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Appendix C: Calculation of initial isotopic compositions and diagrams illustrating alteration effects. Initial isotopic compositions for our samples were calculated using the

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Appendix C: Calculation of initial isotopic compositions and diagrams illustrating alteration effects.

Initial isotopic compositions for our samples were calculated using the 40Ar/39Ar ages determined in this study and an age of 85 Ma is assumed for samples where age data are not available. The reference data were also projected to a common age of 85 Ma to be able to compare them with our data. Exceptions are reference data, which are significantly younger (<50 Ma old) than the samples from the main CLIP phases, namely data of the Galápagos Islands and the younger Galápagos hotspot track. Since melting and differentiation processes can fractionate the parent/daughter ratios of the source, measured ratios cannot be applied to project the isotope ratios of these young rock samples correctly.

Thus we assumed proposed source parent/daughter ratios for average depleted MORB mantle (DMM) from Workman and Hart (2005) for the Atlantic and Pacific MORB fields and for the depleted eastern domain of the Galápagos Islands with the following trace element concentrations in ppm: Pb = 0.018, U = 0.0032, Th = 0.0079, Rb = 0.05, Sr = 7.664, Sm = 0.239, Nd = 0.581, Lu = 0.058, Hf = 0.157. For the three more enriched domains, we used the concentrations in ppm for bulk subducted igneous crust from Stracke et al. (2003): Pb = 0.09, U = 0.027, Th = 0.088, Rb = 0.57, Sr = 81, Sm = 2.69, Nd = 7.45, Lu = 0.45, Hf = 1.78.

For the Galápagos hotspot track, initial isotope ratios were first calculated using measured trace element concentrations and their ages and then projected to 85 Ma using the source parent/daughter ratios from Workman and Hart (2005) for tholeiites and those from Stracke et al. (2003) for alkali basalts.

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Fig. C.1. Initial 87Sr/86Sr versus 143Nd/144Nd diagram. Although many of the samples from the LIP-like and from the depleted group are shifted to higher 87Sr86Sr ratios, the division into the three distinct groups is visible. For the depleted group, Sr isotope data from whole rock samples as well as from plagioclase separates are shown. Data from DSDP Leg 15, Sites 146 and 150-153 are also included (Hauff et al., 2000a). Additionally shown are fields for common CLIP (Hastie et al., 2016; Hastie et al., 2008; Hauff et al., 2000a; Hauff et al., 2000b; Hoernle et al., 2004; White et al., 1999), Hispaniola (Escuder-Viruete et al., 2007;

Lapierre et al., 1999; Lapierre et al., 1997), Tortugal (Hauff et al., 2000b; Trela et al., 2017), ODP Leg 165 Site 1001 (Kerr et al., 2009), depleted samples from the Lower Nicaraguan Rise (LNR; Dürkefälden et al., accepted), Galápagos Islands (Is.) (Blichert‐Toft and White, 2001; White et al., 1993; GEOROC at http://georoc.mpch.gwdg.de/georoc/) and Galápagos hotspot track (Hauff et al., 2000a; Hauff et al., 2000b; Hoernle et al., 2002; Trela et al., 2015) and for Gorgona komatiites, depleted (D-) and enriched (E-)basalts (Aitken and Echeverría, 1984; Révillon et al., 2000; Révillon et al., 2002; Serrano et al., 2011). The Mid-Atlantic and East Pacific Rise (EPR) MORB fields comprise data from the PetDB database (http://www.earthchem.org/petdb). Initial isotopic compositions are calculated at 85 Ma.

Analytical errors are smaller than the symbol size.

(143Nd/144Nd)i

0.5127 0.5128 0.5129 0.5130 0.5131 0.5132

(87Sr/86Sr)i

0.7020 0.7025 0.7030 0.7035 0.7040 0.7045

common CLIP Mid-Atlantic

MORB

EPR MORB

Galápagos Is.

+ hotspot track

Gorgona komatiites

Gorgona D-basalts

Gorgona E-basalts Tortugal Hispaniola

LNR depleted Site 1001

HIMU

EM II

EM I Site 152 (Hess Esc.) Site 151 (Beata Ridge) Sites 146, 150, 153 Beata R. enriched Beata R. depleted Fsp separates Beata R. depleted Beata R. LIP-like

seawater alteration

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Fig. C.2. (a) Initial 206Pb/204Pb versus 208Pb/204Pb and (b) initial 206Pb/204Pb versus 207Pb/204Pb diagrams illustrating that the Pb isotope system is significantly affected by alteration processes. Data sources are the same as in Fig. C.1. Initial isotopic compositions are calculated at 85 Ma. Analytical errors are smaller than the symbol size.

(208Pb/204Pb)i

37.0 37.5 38.0 38.5 39.0 39.5

(206Pb/204Pb)i

17.5 18.0 18.5 19.0 19.5 20.0

HIMU

EM I

common CLIP

Mid-Atlantic MORB EPR MORB

Tortugal

Galápagos Is.

+ hotspot track Gorgona

komatiites

Gorgona D-basalts

Gorgona E-basalts

LNR depleted

Site 1001 Site 152 (Hess Esc.)

Site 151 (Beata R.) Sites 146, 150, 153 Beata R. enriched Beata R. depleted Beata R. LIP-like

(a)

(207Pb/204Pb)i

15.40 15.45 15.50 15.55 15.60 15.65

(206Pb/204Pb)i

17.5 18.0 18.5 19.0 19.5 20.0

EM II HIMU

EM I

common CLIP

Atlantic MORB Mid-

EPR MORB Galápagos Is.

+ hotspot track

Tortugal Gorgona

komatiites

Gorgona

D-basalts Gorgona

E-basalts

LNR depleted Site 1001

(b)

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Fig. C.3. (a) Pb versus Ce/Pb diagram. The gray box shows a Ce/Pb ratio of 25 ± 5, which is typical for MORB and OIB (Hofmann et al., 1986), and the Pb concentrations of samples within this range are assumed to not have been significantly influenced by hydrothermal alteration. A few samples lie above this ratio and have lost Pb, whereas a large number of samples have Ce/Pb ratios lower than 20 and have gained Pb. (b) U versus Nb/U diagram demonstrating that most of the samples from the Beata Ridge are significantly affected by U gain during alteration processes. They lie below the Nb/U ratio of 47 ± 10 typical for MORB and OIB (gray box; Hofmann et al., 1986) and have high U concentrations.

Ce/Pb

0 10 20 30 40 50 60 70 80

Pb [ppm]

0.0 0.5 1.0 1.5 2.0

Ce/Pb = 25 ± 5 Beata Ridge enriched Beata Ridge depleted Beata Ridge LIP-like

Pb gain Pb loss

(a)

Nb/U

0 10 20 30 40 50 60 70

U [ppm]

0.0 0.5 1.0 1.5 2.0

Nb/U = 47 ± 10

(b)

U gain U loss

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Abbildung

Fig. C.1. Initial  87 Sr/ 86 Sr versus  143 Nd/ 144 Nd diagram. Although many of the samples from the  LIP-like and from the depleted group are shifted to higher  87 Sr 86 Sr ratios, the division into the  three  distinct  groups  is  visible
Fig. C.2. (a) Initial  206 Pb/ 204 Pb versus  208 Pb/ 204 Pb and (b) initial  206 Pb/ 204 Pb versus  207 Pb/ 204 Pb  diagrams  illustrating  that  the  Pb  isotope  system  is  significantly  affected  by  alteration  processes
Fig. C.3. (a) Pb versus Ce/Pb diagram. The gray box shows a Ce/Pb ratio of 25 ± 5, which is  typical  for  MORB  and  OIB  (Hofmann  et  al.,  1986),  and  the  Pb  concentrations  of  samples  within  this  range  are  assumed  to  not  have  been  signif

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