Bulletin of the American Physical Society
Annual Meeting of the Four Corners Section of the APS
Volume 58, Number 12
Friday–Saturday, October 18–19, 2013; Denver, Colorado
Session B1: Plenary I |
Hide Abstracts |
Chair: Jonathan Ormes, University of Denver Room: 248 |
Friday, October 18, 2013 9:30AM - 10:05AM |
B1.00001: Precision Cosmology: Past Successes and Future Prospects Invited Speaker: John Mather We now have a Standard Model of cosmology, with all the well-earned pride and possible hubris that entails. We have measured the main cosmological parameters to accuracies of a few percent, and we have even tested inflation theories. But there are some pesky mysteries: dark matter and dark energy, and an apparent deficit of spatial fluctuations on the largest angular scales. And the great current challenge is testing whether gravitational waves were important in the early universe. Then, what happened to produce the galaxies, the black holes, and the remarkable complexity of astrophysics? Combining new measurements and new simulations, we have great hopes to understand a little better, and with luck, to aid in the search for the Theory of Everything, if it exists. I will sketch the history and predict the future. [Preview Abstract] |
Friday, October 18, 2013 10:05AM - 10:40AM |
B1.00002: The Chelyabinsk Airburst: Observations and Models Invited Speaker: Mark Boslough On Feb. 15, 2013, an asteroid exploded about 40 km SSW of the Russian city of Chelyabinsk. It caused many injuries and widespread blast damage, but also yielded a plethora of data from security and dashboard cameras. Combined with seismic, infrasound, and satellite records, this serendipitous source provides a means to determine the projectile size and entry parameters and develop a self-consistent model. Analysis of video with subsequent on-site stellar calibrations enabled precise estimates of entry velocity (19 km/s), angle (17 deg) and altitude of peak brightness (29 km). The inferred pre-entry diameter was $\sim$ 20 m with a mass of $\sim$ 1200 tonnes. Satellite sensors recorded a radiated energy consistent with a total energy of $\sim$ 450 kilotons. The shallow entry angle led to an extended, near-horizontal, linear explosion. The blast was distributed over a large area, and was much weaker than it would be for a steep entry. The orientation also led to different phenomena than expected for a more vertical entry. There was no ballistic plume as calculated for Tunguska ($\sim$ 35 deg). Instead, buoyant instabilities grew into mushroom clouds and bifurcated the trail into two contra-rotating vortices. This event also suggests that the risk from airbursts is greater than previously thought. [Preview Abstract] |
Follow Us |
Engage
Become an APS Member |
My APS
Renew Membership |
Information for |
About APSThe American Physical Society (APS) is a non-profit membership organization working to advance the knowledge of physics. |
© 2025 American Physical Society
| All rights reserved | Terms of Use
| Contact Us
Headquarters
1 Physics Ellipse, College Park, MD 20740-3844
(301) 209-3200
Editorial Office
100 Motor Pkwy, Suite 110, Hauppauge, NY 11788
(631) 591-4000
Office of Public Affairs
529 14th St NW, Suite 1050, Washington, D.C. 20045-2001
(202) 662-8700