A celestial triple-threat: The solar system's first three-lobed asteroid

Astronomers Imaged Asteroid 44 Nysa and Found Something Truly Unexpected · 16:34 · Video: Anton Petrov · Watch at the source

In short: For over 150 years, astronomers knew only that asteroid 44 Nysa was a bright speck in the main belt. It took modern high-contrast imaging to reveal its bizarre anatomy: a massive body composed of three distinct lobes joined together like a cosmic welding project.

Discovered in 1857, 44 Nysa is one of the largest and brightest E-type asteroids, characterized by a surface rich in enstatite. While previous observations from instruments like the Hubble Space Telescope suggested it might be bi-lobed—similar to many other asteroids—new joint observations from the Large Binocular Telescope (LBT) in Arizona and the Very Large Telescope (VLT) in Chile have revealed a much more complex structure.

Measuring approximately 47 miles (75 kilometers) across, these pictures depict an uneven mass containing two distinct 'colli' valleys. Scientists view these as 'necks', implying Nysa is a contact trinary formed by three individual parts merging at low speeds to bond instead of breaking apart. While contact binaries like Comet 67P are known, a triple-lobed object of this nature has never been seen before.

Alternatively, the asteroid could be a single body so severely battered by space debris that it mimics a trinary shape—a possibility that would also be a first for science. Adding to the complexity, the team identified a small moon, designated S/2026 (44) 1, which is about 0.6 miles (1 kilometer) wide and orbits at a distance of at least 106 miles (170 kilometers).

To capture these details, scientists used adaptive optics to counteract atmospheric blurring and specialized image-processing to remove the asteroid's bright halo. These techniques, originally developed for hunting exoplanets, allow researchers to study Nysa's interior strength and formation history without leaving Earth.

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