Monday, April 15, 2019

Cometary Building Block Material from Sun’s Protoplanetary Disk Discovered

Meteorites originating from primitive C-type asteroids are composed of materials from the Sun’s protoplanetary disk, including up to a few percent organic carbon.

A tiny piece of the building blocks from which comets formed has been discovered inside a primitive meteorite. The discovery by a Carnegie Institution of Science-led team, including a researcher now at Arizona State University (ASU), was published April 15 in Nature Astronomy.

The finding could offer clues to the formation, structure, and evolution of the solar system.

"The meteorite is named LaPaz Icefield 02342," says research scientist Jemma Davidson of ASU's Center for Meteorite Studies in the School of Earth and Space Exploration. "The name comes from where it was found in Antarctica's LaPaz Icefield."

The arrow in this view of the LaPaz meteorite points to where the scientists found the carbon-rich cometary fragment. The colors are produced polarized light shining through a thin slice of the meteorite; the grid lines are spaced one millimeter apart.

Credit: Carles Moyano-Cambero, Institute of Space Sciences, Barcelona

She adds that it belongs to a class of primitive carbonaceous chondrite meteorites that have undergone minimal changes since they formed more than 4.5 billion years ago, likely beyond the orbit of Jupiter.

Construction debris

Meteorites were once part of larger bodies, asteroids, which broke up due to collisions in space and survived the trip through Earth's atmosphere. Their makeup can vary substantially from one meteorite to the next, reflecting their origins in diverse parent bodies that formed in different parts of the solar system.

Asteroids and comets both formed from the disk of gas and dust that once surrounded the young Sun, but they aggregated at different distances from it, which affected their chemical makeup. Compared to asteroids, comets contain larger fractions of water ice and far more carbon, and typically formed farther from the Sun where the environment was colder.

By studying a meteorite's chemistry and mineralogy, researchers such as the paper's lead author, Carnegie's Larry Nittler, can unlock details about its formation and how much heating and other chemical processing it experienced during the solar system's formative years.

'Bonbon' with a surprise inside

Inside the LaPaz meteorite, Nittler's team found a very carbon-rich slice of primitive material. It bears some striking similarities to extraterrestrial dust particles that are thought to have originated in comets that formed near the solar system's outer edges.

Approximately 3 to 3.5 million years after the solar system formed, but while Earth was still growing, this tiny object -- about one tenth of a millimeter across -- was captured by the growing asteroid from which the meteorite originated.

The carbon-rich fragment of the material comets are built from is colored red in this scanning electron microscope image. The scale bar shows its size.

Image credit: Larry Nittler, Carnegie Institution for Science

"Primitive meteorites provide a snapshot of the early solar system that we can study in the lab," says Davidson. "The LaPaz meteorite is a nice example since it has experienced minimal terrestrial weathering."

Meteorites like LaPaz, she notes, are great places to hunt for presolar grains, microscopic pieces of stardust formed by stars that predate the solar system. But none of the team expected also to find evidence for a surviving cometary building block inside a meteorite.

Ancient survivor

"When Larry and Carles showed me the first electron images of the carbon-rich material," Davidson says, "I knew we were looking at something very rare. It was one of those exciting moments you live for as a scientist."

By undertaking sophisticated chemical and isotopic analysis of the material, Nittler and his colleagues -- who besides Davidson include Carnegie's Conel Alexander as well as Rhonda Stroud and Bradley De Gregorio of the U.S. Naval Research Laboratory, and Josep Trigo-Rodríguez, Carles Moyano-Cambero, and Safoura Tanbakouei of the Institute of Space Sciences in Barcelona, Catalonia -- were able to show that the encased material likely originated in the icy outer solar system along with objects from the Kuiper Belt, where many comets originate.

"Because this sample of cometary building block material was swallowed by an asteroid and preserved inside this meteorite, it was protected from the ravages of entering Earth's atmosphere," Nittler explains. "It gave us a peek at material that would not have survived to reach our planet's surface on its own, helping us to understand the early solar system's chemistry."

The existence of this primitive material captured inside the meteorite suggests that due to the drag caused by the surrounding gas, particles like it migrated from the outer edges of the solar system, where comets and Kuiper Belt objects formed, to the closer-in area beyond Jupiter, where the carbonaceous chondrites formed. This reveals details about how our solar system's architecture took shape during the early stages of planet formation.

"Discoveries like this demonstrate how important it is to retrieve precious meteorites like LaPaz from Antarctica," says Davidson. "We never know what secrets they'll reveal."

Contacts and sources:
Robert Burnham
Arizona State University

Citation: A cometary building block in a primitive asteroidal meteorite Larry R. Nittler, Rhonda M. Stroud, Josep M. Trigo-Rodríguez, Bradley T. De Gregorio, Conel M. O’D. Alexander, Jemma Davidson, Carles E. Moyano-Cambero & Safoura Tanbakouei Nature Astronomy (2019)

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