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The Boltysh crater fill sediments – a 500,000 year record of the
lower Danian
I. Gilmour1, D.W. Jolley2, R.J. Daly2, S.P. Kelley1, and M.A. Gilmour1
1. Department of Physical Sciences, The Open University, Milton Keynes MK7 6AA, UK
2. Department of Geology & Petroleum Geology, University of Aberdeen, Aberdeen AB9 2UE, UK
The Boltysh crater lacustrine sediments accumulated in around 600m of
accommodation space on the Ukrainian shield. The continuity of this
accommodation space post-impact would have ensured a continuous record of
deposition without the intervals of non-deposition inherent in fluvio-deltaic
depositional settings.
Boltysh Impact Crater
•  25km complex crater
•  Ukrainian Shield – impact on
land
•  Ar/Ar age 65.17 ± 0.64 Ma
(Kelley & Gurov, 2002)
Boltysh Impact Crater
•  25km complex crater
•  Ukrainian Shield – impact on
land
•  Ar/Ar age 65.17 ± 0.64 Ma
(Kelley & Gurov, 2002)
•  Drilled in the 1960s & 70s
•  Cores lost
Boltysh Impact Crater
•  25km complex crater
•  Ukrainian Shield – impact on
land
•  Ar/Ar age 65.17 ± 0.64 Ma
(Kelley & Gurov, 2002)
•  Drilled in the 1960s & 70s
•  Cores lost
•  500m crater-fill sediments central peak
Impact melt
Cross	
  sec(on	
  reconstructed	
  from	
  Russian	
  data	
  
Boltysh Impact Crater
•  25km complex crater
•  Ukrainian Shield – impact on
land
•  Ar/Ar age 65.17 ± 0.64 Ma
(Kelley & Gurov, 2002)
•  Drilled in the 1960s & 70s
•  Cores lost
•  500m crater-fill sediments
•  Paleogeography
n the North-Eastern Peri-Tethys during the Cretaceous
Baraboshkin	
  et	
  al.,	
  2003	
  
Drilled ~12m impact breccia
at base of hole
•  596m	
  cored	
  borehole	
  west	
  of	
  central	
  upliA	
  
•  >95%	
  recovery	
  
•  596	
  -­‐	
  582m	
  –	
  allochthonous	
  impact	
  breccia	
  
•  390m	
  Cenzoic	
  crater	
  fill	
  
•  582	
  –	
  490m	
  cyclic,	
  fining	
  upwards,	
  poorly	
  sorted	
  
sands	
  and	
  sandy	
  muds	
  >	
  turbidity	
  currents	
  
•  490	
  –	
  190m	
  finely	
  laminated	
  organic	
  rich	
  shales	
  
•  Lacustrine,	
  abundant	
  plant	
  macrofossils	
  
•  ~300m	
  abundant	
  ostracods	
  and	
  gastropods	
  (in	
  life	
  
posi(on),	
  interbedded	
  with	
  gypsum	
  lamellae	
  >	
  
shallow	
  evapora(ve	
  lake	
  
Palynology Summary
•  Palynomorphs – most
abundant fossil group
•  Good preservation – no
thermal alteration/degradation
•  Dominated by pollen and
spores but include algae
•  Early Danian throughout
–  Consistent with Cavagnetto and
Gaudant (2000) based on IGCP
pollen stratigraphic scheme of
Meyer (1980)
•  Highly diverse palynoflora
–  crater marginal
–  regional vegetation
Ferns	
  
Swamp	
  cypresses	
  
Normapolles	
  
Relationship between the Boltysh and Chicxulub Impacts
•  Palynological Succession
–  Replacement of one floral
community with another in a given
area
•  Supported by δ13CTOC record
•  Recovery successions
–  Well documented (volcanic)
–  K-Pg from Western Interior (US)
•  “Fern spike” – an influx of fern spores in
post K-Pg sediments
•  Phase 1 – warm temperate, subhumid,
broadleaved evergreeen
•  Phase 2 – leaf, rhizome and cuticles of
ferns
•  Phase 3 – early successional, high ppt
•  Phase 4 – warm temperate, moderately
diverse
Location of K/Pg Boundary
Jolley,	
  D.W.,	
  Gilmour,	
  I.,	
  Gurov,	
  E.P.,	
  Kelley,	
  S.P.,	
  Watson,	
  J.,	
  2010.	
  Geology	
  38,	
  835–838.	
  
	
  
Hopane	
  in	
  sediment	
  (biological	
  configura(on)	
  
Hopane	
  in	
  sediment	
  (geological	
  configura(on)	
  
ββ22R	
  
βα22R	
   αβ22R	
   αβ22S	
  
x
ββ
ββ	
  +	
  αβ	
  +	
  βα
Energy	
  
Reac(on	
  progress	
  
AAer	
  Seifert	
  and	
  Moldowan,	
  1980)	
  
ββ
βα
αβ
ΔG2	
  
ΔG3	
  
ΔG1	
  
ΔG4	
  
Thermal	
  maturity	
  
8.5m	
  
No	
  ββ	
  present	
  
ββ	
  biological	
  
7.1m	
  
ββ	
  transi(on	
  
Modelling cooling of impact hydrothermal systems
Figure 3. Results of a numerical simulation of the hydrothermal system at a 30-km crater on early
Mars. The central peak of the crater is on the left side of each figure. Surface permeability k0 is 10À2
darcies.
Solid arrows and dotted arrows indicate the water and steam fluxes, respectively. The lack of arrows in some
regions indicates that fluxes are less than 2 orders of magnitude smaller than the maximum flux. Solid lines
are isotherms, labeled in degrees Celsius. The length of the arrows scales logarithmically with the flux
magnitude, and the maximum value changes with each plot. (a) 25 years, max. water flux = 6.66 Â
E12S09 ABRAMOV AND KRING: HYDROTHERMAL ACTIVITY ON EARLY MARS E12S09
Abramov	
  &	
  Kring,	
  2005)	
  
8.5m	
  
No	
  ββ	
  present	
  
ββ	
  biological	
  
7.1m	
  
ββ	
  transi(on	
  
ca.	
  20ka	
  
Jolley,	
  D.W.,	
  Gilmour,	
  I.,	
  Gurov,	
  E.P.,	
  Kelley,	
  S.P.,	
  Watson,	
  J.,	
  2010.	
  Geology	
  38,	
  835–838.	
  
	
  
<20ka	
  
Boltysh
•  Pre-dates Chicxulub impact
–  Establishment of an early successional flora post
Boltysh impact implies 5-10ka pre-Chicxulub
•  Cooling hydrothermal system
–  Timescale for post-Boltysh and Post-Chicxulub
recovery
•  Rest of core
–  550 C-isotope measurements
–  Early Danian climate change
Carbon Isotopes
•  algal/higher plant input
•  Significant CIE 537 – 271m
•  Lacustrine δ13Corg
•  Selective preservation
•  Maturation
•  Allochthonous inputs
•  Boltysh OM
•  Immature sapropellic kerogen
•  %C not correlated with δ13Corg
•  Reliable indicator of C cycle change
K	
  
Pg	
  
-38 -36 -34 -32 -30 -28 -26 -24 -22 -20
δ13Corg (‰)
Δδ13C	
  ~	
  -­‐3‰	
  
Δδ13C	
  ~	
  +4‰	
  
	
  
Posi(ve	
  excursion	
  
-38 -36 -34 -32 -30 -28 -26 -24 -22 -20
δ13Corg (‰)
Dan-C2 CIE
!  Atlantic (Quillévéré et al. (2008)
–  Benthic δ13C
–  2 excursions
!  Tethys (Coccioni et al. (2010)
–  Similar to Atlantic
X  Pacific (Westerhold et al. 2011)
–  No record at Shatsky Rise
–  Restricted to Atlantic?
!  Continental
–  Boltysh lacustrine record
–  Global CIE
Quillévéré	
  et	
  al.	
  (2008)	
  
Fig. 2. Changes in δ13
C and δ18
O of bulk sediments, CaCO3 content, and magnetic susceptibility (χ) in the lowermost Danian at Contessa Highway, plotted with changes in δ13
C and δ18
O of bulk sediments, CaCO3 content, and magnetic
susceptibility from the equivalent stratigraphic interval at ODP Hole 1049C (Black Nose, NW Atlantic) and DSDP Holes 527 and 528 (Walvis Ridge, SE Atlantic), where the Dan-C2 event was first recognized by Quillévéré et al. (2008). Reliable
300R.Coccionietal./EarthandPlanetaryScienceLetters297(2010)298–3
Coccioni	
  et	
  al.	
  2010	
  
Comparison with Toarcian and PETM CIEs
In contrast to the marine Dan-C2 records, the Boltysh record more closely
resembles other major CIEs – Isotope stages after Cohen et al. (2007)
CIE Mass Balance
McInerney & Wing (2011)
regional and even global ecosystems. A rapid larly forced, end Maastrichtian extinctions across the
Fig. 1. Present-day Deccan Trap outcrop extent. Major tectonic structures redrawn from Biswas (1991).
Main Deccan Province – from Cripps et al. (2005)
•  Final	
  stages	
  of	
  Deccan	
  –	
  interac(on	
  of	
  basal(c	
  lavas	
  and	
  dykes	
  with	
  con(nental	
  shelf	
  sediments	
  
•  Evidence	
  of	
  interac(on	
  in	
  the	
  Mumbai	
  area	
  organic-­‐rich	
  shales	
  occur	
  as	
  intertrappean	
  sequences	
  
•  δ13Corg	
  ~	
  -­‐26‰	
  	
  
•  Produc(on	
  of	
  thermogenic	
  CH4	
  from	
  sedimentary	
  organic	
  
•  isotopic	
  frac(ona(on	
  =	
  -­‐1.4‰	
  and	
  -­‐17.5‰	
  (Clayton	
  et	
  al.	
  1991)	
  
in the
vitrinit
intrusi
and M
accura
tures
900 °C
An
is that
into ho
as long
ganic m
sins w
emplac
(13) sh
geothe
thickn
and Cesare (1993) contoured for pressures ranging from 100 to 500 MPa. For
methane at $375 °C, while fluids in rocks of 5 wt.% TOC are miscible at $2
Calculated densities of the fluid(s) at 100 MPa. At this pressure the CH4-domina
while the H2O-dominated phase will have a relatively much higher density of $9
totalKarooBasin
westernKarooBasin
wt%TOC
Area intruded by 100 m thick sill [km2]
GenerationpotentialCH4[Gt]
35 000
30 000
25 000
20 000
15 000
10 000
5 000
50 000 250 000 350 000150 000
10
9
8
7
6
5
4
3
2
1
VøringandMøreBasins
Fig. 9. Calculated total methane potential in gigatons, (Gt) as a
function of area covered by a cumulative intrusion thickness of
100 m continuous sill. The generation potentials are for the western
7017	
  Gt	
  
150	
  000	
  km2	
  
Thermogenic methane from contact metamorphism
(Aarnes et al., 2010)
Summary – Boltysh Crater fill sediments
•  24km diameter Boltysh Impact Crater in Ukraine
–  Lacustrine crater fill sequence of fine grained organic carbon-rich sediments
–  Preserve a uniquely complete and detailed negative carbon isotope excursion (CIE) in
an expanded section of several hundred metres.
•  Position of CIE in the early Danian, ca. 200ka above K/Pg
–  Correlates with Dan-C2 CIE in marine record
–  Early Danian Hyperthermal Event
•  Changes in floral communities through the CIE reflect changing biomes
caused by rapidly warming climate, followed by recovery
–  EDH event had a similar duration to the Toarcian and Paleocene/Eocene events
•  Temporal correlation EDH event with late stages of Deccan Continental
Flood basalt province, and initiation of rifting
–  Deccan province: cause of global warming and the carbon-isotope excursion
•  A high resolution record that is potentially resolving the effect of
Chicxulub from the effects of Deccan
•  High resolution/stratigraphically complete records have implications…

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The Boltysh crater fill sediments – a 500,000 year record of the lower Danian

  • 1. The Boltysh crater fill sediments – a 500,000 year record of the lower Danian I. Gilmour1, D.W. Jolley2, R.J. Daly2, S.P. Kelley1, and M.A. Gilmour1 1. Department of Physical Sciences, The Open University, Milton Keynes MK7 6AA, UK 2. Department of Geology & Petroleum Geology, University of Aberdeen, Aberdeen AB9 2UE, UK
  • 2. The Boltysh crater lacustrine sediments accumulated in around 600m of accommodation space on the Ukrainian shield. The continuity of this accommodation space post-impact would have ensured a continuous record of deposition without the intervals of non-deposition inherent in fluvio-deltaic depositional settings.
  • 3. Boltysh Impact Crater •  25km complex crater •  Ukrainian Shield – impact on land •  Ar/Ar age 65.17 ± 0.64 Ma (Kelley & Gurov, 2002)
  • 4. Boltysh Impact Crater •  25km complex crater •  Ukrainian Shield – impact on land •  Ar/Ar age 65.17 ± 0.64 Ma (Kelley & Gurov, 2002) •  Drilled in the 1960s & 70s •  Cores lost
  • 5. Boltysh Impact Crater •  25km complex crater •  Ukrainian Shield – impact on land •  Ar/Ar age 65.17 ± 0.64 Ma (Kelley & Gurov, 2002) •  Drilled in the 1960s & 70s •  Cores lost •  500m crater-fill sediments central peak Impact melt Cross  sec(on  reconstructed  from  Russian  data  
  • 6. Boltysh Impact Crater •  25km complex crater •  Ukrainian Shield – impact on land •  Ar/Ar age 65.17 ± 0.64 Ma (Kelley & Gurov, 2002) •  Drilled in the 1960s & 70s •  Cores lost •  500m crater-fill sediments •  Paleogeography n the North-Eastern Peri-Tethys during the Cretaceous Baraboshkin  et  al.,  2003  
  • 7.
  • 8.
  • 9. Drilled ~12m impact breccia at base of hole
  • 10.
  • 11. •  596m  cored  borehole  west  of  central  upliA   •  >95%  recovery   •  596  -­‐  582m  –  allochthonous  impact  breccia   •  390m  Cenzoic  crater  fill   •  582  –  490m  cyclic,  fining  upwards,  poorly  sorted   sands  and  sandy  muds  >  turbidity  currents   •  490  –  190m  finely  laminated  organic  rich  shales   •  Lacustrine,  abundant  plant  macrofossils   •  ~300m  abundant  ostracods  and  gastropods  (in  life   posi(on),  interbedded  with  gypsum  lamellae  >   shallow  evapora(ve  lake  
  • 12. Palynology Summary •  Palynomorphs – most abundant fossil group •  Good preservation – no thermal alteration/degradation •  Dominated by pollen and spores but include algae •  Early Danian throughout –  Consistent with Cavagnetto and Gaudant (2000) based on IGCP pollen stratigraphic scheme of Meyer (1980) •  Highly diverse palynoflora –  crater marginal –  regional vegetation Ferns   Swamp  cypresses   Normapolles  
  • 13. Relationship between the Boltysh and Chicxulub Impacts •  Palynological Succession –  Replacement of one floral community with another in a given area •  Supported by δ13CTOC record •  Recovery successions –  Well documented (volcanic) –  K-Pg from Western Interior (US) •  “Fern spike” – an influx of fern spores in post K-Pg sediments •  Phase 1 – warm temperate, subhumid, broadleaved evergreeen •  Phase 2 – leaf, rhizome and cuticles of ferns •  Phase 3 – early successional, high ppt •  Phase 4 – warm temperate, moderately diverse
  • 14. Location of K/Pg Boundary Jolley,  D.W.,  Gilmour,  I.,  Gurov,  E.P.,  Kelley,  S.P.,  Watson,  J.,  2010.  Geology  38,  835–838.    
  • 15. Hopane  in  sediment  (biological  configura(on)   Hopane  in  sediment  (geological  configura(on)   ββ22R   βα22R   αβ22R   αβ22S   x
  • 16. ββ ββ  +  αβ  +  βα Energy   Reac(on  progress   AAer  Seifert  and  Moldowan,  1980)   ββ βα αβ ΔG2   ΔG3   ΔG1   ΔG4   Thermal  maturity  
  • 17. 8.5m   No  ββ  present   ββ  biological   7.1m   ββ  transi(on  
  • 18. Modelling cooling of impact hydrothermal systems Figure 3. Results of a numerical simulation of the hydrothermal system at a 30-km crater on early Mars. The central peak of the crater is on the left side of each figure. Surface permeability k0 is 10À2 darcies. Solid arrows and dotted arrows indicate the water and steam fluxes, respectively. The lack of arrows in some regions indicates that fluxes are less than 2 orders of magnitude smaller than the maximum flux. Solid lines are isotherms, labeled in degrees Celsius. The length of the arrows scales logarithmically with the flux magnitude, and the maximum value changes with each plot. (a) 25 years, max. water flux = 6.66 Â E12S09 ABRAMOV AND KRING: HYDROTHERMAL ACTIVITY ON EARLY MARS E12S09 Abramov  &  Kring,  2005)  
  • 19. 8.5m   No  ββ  present   ββ  biological   7.1m   ββ  transi(on   ca.  20ka  
  • 20. Jolley,  D.W.,  Gilmour,  I.,  Gurov,  E.P.,  Kelley,  S.P.,  Watson,  J.,  2010.  Geology  38,  835–838.     <20ka  
  • 21. Boltysh •  Pre-dates Chicxulub impact –  Establishment of an early successional flora post Boltysh impact implies 5-10ka pre-Chicxulub •  Cooling hydrothermal system –  Timescale for post-Boltysh and Post-Chicxulub recovery •  Rest of core –  550 C-isotope measurements –  Early Danian climate change
  • 22. Carbon Isotopes •  algal/higher plant input •  Significant CIE 537 – 271m •  Lacustrine δ13Corg •  Selective preservation •  Maturation •  Allochthonous inputs •  Boltysh OM •  Immature sapropellic kerogen •  %C not correlated with δ13Corg •  Reliable indicator of C cycle change K   Pg   -38 -36 -34 -32 -30 -28 -26 -24 -22 -20 δ13Corg (‰) Δδ13C  ~  -­‐3‰   Δδ13C  ~  +4‰     Posi(ve  excursion  
  • 23. -38 -36 -34 -32 -30 -28 -26 -24 -22 -20 δ13Corg (‰)
  • 24. Dan-C2 CIE !  Atlantic (Quillévéré et al. (2008) –  Benthic δ13C –  2 excursions !  Tethys (Coccioni et al. (2010) –  Similar to Atlantic X  Pacific (Westerhold et al. 2011) –  No record at Shatsky Rise –  Restricted to Atlantic? !  Continental –  Boltysh lacustrine record –  Global CIE Quillévéré  et  al.  (2008)   Fig. 2. Changes in δ13 C and δ18 O of bulk sediments, CaCO3 content, and magnetic susceptibility (χ) in the lowermost Danian at Contessa Highway, plotted with changes in δ13 C and δ18 O of bulk sediments, CaCO3 content, and magnetic susceptibility from the equivalent stratigraphic interval at ODP Hole 1049C (Black Nose, NW Atlantic) and DSDP Holes 527 and 528 (Walvis Ridge, SE Atlantic), where the Dan-C2 event was first recognized by Quillévéré et al. (2008). Reliable 300R.Coccionietal./EarthandPlanetaryScienceLetters297(2010)298–3 Coccioni  et  al.  2010  
  • 25. Comparison with Toarcian and PETM CIEs In contrast to the marine Dan-C2 records, the Boltysh record more closely resembles other major CIEs – Isotope stages after Cohen et al. (2007)
  • 26. CIE Mass Balance McInerney & Wing (2011)
  • 27. regional and even global ecosystems. A rapid larly forced, end Maastrichtian extinctions across the Fig. 1. Present-day Deccan Trap outcrop extent. Major tectonic structures redrawn from Biswas (1991). Main Deccan Province – from Cripps et al. (2005) •  Final  stages  of  Deccan  –  interac(on  of  basal(c  lavas  and  dykes  with  con(nental  shelf  sediments   •  Evidence  of  interac(on  in  the  Mumbai  area  organic-­‐rich  shales  occur  as  intertrappean  sequences   •  δ13Corg  ~  -­‐26‰     •  Produc(on  of  thermogenic  CH4  from  sedimentary  organic   •  isotopic  frac(ona(on  =  -­‐1.4‰  and  -­‐17.5‰  (Clayton  et  al.  1991)  
  • 28. in the vitrinit intrusi and M accura tures 900 °C An is that into ho as long ganic m sins w emplac (13) sh geothe thickn and Cesare (1993) contoured for pressures ranging from 100 to 500 MPa. For methane at $375 °C, while fluids in rocks of 5 wt.% TOC are miscible at $2 Calculated densities of the fluid(s) at 100 MPa. At this pressure the CH4-domina while the H2O-dominated phase will have a relatively much higher density of $9 totalKarooBasin westernKarooBasin wt%TOC Area intruded by 100 m thick sill [km2] GenerationpotentialCH4[Gt] 35 000 30 000 25 000 20 000 15 000 10 000 5 000 50 000 250 000 350 000150 000 10 9 8 7 6 5 4 3 2 1 VøringandMøreBasins Fig. 9. Calculated total methane potential in gigatons, (Gt) as a function of area covered by a cumulative intrusion thickness of 100 m continuous sill. The generation potentials are for the western 7017  Gt   150  000  km2   Thermogenic methane from contact metamorphism (Aarnes et al., 2010)
  • 29.
  • 30. Summary – Boltysh Crater fill sediments •  24km diameter Boltysh Impact Crater in Ukraine –  Lacustrine crater fill sequence of fine grained organic carbon-rich sediments –  Preserve a uniquely complete and detailed negative carbon isotope excursion (CIE) in an expanded section of several hundred metres. •  Position of CIE in the early Danian, ca. 200ka above K/Pg –  Correlates with Dan-C2 CIE in marine record –  Early Danian Hyperthermal Event •  Changes in floral communities through the CIE reflect changing biomes caused by rapidly warming climate, followed by recovery –  EDH event had a similar duration to the Toarcian and Paleocene/Eocene events •  Temporal correlation EDH event with late stages of Deccan Continental Flood basalt province, and initiation of rifting –  Deccan province: cause of global warming and the carbon-isotope excursion •  A high resolution record that is potentially resolving the effect of Chicxulub from the effects of Deccan •  High resolution/stratigraphically complete records have implications…

Editor's Notes

  1. Normapolles is an extinct morphogenus of Late Cretaceous/Early Danian pollen grain – defines the normapolles palynofloral province.
  2. communities in early succession will be dominated by fast-growing, well dispersed species – “early colonisers”
  3. Note – decrease in humid warm temperate flora at base of section marked by Pteridophyta – fernsWinterwet best characterised by Normapolles group – these continue the pre K/Pg regional ‘Normapolles Province’ flora and are meditteranean type winterwet flora. Note absence of humid taxa like Cupressaceae (swamp cypresses) and fernsRecovers to cool temperate flora. This is most like a pine and myrtle moor.
  4. Last Deccan stages Ar/Ar dated as early Danian