摘要:Context.The binary asteroid 288P/(300163) is unusual both for its combination of wide-separation and high mass ratio and for its comet-like activity. It is not currently known whether there is a causal connection between the activity and the unusual orbit or if instead the activity helped to overcome a strong detection bias against such sub-arcsecond systems.Aims.We aim to find observational constraints discriminating between possible formation scenarios and to characterise the physical properties of the system components.Methods.We measured the component separation and brightness using point spread function fitting to high-resolutionHubbleSpace Telescope/Wide Field Camera 3 images from 25 epochs between 2011 and 2020. We constrained component sizes and shapes from the photometry, and we fitted a Keplerian orbit to the separation as a function of time.Results.Approximating the components A and B as prolate spheroids with semi-axis lengthsa