Lava Tubes May Be Havens for Ancient Alien Life and Future Human
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Hawaii Volcanoes National Park Geologic Resources Inventory Report
National Park Service U.S. Department of the Interior Natural Resource Program Center Hawai‘i Volcanoes National Park Geologic Resources Inventory Report Natural Resource Report NPS/NRPC/GRD/NRR—2009/163 THIS PAGE: Geologists have lloongng been monimonittoorriing the volcanoes of Hawai‘i Volcanoes National Park. Here lalava cascades durduriingng the 1969-1971 Mauna Ulu eruption of Kīlauea VolVolcano. NotNotee the Mauna Ulu fountountaiain in the background. U.S. Geologiogicalcal SurSurvveyey PhotPhotoo by J. B. Judd (12/30/1969). ON THE COVER: ContContiinuouslnuouslyy eruptuptiingng since 1983, Kīllaueaauea Volcano contcontiinues to shapshapee Hawai‘Hawai‘i VoVollccanoes NatiNationalonal ParkPark.. Photo courtesy Lisa Venture/UniversiUniversitty of Cincinnati. Hawai‘i Volcanoes National Park Geologic Resources Inventory Report Natural Resource Report NPS/NRPC/GRD/NRR—2009/163 Geologic Resources Division Natural Resource Program Center P.O. Box 25287 Denver, Colorado 80225 December 2009 U.S. Department of the Interior National Park Service Natural Resource Program Center Denver, Colorado The National Park Service, Natural Resource Program Center publishes a range of reports that address natural resource topics of interest and applicability to a broad audience in the National Park Service and others in natural resource management, including scientists, conservation and environmental constituencies, and the public. The Natural Resource Report Series is used to disseminate high-priority, current natural resource management information with managerial application. The series targets a general, diverse audience, and may contain NPS policy considerations or address sensitive issues of management applicability. All manuscripts in the series receive the appropriate level of peer review to ensure that the information is scientifically credible, technically accurate, appropriately written for the intended audience, and designed and published in a professional manner. -
The Cavernicolous Fauna of Hawaiian Lava Tubes, 1
Pacific Insects 15 (1): 139-151 20 May 1973 THE CAVERNICOLOUS FAUNA OF HAWAIIAN LAVA TUBES, 1. INTRODUCTION By Francis G. Howarth2 Abstract: The Hawaiian Islands offer great potential for evolutionary research. The discovery of specialized cavernicoles among the adaptively radiating fauna adds to that potential. About 50 lava tubes and a few other types of caves on 4 islands have been investigated. Tree roots, both living and dead, are the main energy source in the caves. Some organic material percolates into the cave through cracks associated with the roots. Cave slimes and accidentals also supply some nutrients. Lava tubes form almost exclusively in pahoehoe basalt, usually by the crusting over of lava rivers. However, the formation can be quite complex. Young basalt has numerous avenues such as vesicles, fissures, layers, and smaller tubes which allow some intercave and interlava flow dispersal of cavernicoles. In older flows these avenues are plugged by siltation or blocked or cut by erosion. The Hawaiian Islands are a string of oceanic volcanic islands stretching more than 2500 km across the mid-Pacific. The western islands are old eroded mountains which are now raised coral reefs and shoals. The eight main eastern islands total 16,667 km2 and are relatively young in geologic age. Ages range from 5+ million years for the island of Kauai to 1 million years for the largest island, Hawaii (Macdonald & Abbott, 1970). The native fauna and flora are composed of those groups which dis persed across upwards of 4000 km of open ocean or island hopped and became successfully established. -
Applications of Solar Wind Particle Impact Simulations at Lunar Magnetic Anomalies to the Study of Lunar Swirls
47th Lunar and Planetary Science Conference (2016) 2648.pdf APPLICATIONS OF SOLAR WIND PARTICLE IMPACT SIMULATIONS AT LUNAR MAGNETIC ANOMALIES TO THE STUDY OF LUNAR SWIRLS. C. J. Tai Udovicic1, G. Y. Kramer2, and E. M. Harnett3, 1Dept of Earth Sciences, University of Toronto, 22 Russell St, Toronto, ON, Canada, ([email protected]), 2Lunar and Planetary Institute, 3600 Bay Area Bvld, Houston, TX, ([email protected]), 3University of Washington, Earth and Space Sciences, Seattle, WA ([email protected]). Introduction: Lunar swirls are high albedo features highlands often appear to have swirl-like anomalies due that exhibit low spectral maturity. They have been to their complicated topography. To mitigate this, we identified at various sites on the Moon, and all coincide generated a slope map from the WAC GLD100 (SLP), with a lunar magnetic anomaly (magnomaly) [1], which we overlayed with the WAC 643 nm normalized although not all magnomalies have an identifiable swirl. reflectance image to distinguish high albedo swirls from The leading hypothesis for lunar swirl origin is high albedo slopes. Even so, after one pass of the region, presented in [2] as magnetic field standoff of the solar only about half of the swirls could be detected with this wind which causes uneven space weathering at the swirl method alone. The remaining half were found after surface. This hypothesis fails to explain why lunar using particle simulations as a guide. swirls are observed at some but not all of the magnetic Solar wind particle tracking simulations: We anomalies present on the Moon. To investigate the solar used the 2D solar wind particle tracking simulation wind standoff hypothesis further and to improve swirl presented in [2]. -
Apollo 17 Index: 70 Mm, 35 Mm, and 16 Mm Photographs
General Disclaimer One or more of the Following Statements may affect this Document This document has been reproduced from the best copy furnished by the organizational source. It is being released in the interest of making available as much information as possible. This document may contain data, which exceeds the sheet parameters. It was furnished in this condition by the organizational source and is the best copy available. This document may contain tone-on-tone or color graphs, charts and/or pictures, which have been reproduced in black and white. This document is paginated as submitted by the original source. Portions of this document are not fully legible due to the historical nature of some of the material. However, it is the best reproduction available from the original submission. Produced by the NASA Center for Aerospace Information (CASI) Preparation, Scanning, Editing, and Conversion to Adobe Portable Document Format (PDF) by: Ronald A. Wells University of California Berkeley, CA 94720 May 2000 A P O L L O 1 7 I N D E X 7 0 m m, 3 5 m m, A N D 1 6 m m P H O T O G R A P H S M a p p i n g S c i e n c e s B r a n c h N a t i o n a l A e r o n a u t i c s a n d S p a c e A d m i n i s t r a t i o n J o h n s o n S p a c e C e n t e r H o u s t o n, T e x a s APPROVED: Michael C . -
Strategy for Optimal, Long-Term Stationkeeping of Libration Point Orbits in the Earth-Moon System
Strategy for Optimal, Long-Term Stationkeeping of Libration Point Orbits in the Earth-Moon System Thomas A. Pavlak∗ and Kathleen C. Howelly Purdue University, West Lafayette, IN, 47907-2045, USA In an effort to design low-cost maneuvers that reliably maintain unstable libration point orbits in the Earth-Moon system for long durations, an existing long-term stationkeeping strategy is augmented to compute locally optimal maneuvers that satisfy end-of-mission constraints downstream. This approach reduces stationkeeping costs for planar and three- dimensional orbits in dynamical systems of varying degrees of fidelity and demonstrates the correlation between optimal maneuver direction and the stable mode observed during ARTEMIS mission operations. An optimally-constrained multiple shooting strategy is also introduced that is capable of computing near optimal maintenance maneuvers without formal optimization software. I. Introduction Most orbits in the vicinity of collinear libration points are inherently unstable and, consequently, sta- tionkeeping strategies are a critical component of mission design and operations in these chaotic dynamical regions. Stationkeeping is particularly important for libration point missions in the Earth-Moon system since fast time scales require that orbit maintenance maneuvers be implemented approximately once per week. Assuming that acceptable orbit determination solutions require 3-4 days to obtain, stationkeeping ∆V planning activities must be quick, efficient, and effective. Furthermore, the duration of a libration point mission is often dictated by the remaining propellant so a key capability is maintenance maneuvers that are low-cost. Thus, to accommodate a likely increase in future operations in the vicinity of the Earth-Moon libration points, fast, reliable algorithms capable of rapidly computing low-cost stationkeeping maneuvers, with little or no human interaction, are critical. -
Ecological Studies on Hawaiian Lava Tubes
Technical Report No. 16 ECOLOGICAL STUDIES ON HAWAIIAN LAVA TUBES Francis G. Howarth Department of Entooology Bernice P. Bishop Museum Honolulu, Hawaii ISLAND ECOSYSTEMS IRP U. S. International Biological Program Decemb~r 1972 ABSTRACT The Hawaiian Islands offer great potential for evolutionary research. The discovery of specialized cavernicoles among the adaptively radiating fauna adds to that potential. About 50 lava tubes and a few other types of caves on 4 islands have been investigated. Tree roots, both living and dead, are the main energy source in the caves. Some organic material percolates into the cave through cracks associated with the roots. Cave slimes and accidentals also supply some nutrients. Lava tubes form almost exclusively in pahoehoe basalt, usually by the crusting over of lava rivers. However, the formation can be quite complex. Young basalt has numerous avenues such as vesicles, fissures, layers, and smaller tubes which allow some intercave and interlava flow dispersal of cavernicoles. In older flows these avenues are plugged by siltation or blocked or cut by erosion. -~- 2 TABLE 1. Caves Investit~ted in this Survey. Lava Tubes on Hawaii (J.:auna Loa rassif) No. Name of Cave Locality Elevation Len[th Dark Zone1 (approx.) 1. i<aurnana Cave Kaumana 290 m 1500 m + 2. Bird Park Cave #1 Hawaii Volcanoes National Park 1250 m 100 m + 3. Bird Park Cave #2 Hawaii Volcanoes National Park 1250 m 20 m 0 4. Bird Park Cave #3+4 Hawaii Volcanoes National Park 1250 m 400 m + 5. Bird Park Cave #5 Hawaii Vol canoe:!! National Park 1250 m 20 m? 0 6. -
Simulations of Particle Impact at Lunar Magnetic Anomalies and Comparison with Spectral Observations
Simulations of Particle Impact at Lunar Magnetic Anomalies and Comparison with Spectral Observations Erika Harnett∗ Department of Earth and Space Science, University of Washington,Seattle, WA 98195-1310, USA Georgiana Kramer Lunar and Planetary Institute, 3600 Bay Area Blvd, Houston, TX 77058, USA Christian Udovicic Department of Physics, University of Toronto, 60 St George St,Toronto, ON M5S 1A7, Canada Ruth Bamford RAL Space, STFC, Rutherford Appleton Laboratory,Chilton, Didcot Ox11 0Qx, UK (Dated: November 5, 2018) Ever since the Apollo era, a question has remained as to the origin of the lunar swirls (high albedo regions coincident with the regions of surface magnetization). Different processes have been proposed for their origin. In this work we test the idea that the lunar swirls have a higher albedo relative to surrounding regions because they deflect incoming solar wind particles that would otherwise darken the surface. 3D particle tracking is used to estimate the influence of five lunar magnetic anomalies on incoming solar wind. The regions investigated include Mare Ingenii, Gerasimovich, Renier Gamma, Northwest of Apollo and Marginis. Both protons and electrons are tracked as they interact with the anomalous magnetic field and impact maps are calculated. The impact maps are then compared to optical observations and comparisons are made between the maxima and minima in surface fluxes and the albedo and optical maturity of the regions. Results show deflection of slow to typical solar wind particles on a larger scale than the fine scale optical, swirl, features. It is found that efficiency of a particular anomaly for deflection of incoming particles does not only scale directly with surface magnetic field strength, but also is a function of the coherence of the magnetic field. -
Mars Astrobiological Cave and Internal Habitability Explorer (MACIE): a New Frontiers Mission Concept
Mars Astrobiological Cave and Internal habitability Explorer (MACIE): A New Frontiers Mission Concept By: C. Phillips-Lander ([email protected])1, A. Agha-mohamamdi2, J. J. Wynne3, T. N. Titus4, N. Chanover5, C. Demirel-Floyd6, K. Uckert2, K. Williams4, D. Wyrick1, J.G. Blank7,8, P. Boston8, K. Mitchell2, A. Kereszturi9, J. Martin-Torres10,11, S. Shkolyar12, N. Bardabelias13, S. Datta14, K. Retherford1, Lydia Sam11, A. Bhardwaj11, A. Fairén15,16, D. Flannery17, R. Wiens17 1Southwest Research Institute 2 NASA Jet Propulsion Laboratory 3Northern Arizona University 4U.S. Geological Survey 5New Mexico State University 6University of Oklahoma 7Blue Marble Space Institute of Science 8NASA Ames Research Center 9Konkoly Thege Miklos Astronomical Institute, Budapest, Hungary 10Instituto Andaluz de Ciencias de la Tierra (CSIC-UGR), Spain 11University of Aberdeen, United Kingdo 12USRA/NASA Goddard 13University of Arizona 14University of Texas-San Antonio 15Centro de Astrobiogía, Spain 16Cornell University 17Queensland University for Technology, Australia 18Los Alamos National Laboratory Cosigners 1 Summary of Key Points 1. Martian subsurface habitability and astrobiology can be evaluated via a lava tube cave, without drilling. 2. MACIE addresses two key goals of the Decadal Survey (2013-2022) and three MEPAG goals. 3. New advances in robotic architectures, autonomous navigation, target sample selection, and analysis will enable MACIE to explore the Martian subsurface. 1. Martian lava tubes are one of the best places to search for evidence of life The Mars Astrobiological Cave and Internal habitability Explorer (MACIE) mission concept is named for Macie Roberts, one of NASA’s ‘human computers’ (Conway 2007). MACIE would access the Martian subsurface via a lava tube. -
Trajectory Design Tools for Libration and Cislunar Environments
TRAJECTORY DESIGN TOOLS FOR LIBRATION AND CISLUNAR ENVIRONMENTS David C. Folta, Cassandra M. Webster, Natasha Bosanac, Andrew D. Cox, Davide Guzzetti, and Kathleen C. Howell National Aeronautics and Space Administration Goddard Space Flight Center, Greenbelt, MD, 20771 [email protected], [email protected] School of Aeronautics and Astronautics, Purdue University, West Lafayette, IN 47907 {nbosanac,cox50,dguzzett,howell}@purdue.edu ABSTRACT supplies insight into the natural dynamics associated with multi- body systems. In fact, such information enables a rapid and robust Innovative trajectory design tools are required to support methodology for libration point orbit and transfer design when challenging multi-body regimes with complex dynamics, uncertain used in combination with numerical techniques such as targeting perturbations, and the integration of propulsion influences. Two and optimization. distinctive tools, Adaptive Trajectory Design and the General Strategies that offer interactive access to a variety of solutions Mission Analysis Tool have been developed and certified to enable a thorough and guided exploration of the trajectory design provide the astrodynamics community with the ability to design space. ATD is intended to provide access to well-known solutions multi-body trajectories. In this paper we discuss the multi-body that exist within the framework of the Circular Restricted Three- design process and the capabilities of both tools. Demonstrable Body Problem (CR3BP) by leveraging both interactive and applications to confirmed missions, the Lunar IceCube CubeSat automated features to facilitate trajectory design in multi-body mission and the Wide-Field Infrared Survey Telescope Sun-Earth regimes [8]. In particular, well-known solutions from the CR3BP, such as body-centered, resonant and libration point periodic and L2 mission, are presented. -
America's Natural Nuclear Bunkers
America’s Natural Nuclear Bunkers 1 America’s Natural Nuclear Bunkers Table of Contents Introduction ......................................................................................................... 10 Alabama .............................................................................................................. 12 Alabama Caves .................................................................................................. 13 Alabama Mines ................................................................................................. 16 Alabama Tunnels .............................................................................................. 16 Alaska ................................................................................................................. 18 Alaska Caves ..................................................................................................... 19 Alaska Mines ............................................................................................... 19 Arizona ............................................................................................................... 24 Arizona Caves ................................................................................................... 25 Arizona Mines ................................................................................................... 26 Arkansas ............................................................................................................ 28 Arkansas Caves ................................................................................................ -
GRAIL Gravity Observations of the Transition from Complex Crater to Peak-Ring Basin on the Moon: Implications for Crustal Structure and Impact Basin Formation
Icarus 292 (2017) 54–73 Contents lists available at ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus GRAIL gravity observations of the transition from complex crater to peak-ring basin on the Moon: Implications for crustal structure and impact basin formation ∗ David M.H. Baker a,b, , James W. Head a, Roger J. Phillips c, Gregory A. Neumann b, Carver J. Bierson d, David E. Smith e, Maria T. Zuber e a Department of Geological Sciences, Brown University, Providence, RI 02912, USA b NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA c Department of Earth and Planetary Sciences and McDonnell Center for the Space Sciences, Washington University, St. Louis, MO 63130, USA d Department of Earth and Planetary Sciences, University of California, Santa Cruz, CA 95064, USA e Department of Earth, Atmospheric and Planetary Sciences, MIT, Cambridge, MA 02139, USA a r t i c l e i n f o a b s t r a c t Article history: High-resolution gravity data from the Gravity Recovery and Interior Laboratory (GRAIL) mission provide Received 14 September 2016 the opportunity to analyze the detailed gravity and crustal structure of impact features in the morpho- Revised 1 March 2017 logical transition from complex craters to peak-ring basins on the Moon. We calculate average radial Accepted 21 March 2017 profiles of free-air anomalies and Bouguer anomalies for peak-ring basins, protobasins, and the largest Available online 22 March 2017 complex craters. Complex craters and protobasins have free-air anomalies that are positively correlated with surface topography, unlike the prominent lunar mascons (positive free-air anomalies in areas of low elevation) associated with large basins. -
Cave Science News
CAV E SCIENCE NEWS CAVE SCIENCE NEWS KARST MEETING PLANNED AT MAMMOTH CAVE Kempe, S. (1996) Enlargement of lava tubes by downcutting and breakdown. Abstracts and Proceedings of the National A joint meeting of the International Geological Correlation Speleological Society Convention 58(3): 203. Program, Project 379: “Karst Processes and the Global Kempe, S. (1996). Neue Rekorde in Lavahohlen auf Hawaii, Carbon Cycle” along with Friends of Karst will take place on ein Statusbericht. Mitt. Arge f. Karstkunde Harz e.V. September 23, 24, and 25, 1998, at Mammoth Cave, Kentucky, 1996(3): 46-49 und (mit gleichem Text) Lavahohlen auf USA. The meeting will be hosted by the Center for Cave and Hawaii ein Statusbericht. Mitt.Verb. Dt. Hohlen- u. Karst Studies at Western Kentucky University, Mammoth Cave Karstforscher 42 (2): 27-29. (German) National Park, and the Cave Research Foundation. Kempe, S. (in press). Lava Falls: a major factor for the Preliminary plans are to have two days of scientific pre- enlargement of lava tube of the Ai-laau shield phase, sentations on various aspects of karst science, with particular Kilauea, Hawaii. Proceedings of the 10th International sessions so far anticipated on progress in understanding the Congress of Speleology. Switzerland. impact of karst processes on carbon cycling at a variety of Kempe, S., Buchas, H., Hartmann, J., Oberwinder, M., scales, and on recent work in the Central Kentucky Karst. A Strassenburg, J. & Wolniewicz, K. (in press). Mapping third day will be planned for a variety of surface and subsur- lava flows by following their tubes: The Keauhou face field trips in and around the Mammoth Cave System, Trail/Ainahou Ranch Flow Field, Kilauea, Hawaii.