Newsletter Archive the Skyscraper April 2014
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The Evening Sky Map Evening the of Distribution Free and Production Support the Help (127° from Sun, Morning Sky) Sun, Morning (127° from (Evening Sky) at 22H UT
I N E D R I A C A S T N E O D I T A C L E O R N I G D S T S H A E P H M O O R C I . Z N O a r o e u t a n t d o r O t N h o e t Z r N a o I e C r p t h R p I a C R O s e r l C e a H t s L s t i E E , a s l e H ( P d T F o u O l t e i D t R NORTH ( a N N M l E C A n X P O r ) A e H . h C M T t . I r P o N S L n E E P Z m “ o E NORTHERN HEMISPHERE A N r H F O M T R T U Y N H s E e Etamin ” K E ) t W S . h . T e T E U B W B R i g HERCULES N W D The Evening Sky Map E D T T i MARCH 2014 WH p A p E C e FREE* EACH MONTH FOR YOU TO EXPLORE, LEARN & ENJOY THE NIGHT SKY O CEPHEUS μ S r L K ( Y o E ν r R M . P A t A l SKY MAP SHOWS HOW o o Get Sky Calendar on Twitter S P i T u r δ C A g a E h R h J c Sky Calendar – March 2014 ) http://twitter.com/skymaps O THE NIGHT SKY LOOKS B U l n o O DRACO N c w L D a a r t A NE e d I I EARLY MAR PM β 9 - T d T e S 1 New Moon at 8:02 UT. -
TAAS Observing Challenge, March 2016 Deep Sky Object
TAAS Observing Challenge, March 2016 Deep Sky Object NGC 3242 (PN) Hydra ra: 10h 24m 46.2s dec: -18° 38’ 34” Magnitude (visual) = 7.7 Size = 64” Distance = approximately 2,500 light years Description: William Herschel discovered this planetary nebula on February 7, 1785, and cataloged it as H IV.27. John Herschel observed it from the Cape of Good Hope, South Africa, in the 1830s, and numbered it as h 3248, and included it in the 1864 General Catalogue as GC 2102; this became NGC 3242 in J.L.E. Dreyer's New General Catalogue of 1888. This planetary nebula consists of a small dense nebula of about 16" x 26" in diameter, surrounded by a fainter envelop measuring about 40 x 35 arc seconds. This central nebula is embedded in a much larger faint halo, measuring 1250" or about 20.8 arc minutes in diameter. The bright inner nebula is described as looking like an eye by Burnham, and the outer shell gave rise to its popular name, as it is of about the apparent size of Jupiter. This planetary nebula is most frequently called the Ghost of Jupiter, or Jupiter's Ghost, but it is also sometimes referred to as the Eye Nebula, or the CBS Eye. Source: http://messier.seds.org/spider/Misc/n3242.html AL: Herschel 400, Caldwell [59]; TAAS 200 Challenge Object NGC 3962 (GX) Crater ra: 11h 54m 40.0s dec: -13° 58’ 34” Magnitude (visual) = 10.7 Size = 2.6’ x 2.2’ Position angle = 10° Description: NGC3962 is a small, elliptical galaxy in the constellation of Crater. -
Preliminary Program Plan FY2005
O National Radio Astronomy ProgramPlan Observatory FiscalYear-2005 NATIONAL RADIO ASTRONOMY OBSERVATORY Preliminary Program Plan FY2005 October 13, 2004 The National Radio Astronomy Observatory is a facility of the National Science Foundation operated by Associated Universities Inc. Table of Contents Mission Statement............................................................................................................................1 1. Introduction.................................................................................................................................3 2. Science Programs in FY2005......................................................................................................7 Overview..............................................................................................................................7 Cosmology and the Early Universe ....................................................................................8 Radio Galaxies, Quasars, Active Galactic Nuclei, and Gamma Ray Bursts .....................11 Nearby Galaxies and the Galactic Center ..........................................................................16 Molecular Clouds, Star Formation, and Galactic Structure...............................................20 Pulsars and Other Radio Stars............................................................................................24 Solar System; Geophysics..................................................................................................26 3. ALMA Construction -
Stars and Their Spectra: an Introduction to the Spectral Sequence Second Edition James B
Cambridge University Press 978-0-521-89954-3 - Stars and Their Spectra: An Introduction to the Spectral Sequence Second Edition James B. Kaler Index More information Star index Stars are arranged by the Latin genitive of their constellation of residence, with other star names interspersed alphabetically. Within a constellation, Bayer Greek letters are given first, followed by Roman letters, Flamsteed numbers, variable stars arranged in traditional order (see Section 1.11), and then other names that take on genitive form. Stellar spectra are indicated by an asterisk. The best-known proper names have priority over their Greek-letter names. Spectra of the Sun and of nebulae are included as well. Abell 21 nucleus, see a Aurigae, see Capella Abell 78 nucleus, 327* ε Aurigae, 178, 186 Achernar, 9, 243, 264, 274 z Aurigae, 177, 186 Acrux, see Alpha Crucis Z Aurigae, 186, 269* Adhara, see Epsilon Canis Majoris AB Aurigae, 255 Albireo, 26 Alcor, 26, 177, 241, 243, 272* Barnard’s Star, 129–130, 131 Aldebaran, 9, 27, 80*, 163, 165 Betelgeuse, 2, 9, 16, 18, 20, 73, 74*, 79, Algol, 20, 26, 176–177, 271*, 333, 366 80*, 88, 104–105, 106*, 110*, 113, Altair, 9, 236, 241, 250 115, 118, 122, 187, 216, 264 a Andromedae, 273, 273* image of, 114 b Andromedae, 164 BDþ284211, 285* g Andromedae, 26 Bl 253* u Andromedae A, 218* a Boo¨tis, see Arcturus u Andromedae B, 109* g Boo¨tis, 243 Z Andromedae, 337 Z Boo¨tis, 185 Antares, 10, 73, 104–105, 113, 115, 118, l Boo¨tis, 254, 280, 314 122, 174* s Boo¨tis, 218* 53 Aquarii A, 195 53 Aquarii B, 195 T Camelopardalis, -
Ages of Asteroid Families with the YORP-Eye Method
MNRAS 000, 1–15 (2018) Preprint 28 November 2018 Compiled using MNRAS LATEX style file v3.0 Ages of asteroid families with the YORP-eye method Paolo Paolicchi,1⋆ F. Spoto,2 Z. Kneˇzevi´c3 and A. Milani4 1Dept.Physics, University of Pisa, Largo Pontecorvo 3, I-56127 Pisa, Italy 2IMMCE, Observatoire de Paris, Av. Denfert–Rochereau 77, 75014 Paris, France 3Serbian Academy of Sciences and Arts, Kneza Mihaila 35, 11000 Belgrade, Serbia 4Dept.Mathematics, University of Pisa, Largo Pontecorvo 5, I-56127 Pisa, Italy Accepted XXX. Received YYY; in original form ZZZ ABSTRACT We have recently shown the possibility of finding footprints of the YORP effect con- cerning the members of asteroid dynamical families, in a plot proper semimajor axis– magnitude (the so–called “V–plot”), and in spite of several biases and uncertainties. That work introduced the concept of the “YORP–eye”, the depopulated regions in the plot above, whose location is diagnostic of the age of the family. In the present paper we complete the analysis using an improved algorithm and an extended database of families, and we discuss the potential errors due to uncertainties and dispersion of the astronomical data. We confirm that the analysis connected to the search for the YORP-eye can lead to an estimate of the age, which is similar and strongly correlated to that obtained by the analysis of the V–slope size dependent spreading due to the Yarkovsky effect. In principle the YORP-eye analysis alone can lead to an estimate of the ages of other families, which have no independent age estimates. -
April 14 2018 7:00Pm at the April 2018 Herrett Center for Arts & Science College of Southern Idaho
Snake River Skies The Newsletter of the Magic Valley Astronomical Society www.mvastro.org Membership Meeting President’s Message Tim Frazier Saturday, April 14th 2018 April 2018 7:00pm at the Herrett Center for Arts & Science College of Southern Idaho. It really is beginning to feel like spring. The weather is more moderate and there will be, hopefully, clearer skies. (I write this with some trepidation as I don’t want to jinx Public Star Party Follows at the it in a manner similar to buying new equipment will ensure at least two weeks of Centennial Observatory cloudy weather.) Along with the season comes some great spring viewing. Leo is high overhead in the early evening with its compliment of galaxies as is Coma Club Officers Berenices and Virgo with that dense cluster of extragalactic objects. Tim Frazier, President One of my first forays into the Coma-Virgo cluster was in the early 1960’s with my [email protected] new 4 ¼ inch f/10 reflector and my first star chart, the epoch 1960 version of Norton’s Star Atlas. I figured from the maps I couldn’t miss seeing something since Robert Mayer, Vice President there were so many so closely packed. That became the real problem as they all [email protected] appeared as fuzzy spots and the maps were not detailed enough to distinguish one galaxy from another. I still have that atlas as it was a precious Christmas gift from Gary Leavitt, Secretary my grandparents but now I use better maps, larger scopes and GOTO to make sure [email protected] it is M84 or M86. -
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Data analysis of 2005 Regulus occultation and simulation of the 2014 occultation Costantino Sigismondi, ICRANet, UFRJ and Observatorio Nacional, Rio de Janeiro [email protected] Tony George, IOTA North America [email protected] Thomas Flatrès, IOTA European Section [email protected] Abstract On March 20, 2014 at 6:06 UT (2:06 New York time) Regulus, the 1.3 magnitude brighter star of Leo constellation, is going to be occulted by the asteroid 163 Erigone. The unusual event, visible to the naked eye over NYC, can allow to measure the shape of the asteroid, with reaching a space resolution below the diffraction limit of the eye, and of all instruments not based on interferometry. Ultimately the aperture of the instrument is related to the amount of scintillation affecting the light curve of the occultation, limitating the accuracy of video recorded data. The asteroid profile scans the surface of the star at a velocity of 6 mas/s; the diameter of the star is about 1.3 mas and the detection of the stellar limb darkening signature is discussed, taking into consideration also the Fresnel fringes. New data reduction with R-OTE software of the 2005 Regulus occultation and simulations of the 2014 occultation with Fren_difl software are presented. The occultation of Regulus of March 20, 2014 above New York City The total solar eclipse of 1925 above New York area [5] and the occultation of delta Ophiuchi above France and Germany in 2010 [4] have been two occultation events followed by a relatively high number of observers. Potentially the occultation of 1.3 mas [8] first magnitude star Regulus over New York City can be the first asteroidal occultation observed by million people and broadcasted on the internet [23]. -
Issue 2005 Volume 3
ISSUE 2005 PROGRESS IN PHYSICS VOLUME 3 ISSN 1555-5534 The Journal on Advanced Studies in Theoretical and Experimental Physics, including Related Themes from Mathematics PROGRESS IN PHYSICS A quarterly issue scientific journal, registered with the Library of Congress (DC). ISSN: 1555-5534 (print) This journal is peer reviewed and included in the abstracting and indexing coverage of: ISSN: 1555-5615 (online) Mathematical Reviews and MathSciNet (AMS, USA), DOAJ of Lund University (Sweden), 4 issues per annum Referativnyi Zhurnal VINITI (Russia), etc. Electronic version of this journal: OCTOBER 2005 VOLUME 3 http://www.geocities.com/ptep_online To order printed issues of this journal, con- CONTENTS tact the Editor in Chief. Chief Editor H. Arp Observational Cosmology: From High Redshift Galaxies to the Blue Dmitri Rabounski Pacific.. .3 [email protected] S. J. Crothers On the General Solution to Einstein’s Vacuum Field for Associate Editors the Point-Mass when λ = 0 and Its Consequences for Relativistic Cos- Prof. Florentin Smarandache mology...............................................................76 [email protected] Dr. Larissa Borissova H. Ratcliffe The First Crisis in Cosmology Conference. Mon¸cao,˜ Portugal, [email protected] June 23–25, 2005. 19 Stephen J. Crothers [email protected] R. T. Cahill The Michelson and Morley 1887 Experiment and the Discovery of Absolute Motion. 25 Department of Mathematics, University of New Mexico, 200 College Road, Gallup, R. T. Cahill Gravity Probe B Frame-Dragging Effect. 30 NM 87301, USA R. Oros di Bartini Relations Between Physical Constants. 34 S. J. Crothers Introducing Distance and Measurement in General Relativity: Copyright c Progress in Physics, 2005 Changes for the Standard Tests and the Cosmological Large-Scale. -
SAA 100 Club
S.A.A. 100 Observing Club Raleigh Astronomy Club Version 1.2 07-AUG-2005 Introduction Welcome to the S.A.A. 100 Observing Club! This list started on the USENET newsgroup sci.astro.amateur when someone asked about everyone’s favorite, non-Messier objects for medium sized telescopes (8-12”). The members of the group nominated objects and voted for their favorites. The top 100 objects, by number of votes, were collected and ranked into a list that was published. This list is a good next step for someone who has observed all the objects on the Messier list. Since it includes objects in both the Northern and Southern Hemispheres (DEC +72 to -72), the award has two different levels to accommodate those observers who aren't able to travel. The first level, the Silver SAA 100 award requires 88 objects (all visible from North Carolina). The Gold SAA 100 Award requires all 100 objects to be observed. One further note, many of these objects are on other observing lists, especially Patrick Moore's Caldwell list. For convenience, there is a table mapping various SAA100 objects with their Caldwell counterparts. This will facilitate observers who are working or have worked on these lists of objects. We hope you enjoy looking at all the great objects recommended by other avid astronomers! Rules In order to earn the Silver certificate for the program, the applicant must meet the following qualifications: 1. Be a member in good standing of the Raleigh Astronomy Club. 2. Observe 80 Silver observations. 3. Record the time and date of each observation. -
7.5 X 11.5.Threelines.P65
Cambridge University Press 978-0-521-19267-5 - Observing and Cataloguing Nebulae and Star Clusters: From Herschel to Dreyer’s New General Catalogue Wolfgang Steinicke Index More information Name index The dates of birth and death, if available, for all 545 people (astronomers, telescope makers etc.) listed here are given. The data are mainly taken from the standard work Biographischer Index der Astronomie (Dick, Brüggenthies 2005). Some information has been added by the author (this especially concerns living twentieth-century astronomers). Members of the families of Dreyer, Lord Rosse and other astronomers (as mentioned in the text) are not listed. For obituaries see the references; compare also the compilations presented by Newcomb–Engelmann (Kempf 1911), Mädler (1873), Bode (1813) and Rudolf Wolf (1890). Markings: bold = portrait; underline = short biography. Abbe, Cleveland (1838–1916), 222–23, As-Sufi, Abd-al-Rahman (903–986), 164, 183, 229, 256, 271, 295, 338–42, 466 15–16, 167, 441–42, 446, 449–50, 455, 344, 346, 348, 360, 364, 367, 369, 393, Abell, George Ogden (1927–1983), 47, 475, 516 395, 395, 396–404, 406, 410, 415, 248 Austin, Edward P. (1843–1906), 6, 82, 423–24, 436, 441, 446, 448, 450, 455, Abbott, Francis Preserved (1799–1883), 335, 337, 446, 450 458–59, 461–63, 470, 477, 481, 483, 517–19 Auwers, Georg Friedrich Julius Arthur v. 505–11, 513–14, 517, 520, 526, 533, Abney, William (1843–1920), 360 (1838–1915), 7, 10, 12, 14–15, 26–27, 540–42, 548–61 Adams, John Couch (1819–1892), 122, 47, 50–51, 61, 65, 68–69, 88, 92–93, -
Caldwell Catalogue - Wikipedia, the Free Encyclopedia
Caldwell catalogue - Wikipedia, the free encyclopedia Log in / create account Article Discussion Read Edit View history Caldwell catalogue From Wikipedia, the free encyclopedia Main page Contents The Caldwell Catalogue is an astronomical catalog of 109 bright star clusters, nebulae, and galaxies for observation by amateur astronomers. The list was compiled Featured content by Sir Patrick Caldwell-Moore, better known as Patrick Moore, as a complement to the Messier Catalogue. Current events The Messier Catalogue is used frequently by amateur astronomers as a list of interesting deep-sky objects for observations, but Moore noted that the list did not include Random article many of the sky's brightest deep-sky objects, including the Hyades, the Double Cluster (NGC 869 and NGC 884), and NGC 253. Moreover, Moore observed that the Donate to Wikipedia Messier Catalogue, which was compiled based on observations in the Northern Hemisphere, excluded bright deep-sky objects visible in the Southern Hemisphere such [1][2] Interaction as Omega Centauri, Centaurus A, the Jewel Box, and 47 Tucanae. He quickly compiled a list of 109 objects (to match the number of objects in the Messier [3] Help Catalogue) and published it in Sky & Telescope in December 1995. About Wikipedia Since its publication, the catalogue has grown in popularity and usage within the amateur astronomical community. Small compilation errors in the original 1995 version Community portal of the list have since been corrected. Unusually, Moore used one of his surnames to name the list, and the catalogue adopts "C" numbers to rename objects with more Recent changes common designations.[4] Contact Wikipedia As stated above, the list was compiled from objects already identified by professional astronomers and commonly observed by amateur astronomers. -
Biography of Horace Welcome Babcock
NATIONAL ACADEMY OF SCIENCES H O R ACE W ELCOME B A B COC K 1 9 1 2 — 2 0 0 3 A Biographical Memoir by GEO R G E W . P R ESTON Any opinions expressed in this memoir are those of the author and do not necessarily reflect the views of the National Academy of Sciences. Biographical Memoir COPYRIGHT 2007 NATIONAL ACADEMY OF SCIENCES WASHINGTON, D.C. Photograph by Mount Wilson and Los Campanas Observatories HORACE WELCOME BABCOCK September 13, 1912−August 29, 2003 BY GEORGE W . P RESTON ORACE BABCOCK’S CAREER at the Mount Wilson and Palomar H(later, Hale) Observatories spanned more than three decades. During the first 18 years, from 1946 to 1964, he pioneered the measurement of magnetic fields in stars more massive than the sun, produced a famously successful model of the 22-year cycle of solar activity, and invented important instruments and techniques that are employed throughout the world to this day. Upon assuming the directorship of the observatories, he devoted his last 14 years to creating one of the world’s premier astronomical observatories at Las Campanas in the foothills of the Chilean Andes. CHILDHOOD AND EDUCATION Horace Babcock was born in Pasadena, California, the only child of Harold and Mary Babcock. Harold met Horace’s mother, Mary Henderson, in Berkeley during his student days at the College of Electrical Engineering, University of California. After brief appointments as a laboratory assis- tant at the National Bureau of Standards in 1906 and as a physics teacher at the University of California, Berkeley, in 1907, Horace’s father was invited by George Ellery Hale in 1908 to join the staff of the Mount Wilson Observatory (MWO), where he remained for the rest of his career.