Detecting Planets Beyond the Galaxy

Details Detecting Planets Beyond the Galaxy Detecting Planets Beyond the Galaxy

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002nmgm.meet.2135c&link_type=abstract

"THE NINTH MARCEL GROSSMANN MEETING On Recent Developments in Theoretical and Experimental General Relativity, Gravitation and R

Physics

Scientific paper

Photometric and astrometric microlensing (μL) observations are the only way to detect planets around stars at very large distances1. We show that the capability of photometric μL extends to the detection of signals caused by planets around stars in nearby galaxies (e.g. M31). No other method that can achieve this2...

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