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Modeling of double asteroids
with PIKAIA algorithm
Przemysław Bartczak
Astronomical Observatory of A. Mickiewicz University
Idea of modelling
Observation data
Model of binary system
simulation
Model of system
Body frame: The axes are directed along the principal moments of interia of the primary.
Fixed frame: the axes are aligned with some suitably chosen astronomical coordinate system.
Both system of axes are Cartesian, right-handed and share the same origin 0,
located at the center of mass of the primary
Cayley-Klein parameters:
Euler angles:
Rotation angle α
Nutation angle β
Precession angle γ
Drawback:
undetermined for
β=0 or β=π
Model of system
When the primary rotates, the Cayley-Klein parameters change according to
the differential equations
where Ω is the angular rate vector in body frame.
Model of system
Dynamics equations describe the orbital motion of the satelite with respect
to the primary and rotation of primary .
Ω - Angular rate vector
R - Satelite’s radius vector
P - Momentum vector
Γ - Angular momentum vector
J1,J2,J3 – principal moments
Model of system
Constans of motion:
Hamiltonian:
Total angular momentum vector:
Cayley-Klein parameters:
Integrating the equations of motion by means of the Raudau-Everhart RA-15 procedure,
we have obtained highly accurate results within a fairly short computation time.
Model of shape
The dynamical part of the model
(free or forced precession)
Primary:
Satellite:
Three-axial ellipsoid
Spherical
Model of shape
The synchronous double asteroids
Primary and satellite:
Three-axial elipsoids plus
two craters.
Primary and satellite:
Three-axial elipsoids
Model of shape
YORP
Only one body:
Triangular faces
Input parameters
Date of observation
Position of asteroid
(Orbital elements )
Position of Sun and
Earth
Orientation of
binary system
Model of shape
and binary system
Modelling of lightcurve
Model of lightcurve
• Ray tracing is a technique for generating an image by tracing the
path of light through pixels in an image plane and simulating the effects of
its encounters with virtual objects.
Scattering : Lommel-Seeliger law
Model of lightcurve
• Ray tracing
Modelling of lightcurve
• Z-buffering is the management of image depth coordinates in
three-dimensional (3-D) graphics.
The depth of a generated pixel (z coordinate) is stored in a buffer
(the z-buffer or depth buffer)
Modelling of lightcurve
• Z-buffering
PIKAIA – genetic algorithm
Genetic algorithms are a class
of search techniques inspired
from the biological process of
evolution by means of natural
selection.
PIKAIA – genetic algorithm
System:
Determined parameters of model (blue):
Shape:
Period ,
density ,
Rotation angle α,
Nutation angle β
Precession angle γ
primary:
a, b/a, c/a
secoundary: a, b/a, c/a
Deformation:
2 craters: (8 parameters)
Parallel computing
SQL
database
PC
PC
System: Debian
Compilator: gcc,c++
SQL database: MySql , oracleXe
Librares: CORBA, POSIX Threads
PC
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