Direct Detections of the Asteroidal YORP Effect

Lead Research Organisation: University of Kent
Department Name: Sch of Physical Sciences

Abstract

Telescope time has been awarded to study the asteroidal YORP effect.

Proposal Abstract: The YORP effect is a torque experienced by small asteroids that is due to both incident solar radiation pressure and the recoil effect from the anisotropic emission of thermal photons. It can modify their rotation rates and spin-axis orientations, and can explain many observed phenomena in asteroidal science. We will use the INT+WFC to obtain lightcurve coverage of several NEAs which are targets of an ESO Large Programme, the aim of which is to directly detect YORP-induced rotation period changes amongst a large sample of NEAs. The aim of this project is not to determine highly accurate period solutions for the objects, but rather to assist in the measurement of any potential phase offset in the asteroids' rotational lightcurve due to the YORP effect. The lightcurve data obtained at the INT will prove crucial to this programme since some of the targets are now unobservable from ESO.

Publications

10 25 50
 
Description British Astronomical Association, Open University 
Form Of Engagement Activity A talk or presentation
Part Of Official Scheme? No
Geographic Reach National
Primary Audience Public/other audiences
Results and Impact Invited lecture at British Astronomical Association, Open University

See above
Year(s) Of Engagement Activity 2012
URL http://lists.britastro.org/pipermail/comets-disc/2012-May/000021.html
 
Description UKSEDS: March 2012 
Form Of Engagement Activity A talk or presentation
Part Of Official Scheme? No
Geographic Reach Regional
Primary Audience Public/other audiences
Results and Impact Invited Lectuer at UK Students for the Development and Exploration of Space (SEDS) Conference, Hosted at the University of Kent

See above
Year(s) Of Engagement Activity 2012
URL http://ukseds.org/wp-content/uploads/2012/03/conference-poster-2012.pdf