@article{12557,
  keywords = {Space and Planetary Science, Astronomy and Astrophysics},
  author = {L. Iess and S. Asmar and P. Cappuccio and G. Cascioli and F. De Marchi and I. di Stefano and A. Genova and N. Ashby and J. Barriot and Peter Bender and C. Benedetto and J. Border and F. Budnik and S. Ciarcia and T. Damour and V. Dehant and G. Di Achille and A. Di Ruscio and A. Fienga and R. Formaro and S. Klioner and A. Konopliv and A. Lemaître and F. Longo and M. Mercolino and G. Mitri and V. Notaro and A. Olivieri and M. Paik and A. Palli and G. Schettino and D. Serra and L. Simone and G. Tommei and P. Tortora and T. Van Hoolst and D. Vokrouhlický and M. Watkins and X. Wu and M. Zannoni},
  title = {Gravity, Geodesy and Fundamental Physics with BepiColombo’s MORE Investigation},
  abstract = {The Mercury Orbiter Radio Science Experiment (MORE) of the ESA mission BepiColombo will provide an accurate estimation of Mercury's gravity field and rotational state, improved tests of general relativity, and a novel deep space navigation system. The key experimental setup entails a highly stable, multi-frequency radio link in X and Ka band, enabling two-way range rate measurements of 3 micron/s at nearly all solar elongation angles. In addition, a high chip rate, pseudo-noise ranging system has already been tested at 1-2 cm accuracy. The tracking data will be used together with the measurements of the Italian Spring Accelerometer to provide a pseudo drag free environment for the data analysis. We summarize the existing literature published over the past years and report on the overall configuration of the experiment, its operations in cruise and at Mercury, and the expected scientific results.},
  year = {2021},
  journal = {Space Science Reviews},
  volume = {217},
  month = {2021-02},
  publisher = {Springer Science and Business Media LLC},
  issn = {0038-6308, 1572-9672},
  doi = {10.1007/s11214-021-00800-3},
}