Detlef KoschnyPlanetary Scientist
Main Research Fields
My main scientific interest is cosmic dust, meteors, fireballs, and other minor bodies in the solar system, in particular asteroids. I am focussing on the analysis of observational data and the usage of optical cameras.
I am currently sharing my time between working as 'Instrument Coordinator' for the Close-Up Imager (CLUPI) on ExoMars 2020 and as Co-Manager of the near-Earth object segment of ESA's Space Situational Awareness programme (SSA-NEO).
The following bullets focus on my research activities.
- ground-based observations of meteors using image-intensified video systems
- prepare for obtaining meteor observations from space
- follow-up observations of asteroids and testing survey strategies
- impact experiments in ice and regolith targets
- testing cameras for ground- and space-based applications
- Current instrument involvements: Co-I and Instrument Coordinator for the Close-up Imager CLUPI for the ExoMars 2020 rover; Co-I on the scientific camera OSIRIS on Rosetta
- Data analysis of meteor and fireball data and Rosetta dust data with Univ. Oldenburg, Germany
- Near-Earth object research with the Lehrstuhl für Raumfahrttechnik, Technische Universität München
- Part of the NELIOTA science team observing lunar impact flashes
Project/mission at ESA
These are missions I have been/am involved in (not only from a scientific point of view):
Missions which are/have been in operation: Rosetta, Smart-1, Venus Express, Chandrayaan-1 (ISRO), ExoMars 2016
Missions in development: BepiColombo, ExoMars 2020
Before joining ESA, I was working on: Spacelab D2, Cassini-Huygens, Mars Pathfinder, Mars Polar Lander.
Mission studies: MoonNEXT, Marco Polo, MarcoPolo-R, Phootprint, Asteroid Impact Monitoring mission (AIM), Martian Moon Sample Return, Phobos Sample Return (several) - plus several internal studies done in our so-called Concurrent Design Facility.
For the work we do on meteors, see http://cosmos.esa.int/meteor.
For the technical web portal of our SSA-NEO segment, see http://neo.ssa.esa.int.