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  • On the Rotation Period and ...
    Knight, Matthew M.; Protopapa, Silvia; Kelley, Michael S. P.; Farnham, Tony L.; Bauer, James M.; Bodewits, Dennis; Feaga, Lori M.; Sunshine, Jessica M.

    Astrophysical journal. Letters, 12/2017, Letnik: 851, Številka: 2
    Journal Article

    We observed the newly discovered hyperbolic minor planet 1I/'Oumuamua (2017 U1) on 2017 October 30 with Lowell Observatory's 4.3 m Discovery Channel Telescope. From these observations, we derived a partial lightcurve with a peak-to-trough amplitude of at least 1.2 mag. This lightcurve segment rules out rotation periods less than 3 hr and suggests that the period is at least 5 hr. On the assumption that the variability is due to a changing cross-section, the axial ratio is at least 3:1. We saw no evidence for a coma or tail in either individual images or in a stacked image having an equivalent exposure time of 9000 s.