“…For instance, the famous Lense-Thirring effect (Lense and Thirring 1918), that is the precessions of the node and the periapsis of a satellite orniting a central spinning mass, has been analyzed in different contexts: there are the LAGEOS tests around the Earth (Ciufolini and Pavlis 2004; Matteo Luca Ruggiero 1 DISAT, Politecnico di Torino, Corso Duca degli Abruzzi 24, Torino, Italy INFN, Sezione di Torino, Via Pietro Giuria 1, Torino, Italy 2010a), the MGS tests around Mars (Iorio 2006a(Iorio , 2010 and other tests around the Sun and the planets (Iorio 2012a); see Ciufolini (2007); Iorio et al (2011Iorio et al ( , 2013; Renzetti (2013b) for a discussion and a review of the recent results. In February 2012 the LARES mission (Ciufolini et al 2012) has been launched to measure the Lense-Thirring effect of the Earth, and is now gathering data; a comprehensive discussion on this mission can be found in Iorio (2005Iorio ( , 2009); Renzetti (2013aRenzetti ( , 2012; Ciufolini et al (2010bCiufolini et al ( , 2015. In the recent past, the Gravity Probe B (Everitt et al 2011) mission was launched to measure the precession of orbiting gyroscopes (Pugh 1959;Schiff 1960).…”