TY - JOUR
T1 - Evidence for geologic processes on comets
AU - Sunshine, Jessica M.
AU - Thomas, Nicolas
AU - El-Maarry, Mohamed Ramy
AU - Farnham, Tony L.
N1 - Funding Information:
Funding to M.R.E. and N.T. from the Swiss National Science Foundation through grant 200020_165684 and to TLF from NASA's Planetary Mission Data Analysis Program through grant NNX12AQ64G is gratefully acknowledged. Data from cometary missions can be found in NASA's Planetary Data System (PDS) Small Bodies Node (SBN) http://pdssbn.astro.umd.edu and/or ESA's Planetary Science Archive (PSA) http://www.rssd.esa.int/index.php?project=PSA.
Publisher Copyright:
©2016. American Geophysical Union. All Rights Reserved.
PY - 2016/11/1
Y1 - 2016/11/1
N2 - Spacecraft missions have resolved the nuclei of six periodic comets and revealed a set of geologically intriguing and active small bodies. The shapes of these cometary nuclei are dominantly bilobate reflecting their formation from smaller cometesimals. Cometary surfaces include a diverse set of morphologies formed from a variety of mechanisms. Sublimation of ices, driven by the variable insolation over the time since each nucleus was perturbed into the inner Solar System, is a major process on comets and is likely responsible for quasi-circular depressions and ubiquitous layering. Sublimation from near-vertical walls is also seen to lead to undercutting and mass wasting. Fracturing has only been resolved on one comet but likely exists on all comets. There is also evidence for mass redistribution, where material lifted off the nucleus by subliming gases is deposited onto other surfaces. It is surprising that such sedimentary processes are significant in the microgravity environment of comets. There are many enigmatic features on cometary surfaces including tall spires, kilometer-scale flows, and various forms of depressions and pits. Furthermore, even after accounting for the differences in resolution and coverage, significant diversity in landforms among cometary surfaces clearly exists. Yet why certain landforms occur on some comets and not on others remains poorly understood. The exploration and understanding of geologic processes on comets is only beginning. These fascinating bodies will continue to provide a unique laboratory for examining common geologic processes under the uncommon conditions of very high porosity, very low strength, small particle sizes, and near-zero gravity.
AB - Spacecraft missions have resolved the nuclei of six periodic comets and revealed a set of geologically intriguing and active small bodies. The shapes of these cometary nuclei are dominantly bilobate reflecting their formation from smaller cometesimals. Cometary surfaces include a diverse set of morphologies formed from a variety of mechanisms. Sublimation of ices, driven by the variable insolation over the time since each nucleus was perturbed into the inner Solar System, is a major process on comets and is likely responsible for quasi-circular depressions and ubiquitous layering. Sublimation from near-vertical walls is also seen to lead to undercutting and mass wasting. Fracturing has only been resolved on one comet but likely exists on all comets. There is also evidence for mass redistribution, where material lifted off the nucleus by subliming gases is deposited onto other surfaces. It is surprising that such sedimentary processes are significant in the microgravity environment of comets. There are many enigmatic features on cometary surfaces including tall spires, kilometer-scale flows, and various forms of depressions and pits. Furthermore, even after accounting for the differences in resolution and coverage, significant diversity in landforms among cometary surfaces clearly exists. Yet why certain landforms occur on some comets and not on others remains poorly understood. The exploration and understanding of geologic processes on comets is only beginning. These fascinating bodies will continue to provide a unique laboratory for examining common geologic processes under the uncommon conditions of very high porosity, very low strength, small particle sizes, and near-zero gravity.
KW - comets
KW - erosion and weathering
KW - morphology
KW - origin and evolution
KW - Planetary sciences: Comets and small bodies
KW - surfaces
KW - surfaces
UR - http://www.scopus.com/inward/record.url?scp=85000578315&partnerID=8YFLogxK
U2 - 10.1002/2016JE005119
DO - 10.1002/2016JE005119
M3 - Review article
AN - SCOPUS:85000578315
SN - 2169-9097
VL - 121
SP - 2194
EP - 2210
JO - Journal of Geophysical Research: Planets
JF - Journal of Geophysical Research: Planets
IS - 11
ER -