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Title: The Evolution of the Lau Basin, FijiTonga


1
The Evolution of the Lau Basin, Fiji-Tonga
  • Andrew M. Goodliffe
  • Department of Geological Sciences
  • University of Alabama

DGS Brown Bag Seminar, April 7, 2004
2
  • Outline
  • Location of the Lau Basin
  • Brief explanation of backarc basins
  • Data types involved
  • Data collection
  • Explanation of the evolution of key parts of the
    Lau Basin
  • Overview and conclusions

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4
  • A simple model for the growth of a backarc basin
  • Formation of arc
  • Arc breakup with some magmatism
  • Initiation of seafloor spreading
  • Karig 1970 proposed that the Lau Basin was a
    young ocean basin formed by the splitting of an
    island arc.
  • Lawver et al. 1976 proposed that rather than
    forming by conventional seafloor spreading, the
    Lau Basin formed by diffuse deformation and
    magmatism.
  • Taylor et al. 1996 showed that the growth of
    the Lau Basin was formed by conventional seafloor
    spreading.

From Taylor, 1993
5
  • Three main data types will be included in this
    presentation
  • Bathymetry (detailed kinematics from abyssal hill
    fabric)
  • Swath, multibeam, wide beam, predicted, digitized
    charts
  • Magnetic (seafloor age, kinematics)
  • Magnetic anomaly, magnetization
  • Acoustic Imagery (where is the neovolcanic zone,
    active faulting)
  • Sidescan, beam amplitude

6
  • R/V Moana Wave
  • Seafloor mapping (shallow and deep towed)
  • Dredging, coring
  • Magnetic and gravity surveys
  • Single channel seismics
  • Physical oceanography
  • Good food

7
  • R/V Hakurei-Maru No. 2
  • Similar facilities to the R/V Moana Wave
  • Additional seafloor imaging facilities (next
    slide)
  • Food subject to interpretation

8
An example of data types collected aboard a
typical research vessel.
9
Bathymetry
(b) Narrow beam echosounder
(a) Conventional widebeam echosounder
From SeaBeam operators manual
(d) Multibeam
(c) Unstabilized narrow beam echosounder
10
  • Transmit array is long in fore-aft direction,
    creating a narrow beam in the port-starbord
    direction.
  • Receive array is long in the port-starboard
    direction, creating a series of beams that are
    long in the fore-aft direction.
  • In addition to bathymetry, the amplitude of the
    returning signal is recorded, giving an
    indication of seafloor hardness.
  • Susceptible to heavy seas

11
  • The HAWAII-MR1 (Hawaii Wide-Angle Acoustic
    Imaging Instrument) is a towed interferometric
    swath mapping system.
  • Both sidescan and bathymetry data are recorded.

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13
  • Towed behind a depressor weight which is in turn
    attached to the ship -- decouples the system from
    the ships motion.
  • The system is towed beneath the mixed layer
    (60-100 m)
  • Operates better in heavy seas than most scientists

14
  • In a conventional sidescan system a single
    transducer array measures traveltime after the
    transmission of a signal.
  • In the HAWAII-MR1 system two arrays are arranged
    in parallel
  • The phase difference between the same signal
    received at each array indicates the angle from
    which that signal came.
  • This permits the calculation of depth in addition
    to traveltime and amplitude.
  • Pairs of arrays are mounted on each side of the
    system. The port pair operates at 11 kHz, and the
    starboard pair at 12 kHz
  • Bathymetry swath width is in excess of 3.4 times
    water depth (water depth 2.5 km, swath width
    8.5 km).
  • Sidescan swath width is in excess of 7.5 times
    water depth.

Courtesy of Mark Rognstad, University of Hawaii.
15
  • Marine magnetic data is typically collected using
    a towed proton precession magnetometer.
  • Consists of a coil wrapped around a hydrogen rich
    liquid (water, oil)
  • When a current is applied to the coil the protons
    align themselves with the induced magnetic field.
  • When the current is switched off the protons
    revert to the direction of the earths magnetic
    field by the process of precession.
  • This generates a sinusoidal current in the coil,
    the frequency of which is directly related to the
    strength of the magnetic field.
  • Sharks love them

16
(a)
(b)
  • As the Lau Basin is close to the magnetic equator
    and the seafloor lineations trend approximately
    N-S (a), the amplitude of the magnetic anomalies
    is low.
  • Skewness complicates interpretation (ie peak of
    anomaly is not over the source).
  • Reduction to the pole (b) or the calculation of
    the seafloor magnetization (if bathymetry is
    available) helps in the interpretation of
    magnetic anomalies.
  • Early interpretations of the evolution of the Lau
    Basin were limited due to the failure to
    interpret the magnetic anomalies correctly, and
    led to the erroneous interpretation that there
    was no organized seafloor spreading in the basin.

17
Total field magnetic anomaly
Seafloor magnetization
18
Overview of the Evolution of the Lau Basin
  • The basement is Middle Eocene to Early
  • Oligocene arc terrain.
  • Beginning at 10 Ma, the Fiji platform
  • underwent a counterclockwise rotation of
  • 21o to 13517.5o James and Falvey, 1978
  • Inokuchi, 1992 Taylor et al., 2000.
  • Rotation had stopped by 3 Ma, probably
  • coinciding with the start of E-W spreading
  • on the ELSC at gt 3.6 Ma.
  • All reconstructions i.e. Taylor et al.,
  • 2000 ignore the SE motion of the Tonga
  • platform along the Peggy Ridge (PR)
  • transform fault. The magnitude of this
  • motion is uncertain.

19
  • Present day plate motion relative to a fixed
    Australian plate.
  • Present day plate boundaries.

20
WEP Western Extensional Province. ELSC East
Lau Spreading Center. VFR Valu Fa Ridge. PR
Peggy Ridge. MTJ Mangatolu Triple
Junction. FOSC Fonualei Spreading
Center. NWLSC Northwest Lau Spreading
Center. FSC Futuna Spreading Center. LETZ
Lau Extensional Transform Zone
21
  • Parson et al. 1992 proposed a rifted arc origin
    for the WEP based on ODP results and deep graben
    seen in sparse profiles.
  • The more detailed morphology available today is
    consistent with a spreading origin.
  • 3-D magnetization solution shows distinct and
    continuous magnetic anomalies.
  • 3.5 Ma MORB basement was recovered at site 835.
  • This graben was formed by a propagating spreading
    center.
  • This age is consistent with that predicted by the
    magnetization solution (2An.3n, 3.33-3.58 Ma).
  • 5.6 Ma MORB recovered at site 834 is consistent
    with seafloor spreading origin.
  • Crustal thickness from refraction is consistent
    with a seafloor spreading origin (Crawford et
    al., 2002).

Western Extensional Province
22
East Lau Spreading Center and Valu Fa Ridge
  • ELSC originated in the north prior to 3.5 Ma and
    propagated south.
  • The northern segments have progressively died.
  • The only currently active segments are in the
    south

23
  • The depth and cross section of the spreading
    center changes dramatically with latitude.
  • The rock types change from MORB in the north to
    andesites in the south as the spreading center
    gets closer to the arc.
  • Similar changes with distance from axis.
  • Multiple segments, rapid dualing propagators

24
Black and white smokers, andesites, mussel beds,
bacterial mats, shrimps, barnacles.
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26
Fonualei Spreading Center and Mangatolu Triple
Junction
  • Crust as old as Chron 2A (2.58-3.58 Ma) is
    identified on either side of the FOSC and MTJ.
  • The present spreading center, as identified in
    acoustic imagery, cross-cuts Brunhes Chron crust
    (0-0.78 Ma) in the north, showing that this part
    of the spreading center has recently reoriented.
  • The FOSC is currently propagating in the the
    active arc and creating a 1000 m relief graben.

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28
Central Lau Spreading Center and Peggy Ridge
  • PR initiated prior to the CLSC, probably linking
    the ELSC with a spreading center to the
    northwest.
  • The CLSC initiated between 0.78 and 1.77 Ma, but
    probably closer to 0.78 Ma.
  • The LETZ formed by 0.78 Ma. It cut the corner
    formed by the CLSC and PR, shortening the active
    section of the PR.
  • The CLSC is currently propagating south at the
    expense of the ELSC (up to 320 km/Myr).

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30
  • Highly complex seafloor.
  • The relationship of the many spreading centers is
    unclear.

31
Overview and Conclusions
32
R/V Moana Wave in Pago Pago harbor, American
Samoa.
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