Magmatism at an active rift zone in Afar, Ethiopia David Ferguson Lamont-‐Doherty Earth Observatory, Columbia University, NY David Pyle (Oxford), Talfan Barnie (Cambridge), John Maclennan (Cambridge), Gezahegn Yirgu (Addis Ababa), Clive Oppenheimer (Cambridge), Jon Blundy (Bristol) Overview: source to surface magmaIsm at Quaternary riK zones ME R Latitude 12.5o 12o a Se 20 km 40.5o Longitude Ebinger, 2005 asthenosphere Links between melt produc;on/ thermomechanical state of the mantle and recent magma;c ri6 zones/ri6 development? G. Aden xis ta magmatic segments Afar Rif Timescales, volumes and physical mechanisms of melt emplacement at the ri6 surface Dabbahu R. Dabbah-Manda Hararo magmatic segment Melt ascent processes / lithospheric plumbing systems 41o ALI bands 10, 9, 8 (2.20, 1.65, 1.25 um) Dabbah-Manda Hararo magmatic segment Latitude 12.5o ALI bands 7, 5, 3 (0.87, 0.66, 0.48 um) Dabbahu xis ta 12o Rif 20 km 40.5o Longitude Ferguson et al. 2010 Dark material: proximal fire fountain deposits Proximal Sheet flow Scoria cones constructed along vent/ fissure Shear zones evolve into channels, levees develop Toe emplaced as sheet, similar to proximal flow Ferguson et al. 2010 Central flow channel 41o Barnie and Oppenheimer. in prep. ALI bands 10, 9, 8 (2.20, 1.65, 1.25 um) Toe emplaced as sheet, similar to proximal flow Ferguson et al. 2010 Effusion Rate (Qf) ow Shear zones evolve into channels, levees develop g fl nin Wa Scoria cones constructed along vent/ fissure Wadge, 1981 Eruption rate Time Dark material: proximal fire fountain deposits Proximal Sheet flow Waxing flow Radiance curve from SEVIRI data – proxy for effusion rate Mean radiance * pixels ALI bands 7, 5, 3 (0.87, 0.66, 0.48 um) Days Central flow channel Dalla Filla (Erta Ale) Nov. 2008 Dabbahu ri6 June 2009 Dabbahu ri6 Aug. 2007 Dabbahu ri6 May 2010 Melt volumes during Dabbahu riKing phase Wright et al. 2012. Ini;al part of ri6ing cycles are dominated by intrusion, volcanism becomes more likely later in cycle (relaxa;on of tectonic stress e.g. Buck et al. 2006). Dabbahu ri6ing phase has very high intruded to erupted melt ra;o – no ‘excess’ erup;ble melt? Ferguson et al. 2010. Melt generaLon and ascent: Trace element composiLons Rock / PM 100 Ethiopian flood basalts 10 Recent Afar/N.MER 1 Red Sea axial trough Rb Th Nb K Ce Sr Nd Zr Eu Tb Ho Er Yb Ba U Ta La Pb Pr Sm Hf Gd Dy Y Tm Lu • Afar lavas enriched in incompa;ble trace element compared to MORB/Red Sea lavas, similar to pre-‐ri6 flood lavas -‐ Afar lavas are not MORBs! • TE ra;os such Ba/Nb, Ce/Pb and La/Nb similar to OIB Melt ascent Frac;ona;on corrected composi;ons for Dabbahu ri6 lavas shows different mantle-‐melt equilibrium P-‐T condi;ons for melts erupted on-‐ and off-‐ axis. Variable petrogene;c processes for lavas erupted ~20 km apart. 8 P-‐T’s calculated using Si and Mg thermobarometer: Lee et al. 2009 a ME R Afar ta xis 40.5o Longitude 41o l. 2011 y et a Roone Depth (km) Se Dabbahu G. Aden Rif Latitude 12.5o 8.6 8.8 9 10 R. Dabbah-Manda Hararo magmatic segment 12o latitude 8.4 0 White et al. 2008 20 km 8.2 MER lavas show different ranges in crustal frac;ona;on depths depending on distance from ri6 margin -‐ ri6 centre lavas ascend more rapidly 20 30 pyroxene equilibraRon depths for MER lavas Wonji Fault Belt Rooney et al. 2007 Silti-Debre Zeyit F.Z Melt generaLon and ascent at an acLve riK zone in central Afar Separate plumbing systems feeding ri6 axis and off-‐axis volcanoes Vast majority of melt supplied to shallow crust is intruded as dykes Primary mel;ng occurs in hot mantle, significant upwelling and mel;ng limited to depths > 80 km Higher degree melts erupted at axis, suggests mantle upwelling is focused beneath axis of recent segment Future ques;ons…. • How do mel;ng processes vary along strike between the MER and the Red Sea? • Quan;fica;on of melt volumes and volcanic output • Volcanic architecture and erup;ve history/forma;on of ac;ve ri6 segments • Structure and composi;on of the lithospheric plate – xenoliths, melt-‐rock interac;ons, thermal models. • What links mantle processes to recent surface focusing of magma;c-‐tectonic ac;vity? magmatic segments asthenosphere Thank you…….
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