Magnetism of Himalayan rocks reveals the mountains’ complex tectonic history

Breathing quickly in the thin mountain air, my colleagues and I set down our equipment. We are at the base of a jagged outcrop that protrudes upwards out of a steep gravel slope.

The muffled soundscape of the spectacular Himalayan wilderness is punctuated by a military convoy roaring along the Khardung-La road below. It is a reminder how close we are to the long-disputed borders between India, Pakistan and China which lie on the ridgelines just a few miles away.

This area also contains a different type of boundary, a narrow sinuous geological structure that stretches along the length of the Himalayan mountain range. Known as a suture zone, it is only a few kilometres wide and consists of slivers of different types of rocks all sliced together by fault zones. It marks the boundary where two tectonic plates fused together and an ancient ocean disappeared.

Our team of geologists travelled here to collect rocks that erupted as lava more than 60 million years ago. By decoding the magnetic records preserved inside them, we hoped to reconstruct the geography of ancient landmasses – and revise the story of the creation of the Himalayas.

Sliding plates, growing mountains

Tectonic plates make up the surface of Earth, and they are constantly in motion – drifting at the imperceptibly slow pace of just a few centimetres each year. Oceanic plates are colder and denser than the mantle beneath them, so they sink downward into it at subduction zones.

The sinking edge of the ocean plate drags the ocean floor along behind it like a conveyor belt, pulling the continents toward each other. When the entire ocean plate disappears into the mantle, the continents on either side plow into each other with enough force to uplift great mountain belts, like the Himalayas.

Geologists generally thought that the Himalayas formed 55 million years ago in a single continental collision – when the Neotethys Ocean plate subducted under the southern edge of Eurasia and the Indian and Eurasian tectonic plates collided.

But by measuring the magnetism of rocks from northwest India’s remote and mountainous Ladakh region, our team has shown that the tectonic collision that formed the world’s largest mountain range was actually a complex, multi-stage process involving at least two subduction zones.

Magnetic messages

The constant movement of our planet’s metallic outer core creates electric currents which in turn generate Earth’s magnetic field. It is oriented differently depending on where in the world you are. The magnetic field always points toward the magnetic north or the south, which is why your compass works, and averaged over thousands of years it points toward the geographic pole. But it also slopes downward into the ground at an angle which varies depending on how far you are from the equator.

When lava erupts and cools to form rock, the magnetic minerals inside the lock in the direction of the magnetic field of that location. So by measuring the magnetisation of volcanic rocks, scientists like me can determine what latitude they came from. Essentially, this method allows us to unwind millions of years of plate tectonic motions and create maps of the world at different times throughout geologic history.

Over multiple expeditions to the Ladakh Himalayas, our team collected hundreds of 1-inch diameter rock core samples. These rocks originally formed on a volcano active between 66 and 61 million years ago, around the time that the first stages of collision began.

We used a hand-held electric drill with a specially designed diamond coring bit to drill approximately 10 centimetres down into the bedrock. We then carefully marked these cylindrical cores with their original orientation before chiselling them out of the rock with nonmagnetic tools.

The aim was to reconstruct where these rocks originally formed before they were sandwiched between India and Eurasia and uplifted into the high Himalayas. Keeping track of the orientation of the samples as well as the rock layers they came from is essential to calculating which way the ancient magnetic field pointed relative to the surface of the ground as it was over 60 million years ago.

We brought our samples back to the MIT Paleomagnetism Laboratory and, inside a special room that is shielded from the modern-day magnetic field, we heated them in increments up to 680 degrees Celsius to slowly remove the magnetisation.

Different mineral populations acquire their magnetisation at different temperatures. Incrementally heating and then measuring the samples in this way enables us to extract the original magnetic direction by removing more recent overprints that might hide it.

Magnetic traces build a map

Using the average magnetic direction of the whole suite of samples we can calculate their ancient latitude, which we refer to as the paleolatitude.

The original single-stage collision model for the Himalaya predicts that these rocks would have formed close to Eurasia at a latitude of around 20 degrees north, but our data shows that these rocks did not form on either the Indian or the Eurasian continents. Instead, they formed on a chain of volcanic islands, out in the open Neotethys Ocean at a latitude of about eight degrees north, thousands of kilometres south of where Eurasia was located at the time.

This finding can be explained only if there were two subduction zones pulling India rapidly toward Eurasia, rather than just one.

During a geologic time period known as the Paleocene, India caught up with the volcanic island chain and collided with it, scraping up the rocks we eventually sampled onto the northern edge of India. India then continued northward before ramming into Eurasia around 40 million to 45 million years ago – 10 million to 15 million years later than was generally thought.

This final continental collision raised the volcanic islands from sea level up over 4,000 meters to their present-day location, where they form jagged outcrops along a spectacular Himalayan mountain pass.

Craig Robert Martin is a PhD student in Earth, Atmospheric and Planetary Sciences at Massachusetts Institute of Technology.

This article first appeared on The Conversation.