2019-07-01_Discover

(Rick Simeone) #1

42 DISCOVERMAGAZINE.COM


As the World Turns


The theory of plate tectonics took shape in


the 1960s after more precise seafloor maps


and seismic activity monitoring revealed


signs of our planet’s shifting shell. But the


ideas built upon those of early 20th-century


German scientist Alfred Lothar Wegener,


who proposed the theory of continental


drift: The large landmasses we know today


were once joined together in a superconti-


nent. Although first to describe the idea sci-


entifically, Wegener was not the first to think


it. Late 16th-century mapmaker Abraham


Ortelius theorized that the Americas, Africa


and Europe had been torn asunder by cata-


strophic geological events.


Researchers now believe continental


plates have come together more than once


in the deep past. While the very definition


of a supercontinent remains under debate,


researchers agree that many of these mon-


s ter landmas ses were large enough to aff ec t


global climate by shifting ocean and air cur-


rents. These climatic changes, along with


the raising of mountains and other geologi-


cal events driven by plate tectonics, created


new ecological systems that encouraged


species to spread and diversify.


Vaalbara: The First


Supercontinent?


When: Formed as early as 3.6 billion


years ago; broke up as late as 2.1 to


2.7 billion years ago.


What went where: Uncertain; remain-


ing pieces of it are found today in the


Pilbara Craton of Western Australia and


Kaapvaal Craton of southern Africa.


What’s so super about it: Want to


start a fight among geologists? Say


Vaalbara is the oldest supercontinent.


The truth is, most of the crust from


Earth’s early days has been subducted,


eroded or deformed beyond recogni-


tion. So reconstructions of the shape,


location and time frame of the first


supercontinent, however you define it,


remain theoretical and hotly contested.


It’s not yet possible to determine how


much continental crust existed this


far back in the geological record, or


whether large pieces of it were con-


nected. Some researchers consider


Kenor, which may have formed around


2.7 billion years ago, as the true first


supercontinent; others argue for the


earliest mass-merging of crust around
2 billion years ago but can’t agree on

whether to call it Columbia or Nuna.


Rodinia: The


Empty World


When: Formed around 1 billion years


ago; broke up around 750 million


years ago.


What went where: The landmass


was likely centered around the


North American Plate’s craton,


which may have been smashed


against what’s now East Antarctica


and southern Africa.


What’s so super about it: While


Rodinia was not the first superconti-


nent, it’s the earliest one that every-


one seems to agree existed — just


don’t ask what it looked like. Most of


what’s known about the superconti-


nent comes from fragmentary pieces


of its orogens: the edges of individual


continental plates that crunched


up, forming mountains, during mas-


sive collisions. We know little of its


overall shape beyond these crumple


zones, though researchers believe it


covered about 18 percent of Earth’s


surface area. (By comparison, our


planet’s modern land masses cover


about 29 percent.) It was a lonely
place, however; complex terrestrial

organisms did not yet exist.


Get a Move On


It’s unclear why our planet’s plates can’t stay put — or


when they started moving. After Earth formed about


4.6 billion years ago, its surface was a hot mess of


magma for a long time. Isotopic analysis of some of


the oldest known rocks suggests that continental


crust may have started forming as early as 4.4 billion


years ago, but the details and timing of the process


are unknown. Some researchers believe that, when


the magma finally cooled enough to form a crust,


it was a single, contiguous shell. But the mantle


beneath, still hundreds of degrees hotter than it is


today, may have melted and fractured the fragile crust


into pieces, or plates.


What set the plates in motion is still debated, but


most researchers think that subduction — when one


plate overrides another — explains why they remain


in motion. The immense force of the cooler, denser


plate being pushed down into the mantle creates tre-


mendous energy, which then circulates in a convective


flow, pushing up hotter, less dense magma that breaks


through to the surface along divergent boundaries.


Salt crystals left impressions in 3.5 billion-year-old mudstone, part of Western
Australia’s Pilbara Craton. The craton, a stable interior of a continental plate, may
be one of two remaining pieces of Vaalbara, a theoretical supercontinent. The
other piece, the Kaapvaal Craton, is in southern Africa.

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PLATE TECTONICS


EVERYTHING


WORTH


KNOWING

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