Francesco Basile
Modeling and Design for the Attitude Control Phase of the LISA drag-free Mission.
Rel. Carlo Novara, Elisa Capello. Politecnico di Torino, Corso di laurea magistrale in Ingegneria Aerospaziale, 2019
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Abstract
The Laser Interferometer Space Antenna (LISA) is a Space mission led by ESA now entering its phase A. LISA will be the first observatory in space to explore the Gravitational Universe. It will gather revolutionary information about the dark universe. The new LISA mission envisaged as a joint ESA-NASA mission to observe astrophysical and cosmological sources of low frequency gravitational waves. The primary objective of the LISA mission is to detect and observe gravitational waves emitted from massive black holes and galactic binaries in the low-frequency band which ranges from 0:1mHz up to 1Hz with a goal of extending the measurements down to 30mHz.
The underlying measurement principle is a laser interferometry system built up with three satellites that are flying in a triangular constellation with an edge length of 2:5Mkm
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