the role of marine plankton in the global climate bas kooijman dept theoretical biology climate...
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The role of marine plankton in the global climate
Bas KooijmanDept Theoretical Biologyhttp://www.bio.vu.nl/thb/
Climate Center Vrije Universiteit
Tuesday 15 Oct 2002
Biogeochemo- research by Theor Biol VUA
Past projects:Global Emiliania Modelling Initiative (GEM) Peter Westbroek (RUL) & Jan van Hinte (VUA)Mast II: European program NOP II: VUA: modelling nutrient limited growth (Kooijman, Zonneveld) RUL: molecular aspects (Westbroek, Corstjens) NIOZ: growth experiments (Riegman) RUG: DMS (Gieskes, van Rijssel)
Current projects:Stochiometric contraints in producer/consumer interactions Kuijper, Kooi, Kooijman, Andersen (Southampton)Time scale separation in producer/consumer interactions Kooi, Kooijman, Auger (Lyon), Poggiale (Marseille)Primary production in ocean circulation models Kooijman, Kooi, Dijkstra (IMAU)Self organisation of trophic structures in ecosystems Troost, Kooi, Kooijman, Metz (RUL), Loreau (Paris)
Dynamic Energy Budget theoryfor metabolic organisation of all life on earth• first principles• quantitative
Biological equivalent of Theoretical Physics• biogeochemical perspective
Primary target: the individual with consequences for• sub-organismal organization• supra-organismal organization
Relationships between levels of organisation
Practical applications: direct links with empiry• ecotoxicology• biotechnology• medicine/ health care
DEB info athttp://www.bio.vu.nl/thb/deb/
Climate affects marine plankton
• temperature affects all physiological rates• nutrient supply via erosion from terrestrial systems water cycle ocean circulation (wind forcing, plate tectonics) wind-induced primary production• light availability (albedo)
Climate change induces extinction and speciation in combination with biotic factors (competition)
Marine plankton affects climate
• organic carbon pump transport of atmospheric CO2 to deep ocean (1000 year memory) linked to nutrient cycling, terrestrial ecosystems• calcification (inorganic carbon pump) precipitation of CO2 in CaCO3 burial by plate tectonics
• albedo emission of DMS cloud formation, effects on radiation
Half rules:Half of evaporation is from land (plants compensate land/sea difference)Half of present primary production is from marine plankton Half of carbonate precipitation is by reefs (corals), the rest by plankton (forams and coccolithophores)
Rates depend on temperature
Arrhenius plot for the population growth rate of E. coliData Heredeen et al 1979
low and high temperature inactive state of catalysator
103/T, K-1
ln p
op. g
row
th r
ate,
h-1
Arrhenius temperatures Lower 20110 K Midrange 4370 K Upper 69490 K
Tolerance range 293 – 318 K
Rock cycle
SiO2 + CaCO3
CO2 + CaSiO3H4SiO4 + 2 HCO3
- + Ca++
2 CO2 + 3 H2O
weathering
burialsedimentation
out gassing
Photosynthesis: H2O + CO2 + light CH2O + O2
Fossilisation: CH2O C + H2OBurning: C + O2 CO2
Calcification: 2HCO3- + Ca++ CaCO3 + CO2 + H2O
Silification: H4SiO4 SiO2 + 2H2O
pH of seawater = 8.398 % DIC = HCO3
- not available to most org.
evaporationraining
After Peter Westbroek
CalcificationOriginal hypothesis:E.huxleyi uses bicarbonate assupplementary DIC source;CO2 might be growth limiting
However:non-calcifying strains have similar max growth rate
New hypothesis:carbonate is used for protection against grazing
Emiliania huxleyi
Nutrients from rocks to plankton by plants + micro’s
Plants started to explore the terrestrial environment in the Silurian closed vegetations during DevonianFilter-feeding reefs flourished during the Silurian and Devonian
Hypotheses:• reefs developed in presence of plankton • nutrients released by plants from rocks entered oceans and stimulated plankton growth• followed by a reduction due to the formation of Pangaea
landscape lower Devonian
reef upper Devonian
Growth on reserve
Opt
ical
Den
sity
at 5
40 n
m
Con
c. p
otas
sium
, mM
Potassium limited growth of E. coli at 30 CData Mulder 1988; DEB predictions fitted
OD increases by factor 4 during nutrient starvationinternal reserve fuels 9 hours of growth
time, h
Organic carbon pumpWind: weak moderate strong
light + CO2
“warm”no nutrients
coldnutrientsno light
readily degradable
poorly degradable
no growth growth poor growthbloom
producersbind CO2
from atmosphereand transport
organic carbonto deep ocean
recovery ofnutrients tophoto-zone
controls pump
Grazing accelerates exportcopepods tintinnids
appendicularians
Fecal pellets sink fast most nutrients remain in photo-zoneAppendicularians produce marine snow (1 feeding house/ 2 hours)Dead bodies decompose fast
Synthesizing Unit
dots: arrival and production events
gray areas: periods blocked for binding
11111 BABACmC jjjjjjFlux C:
transformation: 1 A + 1 B 1 C
Simultaneous nutrient limitation
Specific growth rate of Pavlova lutheri as function of intracellular phosphorus and vitamin B12 at 20 ºC
Data from Droop 1974; SU-based DEB model fitted
P content, fmol/cell
B12 content,
10 -21 mol/cell
Conclusions:• SU-based model fits well• biomass composition varies considerably
• no high P-high B12
due to damming up• uptake of abundant nutrient is not reduced by rare one• composition control by excretion• growth limiting reserve increases with growth rate, other reserves can decrease
C,N,P-limitation
Nannochloropsis gaditana (Eugstimatophyta) in sea waterData from Carmen Garrido PerezReductions by factor 1/3 starting from 24.7 mM NO3, 1.99 mM PO4
CO2 HCO3- CO2 ingestion only
No maintenance, full excretion
N,P reductions N reductions
P reductions
79.5 h-1
0.73 h-1
C,N,P-limitation
half-saturation parameters KC = 1.810 mM for uptake of CO2
KN = 3.186 mM for uptake of NO3
KP = 0.905 mM for uptake of PO4
max. specific uptake rate parameters jCm = 0.046 mM/OD.h, spec uptake of CO2
jNm = 0.080 mM/OD.h, spec uptake of NO3
jPm = 0.025 mM/OD.h, spec uptake of PO4
reserve turnover rate kE = 0.034 h-1
yield coefficients yCV = 0.218 mM/OD, from C-res. to structure yNV = 2.261 mM/OD, from N-res. to structure yPV = 0.159 mM/OD, from P-res. to structure
carbon species exchange rate (fixed) kBC = 0.729 h-1 from HCO3
- to CO2
kCB = 79.5 h-1 from CO2 to HCO3-
initial conditions (fixed) HCO3
- (0) = 1.89534 mM, initial HCO3- concentration
CO2(0) = 0.02038 mM, initial CO2 concentration
mC(0) = jCm/ kE mM/OD, initial C-reserve density mN(0) = jNm/ kE mM/OD, initial N-reserve density mP(0) = jPm/ kE mM/OD, initial P-reserve density
OD(0) = 0.210 initial biomass (free)
Nannochloropsis gaditana in sea water
Producer/consumer stoichiometry
CjPrPdt
dPAP
ChrCdt
dC )(
NNP
NNP my
mkr
PK
Pjj Pm
PA
1111 CNCPCNCPC rrrrr
MPPACPCP kjyr MNPANCNCN kjmyr
consumer producer reserve density of producer
total nutrient (constant)
no free nutrientno -maintenanceno -reserve
CPC rr
N
PC
Nm
no need for reserve need for reserve
PmnN NNP CnNC
CPC rr
CP
Bifurcation diagramsby Bob Kooi
Diauxic growth
time, h
biom
ass
conc
., O
D43
3 acetate
oxalate
Sub
stra
te c
onc.
, mM
Growth of acetate-adapted Pseudomonas oxalaticus OX1data from Dijkhuizen et al 1980
SU-based DEB curves fitted by Bernd Brandt
Adaptation todifferent substratesis controlled by:
enzyme turnover 0.15 h-1
preference ratio 0.5
cells
Diauxic growthbi
omas
s co
nc.,
OD
590
Growth of succinate-adapted Azospirillum brasilenseintracellular amounts followed with radio labels
data from Mukherjee & Ghosh 1987SU-based DEB curves fitted by Bernd Brandt
Adaptation todifferent substratesis controlled by:
enzyme turnover 0.7 h-1
preference ratio 0.8
time, h
fruc
tose
con
c, m
M
succ
inat
e co
nc, m
M
succinate
fructose cells
suc in cells
fruc in cells
1-species mixotroph communityMixotrophs areproducers, which live off light and nutrientsas well asdecomposers, which live off organic compounds which they produce by aging
Simplest community with full material cycling
1-species mixotroph communityCumulative amounts in a closed community as function of total C, N, light
E: reserveV: structureDE: reserve-detritusDV: structure-detritusrest: DIC or DIN
Note: absolute amountof detritus is constant
Canonical communityShort time scale:Mass recycling in a community closed for mass open for energy
Long time scale:Nutrients leaks and influxes
Memory is controlled by life span (links to body size)Spatial coherence is controlled by transport (links to body size)
Self organisation ofecosystems’ trophic structure
Aim:• understand ecosystem dynamics future application in planetary modelling of life’s actions• characterize functional aspects, and link to structure effects of total nutrient amounts and light
Method:• all organisms in closed ecosystem follow DEB rules constant parameters for each individual during life span• food preference parameters values diffuse across generations• extensive parameters co-diffuse across generations body size scaling relationships for life histories• start with one single mixotroph in well-mixed closed system• use theory for adaptive dynamics to understand speciation
Some conclusions• simultaneous nutrient limitations on producers’ growth is well captured by DEB theory based on SU’s• surface area/volume interactions dominate (transport) kinetics on all space/time scales and are basic to DEB theory• wind is in proximate control of primary production in oceans• rate of organic carbon pump is controlled by nutrient recycling factors: sinking, decomposition, grazing• need for clear time scale separation organic carbon pump is only of interest on time scale of ocean turnover calcification is important at longer time scales plants reduce erosion on short time scale, increase it on long time scale• long term behaviour of ecosystems is controlled by leaks and inputs of nutrients, with important roles for continental drift and vulcanism• climate-life interactions can only be understood in a holistic perspective coupling of biogeochemical cycles with climate (water, heat)
Further readingS. A. L. M. Kooijman 2002 Global aspects of metabolism; on the coevolution of life and its environment. In: J. Miller, P. J. Boston, S. H. Schneider and E. Crist, eds., Scientists on Gaia. MIT Press, , Cambridge, Mass., to appear.
Downloadable from: http://www.bio.vu.nl/thb/research/bib/Kooy2002a.htmlFrom which you can also download this slide collection
Thank you for your attention