June 16, 2022

Astronomers reveal the most detailed map of the asteroid Psyche yet

Astronomers at MIT and elsewhere have mapped the composition of asteroid Psyche, revealing a surface of metal, sand, and rock.
Enlarge / Astronomers at MIT and elsewhere have mapped the composition of asteroid Psyche, revealing a surface of metal, sand, and rock.

Astronomers have produced the most detailed map to date of the surface of 16-Psyche, an asteroid that scientists believe could hold clues to how planets formed in our Solar System. According to a paper published in the Journal of Geophysical Research, 16-Psyche has a highly varied surface of metal, sand, and rock that suggests its history could include metallic eruptions, as well as being hit by other celestial objects. The asteroid is the focus of NASA’s Psyche mission, launching later this year.

As we’ve reported previously, 16 Psyche is an M-type asteroid (meaning it has high metallic content) orbiting the Sun in the main asteroid belt, with an unusual potato-like shape. The longstanding preferred hypothesis is that Psyche is the exposed metallic core of a protoplanet (planetesimal) from our Solar System’s earliest days, with the crust and mantle stripped away by a collision (or multiple collisions) with other objects. In recent years, scientists concluded that the mass and density estimates aren’t consistent with an entirely metallic remnant core. Rather, it’s more likely a complex mix of metals and silicates.

Alternatively, the asteroid might once have been a parent body for a particular class of stony-iron meteorites, one that broke up and re-accreted into a mix of metal and silicate. Or perhaps it’s an object like 1 Ceres, a dwarf planet in the asteroid belt between the orbits of Mars and Jupiter—except 16 Psyche may have experienced a period of iron volcanism while cooling, leaving highly enriched metals in those volcanic centers.

Scientists have long suspected that metallic cores lurk deep within terrestrial planets like Earth. But those cores are buried too far beneath rocky mantles and crusts for researchers to find out. As the only metallic core-like body discovered, Psyche provides the perfect opportunity to shed light on how the rocky planets in our Solar System (Earth, Mercury, Venus, and Mars) may have formed. NASA approved the Psyche mission in 2017, intending to send a spacecraft to orbit the asteroid and collect crucial data about its characteristics.

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

Prior mapping efforts relied on measuring infrared light bouncing off the asteroid’s surface with various telescopes around the world. Last year, astronomers produced a surface map of Psyche with much higher resolution, based on 2019 observational data collected by all 66 radio antennas of the Atacama Large Millimeter/submillimeter Array (ALMA) in Chile.

By combining all those signals into a single synthetic signal, the team achieved the equivalent resolution of a telescope with a diameter of 16 kilometers (10 miles)—about 20 miles per pixel. This view enabled them to resolve many compositional variations on the asteroid’s surface. They used this to create a thermal emissions map of the asteroid’s surface and a high-resolution 3D model of Psyche.

This latest map is based on hundreds of computer-simulated scenarios, each featuring a different combination of surface material composition, taking into account the asteroid’s rotation. The team then compared those simulations to the actual thermal emissions in the ALMA data to determine the likeliest map of 16-Psyche’s surface.

The results: The asteroid is rich in metals, but the distribution varies across its surface. A similar varied distribution of silicates suggests that 16-Psyche may have once had a silicate-rich mantle. Further, the material at the bottom of craters changes temperature faster than along the rim as the asteroid rotates. The authors suggest that those craters may have deposits (“ponds”) of fine-grained sand. This is a bit surprising given the mass of 16-Psyche and its stronger gravity, compared to smaller asteroids that have fine-grained materials.

“These data show that Psyche’s surface is heterogeneous, with possible remarkable variations in composition,” said Simone Marchi of the Southwest Research Institute, a co-investigator on the Psyche mission who was not involved in the current study. “One of the primary goals of the Psyche mission is to study the composition of the asteroid surface using its gamma rays and neutron spectrometer and a color imager. So, the possible presence of compositional heterogeneities is something that the Psyche Science Team is eager to study more.”

DOI: Journal of Geophysical Research, 2022. 10.1029/2021JE007091/a>  (About DOIs).

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