Space Travel News
TECTONICS
Alpine rock reveals dynamics of plate movements in Earth's interior
marker illustration only
Alpine rock reveals dynamics of plate movements in Earth's interior
by Staff Writers
Frankfurt, Germany (SPX) Oct 31, 2023

Geoscientists analyze rocks in mountain belts to reconstruct how they once moved downwards into the depths and then returned to the surface. This history of burial and exhumation sheds light on the mechanisms of plate tectonics and mountain building. Certain rocks that sink far down into Earth's interior together with plates are transformed into different types under the enormous pressure that prevails there. During this UHP metamorphosis (UHP: Ultra High Pressure), silica (SiO2) in the rock, for example, becomes coesite, which is also referred to as the UHP polymorph of SiO2.

Although it is chemically still silica, the crystal lattices are more tightly packed and therefore denser. When the plates move upwards again from the depths, the UHP rocks also come to the surface and can be found in certain places in the mountains. Their mineral composition provides information about the pressures to which they were exposed during their vertical journey through Earth's interior. Using lithostatic pressure as a unit of measurement, it is possible to correlate pressure and depth: the higher the pressure, the deeper the rocks once lay.

Until now, research had assumed that UHP rocks were buried at a depth of 120 kilometers. From there, they returned to the surface together with the plates. In the process, ambient pressure decreased at a stable rate, i.e. statically. However, a new study by Goethe University Frankfurt and the universities of Heidelberg and Rennes (France) calls this assumption of a long, continuous ascent into question. Among those involved in the study on the part of Goethe University Frankfurt were first author Cindy Luisier, who came to the university on a Humboldt Research Fellowship, and Thibault Duretz, head of the Geodynamic Modeling Working Group at the Department of Geosciences. The research team analyzed whiteschist from the Dora Maira Massif in the Western Alps, Italy. "Whiteschists are rocks that formed as a result of the UHP metamorphosis of a hydrothermally altered granite during the formation of the Alps," explains Duretz. "

What is special about them is the large amount of coesite. The coesite crystals in the whiteschist are several hundred micrometers in size, which makes them ideal for our experiments." The piece of whiteschist from the Dora Maira Massif contained pink garnets in a silvery-white matrix composed of quartz and other minerals.

"The rock has special chemical and thus mineralogical properties," says Duretz. Together with the team, he analyzed it by first cutting a very thin slice about 50 micrometers thick and then gluing it onto glass. In this way, it was possible to identify the minerals under a microscope. The next step was computer modeling of specific, particularly interesting areas.

These areas were silica particles surrounded by the grains of pink garnet, in which two SiO2 polymorphs had formed. One of these was coesite, which had formed under very high pressure (4.3 gigapascals). The other silica polymorph was quartz, which lay like a ring around the coesite. It had formed under much lower pressure (1.1 gigapascals).

The whiteschist had evidently first been exposed to very high and then much lower pressure. There had been a sharp decrease in pressure or decompression. The most important discovery was that spoke-shaped cracks radiated from the SiO2 inclusions in all directions: the result of the phase transition from coesite to quartz. The effect of this transition was a large change in volume, and it caused extensive geological stresses in the rock. These made the garnet surrounding the SiO2 inclusions fracture.

"Such radial cracks can only form if the host mineral, the garnet, stays very strong," explains Duretz. "At such temperatures, garnet only stays very strong if the pressure drops very quickly." On a geological timescale, "very quickly" means in thousands to hundreds of thousands of years. In this "short" period, the pressure must have dropped from 4.3 to 1.1 gigapascals. The garnet would otherwise have creeped viscously to compensate for the change in volume in the SiO2 inclusions, instead of forming cracks.

According to Duretz, the previous assumption that UHP rock reaches a depth of 120 kilometers seems less probable in view of this rapid decompression because the ascent from such a depth would take place over a long period of time, which does not equate with the high decompression rate, he says. "We rather presume that our whiteschist lay at a depth of only 60 to 80 kilometers," says the geoscientist. And the processes underway in Earth's interior could also be quite different than assumed in the past. That rock units move continuously upwards over great distances, from a depth of 120 kilometers to the surface, also seems less probable than previously thought.

"Our hypothesis is that rapid tectonic processes took place instead, which led to minimal vertical plate displacements." We can imagine it like this, he says: The plates suddenly jerked upwards a little bit in Earth's interior - and as a result the pressure surrounding the UHP rock decreased in a relatively short time.

Research Report:Garnet microstructures suggest ultra-fast decompression of ultrahigh-pressure rocks.

Related Links
Goethe University Frankfurt
Tectonic Science and News

Subscribe Free To Our Daily Newsletters
Tweet

RELATED CONTENT
The following news reports may link to other Space Media Network websites.
TECTONICS
Dual hydration of oceanic lithosphere
Shenzhen, China (SPX) Nov 08, 2023
This study is led by Dr. Jian Lin (Southern University of Science and Technology) and Dr. Fan Zhang (South China Sea Institute of Oceanology, Chinese Academy of Sciences). "Water is crucial to processes of both Earth's surface and interior, facilitating plate tectonics and making the Earth a habitable planet. Seawater penetrates into oceanic lithosphere through fractures on seafloor and migrates along faults and pores. The distribution of water governs the style of convective flow and distinct tectonic ... read more

TECTONICS
TECTONICS
Glow in the visible range detected for the first time in the Martian night

Cerberus Fossae Identified as Primary Source of Marsquakes

The Ones Who Make Curiosity Go: Sols 4001-4003

Curiosity rover clocks 4,000 sols on Mars

TECTONICS
University of Bern's LIMS Set to Uncover Moon's Mysteries in 2027

Astronaut who led humanity's first mission around the Moon dead at 95

Australian-Backed SPIDER Payload to Fly on Firefly's 2026 Lunar Mission

Propelling NASA closer to the Moon and Mars with Open Innovation

TECTONICS
Salts and organics observed on Ganymede's surface by June

New jet stream discovered in Jupiter's upper atmosphere

Uranus aurora discovery offers clues to habitable icy worlds

How NASA is protecting Europa Clipper from space radiation

TECTONICS
Yucatan underwater caves host diverse microbial communities

Major $200M gift propels scientific research in the search for life beyond earth

Webb findings support long-proposed process of planet formation

Scorching, seven-planet system revealed by new Kepler Exoplanet list

TECTONICS
SpaceX Falcon-9 rocket launches with telecommunications satellites aboard

HK, Macao add thrust to China's space exploration

UK and European Space Agency Commit Funding for Shetland Satellite Launch

ESA further boosts RFA One across Europe

TECTONICS
New scientific experimental samples from China's space station return to Earth

Shenzhou XVI crew return after 'very cool journey'

Chinese astronauts return to Earth with fruitful experimental results

Chinese astronauts return to Earth after 'successful' mission

TECTONICS
SwRI-led Lucy observes first-ever contact binary orbiting an asteroid

SwRI-led Lucy mission shows Dinkinesh asteroid is actually a binary

Dust's Pivotal Role in Dinosaur Extinction Highlighted by Study

In US capital, selfies with asteroid hinting at Earth's origins

Subscribe Free To Our Daily Newsletters




The content herein, unless otherwise known to be public domain, are Copyright 1995-2024 - Space Media Network. All websites are published in Australia and are solely subject to Australian law and governed by Fair Use principals for news reporting and research purposes. AFP, UPI and IANS news wire stories are copyright Agence France-Presse, United Press International and Indo-Asia News Service. ESA news reports are copyright European Space Agency. All NASA sourced material is public domain. Additional copyrights may apply in whole or part to other bona fide parties. All articles labeled "by Staff Writers" include reports supplied to Space Media Network by industry news wires, PR agencies, corporate press officers and the like. Such articles are individually curated and edited by Space Media Network staff on the basis of the report's information value to our industry and professional readership. Advertising does not imply endorsement, agreement or approval of any opinions, statements or information provided by Space Media Network on any Web page published or hosted by Space Media Network. General Data Protection Regulation (GDPR) Statement Our advertisers use various cookies and the like to deliver the best ad banner available at one time. All network advertising suppliers have GDPR policies (Legitimate Interest) that conform with EU regulations for data collection. By using our websites you consent to cookie based advertising. If you do not agree with this then you must stop using the websites from May 25, 2018. Privacy Statement. Additional information can be found here at About Us.