Clive Neal - Academia.edu (original) (raw)
Papers by Clive Neal
New chemical data for 15343,8,181. Trace-element data suggests that the large Opx crystals might ... more New chemical data for 15343,8,181. Trace-element data suggests that the large Opx crystals might be xenocrysts.
Covering Leg 205 of the cruises of the Drilling Vessel JOIDES Resolution Victoria, Canada, to Bal... more Covering Leg 205 of the cruises of the Drilling Vessel JOIDES Resolution Victoria, Canada, to Balboa, Panama Sites 1253–1255 2 September–6 November 2002. Julie D. Morris, Heinrich W. Villinger, Adam Klaus, Dawn Cardace, Valerie MC Chavagnac, Peter D. Clift, Matthias Haeckel, Toshio Hisamitsu, Miriam Kastner, Marion Pfender, Demian M. Saffer, Cara Santelli, Burkhard Schramm, Elizabeth J. Screaton, Evan A. Solomon, Michael Strasser, Moe Kyaw Thu, Paola Vannucchi. Adam Klaus. Julie D. Morris, Heinrich W. Villinger, Adam Klaus. ...
Lunar magma ocean theory (LMO) has been given much consideration recently. This study uses work o... more Lunar magma ocean theory (LMO) has been given much consideration recently. This study uses work on modeling the LMO to create a hybrid model. This will give insight into the formation of the Moon as well as using it for comparative planetary studies.
Analysis of Apollo 14 KREEP samples are presented along with evidence for magma chamber processes.
New mineral trace-element analyses support a cumulate origin of 71597 within a high-Ti basalt flo... more New mineral trace-element analyses support a cumulate origin of 71597 within a high-Ti basalt flow, likely of Type B1 composition.
Astronomy and Geophysics, 2006
We use crystal stratigraphy to explore the petrogenesis of the Apollo 12 ilmenite, pigeonite, and... more We use crystal stratigraphy to explore the petrogenesis of the Apollo 12 ilmenite, pigeonite, and feldspathic suite basalts.
Meteoritics, 1994
— The petrogenesis of Apollo 12 mare basalts has been examined with emphasis on trace‐element rat... more — The petrogenesis of Apollo 12 mare basalts has been examined with emphasis on trace‐element ratios and abundances. Vitrophyric basalts were used as parental compositions for the modelling, and proportions of fractionating phases were determined using the MAGFOX program of Longhi (1991). Crystal fractionation processes within crustal and sub‐crustal magma chambers are evaluated as a function of pressure. Knowledge of the fractionating phases allows trace‐element variations to be considered as either source related or as a product of post‐magma‐generation processes. For the ilmenite and olivine basalts, trace‐element variations are inherited from the source, but the pigeonite basalt data have been interpreted with open‐system evolution processes through crustal assimilation. Three groups of basalts have been examined: (1) Pigeonite basalts — produced by the assimilation of lunar crustal material by a parental melt (up to 3% assimilation and 10% crystal fractionation, with an “r” value of 0.3). (2) Ilmenite basalts — produced by variable degrees of partial melting (4–8%) of a source of olivine, pigeonite, augite, and plagioclase, brought together by overturn of the Lunar Magma Ocean (LMO) cumulate pile. After generation, which did not exhaust any of the minerals in the source, these melts experienced closed‐system crystal fractionation/accumulation. (3) Olivine basalts — produced by variable degrees of partial melting (5–10%) of a source of olivine, pigeonite, and augite. After generation, again without exhausting any of the minerals in the source, these melts evolved through crystal accumulation. The evolved liquid counterparts of these cumulates have not been sampled. The source compositions for the ilmenite and olivine basalts were calculated by assuming that the vitrophyric compositions were primary and the magmas were produced by non‐modal batch melting. Although the magnitude is unclear, evaluation of these source regions indicates that both be composed of early‐ and late‐stage Lunar Magma Ocean (LMO) cumulates, requiring an overturn of the cumulate pile.
Lunar and Planetary …, 1989
... Note that without the insight of our new data, this link between the Type A and B basa ~ ~ co... more ... Note that without the insight of our new data, this link between the Type A and B basa ~ ~ could not have been made. lEFEFENCES: [1] Shervais et at. ... (1975) PLSC 6, 1255-1285; [11] Laul at al. (1975) Origin of Mare Basatts, 91-93; [12] Murali at at. ...
www-odp.tamu.edu
... Rory D. Cottrell, Florence Einaudi, Frederick A. Frey, Jill A. Gudding, Sarah Haggas, Shichun... more ... Rory D. Cottrell, Florence Einaudi, Frederick A. Frey, Jill A. Gudding, Sarah Haggas, Shichun Huang, Randall A. Keller, Bryan C. Kerr, Sten Lindblom, Clive R. Neal, Marcel Regelous, Sidonie Révillon, William G. Siesser, Bernhard Steinberger, Johannes Stoll, Patricia ME ...
Covering Leg 192 of the cruises of the Drilling Vessel JOIDES Resolution Apra Harbor, Guam, to Ap... more Covering Leg 192 of the cruises of the Drilling Vessel JOIDES Resolution Apra Harbor, Guam, to Apra Harbor, Guam Sites 1183–1187 8 September–7 November 2000. John J. Mahoney, J. Godfrey Fitton, Paul J. Wallace, Maria J. Antretter, Neil R. Banerjee, James A. Bergen, Graeme Cairns, Paterno R. Castillo, Lynne M. Chambers, William J. Chazey III, Millard F. Coffin, Marguerite M. Godard, Stuart A. Hall, José Honnorez, Stephanie P. Ingle, Loren ...
... SCIENTIFIC OCEAN DRILLING STATUS QUO AND A LOOK AHEAD BY MILLARD F. COFFIN, ROBERT A. DUNCAN,... more ... SCIENTIFIC OCEAN DRILLING STATUS QUO AND A LOOK AHEAD BY MILLARD F. COFFIN, ROBERT A. DUNCAN, OLAV ELDHOLM, ... 104 Eldholm, Thiede, Taylor, et al., 1987, 1989 152 Larsen, Saunders, Clift, et al., 1994; Saunders, Larsen, and Wise, 1998 ...
We use chemical and textural analyses of olivines to distinguish between the Apollo 14 impact mel... more We use chemical and textural analyses of olivines to distinguish between the Apollo 14 impact melt-generated olivine vitrophyres and the pristine, High-Alumina mare basalts.
New chemical data for 15343,8,181. Trace-element data suggests that the large Opx crystals might ... more New chemical data for 15343,8,181. Trace-element data suggests that the large Opx crystals might be xenocrysts.
Covering Leg 205 of the cruises of the Drilling Vessel JOIDES Resolution Victoria, Canada, to Bal... more Covering Leg 205 of the cruises of the Drilling Vessel JOIDES Resolution Victoria, Canada, to Balboa, Panama Sites 1253–1255 2 September–6 November 2002. Julie D. Morris, Heinrich W. Villinger, Adam Klaus, Dawn Cardace, Valerie MC Chavagnac, Peter D. Clift, Matthias Haeckel, Toshio Hisamitsu, Miriam Kastner, Marion Pfender, Demian M. Saffer, Cara Santelli, Burkhard Schramm, Elizabeth J. Screaton, Evan A. Solomon, Michael Strasser, Moe Kyaw Thu, Paola Vannucchi. Adam Klaus. Julie D. Morris, Heinrich W. Villinger, Adam Klaus. ...
Lunar magma ocean theory (LMO) has been given much consideration recently. This study uses work o... more Lunar magma ocean theory (LMO) has been given much consideration recently. This study uses work on modeling the LMO to create a hybrid model. This will give insight into the formation of the Moon as well as using it for comparative planetary studies.
Analysis of Apollo 14 KREEP samples are presented along with evidence for magma chamber processes.
New mineral trace-element analyses support a cumulate origin of 71597 within a high-Ti basalt flo... more New mineral trace-element analyses support a cumulate origin of 71597 within a high-Ti basalt flow, likely of Type B1 composition.
Astronomy and Geophysics, 2006
We use crystal stratigraphy to explore the petrogenesis of the Apollo 12 ilmenite, pigeonite, and... more We use crystal stratigraphy to explore the petrogenesis of the Apollo 12 ilmenite, pigeonite, and feldspathic suite basalts.
Meteoritics, 1994
— The petrogenesis of Apollo 12 mare basalts has been examined with emphasis on trace‐element rat... more — The petrogenesis of Apollo 12 mare basalts has been examined with emphasis on trace‐element ratios and abundances. Vitrophyric basalts were used as parental compositions for the modelling, and proportions of fractionating phases were determined using the MAGFOX program of Longhi (1991). Crystal fractionation processes within crustal and sub‐crustal magma chambers are evaluated as a function of pressure. Knowledge of the fractionating phases allows trace‐element variations to be considered as either source related or as a product of post‐magma‐generation processes. For the ilmenite and olivine basalts, trace‐element variations are inherited from the source, but the pigeonite basalt data have been interpreted with open‐system evolution processes through crustal assimilation. Three groups of basalts have been examined: (1) Pigeonite basalts — produced by the assimilation of lunar crustal material by a parental melt (up to 3% assimilation and 10% crystal fractionation, with an “r” value of 0.3). (2) Ilmenite basalts — produced by variable degrees of partial melting (4–8%) of a source of olivine, pigeonite, augite, and plagioclase, brought together by overturn of the Lunar Magma Ocean (LMO) cumulate pile. After generation, which did not exhaust any of the minerals in the source, these melts experienced closed‐system crystal fractionation/accumulation. (3) Olivine basalts — produced by variable degrees of partial melting (5–10%) of a source of olivine, pigeonite, and augite. After generation, again without exhausting any of the minerals in the source, these melts evolved through crystal accumulation. The evolved liquid counterparts of these cumulates have not been sampled. The source compositions for the ilmenite and olivine basalts were calculated by assuming that the vitrophyric compositions were primary and the magmas were produced by non‐modal batch melting. Although the magnitude is unclear, evaluation of these source regions indicates that both be composed of early‐ and late‐stage Lunar Magma Ocean (LMO) cumulates, requiring an overturn of the cumulate pile.
Lunar and Planetary …, 1989
... Note that without the insight of our new data, this link between the Type A and B basa ~ ~ co... more ... Note that without the insight of our new data, this link between the Type A and B basa ~ ~ could not have been made. lEFEFENCES: [1] Shervais et at. ... (1975) PLSC 6, 1255-1285; [11] Laul at al. (1975) Origin of Mare Basatts, 91-93; [12] Murali at at. ...
www-odp.tamu.edu
... Rory D. Cottrell, Florence Einaudi, Frederick A. Frey, Jill A. Gudding, Sarah Haggas, Shichun... more ... Rory D. Cottrell, Florence Einaudi, Frederick A. Frey, Jill A. Gudding, Sarah Haggas, Shichun Huang, Randall A. Keller, Bryan C. Kerr, Sten Lindblom, Clive R. Neal, Marcel Regelous, Sidonie Révillon, William G. Siesser, Bernhard Steinberger, Johannes Stoll, Patricia ME ...
Covering Leg 192 of the cruises of the Drilling Vessel JOIDES Resolution Apra Harbor, Guam, to Ap... more Covering Leg 192 of the cruises of the Drilling Vessel JOIDES Resolution Apra Harbor, Guam, to Apra Harbor, Guam Sites 1183–1187 8 September–7 November 2000. John J. Mahoney, J. Godfrey Fitton, Paul J. Wallace, Maria J. Antretter, Neil R. Banerjee, James A. Bergen, Graeme Cairns, Paterno R. Castillo, Lynne M. Chambers, William J. Chazey III, Millard F. Coffin, Marguerite M. Godard, Stuart A. Hall, José Honnorez, Stephanie P. Ingle, Loren ...
... SCIENTIFIC OCEAN DRILLING STATUS QUO AND A LOOK AHEAD BY MILLARD F. COFFIN, ROBERT A. DUNCAN,... more ... SCIENTIFIC OCEAN DRILLING STATUS QUO AND A LOOK AHEAD BY MILLARD F. COFFIN, ROBERT A. DUNCAN, OLAV ELDHOLM, ... 104 Eldholm, Thiede, Taylor, et al., 1987, 1989 152 Larsen, Saunders, Clift, et al., 1994; Saunders, Larsen, and Wise, 1998 ...
We use chemical and textural analyses of olivines to distinguish between the Apollo 14 impact mel... more We use chemical and textural analyses of olivines to distinguish between the Apollo 14 impact melt-generated olivine vitrophyres and the pristine, High-Alumina mare basalts.