| Literature DB >> 25873744 |
Hans-Ulrich Auster1, Istvan Apathy2, Gerhard Berghofer3, Karl-Heinz Fornacon4, Anatoli Remizov5, Chris Carr6, Carsten Güttler7, Gerhard Haerendel8, Philip Heinisch4, David Hercik4, Martin Hilchenbach7, Ekkehard Kührt9, Werner Magnes3, Uwe Motschmann10, Ingo Richter4, Christopher T Russell11, Anita Przyklenk4, Konrad Schwingenschuh3, Holger Sierks8, Karl-Heinz Glassmeier12.
Abstract
Knowledge of the magnetization of planetary bodies constrains their origin and evolution, as well as the conditions in the solar nebular at that time. On the basis of magnetic field measurements during the descent and subsequent multiple touchdown of the Rosetta lander Philae on the comet 67P/Churyumov-Gerasimenko (67P), we show that no global magnetic field was detected within the limitations of analysis. The Rosetta Magnetometer and Plasma Monitor (ROMAP) suite of sensors measured an upper magnetic field magnitude of less than 2 nanotesla at the cometary surface at multiple locations, with the upper specific magnetic moment being <3.1 × 10(-5) ampere-square meters per kilogram for meter-size homogeneous magnetized boulders. The maximum dipole moment of 67P is 1.6 × 10(8) ampere-square meters. We conclude that on the meter scale, magnetic alignment in the preplanetary nebula is of minor importance.Entities:
Year: 2015 PMID: 25873744 DOI: 10.1126/science.aaa5102
Source DB: PubMed Journal: Science ISSN: 0036-8075 Impact factor: 47.728