An Overview of Analogue Models Compared to Natural Calderas ⁎ Valerio Acocella
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Glossary Glossary
Glossary Glossary Albedo A measure of an object’s reflectivity. A pure white reflecting surface has an albedo of 1.0 (100%). A pitch-black, nonreflecting surface has an albedo of 0.0. The Moon is a fairly dark object with a combined albedo of 0.07 (reflecting 7% of the sunlight that falls upon it). The albedo range of the lunar maria is between 0.05 and 0.08. The brighter highlands have an albedo range from 0.09 to 0.15. Anorthosite Rocks rich in the mineral feldspar, making up much of the Moon’s bright highland regions. Aperture The diameter of a telescope’s objective lens or primary mirror. Apogee The point in the Moon’s orbit where it is furthest from the Earth. At apogee, the Moon can reach a maximum distance of 406,700 km from the Earth. Apollo The manned lunar program of the United States. Between July 1969 and December 1972, six Apollo missions landed on the Moon, allowing a total of 12 astronauts to explore its surface. Asteroid A minor planet. A large solid body of rock in orbit around the Sun. Banded crater A crater that displays dusky linear tracts on its inner walls and/or floor. 250 Basalt A dark, fine-grained volcanic rock, low in silicon, with a low viscosity. Basaltic material fills many of the Moon’s major basins, especially on the near side. Glossary Basin A very large circular impact structure (usually comprising multiple concentric rings) that usually displays some degree of flooding with lava. The largest and most conspicuous lava- flooded basins on the Moon are found on the near side, and most are filled to their outer edges with mare basalts. -
Feature of the Month – January 2016 Galilaei
A PUBLICATION OF THE LUNAR SECTION OF THE A.L.P.O. EDITED BY: Wayne Bailey [email protected] 17 Autumn Lane, Sewell, NJ 08080 RECENT BACK ISSUES: http://moon.scopesandscapes.com/tlo_back.html FEATURE OF THE MONTH – JANUARY 2016 GALILAEI Sketch and text by Robert H. Hays, Jr. - Worth, Illinois, USA October 26, 2015 03:32-03:58 UT, 15 cm refl, 170x, seeing 8-9/10 I sketched this crater and vicinity on the evening of Oct. 25/26, 2015 after the moon hid ZC 109. This was about 32 hours before full. Galilaei is a modest but very crisp crater in far western Oceanus Procellarum. It appears very symmetrical, but there is a faint strip of shadow protruding from its southern end. Galilaei A is the very similar but smaller crater north of Galilaei. The bright spot to the south is labeled Galilaei D on the Lunar Quadrant map. A tiny bit of shadow was glimpsed in this spot indicating a craterlet. Two more moderately bright spots are east of Galilaei. The western one of this pair showed a bit of shadow, much like Galilaei D, but the other one did not. Galilaei B is the shadow-filled crater to the west. This shadowing gave this crater a ring shape. This ring was thicker on its west side. Galilaei H is the small pit just west of B. A wide, low ridge extends to the southwest from Galilaei B, and a crisper peak is south of H. Galilaei B must be more recent than its attendant ridge since the crater's exterior shadow falls upon the ridge. -
Inflation of the Aira Caldera (Japan) Detected Over
eEarth, 2, 17–25, 2007 www.electronic-earth.net/2/17/2007/ eEarth © Author(s) 2007. This work is licensed under a Creative Commons License. Inflation of the Aira Caldera (Japan) detected over Kokubu urban area using SAR interferometry ERS data D. Remy1,2,*, S. Bonvalot1,2, M. Murakami3, P. Briole2, and S. Okuyama4 1Institut de Recherche pour le Developpement´ (IRD), UR154, France 2Institut de Physique du Globe de Paris, 4 Place Jussieu, 75005 Paris, France 3Geographical Survey Institute, Mizusawa Geodetic Observatory, Japan 4Kyoto University, Dept. of Geophysics, Kyoto, 606-8502, Japan *presently at: Dept. of Geophysics, University of Chile, Santiago, Chile Received: 20 July 2006 – Published in eEarth Discuss.: 8 August 2006 Revised: 26 October 2006 – Accepted: 30 January 2007 – Published: 2 February 2007 Abstract. Nine ERS-1 and ERS-2 descending orbit data ac- 1 Introduction quired over Aira Caldera between June 1995 and November 1998 were used to create 36 differential interferograms. Al- Numerous papers have shown the potential of SAR (Syn- though the interferograms exhibit a relatively low level of thetic Aperture Radar) interferometry data for ground defor- coherence, even for couples sampling short time intervals (6 mation studies on volcanoes (Massonnet and Sigmundsson, months), Synthetique Aperture Radar (SAR) observations re- 2000; Zebker et al., 2000; Pritchard and Simons, 2002). Un- veal a distinct range change pattern over Kokubu urban area der optimal conditions a differential interferogram derived whose amplitude increases with the time separation between from two SAR images may monitor topographic changes in- SAR images. The analysis of the ground deformation time duced by internal volcanic processes with an accuracy of a series relative to the earliest ERS images showed a maxi- few cm over periods of time up to several months or years. -
Sky and Telescope
SkyandTelescope.com The Lunar 100 By Charles A. Wood Just about every telescope user is familiar with French comet hunter Charles Messier's catalog of fuzzy objects. Messier's 18th-century listing of 109 galaxies, clusters, and nebulae contains some of the largest, brightest, and most visually interesting deep-sky treasures visible from the Northern Hemisphere. Little wonder that observing all the M objects is regarded as a virtual rite of passage for amateur astronomers. But the night sky offers an object that is larger, brighter, and more visually captivating than anything on Messier's list: the Moon. Yet many backyard astronomers never go beyond the astro-tourist stage to acquire the knowledge and understanding necessary to really appreciate what they're looking at, and how magnificent and amazing it truly is. Perhaps this is because after they identify a few of the Moon's most conspicuous features, many amateurs don't know where Many Lunar 100 selections are plainly visible in this image of the full Moon, while others require to look next. a more detailed view, different illumination, or favorable libration. North is up. S&T: Gary The Lunar 100 list is an attempt to provide Moon lovers with Seronik something akin to what deep-sky observers enjoy with the Messier catalog: a selection of telescopic sights to ignite interest and enhance understanding. Presented here is a selection of the Moon's 100 most interesting regions, craters, basins, mountains, rilles, and domes. I challenge observers to find and observe them all and, more important, to consider what each feature tells us about lunar and Earth history. -
Tomographic Image of the Crust Beneath the Aira Caldera in Southern Kyushu
IAVCEI 2013 Scientific Assembly - July 20 - 24, Kagoshima, Japan Forecasting Volcanic Activity - Reading and translating the messages of nature for society 4W_1B-P5 Date/Time: July 24 Poster Tomographic image of the crust beneath the Aira caldera in southern Kyushu Hiroki Miyamachi1, Paul Karson Alanis2, Hiroshi Yakiwara1, Takeshi Tameguri3, Masato Iguchi3 1Kagoshima University, Japan, 2Philippine Institute of Volcanology and Seismology, Philippines, 3Kyoto University, Japan E-mail: [email protected] Associated with the Philippine Sea plate subduction, a nearly straight chain of active Quaternary volcanism runs almost parallel to Nankai Trough in the central part of southern Kyushu. In this region, there are four large calderas: the Kakuto, the Aira, the Ata and the Kikai calderas. We applied the tomography method with a fine grid configuration to the P- and S-wave arrival times of 829 local earthquakes well observed at 101 stations in central and southern Kyushu, and revealed the detailed three-dimensional seismic velocity structure of the crust, especially the region beneath the Aira caldera. In a shallow range from 0 to 10 km depth, low velocity zones (LVZs) are found in the eastern part of Kyushu, where basement rocks are made up of uplifted sedimentary marine terraces (Nakada et al., 2002). The LVZs are also distributed along the volcanic front between Kirishima volcano to Kaimon volcano. Meanwhile, the hypocenters occurred in the inland area are obviously concentrated in regions with a relatively higher velocity and a low Poisson’s ratio at a depth of 10 km. At 20 km depth, the most interesting feature is that a distinctly high Poisson’s ratio zone is located exactly beneath the Aira caldera. -
Apollo 12 Photography Index
%uem%xed_ uo!:q.oe_ s1:s._l"e,d_e_em'I flxos'p_zedns O_q _/ " uo,re_ "O X_ pea-eden{ Z 0 (D I I 696L R_K_D._(I _ m,_ -4 0", _z 0', l',,o ._ rT1 0 X mm9t _ m_o& ]G[GNI XHdV_OOZOHd Z L 0T'I0_V 0 0 11_IdVdONI_OM T_OINHDZZ L6L_-6 GYM J_OV}KJ_IO0VSVN 0 C O_i_lOd-VJD_IfO1_d 0 _ •'_ i wO _U -4 -_" _ 0 _4 _O-69-gM& "oN GSVH/O_q / .-, Z9946T-_D-VSVN FOREWORD This working paper presents the screening results of Apollo 12, 70mmand 16mmphotography. Photographic frame descriptions, along with ground coverage footprints of the Apollo 12 Mission are inaluded within, by Appendix. This report was prepared by Lockheed Electronics Company,Houston Aerospace Systems Division, under Contract NAS9-5191 in response to Job Order 62-094 Action Document094.24-10, "Apollo 12 Screening IndeX', issued by the Mapping Sciences Laboratory, MannedSpacecraft Center, Houston, Texas. Acknowledgement is made to those membersof the Mapping Sciences Department, Image Analysis Section, who contributed to the results of this documentation. Messrs. H. Almond, G. Baron, F. Beatty, W. Daley, J. Disler, C. Dole, I. Duggan, D. Hixon, T. Johnson, A. Kryszewski, R. Pinter, F. Solomon, and S. Topiwalla. Acknowledgementis also made to R. Kassey and E. Mager of Raytheon Antometric Company ! I ii TABLE OF CONTENTS Section Forward ii I. Introduction I II. Procedures 1 III. Discussion 2 IV. Conclusions 3 V. Recommendations 3 VI. Appendix - Magazine Summary and Index 70mm Magazine Q II II R ii It S II II T II I! U II t! V tl It .X ,, ,, y II tl Z I! If EE S0-158 Experiment AA, BB, CC, & DD 16mm Magazines A through P VII. -
Lunar Observers' Feature Finder
Lunar Observers’ Feature Finder This feature finder is a modified version of Charles Wood’s original “Lunar 100” list as published in April 2004 Sky & Telescope. Notes: • The orientation is as seen with the naked eye and binoculars. Different telescopes may reverse the image vertically or laterally or both depending on telescope type and whether a star diagonal is used or not. • Feature visibilities are correct for viewing at about 2200-2300 hrs on the dates given. • See the guidance at the end of this article for help on using the table. That guidance also includes how the table can be used for dates following May 2021. Moon May Diam. or Long. (°) Term. Age Date L V Feature Name Significance length Lat. (°) E -ve Long. (days) 2021 (km) W +ve 85 C Langrenus rays Aged ray system 132 8.9S -60.9 16 A Petavius Crater with domed & fractured 177 25.1S -60.4 3 14 floor -52 10 A Mare Crisium Mare contained in large 540 18.0N -59.0 and (DA) circular basin 58 B Rheita Valley Basin secondary-crater chain 445 42.5S -51.5 25 A Messier & Oblique ricochet-impact pair 11 1.9S -47.6 Messier A 4 15 12 A Proclus Oblique-impact rays 28 16.1N -46.8 -40 31 A Taruntius Young floor-fractured crater 56 5.6N -46.5 72 C Atlas dark-halo Explosive volcanic pits on the 87 46.7N -44.4 craters floor of Atlas 40 B Janssen Rille Rare example of a highland 190 45.4S -39.3 rille across floor of Janssen 48 B Cauchy region Fault, rilles, & domes 130 10.5N -38.0 21 A Fracastorius Crater with subsided & 124 21.5S -33.2 fractured floor 88 C Peary Difficult-to-observe polar 74 -
Workshop on Geology of the Apollo 17 Landing Site
NASA-CR-191637 \ WORKSHOP ON GEOLOGY OF THE APOLLO 17 LANDING SITE (NASA-CR-191637) WORKSHOP ON N93-18786 GEOLOGY OF THE APOLLO 17 LANDING --THRU-- SITE (Lunar Science Inst.) 70 p N93-18817 Unclas G3/91 0141290 __ LPI Technical Report Number 92-09, Part 1 LUNAR AND PLANETARY INSTITUTE 3600 BAY AREA BOULEVARD HOUSTON TX 77058-1113 LPI/TR--92-09, Part 1 WORKSHOP ON GEOLOGY OF THE APOLLO 17 LANDING SITE Edited by G. Ryder, H. H. Schmitt, and P. D. Spudis Held at Houston, Texas December 2-4, 1992 Sponsored by Lunar and Planetary Sample Team Lunar and Planetary Institute Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113 LPI Technical Report Number 92-09, Part 1 LPI/TR--92-09, Part 1 Compiledin 1992by LUNAR AND PLANETARY INSTITUTE TheInstituteis operatedby theUniversitySpaceResearchAssociationunderContractNo. NASW- 4574with theNationalAeronauticsandSpaceAdministration. Materialin this volume may be copied without restraint for library, abstract service, education, or per- sonal research purposes; however, republication of any paper or portion thereof requires the written permission of the authors as well as the appropriate acknowledgment of this publication. This report may be cited as Ryder G., Schmitt H. H., and Spudis P. D., eds. (1992) Workshop on Geology of the Apollo 17 Landing Site. LPI Tech. Rpt. 92-09, Part 1, Lunar and Planetary Institute, Houston. 63 pp. This report is distributed by ORDER DEPARTMENT Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113 Mail order requestors will be invoiced for the cost of shipping and handling. Cover: Station 4 at Taurus-LiUrow, Apollo 17 landing site. -
Volcanic Hazards As Components of Complex Systems: the Case of Japan
Volume 13 | Issue 33 | Number 6 | Article ID 4359 | Aug 17, 2015 The Asia-Pacific Journal | Japan Focus Volcanic Hazards as Components of Complex Systems: The Case of Japan Gregory Smits The past year or so has been a time of the earth’s crust suggested Mt. Fuji is more particularly vigorous volcanic activity in Japan, likely to erupt owing to effects from the 2011 or at least activity that has intruded into public Tōhoku earthquake.3 Well publicized by a press awareness. Perhaps most dramatic was the release on the eve of its publication, mass deadly eruption of Mt. Ontake on September media around the world have reported this 27, 2014, whose 57 fatalities were the first finding, along with speculation regarding volcano-related deaths in Japan since 1991. On possible connections between earthquakes and May 29, 2015, Mt. Shindake, off the southern volcanic eruptions. tip of Kyushu, erupted violently, forcing the evacuation of the island of Kuchinoerabu. That As of June 30, 2015, the Japan Meteorological same day, Sakurajima, located just north in Agency (JMA) designated ten volcanoes in or Kagoshima Bay, erupted more forcefully than near the main Japanese islands as warranting usual. Sakurajima has been erupting in some levels of warning ranging from Mt. Shindake’s fashion almost continuously since 1955, but Level 5 (“Evacuate”), to Level 2 (“Do not since 2006, its activity has become relatively approach the crater”) in seven cases. more vigorous. Indeed, a May 30 Asahi shinbun Sakurajima is at Level 3 (“Do not approach the article characterized these eruptions as “the volcano”), as is Hakoneyama, located near Mt. -
Calderas in Japan
Calderas in Japan ref Main Post-Caldera Volcano Most Recent Caldera Type of Ejecta ref About Period No. About Formation Caldera Name Document No. Name Eruption Period (Symbol) 番号 14 Kishimoto, T., et al. (2009) Tephrostratigraphy and Eruption Mashu f Yamamoto, T., et al. (2010) C ages for the ejecta from Style of Mashu Volcano, During the Last 14,000 years, Eastern Mashu Kamuinupuri, Kamuisshuto 7.6 ka* 1, 5 1 Kutcharo and Mashu calderas, eastern Hokkaido, Japan. Bull. Geol. 5 (Ma-f) Hokkaido, Japan. Bull.Volcanol.Soc.Japan Surv. Japan, 61, 161-170. , 54, 15-37. 14 Hasegawa, T., et al. (2010) The history of caldera-forming Kutcharo 1 Yamamoto, T., et al. (2010) C ages for the ejecta from Kutcharo Atosanupuri, Nakajima 40 ka* 1, 2 1 Kutcharo and Mashu calderas, eastern Hokkaido, Japan. Bull. Geol. 2 eruptions in eastern Hokkaido, Japan. CHIKYU MONTHLY, 33, (Kp I) Surv. Japan, 61, 161-170. 726-734. Hasegawa, T., et al. (2010) The history of caldera-forming Hasegawa, T., et al. (2010) The history of caldera-forming Akan 1 Akan Meakandake, Oakandake 120←→210 ka 2 2 eruptions in eastern Hokkaido, Japan. CHIKYU MONTHLY, 33, 726- 2 eruptions in eastern Hokkaido, Japan. CHIKYU MONTHLY, 33, (Ak1) 734. 726-734. Yamagata, K (1994) Tephrochronological Study on the Shikotsu No. 1 Hiroshi Machida and Fusao Arai (2003) Atlas of tephra in and 3 6 Shikotsu and Kuttara Volcanoes in Southwestern Hokkaido, Shikotsu Eniwadake, Tarumaesan 40←→45 ka* 3, 6 around Japan. Univ. of Tokyo Press, 336p. (Spfl, Spfa-1) Japan. Jour. Geol. Soc. -
Breaking Volcano News
Volcano News & Questions from Students VOLCANIC ERUPTIONS Physical Phenomena Causes – movement at plate boundaries Geography – spatial distribution Forms and eruption styles Magnitude Prediction – looking back & monitoring Hazards – quakes, blasts; release of ash, gas & lava Impacts Fatalities Economic Mitigation & Preparedness Begins with understanding vulnerability Recently, eruption of Icelandic volcano halted air travel Breaking Volcano News http://www.volcanolive.com/news.html …and news of breaking volcanoes History shows that when Eyjafjallajökull erupts, it’s larger neighbour Katla is generally not far behind. Katla is overdue. Katla’s eruption may be 10 or more x the size of the Eyjafjallajökull eruption –significant floods of fresh glacial-melt water into the sea (flow equal to Amazon + Mississippi + Nile + Yangtze occurred following 1755 eruption), a column of ash rising Chaiten, Chile 20km, or more, into the jet stream and spread over N Hemisphere. The Laki eruption in Iceland in 1783 resulted in famine across W Met Office, summer 2010 Europe, and as far S as Egypt, one of the longest and coldest ..as ash entrained in the atmosphere moved from winters on record in N America, and the death of 10,000s of Iceland across the Atlantic. people from gas poisoning and famine. 1 Merapi is at a subduction zone, where the Indo-Australian Plate is sliding NEWS beneath the Eurasian Plate and part of the Pacific Ring of Fire Stratigraphic analysis reveals that eruptions in the Merapi area began about Merapi Eruption 400,000 years ago, and from then until about 10,000 years ago, eruptions were effusive, and outflowing lava emitted was basaltic. -
Inflation of the Aira Caldera (Japan) Detected Over Kokubu
eEarth, 2, 17–25, 2007 www.electronic-earth.net/2/17/2007/ eEarth © Author(s) 2007. This work is licensed under a Creative Commons License. Inflation of the Aira Caldera (Japan) detected over Kokubu urban area using SAR interferometry ERS data D. Remy1,2,*, S. Bonvalot1,2, M. Murakami3, P. Briole2, and S. Okuyama4 1Institut de Recherche pour le Developpement´ (IRD), UR154, France 2Institut de Physique du Globe de Paris, 4 Place Jussieu, 75005 Paris, France 3Geographical Survey Institute, Mizusawa Geodetic Observatory, Japan 4Kyoto University, Dept. of Geophysics, Kyoto, 606-8502, Japan *presently at: Dept. of Geophysics, University of Chile, Santiago, Chile Received: 20 July 2006 – Published in eEarth Discuss.: 8 August 2006 Revised: 26 October 2006 – Accepted: 30 January 2007 – Published: 2 February 2007 Abstract. Nine ERS-1 and ERS-2 descending orbit data ac- 1 Introduction quired over Aira Caldera between June 1995 and November 1998 were used to create 36 differential interferograms. Al- Numerous papers have shown the potential of SAR (Syn- though the interferograms exhibit a relatively low level of thetic Aperture Radar) interferometry data for ground defor- coherence, even for couples sampling short time intervals (6 mation studies on volcanoes (Massonnet and Sigmundsson, months), Synthetique Aperture Radar (SAR) observations re- 2000; Zebker et al., 2000; Pritchard and Simons, 2002). Un- veal a distinct range change pattern over Kokubu urban area der optimal conditions a differential interferogram derived whose amplitude increases with the time separation between from two SAR images may monitor topographic changes in- SAR images. The analysis of the ground deformation time duced by internal volcanic processes with an accuracy of a series relative to the earliest ERS images showed a maxi- few cm over periods of time up to several months or years.