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Spring 2008 (PDF)
SKYWARNEWS National Weather Service State College, PA Spring/Summer 2008 “Working Together To Save Lives” The Cooperative Observers meteorological data in near real-time, to support forecast, warning and other public – Creators of Our service programs of the National Weather Country’s Weather History Service. By Victor Cruz, Observation Program Volunteers in the Cooperative Program are Leader trained by National Weather Service personnel and receive the equipment to And so, my fellow Americans: ask not perform their duties. In Central what your country can do for you—ask Pennsylvania, the oldest and longest what you can do for your country. The continuous Cooperative Program is located aforementioned sentence was uttered by in Lancaster County. The City of Lancaster President John F. Kennedy during his Filter Plant has been a cooperative weather Inaugural Address on January 20, 1961. site since May 01, 1887. Our newest However, long before President Kennedy Cooperative Observer is in Chandler’s had spoken those words, the Cooperative Valley, which was established on June 19, Weather Observer Program had been in 2004. Approximately 115 cooperative full swing, since its creation in 1890 under observers help to maintain the Cooperative the Organic Act. Observer Program in Central Pennsylvania. The National Weather Service (NWS) Everyday more than 12,000 weather Cooperative Observer Program (COOP) is volunteers take cooperative observations truly the Nation's weather and climate on farms, at homes in urban and suburban observing network of, by and for the areas, National Parks, seashores, and people. mountaintops. The data they collect are an invaluable measurement of atmospheric The basic equipment for most new Coop conditions where people live, work and Stations is a Standard Rain Gage, play. -
BRAS Newsletter August 2013
www.brastro.org August 2013 Next meeting Aug 12th 7:00PM at the HRPO Dark Site Observing Dates: Primary on Aug. 3rd, Secondary on Aug. 10th Photo credit: Saturn taken on 20” OGS + Orion Starshoot - Ben Toman 1 What's in this issue: PRESIDENT'S MESSAGE....................................................................................................................3 NOTES FROM THE VICE PRESIDENT ............................................................................................4 MESSAGE FROM THE HRPO …....................................................................................................5 MONTHLY OBSERVING NOTES ....................................................................................................6 OUTREACH CHAIRPERSON’S NOTES .........................................................................................13 MEMBERSHIP APPLICATION .......................................................................................................14 2 PRESIDENT'S MESSAGE Hi Everyone, I hope you’ve been having a great Summer so far and had luck beating the heat as much as possible. The weather sure hasn’t been cooperative for observing, though! First I have a pretty cool announcement. Thanks to the efforts of club member Walt Cooney, there are 5 newly named asteroids in the sky. (53256) Sinitiere - Named for former BRAS Treasurer Bob Sinitiere (74439) Brenden - Named for founding member Craig Brenden (85878) Guzik - Named for LSU professor T. Greg Guzik (101722) Pursell - Named for founding member Wally Pursell -
Obdelava Slik
PROJEKTNA NALOGA ASTRONOMIJA Magnituda Rimske ceste Avtorji: Matic Ocepek Jernej Cucek Goran Bezjak Bernard Pavlovič Nikola Milijevski Mentor: prof. dr. Andrej Čadež Fakulteta za matematiko in fiziko, 2010 Projektna naloga astronomija: Magnituda Rimske ceste KAZALO UVOD ........................................................................................................................................ 3 KAKO DO FOTOGRAFIJ IN KAJ Z NJIMI ............................................................................ 4 IZPELJAVA ENAČBE .............................................................................................................. 5 IZRAČUNI IN REZULTATI..................................................................................................... 9 NAPAKE .................................................................................................................................. 15 ZAKLJUČEK ........................................................................................................................... 17 VIRI .......................................................................................................................................... 18 2 Projektna naloga astronomija: Magnituda Rimske ceste UVOD Rimska ali Mlečna cesta je megličast pas bele svetlobe sestavljen iz okoli 200 milijard zvezd, ki je ob jasnih nočeh viden na nočnem nebu in se vije po celotni nebesni sferi. Sestavljajo jo zvezde, zvezdni prah in plini v galaktični ravnini, ki je glede na nebesni ekvator nagnjena okoli 63 stopinj -
Meteor Shower Detection with Density-Based Clustering
Meteor Shower Detection with Density-Based Clustering Glenn Sugar1*, Althea Moorhead2, Peter Brown3, and William Cooke2 1Department of Aeronautics and Astronautics, Stanford University, Stanford, CA 94305 2NASA Meteoroid Environment Office, Marshall Space Flight Center, Huntsville, AL, 35812 3Department of Physics and Astronomy, The University of Western Ontario, London N6A3K7, Canada *Corresponding author, E-mail: [email protected] Abstract We present a new method to detect meteor showers using the Density-Based Spatial Clustering of Applications with Noise algorithm (DBSCAN; Ester et al. 1996). DBSCAN is a modern cluster detection algorithm that is well suited to the problem of extracting meteor showers from all-sky camera data because of its ability to efficiently extract clusters of different shapes and sizes from large datasets. We apply this shower detection algorithm on a dataset that contains 25,885 meteor trajectories and orbits obtained from the NASA All-Sky Fireball Network and the Southern Ontario Meteor Network (SOMN). Using a distance metric based on solar longitude, geocentric velocity, and Sun-centered ecliptic radiant, we find 25 strong cluster detections and 6 weak detections in the data, all of which are good matches to known showers. We include measurement errors in our analysis to quantify the reliability of cluster occurrence and the probability that each meteor belongs to a given cluster. We validate our method through false positive/negative analysis and with a comparison to an established shower detection algorithm. 1. Introduction A meteor shower and its stream is implicitly defined to be a group of meteoroids moving in similar orbits sharing a common parentage. -
Meteor Showers # 11.Pptx
20-05-31 Meteor Showers Adolf Vollmy Sources of Meteors • Comets • Asteroids • Reentering debris C/2019 Y4 Atlas Brett Hardy 1 20-05-31 Terminology • Meteoroid • Meteor • Meteorite • Fireball • Bolide • Sporadic • Meteor Shower • Meteor Storm Meteors in Our Atmosphere • Mesosphere • Atmospheric heating • Radiant • Zenithal Hourly Rate (ZHR) 2 20-05-31 Equipment Lounge chair Blanket or sleeping bag Hot beverage Bug repellant - ThermaCELL Camera & tripod Tracking Viewing Considerations • Preparation ! Locate constellation ! Take a nap and set alarm ! Practice photography • Location: dark & unobstructed • Time: midnight to dawn https://earthsky.org/astronomy- essentials/earthskys-meteor-shower- guide https://www.amsmeteors.org/meteor- showers/meteor-shower-calendar/ • Where to look: 50° up & 45-60° from radiant • Challenges: fatigue, cold, insects, Moon • Recording observations ! Sky map, pen, red light & clipboard ! Time, position & location ! Recording device & time piece • Binoculars Getty 3 20-05-31 Meteor Showers • 112 confirmed meteor showers • 695 awaiting confirmation • Naming Convention ! C/2019 Y4 (Atlas) ! (3200) Phaethon June Tau Herculids (m) Parent body: 73P/Schwassmann-Wachmann Peak: June 2 – ZHR = 3 Slow moving – 15 km/s Moon: Waning Gibbous June Bootids (m) Parent body: 7p/Pons-Winnecke Peak: June 27– ZHR = variable Slow moving – 14 km/s Moon: Waxing Crescent Perseid by Brian Colville 4 20-05-31 July Delta Aquarids Parent body: 96P/Machholz Peak: July 28 – ZHR = 20 Intermediate moving – 41 km/s Moon: Waxing Gibbous Alpha -
Binocular Double Star Logbook
Astronomical League Binocular Double Star Club Logbook 1 Table of Contents Alpha Cassiopeiae 3 14 Canis Minoris Sh 251 (Oph) Psi 1 Piscium* F Hydrae Psi 1 & 2 Draconis* 37 Ceti Iota Cancri* 10 Σ2273 (Dra) Phi Cassiopeiae 27 Hydrae 40 & 41 Draconis* 93 (Rho) & 94 Piscium Tau 1 Hydrae 67 Ophiuchi 17 Chi Ceti 35 & 36 (Zeta) Leonis 39 Draconis 56 Andromedae 4 42 Leonis Minoris Epsilon 1 & 2 Lyrae* (U) 14 Arietis Σ1474 (Hya) Zeta 1 & 2 Lyrae* 59 Andromedae Alpha Ursae Majoris 11 Beta Lyrae* 15 Trianguli Delta Leonis Delta 1 & 2 Lyrae 33 Arietis 83 Leonis Theta Serpentis* 18 19 Tauri Tau Leonis 15 Aquilae 21 & 22 Tauri 5 93 Leonis OΣΣ178 (Aql) Eta Tauri 65 Ursae Majoris 28 Aquilae Phi Tauri 67 Ursae Majoris 12 6 (Alpha) & 8 Vul 62 Tauri 12 Comae Berenices Beta Cygni* Kappa 1 & 2 Tauri 17 Comae Berenices Epsilon Sagittae 19 Theta 1 & 2 Tauri 5 (Kappa) & 6 Draconis 54 Sagittarii 57 Persei 6 32 Camelopardalis* 16 Cygni 88 Tauri Σ1740 (Vir) 57 Aquilae Sigma 1 & 2 Tauri 79 (Zeta) & 80 Ursae Maj* 13 15 Sagittae Tau Tauri 70 Virginis Theta Sagittae 62 Eridani Iota Bootis* O1 (30 & 31) Cyg* 20 Beta Camelopardalis Σ1850 (Boo) 29 Cygni 11 & 12 Camelopardalis 7 Alpha Librae* Alpha 1 & 2 Capricorni* Delta Orionis* Delta Bootis* Beta 1 & 2 Capricorni* 42 & 45 Orionis Mu 1 & 2 Bootis* 14 75 Draconis Theta 2 Orionis* Omega 1 & 2 Scorpii Rho Capricorni Gamma Leporis* Kappa Herculis Omicron Capricorni 21 35 Camelopardalis ?? Nu Scorpii S 752 (Delphinus) 5 Lyncis 8 Nu 1 & 2 Coronae Borealis 48 Cygni Nu Geminorum Rho Ophiuchi 61 Cygni* 20 Geminorum 16 & 17 Draconis* 15 5 (Gamma) & 6 Equulei Zeta Geminorum 36 & 37 Herculis 79 Cygni h 3945 (CMa) Mu 1 & 2 Scorpii Mu Cygni 22 19 Lyncis* Zeta 1 & 2 Scorpii Epsilon Pegasi* Eta Canis Majoris 9 Σ133 (Her) Pi 1 & 2 Pegasi Δ 47 (CMa) 36 Ophiuchi* 33 Pegasi 64 & 65 Geminorum Nu 1 & 2 Draconis* 16 35 Pegasi Knt 4 (Pup) 53 Ophiuchi Delta Cephei* (U) The 28 stars with asterisks are also required for the regular AL Double Star Club. -
A Guide to Smartphone Astrophotography National Aeronautics and Space Administration
National Aeronautics and Space Administration A Guide to Smartphone Astrophotography National Aeronautics and Space Administration A Guide to Smartphone Astrophotography A Guide to Smartphone Astrophotography Dr. Sten Odenwald NASA Space Science Education Consortium Goddard Space Flight Center Greenbelt, Maryland Cover designs and editing by Abbey Interrante Cover illustrations Front: Aurora (Elizabeth Macdonald), moon (Spencer Collins), star trails (Donald Noor), Orion nebula (Christian Harris), solar eclipse (Christopher Jones), Milky Way (Shun-Chia Yang), satellite streaks (Stanislav Kaniansky),sunspot (Michael Seeboerger-Weichselbaum),sun dogs (Billy Heather). Back: Milky Way (Gabriel Clark) Two front cover designs are provided with this book. To conserve toner, begin document printing with the second cover. This product is supported by NASA under cooperative agreement number NNH15ZDA004C. [1] Table of Contents Introduction.................................................................................................................................................... 5 How to use this book ..................................................................................................................................... 9 1.0 Light Pollution ....................................................................................................................................... 12 2.0 Cameras ................................................................................................................................................ -
The 2019 Meteor Shower Activity Forecast for Low Earth Orbit 1 Overview
NASA METEOROID ENVIRONMENT OFFICE The 2019 meteor shower activity forecast for low Earth orbit Issued 15 October 2018 The purpose of this document is to provide a forecast of major meteor shower activity in low Earth orbit. Several meteor showers – the Draconids, Perseids, eta Aquariids, Orionids, and potentially the Androme- dids – are predicted to exhibit increased rates in 2019. However, no storms (meteor showers with visual rates exceeding 1000 [1, 2]) are predicted. 1 Overview Both the MSFC stream model [3] and the Egal et al. Draconid model [4] predict a second Draconid outburst in 2019. The 2019 Draconids are expected to have nearly the same level of activity as the 2018 Draconids, which reached a zenithal hourly rate (or ZHR) of about 100. Twin outbursts also occurred in 2011 and 2012 [5, 6]. The Perseids, eta Aquariids, and Orionids are expected to show mild enhancements over their baseline activity level in 2019. The Perseids are expected to be slightly more active in 2019 than in 2018, with a peak ZHR around 112. The eta Aquariids and Orionids, which belong to a single meteoroid stream generated by comet 1P/Halley, are thought to have a 12-year activity cycle and are currently increasing in activity from year to year. A review of eta Aquariid literature [7, 8, 9, 10] also indicates that the overall activity level is higher than previously believed, and this is reflected in higher forecasted rates (a ZHR of 75) and fluxes for this shower. We may see enhanced beta Taurid activity in 2019. The beta Taurids are part of the same stream as the Northern and Southern Taurids but produce daytime meteors. -
Symposium on Telescope Science
Proceedings for the 26th Annual Conference of the Society for Astronomical Sciences Symposium on Telescope Science Editors: Brian D. Warner Jerry Foote David A. Kenyon Dale Mais May 22-24, 2007 Northwoods Resort, Big Bear Lake, CA Reprints of Papers Distribution of reprints of papers by any author of a given paper, either before or after the publication of the proceedings is allowed under the following guidelines. 1. The copyright remains with the author(s). 2. Under no circumstances may anyone other than the author(s) of a paper distribute a reprint without the express written permission of all author(s) of the paper. 3. Limited excerpts may be used in a review of the reprint as long as the inclusion of the excerpts is NOT used to make or imply an endorsement by the Society for Astronomical Sciences of any product or service. Notice The preceding “Reprint of Papers” supersedes the one that appeared in the original print version Disclaimer The acceptance of a paper for the SAS proceedings can not be used to imply or infer an endorsement by the Society for Astronomical Sciences of any product, service, or method mentioned in the paper. Published by the Society for Astronomical Sciences, Inc. First printed: May 2007 ISBN: 0-9714693-6-9 Table of Contents Table of Contents PREFACE 7 CONFERENCE SPONSORS 9 Submitted Papers THE OLIN EGGEN PROJECT ARNE HENDEN 13 AMATEUR AND PROFESSIONAL ASTRONOMER COLLABORATION EXOPLANET RESEARCH PROGRAMS AND TECHNIQUES RON BISSINGER 17 EXOPLANET OBSERVING TIPS BRUCE L. GARY 23 STUDY OF CEPHEID VARIABLES AS A JOINT SPECTROSCOPY PROJECT THOMAS C. -
David Levy's Guide to the Night Sky Da
Cambridge University Press 0521797535 - David Levy’s Guide to the Night Sky David H. Levy Index More information INDEX AAVSO, 200–201, 331, 332 binoculars, 57–59 absolute magnitudes, 36 Bobrovnikoff method, estimating comet Adams, John Couch, 156 brightness, 178 aetheria darkening, 138 Bode, Johann, 163 Alcock, George, 44, 185 Bode’s Law, 163–165 Algol, 325 Brahe, Tycho, 81 aligning, 67 Brasch, Klaus, 126 Alpha Capricornids, 47 Brashear, John, 60 altazimuth, 62, 65 bright nebulae, 232–233 altitude, 67 Brooks, William, 182 Amalthea, 111 Burnham, Sherbourne Wesley, 193 amateur astronomy, introduced, xvii, xviii Andromedids, 48, 49, 68 Callisto, 111, 119, 121 Antoniadi, Eugenios, 112 Carrington, Christopher, 103 aphelic oppositions, 134 Cassini spacecraft, 130 aphelion, 134 Cassini, Giovanni, 81, 124 apochromat, 60 Cassini’s Division, 124, 125 apparent magnitude, 36 CCD technology, 275–280 apparitions, of comets, 134, 135 CCDs, for astrometry, 283 Arago, Francois, 156 Celestial Police, 163–164 Ariel, 159 celestial equator, 8 ashen light, Venus, 152 Central Bureau for Astronomical Association of Lunar and Planetary Telegrams,120, 121, 186–187, 280 Observers, 331, 332 Challis, James, 156 Asteroids, 163–172 Chapman, Clark, 170 naming of, 165–166 Chaucer, Geoffrey, 318 Astronomical League, 333 chromosphere, 293 astrophotography, 262 Clark, Alvin, 60 Aurigids, 46 Clavius, Christopher, 82 Aurora, 28–33 Collins, Peter, 158, 217 Auroral Data Center in the US, 29 Coma Berenicids, 50 averted vision, 41 comets, 172–189, 294 azimuth, 67 Arend–Roland, 43 Biela, 49, 68 Baker, Lonny, xxii Bradfield, 69 Barnard, E. E. 111, 181–182 Denning–Fujikawa, 181 Beyer method, estimating comet brightness, Encke, 49, 175 179 Giacobini–Zinner, 48 Beyond the Observatory (Shapley), 35 Halley, 44, 46, 48, 55, 78, 175, 225 big bang, 65 Hartley–IRAS, 175 339 © Cambridge University Press www.cambridge.org Cambridge University Press 0521797535 - David Levy’s Guide to the Night Sky David H. -
Spectra and Physical Properties of Taurid Meteoroids
Spectra and physical properties of Taurid meteoroids Pavol Matloviˇca, Juraj T´otha, Regina Rudawskab, Leonard Kornoˇsa aFaculty of Mathematics, Physics and Informatics, Comenius University, Bratislava, Slovakia bESA European Space Research and Technology Centre, Noordwijk, Netherlands Abstract Taurids are an extensive stream of particles produced by comet 2P/Encke, which can be observed mainly in October and November as a series of me- teor showers rich in bright fireballs. Several near-Earth asteroids have also been linked with the meteoroid complex, and recently the orbits of two car- bonaceous meteorites were proposed to be related to the stream, raising interesting questions about the origin of the complex and the composition of 2P/Encke. Our aim is to investigate the nature and diversity of Taurid mete- oroids by studying their spectral, orbital, and physical properties determined from video meteor observations. Here we analyze 33 Taurid meteor spectra captured during the predicted outburst in November 2015 by stations in Slo- vakia and Chile, including 14 multi-station observations for which the orbital elements, material strength parameters, dynamic pressures, and mineralog- ical densities were determined. It was found that while orbits of the 2015 Taurids show similarities with several associated asteroids, the obtained spec- tral and physical characteristics point towards cometary origin with highly heterogeneous content. Observed spectra exhibited large dispersion of iron content and significant Na intensity in all cases. The determined material strengths are typically cometary in the KB classification, while PE criterion is on average close to values characteristic for carbonaceous bodies. The studied meteoroids were found to break up under low dynamic pressures of 0.02 - 0.10 MPa, and were characterized by low mineralogical densities of 1.3 arXiv:1704.06482v1 [astro-ph.EP] 21 Apr 2017 - 2.5 g cm-3. -
MSS30-2009.Pdf
MSS-120 (2008 年 10 月 5 日) ふたご座流星群の等級別出現数(VMDB より) 内山茂男 1. VMDB とは * IMO(国際流星機構)の収集した眼視観測データ * Visual Meteor Data Base (http://www.imo.net/data/visual) * Rate data と Mag data がある。基本的に Mag data を使用。ただし、Mag data には Teff と F が記 載されていないため、Rate data との照合が必要。 2. データ使用条件 (1) 月明かりの影響が少ない年(1993、1996、1998、1999、2001、2002、2004、2007 年) (2) 輻射点高度 25 度以上 (3) 視野遮蔽係数 F が 1.4 未満(雲量 2.9 未満) (4) 観測区分時間 2 時間以内 (5) 個人補正(最微星補正)の絶対値が 1.0 等未満 (6) 最微星 5.0 等以上 かつ 個人補正後の最微星 5.0 等以上 3. 使用データ量 年 1993 1996 1998 1999 2001 2002 2004 2007 合計 観測時間(hr) 58.8 124.9 106.5 170.6 160.1 107.0 317.7 252.9 1298.3 群流星数 4646 7206 5309 8812 8577 5473 20727 12492 73242 等級 ≦-5 -4 -3 -2 -1 0 1 2 3 4 5 流星数 165 244.5 596.5 1545.5 3377.5 6763.5 10519 14808 16651 12194 4986.5 4. 全ふたご群 ZHR 5. ローレンツ曲線 2 Wh ZHR = ZHRmax × 2 2 (T − Tmax ) +Wh 極大値 ZHRmax、極大太陽黄経 Tmax、半値半幅 Wh(極 大前 Wa と極大後 Wd)の値は、最小二乗法(誤差で 重み)で決定。 ※ 各等級の極大時刻はピークだけでなく全体の出現 状況から決定 6. 等級別 ZHR (ZHRm) 集計結果 (※ ピンクのラインは全 ZHR と同じ形で各 ZHRm の極大値に合わせたもの) Ls,max = 262.33 – 0.055・M (1 等級あたり 1.3 時間変化) Wa = 0.956 + 0.088・M Wd = 0.390 + 0.029・M FWHM= 1.347 + 0.119・M (FWHM は 1 等級あたり 2.8 時間変化) MSS-121用 観測結果 ペルセウス群輻射点拡大撮影 重野好彦 撮影日時 2008年8月11/12日 00時00分から03時32分(JST) 12/13日 00時30分から04時00分(JST) 観測地 新潟八海山 撮影機材 IIによる動画像(DV-AVI)撮影 高橋P型+ビクセンモードラ自動ガイド レンズ50mmF1.4 写野 20度×15度 撮影方向 ペルセウス座流星群輻射点 画像処理 ペルセウス群13流星(11/12)、12流星(12/13)をコンポジット 2008.08.11/12 2006.08.13/14 50mm F1.4 170mm F2.4 2008.08.12/13 50mm F1.4 !"#$%&' ()* +,-./012345 1.