Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
9827980 | New Astronomy Reviews | 2005 | 6 Pages |
Abstract
Using gravitational microlensing, a space-based wide-field imager could carry out a search for planets with greater sensitivity than any other technique. Because the amplitude of the microlensing signature is independent of planet mass, the survey would extend down to Mars-mass planets, at least a decade below other techniques. While most sensitive to planets in the so-called “lensing zone” (roughly 1-5Â AU from star), the microlensing technique probes planets over a broad range of separations, and is the only method that is sensitive to free-floating planets. It is also the only technique capable of conducting a planetary census at a wide range of Galactocentric distances.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
Andrew Gould,