English

Arrokoth's Necklace

Earth and Planetary Astrophysics 2021-03-09 v4

Abstract

Flyby images of (486958) Arrokoth (Ultima Thule, 2014 MU69_{69}) show a comparatively bright "necklace" in the neck, or cleft between its two lobes, in contrast to its generally low albedo. We suggest that the necklace may be the result of thermally controlled ice deposition. The necklace is found in the most (orbitally averaged) shaded part of its surface. It may consist of clean, high albedo, ice condensed from vapor sublimed by dirty, low albedo, ice elsewhere; clean ice accumulates where the maximum temperatures are the lowest. Ammonia and propane have the necessary mesovolatile vapor pressure. Surrounding gas in the proto-Solar System would facilitate redeposition of molecules sublimed by warmer parts of the surface into the cleft, as well as smoothing the surface and explaining, by hydrodynamic drag, Arrokoth's slow (compared to its breakup rate) rotation. Alternatively, a layer of hoarfrost thick enough (0.1μ\gtrsim 0.1\,\mu) to have a high albedo could have formed more recently.

Keywords

Cite

@article{arxiv.1902.00997,
  title  = {Arrokoth's Necklace},
  author = {J. I. Katz and S. Wang},
  journal= {arXiv preprint arXiv:1902.00997},
  year   = {2021}
}

Comments

10 pp., 7 figs. Much revised, added references; includes former arXiv:1903.04960 as Appendix

R2 v1 2026-06-23T07:30:57.619Z