Melbourne's ASTRONOMY CENTRAL

Gravitational Lensing

Gravitational lensing describes how a massive object (for example a star or galaxy) changes the path of light from a distant object. The most obvious observational examples of gravitational lensing are the production of multiple images of distant objects.

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    This page created on: 16th August, 1997. Last updated: 2nd January, 1998
    Maintained by: Chris Fluke, cfluke@physics.unimelb.edu.au
    Authorised by R.Webster