Award Abstract # 1635909
4D physical models of migrating mid-ocean ridges: Implications for shallow mantle flow, melt distribution and seafloor topography

NSF Org: OCE
Division Of Ocean Sciences
Recipient: UNIVERSITY OF RHODE ISLAND
Initial Amendment Date: September 15, 2016
Latest Amendment Date: June 8, 2021
Award Number: 1635909
Award Instrument: Standard Grant
Program Manager: Kevin Johnson
ktjohnso@nsf.gov
 (703)292-7442
OCE
 Division Of Ocean Sciences
GEO
 Directorate for Geosciences
Start Date: September 15, 2016
End Date: August 31, 2022 (Estimated)
Total Intended Award Amount: $357,747.00
Total Awarded Amount to Date: $357,747.00
Funds Obligated to Date: FY 2016 = $357,747.00
History of Investigator:
  • Christopher Kincaid (Principal Investigator)
    kincaid@uri.edu
  • Robert Pockalny (Co-Principal Investigator)
Recipient Sponsored Research Office: University of Rhode Island
75 LOWER COLLEGE RD RM 103
KINGSTON
RI  US  02881-1974
(401)874-2635
Sponsor Congressional District: 02
Primary Place of Performance: University of Rhode Island
215 South Ferry Rd.
Narragansett
RI  US  02882-1197
Primary Place of Performance
Congressional District:
02
Unique Entity Identifier (UEI): CJDNG9D14MW7
Parent UEI: NSA8T7PLC9K3
NSF Program(s): Marine Geology and Geophysics
Primary Program Source: 01001617DB NSF RESEARCH & RELATED ACTIVIT
Program Reference Code(s): 1620, 9150
Program Element Code(s): 162000
Award Agency Code: 4900
Fund Agency Code: 4900
Assistance Listing Number(s): 47.050

ABSTRACT

Plate tectonics and planetary convection in the form of mid-ocean ridge spreading, plate subduction and mantle plumes drive the natural mass/energy cycling of the solid earth-hydrosphere-atmosphere system over geological time scales and provides important context for present day global climate change. It is estimated that roughly half of the carbon provided to the hydrosphere/ atmosphere from magmatic processes generated by these geological drivers is attributed to plate spreading of the world's 80,000 km long mid-ocean ridge system. This project will use a physical laboratory apparatus to develop improved models of convective mantle flow driving plate motion and magmatic production beneath mid-ocean ridges by characterizing the essential processes not only in 3-dimensions but also their time evolution. Previous models that attempt to connect mantle flow, magma production and mass/energy flux to Earth's oceans/atmosphere have typically only been conducted in two-dimensions. The combination of recent geological and geophysical data and model upgrades clearly show that 2D model representations are insufficient. The project includes support for a graduate student and research opportunities for undergraduates from under-represented groups including local native american students through the Research Experience for Undergraduates program at the University of Rhode Island. Physical models will also provide a visually accessible experience of deep earth processes for university, school and public outreach audiences.

This project will design and construct geodynamic models that build and expand on established and tested laboratory apparatus for exploring the essential four-dimensional processes related to mid-ocean spreading ridges. While numerical models suffer from resolution issues and are approximations to a set of governing equations with errors that are usually entirely unknown, physical models are particularly useful as they permit high resolution 3D physics with a natural time dependency in regions of interest (e.g. in the melt generation regions beneath ridges) and allow model boundary artifacts to be minimized. The project will investigate both basic ridge geometries and models with more complex attributes such as mid-ocean ridge migration and its role on upper mantle dynamics, seafloor topography, and mid-ocean ridge magmatic processes. This new lab apparatus will investigate several previously proposed but untested models: (1) asymmetric upwelling of the upper mantle below the leading tectonic plate, (2) asymmetric distribution of seamounts across migrating mid-ocean ridge systems, (3) magmatic segmentation and melt scavenging of offset mid-ocean ridges, and (4) enhanced upwelling at ridge-transform intersections. The design of the migrating ridge apparatus will allow transform offsets, spreading rates, and migration vectors that can scale to the full spectrum of known mid-ocean ridge systems. The laboratory model and suite of modeling results will provide a unique test of the 4D character of mid-ocean ridges and provide insight into geodynamic and melting processes at mid-ocean spreading centers. Results are expected to have important implications for understanding fundamental mantle processes and how these influence mass/energy fluxes to the hydrosphere/atmosphere systems on geologic time scales. These models will also provide important benchmarks for related fields, such as mantle properties, seismic tomography and estimates of absolute plate motions.

PROJECT OUTCOMES REPORT

Disclaimer

This Project Outcomes Report for the General Public is displayed verbatim as submitted by the Principal Investigator (PI) for this award. Any opinions, findings, and conclusions or recommendations expressed in this Report are those of the PI and do not necessarily reflect the views of the National Science Foundation; NSF has not approved or endorsed its content.

This project has focused on studying how mid-ocean ridges move over geologic time and what that means for the source region of erupted lavas on the seafloor. The Earth’s surface layer, the crust, is broken into many tectonic plates that move with respect to one another over millions of years. Where two tectonic plates separate from each other, mid-ocean ridges form. These seafloor volcanic mountain chains continually create new crust - 21 cubic kilometers per year, or about ⅓ of the volume of the most voluminous mountain in the world, Mauna Loa in Hawaii. They also drift across the surface of the Earth over time in a process called migration. This happens due to the collective motion of all the plates on a spherical globe, coupled with the fact that there are differences in density in the upper Earth layers. Understanding mid-ocean ridge migration is important for our understanding of plate tectonics on Earth, which subsequently ties into many other key topics, such as climate change and carbon cycling, the presence of water on Earth, geohazards like earthquakes and volcanic eruptions. 

 

Other methods have struggled to simulate this process, namely because our computing abilities still lack for such a complex problem, but also because data collection and physical observations are so difficult to obtain for such a remote part of the Earth. For this work, we have used a scaled laboratory model that is capable of mimicking a migrating mid-ocean ridge. This works by dragging (the migration component) a set of conveyor belts (which act as the tectonic plates) over the surface of a tank full of viscous corn syrup (representing the Earth’s second layer, the mantle). We analyze time-lapse movies taken during experiments and track tiny beads in the syrup to find patterns in the speed and direction of the flow. 

 

A key finding is that ridge migration fundamentally alters where mantle is drawn to the ridge from. By performing approximately 120 experiments, we have been able to simulate how the mantle flows in 3-D over ~50 million year timescales beneath a mid-ocean ridge. We compare experiments with a stationary ridge to experiments with a migrating ridge, and we assess how the migration speed and direction influence the resulting speed and direction of flow.    the source region in the mantle for newly erupted lavas at mid-ocean ridges is much shallower than was previously thought. Instead of sourcing rock thousands of kilometers directly beneath the ridge, our work shows that rock is sampled from shallow depths and from across large horizontal areas. This finding relates to how we interpret the layering and composition of the Earth’s interior.

 

We also look at how heating from the Earth’s core causes hot pulses of mushroom-cloud shaped material to rise towards the surface. These features, called plumes, rise through the mantle because they are less dense than the surrounding rock, but they are also incredibly sensitive to the mantle flow of that surrounding rock. In our experiments, we show that plumes are distorted when a ridge migrates over the top, causing hot plume rock to erupt to either side of the mid-ocean ridge. In fact, the faster the mid-ocean ridge migrates, the more deformed the plume becomes and the less likely it is to cause volcanic eruptions at the surface.

 

Over the course of this project, we have had as many as 300 visitors to the lab per year. Some of the key facts that we have found to be most interesting for guests are as follows:

  • Tectonic plates can crash into one another, move alongside one another, or separate from one another. In the Atlantic ocean where the plates separate from one another, the entire ocean basin is actually getting wider over time.

  • Mid-ocean ridges create new seafloor at roughly the speed at which your fingernails grow, so this is a very slow process!

  • The entire underwater mid-ocean ridge volcanic mountain chain is long enough to wrap around the Earth twice.

  • Corn syrup is very viscous, which means that it’s gooey and doesn’t want to flow as easily as (for example) water. Rock inside the Earth moves over millions of years, so it’s a lot like a viscous fluid. This is the basis for our experimental setup.

  • When these mid-ocean ridges migrate (or drift) across the surface of the Earth, it’s a little like dragging a vacuum cleaner over a thick shag carpet. If the vacuum cleaner is held in one place for a long time, it can suck up dirt buried deep inside the carpet. But if the vacuum cleaner is moved around, it sucks up dirt only from the surface of the carpet, and over a much larger area. Of course mid-ocean ridges aren’t really “sucking up” mantle rock to make new seafloor, but you can think of our findings similarly.

 

 


Last Modified: 12/12/2022
Modified by: Christopher R Kincaid

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