Dr. Ryan B. Anderson (@Ryan_B_Anderson) is a planetary scientist at the U.S. Geological Survey Astrogeology Science Center in Flagstaff, AZ, where he works on a mix of research and software development. He got his PhD in Planetary Science from Cornell University. His thesis research played a role in the selection of Gale Crater as the landing site for the Curiosity Mars rover, and his work on analyzing Laser-Induced Breakdown Spectroscopy (LIBS) data with neural networks and other methods led to a role on the ChemCam science team. Ryan is also a member of the science team for the SuperCam instrument on the upcoming Mars 2020 rover and has a few smaller grants of his own, including two Mars geomorphology projects, and one to develop an open-source Python tool for analyzing LIBS (and other) spectra. He is also involved in a NASA-funded project to develop planetary science-themed after school activities for middle school students.
Ryan is passionate about science communication and education. He founded the Martian Chronicles blog, and enjoys giving public talks and generally sharing the excitement of science and planetary exploration.
Outside of work, Ryan enjoys spending time with his wife, baby, and two dogs. He also writes at his personal blog about non-science topics, and sometimes dabbles in fiction writing. He spends too much time on social media, and not enough on fun things like hiking and skiing.
I am a 5th year Ph.D Candidate at The Ohio State University working in the School of Earth Science. My research looks at what it takes to build a habitable planet from a geologic perspective rather than the more traditional definition of the “habitable zone”. My work blends astronomy, geology and physics to understand which planetary compositions produce a planet able to sustain liquid water on its surface as well as control the carbon content of the atmosphere. On the Earth, this regulation of water/carbon is a consequence of plate tectonics, which in turn is driven by compositional differences in the mantle and an internal heat budget great enough to support interior convection. My previous work has looked at some of the extremes of this “geologic habitable zone”, such as so called “diamond planets” as well as measuring stellar Thorium abundance as a proxy for extrasolar heat budgets. The end goal of my research is to understand just how special the Earth may be with regards to it being habitable, or perhaps there are a range of compositions, perhaps even very un-Earth-like ones, that are able to produce dynamic planets capable of sustaining surface water and maybe even conditions to support life.
This week we have Fred Calef III hosting astrotweeps. Fred graduated from the University of Alaska Fairbanks (UAF) in Geological Sciences in 2010. His dissertation was on fresh small rayed impact craters on Mars, looking at ejecta retention rates and what they tell us about the current environment and geomorphic evolution of the surface. He postdoc’d at California Institute of Technology (Caltech) via the Jet Propulsion Laboratory (JPL) doing landing site analysis for the Mars Science Laboratory (MSL, aka Curiosity) as well as trained as an Engineering Camera Payload Uplink Lead (ECAM-PUL) for the Mars Exploration Rover (MER) Opportunity. Towards the end of his postdoc, he was hired at JPL as the Geospatial Information Scientist, aka ‘Keeper of the Maps’, and Co-Localization Scientist for MSL. Besides work on MER and MSL, Fred is on the InSight lander science team as ‘Keeper of the Map’ for placement of a seismometer (SEIS) and heatprobe (HP3) as well as doing landing site analysis for InSight and the Mars2020 rover. You can find Fred on twitter at @cirquelar