MARS 2020 ARRIVES at the RED Planetp. 24
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Optical Astronomy Catalogues, Coordinates Visible Objects on the Sky • Stars • Planets • Comets & Asteroids • Nebulae & Galaxies
Astrophysics Content: 2+2, 2×13×90 = 2 340 minutes = 39 hours Tutor: Martin Žáček [email protected] department of Physics, room 49 On-line informations: http://fyzika.feld.cvut.cz/~zacek/ … this presentation Many years (20?) teaching astrophysics (Prof. Petr Kulhanek), many texts and other materials but mostly in Czech (for example electronic journal Aldebaran Bulletin). 2011 … first year of teaching Astrophysics in English 2012-16 … 2017 … about 6 students, lextures on Thursday 11:00 lecture and 12:45 exercise https://www.fel.cvut.cz/cz/education/bk/predmety/12/77/p12773704.html ... AE0B02ASF https://www.fel.cvut.cz/cz/education/bk/predmety/12/78/p12784304.html ... AE0M02ASF Syllabus Classes: Astronomy & astrophysics 1. Astrophysics, history and its place in context of natural sciences. 2. Foundations of astronomy, history, its methods, instruments. 3. Solar system, inner and outer planets, Astronomical coordinates. Physics of stars 4. Statistics of stars, HR diagram. The star formation and evolution. Hyashi line. 5. Final evolutionary stages. White dwarfs, neutron stars, black holes. 6. Variable stars. Cepheids. Novae and supernovae stars. Binary systems. 7. Other galactic and extragalactic objects, nebulae, star clusters, galaxies. Cosmology 8. Principle of special and general theory of relativity. Relativistic experiments. 9. Cosmology. The Universe evolution, cosmological principle. Friedman models. 10. Supernovae Ia, cosmological parameters of the Universe, dark matter and dark energy. 11. Elementary particles, fundamental forces, quantum field theory, Feynman diagrams. 12. The origin of the Universe. Quark-gluon plasma. Nucleosynthesis. Microwave background radiation. 13. Cosmology with the inflationary phase, long-scale structure of the Universe. 14. Reserve Syllabus Practices: Astronomy & astrophysics 1. -
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. -
Journal Issue 26 | October 2019
journal Issue 26 | October 2019 Communicating Astronomy with the Public Spotlighting a Black Hole What did it take to create the largest outreach campaign for an astronomical result? Tactile Subaru A project to make telescope technology accessible Naming ExoWorlds Update on the IAU100 NameExoWorlds campaign www.capjournal.org As part of the 100th anniversary commemorations, the International Astronomical Union (IAU) is organising the IAU100 NameExoWorlds global competition to allow any country in the world to give a popular name to a selected exoplanet and its News News host star. The final results of the competion will be announced in Decmeber 2019. Credit: IAU/L. Calçada. Editorial Welcome to the 26th edition of the CAPjournal! To start off, the first part of 2019 brought in a radical new era in astronomy with the first ever image showing a shadow of a black hole. For CAPjournal #26, part of the team who collaborated on the promotion of this image hs written a piece to show what it took to produce one of the largest astronomy outreach campaigns to date. We also highlight two other large outreach campaigns in this edition. The first is a peer-reviewed article about the 2016 solar eclipse in Indonesia from the founder of the astronomy website lagiselatan, Avivah Yamani. Next, an update on NameExoWorlds, the largest IAU100 campaign, as we wait for the announcement of new names for the ExoWorlds in December. Additionally, this issue touches on opportunities for more inclusive astronomy. We bring you a peer-reviewed article about outreach for inclusion by Dr. Kumiko Usuda-Sato and the speech “Diversity Across Astronomy Can Further Our Research” delivered by award-winning astronomy communicator Dr. -
Messier Objects
Messier Objects From the Stocker Astroscience Center at Florida International University Miami Florida The Messier Project Main contributors: • Daniel Puentes • Steven Revesz • Bobby Martinez Charles Messier • Gabriel Salazar • Riya Gandhi • Dr. James Webb – Director, Stocker Astroscience center • All images reduced and combined using MIRA image processing software. (Mirametrics) What are Messier Objects? • Messier objects are a list of astronomical sources compiled by Charles Messier, an 18th and early 19th century astronomer. He created a list of distracting objects to avoid while comet hunting. This list now contains over 110 objects, many of which are the most famous astronomical bodies known. The list contains planetary nebula, star clusters, and other galaxies. - Bobby Martinez The Telescope The telescope used to take these images is an Astronomical Consultants and Equipment (ACE) 24- inch (0.61-meter) Ritchey-Chretien reflecting telescope. It has a focal ratio of F6.2 and is supported on a structure independent of the building that houses it. It is equipped with a Finger Lakes 1kx1k CCD camera cooled to -30o C at the Cassegrain focus. It is equipped with dual filter wheels, the first containing UBVRI scientific filters and the second RGBL color filters. Messier 1 Found 6,500 light years away in the constellation of Taurus, the Crab Nebula (known as M1) is a supernova remnant. The original supernova that formed the crab nebula was observed by Chinese, Japanese and Arab astronomers in 1054 AD as an incredibly bright “Guest star” which was visible for over twenty-two months. The supernova that produced the Crab Nebula is thought to have been an evolved star roughly ten times more massive than the Sun. -
Gamma Ray Bursts (Grbs)
15 Epilogue Roger D. Blandford Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA The preceding fourteen chapters have been written at a good time to take stock of the field of Gamma Ray Bursts (GRBs). The extraordinary discov- eries made over the last decade or so about a phenomenon that has been around for over four decades seem to have attained a mature state. Thou- sands of bursts have been observed, classified and followed up and it is now the special and rare cases, that are extreme by some important measure, that are most likely to advance our understanding as radically new γ−ray and X-ray observing capabilities are at least a decade away. On the theoret- ical front, some prescient inferences have been vindicated, phenomenological models that are usable by observers have been developed, and simulation has made great strides. The greatest challenge is to explore the underlying physical processes in much more detail and this is likely to require a new generation of high performance computers. Nonetheless, the GRB pace of discovery like much of contemporary astrophysics will likely exceed that in most other subfields of physical science. I was asked to write a critique of where we are today and what I think will be the major developments going forward. My qualifications for this task are not promising. I have probably contributed most to the study of a high energy γ−ray stellar phenomenon unintentionally in the context of trying to explain variability of the lowest frequency radio emission from active galaxies and my largest attempt to work on what I thought was relevant turned out to be only applicable, at best, to X-ray bursting neutron stars. -
Space Sector Brochure
SPACE SPACE REVOLUTIONIZING THE WAY TO SPACE SPACECRAFT TECHNOLOGIES PROPULSION Moog provides components and subsystems for cold gas, chemical, and electric Moog is a proven leader in components, subsystems, and systems propulsion and designs, develops, and manufactures complete chemical propulsion for spacecraft of all sizes, from smallsats to GEO spacecraft. systems, including tanks, to accelerate the spacecraft for orbit-insertion, station Moog has been successfully providing spacecraft controls, in- keeping, or attitude control. Moog makes thrusters from <1N to 500N to support the space propulsion, and major subsystems for science, military, propulsion requirements for small to large spacecraft. and commercial operations for more than 60 years. AVIONICS Moog is a proven provider of high performance and reliable space-rated avionics hardware and software for command and data handling, power distribution, payload processing, memory, GPS receivers, motor controllers, and onboard computing. POWER SYSTEMS Moog leverages its proven spacecraft avionics and high-power control systems to supply hardware for telemetry, as well as solar array and battery power management and switching. Applications include bus line power to valves, motors, torque rods, and other end effectors. Moog has developed products for Power Management and Distribution (PMAD) Systems, such as high power DC converters, switching, and power stabilization. MECHANISMS Moog has produced spacecraft motion control products for more than 50 years, dating back to the historic Apollo and Pioneer programs. Today, we offer rotary, linear, and specialized mechanisms for spacecraft motion control needs. Moog is a world-class manufacturer of solar array drives, propulsion positioning gimbals, electric propulsion gimbals, antenna positioner mechanisms, docking and release mechanisms, and specialty payload positioners. -
Ice& Stone 2020
Ice & Stone 2020 WEEK 51: DECEMBER 13-19 Presented by The Earthrise Institute # 51 Authored by Alan Hale COMET OF THE WEEK: The Great Comet of 1680 Perihelion: 1680 December 18.49, q = 0.006 AU The Great Comet of 1680 over Rotterdam in The Netherlands, during late December 1680 as painted by the Dutch artist Lieve Verschuier. This particular comet was undoubtedly one of the brightest comets of the 17th Century, but it is also one of the most important comets in history from a scientific perspective, and perhaps even from the perspective of overall human history. While there were certainly plenty of superstitions attached to the comet’s appearance, the scientific investigations made of it were among the beginnings of the era in European history we now call The Enlightenment, and indeed, in a sense the Great Comet of 1680 can perhaps be considered as one of the sparks of that era. The significance began with the comet’s discovery, which was made on the morning of November 14, 1680, by a German astronomer residing in Coburg, Gottfried Kirch – the first comet ever to be discovered by means of a telescope. It was already around 4th magnitude at that time, and located near the star Regulus in the constellation Leo; from that point it traveled eastward and brightened rapidly, being closest to Earth (0.42 AU) on November 30. By that time it was a conspicuous naked-eye object with a tail 20 to 30 degrees long, and it remained visible for another week before disappearing into morning twilight. -
Exoplanet Community Report
JPL Publication 09‐3 Exoplanet Community Report Edited by: P. R. Lawson, W. A. Traub and S. C. Unwin National Aeronautics and Space Administration Jet Propulsion Laboratory California Institute of Technology Pasadena, California March 2009 The work described in this publication was performed at a number of organizations, including the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration (NASA). Publication was provided by the Jet Propulsion Laboratory. Compiling and publication support was provided by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. Reference herein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or otherwise, does not constitute or imply its endorsement by the United States Government, or the Jet Propulsion Laboratory, California Institute of Technology. © 2009. All rights reserved. The exoplanet community’s top priority is that a line of probeclass missions for exoplanets be established, leading to a flagship mission at the earliest opportunity. iii Contents 1 EXECUTIVE SUMMARY.................................................................................................................. 1 1.1 INTRODUCTION...............................................................................................................................................1 1.2 EXOPLANET FORUM 2008: THE PROCESS OF CONSENSUS BEGINS.....................................................2 -
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. -
GCSE Astronomy Coursework
GCSE Astronomy Coursework A5 & B5 Drawings or Photos of Celestial Event Produce a series of drawings (A5) or detailed telescopic drawings or photographs (B5) to record the passage of a suitable celestial event, for example a transit, occultation or comet. Venus and Mercury are the two inferior planets (planets that orbit between the Earth and the Sun). Their orbits are slightly inclined with respect to the Earth’s orbital plane but sometimes they pass in between the Earth and the Sun – this is called a transit. Dates for the next set of transits can be found here: http://eclipse.gsfc.nasa.gov/transit/transit.html When an object is eclipsed by another object in the sky it is called an occultation. Information about future occultations and all other celestial events can be found here: www.theguardian.com/science/series/starwatch Comets are balls of ice and rock that exist in two regions in the outer Solar System: the Kuiper Belt and the Oort Cloud. Occasionally they are knocked and are sent flying past the planets. When they reach the Sun the ice sublimates leaving behind a tail. A list of visible comets can be found here: www.ast.cam.ac.uk/~jds/future.htm To locate objects use www.stellarium.org or alternatively download an app for your mobile: http://downloads.bbc.co.uk/tv/guides/ BBC_Stargazing_Live_2012_Mobile_App_guides.pdf To find sunrise, sunset, moonrise and moonset times and the phase of the Moon use www.timeanddate.com Check the weather forecast - www.metoffice.gov.uk See our useful guides for help on how to carry out observations and take photographs of various objects: www.rmg.co.uk/discover/astronomy- photographer-competition/how-to-guides For examples of reports with moderator comments visit the Edexcel GCSE Astronomy website: http://www.edexcel.com/quals/gcse/gcse09/ astronomy/Pages/default.aspx Here you will find two documents that will help you write a report: Under ‘Controlled assessment’ download ‘Controlled Assessment Teacher Support Book’ and under ‘Teacher Support Materials’ download ‘GCSE Astronomy Teachers Guide’. -
Prime Focus Page 2 August 2020 the Third Time Is Indeed the Charm
Highlights of the August Sky - - - 1st - - - DAWN: Venus and Zeta (ζ) Tauri are less than 2° apart. DUSK: A waxing gibbous Moon, Jupiter, and Saturn form a triangle. - - - 3rd - - - Full Moon 11:59 am EDT KAS - - - 9th - - - AM: Mars and a waning gibbous Moon are 1° apart. Perseid Potluck Picnic: Saturday, August 8 @ 6:00 pm - - - 11th - - - Last Quarter Moon ― Canceled Due to the Coronavirus Pandemic ― 12:45 pm EDT PM: Perseid Meteor Shower Member Observing: Saturday, August 8 @ 9:00 pm peaks. Jupiter, Saturn & The Summer Triangle • See Page 13 for Details th - - - 13 - - - AM: A waning crescent Moon and Aldebaran are Training Session: August 14, 21 & 28 @ 8:00 pm less than 4° apart. Owl Observatory • See Page 14 for Details and to Register th - - - 15 - - - DAWN: A slender waning crescent Moon is 3.5° to the Member Observing: Saturday, August 22 @ 9:00 pm upper le of Venus. Jupiter, Saturn & Summer Nebulae • See Page 13 for Details - - - 18th - - - New Moon 10:42 pm EDT - - - 22nd - - - Inside the Newsletter. DUSK: A waxing crescent Moon is over 5° to Spica’s upper right. Board Meeng Minutes..................... p. 2 - - - 25th - - - Observaons of NEOWISE................. p. 3 First Quarter Moon 1:58 pm EDT Member NEOWISE Images................ p. 4 DUSK: The Moon is 6° to the KAS Member Observatories...............p. 7 upper right of Antares. Stellar Walkabout.............................. p. 8 th - - - 27 - - - NASA Night Sky Notes........................ p. 10 DUSK: The Moon, Jupiter, and Saturn form a line. Membership of the KAS..................... p. 11 - - - 28th - - - August Night Sky................................ p. 12 DUSK: A gibbous Moon and Jupiter are separated by 2°. -
Stars and Their Spectra: an Introduction to the Spectral Sequence Second Edition James B
Cambridge University Press 978-0-521-89954-3 - Stars and Their Spectra: An Introduction to the Spectral Sequence Second Edition James B. Kaler Index More information Star index Stars are arranged by the Latin genitive of their constellation of residence, with other star names interspersed alphabetically. Within a constellation, Bayer Greek letters are given first, followed by Roman letters, Flamsteed numbers, variable stars arranged in traditional order (see Section 1.11), and then other names that take on genitive form. Stellar spectra are indicated by an asterisk. The best-known proper names have priority over their Greek-letter names. Spectra of the Sun and of nebulae are included as well. Abell 21 nucleus, see a Aurigae, see Capella Abell 78 nucleus, 327* ε Aurigae, 178, 186 Achernar, 9, 243, 264, 274 z Aurigae, 177, 186 Acrux, see Alpha Crucis Z Aurigae, 186, 269* Adhara, see Epsilon Canis Majoris AB Aurigae, 255 Albireo, 26 Alcor, 26, 177, 241, 243, 272* Barnard’s Star, 129–130, 131 Aldebaran, 9, 27, 80*, 163, 165 Betelgeuse, 2, 9, 16, 18, 20, 73, 74*, 79, Algol, 20, 26, 176–177, 271*, 333, 366 80*, 88, 104–105, 106*, 110*, 113, Altair, 9, 236, 241, 250 115, 118, 122, 187, 216, 264 a Andromedae, 273, 273* image of, 114 b Andromedae, 164 BDþ284211, 285* g Andromedae, 26 Bl 253* u Andromedae A, 218* a Boo¨tis, see Arcturus u Andromedae B, 109* g Boo¨tis, 243 Z Andromedae, 337 Z Boo¨tis, 185 Antares, 10, 73, 104–105, 113, 115, 118, l Boo¨tis, 254, 280, 314 122, 174* s Boo¨tis, 218* 53 Aquarii A, 195 53 Aquarii B, 195 T Camelopardalis,