TY - JOUR
T1 - Arrokoth's necklace
AU - Katz, J. I.
AU - Wang, S.
N1 - Publisher Copyright:
© 2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society.
PY - 2021/6/1
Y1 - 2021/6/1
N2 - Fly-by images of (486958) Arrokoth (Ultima Thule, 2014 MU69) 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 the surface. It may consist of clean, high albedo, ice condensed from vapour sublimed by dirty, low albedo, ice elsewhere; ice accumulates where the maximum temperatures are the lowest. Ammonia and propane have the necessary mesovolatile vapour 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 break-up rate) rotation. Alternatively, a layer of hoarfrost thick enough (≳ 0.1, μ) to have a high albedo could have formed more recently.
AB - Fly-by images of (486958) Arrokoth (Ultima Thule, 2014 MU69) 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 the surface. It may consist of clean, high albedo, ice condensed from vapour sublimed by dirty, low albedo, ice elsewhere; ice accumulates where the maximum temperatures are the lowest. Ammonia and propane have the necessary mesovolatile vapour 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 break-up rate) rotation. Alternatively, a layer of hoarfrost thick enough (≳ 0.1, μ) to have a high albedo could have formed more recently.
KW - Kuiper Belt Objects: individual: (486958) Arrokoth (Ultima Thule, 2014 MU)
UR - https://www.scopus.com/pages/publications/85107981305
U2 - 10.1093/mnras/stab718
DO - 10.1093/mnras/stab718
M3 - Article
AN - SCOPUS:85107981305
SN - 0035-8711
VL - 504
SP - 601
EP - 609
JO - Monthly Notices of the Royal Astronomical Society
JF - Monthly Notices of the Royal Astronomical Society
IS - 1
ER -