Incredible New Maps of Asteroid Psyche Reveal an Ancient World of Metal and Rock

Astronomers at MIT and elsewhere have mapped the composition of asteroid Psyche, revealing a surface of metal, sand and rock. Credit: Screenshot courtesy of NASA

Asteroid Psyche’s varied surface suggests a dynamic history, which could include metallic eruptions, asteroid tremor impacts, and a lost rocky mantle.

Later this year,[{” attribute=””>NASA is set to launch a probe the size of a tennis court to the asteroid belt, a region between the orbits of

Ahead of the mission, which is led by principal investigator Lindy Elkins-Tanton ’87, SM ’87, PhD ’02, planetary scientists at Psyche Spacecraft at the Asteroid Psyche (Illustration)

This illustration, updated in April 2022, depicts NASA’s Psyche spacecraft. Set to launch in August 2022, the Psyche mission will explore a metal-rich asteroid of the same name that lies in the main asteroid belt between Mars and Jupiter. The spacecraft will arrive in early 2026 and orbit the asteroid – also shown in this illustration – for nearly two years to investigate its composition. Credit: NASA/JPL-Caltech/ASU

Overall, Psyche’s surface was found to be surprisingly varied in its properties.

The new maps hint at the asteroid’s history. Its rocky regions could be vestiges of an ancient mantle — similar in composition to the rocky outermost layer of Earth, Mars, and the asteroid Vesta — or the imprint of past impacts by space rocks. Finally, craters that contain metallic material support the idea proposed by previous studies that the asteroid may have experienced early eruptions of metallic lava as its ancient core cooled.

“Psyche’s surface is very heterogeneous,” says lead author Saverio Cambioni, the Crosby Distinguished Postdoctoral Fellow in MIT’s Department of Earth, Atmospheric and Planetary Sciences (EAPS). “It’s an evolved surface, and these maps confirm that metal-rich asteroids are interesting, enigmatic worlds. It’s another reason to look forward to the Psyche mission going to the asteroid.”

Cambioni’s co-authors are Katherine de Kleer, assistant professor of planetary science and astronomy at Caltech, and Michael Shepard, professor of environmental, geographical, and geological sciences at Bloomsburg University.

Telescope Power

The surface of Psyche has been a focus of numerous previous mapping efforts. Researchers have observed the asteroid using various telescopes to measure light emitted from the asteroid at infrared wavelengths, which carry information about Psyche’s surface composition. However, these studies could not spatially resolve variations in composition over the surface.

Cambioni and his colleagues instead were able to see Psyche in finer detail, at a resolution of about 20 miles per pixel, using the combined power of the 66 radio antennas of the Atacama Large Millimeter/submillimeter Array (

On the left, this map shows surface properties on Psyche, from sandy areas (purple/bottom) to rocky areas (yellow/top). The map on the right shows metal abundances on Psyche, from low (purple) to high (yellow).

To catch a match

In the new study, Cambioni ran Psyche simulations to see which surface properties might best match and explain the measured thermal emissions. In each of the hundreds of simulated scenarios, he defined the asteroid’s surface with different combinations of materials, such as areas of different metal abundances. He modeled the rotation of the asteroid and measured how simulated materials on the asteroid would give off thermal emissions. Cambioni then searched for the simulated emissions that best matched the actual emissions measured by ALMA. This scenario, he reasoned, would reveal the most likely map of the asteroid’s surface materials.

“We ran these simulations area by area so that we could detect differences in surface properties,” Cambioni explains.

The study produced detailed maps of Psyche’s surface properties, showing that the asteroid’s facade is likely covered in a wide variety of materials. The researchers confirmed that, overall, the surface of Psyche is rich in metals, but the abundance of metals and silicates varies across its surface. This may be a further clue that early in its formation the asteroid may have had a silicate-rich mantle that has since disappeared.

They also found that as the asteroid rotates, the material at the bottom of a large depression – likely a crater – changes temperature much faster than the material along the edge. This suggests that the crater floor is lined with “pools” of fine-grained material, like sand on Earth, which heats up quickly, while the crater rims are composed of rockier, slower-heating material.

“Pools of fine-grained material have been observed on small asteroids, whose gravity is low enough that impacts shake the surface and cause finer material to accumulate,” Cambioni explains. “But Psyche is a large body, so if fine-grained material accumulates at the bottom of the depression, it’s interesting and somewhat mysterious.”

“These data show that the surface of Psyche is heterogeneous, with possible remarkable variations in composition,” said Simone Marchi, a scientist at the Southwest Research Institute and co-investigator of NASA’s Psyche mission, who was not involved in the study. current study. “One of the main objectives of the Psyche mission is to study the composition of the asteroid’s surface using its gamma-ray and neutron spectrometer and a color imager. Thus, the possible presence of compositional heterogeneities is something the Psyche Science team is eager to investigate further.

Reference: “The Heterogeneous Surface of Asteroid (16) Psyche” by Saverio Cambioni, Katherine de Kleer and Michael Shepard, May 19, 2022, Journal of Geophysical Research: Planets.
DOI: 10.1029/2021JE007091

This research was supported by the EAPS Crosby Distinguished Postdoctoral Fellowship and in part by the Heising-Simons Foundation.

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