President Larry Millstein called the 2349th meeting of the Society to order on September 11, 2015 at 8:07 p.m. He announced the order of business and welcomed new members. Vice President Lloyd Mitchell presented the Audit Committee’s annual report which found the Society’s financial records to be in good order for the fiscal year ended June 30, 2015. The minutes of the previous meeting were read and approved. President Millstein presented a summary of the 22nd meeting of the Society held March 9, 1872, and then introduced the speaker for the evening, Mark H. Thiemens of the University of California, San Diego. His lecture was titled “Isotopes: Magic Keys to Understanding Life and the Cosmos.”
Dr. Thiemens began his lecture by explaining the fundamental nature of an isotope, which is a change in the weight of an element by the removal or addition of one or more neutrons. Dr. Thiemens likened the study of isotopes to psychology, noting that an isotope modifies the character of an element and, thus, its behavior.
Dr. Thiemens first focused on the state of the universe at 5 billion years. At that time, a curious discontinuity in the relative abundance of various elements shows that, although most of the elements are made in stars, a select few were formed directly out of the Big Bang.
Subsequently, elements have been formed in the conventional way, within stars. The inner workings of stars may be examined spectroscopically, but this method does not provide data below the upper layers. Meteorites, however, can provide more data. When a star explodes, physical grains condense immediately and trap elements the star has formed. These grains are found in meteorites, which therefore function as a record of element-forming activity beyond the outermost layers of a star. Everything is recorded, Dr. Thiemens stated; the trick is to interpret it.
To help with this interpretation, scientists need to know what the sun is made of and, specifically, what the isotope composition is. One way to gather information on the composition of the sun is to gather the sun’s emissions directly. But getting a sample of the sun is difficult, as the myth of Icarus demonstrated. Undaunted, Dr. Thiemens successfully proposed a project to NASA which would do just that. NASA approved the Genesis project, which was stationed at the L1 Lagrange point, and it captured a nanogram of particles out of the solar wind. Although it crashed upon its return to Earth, good data could be recovered. This and other experiments showed that the early sun played a large role in the formation of molecules of the planet.
Some meteorites contain organic molecules such as amino acids. The question is how the organic molecules came to be present in the meteorites. This mystery brings us to meteorite ALH840001 – the famous meteorite that suggested there is life on Mars. Calcium carbonate globules on the meteorite were identified as potentially biogenic features. This meteorite originated from the “wet Mars” period of 17 million years ago, and provides some of our limited insight into the state of Mars during that period.
To get similar data from Earth, we must journey south, an endeavor that Dr. Thiemens noted still involves small wages, bitter cold and long months of complete darkness . . . although with less danger and significantly less honor and recognition than in the past. Samples of Antarctic ice, uncontaminated by human presence, offer very high resolution time scales, as accurate as 6 months and as recent as this decade.
These samples provide an isotopic record that shows climate perturbations. Two such perturbations, as expected, are the eruptions of El Chichón in 1982 and Mount Pinatubo and Cerro Hudson in 1991, both of which raised global atmospheric sulfate and oxygen concentration. Another spike was in 1998, this time because of widespread fires in the equatorial regions. This occurred because of a spike in the El Niño which was followed by cold pacific and dry weather which ushered in La Niña. This record provides useful evidence to view the causes and effects of the cycles of the planet.
This cause and effect lens leads naturally to questions about the global climate system. Dr. Thiemens said that regardless of whether you believe in climate change, the water system is clearly perturbed. The California drought is a visible example of this. Drinking water is a less visible but more urgent global concern. 60% of the world gets its water from the rivers of the Tibetan plateau, the Ganges and the Mekong in particular. The melt rate of the glacier ice that feeds these rivers is far higher than it should be, and examining the glacier ice can give us clues as to why this is happening.
Along the way to unraveling this mystery we are also learning about the climate forces that created the mysterious “snowball Earth” period 650 million years ago. Atmospheric carbon dioxide levels plunged and the Earth froze about 1 million years later. Then about 100,000 years later, it unfroze, and nearly simultaneously precipitated a worldwide carbonate layer that can be found in the strata everywhere on Earth. The causes of this great swing — and its implications for our current climate — are still being analyzed.
After the question and answer period, President Millstein thanked the speaker, made the usual housekeeping announcements, and invited guests to join the Society. At 9:35 p.m., President Millstein adjourned the 2349th meeting of the Society to the social hour.
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