UACNJ Astro Rally 2011

Total Page:16

File Type:pdf, Size:1020Kb

UACNJ Astro Rally 2011 Address: __________________________________ First name: ___________________________________ UACNJ 2011 City / Zip / State: __________________________________ Email: __________________________________ Last name: _______________________________________ Astro Rally Phone: __________________________________ p UACNJ Observer Best seen u Coordinates o Club Season Object r Description Direction G Date Power Solar System Moon 1 Obs: ___________ All season Diameter: 3476km (27% Earth) Distance to earth: 384,000km Wandering 1 Terminator A Club: ___________ 50x Mass: 7.350 x 1019 t (1.2% Earth) (199 000 miles) (bright/dark area) Date: ___/___/___ Density: 3.341 g/cm3 (61% Earth) Visual size 0.5 arc deg Moon 2 Obs: ___________ All season 7/20/1969 Apollo 11, first man on the are meteorite craters that later flooded Wandering 2 Mare Tranquilitatis A Club: ___________ 100x moon. Initially thought to be seas with lava. Lava layers can be up to 10 Moon coord.: (Sea of Tranquility) Date: ___/___/___ called mare (Latin for sea), maria km thick, higher than Mount Everest 8.5°N / 31.4°E Obs: ___________ Fall Diameter: 142980km (11.2 Earth) Sun distance: 4.95 AU Aries Sep-Nov 3 Jupiter A Club: ___________ 50x, 150x Mass: 1.899 x 1024 t (318 Earth) Gas giant, 100+ moons , Galilean Date: ___/___/___ Density: 1.32 g/cm3 (24% Earth) moons: Io, Europa, Ganymede, Callisto Obs: ___________ Spring, Diameter: 123 000 km (9.4 Earth) Sun Distance: 9.54 AU Virgo: Apr-Aug 4 Saturn A Club: ___________ Summer Mass: 5.685 x 1023 t (95 Earth) Gas giant, ring, low density, floats on Date: ___/___/___ 50x, 150x Density: 0.67 g/cm3 (12% Earth) water, 62+ moons, largest Titan, Rhea Stars Obs: ___________ Spring Double: A 2.3, 3.4, Sep 4” Type: K0/G7, Dist: 126 LY RA 10h19’30” Algieba 5 B Club: ___________ Early Summer Two giants, bright bluish-orange & Mass: 3/2, Dia: 23/10 DEC 19°50’30’ Gamma Leonis Date: ___/___/___ 150x greenish-yellow, have planets Lum: 320/50 South Obs: ___________ Spring Double: A 4.8, 6.8 Sep 7” Type: G8/K4, Dist: 22 LY RA 14h51’23” 6 Bootes xi C Club: ___________ Early Summer A is very similar to sun, may have Mass: 0.9/0.7, Dia: 0.9/0.7 DEC 19°06’02” Date: ___/___/___ 150x planet < 9x Jupiter mass Lum: 0.5/0.06 Ovrhd Ras Algheti Obs: ___________ Late Spring Double A 3.0 – 4.6 B 5.4, Sep 4.6” Type: M5/F8, Dist: 382 LY RA 17h14’39” 7 “Head of the Kneeler” C Club: ___________ Summer Beautiful double, A: red giant (var.) Mass: 7 , Dia: 400:, Lum: 17,000 DEC 14°23’25” Alpha Herculis Date: ___/___/___ 150x shedding gas cloud engulfing B (in solar system expansion to Mars) Ovrhd Obs: ___________ Spring Optical double: A 3.1, B 5.1 Sep 35” Type: K3/B0, Dist: 390/380 LY Mass: RA 19h31’ Albireo 8 D Club: ___________ Summer 5/3.2, Dia: 16/2.7, Lum: 950/120 DEC 27°57’ Beta Cygni Date: ___/___/___ 50-100x Beautiful double, orange & blue NE, Ovrhd, NW Obs: ___________ Summer Fast rotation (286 km/s) causes Type: A7, Mag: 0.8, Dist: 16.8 LY RA 19h50’47” 9 Altair D Club: ___________ early Fall flattened poles. Star rotates within 9h Mass 1.8 , Dia 1.6 x 2.0, Lum 11 DEC 08°52’06” Date: ___/___/___ 150x (sun 25d). Age: 10 Billion years SE, S, SW Obs: ___________ Summer Double: A 4.3, 5.4, Sep 10” Type: F7/K1, Dist: 101 LY RA 20h46’39” 10 Gamma Delphini D Club: ___________ Fall Yellow-white dwarf and orange sub Mass: 1.7/1.6, Dia: 6.4/2.1 DEC 16°07’38” Date: ___/___/___ 150x giant Lum: 21/7 E, S, SW Legend UACNJ, Inc Numbers after double stars show magnitude of star A and B and their separation (Sep) in arc seconds. United Astronomy Clubs of New Jersey Web www.uacnj.org Mag: Magnitude LY: Light Year Mass: x sun mass Type: Star classes (OBAFGKM) Email: [email protected] Dist: Distance Dia: Diameter/sun/LY Dim: Dimensions MW: Milky Way p UACNJ Observer Best seen u Coordinates Object o Club Season Description r Direction G Date Power Obs: ___________ Fall Quadruple system (only one pair Type: K3 A0, Dist: 355 LY RA 02h03’54” Almach 11 B Club: ___________ 150x visible): A 2.3, B 6.3 Sep 10” (A) Dia: 80 Lum: 2000 DEC 42°19’47” Gamma Andromedae Date: ___/___/___ A: RG, red orange & bluish green NE, Ovrhd Polaris Obs: ___________ All Season Within 0.8 deg of north celestial pole, Type F7, 430LY, Mass: 6, Dia: 30 RA 02h31’50” 12 “Northern Star” B Club: ___________ 150x used for navigation and telescope Lum: 2200 DEC 89°15’51” Alpha Ursae Minoris Date: ___/___/___ alignment North Obs: ___________ All Season Fast rotation (274 km/s) causes Type: A0, Mag: 0.03, Dist: 25.3 LY RA 18h36’56” Vega 13 D Club: ___________ 150x flattened poles. Star rotates within Mass 2.1 , Dia 2.3x2.8, Lum: 37 DEC 38°47’01” Alpha Lyrae Date: ___/___/___ 12h (sun 25d). Was north star about 12,000BC NE, Ovrhd, W Obs: ___________ All Season Ten star system (4 brightest listed): Type: A3/A7/A5/A5, Dist: 162 LY RA 18h44’23” The Double Double 14 D Club: ___________ 150x A1 5.0, A2 6.0, B1 5.1, B2 5.4, Mass: 1.9/1.5/1.9/1.8, Dia: 23/10 DEC 39°36’46” Epsilon Lyrae Date: ___/___/___ Sep A-B 208” Lum: 18/8/17/14 NE, Ovrhd, NW Nebulae Obs: ___________ Summer Young planetary nebulae (PN), first Mag: 7.5, Dist: 1,360 LY RA 19h59’36” M27 15 D Club: ___________ Early Fall PN discovered (Messier 1764). Dim: 1.44 LY, Age: only 9,800 years DEC 22°43’16” Dumbbell nebulae Date: ___/___/___ 50x M27 illuminated by white dwarf (14) Central star: Dia: 0.055, Mass 0.56 NE Obs: ___________ All Season Gas expelled as hot super winds and Mag: 8.8, Dist: 2,300 LY RA 18h53’35” M57 16 D Club: ___________ 50-100x illuminated by central star Dia: 1.3 LY DEC 33°01’45” The Ring Nebulae Date: ___/___/___ Constellation Lyra Central star Mass 0.6, Mag: 16 NE, Ovrhd, NW Galaxies & Clusters Obs: ___________ Spring Spiral Galaxy, active nucleus with Mag: 7.0, Dist: 11.8 Mill LY RA 9h55’33” M81 17 B Club: ___________ 50x massive black hole mass (70 Mill x Mass:250 Billion, Dia: 70,000 LY DEC 69°03’55” Bode’s Galaxy Date: ___/___/___ sun), close by: M82 galaxy Constellation Ursa Major North M13 Obs: ___________ Late Spring Globular Cluster very old, 1 million Mag: 5.8, Dist: 25,100 LY RA 16h41’41” 18 Hercules Global C Club: ___________ Summer stars Dia: 168 LY, Mass: 600,000x sun Age: DEC 36°27’37” Cluster Date: ___/___/___ 50x 14 Bill Years Ovrhd Obs: ___________ Early Spring Open cluster, 150 white dwarfs, 100 Mag: 6.1, Dist: 2,700 LY RA 08h51’24” 19 M67 B Club: ___________ 50x sun like, 500 red giants Dia: 20 LY, Mass: 1,400 x sun DEC 11°49’ Date: ___/___/___ Age: 3.2 - 5 Billion years S (high) Obs: ___________ Late Summer Spiral galaxy, estimated 1 Trillion Mag: 3.44, Dist: 2.54 Mill LY RA 00h42’44” M31 20 B Club: ___________ Fall stars (Milky Way 200-400 Billion) Dia: 260,000 LY, Mass: 1.5x MW DEC 41°16’09 Andromeda Galaxy Date: ___/___/___ 30-50x merges with MW in 4.5 Billion years Farthest object naked eye can see NE, Ovrhd Obs: ___________ Summer Globular cluster, 100,000 stars, Mag: 6.65, Dist: 24,500 LY, Dia: 165 RA 15h18’34” 21 M5 C Club: ___________ 50x almost as old as the universe LY, Age: 13 Billion Years DEC 02°04’58” Date: ___/___/___ South Legend UACNJ, Inc Numbers after double stars show magnitude of star A and B and their separation (Sep) in arc seconds. United Astronomy Clubs of New Jersey Mag: Magnitude LY: Light Year Mass: x sun mass Type: Star classes (OBAFGKM) Web www.uacnj.org Dist: Distance Dia: Diameter/sun/LY Dim: Dimensions MW: Milky Way Email: [email protected] .
Recommended publications
  • Gamma Leonis B
    Gamma Leonis b The planetary system Gamma Leonis hosts at least one planet. Note that the system is a multiple star system. It hosts at least 2 stellar components. System parameters. Primary system name. Gamma Leonis. Alternative system names. N/A. Gamma-2 Leonis. Alternative star names. gamma 1 Leo, gam01 Leo, γ1 Leo, γ1 Leonis, γ Leo A, Gamma Leonis A, gamma Leo A, gam Leo A, Algieba A, Al Gieba A, HD 89484, HIP 50583 A, TYC 1423-1349-1, SAO 81298, BD+20 2467 A, WDS J10200+1950 A, STF 1424 A. Gamma Leonis's wiki: Gamma Leonis (γ Leo, γ Leonis) is a binary star system in the constellation Leo. It has the traditional name Algieba or Al Gieba . Name origin and history The name Algieba originates from the Arabic الجبهة Al-Jabhah Gamma Leonis b is an extrasolar planet located 125.5 light years away in the constellation Leo, orbiting the giant star Gamma Leonis. On November 6, 2009, a planetary companion around primary star Gamma1 Leonis has been announced. Moreover radial velocity variations would also hint two strong signals at 8.5 and 1340 days. The former periodicity is likely due to stellar pulsation, whereas the latter could be indicative of the presence of an additional planetary companion with 2.14 Jupiter masses Gamma Leonis (γ Leo / γ Leonis) is a binary star system in the constellation Leo. It also has the traditional name Algieba or Al Gieba. Name origin and history. The name "Algieba" originates from the Arabic "Al-Jabhah", meaning "the forehead".
    [Show full text]
  • Exo-Mercat a Merged Exoplanet Catalog
    Exo-MerCat a merged exoplanet catalog 1,2 Eleonora Alei , Riccardo Claudi1, Andrea Bignamini3, Marco Molinaro3 1 INAF – Osservatorio Astronomico di Padova 2 DFA-UNIPD – Dipartimento di Fisica e Astronomia dell’Università degli Studi di Padova 3 INAF – Osservatorio Astronomico di Trieste IVOA Interoperability meeting Paris, 12-17 May 2019 Overview • Online exoplanet catalogs: state of the art • Raw statistics with the current datasets • Known Issues: updates, errors, selection criteria • Exo-MerCat: aims, description, efficiency • Update workflow and VO resource NASA Exoplanet Archive (NASA) Exoplanets Orbit Database (ORG) Open Exoplanet Catalogue (OEC) Extrasolar Planets Encyclopaedia (EU) Yikes! Raw statistics Raw Problems Selection Criteria Aliases Coordinates Updates - Names appear in different - Human errors (plus-minus - False positives are present in formats; signs); the catalogs because of lags - Whitespaces are present; - Not updated coordinates; in the updates; - Different aliases for the same - Different epochs. - New candidates have yet to be planet; included in the database. Algieba, gamma Leonis: Proxima Centauri b (ra,dec): in NASA: gam 1 Leo in NASA: (217.428995,-62.679485) in ORG: gamma Leo A in ORG: (217.448946,-62.681353) in EU: gamma 1 Leo in EU: (217.429167,-62.679444) in OEC: Gamma Leonis in OEC: (219.990850,-60.835619) 5 Aims • Provide greater uniformity among the databases; • More effective associations among the datasets; • Identify and correct errors, to warn the catalog maintainers; Exo-MerCat • Provide a direct link with most stellar sources archives; • Provide the user with an intuitive Graphical Interface to download and filter data. 6 Icons made by https://www.flaticon.com/authors/gregor-cresnar from www.flaticon.com Description Initialization • Create a nested folder to contain all useful files; • Use various Virtual Observatory tools to download raw datasets: Exo-MerCat • wget command to access NASA/ORG database; • git commands and an *.xml reader to access the OEC database; • VO TAP service for the EU database.
    [Show full text]
  • 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.
    [Show full text]
  • Stansbury Brings Listening Tour to Placitas by the Numbers
    SANDOVAL PLACITAS PRSRT-STD U.S. Postage Paid BERNALILLO Placitas, NM Permit #3 CORRALES SANDOVAL Postal Customer or Current Resident COUNTY ECRWSS NEW MEXICO SignA N INDEPENDENT PLOCAL NEWSPAPER St S INCE 1988 • VOL. 32 / NO 9 • SEPTEMBER 2021 • FREE IVEN By the numbers: D ILL New Mexico and —B the 2020 Census ~SIGNPOST STAFF While Sandoval County remains among the fastest growing counties in the state, New Mexico’s overall growth rate lags well behind its neighbors, according to data from the 2020 Census released last month. Over the last ten years, Sandoval County grew by 17,273 residents for a total population of 148,834, a 13.1 percent increase. Faster growth was noted only in Eddy County, 15.8 percent, and Lea County, 15 percent, both in the southeast Oil Patch. Sandoval remains the fourth-largest county by pop- ulation behind Bernalillo, Doña Ana, and Santa Fe counties. The state’s population reached 2.1 million with 58,343 more residents, up 2.8 percent since the 2010 Census. The nation as a whole grew by 7.4 percent, the lowest rate since the 1930s, and compares to rates U.S. Rep. Melanie Stansbury visits with John Stebbins of Placitas after her listening session of ten percent or more in states surrounding New at the Placitas Community Library. Stansbury, elected in June to fill out Rep. Deb Haaland’s term, Mexico except Oklahoma. was touring the district with her staff during the August congressional recess. Data also show New Mexico to be among the most racially and ethnically diverse state.
    [Show full text]
  • Interstellarum 25 Schließen Wir Den Ersten Jahrgang Der Neuen Interstellarum-Hefte Ab
    Liebe Leserinnen, liebe Leser, Meade gegen Celestron, das ist das große Duell der beiden Teleskopgiganten aus Amerika. Wir sind stolz darauf, als erste deutschsprachige Zeitschrift einen fairen Zweikampf der weltgröß- ten Fernrohrhersteller anbieten zu können; un- getrübt von wirtschaftlichen oder redaktionellen Vorbehalten. Dazu haben wir die neuen aufre- genden GPS-Teleskope von Meade und Celes- tron in einem Produktvergleich gegenüberge- stellt. Im ersten Teil in diesem Heft erfahren Sie mehr über Mechanik und Elektronik der beiden Computerteleskope (Seite 60); die Ergebnisse der Praxis unter den Sternen lesen Sie dann in einem kommenden Heft. Mit interstellarum 25 schließen wir den ersten Jahrgang der neuen interstellarum-Hefte ab. Ein Plus von 30% bei den Abonnentenzahlen spricht für unseren Weg, den wir konsequent fortsetzen Polarlichter in Deutschland (Foto: Thomas Jäger) werden. Dabei möchten wir verstärkt das Augen- merk auf hochqualitative Beiträge für praktisch tätige Amateurastronomen lenken. werden wir uns zusätzlich der Jupiterbeobach- tung und dem Merkurdurchgang vom 7.5.2003 2003 wird bei interstellarum zum Jahr der widmen. Schließlich stehen 2003 mit zwei Planetenbeobachtung ernannt. Auftakt ist der Mondfinsternissen und einer partiellen Sonnen- Beitrag zur Beobachtung der Saturnringe in die- finsternis drei weitere Großereignisse auf dem ser Ausgabe (Seite 34). Mit dem nächsten Heft Programm. beginnen wir zusätzlich eine intensive Vorberei- tung auf die große Mars-Opposition in diesem Was wir noch 2003 geplant haben, ist auf Sommer mit Beiträgen zu verschiedenen prakti- www.interstellarum.de nachzulesen. Ihren eige- schen Themenkreisen in jedem Heft. Verstärkt nen Bericht nehmen wir gerne entgegen. Mit interstellarum 25 endet die Comic-Serie Astromax (Seite 80), die Schöpfer Rainer Töpler aus Zeitgründen aufgeben muss – vielen Dank für die sechs kurzweiligen Geschichtchen.
    [Show full text]
  • Australian Sky & Telescope
    TRANSIT MYSTERY Strange sights BINOCULAR TOUR Dive deep into SHOOT THE MOON Take amazing as Mercury crosses the Sun p28 Virgo’s endless pool of galaxies p56 lunar images with your smartphone p38 TEST REPORT Meade’s 25-cm LX600-ACF P62 THE ESSENTIAL MAGAZINE OF ASTRONOMY Lasers and advanced optics are transforming astronomy p20 HOW TO BUY THE RIGHT ASTRO CAMERA p32 p14 ISSUE 93 MAPPING THE BIG BANG’S COSMIC ECHOES $9.50 NZ$9.50 INC GST LPI-GLPI-G LUNAR,LUNAR, PLANETARYPLANETARY IMAGERIMAGER ANDAND GUIDERGUIDER ASTROPHOTOGRAPHY MADE EASY. Let the LPI-G unleash the inner astrophotographer in you. With our solar, lunar and planetary guide camera, experience the universe on a whole new level. 0Image Sensor:'+(* C O LOR 0 Pixel Size / &#*('+ 0Frames per second/Resolution• / • / 0 Image Format: #,+$)!&))'!,# .# 0 Shutter%,*('#(%%#'!"-,,* 0Interface: 0Driver: ASCOM compatible 0GuiderPort: 0Color or Monochrome Models (&#'!-,-&' FEATURED DEALERS: MeadeTelescopes Adelaide Optical Centre | www.adelaideoptical.com.au MeadeInstrument The Binocular and Telescope Shop | www.bintel.com.au MeadeInstruments www.meade.com Sirius Optics | www.sirius-optics.com.au The device to free you from your handbox. With the Stella adapter, you can wirelessly control your GoTo Meade telescope at a distance without being limited by cord length. Paired with our new planetarium app, *StellaAccess, astronomers now have a graphical interface for navigating the night sky. STELLA WI-FI ADAPTER / $#)'$!!+#!+ #$#)'#)$##)$#'&*' / (!-')-$*')!($%)$$+' "!!$#$)(,#%',).( StellaAccess app. Available for use on both phones and tablets. /'$+((()$!'%!#)'*")($'!$)##!'##"$'$*) stars, planets, celestial bodies and more /$,'-),',### -' ($),' /,,,$"$')*!!!()$$"%)!)!($%( STELLA is controlled with Meade’s planetarium app, StellaAccess. Available for purchase for both iOS S and Android systems.
    [Show full text]
  • List of Easy Double Stars for Winter and Spring  = Easy  = Not Too Difficult  = Difficult but Possible
    List of Easy Double Stars for Winter and Spring = easy = not too difficult = difficult but possible 1. Sigma Cassiopeiae (STF 3049). 23 hr 59.0 min +55 deg 45 min This system is tight but very beautiful. Use a high magnification (150x or more). Primary: 5.2, yellow or white Seconary: 7.2 (3.0″), blue 2. Eta Cassiopeiae (Achird, STF 60). 00 hr 49.1 min +57 deg 49 min This is a multiple system with many stars, but I will restrict myself to the brightest one here. Primary: 3.5, yellow. Secondary: 7.4 (13.2″), purple or brown 3. 65 Piscium (STF 61). 00 hr 49.9 min +27 deg 43 min Primary: 6.3, yellow Secondary: 6.3 (4.1″), yellow 4. Psi-1 Piscium (STF 88). 01 hr 05.7 min +21 deg 28 min This double forms a T-shaped asterism with Psi-2, Psi-3 and Chi Piscium. Psi-1 is the uppermost of the four. Primary: 5.3, yellow or white Secondary: 5.5 (29.7), yellow or white 5. Zeta Piscium (STF 100). 01 hr 13.7 min +07 deg 35 min Primary: 5.2, white or yellow Secondary: 6.3, white or lilac (or blue) 6. Gamma Arietis (Mesarthim, STF 180). 01 hr 53.5 min +19 deg 18 min “The Ram’s Eyes” Primary: 4.5, white Secondary: 4.6 (7.5″), white 7. Lambda Arietis (H 5 12). 01 hr 57.9 min +23 deg 36 min Primary: 4.8, white or yellow Secondary: 6.7 (37.1″), silver-white or blue 8.
    [Show full text]
  • April 14 2018 7:00Pm at the April 2018 Herrett Center for Arts & Science College of Southern Idaho
    Snake River Skies The Newsletter of the Magic Valley Astronomical Society www.mvastro.org Membership Meeting President’s Message Tim Frazier Saturday, April 14th 2018 April 2018 7:00pm at the Herrett Center for Arts & Science College of Southern Idaho. It really is beginning to feel like spring. The weather is more moderate and there will be, hopefully, clearer skies. (I write this with some trepidation as I don’t want to jinx Public Star Party Follows at the it in a manner similar to buying new equipment will ensure at least two weeks of Centennial Observatory cloudy weather.) Along with the season comes some great spring viewing. Leo is high overhead in the early evening with its compliment of galaxies as is Coma Club Officers Berenices and Virgo with that dense cluster of extragalactic objects. Tim Frazier, President One of my first forays into the Coma-Virgo cluster was in the early 1960’s with my [email protected] new 4 ¼ inch f/10 reflector and my first star chart, the epoch 1960 version of Norton’s Star Atlas. I figured from the maps I couldn’t miss seeing something since Robert Mayer, Vice President there were so many so closely packed. That became the real problem as they all [email protected] appeared as fuzzy spots and the maps were not detailed enough to distinguish one galaxy from another. I still have that atlas as it was a precious Christmas gift from Gary Leavitt, Secretary my grandparents but now I use better maps, larger scopes and GOTO to make sure [email protected] it is M84 or M86.
    [Show full text]
  • Double and Multiple Star Measurements in the Northern Sky with a 10” Newtonian and a Fast CCD Camera in 2006 Through 2009
    Vol. 6 No. 3 July 1, 2010 Journal of Double Star Observations Page 180 Double and Multiple Star Measurements in the Northern Sky with a 10” Newtonian and a Fast CCD Camera in 2006 through 2009 Rainer Anton Altenholz/Kiel, Germany e-mail: rainer.anton”at”ki.comcity.de Abstract: Using a 10” Newtonian and a fast CCD camera, recordings of double and multiple stars were made at high frame rates with a notebook computer. From superpositions of “lucky images”, measurements of 139 systems were obtained and compared with literature data. B/w and color images of some noteworthy systems are also presented. mented double stars, as will be described in the next Introduction section. Generally, I used a red filter to cope with By using the technique of “lucky imaging”, seeing chromatic aberration of the Barlow lens, as well as to effects can strongly be reduced, and not only the reso- reduce the atmospheric spectrum. For systems with lution of a given telescope can be pushed to its limits, pronounced color contrast, I also made recordings but also the accuracy of position measurements can be with near-IR, green and blue filters in order to pro- better than this by about one order of magnitude. This duce composite images. This setup was the same as I has already been demonstrated in earlier papers in used with telescopes under the southern sky, and as I this journal [1-3]. Standard deviations of separation have described previously [1-3]. Exposure times varied measurements of less than +/- 0.05 msec were rou- between 0.5 msec and 100 msec, depending on the tinely obtained with telescopes of 40 or 50 cm aper- star brightness, and on the seeing.
    [Show full text]
  • Culmination of a Constellation
    Culmination of a Constellation Over any night, stars and constellations in the sky will appear to move from east to west due to the Earth’s rotation on its axis. A constellation will culminate (reach its highest point in the sky for your location) when it centres on the meridian - an imaginary line that runs across the sky from north to south and also passes through the zenith (the point high in the sky directly above your head). For example: When to Observe Constellations The taBle shows the approximate time (AEST) constellations will culminate around the middle (15th day) of each month. Constellations will culminate 2 hours earlier for each successive month. Note: add an hour to the given time when daylight saving time is in effect. The time “12” is midnight. Sunrise/sunset times are rounded off to the nearest half an hour. Sun- Jan Feb Mar Apr May Jun Jul Aug Sep Oct Nov Dec Rise 5am 5:30 6am 6am 7am 7am 7am 6:30 6am 5am 4:30 4:30 Set 7pm 6:30 6pm 5:30 5pm 5pm 5pm 5:30 6pm 6pm 6:30 7pm And 5am 3am 1am 11pm 9pm Aqr 5am 3am 1am 11pm 9pm Aql 4am 2am 12 10pm 8pm Ara 4am 2am 12 10pm 8pm Ari 5am 3am 1am 11pm 9pm Aur 10pm 8pm 4am 2am 12 Boo 3am 1am 11pm 9pm 7pm Cnc 1am 11pm 9pm 7pm 3am CVn 3am 1am 11pm 9pm 7pm CMa 11pm 9pm 7pm 3am 1am Cap 5am 3am 1am 11pm 9pm 7pm Car 2am 12 10pm 8pm 6pm Cen 4am 2am 12 10pm 8pm 6pm Cet 4am 2am 12 10pm 8pm Cha 3am 1am 11pm 9pm 7pm Col 10pm 8pm 4am 2am 12 Com 3am 1am 11pm 9pm 7pm CrA 3am 1am 11pm 9pm 7pm CrB 4am 2am 12 10pm 8pm Crv 3am 1am 11pm 9pm 7pm Cru 3am 1am 11pm 9pm 7pm Cyg 5am 3am 1am 11pm 9pm 7pm Del
    [Show full text]
  • Gov Aker Telescope Operators Manual
    Gov Aker Telescope Operators Manual Revised September 3, 2014 Craig Nance Director Mount Graham International Observatory Steward Observatory University of Arizona [email protected] Page 1 of 97 Governor Hunt Aker Governor Hunt Aker was born on Dec 24, 1917. “Gov Aker” served in the Army Air Corps during World War II. After the war he became an assistant football coach at Northern Arizona University and then was a teacher and coach at Safford High School during the 1950’s. He went on to become assistant superintendent of public instruction at the State capital in Phoenix. In 1964 he became the director of youth programs for the Secretary of the Interior. Later, starting in 1986 he served as the mayor of Safford and was a member of the Safford High School Scholarship and Educational Foundation. He passed away on June 30, 1993. His resting place is the Safford Cemetery. To those that knew him Gov Aker was known for his incredible dedication and commitment to Arizona, his sense of humor, his love of golf, and his love of the people he represented. Source: Various public records, including Congressional Record, 103rd Congress, Page S9053 Page 2 of 97 Introduction The Gov Aker telescope is a research-class telescope that is presently used primarily for public education. It is hoped that through this manual that the telescope enjoys a strong level of usage, as this is what benefits the telescope the most. Operators should not be hesitant to use the telescope, being mindful of a reasonable number of safety precautions that are highlighted in this manual.
    [Show full text]
  • Earth and Space Science. a Guide for Secondary Teachers. INSTITUTION Pennsylvania State Dept
    DOCUMENT RESUME ED 094 956 SE 016 611 AUTHOR Bolles, William H.; And Others TITLE Earth and Space Science. A Guide for Secondary Teachers. INSTITUTION Pennsylvania State Dept. of Education, Harrisburg. Bureau of Curriculum Services. PUB DATE 73 NOTE 200p. EDRS PRICE MF-$O.75 HC-$9.00 PLUS POSTAGE DESCRIPTORS Aerospace Education; *Astronomy; *Curriculum Guides; *Earth Science; Geology; Laboratory Experiments; Oceanology; Science Activities; Science Education; *Secondary School Science IDENTIFIERS Pennsylvania ABSTRACT Designed for use in Pennsylvania secondary school science classes, this guide is intended to provide fundamental information in each of the various disciplines of the earth sciences. Some of the material contained in the guide is intended as background material for teachers. Five units are presented: The Earth, The Oceans, The Space Environment, The Atmosphere, and The Exploration of Space. The course is organized so that students proceed from the familiar, everyday world to the atmosphere and the space environment. Teaching geology in the fall takes advantage of weather conditions which permit field study. The purpose of the Earth and Space Science course is to encourage student behaviors which will be indicative of a broad understanding of man1s physical environment of earth and space as well as an awareness of the consequences which could result from changes which man may effect.(PEB) BEST COPY AVAILABLE U S DEPARTMENT OF HEALTH. EDUCATION & WELFARE NATIONAL INSTITUTE OF 6 Fe elz+C EDUCATION Try,' DOCUMENT FIRSBEEN REPRO
    [Show full text]