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American Focus > Blog > Tech and Science > The Kuiper Belt is packed with weird peanut-shaped objects. Astronomers think they know why
Tech and Science

The Kuiper Belt is packed with weird peanut-shaped objects. Astronomers think they know why

Last updated: February 22, 2026 4:40 am
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The Kuiper Belt is packed with weird peanut-shaped objects. Astronomers think they know why
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A recent study sheds light on the peculiar peanut-shaped objects that populate our solar system. These objects, known as planetesimals, are believed to be the building blocks of planets. The study, published in the Monthly Notices of the Royal Astronomical Society, offers an explanation for the origin of these enigmatic shapes.

The Kuiper Belt, a region of debris beyond Neptune, is home to a significant number of kilometer-scale objects with a unique peanut-like shape. Unlike traditional spherical planetesimals, these objects consist of two lobes of different sizes, resembling a snowman or a peanut.

NASA’s New Horizons mission provided a clearer view of these peculiar objects when it flew by the two-lobed Kuiper Belt object Arrokoth in 2019. Subsequent observations have revealed additional examples of these snowman-like planetesimals, sparking curiosity among astronomers.

The study suggests that these contact binaries, as they are called, formed in unison rather than as two separate bodies that merged over time. Using advanced simulations, the researchers demonstrated that these peanut-shaped objects could have originated from a single cloud of gas and dust collapsing under its own gravity.

Approximately 4.6 billion years ago, the remnants of this collapsed cloud formed a dusty disk around the sun, giving rise to planetesimals in the outer reaches of the protoplanetary disk, such as the Kuiper Belt. The slow movement and sparse distribution of these planetesimals prevented them from merging into planets.

The simulations conducted in the study revealed that about 4 percent of the collapsed cloud scenarios resulted in contact binaries, similar to the observed prevalence in the Kuiper Belt. While the model is not perfect and struggles to reproduce certain features of known objects like Arrokoth, it represents a significant step towards understanding the formation of these unique planetesimals.

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The findings of this study have important implications for our understanding of planetary formation processes. By unraveling the mystery of these peanut-shaped objects, astronomers hope to gain insights into the early stages of planet formation and the evolution of our solar system. As we continue to explore the cosmos, studies like this provide valuable clues about the origins of the celestial bodies that surround us.

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