Meteornews Vol 5 Issue 3 May 2020
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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 -
Five Wild Years Reminiscences of the Leonids Experience 1998 – 2002
Proceedings IMC Bollmannsruh 2003 29 Five wild years Reminiscences of the Leonids experience 1998 – 2002 Daniel Fischer K¨onigswinter, Germany Abstract This is not a scientific review of the surprises, discoveries and sensations the Leonids brought from 1998 to 2002, but a look back by one observer (and science writer) who often witnessed first-hand what went on in the sky — and also how science finally got its grip on the elusive and striking phenomenon of meteor storms. It was a truly an experience with a deep impact (no pun intended) that is not likely to be repeated... I admit it: before about ten years ago I had considered meteor observing, especially with your own eye, as one of the most useless branches of (amateur) astronomy, with no serious data reduction possible and dubious results. This was not true, at least at that time, of course (see Roggemans, 2004), but the progress made by the IMO had not been widely known to the outside world. Not in- terested at all in systematic meteor watching, I was struck by the idea of meteor storms nonetheless: I had read a lot about the fabulous Leonids storm of 1966 and eagerly devoured two big reviews of meteor storms in British journals. Beech et al (1995) had described these rare phenomena as both spectacular and little understood, while Mason (1995) predicted — using a crude model — storms of the Leonids with ZHRs around 5000 in 1998 and 1999. Would it be worth chasing after those possible storms? I was already travelling a lot for astronomy’s sake, both in the quest for eclipses (1983, 1988, 1990, 1991, 1992, 1994, 1995 and so on) and comets (Halley in 1986), but for meteors? Then again, Brad Schaefer, the American astronomer famous for his professional work on astronomy with the naked eye, had told me in 1988 that for him one meteor storm would be “worth ten eclipses”. -
Reading Canadian Literature in a Light-Polluted Age
Western University Scholarship@Western Electronic Thesis and Dissertation Repository 12-16-2013 12:00 AM After Dark: Reading Canadian Literature in a Light-Polluted Age David S. Hickey The University of Western Ontario Supervisor Dr. D.M.R. Bentley The University of Western Ontario Graduate Program in English A thesis submitted in partial fulfillment of the equirr ements for the degree in Doctor of Philosophy © David S. Hickey 2013 Follow this and additional works at: https://ir.lib.uwo.ca/etd Part of the Literature in English, North America Commons Recommended Citation Hickey, David S., "After Dark: Reading Canadian Literature in a Light-Polluted Age" (2013). Electronic Thesis and Dissertation Repository. 1805. https://ir.lib.uwo.ca/etd/1805 This Dissertation/Thesis is brought to you for free and open access by Scholarship@Western. It has been accepted for inclusion in Electronic Thesis and Dissertation Repository by an authorized administrator of Scholarship@Western. For more information, please contact [email protected]. After Dark: Reading Canadian Literature in a Light-Polluted Age Monograph by David Hickey Graduate Program in English A thesis submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy in English The School of Graduate and Postdoctoral Studies The University of Western Ontario London, Ontario, Canada © Hickey 2013 i Abstract A threat to nocturnal ecosystems and human health alike, light pollution is an unnecessary problem that comes at an enormous cost. The International Dark-Sky Association has recently estimated that the energy expended on light scatter alone is responsible for no less than twelve million tons of carbon dioxide and costs municipal governments at least $1 billion annually (“Economic Issues” 2). -
„Ordinary“ Showers
„Ordinary“ Showers # MDC Show Shower Name MDC Number Solar Longitude Right Declination Vgeo Comment Num Code Status of Ascension ber Meteors Mean/ Max Interval Mean Drift Mean Drift Mean Drift [°] [°] [°] [°] [°] [°] [km/s] [km/s] 1 40 ZCY zeta Cygnids W 500 16 13-20 302 +0.3 +40 +0.2 40 - NM; SS: α,δ,v geo ; DM: δ 2 131 DAL delta Aquilids W 200 20 17-23 308 +1.0 +12 +0.3 63 - DM: δ 3 136 SLE sigma Leonids W 1,000 26 18-35 201 +0.6 +3 +0.0 19 -0.16 NM; DM: α,v geo 348 ARC April rho Cygnids E 4 1,700 33 13-44 314 +0.8 +44.5 +0.3 42 +0.00 ARC and NCY are identical 409 NCY nu Cygnids W 5 346 XHE x Herculids W 300 352 350-355 256 +0.8 +48.5 -0.0 35 - NM 6 6 LYR April Lyrids E 4,000 32.5 28-35 272.6 +0.65 +33.2 -0.3 45.5 +0.25 7 343 HVI H Virginids W 200 41 39-43 205 +0.7 -11 -0.5 17 - NM; SD; NAD 8 31 ETA eta Aquariids E 3,800 47 38-59 339.1 +0.64 -0.5 +0.33 66.5 +0.1 9 531 GAQ gamma Aquilids W 320 48 45-52 307 -0.1 +14.5 -0.1 66 - NM; SS: α; Part of N Apex? 10 145 ELY eta Lyrids E 800 50 45-52 291.3 +0.15 +43.4 +0.0 42.6 - Maybe active longer; DM: δ 11 520 MBC May beta Capricornids W 150 59 56-61 305 +0.7 -15 +0.3 68 - NM; WS; similar to 7CCA 12 362 JMC June mu Cassiopeiids W 150 71 69-74 11 +2.8 +53 +0.5 42 - WS; SS: α,δ,v geo 13 171 ARI Daytime Arietids E 70 77 74-79 44 +1.0 +23.5 +0.1 42 NM; Daytime shower; DM: v geo 14 164 NZC Northern June Aquilids E 200 82 79-84 293 +1.0 -12 -0.4 42 - DM: v geo 510 JRC NM; SD; NAD; short & strong; 15 June rho Cygnids W 190 84 83-85 320.4 +0.8 44.7 -0.8 48 - 521 JRP JRP is identical to JRC 16 410 DPI -
The Leonid Meteor Shower3
135 Chapter 5: Observational Record of the Leonid Meteor Shower3 5.1 Introduction Meteor Science in its modern form was born on the morning of November 13, 1833. It was the great Leonid return of that year which provoked widespread interest in the subject after being observed extensively in North America (Olmsted, 1834). With its unique nature of producing strong showers every 33 years, the Leonid shower is probably the most extensively written-about meteoroid stream. This observational database permits useful constraints to be placed on modern theories of the stream’s evolution. Numerous past works have examined Leonid records both ancient (e.g. Hasegawa 1993) and more modern (e.g. Mason 1995). However, in virtually all of these secondary works, no examination of the original records was attempted and the actual activity profiles, locations of peak activity and other characteristics are ill-defined. Our motivation is to re- examine as many original accounts of the shower contains usable numerical information as possible and determine the characteristics of past showers, independent of the many secondary accounts which appear in the literature, in an effort to better understand the stream’s past activity and interpret its basic physical properties. These data will also provide the basis for comparison with the numerical modelling of the stream, which is developed in Chapter 6. We examine the available original records of the Leonids for modern returns of the shower (here defined to be post-1832). In doing so, we attempt to establish characteristics of the stream near its peak activity, as borne out by the original records, for the years near the passage of 55P/Tempel-Tuttle. -
Meteor Activity Outlook for January 2-8, 2021
Meteor Activity Outlook for January 2-8, 2021 Daniel Bush captured this impressive fireball at 04:11 UT (23:11 CDT on Sept. 5) on 6 Septmeber 2020, from Albany, Missouri, USA. For more details on this particular event visit: https://fireball.amsmeteors.org/members/imo_view/event/2020/5020. Credit Daniel Bush January is best known for the Quadrantids, which have the potential of being the best shower of the year. Unfortunately, this shower is short lived and occurs during some of the worst weather in the northern hemisphere. Due to the high northern declination (celestial latitude) and short summer nights, little of this activity can be seen south of the equator. There are many very minor showers active throughout the month. Unfortunately, most of these produce less than 1 shower member per hour and do not add much to the overall activity total. Activity gets interesting as seen from the southern hemisphere as ill-defined radiants in Vela, Carina, and Crux become active this month. This activity occurs during the entire first quarter of the year and moves eastward into Centaurus in February and ends in March with activity in Norma and Lupus. Sporadic rates are generally similar in both hemispheres this month. Sporadic rates are falling though for observers in the northern hemisphere and rising as seen from the southern hemisphere. During this period, the moon reaches its last quarter phase on Wednesday January 6th. At this time, the moon is located 90 degrees west of the sun in the sky and will rise near midnight standard time. -
Ongoing Meteor Work
WGN, the Journal of the IMO 35:1 (2007) 13 Ongoing meteor work Spanish Meteor Network: 2006 continuous monitoring results J. M. Trigo-Rodr´ıguez 1,2,J.M.Madiedo3, A.J. Castro-Tirado 4, J.L. Ortiz 4,J.Llorca5, J. Fabregat 6,S.V´ıtek 4,P.S.Gural7, B. Troughton 8,P.Pujols9 and F. G´alvez 8 Initial results from the first year of continuous CCD low-scan-rate all-sky and video monitoring by the SPanish Meteor Network (SPMN) are presented. Under extraordinary weather conditions, the SPMN recorded almost 40 bright (over m = −6) fireballs, some of which were observed simultaneously from several stations. Daily observations of meteor activity have helped to increase our knowledge on cometary and asteroidal-origin meteoroid streams. The focus herein will be on the overall description of the fireballs recorded, first estimations of the measured spatial fluxes of selected streams, and information on unexpected activity from poorly-known meteoroid streams. Received 2007 February 5 1 Introduction We previously reported on the first steps in the de- velopment of the SPanish Meteor Network (SPMN) by using innovative low-scan-rate all-sky CCD cameras that achieve +2/+3 meteor limiting magnitude (Trigo- Rodr´ıguez et al., 2004). The year 2006 was extraor- dinary for the SPMN network, especially due to the excellent weather conditions during autumn and winter that guaranteed almost a continuous record of meteor activity from the different SPMN stations. During 2006 new progress has been made by having set up two addi- tional all-sky CCD stations in Catalonia and three video stations in Andalusia with the main goal to increase our atmospheric coverage of meteor and fireball activity (Trigo-Rodr´ıguez et al., 2006b). -
The Status of the NASA All Sky Fireball Network
https://ntrs.nasa.gov/search.jsp?R=20120004179 2019-08-30T19:42:51+00:00Z The Status of the NASA All Sky Fireball Network William J. Cooke Meteoroid Environment Office, NASA Marshall Space Flight Center, Huntsville, AL 35812 USA. [email protected] Danielle E. Moser MITS/Dynetics, NASA Marshall Space Flight Center, Huntsville, AL 35812 USA. [email protected] Abstract Established by the NASA Meteoroid Environment Office, the NASA All Sky Fireball Network consists of 6 meteor video cameras in the southern United States, with plans to expand to 15 cameras by 2013. As of mid-2011, the network had detected 1796 multi-station meteors, including meteors from 43 different meteor showers. The current status of the NASA All Sky Fireball Network is described, alongside preliminary results. 1 Introduction The NASA Meteoroid Environment Office (MEO), located at the Marshall Space Flight Center in Huntsville, Alabama, USA, is the NASA organization responsible for meteoroid environments as they pertain to spacecraft engineering and operations. Understanding the meteoroid environment can help spacecraft designers to better protect critical components on spacecraft or avoid critical operations such as extravehicular activities during periods of higher flux such as meteor showers. In mid-2008, the MEO established the NASA All Sky Fireball Network, a network of meteor cameras in the southern United States. The objectives of this video network are to 1) establish the speed distribution of cm-sized meteoroids, 2) determine which sporadic sources produce large particles, 3) determine (low precision) orbits for bright meteors, 4) attempt to discover the size at which showers begin to dominate the meteoroid flux, 5) monitor the activity of major meteor showers, and 6) assist in the location of meteorite falls. -
Confirmation of the Northern Delta Aquariids
WGN, the Journal of the IMO XX:X (200X) 1 Confirmation of the Northern Delta Aquariids (NDA, IAU #26) and the Northern June Aquilids (NZC, IAU #164) David Holman1 and Peter Jenniskens2 This paper resolves confusion surrounding the Northern Delta Aquariids (NDA, IAU #26). Low-light level video observations with the Cameras for All-sky Meteor Surveillance project in California show distinct showers in the months of July and August. The July shower is identified as the Northern June Aquilids (NZC, IAU #164), while the August shower matches most closely prior data on the Northern Delta Aquariids. This paper validates the existence of both showers, which can now be moved to the list of established showers. The August Beta Piscids (BPI, #342) is not a separate stream, but identical to the Northern Delta Aquariids, and should be discarded from the IAU Working List. We detected the Northern June Aquilids beginning on June 14, through its peak on July 11, and to the shower's end on August 2. The meteors move in a short-period sun grazing comet orbit. Our mean orbital elements are: q = 0:124 0:002 AU, 1=a = 0:512 0:014 AU−1, i = 37:63◦ 0:35◦, ! = 324:90◦ 0:27◦, and Ω = 107:93 0:91◦ (N = 131). This orbit is similar to that of sungrazer comet C/2009 U10. ◦ ◦ 346.4 , Decl = +1.4 , vg = 38.3 km/s, active from so- lar longitude 128.8◦ to 151.17◦. This position, however, 1 Introduction is the same as that of photographed Northern Delta Aquariids. -
Activity of the Eta-Aquariid and Orionid Meteor Showers A
Astronomy & Astrophysics manuscript no. Egal2020b ©ESO 2020 June 16, 2020 Activity of the Eta-Aquariid and Orionid meteor showers A. Egal1; 2; 3,?, P. G. Brown1; 2, J. Rendtel4, M. Campbell-Brown1; 2, and P. Wiegert1; 2 1 Department of Physics and Astronomy, The University of Western Ontario, London, Ontario N6A 3K7, Canada 2 Institute for Earth and Space Exploration (IESX), The University of Western Ontario, London, Ontario N6A 3K7, Canada 3 IMCCE, Observatoire de Paris, PSL Research University, CNRS, Sorbonne Universités, UPMC Univ. Paris 06, Univ. Lille, France 4 Leibniz-Institut f. Astrophysik Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany, and International Meteor Organization, Eschenweg 16, 14476 Potsdam, Germany Received XYZ; accepted XYZ ABSTRACT Aims. We present a multi-instrumental, multidecadal analysis of the activity of the Eta-Aquariid and Orionid meteor showers for the purpose of constraining models of 1P/Halley’s meteoroid streams. Methods. The interannual variability of the showers’ peak activity and period of duration is investigated through the compilation of published visual and radar observations prior to 1985 and more recent measurements reported in the International Meteor Organization (IMO) Visual Meteor DataBase, by the IMO Video Meteor Network and by the Canadian Meteor Orbit Radar (CMOR). These techniques probe the range of meteoroid masses from submilligrams to grams. The η-Aquariids and Orionids activity duration, shape, maximum zenithal hourly rates (ZHR) values, and the solar longitude of annual peaks since 1985 are analyzed. When available, annual activity profiles recorded by each detection network were measured and are compared. Results. Observations from the three detection methods show generally good agreement in the showers’ shape, activity levels, and annual intensity variations. -
Investigating the Radiant Sources of Meteors Anamol Mittal, Dr
International Journal of Scientific & Engineering Research Volume 8, Issue 10, October-2017 1369 ISSN 2229-5518 Investigating the radiant sources of meteors Anamol Mittal, Dr. K. Kishore Kumar Abstract— The results obtained in the present study, which are related to basic meteor phenomenon such as meteor velocity distribution, height distribution and annual variability of meteors are discussed. An attempt is also made to identify the peak radiant sources of the observed meteors. The results are found to be consistent with the present understanding of the meteor phenomenon. Further studies are required to estimate the orbits of the meteors using single station observations. The important outcome of the present study is the algorithm for estimating the radiant sources using azimuth, zenith angle observations of meteor radar. Index Terms— Astronomy, earth sciences, entrance velocity distribution, meteor wind radar, meteors, radiant sources, Thumba —————————— —————————— 1 INTRODUCTION eople have always wondered about the worlds that lie 3. Epoch: In astronomy, an epoch is a moment in time P beyond the boundaries of sky, the purpose of our exis- used as a reference point for some time-varying as- tence, whether the existence of earth is a result of some tronomical quantity, such as the celestial coordinates higher purpose or just a lucky coincidence? Well, answers to or elliptical orbital elements of a celestial body, be- these questions are not known and beyond the reach of present technology. One such question asks: Where do the cause these are subject to perturbations and vary with meteoroids (most commonly known as falling stars) come time.[2] from and how is their distribution in solar system related to the formation of planets and other solar system bodies? You may find answers to these questions as you proceed through the report. -
ISSN 2570-4745 VOL 4 / ISSUE 5 / OCTOBER 2019 Bright Perseid With
e-Zine for meteor observers meteornews.net ISSN 2570-4745 VOL 4 / ISSUE 5 / OCTOBER 2019 Bright Perseid with fares. Canon 6D with Rokinon 24mm lens at f/2.0 on 2019 August 13, at 3h39m am EDT by Pierre Martin EDMOND Visual observations CAMS BeNeLux Radio observations UAEMM Network Fireballs 2019 – 5 eMeteorNews Contents Problems in the meteor shower definition table in case of EDMOND Masahiro Koseki ..................................................................................................................................... 265 July 2019 report CAMS BeNeLux Paul Roggemans ...................................................................................................................................... 271 August 2019 report CAMS BeNeLux Paul Roggemans ...................................................................................................................................... 273 The UAEMMN: A prominent meteor monitoring system in the Gulf Region Dr. Ilias Fernini, Aisha Alowais, Mohammed Talafha, Maryam Sharif, Yousef Eisa, Masa Alnaser, Shahab Mohammad, Akhmad Hassan, Issam Abujami, Ridwan Fernini and Salma Subhi .................... 275 Summer observations 2019 Pierre Martin........................................................................................................................................... 278 Radio meteors July 2019 Felix Verbelen ......................................................................................................................................... 289 Radio meteors August 2019