Geology of Selected Lava Tubes in the Bend Area, Oregon

Total Page:16

File Type:pdf, Size:1020Kb

Geology of Selected Lava Tubes in the Bend Area, Oregon STATE OF OREGON DEPARTMENT OF GEOLOGY AND MINERAL INDUSTRIES 1069 State Office Building Portland, Oregon 97201 BUL LETI N 71 GEOLOGY OF SELECTED LAVA TUBES IN THE BEND AREA, OREGON By Ronald Greeley Space Sciences Division National Aeronautics and Space Administration Moffett Field, California 1971 GOVERNING BOARD Fayette I. Bristol, Rogue River, Chairman R. W. deWeese, Portland Harold Banta, Baker STATE GEOLOGIST R. E. Corcoran FOREWORD Oregon probably has the greatest diversity of volcanic rock types and landforms of any region in the conterminous United States. The area centering around Bend has come to be known as Oregon's "moon country" because the very young volcanic rocks in this vicinity show features similar to what have been photographed on the lunar surface. The National Aeronautics and Space Administration has, therefore, spent considerable time studying various aspects of the terrain in central Oregon because its scientists have interpreted certain lunar forms, such as the sinuous rilles, as volcanic structures. Mr. Ronald Greeley, the author of this report, believes that some of the smaller lunar rilles probably resuI ted from I ova-tube coli apse. Up to the present time, there has been relatively little study of lava tubes in the western United States to determine their origin, nor have these unusual structures been described in sufficient detail to be classified into different types. Mr. Greeley has selected several lava tubes in the Bend area for such a study because of their excellent development and relative ease of access. The Department presents this publication with the hope that it will stimulate the interest of others in exploring the many unusual and fascinating geologic features that occur in our "moon country. " R. E. Corcoran Oregon State Geologist ii CONTENTS Page -- Abstract . 1 Introduction Field methods 3 Geology and physiography 3 Lava tube formation . 5 Lava tube descriptions 12 Arnold Lava Tube System 12 Upper section . 12 Charcoal Cave 12 Arnold Ice Cave 15 Middle section 15 Collapsed Lava Pond No. 15 Deg Cave 18 Bat Cave 18 Lower section . 18 Wind Cave 18 CoII apsed Lava Pond No. 2 22 Pictograph Cave 22 Coli apsed Lava Pond No. 3 24 2 24 Charcoal Cave No. Collapsed Lava Pond No. 4 24 Stookey Ranch Cave 27 Collapsed Lava Pond No. 5 27 Horse Lava Tube System 27 Lewis Farm Caves 27 Garbage Caves 31 Garbage Cave No. 2 31 Stevens Road Cave 31 Horse Cave 31 Wilson Cave 31 Barlow Cave 31 iii Page Miscellaneous lava tubes . 33 Lava Top Butte Caves 33 Log Crib Cave 33 South Ice Cave 34 Skeleton Cave 34 Boyd Cave 36 Lava River Cave . 40 Conclusions 45 Acknowledgments 45 References cited 46 Appendix (location of surveyed lava tubes near Bend) 47 iv ILLUSTRATIO NS Figures Page Marius Hills region of the Moon . Structure interpreted to be a partly col l apsed lava tube l. 2 2. Location map and physi ography of central Oregon showing area of investigation near Bend 4 3. D iagram of a minor lava tube system in north ern California 6 4a. Bear Trap Lava Tube , Idaho, showing layered lava 7 4b. Jug Cave, Washington, showing layered lava 7 5. W ind Cave showi ng flow lines and cut bank at meander bend 8 Rim of col l apse pit, Barlow Cave, sh owing plastic deformation of lava crust 10 6. Boyd Cave Lava Tube sh ow ing sand at surface draining into tube 11 7. Boyd Cave Lava Tube sh owing sand draining through roof fracture 8. 11 Map of Arnold LavaTube System . 9. 13 10. Obl ique aerial view of upper Arnold Lava Tu be System 14 . Arnold Ice Cave near entrance 11 16 12. Arnold Lava Tube System; cross sections transverse to lava tube axis ; 7 o . 13. Diagrams of coll apse lava ponds f Ar nold Lava Tu be System 17 Bat Cave sh owing p lastically deformed lining curling from wa ll 14. 19 Wind Cave sh owing plastic deformation of wall lining 15. 21 Entrance to Pictograph Cave . 23 16. En trance to Pictograph Cave showi ng possible gas pocket 23 17. Pictograph Cave downtube from entrance 18. 25 Oblique aerial view of Collapsed Lava Ponds No . 3 and No . 4 26 19. 20. Map of Horse Lava Tu be System . 28 Di agrams of Le wis Farm Cave, Horse Lava Tube System 21. 29 v Page Diagrams of Garbage Caves Nos . and Horse Lava Tube System 30 22. I 2, 23. Diagrams of Horse Cave, Horse Lava Tube System 32 24. South Ice Cave viewed toward entrance 35 25. Diagram of South Ice Cave 37 26. Skeleton Cave Interior . 37 27. Planimetric diagram of Lava River Cave 38 28. Longi tudinal profi le of Lava River Cave 39 29. Lava River Cave near entrance . 41 30. Lava River Cave interior showing roof col lapse and multiple flow lines on wa lls 42 31. Lava River Cave interior partly fi lled with sand 42 32. Lava River Cave interior at the Sand Gardens 43 33. Lava River Cave interior cross sec ti on 44 Plates (fo ld-outs at end of bul letin) 1. Arnol d Lava Tube System Selected lava tubes n ear Bend, Oregon 2. 3. Ph otogeolog ic map of th e lava tubes of parts of Bend and Newberry 30' quadrangles, Oregon VI GEOLOGY OF SELECTED LAVA TUBES IN THE BEND AREA, OREGON by Ronald Greeley ABSTRAC T Lava tubes in the vicinity of Bend, Oregon, we re mapped and studied in detail to determine their geomorphology and mode of formation . Longitudinal profiles representing 5872.5 m of mapped lava tubes and a photogeologic map relating lava tube s to surface geology, regional structure and topography are prese nted. Three sets of lava tubes we re examined: 1) Arnold Lava Tube System (7km long) composed of col l apsed and uncal lapsed tube segments and lava ponds, 2) Horse Lava Tube System (11 km long) composed of parallel and anastomosing lava tube segments, and 3) miscell aneous lava tubes. Results of this study te nd to confirm the "l ayered lava" hypothesis of Oilier and Brown (1965) for lava tube forma­ tion; however, th ere are probably several modes of formation for lava tubes in general . Arnold System is a single series of tubes apparently formed in a single basalt flow on a relatively steep gradient. The advancing flow in wh ich the tubes formed wa s apparently temporarily halted, resulting in the formation of lava ponds wh ich we re inflated and later drained by the lava tube system. Horse System probably fo rmed in multiple, interconnected flaws . Pre-flow gradient appears to have been less than for Arnold System, and resulted in meandrous, multiple tube networks. INTRO DUCTION Interpretation of certain lunar surface features as vol canic structures has resulted in increased in terest in the geomorphology of te rrestrial val conic ana logs. A recent report (Oberbeck an d others, 19 69) propose d that some smaller lunar sinuous rilles (general ly, those less than about 0.5 km wide) probably resulted from lava tube collapse . Other structures (figure l) may be partially col l apse d lunar I avo tubes (Greeley, 1970) Unfortunately, I ittle is known about the formational mechanisms and geomorphology of lava tubes an d it is difficul t to establish criteria to distinguish lunar lava tubes, both collapsed and partly col l apsed, from oth er lunar structures without data on terrestrial counterparts. For th is reason , some of th e major lava tu bes in th e western United States were examined and surveyed to gain an understanding of the geology of these complex structures . The tubes are of interest to several groups besides geol ogists, including zool o­ gists interested i n cave biota, an thropo logists concerned with historic and preh istoric inhabitants, U. S. Forest Service personnel responsible for recreational facilities and safety of National Fo rest visi tors, an d the National S peleological Society, an organization of amateur and professional cave expiorers. The Bend, Oregon area is characterized by relatively young, unweathered vol canic fe atures that are we ll suited for study . In the initial stages of examination of te rre strial analogs to lunar strudures, a field conference was held in Bend to study some of the volcan ic structures (Peterson Groh, 1965). and L a tubes, ho wever, we re only br iefly considered during the conference. This report presents de ta i led av de scriptions of se lected lava tubes, theory of tube formation, and a sketch of the general geology of the Be nd are a. There are many lava tubes in the Bend area. Those th at we re se lected for mapping and study I ie mai nl y an d southeast of Bend. They comprise the Arnold Lava Tube System, i·he Horse Lava Tube east Sy stem, and miscellaneous lava tubes such as Skeleton Cave, Boyd Cave , an d South Ice Cave . Lava River Cave so uth of Bend has al so been in cluded because of its general interest to the publ ic and its ac cessibility as a State Park. 2 LAVA TUBES IN THE BEND AREA MAR IUS HILLS LO ::2:-51 M-212 � N � 0 5 km Figure l. Morius Hills region of the Moon (west-central Oceanus Procellorum). Structure is interpreted to be a portly collapsed lava tube originating from on endogenous crater-vent. From its morphology, the Iorge crater is consid­ ered impact generated. Photograph from NASA Lunar Orbiter V, Site 51, Frome M-21 2.
Recommended publications
  • NEWSLETTERS NUMBER 46, Dec
    International Union of Speleology Union Internationale de Speleologie Commission on Volcanic Caves \ \ I \ \ i i I I ; j December 2005 / .- 1 - U.I.S. is affiliated with UNESCO I The Newsletter is send free to members of the Commission, and others who are interested in lava-tube caves. Jt is not possible to subscribe - but news and information is always appreciated .... I 11 Honorary President: Dr. W.R. Halliday bnawrh @webtv .net j I Chairman & editorial address: a.i. '! J.P. van der Pas Vauwerhofweg 3 6333 CB Schimmert Netherlands jpgvanderpas@ hetnet.nl _.._::- .... "'....... 4 ... .."' \ ' ... ..... - 2- ----~~---~ -~ GIUSEPPE LICITRA 1938 - 5 September 2005 We lost again a monument of Vulcanospe/eology. Below the message which arrived from Nicola Barone, with a description of the works of Guiseppe. I think little can be added to this. I think most of us have met him in person, certainly at 'his' last symposium in Catania 1999. Sincere condolences to his relatives and the Centro Speleo/ogico Etneo, the Commission on Vulcanospeleology I regret to inform you that our member and great friend Giuseppe Licitra died Monday 5111 of September . He was 67 years old. The cause was an heart attack during the night, probably while he was sleeping. Volcanospeleology and lava tubes had a special space into both his heart and mind. He spent more than 30 years of his life for their study and published many papers on journals and conference proceedings. Giuseppe licitra formulated also an interesting theory on the formation of lava tubes. According to this theory, lava flowing inside tubes erodes the ground in such a way that the floor of the tube is the surface of the last lava flow during the active phase of the eruption instead that the material left after lava drain and its subsequent cooling.
    [Show full text]
  • No. 40. the System of Lunar Craters, Quadrant Ii Alice P
    NO. 40. THE SYSTEM OF LUNAR CRATERS, QUADRANT II by D. W. G. ARTHUR, ALICE P. AGNIERAY, RUTH A. HORVATH ,tl l C.A. WOOD AND C. R. CHAPMAN \_9 (_ /_) March 14, 1964 ABSTRACT The designation, diameter, position, central-peak information, and state of completeness arc listed for each discernible crater in the second lunar quadrant with a diameter exceeding 3.5 km. The catalog contains more than 2,000 items and is illustrated by a map in 11 sections. his Communication is the second part of The However, since we also have suppressed many Greek System of Lunar Craters, which is a catalog in letters used by these authorities, there was need for four parts of all craters recognizable with reasonable some care in the incorporation of new letters to certainty on photographs and having diameters avoid confusion. Accordingly, the Greek letters greater than 3.5 kilometers. Thus it is a continua- added by us are always different from those that tion of Comm. LPL No. 30 of September 1963. The have been suppressed. Observers who wish may use format is the same except for some minor changes the omitted symbols of Blagg and Miiller without to improve clarity and legibility. The information in fear of ambiguity. the text of Comm. LPL No. 30 therefore applies to The photographic coverage of the second quad- this Communication also. rant is by no means uniform in quality, and certain Some of the minor changes mentioned above phases are not well represented. Thus for small cra- have been introduced because of the particular ters in certain longitudes there are no good determi- nature of the second lunar quadrant, most of which nations of the diameters, and our values are little is covered by the dark areas Mare Imbrium and better than rough estimates.
    [Show full text]
  • TRANSIENT LUNAR PHENOMENA: REGULARITY and REALITY Arlin P
    The Astrophysical Journal, 697:1–15, 2009 May 20 doi:10.1088/0004-637X/697/1/1 C 2009. The American Astronomical Society. All rights reserved. Printed in the U.S.A. TRANSIENT LUNAR PHENOMENA: REGULARITY AND REALITY Arlin P. S. Crotts Department of Astronomy, Columbia University, Columbia Astrophysics Laboratory, 550 West 120th Street, New York, NY 10027, USA Received 2007 June 27; accepted 2009 February 20; published 2009 April 30 ABSTRACT Transient lunar phenomena (TLPs) have been reported for centuries, but their nature is largely unsettled, and even their existence as a coherent phenomenon is controversial. Nonetheless, TLP data show regularities in the observations; a key question is whether this structure is imposed by processes tied to the lunar surface, or by terrestrial atmospheric or human observer effects. I interrogate an extensive catalog of TLPs to gauge how human factors determine the distribution of TLP reports. The sample is grouped according to variables which should produce differing results if determining factors involve humans, and not reflecting phenomena tied to the lunar surface. Features dependent on human factors can then be excluded. Regardless of how the sample is split, the results are similar: ∼50% of reports originate from near Aristarchus, ∼16% from Plato, ∼6% from recent, major impacts (Copernicus, Kepler, Tycho, and Aristarchus), plus several at Grimaldi. Mare Crisium produces a robust signal in some cases (however, Crisium is too large for a “feature” as defined). TLP count consistency for these features indicates that ∼80% of these may be real. Some commonly reported sites disappear from the robust averages, including Alphonsus, Ross D, and Gassendi.
    [Show full text]
  • A Guideline for a Sustainable Lunar Base Design for Constructed in Lunar Lava Tubes and Their Vertical Skylights
    50th International Conference on Environmental Systems ICES-2021-186 12-15 July 2021 A Guideline for a Sustainable Lunar Base Design for Constructed in Lunar Lava Tubes and Their Vertical Skylights Masato Sakurai1, Asuka Shima2, Isao Kawano3, Junichi Haruyama4 Japan Aerospace Exploration Agency (JAXA), Chofu-shi, Tokyo, 182-8522, Japan. and Hiroyuki Miyajima5 International University of Health and Welfare, Narita Campus 1, 4-3, Kōzunomori, Narita, Chiba, 286-8686 Japan The lunar surface is a hostile environment subject to harmful radiation and meteorite impacts. A recently discovered lava tube avoids these risks and, as it undergoes only slight temperature changes, it is a promising location for constructing a lunar base. JAXA engages in research in regenerative ECLSS (Environmental Control Life Support Systems), particularly addressing water and air recycling and treating organic waste. Overcoming these challenges is essential for long-term lunar habitation. This paper presents a guideline for a sustainable lunar base design. Nomenclature ECLSS = Environmental Control Life Support System HTV = H-II Transfer Vehicle ISS = International Space Station JAXA = Japan Aerospace Exploration Agency JSASS = Japan Society for Aeronautical and Space Science MHH = Marius Hills Hole MIH = Mare Ingenii Hole MTH = Mare Tranquillitatis Hole SELENE = Selenological and Engineering Explorer UZUME = Unprecedented Zipangu Underworld of the Moon Exploration (name of the research group for vertical holes) SDGs = Sustainable Development Goals SELENE = Selenological and Engineering Explorer I. Introduction uture space exploration will extend beyond low Earth orbit and dramatically expand in scope. In particular, F industrial activities are planned for the Moon with the development of infrastructure that includes lunar bases. This paper summarizes our study of the construction of a crewed permanent settlement, which will be essential to support long-term habitation, resource utilization, and industrial activities on the Moon.
    [Show full text]
  • Insights from the Spatial Distribution of Floor-Fractured and Concentric Craters
    52nd Lunar and Planetary Science Conference 2021 (LPI Contrib. No. 2548) 2245.pdf EVIDENCE FOR THE LUNAR PROCELLARUM BASIN: INSIGHTS FROM THE SPATIAL DISTRIBUTION OF FLOOR-FRACTURED AND CONCENTRIC CRATERS. S. Ravi and M.S. Robinson, School of Earth and Space Exploration, Arizona State University, Tempe, AZ – 85282, USA (Email: [email protected]) Introduction: Floor-fractured (FFCs) and Camera (LROC) Wide Angle Camera (WAC) GLD 100 DTM concentric craters (CCs) are impact craters that [13]. underwent modification by volcano-tectonic processes Both FFCs and CCs appear to be clustered within such as viscous relaxation or magmatic intrusion impact basins, with >60% of FFCs and CCs following basin-forming events (Fig. 1) [1-6]. concentrated along the western boundary of the proposed Procellarum basin [10] (Fig. 2). Whether the spatial distribution of FFCs and CCs are random or genetically related to impact basins is not well understood. If the latter is true, then we can not only use FFCs and CCs as proxies for identifying ancient basin Figure 1: Characteristics of floor-fractured and concentric rims, but we can also infer local and regional variations craters. (A) Vitello crater (D = 40km) exhibits radial/concentric fractures, (B) Gassendi crater (D = 100km) in the strength of the lunar lithosphere. Therefore, the exhibits mare basalt infill, and (C) an unnamed concentric overarching goal of this study is to determine and crater (D = 5km) exhibits an uplifted concentric ridge. analyze the statistical significance of the spatial distribution of FFCs and CCs with respect to impact The Procellarum KREEP Terrane (PKT) is one of basins.
    [Show full text]
  • Lava Caves of the Republic of Mauritius, Indian Ocean
    87 Inl. J. Spcleol .. 2713 (1/4), (1998): 87-93. LAVA CAVES OF THE REPUBLIC OF MAURITIUS, INDIAN OCEAN Gregory J. Middleton' ABSTRACT In their Unde/growlll Atlas. MIDDLETON &. WALTHAM (1986) dismissed Mauritius as: "very old vol- canic islands with no speleological interest". Recent investigations indicate this judgement is inaccurate; there arc over 50 significant caves. including lava tube caves up to 687 m long (one 665 m long was surveyed as early as 1769) and 35 m wide. Plaine des Roches contains the most extensive system of lava tube caves with underground drainage rising at the seashore. Notable fauna includes an insectivorous bat and a cave swiftlet (Col/ocalia Fancica), the nests of which are unfortunately prized for "soup". The caves are generally not valued by the people and are frequently used for rubbish disposal or tilled in for agricultural development. Keywords: vulcanospeleology. lava luhcs, Mauritius RESUME Bien que les iles Maurice ne soient pas connues pour leur interet spelt'ologique, de recentes recherches indiquent qu'il y a plus de cinquante cavernes importantes. comprenant des tunncls de lave allant jusqu'a de 687 m de long et 35 m de large, I'un d'entre eux, de 665 m de long a ete decouvert des 1769. La Plaine des Roches contient Ie systeme Ie plus etendu de tunnels de lave avec un ecoulement souterrain qui s'clcve au niveau du rivagc. La t~lUnc importantc de ces caves comprend de chauvcs-souris insectivores et de petites hirondelles (Col/ocalia fnlllcica), les nids desquelles sont malheureusement recherches pour soupes de gourmets.
    [Show full text]
  • EXPLORING SUBSURFACE LUNAR VOIDS USING SURFACE GRAVIMETRY. Kieran A. Carroll, Da- Vid Hatch2, R. Ghent3, S. Stanley3, N. Urbancic3, Marie-Claude Williamson, W.B
    46th Lunar and Planetary Science Conference (2015) 1746.pdf EXPLORING SUBSURFACE LUNAR VOIDS USING SURFACE GRAVIMETRY. Kieran A. Carroll, Da- vid Hatch2, R. Ghent3, S. Stanley3, N. Urbancic3, Marie-Claude Williamson, W.B. Garry4, Manik Talwani5 1Gedex Inc., 407 Matheson Blvd. East, Mississauga, Ontario, Canada L4Z 2H2, [email protected], 2Gedex Inc., 3University of Toronto, 4NASA GSFC, 5Rice University. Introduction: Surface gravimetry is a standard been found to be linear but discontinuous…the space terrestrial geophysics exploration technique. As noth- between such features likely represents uncollapsed ing blocks gravity, this approach can detect subsurface tube.” structures with contrasting densities, both shallow and The structure of these voids is currently unknown, deep. Recently-collected high-resolution imagery of being unobservable via imagery from orbit. Lava tube the Moon has identified numerous pits, indicative of voids presumably might be like terrestrial lava tubes -- subsurface voids. Here we analyze the anomalous - long, linear or sinuous tunnels. In [5], Wagner et al. gravity signal expected at the Moon’s surface due to speculate that “a complex plumbing system may form both localized voids and more-extensive lava tubes, in some impact melt deposits,” and that “where multi- and find that the signal can be large enough to be ple pits were found in a single pond, the pits often oc- measured with Lunar-compatible gravimeters. A po- cur in one or more small regions (~2-5 km square) tential near-term Lunar surface survey of a mare pit within the melt deposit…occasionally, several pits crater in Lacus Mortis is discussed. occur within tens of meters of each other, indicating a possible subsurface connection.” Presumably some Lunar Lava Tubes and Other Subsurface other Lunar subsurface voids might instead be much Voids: Lava tubes can form when an exposed magma more compact, resulting from the draining of a single flow cools at its top surface, forming a solid “lid” over small melt pond.
    [Show full text]
  • Volcanic Vistas Discover National Forests in Central Oregon Summer 2009 Celebrating the Re-Opening of Lava Lands Visitor Center Inside
    Volcanic Vistas Discover National Forests in Central Oregon Summer 2009 Celebrating the re-opening of Lava Lands Visitor Center Inside.... Be Safe! 2 LAWRENCE A. CHITWOOD Go To Special Places 3 EXHIBIT HALL Lava Lands Visitor Center 4-5 DEDICATED MAY 30, 2009 Experience Today 6 For a Better Tomorrow 7 The Exhibit Hall at Lava Lands Visitor Center is dedicated in memory of Explore Newberry Volcano 8-9 Larry Chitwood with deep gratitude for his significant contributions enlightening many students of the landscape now and in the future. Forest Restoration 10 Discover the Natural World 11-13 Lawrence A. Chitwood Discovery in the Kids Corner 14 (August 4, 1942 - January 4, 2008) Take the Road Less Traveled 15 Larry was a geologist for the Deschutes National Forest from 1972 until his Get High on Nature 16 retirement in June 2007. Larry was deeply involved in the creation of Newberry National Volcanic Monument and with the exhibits dedicated in 2009 at Lava Lands What's Your Interest? Visitor Center. He was well known throughout the The Deschutes and Ochoco National Forests are a recre- geologic and scientific communities for his enthusiastic support for those wishing ation haven. There are 2.5 million acres of forest including to learn more about Central Oregon. seven wilderness areas comprising 200,000 acres, six rivers, Larry was a gifted storyteller and an ever- 157 lakes and reservoirs, approximately 1,600 miles of trails, flowing source of knowledge. Lava Lands Visitor Center and the unique landscape of Newberry National Volcanic Monument. Explore snow- capped mountains or splash through whitewater rapids; there is something for everyone.
    [Show full text]
  • The Role of Surface Tension on the Formation of Lava Stalactite and Lava
    The role of surface tension on the formation of lava stalactite and lava stalagmite Tsutomu Honda NPO Vulcano-Speleological Society 3-14-5,Tsurumaki,Setagaya-ku,Tokyo,Japan 154-0016 [email protected] Abstract The role of surface tension of lava on the formation of lava stalactite and lava stalagmite is analysed by two different physical models. A hydrodynamic instability model is used for a lava stalactite formation and a fallen droplet model is used for a lava stalagmite formation. The surface tensions estimated from two different models show a good coincidence and reasonable value as surface tension of lava. 1.Introduction Inside the lava caves and lava tree mold voids formed by the basalt lava flow, lava stalactites and lava stalagmites are often observed. It is a phenomenon in which the droplet of lava falls from a ceiling and deposits on the floor. By using two simple models where the balance between gravity and surface tension acting on lava surface are taken into consideration, the estimation of surface tension of lava from the pitch of lava stalactite and size of lava stalagmite appeared in lava tube cave and tree mold void are performed Fig.1 Void in Funatsu Tainai Lava Tree Mold and compared with various lavas. 2.Estimate of surface tension from lava stalactite Fig.1 shows a genral feature of the inside of lava tree mold. Lava stalactites are positioned periodically on the surface of the ceiling wall or side wall. From the periodical pitch of the stalactites, we can obtain the surface tension of the lava1~3).
    [Show full text]
  • Water on the Moon, III. Volatiles & Activity
    Water on The Moon, III. Volatiles & Activity Arlin Crotts (Columbia University) For centuries some scientists have argued that there is activity on the Moon (or water, as recounted in Parts I & II), while others have thought the Moon is simply a dead, inactive world. [1] The question comes in several forms: is there a detectable atmosphere? Does the surface of the Moon change? What causes interior seismic activity? From a more modern viewpoint, we now know that as much carbon monoxide as water was excavated during the LCROSS impact, as detailed in Part I, and a comparable amount of other volatiles were found. At one time the Moon outgassed prodigious amounts of water and hydrogen in volcanic fire fountains, but released similar amounts of volatile sulfur (or SO2), and presumably large amounts of carbon dioxide or monoxide, if theory is to be believed. So water on the Moon is associated with other gases. Astronomers have agreed for centuries that there is no firm evidence for “weather” on the Moon visible from Earth, and little evidence of thick atmosphere. [2] How would one detect the Moon’s atmosphere from Earth? An obvious means is atmospheric refraction. As you watch the Sun set, its image is displaced by Earth’s atmospheric refraction at the horizon from the position it would have if there were no atmosphere, by roughly 0.6 degree (a bit more than the Sun’s angular diameter). On the Moon, any atmosphere would cause an analogous effect for a star passing behind the Moon during an occultation (multiplied by two since the light travels both into and out of the lunar atmosphere).
    [Show full text]
  • Get Down and Dirty!
    Get down and dirty! ICE CAVE and NATURAL BRIDGES, MT. ADAMS RANGER DISTRICT The "Ice Cave" was discovered at least 100 years ago and provided ice for the towns of Hood River and The Dalles in pioneer years. This well-known cave has four sections, separated by three collapsed sink about 15 feet in diameter and 14 feet deep. A wooden stairway leads to the neve cone beneath the main entrance of this lava tube glaciere. Most visitors are aware only of the 120-foot glaciere section that slopes southeastward from the ladder, but some penetrate the more constricted, sinuous 200-foot passage leading west to another collapsed sink. The other three sections of the tube, sloping downward from the west, are generally overlooked. The total length of the cavern passages is about 650 feet. The western, uppermost section of the cave is a low, rather unremarkable passage about 150 feet long. It is the widest part of the cave system, and is floored with smooth lava. On the north side of the sink, at its lower end, is a short, broad, low passage from which another lava flow entered the tube. The next section, to the east, is about 100 feet long and 15 feet wide. It is the only section of the cave where one may stroll from one sink to the next, despite the irregular breakdown on the floor. Between the sink at the lower end of this section and that at the upper end of the "main" section, the tube divides into two smaller tubes about 60 feet long and five feet high.
    [Show full text]
  • High Desert Region Around Bend, Oregon by Lee Foster
    High Desert Region Around Bend, Oregon by Lee Foster Beauty of nature in an alpine setting and diverse outdoor sports attract visitors to the Bend region of Central Oregon. Perusing natural beauty is the most universal pleasure here. Snow-capped mountains, pristine lakes, white-water rivers, and pine forests abound. At any time, the wilderness scenery is striking, with one of the dominant peaks, Mt. Bachelor, Broken Top, and the Sisters, usually present on your horizon. The main natural imprint on the land is a black volcanic presence. For the geology enthusiast, the Lava Lands Visitor Center explains the historic volcanic flows that form a stark legacy. Lava Butte is a 500-foot-high cinder cone, a silent reminder of past volcanic upheavals. A Rockhound Pow-Wow gathers amateur geologists here each July. Since opening in 1982, the High Desert Museum, south of Bend, has emerged as the most important nature interpretive effort in the state. (The High Desert Museum at Bend parallels Tucson’s Arizona-Sonora Desert Museum.) The raptor exhibit alone is worth the visit, putting you as close as you may ever get to a great horned owl, a red-tailed hawk, and an American kestrel. Foremost among the outdoor sports here is skiing at Mt. Bachelor. An extremely long ski season, both for alpine and nordic skiing, lasts into summer. The high- elevation chair lift to the top of Bachelor is popular also with non-skiers who seek an inspiring view of the region. In summer, hikers and campers depart from Bend for the nearby wilderness areas.
    [Show full text]