GRAVITY ANOMALIES IN THE WESTERN PACIFIC OF THEIR …
Transcript of GRAVITY ANOMALIES IN THE WESTERN PACIFIC OF THEIR …
J. Phys. Earth, 29, 387-419, 1981
GRAVITY ANOMALIES IN THE WESTERN PACIFIC
AND GEOPHYSICAL INTERPRETATION
OF THEIR ORIGIN
Yoshibumi TOMODA and Hiromi FUJIMOTO
Ocean Research Institute, the University of Tokyo, Tokyo, Japan
(Received April 22, 1981; Revised August 19, 1981)
Maps of free air and Bouguer gravity anomalies in the western Pacific arecompiled on the basis of the sea gravity data obtained during a period 1963-1980 by use of the Tokyo Surface Ship Gravity Meter.
Outer gravity high seaward of trench and negative gravity moat around
seamounts can be interpreted as caused by anomalous thickness of the litho-sphere.
Mutual interference between trench and seamount or rise is discussed fromthe view point of thickness of the lithosphere. Seamounts or rises can be
classified into three types;1) seamount which can easily subduct as represented by Kashima No. 1
Seamount,
2) sizable seamounts which take a long time to subduct,3) rises which will never subduct.
It is suggested that a new subduction zone seaward of the old trench isformed if the rises of the type 3 encounter a trench. In such a case a relic of
trench and a fore-arc ridge may be left in topography. After seamount of type2 eventually subduct, they give rise to an acute bending of trench accompanied
by a zone of negative gravity anomaly in the landward side of the trench.
1. Gravity Anomalies in the Western Pacific
1.1 Gravity measurements at sea and mapping of gravity anomaliesGravity data at sea have been obtained mostly in the western Pacific since
1963 by use of a vibrating string gravity meter stabilized by a vertical gyroscope-T.S.S.G.
We have now 18 years' collection of sea gravity data measured by the T.S.S.G.
The data obtained before 1971 have already been published (TOMODA, 1974),and maps of free air and Bouguer gravity anomalies in and around Japan have
also been published (TOMODA, 1973a). Since 1972, stabilization of the meter's
plarform and data aquisition system have been greatly improved. Since thenship's position has been determined by use of N.N.S.S., and, therefore, the qualityof gravity data since 1972 has been greatly improved (FUJIMOTO, 1976). Ship's
tracks along which the sea gravity data were obtained by T.S.S.G. chiefly onboard the R/V Hakuho-maru (3,200t) are shown in Fig. 1.
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388 Y. TOMODA and H. FUJIMOTO
Fig. 1. Ship's tracks along which sea gravity data were obtained by T .S.S.G. chieflyon board the R/V Hakuho-maru.
The first step of compilation of these gravity data was "debugging" of the"raw data
," most of "bugs" being caused by unexpected errors in N.N.S.S.Ship's position determined by N.N.S.S. and dead-reckoning navigation with theaid of gyrocompass and an electromagnetic log is not always sufficiently accurate
for the Eotvos correction in the order of a few mgal, although the accuracy hasbeen dramatically improved compared with that prior to 1971. For this reasonit was necessary to adjust the data by hand with careful reference to bottom to-
pography and ship's log.The second step of data compilation was the adjustment of inconsistency
between data obtained at different times at the same position. An example ofsuch inconsistency at an intersection is shown in Fig. 2. T.S.S.G. data in its earlystage (before 1971) have sometimes systematic errors more than 10 mgal . Theerrors seem to have occurred when an unexpected vibration of the vertical gyro-scope was existent or when the ship set sail without enough warming -up time fora temperature regulating housing of the string gravimeter. Gravity data meas-
Gravity Anomalies in the Western Pacific 389
Fig. 2. An example of inconsistency of gravity or bathymetric data at intersections of
different cruises.
Fig. 3. Free air gravity anomaly in the northwestern Pacific.
390 Y. TOMODA and H. FUJIMOTO
Fig. 4. Bouguer gravity anomaly in the northwestern Pacific.
ured by T.S.S.G. on board the Hakuho-maru generally well agree with eachother.
These inconsistencies were carefully adjusted and maps of gravity anomalyin the northern part of the western Pacific were compiled (TOMODA and FUJIMOTO ,1981). Free air and Bouguer gravity anomalies are simplified and shown forthree regions; northwestern Pacific east of the Japan trench (Figs. 3 and 4), centralpart of the western Pacific in and around the Izu-Ogasawara trench (Figs. 5 and6), and northern part of the Philippine Sea (Figs. 7 and 8).
1.2 Characteristics of gravity anomaly in the western Pacifica) "Outer gravity high" seaward of the Japan trench (WATTS and TALWANI ,
1974) was observed by the sea gravity measurement on board the submarine
Gravity Anomalies in the Western Pacific 391
Fig. 5. Free air gravity anomaly in the central part of the western Pacific in and around
the Izu-Ogasawara trench.
Fig. 6. Bouguer gravity anomaly in the central part of the western Pacific in and around
the Izu-Ogasawara trench.
392 Y. TOMODA and H. FUJIMOTO
Fig. 7. Free air gravity anomaly in the northern part of the Philippine sea.
Ro-57 (MATUYAMA, 1934). It was mentioned that it cannot be interpreted as
caused by crustal structure (KUMAGAI, 1953). In the map of free air gravity
anomaly in and around Japan (TOMODA, 1973a), the distribution of the outer
gravity high is clearly shown, though partially. It is also shown that the outer
gravity high seaward of the trench is compensated by gravimetric low around a
seamount if it is situated close to the trench.
Figure 3 shows the general features of the outer gravity high seaward of the
Japan trench, where the gravity high larger than 20 mgal extends seawards more
than 200km. The maximum height of the positive gravity anomaly amounts to
50 mgal in the region east of the Japan trench along 39° N .
Gravity Anomalies in the Western Pacific 393
Fig. 8. Bouguer gravity anomaly in the northern part of the Philippine sea.
b) The western Pacific is characterized by the existence of many seamounts
and seamount chains as represented by the Emperor seamounts, Marcus-Necker
seamounts, and Magellan seamounts. It is well known that significant positive
gravity anomalies as large as 200-300 mgal due to the body of seamounts areobserved. However, more important gravity characteristics for the interpreta-tion of its root seem to be the negative free air gravity anomaly observed around
seamounts (TOMODA, 1973b).
394 Y. TOMODA and H. FUJIMOTO
As illustrated in the gravity anomalies seaward of the Japan trench, positiveanomalies seaward of the trench are compensated by the negative free air gravity
anomalies around seamounts close to the trench axis. Although this situationis recognized in the southern part of the Japan trench, the interference betweenseamounts and trench is observed typically in the region of the Ogasawara rise
where the Ogasawara trench and Marcus-Necker rise are supposed to collide witheach other (Figs. 5 and 6).
c) Northern part of the Shikoku basin in the Philippine sea is bordered by
the Nankai trough. The outer gravity high seems to exist seaward of the trough,but the magnitude is not so large as that seaward of the Japan trench and the
Philippine trench. The maximum value of free air gravity anomalies seawardof the trough is about 25 mgal, and its mean value is about 10 mgal. As de-scribed by WATTS and TALWANI (1974) the outer gravity high seaward of the trough
is different in its character from that of the Japan trench.The negative gravity anomaly lower than -20 mgal in the northern part of
the Ryukyu trench appears to extend to the gravity low off Miyazaki in Kyushudistrict and further north to the Japan Sea through the Bungo and Kanmon
Strait between Honshu and Kyushu islands.The northern part of the Philippine basin is bordered by the Palau-Kyushu
ridge in its west. The Daito ridge runs nearly perpendicular to the Palau-Kyushu
ridge. Gravity lows are observed at both sides of the Daito ridge, similarlywith those observed in the western end of the Marcus-Necker rise.
2. Gravity Anomaly Expected from the Crustal Structure Disclosed by Explosion
Seismology
A great number of seismic works have been carried out and the structureabove the Moho is determined at more than 470 points in the Pacific region
(SHOR, 1960, 1962, 1964; FISHER and RAITT, 1962; RAITT, 1963; SHOR and POLLARD,1964; FURUMOTO et al., 1965, 1968, 1970, 1971, 1973; LUDWIG et al., 1966, 19711973; MURAUCHI et al., 1967, 1968, 1973; SHOR et al., 1968, 1970, 1971; RYALL
and BENNETT, 1968; DEN et al., 1969, 1971a, b; HILL, 1969; SHOR and RAITT,1969; EWING et al., 1970; HOTTA, 1970; LUDWIG, 1970; YOSHII et al., 1973;
HOUTZ et al., 1980; MURAUCHI and LUDWIG, 1980).Recently, a long shot experiment as long as 1,800km was carried out at the
Mid Pacific as one of the items of the Geodynamics Project (ASADA et al., 1981;NAGUMO et al., 1981). Long velocity profiles are also determined from the Japantrench to Shatsky rise (HOUTZ et al., 1980). Now, the general feature of the
crustal structure above the Moho in the western Pacific basin seems to be clarified.By use of the subterranean velocity structure obtained by explosion seis-
mology, the density structure can be brought out by use of the velocity-densityrelationship and so gravity anomaly caused by the structure below the Moho canbe estimated. The difference between gravity anomaly actually measured and
Gravity Anomalies in the Western Pacific 395
that estimated from the crustal density structure was called "the residual gravity
anomaly (R.G.A.)" by YOSHII (1972). The R.G.A. puts forth the information
on the density anomaly below the Moho, which is not easily determined by ex-
plosion seismology.Figure 9 shows a map of the free air gravity anomaly in the Pacific basin calcu-
lated from the crustal structure determined by the above-mentioned explosion
seismology works. The gravity values at 470 points in the Pacific were calculatedby use of the velocity-density relationship compiled by LUDWIG et al. (1970), and
the standard gravity value calculated by use of the standard crust given by SHORand RAITT (1969) for the Pacific and Indian basins was subtracted. Figure 10
shows the profiles of the crustal structure and the residual gravity anomaly fromthe Japan Sea to Gorda ridge off the West Coast of U.S.A. along the line A to B
in Fig. 9. East part of the crustal structure section is the same as that shown by
HOTTA (1972). As shown by these profiles, the R.G.A. in the western Pacificbasin is systematically about 300 mgal larger than that in the eastern part. Thisdiscrepancy is more than 10 times as large as the observed gravity anomaly.
Based on these facts, YOSHII (1973) postulated a new model of thickening
lithosphere. According to his postulation the lithosphere produced at the midoceanic ridge becomes thicker toward the trench as material of the asthenosphere
is condensed at its bottom. Analysis by use of the R.G.A. is a useful means forestimation of the regional thickness of lithosphere. We think that the R.G.A.
Fig. 9. Map of the free air gravity anomaly in the Pacific basin calculated from the
crustal structure determined by explosion seismology.
396 Y. TOMODA and H. FUJIMOTO
Fig. 10. Profiles of crustal structure and the residual gravity anomaly in the northern
Pacific.
is also useful for inferring the deep structure beneath a minor topographic struc-
ture such as a seamount.It is naturally expected that a seismological analysis puts forward possible
crustal structures that satisfy the time travel curve, resulting in various kinds ofestimation of the R.G.A. According to Yoshii (personal communication), how-
ever, the R.G.A. is always the same as far as the structure strictly satisfies theobserved time travel curve.
The R.G.A. will be applied to the interpretation of gravity lows around
seamounts or outer gravity high seaward of the trench.
3. Outer Gravity High Seaward of the Trench
3.1 Outer gravity high and R.G.A.The results of explosion seismology by LUDWIG et al. (1966), HOUTZ et al.
(1980), and MURAUCHI and LUDWIG (1980) seem to provide sufficient data to in-vestigate the origin of the outer gravity high and the thickness of lithosphere
seaward of the Japan trench, if they are correlated to the gravity data. Figure 11
shows the profiles of velocity structure, free air gravity anomaly, and R.G.A.
Gravity Anomalies in the Western Pacific 397
Fig. 11. Profiles of velocity structure, free air gravity anomaly and R.G.A. deviation
from the standard value seaward of the Japan trench along the 33° N parallel.
along the 33° N latitude. The R.G.A. was calculated according to the following
formula.
R.G.A.=F.G.A.+2πkk2Hi(ρm-ρi),
where F.G.A. and kk2 indicate free air gravity anomaly and the gravitational con-
stant, respectively. The density of the upper mantle ρm is assumed to be 3.3g/
cm3, which value corresponds to the Pn velocity 8.1km/sec. Hi and ρi indicate
the thickness and the density of the i-th layer, respectively. The R.G.A. thus
obtained minus 587 mgal is shown in Fig. 11. This is the R.G.A. deviation from
the standard value estimated with the standard crust given by SHOR and RAITT
(1969). The profiles of the R.G.A. deviation are also calculated by the same
method along the parallel of 39° N and shown in Fig. 12. The R.G.A. seaward
of the trench is not so complicated as that landward of the trench, and it is pos-
sible to compile a map of relative values of R.G.A. Figure 13 (a) shows the iso-
anomaly lines, drawn by use of 2.5° means of R.G.A. Figure 13 (b) shows the
distribution of depth to the Moho.
The map of R.G.A. as well as its profiles shows that the thickness of litho-
sphere becomes larger toward the trench. According to the model presented by
YOSHII (1973), changes in thickness of lithosphere and accordingly in the theo-
retical R.G.A. value are nearly constant, since the ages of this region are older
than 100 million year. Therefore, variations in the estimated R.G.A. should be
caused by other origins. The observed increase in lithosphere thickness may
398 Y. TOMODA and H. FUJIMOTO
Fig. 12. Profiles of velocity structure, free air gravity anomaly and R.G.A. deviation
seaward of the Japan trench along 39°N parallel.
possibly be attributed to a rapid cooling of the oceanic lithosphere close to the
trench.
This fact seems to suggest that extra heat loss must exist in the lithosphere
near the trench axis in addition to heat transfer by conduction, if thickening of
lithosphere is due to cooling process.
Although the R.G.A. landward of the trench seems very important for in-
terpreting the origin of mass excess or deficiency at the trench region, the seismic
data are not as yet sufficient for such analysis.
3.2 Origin of the outer gravity high and driving force of subduction
In order to explain the outer gravity high seaward of the trench, two models
have so far been proposed.
One of the models can be schematically shown in Fig. 14(a). In this model
the trench is formed by the subduction of a mass heavier than its surrounding
material, and the positive free air gravity anomaly seaward of the trench or the
positive Bouguer anomaly at the trench represents this mass excess (MORGAN,
1965). The mass excess can also be interpreted as caused by the density contrast
between the sinking lithosphere and the asthenosphere, or it may also be inter-
preted as caused by the lithosphere which suddenly thickens near the trench
Gravity Anomalies in the Western Pacific 399
Fig. 13. (a) Map of the R.G.A. deviation seaward of the Japan trench. (b) Map ofthe depth to the Moho seaward of the Japan trench.
400 Y. TOMODA and H. FUJIMOTO
Fig. 14. (a) A model showing that the driving force of subduction is produced by thepossible negative buoyancy due to the density contrast near the trench, and that theouter gravity high shows this mass excess (MORGAN, 1965). (b) A model showingthat the outer gravity high is caused by the swollen mantle material near the trench(WATTS and TALWANI, 1974).
(FUJIMOTO, 1976; FUJIMOTO and TOMODA, 1977). The model represented byFig. 14(a) shows essentially that the driving force of subduction is produced bynegative buoyancy due to the density contrast near the trench, and that the outer
gravity high shows this mass excess.On the other hand, Fig. 14(b) shows the model presented by WATTS and
TALWANI (1974). In their model, the driving force of subduction does not directly
connected to outer gravity high, because they explain the gravity high as causedby the swollen mantle material near the trench, which is caused by the elastic
bending of the lithosphere. The structure of the Moho seismically determined,however, does not disclose such an elastic bending of the lithosphere (LUDWIGet al., 1966; HOUTZ et al., 1980; MURAUCHI and LUDWIG, 1980). The outer
gravity high is recognized independently of the outer topographic high which iscaused by the elastic bending.
The essential difference between the two models depends on the assumption
whether the lithosphere is an elastic plate or a plastic plate where isostatic equi-librium is easily achieved.
As shown in Figs. 11 and 12, the R.G.A. shows that the outer gravity highseaward of the trench is caused by density anomaly below the Moho. The
lithosphere thickens towards the trench, so that the horizontal gradient of thick-ness of the lithosphere near the trench is twice or three times as large as the litho-sphere near to the ridge crest (Fig. 10). This extraordinary thickening of the
lithosphere near the trench may possibly cause a driving force of subduction oflithosphere. However, the cause of such an enhanced cooling process is notcertain yet.
4. Gravity Lows around Seamounts
4.1 Gravity anomaly of a seamountPositive free air gravity anomalies relevant to seamounts in the western
Gravity Anomalies in the Western Pacific 401
Pacific are generally correlated with the topography, but we should also pay
attention to the negative anomaly zones extending over a wider area around the
seamount. The horizontal extent of the negative anomaly zone is generally
more than twice as large as the topographic extent of seamount. These features
are shown by a long north-south profile crossing the crests of seamounts along
about 150°E longitude (Fig. 15). The horizontal extent of the gravimetric moat
is very large and its amplitude is 20-50 mgal.
In order to investigate the origin of the negative free air anomaly surrounding
a seamount, detailed gravity surveys were carried out at the Suiko seamount located
in the Emperor ridge (TOMODA et al., 1968b; SEGAWA, 1970) and at the Shunsetsu
seamount (23°54′N, 148°50′E) in the Marcus-Necker seamount chain (FUJIMOTO,
1976).
One of the gravity profiles across the Shunsetsu seamount is shown in Fig. 16.
The positive free air gravity anomaly has a very good correlation with the seamount
topography. Using this correlation, the density of the seamount has been de-
termined on the basis of the principle that the correlation between Bouguer
anomaly and topography becomes minimum when an optimum density is selected.
As is shown in Fig. 16, the density is 2.9g/cm3 for the Shunsetsu seamount. The
same value is also obtained for the Suiko seamount (SEGAWA, 1970; FUJIMOTO,
1976). Using this density, the Bouguer gravity anomalies are calculated for the
two seamounts. The horizontal extents of Bouguer anomalies probably rep-
resenting roots of Suiko and Shunsetsu seamounts are about 230 and 150km,
respectively. Three models of sub-bottom structure seem to satisfy the gravi-
metric results (Fig. 17), if the structure above the Moho is taken into account.
A) First model (Airy-Heiskanen's model): This is one of the idealized
models of isostasy, where mass of a seamount body is supported by buoyancy
caused by the root in the crust. Gravimetric effect can easily be calculated if
depth of compensation and density contrast between the crust and the mantle
are assumed. The results of calculation for the Shunsetsu seamount (Fig. 18(A))
show that this model does not satisfy the gravimetric results, as far as the com-
pensation depth is in the order of 10km, as expected from the thickness of the
Fig. 15. Profile of the free air gravity anomaly along about the 150°E meridian cross-
ing the crests of seamounts (TOMODA, 1973b).
402 Y. TOMODA and H. FUJIMOTO
Fig. 16. Gravity and bathymetric profiles of Shunsetsu seamount.
crust. Airy-Heiskanen's model seems unreasonable, when the isostatic equilibri-um above the Moho is assumed. However, the model fits in the observed results
when a compensation depth of 100km is assumed, as will be mentioned in thefollowing section.
B) Second model ("elastic bending of the crust"): The crust is bent bythe weight of a seamount forming a topographic moat around the seamount asschematically shown in Fig. 17(B), the moat may be filled with sediments of lowdensity amounting to about 2.0g/cm3. In such a model, the bending of the crust
can easily be verified by a acoustic reflection profiling (air gun) around the sea-mount. Figure 19 shows an example of acoustic reflection profiling suggesting
that the thickness of sedimentary layer becomes thicker with the distance fromthe seamount. This is inconsistent with the model.
C) In the third model, the thickness of crust is made large over a wide area
(twice or three times of horizontal extent of the seamount) around a seamountto satisfy the Bouguer gravity anomaly, as shown in Fig. 17(C). The concept ofisostasy is not taken into account explicitly in this model.
Gravity Anomalies in the Western Pacific 403
Fig. 17. Three types of sea-
mount models viewed
from the gravimetric and
seismic stand points.
Fig. 18. Bouguer gravity anomaly expected from models A, B,
and C shown in Fig. 17.
Fig. 19. Example of acoustic reflection profiling near the foot of a seamount.
4.2 Gravity low around seamounts and anomalous structure of the lithosphereExplosion seismic surveys of the crust are usually carried out in the region
which are away from seamounts. However, if the horizontal extent of the root
of seamount is twice to four times as large as that of the seamount body, the rootof the seamounts can be observed.
As far as the seismic results so far obtained is concerned, it is difficult to
prove that the crust near the seamount becomes thicker. In the case of theEmperor ridge, the crust becomes thinner near the seamount chain as shown in
Fig. 20(a) (DEN et al., 1969). In the case of Bikini Atoll, it seems difficult to
point out any change of crustal structure near the seamount, as shown in Fig.20(b) (RAITT, 1954).
404 Y. TOMODA H. and FUJIMOTO
Fig. 20. Examples of structure crossing near seamounts. (a) Emperor ridge (DENet al., 1969), (b) Bikini Atoll (RAITT, 1954).
Fig. 21. Proposed structure of a seamount. The weight of seamount is supported bythe buoyancy of the root in the asthenosphere underneath the seamount.
Taking such seismic results into consideration it is necessary to attribute the
origin of gravity low to the structure beneath the Moho. Judging from the
horizontal scale of the gravity low, it is reasonably concluded that the lithosphere
beneath a seamount is 20-30km thinner than the surrounding lithosphere as shown
in Fig. 21. In this model weight of a seamount is supported by buoyancy of the
root in the asthenosphere underneath the seamount.
According to the theory of plate tectonics, a seamount chain is produced by
Gravity Anomalies in the Western Pacific 405
a volcanism when the lithosphere moves above the hot spot (WILSON , 1963;
MORGAN, 1972). Therefore, it will be quite reasonable to assume that the thick-
ness of lithosphere becomes thinner when heated by the hot spot (KONO and YOSHII ,
1975; OGAWARA and KONO, 1981).
A long distance seismic explosion work was carried out at Mariana region in
1976 (ASADA et al., 1981). In this experiment, the line of survey was 1,800km
long, crossing the Marcus-Necker seamount chain, and the maximum explosives
fired were 8.5t. Extraordinarily large attenuation of seismic wave was observed
for the area across the seamounts, compared with that observed in the north-
western Pacific, where there is no seamount chains.
In the northern Pacific region initial phases can easily be detected in seis-
mogram obtained from an explosion of 0.5t by a ocean bottom seismogram
deployed 1,000km apart from the shot point, even if the bottom noise was the
same as that of the Mariana's region. However, when the explosives are fired
across the Marcus-Necker seamount chain, we could not obtain such a seismo-
gram in spite of the large amount of explosive of 8.5t. One of the interpretations
of the fact is that the asthenosphere beneath the Marcus-Necker seamount chain
is responsible for this large attenuation of seismic waves.
Whether or not this idea is also plausible for the seamounts in the Philippine
Sea is an important problem. It is difficult to recognize gravity lows around
seamounts as seen in Fig. 7 which represents the case of the Kinan No. 2 seamount
(30°15′N, 136°40′E). The result may be consistent with magnetic and micro-
paleontological data showing the ages of ocean floor and seamount are nearly
equal there (FURUTA et al., 1980).
4.3 Subducting seamount-Kashima No. 1 seamount
The Kashima No. 1 seamount is located exactly at the axis of the Japan
trench. The seamount has been surveyed in detail by the Hydrographic Depart-
ment, Maritime Safety Agency, Japan, and it was found that the landward half
of the seamount has broken down and subsided by about 1,500m (MOGI and
NISHIZAWA, 1980). Detailed gravity surveys were carried out along tracks with
a spacing of 5 nautical miles in this area. The bottom topography and ship's
tracks along which the gravity profiles are made are shown in Fig. 22. Six sec-
tions crossing above or near the seamount are prepared with respect to the free
air anomaly, the Bouguer anomaly, and the bottom topography, and shown in
(a) through (f) of Fig. 23 (TOMODA et al., 1980). As mentioned above, most
seamounts in the western Pacific have large roots of compensation, which are
represented by relatively smaller Bouguer anomalies or negative free air anomalies
around them. However, the Bouguer gravity anomaly of Kashima No. 1 sea-
mount does not show such characteristics. This is clearly seen in the profile of
mean Bouguer anomaly of the 6 sections of Fig. 23, in which we see only a linear
trend (Fig. 24) of gravity change.
If a depression of Bouguer anomaly around a seamount should reveal the
406 Y. TOMODA and H. FUJIMOTO
Fig. 22. Bottom topography and ship's track along which gravity profiles are con-structed at the Kashima No. 1 seamount.
presence of a root of the seamount-a thinner lithosphere beneath the seamount,it can be said that the Kashima No. 1 seamount is lacking in such a root.
A seamount must be supported by buoyancy of asthenosphere. The results
of the Kashima No. 1 seamount suggest that there exists no buoyancy whichsupports this seamount, and this may be the reason why the Kashima No. 1seamount has broken down. The results of acoustic profiling and bottom topo-
graphy show that the breakdown is confined to the seamount body, and that nodepression of the basin around the seamount is recognized. Although this fact
sounds somewhat strange, it would not be impossible that the seamount calmlysinks down when the root which existed just beneath the seamount has disappeared.
The reason why the root of a seamount has disappeared may be attributedto a process by which the lithosphere becomes thicker by cooling due to the hydro-thermal process in the rock (ANDERSON et al., 1979). Gigantic faults observed
seaward of active trenches seem to provide one of the processes releasing theheat preserved there (FUJIMOTO, 1976).
5. Mutual Interference between Seamount and Trench
5.1 Positive gravity anomaly seaward of a trench and negative gravity anomalyaround a seamount
In order to satisfy both seismic and gravimetric results, it would be necessary
Gravity Anomalies in the Western Pacific 407
Fig. 23. Profiles of free air, Bouguer, and bottom topography along 6 sections cross-
ing above or near the seamount.
to assume that (1) the lithosphere is thinner beneath a seamount due to the rise
of a partially molten layer, and that (2) the lithosphere is thicker near the trenchdue to the possible accretion of high density materials at the bottom of the litho-
sphere. These two phenomena must mutually interfere each other at the trenchmargin.
Figure 25 shows gravity profiles for a case when a seamount exists far from
the trench. When the distance between a trench and a seamount is larger than500km, their gravimetric characteristics can be recognized separately. When
a seamount is near a trench, the outer gravity high seems to be disturbed by thenegative anomaly zone around the seamount, as shown in Fig. 26. Figure 27
shows that the positive anomaly is completely cancelled by the negative anomaly.
408 Y. TOMODA and H. FUJIMOTO
Fig. 24. Mean Bouguer anomaly of 6 sections of Fig. 23. It should be noted that onlylinear trend can be seen.
One of the typical examples of gravimetric interference between seamounts
and a trench can be seen between the outer gravity high seaward of the Ogasawaratrench and negative anomaly around the Marcus-Necker seamount chain as shown
in the maps of free air anomaly (Fig. 5) and Bouguer anomaly (Fig. 6). It isreadily concluded that this kind of gravimetric interference must represent thedegeneration of lithospheric anomaly.
5.2 Bending of trench axisIf the thickening of lithosphere is the main cause of the driving force of
lithospheric subduction, and if the thickness anomaly is cancelled by the root of
a seamount, the subduction should stop. In that case the seamount becomes anobstacle of subduction and gives rise to a bending of the trench axis (VOGT, 1973).
An example of such a bending is seen at the intersection of the Kuril and the
Aleutian trenches where the Emperor seamount chain meets with the trenches,and at the intersection of the Ryukyu trench and the Nankai trough where thePalau-Kyushu ridge meets with the trench and trough.
As described before, Kashima No. 1 seamount would subduct without beingaccompanied by a bending of trench axis. Many profiles of acoustic reflection
profiling surveys at the foot of this seamount do not show any faulting whichsuggests the possible effect of horizontal stress near the foot of the seamount
(MURAUCHI and ASANUMA, 1977). A seamount was also found at the trenchaxis to the north of Kashima No. 1 seamount, where it is buried in the sediment
(Kagami, personal communication).This fact shows that seamounts of such a small scale causes no bending of
trench axis. This seems to suggest that bending of trench axis due to difference
Gravity Anomalies in the Western Pacific 409
Fig. 25. Gravity profiles when a seamount is located far from the trench.
Fig. 26. Gravity profiles when a seamount is located near the trench.
Fig. 27. An example of cancellation of the outer gravity high seaward of the trench
by the gravity low around the seamount.
in the thickness of lithosphere depends on the scale of the seamount or on the
characteristics of the crust of the seamount.
Suppose that a sizable seamount approaches a trench in the course of a plate
410 Y. TOMODA and H. FUJIMOTO
motion. The seamount would not break down until the thickness of the litho-
sphere beneath the seamount reaches a certain limit by cooling. Assuming thatthe model is two-dimensional, the thickness of lithosphere beneath a seamount
as high as 5km is 10km thinner than the surrounding lithosphere. It wouldtake about 10 million years for the negative root of seamount of 10km thick
to disappear, if the normal cooling process of lithosphere continues. However,the negative root would persist only for about 1 million year, because, heat transfernear the trench seems about 10 times larger than in the normal place as estimated
from the thickening rate of the lithosphere near the trench as previously shownin Fig. 10. Therefore when the subducting force around the seamount is large,the trench axis would be compelled to flip over the seamount, leaving the seamount
behind. About 1 million year later, root of the seamount would disappear andthe normal subduction would take place.
5.3 Relics of seamount landward of trench
The maximum negative free air gravity anomaly off Urakawa in Hokkaidois -200 mgal and horizontal extent of the region where gravity value is lowerthan -20 mgal is larger than 100km. The scale of the negative zone is com-
parable to that of the trench, but the water depth is smaller than 200m.Asimilar negative anomaly zone off Miyazaki in Kyushu district (TSUBOI
et al., 1956; TOMODA et al., 1968a), which is not so large as that off Urakawa,
indicates the lowest negative value amounting to about -150 mgal. It is im-
portant that these negative zones are both located at the landward side of junctionof two trenches.
These negative zones can be interpreted as a result of delayed subduction ofrelics of seamounts, started to subduct later to form an anomalously swollen
subduction zone. Such a configuration of subduction zone may cause a negativebuoyancy resulting in the observed negative free air anomaly at the landward
side of trench junctions.
5.4 Non-subducting seamount
There are a number of oceanic ridges or rises in the western Pacific. Oneof the largest ones is the Shatsky rise the horizontal extent of which is more than400km, and the thickness of the crust determined by explosion seismic surveys
is about 18km (Fig. 28).The crustal structure of the rise brought out by the explosion seismic surveys
and the free air gravity anomaly show that the rise is quite isostatic.The R.G.A. over the Shatsky rise is almost the same as that in the west of
the rise, showing that the isostatic equilibrium is perfectly achieved above the
Moho. If such a ridge or rise arrives at the trench, a collision must occur as wecan see in the case of the collision between the Eurasian and the Indian plates.
In the case of the Ogasawara rise, however, the situation seems to be in-termediate stage between a seamount supported by the asthenosphere and a rise
Gravity Anomalies in the Western Pacific 411
Fig. 28. Profiles of velocity structure (DEN et al., 1969), free air gravity anomaly, and
R.G.A. deviation from the standard value over the Shatsky rise.
supported by the upper mantle.The density of a seamount is usually 2.8-2.9g/cm3, as described in Sec. 4.
The density estimated from the correlation between free air gravity anomaly andtopography of a seamount is likely to give a lower density according to the degree
of isostatic compensation of crustal structure. In the central continental districtof Japan, for example, a density of 2.67g/cm3 is obtained from the area with a
topography smaller than 20km in scale, but a density of 2.0-1.5g/cm3 with thetopography of 50-200km in scale (YAMAMOTO et al., 1980).
Profiles of free air, Bouguer, and bottom topography along the Ogasawaratrench axis is shown in Fig. 29. If the same analysis as that in Sec. 4 is applied
to the Ogasawara rise, extraordinarily small value of density less than 2.0g/cm3
will be given. Such an apparently low density given for the Ogasawara rise sug-
gests that the depth of compensation is not so deep as that of isolated seamounts,and that the crustal structure in this region is partially isostatic.
412 Y. TOMODA and H. FUJIMOTO
Fig. 29. Profiles of free air, Bouguer, and bottom topography along the Ogasawara
trench axis.
The depth of compensation can be determined, as Hayford calculated assum-ing Airy isostasy, i.e., depth is given as an optimum depth which gives the best cor-
relation between topography and equivalent Bouguer anomaly.As seen in Fig. 29, the correlation between Bouguer gravity anomaly and
topography is good unlike the case of the isolated seamount mentioned above,and so it is concluded that the depth of compensation is shallow.
The Ogasawara rise is partially isostatic equilibrium by buoyancy of the crust,
and the rise is not so easily subducted as the Kashima No. 1 seamount.When such a fragment arrives at the trench, subduction will stop at least
temporarily. Seaward jump of trench axis will take place, if subduction process
proceeds in the surrounding trench.
Gravity Anomalies in the Western Pacific 413
Fig. 30. Relics of trench in the west of Hokkaido district.
5.5 Relics of trench
When jump of the trench axis takes place, the old trench continues to existas the fragment of lithosphere heavier than asthenosphere still subducts. Arelic of trench will be recognized until the fragment subducts deeper into the
asthenosphere.An example of such relics of trench is seen in the west of Hokkaido district,
where a negative zone of free air gravity anomaly runs from the Urakawa lownorth to the west of Sakhalin as schematically shown in Fig. 30.
In the case of the Ogasawara trench, we can see double arc: One is representedby Iwozima islands and the other by Ogasawara islands. The Ogasawara troughbetween these two topographic highs is interpreted as a relic of trench. TheOgasawara trench must have stopped its subduction near the Ogasawara islands
after the islands collided with the trench. As shown by the outer gravity highrunning from the north to the south in this collisional region (Fig. 5), the drivingforce of lithospheric subduction there must be larger than that for a normallithosphere, should the outer gravity high seaward of trench be a measure of the
driving force of subduction. These situation must have resulted in jump of
414 Y. TOMODA and H. FUJIMOTO
Fig. 31. Role of "A," "sizable A," and "B" types seamount or rises at a trench.
trench axis toward east, and the Ogasawara trough was formed as relics of the
old trench.
6. Summary-Role of Seamount and Rise at a Plate Boundary
Seamounts and rises are classified into three classes-A type, sizable A type,
and B type as shown in Fig. 31. An "A" type seamount is supported by the
asthenosphere. A "sizable A" type seamount is supported by the asthenosphere,
although it is hard to be broken down by a cooling process as in the case of type
"A." A type "B" seamount is a rise supported by the crust.
When these seamounts are in line and move towards the trench (Fig. 31),
the type "A" would easily be subducted with the slab, the type "sizable A" would
not be subducted so easily as the type "A" and jumping of trench axis would take
place and relics of trench or seamount would be seen. The type "B" would never
be subducted and jumping of trench axis would take place and consequently the
type "B" will be accreted.
In a three-dimensional case (Fig. 32), suppose that plate α and plate β are
bounded by a trench and moving in different directions.
The type A will easily sink at the trench and the type B will be accreted to
plate a at the trench and jump of the trench axis will take place.
In such case, type "B" changes its plate from β to α, and accordingly the
Gravity Anomalies in the Western Pacific 415
Fig. 32. Role of "A" type seamounts and "B" type rises at a trench. Type "B"
changes its plate from α to β, md accordingly the "B" type rise changes its moving
direction.
"B" type rise changes its moving direction.The Philippine sea, especially its northern part, seems to be very complicated,
and the authors suggest that at least some complexities of the Philippine basin
are due to situation mentioned above.For example, Ogasawara islands including Chichijima and Hahajima islands
and Daito ridge are similar to each other from the view points of geochronology
(KANEOKA et al., 1970; OZIMA et al., 1980) and paleontology.If these islands and ridge are assumed to be separated by the opening of the
north Philippine basin, it seems difficult to explain why the inactive Ogasawara
islands and the Ogasawara trough now exist east of the active Iwojima islandson the Philippine plate. However, this fact may be explained as that the Ogasa-
wara islands which had previously belonged to the Marcus-Necker seamounts,changed their plate from the Pacific to the Philippine by eastward jumping of the
trench axis by collision of Ogasawara islands. Low heat flow at the Ogasawara
trough and westward penetration of Bouguer anomaly over the Ogasawara riseseem to support these hypothesis.
416 Y. TOMODA and H. FUJIMOTO
We wish to thank Professor Kazuo Kobayashi for many helpful discussions and for readingthe manuscript critically. We thank Professors Sadanori Murauchi, Toshi Asada and Toshi-
katsu Yoshii for helpful discussions on interpretation and evaluation of results of explosionseismology.
We thank Dr. Jiro Segawa, Dr. Kazuhiro Kitazawa, Messrs. Kin-ichiro Koizumi, TakaoIgarashi, Akinori Uchiyama, and Takeshi Matsumoto for their able assistance in gravity meas-
urement at sea.The R/V Hakuho-Maru is opened for all kinds of basic research for the ocean and therefore
only 13% of the whole cruise is available for solid geophysical use. To cover the West Pacific,measurement was carried out in almost all cruises, and we wish to thank chief scientists of the
cruises for giving us chances of gravity measurement even if the cruises were planned for fisherysciences, biology, chemistry, physical oceanography or meteorology.
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