Lecture Description
April 30, 2010
PAHs and the Diffuse Interstellar Bands: From the Laboratory to Space
The diffuse interstellar bands (DIBs) are absorption features that are seen toward reddened stars. They are caused by the absorption of light by the interstellar medium. Numbering hundreds of bands, the DIBs vary in strengths and in profiles and are detected in the near ultraviolet to the near infrared range. The bands are the signature of carriers that are ubiquitous in the interstellar medium making their identification an essential element for a correct understanding of the nature and the evolution of the interstellar medium. The diffuse bands have represented a long standing, fascinating challenge for astrophysics since they were first discovered more than a century ago. The search for the carriers of the DIB has motivated efforts at the frontiers of science, leading, among other things, to advances in spectroscopy and to the discovery of the fullerene molecules. Recent findings have shed light on the nature of the carriers of the DIBs and the role played by complex organic molecules in space. Recent progress in astronomical observations and in laboratory studies will be presented together with a discussion of the current consensus regarding this important issue.
Course Index
- Dale Cruikshank: Outer Solar System Ices
- Adrian Brown: Poles of Mars
- Bruce Damer: Simulating Life's Origin
- Laurance Doyle: Mongolian and other Historic Solar Eclipses
- Daniel Rasky: Augustine Commission - The Way Forward on US Manned Spaceflight
- Sergei Dubovsky: Observing String Multiverse with Astrophysical Black Holes
- Conny Aerts - Asteroseismology
- Carol Stoker - Phoenix Mission and Habitability
- ames Benford - Interstellar Beacons
- Brad Bailey - Life in Basaltic Glass in the oceanic basins
- Nancy McKeown: Mawrth Vallis, Mars
- Bob Pappalardo: Europa Jupiter Orbiter
- David Jewitt:- Solar System Primordial Ice Reservoirs
- Harry Jones: Starship Life Support
- Jeff Moore: Mysteries on Titan
- Farid Salama: Interstellar Clouds
- Mark Showalter: Marine Biodiversity
- Jen Blank: ChemCam on Mars Science Lab Rover
- Pete Worden, Pavel Podvig, Will Marshall: Nuclear Weapons and Space Weapons
- Samantha Blair: Interstellar Medium Interference
- Jon Jenkins: Kepler Worlds
- Dan Lubin: Maunder Minimum
- Monika Kress: Habitable Planets
- Intersection of Physics and Biology - Jan Liphardt
- Mark Marley: Atmospheres of Brown Dwarfs and Exoplanets
- Sarah Church: Polarized Cosmic Microwave Background
- Peter Jenniskens: Hayabusa Reentry
- Don Lowe: Late Heavy Bombardment
- Mark Krumholz: Star Formation Rate
- Heather Knutson: Exoplanet Atmospheres
- David Des Marais: Exploring Mars for Habitable Environments
- Ralph Lorenz: Titan Unveiled
- REU Students Review 2010
- Nick Kanas: Psychology of Spaceflight
- Rus Belikov: Beyond Kepler - Imaging Exo-Earths
- Bill Colson: Free Electron Laser Communications
- David Korsmeyer: NASA Future Human Missions
- Pascal Lee: Haughton-Mars Project
- Chris McKay: Titan - Past, Present, Future
- Nathalie Cabrol: Lakes on Mars
- Margarita Marinova: Martian Dichotomy
- Ellen Howell: Radar videos of asteroids
Course Description
Carl Sagan Center/SETI Institute Colloquium Series
Attend a colloquium! They are FREE, open to the public and held from noon to 1pm, every Wednesday at the SETI Institute, 515 N. Whisman Road, Mountain View, California.