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arXiv · 1911.08546

The Complex Rotational Light Curve of (385446) Manwë-Thorondor, a Multi-Component Eclipsing System in the Kuiper Belt

David L. Rabinowitz·Susan D. Benecchi·William M. Grundy·Anne J. Verbiscer·Audrey Thirouin
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Abstract

Kuiper Belt Object (385446) Manwë-Thorondor is a multi-object system with mutual events predicted to occur from 2014 to 2019. To detect the events, we observed the system at 4 epochs (UT 2016 Aug 25 and 26, 2017 Jul 22 and 25, 2017 Nov 9, and 2018 Oct 6) in g, r, and VR bands using the 4-m SOAR and the 8.1-m Gemini South telescopes at Cerro Pachón, Chile and Lowell Observatory ' s 4.3-m Discovery Channel Telescope at Happy Jack, Arizona. These dates overlap the uncertainty range (+/- 0.5 d) for four inferior events (Thorondor eclipsing Manwë). We clearly observe variability for the unresolved system with a double-peaked period 11.88190 +/- 0.00005 h and ~0.5 mag amplitude together with much longer-term variability. Using a multi-component model, we simultaneously fit our observations and earlier photometry measured separately for Manwë and Thorondor with the Hubble Space Telescope. Our fit suggests Manwë is bi-lobed, close to the barbell shape expected for a strengthless body with density ~0.8 g/cm3 in hydrostatic equilibrium. For Manwë, we thereby derive maximum width to length ratio ~0.30, surface area equivalent to a sphere of diameter 190 km, geometric albedo 0.06, mass 1.4x1018 kg, and spin axis oriented ~75 deg from Earth ' s line of sight. Changes in Thorondor ' s brightness by ~0.6 mag with ~300-d period may account for the system ' s long-term variability. Mutual events with unexpectedly shallow depth and short duration may account for residuals to the fit. The system is complex, providing a challenging puzzle for future modeling efforts.

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David L. Rabinowitz, Susan D. Benecchi, William M. Grundy, Anne J. Verbiscer, Audrey Thirouin. 2019-11-19. The Complex Rotational Light Curve of (385446) Manwë-Thorondor, a Multi-Component Eclipsing System in the Kuiper Belt. https://arxiv.org/abs/1911.08546

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