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Oceanographic changes in the Southern Ocean and Antarctic cryosphere dynamics during the mid-Miocene: a view from offshore Wilkes Land

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Oceanographic changes in the Southern Ocean and Antarctic cryosphere dynamics during the mid-Miocene: a

view from offshore Wilkes Land

Francesca  Sangiorgi1  (f.sangiorgi@uu.nl),  Peter  Bijl1,    Julian  Hartman1,  Stefan  Schouten2,  Henk  Brinkhuis1,  2     and  the  IODP  Exp.  318  ScienHsts    

1Marine  Palynology  &  Paleoceanography,  Dept.  Earth  Sciences,  LPP,  Utrecht  University,  The  Netherlands;    2  NIOZ  Royal  Netherlands  InsEtute  for  Sea  Research,  Texel,  The  Netherlands  

INTRODUCTION  

The  mid-­‐Miocene  Clima;c  Op;mum  (MCO,  ~17-­‐15  Ma)  is  one  of  the  most  pronounced  warming  events  since  the  onset  of  AntarcHc  glaciaHon  

~34  Ma  (1).  Ocean  temperatures  were  ~3-­‐6  °C  above  present-­‐day  (2,  3)  and  CO2  concentraHons  were  as  high  as  400  –  500  parts  per  million  in   volume  (ppmv)  (4),  condiHons  very  similar  to  those  projected  for  the  near  future.  Progressive  cooling  and  expansion  of  global  ice  volume4,  14   occurred  at  the  mid-­‐Miocene  Clima;c  Transi;on  (MCT  ~14.2  –  13.8  Ma)  together  with  a  decline  in  atmospheric  pCO2  to  close  to  200-­‐300  ppmv   (2,  4).  Studying  the  variability  of  the  EAIS  during  the  mid-­‐Miocene  can  help  understanding  its  sensiHvity  and  improving  sea  level  change   projecHons.  For  this,  ice-­‐proximal  records  covering  the  mid-­‐Miocene  are  essenHal  but  scarce.    

Here  we  present  new  paleoenvironmental  reconstrucHons  from  well-­‐dated  (5)  sediment  record  of  Integrated  Ocean  Drilling  Program  (IODP)   Site  1356,  offshore  Wilkes  Land  and  compare  to  those  from  Ross  Sea  ANDRILL  (AntarcHc  Drilling)  AND-­‐2A  (6)  and  Ocean  Drilling  Program  (ODP)   Site  1171  South  of  Tasmania  (2)  during  the  mid-­‐Miocene  to  get  insight  into  the  laHtudinal  temperature  gradients  and  role  of  oceanography  for   the  EAIS  dynamics.  ConHnental  temperatures  compared  to  those  of  a  paleolake  in  New  Zealand  (Lake  Manuherikia)  (7)  

MCO   was   warm   enough   to   sustain   melHng   of   conHnental   ice   and   was   mostly   sea-­‐ice   free   at   the   Wilkes   Land   margin.   Reduced   laHtudinal   temperature  gradient  between  Wilkes  Land  and  ODP  1171  (Figure  3)  indicates  weaker  oceanographic  fronts.  A  clear  temperature  gradient  exist   between  the  Wilkes  Land  margin  and  the  Ross  Sea  ANDRILL  drill  sites  throughout  the  MCO.  Aaer  the  MCO  the  climate  becomes  on  average   relaHvely   colder   at   Wilkes   Land   and   yet   very   variable.   Both   conHnental   and   marine   proxies   indicate   much   warmer   than   present-­‐day   temperatures  even  with  CO2  concentraHons  at  pre-­‐industrial  level.  Oceanography  plays  an  important  role  for  the  stability  of  the  EAIS    

MATERIALS  AND  METHODS    

IODP  Site  1356:  palynology  (pollen  and  dinoflagellate  cysts)  for  terrestrial  and  marine  

environmental  and  oceanographic  changes,  sedimentology  (clast  counts  as  Ice  Raaed  Debris)  and   organic  geochemistry  (TEX86L,  MBT/CBT  and  BIT  indices)  (8,  9,  10)  for  ocean  and  land  temperature   and  input  soil  organic  mager.  Record  covers  the  interval  ~16.7  –  12.7  Ma    

We  use  present  day  distribuHon  of  dinoflagellate  cysts  across  the  Southern  Ocean  fronts  (11,   Figure  1)  to  reconstruct  Miocene  environmental  condiHons  and  oceanography  

AND-­‐2A:    TEX86L    for  sub-­‐surface  ocean  temperature  (8)   ODP  Site  1171:  Mg/Ca  for  subsurface  ocean  temperature  (2)  

SAF STF

AAPF

Oceanic fronts Dinocysts

AAPF Antarctic Polar Front Selenopemphix antarctica SAF SubAntarctic Front Other Protoperidinioids STF Subtropical Front Impagidinium spp.

Nematosphaeropsis labyrinthus Operculodinium spp.

Other Gonyaulacoids U1356

AND-2A

1171 Paleolake

30˚S

150˚W

120˚W 180˚

150˚E 90˚W

60˚W

60˚S 60˚S

30˚S

RESULTS  MCO  Site  1356,  Wilkes   Land  (Figure  2)  

•  Absence  of  sea-­‐ice  dinocyst   indicator  Selenopemphix  antarcEca,   presence  of  temperate  dinocysts    

•  Absence  of  clasts  (IRD)  

•  High  pollen  percentages  of   temperate  pollen  Podocarpites  sp.,    

•  Mean  annual  conHnental   temperatures  (MATs)  of  6-­‐11OC,  

•  High  BIT  (high  input  of  soil  organic   material)    

•  High  TEX86L-­‐based  SSTs  (11-­‐16)OC    

AFTER  MCO    

•  Presence  of  S.  antarcEca  

•  Episodic  occurrence  N.  labyrinthus   (oceanic  fronts)    

•  High  Nothofagidites  pollen  (tundra-­‐

shrub)    

•  Pulses  of  IRD  

•  MATs  of  5OC  and  lower  SSTs  

Figure  1:  present-­‐day  dinoflagellate  cyst  assemblages  across  the   Southern  Ocean  fronts  (Prebble  et  al.,  2013)  and  locaHon  of  the   record  presented  

Site  1356  (WL)    

Figure  2:  clast  counts,  dinoflagellate  cysts,  BIT  index  and  pollen  at  Wilkes  Land    

Figure  3:  Average  marine  and  conHnental  temperatures  during   the  MCO  (below)  and  aaer  the  MCO  (above)  at  the  paleo-­‐

laHtude  locaHons  (12)  

DISCUSSION  AND  CONCLUSIONS  

References:  (1)  Zachos  et  al.,  2008,  Nature;  (2)  Shevenell  et  al.,  2004,  Science;  (3)  Herold  et  al.,  2011,  J.  Clim.;  (4)  Greenop  et  al.,  2014,  Paleoceanography;  (5)  Tauxe  et  al.,  2012,  Paleoceanography;  (6)  Levy  et  al.,   2016,  PNAS;  (7)  Reicheldt  et  al.,  Paleo3;  (8)  Kim  et  al.,  2012,  GJR;  (9)  Hopmans  et  al.,  2004,    EPSL;  (10)  Peterse  et  al.,  2012  GCA;  (11)  Prebble  et  al.,  2013,  Mar.  Micropal.;  (12)  Van  Hinsberger  et  al.  2015,  PLosOne  

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