7 Astronomical Observations
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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. -
Where Are the Distant Worlds? Star Maps
W here Are the Distant Worlds? Star Maps Abo ut the Activity Whe re are the distant worlds in the night sky? Use a star map to find constellations and to identify stars with extrasolar planets. (Northern Hemisphere only, naked eye) Topics Covered • How to find Constellations • Where we have found planets around other stars Participants Adults, teens, families with children 8 years and up If a school/youth group, 10 years and older 1 to 4 participants per map Materials Needed Location and Timing • Current month's Star Map for the Use this activity at a star party on a public (included) dark, clear night. Timing depends only • At least one set Planetary on how long you want to observe. Postcards with Key (included) • A small (red) flashlight • (Optional) Print list of Visible Stars with Planets (included) Included in This Packet Page Detailed Activity Description 2 Helpful Hints 4 Background Information 5 Planetary Postcards 7 Key Planetary Postcards 9 Star Maps 20 Visible Stars With Planets 33 © 2008 Astronomical Society of the Pacific www.astrosociety.org Copies for educational purposes are permitted. Additional astronomy activities can be found here: http://nightsky.jpl.nasa.gov Detailed Activity Description Leader’s Role Participants’ Roles (Anticipated) Introduction: To Ask: Who has heard that scientists have found planets around stars other than our own Sun? How many of these stars might you think have been found? Anyone ever see a star that has planets around it? (our own Sun, some may know of other stars) We can’t see the planets around other stars, but we can see the star. -
FOIA Logs for US Army for 2000
Description of document: FOIA CASE LOGS for: United States Army, Alexandria, VA for 2000 - 2003 Released date: 2003 Posted date: 04-March-2008 Date/date range of document: 03-January-2000 – 27-March-2003 Source of document: Department Of The Army U.S. Army Freedom of Information and Privacy Office Casey Building, Suite 144 Attn: JDRP-RDF 7701 Telegraph Road Alexandria, VA 22315-3905 Phone: (703) 428-6494 Fax: (703) 428-6522 Email: [email protected] The governmentattic.org web site (“the site”) is noncommercial and free to the public. The site and materials made available on the site, such as this file, are for reference only. The governmentattic.org web site and its principals have made every effort to make this information as complete and as accurate as possible, however, there may be mistakes and omissions, both typographical and in content. The governmentattic.org web site and its principals shall have neither liability nor responsibility to any person or entity with respect to any loss or damage caused, or alleged to have been caused, directly or indirectly, by the information provided on the governmentattic.org web site or in this file 2000 FOIA# Rec'd Closed Susp Days Subject Refer By Control # Class AO Action 1 Action 2 Action 3 # Refer Q 00-0433 01/03/2000 04/06/2000 01/14/2000 67 Information on what the name or number of the group or company U SLF CATEGORY 9 0 S stationed in St. John's, Newfoundland during World War II in 1945 (E-Mail) 00-0434 01/03/2000 01/04/2000 01/14/2000 2 Information on the mortality rate of the former -
Volume 25, Number 9 September 2018
Volume 25, Number 9 September 2018 From The Chair’s Report by Bernie Venasse Editor Wow, has Summer I hope everyone has had a great summer. After a two month break, we are about 2018 flown by so to start our monthly meetings again. fast! Some summer events: Our June event was rained out, the July event was clouded-out. I hope you enjoy this first Event Horizon of The public Perseid event was attended by over 900 visitors. A great effort was put the new “school forward by all the volunteers who handled the masses. Thank you all!! year”. Lakeland Park was the site of the August Solar and Celestial event. We welcomed Enjoy! several visitors to the Solar portion of the event. I was joined in the evening by several members who brought their scopes Although cloud and smoke obscured Bob Christmas, the night sky, we managed to get decent views of the moon to show the visiting Editor public. editor ‘AT’ Our September 14 speaker will be Kevin Salwach. Kevin will speak to us about amateurastronomy.org Naked-eye Astronomy. (Continued on page 2) IN THIS ISSUE: § Eye Candy § § The Sky For September 2018 Treasurer’s Report § § Upcoming McCallion Planetarium Shows Cartoon Corner § § CANON and NIKON…taking a walk on the DARK side… Upcoming Events § NASA’s Space Place Contact Information Hamilton Amateur Astronomers Event Horizon September 2018 Page 1 Chair’s Report (continued) Our Annual General Meeting takes place at the October meeting. It’s at this meeting that we look after most of the club’s business for the year, (the delivery of the club’s financial report and the election of the club’s council for the upcoming year). -
The Denver Observer June 2016
The Denver JUNE 2016 OBSERVER Mercury transits the Sun on May 9, 2016. The planet, seen at the lower left of the Sun's face, has a diameter of about 3,000 miles, but the Sun's 870,000 mile cross-section dwarfs the planet—even though the Sun is seen here at twice Mercury's distance from us. (Note the planet-sized sunspots above-left of solar center.) Image © Ron Pearson. JUNE SKIES by Zachary Singer The Solar System the Martian surface reveals itself. On observing runs over the last few If you haven’t been observing Mars, the “unusually bright orange weeks, with good seeing, early views did indeed yield so-so results, but object in Libra,” now is a really good time: As June begins, the plan- improved noticeably as the planet neared its highest point in the south. et is just past opposition, and even more recently past its closest ap- I was able to make out the Syrtis Major region easily, even though proach to Earth, when the planet’s disk spanned a full 18.6 arcseconds. moonlight was a factor in the initial sessions. It looms large in a telescope now, and even instruments of moderate One great tool for power bring satisfying images at 100 or 150X. By midmonth, Mars improving your view Sky Calendar will be highest around 11 PM, with the disk slightly smaller, at 17.9”; is a “Moon filter.” 4 New Moon by June 30th, though, the planet will have already crossed the Meridian By bringing the sheer 12 First-Quarter Moon at 10 PM, before the sky brightness of Mars’ mag- 20 Full Moon In the Observer is fully dark, and the disk nitude -2 disk down a 27 Last-Quarter Moon will have shrunk some- notch, the moon filter President’s Message . -
Torresstrait Islander Peoples' Connectiontosea Country
it Islander P es Stra eoples’ C Torr onnec tion to Sea Country Formation and history of Intersection of the Torres Strait the Torres Strait Islands and the Great Barrier Reef The Torres Strait lies north of the tip of Cape York, Torres Strait Islanders have a wealth of knowledge of the marine landscape, and the animals which inhabit it. forming the northern most part of Queensland. Different marine life, such as turtles and dugong, were hunted throughout the Torres Strait in the shallow waters. Eighteen islands, together with two remote mainland They harvest fish from fish traps built on the fringing reefs, and inhabitants of these islands also embark on long towns, Bamaga and Seisia, make up the main Torres sea voyages to the eastern Cape York Peninsula. Although the Torres Strait is located outside the boundary of the Strait Islander communities, and Torres Strait Islanders Great Barrier Reef Marine Park, it is here north-east of Murray Island, where the Great Barrier Reef begins. also live throughout mainland Australia. Food from the sea is still a valuable part of the economy, culture and diet of Torres Strait Islander people who have The Torres Strait Islands were formed when the land among the highest consumption of seafood in the world. Today, technology has changed, but the cultural use of bridge between Australia and Papua New Guinea the Great Barrier Reef by Torres Strait Islanders remains. Oral and visual traditional histories link the past and the was flooded by rising seas about 8000 years ago. present and help maintain a living culture. -
Naming the Extrasolar Planets
Naming the extrasolar planets W. Lyra Max Planck Institute for Astronomy, K¨onigstuhl 17, 69177, Heidelberg, Germany [email protected] Abstract and OGLE-TR-182 b, which does not help educators convey the message that these planets are quite similar to Jupiter. Extrasolar planets are not named and are referred to only In stark contrast, the sentence“planet Apollo is a gas giant by their assigned scientific designation. The reason given like Jupiter” is heavily - yet invisibly - coated with Coper- by the IAU to not name the planets is that it is consid- nicanism. ered impractical as planets are expected to be common. I One reason given by the IAU for not considering naming advance some reasons as to why this logic is flawed, and sug- the extrasolar planets is that it is a task deemed impractical. gest names for the 403 extrasolar planet candidates known One source is quoted as having said “if planets are found to as of Oct 2009. The names follow a scheme of association occur very frequently in the Universe, a system of individual with the constellation that the host star pertains to, and names for planets might well rapidly be found equally im- therefore are mostly drawn from Roman-Greek mythology. practicable as it is for stars, as planet discoveries progress.” Other mythologies may also be used given that a suitable 1. This leads to a second argument. It is indeed impractical association is established. to name all stars. But some stars are named nonetheless. In fact, all other classes of astronomical bodies are named. -
Cr> Γ- ΟΟ [ Publications of the Astronomical Society of the Pacific
cr> - ΟΟΓ [ Publications of the Astronomical Society of the Pacific cs] 102:379-411, April 1990 \—I0 ωCu 1 PUBLICATIONS OF THE 2 ASTRONOMICAL SOCIETY OF THE PACIFIC Vol. 102 April 1990 No. 650 CONTEMPORARY OPTICAL SPECTRAL CLASSIFICATION OF THE OB STARS: A DIGITAL ATLAS* NOLAN R. WALBORNt Space Telescope Science Institute, φ 3700 San Martin Drive, Baltimore, Maryland 21218 AND EDWARD L. FITZPATRICKf Princeton University Observatory, Peyton Hall, Princeton, New Jersey 08544 Received 1990 ABSTRACT Some recent developments in the optical classification of OB spectra are reviewed in terms of a comprehensive atlas of new blue-violet digital data from the CTIO 1-meter photon-counting system. These developments include the OS spectral type; luminosity criteria for the O stars; OBN/OBC anomalies; and refined, interpolated late-O/early-B types. Examples of these phenom- ena are included among extensive spectral- and luminosity-class sequences, comprising 75 standard objects arranged into 27 montages and covering the wavelength range 3950 Â-4750 A for types OS-BS (-B8 at Iö). It is intended that this atlas serve a reference function analogous to that of the printed MK atlases, for morphological investigations of OB spectra based on digital data, which will supersede photographic techniques in most future applications. Key words: spectral atlas-OB stars 1. Introduction and Background The Μ Κ classification was based on blue-violet The system of spectral classification provided one (3900 Â-4900 A) photographic spectrograms of disper- Μ Κ -1 of the foundations of stellar astrophysics. Far from being sion ~ 100 A mm (resolution ~ 2 A) and widening at rendered obsolete by the development of the latter, how- least 0.5 mm. -
Spring Constellations Leo
Night Sky 101: Spring Constellations Leo Leo, the lion, is very recognizable by the head of the lion, which looks like a backwards question mark, and is commonly known as “the sickle.” Regulus, Leo’s brightest star, is also easy to pick out in most lights. The constellation is best seen in April and May, but rises after the Spring Equinox in March. Within the constellation, there are several spiral galaxies: M65, M66, M95, and M96. It is possible to fit M65 and M66 into the same view on a low powered telescope. In Greek mythology, Leo was the Nemean lion, who was completely impervious to bronze, steel and any kind of metal. As part of his 12 labors, Hercules was charged to fight the lion and killed him Photo Credit: Starry Night by strangling him. Hercules took the lion’s pelt as a prize and Leo, the lion, was placed in the stars to commemorate their fight. Virgo Virgo is best seen in the late spring and early summer, usually May to June. The bright star Arcturus, in the constellation Boötes, lines up with the Virgo’s brightest star Spica, which makes it easy to find. Within the constellation is the Virgo Galaxy Cluster, which is a conglomerate of thousands of unnamed galaxies. These galaxies are about 65 million light years away, and usually only appear as smudges in a telescope. Virgo, the maiden, is also known as Persephone, or the daughter of the Demeter. Hades, god of the Un- derworld, fell in love with Virgo and took her to the Underworld. -
The Denver Observer July 2018
The Denver JULY 2018 OBSERVER The globular cluster, Messier 19, one of this month’s targets in “July Skies,” in a Hubble Space Telescope image. Credit: NASA, ESA, STScI and I. King (Univer- sity of California – Berkeley) JULY SKIES by Zachary Singer The Solar System ’scopes towards the planets when they’re Sky Calendar The big news for July is that Mars comes highest in the sky on a given night, to get the 6 Last-Quarter Moon to opposition on the 27th, meaning that it sharpest image—but Mars is worth viewing 12 New Moon will be at its highest in the south on that date naked-eye when it’s rising. Surprised? The 19 First-Quarter Moon around 1 AM, and also more or less at its red (well, orange) planet appears even redder 27 Full Moon largest as seen from Earth. Now, don’t let that when rising, making for much deeper color. fool you—Mars is already very good as July It’s a guilty pleasure on an aesthetic level, if begins, showing a disk 21” across, which is not a scientific one. If you want to indulge better than we got two years ago, and only yourself, Mars rises around 10:30 PM at In the Observer slightly smaller than the 24” expected at the beginning of July, an hour earlier mid- the end of the month. (Observations in my month, and about 8:20 PM at month’s end. President’s Message . .2 6-inch reflector at the end of June showed an Meanwhile, Mercury is an evening Society Directory. -
Proto-Micronesian Reconstructions—1
Proto-Micronesian Reconstructions—1 Byron W. Bender, Ward H. Goodenough, Frederick H. Jackson, Jeffrey C. Marck, Kenneth L. Rehg, Ho-min Sohn, Stephen Trussel, and Judith W. Wang1 university of hawai‘i and university of pennsylvania Part 1 presents some 980 reconstructions for Proto-Micronesian, Proto–Central Micronesian, and Proto–Western Micronesian. Part 2 (to appear in volume 42 [2]) gives reconstructions for two additional subgroups within Proto-Micronesian: Proto-Pohnpeic and Proto-Chuukic, and their immediate ancestor, Proto– Pohnpeic-Chuukic. A handful of putative loans are also identi²ed, and a single English ²nder list is provided for all of the reconstructions. INTRODUCTION. Lexical data for a number of Micronesian languages began to be collected systematically in the mid-1960s as part of the development of language lessons for the U.S. Peace Corps and in connection with other Micronesian language projects that followed at the University of Hawai‘i. These data were stored on a main- frame computer using programs then being developed (Hsu and Peters 1984), and eventually dictionaries were published for a number of the languages included in this study (Elbert 1972, Abo et al. 1976, Lee 1976, Sohn and Tawerilmang 1976, Harrison and Albert 1977, Jensen 1977, Rehg and Sohl 1979, Goodenough and Sugita 1980, Jackson and Mark 1991). Comparative work using these data began with Marck 1977, focusing on the group of languages referred to as Nuclear Micronesian. In the next several years, the authors of the current study put the initial data on computer and sub- stantially added to them by directly eliciting information from speakers of Microne- sian languages who were students in the Bilingual Education Project for Micronesia at the University of Hawai‘i.