Granular segregation on the rubble-pile asteroid Itokawa

We investigate the dynamics of regolith on rubble-pile asteroids to explain granular processes observed in reality. In particular, we explain how the appearance of boulders on the surface of asteroid Itokawa could have resulted from a size sorting process in granular media called the Brazil Nut Effe...

Full description

Bibliographic Details
Main Authors: Ghosh Sohanjit, Sharma Ishan, Dhingra Deepak
Format: Article
Language:English
Published: EDP Sciences 2021-01-01
Series:EPJ Web of Conferences
Online Access:https://www.epj-conferences.org/articles/epjconf/pdf/2021/03/epjconf_pg2021_03042.pdf
id doaj-c1b6533fdabe492cb7d9d4fdbf9baf37
record_format Article
spelling doaj-c1b6533fdabe492cb7d9d4fdbf9baf372021-08-03T00:59:02ZengEDP SciencesEPJ Web of Conferences2100-014X2021-01-012490304210.1051/epjconf/202124903042epjconf_pg2021_03042Granular segregation on the rubble-pile asteroid ItokawaGhosh Sohanjit0Sharma Ishan1Dhingra Deepak2Department of Mechanical EngineeringDepartment of Mechanical EngineeringDepartment of Earth Sciences Mechanics and Applied Mathematics Group, Indian Institute of Technology KanpurWe investigate the dynamics of regolith on rubble-pile asteroids to explain granular processes observed in reality. In particular, we explain how the appearance of boulders on the surface of asteroid Itokawa could have resulted from a size sorting process in granular media called the Brazil Nut Effect (BNE). The Discrete Element Method (DEM) is implemented to perform numerical simulations of the BNE in a micro-gravity environment caused by inter-particle collisions during seismic vibrations. Firstly, we present the results of how the BNE depends on the magnitude of surface gravity. It is estimated that segregation processes on Itokawa occur over much longer time-scales (in the order of a few hundred years) than the same processes would require in the presence of a strong gravitational field, like on Earth. Secondly, we also find that the size sorting could also result from kinetic sieving encountered during granular avalanches. Finally, we discuss how the void-filling mechanism becomes more efficient when there is a higher relative size difference between the boulders and the surrounding grains. Our model has important implications in understanding the resurfacing of Itokawa by trying to explain one of the many complex geophysical processes that occur in such unique conditions.https://www.epj-conferences.org/articles/epjconf/pdf/2021/03/epjconf_pg2021_03042.pdf
collection DOAJ
language English
format Article
sources DOAJ
author Ghosh Sohanjit
Sharma Ishan
Dhingra Deepak
spellingShingle Ghosh Sohanjit
Sharma Ishan
Dhingra Deepak
Granular segregation on the rubble-pile asteroid Itokawa
EPJ Web of Conferences
author_facet Ghosh Sohanjit
Sharma Ishan
Dhingra Deepak
author_sort Ghosh Sohanjit
title Granular segregation on the rubble-pile asteroid Itokawa
title_short Granular segregation on the rubble-pile asteroid Itokawa
title_full Granular segregation on the rubble-pile asteroid Itokawa
title_fullStr Granular segregation on the rubble-pile asteroid Itokawa
title_full_unstemmed Granular segregation on the rubble-pile asteroid Itokawa
title_sort granular segregation on the rubble-pile asteroid itokawa
publisher EDP Sciences
series EPJ Web of Conferences
issn 2100-014X
publishDate 2021-01-01
description We investigate the dynamics of regolith on rubble-pile asteroids to explain granular processes observed in reality. In particular, we explain how the appearance of boulders on the surface of asteroid Itokawa could have resulted from a size sorting process in granular media called the Brazil Nut Effect (BNE). The Discrete Element Method (DEM) is implemented to perform numerical simulations of the BNE in a micro-gravity environment caused by inter-particle collisions during seismic vibrations. Firstly, we present the results of how the BNE depends on the magnitude of surface gravity. It is estimated that segregation processes on Itokawa occur over much longer time-scales (in the order of a few hundred years) than the same processes would require in the presence of a strong gravitational field, like on Earth. Secondly, we also find that the size sorting could also result from kinetic sieving encountered during granular avalanches. Finally, we discuss how the void-filling mechanism becomes more efficient when there is a higher relative size difference between the boulders and the surrounding grains. Our model has important implications in understanding the resurfacing of Itokawa by trying to explain one of the many complex geophysical processes that occur in such unique conditions.
url https://www.epj-conferences.org/articles/epjconf/pdf/2021/03/epjconf_pg2021_03042.pdf
work_keys_str_mv AT ghoshsohanjit granularsegregationontherubblepileasteroiditokawa
AT sharmaishan granularsegregationontherubblepileasteroiditokawa
AT dhingradeepak granularsegregationontherubblepileasteroiditokawa
_version_ 1721224562858786816