Lecture Description
August 03, 2010
SETI Talks Archive: seti.org/talks
Lunar evidence of Late Heavy Bombardment has been interpreted to suggest that large-body impacting declined rapidly after about 3.8 Ga and that by 3.5 Ga the terrestrial bombardment rate was not much greater than the impact rates of today. In 1986 and 1989 Dr. Lowe and colleagues described four major layers of spherical particles in the 3.22-3.55 Ga Barberton greenstone belt (BGB), South Africa, ranging from 3,472 to 3,243 Ma, and interpreted them to represent the products of large terrestrial impacts of bolides 20-50 km in diameter. Since describing and interpreting these early impact layers, they have identified at least three additional thick layers of spherules in the Barberton belt that likely represent deposits of large impacts, and two new layers that display some geological features associated with impacts. Large impact layers have been identified to date in most of the major sedimentary units in the BGB. Intervening sections are composed largely of volcanic rocks where the record of impact events is unlikely to be preserved: it seems likely that other large impacts occurred during this period without leaving a record. These layers suggest that Earth continued to be bombarded by large extraterrestrial objects late into the Archean, at least until 3.2 Ga. The large sizes possible for these objects means that, while none was probably a sterilizing impact, many may have severely heated the oceans and atmosphere, boiled off the upper layer of seawater. The 3.8-3.2 Ga development of the Earth's surface environment and life may have been constrained largely by the continuing flux of large impactors. Only as that flux declined in the Late Archean were stable surface systems established within which non-thermophilic organisms and a stable geodynamic system could develop and evolve.
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.