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GRAINS SIGNED

Gravitation of Rubble-pile Asteroid with Internal N-body Structure

Total Cost €

0

EC-Contrib. €

0

Partnership

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Project "GRAINS" data sheet

The following table provides information about the project.

Coordinator
POLITECNICO DI MILANO 

Organization address
address: PIAZZA LEONARDO DA VINCI 32
city: MILANO
postcode: 20133
website: www.polimi.it

contact info
title: n.a.
name: n.a.
surname: n.a.
function: n.a.
email: n.a.
telephone: n.a.
fax: n.a.

 Coordinator Country Italy [IT]
 Project website https://www.researchgate.net/project/GRAINS
 Total cost 176˙203 €
 EC max contribution 176˙203 € (100%)
 Programme 1. H2020-EU.1.3.2. (Nurturing excellence by means of cross-border and cross-sector mobility)
 Code Call H2020-MSCA-IF-2017
 Funding Scheme MSCA-IF-GF
 Starting year 2018
 Duration (year-month-day) from 2018-06-01   to  2020-05-31

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    POLITECNICO DI MILANO IT (MILANO) coordinator 176˙203.00
2    NATIONAL AERONAUTICS AND SPACE ADMINISTRATION US (WASHINGTON) partner 0.00

Map

 Project objective

The study of asteroids addresses a number of questions relevant for space engineers, planetary scientists and physicists. Near Earth Asteroids are a great opportunity for technological, human exploration missions and for asteroids resources exploitation. Sadly, they can also represent a threat for the planet. The scientific and technological exploitation and the implementation of mitigation actions for hazardous asteroids rely upon our knowledge of their properties. Remote surveys play a fundamental role to estimate asteroid properties, but they can only provide limited information: there is no mean to reconstruct their internal structure. GRAINS addresses such problem through N-body numerical simulations of gravitational aggregation. This method is suitable to estimate the internal properties of rubble-pile asteroids: gravitational aggregates with very low tensile strength and high level of porosity. The study of aggregation phenomena currently relies on codes optimized for a large number of mutually interacting particles, regardless of their individual shape and rigid body motion. Although not relevant for many applications, this limitation could be relevant for the case of asteroids, as suggested by results of granular dynamics in terrestrial engineering applications. The latter are commonly studied using multi-body codes, able to simulate contact interactions between a large number of complex-shaped bodies, but not suitable for gravitational dynamics. The goal of the project is to joint the advantages of both classes of codes into a single implementation, able to reproduce N-body gravitational dynamics between a large number of complex-shaped rigid bodies. GRAINS plans to use the implemented code to study relevant aggregation scenarios and to assess the accuracy of obtained asteroid models. The outcome of the GRAINS project will be a new and powerful tool to study asteroids and their internal properties based on information available from remote observations.

 Publications

year authors and title journal last update
List of publications.
2020 Fabio Ferrari, Michèle Lavagna, Emmanuel Blazquez
A parallel-GPU code for asteroid aggregation problems with angular particles
published pages: 749-761, ISSN: 0035-8711, DOI: 10.1093/mnras/stz3458
Monthly Notices of the Royal Astronomical Society 492/1 2020-03-24
2019 Ferrari, F.
A New Environment to Simulate the Dynamics in the Close Proximity of Rubble-Pile Asteroids
published pages: 2065-2075, ISSN: , DOI:
Advances in the Astronautical Sciences 168 2020-01-27
2018 F. Ferrari, M. Lavagna
A code for the study of gravitational aggregates with non-spherical particles
published pages: , ISSN: , DOI:
Proceedings of the 2018 European Planetary Science Congress (EPSC) 2019-06-06
2018 F. Ferrari, M. Lavagna
GRAINS: a new numerical method for the study of gravitational aggregates
published pages: , ISSN: , DOI:
Proceedings of the 42nd COSPAR Scientific Assembly 2019-05-29

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