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About

Paolo Tortora is a leading figure in planetary science and space exploration, whose work has profoundly shaped our understanding of the outer Solar System. His primary research focuses on the dynamics, interiors, and exploration of ice giants—Uranus and Neptune—as well as the development of advanced radio science techniques for spacecraft navigation. Tortora’s major contributions include co-authoring the influential "Ice giant system exploration within ESA’s Voyage 2050" paper, which laid the scientific and technical groundwork for a flagship mission to these enigmatic worlds. This work, cited over a dozen times, has been instrumental in prioritizing ice giant exploration as a key objective for the European Space Agency. Beyond this, Tortora has made significant strides in improving the accuracy of interplanetary trajectory determination, enabling more precise measurements of planetary gravity fields and atmospheric properties. His research has directly supported missions like BepiColombo and JUICE, cementing his reputation as a bridge between theoretical planetary science and practical spaceflight engineering. With a career marked by high-impact studies and leadership in mission concept development, Tortora continues to inspire the next generation of planetary scientists.