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1922 Elizabeth T
co.rYRIG HT, 192' The Moootainetro !scot1oror,d The MOUNTAINEER VOLUME FIFTEEN Number One D EC E M BER 15, 1 9 2 2 ffiount Adams, ffiount St. Helens and the (!oat Rocks I ncoq)Ora,tecl 1913 Organized 190!i EDITORlAL ST AitF 1922 Elizabeth T. Kirk,vood, Eclttor Margaret W. Hazard, Associate Editor· Fairman B. L�e, Publication Manager Arthur L. Loveless Effie L. Chapman Subsc1·iption Price. $2.00 per year. Annual ·(onl�') Se,·ent�·-Five Cents. Published by The Mountaineers lncorJ,orated Seattle, Washington Enlerecl as second-class matter December 15, 19t0. at the Post Office . at . eattle, "\Yash., under the .-\0t of March 3. 1879. .... I MOUNT ADAMS lllobcl Furrs AND REFLEC'rION POOL .. <§rtttings from Aristibes (. Jhoutribes Author of "ll3ith the <6obs on lltount ®l!!mµus" �. • � J� �·,,. ., .. e,..:,L....._d.L.. F_,,,.... cL.. ��-_, _..__ f.. pt",- 1-� r�._ '-';a_ ..ll.-�· t'� 1- tt.. �ti.. ..._.._....L- -.L.--e-- a';. ��c..L. 41- �. C4v(, � � �·,,-- �JL.,�f w/U. J/,--«---fi:( -A- -tr·�� �, : 'JJ! -, Y .,..._, e� .,...,____,� � � t-..__., ,..._ -u..,·,- .,..,_, ;-:.. � --r J /-e,-i L,J i-.,( '"'; 1..........,.- e..r- ,';z__ /-t.-.--,r� ;.,-.,.....__ � � ..-...,.,-<. ,.,.f--· :tL. ��- ''F.....- ,',L � .,.__ � 'f- f-� --"- ��7 � �. � �;')'... f ><- -a.c__ c/ � r v-f'.fl,'7'71.. I /!,,-e..-,K-// ,l...,"4/YL... t:l,._ c.J.� J..,_-...A 'f ',y-r/� �- lL.. ��•-/IC,/ ,V l j I '/ ;· , CONTENTS i Page Greetings .......................................................................tlristicles }!}, Phoiitricles ........ r The Mount Adams, Mount St. Helens, and the Goat Rocks Outing .......................................... B1/.ith Page Bennett 9 1 Selected References from Preceding Mount Adams and Mount St. -
INSTRUCTION MANUAL Synscantm
INSTRUCTION MANUAL SynScanTM SynScan TM SSHCV3-F-141031V1-EN Copyright © Sky-Watcher CONTENT Basic Operations PART I : INTRODUCTION 1.1 Outline and Interface .......................................................................................... 4 1.2 Connecting to a Telescope Mount ...................................................................... 4 1.3 Slew the Mount with the Direction Keys .............................................................. 4 1.4 SynScan Hand control’s Operating Modes ......................................................... 5 PART II : INITIALIZATION 2.1 Setup Home Position of the Telescope Mount ..................................................... 7 2.2 Initialize the Hand Control .................................................................................. 7 PART III : ALIGNMENT 3.1 Choosing an Alignment Method .........................................................................11 3.2 Aligning to Alignment Stars ...............................................................................11 3.3 Alignment Method for Equatorial Mounts ..........................................................11 3.4 Alt-Azimuth Mounts using Brightest Star Alignment Method ............................12 3.5 Alt-Azimuth Mounts using 2-Star Alignment Method ........................................15 3.6 Tips for Improving Alignment Accuracy .............................................................16 3.7 Comparison of Alignment Methods ....................................................................16 -
Annual Report, Fiscal Year 1965
1965 TECHNICAL HIGHLIGHTS OF THE NATIONAL BUREAU OF STANDARDS Annual Report for: INSTITUTE FOR BASIC STANDARDS INSTITUTE FOR MATERIALS RESEARCH INSTITUTE FOR APPLIED TECHNOLOGY CENTRAL RADIO PROPAGATION LABORATORY n UNITED STATES DEPARTMENT OF COMMERCE John T. Connor, Secretary J. Herbert Hollomon, Assistant Secretary for Science and Technology NATIONAL BUREAU OF STANDARDS A. V. Astin, Director 1965 Technical Highlights of the National Bureau of Standards Annual Report, Fiscal Year 1965 May 1966 Miscellaneous Publication 279 For sale by the Superintendent of Documents, U.S. Government Printing Office Washington, D. C, 20402 — Price 65 cents Library of Congress Catalog Card Number: 6-23979 CONTENTS THE DIRECTOR'S STATEMENT _ 1 NBS—An Evolving Institution 1 Management Progress 3 NBS As a Scientific Laboratory 5 INSTITUTE FOR BASIC STANDARDS 11 Physical Quantities, Constants, and Calibration Services 12 International Base L nits 13 Length. Mass. Frequency and Time. Temperature. Luminous Intensity. Electric Current. Mechanical Quantities 19 Force. Pressure. Vacuum. Electrical Quantities—DC 24 Resistance Ratios. Voltage. Current Ratio Standards. New Compensated Current Comparator. Absolute Electrical Meas- urements. AC-DC Transfer Standards. Voltage Ratio Detector for Millivolt Signals. Electrical Quantities—Radio 25 Low-Frequency Calibration. High-Frequency Electrical Stand- ards. High-Frequency Impedance Standards. High-Frequency Calibrations. Microwave Standards. Microwave Calibrations. Photometric and Radiometric Quantities 30 Ionizing Radiations 32 Engineering Measurement and Standards 36 Phyical Properties 39 National Standard Reference Data System 40 Nuclear Data. Atomic and Molecular Data. Solid State Data. Thermodynamics and Transport Data. Chemical Kinetics. Col- loid and Surface Properties. Information Services. Measurement 48 Nuclear Properties. Atomic and Molecular Properties. Solid State Properties. -
12-Inch Alvan Clark Telescope Restoration
12-Inch Alvan Clark Telescope Restoration: Summary of Research and Final Recommendations Deborah Culmer and Hannah Johnson September, 2011 Introduction The first telescope installed at Lick Observatory was a second-hand purchase, with the telescope and its optic made by the premier telescope makers of the time, Alvan Clark and Sons of Cambridge, MA. The dome that housed it was the first structure built on Mt. Hamilton, from bricks fired in a kiln on location. That dome still stands; and until the 1970’s, the 12-inch refracting telescope was in operation, but without its original driver clock and gears (replaced with an electronic drive, perhaps in the 1950’s). Since it was decommissioned, the 12-inch has been in storage. The Lick Instrument Lab has retrieved it, and it is currently on location at UC Santa Cruz in anticipation of total restoration. In the summer of 2011, a research project was launched to determine to what era and condition the telescope should be restored. In recent years, there has been great interest in historical restoration of Alvan Clark telescopes (and others, to be sure). As a result of that interest, we had a pool of organizations and institutions from which to glean information. Two we visited in person; many more we contacted via email and conference calls. Based on our research and interviews, we offer our recommendations on the restoration of this historically important telescope. 1. Research In beginning this project, it was very important to understand the history of the 12-inch Alvan Clark, especially since it was the first telescope set up on Mt. -
As the Dome of Twilight Sinks Below The
As the dome of twilight sinks below the horizon, a mechanical corps de ballet starts a slow-motion pirouette with each dancer keeping the unblinking eye of a telescope locked on a single spot in the heavens. Shutters open and ancient photons, ending a journey that may have started before the earth was born, collide with sensors that store an electron to mark that photon's arrival. With the dance in motion the directors sit back to watch the show; another imaging session has begun... Image by Marcus Stevens A Full and Proper Kit An introduction to the gear of astro-photography The young recruit is silly – 'e thinks o' suicide; 'E's lost his gutter-devil; 'e 'asn't got 'is pride; But day by day they kicks him, which 'elps 'im on a bit, Till 'e finds 'isself one mornin' with a full an' proper kit. Rudyard Kipling Like the young recruit in Kipling's poem 'The 'Eathen', a deep-sky imaging beginner starts with little in the way of equipment or skill. With 'older' imagers urging him onward, providing him with the benefit of the mistakes that they had made during their journey and allowing him access to the equipment they've built or collected, the newcomer gains the 'equipment' he needs, be it gear or skills, to excel at the art. At that time he has acquired a 'full and proper kit' and ceases to be a recruit. This paper is a discussion of hardware, software, methods and actions that a newcomer might find useful. It is not meant to be an in-depth discussion of all forms of astro-photography; that would take many books and more knowledge than I have available. -
Sirius - Wikipedia Coordinates: 06 H 4 5 M 08.9 1 7 3 S, −1 6 ° 4 2 ′ 5 8.01 7 ″
12/2/2018 Sirius - Wikipedia Coordinates: 06 h 4 5 m 08.9 1 7 3 s, −1 6 ° 4 2 ′ 5 8.01 7 ″ Sirius Sirius (/ˈsɪriəs/, a romanization of Greek Σείριος, Seirios, lit. "glowing" or "scorching") is a star system Sirius A and B and the brightest star in the Earth's night sky. With a visual apparent magnitude of −1.46, it is almost twice as bright as Canopus, the next brightest star. The system has the Bayer designation Alpha Canis Majoris (α CMa). What the naked eye perceives as a single star is a binary star system, consisting of a white main-sequence star of spectral type A0 or A1, termed Sirius A, and a faint white dwarf companion of spectral type DA2, called Sirius B. The distance separating Sirius A from its companion varies between 8.2 and 31.5 AU.[24] Sirius appears bright because of its intrinsic luminosity and its proximity to Earth. At a distance of 2.6 parsecs (8.6 ly), as determined by the Hipparcos astrometry satellite,[2][25][26] the Sirius system is one of Earth's near neighbours. Sirius is gradually moving closer to the Solar System, so it will slightly increase in brightness over the next 60,000 years. After that time its distance will begin to increase and it will become fainter, but it will continue to be the brightest star in the Earth's night sky for the next 210,000 years.[27] The position of Sirius (circled). Sirius A is about twice as massive as the Sun (M☉) and has an absolute visual magnitude of 1.42. -
Its Founding and Early Years Ewen A. Whitaker
The University of Arizona's LUNAR AND PLANETARY LABORATORY Its Founding and Early Years Ewen A. Whitaker Set in Varityper Times Roman and printed at the University of Arizona Printing-Reproductions Department Equal Employment Opportunity· Affirmative Action Employer CONTENTS THE PRE-TUCSON ERA Historical background ........................................ I Enter Gerard P. Kuiper ....................................... 2 The Moon enters the picture ................................... 3 A call for suggestions ......................................... 5 The Harold Urey affair ....................................... 6 Preliminaries for the Lunar Atlas ............................... 7 1957 - a dream begins to take shape ............................. 7 The shot that was seen (and heard) around the world ............... 8 Other irons in the fire ......................................... 9 Kuiper seeks full-time help for the Lunar Project .................. 9 1959 - the Lunar Project gathers momentum ..................... 11 A new factor in the Lunar Project LPL story ................... 12 The Air Force enters the lunar cartography business ............... 13 The Lunar Atlas published at last .............................. 14 Big problems with the Yerkes set-up ............................ : 6 The southwestern U.S. begins to beckon ........................ 17 "There is a tide in the affairs of men ..." ....................... 18 Preparing for the move ...................................... 23 THE TUCSON ERA The Lunar Project makes the transfer -
Thestargazer
The StarGazer http://www.raclub.org/ Newsletter of the Rappahannock Astronomy Club No. 2 Vol. 7 August 2018–October 2018 Pilgrimage to the Great Refractor By Scott Busby “Time always takes from us those things we hold most dear” The Yerkes Observatory belongs to the Department of Astronomy and Astrophysics of the University of Chicago (UChicago). Established in 1897 on Lake Geneva in Williams Bay, Wisconsin, the observatory, situated on a 78-acre park site, houses all the Department’s activities. Most of the important history of Yerkes Observatory can be found at astro.uchicago.edu. I won’t elaborate too much on its history here; suffice it to say that this great observatory was the result of the hard work and dedication of George Ellery Hale (1868– 1938). Hale had a unique ability to talk wealthy tycoons into funding his astronomical endeavors—pun intended. We can thank him for some of the great telescopes of our time. Some of the more familiar are the 60- and 100-inch Hooker reflecting telescopes on Mount Wilson near Pasadena and his namesake, the Great 200-inch Hale reflecting telescope at Mount Palomar observatory near San Diego. On March 7, 2018, UChicago announced plans to wind down its activities at Yerkes Observatory. As a result, the observatory will close its doors to visitors and researchers on October 1, 2018, with no prospects and no immediate plans to reopen In the last month, my wife Debbie and I decided to take a trip to Williams Bay to visit the Yerkes Observatory and its great 40- The 40-Inch Alvan Clark & Sons Refractor Credit: inch refractor telescope. -
Appendix I Lunar and Martian Nomenclature
APPENDIX I LUNAR AND MARTIAN NOMENCLATURE LUNAR AND MARTIAN NOMENCLATURE A large number of names of craters and other features on the Moon and Mars, were accepted by the IAU General Assemblies X (Moscow, 1958), XI (Berkeley, 1961), XII (Hamburg, 1964), XIV (Brighton, 1970), and XV (Sydney, 1973). The names were suggested by the appropriate IAU Commissions (16 and 17). In particular the Lunar names accepted at the XIVth and XVth General Assemblies were recommended by the 'Working Group on Lunar Nomenclature' under the Chairmanship of Dr D. H. Menzel. The Martian names were suggested by the 'Working Group on Martian Nomenclature' under the Chairmanship of Dr G. de Vaucouleurs. At the XVth General Assembly a new 'Working Group on Planetary System Nomenclature' was formed (Chairman: Dr P. M. Millman) comprising various Task Groups, one for each particular subject. For further references see: [AU Trans. X, 259-263, 1960; XIB, 236-238, 1962; Xlffi, 203-204, 1966; xnffi, 99-105, 1968; XIVB, 63, 129, 139, 1971; Space Sci. Rev. 12, 136-186, 1971. Because at the recent General Assemblies some small changes, or corrections, were made, the complete list of Lunar and Martian Topographic Features is published here. Table 1 Lunar Craters Abbe 58S,174E Balboa 19N,83W Abbot 6N,55E Baldet 54S, 151W Abel 34S,85E Balmer 20S,70E Abul Wafa 2N,ll7E Banachiewicz 5N,80E Adams 32S,69E Banting 26N,16E Aitken 17S,173E Barbier 248, 158E AI-Biruni 18N,93E Barnard 30S,86E Alden 24S, lllE Barringer 29S,151W Aldrin I.4N,22.1E Bartels 24N,90W Alekhin 68S,131W Becquerei -
Asteroid Regolith Weathering: a Large-Scale Observational Investigation
University of Tennessee, Knoxville TRACE: Tennessee Research and Creative Exchange Doctoral Dissertations Graduate School 5-2019 Asteroid Regolith Weathering: A Large-Scale Observational Investigation Eric Michael MacLennan University of Tennessee, [email protected] Follow this and additional works at: https://trace.tennessee.edu/utk_graddiss Recommended Citation MacLennan, Eric Michael, "Asteroid Regolith Weathering: A Large-Scale Observational Investigation. " PhD diss., University of Tennessee, 2019. https://trace.tennessee.edu/utk_graddiss/5467 This Dissertation is brought to you for free and open access by the Graduate School at TRACE: Tennessee Research and Creative Exchange. It has been accepted for inclusion in Doctoral Dissertations by an authorized administrator of TRACE: Tennessee Research and Creative Exchange. For more information, please contact [email protected]. To the Graduate Council: I am submitting herewith a dissertation written by Eric Michael MacLennan entitled "Asteroid Regolith Weathering: A Large-Scale Observational Investigation." I have examined the final electronic copy of this dissertation for form and content and recommend that it be accepted in partial fulfillment of the equirr ements for the degree of Doctor of Philosophy, with a major in Geology. Joshua P. Emery, Major Professor We have read this dissertation and recommend its acceptance: Jeffrey E. Moersch, Harry Y. McSween Jr., Liem T. Tran Accepted for the Council: Dixie L. Thompson Vice Provost and Dean of the Graduate School (Original signatures are on file with official studentecor r ds.) Asteroid Regolith Weathering: A Large-Scale Observational Investigation A Dissertation Presented for the Doctor of Philosophy Degree The University of Tennessee, Knoxville Eric Michael MacLennan May 2019 © by Eric Michael MacLennan, 2019 All Rights Reserved. -
Cemetery Files - April 2020 - Owner's Name - C 1
Cemetery Files - April 2020 - Owner's Name - C 1 Year Year Cemetery No Person Buried Owner Buried Purchased 200-02-297-07-1 CABBAGE, ALICE 1958 CABBAGE, ALICE N. 1956 200-02-297-08-1 CABBAGE, BENJAMIN 1956 CABBAGE, ALICE N. 1956 130-06-053-09-2 CABRERO, PIDRO-INF OF 1952 CABRERO, PEDRO P. 1952 200-07-040-08-1 CADWALLADER, HELEN 1998 CADWALLADER, HELEN 1998 200-02-179-03-2 CADY, LOIS (ASHES) 1999 CADY 0 105-10-003-02-1 ALLISON, ELSIE HELEN 1974 CAFER, MRS. JOHN 0 200-06-169-03-1 0 CAIN, BARBARA & LOREN 1997 200-06-169-04-1 CAIN,LOREN 1997 CAIN, BARBARA & LOREN 1997 200-06-135-03-1 CAIN, LOTTIE 1993 CAIN, LOTTIE 1988 200-06-135-04-1 CAIN, PAUL F. 1988 CAIN, LOTTIE 1988 200-06-134-03-1 CAIN, MICHAEL 2001 CAIN, LUCINDA 2001 105-01-072-01-1 0 CAIN, ROBERT 1920 105-01-072-02-1 0 CAIN, ROBERT 1920 105-01-072-03-1 BARTHOLOMEW, ETTA MAE 1942 CAIN, ROBERT 1920 105-01-072-03-2 CAIN, MILDRED 1920 CAIN, ROBERT 1920 105-01-072-04-1 0 CAIN, ROBERT 1920 105-04-008-04-1 CAIN, LILY F. 1942 CAIN, THOMAS A. 1942 105-04-008-05-1 CAIN, THOMAS A. 1957 CAIN, THOMAS A. 1942 190-07-020-01-1 0 CALAHAN, J.W. 0 190-07-020-02-1 CALLADAN, DORA 1928 CALAHAN, J.W. 0 190-07-020-03-1 CALLAHAN, JOHN W 1927 CALAHAN, J.W. 0 190-07-020-04-1 CALLAHN, CARL C. -
Lick Observatory Records: Photographs UA.036.Ser.07
http://oac.cdlib.org/findaid/ark:/13030/c81z4932 Online items available Lick Observatory Records: Photographs UA.036.Ser.07 Kate Dundon, Alix Norton, Maureen Carey, Christine Turk, Alex Moore University of California, Santa Cruz 2016 1156 High Street Santa Cruz 95064 [email protected] URL: http://guides.library.ucsc.edu/speccoll Lick Observatory Records: UA.036.Ser.07 1 Photographs UA.036.Ser.07 Contributing Institution: University of California, Santa Cruz Title: Lick Observatory Records: Photographs Creator: Lick Observatory Identifier/Call Number: UA.036.Ser.07 Physical Description: 101.62 Linear Feet127 boxes Date (inclusive): circa 1870-2002 Language of Material: English . https://n2t.net/ark:/38305/f19c6wg4 Conditions Governing Access Collection is open for research. Conditions Governing Use Property rights for this collection reside with the University of California. Literary rights, including copyright, are retained by the creators and their heirs. The publication or use of any work protected by copyright beyond that allowed by fair use for research or educational purposes requires written permission from the copyright owner. Responsibility for obtaining permissions, and for any use rests exclusively with the user. Preferred Citation Lick Observatory Records: Photographs. UA36 Ser.7. Special Collections and Archives, University Library, University of California, Santa Cruz. Alternative Format Available Images from this collection are available through UCSC Library Digital Collections. Historical note These photographs were produced or collected by Lick observatory staff and faculty, as well as UCSC Library personnel. Many of the early photographs of the major instruments and Observatory buildings were taken by Henry E. Matthews, who served as secretary to the Lick Trust during the planning and construction of the Observatory.