Physical properties of centaur (54598) Bienor from photometry
E. Fern\'andez-Valenzuela, J. L. Ortiz, R. Duffard, N. Morales, P., Santos-Sanz

TL;DR
This study analyzes photometric data of Centaur (54598) Bienor over 16 years, revealing changes in its rotation axis orientation, shape, and possible ring system, with implications for its density and surface properties.
Contribution
It provides the first detailed analysis of Bienor’s rotational axis orientation, shape, and potential ring system based on long-term photometry, expanding understanding of Centaur physical characteristics.
Findings
Rotation axis orientation determined as βp=50±3°, λp=35±8°.
Best-fit axial ratio b/a=0.45±0.05 implies a density of ~594 kg/m³.
Including a ring system improves fit to light curve and magnitude data, suggesting possible rings.
Abstract
We present time series photometry of Bienor in four observation campaigns from 2013 to 2016 and compare them with previous observations in the literature dating back to 2000. The results show a remarkable decline in the amplitude of the rotational light curve and in the absolute magnitude. This suggests that the angle between the rotation axis and the line of sight has changed noticeably during the last 16 years as Bienor orbits the Sun. From the light curve amplitude data we are able to determine the orientation of the rotation axis of Bienor (, ). We are also able to constrain the axial ratio of a triaxial Jacobi ellipsoidal body (with semi-axis ). The best fit is for , which corresponds to a density value of kgm under the usual assumption of hydrostatic equilibrium and given…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
