Warren Wiscombe

NASA/GSFC: Climate and Radiation Laboratory

  0 0 1 188 1075 GEST/UMBC 8 2 1261 14.0 Normal 0 false false false EN-US JA X-NONE /* Style Definitions */ table.MsoNormalTable {mso-style-name:"Table Normal"; mso-tstyle-rowband-size:0; mso-tstyle-colband-size:0; mso-style-noshow:yes; mso-style-priority:99; mso-style-parent:""; mso-padding-alt:0in 5.4pt 0in 5.4pt; mso-para-margin:0in; mso-para-margin-bottom:.0001pt; mso-pagination:widow-orphan; font-size:10.0pt; font-family:"New York","serif";} I will first explain how I got interested in exoplanets--a confluence of Dan Goldin's 1998 AGU speech and joining the Triana Science Team.  Exoplanets are being discovered at an accelerating rate since the first one around a Sun-like star was confirmed in 1995.  Beginning with Jupiter-sized and larger planets, the exoplanet zoo has enlarged to include super-Earths (1.2 to 2x the radius of Earth) and bodies smaller than Earth as well.  There are no less than five different methods used to detect exoplanets.  The transit method, exemplified by the Kepler space telescope, gets the most press and has bagged by far the largest number of exoplanet candidates (4300+), but the Doppler or radial-velocity method still has the most confirmed detections.  The evolving theme in exoplanet research has become "we can predict nothing" since many of the discoveries like hot Jupiters have defied traditional theories and given us new insights into our own solar system, in particular about migrating planets.  Categories of exoplanets have been discovered that "should not" exist, for example planets around binary stars.  This talk shall attempt to overview the methods used to detect exoplanets, a few of the important and most fun discoveries, and what lies ahead.