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Regional Structural Setting of Yucca Mountain, Southwestern Nevada
) i WM RECORD COPY I: // lt- USGS-OFR-84-854 - USGS-OFR-84-854 UNITED STATES DEPARTMENT OF THE INTERIOR GEOLOGICAL SURVEY REGIONAL STRUCTURAL SETTING OF YUCCA MOUNTAIN, SOUTHWESTERN NEVADA, AND LATE CENOZOIC RATES OF TECTONIC ACTIVITY IN PART OF THE SOUTHWESTERN GREAT BASIN, NEVADA AND CALIFORNIA by U. J. Carr 06 : . , CD CD. Open-File Report 84-854 Prepared in cooperation with the Nevada Operations Office U.S. Department of Energy (Interagency Agreement DE-AI08-78ET44802) This report is preliminary and has not been reviewed for-conformity with U.S. Geological Survey editorial standards and stratigraphic nomenclature. Company names are for descriptive purposes only and do not constitute endorsement by the U.S. Geological Survey. Denver, Colorado 1984 ~~- ~ - ~~ ___~~~ Copies of this Open-File Report may be purchased from Open-File Services Secton Branch of Distribution U.S. Geological Survey Box 25425, Federal Center Denver, Colorado 80225 PREPAYMENT IS REQUIRED Price information will be published in the monthly listing 'New Publications of the Geological Survey" FOR ADDITIONAL ORDERING INFORMATION CALL: Commercial: (303) 236-7476 FTS: 776-7476 USGS-OFR-84-854 USGS-OFR-84-854 UNITED STATES DEPARTMENT OF THE INTERIOR GEOLOGICAL SURVEY Denver, Colorado REGIONAL STRUCTURAL SETTING OF YUCCA MOUNTAIN, SOUTHWESTERN NEVADA, AND LATE CENOZOIC RATES OF TECTONIC ACTIVITY IN PART OF THE SOUTHWESTERN GREAT BASIN, NEVADA AND CALIFORNIA by W. J. Carr CONTENTS Page Abstract................................................................... 1 Introduction.................................................................................................. 4 Structural-physiographic subsections of the southwestern Great Basin ....... 9 Walker Lane belt ........................................ ...... ** 9 Basin-range subsection ..................................................21 Inyo-Mono subsection ............................................................26 Boundary between Inyo-Mono and Walker Lane belt subsections ...... -
Lurking in the Shadows: Wide-Separation Gas Giants As Tracers of Planet Formation
Lurking in the Shadows: Wide-Separation Gas Giants as Tracers of Planet Formation Thesis by Marta Levesque Bryan In Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy CALIFORNIA INSTITUTE OF TECHNOLOGY Pasadena, California 2018 Defended May 1, 2018 ii © 2018 Marta Levesque Bryan ORCID: [0000-0002-6076-5967] All rights reserved iii ACKNOWLEDGEMENTS First and foremost I would like to thank Heather Knutson, who I had the great privilege of working with as my thesis advisor. Her encouragement, guidance, and perspective helped me navigate many a challenging problem, and my conversations with her were a consistent source of positivity and learning throughout my time at Caltech. I leave graduate school a better scientist and person for having her as a role model. Heather fostered a wonderfully positive and supportive environment for her students, giving us the space to explore and grow - I could not have asked for a better advisor or research experience. I would also like to thank Konstantin Batygin for enthusiastic and illuminating discussions that always left me more excited to explore the result at hand. Thank you as well to Dimitri Mawet for providing both expertise and contagious optimism for some of my latest direct imaging endeavors. Thank you to the rest of my thesis committee, namely Geoff Blake, Evan Kirby, and Chuck Steidel for their support, helpful conversations, and insightful questions. I am grateful to have had the opportunity to collaborate with Brendan Bowler. His talk at Caltech my second year of graduate school introduced me to an unexpected population of massive wide-separation planetary-mass companions, and lead to a long-running collaboration from which several of my thesis projects were born. -
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. -
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. -
Petrogenes1.S of Apollo 11 Basalts and Implications
PETROGENES1.S OF APOLLO 11 BASALTS AND IMPLICATIONS FOR LUNAR ORIGIN A, E. Rinqwood Department of Geophysics and Geochemistry Australian National University Canberra ABSTRACT The origin of Apollo 11 basalts is discussed in terms of two hypotheses: (i) formation by a small degree of partial melting in the lunar interior and (ii) formation by prolonged near-surface crystallization differentiation in a lava lake. The second hypoth- esis is rejected on the following grounds: Most Apollo 11 magmas are far removed from the plagioclase-pyroxene-ilmenite cotectic; fractional crystallization cannot explain the large variations in concentrations of incompatible trace elehents in conjunction with the small variations in major element compositions, particularly, _IMg ratios; experimentally determined partition coefficients show Fe Pack3 that the high abundances of Cr and V in Apollo 11 cannot be reconciled A with the previous separation of large quantities of ore minerals and pyroxenes. On the other hand, the major element and trace element jq contents of Apollo 11 rocks can be explained by partial melting of sovvromaterial which buffers the major element compositions and causes enrichments of incompatible elements according to the degree of partial melting( fiisk hypbthesis) Two alternative sources have been suggested for Apollo 11 basalts formed by partial melting: (i) unfractionated pyroxenite source region at depths of 200-600 km, (ii) fractionated source region with incompatible elements (e-g. Ba, U, rare 'earths) strongly enriched over chondritic abundances and containing plagioclase (approximate eucritic composition). Mass balance calculations'and plagioclase stability conditions show that the second hypothesis requires Apollo 1l.basalts to be generated by partial melting in the outer 150 km of the moon. -
Alpha ELT Listing
Lienholder Name Lienholder Address City State Zip ELT ID 1ST ADVANTAGE FCU PO BX 2116 NEWPORT NEWS VA 23609 CFW 1ST COMMAND BK PO BX 901041 FORT WORTH TX 76101 FXQ 1ST FNCL BK USA 47 SHERMAN HILL RD WOODBURY CT 06798 GVY 1ST LIBERTY FCU PO BX 5002 GREAT FALLS MT 59403 ESY 1ST NORTHERN CA CU 1111 PINE ST MARTINEZ CA 94553 EUZ 1ST NORTHERN CR U 230 W MONROE ST STE 2850 CHICAGO IL 60606 GVK 1ST RESOURCE CU 47 W OXMOOR RD BIRMINGHAM AL 35209 DYW 1ST SECURITY BK WA PO BX 97000 LYNNWOOD WA 98046 FTK 1ST UNITED SVCS CU 5901 GIBRALTAR DR PLEASANTON CA 94588 W95 1ST VALLEY CU 401 W SECOND ST SN BERNRDNO CA 92401 K31 360 EQUIP FIN LLC 300 BEARDSLEY LN STE D201 AUSTIN TX 78746 DJH 360 FCU PO BX 273 WINDSOR LOCKS CT 06096 DBG 4FRONT CU PO BX 795 TRAVERSE CITY MI 49685 FBU 777 EQUIPMENT FIN LLC 600 BRICKELL AVE FL 19 MIAMI FL 33131 FYD A C AUTOPAY PO BX 40409 DENVER CO 80204 CWX A L FNCL CORP PO BX 11907 SANTA ANA CA 92711 J68 A L FNCL CORP PO BX 51466 ONTARIO CA 91761 J90 A L FNCL CORP PO BX 255128 SACRAMENTO CA 95865 J93 A L FNCL CORP PO BX 28248 FRESNO CA 93729 J95 A PLUS FCU PO BX 14867 AUSTIN TX 78761 AYV A PLUS LOANS 500 3RD ST W SACRAMENTO CA 95605 GCC A/M FNCL PO BX 1474 CLOVIS CA 93613 A94 AAA FCU PO BX 3788 SOUTH BEND IN 46619 CSM AAC CU 177 WILSON AVE NW GRAND RAPIDS MI 49534 GET AAFCU PO BX 619001 MD2100 DFW AIRPORT TX 75261 A90 ABLE INC 503 COLORADO ST AUSTIN TX 78701 CVD ABNB FCU 830 GREENBRIER CIR CHESAPEAKE VA 23320 CXE ABOUND FCU PO BX 900 RADCLIFF KY 40159 GKB ACADEMY BANK NA PO BX 26458 KANSAS CITY MO 64196 ATF ACCENTRA CU 400 4TH -
A Basic Requirement for Studying the Heavens Is Determining Where In
Abasic requirement for studying the heavens is determining where in the sky things are. To specify sky positions, astronomers have developed several coordinate systems. Each uses a coordinate grid projected on to the celestial sphere, in analogy to the geographic coordinate system used on the surface of the Earth. The coordinate systems differ only in their choice of the fundamental plane, which divides the sky into two equal hemispheres along a great circle (the fundamental plane of the geographic system is the Earth's equator) . Each coordinate system is named for its choice of fundamental plane. The equatorial coordinate system is probably the most widely used celestial coordinate system. It is also the one most closely related to the geographic coordinate system, because they use the same fun damental plane and the same poles. The projection of the Earth's equator onto the celestial sphere is called the celestial equator. Similarly, projecting the geographic poles on to the celest ial sphere defines the north and south celestial poles. However, there is an important difference between the equatorial and geographic coordinate systems: the geographic system is fixed to the Earth; it rotates as the Earth does . The equatorial system is fixed to the stars, so it appears to rotate across the sky with the stars, but of course it's really the Earth rotating under the fixed sky. The latitudinal (latitude-like) angle of the equatorial system is called declination (Dec for short) . It measures the angle of an object above or below the celestial equator. The longitud inal angle is called the right ascension (RA for short). -
Virgo the Virgin
Virgo the Virgin Virgo is one of the constellations of the zodiac, the group tion Virgo itself. There is also the connection here with of 12 constellations that lies on the ecliptic plane defined “The Scales of Justice” and the sign Libra which lies next by the planets orbital orientation around the Sun. Virgo is to Virgo in the Zodiac. The study of astronomy had a one of the original 48 constellations charted by Ptolemy. practical “time keeping” aspect in the cultures of ancient It is the largest constellation of the Zodiac and the sec- history and as the stars of Virgo appeared before sunrise ond - largest constellation after Hydra. Virgo is bordered by late in the northern summer, many cultures linked this the constellations of Bootes, Coma Berenices, Leo, Crater, asterism with crops, harvest and fecundity. Corvus, Hydra, Libra and Serpens Caput. The constella- tion of Virgo is highly populated with galaxies and there Virgo is usually depicted with angel - like wings, with an are several galaxy clusters located within its boundaries, ear of wheat in her left hand, marked by the bright star each of which is home to hundreds or even thousands of Spica, which is Latin for “ear of grain”, and a tall blade of galaxies. The accepted abbreviation when enumerating grass, or a palm frond, in her right hand. Spica will be objects within the constellation is Vir, the genitive form is important for us in navigating Virgo in the modern night Virginis and meteor showers that appear to originate from sky. Spica was most likely the star that helped the Greek Virgo are called Virginids. -
The Multidimensional Guide to Science Fiction and Fantasy of the Twentieth Century, Volume 1
THE MULTIDIMENSIONAL GUIDE TO SCIENCE FICTION AND FANTASY OF THE TWENTIETH CENTURY, VOLUME 1 EDITED BY NAT TILANDER 2 Copyright © 2010 by Nathaniel Garret Tilander All rights reserved. No part of this book may be reproduced, stored, or transmitted by any means—whether auditory, graphic, mechanical, or electronic—without written permission of both publisher and author, except in the case of brief excerpts used in critical articles and reviews. Unauthorized reproduction of any part of this work is illegal and is punishable by law. Cover art from the novella Last Enemy by H. Beam Piper, first published in the August 1950 issue of Astounding Science Fiction, and illustrated by Miller. Image downloaded from the ―zorger.com‖ website which states that the image is licensed under a Creative Commons Public Domain License. Additional copyrighted materials incorporated in this book are as follows: Copyright © 1949-1951 by L. Sprague de Camp. These articles originally appeared in Analog Science Fiction. Copyright © 1951-1979 by P. Schuyler Miller. These articles originally appeared in Analog Science Fiction. Copyright © 1975-1979 by Lester Del Rey. These articles originally appeared in Analog Science Fiction. Copyright © 1978-1981 by Spider Robinson. These articles originally appeared in Analog Science Fiction. Copyright © 1979-1999 by Tom Easton. These articles originally appeared in Analog Science Fiction. Copyright © 1950-1954 by J. Francis McComas. These articles originally appeared in Fantasy and Science Fiction. Copyright © 1950-1959 by Anthony Boucher. These articles originally appeared in Fantasy and Science Fiction. Copyright © 1959-1960 by Damon Knight. These articles originally appeared in Fantasy and Science Fiction. -
NINETY-NINE 9\Je\Ns
NINETY-NINE THE INTERNATIONAL WOMEN PILOT S MAGAZINE J _________ November-December,N 1993 • Crater Lake Flyers • !Ange(s — Corporate Angel Network • Becoming a “FED” Successful Board Meeting Reflects Fresh Outlook Just ask the Governors who were present; they didn’t pick up their knitting once - well, maybe once! The fall Board agenda was packed with items for discussion and action. On pages 10, 11 and 15 of this issue you’ll find detailed reports covering many of the items we evaluated, discussed, voted on, remanded for additional President’s Message information or to a committee, etc. We selected a new N e w s editor, Betty Rowley, and extended our thanks to Ann Cooper for her wonderful effort as editor. We discussed an informal proposal made by a member of the Atchison Historical Society Board that The 99s consider deeding 60 percent ownership of the Amelia Earhart Birthplace Museum to the Historical Society. In exchange, an undefined amount of funding for restoration would be made available. The Board unanimously decided they needed considerably more information Board members Alexis Koehler, Connie Woods, Joyce Wells, Gene Nora Jessen, Doris before an accurate assessment of this Abbate, Lee Orr, Carolyn Carpp, Lu Hollander and Lois Erickson pause during a full early-stage proposal could be fairly Board meeting schedule to look at one of the many early-day scrapbooks housed at 99s' International Headquarters. evaluated and acted upon. This addi tional information has been requested from the 99s’ Birthplace Museum Board, and will be available for further consideration prior to the spring Board meeting. -
The Observer, November
The OBSERVER The Newsletter of the Twin City Amateur Astronomers, Inc. November 2001 Volume 26, Number 11 Adventures in Meteor Hunting — Duane Yockey In This Issue: REETINGS to my brother and and binoculars just in case the meteors sister sky watchers, didn't live up to their billing. Saturday G was clear here in central Illinois, and • Meteor Hunting Adventures ...1 when I got back from a Duane shows that he has the The long awaited day play at Illinois State right stuff as he tears after the of the Leonid meteor University around Leonids and finds them! shower arrived Satur- 10:30 p.m. the sky was day. I was really still showing lots of • TCAA Calendar ........................1 looking forward to stars. I called Laura Use our calendar to mark going out to the (my oldest daughter), your calendar. observatory with who said the skies were other Twin City clear down in southern • TCAA Annual Holiday Bash....3 Amateur Indiana and I could Party like it’s, um, 2001, at Astronomers and see- drive down there, if the Vic & Cindy’s! ............................ ing the "show" from clouds rolled in (ha, 2:00 a.m. to 6:00 a.m. ha). I assured her that • Club Notes................................4 early Sunday morn- the sky would cooper- Wow, it’s been a busy month! ing. So I packed my ate, and it was looking car early with a lawn good then, and I wished • Software Review: DSE ...........5 chair and threw in my her good luck (if she And just think, if you never telescope, star charts turn to page 5, you’ll never know continued on next page what DSE stands for.. -
The Moon Greets the Planets in the November Dawn 4 November 2015, by David Dickinson
The moon greets the planets in the November dawn 4 November 2015, by David Dickinson Watch the scene shift, as the moon joins the dance this weekend. The mornings of Friday, October 6th and Saturday, October 7th are key, as the moon passes just two degrees from the Jupiter and Mars pair and just over one degree from Venus worldwide. Similar close pairings of the moon and Venus adorn many national flags, possibly inspired by a close grouping of Venus and the moon witnessed by skywatchers of yore. Saturday November 7th is also a fine time to try your hand at seeing Venus in the daytime, using the nearby crescent moon as a guide. The moon will be only four days from New, and the pair will be 46 degrees west of the sun, an optimal situation as A tri-planetary grouping from the morning of October Venus just passed greatest western elongation 31st. Credit: Joseph Brimacombe 46.4 degrees west of the sun on October 26th. So did this past weekend's shift back to Standard Time for most of North America throw you for a loop? Coming the day after Halloween, 2015 was the earliest we can now shift back off Daylight Saving Time. Sunday won't fall on November 1st again until 2020. Expect evenings get darker sooner for northern hemisphere residents, while the planetary action remains in the dawn sky. Though Mercury has exited the morning twilight stage, the planets Jupiter, Venus and Mars continue to put on a fine show, joined by the waning crescent moon later this week.