- 45 -hundred meters deep, where <strong>the</strong> <strong>Oligo</strong>cene clastics overlie upper Eocene strata (Fig. 24c and 25 andBuchbinder et al., 2005).In <strong>the</strong> Hanaha-1 borehole <strong>the</strong> <strong>Oligo</strong>cene incision cuts about 968 m (<strong>the</strong> thickness <strong>of</strong> <strong>the</strong> entire<strong>Oligo</strong>cene fill), breaching a NE-SW trending Syrian Arc fold structure (Figs. 5 and 24), thusindicating that <strong>the</strong> water depth during <strong>the</strong> Early <strong>Oligo</strong>cene exceeded 1,000 m. In comparison, arange <strong>of</strong> 1,600 m water depth was estimated for <strong>the</strong> Afiq Canyon (Druckman et al., 1995) in <strong>the</strong>Early <strong>Oligo</strong>cene.A Late Tortonian incision was interpreted in <strong>the</strong> Hannah-1 borehole, based on <strong>the</strong> dating <strong>of</strong> <strong>the</strong>channel fill underlying <strong>the</strong> Messinian evaporites (Fig. 24a). No stratigraphic gap was found between<strong>the</strong> evaporites and <strong>the</strong> underlying section <strong>of</strong> <strong>the</strong> channel fill. Both were assigned <strong>the</strong> MessinianNN11a nann<strong>of</strong>ossil zone (Micro-Strat, 2003). A major stratigraphic gap was found between <strong>the</strong>Late Tortonian, at <strong>the</strong> base <strong>of</strong> <strong>the</strong> channel, and <strong>the</strong> Early Langhian (early Middle <strong>Miocene</strong>)underlying section (Fig. 25). <strong>The</strong> Late Tortonian incision carved up to 965 m meters (<strong>the</strong>cumulative thickness <strong>of</strong> <strong>the</strong> Late Tortonian and Messinian canyon fill) (Fig. 24a,b).Based on <strong>the</strong> above observation it is concluded that <strong>the</strong> N marker (base evaporates) is, in fact,merely a velocity contrast between evaporites and low velocity sediments, and does not reflect anunconformity surface. <strong>The</strong> relief into which <strong>the</strong> Messinian evaporites were deposited was carved inLate Tortonian time.Near <strong>the</strong> coastline, in <strong>the</strong> Ashdod-1 borehole, <strong>the</strong> Late Tortonian canyon is about 700 m deep andalso overlies unconformably Langhian clastics similarly to <strong>the</strong> Hannah-1 borehole. It is filled by 50m <strong>of</strong> Messinian carbonate reefal debris overlain by a 150 m thick evaporitic section, which in turn isoverlain by a thick Pliocene section <strong>of</strong> ~ 1,740 m (Buchbinder et al., 2005) (Figs. 18, 21, 24 and25).<strong>The</strong> reduced evaporitic section and <strong>the</strong> significantly thicker Pliocene section overlying it (Fig. 24c)indicate <strong>the</strong> removal <strong>of</strong> part <strong>of</strong> <strong>the</strong> evaporites due to a ~ 800 m fall <strong>of</strong> <strong>the</strong> Messinian sea level(Druckman et al., 1995; Cartwright and Jackson, 2007) and thus signifies <strong>the</strong> post-evaporite incisionevent. This event is better pronounced in <strong>the</strong> Afiq Canyon, where <strong>the</strong> evaporites are overlain bylacustrine clastic sediment, reflecting <strong>the</strong> Lago Mare circum Mediterranean event.
- 46 -BMSL1400m.1500200025003000Hanna 1 H<strong>of</strong> Ashdod 1 Ashdod 1A(sidetracking)49.5Km 1.75Km 3.5Km1921195927862869288629952914U. Torton.3040MavqiimE. LanghianYafoMessinianU. <strong>Oligo</strong>cene BurdigalianLower <strong>Oligo</strong>ceneZiqim Fm.173918591901Bet GuvrinFm.........22202361(Pliocene)Pattish reef debrisUpper sands2460LowerclasticsLower sandsL. EoceneE - M EoceneSenonian25832964MavqiimBurdigalianShederot (Bathonian)16901785E. LanghianTalme Yafe (Albian)206121202151220523012592Legend:T.D. 2741mShaleMarlstoneZohar (Callovian)Karmon(Messinian)Bet GuvrinShetulim 11630LimestoneDolomiteT.D. 1670m?T.D. 3152mSandstoneConglomerateAnhydriteHalite350040003963?T.D. 4303mGevaram (upper Barremian)Stratigraphic contactHiatal or unconformity contactFigure 25: Stratigraphic cross section along <strong>the</strong> axis <strong>of</strong> <strong>the</strong> AshdodCanyon. <strong>The</strong> Early <strong>Oligo</strong>cene canyon breached <strong>the</strong> Hanna anticline andcut deep into <strong>the</strong> Early Cretaceous section. Onshore, <strong>the</strong> Late Tortonian(pre-Pattish reef) erosion removed <strong>the</strong> entire <strong>Miocene</strong> section. Offshore,in <strong>the</strong> Hanna 1well, part <strong>of</strong> <strong>the</strong> Early and Midlle <strong>Miocene</strong> escaped thiserosion event. Sedimentation was continuous from Late Tortonian to<strong>the</strong> Messinian in <strong>the</strong> Hanna 1 well, clearly indicating that <strong>the</strong> steep relieffilled by <strong>the</strong> Messinian evaporites originated already in Late Tortoniantimes and was not connected to Messinian sea-level fluctuations. <strong>The</strong>minor dips <strong>of</strong> post <strong>Oligo</strong>cene strata in Ashdod-1A to H<strong>of</strong> Ashdod-1wells are not in favor <strong>of</strong> basinward downfaulting during <strong>the</strong> <strong>Miocene</strong>as postulated by Gvirtzman et al. (2008). Datum: 1400 m BSL.
- Page 1 and 2: The Oligo-Miocene deepwater system
- Page 4 and 5: ITable of contentPageAbstract …
- Page 6: IIIFigure 16: Depth map of the base
- Page 9 and 10: - 2 -Oligo-Miocene sands were depos
- Page 11 and 12: - 4 -The discoveries of the early 2
- Page 13 and 14: - 6 -the southeastern part of the b
- Page 15 and 16: - 8 -Legend2D survey A2D survey B2D
- Page 17 and 18: - 10 -2.2 Seismic dataThe seismic i
- Page 19 and 20: - 12 -conditions, and possibly sedi
- Page 21 and 22: - 14 -3.3.2 Lower Oligocene sedimen
- Page 23 and 24: - 16 -Druckman, 2006; Bertoni and C
- Page 25 and 26: - 18 -aSWNETWT (ms)bSWHanaha-1NEMav
- Page 27 and 28: - 20 -aNWSETWT (ms)bYam West-1Ziqim
- Page 29 and 30: - 22 -WETWT (ms)aYam Yafo-1multiple
- Page 31 and 32: - 24 -NW SEaYam West-2Plio-Pleistoc
- Page 33 and 34: - 26 -A third incision surface, mar
- Page 35 and 36: - 28 -4.2.2 Deep, central part of t
- Page 37 and 38: - 30 -10812591167Figure 13: Time st
- Page 39 and 40: - 32 -10812591167Figure 15: Time st
- Page 41 and 42: - 34 -HaifaQishon302829AtlitCaesare
- Page 43 and 44: - 36 -Figure 19: Depth map on the t
- Page 45 and 46: - 38 -SW NEAfiq Canyon Ashdod Canyo
- Page 47 and 48: - 40 -The Beer Sheva-Afiq Canyon lo
- Page 49 and 50: - 42 -SWNE SW NE SW NEPlio-Pleistoc
- Page 51: - 44 -SWHanaha-1NE SW NE SW Hof Ash
- Page 55 and 56: - 48 -WE W E NW SEPlio-PleistoceneC
- Page 57 and 58: - 50 -W EPlio-PleistoceneMessinian
- Page 59 and 60: - 52 -S NPlio-PleistoceneM.-U. Mioc
- Page 61 and 62: Figure 31: Stratigraphic section al
- Page 63 and 64: - 56 -W ELower-slope and basin floo
- Page 65 and 66: - 58 -SlopeSusita + En-GevsandsShel
- Page 67 and 68: - 60 -In the Hadera Canyon the seis
- Page 69 and 70: - 62 -Additional mechanisms for tra
- Page 71 and 72: - 64 -The existence of channel fill
- Page 73 and 74: - 66 -SlopePartly Uplifted ?Hordos
- Page 75 and 76: - 68 -Oligo-Miocene sands were depo
- Page 77 and 78: - 70 -Druckman, Y., Conway, B.H., E
- Page 79 and 80: - 72 -Neev, D., 1960, A pre-Neogene