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Draft Minutes for the 1518th Meeting of the Geological Society of Washington Wednesday, March 29th, 2017 John Wesley Powell Auditorium Cosmos Club, Washington, D.C. The 62 ladies, gentlemen, and geologists in attendance of the 1518th meeting ignored President Bentley’s call to order at 20:01 EDT. At the behest of Former President Toulmin, President Bentley called forth the power of Odin and laid down the Special Gavel with the force of 1000 mighty Viking warriors, at which point, the attendees shuffled to their seats, beers in hand. The minutes of the 1517th meeting were accepted with one correction. Five guests were not intimidated by President Bentley’s forceful blow, and remained: Catherine Thompson (affiliation unidentified) Nicholas Mecholsky of Catholic University of America’s Vitreous State Laboratory David Smallwood Robert Smith, formerly of the EPA and USGS Jennifer Mayo of NASA’s Goddard Spaceflight Center One new member was announced: Walter Guidroz of the USGS President Bentley assumed the somber duty of announcing the passing of Robert G. Luedke. Robert was a talented geologist, dedicating his work to mineral resources and volcanic rocks of the Colorado Plateau. In 1966, he co-authored a GSW talk with Wilbur Sweat Burbank, a talk that subsequently won Best Paper of the Year. Robert devoted more than 60 years of his life to the USGS, from the early 1950’s, past his retirement in 1995, and as emeritus until 2015. Roberts was a GSW member from 1955 until 1997 and passed away on March 21st, 2017. Members observed a moment of silence. Announcements: Kori Newman was not in attendance this week to solicit judges for local science fairs. President Bentley announced the Annual Bradley Lecture will be rescheduled for November 8th. This year’s speaker is Iain Stewart, possibly the only geologist to have his own IMDB page. President Bentley announced the National Association of Geoscience Teachers Eastern Section meeting to be held June 8-11, 2017 in Catonsville, Maryland. Flyers were available on the back table. Informal Communications: Member Jim Hayes spoke briefly regarding Holocene temperature variations. Mr. Hayes presented temperature curves from eight sources (listed in a handout provided by Mr. Hayes) recording temperature variability throughout the Holocene on a multi-centennial scale. Because of limitations of data sampling, the chart cannot resolve temperature fluctuations faster than ~300 years. Due to the resolution, it is impossible to know if other, short-term temperature fluctuations have occurred and only time, or better resolution data, will tell. Dr. Dan Doctor gave a brief synopsis about the Spring Field Trip to Sugarloaf Mountain, MD. Sixteen attendees managed to make it to the East View Parking Area, thanks to Dan’s excellent directions given during the previous meeting. The hikers enjoyed a brisk, cloudy day exploring the mysterious geology of Sugarloaf Mountain, an overturned anticlinal fold of pre-Cambrian quartzose sandstone and quartzite, thrust from the Blue Ridge, eastward, overtop of the younger rocks of the Piedmont by the Martic fault. Formal Program: Jean-Arthur Olive of Columbia University’s Lamont Doherty Earth Observatory gave a talk titled “What’s Shaping the Ocean Floor?” In his talk, Dr. Olive presented simple models that relate the texture of the ocean floor (abyssal hill spacing and amplitude) to magmatic and tectonic activity at the mid-ocean ridge where it formed. These models were used to assess the bathymetric expression of spatio-temporal variability in mid-ocean ridge magma supply, and better understand the deep and shallow processes that may affect this variability. Essentially, the amplitude and spacing (wavelength), are directly proportional to the spreading rate, and therefore, magma supply, of the associated spreading center. Questions were asked by Ved Lekic of UMD, Past President Jamie Allen (NSF), An unidentified gentleman in a yellow shirt and tie next to Laura Helmuth, Kevin Marvel of the American Astronomical Society, and Pete Toulmin (USGS, retired). Carrie M. Anderson gave a talk titled “Organic Inventory at Titan’s poles Inferred from nearly 15 years of Cassini Observations”. Titan possesses high amounts of organic aerosol particles in the atmosphere, which creates abundant smog. Dr. Anderson explained that these aerosol particles are important for nucleation sites for organic ice clouds, which form successive ice layers as particles descend in the atmosphere. Abundances and chemical compositions of the clouds in north and south winter polar stratospheric ices are different. These differences may be due to 1) Reversal of meridianal circulation, 2) differences in relative organic abundances, or 3) temperature differentials. Regardless of season, however, Titan’s aerosol ices precipitate and settle giving observed soil conditions. One question was asked by Pete Toulmin (USGS, retired). Michael Ackerson gave a talk titled “New Perspectives on an Age-Old Question: How do granites form?” In his talk, Dr. Ackerson discussed novel analytical and experimental techniques, which allowed him to investigate the thermal and chemical evolution of granite formation. Using the Tuolumne Intrusive Suite from the Sierra Nevada Batholith as a case study, Dr. Ackerson demonstrated that granitic rocks can crystallize at temperatures hundreds of degrees below the traditional wet solidus. These observations are helping to re-evaluate long-held petrologic models for granite formation and the relationships between plutonic and volcanic rocks. Questions were asked by 2nd VP Carl-Henry Geschwind, Jane Hammerstrom of the USGS, an unidentified gentleman in blue denim, Past President Pete Toulmin, Laura Waters of the Smithsonian Institution, and Dan Doctor of the USGS. Following the final question, President Bentley announced the program for the 1519th meeting on April 12th and adjourned the 1518th meeting at 2155 EDT.