbf8-O9NueppH4Z4rtaxiiHyf8z57vrcc8RDqUHsAHG0GBHg</recordid><startdate>19680101</startdate><enddate>19680101</enddate><creator>SONETT, C. P</creator><creator>COLBURN, D. S</creator><creator>SCHWARTZ, K</creator><general>Nature Publishing Group UK</general><scope>AAYXX</scope><scope>CITATION</scope><scope>OTOTI</scope></search><sort><creationdate>19680101</creationdate><title>Electrical Heating of Meteorite Parent Bodies and Planets by Dynamo Induction from a Pre-main Sequence T Tauri "Solar Wind"</title><author>SONETT, C. P ; COLBURN, D. S ; SCHWARTZ, K</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a332t-4524c2695e8a53f6d4ffea43843fea679b89f0520e23280d06e2e091034feb813</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1968</creationdate><topic>HEATING</topic><topic>Humanities and Social Sciences</topic><topic>INDUCTION</topic><topic>letter</topic><topic>METEORITES</topic><topic>multidisciplinary</topic><topic>N32150 --Physics--Astrophysics--Solar Phenomena</topic><topic>PLANETS</topic><topic>PLANETS/heating by dynamo induction from pre-main sequence T Tauri solar wind, (T)</topic><topic>RADIATIONS</topic><topic>Science</topic><topic>Science (multidisciplinary)</topic><topic>SOLAR WIND</topic><topic>SOLAR WIND/effects on heating of planets and meteorite parent bodies by dynamo induction</topic><topic>STARS</topic><topic>STELLAR EVOLUTION</topic><topic>SUN METEORITES/heating by dynamo induction from pre-main sequence T Tauri solar wind, (T)</topic><topic>SUN/solar wind emission from pre- main sequence T Tauri phase of, (T)</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>SONETT, C. P</creatorcontrib><creatorcontrib>COLBURN, D. S</creatorcontrib><creatorcontrib>SCHWARTZ, K</creatorcontrib><creatorcontrib>Ames Research Center, Moffett Field, Calif</creatorcontrib><collection>CrossRef</collection><collection>OSTI.GOV</collection><jtitle>Nature (London)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>SONETT, C. P</au><au>COLBURN, D. S</au><au>SCHWARTZ, K</au><aucorp>Ames Research Center, Moffett Field, Calif</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Electrical Heating of Meteorite Parent Bodies and Planets by Dynamo Induction from a Pre-main Sequence T Tauri "Solar Wind"</atitle><jtitle>Nature (London)</jtitle><stitle>Nature</stitle><date>1968-01-01</date><risdate>1968</risdate><volume>219</volume><issue>5157</issue><spage>924</spage><epage>926</epage><pages>924-926</pages><issn>0028-0836</issn><eissn>1476-4687</eissn><abstract>SEVERAL lines of evidence suggest that the time interval of early heating in the solar system was short in comparison with the total age of solid matter. The fast heating process has been attributed to radiogenic matter of short half life. Urey was the first to point out the possible significance of
26
Al in this respect
1
, but certain difficulties eventually led him to question this hypothesis
2
. Interest was again aroused with Reynolds's discovery
3,4
of radiogenic daughter
129
Xe and, together with
244
Pu fission tracks
5
, this attests to the presence of short-lived sources of radiogenic heat in the protosolar nebula. Fish, Goles and Anders have studied the hypothesis of extinct radionuclide heating in great detail and have provided specific estimates of the required nuclide concentration for melting and differentiation
6
.</abstract><cop>London</cop><pub>Nature Publishing Group UK</pub><doi>10.1038/219924a0</doi><tpages>3</tpages></addata></record> |
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| identifier | ISSN: 0028-0836 |
| ispartof | Nature (London), 1968-01, Vol.219 (5157), p.924-926 |
| issn | 0028-0836 1476-4687 |
| language | eng |
| recordid | cdi_crossref_primary_10_1038_219924a0 |
| source | Nature; Alma/SFX Local Collection |
| subjects | HEATING Humanities and Social Sciences INDUCTION letter METEORITES multidisciplinary N32150 --Physics--Astrophysics--Solar Phenomena PLANETS PLANETS/heating by dynamo induction from pre-main sequence T Tauri solar wind, (T) RADIATIONS Science Science (multidisciplinary) SOLAR WIND SOLAR WIND/effects on heating of planets and meteorite parent bodies by dynamo induction STARS STELLAR EVOLUTION SUN METEORITES/heating by dynamo induction from pre-main sequence T Tauri solar wind, (T) SUN/solar wind emission from pre- main sequence T Tauri phase of, (T) |
| title | Electrical Heating of Meteorite Parent Bodies and Planets by Dynamo Induction from a Pre-main Sequence T Tauri "Solar Wind" |
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