Modeling and Simulation of Asteroid Capture Using a Deformable Membrane Capture Device

Author(s):  
Håvard Fjær Grip ◽  
Miguel San Martin ◽  
Abhinandan Jain ◽  
Bob Balaram ◽  
Jonathan Cameron ◽  
...  

The National Aeronautics and Space Administration have recently been investigating a mission concept known as the Asteroid Redirect Mission, aimed at collecting a large amount of asteroid material and transporting it into lunar orbit for inspection by human astronauts. Of the two mission options that have been considered, one involves the capture of an entire near-Earth asteroid in the 10-m class by a robotic spacecraft. The spacecraft would first make contact with the asteroid through a deformable membrane, before securing it inside a large flexible bagging mechanism. In this paper we describe the development and implementation of a model designed for simulation of the capture process, which includes a low-complexity representation of the interaction dynamics.

2018 ◽  
Vol 61 (8) ◽  
pp. 2099-2115 ◽  
Author(s):  
Minghu Tan ◽  
Colin McInnes ◽  
Matteo Ceriotti

2018 ◽  
Vol 41 (3) ◽  
pp. 632-643 ◽  
Author(s):  
Minghu Tan ◽  
Colin R. McInnes ◽  
Matteo Ceriotti

2013 ◽  
Vol 37 ◽  
pp. 1855-1862 ◽  
Author(s):  
Youngsub Lim ◽  
Jeongnam Kim ◽  
Jaeheum Jung ◽  
Chi Seob Lee ◽  
Chonghun Han

2014 ◽  
Vol 9 (S310) ◽  
pp. 142-145
Author(s):  
D. Farnocchia ◽  
M. Mommert ◽  
J. L. Hora ◽  
S. R. Chesley ◽  
D. Vokrouhlický ◽  
...  

AbstractWe analyze the trajectory of near-Earth asteroid 2009~BD, which is a candidate target of the NASA Asteroid Redirect Mission. The small size of 2009 BD and its Earth-like orbit pose challenges to understanding the dynamical properties of 2009 BD. In particular, nongravitational perturbations, such as solar radiation pressure and the Yarkovsky effect, are essential to match observational data and provide reliable predictions. By using Spitzer Space Telescope IRAC observations and our model for the thermophysical properties and the nongravitational forces acting on 2009 BD we obtain probabilistic derivations of the physical properties of this object. We find two physically possible solutions. The first solution shows 2009 BD as a 2.9 ± 0.3 m diameter rocky body with an extremely high albedo that is covered with regolith-like material, causing it to exhibit a low thermal inertia. The second solution suggests 2009 BD to be a 4 ± 1 m diameter asteroid with albedo 0.45 ± 0.35 that consists of a collection of individual bare rock slabs. We are unable to rule out either solution based on physical reasoning. 2009 BD is the smallest asteroid for which physical properties have been constrained, providing unique information on the physical properties of objects in the size range smaller than 10 m.


2009 ◽  
Vol 1 (1) ◽  
pp. 1381-1386 ◽  
Author(s):  
Bhurisa Thitakamol ◽  
Amornvadee Veawab ◽  
Adisorn Aroonwilas

1999 ◽  
Vol 173 ◽  
pp. 327-338 ◽  
Author(s):  
J.A. Fernández ◽  
T. Gallardo

AbstractThe Oort cloud probably is the source of Halley-type (HT) comets and perhaps of some Jupiter-family (JF) comets. The process of capture of Oort cloud comets into HT comets by planetary perturbations and its efficiency are very important problems in comet ary dynamics. A small fraction of comets coming from the Oort cloud − of about 10−2− are found to become HT comets (orbital periods < 200 yr). The steady-state population of HT comets is a complex function of the influx rate of new comets, the probability of capture and their physical lifetimes. From the discovery rate of active HT comets, their total population can be estimated to be of a few hundreds for perihelion distancesq <2 AU. Randomly-oriented LP comets captured into short-period orbits (orbital periods < 20 yr) show dynamical properties that do not match the observed properties of JF comets, in particular the distribution of their orbital inclinations, so Oort cloud comets can be ruled out as a suitable source for most JF comets. The scope of this presentation is to review the capture process of new comets into HT and short-period orbits, including the possibility that some of them may become sungrazers during their dynamical evolution.


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