Unexpected Discoveries on a Metal World
Press release issued by the University of Arizona to coincide with presentation at the joint 48th annual meeting of the Division for Planetary Sciences (DPS) of the American Astronomical Society (AAS) and 11th annual European Planetary Science Congress (EPSC).
Summary – Psyche, a large asteroid thought to be the metallic core of a destroyed protoplanet, appears to have volatiles on its surface that shouldn’t be there unless they were delivered by other asteroids, according to a new study.
Astronomers have discovered possible evidence for water on the surface of the largest metallic asteroid in the solar system. Named 16 Psyche, the object is one of the most massive in the asteroid belt, measuring 186 miles across and consisting of almost pure nickel-iron metal. It is thought to be the remnant core of a planetary embryo that was mostly destroyed by impacts billions of years ago.
Previous observations of Psyche had shown no evidence for water on its surface. But in a paper accepted in The Astronomical Journal, Vishnu Reddy, an assistant professor at the University of Arizona’s Lunar and Planetary Laboratory, argues that new observations from the NASA Infrared Telescope Facility show evidence for volatiles such as water or hydroxyl, a free radical consisting of one hydrogen atom bound to one oxygen atom, on Psyche’s surface. In Earth’s atmosphere, hydroxyl is extremely reactive and helps remove many chemical compounds. Hence it is also known as the “detergent of the atmosphere.”
“We did not expect a metallic asteroid like Psyche to be covered by water and/or hydroxyl,” Reddy said, who is presenting these results today at the joint 48th meeting of the American Astronomical Society’s Division for Planetary Sciences (DPS) and 11th European Planetary Science Congress (EPSC) in Pasadena, California. Reddy is second author on the paper led by Driss Takir at the U.S. Geological Survey in Flagstaff, Arizona. “Metal-rich asteroids like Psyche are thought to have formed under dry conditions without the presence of water or hydroxyl, so we were puzzled by our observations at first.”
The findings are interesting in the context of a proposed $500 million mission to send a spacecraft to Psyche, currently under review by NASA. Images taken by a spacecraft orbiting Psyche may enable us to distinguish between water and hydroxyl on the surface.
Asteroids are remaining fragments from the formation of the solar system that today orbit the Sun between the orbits of Mars and Jupiter. Most of them fall into two broad categories: those rich in silicates, and those rich in carbon and volatiles. Metallic asteroids such as Psyche are extremely rare, making it a laboratory to study how planets formed.
While the source of this water on Psyche remains a mystery, Reddy and his colleagues propose two possible mechanisms for its formation. “We think the water we see on Psyche might have been delivered to its surface by carbonaceous asteroids that impacted Psyche in the distant past,” says Reddy.
“Our discovery of carbon and water on an asteroid that isn’t supposed to have those compounds supports the notion that these building blocks of life could have been delivered to our Earth early in the history of our solar system,” said Reddy, who discovered similar dark, carbonaceous impactors rich in volatiles on the surface of asteroid Vesta by studying images from NASA’s Dawn mission. Alternatively, the hydroxyl could be the product of solar wind interacting with silicate minerals on Psyche’s surface.
To further explore the hypothesis of carbon and water delivered to protoplanetary bodies by asteroids in the early solar system, the UA is leading NASA’s OSIRIS-REx mission to bring back a sample from carbonaceous asteroid 101955 Bennu in 2023.
Daniel W. Stolte
Video Caption: Movie showing the radar shape model of main belt asteroid (16) Psyche with high (red) and low (blue) areas on its surface. The radar data were acquired with the Arecibo Radio Observatory. New observations of Psyche by the NASA Infrared Telescope Facility on Mauna Kea, Hawai’i, show that its surface is covered with water/hydroxyl. These volatiles are thought to have been delivered via carbonaceous chondrite impactors or by solar wind interacting with the surface. (Movie Credit: James Richardson (PSI)/Shepard et al. 2016)
“Detection of Water and/or Hydroxyl on Asteroid (16) Psyche,” Driss Takir, Vishnu Reddy et al., 2016, Astronomical Journal [http://aj.aas.org, preprint: https://arxiv.org/abs/1610.00802].
Reddy’s research on Psyche is funded by NASA’s Planetary Science Division’s Planetary Geology and Geophysics program.
The joint 48th meeting of the Division for Planetary Sciences (DPS) and 11th European Planetary Science Congress (EPSC) in Pasadena, California, is second time DPS and EPSC have been joined into one meeting. The goal of the joint meeting is to strengthen international scientific collaboration in all areas of planetary science. This is the first time that EPSC, which provides the dissemination platform for the Europlanet 2020 Research Infrastructure, is held outside Europe. For more information, see: https://aas.org/meetings/dps48. Follow: #dpsepsc, @DPSMeeting, @europlanetmedia, and @AAS_Press on Twitter.