Meteor Activity Outlook for November 30 - December 6, 2019
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Mathématiques Et Espace
Atelier disciplinaire AD 5 Mathématiques et Espace Anne-Cécile DHERS, Education Nationale (mathématiques) Peggy THILLET, Education Nationale (mathématiques) Yann BARSAMIAN, Education Nationale (mathématiques) Olivier BONNETON, Sciences - U (mathématiques) Cahier d'activités Activité 1 : L'HORIZON TERRESTRE ET SPATIAL Activité 2 : DENOMBREMENT D'ETOILES DANS LE CIEL ET L'UNIVERS Activité 3 : D'HIPPARCOS A BENFORD Activité 4 : OBSERVATION STATISTIQUE DES CRATERES LUNAIRES Activité 5 : DIAMETRE DES CRATERES D'IMPACT Activité 6 : LOI DE TITIUS-BODE Activité 7 : MODELISER UNE CONSTELLATION EN 3D Crédits photo : NASA / CNES L'HORIZON TERRESTRE ET SPATIAL (3 ème / 2 nde ) __________________________________________________ OBJECTIF : Détermination de la ligne d'horizon à une altitude donnée. COMPETENCES : ● Utilisation du théorème de Pythagore ● Utilisation de Google Earth pour évaluer des distances à vol d'oiseau ● Recherche personnelle de données REALISATION : Il s'agit ici de mettre en application le théorème de Pythagore mais avec une vision terrestre dans un premier temps suite à un questionnement de l'élève puis dans un second temps de réutiliser la même démarche dans le cadre spatial de la visibilité d'un satellite. Fiche élève ____________________________________________________________________________ 1. Victor Hugo a écrit dans Les Châtiments : "Les horizons aux horizons succèdent […] : on avance toujours, on n’arrive jamais ". Face à la mer, vous voyez l'horizon à perte de vue. Mais "est-ce loin, l'horizon ?". D'après toi, jusqu'à quelle distance peux-tu voir si le temps est clair ? Réponse 1 : " Sans instrument, je peux voir jusqu'à .................. km " Réponse 2 : " Avec une paire de jumelles, je peux voir jusqu'à ............... km " 2. Nous allons maintenant calculer à l'aide du théorème de Pythagore la ligne d'horizon pour une hauteur H donnée. -
Annual Report 2016–2017 AAVSO
AAVSO The American Association of Variable Star Observers Annual Report 2016–2017 AAVSO Annual Report 2012 –2013 The American Association of Variable Star Observers AAVSO Annual Report 2016–2017 The American Association of Variable Star Observers 49 Bay State Road Cambridge, MA 02138-1203 USA Telephone: 617-354-0484 Fax: 617-354-0665 email: [email protected] website: https://www.aavso.org Annual Report Website: https://www.aavso.org/annual-report On the cover... At the 2017 AAVSO Annual Meeting.(clockwise from upper left) Knicole Colon, Koji Mukai, Dennis Conti, Kristine Larsen, Joey Rodriguez; Rachid El Hamri, Andy Block, Jane Glanzer, Erin Aadland, Jamin Welch, Stella Kafka; and (clockwise from upper left) Joey Rodriguez, Knicole Colon, Koji Mukai, Frans-Josef “Josch” Hambsch, Chandler Barnes. Picture credits In additon to images from the AAVSO and its archives, the editors gratefully acknowledge the following for their image contributions: Glenn Chaple, Shawn Dvorak, Mary Glennon, Bill Goff, Barbara Harris, Mario Motta, NASA, Gary Poyner, Msgr. Ronald Royer, the Mary Lea Shane Archives of the Lick Observatory, Chris Stephan, and Wheatley, et al. 2003, MNRAS, 345, 49. Table of Contents 1. About the AAVSO Vision and Mission Statement 1 About the AAVSO 1 What We Do 2 What Are Variable Stars? 3 Why Observe Variable Stars? 3 The AAVSO International Database 4 Observing Variable Stars 6 Services to Astronomy 7 Education and Outreach 9 2. The Year in Review Introduction 11 The 106th AAVSO Spring Membership Meeting, Ontario, California 11 The -
The Brightest Stars Seite 1 Von 9
The Brightest Stars Seite 1 von 9 The Brightest Stars This is a list of the 300 brightest stars made using data from the Hipparcos catalogue. The stellar distances are only fairly accurate for stars well within 1000 light years. 1 2 3 4 5 6 7 8 9 10 11 12 13 No. Star Names Equatorial Galactic Spectral Vis Abs Prllx Err Dist Coordinates Coordinates Type Mag Mag ly RA Dec l° b° 1. Alpha Canis Majoris Sirius 06 45 -16.7 227.2 -8.9 A1V -1.44 1.45 379.21 1.58 9 2. Alpha Carinae Canopus 06 24 -52.7 261.2 -25.3 F0Ib -0.62 -5.53 10.43 0.53 310 3. Alpha Centauri Rigil Kentaurus 14 40 -60.8 315.8 -0.7 G2V+K1V -0.27 4.08 742.12 1.40 4 4. Alpha Boötis Arcturus 14 16 +19.2 15.2 +69.0 K2III -0.05 -0.31 88.85 0.74 37 5. Alpha Lyrae Vega 18 37 +38.8 67.5 +19.2 A0V 0.03 0.58 128.93 0.55 25 6. Alpha Aurigae Capella 05 17 +46.0 162.6 +4.6 G5III+G0III 0.08 -0.48 77.29 0.89 42 7. Beta Orionis Rigel 05 15 -8.2 209.3 -25.1 B8Ia 0.18 -6.69 4.22 0.81 770 8. Alpha Canis Minoris Procyon 07 39 +5.2 213.7 +13.0 F5IV-V 0.40 2.68 285.93 0.88 11 9. Alpha Eridani Achernar 01 38 -57.2 290.7 -58.8 B3V 0.45 -2.77 22.68 0.57 144 10. -
Astronomical Optical Interferometry, II
Serb. Astron. J. } 183 (2011), 1 - 35 UDC 520.36{14 DOI: 10.2298/SAJ1183001J Invited review ASTRONOMICAL OPTICAL INTERFEROMETRY. II. ASTROPHYSICAL RESULTS S. Jankov Astronomical Observatory, Volgina 7, 11060 Belgrade 38, Serbia E{mail: [email protected] (Received: November 24, 2011; Accepted: November 24, 2011) SUMMARY: Optical interferometry is entering a new age with several ground- based long-baseline observatories now making observations of unprecedented spatial resolution. Based on a great leap forward in the quality and quantity of interfer- ometric data, the astrophysical applications are not limited anymore to classical subjects, such as determination of fundamental properties of stars; namely, their e®ective temperatures, radii, luminosities and masses, but the present rapid devel- opment in this ¯eld allowed to move to a situation where optical interferometry is a general tool in studies of many astrophysical phenomena. Particularly, the advent of long-baseline interferometers making use of very large pupils has opened the way to faint objects science and ¯rst results on extragalactic objects have made it a reality. The ¯rst decade of XXI century is also remarkable for aperture synthesis in the visual and near-infrared wavelength regimes, which provided image reconstruc- tions from stellar surfaces to Active Galactic Nuclei. Here I review the numerous astrophysical results obtained up to date, except for binary and multiple stars milli- arcsecond astrometry, which should be a subject of an independent detailed review, taking into account its importance and expected results at micro-arcsecond precision level. To the results obtained with currently available interferometers, I associate the adopted instrumental settings in order to provide a guide for potential users concerning the appropriate instruments which can be used to obtain the desired astrophysical information. -
Desert Skies Tucson Amateur Astronomy Association
Desert Skies Tucson Amateur Astronomy Association Volume LIV, Number 11 November, 2008 TAAA Members Tour the Large Binocular Telescope ♦ Members’ Night ♦ 2008 Aaronson Lecture ♦ School star parties ♦ TAAA Website & Electronic Newsletter ♦ Constellation of the month ♦ TAAA Astronomy Complex Updates ♦ TAAA Holiday Party ♦ Websites: Trips On The Internet Super- ♦ Observatory Dedication at TIMPA Skyway Desert Skies: November, 2008 2 Volume LIV, Number 11 Cover Photo: TAAA members enjoyed a tour of the large binocular telescope. Photo by Bill Lofquist. TAAA Web Page: http://www.tucsonastronomy.org TAAA Phone Number: (520) 792-6414 Office/Position Name Phone E-mail Address President Ken Shaver 762-5094 [email protected] Vice President Keith Schlottman 290-5883 [email protected] Secretary Luke Scott 749-4867 [email protected] Treasurer Terri Lappin 977-1290 [email protected] Member-at-Large George Barber 822-2392 [email protected] Member-at-Large John Kalas 620-6502 [email protected] Member-at-Large Teresa Plymate 883-9113 [email protected] Chief Observer Dr. Mary Turner 586-2244 [email protected] AL Correspondent (ALCor) Nick de Mesa 797-6614 [email protected] Astro-Imaging SIG Steve Peterson 762-8211 [email protected] Computers in Astronomy SIG Roger Tanner 574-3876 [email protected] Beginners SIG JD Metzger 760-8248 [email protected] Newsletter Editor George Barber 822-2392 [email protected] -
Measurement of Neglected Double Stars with a Mintron Video Camera 43 Rafael Benavides Palencia
University of South Alabama Journal of Double Star Observations VOLUME 5 NUMBER 1 WINTER 2009 Image from "On the Accuracy of Double Star Measurements from "Lucky" Images ..." by Rainer Anton. on page 65 ff. Inside this issue: Divinus Lux Observatory Bulletin: Report #16 2 Dave Arnold An Investigation on the Relative Proper Motion of some Optical Double Stars 10 Joerg S. Schlimmer CCD Double-Star Measurements at Observatorio Astronómico Camino de Palomares (OACP)First Series 18 Edgardo Rubén Masa Martín Measurement of Neglected Double Stars with a Mintron Video Camera 43 Rafael Benavides Palencia Double Star Measures Using a DSLR Camera #2 49 Ernõ Berkó A Comparison of the Astrometric Precision and Accuracy of Double Star Observations with Two Telescopes Pablo Alvarez, Amos E. Fishbein, Michael W. Hyland, Cheyne L. Kight, Hairold Lopez, Tanya 60 Navarro, Carlos A. Rosas, Aubrey E. Schachter, Molly A. Summers, Eric D. Weise, Megan A. Hoffman, Robert C. Mires, Jolyon M. Johnson, Russell M. Genet, and Robin White On the Accuracy of Double Star Measurements from “Lucky” Images, a Case Study of Zeta Aqr and Beta Phe 65 Rainer Anton Vol. 5 No. 1 Winter 2009 Journal of Double Star Observations Page 2 Divinus Lux Observatory: Report #16 Dave Arnold Program Manager for Double Star Research 2728 North Fox Fun Drive Flagstaff, AZ 86004 E-Mail: [email protected] Abstract: This report contains theta/rho measurements from 97 different double star systems. The time period spans from 2008.432 to 2008.721. Measurements were obtained using a 20-cm Schmidt- Cassegrain telescope and an illuminated reticle micrometer. -
The COLOUR of CREATION Observing and Astrophotography Targets “At a Glance” Guide
The COLOUR of CREATION observing and astrophotography targets “at a glance” guide. (Naked eye, binoculars, small and “monster” scopes) Dear fellow amateur astronomer. Please note - this is a work in progress – compiled from several sources - and undoubtedly WILL contain inaccuracies. It would therefor be HIGHLY appreciated if readers would be so kind as to forward ANY corrections and/ or additions (as the document is still obviously incomplete) to: [email protected]. The document will be updated/ revised/ expanded* on a regular basis, replacing the existing document on the ASSA Pretoria website, as well as on the website: coloursofcreation.co.za . This is by no means intended to be a complete nor an exhaustive listing, but rather an “at a glance guide” (2nd column), that will hopefully assist in choosing or eliminating certain objects in a specific constellation for further research, to determine suitability for observation or astrophotography. There is NO copy right - download at will. Warm regards. JohanM. *Edition 1: June 2016 (“Pre-Karoo Star Party version”). “To me, one of the wonders and lures of astronomy is observing a galaxy… realizing you are detecting ancient photons, emitted by billions of stars, reduced to a magnitude below naked eye detection…lying at a distance beyond comprehension...” ASSA 100. (Auke Slotegraaf). Messier objects. Apparent size: degrees, arc minutes, arc seconds. Interesting info. AKA’s. Emphasis, correction. Coordinates, location. Stars, star groups, etc. Variable stars. Double stars. (Only a small number included. “Colourful Ds. descriptions” taken from the book by Sissy Haas). Carbon star. C Asterisma. (Including many “Streicher” objects, taken from Asterism. -
Star Birds of Paradise
deepsky delights Apus the Bird of Paradise says it all and Star Birds of was without doubt the most appreciated feathered bird. Apus the constellation is Paradise located just off the constellation Southern by Magda Streicher Triangle approximately 13 degrees from the South Pole. The ancient Greeks saw [[email protected]] the constellations Apus as the swallow without legs, but it was documented as the Our forefathers, the seafarers and bird of paradise. The German edition of hunters of ancient times most prob- Bayer’s work, issued in 1720, called it the ably developed names for the patterns “Indianischer Vogel” thus it is still some- and shapes outlined by the stars of the times called the “Indian Bird”. In China night sky. Most of them are associ- it is called the Curious Sparrow, or Little ated with the legends of their cultures Wonder Bird. and ways of life. Most of the constel- lation names have Greek and Latin The best-known star-bird constellation shape roots and some are very original. The projected against the night sky is probably Greek language refers to constella- Aquila the Eagle. Situated west of the tions as “signs”, while Hipparchos, constellation Delphinius, this eagle spreads Ptolomy and the Arabians referred its wings and flies eastward over the Milky to them as “figures”. It is generally Way. Already in 1200 B.C. this bird figure accepted that various animals and was represented on a Euphratean stone birds played prominent roles in peo- known as The Eagle, the Living Eye or the ples’ minds in ancient times as can be Bird of Zeus. -
Almanac08 Cov PDF Maker
WESTERN AUSTRALIAN AASTRONOMSTRONOMYY ALMANACALMANAC FREEINCLUDES CD TheThe reallyreally usefuluseful guideguide toto thethe wonderswonders ofof thethe nightnight skysky Highlights: January 24 Lunar Occultation of Regulus February 1 Venus in conjunction with Jupiter February 2 Lunar Occultation of Antares March Venus close to Mercury April 23 Lunar Occultation of Antares July 11 Mars in conjunction with Saturn July 14 Lunar Occultation of Antares August 13 Venus in conjunction with Saturn August 17 Partial lunar eclipse September Mercury, Venus and Mars close in evening twilight October 4 Lunar Occultation of Antares December 1 Venus in conjunction with Jupiter December 29 Lunar Occultation of Jupiter December 31 Mercury in conjunction with Jupiter 20082008 2008 JANUARY 2008 FEBRUARY 2008 MARCH 2008 Sun Mon Tue Wed Thu Fri Sat Sun Mon Tue Wed Thu Fri Sat Sun Mon Tue Wed Thu Fri Sat 12345 12 30 31 1 6 7 8 9101112 3456789 2345678 13 14 15 16 17 18 19 10 11 12 13 14 15 16 9101112131415 20 21 22 23 24 25 26 17 18 19 20 21 22 23 16 17 18 19 20 21 22 27 28 29 30 31 24 25 26 27 28 29 23 24 25 26 27 28 29 APRIL 2008 MAY 2008 JUNE 2008 Sun Mon Tue Wed Thu Fri Sat Sun Mon Tue Wed Thu Fri Sat Sun Mon Tue Wed Thu Fri Sat 12345 123 1234567 6 7 8 9 10 11 12 45678910 8 9 10 11 12 13 14 13 14 15 16 17 18 19 11 12 13 14 15 16 17 15 16 17 18 19 20 21 20 21 22 23 24 25 26 18 19 20 21 22 23 24 22 23 24 25 26 27 28 27 28 29 30 25 26 27 28 29 30 31 29 30 JULY 2008 AUGUST 2008 SEPTEMBER 2008 Sun Mon Tue Wed Thu Fri Sat Sun Mon Tue Wed Thu Fri Sat Sun Mon Tue -
Meteor Activity Outlook for December 5-11, 2020
Meteor Activity Outlook for December 5-11, 2020 Samer Hobeika was photographing this nighttime scene when this bright fireball occurred just above the horizon. It occurred at 04:34 UT (12:34am EST) on 22 August 2020 from Dalkeith, Ontario, Canada. For more details on this particular event visit: https://fireball.amsmeteors.org/members/imo_view/event/2020/4701. Credit Samer Hobeika During this period, the moon reaches its last quarter phase on Tuesday December 8th. At this time, the moon is located 90 degrees west of the sun and rises near midnight local standard time (LST). The evening hours will be free of interfering moonlight and the morning hours can also be used for observing as long as you keep the moon out of your field of view. The estimated total hourly meteor rates for evening observers this week is near 4 as seen from mid-northern latitudes and 3 as seen from tropical southern locations (25S). For morning observers, the estimated total hourly rates should be near 12 as seen from mid-northern latitudes (45N) and 8 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. Rates are reduced during the morning hours due to interfering 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. -
A Collection of Curricula for the STARLAB Constellation Cylinder
A Collection of Curricula for the STARLAB Constellation Cylinder Including: Constellation Identification by Science First/STARLAB. A Look at the Constellations Cylinder by Joyce Kloncz Stories in the Stars by Gary D. Kratzer ©2008 by Science First/STARLAB, 95 Botsford Place, Buffalo, NY 14216. www.starlab.com. All rights reserved. Curriculum Guide Contents Constellation Identification .......................................3 Cancer (The Crab) ...........................................13 Alphabetical Listing of Constellations ........................3 Centaurus (The Centaur) ...................................14 Northern Celestial Pole Constellations .......................4 Corvus (The Crow) ..........................................14 Cassiopeia .......................................................4 Hydra (The Water Snake) .................................14 Cepheus ...........................................................4 Leo (The Lion) ..................................................15 Draco (The Dragon) ...........................................4 Lupus (The Wolf) ..............................................15 Ursa Major (The Great Bear) ..............................5 Virgo (The Virgin) ............................................15 Ursa Minor (The Little Bear) .................................5 Summer Constellations ..........................................17 Autumn Constellations .............................................6 Aquila (The Eagle) ...........................................17 Andromeda (Andromeda) ..................................6 -
Double Star Measurements at the Southern Sky with 50 Cm Reflectors and Fast CCD Cameras in 2012
Vol. 10 No. 3 July 1, 2014 Journal of Double Star Observations Page 232 Double Star Measurements at the Southern Sky with 50 cm Reflectors and Fast CCD Cameras in 2012 Rainer Anton Altenholz/Kiel, Germany e-mail: rainer.anton”at”ki.comcity.de Abstract: A Cassegrain and a Ritchey-Chrétien reflector, both with 50 cm aperture, were used in Namibia for recordings of double stars with fast CCD cameras and a notebook computer. From superposition of “lucky images”, measurements of 39 double and multiple systems were obtained and compared with literature data. Occasional deviations are discussed. Images of some remarkable systems are also presented. the other of type “Chameleon” (Point Grey). The main Introduction difference is the number and size of the pixels, 1024 x As in earlier work, the technique of “lucky imag- 768 of 4.65 µm square for the DMK31, and 1296 x 964 ing” was applied to effectively reduce seeing effects of 3.75 µm for the Chameleon. While the smaller pixel during recording of double star images by using short size of the latter helps in resolving close doubles, it pro- exposure times. With only the best frames being regis- duces somewhat more noise which, however, does vir- tered and stacked, the resolution can approach the theo- tually no harm in short exposures. Resolution values in retical limit of the telescope, and the accuracy of posi- terms of arcsec per pixel for the combinations of tele- tion measurements can even be better than this by about scopes and cameras are listed in Table 1 below.