The size, density, and formation of the Orcus-Vanth system in the Kuiper belt
M.E. Brown, D. Ragozzine, J. Stansberry, W.C. Fraser

TL;DR
This study characterizes the Orcus-Vanth system in the Kuiper belt, revealing its size, orbit, and composition, and discusses possible formation scenarios including giant impact and capture.
Contribution
It provides detailed measurements of the Orcus-Vanth system's size, orbit, and composition, and evaluates different formation hypotheses.
Findings
Vanth has a nearly face-on circular orbit with a 9.54-day period.
System mass is approximately 6.32 x 10^20 kg, about 3.8% of Eris.
Density is roughly 1.5 g/cm^3, depending on albedo assumptions.
Abstract
The Kuiper belt object Orcus and its satellite Vanth form an unusual system in the Kuiper belt. Orcus is amongst the largest objects known in the Kuiper belt, but the relative size of Vanth is much larger than that of the tiny satellites of the other large objects. From Hubble Space Telescope observations we find that Orcus and Vanth have different visible colors and that Vanth does not share the water ice absorption feature seen in the infrared spectrum of Orcus. We also find that Vanth has a nearly face-on circular orbit with a period of 9.5393 +-0.0001 days and semimajor axis of 8980+-20 km, implying a system mass of 6.32+- 0.01 X 10^20 kg or 3.8% the mass of dwarf planet Eris. From Spitzer Space Telescope observations we find that the thermal emission is consistent with a single body with diameter 940+-70 km and a geometric albedo of 0.28+-0.04. Assuming equal densities and…
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