EGU26-22731, updated on 14 Mar 2026
https://doi.org/10.5194/egusphere-egu26-22731
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Oral | Thursday, 07 May, 09:30–09:40 (CEST)
 
Room 0.96/97
Science objectives of ESA's Genesis mission: a flying geodetic observatory to improve ITRF accuracy and stability 
Özgür Karatekin1, Francesco Vespe2, Zuheir Altamimi3, Florian Seitz4, Rolf Dach5, Benjamin Männel6, Rüdiger Haas7, Guilhem Moreaux8, Clément courde9, Antonia Bieringer10, Erik Schoenemann10, Pierre Waller10, Gaia Fusco10, Sara Gidlund10, and the Genesis Science Exploitation Team*
Özgür Karatekin et al.
  • 1Royal Observatory of Belgium
  • 2ASI Space Geodesy Centre at Matera, Italy
  • 3Institut national de l'information géographique et forestière – IGN, France
  • 4Deutsches Geodätisches Forschungsinstitut-Technische Universität München – DGFI-TUM, Germany
  • 5Universität Bern, Switzerland
  • 6Deutsches GeoForschungsZentrum – GFZ, Germany
  • 7Chalmers Tekniska Högskola, Sweden
  • 8CLS-Collecte Localisation Satellites, Franc
  • 9Centre national de la recherche scientifique-Géoazur, France
  • 10ESA ESTEC, Netherlands
  • *A full list of authors appears at the end of the abstract

Genesis is an ESA mission in preparation within the Navigation Directorate under the FutureNAV Programme, dedicated to advancing space geodetic science and the International Terrestrial Reference Frame (ITRF). It co-locates GNSS, SLR, DORIS, and a pioneering VLBI transmitter on a single satellite in near-polar orbit (~6000 km), creating a dynamic space geodetic observatory that delivers well-calibrated space ties between all techniques.

These co-located measurements enable rigorous integration of space-geodetic techniques, revealing and mitigating inter-technique biases that currently limit ITRF scale, origin, and orientation. The Genesis objectives demand a stable and well-characterised platform as well as rigorous calibration of instruments and antennas, including phase/group delays and phase center offsets. The mission's novelty and methodology at mm-level demand also the careful preparation of observation strategies and adoption of data analysis and combination techniques for Genesis data exploitation.

Here, we present an overview of the ongoing activities relevant to the science community and ITRF realisation, including the scientific objectives and the status and plans of science instruments and calibrations. The scientific datasets and expected data products, along with their planned availability to the scientific community, will also be discussed.

Genesis Science Exploitation Team:

Genesis Science Exploitation Team

How to cite: Karatekin, Ö., Vespe, F., Altamimi, Z., Seitz, F., Dach, R., Männel, B., Haas, R., Moreaux, G., courde, C., Bieringer, A., Schoenemann, E., Waller, P., Fusco, G., and Gidlund, S. and the Genesis Science Exploitation Team: Science objectives of ESA's Genesis mission: a flying geodetic observatory to improve ITRF accuracy and stability , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22731, https://doi.org/10.5194/egusphere-egu26-22731, 2026.