It was observed at the next predicted apparition by Gérard Sause at the Observatoire de Haute Provence, France on 6 August 1976 with a brightness of magnitude 12. It was successfully observed in 1987 when J. Gibson of the Palomar Observatory, California, obtained images with the 1.5-meter reflector on 16 February. It appeared essentially stellar, with a faint magnitude of 19. It was observed again on 29 March 1997 by Carl W. Hergenrother at the F. L. Whipple Observatory, with perihelion on 1 May 1998.
68P came to opposition on 14 June 2019 and perihelion on November 9, 2019.[3]
^Fernández, Julio Angel (2005), Comets: nature, dynamics, origin, and their cosmogonical relevance, Springer Science + Business Media, p. 344, ISBN1-4020-3490-3