Meteor Activity Outlook for November 14-20, 2020
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
THE STAR FORMATION NEWSLETTER an Electronic Publication Dedicated to Early Stellar Evolution and Molecular Clouds
THE STAR FORMATION NEWSLETTER An electronic publication dedicated to early stellar evolution and molecular clouds No. 90 — 27 March 2000 Editor: Bo Reipurth ([email protected]) Abstracts of recently accepted papers The Formation and Fragmentation of Primordial Molecular Clouds Tom Abel1, Greg L. Bryan2 and Michael L. Norman3,4 1 Harvard Smithsonian Center for Astrophysics, MA, 02138 Cambridge, USA 2 Massachusetts Institute of Technology, MA, 02139 Cambridge, USA 3 LCA, NCSA, University of Illinois, 61801 Urbana/Champaign, USA 4 Astronomy Department, University of Illinois, Urbana/Champaign, USA E-mail contact: [email protected] Many questions in physical cosmology regarding the thermal history of the intergalactic medium, chemical enrichment, reionization, etc. are thought to be intimately related to the nature and evolution of pregalactic structure. In particular the efficiency of primordial star formation and the primordial IMF are of special interest. We present results from high resolution three–dimensional adaptive mesh refinement simulations that follow the collapse of primordial molecular clouds and their subsequent fragmentation within a cosmologically representative volume. Comoving scales from 128 kpc down to 1 pc are followed accurately. Dark matter dynamics, hydrodynamics and all relevant chemical and radiative processes (cooling) are followed self-consistently for a cluster normalized CDM structure formation model. Primordial molecular clouds with ∼ 105 solar masses are assembled by mergers of multiple objects that have formed −4 hydrogen molecules in the gas phase with a fractional abundance of ∼< 10 . As the subclumps merge cooling lowers the temperature to ∼ 200 K in a “cold pocket” at the center of the halo. Within this cold pocket, a quasi–hydrostatically > 5 −3 contracting core with mass ∼ 200M and number densities ∼ 10 cm is found. -
Kugelsternhaufen
www.vds-astro.de ISSN 1615-0880 IV/2010 Nr. 35 Zeitschrift der Vereinigung der Sternfreunde e.V. Schwerpunktthema Kugelsternhaufen Klein, rund und plump! Die Botschaft von den Grundlagen der JPG-Foto- Seite 54 Sternen metrie Seite 87 Seite 111 [email protected] • www.astro-shop.com Tel.: 040/5114348 • Fax: 040/5114594 Eiffestr. 426 • 20537 Hamburg Astroart 4.0 Canon EOS 1000D Astro Photoshop Astronomy Die aktuellste Version Ab sofort erhalten Sie bei uns speziell für die Der Autor arbeitet seit fast 10 Jahren mit Photo- des bekannten Bildbe- Astronomie modizierte Canon EOS Kameras, shop, um seine Astrofotos zu bearbeiten. Die arbeitungspro- ab Lager und mit Garantie! dabei gemachten Erfahrungen hat er in diesem grammes gibt es jetzt Die 1000D Astro hat eine um den Faktor 5 speziell auf die Bedürfnisse des Amateurastro- mit interessanten höhere Rotempndlichkeit im Bereich von nomen zugeschnitte- neuen Funktionen. H-alpha nen Buch gesammelt. Moderne Dateifor- bzw. SII. Die behandelten The- men sind unter ande- mate wie DSLR-RAW Endlich rem: die technische werden unterstützt, können Ausstattung, Farbma- Bilder können Regionen nagement, Histo- durch automa- am Himmel gramme, Maskie- tische Sternfelderken- sichtbar rungstechniken, nung direkt überlagert werden, was die Bild- gemacht Addition mehrerer feldrotation vernachlässigbar macht. Auch die werden, die Bilder, Korrektur von Bearbeitung von Farbbildern wurde erweitert. vorher auf Astroaufnahmen nur ansatzweise Vignettierungen, Besonderes Augenmerk liegt auf der Erken- sichtbar waren oder im Himmelshintergrund Farbhalos, Deformationen oder nung und Behandlung von Pixelfehlern der schlicht 'abgesoen' sind. Somit stellt die EOS überbelichteten Sternen, LRGB und vieles Aufnahme-Chips. 1000D Astro eine preisgünstige Alternative zu mehr. -
Sky-High 2009
Sky-High 2009 Total Solar Eclipse, 29th March 2006 The 17th annual guide to astronomical phenomena visible from Ireland during the year ahead (naked-eye, binocular and beyond) By John O’Neill and Liam Smyth Published by the Irish Astronomical Society € 5 P.O. Box 2547, Dublin 14, Ireland. e-mail: [email protected] www.irishastrosoc.org Page 1 Foreword Contents 3 Your Night Sky Primer We send greetings to all fellow astronomers and welcome them to this, the seventeenth edition of 5 Sky Diary 2009 Sky-High. 8 Phases of Moon; Sunrise and Sunset in 2009 We thank the following contributors for their 9 The Planets in 2009 articles: Patricia Carroll, John Flannery and James O’Connor. The remaining material was written by 12 Eclipses in 2009 the editors John O’Neill and Liam Smyth. The Gal- 14 Comets in 2009 lery has images and drawings by Society members. The times of sunrise etc. are from SUNRISE by J. 16 Meteors Showers in 2009 O’Neill. 17 Asteroids in 2009 We are always glad to hear what you liked, or 18 Variable Stars in 2009 what you would like to have included in Sky-High. If we have slipped up on any matter of fact, let us 19 A Brief Trip Southwards know. We can put a correction in future issues. And if you have any problem with understanding 20 Deciphering Star Names the contents or would like more information on 22 Epsilon Aurigae – a long period variable any topic, feel free to contact us at the Society e- mail address [email protected]. -
Nov 2016 Newsletter
Volume22, Issue 3 NWASNEWS November 2016 Newsletter for the Wiltshire, Swindon, Beckington WHAT DO WANT FROM YOUR SOCIETY? Astronomical Societies and Salisbury Plain Firstly can I welcome our returning In the early years there may have been Wiltshire Society Page 2 speaker Philip Perkins who last came to more beginners experiences, especially us when we met over the road in the WI where I was learning the hard way myself, Swindon Stargazers 3 hall. not worried about putting my mistakes to the society so, hopefully, they may learn Beckington and SPOG 4 His imaging of the night sky is really in- from my mistakes. spirational, making the transition from Space Place What kind of plan- 5 film (hyposensitising film was no joke) Would somebody like to write a beginners ets could be at Proxima then moving over to digital. piece every month? It doesn't have to be Centauri. all your own work. His work can be seen on his website Space News: Falcon X, 6-13 Astrocruise.com. He has an observatory Saturn’s hex changes colour. in the south of France, but also does a lot At last we have our darker skies with Mars probe crash site. of imaging from here in Wiltshire near longer nights, it may bring cold and some How many planets in Milky Way Aldbourne. cloud, but did you know there are more Pluto and Charon data at last cloudy nights in August than in Decem- Argentine 30tonne meteorite ber? It is just a case of wrapping up warm Formation of the Earth What I have noticed is the drop in sub- and getting out there. -
The Observer, November
The OBSERVER The Newsletter of the Twin City Amateur Astronomers, Inc. November 2001 Volume 26, Number 11 Adventures in Meteor Hunting — Duane Yockey In This Issue: REETINGS to my brother and and binoculars just in case the meteors sister sky watchers, didn't live up to their billing. Saturday G was clear here in central Illinois, and • Meteor Hunting Adventures ...1 when I got back from a Duane shows that he has the The long awaited day play at Illinois State right stuff as he tears after the of the Leonid meteor University around Leonids and finds them! shower arrived Satur- 10:30 p.m. the sky was day. I was really still showing lots of • TCAA Calendar ........................1 looking forward to stars. I called Laura Use our calendar to mark going out to the (my oldest daughter), your calendar. observatory with who said the skies were other Twin City clear down in southern • TCAA Annual Holiday Bash....3 Amateur Indiana and I could Party like it’s, um, 2001, at Astronomers and see- drive down there, if the Vic & Cindy’s! ............................ ing the "show" from clouds rolled in (ha, 2:00 a.m. to 6:00 a.m. ha). I assured her that • Club Notes................................4 early Sunday morn- the sky would cooper- Wow, it’s been a busy month! ing. So I packed my ate, and it was looking car early with a lawn good then, and I wished • Software Review: DSE ...........5 chair and threw in my her good luck (if she And just think, if you never telescope, star charts turn to page 5, you’ll never know continued on next page what DSE stands for.. -
Arxiv:0706.2206V1 [Astro-Ph] 14 Jun 2007 1983; Beichman Et Al
Accepted to the Astrophysical Journal Supplemental Series Preprint typeset using LATEX style emulateapj v. 08/22/09 A CASE STUDY OF LOW-MASS STAR FORMATION Jonathan J. Swift Institute for Astronomy, 2680 Woodlawn Dr., Honolulu, HI 96822-1897: [email protected] William J. Welch Department of Astronomy and Radio Astronomy Laboratory, University of California, 601 Campbell Hall, Berkeley, CA 94720-3411 Accepted to the Astrophysical Journal Supplemental Series ABSTRACT This article synthesizes observational data from an extensive program aimed toward a comprehensive understanding of star formation in a low-mass star-forming molecular cloud. New observations and published data spanning from the centimeter wave band to the near infrared reveal the high and low density molecular gas, dust, and pre-main sequence stars in L1551. The total cloud mass of ∼ 160 M contained within a 0.9 pc has a dynamical timescale, tdyn = 1:1 Myr. Thirty-five pre-main sequence stars with masses from ∼ 0:1 to 1.5 M are selected to be members of the L1551 association constituting a total of 22 ± 5 M of stellar mass. The observed star formation efficiency, SFE = 12%, while the total efficiency, SFEtot, is estimated to fall between 9 and 15%. L1551 appears to have been forming stars for several tdyn with the rate of star formation increas- ing with time. Star formation has likely progressed from east to west, and there is clear evidence that another star or stellar system will form in the high column density region to the northwest of L1551 IRS5. High-resolution, wide-field maps of L1551 in CO isotopologue emission display the structure of the molecular cloud at 1600 AU physical resolution. -
January 2015 BRAS Newsletter
January, 2015 Next Meeting: January 12th at 7PM at HRPO Artist concept of New Horizons. For more info on it and its mission to Pluto, click on the image. What's In This Issue? President's Message Astro Short: Wild Weather on WASP -43b Secretary's Summary Message From HRPO IYL and 20/20 Vision Campaign Recent BRAS Forum Entries Observing Notes by John Nagle President's Message Welcome to a new year. I can see lots to be excited about this year. First up are the Rockafeller retreat and Hodges Gardens Star Party. Go to our website for details: www.brastro.org Almost like a Christmas present from heaven, Comet Lovejoy C/2014 Q2 underwent a sudden brightening right before Christmas. Initially it was expected to be about magnitude 8 at its brightest but right after Christmas it became visible to the naked eye. At the time of this writing, it may become as bright as magnitude 4.5 or 4. As January progresses, the comet will move farther north, and higher in the sky for us. Now all we need is for these clouds to move out…. If any of you received (or bought yourself) any astronomical related goodies for Christmas and would like to show them off, bring them to the next meeting. Interesting geeky goodies qualify also, like that new drone or 3D printer. BRAS members are invited to a star party hosted by a group called the Lake Charles Free Thinkers. It will be January 24, 2015 from 3:00 PM on, at 5335 Hwy. -
About Ten Stars Orbit Eclipsing Binary XZ
About ten stars orbit eclipsing binary XZ Andromedae Lauri Jetsu Department of Physics, P.O. Box 64, FI-00014, University of Helsinki, Finland; email: lauri.jetsu@helsinki.fi June 2, 2020 Abstract A third body in an eclipsing binary system causes regular periodic changes in the observed (O) minus the computed (C) eclipse epochs. Fourth bodies have rarely been detected from the O-C data. We apply the new Discrete Chi-square Method (DCM) to the O-C data of the eclipsing binary XZ Andromedae. These data contain the periodic signatures of at least ten wide orbit stars (WOSs). Their orbital periods are between 1.6 and 91.7 years. Since no changes have been observed in the eclipses of XZ And during the past 127 years, the orbits of all these WOSs are most probably co-planar. We give detailed instructions of how the professional and the amateur astronomers can easily repeat all stages of our DCM analysis with an ordinary PC, as well as apply this method to the O-C data of other eclipsing binaries. Key words: methods: data analysis - methods: numerical - methods: statistical - binaries: eclipsing 1 Introduction 2 Data In September 2019, we retrieved the observed (O) minus the Naked eye observations of Algol’s eclipses have been recorded computed (C) primary eclipse epochs of XZ And from the into the Ancient Egyptian Calendar of Lucky and Un- Lichtenknecker-Database of the BAV. These data had lucky days (Jetsu and Porceddu, 2015; Jetsu et al., 2013; been computed from the ephemeris Porceddu et al., 2018, 2008). -
October 2015 BRAS Newsletter
October, 2015 Next Meeting: Monday, Oct. 12th at 7pm at the HRPO Lunar Eclipse on Sept 27th, 2015. Image by BRAS member David Leadingham, one of the few that got a clear view for a couple of minutes through the clouds in our area! Click on the pic for more info on upcoming eclipses What's In This Issue? President's Message AstroShort: Simulating the Universe Secretary's Summary of Sept. Meeting Message From the HRPO Recent BRAS Forum Entries 20/20 Vision Campaign Observing Notes by John Nagle (He's Back!) President's Message “Astronomy is useful because it raises us above ourselves; it is useful because it is grand. It shows us how small is man’s body, how great his mind, since his intelligence can embrace the whole of this dazzling immensity, where his body is only an obscure point, and enjoy its silent harmony." – Henri Poincare, 19th Century mathematician and physicist We all have our reasons for being involved in astronomy. That quote elegantly expresses just one man’s thoughts. What attracted you to astronomy? What do you tell people who ask? I think we all have experienced some indefinable draw to the night sky and the wonders of the universe. Maybe that is it. Wonder. At least for me it is. Wonder, beauty, harmony, perspective. Where does it end? Think about those things and let me know if you have something about that you would like to say at our next meeting. Alternately, you could write up something for this newsletter. Well the total lunar eclipse certainly was a washout. -
Macrocosmo Nº24
A PRIMEIRA REVISTA ELETRÔNICA BRASILEIRA EXCLUSIVA DE ASTRONOMIA macroCOSMO .com ISSN 1808-0731 Ano II - Edição n° 24 - Novembro de 2005 Eclipse Anular 3 de outubro de 2005 O O ^^Q uando a W Lua S o l oculta o w l Cratera de Colônia 25 anos da Aspectos Gerais The Planetary Society revista macroCOSMO .com Ano II - Edição n° 24 - Novembro de 2005 Editorial Redação [email protected] Assim como tantos outros fenômenos naturais, para as primeiras civilizações, os eclipses já foram atribuídos à sinais de múltiplas Diretor Editor Chefe divindades. Eclipses Solares e Lunares, eventos estes repentinos que Hemerson Brandão quebravam a imutabilidade do céu, eram interpretados como [email protected] manifestações de ira dos deuses, predizendo morte de chefes de estado, grandes catástrofes, guerras, e várias pragas. Diagramadores Mesmo nos dias de hoje, com toda a tecnologia e conhecimento Hemerson Brandão adquirido é comum pessoas ficarem receosas com o desaparecimento [email protected] repentino temporário do Sol ou da Lua. Exemplo disso são alguns cristãos Rodolfo Saccani fanáticos, que afirmam que os eclipses são indícios do “fim do mundo”. [email protected] Durante a história, enquanto alguns povos nômades cultivavam um Sharon Camargo temor mítico por esses fenômenos, povos sedentários se empenhavam [email protected] em entender sobre a periodicidade desses fenômenos raros, tentando encontrar padrões que permitissem a previsão dos eclipses. Para isso, Revisão muitos povos erigiram grandes templos e observatórios para estudo e Tasso Napoleão previsão de eclipses além de outros fenômenos celestes. Há quem afirme [email protected] que as pedras megalíticas de Stonehenge, nas ilhas britânicas, estão Walkiria Schulz dispostas numa posição que permitia ao povo que o construiu, prever [email protected] eclipses, há mais de 3700 anos. -
C Curves for Contact Binaries in the Kepler Catalog
The Behavior of 0 - C Curves for Contact Binaries in the Kepler Catalog by Kathy Tran Submitted to the Department of Physics in partial fulfillment of the requirements for the degree of ARCHVES Bachelor of Science in Physics H INSTI UE /i""L HNOLOGY at the SEP 0 4 2013 MASSACHUSETTS INSTITUTE OF TECHNOLOGY :,!R)ARIES June 2013 ©Massachusetts Institute of Technology 2013. All rights reserved. Author ................. ........................ Department of Physics May 17, 2013 Certified by..... ... .. ..... ..... .S .a.. ...... ...... ...... .... Saul A. Rappaport Professor Emeritus Thesis Supervisor A ccepted by .................. .... ............................... Nergis Mavalvala Thesis Coordinator 2 The Behavior of 0 - C Curves for Contact Binaries in the Kepler Catalog by Kathy Tran Submitted to the Department of Physics on May 17, 2013, in partial fulfillment of the requirements for the degree of Bachelor of Science in Physics Abstract In this thesis, we study the timing of eclipses for contact binary systems in the Ke- pler catalog. Observed eclipse times were determined from Kepler long-cadence light curves and "observed minus calculated" (0 - C) curves were generated for both pri- mary and secondary eclipses of the contact binary systems. We found the 0 - C curves of contact binaries to be clearly distinctive from the curves of other binaries. The key characteristics of these curves are random-walk like variations, with typical semi-amplitudes of 200 to 300 seconds, quasi-periodicities, and anti-correlated behav- ior between the curves of the primary and secondary eclipses. We performed a formal analysis of systems with dominant anti-correlated behavior, calculating correlation coefficients as low as -0.77, with a mean value of -0.42. -
Detection and Characterization of Io's Atmosphere from High
Detection and characterization of Io’s atmosphere from high-resolution 4-µm spectroscopy E. Lellouch1, M. Ali-Dib1,2, K.-L. Jessup3, A. Smette4, H.-U. Käufl4, and F. Marchis5 1Laboratoire d’Études Spatiales et d’Instrumentation en Astrophysique (LESIA), Observatoire de Paris, CNRS, UPMC, Université Paris Diderot, F-92195 Meudon, France ; [email protected] 2Institut UTINAM, CNRS/INSU, Université de Franche-Comté, UMR 6213, Observatoire de Besançon, BP 1615, F-25010, Besançon Cedex, France 3 Dept. Space Studies, Southwest Research Institute, 1050 Walnut St., Suite 300, Boulder, CO 80302, United States 4European Southern Observatory (ESO), Karl-Schwarzschildst. 2, D-85748 Garching, Germany 5SETI Institute, 189 Bernardo Av, Mountain View CA, USA. Icarus, in press. Abstract We report on high-resolution and spatially-resolved spectra of Io in the 4.0 µm region, recorded with the VLT/CRIRES instrument in 2008 and 2010, which provide the first detection of the 1+3 band of SO2 in Io’s atmosphere. Data are analyzed to constrain the latitudinal, longitudinal, and diurnal distribution of Io’s SO2 atmosphere as well as its characteristic temperature. equatorial SO2 column densities clearly show longitudinal 17 -2 asymmetry, but with a maximum of ~1.5x10 cm at central meridian longitude L = 200-220 16 -2 and a minimum of ~3x10 cm at L = 285-300, the longitudinal pattern somewhat differs from earlier inferences from Ly α and thermal IR measurements. Within the accuracy of the measurements, no evolution of the atmospheric density from mid-2008 to mid-2010 can be distinguished. The decrease of the SO2 column density towards high latitude is apparent, and the typical latitudinal extent of the atmosphere found to be ±40° at half-maximum.