ISSN 2570-4745 VOL 5 / ISSUE 1 / JANUARY 2020 Meteor Over
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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 -
Arxiv:2008.06761V1 [Astro-Ph.EP] 15 Aug 2020 We Present a Novel Algorithm to Reduce Scatter and Increase Precision in a Lightcurve Compiled from Many Sources
, USA Draft version August 18, 2020 Typeset using LATEX modern style in AASTeX62 The visual lightcurve of comet C/1995 O1 (Hale-Bopp) from 1995 - 1999 M. Womack,1, 2 O. Curtis,3 D.A. Rabson,4, 5 O. Harrington Pinto,2 K. Wierzchos,6 S. Cruz Gonzalez,4 G. Sarid,7 C. Mentzer,8 N. Lastra,9 N. Pichette,10 N. Ruffini,11 T. Cox,4 I. Rivera,2 A. Micciche,4 C. Jackson,4 A. Homich,12 A. Tollison,12 S. Reed,12 J. Zilka,12 B. Henning,12 M. Spinar,12 S. Rosslyn Escoto,13 T. Erdahl,12 Marcel P. Goldschen-Ohm,14 and W.T. Uhl15, 16 1Florida Space Institute, University of Central Florida, Orlando FL USA 2Department of Physics, University of Central Florida 3Institute for Astrophysical Research, Boston University, Boston, MA 02215, USA 4Department of Physics, University of South Florida, Tampa, FL 33620, USA 5National Science Foundation, Alexandria, VA 22314, USA 6Catalina Sky Survey, Lunar and Planetary Lab, University of Arizona, Tucson, AZ 85721 7SETI Institute, Mountain View, CA 8Department of Physics and Astronomy, University of Missouri, Columbia, MO 9Department of Physics and Astronomy, Bowling Green State University, OH 10Department of Physics, Montana State University, Bozeman, MT 11Monash University, Australia 12St. Cloud State University, St. Cloud, MN 56301, USA 13Instituto de Astronomia, Universidad Nactional Autonoma de Mexico, Mexico 14Department of Neuroscience, University of Texas at Austin, Austin TX 15Department of Astronomy, Yale University, New Haven, CT 06511 16Dialectic Capital Management, Rowayton, CT 06853 ABSTRACT The long-term brightness evolution of the great comet C/1995 O1 (Hale-Bopp) pre- sented a remarkable opportunity to study the behavior of its coma over four years. -
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. -
1 Accepted for Publication in the Journal of the British
1 David Elijah Packer: cluster variables, meteors and the solar corona Jeremy Shears Abstract David Elijah Packer (1862-1936), a librarian by profession, was an enthusiastic amateur astronomer who observed from London and Birmingham. He first came to the attention of the astronomical community in 1890 when he discovered a variable star in the globular cluster M5, only the second periodic variable to be discovered in a globular cluster. He also observed meteors and nebulae, on one occasion reporting a brightening in the nucleus of the galaxy M77. However, his remarkable claims in 1896 that he had photographed the solar corona in daylight were soon shown to be flawed. Biographical sketch David Elijah Packer was born in Bermondsey, London, in 1862 April (1) the eldest child of Edward Packer (1820-1896) and Emma (Bidmead) Packer (1831-1918) (2). David attended the Free Grammar School of Saint Olave and Saint John at Southwark, where he performed well, especially in arithmetic, algebra and general mathematics (3). Edward Packer was a basket maker, as was his father and grandfather before him, the Packer family originally coming to London from Thanet, in Kent. The English basket-making industry was in decline during the second half of the nineteenth century due to the availability of cheaper imports from the continent. In spite of this, Edward was still in business in 1881, but the prospects for his son continuing in a trade that had made a living for generations of his ancestors were probably limited (4). Thus at the age of 18 we find David Elijah Packer working as an Oilman’s Assistant, supplying fuel for the oil lamps of London (5). -
Absolute Magnitudes of Asteroids and a Revision of Asteroid Albedo Estimates from WISE Thermal Observations ⇑ Petr Pravec A, , Alan W
Icarus 221 (2012) 365–387 Contents lists available at SciVerse ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations ⇑ Petr Pravec a, , Alan W. Harris b, Peter Kušnirák a, Adrián Galád a,c, Kamil Hornoch a a Astronomical Institute, Academy of Sciences of the Czech Republic, Fricˇova 1, CZ-25165 Ondrˇejov, Czech Republic b 4603 Orange Knoll Avenue, La Cañada, CA 91011, USA c Modra Observatory, Department of Astronomy, Physics of the Earth, and Meteorology, FMFI UK, Bratislava SK-84248, Slovakia article info abstract Article history: We obtained estimates of the Johnson V absolute magnitudes (H) and slope parameters (G) for 583 main- Received 27 February 2012 belt and near-Earth asteroids observed at Ondrˇejov and Table Mountain Observatory from 1978 to 2011. Revised 27 July 2012 Uncertainties of the absolute magnitudes in our sample are <0.21 mag, with a median value of 0.10 mag. Accepted 28 July 2012 We compared the H data with absolute magnitude values given in the MPCORB, Pisa AstDyS and JPL Hori- Available online 13 August 2012 zons orbit catalogs. We found that while the catalog absolute magnitudes for large asteroids are relatively good on average, showing only little biases smaller than 0.1 mag, there is a systematic offset of the cat- Keywords: alog values for smaller asteroids that becomes prominent in a range of H greater than 10 and is partic- Asteroids ularly big above H 12. The mean (H H) value is negative, i.e., the catalog H values are Photometry catalog À Infrared observations systematically too bright. -
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 -
Craters and Airbursts
Craters and Airbursts • Most asteroids and comets fragments explode in the air as fireballs or airbursts; only the largest ones make craters. • Evidence indicates that the YDB impact into the Canadian ice sheet made ice-walled craters that melted away long ago. • The YDB impact also possibly created rocky craters, most likely along the edge of the ice sheet in Canada or underwater in the oceans. • Our group is planning expeditions to search for impact evidence and hidden craters, for example to North Dakota, Montana, Quebec, and Nova Scotia. The following pages show what could happen during an impact NOTE: this website is a brief, non-technical introduction to the YDB impact hypothesis. For in-depth information, go to “Publications” to find links to detailed scientific papers. NAME OF SHOWER NAME OF SHOWER Alpha Aurigids Leo Minorids Meteor Showers Alpha Bootids Leonids Alpha Capricornids Librids Alpha Carinids Lyrids Comet impacts are common, Alpha Centaurids Monocerotids Alpha Crucids Mu Virginids but usually, they are harmless Alpha Cygnids Northern Delta Aquariids Alpha Hydrids Northern Iota Aquariids Alpha Monocerotids Northern Taurids Alpha Scorpiids October Arietids • Earth is hit by 109 meteor Aries-triangulids Omega Capricornids Arietids Omega Scorpiids showers every year (listed at Beta Corona Austrinids Omicron Centaurids right), averaging 2 collisions Chi Orionids Orionids Coma Berenicids Perseids with streams each week Delta Aurigids Phoenicids Delta Cancrids Pi Eridanids Delta Eridanids Pi Puppids • Oddly, most “meteor showers” -
Jopekkokhirova2021.Pdf
ИЗВЕСТИЯ НАЦИОНАЛЬНОЙ АКАДЕМИИ НАУК ТАДЖИКИСТАНА ОТДЕЛЕНИЕ ФИЗИКО-МАТЕМАТИЧЕСКИХ, ХИМИЧЕСКИХ, ГЕОЛОГИЧЕСКИХ И ТЕХНИЧЕСКИХ НАУК №2 (183), 2021 г. АСТРОНОМИЯ УДК 523.532 T.J.JOPEK, G.I.KOKHIROVA*, P.JENNISKENS**, D.JANCHES***, M.HAJDUKOVA*****, R.RUDAWSKA****** IAU METEOR DATA CENTER: THE SHOWER DATABASE Astronomical Observatory Institute, Faculty of Physics, A. M. University, Poznan, Poland, **Institute of Astrophysics, National Academy of Sciences of Tajikistan, ***SETI Institute, 189 Bernardo Ave, Mountain View, CA, 94043, USA, ****NASA Goddard Space Flight Center, Greenbelt, MD, 20771, USA, *****Astronomical Institute of the Slovak Academy of Sciences, Bratislava, Slovakia, ******ESA/ESTEC, Keplerlaan 1, 2201, AZ Noordwijk, the Netherlands Поступила в редакцию 22.01.2021 г. The IAU Working Group on Meteor Shower Nomenclature was established in 2006 to regulate the nomenclature of meteor showers reported in the scientific literature. One year later the International Astronomical Union Meteor Data Center shower database was implemented (IAU MDC). The database does not contain all information about the meteor showers. Its purpose is to give each new meteoroid stream, published in the scientific literature, a unique name and codes. During the “Meteoroids 2019” conference held in Bratislava, the IAU Working Group on Meteor Shower Nomenclature established new rules for the introduction and removal of meteor showers from the MDC. In this paper, we present a concise description of the meteor shower database, its origin, and struc- ture and, in particular, the current requirements for the introduction of new data, and unknown as well as known meteor showers. Key words: meteoroid stream, meteor shower, IAU MDC shower database, meteor shower nomenclature rules, new meteor shower submission rules. -
AAS NEWSLETTER a Publication for the Members of the American Astronomical Society
June 2006 Issue 129 AAS NEWSLETTER A Publication for the members of the American Astronomical Society FROM THE (RETIRING) EXECUTIVE OFFICER - BOB MILKEY The past eleven years have been both extremely challenging and rewarding for me in serving as your 3 Executive Officer. Many things have changed over that period and there are still many challenges for Letters to the Society to face. While overall, the Society is in a very good position, I am certainly not passing my the Editor successor a position without ongoing challenges. From my perspective, the most significant AAS accomplishment of the past decade was the introduction 5 of the electronic versions of the AAS journals, but the development of these is still an ongoing process. Chrétien Grant It was well in progress when I joined the Society as the result of an outstanding display of teamwork Award Winner between the AAS staff, volunteers, and the personnel at the University of Chicago Press. At present, the journals are serving the authors and readers well, but both publishing technology and economics are in a state of flux. The challenge will be to introduce new features into the journals while at the same 6 time reducing the overall costs of publication. The choices to be made in balancing these two goals will be best made with input from both the authors and readers of the journals. The stewardship of The Hale & Harvey Astrophysical Journal and The Astronomical Journal is one of the most important services the AAS Prize Winners performs for the astronomical community and arguably the selection of Editors for these journals is one of the most important acts that your elected Council performs. -
The Valley Skywatcher
THE VALLEY SKYWATCHER The Official Publication of the Chagrin Valley Astronomical Society CONTENTS Est. 1963 President’s Corner Articles Friends, as we start a new year, I want to recognize the contribu- Winter Astronomy Links 6 tions of some long-time members. Reflection Nebulae For Winter Astophotography 7 Former member Marty Edwards recently returned a very nice star Book Review: atlas, Becvar’s Atlas of the Heav- American Eclipse 9 ens – Atlas Coeli 1950.0, that was given to him and his brother, Bill About The New Look For Edwards, by CVAS when he and The Valley Skywatcher 12 his family moved from the area in 1966! (See photos page 12.) He Sundial Theory also sent us some vintage Valley Skywatcher issues and & Construction 13 several photographs from the very early years of CVAS. We send Marty our sincere thanks, and I send him my sincere apologies for the delay acknowledging his donation. Regular Features Tony Mallama has donated three fine books with an Observer’s Log 2 Astrophotography 3 astronomical bent, written by Dennis E. Taylor: We are Notes & News 8 Legion, For We are Many, and All These Worlds. We’ll keep Constellation Quiz 25 these in the warm room at Indian Hill where they will be Reflections 27 available for loan to CVAS members. We’ve also had several members, often anony- CVAS Officers mously, contribute with financial donations to CVAS. So I Marty Mullet President want to thank each of you and all of you for your part in George Trimble Vice President keeping CVAS alive and well! We wouldn’t be the same Steve Fishman Treasurer without you. -
Dr. PETER JENNISKENS 2019 Jenniskens, P., Popova, O. P
Dr. PETER JENNISKENS 2019 Jenniskens, P., Popova, O. P., Glazachev, D. O., Podobnaya, E. D., Kartashova, A. P., 2019. Tunguska eyewitness accounts, injuries, and casualties. Icarus (in press) [#204]. Jenniskens, P., 2019. Review of asteroid-family and meteorite-type links. In: A century of asteroid families. J. Masseido, ed., IAU Transactions (in press) [#203]. Jenniskens, P., Utas J., Qing-zhu Yin, Matson R. D., Fries M., Howell J. A., Free D., Albers J., Devillepoix H., Bland P., Miller A., Verish R., Garvie L. A. J., Zolensky M. E., Ziegler K., Sanborn M. E., Verosub K. ., Rowland D. J., Ostrowski D. R., Bryson K., Laubenstein M, Zhou Q., Li, Q.-L., Li X.-H., Liu Y., Tang G.-Q., Welten K., Meier M. M. M., Plant A. A., Maden C., Busemann H., Granvik M., 2018. The Creston, California, meteorite fall and the origin of L chondrites. MAPS (in press) [#202]. Harp, G. R., Richards, J., Jenniskens, P., Shostak, S., Tarter, J. C., 2019. Radio SETI observations of the interstellar object 'OUMUAMUA. Acta Astronautica 155, 51–54 [#201]. 2018 Jenniskens, P., 2018. A shower look-up table to trace the dynamics of meteoroid streams and their sources. AAS DPA meeting #49, San Jose, id.102.04 (abstract). Kartashova, A. P., Popova, O. P., Glazachev, D. O., Jenniskens, P., Podobnaya, E. D., 2018. Eyewitness accounts and modeling results for Chelyabinsk Airburst. 81st. Annual Meeting of the Meteoritical Society, 22-27 July 2018 in Mosow, Russia, LPI Contr. No. 2067, 2018, id.6169. Goodrich, C. A., Fioretti, A., Zolensky, M., Shaddad, M., Hiroi, T., Kohl, I., Young, E., Kita, N., Sanborn, M., Yin, Q.-Z., Downes, H., Ross, D., Jenniskens, P., 2018. -
X-Ray Monitoring of Optical Novae in M31 from July 2004 to February 2005
Astronomy & Astrophysics manuscript no. 6812 c ESO 2021 July 7, 2021 X-ray monitoring of optical novae in M 31 from July 2004 to February 2005⋆,⋆⋆ W. Pietsch1, F. Haberl1, G. Sala1, H. Stiele1, K. Hornoch2, A.Riffeser1,3, J. Fliri3, R. Bender1,3, S. B¨uhler3, V. Burwitz1, J. Greiner1, and S. Seitz3 1 Max-Planck-Institut f¨ur extraterrestrische Physik, Giessenbachstraße, 85741 Garching, Germany e-mail: [email protected] 2 66431 Lelekovice 393, Czech Republic 3 Universit¨atssternwarte M¨unchen, Scheinerstraße, 81679 M¨unchen, Germany Received 27 November 2006 / Accepted 12 December 2006 ABSTRACT Context. Optical novae have recently been identified as the major class of supersoft X-ray sources in M 31 based on ROSAT and early XMM-Newton and Chandra observations. Aims. This paper reports on a search for X-ray counterparts of optical novae in M 31 based on archival Chandra HRC-I and ACIS-I as well as XMM-Newton observations of the galaxy center region obtained from July 2004 to February 2005. Methods. We systematically determine X-ray brightness or upper limit for counterparts of all known optical novae with outbursts between November 2003 to the end of the X-ray coverage. In addition, we determine the X-ray brightnesses for counterparts of four novae with earlier outbursts. Results. For comparison with the X-ray data we created a catalogue of optical novae in M 31 based on our own nova search programs and on all novae reported in the literature. We collected all known properties and named the novae consistently following the CBAT scheme.