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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. -
Toxicology in Antiquity
TOXICOLOGY IN ANTIQUITY Other published books in the History of Toxicology and Environmental Health series Wexler, History of Toxicology and Environmental Health: Toxicology in Antiquity, Volume I, May 2014, 978-0-12-800045-8 Wexler, History of Toxicology and Environmental Health: Toxicology in Antiquity, Volume II, September 2014, 978-0-12-801506-3 Wexler, Toxicology in the Middle Ages and Renaissance, March 2017, 978-0-12-809554-6 Bobst, History of Risk Assessment in Toxicology, October 2017, 978-0-12-809532-4 Balls, et al., The History of Alternative Test Methods in Toxicology, October 2018, 978-0-12-813697-3 TOXICOLOGY IN ANTIQUITY SECOND EDITION Edited by PHILIP WEXLER Retired, National Library of Medicine’s (NLM) Toxicology and Environmental Health Information Program, Bethesda, MD, USA Academic Press is an imprint of Elsevier 125 London Wall, London EC2Y 5AS, United Kingdom 525 B Street, Suite 1650, San Diego, CA 92101, United States 50 Hampshire Street, 5th Floor, Cambridge, MA 02139, United States The Boulevard, Langford Lane, Kidlington, Oxford OX5 1GB, United Kingdom Copyright r 2019 Elsevier Inc. All rights reserved. No part of this publication may be reproduced or transmitted in any form or by any means, electronic or mechanical, including photocopying, recording, or any information storage and retrieval system, without permission in writing from the publisher. Details on how to seek permission, further information about the Publisher’s permissions policies and our arrangements with organizations such as the Copyright Clearance Center and the Copyright Licensing Agency, can be found at our website: www.elsevier.com/permissions. This book and the individual contributions contained in it are protected under copyright by the Publisher (other than as may be noted herein). -
Δ13c of Aromatic Compounds in Sediments, Oils And
1 δ13C of aromatic compounds in sediments, oils and 2 atmospheric emissions: a review 3 Alex I. Holman a, Kliti Grice a* 4 5 a Western Australia Organic and Isotope Geochemistry Centre, The Institute for 6 Geoscience Research, School of Earth and Planetary Sciences, Curtin University, 7 GPO Box U1987, Perth, WA 6845, Australia 8 9 * Corresponding author 10 Alex Holman: Tel.: +61(0) 8 9266 9723. E-mail address: [email protected] 11 Kliti Grice: Tel.: +61(0) 8 9266 2474. E-mail address: [email protected] 12 13 14 15 16 17 18 19 Abstract 20 This review discusses major applications of stable carbon isotopic 21 measurements of aromatic compounds, along with some specific technical aspects 22 including purification of aromatic fractions for baseline separation. δ13C 23 measurements of organic matter (OM) in sediments and oils are routine in all 24 fields of organic geochemistry, but they are predominantly done on saturated 25 compounds. Aromatic compounds are important contributors to sedimentary 26 organic matter, and provide indication of diagenetic processes, OM source, and 27 thermal maturity. Studies have found evidence for a small 13C-enrichment during 28 diagenetic aromatisation of approximately 1 to 2 ‰, but the formation of polycyclic 29 aromatic hydrocarbons (PAHs) from combustion and hydrothermal processes 30 seems to produce no effect. Likewise, maturation and biodegradation also produce 31 only small isotopic effects. An early application of δ13C of aromatic compounds was 32 in the classification of oil families by source. Bulk measurements have had some 33 success in differentiating marine and terrigenous oils, but were not accurate in all 34 settings. -
Featured: Simon Brassell 9/18/2020 PRE-SCRIPT in the Fourth Episode
Featured: Simon Brassell 9/18/2020 PRE-SCRIPT In the fourth episode of BIOmarkers, the audio series that archives the oral history of organic geochemistry, we speak with Dr. Simon Brassell, Professor of Geological Sciences, Biogeochemistry, and Molecular Organic Geochemistry at the Department of Earth and Atmospheric Sciences at Indiana University Bloomington. In his interview, Simon discusses his time at the University of Bristol, proxies, and what piques his interest today. SCRIPT Fatima Husain: Welcome to BIOmarkers, an audio series that archives the oral history of organic geochemistry. I’m your host, Fatima Husain, and I’m here today with my series co-creators and fellow organic geochemists Angel Mojarro and Juliana Drozd. Angel Mojarro: For today’s episode, we spoke with Dr. Simon Brassell. Simon Brassell: I'm Simon Brassell, I'm a professor of Earth and Planetary Sciences at Indiana University. When anyone asked me what I am, I would say I'm a molecular organic geochemistry and molecular bio bio geochemist, because my area of expertise started in looking at biomarkers, and I have pretty much stayed in that area all along. Juliana Drozd: We spoke with Simon briefly in between sessions at the 2019 International Meeting on Organic Geochemistry about his career pathway and insights into the field. Fatima Husain: It turns out, this isn’t too hard to do: Simon Brassell: This is about something like the 14th, 15th time I've come to IMOG and every year there are two, two. There's one meeting each year that I always try and get to and it's the IMOG and then even years, it's the Gordon research conference on organic chemistry because I learn more at those meetings about the specifics of the subject than I do at any other bigger or meetings that aren't a less focused on organic geochemistry, and it's always great to come back and see people who I've known some for 10 years, some for 20 years, some 30 years, some 40 years. -
Glossary of Lunar Terminology
Glossary of Lunar Terminology albedo A measure of the reflectivity of the Moon's gabbro A coarse crystalline rock, often found in the visible surface. The Moon's albedo averages 0.07, which lunar highlands, containing plagioclase and pyroxene. means that its surface reflects, on average, 7% of the Anorthositic gabbros contain 65-78% calcium feldspar. light falling on it. gardening The process by which the Moon's surface is anorthosite A coarse-grained rock, largely composed of mixed with deeper layers, mainly as a result of meteor calcium feldspar, common on the Moon. itic bombardment. basalt A type of fine-grained volcanic rock containing ghost crater (ruined crater) The faint outline that remains the minerals pyroxene and plagioclase (calcium of a lunar crater that has been largely erased by some feldspar). Mare basalts are rich in iron and titanium, later action, usually lava flooding. while highland basalts are high in aluminum. glacis A gently sloping bank; an old term for the outer breccia A rock composed of a matrix oflarger, angular slope of a crater's walls. stony fragments and a finer, binding component. graben A sunken area between faults. caldera A type of volcanic crater formed primarily by a highlands The Moon's lighter-colored regions, which sinking of its floor rather than by the ejection of lava. are higher than their surroundings and thus not central peak A mountainous landform at or near the covered by dark lavas. Most highland features are the center of certain lunar craters, possibly formed by an rims or central peaks of impact sites. -
This Article Was Published in an Elsevier Journal. the Attached Copy
This article was published in an Elsevier journal. The attached copy is furnished to the author for non-commercial research and education use, including for instruction at the author’s institution, sharing with colleagues and providing to institution administration. Other uses, including reproduction and distribution, or selling or licensing copies, or posting to personal, institutional or third party websites are prohibited. In most cases authors are permitted to post their version of the article (e.g. in Word or Tex form) to their personal website or institutional repository. Authors requiring further information regarding Elsevier’s archiving and manuscript policies are encouraged to visit: http://www.elsevier.com/copyright Author's personal copy Available online at www.sciencedirect.com Geochimica et Cosmochimica Acta 72 (2008) 1396–1414 www.elsevier.com/locate/gca Okenane, a biomarker for purple sulfur bacteria (Chromatiaceae), and other new carotenoid derivatives from the 1640 Ma Barney Creek Formation Jochen J. Brocks a,*, Philippe Schaeffer b a Research School of Earth Sciences and Centre for Macroevolution and Macroecology, The Australian National University, Canberra, ACT 0200, Australia b Laboratoire de Ge´ochimie Bio-organique, CNRS UMR 7177, Ecole Europe´enne de Chimie, Polyme`res et Mate´riaux, 25 rue Becquerel, 67200 Strasbourg, France Received 20 June 2007; accepted in revised form 12 December 2007; available online 23 December 2007 Abstract Carbonates of the 1640 million years (Ma) old Barney Creek Formation (BCF), McArthur Basin, Australia, contain more than 22 different C40 carotenoid derivatives including lycopane, c-carotane, b-carotane, chlorobactane, isorenieratane, b-iso- renieratane, renieratane, b-renierapurpurane, renierapurpurane and the monoaromatic carotenoid okenane. -
What's Hot on the Moon Tonight?: the Ultimate Guide to Lunar Observing
What’s Hot on the Moon Tonight: The Ultimate Guide to Lunar Observing Copyright © 2015 Andrew Planck All rights reserved. No part of this book may be reproduced in any written, electronic, recording, or photocopying without written permission of the publisher or author. The exception would be in the case of brief quotations embodied in the critical articles or reviews and pages where permission is specifically granted by the publisher or author. Although every precaution has been taken to verify the accuracy of the information contained herein, the publisher and author assume no responsibility for any errors or omissions. No liability is assumed for damages that may result from the use of information contained within. Books may be purchased by contacting the publisher or author through the website below: AndrewPlanck.com Cover and Interior Design: Nick Zelinger (NZ Graphics) Publisher: MoonScape Publishing, LLC Editor: John Maling (Editing By John) Manuscript Consultant: Judith Briles (The Book Shepherd) ISBN: 978-0-9908769-0-8 Library of Congress Catalog Number: 2014918951 1) Science 2) Astronomy 3) Moon Dedicated to my wife, Susan and to my two daughters, Sarah and Stefanie Contents Foreword Acknowledgments How to Use this Guide Map of Major Seas Nightly Guide to Lunar Features DAYS 1 & 2 (T=79°-68° E) DAY 3 (T=59° E) Day 4 (T=45° E) Day 5 (T=24° E.) Day 6 (T=10° E) Day 7 (T=0°) Day 8 (T=12° W) Day 9 (T=21° W) Day 10 (T= 28° W) Day 11 (T=39° W) Day 12 (T=54° W) Day 13 (T=67° W) Day 14 (T=81° W) Day 15 and beyond Day 16 (T=72°) Day 17 (T=60°) FINAL THOUGHTS GLOSSARY Appendix A: Historical Notes Appendix B: Pronunciation Guide About the Author Foreword Andrew Planck first came to my attention when he submitted to Lunar Photo of the Day an image of the lunar crater Pitatus and a photo of a pie he had made. -
Lunar Club Observations
Guys & Gals, Here, belatedly, is my Christmas present to you. I couldn’t buy each of you a lunar map, so I did the next best thing. Below this letter you’ll find a guide for observing each of the 100 lunar features on the A. L.’s Lunar Club observing list. My guide tells you what the features are, where they are located, what instrument (naked eyes, binoculars or telescope) will give you the best view of them and what you can expect to see when you find them. It may or may not look like it, but this project involved a massive amount of work. In preparing it, I relied heavily on three resources: *The lunar map I used to determine which quadrant of the Moon each feature resides in is the laminated Sky & Telescope Lunar Map – specifically, the one that shows the Moon as we see it naked-eye or in binoculars. (S&T also sells one with the features reversed to match the view in a refracting telescope for the same price.); and *The text consists of information from (a) my own observing notes and (b) material in Ernest Cherrington’s Exploring the Moon Through Binoculars and Small Telescopes. Both the map and Cherrington’s book were door prizes at our Dec. Christmas party. My goal, of course, is to get you interested in learning more about our nearest neighbor in space. The Moon is a fascinating and lovely place, and one that all too often is overlooked by amateur astronomers. But of all the objects in the night sky, the Moon is the most accessible and easiest to observe. -
Thumbnail Index
Thumbnail Index The following five pages depict each plate in the book and provide the following information about it: • Longitude and latitude of the main feature shown. • Sun’s angle (SE), ranging from 1°, with grazing illumination and long shadows, up to 72° for nearly full Moon conditions with the Sun almost overhead. • The elevation or height (H) in kilometers of the spacecraft above the surface when the image was acquired, from 21 to 116 km. • The time of acquisition in this sequence: year, month, day, hour, and minute in Universal Time. 1. Gauss 2. Cleomedes 3. Yerkes 4. Proclus 5. Mare Marginis 79°E, 36°N SE=30° H=65km 2009.05.29. 05:15 56°E, 24°N SE=28° H=100km 2008.12.03. 09:02 52°E, 15°N SE=34° H=72km 2009.05.31. 06:07 48°E, 17°N SE=59° H=45km 2009.05.04. 06:40 87°E, 14°N SE=7° H=60km 2009.01.10. 22:29 6. Mare Smythii 7. Taruntius 8. Mare Fecunditatis 9. Langrenus 10. Petavius 86°E, 3°S SE=19° H=58km 2009.01.11. 00:28 47°E, 6°N SE=33° H=72km 2009.05.31. 15:27 50°E, 7°S SE=10° H=64km 2009.01.13. 19:40 60°E, 11°S SE=24° H=95km 2008.06.08. 08:10 61°E, 23°S SE=9° H=65km 2009.01.12. 22:42 11.Humboldt 12. Furnerius 13. Stevinus 14. Rheita Valley 15. Kaguya impact point 80°E, 27°S SE=42° H=105km 2008.05.10. -
THE GEOCHEMICAL NEWS Newsletter of the Geochemical Society in Cooperation with the European Association of Geochemistry
January 2005 1 THE GEOCHEMICAL NEWS Newsletter of The Geochemical Society in cooperation with The European Association of Geochemistry In This Issue... An Interview with David Des Marais Geochemistry at Oak Ridge National Laboratory January 2005 Number 122 Newsletter of the Geochemical Society ISSN 0016-7010 2 The Geochemical News EAG OFFICERS - 2005 PRESIDENT Terry Seward, ETH, Zurich PRESIDENT ELECT Bruce Yardley, Leeds, UK OUTGOING PRESIDENT Francis Albarede, Lyon, France TREASURER Catherine Chauvel, Grenoble, France SECRETARY Mark Hodson, Reading, UK EAG COMMITTEE THE GEOCHEMICAL SOCIETY MIRA BAR-MATTHEWS, ISREAL Larryn Diamond, Switzerland Jérôme GAILLARDET, FRANCE Alex Halliday, Switzerland SUSAN STIPP, DENMARK Riccardo Vannucci, Italy The Geochemical Society is a nonprofit scientific society founded to en- GERHARD WORNER, GERMANY Bruce Yardley, UK courage the application of chemistry to the solution of geological and cosmologi- cal problems. Membership is international and diverse in background, encom- passing such fields as organic geochemistry, high- and low-temperature geochem- THE GEOCHEMICAL NEWS istry, petrology, meteoritics, fluid-rock interaction, and isotope geochemistry. The Society produces a Special Publications Series, The Geochemical News (this January 2005 quarterly newsletter), the Reviews in Mineralogy and Geochemistry Series (jointly with the Mineralogical Society of America), the journal Geochimica et Editors Cosmochimica Acta (jointly with the Meteoritical Society), and co-publishes the Johnson R. Haas and Carla M. Koretsky electronic journal G3 (jointly with the American Geophysical Union: AGU); grants Department of Geosciences the V.M. Goldschmidt, F.W. Clarke and Clair C. Patterson Awards, and, jointly Western Michigan University with the European Association of Geochemistry (EAG), the Geochemistry Fel- Kalamazoo, MI 49008 lows title; sponsors the V.M. -
Vascular Plant Biomarker Distributions and Stable Carbon Isotopic
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by NERC Open Research Archive 1 Palaeogeography, Palaeoclimatology, Palaeoecology 2 3 Vascular plant biomarker distributions and stable carbon isotopic 4 signatures from the Middle and Upper Jurassic (Callovian–Kimmeridgian) 5 strata of Staffin Bay, Isle of Skye, northwest Scotland 6 7 Kliti Grice 1,*, Clinton B. Foster 2, James B. Riding 3, Sebastian Naeher 1, Paul F. 8 Greenwood 1,4 9 10 1 WA Organic and Isotope Geochemistry Centre, The Institute for Geoscience Research, 11 Department of Chemistry, Curtin University, GPO Box U1987 Perth, WA 6845, Australia 12 2 Geoscience Australia, GPO Box 378, Canberra, ACT, 2601, Australia 13 3 British Geological Survey, Environmental Science Centre, Keyworth, Nottingham NG12 14 5GG, United Kingdom 15 4 Centre for Exploration Targeting and WA Biogeochemistry Centre (M090), The University 16 of Western Australia, 35 Stirling Highway, Crawley, WA, 6009, Australia 17 18 19 20 21 22 23 * Corresponding author. Tel.: +61 8 9266 2474; Fax: +61 8 9266 2300 24 E-mail address: [email protected] (K. Grice) 1 25 Abstract 26 The molecular and stable carbon isotopic composition of higher plant biomarkers was 27 investigated in Middle to Upper Jurassic strata of the Isle of Skye, northwest Scotland. 28 Aromatic hydrocarbons diagnostic of vascular plants were detected in each of nineteen 29 sedimentary rock samples from the Early Callovian to Early Kimmeridgian interval, a 30 succession rich in fossil fauna including ammonites that define its constituent chronozones. 31 The higher plant parameter (HPP) and higher plant fingerprint (HPF) calculated from the 32 relative abundance of retene, cadalene and 6-isopropyl-1-isohexyl-2-methylnaphthalene (ip- 33 iHMN) exhibit several large fluctuations throughout the Skye succession studied.