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EES Graduate Student Jackson Barnes discovery gets national and international press attention

Image of Kuiper belt object Arrokoth from New HorizonsPlanetary scientists have long been puzzled by the snowman‑like shapes of many icy bodies in the Kuiper Belt where roughly 10–25% of planetesimals consist of two spherical lobes joined together. The NASA New Horizons spacecraft flew by Kuiper Belt object Arrokoth (pictured right), which is a prototypical primordial contact binary.
 

The Breakthrough Research

EES planetary scientists, graduate student Jackson Barnes and Prof. Seth Jacobson, working with Dr. Steve Schwartz, have recently published a paper that demonstrates how these unique "contact binaries" are formed. Their study, which has been featured in a press release from the publisher The Royal Astronomical Society and major science news publications like Scientific American and The Guardian, uses numerical simulations to show that these shapes result from the gravitational collapse that first produced planetesimals in our solar system. The computer models reveal a process where rotating clouds of pebbles break into two separate planetesimals. These bodies then orbit each other, gradually spiraling inward until they gently fuse while maintaining their round, spherical shapes. This pioneering work incorporates the necessary physics to reproduce these binaries, providing critical insights into the early stages of planet formation.
 

International Recognition

The scientific community has responded with significant praise for the findings:

It is marvelous work,” says William McKinnon, a planetary scientist at Washington University in St. Louis who was not involved with the new work. “What the authors have done is demonstrate that the most direct pathway is indeed quite physically plausible”.

Alan Stern, a planetary scientist at the Southwest Research Institute and principal investigator of Nasa’s New Horizons mission to the Kuiper belt, welcomed the study. “It’s in agreement with previous work and support[s] the hypothesis that Kuiper belt object Arrokoth, which New Horizons explored in a close flyby, is the result of gentle formation processes,” he said.
 

Explore Further

For more details, including movies of the simulations and the full peer-reviewed article, please see the Publisher's press release and news coverage linked below:
Royal Astronomical Society: Why some objects in space look like snowme.