Scan reveals new clues into asteroid Bennu's surface, finding 'missing piece' for scientists

The research done into Bennu's surface will help future research into asteroid study.

The surface of asteroid Bennu has long left questions for scientists after a NASA planetary science mission showed the asteroid was actually more rough and jagged than previously expected.

NASA's Origins, Spectral Interpretation, Resource Identification and Security-Regolith Explorer (OSIRIS-REx) departed Earth in 2016 to collect samples of Bennu, a near-Earth asteroid.

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Images taken by NASA's Spitzer Space Telescope in 2007 indicated low thermal inertia, meaning Bennu's surface rapidly heated up and cooled down as it moved in and out of sunlight.

OSIRIS-Rex arrived in December 2018, and scientists were surprised to find that the asteroid was actually covered in large boulders, not smooth patches like researchers and the prior observations from Earth had shown, according to a report by NASA's Science Editorial Team

What this should've meant is the boulders held onto heat for long periods of time, not rapidly cooled down. 

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"We expected some boulders, but we anticipated at least some large regions with smoother, finer regolith that would be easy to collect. Instead, it looked like it was all boulders, and we were scratching our heads for a while," Andrew Ryan, a scientist with the University of Arizona’s Lunar and Planetary Laboratory, said in the report. 

OSIRIS-Rex collected its samples of Bennu and returned to Earth in 2023. Since then, NASA scientists and researchers have been studying the samples and collecting data from them to better understand the early solar system and how asteroids impact Earth.

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Multiple techniques were used by Ryan's team to study the samples.

A study published in Nature Communications showed that the boulders are indeed porous enough to account for some of the heat loss, but not all of it. Many of the boulders turned out to be riddled with cracks.

In order to determine if the cracks were the reason for the heat loss, more tests and research began. One such test, done by Nagoya University in Japan, used lock-in thermography to measure the sample's inertia.

The study revealed the thermal inertia to be much higher than what OSIRS-Rex recorded.

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NASA's Johnson Space Center in Houston conducted another test to determine how the boulders would behave on the asteroid, scaling up the operation.

Using a glove box, the team sealed samples in an airtight container under a protective nitrogen atmosphere, then transferred them to a lab where they could perform X-ray computed tomography, or XCT scans.

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After it was scanned, the particles were returned to the glove box.

"X-ray computed tomography allows us to look at the inside of an object in three dimensions, without damaging it," study co-author and NASA Johnson X-ray scientist Scott Eckley said in the report.

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The XCT scan created a permanent three-dimensional scan of the sample, including its shape and interior.

Ryan's team then used the XCT data to model heat flow and thermal inertia, scaling it up to boulder size. Doing this matched OSIRIS-REx's findings on Bennu, the report said.

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The samples revealed exactly what they needed to know.

"It turns out that they’re really cracked, too, and that was the missing piece of the puzzle," Ryan said.

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The research done into Bennu's surface will help future research into asteroid studies.

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