con(nents, oceans, atmosphere and life evolu(on Ricardo Trindad

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University of São Paulo Ins4tute of Astronomy, Geophysics and Atmospheric Sciences The Precambrian Earth: con1nents, oceans, atmosphere and life evolu1on Ricardo Trindade www.iag.usp.br/interna4onal

Transcript of con(nents, oceans, atmosphere and life evolu(on Ricardo Trindad

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                                                   University  of  São  Paulo                                              Ins4tute  of  Astronomy,  Geophysics  and  Atmospheric  Sciences  

The  Precambrian  Earth:  con1nents,  oceans,  atmosphere  and  life  evolu1on                                                          Ricardo  Trindade  

www.iag.usp.br/interna4onal  

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Atmospheric  Sciences  Head  of  Department:  Fabio  Gonçalves  ([email protected])    

v Climatology  v Large  and  Mesoscale  Dynamics  v Ocean-­‐Atmosphere  and  Biosphere-­‐Atmosphere  interac:ons  v Micrometeorology  v Atmospheric  Pollu:on  v Hydrometeorology  

Par:cipa:on  in:  Go-­‐Amazon,  LBA    

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Astronomy  Head  of  Department:  Roberto  Costa  ([email protected])    

Brazilian  coordina:on  of:  GMT,  LLAMA,  mini-­‐CTA,  J-­‐PAS  

v Astrophysics  (stellar,  galac:c  and  extragalac:c)  v Cosmology  v Celes:al  Mechanics  v Astrometry  v Astronomical  Instrumenta:on    

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Astrobiology  &  Exoplanets  Group  (AstrobEx)  Coordinator:  Eduardo  Janot  Pacheco  ([email protected])    

AstroCam  (Hypobaric  Chamber)    

v Biomolecules  in  protoplatenary  disks  (ALMA)  v Exoplanets  and  habitability  (CoRoT,  KEPLER,  PLATO)  v Biomolecules  on  plametary  atmospheres  

     

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Geophysics  Head  of  Department:  Ricardo  Trindade  ([email protected])    v South  American  Plate  structure  and  dynamics    v Applied  Geophysics  (Environment,  Mineral  Resources)  

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Magne:c  anomaly  map  (WDMAM)  

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Magne:c  anomaly  map  (WDMAM)  

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Electrical  proper:es  in  depth  (resis:vity)  

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Li  et  al.  (2013)  Paleo-­‐3  

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Li  et  al.  (2013)  Paleo-­‐3  

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Li  et  al.  (2013)  Paleo-­‐3  

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Li  et  al.  (2013)  Paleo-­‐3  

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Age  (Ga)  

Och and Shields (2011) Earth Sci. Rev., Sahoo et al. (2012) Science, Lyons et al. (2014) Nature

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Och and Shields (2011) Earth Sci. Rev., Sahoo et al. (2012) Science, Lyons et al. (2014) Nature

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Oxida4on  aKer  glacia4on:  Fe  and  Mn  deposits  Mamatwan (Mn), South Africa

Pilbara (Fe), Australia Qudrilátero Ferrífero (Fe), Brazil

Huronian glacial rocks, Canada

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Och and Shields (2011) Earth Sci. Rev., Sahoo et al. (2012) Science, Lyons et al. (2014) Nature

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Workshop  in  NoVnghan,  April  2014  Accelera:ng  Neoproterozoic  Research  through  Scien:fic  Drilling    Three  key  areas  for  drilling:    v  South  China  (Yangtze  region)  

v West  Brazil  (MS  State)  

v White  Sea  (Russia)  

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The  actual  extension  of  glacial  caps:  Did  they  cover  the  en1re  Earth?  

What  did  cause  these  glacial  events?  

Neoproterozoic  Snowball  Earth  

How  did  we  scape  the  Snowball  Earth  events?  

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albedo ~ 0.3 pCO2 ~ 1.0 PAL

Hoffman & Schrag (2000). Scientific American, 282 , 68-75

albedo ~ 0.6 pCO2 ~ 0.1 PAL

The  Snowball  Earth  hypothesis:  Freezing  

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Results suggest that having continents in tropical latitudes is not

sufficient to bring the Earth in total freeze: Snowball

Earth

Donnadieu et al. (2004) Nature

Freezing  the  Earth:  Climate  and  Geochemical  model  

Supercontinent configuration (800 Ma): -  pCO2 equilibrates at 1800 ppm -  It corresponds to na average surface temperature of 10.2 °C

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Donnadieu et al. (2004) Nature

Freezing  the  Earth:  Climate  and  Geochemical  model  

Dispersed continents (Rodinia Break-Up at 750 Ma): -  pCO2 equilibrates at 500 ppm -  It corresponds to na average surface temperature of 2 °C (-8.2 °C)

A paleogeography with dispersed continents is more favorable to CO2

drawdawn.

It may trigger a large glaciation but not a Snowball Earth

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Redox  evolu1on  aKer  glacial  events?  

Mul1ple-­‐layered  stra1fied  oceans  (local  vs.  global  signals)?  

Neoproterozoic  Oxygena1on  Event  

Ocecan  and  atmospheric  oxygena1on  and  biological  evolu1on  

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 δ13CDIC  (‰)

DIC<2 mM

DIC>10 mM

depth  (m

)

0

20

40

60

80

0 2 4 -­‐2 -­‐4 -­‐6 Volcanic Lake Pavin (France)

Meromitic, Stratified

(Assayag et al., 2006, Appl. Geochem.)

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Ocean redox stratification and metabolic paths

Ccarb from OM

Ccarb from CH4

Ccarb from atm CO2

Ader  et  al.  (2009)  EPSL  

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Ader  et  al.  (2009)  EPSL  

Doushantuo  Forma:on,  South  China  

Ader  et  al.  (2009)  EPSL  

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…  But  do  animals  require  a  lot  of  oxygen?  

Sperling  et  al.  (2013)  EPSL    

Experiments  with  the  AstroCam:  Can  we  iden:fy  plesiomorphic  adapta:ons  of  early  metazoans  to  Neopropterozoic  ocean  chemistry  on  extant  animal  phyla?  

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In  fact,  oxygen  rise  may  have  been  driven  by  biological  innova:on…  

Lenton  et  al.  (2014)  Nat.  Geosciences  

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low O2 flux

high O2 flux

Did life evolution had impact on oxygenation? (Logan et al., 1995, Cohen et al., 2009)

To be tested through Sulphur isotopes…

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Och  and  Shields-­‐Zhou,  2011  

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Fike and Grotzinger, 2008

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Mul:ple  sulphur  isotopes  =  insight  into  the  non  steady  state  model  

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30%  

60%  

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Coupling between carbon and sulphur cycles

CO2  +  H2O  <=>  CH2O  +  O2   2CH2O  +  SO42-­‐  <=>  2HCO3-­‐  +  H2S  

Forg   Fpyr  

Photosynthesis   Bacterial  sulphate-­‐reduc:on  (BSR)  

O2  produc:on,  NOE  

=  Increase  of  30  to  70  %  PAL  pO2    

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Thanks

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2CO2  +  2H2O  <=>  2CH2O  +  2O2  

2CH2O  +  SO42-­‐  <=>  2HCO3

-­‐  +  H2S  

 [SO42-­‐]  =  3  -­‐  6  mM     8*1018  mol  of  sulphate,    

60%  (from  dis:lla:on)  =  5.6*1018  mol      

1.2*1019  mol  of  O2  liberated  into  the  Oc-­‐At  system  

=  Increase  of  30  to  70  %  PAL  pO2    

«  Back-­‐of-­‐the-­‐envelope  »  O2  quan:fica:on  

Es:ma:on  of  Kah  et  al.  2004  

*Vocean  I  

II  

III  

IV  

Catling  2011  Sansjofre  et  al.,  submised