ELSEVIER
Tectonophysics 236 (1994) 465-483
The East African rift system in the light of KRISP 90
G.R. Keller a, C. Prodehl b, J. Mechie b,l, K. Fuchs b, M.A. Khan ‘, P.K.H. Maguire ‘,
W.D. Mooney d, U. Achauer e, P.M. Davis f, R.P. Meyer g, L.W. Braile h,
1.0. Nyambok i, G.A. Thompson J
aDepartment
zyxwvutsrqponmlkjihgfedcbaZYXWVUTSRQPONMLKJIHGFEDCBA
of Geological Sciences, University of Texas at El Paso, El Paso, TX 79968-0555, USA
b Geophy sikalisches Institut, Universitdt Karlwuhe, Hertzstrasse 16, D- 76187Karlsruhe,
’ Department of Geology , University of Leicester, University Road, Leicester LEl
Germany
7RH, UK
d U.S. Geological Survey, O ffice of Earthquake Research, 345 M iddlefield Road, M enlo Park, CA 94025, USA
’ Institut de Phy sique du Globe, Universite’ de Strasbourg, 5 Rue Ret& Descartes, F- 67084 Strasbourg, France
‘Department
of Earth and Space Sciences, University of California at Los Angeles, Los Angeles, CA 90024, USA
’ Department of Geology and Geophy sics, University of W uconsin at M adison, M adison, W I 53706, USA
h Department of Earth and Atmospheric Sciences, Purdue University , W est Lafay ette, IN 47907, USA
i Department of Geology , University of Nairobi, P.O. Box 14576, Nairobi, Kenya
’ Department of Geophy sics, Stanford University , Stanford, CA 94305, USA
Received 21 September 1992; accepted 8 November 1993 zyxwvutsrqponmlkjihgfedcbaZYXWVU
Abstract
On the basis of a test experiment in 1985 (KRISP 85) an integrated seismic-refraction/
teleseismic survey (KRISP
90) was undertaken to study the deep structure beneath the Kenya rift down to depths of NO-150 km. This paper
summarizes the highlights of KRISP 90 as reported in this volume and discusses their broad implications as well as
the structure of the Kenya rift in the general framework of other continental rifts. Major scientific goals of this phase
of KRISP were to reveal the detailed crustal and upper mantle structure under the Kenya rift, to study the
relationship between mantle updoming and the development of sedimentary basins and other shallow structures
within the rift, to understand the role of the Kenya rift within the Afro-Arabian
rift system and within a global
perspective, and to elucidate fundamental questions such as the mode and mechanism of continental rifting.
The KRISP results clearly demonstrate that the Kenya rift is associated with sharply defined lithospheric thinning
and very low upper mantle velocities down to depths of over 150 km. In the south-central portion af the rift, the
lithospheric mantle has been thinned much more than the crust. To the north, high-velocity layers detected in the
upper mantle appear to require the presence of anistropy in the form of the alignment of olivine crystals. Major axial
variations in structure were also discovered, which correlate very well with variations in the amount of extension, the
physiographic width of the rift valley, the regional topography, and the regional gravity anomalies. Similar
relationships are particularly well documented in the Rio Grande rift.
To the extent that truly comparable data sets are available, the Kenya rift shares many features with other rift
zones. For example, crustal structure under the Kenya, Rio Grande, and Baikal rifts and the Rhine Graben is
generally symmetrically centered on the rift valleys. However, the Kenya rift is distinctive, but not unique, in terms of
the amount of volcanism. This volcanic activity would suggest large-scale modification of the crust by magmatism.
’ Present address: GeoForschungsZentrum,
Telegrafenberg
A3, D-14407 Potsdam, Germany.
0040-1951/94/$07.00 0 1994 Elsevier Science B.V. All rights reserved
SSDI 0040-1951(94)00046-C
466
G. R. h’dler et al / Tectonophysrcs
236 (1994) 46S -4%~
Although there is evidence of underplating
in the form of a relatively high-velocity lower crustal layer, there are no
major seismic velocity anomalies in the middle and upper crust which would suggest pervasive magrnatism. This
apparent lack of major modification is an enigma which requires further study. zyxwvutsrqponmlkjihgfedcbaZYXWVUTSR
1. introduction
As is described in detail by Swain et al. (1994),
the Kenya Rift International
Seismic Project
(KRISP) started in 1968 as a largely British effort
and has culminated to date with the large, integrated seismic investigations of KRISP 85 (KRISP
Working Group, 1987; Khan et al., 1989; Henry
et al., 1990; Achauer, 1990; Green et al., 1991)
and KRISP 89-90 (KRISP Working Group, 1991;
KRISP Working Party, 1991; Keller et al., 1992;
Achauer et al., 1992) whose results have been
described in detail in this volume. The purpose of
this contribution is to summarize the results of
the individual studies of the various seismic refraction/ wide-angle reflection lines (Gajewski et
al., 1994; Mechie et al., 1994a; Keller et al., 1994;
Maguire et al., 1994; Braile et al., 1994; Prodehl
investigations
et al., 1994) and teleseismic
(Achauer et al., 1994; Slack and Davis, 1994;
Ritter and Achauer, 1994), analyze these results
within the larger perspective of the East African
rift system, and evaluate their implications for
our understanding of continental rifting in general. We will also point out key questions which
we believe need to be addressed in future studies.
2. Lithospheric structure of the Kenya rift and its
implications
An index map of the KRISP teleseismic networks and explosion profiles is shown in Fig. 1. In
order to facilitate the comparison of these results,
a fence diagram showing the velocity models obtained is shown in Fig. 2. The new picture of
crustal structure obtained from the KRISP effort
was combined with previous results to revise the
contour map of crustal thickness constructed by
Keller at al. (1991). Previous results from the
Kaptagat and Ngurunit areas indicated a crustal
thickness of just over 40 km under portions of the
rift flanks (Maguire and Long, 1976; Pointing and
Maguire, 1990). In addition, studies of teleseismic
waveforms recorded at Nairobi (Bonjer et al.,
1970; Herbert and Langston, 1985) indicated a
crustal thickness of about 40 km which is consistent with recent xenolith data (Henjes-Kunst and
Altherr, 1992). These xenolith data indicate a
systematic crustal thickening along the eastern
flank of the rift valley from 33 km near Marsabit
in northeastern Kenya to 42 km under the Chyulu
Hills in southeastern Kenya (Fig. 3). Finally, seismic reflection and gravity data in the Anza rift
(Fig. 1) also suggest crustal thinning in northeastern Kenya (Greene et al., 1991; Dindi, 1994). The
revised crustal thickness map is shown in Fig. 3.
In the vicinity of the rift, the structure in the
south near Tanzania is poorly constrained. Away
from the rift, particularly in eastern Kenya, the
only control is the intuitive interpretation that the
crust thins towards the coast and continental
margin.
In terms of crustal structure, the most significant discovery from KRISP 89-90 was that the
crustal thickness along the rift axis varies from as
little as 20 km beneath Lake Turkana to about 35
km under the culmination of the Kenya dome
near Lake Naivasha (Fig. 3). The transition in
crustal thickness occurs over a horizontal distance of about 150 km (Fig. 3) between Lokori
(LKO) and Lake Baring0 (BAR) and thus the
discrepancy between the model of Henry et al.
(1990) and the tentative model of Griffiths et al.
(1971) has been resolved. The change in crustal
thickness along the rift is accomplished by thinning of all layers, but especially by the thinning of
the lowermost crustal layer. The seismic data
agree very well with the north to south increase
in Bouguer gravity anomaly values (Survey of
Kenya, 1982; Swain and Khan, 1978). The area of
thickest crust correlates with the apex of the
Kenya dome where the elevation of the rift valley
floor is highest. As one proceeds northward along
the rift valley from the Lake Naivasha area, the
physiographic expression of the rift valley widens
from its minimum of about 60 km to about 180
G.R. Keller et al. / Tec~o~~hys~~ 236 (1994) 465-483
km in the area of thinnest crust (Fig. 1). In
addition to these obse~ations, recent seismic reflection results near Lake Turkana (Morley et al.,
1992; Morley, 1994) indicate that the amount of
extension across the rift increases from about
5-10 km in the Naivasha-Nakuru
region (Baker
and Wohlenberg, 1971; Strecker, 1991; Strecker
and Bosworth, 1991) to about 35-40 km in the
467
Lake Turkana area (Morley et al., 1992; Hendrie
et al., 1994). The limited KRISP data south of
Lake Naivasha suggest that there may be a decrease in crustal thickness southwards along the
rift valley towards Lake Magadi. However, the
need for additional data in the southern portion
of the rift can be identified as a result of KRISP
89-90.
4.c
2x
OX
2.0’
36.0°
38.0”
Fig. 1. KRISP 90 location map showing the seismic refraction/ wide-angle reflection lines and the configuration oft the teleseismic
networks in 1985 and 1989-1990. The 1985 refraction/wide-angle
reflection lines extended from Lake Baring0 tb Lake Magadi
and across the rift valley just north of the Susua volcano.
CLR. K&r ct ul / lectonophysrcs 236 (IYY4/ 465-383
Fig. 2. Fence diagram showing crustal and upset-mantle
structure of the Kenya rift from Lake Turkana to Lake Naivasha and
beneath the neighboring flanks from Lake Victoria to Archers Post. P-wave velocities are shown in km/s. Also shown are relative
velocity variations from teleseismic delay time studies across the rift at 15 (Achauer et al., 1994). For more detailed velocity
information for the crustal sections 071, VW, and IX), see corresponding cross-sections in enlarged form in individual papers of
this vohrme (profile i/E Mechie et al., 199% profife VIZi: Maguire et al., 1994; Braiie et al., 1994; profiie IX: Prodehl et &, 1994).
Teteseismic vetocity perturbations are contoured at 1% intervals and shaded at 2% intervals. Slow ~rtu~tioas
are light cohntred,
fast perturbations are dark coloured.
G.R. Kelleret al. / Tectompty sics 236 (1994) 465- 483
Another interesting aspect of the crustal structure is that both Maguire et al. (1994) and Braile
et al. (1994) show the thickest crust (almost 40
km) beneath the western flank to occur immediately adjacent to the rift valley. Normal continental uppermost mantle velocities of 8.0-8.2 km/s
are also found under the flanks. These values of
crustal thickness and upper mantle velocity are
consistent with the result obtained from the Kaptagat seismic array by Maguire and Long (19761.
Beneath the eastern flank, the model of Braile et
al. (1994) shows the thickest crust occurring immediately adjacent to the rift valley, while the
model of Maguire et al. (1994) shows the thickest
469
crust occurring somewhat more to the east. Nevertheless, on this cross-section the thickest crust
beneath both flanks occurs close to the rift.
Maguire et al. (1994) have suggested that if this
crustal thickening had been present before the
rifting started then it could have influenced the
position of the rift according to the model of
Vink et al. (1984). In this model, rifting tends to
occur where the crust is thickest as this creates an
overall weaker lithosphere because it contains a
higher proportion of weaker minerals (e.g., quartz
and feldspar) which are dominant in the crust
and a lower proportion of stronger minerals (e.g.,
olivine) which are dominant in the mantle. Braile
Fig. 3. Crustal thickness map for the Kenya rift region. The contour interval is 5 km. BAR, NAZ,CHF, and LKO iddntify shotpoints
at Lake Baringo, Lake Naivasha, Chanler’s Falls, and Lokori, respectively. MAR and CHY indicate estimates of chustai thickness
from xenoliths from the Marsabit and Chyulu Hills areas, respectively.
et al. (19941, on the other hand, suggest that this
crustal thickening, which is also manifested by
the isostatic effect of rift shoulder uplift, is the
result of intrusion/ underplating. Of course, the
thickening may partly have existed prior to the
rift initiation and may be partly due to lower
crustal intrusion during rifting isostatically balancing the shoulrler uplift. A seismic profile across
the rift where little or no shoulder uplift is observed may help to solve the question of to what
extent was the crust thicker before rifting began
and to what extent has it been thickened below
the shoulders due to the rifting process.
East of the eastern flank, the crust thins again
to about 33-34 km in the vicinity of Chanler’s
Falls (Fig. 3). ~though Quaterna~ volcanism is
observed in the area, the influence of the Mesozoic to Early Tertiary Anza rift (Fig. 1) in northeastern Kenya (Greene et al., 1991; Bosworth and
Morley, 1994; Dindi, 1994) may play some role in
this off-rift crustal thinning. Nevertheless, the
flank profile lies between the Anza rift and the
Kenya rift south of Lake Turkana; thus, we can
conclude that the crustal thinning along the Kenya
rift with respect to that beneath the flank line
must have been caused by the late Cenozoic
rifting episode.
Tbe rift infill thickness along the axial and
cross-rift profiles is generally 3-5 km. However,
large variations occur. For example, the rift infill
is zero where Precambrian crystalline basement is
exposed on the crests of steeply tilted fault blocks.
On the other hand, the rift infill thickness approaches 10 km in the deepest part of the Elgeyo
basin at the foot of the Elgeyo escarpment along
the cross-rift profile (Fig. 1). The effect of the
well documented basins in the Lake Turkana
region (Morley et al., 1992; Hendrie et al., 1994)
can also be recognized on a band-pass filtered
(15-125 km) residual gravity anomaly map in
which they are associated with local minima of
some tens of milligals. Within the crystalline crust,
three principal layers can be recognized (Fig. 2).
The top of the upper crystalline crust generally
has velocities of 6.0-6.3 km/s. However, “blocks”
or “layers” with velocities about 0.2 km/s greater
than the average background values have been
recognized. Examples are found within the upper
crystalline crust beneath the rift flanks on the
cross-rift and flank profiles (Maguire et al., 1994:
Prodehl et al., 1994) and within the crystalline
crust beneath the central part of the rift vailey
itself (Ritter and Achauer, 1994). These highvelocity zones may represent regions which have
experienced significant amounts of mafic intrusive activity. Individual intrusions, most probably
dikes, would be too small to be detected by the
KRISP data. However, enough of them could
raise the average velocity and density of a region
of the upper crust enough to be detected. Swain
f 1992) has made a similar argument in his interpretation of the source of part of the axial gravity
high along the rift.
The top of the lower crust is marked by a jump
in velocity up to 6.4-6.6 km/s, and the depth to
the top of the lower crust varies from 9 to 18 km.
Shallower depths are encountered beneath the
northern part of the rift valley where extension
has been the greatest and beneath the flank profile. The basal 2-10 km of the lower crust is
marked by higher velocities generally in the range
of 6.7-6.9 km/s. The inversion analysis of Braile
et al. (1994) shows that the highest velocities in
this basal layer may be restricted to the rift valley
region. Beneath the Nyanza craton (Fig. 11, the
top of this basal crustal layer is a good reflector.
Beneath the Mozambique belt, there is no reflection from the top of this basal layer except within
the southern part of the rift valley. Beneath the
northern part of the rift valley, this basal layer is
too thin for the reflection from it to be distinguished from the reflection from the crust-mantle boundary (Moho), and it is represented as a 2
km thick crust-mantle
transition zone beneath
the northernmost 100 km of the axial profile (Fig.
2). However, the continuity of this layer from
south to north, while convenient for the computer
modeling, may not be real.
Crustal velocities within the rift valley itself
are not significantly different from those beneath
the rift flanks. Thus, it would appear that the
expected lowering of seismic velocity due to increased temperature beneath the rift is either
masked by pre-rift compositional variations or is
compensated for by intrusion of mafic material
into the crust beneath the rift itself. Crustaf thin-
GA. Keller ei al. / Tectonophysics 236 (1994) 465-483
ning across the rift is accomplished by thinning of
both the upper and lower crusts beneath the rift
valley. Along the rift, the thinning is most pronounced in the basal - 6.8 km/s layer, and as
mentioned above, it may disappear altogether
beneath the Lake Turkana area.
While the teleseismic tomography is not able
to provide a detailed picture of the crustal velocity-depth distribution it nevertheless (in contrast
to the refraction profiles) provides a long-wavelength, 3D velocity image sampling the depth
range from 10 to 35 km (Achauer et al., 1994) for
the central portion of the rift and neighboring
areas. In contrast to the less extensive observations of Green et al. (19911, the most recent
results (Achauer et al., 1994) suggest that, for the
southern section of the rift, the velocities of the
middle and lower crust within the rift are similar
to, and in some places slightly lower (l-3%) than,
those of the adjacent shoulders. Only in the north
near Lake Baring0 and in the south near Mt.
Susua does there seem to be some spots of higher
velocities in the lower crust. As pointed out by
Achauer et al. (1994), it is stretching the resolution of these data to make definitive statements
about crustal structure. I-Iowever, we can conclude that the teleseismic data show no evidence
for wholesale intrusion of mafic material in the
crust.
The entire lithosphere was the target of KFUSP
89-90, and good data concerning mantle structures were obtained in both the explosion and
teleseismic portions of the experiment. Arrivals
from two, at least somewhat, continuous seismic
discontinuities were observed in the data from
the long profiles extending along and across the
rift (Keller et al., 1994; Maguire et al., 1994) and
the teleseismic data provided a 3D picture of
velocity variations down to depths of about 165
km (Achauer et al., 1994; Slack and Davis, 1994).
Beneath the northern part of the axial profile,
two upper mantle high-vel~i~
layers separated
by a low-velocity zone have been identified. The
upper of these two layers, at 40-45 km depth, has
a velocity of 8.05-8.15 km/s and a thickness of at
least 8 km. Below the low-velocity zone which has
an average velocity of 7.9 km/s, the lower of the
two high-velocity layers, at 60-65 km depth, has a
471
velocity of about 8.3 km/s. Beneath the southern
part of the axial profile, the upper mantle is
characterized by velocities of 7.5-7.6 km/s down
to about 60 km depth where the velocity increases to about 7.7-7.8 km/s. Beneath the
cross-rift profile, upper mantle reflectors at about
55 km depth have been identified beneath both
rift flanks while beneath the flank line an upper
mantle reflection at 45-48 km depth has been
recognized.
The teleseismic results (Achauer et al., 1994;
Slack and Davis, 1994) indicate that below the
southern part of the Kenya rift, a low-velocity
body exists which extends from the Moho down
to a depth of at least 165 km. For the uppermost
mantle (35-65 km depth) the lateral extent of this
low-velocity body appears to be similar to that of
the surface expression of the rift. The overall
shape of the low-vel~i~ body is that of a steepsided wedge of low-velocity material which is
more or less confined to the rift and its western
prolongation, the Nyanza trough (Fig. 11, and
which only broadens at depths greater than 125
km. Within this generally N-S-trending wedge of
lower-velocity material, there is a NW-SE lineation along the direction of the old Aswa shear
zone of Pan-African age (Nandi fault, Fig. 1).
Both trends are most pronounced in the depth
range of 65-95 km, but are also visible at other
depth ranges. Velocity contrasts in the upper
mantle beneath the rift and its flanks are generally about 6-lo%, but reach a maximum of up to
12% for some small pockets. The strong variation
of velocities even within the low-velocity body
reflects either areas with quite large differences
in temperature or pockets which contain a somewhat larger fraction of partial melt.
At first glance, the models of crustal and upper mantle structure across the rift are similar to
those earlier drawn as schematic cross-sections of
rifts (e.g., Baker and Wohlenberg, 1971). However, in both the teleseismic and explosion results, the abruptness of the variations from the
rift flanks to the rift valley region are surprising.
This abruptness is particularly evident in the teleseismic results which are from depths where the
diffusion of heat would be expecte(l to produce
broader velocity anomalies. A wide variety of
western branches of the rift are so different in
terms of volcanism. The volumes of surface volcanics differ by as much as a factor of 100 and the
chemistry of the extrusives varies considerably
(e.g., Williams, 1982). At present, we are unable
to discern if these dissimilarities are due to variations in the mechanism of rifting or if they are
simply the result of the response of different
pre-rift lithospheric structures.
Bram (1975) gathered data from earthquakes
to compile two refraction “profiles” for the western rift region (Fig. 4). These sections show some
evidence of crustal thinning beneath the western
rift valley and show rift flank crustal structures
similar to those observed in Kenya. However,
there is not enough information to draw detailed
comparisons on such points as the nature of the
transition from rift valley to flank or axial variations in structure.
Much more information is available in the
Ethiopian-Afar
section of the rift system (Ruegg,
1975; Berckhemer et al., 1975). These results
have been synthesized by Makris and Ginzburg
(1987) and Prodehl and Mechie (19911, and some
interesting comparisons with Kenya are evident.
Like the Kenya rift, the crust and uppermost
mantle of the Ethiopian plateau appears to be
similar to that of shield areas, the transition to
rifted crust appears to be abrupt, and uppermost
mantle velocities under rifted areas are low ( < 7.8
km/s). Unlike Kenya, the crust of the Afar has
little similarity to that of typical continental areas. A very thin sialic (V, = 6.1 to 6.3 km/s) layer
and a large thickness of material with velocities
of 6.6-7.2 km/s led Berckhemer et al. (1975) and
Mohr (1989) to conclude that the original continental crust cannot merely have been stretched
3. zyxwvutsrqponmlkjihgfedcbaZYXWVUTSRQPONMLKJIHGFEDCBA
The Kenya rift within the framework of the
Afro-Arabian
rity system
and thinned uniformly as proposed by the mechanical stretching model of McKenzie (1978). In
A recent compilation of seismic investigations
addition, material must have been accreted to the
of lithospheric structure in the East African rift
base of the lower crust by magmatic processes
system (Prodehl and Mechie, 1991) has been upwithin the mantle, and Mohr (19891 argues that
dated and is shown in Fig. 4. An obvious point is
almost the entire crust in Afar is new igneous
that our knowledge of deep structure in the westmaterial. The 6.8-6.9 km/s lower crust layer
ern rift remains very rudimentary, and this region
beneath the Kenya rift and its flanks could also
represent underplated material.
needs additional study. The need for additional
data on deep structure is crucial from the standIn the vicinity of the major boundaries of the
point of rift processes because the eastern and
Kenya rift on the cross-rift line, Moho depths
starting models and parameterizations
was employed in the inversion scheme which was used to
interpret the teleseismic data. In all cases, the
abrupt velocity anomaly in the upper mantle was
derived from the inversion. Such an anomaly
clearly must be very young or diffusion would
have smeared it out laterally. A young origin for
this anomaly is also suggested by the fact that
normal heat flow values are found on the rift
flanks in Kenya with the high values being restricted to the rift valley region (Morgan, 1973,
1982; Nyblade et al., 1990; Wheildon et al., 1994).
At least in central Kenya, the lithosphere east
and west of the rift valley has experienced fundamentally different geologic histories (Nyblade and
Pollack, 1992; Smith, 1994). The Tanzanian craton is located to the west, and the Proterozoic/
Cambrian Mozambique mobile belt is located to
the east. In central Kenya, the rift valley locally
does seem to follow the boundary between these
provinces (e.g., Baker et al., 19721, and one might
expect the deep structure of these areas to be
different enough to be reflected in the KRISP
results. There are no striking differences between
crustal and upper mantle structure east and west
of the rift valley (Achauer et al., 1994; Braile et
al., 1994; Maguire et al., 1994; Slack and Davis,
19941. The crust is slightly thinner to the east, but
this may be due to the proximity of the Anza rift
(Prodehl et al., 1994). However, as discussed
above, the NW-SE-trending
Aswa suture zone
west of the rift valley may be associated with an
anomaly in the teleseismic inversion results even
at depths of about 100 km.
473
G.R. Keller et al. / Tectonophy sics 236 (1994) 465- 483
20-t
zyxwvuts
zyxwvutsrqponmlkjihgfedcbaZYXWVUTSRQPONMLKJIHGFEDCBA
/
16O’
. KHARTOUM
+
+
18
Fig. 4. Map showing the locations of seismic lines and corresponding crustal structure columns or models derived :from studies in
the area of the East African rift system between the Gulf of Aden and Tanzania. P-wave velocities are shown in #m/s.
474
G.R. Keller et trl / Tectonophysm
236 (19941 465-483
change quite abruptly by about 5 km over lateral
19871, and rift propagation (Vink et al., 19841 as
distances of lo-20 km. Abrupt changes in crustal
applied to the northern Red Sea-Gulf of Suez--thickness are also known to occur at some places
Jordan-Dead
Sea rift area (Steckler and ten
along the western boundary of the Jordan-Dead
Brink, 1986). However, the new results from the
Sea rift (El-Isa et al., 1987). In southwestern
KRISP-90 experiment show that the northern
Saudi Arabia, the transition from the Red Sea
Kenya rift does not quite fit into the sequence as
depression to the Arabian Shield, with a change
here the crust is thinner than in the southern
in Moho depth in excess of 20 km over a lateral
Afar depression to the north (Fig. 5). It is obvious
distance of a few tens of kilometers (Mechie et
that the evolution of the East African rift is more
al., 1986; Mechie and Prodehl, 19881, appears to
complex than simple propagation southward from
be the major lateral discontinuity beneath the
Afar.
region.
This sequence (Fig. 5) may also be thought of
As the sequence of crustal columns (Fig. 5)
as an evolutionary progression in terms of intenshows, the central portion of the Kenya rift is one
sity of rifting (see also Girdler, 1983), but this
of the end members of the Afro-Arabian
rift
would seem most applicable to a stretching (passystem. The sequence may be viewed as an evolusive) component of rifting. It may not be a useful
tion in space with the thin oceanic crust of the
measure of an active component of rifting as
Gulf of Aden and the axial trough of the southillustrated by the southern Kenya rift. Here geoern Red Sea at the center. Progressing away from
logical estimates of extension from structural
the center, the crustal thickness generally inmapping (Baker and Wohlenberg, 1971; Strecker,
creases until the thickest and closest to “normal”
1991) and crustal thickness indications of extencontinental type of crusts of the Jordan-Dead
sion (Mechie et al., 1994a; Maguire et al., 19941
Sea and the East African rifts are encountered
suggest only a small amount of stretching while
(Mechie and Prodehl, 1988; Prodehl and Mechie,
teleseismic estimates of the depth of the litho1991). This proposed spatial evolution may be
sphere-asthenosphere
boundary (Achauer et al.,
supported by the hypothesis of punctiform initia1994; Slack and Davis, 1994) suggest that there is
tion of sea-floor spreading in the Red Sea bea large active component thinning the lithosphere
tween latitudes 22” and 24”N (Bonatti, 1985, zyxwvutsrqponmlkjihgfedcbaZYXWVUTSRQPONMLKJIHGFEDCBA
from below. Morley (1994) further discusses the
AFRO-ARABIAN
N
Jar+_DSOdSSO-
RIFT
- .Red !5ea -Aden
-
Gulf of
SYSTEM
._
Afar
tmnsition -
S
bnyo
conti
r
fit”fd
1 -O
- 10
- 20
-30
Fig. 5. Evolutionary sequence of crustal structure columns of the Afro-Arabian rift system from the Jordan-Dead Sea rift in the
north through Red Sea-Gulf of Aden-Afar triangle to the East African rift in Kenya. W= water, C = cover rocks, U- upper
crust, L = lower crust, HL = high-velocity lower crust, M = mantle.
G.R. Keller et al. / Tectonophy sics 236 (1994) 465- 483
interaction of deep and shallow processes in the
evolution of the Kenya rift.
47.5
basic data for the Baikal rift zone has been published in western journals, thus making comparisons difficult. For all of these rifts, one must
remember that they present only discrete sections
4. zyxwvutsrqponmlkjihgfedcbaZYXWVUTSRQPONMLKJIHGFEDCBA
Comparison with other rifts
of considerably larger zones of extension (East
African rift, western North America, Central EuComparative studies are useful to organize inropean rift zone, Baikal rift zone). None-the-less,
formation and to look for key relationships. Since
some interesting observations can be made rethe Kenya rift is the classic continental rift zone,
garding the lithospheric structure of these four
it has often been compared to other features. For
rifts.
example, Keller et al. (1991) conducted a detailed
comparison between the Kenya and Rio Grande
4.1. Phy siography and crustal structure
rifts, and Logatchev et al. (1983) compared the
Kenya and Baikal rifts. In any comparison with
An obvious observation is that all of these rifts
other Cenozoic rift zones (e.g., Rio Grande,
have thinned crust as a result of extension. HowBaikal, Rhine Graben, eastern China, southern
ever, as more information has become available,
Mexico/Colima
graben etc.), the Kenya and
considerable variations in crustal thickness have
Ethiopian sections of the East African rift are
been observed along these rifts (Fig. 3). In the
distinct in terms of volume of volcanic rocks (e.g.,
Kenya and Rio Grande rifts, there is a regular
Williams, 1982; Karson and Curtis, 1989; Macvariation in crustal thickness which correlates with
donald, 1994). For example, in Kenya, the volume
the amount of extension suggested by the number
of volcanics is on the order of 50 times greater
and geometry of basins and the physiographic
than that found in the Rio Grande rift. However,
widths of the rifts. The Rio Grande rift experiseveral paleorifts (e.g., midcontinent rift system
ences a north to south increase in extension and
of North America, Hutchinson et al., 1990; Oslo
width and a corresponding decrease in crustal
Graben, Neumann et al., 1992) were magmatithickness and elevation of the flanks and valley
tally active and may have surpassed the Kenyan
floor (Cordell, 1982; Keller et al., 1991). At least
and Ethiopian rifts in volume of magmatic prodfrom the apex of the Kenya dome (Naivasha area)
ucts per unit length. A major result of the KRISP
northward, similar variations occur in the Kenya
effort has been to show the extent of the modifirift (Morley et al., 1992; Mechie et al., 1994b). In
cation of the lithosphere caused by the Kenya
the Rhine Graben area, there is a zone of strong
rift. Although this modification is extensive, it is
crustal thinning in the south (Edel et al., 1975)
similar to that found in some other rift zones.
which does not correlate with increased extension
Thus, despite its large volume of volcanics, this
but does correlate with the highest (not lowest)
rift does not appear to need a special explanation
flank elevations. At the southern end of the Cenfor its evolution, and it can be studied in the
tral European rift, at the mouth of the Rhone
context of other rift zones.
river, a strong thinning of the crust correlates
One problem in comparative studies is that
with increased apparent extension (Sapin and
data for features one would like to compare are
Hirn, 1974; Prodehl, 1981). Crustal structure is
often not of comparative quality and quantity.
not well defined at its northwestern end, the
This problem is certainly the case for lithospheric
Lower Rhine embayment, which is a center of
structure. With the completion of KRISP 89-90,
recent increased seismicity and exten$ion and may
the lithospheric structure data bases for the Kenya
be associated with progressive litho$pheric thinrift, Rio Grande rift, and Rhine Graben are
ning (Prodehl et al., 1992; Ziegler, 1992).
comparable. The data base for the Lake Baikal
Lake Baikal occupies the middle third of the
region is considerable and is being greatly exBaikal rift zone (Logatchev and Zorin, 19871, and
panded as a result of new cooperative efforts
there is no obvious difference in tie structure
(e.g., Hutchinson et al., 1992). However, little
along the lake or in the physiographic expression
of the rift in the region of the lake. Recent
reflection data collected in the lake indicate that
the basins in the southern portion are larger and
perhaps older than the basins in the northern
portion of the lake (Hutchinson et al., 1992). The
rift zone widens both north and south of the lake,
and to the north, the variations are reminiscent
of the axial variations found in the Kenya and
Rio Grande rifts. However, published geological
and geophysical data are not sufficient to evaluate the crustal structure of this region in detail.
From all of these results, we can deduce that
there are often correlatable variations in regional
topography, width of the rift zone, and crustal
thickness which are generally consistent with
varying degrees of extension via pure shear. Relations with upper mantle structure and the amount
of magmatic activity are less clear as one compares the various rift zones.
against magmatic additions but it does indicate
that these additions either predate or have not
kept up with the mechanical thinning which appears to have been concentrated in the lower
crust. In the Rio Grande rift, there is also an
axial variation in crustal thickness which correlates with the amount of extension (e.g., Keller et
al., 19911, but this variation is not as pronounced
as in Kenya. In addition, in the Rio Grande rift,
the thinning is not concentrated in the lower
crust. The P-wave velocities in the Rio Grande
rift lower crust ( N 6.5 km/s) are not unusually
high, and thus do not suggest extensive mafic
magmatic additions to the lower crust (Wendlandt et al., 1991). For the Central European rift,
as far as data are available for the areas of the
Rhine Graben and the grabens in the French
Massif Central region, no considerable thinning
of the lower crust which might be related to
extensive magmatism has been detected (Prodehl,
1981; Prodehl et al., 1992). In the Lake Baikal
4.2. zyxwvutsrqponmlkjihgfedcbaZYXWVUTSRQPONMLKJIHGFEDCBA
The lower crust
area, existing data are not sufficiently detailed to
reveal details of the lower crust.
The lower crust is another potential source of
Thus, the lower crust of the Kenya rift is an
information on rift processes, and the KRISP
results have provided some unexpected results.
enigma in that its velocity structure appears typiOne reason the lower crust is important is the
cal of continental areas, its thickness varies in a
role of rift-related magmatic processes in its forpredictable way with the amount of extension,
mation (e.g., Wendlandt et al., 1991). Recent
but its geometry does not reflect the known magmatic history in a straightforward way. Morley
studies (e.g., Lachenbruch and Sass, 1978; Griffin
and O’Reilly, 1987; McCarthy and Thompson,
(1994) suggests that this enigma indicates that
1988; Buck, 1991) have indicated that the Moho
either the amount of magma emplaced in the
crust in association with the volcanism is smaller
is sometimes a transient feature during extension
due to magmatic underplating and lower crustal
than generally believed or that significant crustal
flow. The pre-rift crust is thinned by extension
material has been lost into the asthenosphere.
but magmatic additions to the crust and/or flow
may cause the Moho to remain at a nearly con4.3. Deep lithospheric structure
stant depth.
The axial variations in the lower crust delinThe overall geometry of the lithosphere as a
eated as a result of the KRISP study address the
result of rifting is an important issue in efforts to
role of the lower crust in rifting. The volume of
model rift processes (e.g., Buck, 1991). In Kenya,
volcanics associated with the Kenya rift strongly
the transitions in the crust and upper mantle
suggests complementary magmatic additions to
from the flanks to the rift valley are very abrupt.
the lower crust and upper mantle (e.g., Karson
In the Rio Grande rift, the transitions in crustal
and Curtis, 1989; Wendlandt et al., 1991; Macstructure are not well known in the northern rift,
donald, 1994). However, the observed south-tobut in the south, the crust gradually thins into the
north thinning of the lower crust is in excellent
rifted area (e.g., Keller et al., 1991). All along the
agreement with the south-to-north
increase in
Rio Grande rift, the zone of reduced velocities in
extension. This result does not necessarily argue
the upper mantle is broad and only approxi-
G.R. Keller et al. / Tectonophy sics 236 (1994) 465- 483
mately correlates with the rift valley (e.g., Davis,
1991). In addition, the velocity and attenuation
anomalies are significant but not as large as those
associated with the Kenya rift (Halderman and
Davis, 1991). In the Rhine Graben, crustal structure changes abruptly when crossing the graben
boundaries, though the overall crustal thickness
decreases only gradually when approaching the
graben axis (e.g., Brun et al., 1992; Edel et al.,
1975; Prodehl, 1981; Prodehl et al., 1992). This
result also applies to the French Bresse and Limagne grabens and the southern Rh8ne Valley
(e.g., Sapin and Hirn, 1974; Him, 1976; Bergerat
et al., 1990; Prodehl et al., 1992). There is no
clear relationship of the subcrustal lithospheric
structure below 50 km depth to the Rhine Graben
proper (Glahn and Granet, 1992). However, under the Rhenish Massif and Lower Rhine embayment, in the seismically active continuation of the
Rhine Graben to the northwest, a well pronounced low-velocity zone at 50-150 km depth is
clear evidence for progressive lithospheric thinning (Raikes and Bonjer, 1983; Prodehl et al.,
1992) which, however, is only observed to the
southwest of the Rhine river. In the Lake Baikal
area, a low-velocity zone is observed in the upper
mantle. However, this zone is also asymmetrical,
being offset to the southeast (e.g., Logatchev et
al., 1983). The basin geometry, physiographic expression, and heat flow data argue that the crustal
thinning beneath Lake Baikal is abrupt (e.g.,
Ruppel et al., 1992), but more data are needed to
confirm this interpretation. The differences between the gradual transitions observed in the
southern Rio Grande rift and the abrupt transitions observed in the Kenya, Central European
and Baikal rifts may be due to differences in the
state of the lithosphere prior to rifting. In the Rio
Grande rift, the lithosphere was in a hot back-arc
setting, in Central Europe the lithosphere was in
a Variscan erogenic terrain setting, and in Kenya
and the Baikal area, the lithosphere was in cool
cratonal setting.
The new tomographic data from the Kenya rift
(Achauer et al., 1994; Slack and Davis, 1994)
confirm the observation of Green et al. (1991)
that the velocity-depth pattern related to the rift
reveals areas with distinct variations which make
477
the Kenya rift a truly 3D feature. The situation is
less pronounced but is similar in the Rio Grande
rift where a low-velocity upper-mantle anomaly is
offset slightly with respect to the direction of the
main rift valley (Davis et al., 1993). Davis et al.
(1993) have summarized the results of teleseismic
studies of the upper mantle structure beneath the
southern part of the Kenya rift, the Rio Grande
rift and the Rhine Graben. Beneath the southern
Kenya rift and the Rio Grande rift, large velocity,
density and attenuation anomalies in the upper
mantle, interpreted to be caused by partial melting, suggest that the lithosphere has been thinned
much more significantly than the crust. The extensional shear processes which caused the limited amount of crustal extension (about 10 km)
are unable to explain the magnitude of lithospheric thinning. An active mantle plume thinning the lithosphere from below is a more reasonable source for the observed mantle anomaly.
Thus, Davis et al. (1993) place these two rifts in
the category of active rifts. In contrast, the Rhine
Graben which has no such mantle anomaly (Glahn
and Granet, 1992) is placed by Davis et al. (1993)
in the category of passive rifts. In the Baikal rift,
we unfortunately lack high-resolution data. This
situation will hopefully change with the joint Russian-American
Baikal project currently underway. (e.g., Scholz et al., 1993).
4.4. Sy mmetry us asy mmetry
Deep crustal structure is essentially symmetrical in the Kenya rift, Rio Grande rift, Rhine
Graben, and Baikal rift in that the maximum
crustal thinning is approximately centered in the
rift valleys. However, the upper crudal structure
as revealed in the basins and tilted horst blocks is
generally asymmetrical. The Lake Baikal and
Rhine Graben basins are relatively simple and
mildly tilted, but in the Rhine Graben the polarity of tilting switches from one flank to the other
(e.g., Brun et al., 1992). The Rio Grande rift is
distinctive in that it contains a continuous series
of large, complex, en-echelon basins along its
extent. These basins are generally asymmetrical
and flip polarity often (e.g., Keller and Cather,
1994). A lack of drilling and seismic reflection
47x
G.R. Keller et ~1./ Tectonophy srcs 236 (1994) 4tS483
metric development of the rift with the major
crustal and lithospheric thinning being significantly offset to one side of the rift (e.g., Bosworth,
1987) are inconsistent with the present seismic
results.
Mechie et al. (1994b) and Keller et al. (19941
have provided quantitative petrological interpretations of the seismic P-wave velocities in the
uppermost mantle down to 60-70 km depth beneath the rift, while Halderman and Davis (1991)
Achauer et al. (19941, and Slack and Davis (1994)
have provided estimates of partial melting in the
low-velocity body identified by the teleseismic
data in the upper mantle down to about 165 km
depth. Mechie et al. (1994b) have explained the
5. zyxwvutsrqponmlkjihgfedcbaZYXWVUTSRQPONMLKJIHGFEDCBA
Discussion
low Pn velocities of 7.5-7.7 km/s beneath the rift
by 3-5% partial melt of basaltic magma rising
Cross-sections through the central Kenya rift
from greater depths and being trapped below the
derived from the KRISP-90 data (Fig. 2) constrain the crustal thinning and anomalously low
Moho. At depths between the maximum penetration of the Pn wave and 60-70 km depth, velociupper mantle P-wave velocities down to around
ties lower than 7.8 km/s can also be explained by
165 km depth to be confined essentially to bea few percent partial melt. The teleseismic results
neath the rift valley itself. In the vicinity of the
major boundaries of the rift valley at the surface,
can be explained by low P-wave velocities in the
the crustal thickness, upper mantle velocity, and
upper mantle down to about 150 km depth which
heat flow change abruptly to attain normal contiare due to 3-6% partial melt. Thus, the estimates
for the amounts of partial melt beneath the rift
nental values beneath both rift flanks. Abrupt
changes in crustal thickness have also been deterderived by both the long axial profile and telemined for parts of the western flank of the Jorseismic data are in agreement with the value of
dan-Dead Sea rift which is at a similar stage of
3% given by Macdonald (1994) from consideradevelopment as the Kenya rift and the Arabian
tion of the petrogenesis of the volcanic rocks.
margin of the southern Red Sea, which is at a
Mechie et al. (1994b) and Keller et al. (1994)
more advanced stage of development.
What
have explained the layers with high velocities
(8.0-8.3 km/s) in the uppermost mantle beneath
causes these changes to be so abrupt should be a
topic of further research, but they seem to be
the northern part of the rift in terms of preferred
evidence for the major phase of lithospheric thinorientation of olivine and depletion of basalt.
ning and extension to be young. Otherwise, latDepletion alone cannot explain the high velccieral diffusion of heat would tend to spread the
ties as even pure isotropic olivine rock does not
geophysical signatures out.
have high enough velocities at the high temperaCrustal thinning is accomplished by thinning of
tures existing beneath the rift. Depletion does,
both the upper and lower crusts (Fig. 2). The
however, serve to reduce the amount of preferred
upper crust is thinned primarily by simple shear
mineral orientation required to obtain the high
along normal faults leading to asymmetric basins
velocities. The preferred orientation of olivine
and tilted fault blocks. The concentration of the
could either produce an orthorhombic structure
crustal thinning and the anomalously low upper
or a transverse isotropic structure. In the case of
mantle velocities down to about 165 km depth
the orthorhombic structure, and in the absence of
beneath the rift valley itself is consistent with the
depletion, at least 40-55% of the olivine should
lower crust and the lithospheric mantle being
be oriented with its u-axis oriented horizontally
thinned by pure shear. Models requiring asymalong the rift axis. This orientation would result
data in Kenya along with the extensive volcanic
cover limit our knowledge of its basins. However,
the Project PROBE results in Lake Turkana
(Dunkelman et al., 19881, the AMOCO reflection
data in the Turkana area (Morley et al., 1992;
Hendrie et al., 1994) and KRISP results reveal
several large generally asymmetrical basins and
many smaller complex basins. Gravity data do not
suggest that these basins are as extensive as in
the Rio Grande rift. However, dense volcanic fill
in some basins could mask the negative gravity
anomalies expected from large fill thicknesses.
G.R. Kelleret al. / Tectonophy sics236 (1994) 465- 483
in ~imuthal dependence of velocities in the refraction data, In the case of the transverse
isotropic structure, there would be no azimuthal
dependence of the refraction velocities because
the a- and c-axes of the olivine should be randomly oriented in the horizontal plane and the
slow b-axis should be oriented vertically. In fact,
for the deeper layer (60-65 km), both preferred
mineral orientation and depletion are required to
explain the high velocity of 8.3 km/s. Mechanisms which cause olivine to show preferred orientation tend to orient the ‘b-axis pe~endi~ular
to the plane of the flow (Nicolas et al., 1971;
Bussod, pers. commun., 1992). Thus, we envisage
that a horizontal flow possibly caused by shearing
has occurred in the high-velocity mantle layers.
Nicolas et al. (1971) also describe the situation in
which the flow (shearing) is accompanied by recrystallization. The two processes acting together
can yield randomly oriented a- and c-axes in the
plane of the flow (Nicolas et al., 1971).
The plate boundaries surrounding Africa suggest that the whole continent is in a compressional state of stress. The Cenozoic rifting and
the tensional state of stress in many areas of
Africa can therefore only be explained by a
mechanism involving movements within the asthenospheric mantle. Zoback (1992) has stated
that the buoyancy force due to the low-velocity,
low-density upper mantle anomaly beneath the
Kenya rift is more dominant than the ridge push
compression and thus produces the present-day
NW-SE extension. In contrast, Strecker and
Bosworth (1991) and Bosworth et al. (1992) have
suggested that the rotation of the stress field in
the vicinity of the Kenya rift from an E-W direction to a NW-SE direction during the Quaternary is a result of far-field tectonic stresses (e.g.,
ridge push forces generated at the Red Sea/ Gulf
of Aden spreading centers).
In the southern part of the Kenya rift in the
vicinity of the Kenya dome, the teleseismic results
show that the lithosphere has been thinned considerably, whereas the refraction results and surface structural estimates provide evidence for
modest crustal thinning and only 5-10 km extension. This situation is complicated due to the
probability of magmatic additions to the crust,
479
but active mantle upwelling seems required. The
abrupt lithospheric boundaries between the flanks
and rift valley and the low heat flow on the flanks
are evidence that the major activity has been
recent. The high surface heat flow in the rift
valley, the earthquake activity and its concentration in the upper lo-12 km of the crust, and the
recent volcanicity all suggest that the rift is active
today.
The results of KRISP 90 have shed considerable light on the structure and evolution of the
Kenya rift. I-Iowever, many questions remain
unanswered, and this feature is clearly an ideal
place to study the relationships between the crust
and mantle during extension and the role magmatism plays in the evolution of volcanCcally active
continental rifts. zyxwvutsrqponmlkjihgfedcbaZYXWVUTSR
Acknowledgements
This work was financed by the National Science Foundation Continental Dynamics program
in the U.S.A. (Universi~ of Texas at El Paso
grant EAR-8708388, Purdue University, and
Stanford University), the European Community
under SC1 contract 00064 involving U.K., Denmark, France, Germany, Ireland, and Italy, and
the German R&search Society (DFG) via the special research project SFB 108 “Stress and Stress
Release in the Lithosphere” at the University of
Karlsruhe. A small contribution by the N.E.R.C.
(Natural Environmental Research Council) in the
U.K, helped to establish a local array around
Lake Baringo. The support and cooperation of
the U.S. Geological Survey is also gratefully acknowledged. The help of the diplomatic representatives of the E.C., U.K., France, U.S.A., and
UNESCO (Mr. Driessle) and, in particular, the
continuous support of the German Embassy (Mr.
Bock and Freiherr von Fritsch) are greatly acknowledged. The sponsorship of the International Lithosphere Program in cooperation with
the Kenya Academy of Sciences is also acknowledged.
Special thanks are due to the Ke yan Government and the ~derst~ding
officia s who made
?
the work possible. The University’ of Nairobi,
Bonjer, K.-P., Fuchs, K. and Wohlenberg, J., lY70. Crustal
Egerton College, Kenyatta University, the Minstructures of the East African rift system from spectral
istry of Energy, the Department of Mines and
response ratios of long period body waves. Z. Geopys.. 36:
Geology, the Survey of Kenya, the Department of
287-297.
Fisheries, the Ministry of Water Development,
Bosworth. W.. 1987. Off axis volcanism in the Gregory rift.
the National Environment Secretariat, the NaEast Africa: implications for models of continental rifting.
Geology, 15: 397-400.
tional Council for Science and Technology, the
Bosworth,
W. and Morley, C.K., 1994. Structural and stratiKenya Marine and Fisheries Research Institute,
graphic evolution of the Anza rift, Kenya. In: C. Prodehl,
the Kenya Posts and Telecommunications CorpoG.R. Keller and M.A. Khan (Editors), Crustal and Upper
ration, the Kenya Police, Contratours.
Inside
Mantle Structure of the Kenya Rift. Tectonophysics. 236:
Africa Safaris, Hertz Corporation,
Aquadrill,
93-115.
Bosworth, W., Strecker, M.R. and Blisniuk, P.M., lY92. InteTWIGA Chemical Industries all made vital congration of East African paleostress and present-day stress
tributions to the program. Helpful reviews by
data: implications for continental stress field dynamics. J
Paul Morgan and Henry Pollack are also grateGeophys. Res., 97: 11851-11865.
fully acknowledged. zyxwvutsrqponmlkjihgfedcbaZYXWVUTSRQPONMLKJIHGFEDCBA
Braile, L.W., Wang, B., Daudt, C.R., Keller, G.R. and Patel,
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