Feb. 9, 2012: An overview of fusion energy research: taming turbulence and transport in magnetized plasmas

Speaker:
Troy Carter
UCLA

Abstract:

I will give an overview of the challenges associated with harnessing nuclear fusion as a terrestrial power source and the progress that has been made in research in this area. In particular, I will discuss turbulence in magnetically-confined plasmas and how transport associated with this turbulence limits the confinement achievable in current and planned experiments. I will present recent UCLA research that has helped advance our understanding of the basic physics of turbulence and turbulent transport in magnetized plasmas.

Feb. 2, 2012: Mapping the Amorphous-to-Crystalline Transitions in CaCO3 Biominerals

Speaker:
P.U.P.A. Gilbert
University of Wisconsin

Abstract:

Mapping the Amorphous-to-crystalline transitions in CaCO3 biominerals with 20-nm resolution One of the most fascinating aspects of calcite biominerals is their intricate and curved morphology, quite different from the rhombohedral crystal habit of geologic calcite. These morphologies, as well as space-filling and greater resistance to fracture, are achieved via amorphous precursor mineral phases (1). In this talk we will show that in sea urchin larval spicules two distinct phase transitions occur, 12 and 23 (2). Both transitions are regulated by inhibiting proteins, which introduce activation barriers between states otherwise spontaneously transforming because they are energetically downhill (3). 1. Y Politi, RA Metzler, M Abrecht, B Gilbert, FH Wilt, I Sagi, L Addadi, S Weiner, and PUPA Gilbert. Mechanism of transformation of amorphous calcium carbonate into calcite in the sea urchin larval spicule. Procs. Natl. Acad. Sci. USA 105, 17362-17366, 2008. 2. AV Radha, TZ Forbes, CE Killian, PUPA Gilbert, and A Navrotsky. Transformation and crystallization energetics of synthetic and biogenic amorphous calcium carbonate. Procs. Natl. Acad. Sci. USA 107, 16438–16443, 2010. 3. YUT Gong, CE Killian, IC Olson, NP Appathurai, RA Metzler, AL Amasino, FH Wilt, PUPA Gilbert. Phase Transitions in Sea Urchin Larval Spicules. Under review.

Jan. 26, 2012: Is the Earth Normal?

Speaker:
Michael Jura
UCLA

Abstract:
Knowing that extrasolar planetary systems are common, we would like to learn whether the Earth is normal or distinctive. Bulk Earth is 94% composed of O, Mg, Si and Fe and very deficient compared to the Sun in volatiles such as C and N. With our recent observations of white dwarf stars that have recently accreted tidally-disrupted minor planets that are about 300 km in diameter, we find a similar compositional pattern in extrasolar asteroids. While there must be individual exceptions, in aggregate, the studied extrasolar asteroids also are as “dry”; they probably formed interior to a snow line. Although the current sample is tiny, it appears that bulk Earth is compositionally normal for a rocky body. In the future, we may learn whether extrasolar planetesimals have undergone differentiation, a fundamentally important process in the history of our own planet.

Jan. 19, 2012: The Bucaramanga Nest: A Natural Lab for Understanding the Physics of Intermediate-depth Earthquakes

Speaker:
German Prieto
Universidad de los Andes, Bogotá, Colombia

Abstract:
The physical mechanism of intermediate-depth earthquakes is still under debate. In contrast to conditions in the crust and shallow lithosphere, at temperatures and pressures corresponding to depths >50 km one would expect rocks to yield by creep or flow and not by brittle failure, so there has to be a physical mechanism that allows for brittle or brittle-like failure for intermediate-depth earthquakes. Two such mechanisms have been proposed: dehydration embrittlement and thermal shear runaway. Earthquake nests represent a region with high earthquake concentration that is isolated from nearby activity. I will discuss general observations on the three famous intermediate-depth earthquake nests – Vrancea, Hindu-Kush and Bucaramanga. The emphasis will be on the Bucaramanga nest (Colombia) and how high-resolution seismological observations (tectonic setting, precise earthquake locations, focal mechanisms, stress drops, etc.) may provide key constraints on the mechanism responsible. Given the nature and characteristics of this nest, it can be thought as natural laboratory for understanding the physics of intermediate-depth earthquakes.

Astrobiology Science Conference, 2012 April 16 – 20, Atlanta, Georgia

AbSciCon 2012 is the next in a biennial series of meetings organized by the astrobiology community. The conference will convene scientists from all over the world who are working in the multidisciplinary field of astrobiology – the study of the origin, evolution, distribution, and future of life in the universe – to report on research findings and plan future endeavors.

The theme for AbSciCon 2012 is “Exploring Life: Past and Present, Near and Far.” The conference will address our current understanding of life – from processes at the molecular level to those which operate at planetary scales. Studying these aspects of life on Earth provides an essential platform from which to examine the potential for life on other worlds, both within our solar system and beyond.
The origin and evolution of life on Earth lies at the core of Astrobiology. What is necessary for life, and where does it come from? How do habitable environments develop and change? How does life begin and evolve? What are the interconnections between life and environmental change? Answering these questions about life near ‘home’ can help us determine the potential distribution of life at the far reaches of the Universe. AbSciCon 2012 will provide a forum for reporting on new discoveries, sharing data and insights, advancing collaborative efforts and initiating new ones, planning new projects, and educating the next generation of astrobiologists.

Asteroids, Comets, Meteors (ACM) meeting

The Asteroids, Comets, Meteors (ACM) meeting is the premier international gathering of scientists who study small bodies. The ACM series began in 1983 in Uppsala, Sweden, as a means of bringing together different groups within the asteroid, comet, and meteor communities who do not often have the opportunity to interact. From this first ACM meeting, a regular conference began. The conference now takes place every three years*, and it is the pre-eminent meeting for small-bodies research, with attendance usually in excess of 400. The 2012 ACM meeting will be the 11th in the series and will be the first time in Asian Region. Asteroids, Comets, Meteors (ACM) 2012 will be held 16 – 20 May, 2012, in Niigata, Japan, at TOKI Messe (Niigata Convention Center). The meeting will start on Wednesday (16th) and end on Sunday (20th). For more information, visit: http://chiron.mtk.nao.ac.jp/ACM2012/