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High precision astrometry provides the foundation to resolve many fundamentalproblems in astrophysics. The application of astrometric studies spans a widerange of fields, and has undergone enormous growth in recent years. This is asa consequence of the increasing measurement precision and wide applicability,which is due in turn to the development of new techniques. Forthcoming nextgeneration observatories have the potential to further increase the astrometricprecision, providing there is a matching improvement in the methods to correctfor systematic errors. The EVN and other observatories are providingdemonstrations of these and are acting as pathfinders for next-generationtelescopes such as the SKA and ngVLA. We will review the perspectives for thecoming facilities and examples of the current state-of-the-art for astrometry.

(Ultra) Precise Astrometry today and tomorrow, with Next-generation Observatories