Space

Donaldjohanson: a tumbling cosmic peanut

Lucy’s second rehearsal revealed a narrow waist, two lobes, and complex rotation. Even a modest asteroid can carry a history of reassembly.

A stereo image pair from Lucy observations showing two views of the same asteroid, Donaldjohanson. NASA / Goddard / SwRI / Johns Hopkins APL.
A stereo image pair from Lucy observations showing two views of the same asteroid, Donaldjohanson. NASA / Goddard / SwRI / Johns Hopkins APL.

Named for fossil discoverer Donald Johanson, this asteroid has a scholarly name and a familiar shape: Lucy’s 2025 flyby revealed two peanut-like lobes joined by a narrow waist.

From a point to a detailed world

Ground observations estimate size from brightness and other information, but a flyby reveals the actual outline. This elongated body cannot be described by one diameter alone: maximum length and equivalent diameter are different, compatible measurements.

Why doesn’t it spin like a tidy top?

Research published in 2026 examined complex tumbling. An irregular object need not rotate neatly about one fixed axis. Shape, spin, and mass distribution interact; sequential images reconstruct the motion better than a single photograph.

Lucy’s instrument platform, whose cameras and spectrometers record shape, color, and thermal clues. NASA
Lucy’s instrument platform, whose cameras and spectrometers record shape, color, and thermal clues. NASA

Reassembled worlds in the main belt

Impacts can fragment a parent body, after which gravity gathers pieces again. Family associations, lobes, and surface features provide evidence, but a peanut outline alone does not uniquely establish the formation history.

A gift from a rehearsal

This encounter tested tracking and instrument coordination before the Trojans, while revealing an independently fascinating target. Planned questions and unexpected images both advance our understanding.

References