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Image of the Moon obtained by the narrow-angle camera (UTK TSNN)
Imaging results validated resolution and sensitivity of UTK TSNN and confirmed the possibility of its use for the imaging Phobos with high-resolution from Martian artifial satellite orbits.
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Images of the Moon obtained by the wide-angle camera (UTK TSNN) with different accumulation periods
The linearity of TSNN cameras light-signal is confirmed. The absence of charge spreading for maximum accumulation periods is checked. This will make it possible to image Phobos on the background of stars for the solution of navigational problems.
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The observation of stars passing through a wide-angle camera's (ShTK TSNN) field of view
The possibility of registering by ShTK the stars of up to 5th magnitude is confirmed. Monitoring the movements of the stars in the TSNN cameras' field of view will, allow in particular, to check s/c attitude control system in flight.
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