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The findings of Micheli et al. (Nature2018, 559, 223–226) that 1I/2017 U1 ('Oumuamua) showed anomalous orbital accelerations have motivated us to apply an impact model of gravity in search for an explanation. A small deviation from the 1/r potential, where r is the heliocentric distance, is expected for the gravitational interaction of extended bodies as a consequence of this model. This modification of the potential results from an offset of the effective gravitational centre from thedoi:10.3390/galaxies8040083 fatcat:ozhrdn3prnfxje2w4m2gu5542q