UK Activities: NEO Characterisation

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Presentation transcript:

UK Activities: NEO Characterisation Simon F. Green Planetary and Space Sciences Department of Physical Sciences The Open University Apologies for the very brief abstract. Will briefly review the evidence for grain fragmentation and outline its possible consequences for Rosetta. SMPAG, Vienna, 12-13 June 2014

Dynamics Composition Surveys/Astrometry Dynamical modelling Queen’s Belfast Pan-STARRS1 asteroid science co-lead Cometary activity, collisions LSST data products UK proposal lead Dynamical modelling Armagh, Queen Mary London Long-term evolution, Yarkovsky effect Composition Remote sensing Queen’s Belfast, Kent, Oxford Vis/NIR & mid-IR spectroscopy Returned samples/meteorites Open Univ., Imperial, Manchester, NHM, UCL/Birkbeck, Leicester, Oxford, Bristol, Glasgow, Kent, Edinburgh UK Cosmochemistry Analysis Network

Instruments for missions Physical Properties Shapes and Spin Kent, Queen’s Belfast, Open Univ. Shape, spin rate & axis orientation from light curve observation & inversion Spin/obliquity changes from observations & thermophysical modelling Thermophysical properties Open Univ., Oxford Albedo, Diameter, Temperature, thermal inertia, surface roughness from IR observation & thermal models. YORP/Yarkovsky effect, density Instruments for missions Oxford: IR spectrometer, electrical charging MSSL/UCL: Cameras Open Univ.: Mass spectrometer Leicester: X-ray spectrometer Imperial: Magnetometer