Ka. Farley et al., HE, SR AND ND ISOTOPIC VARIATIONS IN LAVAS FROM THE JUAN-FERNANDEZ ARCHIPELAGO, SE PACIFIC, Contributions to Mineralogy and Petrology, 115(1), 1993, pp. 75-87
Helium. Sr, and Nd isotopic ratios and major and trace element composi
tions have been measured on a suite of lavas from the intra-plate volc
anos of the Juan Fernandez Archipelago, Chile. Lavas from the islands
of Mas Afuera and Mas a Tierra and from Monte Alpha and Friday seamoun
ts have Sr and Nd isotopic ratios lying on the low Nd-143/Nd-144 side
of the mantle array (Sr-87/Sr-86: 0.7034-0.7037; Nd-143/Nd-144:0.51281
-0.51289). The homogeneity of these tracers suggests the involvement o
f a restricted range of mantle source compositions throughout Juan Fer
nandez volcanism. In marked contrast is the large range in He-3/He-4,
from 7.8 to 18.0 R(A). A bimodal He-3/He-4 distribution on Mas a Tierr
a is associated with two distinct volcanic lineages, He-3/He-4 ratios
of 14.5-18.0 R(A) (n = 15) occur in alkalic and tholeiitic shield basa
lts, whereas post-shield basanites range from 11.2 to 13.6 R(A) (n = 1
2). Elemental and isotopic systematics demonstrate a transition from a
n enriched (Loihi-like) plume source in the shield lavas to a more MOR
B-like source in the post-shield volcanics. The transition between the
se sources is much more pronounced in He-3/He-4 than in the other isot
opic tracers. The predominantly tholeiitic basalts of Mas Afuera have
exceptionally uniform isotopic and elemental characteristics; Sr and N
d ratios are similar to those of Mas a Tierra, but He-3/He-4 ratios ar
e lower and more uniform at 8.3 +/- 0.5 R(A) (n = 17). The dramatic di
stinction between Mas Afuera and Mas a Tierra helium is surprising giv
en the great similarity between the two islands in other geochemical c
haracteristics. Both the Mas Afuera and Mas a Tierra results demonstra
te that helium records systematic processes not readily apparent from
other isotopic or elemental indicators. Neither magma chamber degassin
g nor local metasomatic events are likely to be responsible. We sugges
t that the observed variations may be attributed to mixing of plume an
d asthenospheric sources in which the plume component is characterized
by a heterogeneous distribution of volatiles or has suffered extracti
on of small degree partial melts prior to mixing.