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Consequences of diffuse and channelled porous melt migration on uranium series disequilibria
Magmas erupted at mid-ocean ridges (MORB) result from decompression melting of upwelling mantle. However, the mechanism of melt transport from the source region to the surface is poorly understood. It is debated whether melt is transported through melt-filled conduits or cracks on short time scales...
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Published in: | Geochimica et cosmochimica acta 2002-12, Vol.66 (23), p.4133-4148 |
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description | Magmas erupted at mid-ocean ridges (MORB) result from decompression melting of upwelling mantle. However, the mechanism of melt transport from the source region to the surface is poorly understood. It is debated whether melt is transported through melt-filled conduits or cracks on short time scales (∼ 10
3–10
4 yrs). Radiogenic excess
226Ra in MORB indicates that melt is transported from the melting region on time scales less than the half life of
226Ra (∼1600 yrs), and has been used to argue for fast melt transport from the base of the melting column. However, excess
226Ra can be generated at the bottom of the melt column, during the onset of melting, and at the top of the melt column by reactive porous flow. Determining the depth at which
226Ra is generated is critical to interpreting the rate and mechanism of magma migration. A recent compilation of high quality U-series isotope data show that in many young basalts,
226Ra excess in MORB is negatively correlated with
230Th excess. The data suggest that
226Ra excess is generated independently of
230Th excess, and cannot be explained by “dynamic” or fractional melting, where observed radiogenic excesses are all generated at the base of the melt column. One explanation is that the negative correlation of activity ratios is a result of mixing of slow moving melt that has travelled through reactive, low-porosity pathways and relatively fast moving melt that has been transported in unreactive high-porosity channels. We investigate this possibility by calculating U-series disequilibria in a melting column in which high-porosity, unreactive channels form within a low-porosity matrix that is undergoing melting. The results show that the negative correlation of
226Ra and
230Th excesses observed in MORB can be produced if ∼60% of the total melt flux travels through the low-porosity matrix. This melt maintains
226Ra excesses via chromatographic fractionation of Ra and Th during equilibrium transport. Melt that travels through the unreactive, high-porosity channels is not able to maintain significant
226Ra excesses because Ra and Th are not fractionated from each other during transport and the transport time for melt in the channels to reach the top of the melt column is longer than the time scale for
226Ra excesses to decay. Mixing of melt from the high porosity channels with melt from the low-poro |
doi_str_mv | 10.1016/S0016-7037(02)00984-5 |
format | article |
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3 yrs), or whether there is a significant component of slow, equilibrium porous flow on much longer time scales (>∼ 10
3–10
4 yrs). Radiogenic excess
226Ra in MORB indicates that melt is transported from the melting region on time scales less than the half life of
226Ra (∼1600 yrs), and has been used to argue for fast melt transport from the base of the melting column. However, excess
226Ra can be generated at the bottom of the melt column, during the onset of melting, and at the top of the melt column by reactive porous flow. Determining the depth at which
226Ra is generated is critical to interpreting the rate and mechanism of magma migration. A recent compilation of high quality U-series isotope data show that in many young basalts,
226Ra excess in MORB is negatively correlated with
230Th excess. The data suggest that
226Ra excess is generated independently of
230Th excess, and cannot be explained by “dynamic” or fractional melting, where observed radiogenic excesses are all generated at the base of the melt column. One explanation is that the negative correlation of activity ratios is a result of mixing of slow moving melt that has travelled through reactive, low-porosity pathways and relatively fast moving melt that has been transported in unreactive high-porosity channels. We investigate this possibility by calculating U-series disequilibria in a melting column in which high-porosity, unreactive channels form within a low-porosity matrix that is undergoing melting. The results show that the negative correlation of
226Ra and
230Th excesses observed in MORB can be produced if ∼60% of the total melt flux travels through the low-porosity matrix. This melt maintains
226Ra excesses via chromatographic fractionation of Ra and Th during equilibrium transport. Melt that travels through the unreactive, high-porosity channels is not able to maintain significant
226Ra excesses because Ra and Th are not fractionated from each other during transport and the transport time for melt in the channels to reach the top of the melt column is longer than the time scale for
226Ra excesses to decay. Mixing of melt from the high porosity channels with melt from the low-porosity matrix at the top of the melting column can produce a negative correlation of
226Ra and
230Th excesses with the slope and magnitude observed in MORB. This transport process can also account for other aspects of the geochemistry of MORB, such as correlations between La/Yb, α
Sm/Nd, and Th/U and
226Ra and
230Th excess.</description><identifier>ISSN: 0016-7037</identifier><identifier>EISSN: 1872-9533</identifier><identifier>DOI: 10.1016/S0016-7037(02)00984-5</identifier><language>eng</language><publisher>Elsevier Ltd</publisher><subject>Marine</subject><ispartof>Geochimica et cosmochimica acta, 2002-12, Vol.66 (23), p.4133-4148</ispartof><rights>2002 Elsevier Science Ltd</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-a392t-fc8bdabe17da15e052fe4122ad17ebeaf733ce697c770138fb9091485e1f9453</citedby><cites>FETCH-LOGICAL-a392t-fc8bdabe17da15e052fe4122ad17ebeaf733ce697c770138fb9091485e1f9453</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids></links><search><creatorcontrib>Jull, M</creatorcontrib><creatorcontrib>Kelemen, P.B</creatorcontrib><creatorcontrib>Sims, K</creatorcontrib><title>Consequences of diffuse and channelled porous melt migration on uranium series disequilibria</title><title>Geochimica et cosmochimica acta</title><description>Magmas erupted at mid-ocean ridges (MORB) result from decompression melting of upwelling mantle. However, the mechanism of melt transport from the source region to the surface is poorly understood. It is debated whether melt is transported through melt-filled conduits or cracks on short time scales (<∼ 10
3 yrs), or whether there is a significant component of slow, equilibrium porous flow on much longer time scales (>∼ 10
3–10
4 yrs). Radiogenic excess
226Ra in MORB indicates that melt is transported from the melting region on time scales less than the half life of
226Ra (∼1600 yrs), and has been used to argue for fast melt transport from the base of the melting column. However, excess
226Ra can be generated at the bottom of the melt column, during the onset of melting, and at the top of the melt column by reactive porous flow. Determining the depth at which
226Ra is generated is critical to interpreting the rate and mechanism of magma migration. A recent compilation of high quality U-series isotope data show that in many young basalts,
226Ra excess in MORB is negatively correlated with
230Th excess. The data suggest that
226Ra excess is generated independently of
230Th excess, and cannot be explained by “dynamic” or fractional melting, where observed radiogenic excesses are all generated at the base of the melt column. One explanation is that the negative correlation of activity ratios is a result of mixing of slow moving melt that has travelled through reactive, low-porosity pathways and relatively fast moving melt that has been transported in unreactive high-porosity channels. We investigate this possibility by calculating U-series disequilibria in a melting column in which high-porosity, unreactive channels form within a low-porosity matrix that is undergoing melting. The results show that the negative correlation of
226Ra and
230Th excesses observed in MORB can be produced if ∼60% of the total melt flux travels through the low-porosity matrix. This melt maintains
226Ra excesses via chromatographic fractionation of Ra and Th during equilibrium transport. Melt that travels through the unreactive, high-porosity channels is not able to maintain significant
226Ra excesses because Ra and Th are not fractionated from each other during transport and the transport time for melt in the channels to reach the top of the melt column is longer than the time scale for
226Ra excesses to decay. Mixing of melt from the high porosity channels with melt from the low-porosity matrix at the top of the melting column can produce a negative correlation of
226Ra and
230Th excesses with the slope and magnitude observed in MORB. This transport process can also account for other aspects of the geochemistry of MORB, such as correlations between La/Yb, α
Sm/Nd, and Th/U and
226Ra and
230Th excess.</description><subject>Marine</subject><issn>0016-7037</issn><issn>1872-9533</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2002</creationdate><recordtype>article</recordtype><recordid>eNqFkE1LxDAQhoMouK7-BCEn0UN10jSb9iSy-AULHtyjENJkopE2XZNW8N_b7orXhSFzefPwzkPIOYNrBmxx8wrjm0ng8hLyK4CqLDJxQGaslHlWCc4Pyew_ckxOUvoEACkEzMjbsgsJvwYMBhPtHLXeuSEh1cFS86FDwKZBSzdd7IZEW2x62vr3qHvfBTrOEHXwQ0sTRj8SrJ9ovvF19PqUHDndJDz723OyfrhfL5-y1cvj8_JulWle5X3mTFlbXSOTVjOBIHKHBctzbZnEGrWTnBtcVNJICYyXrq6gYkUpkLmqEHxOLnbYTezGS1KvWp_M2FsHHEurXIKUlSj2Blk5gRd8DIpd0MQupYhObaJvdfxRDNTkXG2dq0moglxtnaupye3uH47XfnuMKhk_qbU-oumV7fwewi_aNoqe</recordid><startdate>20021201</startdate><enddate>20021201</enddate><creator>Jull, M</creator><creator>Kelemen, P.B</creator><creator>Sims, K</creator><general>Elsevier Ltd</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TN</scope><scope>F1W</scope><scope>H96</scope><scope>L.G</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>20021201</creationdate><title>Consequences of diffuse and channelled porous melt migration on uranium series disequilibria</title><author>Jull, M ; Kelemen, P.B ; Sims, K</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a392t-fc8bdabe17da15e052fe4122ad17ebeaf733ce697c770138fb9091485e1f9453</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2002</creationdate><topic>Marine</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Jull, M</creatorcontrib><creatorcontrib>Kelemen, P.B</creatorcontrib><creatorcontrib>Sims, K</creatorcontrib><collection>CrossRef</collection><collection>Oceanic Abstracts</collection><collection>ASFA: Aquatic Sciences and Fisheries Abstracts</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) 2: Ocean Technology, Policy & Non-Living Resources</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) Professional</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Geochimica et cosmochimica acta</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Jull, M</au><au>Kelemen, P.B</au><au>Sims, K</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Consequences of diffuse and channelled porous melt migration on uranium series disequilibria</atitle><jtitle>Geochimica et cosmochimica acta</jtitle><date>2002-12-01</date><risdate>2002</risdate><volume>66</volume><issue>23</issue><spage>4133</spage><epage>4148</epage><pages>4133-4148</pages><issn>0016-7037</issn><eissn>1872-9533</eissn><abstract>Magmas erupted at mid-ocean ridges (MORB) result from decompression melting of upwelling mantle. However, the mechanism of melt transport from the source region to the surface is poorly understood. It is debated whether melt is transported through melt-filled conduits or cracks on short time scales (<∼ 10
3 yrs), or whether there is a significant component of slow, equilibrium porous flow on much longer time scales (>∼ 10
3–10
4 yrs). Radiogenic excess
226Ra in MORB indicates that melt is transported from the melting region on time scales less than the half life of
226Ra (∼1600 yrs), and has been used to argue for fast melt transport from the base of the melting column. However, excess
226Ra can be generated at the bottom of the melt column, during the onset of melting, and at the top of the melt column by reactive porous flow. Determining the depth at which
226Ra is generated is critical to interpreting the rate and mechanism of magma migration. A recent compilation of high quality U-series isotope data show that in many young basalts,
226Ra excess in MORB is negatively correlated with
230Th excess. The data suggest that
226Ra excess is generated independently of
230Th excess, and cannot be explained by “dynamic” or fractional melting, where observed radiogenic excesses are all generated at the base of the melt column. One explanation is that the negative correlation of activity ratios is a result of mixing of slow moving melt that has travelled through reactive, low-porosity pathways and relatively fast moving melt that has been transported in unreactive high-porosity channels. We investigate this possibility by calculating U-series disequilibria in a melting column in which high-porosity, unreactive channels form within a low-porosity matrix that is undergoing melting. The results show that the negative correlation of
226Ra and
230Th excesses observed in MORB can be produced if ∼60% of the total melt flux travels through the low-porosity matrix. This melt maintains
226Ra excesses via chromatographic fractionation of Ra and Th during equilibrium transport. Melt that travels through the unreactive, high-porosity channels is not able to maintain significant
226Ra excesses because Ra and Th are not fractionated from each other during transport and the transport time for melt in the channels to reach the top of the melt column is longer than the time scale for
226Ra excesses to decay. Mixing of melt from the high porosity channels with melt from the low-porosity matrix at the top of the melting column can produce a negative correlation of
226Ra and
230Th excesses with the slope and magnitude observed in MORB. This transport process can also account for other aspects of the geochemistry of MORB, such as correlations between La/Yb, α
Sm/Nd, and Th/U and
226Ra and
230Th excess.</abstract><pub>Elsevier Ltd</pub><doi>10.1016/S0016-7037(02)00984-5</doi><tpages>16</tpages></addata></record> |
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subjects | Marine |
title | Consequences of diffuse and channelled porous melt migration on uranium series disequilibria |
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