Don't Forget the Grazers! Don Mccarthy February 8, 2014
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Major Meteor Showers Throughout the Year
Major Meteor Showers Throughout the Year Courtesy of The Catawba Valley Astronomy Club - www.catawbasky.org Information taken from http://www.amsmeteors.org/showers.html The meteor showers discussed below recur each year; in some cases they have been recognized for hundreds of years. The name of the shower in most cases indicates the constellation from which the meteors appear. Sporadic meteors are those random meteors not associated with a particular shower; they are the random detritus left over from the creation of the solar system or are old dispersed debris not recognizable today as shower meteors. For meteor observers, those located in the northern hemisphere have a distinct advantage as shower activity is stronger there than that seen by observers located south of the equator. The reason for this is that most of the major showers have meteors that strike the Earth in areas located far above the equator. As seen from the northern hemisphere these meteors would appear to rain down from high in the sky in all directions. The year begins with the intense but brief Quadrantid maximum (January 3/4). Its brevity combined with typically poor winter weather hampers observation. January overall has good meteor rates restricted to the last third of the night. Rates to 20/hour can be obtained. A large number of radiants spread along the ecliptic from Cancer to Virgo. This activity diminishes somewhat in February with the same areas active. Late-night rates are fair in the first half of March, but become poor rather suddenly after mid-March. The very poor rates, seldom reaching 10/hour, continue into early June. -
Teachers' Guide to Meteor Showers Leonids Meteor Shower
Education and Public Outreach Look Up! Event Guides Teachers’ Guide to Meteor Showers Leonids Meteor Shower - November 17/18, 2015 What is a meteor shower? A meteor shower is a predictable celestial event in which a relatively large number of meteors streak across the sky on a given night or series of nights. Meteor showers appear to originate from one point (called the radiant) in the night sky, often a constellation. Meteor showers get their name from the constellation from which they appear to originate. Meteor showers are caused by debris called meteoroids entering Earth’s atmosphere at extremely high speeds. This debris usually comes from comets that intersect Earth’s orbit. As Earth orbits the Sun, it collides with the debris left by passing comets and the result are meteors streaking through Earth’s atmosphere. Most meteors are smaller than a grain of sand, so almost all of them disintegrate before having a chance to hit the ground. In 2015, the annual Leonid meteor shower will peak the night of November 17/18. The Leonids are so named because they appear to originate from the constellation of Leo (the lion). The debris responsible for the Leonids comes from the comet Tempel- Tuttle. It is possible to view about 20 meteors in one hour at the peak of the Leonids meteor shower. Upcoming Events Find information and resources about upcoming celestial events and NASA mission milestones to share with your students at http://www.lpi.usra.edu/education/look_up. Meteor Showers/Comets in Your Classroom! Use the resources below to enable your students to explore meteor showers. -
Meteor Showers' Activity and Forecasting
Meteoroids 2007 – Barcelona, June 11-15 About the cover: The recent fall of the Villalbeto de la Peña meteorite on January 4, 2004 (Spain) is one of the best documented in history for which atmospheric and orbital trajectory, strewn field area, and recovery circumstances have been described in detail. Photometric and seismic measurements together with radioisotopic analysis of several recovered specimens suggest an original mass of about 760 kg. About fifty specimens were recovered from a strewn field of nearly 100 km2. Villalbeto de la Peña is a moderately shocked (S4) equilibrated ordinary chondrite (L6) with a cosmic-ray-exposure age of 48±5 Ma. The chemistry and mineralogy of this genuine meteorite has been characterized in detail by bulk chemical analysis, electron microprobe, electron microscopy, magnetism, porosimetry, X-ray diffraction, infrared, Raman, and 57Mössbauer spectroscopies. The picture of the fireball was taken by M.M. Ruiz and was awarded by the contest organized by the Spanish Fireball Network (SPMN) for the best photograph of the event. The Moon is also visible for comparison. The picture of the meteorite was taken as it was found by the SPMN recovery team few days after the fall. 2 Meteoroids 2007 – Barcelona, June 11-15 FINAL PROGRAM Monday, June 11 Auditorium conference room 9h00-9h50 Reception 9h50-10h00 Opening event Session 1: Observational Techniques and Meteor Detection Programs Morning session Session chairs: J. Borovicka and W. Edwards 10h00-10h30 Pavel Spurny (Ondrejov Observatory, Czech Republic) et al. “Fireball observations in Central Europe and Western Australia – instruments, methods and results” (invited) 10h30-10h45 Josep M. -
The Leonid Meteor Shower: Historical Visual Observations
Icarus 138, 287–308 (1999) Article ID icar.1998.6074, available online at http://www.idealibrary.com on The Leonid Meteor Shower: Historical Visual Observations P. Brown Department of Physics and Astronomy, University of Western Ontario, London, Ontario, N6A 3K7, Canada E-mail: [email protected] Received July 20, 1998; revised December 10, 1998 of past showers, independent of the many secondary accounts The original visual accounts of the Leonids from 1799 to 1997 which appear in the literature, in an effort to better understand are examined and the times and magnitude of peak activity are the stream’s past activity, its formation, and as a way to predict established for 32 Leonid returns during this two-century interval. what may happen in the years from 1999 onwards. In addition, Previous secondary accounts of many of these returns are shown this revised set of historical Leonid data provides a set of obser- to differ from the information contained in the original accounts vations reduced in a common manner, which any model of the due to misinterpretations, typographical errors, and unsupported stream must be able to explain and to which others can easily assumptions. The strongest Leonid storms are shown to follow a examine and apply their own corrections. Gaussian activity profile and to occur after the perihelion passage In this work, we examine in detail available original records and nodal longitude of 55P/Tempel–Tuttle. The relationship be- tween the Gaussian width of the strongest returns and their peak of the Leonids for modern returns of the shower (here defined activity is established, and the particle density/stream width rela- to be post-1799). -
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 -
7 X 11 Long.P65
Cambridge University Press 978-0-521-85349-1 - Meteor Showers and their Parent Comets Peter Jenniskens Index More information Index a – semimajor axis 58 twin shower 440 A – albedo 111, 586 fragmentation index 444 A1 – radial nongravitational force 15 meteoroid density 444 A2 – transverse, in plane, nongravitational force 15 potential parent bodies 448–453 A3 – transverse, out of plane, nongravitational a-Centaurids 347–348 force 15 1980 outburst 348 A2 – effect 239 a-Circinids (1977) 198 ablation 595 predictions 617 ablation coefficient 595 a-Lyncids (1971) 198 carbonaceous chondrite 521 predictions 617 cometary matter 521 a-Monocerotids 183 ordinary chondrite 521 1925 outburst 183 absolute magnitude 592 1935 outburst 183 accretion 86 1985 outburst 183 hierarchical 86 1995 peak rate 188 activity comets, decrease with distance from Sun 1995 activity profile 188 Halley-type comets 100 activity 186 Jupiter-family comets 100 w 186 activity curve meteor shower 236, 567 dust trail width 188 air density at meteor layer 43 lack of sodium 190 airborne astronomy 161 meteoroid density 190 1899 Leonids 161 orbital period 188 1933 Leonids 162 predictions 617 1946 Draconids 165 upper mass cut-off 188 1972 Draconids 167 a-Pyxidids (1979) 199 1976 Quadrantids 167 predictions 617 1998 Leonids 221–227 a-Scorpiids 511 1999 Leonids 233–236 a-Virginids 503 2000 Leonids 240 particle density 503 2001 Leonids 244 amorphous water ice 22 2002 Leonids 248 Andromedids 153–155, 380–384 airglow 45 1872 storm 380–384 albedo (A) 16, 586 1885 storm 380–384 comet 16 1899 -
Events: No General Meeting in April
The monthly newsletter of the Temecula Valley Astronomers Apr 2020 Events: No General Meeting in April. Until we can resume our monthly meetings, you can still interact with your astronomy associates on Facebook or by posting a message to our mailing list. General information: Subscription to the TVA is included in the annual $25 membership (regular members) donation ($9 student; $35 family). President: Mark Baker 951-691-0101 WHAT’S INSIDE THIS MONTH: <[email protected]> Vice President: Sam Pitts <[email protected]> Cosmic Comments Past President: John Garrett <[email protected]> by President Mark Baker Treasurer: Curtis Croulet <[email protected]> Looking Up Redux Secretary: Deborah Baker <[email protected]> Club Librarian: Vacant compiled by Clark Williams Facebook: Tim Deardorff <[email protected]> Darkness – Part III Star Party Coordinator and Outreach: Deborah Baker by Mark DiVecchio <[email protected]> Hubble at 30: Three Decades of Cosmic Discovery Address renewals or other correspondence to: Temecula Valley Astronomers by David Prosper PO Box 1292 Murrieta, CA 92564 Send newsletter submissions to Mark DiVecchio th <[email protected]> by the 20 of the month for Members’ Mailing List: the next month's issue. [email protected] Website: http://www.temeculavalleyastronomers.com/ Like us on Facebook Page 1 of 18 The monthly newsletter of the Temecula Valley Astronomers Apr 2020 Cosmic Comments by President Mark Baker One of the things commonly overlooked about Space related Missions is time, and of course, timing…!!! Many programs take a decade just to get them in place and off the ground, and many can take twice that long…just look at the James Webb Telescope!!! So there’s the “time” aspect of such endeavors…what about timing?? I mentioned last month that July is looking like a busy month for Martian Missions… here’s a refresher: 1) The NASA Mars 2020 rover Perseverance and its helicopter drone companion (aka Lone Ranger and Tonto, as I called them) is still on schedule. -
Backyard Astronomy Santa Fe Public Library
Backyard Astronomy Santa Fe Public Library Photo Credit: NASA, A Mess of Stars,08-10-2015 1. What will you need? 2. What am I looking at? 3. What you can See a. August 2020 b. September 2020 c. October 2020 4. Star Stories 5. Activities a. Tracking the Sunset/Sunrise b. Moon Watching c. Tracking the International Space Station d. Constellation Discovery 6. What to Read Backyard Astronomy Santa Fe Public Library What will you need? The most important things you will need are your curiosity, your naked eyes, and the ability to observe. You do not need fancy telescopes to begin enjoying the wonders of our amazing night skies. Here in Northern New Mexico, we are blessed with the ability to step out of our homes, look up, and see the Milky Way displayed above us without too much obstruction. Photo Credit: NASA, A Glimpse of the Milky Way, 12-13-2005 While the following Items can help you to begin exploring the wonders of the Universe, they are not required. These items include: 1. Binoculars 2. Telescope (a small inexpensive one is fine) 3. Star Chart Planisphere 4. Free Astronomy Apps for both iPhones and Androids There are several really good free apps that help you identify, locate, and track celestial objects. One that I use is Star Walk 2 but there are other good apps available. Backyard Astronomy Santa Fe Public Library What am I looking at? When you look up at night, what do you see? Probably more than you think! Below is a list of the Celestial Items you can see. -
For the Love of Meteors by Cathy L
For the Love of Meteors by Cathy L. Hall, Kingston Centre ([email protected]) November 17/18, 1999 igh in the mountains above Malaga, Spain, far above the Hbeaches of the Costa Del Sol, eight meteor observers from several continents were treated to a memorable display of Leonid meteors. The group included Jürgen Rendtel, Manuela Trenn, Rainer Arlt, Sirko Molau, and Ralf Koschack from Germany, Robert Lunsford from California, and Pierre Martin and myself from Canada. Further east, another group of Canadians, Les MacDonald, Joe Dafoe, and Gwen Hoover, observed from northern Cyprus. Over the course of more than five hours that night, those of us in southern Spain recorded an incredible number of meteors, with most of us seeing between 1,000 and 2,000 Leonids. The group in Cyprus was Left to right: Robert Lundsford of San Diego, California (IMO Secretary-General and AMS Visual hindered by cloud, but was still delighted Program Co-ordinator), the author, Pierre Martin of Orleans, Ontario (Ottawa Centre’s Meteor Co- with the Leonids’ performance. ordinator), and Sirko Molau of Aachen, Germany (IMO Video Commission Director). The photo was It was a beautiful display in the taken at the Berlin Observatory prior to flying to southern Spain to observe the Leonids. mountains over Malaga. The meteors and comets I have seen over the years have mountains as the Leonids started to fall. like soft notes on a flute. There would be always been very personal things. I like The earliest Leonid meteors were a a brief lull, followed by another tiny burst to enjoy them alone, if possible. -
Radio Echo Observations of Meteors in the Southern Hemisphere
RADIO ECHO OBSERVATIONS OF METEORS IN THE SOUTHERN HEMISPHERE By A. A. WEISS* [Manuscript received September 20, 1954] Summary The results of a radio survey of meteor activity at Adelaide are presented. The radiants and activities of six major meteor showers (Geminids, day-time Arietids, ~-Perseids, a-Aquarids, Corona Australids, Orionids) have been measured by methods which are described, and the mass distributions in three of these showers are discussed. Seasonal and diurnal variations in the background activity of sporadic meteors are examined in relation to the radiation patterns of the aerial systems_ Height distribut.ions for meteors of three showers (Geminids, day-time Arietids, ~-Perseids) are given. Diurnal variations in the height distribution of sporadic meteors do not conform to those expected from the motion of the apex of the Earth's way. I. INTRODUCTION The successful application, at the Jodrell Bank Experimental Station of the University of Manchester, of radio echo techniques to the continuous monitoring of meteor activity in the northern hemisphere, prompted the initiation ()f a complementary survey in the southern hemisphere. Up to the time of (lommencement of this survey lists of southern hemisphere visual observations had been published by McIntosh and by Hoffmeister, and McIntosh (1935) had compiled" An Index to Southern Meteor Showers" which lists 320 radiants visible at mid-southern latitudes. These visual observations have since been supplemented by radio echo observations on the a-Aquarid shower by Hawkins and Almond (1952) and by Lindblad (1952). Although it is certain that all major southern night-time showers have been detected by the visual workers, the cover in the months September to March is not altogether satisfactory (McIntosh 1935). -
Multi-Instrumental Observations of the 2014 Ursid Meteor Outburst
Multi‐instrumental observations of the 2014 Ursid meteor outburst Monthly Notices of the Royal Astronomical Society, Volume 468, Issue 2, p.2206‐2213 Manuel Moreno‐Ibáñez, Josep Ma. Trigo‐Rodríguez, José María Madiedo, Jérémie Vaubaillon, Iwan P. Williams, Maria Gritsevich, Lorenzo G. Morillas, Estefanía Blanch, Pep Pujols, François Colas, Philippe Dupouy ‐ Instituto de Ciencias del Espacio ‐ 2014 Ursid meteor shower 1. Introduction Why so poor work on the Ursids? Why so poor work on the Ursids? • Similar date than Geminids, which • Similar date than Geminids, which are are more predictable and more predictable and numerous. numerous. • Usually low ZHR? (<10) • Usually low ZHR (<10) • Bad weather conditions in mid‐ • Bad weather conditions in mid‐ December. December. Any explanation? Why are they interesting? • ZHR > 100 when the comet is • Mean motion resonances. at its aphelion. • The meteor swarms detached during • This increase occurs each 13.6 certain years evolve to a different orbit an years approx. get trapped in a 7:6 resonance with • Annual shower? also increases Jupiter=> Period ?roughly fixed. remarkably when the comet is • T swarm/ T comet = 1,011 => In around 45 at its perihelion but not or 46 orbits the comet and the swarm are always. out of phase. 2 2014 Ursid meteor shower 1. Introduction Who is their parent body? Why so poor work on the Ursids? • Comet 8P/Tuttle (Ceplecha (1951)) • Similar date than Geminids, which are • Jupiter Family more predictable and numerous. • Trapped in a 15:13 resonance with • Usually low ZHR (<10) Jupiter => T~13.6 yr. • Bad weather conditions in mid‐ • Aphelion: 10 AU. -
Librarians' Guide to Meteor Showers Leonids Meteor Shower
Education and Public Outreach Look Up! Event Guides Librarians’ Guide to Meteor Showers Leonids Meteor Shower - November 17/18, 2015 What is a meteor shower? A meteor shower is a predictable celestial event in which a relatively large number of meteors streak across the sky on a given night or series of nights. Meteor showers appear to originate from one point (called the radiant) in the night sky, often a constellation. Meteor showers get their name from the constellation from which they appear to originate. Meteor showers are caused by debris called meteoroids entering Earth’s atmosphere at extremely high speeds. This debris usually comes from comets that intersect Earth’s orbit. As Earth orbits the Sun, it collides with the debris left by passing comets and the result are meteors streaking through Earth’s atmosphere. Most meteors are smaller than a grain of sand, so almost all of them disintegrate before having a chance to hit the ground. In 2015, the annual Leonid meteor shower will peak the night of November 17/18. The Leonids are so named because they appear to originate from the constellation of Leo (the lion). The debris responsible for the Leonids comes from the comet Tempel- Tuttle. It is possible to view about 20 meteors in one hour at the peak of the Leonids meteor shower. Upcoming Events Find information and resources about upcoming celestial events and NASA mission milestones to share with your child at http://www.lpi.usra.edu/education/look_up. night sky http://www.lpi.usra.edu/education/look_up @earthskyscience Meteor Showers/Comets in Your Library! Use the resources below to create a program for your patrons to explore meteor showers.