An impact crater on Earth can be traced back to the asteroid belt object Vesta

The crater in Turkey originated from a fragment of Vesta that was expelled 22 million years ago


A collision on asteroid Vesta that created the U-shaped Antonia impact crater 22 million years ago produced the meteorites that fell near the village of Sariçiçek in Turkey in 2015, according to an international team of 79 researchers. Their 56-page study is published in the journal Meteoritics & Planetary Science.

“We visited Sariçiçek shortly after the fall,” says Ozan Unsalan, lead author and planetary scientist from Ege University in Izmir, Turkey. “The villagers and scientists from nearby Bingöl University provided meteorites for study and mapped the location of 343 finds.”

The meteorites were found to be of a type called howardite, part of a clan of meteorites called howardite-eucrite-diogenites (HED).

The meteorites reflect light much like asteroid Vesta and its family of Vestoids. 525-kilometre (326-mile) Vesta is the second largest body in the asteroid belt. The 0.8 to eight kilometre (0.5 mile to five mile) sized Vestoids are fragments from a massive collision that created the Rheasilvia impact basin on Vesta.

“Scientists have long suspected that HED meteorites originate from Vesta or its Vestoids, but were unable to point to a specific impact site,” says Takahiro Hiroi of Brown University, United States, who measured the reflectance properties of the meteorites.

About one third of all HED that fall to Earth were created in a collision 22 million years ago.

“Isotopic studies showed Sariçiçek belongs to this most common group of HED meteorites,” says Qing-zhu Yin, a cosmochemist at UC Davis in California.” Sariçiçek meteorites must have come from a significant collision.”

Noble gas studies showed that the terrain surface where the collision happened was covered in howardite material like Sariçiçek prior to this collision, and was refreshed by impacts or landslides 13 million years earlier.

“This meteorite sat just below the surface of a larger asteroid for about 13 million years before the collision happened,” says Matthias Meier, a geochemist at ETH Zürich in Switzerland. “It was exposed to solar wind, leaving telltale noble gases.”

This fall was the first time that a common HED was photographed impacting Earth.

“We used video security camera footage in nearby cities to determine the meteor’s trajectory and orbit,” says Peter Jenniskens, a SETI Institute researcher at NASA Ames Research Center, who participated in the field study to investigate the meteorite’s origins. “The orbit provided the first dynamical link between the normal HED meteorite clan and the inner main belt where Vesta is located.”

NASA’s Dawn spacecraft was at Vesta from July 2011 to September 2012 before moving onto the dwarf planet Ceres. Image credit: NASA/JPL/MPS/DLR/IDA/D. Macháček

The meteoroid was about one metre (three foot) in size when it entered Earth’s atmosphere at a speed of 17 kilometres (11 miles) per second from a north-western direction. It fragmented at an altitude of 27 kilometres (17 miles), based on how the meteorites were scattered near the village of Sariçiçek.

“With the information about how the meteoroid broke into fragments and how often HED meteorites fall to Earth, we calculated that the source crater on Vesta needed to be at least 10-kilometre (six-mile) in diameter,” says Jenniskens. “Most material ended up in meteoroids 0.25 to 1.25 metres (0.8 to 4.1 feet) in size.”

Alternatively, a Vestoid of at least a kilometre in size could have broken into such small pieces, but Jenniskens found that even after adding up all Vestoids it was more likely that the much larger Vesta itself got hit.

Vesta was visited by NASA’s DAWN spacecraft in 2011 and 2012, when many impact craters were photographed. A number of craters still showed the material excavated in the impact scattered in a curtain around the crater, suggesting these are the youngest craters.

“We counted the small craters on those curtains and used the expected rate of small impacts to estimate the age of each crater,” says Nico Schmedemann of the Max Planck Institute for Solar System Research in Göttingen, Germany.

One crater stood out, named Antonia. This 16.7-kilometre (10.4-mile) diameter crater is relatively large and has the right age of 22 million years.

Antonia is located in the Rheasilvia impact basin and is covered by Sariçiçek-like rubble from landslides of nearby terrain surface material. The age of the terrain, based on crater counts is about two billion years.

“It turns out that the terrain age also matches that derived from the lost helium in Sariçiçek,” says Meyer. “Many small impacts caused that noble gas to be lost from the meteorites.”

Knowing their source crater makes the Sariçiçek meteorites, and the other HED meteorites from that 22 million year old impact, a convenient sample return from Vesta.

“Because Antonia is in the Rheasilvia impact basin, we can now study the physical properties of Sariçiçek to learn more about the dangerous Vestoids that sometimes impact Earth,” says Jenniskens.” That may help us understand what to do when a Vestoid is discovered on approach to Earth.”

Keep up to date with the latest news in All About Space – available every month for just £4.99. Alternatively you can subscribe here for a fraction of the price!

Tags: , , , , , , , , ,