Now we can sample other planets without leaving home
Published in Nature Communications
Five to ten million years ago an asteroid smashed into Mars. It created a massive crater and propelled a chunk of ancient Martian crust into space as a new meteorite, which eventually crashed into Africa.
We now know where on Mars that meteorite came from, thanks to a supercomputer-powered technology that allows us to explore the geology of planets without leaving home.
Remains of meteorite NWA 7034, known as Black Beauty, were discovered in Western Sahara in 2011. The story of its creation is told for the first time in Nature Communications by a global team led by researchers from Curtin University, supported by the Pawsey Supercomputer in Perth, Australia, and with colleagues in France, Côte d’Ivoire, and the United States.
Black Beauty is formed of Martian rocks formed nearly 4.5 billion years ago when the crusts of both Earth and Mars were still young. Now we know the source of Black Beauty, researchers can use it to compare the formation of Mars and Earth.
The technology behind the discovery will be used to identify the source of other Martian meteorites but also to identify billions of impact craters on the surface of Mercury and the Moon. More than 300 Martian meteorites have been found on Earth to date.
Researchers named the crater Karratha after a city in Western Australia that is home to one of the Earth’s oldest rocks. The team want NASA to prioritise the area around Karratha Crater as a future landing site on Mars.
The source of the rocks on Mars was found by analysing thousands of high-resolution planetary images from a range of Mars missions.
The team identified about 90 million impact craters by running a machine learning algorithm on one of the fastest supercomputers in the Southern Hemisphere, at the Pawsey Supercomputing Research Centre. The algorithm was partially developed by Kosta Servis, a senior data scientist at the Centre.
The research was led by Dr Anthony Lagain, from Curtin University’s Space Science and Technology Centre, with co-authors from Paris-Saclay University, Paris Observatory, Muséum National d’Histoire Naturelle, the French National Centre for Scientific Research, the Félix Houphouët-Boigny University, Côte d’Ivoire, and Northern Arizona University and Rutgers University in the US.
Captions and credits top to bottom
- The distribution of 90 million craters on the surface of Mars obtained from the Crater Detection Algorithm. Colours indicate crater size and their intensities are linked to the crater density on the surface. Blue spots and rayed patterns are associated with the youngest and largest craters formed on the surface. The red circle pinpoint the Karratha crater that has ejected the Black Beauty meteorite. Credit: Lagain et al. 2022, Nature Communications.
- Mars meteorite analysis. Left, artistic impression of where an asteroid hit the surface of Mars 5-10Ma ago, ejected Black Beauty and its transit to the Earth (white line). On the right, the dataset and methods used to identify the ejection site of the meteorite.
- The Black Beauty meteorite, source NASA.
- Karratha Crater on Mars, source NASA MRO.
- Dr Anthony Lagain, Curtin University.
- Kosta Servis, Pawsey Supercomputing Research Centre.
- For use in news stories associated with this paper only
For media and interview requests, contact:
- Karina Nunez, +61 430 429 120, firstname.lastname@example.org
- Niall Byrne, +61 417 131 977, email@example.com
For Curtin University:
Yasmine Phillips, Media Relations Manager, Curtin University
+61 8 9266 9085, +61 401 103 877
‘Early crustal processes revealed by the ejection site of the oldest martian meteorite’,
Nature Communications, 12 July 2022,
A. Lagain1*, S. Bouley2,3, B. Zanda3,4, K. Miljković1, A. Rajšić1, D. Baratoux5,6, V. Payré7, L. S. Doucet8, N. E. Timms1,9, R. Hewins4,10, G. K. Benedix1,11,12, V. Malarewic2,4, K. 4 Servis1, P. A. Bland1.
1 Space Science and Technology Centre, School of Earth and Planetary Science, Curtin University: 8 Perth, Australia.
2 Université Paris-Saclay, CNRS, GEOPS: 91405, Orsay, France
3 IMCCE, Observatoire de Paris, 77 avenue Denfert-Rochereau, 75005 – Paris
4 Institut de Minéralogie, de Physique des Matériaux et de Cosmochimie (IMPMC),
Muséum national d’Histoire naturelle, Sorbonne Université et CNRS: 75005, Paris, France
5 Géosciences Environnement Toulouse, University of Toulouse, CNRS and IRD,
Toulouse, 31400, France
6 Université Félix Houphouët-Boigny, Abidjan, Côte d’Ivoire.
7 Department of Astronomy and Planetary Science, Northern Arizona University: Flagstaff, Arizona, USA
8 Earth Dynamics Research Group, TIGeR, School of Earth and Planetary Sciences, Curtin University: Perth, Western Australia, Australia
9 The Institute for Geoscience Research (TIGeR), Curtin University: Perth, 6845, WA, Australia
10 EPS, Rutgers University: Piscataway, NJ 08854, USA 22
11 Department of Earth and Planetary Sciences: Western Australian Museum, WA, Australia
12 Planetary Sciences Institute: Tucson, Arizona, USA
13 Pawsey Supercomputing Centre, CSIRO: Kensington, WA, Australia
*Corresponding author. Email: firstname.lastname@example.org
The formation and differentiation of the crust of Mars in the first tens of millions of years after its accretion can only be deciphered from incredibly limited records.
The martian breccia NWA 7034 and its paired stones is one of them. This meteorite contains the oldest martian igneous material ever dated: ~4.5 Ga old. However, its source and geological context have so far remained unknown.
Here, we show that the meteorite was ejected 5-10 Ma ago from the north-east of the Terra Cimmeria – Sirenum province, in the southern hemisphere of Mars. More specifically, the breccia belongs to the ejecta deposits of the Khujirt crater formed 1.5 Ga ago, and it was ejected as a result of the formation of the Karratha crater 5-10 Ma ago.
Our findings demonstrate that the Terra Cimmeria – Sirenum province is a relic of the differentiated primordial martian crust, formed shortly after the accretion of the planet, and that it constitutes a unique record of early crustal processes.
This province is an ideal landing site for future missions aiming to unravel the first tens of millions of years of the history of Mars and, by extension, of all terrestrial planets, including the Earth.
The Pawsey Supercomputing Research Centre is a world-class high-performance computing facility accelerating scientific discoveries for Australia’s researchers. Named for Australian scientist Joseph Pawsey, known as one of the pioneers of Australian radio astronomy for his work in the field of interferometry, the Centre enables science and accelerates discovery, by contributing to the delivery of globally significant research. Pawsey is currently serving over 40 organisations and achieving unprecedented results, in domains such as radio astronomy, energy and resources, engineering, bioinformatics and health sciences.
The Pawsey Centre is an unincorporated joint venture of CSIRO – Australia’s national science agency, Curtin University, Edith Cowan University, Murdoch University and The University of Western Australia. Pawsey is funded by the Australian Government under the National Collaborative Research Infrastructure Strategy (NCRIS), the Western Australian Government and its partner organisations.