June 20 to July 18, 2018 (Times in EDT) by Chris Vaughan
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Binocular Universe
Binocular Universe: Flying High September 2014 Phil Harrington he North America Nebula (NGC 7000) is a large expanse of glowing hydrogen gas mixed with opaque clouds of cosmic dust just 3° east of Deneb [Alpha (α) Cygni] and T 1° to the west of 4th-magnitude Xi (ξ) Cygni. Famous as one of the most luminous blue supergiants visible in the night sky, Deneb marks the tail of Cygnus the Swan, or if you prefer, the top of the Northern Cross asterism. Above: Summer star map from Star Watch by Phil Harrington. Above: Finder chart for this month's Binocular Universe. Chart adapted from Touring the Universe through Binoculars Atlas (TUBA), www.philharrington.net/tuba.htm The North America Nebula epitomizes how observational astronomy has evolved over the years. When he discovered it on October 24, 1786, Sir William Herschel (1738-1822) described the view through his 18.7-inch reflecting telescope as "very large diffused nebulosity, brighter in the middle." Honestly, I am surprised he could see it at all because of his instrument's very narrow field of view. That's one of the biggest challenges to seeing the North America Nebula through a telescope -- it spans an area nearly 2° in diameter. From the sounds of Herschel's notes, the thought of trying to spot it in anything less never crossed his mind. Five score and four years later, the German astronomer Max Wolf became the first to photograph the full span of NGC 7000. Upon seeing his results, he christened it the North America Nebula for its eerie resemblance to that continent. -
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. -
CAAC 2018-11.Pdf
Charlotte Amateur Astronomers Club www.charlotteastronomers.org Next Meeting: Friday November 16th, 2018 Time: 7:00 PM Place: Myers Park Baptist Church Education Building – Shalom Hall (Basement) Address: 1900 Queens Road Charlotte, NC 28207 CAAC November 2018 Meeting Appalachian State has had an active astronomy program for about 40 years. The research programs at DSO will be described as well as the Public Outreach program. Our undergraduate and graduate astronomy education activities will also be described. All of these center on state-of-the-art facilities at the off-campus Dark Sky Observatory and the on-campus, roll-off roof, GoTo instructional astronomy lab.All instruments at DSO as well as at the GoTo lab are now controllable from home (DSO) or the adjacent teaching classroom (the GoTo facility). Lots of the details will be of interest to amateurs who can use the same techniques to control their telescopes. Indeed, some of our research programs are within access of equipment and skills possessed by hobbyists. Speaker Dan Caton grew up in Tampa, Florida and attended the University of South Florida, graduating in 1973 with B.A.'s in astronomy and physics. He stayed on to get a Masters in astronomy, and then his Ph.D. in astronomy at Gainesville. After three years of temporary positions, he took a tenure-track position at Appalachian State, where he eventually became a tenured full professor of physics and astronomy, and Director of Observatories. Dan is still there, living in Boone with his wife Susan. His area of expertise is in the study of binary stars. -
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. -
Cosmic Raw Material Fig 20-CO, P.438
Stars form in greatStars clouds form of gas in and great dust clouds of gas and dust Slide 1 Cosmic raw material Fig 20-CO, p.438 Chapter Opener The Eagle Nebula (M16) Stars form in great clouds of gas and dust, and this image shows a large region of such cosmic raw material. The gas is visible because, about 2 million years ago, the cloud produced a cluster of bright stars, whose light ionizes the hydrogen gas nearby, causing it to glow. The cluster can be seen just above and to the left of the darker columns of dust at the center of the image. The dark columns or “elephant trunks” of material are seen in much more detail in Figures 20.1 and 20.2. This false-color image was created by combining images taken through filters that select lines of hydrogen alpha (green), oxygen (blue), and sulfur (red). (T.A. Rector, B.A. Wolpa, and OAO/NRAO/AURA/NSF) 1 The Central Region of the Orion Nebula Slide 2 Fig 20-5a, p.443 Figure 20.5 The Central Region of the Orion Nebula The Orion Nebula harbors some of the youngest stars in the solar neighborhood. At the heart of the nebula is the Trapezium cluster, which includes four very bright stars that provide much of the energy that causes the nebula to glow so brightly. In these images, we see a section of the nebula in visible light (left) and infrared (right). The four bright stars in the center of the visible-light image are the Trapezium stars. -
Cygnus a Monthly Sky Guide for the Beginning to Intermediate Amateur Astronomer Tom Trusock 10-Aug-2005
Small Wonders: Cygnus A monthly sky guide for the beginning to intermediate amateur astronomer Tom Trusock 10-Aug-2005 Figure 1: Widefield Map 2/16 Small Wonders: Cygnus Target List Object Type Size Mag RA Dec α (alpha) Cygni (Deneb) Star 1.3 20h 41m 38.7s 45 17' 59" β (beta) Cygni (Albireo) Star 3 19h 30m 57.9s 27 58' 18" NGC 7000 Bright Nebula 120.0'x100.0' 4 20h 59m 03.2s 44 32' 16" IC 5070 Bright Nebula 60.0'x50.0' 8 20h 51m 01.1s 44 12' 13" NGC 6960 Supernova Remnant 70.0'x6.0' 7 20h 45m 57.0s 30 44' 12" NGC 6979 Bright Nebula 7.0'x3.0' 20h 51m 14.9s 32 10' 14" NGC 6992 Bright Nebula 60.0'x8.0' 7 20h 56m 39.0s 31 44' 16" M 29 Open Cluster 10.0' 6.6 20h 24m 11.6s 38 30' 58" M 39 Open Cluster 31.0' 4.6 21h 32m 10.4s 48 26' 40" NGC 6826 Planetary Nebula 36" 8.8 19h 44m 58.8s 50 32' 21" NGC 7026 Planetary Nebula 45" 10.9 21h 06m 31.4s 47 52' 28" NGC 6888 Bright Nebula 18.0'x13.0' 10 20h 12m 20.0s 38 22' 18" NGC 6946 Galaxy 11.5'x9.8' 9 20h 35m 01.0s 60 10' 19" Challenge Objects Object Type Size Mag RA Dec PK 64+ 5.1 Planetary Nebula 5" 9.6 19h 35m 02.3s 30 31' 45" Sh2-112 9.0'x7.0' Cygnus ygnus is a spectacular summer constellation. -
GEORGE HERBIG and Early Stellar Evolution
GEORGE HERBIG and Early Stellar Evolution Bo Reipurth Institute for Astronomy Special Publications No. 1 George Herbig in 1960 —————————————————————– GEORGE HERBIG and Early Stellar Evolution —————————————————————– Bo Reipurth Institute for Astronomy University of Hawaii at Manoa 640 North Aohoku Place Hilo, HI 96720 USA . Dedicated to Hannelore Herbig c 2016 by Bo Reipurth Version 1.0 – April 19, 2016 Cover Image: The HH 24 complex in the Lynds 1630 cloud in Orion was discov- ered by Herbig and Kuhi in 1963. This near-infrared HST image shows several collimated Herbig-Haro jets emanating from an embedded multiple system of T Tauri stars. Courtesy Space Telescope Science Institute. This book can be referenced as follows: Reipurth, B. 2016, http://ifa.hawaii.edu/SP1 i FOREWORD I first learned about George Herbig’s work when I was a teenager. I grew up in Denmark in the 1950s, a time when Europe was healing the wounds after the ravages of the Second World War. Already at the age of 7 I had fallen in love with astronomy, but information was very hard to come by in those days, so I scraped together what I could, mainly relying on the local library. At some point I was introduced to the magazine Sky and Telescope, and soon invested my pocket money in a subscription. Every month I would sit at our dining room table with a dictionary and work my way through the latest issue. In one issue I read about Herbig-Haro objects, and I was completely mesmerized that these objects could be signposts of the formation of stars, and I dreamt about some day being able to contribute to this field of study. -
Week 5: January 26-February 1, 2020
5# Ice & Stone 2020 Week 5: January 26-February 1, 2020 Presented by The Earthrise Institute About Ice And Stone 2020 It is my pleasure to welcome all educators, students, topics include: main-belt asteroids, near-Earth asteroids, and anybody else who might be interested, to Ice and “Great Comets,” spacecraft visits (both past and Stone 2020. This is an educational package I have put future), meteorites, and “small bodies” in popular together to cover the so-called “small bodies” of the literature and music. solar system, which in general means asteroids and comets, although this also includes the small moons of Throughout 2020 there will be various comets that are the various planets as well as meteors, meteorites, and visible in our skies and various asteroids passing by Earth interplanetary dust. Although these objects may be -- some of which are already known, some of which “small” compared to the planets of our solar system, will be discovered “in the act” -- and there will also be they are nevertheless of high interest and importance various asteroids of the main asteroid belt that are visible for several reasons, including: as well as “occultations” of stars by various asteroids visible from certain locations on Earth’s surface. Ice a) they are believed to be the “leftovers” from the and Stone 2020 will make note of these occasions and formation of the solar system, so studying them provides appearances as they take place. The “Comet Resource valuable insights into our origins, including Earth and of Center” at the Earthrise web site contains information life on Earth, including ourselves; about the brighter comets that are visible in the sky at any given time and, for those who are interested, I will b) we have learned that this process isn’t over yet, and also occasionally share information about the goings-on that there are still objects out there that can impact in my life as I observe these comets. -
Index to JRASC Volumes 61-90 (PDF)
THE ROYAL ASTRONOMICAL SOCIETY OF CANADA GENERAL INDEX to the JOURNAL 1967–1996 Volumes 61 to 90 inclusive (including the NATIONAL NEWSLETTER, NATIONAL NEWSLETTER/BULLETIN, and BULLETIN) Compiled by Beverly Miskolczi and David Turner* * Editor of the Journal 1994–2000 Layout and Production by David Lane Published by and Copyright 2002 by The Royal Astronomical Society of Canada 136 Dupont Street Toronto, Ontario, M5R 1V2 Canada www.rasc.ca — [email protected] Table of Contents Preface ....................................................................................2 Volume Number Reference ...................................................3 Subject Index Reference ........................................................4 Subject Index ..........................................................................7 Author Index ..................................................................... 121 Abstracts of Papers Presented at Annual Meetings of the National Committee for Canada of the I.A.U. (1967–1970) and Canadian Astronomical Society (1971–1996) .......................................................................168 Abstracts of Papers Presented at the Annual General Assembly of the Royal Astronomical Society of Canada (1969–1996) ...........................................................207 JRASC Index (1967-1996) Page 1 PREFACE The last cumulative Index to the Journal, published in 1971, was compiled by Ruth J. Northcott and assembled for publication by Helen Sawyer Hogg. It included all articles published in the Journal during the interval 1932–1966, Volumes 26–60. In the intervening years the Journal has undergone a variety of changes. In 1970 the National Newsletter was published along with the Journal, being bound with the regular pages of the Journal. In 1978 the National Newsletter was physically separated but still included with the Journal, and in 1989 it became simply the Newsletter/Bulletin and in 1991 the Bulletin. That continued until the eventual merger of the two publications into the new Journal in 1997. -
The Birth and Evolution of Planetary Systems
CHAPTER 7 The Birth and Evolution of Planetary Systems hn hk io il sy SY hn hk io il sy SY hn hk io il sy SY Ideas about the origins of the Sun, the Moon, and Earth objects in the Solar System. It is important for the stu- hn hk io il sy SY are older than written history. Greek and Roman mythol- dents to realize that you can determine many of the prop- ogy, as well as creation myths of the Bible, represent some erties of a planet by knowing its mass, size, and distance hn hk io il sy SY of humanity’s earliest attempts to explain how the heav- from the Sun. hn hk io il sy SY ens and Earth were created. Thousands of years and Although planetary scientists are confident they have hn hk io il sy SY the scientific revolution have ultimately debunked many the big picture of Solar System formation correct, the ancient creation stories, but our new theories of solar sys- details are still in question. Questions remain concerning hn hk io il sy SY tem formation are still relatively in their infancy. Jupiter’s formation. It might not have been able to form hn hk io il sy SY The nebular model of solar system formation was first via accretion but may have formed similarly to the Sun. proposed by Immanuel Kant in 1755. It has undergone To complicate matters further, Uranus and Neptune significant revision in the last 250 years, but the details of appear to be too large to have formed at their current posi- the pro cess remain elusive. -
Occuttation3newstetter
- "* Occuttation3Newstetter Volume III, Number 12 August, 1985 IOTA Tenth Anniversary Issue Occultation Newsletter is published by the International Occultation Timing Association. Editor and compos- itor: H. F. DaBoII; 6 N 106 White Oak Lane; St. Charles, IL 60174; U. S. A. Please send editorial matters, renewals, address changes, and reimbursement requests to the above, but for new memberships, new subscrip- tions, back issues, and any special requests, write to IOTA; P. 0. Box 3392; Columbus, OH 43210-0392; U.S.A. FROM THE PUBLISHER Tony Murray, Georgetown, GA, has provided IOTA let- terhead and envelopes, as was announced in the last This is the second issue of 1985. It marks the com- issue. I have not had time to prepare a design for pletion of eleven years of publication of o.n. a membership card. If you would be interested in preparing such a design, send it to me at P.0. Box When renewing, please give your name and address ex- 7488, Silver Spring, MD 20907 for consideration. m. actly as they appear on your mailing label, so that That would expedite this project; Murray is ready to we can locate your file; if the label should be re- generate them when we settle on a design. vised, tell us how it should be changed. Pressure of generating the material about the occu1- If you wish, you may use your VISA or MasterCard for tations by comets during the rest of the year, in payments to IOTA; include the account number, the particular, the numerous events involving Comet Gia- expiration date, and your signature. -
Astrophysics
Publications of the Astronomical Institute rais-mf—ii«o of the Czechoslovak Academy of Sciences Publication No. 70 EUROPEAN REGIONAL ASTRONOMY MEETING OF THE IA U Praha, Czechoslovakia August 24-29, 1987 ASTROPHYSICS Edited by PETR HARMANEC Proceedings, Vol. 1987 Publications of the Astronomical Institute of the Czechoslovak Academy of Sciences Publication No. 70 EUROPEAN REGIONAL ASTRONOMY MEETING OF THE I A U 10 Praha, Czechoslovakia August 24-29, 1987 ASTROPHYSICS Edited by PETR HARMANEC Proceedings, Vol. 5 1 987 CHIEF EDITOR OF THE PROCEEDINGS: LUBOS PEREK Astronomical Institute of the Czechoslovak Academy of Sciences 251 65 Ondrejov, Czechoslovakia TABLE OF CONTENTS Preface HI Invited discourse 3.-C. Pecker: Fran Tycho Brahe to Prague 1987: The Ever Changing Universe 3 lorlishdp on rapid variability of single, binary and Multiple stars A. Baglln: Time Scales and Physical Processes Involved (Review Paper) 13 Part 1 : Early-type stars P. Koubsfty: Evidence of Rapid Variability in Early-Type Stars (Review Paper) 25 NSV. Filtertdn, D.B. Gies, C.T. Bolton: The Incidence cf Absorption Line Profile Variability Among 33 the 0 Stars (Contributed Paper) R.K. Prinja, I.D. Howarth: Variability In the Stellar Wind of 68 Cygni - Not "Shells" or "Puffs", 39 but Streams (Contributed Paper) H. Hubert, B. Dagostlnoz, A.M. Hubert, M. Floquet: Short-Time Scale Variability In Some Be Stars 45 (Contributed Paper) G. talker, S. Yang, C. McDowall, G. Fahlman: Analysis of Nonradial Oscillations of Rapidly Rotating 49 Delta Scuti Stars (Contributed Paper) C. Sterken: The Variability of the Runaway Star S3 Arietis (Contributed Paper) S3 C. Blanco, A.