TL;DR
This study models `Oumuamua's light curve considering shape and torque, finding a thin disc shape with moderate outgassing torque best explains observed features, suggesting a tumbling, disc-like interstellar object.
Contribution
First physical model fitting `Oumuamua's light curve including torque, favoring a thin disc shape over cigar shape based on probability analysis.
Findings
Disc-shaped models have a 91% probability to produce observed minima.
Cigar-shaped models suffer from fine-tuning issues with only 16% probability.
`Oumuamua is most likely a tumbling, thin disc object experiencing moderate torque.
Abstract
We present the first attempt to fit the light curve of the interstellar visitor `Oumuamua using a physical model which includes optional torque. We consider both conventional (Lommel-Seeliger triaxial ellipsoid) and alternative ("black-and-white ball", "solar sail") brightness models. With all the brightness models, some torque is required to explain the timings of the most conspicuous features -- deep minima -- of the asteroid's light curve. Our best-fitting models are a thin disc (aspect ratio 1:6) and a thin cigar (aspect ratio 1:8) which are very close to being axially symmetric. Both models are tumbling and require some torque which has the same amplitude in relation to `Oumuamua's linear non-gravitational acceleration as in Solar System comets which dynamics is affected by outgassing. Assuming random orientation of the angular momentum vector, we compute probabilities for our…
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