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NARROW
GeoRef Subject
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all geography including DSDP/ODP Sites and Legs
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Grand Canyon (1)
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North America
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Basin and Range Province (1)
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North American Cordillera (1)
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United States
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Arizona
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Coconino County Arizona
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Flagstaff Arizona (9)
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Mogollon Plateau (1)
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San Francisco Peaks (2)
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Colorado Plateau (4)
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fossils
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Chordata
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Vertebrata
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Pisces
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Chondrichthyes (1)
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Invertebrata (1)
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geologic age
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Cenozoic (1)
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Paleozoic
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Permian
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Guadalupian (1)
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Kaibab Formation (2)
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Middle Permian (1)
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Primary terms
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Cenozoic (1)
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Chordata
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Vertebrata
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Pisces
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Chondrichthyes (1)
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crust (1)
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earthquakes (5)
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education (1)
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engineering geology (1)
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faults (3)
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fractures (1)
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geophysical methods (1)
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Invertebrata (1)
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North America
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Basin and Range Province (1)
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North American Cordillera (1)
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paleoecology (2)
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Paleozoic
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Permian
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Guadalupian (1)
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Kaibab Formation (2)
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Middle Permian (1)
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seismology (1)
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tectonics
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neotectonics (1)
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United States
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Arizona
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Coconino County Arizona
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Flagstaff Arizona (9)
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Mogollon Plateau (1)
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San Francisco Peaks (2)
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Colorado Plateau (4)
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Flagstaff Arizona
Walk in the footsteps of the Apollo astronauts: A field guide to northern Arizona astronaut training sites
ABSTRACT Every astronaut who walked on the Moon trained in Flagstaff, Arizona. In the early 1960s, scientists at the newly formed United States Geological Survey (USGS) Branch of Astrogeology led this training, teaching geologic principles and field techniques to the astronaut crews. USGS scientists and engineers also developed and tested scientific instrument prototypes, and communication and transportation technologies that would aid in lunar exploration. Astronomers and cartographers based at the USGS and Lowell Observatory, using telescopes at Lowell Observatory and the U.S. Naval Observatory, also played a key role, preparing lunar navigation charts and landing site maps. This historical and educational field trip will take participants along a historical path to some of the key sites where the Apollo astronauts trained. Field trip participants will see: (1) Grover , the geologic rover simulator on which the Apollo astronauts trained, which is on display at the USGS Astrogeology Science Center; (2) telescopes at Lowell Observatory used to map the lunar surface, as well as some of the original airbrushed maps; (3) the Bonito Lava Flow training area at Sunset Crater Volcano National Monument; (4) the Cinder Lake crater field, which was created in 1967 to simulate the lunar landscape for training astronauts and testing equipment; and (5) Meteor Crater, the best-preserved exposed impact crater on Earth. During this field trip we celebrate the 50th anniversary of one of the most remarkable events and most significant achievements in the history of humankind. We hope that the sites we visit will connect participants with the experiences of the astronauts and the excitement and inspiration of the origins of human space exploration. We also hope to communicate the historical significance of these sites, facilitate continued visitation of the sites (e.g., through class field trips), and educate the broader scientific and science education communities about the role that Flagstaff scientists and engineers played in the Apollo expeditions to the Moon.
ABSTRACT The San Francisco volcanic field stretches from Williams, Arizona, in the west, to northeast of Flagstaff, Arizona, on the east. Within the ~5000 km 2 area, more than 600 volcanoes are primarily monogenetic and basaltic, but silicic stratovolcanoes and domes are present as well. This field guide focuses on five broadly basaltic cones (Government Prairie vent, Red Mountain, SP Crater, Colton Crater, and Sunset Crater) and two silicic volcanoes (Kendrick Peak and San Francisco Mountain) in the field, with an emphasis on the different kinds of volcanic activity represented and the petrological variations. Hazards assessment indicates that is it possible for future eruptions to affect Flagstaff, but the probability is low. As information in this guide indicates, hazard assessments need to be improved to encompass a wide range of eruption types, and additional data are needed to improve models of the rate of volcanic activity and how the locus of activity has shifted over time.