“…Concerning the solar system objects, Gaia will determine the orbits of hundreds of thousands of main-belt asteroids, near-Earth and Kuiper-Belt objects (Tanga & Mignard 2012). Gaia will be complemented by on-going or proposed large-scale photometric and spectroscopic surveys, both in the visible and in the infrared: VPHAS+ (Drew 2012, UKIDSS, VVV VISTA (Saito et al 2012) RAVE (Siebert 2012)), APOGEE (Majewski 2010), Hermes (Freeman 2012), Gaia-ESO Survey (Gilmore et al 2012) and LAMOST Surveys as discussed in this Conference. …”