We received this interesting question submitted through our blog at http://the-earth-story.com/ (Seriously, visit & follow us, I just paid the fee to reregister the domain name).
“I have a question I was hoping you guys might be able to explain, please. I'm fascinated by plate tectonics, and reconstructing ancient continents, but how do they do it? I get the principle of 'rewinding' current continental movement to get to Pangaea, but how can they produce a map of, say, the Ordovician or the Precambrian, and say with any certainty that's how the continents were arranged so far back in time?”
To use that term, “rewinding” the Atlantic Ocean is pretty easy, you just have to move the continents back together like puzzle pieces. However, the Pacific and Indian Oceans are much tougher; you can’t easily tell exactly how places like Antarctica and Australia fit together, and parts of Asia were only assembled out of volcanic arcs over the last 250 million years.
To fit these plates back together, we use magnetic anomalies on the seafloor. Every few hundred thousand years on average, the Earth’s magnetic field flips, switching the North and South Poles. If we tow an instrument called a magnetometer behind a boat and measure areas where the magnetic field in the ocean is strong and weak, we get a measurement that tells us the orientation of mid-ocean ridges and how they were moving.
Igneous rocks contain minerals like magnetite that record the direction of the magnetic field when they formed. When a magnetic mineral cools through its Curie Temperature, it picks up whatever magnetic field is present and locks that magnetic field in. The rocks of the ocean floor therefore record the flips between north and south; if they are measured across the ocean floor they provide a record of the motion of any oceanic plate.
The oldest oceanic crust on Earth is Jurassic in age, about 200 million years old. By measuring oceanic magnetic anomalies we can therefore project the motion of the continents going as far back as 200 million years, about the time Pangaea began breaking apart.
This image, however, is a reconstruction of Rodinia, a proposed supercontinent 700 million years ago. How on Earth do we get information going back that far?
Part of the answer is continents. Igneous rocks that form on continents also record the ambient magnetic field and point to the North Pole as well. Sedimentary rocks on a continent also record the magnetic field since magnetic minerals in sediments adjust to the magnetic field while they flow in water. But, not only will those rocks tell you about magnetic flips, other properties of magnetism can be measured as well.
The magnetic field in a rock points towards the pole whenever it forms. If you measure the preserved magnetic field in rocks of different ages on a single continent, all of them point to the same North Pole. If the observed North Pole changes over time and a continent is actually solid, then any change in the North Pole direction is actually reflecting movement or rotation of the continent. Measuring the changes in North Pole direction within a continent produces a curve called an “apparent polar wander” curve – a measurement of how the continent has moved assuming the pole is actually fixed.
This gives us several new tools. For example, if 2 continents show a similar apparent polar wander curve over several hundred million years, you can project that they were likely joined together at that time (see more here: http://tmblr.co/Zyv2Js1LJUEUa).
Magnetics also gives another piece of information: inclination. We’re used to magnetic declination; that’s what a standard handheld compass measures, the angle to the North Pole. Although a normal compass can’t measure it, the Earth’s magnetic field also dips up and down. The dip of the magnetic field can tell the latitude of a continent. Steep magnetic inclinations means a rock formed at high latitudes near the pole, and shallow magnetic inclinations means a rock formed near the equator.
Therefore, using magnetic measurements on continents, we can tell where continents sat even without oceanic crust. However, none of these measurements are as good as oceanic north/south anomalies, so there are larger errors. Furthermore, sometimes you just don’t have the right rocks; if rocks are metamorphosed or eroded it will destroy previous magnetic information.
To build upon that measurement, you can use plate tectonic information. If you can match mountain ranges from one continent to another, you can come up with better estimates of which continents were in contact. If you find limestones, which commonly form in warm waters near the tropics, you can estimate that a continent must have been near the equator even if the rocks don’t have a strong magnetic signal. If you find glacial sediments, a continent must have been near the poles.
None of those are perfect. In fact, there is variation even in reconstructions of continental movement over the last 200 million years. Even when we have oceanic magnetic anomalies it isn’t always clear how continents moved; 2 different groups trying to reconstruct continental motion over the past 200 million years will often find important differences.
Even farther back in time the differences increase. There are some scientists who have argued that the supercontinent Rodinia didn’t even exist. However, enough scientists have argued for it that its name is well known and has its own Wikipedia entry.
That’s the way ancient continental movements have been reconstructed. Continent collisions leave a record in rocks. Continental motions leave a paleomagnetic record. However, there are gaps. There are proposals for multiple supercontinents before Rodinia, but those are even more poorly constrained and less accepted. One proposal even argues based on ancient paleomagnetic measurements that all the continental cores originally formed as one supercontinent and rifted apart, but ideas like that will remain controversial until we figure out ways to produce much better evidence than what we currently have.
Image credit: https://en.wikipedia.org/wiki/Rodinia#/media/File:Rodinia_reconstruction.jpg
References: http://www.sciencedirect.com/science/article/pii/S0040195113000267 http://www.utm.utoronto.ca/~w3gibo/How%20to%20do%20field%20studies/properties_of_magnetic_field_at_.htm http://austhrutime.com/rodinia.htm http://www.earth.ox.ac.uk/~conallm/Rodinia.pdf