the heat loss of the earth claude jaupart jean-claude mareschal stéphane labrosse institut de...
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THE HEAT LOSSOF
THE EARTH
Claude JaupartJean-Claude Mareschal
Stéphane Labrosse
Institut de Physique du Globede Paris
SECULAR COOLING EQUATION
M Cp = - ∫ qr dA + ∫ H dV + ∫ dV
= - heat loss + internal heat production+ external energy tranfers (ex: tidal interaction)
Note (1) : negligible contribution of contraction,zero contribution of dissipation
Note (2) : external energy transfers are negligible
dTdt
AIMS
(1) Evaluate heat loss and uncertainty(2) Constraints on secular cooling
(3) Breakdown between core and mantle
k TmQ = √ t
Cooling model(based on boundary layer theory,
consistent with laboratory experiments and numerical simulations)
Tm = mid-ocean ridge temperaturek, = thermal conductivity, diffusivity t = age
Check no.1 = depth variations of the ocean floor(contraction due to cooling)
Check no.2 = temperature at mid-ocean ridges
Tm = 1350 ± 50 °C consistent with basalt composition
k TmQ = √ t
OCEANIC HEAT LOSS = 32 ± 2 TW(includes contributions from “hot spots” (mantle
plumes)Main uncertainty :time-variations of age distribution
CRUSTEnriched in U, Th and K
Lithospheric mantle(rigid root)
Radiogenic heat productionin continental lithosphere
Qs = Qc + QLM + Qb
Qc
QLM
Basal heat flux Qb
Scale (Q) (Q) N
CANADIAN SHIELDAll values 40.6 8.9 31650 km 39.8 8.8250 km 39.5 7.3500 km 39.9 4.3
Continental Heat FlowAveraging over different scales (windows)
Scale (Q) (Q) N
CANADIAN SHIELDAll values 40.6 8.9 31650 km 39.8 8.8250 km 39.5 7.3500 km 39.9 4.3
WORLDAll values 79.7 162 141231°x 1° (≈100 km) 65.3 822°x 2° 64.0 575°x 5° 63.3 35
Continental Heat FlowAveraging over different scales (windows)
From Abbott et al. (1994)
Earth’s secular cooling rate
From the composition of mid-ocean ridge basaltsand similar magmas
(1) Assume same secular cooling rate than the mantle.Accounting for latent heat release and potential energychange due to crystallization:
2 - 6 TW
(2) Use magnetic field intensity and dynamo efficiency.
5 - 10 TW
CORE HEAT LOSS2 methods
(Upper bound preferred becauseof constraints on boundary layerat the core-mantle boundary)
M Cp = - ∫ qr dA + ∫ H dV
Secular cooling rate ≈ 25 - 75 K Gy-1 ≈ 4 - 12 TW (for mantle + crust)
Present-day crust + mantle heat loss= surface heat loss - heating from the core
≈ 33 - 44 TW
Bulk Silicate Earth (BSE) radiogenic heat production≈ 21 - 41 TW
dTdt
Bulk Silicate Earth (BSE) radiogenic heat production≈ 21 - 41 TW
Mean Uranium concentration(assuming chondritic Th/U and K/U)
≈ 0.022 - 0.044 ppm
CRUSTEnriched in U, Th and K
Lithospheric mantle(rigid root)
Radiogenic heat productionin continental lithosphere
Qs = Qc + QLM + Qb
Qc
QLM
Basal heat flux Qb
BSE radiogenic heat production≈ 21 - 41 TW
Heat production in continental crust (+ lithos. mantle)≈ 6 - 8 TW
Internal heat generation for mantle convection≈ 13 - 35 TW