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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Chris Fluke: cfluke@physics.unimelb.edu.au
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