'3-D' Lyrid Meteor Shower: up All Night NASA Chat Experts Dr. Bill
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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 -
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. -
Occurrence and Altitude of the Non-Specular Long-Lived Meteor Trails During Meteor Showers at High Latitudes
EGU2020-1543 https://doi.org/10.5194/egusphere-egu2020-1543 EGU General Assembly 2020 © Author(s) 2021. This work is distributed under the Creative Commons Attribution 4.0 License. Occurrence and altitude of the non-specular long-lived meteor trails during meteor showers at high latitudes Alexander Kozlovsky1, Renata Lukianova2, and Mark Lester3 1University of Oulu, Sodankyla Geophysical Observatory, Sodankyla, Finland ([email protected]) 2Space Research Institute, Moscow, Russia 3Department of Physics and Astronomy, University of Leicester, Leicester, UK Meteoroids entering the Earth’s atmosphere produce ionized trails, which are detectable by radio sounding. Majority of such radar detections are the echoes from cylindrical ionized trails, which occur if the radar beam is perpendicular to the trail, i.e., the reflection is specular. Typically such echoes detected by VHF radars last less than one second. However, sometimes meteor radars (MR) observe unusually long-lived meteor echoes and these echoes are non-specular (LLNS echoes). The LLNS echoes last up to several tens of seconds and show highly variable amplitude of the radar return. The LLNS echoes are received from the non-field-aligned irregularities of ionization generated along trails of bright meteors and it is believed that key role in their generation belongs to the aerosol particles arising due to fragmentation and burning of large meteoroids. The occurrence and height distributions of LLNS are studied using MR observations at Sodankylä Geophysical Observatory (SGO, 67° 22' N, 26° 38' E, Finland) during 2008-2019. Two parameters are analyzed: the percentage and height distribution of LLNS echoes. These LLNS echoes constitute about 2% of all MR detections. -
Meteor Activity Outlook for April 17-23, 2021
Meteor Activity Outlook for April 17-23, 2021 Greg Johnson captured this fireball in the constellation of Cassiopeia on 12 March 2021 from Hansville, Washington, USA. During this period the moon reaches its first quarter phase on Tuesday April 20th. On this date the moon is located 90 degrees east of the sun and sets near 03:00 local daylight saving time (LDST). As the week progresses the waxing gibbous moon will encroach into the late morning sky, limiting the opportunity to view under dark skies. The estimated total hourly meteor rates for evening observers this week is near 2 as seen from mid-northern latitudes (45N) and 3 as seen from tropical southern locations (25S). For morning observers, the estimated total hourly rates should be near 7 as seen from mid-northern latitudes (45N) and 11 as seen from tropical southern locations (25S). The actual rates will also depend on factors such as personal light and motion perception, local weather conditions, alertness, and experience in watching meteor activity. Evening rates are reduced during this period due to moonlight. Note that the hourly rates listed below are estimates as viewed from dark sky sites away from urban light sources. Observers viewing from urban areas will see less activity as only the brighter meteors will be visible from such locations. The radiant (the area of the sky where meteors appear to shoot from) positions and rates listed below are exact for Saturday night/Sunday morning April 17/18. These positions do not change greatly day to day so the listed coordinates may be used during this entire period. -
Specular Long-Lived Meteor Trails During Meteor Showers at High Latitudes
Occurrence and altitude of the non- specular long-lived meteor trails during meteor showers at high latitudes EGU2020-1543 https://doi.org/10.5194/egusphere-egu2020-1543 Alexander Kozlovsky1, Renata Lukianova2, and Mark Lester3 (1) Sodankylä Geophysical Observatory, Finland (2) Space Research Institute, Moscow, Russia (3) University of Leicester, UK Abstract Meteoroids entering the Earth’s atmosphere produce ionized trails, which are detectable by radio sounding. Majority of such radar detections are the echoes froM cylindrical ionized trails, which occur if the radar beam is perpendicular to the trail, i.e., the reflection is specular. Typically such echoes detected by VHF radars last less than one second. However, soMetiMes Meteor radars (MR) observe unusually long-lived Meteor echoes and these echoes are non-specular (LLNS echoes). The LLNS echoes last up to several tens of seconds and show highly variable amplitude of the radar return. The LLNS echoes at high latitudes are received froM the non-field- aligned irregularities of ionization generated along trails of bright Meteors and it is believed that key role in their generation belongs to the aerosol particles arising due to fragMentation and burning of large Meteoroids. The occurrence and height distributions of LLNS are studied using MR observations at Sodankylä Geophysical Observatory (SGO, 67° 22' N, 26° 38' E, Finland) during 2008-2019. Two parameters are analyzed: the percentage and height distribution of LLNS echoes. These LLNS echoes constitute about 2% of all MR detections. However during certain Meteor showers (GeMinids, Perseids, Quadrantids, Arietids or/and DaytiMe ζ-Perseids, and Lyrids) the percentage of LLNS echoes is noticeably higher (about 10, 8, 7, 7, and 4%, respectively). -
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” -
Lunar Meteor Schedule and Observing Plan for 2021
Lunar Meteor Schedule and Observing Plan for 2021 This form outlines the plan to monitor the moon on a regular basis both inside and outside normal annual showers. Each month, for a total of up to 14 days per month, we are coordinating observations of the Earthshine portion of the moon for background (including the minor showers when they fall during this time) meteor impact flux. A typical run of observations starts three days after New Moon and continues until two days past First Quarter. The run resumes two days before Last Quarter and continues until three days prior to New Moon. The actual interval will depend on the lunar elevation and elongation as well as the ability of the observer to control stray light in one’s system. Shower Activity Maximum Radiant V∞ r ZHR Date λ⊙ α δ km/s Antihelion Source Mar-Apr, late Dec 10 – Sep 10 Varies Varies 30 3.0 4 (ANT) May, late June Quadrantids (010 QUA) Dec 28 - Jan 12 Jan 03 283.15° 230° +49° 41 2.1 110 γ-Ursae Minorids (404 Jan 10 - Jan 22 Jan 19 298° 228° +67° 31 3.0 3 GUM) α-Centaurids (102 ACE) Jan 31 - Feb 20 Feb 08 319.2° 210° -59° 58 2.0 6 γ-Normids (118 GNO) Feb 25 - Mar 28 Mar 14 354° 239° -50° 56 2.4 6 Lyrids (006 LYR) Apr 14 - Apr 30 Apr 22 32.32° 271° +34° 49 2.1 18 π-Puppids (137 PPU) Apr 15 – Apr 28 Apr 23 33.5° 110° -45° 18 2.0 Var η-Aquariids (031 ETA) Apr 19 - May 28 May 05 45.5° 338° -01° 66 2.4 50 η-Lyrids (145 ELY) May 03 - May 14 May 08 48.0° 287° +44° 43 3.0 3 June Bootids (170 JBO) Jun 22 - Jul 02 Jun 27 95.7° 224° +48° 18 2.2 Var Piscis Austr. -
NASA Chat: Stay 'Up All Night' to Watch the Perseids! Experts Dr. Bill Cooke, Danielle Moser and Rhiannon Blaauw August
NASA Chat: Stay ‘Up All Night’ to Watch the Perseids! Experts Dr. Bill Cooke, Danielle Moser and Rhiannon Blaauw August 11, 2012 _____________________________________________________________________________________ Moderator Brooke: Good evening, everyone, and thanks for joining us tonight to watch the 2012 Perseid meteor shower. Your chat experts tonight are Bill Cooke, Danielle Moser, and Rhiannon Blaauw from NASA's Marshall Space Flight Center in Huntsville, Ala. This is a moderated chat, and we expect a lot of questions, so please be patient -- it may take a few minutes for the experts to get to your question. So here we go -- let's talk Perseids! Boady_N_Oklahoma: Good evening!! Rhiannon: Welcome! We look forward to answering your questions tonight! StephenAbner: I live in Berea, Kentucky. Can you please tell me which part of the sky I should focus on for best viewing? Bill: Lie on your back and look straight up. Avoid looking at the Moon. Victoria_C.: Because we pass through the cloud every year, does the amount of meteors decline in time, too? Rhiannon: The meteoroid stream is replenished as the particles are travelling around the orbit of the stream. We will have Perseids for a long time still. Jerrte: When will the Perseids end? What year will be the last to view? Bill: The Perseids will be around for the next few centuries. Victoria_C.: Why do meteors fall more on one night than different nights? Bill: On certain nights, the Earth passes closest to the debris left behind by the comet. When this happens, we get a meteor shower with higher rates. Boady_N_Oklahoma: I'm in central rural oklahoma with crystal clear skies. -
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. -
Luminous Efficiency of Hypervelocity Meteoroid Impacts on the Moon Derived from the 2006 Geminids, 2007 Lyrids, and 2008 Taurids
https://ntrs.nasa.gov/search.jsp?R=20110016597 2019-08-29T18:25:21+00:00Z View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by NASA Technical Reports Server Luminous Efficiency of Hypervelocity Meteoroid Impacts on the Moon Derived from the 2006 Geminids, 2007 Lyrids, and 2008 Taurids D. E. Moser1• R. M. Suggs2• W. R. Swift3• R. J. Suggs2• W. J. Cooke2• A. M. Diekmann4• H. M. Koehler2 Abstract Since early 2006, NASA’s Marshall Space Flight Center has been routinely monitoring the Moon for impact flashes produced by meteoroids striking the lunar surface. During this time, several meteor showers have produced multiple impact flashes on the Moon. The 2006 Geminids, 2007 Lyrids, and 2008 Taurids were observed with average rates of 5.5, 1.2, and 1.5 meteors/hr, respectively, for a total of 12 Geminid, 12 Lyrid, and 12 Taurid lunar impacts. These showers produced a sufficient, albeit small sample of impact flashes with which to perform a luminous efficiency analysis similar to that outlined in Bellot Rubio et al. (2000a, b) for the 1999 Leonids. An analysis of the Geminid, Lyrid, and Taurid lunar impacts is carried out herein in order to determine the luminous efficiency in the 400-800 nm wavelength range for each shower. Using the luminous efficiency, the kinetic energies and masses of these lunar impactors can be calculated from the observed flash intensity. keywords hypervelocity impact · impact flash · luminous efficiency · lunar impact · meteoroid 1 Introduction When a meteoroid strikes the Moon, a large portion of the impact energy goes into heat and crater production. -
Lyrid Meteor Shower in 2006 and 2007 J¨Urgen Rendtel 1 and Rainer Arlt 2
74 WGN, the Journal of the IMO 35:4 (2007) Lyrids The Lyrid meteor shower in 2006 and 2007 J¨urgen Rendtel 1 and Rainer Arlt 2 Visual meteor observations during the 2007 Lyrids are analysed. A peak ZHR of 20.4 ± 1.1 and occurred at ◦ ◦ h m λ⊙ = 32 . 31 ± 0 . 05 (corresponding to 2007 April 22, 22 20 UT), quite similar to other recent returns. Since there were some expectations for enhanced rates in 2006 due to the 1-revolution dust trail of comet C1861/G1 (Thatcher), this data was re-analysed. No significant activity increase was found. Received 2007 August 23 1 Introduction Table 1 – The table summarizes visual outburst data listed in (Arter & Williams, 1995), 1988–2000 data from Table 2 The Lyrids are related with comet C 1861/G1 in (Dubietis & Arlt, 2000), 2003 data from (Dubietis & Arlt, (Thatcher). Details of early observations and outbursts 2003) and the recent 2006 and 2007 results calculated in this is given by Arter & Williams (1995), Rendtel, Arlt & work. All solar longitudes refer to J2000. McBeath (1995) and Arter & Williams (1997). The Year λ⊙ ZHR shower recurs annually with a relatively constant ac- 1803 32 ◦. 05 670 tivity. The radiant reaches sufficient elevation for use- 1922 31 ◦. 994 360–600 ful observations already before local midnight in north- 1922 32 ◦. 006 180 ern latitudes, and the activity can be monitored for 1934 32 ◦. 07 56–80 about five hours per night at best. Average ZHRs are 1945 31 ◦. 943 100 of the order of 15 to 20. The typical duration of a 1946 31 ◦. -
The 2012 Lyrids from Non-Traditional Observing Platforms
The 2012 Lyrids from non-traditional observing platforms D. E. Moser1, R. M. Suggs2, W. J. Cooke3, and R. C. Blaauw1 1MITS/Dynetics, NASA Marshall Space Flight Center, Huntsville, AL 35812 USA [email protected], [email protected] 2EV44 Space Environments Team, NASA Marshall Space Flight Center, Huntsville, AL 35812 USA [email protected] 3Meteoroid Environment Office, NASA Marshall Space Flight Center, Huntsville, AL 35812 USA [email protected] The NASA Meteoroid Environment Office (MEO) observed meteors during the Lyrid meteor shower peak on 22 April 2012 from three different observing platforms: the ground, a helium-filled balloon, and from the International Space Station (ISS). Even though the Lyrids are not noted for spectacular rates, the combination of New Moon and a favorable viewing geometry from ISS presented a unique opportunity to simultaneously image shower meteors from above the atmosphere and below it. In the end, however, no meteors were observed simultaneously, and it was impossible to identify Lyrids with 100% confidence among the 155 meteors observed from ISS and the 31 observed from the balloon. Still, this exercise proved successful in that meteors could be observed from a simple and inexpensive balloon-based payload and from less-than-optimal cameras on ISS. 1 Introduction The Lyrids in 2012 attracted the attention of the Meteoroid Environment Office (MEO) for three reasons. First, though their zenith hourly rate (ZHR) isn’t particularly high – only 18 or so – the Moon was new on 21 April, so the Lyrid peak on 22 April could be observed with little to no lunar interference.