Yellowstone Science
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
A Possible Albian Impact Crater at Murshid, Southern Oman
GeoArabia, Vol. 7, No. 4, 2002 Gulf PetroLink, Bahrain A possible Albian impact crater at Murshid, southern Oman Bruce Levell1, Pascal Richard2 and Folco Hoogendijk2, Petroleum Development Oman ABSTRACT During interpretation of a 3-D seismic survey in southern Oman a solitary, 2.5-km-wide circular basin with a central peak and raised rim was identified in the subsurface 35 km west of the Marmul oil field. The feature is the only one of its kind in the area. The basinal structure is probably of Late Cretaceous (Albian) age and the regional geology strongly suggests that it is neither a volcanic crater nor related to salt-dome tectonics or salt dissolution. It possibly represents a crater formed by a terrestrial impact event and has been named the Murshid crater. This report does not constitute a detailed investigation of the possible impact crater but rather records the 3-D seismic observations and the drilling that has taken place near the structure so far. INTRODUCTION During interpretation of a newly acquired 3-D seismic survey for oil exploration in southern Oman, a solitary 2.5-km-diameter circular basinal feature was identified as a possible impact structure and was named the Murshid crater. It lies 35 km west of the Marmul oil field in the South Oman Salt Basin (Figure 1). The center of the structure is at latitude 18º10’59"N, longitude 54º55’08”E, and it is buried at a depth of approximately 380 m below mean sea level (680 m below the ground surface). The authors are petroleum geologists who felt that the Murshid basinal structure needed reporting to the wider scientific community. -
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. -
March 21–25, 2016
FORTY-SEVENTH LUNAR AND PLANETARY SCIENCE CONFERENCE PROGRAM OF TECHNICAL SESSIONS MARCH 21–25, 2016 The Woodlands Waterway Marriott Hotel and Convention Center The Woodlands, Texas INSTITUTIONAL SUPPORT Universities Space Research Association Lunar and Planetary Institute National Aeronautics and Space Administration CONFERENCE CO-CHAIRS Stephen Mackwell, Lunar and Planetary Institute Eileen Stansbery, NASA Johnson Space Center PROGRAM COMMITTEE CHAIRS David Draper, NASA Johnson Space Center Walter Kiefer, Lunar and Planetary Institute PROGRAM COMMITTEE P. Doug Archer, NASA Johnson Space Center Nicolas LeCorvec, Lunar and Planetary Institute Katherine Bermingham, University of Maryland Yo Matsubara, Smithsonian Institute Janice Bishop, SETI and NASA Ames Research Center Francis McCubbin, NASA Johnson Space Center Jeremy Boyce, University of California, Los Angeles Andrew Needham, Carnegie Institution of Washington Lisa Danielson, NASA Johnson Space Center Lan-Anh Nguyen, NASA Johnson Space Center Deepak Dhingra, University of Idaho Paul Niles, NASA Johnson Space Center Stephen Elardo, Carnegie Institution of Washington Dorothy Oehler, NASA Johnson Space Center Marc Fries, NASA Johnson Space Center D. Alex Patthoff, Jet Propulsion Laboratory Cyrena Goodrich, Lunar and Planetary Institute Elizabeth Rampe, Aerodyne Industries, Jacobs JETS at John Gruener, NASA Johnson Space Center NASA Johnson Space Center Justin Hagerty, U.S. Geological Survey Carol Raymond, Jet Propulsion Laboratory Lindsay Hays, Jet Propulsion Laboratory Paul Schenk, -
A Study About the Temporal Constraints on the Martian Yardangs’ Development in Medusae Fossae Formation
remote sensing Article A Study about the Temporal Constraints on the Martian Yardangs’ Development in Medusae Fossae Formation Jia Liu 1,2 , Zongyu Yue 1,3,*, Kaichang Di 1,3 , Sheng Gou 1,4 and Shengli Niu 4 1 State Key Laboratory of Remote Sensing Science, Aerospace Information Research Institute, Chinese Academy of Sciences, Beijing 100101, China; [email protected] (J.L.); [email protected] (K.D.); [email protected] (S.G.) 2 University of Chinese Academy of Sciences, Beijing 100049, China 3 CAS Center for Excellence in Comparative Planetology, Hefei 230026, China 4 State Key Laboratory of Lunar and Planetary Sciences, Macau University of Science and Technology, Macau 999078, China; [email protected] * Correspondence: [email protected]; Tel.: +86-10-64889553 Abstract: The age of Mars yardangs is significant in studying their development and the evolution of paleoclimate conditions. For planetary surface or landforms, a common method for dating is based on the frequency and size distribution of all the superposed craters after they are formed. However, there is usually a long duration for the yardangs’ formation, and they will alter the superposed craters, making it impossible to give a reliable dating result with the method. An indirect method by analyzing the ages of the superposed layered ejecta was devised in the research. First, the layered ejecta that are superposed on and not altered by the yardangs are identified and mapped. Then, the ages of the layered ejecta are derived according to the crater frequency and size distribution on them. These ages indicate that the yardangs ceased development by these times, and the ages are valuable for studying the evolution of the yardangs. -
Pre-Mission Insights on the Interior of Mars Suzanne E
Pre-mission InSights on the Interior of Mars Suzanne E. Smrekar, Philippe Lognonné, Tilman Spohn, W. Bruce Banerdt, Doris Breuer, Ulrich Christensen, Véronique Dehant, Mélanie Drilleau, William Folkner, Nobuaki Fuji, et al. To cite this version: Suzanne E. Smrekar, Philippe Lognonné, Tilman Spohn, W. Bruce Banerdt, Doris Breuer, et al.. Pre-mission InSights on the Interior of Mars. Space Science Reviews, Springer Verlag, 2019, 215 (1), pp.1-72. 10.1007/s11214-018-0563-9. hal-01990798 HAL Id: hal-01990798 https://hal.archives-ouvertes.fr/hal-01990798 Submitted on 23 Jan 2019 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Open Archive Toulouse Archive Ouverte (OATAO ) OATAO is an open access repository that collects the wor of some Toulouse researchers and ma es it freely available over the web where possible. This is an author's version published in: https://oatao.univ-toulouse.fr/21690 Official URL : https://doi.org/10.1007/s11214-018-0563-9 To cite this version : Smrekar, Suzanne E. and Lognonné, Philippe and Spohn, Tilman ,... [et al.]. Pre-mission InSights on the Interior of Mars. (2019) Space Science Reviews, 215 (1). -
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). -
Restoration in Action
“I am honored to have helped to create the Forest Service Legacy Roads and Trails Program. I have watched the work across the nation, especially in the Skokomish Valley in the Sixth Congressional District. This work has helped restore watersheds and improve water quality and !sh habitat, and at the same time provided jobs that are desperately needed in our rural communities. This is a great program and one that I am proud to have sponsored. A lot more restoration work is needed, so I hope this program will continue to help the Forest Service get the job done.” — The Honorable Norm Dicks U.S. Representative for Washington’s 6th Congressional District, 1977 – 2012 We thank USDA Forest Service staff for their assistance in providing data and images, and Marlies Wierenga, Dave Heller, and Dan Funsch for their dedication, long hours, and hard work. Cover photo credits: Recontoured road on the Gallatin National Forest, MT, credit: Wildlands CPR; fisherperson, photo credit: Kent Miller. he Legacy Roads and Trails Remediation Program T(Legacy Roads and Trails) is a cornerstone of watershed restoration in our National Forests. Created to !x environmental problems resulting from the Forest Service’s extensive road and trail system, Legacy Roads and Trails has reduced stream pollution, restored !sh and wildlife habitat, created jobs, and improved essential roads to ensure safe access. Legacy Roads and Trails has been a success from the start; it is smartly and e"ciently managed, and achieves on-the-ground results in real time. Since its inception in 2008, Congress has appropriated $270 million to Legacy Roads and Trails. -
Nicholas Murray BUTLER Arranged Correspondence Box Contents Box
Nicholas Murray BUTLER Arranged Correspondence Box contents Box# Box contents 1 Catalogued correspondence 2 A-AB 3 AC - ADAMS, J. 4 ADAMS, K.-AG 5 AH-AI 6 AJ-ALD 7 ALE-ALLEN, E. 8 ALLEN, F.-ALLEN, W. 9 ALLEN, Y. - AMERICAN AC. 10 AMERICAN AR. - AMERICAN K. 11 AMERICAN L.-AMZ 12 ANA-ANG 13 ANH-APZ 14 AR-ARZ 15 AS-AT 16 AU-AZ 17 B-BAC 18 BAD-BAKER, G. 19 BAKER, H. - BALDWIN 20 BALE-BANG 21 BANH-BARD 22 BARD-BARNES, J. 23 BARNES, N.-BARO 24 BARR-BARS 25 BART-BAT 26 BAU-BEAM 27 BEAN-BED 28 BEE-BELL, D. 29 BELL,E.-BENED 30 BENEF-BENZ 31 BER-BERN 32 BERN-BETT 33 BETTS-BIK 34 BIL-BIR 35 BIS-BLACK, J. 36 BLACK, K.-BLAN 37 BLANK-BLOOD 38 BLOOM-BLOS 39 BLOU-BOD 40 BOE-BOL 41 BON-BOOK 42 BOOK-BOOT 43 BOR-BOT 44 BOU-BOWEN 45 BOWER-BOYD 46 BOYER-BRAL 47 BRAM-BREG 48 BREH-BRIC 49 BRID - BRIT 50 BRIT-BRO 51 BROG-BROOKS 52 BROOKS-BROWN 53 BROWN 54 BROWN-BROWNE 55 BROWNE -BRYA 56 BRYC - BUD 57 BUE-BURD 58 BURE-BURL 59 BURL-BURR 60 BURS-BUTC 61 BUTLER, A. - S. 62 BUTLER, W.-BYZ 63 C-CAI 64 CAL-CAMPA 65 CAMP - CANFIELD, JAMES H. (-1904) 66 CANFIELD, JAMES H. (1905-1910) - CANT 67 CAP-CARNA 68 CARNEGIE (1) 69 CARNEGIE (2) ENDOWMENT 70 CARN-CARR 71 CAR-CASTLE 72 CAT-CATH 73 CATL-CE 74 CH-CHAMB 75 CHAMC - CHAP 76 CHAR-CHEP 77 CHER-CHILD, K. -
5648 Village of Warsaw Vlge SWIS Code - 564801
NYS - Real Property System Cross Reference Report - 2021 - Current Year File RPS345/V04/L001 County of Wyoming Parcel Address Sequence Town of Warsaw - 5648 Village of Warsaw Vlge SWIS Code - 564801 Location School Res Pr O R T Parcel Id Name Nbr Name Dist Land Av Total Av Pct Cl C S S C 648.1-9999-131.600/1004 NYS Electric & Gas Corp 564801 0309831 0 882 6 648.1-9999-131.600/1014 NYS Electric & Gas Corp 564801 062572 0 882 6 85.16-1-8 Town Of Warsaw Allen St 564801 61006100 0 653 8 A 85.12-1-30.1 Buzz & Val Properties Inc Allen St 564801 2560028100 0 449 1 A 85.12-1-37 Gott, Donald James Estate. Allen St 564801 1440014400 0 340 1 A 85.12-1-27 Williams, Richard A. 6 Allen St 564801 960034000 0 210 1 A 85.12-2-50 Purdy, Larry L. 21 Allen St 564801 870075000 0 210 1 A 85.12-2-49 Mayer, Cory 25 Allen St 564801 1240055300 0 210 1 A 85.12-2-48 Schneider, Daryl A. 29 Allen St 564801 1710051700 0 210 1 A 85.12-2-47 Skidmore, Benjamine J. 37 Allen St 564801 1320055600 0 210 1 A 85.12-2-46 Vickers, II, Kevin M. 41 Allen St 564801 1240060700 0 220 1 A 85.12-2-45 Hampton, Charlotte 45 Allen St 564801 1240060600 0 210 1 A 85.12-2-44 Bernard, Marjorie A. 49 Allen St 564801 1160049500 50 210 1 A 85.12-3-20 Berkemeier, Jeremy B. -
Edited by Thomas W. Henry and Bruce R. Wardlaw U.S. Geological
UNITED STATES DEPARTMENT OF THE INTERIOR GEOLOGICAL SURVEY Pacific Enewetak Atoll Crater Exploration (PEACE) Program Enewetak Atoll, Republic of the Marshall Islands Part 3: Stratigraphic analysis and other geologic and geophysical studies in vicinity of OAK and KOA craters edited by Thomas W. Henry and Bruce R. Wardlaw U.S. Geological Survey Open File Report 86-555 Prepared in cooperation with the Defense Nuclear Agency This report is preliminary and has not been reviewed for conformity with U.S. Geological Survey editorial standards and stratigraphic nomenclature. 1987 CLAY A sedimentologic term for a rock or mineral fragment or a detrital particle of any composition smaller than a very fine silt grain, having a diameter less than 1/256 mm (4 microns, or 0.00026 in., or 8 phi units). COBBLE A sedimentologic term for a rock fragment or detrital particle larger than a pebble and smaller than a boulder, having a diameter in the range of 64 to 256 mm (2.5 to 10 in., or -6 to -8 phi units). CONSOLIDATION Gradual or slow reduction in volume and increase in density of a material mass in response to increased loads or compressive stress; e.g., the adjustment of a saturated material involving the squeezing of water from pore spaces. COMPACTION Any process by which a material mass loses pore space and achieves a higher density, thereby increasing the bearing capacity, reducing the tendency to settle or deform under load, and increasing the general stability of the material mass (soil). CRATER A typically bowl-shaped or saucer-shaped pit or depression, generally of considerable size and with steep inner slopes, formed on a terrestrial or planetary surface or in the ground by the explosive release of chemical or kinetic energy; e.g., an impact crater or an explosion crater. -
Arxiv:0706.3947V1
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 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 still controversial. Nonetheless, a review of TLP data shows regularities in the observations; a key question is whether this structure is imposed by human observer effects, terrestrial atmospheric effects or processes tied to the lunar surface. I interrogate an extensive catalog of TLPs to determine if human factors play a determining role in setting the distribution of TLP reports. We divide the sample according to variables which should produce varying results if the determining factors involve humans e.g., historical epoch or geographical location of the observer, and not reflecting phenomena tied to the lunar surface. Specifically, we bin the reports into selenographic areas (300 km on a side), then construct a robust average count for such “pixels” in a way discarding discrepant counts. Regardless of how we split the sample, the results are very similar: roughly 50% of the report count originate from the crater Aristarchus and vicinity, 16% from Plato, 6% from recent, major impacts (Copernicus, ∼ ∼ Kepler and Tycho - beyond Aristarchus), plus a few at Grimaldi. Mare Crisium produces a robust signal for three of five averages of up to 7% of the reports (however, Crisium subtends more than one pixel). The consistency in TLP report counts for specific features on this list indicate that 80% of the reports arXiv:0706.3947v1 [astro-ph] 27 Jun 2007 ∼ are consistent with being real (perhaps with the exception of Crisium). -
Wilderness Air Quality Value Plan for the Shoshone National Forest
Wilderness Air Quality Value Plan Shoshone National Forest Clocktower Creek and Wapiti Ridge, Washakie Wilderness Prepared by: /s/ Greg Bevenger __________________________________ Greg Bevenger, Air Program Manager Recommended by: /s/ Bryan Armel ______________________________________________ Bryan Armel, Resources Staff Officer Recommended by: /s/ Loren Poppert ______________________________________________ Loren Poppert, Recreation Staff Officer Approved by: /s/ Rebecca Aus ______________________________________________ Rebecca Aus, Forest Supervisor May 2010 Wilderness Air Quality Value Plan Introduction Background As part of the USDA Forest Service effort to better understand and monitor wilderness areas, the agency has adopted the 10-Year Wilderness Stewardship Challenge (Forest Service 2005). The 10-Year Wilderness Stewardship Challenge was developed by the Chief’s Wilderness Advisory Group (WAG) as a quantifiable measurement of the Forest Service’s success in wilderness stewardship. The goal identified by the Wilderness Advisory Group, and endorsed by the Chief, is to bring each wilderness under Forest Service management to a minimum stewardship level by the year 2014, the fiftieth anniversary of the Wilderness Act. The Challenge was initiated in fiscal year 2005. The Challenge contains ten items that highlight elements of wilderness stewardship. These elements are 1) the natural role of fire, 2) invasive plants, 3) air quality, 4) education, 5) protection of recreational opportunities, 6) recreational site inventory, 7) outfitters