TY  - JOUR
A1  - Postberg, Frank
A1  - Grün, Eberhard
A1  - Horanyi, Mihaly
A1  - Kempf, Sascha
A1  - Krueger, Harald
A1  - Schmidt, Jürgen
A1  - Spahn, Frank
A1  - Srama, Ralf
A1  - Sternovsky, Zoltan
A1  - Trieloff, Mario
T1  - Compositional mapping of planetary moons by mass spectrometry of dust ejecta
T2  - Planetary and space science
N2  - Classical methods to analyze the surface composition of atmosphereless planetary objects from an orbiter are IR and gamma ray spectroscopy and neutron backscatter measurements. The idea to analyze surface properties with an in-situ instrument has been proposed by Johnson et al. (1998). There, it was suggested to analyze Europa's thin atmosphere with an ion and neutral gas spectrometer. Since the atmospheric components are released by sputtering of the moon's surface, they provide a link to surface composition. Here we present an improved, complementary method to analyze rocky or icy dust particles as samples of planetary objects from which they were ejected. Such particles, generated by the ambient meteoroid bombardment that erodes the surface, are naturally present on all atmosphereless moons and planets. The planetary bodies are enshrouded in clouds of ballistic dust particles, which are characteristic samples of their surfaces. In situ mass spectroscopic analysis of these dust particles impacting onto a detector of an orbiting spacecraft reveals their composition. Recent instrumental developments and tests allow the chemical characterization of ice and dust particles encountered at speeds as low as 1 km/s and an accurate reconstruction of their trajectories. Depending on the sampling altitude, a dust trajectory sensor can trace back the origin of each analyzed grain with about 10 km accuracy at the surface. Since the detection rates are of the order of thousand per orbit, a spatially resolved mapping of the surface composition can be achieved. Certain bodies (e.g., Europa) with particularly dense dust clouds, could provide impact statistics that allow for compositional mapping even on single flybys. Dust impact velocities are in general sufficiently high at orbiters about planetary objects with a radius > 1000 km and with only a thin or no atmosphere. In this work we focus on the scientific benefit of a dust spectrometer on a spacecraft orbiting Earth's Moon as well as Jupiter's Galilean satellites. This 'dust spectrometer' approach provides key chemical and isotopic constraints for varying provinces or geological formations on the surfaces, leading to better understanding of the body's geological evolution.
KW  - Moon
KW  - Europa
KW  - Ganymede
KW  - Dust
KW  - Surface composition
KW  - Spectrometry
Y1  - 2011
UR  - https://publishup.uni-potsdam.de/frontdoor/index/index/docId/36536
SN  - 0032-0633
VL  - 59
IS  - 14
SP  - 1815
EP  - 1825
PB  - Elsevier
CY  - Oxford
ER  -