This is one of four year-long projects, that I produced in High School. You can go back to the main page of these projects.
Embedded Files
Asteroid modelling
Asteroid modelling
limity_inverzni_metody_SOC2020_marco_souzadejoode.pdf
Stefanik observatory, Prague
Stefanik observatory, Prague
Stefanik observatory, Prague
Stefanik observatory, Prague
Probability of direction of the rotation axis of an asteroid
Probability of direction of the rotation axis of an asteroid
Observation of the asteroid (511) Davida from Prague Observatory
Observation of the asteroid (511) Davida from Prague Observatory
Dark areas correspond to probable directions of the axis of rotation.
Dark areas correspond to probable directions of the axis of rotation.
Each map like this demanded approx. 30 CPU hours.
Each map like this demanded approx. 30 CPU hours.
Philiosophia
Philiosophia
Lucretia
Lucretia
This work quantifies the quality of the observation of a given asteroid based on the variety of the observational geometries.
This asteroid has been sparsely observed.
With more observations, the multiplicity of possible solutions collapse.
With a set of observations like this, a unique (convex) solution of the shape of the asteroid can be probably derived.
Occultation of a dim star by an asteroid
Occultation of a dim star by an asteroid
The asteroid Juno
The asteroid Juno
3D printed models
3D printed models
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