The 2025 meeting of the European Geosciences Union has occurred. And yes, there was relevant content in a geophysics conference. Small bodies are subject to physical laws too:
https://meetingorganizer.copernicus.org/EGU25/meetingprogramme
Monday, 28 April
Tue, 29 Apr
Wed, 30 Apr
Thu, 01 May
Fri, 02 May
EGU25-17253
Seismic Instrument for Asteroids (SIA): a seismometer based on geophone sensors for the RAMSES mission to Apophis
EGU25-19903
EGU25-13874
Gravity Science Goals for the UAE EMA MissionOrals | PS1.2
EGU25-4502
Meteoric Metal Layers in the Upper Atmosphere of VenusOrals | PS3.1
EGU25-2571
Asteroids fail to retain cometary impact signatures
EGU25-11674
A nearly terrestrial D/H for comet 67P/Churyumov-GerasimenkoEGU25-11684
Insights into Resolving the Sub-surface Structure of Cometary Analogues using THz SpectroscopyEGU25-14120
Apophis Recon Swarm (ARS): Rapid-response Multi-flyby mission to Apophis using a CubeSats Swarm
EGU25-16419
Exploring Meteorite Diversity: A Statistical and Compositional Review of the Meteorites in the SAASST CollectionEGU25-18541
Insights into Asteroid Vesta: Mineralogical and Elemental Characterization of HED MeteoriteEGU25-21780
The sample analysis laboratory (SAL) at the German Aerospace Center (DLR) Berlin – A cutting edge laboratory for extraterrestrial material analysisEGU25-16881
Detection of NH-rich compounds in Bennu pristine samples via IR characterization at JAXA Curation Center and comparison with Ryugu Te Jiang et al.
PICO | GD3.1
EGU25-8161
Provenance of Earth’s volatile building blocks inferred from the behaviour of nitrogen during core formation
EGU25-4563
Colour and Time: The Evolution of Crater Rays on the Moon and the Asteroid 4Vesta
Orals | PS4.1
EGU25-8733
Solar wind interaction with comet 67P around perihelion – the formation of a cometosheathOrals | PS1.4
EGU25-19582
First Results from Thermal Infra-Red Imager (TIRI) during Hera’s Mars Swing-ByEGU25-12293
Determining a good Phobos simulant: An organic analysis based on spectral similarities between Phobos, Tagish Lake, and CM chondritic meteorites
Orals | MAL27-GMPVEGU25-4830
Application of the finite element method to the modelling of the gravitational field of asteroidsl.
EGU25-10368
Global gravitational field modelling for spheroidal planetary bodies: non-singular solutionsPosters on site | PS3.1
EGU25-18272
Predictions for the interior of asteroid Dimorphos through the DART-scale impact modeling Cem Berk Senel et al.
EGU25-8804
Kalliope: Discovery of the first metallic asteroid familyEGU25-19303
Mission AVERT: A Geoscience Escape RoomEGU25-2732 | Posters on site | PS6.1
Comparison of micro-spectroscopic signatures of 2 peculiar CM-type meteorites: Asuka 12236 and Paris. Zahia Djouadi et al.
EGU25-21930 | ECS | Posters on site | PS6.1
EGU25-11994 | ECS | Posters on site | PS7.2
Composition Analysis of an Allende Chondrule using a Space-Prototype Laser Ablation Ionization Mass Spectrometer l.EGU25-12911 | ECS | Posters on site | AS5.13
Spectroscopy of gas plumes in the laboratory: remote sensing of comets and icy satellitesEGU25-6228 | Posters virtual | VPS27
Finding the optimal flyby distance for the Comet Interceptor comet missionEGU25-12930 | ECS | Posters virtual | VPS27
Salts produced by hydrothermal alteration of soluble organic matter in CI chondrite parent bodies Sidonie Coker et al.