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Asteroid Bennu Mosaic OSIRIS-REx

This mosaic of asteroid Bennu was created utilizing observations made by NASA’s OSIRIS-REx spacecraft that was in shut proximity to the asteroid for over two years. Credit score: NASA/Goddard/College of Arizona

Just lately, scientists from NASA’s OSIRIS-REx mission found that floor regeneration happens on asteroids much more shortly than on Earth. By analyzing high-resolution pictures of rock fractures on asteroid Bennu taken by the Nature Geoscience is a monthly peer-reviewed scientific journal published by the Nature Publishing Group that covers all aspects of the Earth sciences, including theoretical research, modeling, and fieldwork. Other related work is also published in fields that include atmospheric sciences, geology, geophysics, climatology, oceanography, paleontology, and space science. It was established in January 2008.

” data-gt-translate-attributes=”[{” attribute=””>Nature Geoscience. “We were surprised to learn that the aging and weathering process on asteroids happens so quickly, geologically speaking.”

Although landslides, volcanoes, and earthquakes may abruptly alter the Earth’s surface, most changes occur gradually. Over millions of years, water, wind, and temperature changes slowly erode rock to create new surfaces. For instance, if you hiked into the Grand Canyon, you would see distinct rock layers; the top layers tend to be the youngest rocks, dating around 270 million years old, and the layers at the bottom of the canyon are the oldest, about 1.8 billion years old. The Colorado River has been chiseling away at rocks in the Grand Canyon for 5 million to 6 million years, according to the U.S. National Park Service.

Bennu Surface PolyCam

The PolyCam aboard NASA’s OSIRIS-REx spacecraft provided high-resolution, microscope-like images of asteroid Bennu’s surface. This made it possible for researchers to map more than 1,500 rock fractures. Credit: NASA/Goddard/University of Arizona

Rapid temperature changes on asteroid Bennu create internal stress that fractures and breaks down rocks, comparable to how a cold glass breaks under hot water. On Bennu, the Sun rises every 4.3 hours. At the equator, daytime highs can reach almost 260°F (about 127°C), and nighttime lows plummet to nearly minus 10°F (about minus 23°C).

OSIRIS-REx scientists spotted cracks in the rocks in spacecraft images from the first surveys of the asteroid. All of the fractures seemed to point in the same direction, “a distinct signature that temperature shocks between the day and the night could be the cause,” said Delbo.

Bennu Surface PolyCam Fractures Highlighted

Same image as above, but with the fractures highlighted in red. Credit: NASA/Goddard/University of Arizona

Delbo and his colleagues measured the length and angles of more than 1,500 fractures in OSIRIS-REx images by hand: some shorter than a tennis racket, others longer than a tennis court. They found the fractures predominantly align in the northwest-southeast direction, indicating they were caused by the Sun, which is shown here to be the primary force changing Bennu’s landscape.

“We were surprised to learn that the aging and weathering process on asteroids happens so quickly, geologically speaking.” — Marco Delbo

“If landslides or impacts were moving boulders faster than the boulders were cracking, the fractures would point in random directions,” said Delbo.

The research team used a computer model and their fracture measurements to calculate the 10,000- to 100,000-year timeframe for thermal fractures to propagate and split rocks.

“The thermal fractures on Bennu are quite similar to what we find on Earth and on

Reference: “Alignment of fractures on Bennu’s boulders indicative of speedy asteroid floor evolution” by Marco Delbo, Kevin J. Walsh, Christophe Matonti, Justin Wilkerson, Maurizio Pajola, Manar M. Al Asad, Chrysa Avdellidou, Ronald-Louis Ballouz, Carina A. Bennett, Harold C. Connolly Jr., Daniella N. DellaGiustina, Dathon R. Golish, Jamie L. Molaro, Bashar Rizk, Stephen R. Schwartz and Dante S. Lauretta, 23 Could 2022, Nature Geoscience.
DOI: 10.1038/s41561-022-00940-3

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