An illustration of the early solar system, when the planet body of the Almahata Sitta meteorite may have existed. Image / Nasa
An illustration of the early solar system, when the planet body of the Almahata Sitta meteorite may have existed. Image / Nasa
Ten years ago, an Arizona astronomer spotted an asteroid that was headed straight for Earth.
Swiftly he summoned the help of colleagues and casual stargazers, who tracked the space rock as it exploded in the sky, raining shrapnel down on the Nubian desert in Sudan.
Students from the University ofKhartoum volunteered to search for fragments, ultimately recovering more than 600 pieces of the meteorite now known as Almahata Sitta.
It was the first time scientists had ever traced an asteroid in the sky to a rock they could hold in their hands.
But that is not even the coolest thing about Almahata Sitta. Not nearly.
A new study published in the journal Nature Communications reports that the meteorite contains tiny diamonds - yes, diamonds.
Those diamonds contain even tinier impurities called inclusions. And within those inclusions are signatures of a long-lost planet as large as Mars - a 4.5 billion-year-old relic that was destroyed during the earliest days of the solar system.
"These samples are coming from an era that we don't have any access to," said Farhang Nabiei, a materials scientist at the Swiss Federal Institute of Technology in Lausanne and the lead author of the new report.
The diamonds with the Almahata Sitta meteorite formed during a transition era in the solar system, when the dust and gas that swirled around the sun coalesced into planetary embryos, then grew into planets.
"And we are part of the planets," Nabiei said. "This is part of the story of how we came to be."
Almahata Sitta belongs to a class of rocks known as ureilites. They are partly differentiated - not made of the primitive material that constituted the solar nebula, but also not as well mixed and baked as rocks that come from modern planets.
Unlike other meteorites, which can be traced to parent bodies such as asteroids, Mars or the moon by comparing the ratios of different varieties of elements, these rocks have no known source. They seem to have been formed inside bodies that no longer exist.
And they always contain tiny flecks of diamond.
Because the crystals are so small - less than a fraction of a percentage of an inch in diameter - many researchers assumed that they formed when graphite (an alternate form of carbon) was "shocked" by a collision with another body.
But Nabiei and his colleagues noticed that the diamonds in Almahata Sitta were orders of magnitude larger than the kind that result from a shock event. They suspected that these crystals may have formed the same way diamonds do on Earth - under the unbelievably high temperatures and pressures that exist in the interior of a planet - and only afterward were broken by a shock wave into smaller fragments.
Photo provided by Hillary Sanctuary of EPFL shows a thin slice of the meteorite sample. Photo / AP
"Then this opens whole new idea," Nabiei said. Diamond is so strong it serves as a powerful protective packaging for anything trapped inside; it's nature's safety vault, capable of preserving samples for billions of years.
"I thought, if there were diamonds forming inside a planet, inside a parent body, they could have trapped some material from their environment," Nabiei said. He laughed. "And indeed they did."
The impurities trapped within the Almahata Sitta diamonds - crystals of chromite, phosphate and iron-nickel-sulfide - are the first to have been discovered in an extraterrestrial diamond. They could only have formed under incredible pressure - the equivalent of diving 600km into Earth's interior or attempting to hold up 100,000 tonnes with your bare hands.
To create these conditions, Nabiei said, the meteorite's parent body would have to have been a planet at least as big as Mercury and possibly as large as Mars.
Whatever happened to this lost world? Nabiei can't say for sure. Many researchers believe that the early inner solar system was crowded with large protoplanets that yanked and tugged at each other's orbits until they finally crashed, coalesced or disintegrated. By the end of that era, about 100 million years after the birth of the solar system, only the four current terrestrial planets remained.
Nabiei thinks it's likely that all ureilites come from the same parent body, a protoplanet that lasted just a few million years before it was destroyed in a collision. He plans to seek out similar meteorites and search them for inclusions that might provide clues about their origins.
