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Sisällön tarjoaa Richard Pogge. Richard Pogge tai sen podcast-alustan kumppani lataa ja toimittaa kaiken podcast-sisällön, mukaan lukien jaksot, grafiikat ja podcast-kuvaukset. Jos uskot jonkun käyttävän tekijänoikeudella suojattua teostasi ilman lupaasi, voit seurata tässä https://fi.player.fm/legal kuvattua prosessia.
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Lecture 37: Strange New Worlds

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Sisällön tarjoaa Richard Pogge. Richard Pogge tai sen podcast-alustan kumppani lataa ja toimittaa kaiken podcast-sisällön, mukaan lukien jaksot, grafiikat ja podcast-kuvaukset. Jos uskot jonkun käyttävän tekijänoikeudella suojattua teostasi ilman lupaasi, voit seurata tässä https://fi.player.fm/legal kuvattua prosessia.
What are the properties of the 400+ exoplanets we have discovered so far? This lecture reviews the properties of exoplanets, and finds a couple of surprises: Jupiter-mass planets orbiting close to their parent stars, and Jupiter-mass planets in very elliptical orbits. Both seem to require some mechanism for migration: strong gravitational interactions with either the protoplanetary disk or other giant planets to cause the planets to move inward from their birth places beyond the "Ice Line". We will then briefly discuss why we are seeing systems very different from our own, mostly we think a selection effect due to our search methods to date. Microlensing, however, is more sensitive to systems like ours, and is starting to find them. Earths, however, remain elusive so far, but the hunt is on. Recorded live on 2009 Nov 18 in Room 1005 Smith Laboratory on the Columbus campus of The Ohio State University.
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Manage episode 362658403 series 3473824
Sisällön tarjoaa Richard Pogge. Richard Pogge tai sen podcast-alustan kumppani lataa ja toimittaa kaiken podcast-sisällön, mukaan lukien jaksot, grafiikat ja podcast-kuvaukset. Jos uskot jonkun käyttävän tekijänoikeudella suojattua teostasi ilman lupaasi, voit seurata tässä https://fi.player.fm/legal kuvattua prosessia.
What are the properties of the 400+ exoplanets we have discovered so far? This lecture reviews the properties of exoplanets, and finds a couple of surprises: Jupiter-mass planets orbiting close to their parent stars, and Jupiter-mass planets in very elliptical orbits. Both seem to require some mechanism for migration: strong gravitational interactions with either the protoplanetary disk or other giant planets to cause the planets to move inward from their birth places beyond the "Ice Line". We will then briefly discuss why we are seeing systems very different from our own, mostly we think a selection effect due to our search methods to date. Microlensing, however, is more sensitive to systems like ours, and is starting to find them. Earths, however, remain elusive so far, but the hunt is on. Recorded live on 2009 Nov 18 in Room 1005 Smith Laboratory on the Columbus campus of The Ohio State University.
  continue reading

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