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Astronomie in Theorie Und Praxis 8. Auflage in Zwei Bänden Erik Wischnewski
Astronomie in Theorie und Praxis 8. Auflage in zwei Bänden Erik Wischnewski Inhaltsverzeichnis 1 Beobachtungen mit bloßem Auge 37 Motivation 37 Hilfsmittel 38 Drehbare Sternkarte Bücher und Atlanten Kataloge Planetariumssoftware Elektronischer Almanach Sternkarten 39 2 Atmosphäre der Erde 49 Aufbau 49 Atmosphärische Fenster 51 Warum der Himmel blau ist? 52 Extinktion 52 Extinktionsgleichung Photometrie Refraktion 55 Szintillationsrauschen 56 Angaben zur Beobachtung 57 Durchsicht Himmelshelligkeit Luftunruhe Beispiel einer Notiz Taupunkt 59 Solar-terrestrische Beziehungen 60 Klassifizierung der Flares Korrelation zur Fleckenrelativzahl Luftleuchten 62 Polarlichter 63 Nachtleuchtende Wolken 64 Haloerscheinungen 67 Formen Häufigkeit Beobachtung Photographie Grüner Strahl 69 Zodiakallicht 71 Dämmerung 72 Definition Purpurlicht Gegendämmerung Venusgürtel Erdschattenbogen 3 Optische Teleskope 75 Fernrohrtypen 76 Refraktoren Reflektoren Fokus Optische Fehler 82 Farbfehler Kugelgestaltsfehler Bildfeldwölbung Koma Astigmatismus Verzeichnung Bildverzerrungen Helligkeitsinhomogenität Objektive 86 Linsenobjektive Spiegelobjektive Vergütung Optische Qualitätsprüfung RC-Wert RGB-Chromasietest Okulare 97 Zusatzoptiken 100 Barlow-Linse Shapley-Linse Flattener Spezialokulare Spektroskopie Herschel-Prisma Fabry-Pérot-Interferometer Vergrößerung 103 Welche Vergrößerung ist die Beste? Blickfeld 105 Lichtstärke 106 Kontrast Dämmerungszahl Auflösungsvermögen 108 Strehl-Zahl Luftunruhe (Seeing) 112 Tubusseeing Kuppelseeing Gebäudeseeing Montierungen 113 Nachführfehler -
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. -
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. -
Anousheh Ansari
: Fort Worth Astronomical Society (Est. 1949) August 2010 Astronomical League Member At the August Meeting: Special Guest Anousheh Ansari Club Calendar – 2 – 3 Skyportunities Star Party & Club Reports – 5 House Calls by Ophiuchus – 6 Hubble’s Amazing Rescue – 8 Your Most Important Optics -- 9 Stargazers’ Diary – 11 1 Milky Way Over Colorado by Jim Murray August 2010 Sunday Monday Tuesday Wednesday Thursday Friday Saturday 1 2 3 4 5 6 7 Third Qtr Moon Challenge binary star for August: Make use of the New Viking 1 Orbiter 11:59 pm Moon Weekend for Alvan Clark 11 (ADS 11324) (Serpens Cauda) ceases operation better viewing at the 30 years ago Notable carbon star for August: Dark Sky Site Mars : Saturn O V Aquilae 1.9 Conjunction Mercury at greatest Challenge deep-sky object for August: eastern elongation Venus, Mars and Abell 53 (Aquila) Saturn all within a this evening binocular field of First in-flight New Moon view for the first 12 New Moon shuttle repair Neal Armstrong Weekend Weekend days of August. 15 years ago born 80 years ago 8 9 10 11 12 13 14 New Moon Moon at Perigee Double shadow (224,386 miles) transit on Jupiter 3RF Star Party 10:08 pm 1 pm 5:12am High in SSW Museum Star (A.T. @ 5:21 am) Party Venus : Saturn O . 3 of separation Perseid Meteor Watch Party @ 3RF New Moon Magellan enters Fairly consistent show Weekend orbit around Venus of about 60 per hour 20 years ago 15 16 17 18 19 20 21 Algol at Minima 2:45 am - In NE First Qtr Moon Total Solar 1:14 pm Eclipse in 7 years Nearest arc of totality takes in FWAS Grand Island NE St Joseph MO Meeting With Neptune @ Columbia MO Venus at greatest Opposition Anousheh Algol at Minima eastern elongation N of Nashville TN 11:34pm Low In NE 5 am N of Charleston SC Ansari this evening 22 23 24 25 26 27 28 Full Moon Moon at Apogee 2:05 pm (252,518.miles) GATE CODES Smallest of 2010 1 am to the (within 11 hrs of apogee) DARK SKY SITE will be changed st September 1 BE SURE YOU ARE CURRENT WITH DUES to Astroboy’s Day Job Venus : Mars receive new codes O 2 Conjunction 29 31 30 Anousheh Ansari’s Mission Patch at right. -
GTO Keypad Manual, V5.001
ASTRO-PHYSICS GTO KEYPAD Version v5.xxx Please read the manual even if you are familiar with previous keypad versions Flash RAM Updates Keypad Java updates can be accomplished through the Internet. Check our web site www.astro-physics.com/software-updates/ November 11, 2020 ASTRO-PHYSICS KEYPAD MANUAL FOR MACH2GTO Version 5.xxx November 11, 2020 ABOUT THIS MANUAL 4 REQUIREMENTS 5 What Mount Control Box Do I Need? 5 Can I Upgrade My Present Keypad? 5 GTO KEYPAD 6 Layout and Buttons of the Keypad 6 Vacuum Fluorescent Display 6 N-S-E-W Directional Buttons 6 STOP Button 6 <PREV and NEXT> Buttons 7 Number Buttons 7 GOTO Button 7 ± Button 7 MENU / ESC Button 7 RECAL and NEXT> Buttons Pressed Simultaneously 7 ENT Button 7 Retractable Hanger 7 Keypad Protector 8 Keypad Care and Warranty 8 Warranty 8 Keypad Battery for 512K Memory Boards 8 Cleaning Red Keypad Display 8 Temperature Ratings 8 Environmental Recommendation 8 GETTING STARTED – DO THIS AT HOME, IF POSSIBLE 9 Set Up your Mount and Cable Connections 9 Gather Basic Information 9 Enter Your Location, Time and Date 9 Set Up Your Mount in the Field 10 Polar Alignment 10 Mach2GTO Daytime Alignment Routine 10 KEYPAD START UP SEQUENCE FOR NEW SETUPS OR SETUP IN NEW LOCATION 11 Assemble Your Mount 11 Startup Sequence 11 Location 11 Select Existing Location 11 Set Up New Location 11 Date and Time 12 Additional Information 12 KEYPAD START UP SEQUENCE FOR MOUNTS USED AT THE SAME LOCATION WITHOUT A COMPUTER 13 KEYPAD START UP SEQUENCE FOR COMPUTER CONTROLLED MOUNTS 14 1 OBJECTS MENU – HAVE SOME FUN! -
Downloaded at %20Package.Zip
Data analysis of 2005 Regulus occultation and simulation of the 2014 occultation Costantino Sigismondi, ICRANet, UFRJ and Observatorio Nacional, Rio de Janeiro [email protected] Tony George, IOTA North America [email protected] Thomas Flatrès, IOTA European Section [email protected] Abstract On March 20, 2014 at 6:06 UT (2:06 New York time) Regulus, the 1.3 magnitude brighter star of Leo constellation, is going to be occulted by the asteroid 163 Erigone. The unusual event, visible to the naked eye over NYC, can allow to measure the shape of the asteroid, with reaching a space resolution below the diffraction limit of the eye, and of all instruments not based on interferometry. Ultimately the aperture of the instrument is related to the amount of scintillation affecting the light curve of the occultation, limitating the accuracy of video recorded data. The asteroid profile scans the surface of the star at a velocity of 6 mas/s; the diameter of the star is about 1.3 mas and the detection of the stellar limb darkening signature is discussed, taking into consideration also the Fresnel fringes. New data reduction with R-OTE software of the 2005 Regulus occultation and simulations of the 2014 occultation with Fren_difl software are presented. The occultation of Regulus of March 20, 2014 above New York City The total solar eclipse of 1925 above New York area [5] and the occultation of delta Ophiuchi above France and Germany in 2010 [4] have been two occultation events followed by a relatively high number of observers. Potentially the occultation of 1.3 mas [8] first magnitude star Regulus over New York City can be the first asteroidal occultation observed by million people and broadcasted on the internet [23]. -
Lllrd General Assembly Leiden The
.lllrd General Assembly Leiden The Netherlands 1928 Ille Assemblée Générale Leiden, Pays Bas 1928 IIIrd General Assembly, Leiden, The Netherlands, 1928 IIIe Assemblée Générale, Leiden, Pays Bas, 1928 Proposée par le Comité Exécutif I. Le Comité exécutif est prié de formuler les règles fixant la qualité de membre de l'Union, indépendamment de celle de membre d'une commission. 2. Le Comité exécutif est prié de nommer, au moment le plus opportun, une commission pour procéder à la révision des statuts et présenter un rapport à l'Assemblée générale. 3· La Commission 15 est incorporée à la Commission 12. 4. Le nom de la Commission 29 est changé en "Commission des spectres stellaires." 5· Le Comité exécutif exprime le vœu que jusqu'à la fin de la présente con vention (31 décembre 1931) la Direction du Bureau de l'Heure soit assumée par le Directeur de l'Observatoire de Paris et qu'après cette époque les fonctions actuelles du Bureau de l'Heure puissent être continuées sans grever le budget de l'Union, par exemple avec l'aide éventuelle des observatoires ou d'autres institutions. 6. Une nouvelle commission (35) "De la constitution des étoiles" est formée. Illrd General Assembly, Leiden, The Netherlands, 1928 Ille Assemblée Générale, Leiden, Pays Bas, 1928 Proposée par le Comité des Finances Commission des finances. 1. L'unité de cotisation pour les années 1929, 1930 et 1931 est fixée à 450 francs or (soit 2250 francs actuels (Paris), ou 86·87 dollars (New-York), ou f I 7· 17s. (London) ). 2. A l'avenir, la balance des comptes en fin d'exercice sera donnée en francs or et en livres sterling. -
Occultations with Video
Observing Asteroidal Occultations from Multiple Stations 2012 August 26 ESOP-31, Pescara, Italy David W. Dunham, IOTA Remote Stations for Asteroidal Occultations • Separation should be many km, much larger than for grazes, so tracking times & errors are too large • Unguided is possible since the prediction times are accurate enough, to less that 1 min. = ¼° • Point telescope beforehand to same altitude and azimuth that the target star will have at event time and keep it fixed in that direction • Plot line of target star’s declination on a detailed star atlas; I used the Millennium Atlas, but now use Guide 8 to produce the charts • From the RA difference and event time for the area of observation, calculate times along the declination line • Adjust the above for sidereal rate that is faster than solar rate, add 10 seconds for each hour before the event • Can usually find “guide stars” that are easier to find than the target • Find a safe but accessible place for both the attended & remote scopes • Separation distance limited by travel time & tape to start tapes, but we have had some success with programmable remote control devices to turn on the recordings; then the only limit is battery life, which can be several hours • Roger Venable uses VCR’s with timed starts, allows larger separation • Sometimes it is better to have remote sites attended for starting equipment later (allows larger separations) and security Occultation of the 6.0-mag. Close Double Star SAO 78349 by (9) Metis on 2001 September 7 • The star was known to be a close double, sep. -
University Microfilms, a XEROX Company, Ann Arbor, Michigan
CARBON-MONOXIDE ABSORPTION IN K AND M GIANTS AND THE CARBON-12/CARBON-13 ABUNDANCE RATIO Item Type text; Dissertation-Reproduction (electronic) Authors Bailey, Wayne Lewis, 1942- Publisher The University of Arizona. Rights Copyright © is held by the author. Digital access to this material is made possible by the University Libraries, University of Arizona. Further transmission, reproduction or presentation (such as public display or performance) of protected items is prohibited except with permission of the author. Download date 23/09/2021 15:08:21 Link to Item http://hdl.handle.net/10150/290269 71-24,887 BAILEY, Wayne Lewis, 1942- CARBON MONOXIDE ABSORPTION IN K AND M GIANTS AND THE C12/C13 ABUNDANCE RATIO. The University of Arizona, Ph.D., 1971 Astrophysics University Microfilms, A XEROX Company, Ann Arbor, Michigan THIS DISSERTATION HAS BEEN MICROFILMED EXACTLY AS RECEIVED CARBON MONOXIDE ABSORPTION IN K AND M GIANTS AND THE C12/C13 ABUNDANCE RATIO by Wayne Lewis Bailey A Dissertation Submitted to the Faculty of the DEPARTMENT OF ASTRONOMY In Partial Fulfillment of the Requirements For the Degree of DOCTOR OF PHILOSOPHY In the Graduate College THE UNIVERSITY OF ARIZONA 19 7 1 THE UNIVERSITY OF ARIZONA GRADUATE COLLEGE I hereby recommend that this dissertation prepared under my direction by Wayne Lewis Bailey entitled Carbon Monoxide Absorption in K and M Giants and the C*VC*3 Abundance Ratio be accepted as fulfilling the dissertation requirement of the degree of Doctor of Philosophy Dissertation Director f Date/7 After inspection of the final copy of the dissertation, the following members of the Final Examination Committee concur in its approval and recommend its acceptance:* P {.i/flo. -
University Microfilms, a XEROX Company, Ann Arbor, Michigan
CARBON-MONOXIDE ABSORPTION IN K AND M GIANTS AND THE CARBON-12/CARBON-13 ABUNDANCE RATIO Item Type text; Dissertation-Reproduction (electronic) Authors Bailey, Wayne Lewis, 1942- Publisher The University of Arizona. Rights Copyright © is held by the author. Digital access to this material is made possible by the University Libraries, University of Arizona. Further transmission, reproduction or presentation (such as public display or performance) of protected items is prohibited except with permission of the author. Download date 05/10/2021 18:12:40 Link to Item http://hdl.handle.net/10150/290269 71-24,887 BAILEY, Wayne Lewis, 1942- CARBON MONOXIDE ABSORPTION IN K AND M GIANTS AND THE C12/C13 ABUNDANCE RATIO. The University of Arizona, Ph.D., 1971 Astrophysics University Microfilms, A XEROX Company, Ann Arbor, Michigan THIS DISSERTATION HAS BEEN MICROFILMED EXACTLY AS RECEIVED CARBON MONOXIDE ABSORPTION IN K AND M GIANTS AND THE C12/C13 ABUNDANCE RATIO by Wayne Lewis Bailey A Dissertation Submitted to the Faculty of the DEPARTMENT OF ASTRONOMY In Partial Fulfillment of the Requirements For the Degree of DOCTOR OF PHILOSOPHY In the Graduate College THE UNIVERSITY OF ARIZONA 19 7 1 THE UNIVERSITY OF ARIZONA GRADUATE COLLEGE I hereby recommend that this dissertation prepared under my direction by Wayne Lewis Bailey entitled Carbon Monoxide Absorption in K and M Giants and the C*VC*3 Abundance Ratio be accepted as fulfilling the dissertation requirement of the degree of Doctor of Philosophy Dissertation Director f Date/7 After inspection of the final copy of the dissertation, the following members of the Final Examination Committee concur in its approval and recommend its acceptance:* P {.i/flo. -
The Fixed Stars Report Hillary Rodham Clinton
The Fixed Stars Report by Tara Cochrane for Hillary Rodham Clinton October 26, 1947 8:00 PM Chicago, Illinois Calculated for: Standard time, Time Zone 6 hours West Latitude: 41 N 51 Longitude: 87 W 39 Introduction Report and Text Copyright 2009 Cosmic Patterns Software, Inc. The contents of this report are protected by Copyright law. By purchasing this report you agree to comply with this Copyright. This report interprets conjunctions of nearly every fixed star that has been given an astrological name to the planets, Asc, MC, 7th house cusp, and 4th cusp. Each interpretation given in this report is based on extensive research on the historical astrological meanings and myths associated with the fixed stars. A list of notable people who have the same conjunction aspect as you do is also given. This comprehensive analysis of the influence of the fixed stars combined with a list of notable people who also have this aspect provides you with extensive information, and hopefully astrologers who use this report can use this information to develop an even more refined and clearer understanding of the meaning of every fixed stars. Interpretations of the Fixed Stars Sun conjunct Alkalurops, Orb: 0 deg 22 min Independent, stable, autonomous, willful, assertive and decisive attributes are indicated. The individual may feel called to provide wisdom, guidance, oversight or direction to others. A position of authority and respect may be attained. Political, executive, regulatory and custodial pursuits are favored. Alkalurops is Mu 1 Bootis in the constellation of Bootes, the Herdsman. The name Alkalurops is derived from the Greek word for a shepherd's crooked staff. -
GTO KEYPAD Version V4.19.3
ASTRO-PHYSICS GTO KEYPAD Version v4.19.3 Flash RAM Updates Keypad flash RAM updates can be accomplished through the Internet. Check our web site www.astro-physics.com periodically for further information. July 29, 2016 Contents About this mAnuAl 5 GTO KeypAd ContRolleR 6 layout and buttons of the Keypad 6 Vacuum Fluorescent display 6 n-s-e-W directional buttons 6 RA/deC ReV button: 6 STOP button 7 number buttons 7 <pReV and neXt> buttons 7 Goto button 7 ± button 7 menu button 7 FoC button 7 Retractable hanger 7 Keypad protector 7 installation: 8 Keypad Care and Warranty 8 Warranty 8 Keypad battery for 256K memory boards 8 Keypad battery for 512K memory boards 8 Cleaning Keypad display 8 temperature Ratings 8 GettinG stARted – do this At home, iF possible 9 setup your mount and Cable Connections 9 Gather basic information 9 enter your location, date and time 9 practice using your Keypad 11 youR FiRst obseRVinG session & FoR poRtAble mounts 12 normal startup sequence for mounts that are in the field 12 Assemble your mount 12 startup sequence 12 star sync 12 Resume last position 13 new setup → new setup start From park position (press 1, 2, 3, or 4) 13 helpful hints 13 AUTO-ConneCt seQuenCe – FoR peRmAnent, polAR-AliGned mounts 14 important points 14 eXteRnAl stARtup seQuenCe – FoR ComputeR ContRolled mounts 15 important points 15 polAR AliGnment – WhiCh method to Choose? 16 n polar Calibrate - Calibrating with polaris 16 two-star Calibration 17 polar Aligning in the daytime – northern hemisphere 20 polar Aligning in the daytime – southern