Definition of multispectral camera system parameters to model the asteroid 2001 SN263

TL;DR

This paper defines parameters for a multispectral camera system to study the triple asteroid 2001 SN263, using software simulations to assist mission planning and improve imaging strategies.

Contribution

It introduces a simulation-based method to determine optimal multispectral camera parameters for asteroid imaging, aiding the ASTER mission planning.

Findings

Alpha is fully visible only in WAC images.

NAC reveals surface details and broad views at 100 km.

Camera orbit adjustments are needed to image Gamma behind Alpha.

Abstract

In 2012, Brazil began the studies to send its first deep space exploration mission, ASTER, which would be the first mission to orbit a triple asteroid system, 2001 SN263. We aim to contribute to the ASTER mission by defining the parameters of a multispectral camera system that will be used to study the asteroid system 2001 SN263, through software simulations that should help planning the data collection. We inserted the shape model of the objects in the software POV-Ray and modeled two cameras, a Wide Angle (WAC) and a Narrow Angle (NAC). We inserted the asteroid's parameters and simulated the satellite position. We created various scenes so we could obtain a good view of the asteroid. Alpha is entirely visible only in the WAC images, while the NAC is expected to reveal surface details. Beta seems relatively small in the WAC images, whereas we obtain a broad view from the NAC at 100 km distance. Gamma, smaller than Beta, should provide more detailed images through the NAC, whereas the WAC images should be able to show its inclined orbit around Alpha. To see Gamma behind Alpha in its revolution movement, we would have to elevate the camera's orbit. The method employed to simulate images generated by satellite cameras can be applied to other scenarios where the target requires imaging, extending beyond the field of planetary geology.