The Project Gutenberg Ebook of Astronomy of To-Day, by Cecil G
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The Nearest Stars: a Guided Tour by Sherwood Harrington, Astronomical Society of the Pacific
www.astrosociety.org/uitc No. 5 - Spring 1986 © 1986, Astronomical Society of the Pacific, 390 Ashton Avenue, San Francisco, CA 94112. The Nearest Stars: A Guided Tour by Sherwood Harrington, Astronomical Society of the Pacific A tour through our stellar neighborhood As evening twilight fades during April and early May, a brilliant, blue-white star can be seen low in the sky toward the southwest. That star is called Sirius, and it is the brightest star in Earth's nighttime sky. Sirius looks so bright in part because it is a relatively powerful light producer; if our Sun were suddenly replaced by Sirius, our daylight on Earth would be more than 20 times as bright as it is now! But the other reason Sirius is so brilliant in our nighttime sky is that it is so close; Sirius is the nearest neighbor star to the Sun that can be seen with the unaided eye from the Northern Hemisphere. "Close'' in the interstellar realm, though, is a very relative term. If you were to model the Sun as a basketball, then our planet Earth would be about the size of an apple seed 30 yards away from it — and even the nearest other star (alpha Centauri, visible from the Southern Hemisphere) would be 6,000 miles away. Distances among the stars are so large that it is helpful to express them using the light-year — the distance light travels in one year — as a measuring unit. In this way of expressing distances, alpha Centauri is about four light-years away, and Sirius is about eight and a half light- years distant. -
Sunnyvale Heritage Resources
CARIBBEAN DR 3RD AV G ST C ST BORDEAUX DR H ST 3RD AV Heritage Trees CARIBBEAN DR CASPIAN CT GENEVA DR ENTERPRISE WY 4TH AV Local Landmarks E ST CASPIAN DR BALTIC WY Heritage Resources 5TH AV JAVA DR 5TH AV MOFFETT PARK DR CROSSMAN AV 300-ft Buffer CHESAPEAKE TR GIBRALTAR CT GIBRALTAR DR ORLEANS DR MOFFETT PARK DR 7TH AV MACON RD ANVILWOOD City Boundary ENTERPRISEWY CT G ST C ST MOFFETT PARK CT 8TH AV HUMBOLDT CT PERSIAN DR FORGEWOODAV SR-237 ANVILWOODAV INNSBRUCK DR ELKO DR 9TH AV E ST FAIR OAKS WY BORREGAS AV D ST P O R P O I S ALDERWOODAV 11TH AV MOFFETT PARK DR E BA Y TR PARIA BIRCHWOODDR MATHILDA AV GLIESSEN JAEGALS RD GLIN SR-237 PLAZA DR PLENTYGLIN LA ROCHELLE TR TASMAN DR ENTERPRISE WY ENTERPRISE MONTEGO VIENNA DR KASSEL INNOVATION WAY BRADFORD DR MOLUCCA MONTEREY LEYTE MORSE AV KIHOLO LEMANS ROSS DR MUNICH LUND TASMAN CT KARLSTAD DR ESSEX AV COLTON AV FULTON AV DUNCAN AV HAMLIN CT SAGINAW FAIR OAKS AV TOYAMA DR SACO LAWRENCEEXPRESSWAY GARNER DR LYON US-101 SALERNO SAN JORGEKOSTANZ TIMOR KIEL CT SIRTE SOLOMON SUEZ LAKEBIRD DR CT DRIFTWOOD DRIFTWOOD CT CHARMWOOD CHARMWOOD CT SKYLAKE VALELAKE CT CT CLYDE AV BREEZEWOOD CT LAKECHIME DR JENNA PECOS WY AHWANEE AV LAKEDALE WY WEDDELL LOTUSLAKE CT GREENLAKE DR HIDDENLAKE DR WEDDELL DR MEADOWLAKE DR ALMANOR AV FAIRWOODAV STONYLAKE SR-237 LAKEFAIR DR CT CT LYRELAKE LYRELAKE HEM BLAZINGWOOD DR REDROCK CT LO CT CK ALTURAS AV SILVERLAKEDR AV CT CANDLEWOOD LAKEHAVEN DR BURNTWOOD CT C B LAKEHAVEN A TR U JADELAKE SAN ALESO AV R N MADRONE AV LAKEKNOLL DR N D T L PALOMAR AV SANTA CHRISTINA W CT -
Transactions 1905
THE Royal Astronomical Society of Canada TRANSACTIONS FOR 1905 (INCLUDING SELECTED PAPERS AND PROCEEDINGS) EDITED BY C. A CHANT. TORONTO: ROYAL ASTRONOMICAL PRINT, 1906. The Royal Astronomical Society of Canada. THE Royal Astronomical Society of Canada TRANSACTIONS FOR 1905 (INCLUDING SELECTED PAPERS AND PROCEEDINGS) EDITED BY C. A CHANT. TORONTO: ROYAL ASTRONOMICAL PRINT, 1906. TABLE OF CONTENTS. The Dominion Observatory, Ottawa (Frontispiece) List of Officers, Fellows and A ssociates..................... - - 3 Treasurer’s R eport.....................--------- 12 President’s Address and Summary of Work ------ 13 List of Papers and Lectures, 1905 - - - - ..................... 26 The Dominion Observatory at Ottawa - - W. F. King 27 Solar Spots and Magnetic Storms for 1904 Arthur Harvey 35 Stellar Legends of American Indians - - J. C. Hamilton 47 Personal Profit from Astronomical Study - R. Atkinson 51 The Eclipse Expedition to Labrador, August, 1905 A. T. DeLury 57 Gravity Determinations in Labrador - - Louis B. Stewart 70 Magnetic and Meteorological Observations at North-West River, Labrador - - - - R. F. Stupart 97 Plates and Filters for Monochromatic and Three-Color Photography of the Corona J. S. Plaskett 89 Photographing the Sun and Moon with a 5-inch Refracting Telescope . .......................... D. B. Marsh 108 The Astronomy of Tennyson - - - - John A. Paterson 112 Achievements of Nineteenth Century Astronomy , L. H. Graham 125 A Lunar Tide on Lake Huron - - - - W. J. Loudon 131 Contributions...............................................J. Miller Barr I. New Variable Stars - - - - - - - - - - - 141 II. The Variable Star ξ Bootis -------- 143 III. The Colors of Helium Stars - - - ..................... 144 IV. A New Problem in Solar Physics ------ 146 Stellar Classification ------ W. Balfour Musson 151 On the Possibility of Fife in Other Worlds A. -
November/December 2015 Interior
BRINGING HISTORY INTO ACCORD WITH THE FACTS IN THE TRADITION OF DR. HARRY ELMER BARNES The Barnes Review A JOURNAL OF NATIONALIST THOUGHT & HISTORY 1781 VOLUME XXII NUMBER 1 JANUARY/FEBRUARY 2016 WWW.BARNESREVIEW.COM THE DECISIVE YEAR OF THE REVOLUTIONARY WAR What Really Caused the he Treaty of Paris in 1783 formal- and continue to fight on, assisted by Swamp ly ended the American Revolu- Fox Francis Marion and Light Horse Harry tionary War, but it was the pivotal Lee. While luring Cornwallis north, Greene campaigns and battles of 1781 was able to gather new strength and launch a T that decided the final outcome. counterattack, until it was Cornwallis who felt 1781 was one of those rare years in American compelled to seek succor in Virginia. He history when the future of the nation hung by marched his main army to Yorktown on the Chicago Fire? a thread, and only the fortitude, determination peninsula, upon which the American and and sacrifice of its leaders and citizenry ensured French armies and the French fleet all con- its survival. By 1781, America had been at war verged. On Oct. 19, 1781, Cornwallis surren- with the world's strongest empire for six years dered his weary and bloodied army. with no end in sight. British troops occupied In this book, renowned historian Robert key coastal cities, from New York to Savannah, L. Tonsetic provides a detailed analysis of the and the Royal Navy prowled the waters off the key battles and campaigns of 1781, supported American coast. The remaining patriot forces by numerous eyewitness accounts from pri- were hunkered down in the hinterland, giving vates to generals in the American, French and battle only at opportunities when British col- British armies. -
Stellar Distances Teacher Guide
Stars and Planets 1 TEACHER GUIDE Stellar Distances Our Star, the Sun In this Exploration, find out: ! How do the distances of stars compare to our scale model solar system?. ! What is a light year? ! How long would it take to reach the nearest star to our solar system? (Image Credit: NASA/Transition Region & Coronal Explorer) Note: The above image of the Sun is an X -ray view rather than a visible light image. Stellar Distances Teacher Guide In this exercise students will plan a scale model to explore the distances between stars, focusing on Alpha Centauri, the system of stars nearest to the Sun. This activity builds upon the activity Sizes of Stars, which should be done first, and upon the Scale in the Solar System activity, which is strongly recommended as a prerequisite. Stellar Distances is a math activity as well as a science activity. Necessary Prerequisite: Sizes of Stars activity Recommended Prerequisite: Scale Model Solar System activity Grade Level: 6-8 Curriculum Standards: The Stellar Distances lesson is matched to: ! National Science and Math Education Content Standards for grades 5-8. ! National Math Standards 5-8 ! Texas Essential Knowledge and Skills (grades 6 and 8) ! Content Standards for California Public Schools (grade 8) Time Frame: The activity should take approximately 45 minutes to 1 hour to complete, including short introductions and follow-ups. Purpose: To aid students in understanding the distances between stars, how those distances compare with the sizes of stars, and the distances between objects in our own solar system. © 2007 Dr Mary Urquhart, University of Texas at Dallas Stars and Planets 2 TEACHER GUIDE Stellar Distances Key Concepts: o Distances between stars are immense compared with the sizes of stars. -
Auditorium Features Duo Pianists- a Special Homecoming Is- to Meet Today Sue on Saturday
I \RY tttei Weather Editorial He Who Hesitates Windy and Mild (llimtwrttntt latlg (EampttH (See Page 2) Serving Storrs Since 1896" VOL CXIII. No 40 Offices in Student Union Building STORRS. CONNECTICUT Complete UPI Wire Service THURSDAY, NOVEMBER 12, 1959 No IS$U9 The llaily Campus will Senior Council not publish an Issue tomor- row. Instead, there will he Auditorium Features Duo Pianists- a special Homecoming Is- To Meet Today sue on Saturday. The Homecoming paper will be six pages. Instead president and approved by The senior class council will of four, and will feature Lowe, Whittemore Monday Night the senior class council Itself. Beet Mils afternoon at 3:30 several departures from our p.m. in the HUB UnMed Na- AMONG THE DUTIES of regular norm. Page one One of the most popular Weal waa a member of the Denver Eastman School ol Music BV THE ul llllll \K n{ tions Room, not at 4 p.m. as this council would be to act will be In color, with a spe- concert attractions in Amer- Arthur Whittemore was Symphony. At Colorado thai Whittemore and Lowe World War 11 they were es- 11 d been previously an- in a planning and advisory ca- cial color cartoon by Young ica will appear In the ' born and raised In the college Teachers College, he turned first met Good friends, they tablished as one of the coun- Richmond. town of Verrmllion. South to the piano. "Buck" Whine often played two -piano music pacity to the senior class versity Auditorium next Moil- try s most popular two-piano ponced, council. -
Large Impact Basins on Mercury: Global Distribution, Characteristics, and Modification History from MESSENGER Orbital Data Caleb I
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 117, E00L08, doi:10.1029/2012JE004154, 2012 Large impact basins on Mercury: Global distribution, characteristics, and modification history from MESSENGER orbital data Caleb I. Fassett,1 James W. Head,2 David M. H. Baker,2 Maria T. Zuber,3 David E. Smith,3,4 Gregory A. Neumann,4 Sean C. Solomon,5,6 Christian Klimczak,5 Robert G. Strom,7 Clark R. Chapman,8 Louise M. Prockter,9 Roger J. Phillips,8 Jürgen Oberst,10 and Frank Preusker10 Received 6 June 2012; revised 31 August 2012; accepted 5 September 2012; published 27 October 2012. [1] The formation of large impact basins (diameter D ≥ 300 km) was an important process in the early geological evolution of Mercury and influenced the planet’s topography, stratigraphy, and crustal structure. We catalog and characterize this basin population on Mercury from global observations by the MESSENGER spacecraft, and we use the new data to evaluate basins suggested on the basis of the Mariner 10 flybys. Forty-six certain or probable impact basins are recognized; a few additional basins that may have been degraded to the point of ambiguity are plausible on the basis of new data but are classified as uncertain. The spatial density of large basins (D ≥ 500 km) on Mercury is lower than that on the Moon. Morphological characteristics of basins on Mercury suggest that on average they are more degraded than lunar basins. These observations are consistent with more efficient modification, degradation, and obliteration of the largest basins on Mercury than on the Moon. This distinction may be a result of differences in the basin formation process (producing fewer rings), relaxation of topography after basin formation (subduing relief), or rates of volcanism (burying basin rings and interiors) during the period of heavy bombardment on Mercury from those on the Moon. -
Planets and Exoplanets
NASE Publications Planets and exoplanets Planets and exoplanets Rosa M. Ros, Hans Deeg International Astronomical Union, Technical University of Catalonia (Spain), Instituto de Astrofísica de Canarias and University of La Laguna (Spain) Summary This workshop provides a series of activities to compare the many observed properties (such as size, distances, orbital speeds and escape velocities) of the planets in our Solar System. Each section provides context to various planetary data tables by providing demonstrations or calculations to contrast the properties of the planets, giving the students a concrete sense for what the data mean. At present, several methods are used to find exoplanets, more or less indirectly. It has been possible to detect nearly 4000 planets, and about 500 systems with multiple planets. Objetives - Understand what the numerical values in the Solar Sytem summary data table mean. - Understand the main characteristics of extrasolar planetary systems by comparing their properties to the orbital system of Jupiter and its Galilean satellites. The Solar System By creating scale models of the Solar System, the students will compare the different planetary parameters. To perform these activities, we will use the data in Table 1. Planets Diameter (km) Distance to Sun (km) Sun 1 392 000 Mercury 4 878 57.9 106 Venus 12 180 108.3 106 Earth 12 756 149.7 106 Marte 6 760 228.1 106 Jupiter 142 800 778.7 106 Saturn 120 000 1 430.1 106 Uranus 50 000 2 876.5 106 Neptune 49 000 4 506.6 106 Table 1: Data of the Solar System bodies In all cases, the main goal of the model is to make the data understandable. -
Daily Iowan (Iowa City, Iowa), 1946-01-19
Partly Cloudy Good Morning IOWA: Mostly eloudy today. Iowa City Mueh eolder. • Iowa City's Morning Newspaper . THE A880ClATED •••81 IOWA CITY, lOW A SATURDAY, JANUARY 19,1946 AP WlIIEP80TO ESTABLISHED 1868 VOL. 78 NUMBER 98 tee or e·rs tri e on ay. '· · General Eis,enhower Government Shipment 260 Trailers Be gin S Assures 61 s, Parents . ' * * * * * * * * * * * * * * *' Of Prompt Shipments Efforts Fall FPHA Okays Half' of U. S. Forces Walkout of 750,000 In China to Be Home Workers Scheduled Quick Aclion In April-Wedemeyer For Noon Tomorrow WASHINGTON (AP)-Gcneral b r TOE A 80CIATED PltES8 Dwight D. Eisenhow!fJ' promised Direct government ectorts to Contractors Transport homesick Gl's and their families setUe the nation's two biggest last night that the revised demo- labor controversies failed yester Equipment to Iowa bilization schedule will be "car- day. itferent Field for Installation rled oul to the letter." The threatened gtrike of 750,000 - The chief of staff said, however, CIO steel workers-excluding iron The university has received in an address prepared for broad- ore miner members in Minnesota hb or governmenl permission to slart cast to the nation and by 5ho(t- -was "on" again for 12:01 a. m. d in I wave to posts all over the world, Monday, alter the United Stales Ilion 01 shipping 260 house-u'ailers to Iowa City, and work to transport that the army will have to aban- Steel corporation rejected Presi : of the don some of Its present occupation dent Truman's un ion-accepted and install the units will begin and liquidation tasks if it fails to yor ~ loday, President Virgil M. -
Exoplanet Atmosphere Measurements from Direct Imaging
Exoplanet Atmosphere Measurements from Direct Imaging Beth A. Biller and Mickael¨ Bonnefoy Abstract In the last decade, about a dozen giant exoplanets have been directly im- aged in the IR as companions to young stars. With photometry and spectroscopy of these planets in hand from new extreme coronagraphic instruments such as SPHERE at VLT and GPI at Gemini, we are beginning to characterize and classify the at- mospheres of these objects. Initially, it was assumed that young planets would be similar to field brown dwarfs, more massive objects that nonetheless share sim- ilar effective temperatures and compositions. Surprisingly, young planets appear considerably redder than field brown dwarfs, likely a result of their low surface gravities and indicating much different atmospheric structures. Preliminarily, young free-floating planets appear to be as or more variable than field brown dwarfs, due to rotational modulation of inhomogeneous surface features. Eventually, such inho- mogeneity will allow the top of atmosphere structure of these objects to be mapped via Doppler imaging on extremely large telescopes. Direct imaging spectroscopy of giant exoplanets now is a prelude for the study of habitable zone planets. Even- tual direct imaging spectroscopy of a large sample of habitable zone planets with future telescopes such as LUVOIR will be necessary to identify multiple biosigna- tures and establish habitability for Earth-mass exoplanets in the habitable zones of nearby stars. Introduction Since 1995, more than 3000 exoplanets have been discovered, mostly via indirect means, ushering in a completely new field of astronomy. In the last decade, about a dozen planets have been directly imaged, including archetypical systems such as arXiv:1807.05136v1 [astro-ph.EP] 13 Jul 2018 Beth A. -
Variabelbulletinen Nr. 1
Variabelbulletinen Nr 1 Augusti 2012 54600 54800 55000 55200 55400 55600 55800 56000 56200 3 4 5 6 7 8 9 10 11 12 13 14 Ljuskurva för miran Chi Cygni 2 Variabelbulletinen Nr 1. Augusti 2012. ISSN 2001-3930 En publikation från Svensk AmatörAstronomisk Förening Variabelsektionen (SAAF/V) Sektionsledare Chris Allen Ansvariga för databasen SVO Thomas Karlsson och Robert Wahlström Redaktör Hans Bengtsson Icke signerat material har författats av redaktören. Innehållsförteckning Introduktion. …………………...…………………………………………………………………….……………………….…… 4 Hans Bengtsson: Klassiska miror och legendariska variabilister. ………………...…….…..... 4 Thomas Karlsson: Epsilon Aurigae. ….……………………...……………………………...………………..…. 16 Hans Bengtsson: Våra variabler. Första delen. ………………………………………..…….....….……. 16 Thomas Karlsson: Ljusstark supernova i M101. ………………………………………………..…….… 26 Gustav Holmberg: Några RCB-stjärnor säsongen 2011-2012. …....…………...……….……. 28 Thomas Karlsson: Bestämning av period för 58 variabler. …………..……………...……….…... 31 Thomas Karlsson: Maxima för miror. ………………………………………………………………...……….… 33 Thomas Karlsson: Fotometri i Sagitta och Vulpecula. …………………………………………….… 34 Statistisk från SVO. ……………..…………………………………………...………………………………………...…… 38 Hans Bengtsson: Variabelmöten – en ny tradition. …………...……………………………………….. 39 Hans Bengtsson: Flera flugor i samma smäll. …………………………...............................…………... 40 Förstasidan Ljuskurva för miran Chi Cygni. Följande observatörer har bidragit till diagrammet: Chris Allen (45), Hans Bengtsson (102), Göran Fredriksson (9), -
Human/Environment Relations Analysis & Simulation Using
Human/Environment Relations Analysis & Simulation Using Human-Centered Systems Methods for Design and Evaluation of Complex Habitable Environments by Simonetta Andrea Rodriguez B.S. Architectural Engineering The University of Texas at Austin, 1988 Submitted to the Department of Civil and Environmental Engineering in Partial Fulfillment of the Requirements for the Degree of MASTER OF SCIENCE IN CIVIL AND ENVIRONMENTAL ENGINEERING at the MASSACHUSETTS INSTITUTE OF TECHNOLOGY January 2000 C 2000 Simonetta A. Rodriguez. All rights reserved The author hereby grants to MIT permission to reproduce and to distribute publicly paper and electronic copies of this thesis document in whole or in part. Signature of Author: epartment of Civil and nviro e tal g' eering anuary 24, 2000 Certified by: Steven Lerman Class of 1922 Professor of Civil and Environmental Engineering Thesis Supervisor Accepted by: Daniele Veneziano Chairman, Departmental Committee on Graduate Studies Civil and Environmental Engineering MASSACHUSETTS INSTITUTE OF TECHNOLOGY FBR1 4 2000 LIBRARIES -4 Page intentionally left blank. 2 Human/Environment Relations Analysis & Simulation Using Human-Centered Systems Methods for Design and Evaluation of Complex Habitable Environments by Simonetta Andrea Rodriguez Submitted to the Department of Civil and Environmental Engineering, on January 14, 2000 in partial fulfillment of the requirements for the degree of Master of Science in Civil and Environmental Engineering. ABSTRACT An exploration with two main goals is presented: 1. Modeling a self-contained "intelligent building," the Mars Arctic Research Station (MARS) habitation unit, and interaction with its users. The modeling effort seeks representation of invisible aspects of the interactions between the station and its users rather than visible forms.