November 2004

Total Page:16

File Type:pdf, Size:1020Kb

November 2004 San Diego Astronomy Association Celebrating Over 40 Years of Astronomical Outreach Office (619) 645-8940 December 2004 Observatory (619) 766-9118 http://www.sdaa.org A Non-Profit Educational Association Banquet News! P.O. Box 23215, San Diego, CA 92193-3215 By Scott Baker Mark your calendars, the annual SDAA Banquet and New Officer Installation is SDAA Business Meeting coming soon! The Banquet will be held at the Town and Country Resort in Mission Next meeting will be held at: Valley on the 22nd of January. That’s a near full moon weekend, so there’s no reason SKF Condition Monitoring not to attend. Our guest speaker this year will be Tim Castellano, an astronomer at 5271 Viewridge Court NASA’s Ames Research Center, Mountain View, California. This year it will be a sit- San Diego, CA 92123 down dinner (no buffet lines, yeah!) with two choices of main course, either Chicken February 10th at 7:00pm Floresco or California Tri-Tip. Of course there will be the usual raffle and live auction with an added silent auction on some special items. Invitations will be mailed the first week in December, so watch your mailbox! You’ll also have the ability to order tickets on-line using PayPal, just like last year. Ticket prices are still being negotiated but will be in the invitations and next month’s newsletter. The club has ANNUAL BOARD ELECTIONS decided to pick up the parking so that will be free to members. Mark you calendars Must be postmarked by now and I hope to see all of you there! December 31, 2004 See page 5 for details Treasurer’s Report by Michael Finch With the addition of our new members we now have a total of 590 SDAA mem- bers. We have several new members last month. Please welcome Cathryn CONTENTS Campbell, Marcee Chipman, William Hultman, Jeff Redwine, Scott Speights, and December 2004 Vol XL, Issue 12 Mark Stewart. Welcome to SDAA and may you enjoy clear dark skies! Published Monthly by the San Diego Astronomy Association Observatory Owners: It’s that time of year. By now you should have received 75¢ /$8.00 year your property tax letter in the mail. Please ensure your payment is received by Incorporated in California in 1963 January 10, 2005. Payment can be made by PayPal or by mailing to the SDAA PO box. Banquet News.......................................1 Treasurer’s Report...........................................1 Do you have questions about SDAA membership? Has your address changed? Astronomy 101......................................3 Please contact me at [email protected]. Thank you. Sky Watch..........................................................4 SDAA Director Bio’s..................................6 Second Site Fund balance: $6,705.79 Galactic Surprise..........................................7 The Back Page...........................................8 SanSan DiegoDiego AstronomyAstronomy AssociationAssociation For the double star devotees, take a Object name: Capella peek at omega Aur. It can be viewed Magnitude: 0.08 with small telescopes, consisting of a Equatorial 2000: RA: 05h 16m 41.395s 5th magnitude primary and a 8th Dec: +45°59’50.677" By Scott Baker magnituded secondary. For a little Alternate names: HIP 24608 SAO more challenge, scope of 4" or more 40186 GSC 3358:3141 Auriga - The Charioteer (with high magnification) should try Flamsteed-Bayer: 13-Alpha Aurigae This month’s constellation is Auriga, theta Auriga. Theta, with a 2.6 primary Object type: Star The Charioteer or Wagoneer. The name and a 7th magnitude secondary can be a Spectral: G0 Auriga is Latin for “charioteer.” The challenge if the conditions aren’t right. early civilizations of Greeks, Arabs, Object name: Menkalinan Chinese and Babylonians all associated For the open cluster folks, Sir Messier Magnitude: 1.90 this part of the sky with a charioteer. made a stop here, while cataloging Equatorial 2000: RA: 05h 59m 31.697s The Greeks had one myth that told that objects. Here you’ll find M36, M37 Dec: +44°56’50.754" the charioteer was Hephaestus, the son and M38. M36, a nice open cluster of Alternate names: HIP 28360 SAO of Helios and Hera. Hephaestus was about 100 stars, is rather concentrated 40750 GSC 2924:2742 born severely crippled, yet he managed for an open cluster. M37, another open Flamsteed-Bayer: 34-Beta Aurigae to learn to be a blacksmith, making cluster of about 150 stars, is very Object type: Star wonderful armor for the gods. His impressive. It is about 25 minutes of Spectral: A2V fame as the “lame smith” grew through- arc in diameter and contains a bright out the land. When King Oenopion, orange tinted star at it’s center. M38, Object name: Theta AUR blinded Orion for kidnapping his Easily spotted in binoculars, is also Magnitude: 2.6 daughter Merope, Hephaestus came to about 25' in diameter and composed of Equatorial 2000: RA: 05h 59m 43s his aide, earning his position in the about 100 stars. In the same field of Dec: +37°12’45" heavens by Zeus. Hephaestus, it was view, using a low power eyepiece, look Object type: Double Star said, became the first “charioteer”, for a companion cluster just South of Common name: Theta AUR when he invented the chariot to help M38, NGC1907. NGC1907 only Notes: 3.6" separation at PA 313(A-B); him get about. contains about 10 to 12 stars. 2.6-7.1M; blue/yellow; C = 10.6M, 50" distant at PA 297 Auriga, a winter constellation, rises in For the deep sky enthusiast, Auriga is Hour angle: -06h 58m 57s the Northeast, shortly after sunset and lacking, in a way, anything to look at offers many fine objects for the amateur that can be reached with amateur Object name: Omega AUR astronomer. One of Auriga’s most equipment. Loaded with galaxies, all Magnitude: 5.0 outstanding objects is it’s primary star, 15th magnitude or dimmer, I could only Equatorial 2000: RA: 04h 59m 15s Capella. Capella, at sixth brightest, a find two objects worthy of a hunt. The Dec: +37°53’24" winter landmark, or should I say first is PGC18078, a barred spiral Object type: Double Star skymark, is a spectroscopic double with galaxy at 13.5 magnitude. The other is Common name: Omega AUR a period of only 104 days. The a planetary nebula, IC 2149. At lower Notes: 5.4" separation at PA 000; 5- constellations second brightest star, powers, IC 2149 is stellar in appear- 8M; both blue-white; just S of AUR’s Menkalinen(beta Auriga), is also a ance, but you may notice something “Kids” spectroscopic binary. With a period of about it’s color, being “off”. As you Hour angle: -05h 53m 28s only four days, the stars complete their crank up the magnification, it starts to revolution much faster than those of show an egg shape. At very high Object name: M 36 Capella. Since they are eclipsing each magnification, you can pick up the Magnitude: 6.0 other the brightness of beta Aur seems central star and the nebula will blink in Equatorial 2000: RA: 05h 36m 18s to vary. and out as you avert your vision. Dec: +34°08’27" Size: 10.0 x 10.0 Get out an enjoy Auriga when you get a Object type: Open Cluster chance. Other ID: NGC1960 Page 2 SAN DIEGO ASTRONOMY ASSOCIATION NEWS AND NOTES, OCTOBER 2004 San Diego Astronomy Association Object name: M 37 Dec: +46°26’22" Magnitude: 5.6 Size: 2.3 x 1.8 Equatorial 2000: RA: 05h 52m 18s Alternate names: MCG8-11-11, Dec: +32°33’11" CGCG232-3, IRAS05511+4625 Address Change? Size: 15.0 x 15.0 Object type: Spiral Galaxy Submit your new information to: Object type: Open Cluster Type: SBbc Other ID: NGC2099 Bar: B [email protected] to ensure you don’t miss out on SDAA news. If Object name: M 38 Object name: IC 2149 you ordered a magazine subscrip- Magnitude: 6.4 Magnitude: 11.0 tion through the club, you will still Equatorial 2000: RA: 05h 28m 42s Equatorial 2000: RA: 05h 56m 24s need to notify the magazine as Dec: +35°51’18" Dec: +46°06’19" Size: 15.0 x 15.0 Notes: 10M; 10" diameter; very small! well Object type: Open Cluster requires high-+; diffuse at edges with (see each magazine for change of central condensation; 11.5M; central address instructions). Object name: PGC 18078 star not easily visible against interior Magnitude: 13.5 glow; NEAT! find it 40' WNW of Pi (p) Equatorial 2000: RA: 05h 54m 54s AUR, the 4.5M star 1 degs N of 2M Beta (b) AUR SAN DIEGO ASTRONOMY ASSOCIATION NEWS AND NOTES, OCTOBER 2004 Page 3 San Diego Astronomy Association SkyWatch for December, 2004 John Mood [ Times PST] [ * = 1 star = EZ ] [ ** = 2 stars = Moderate ] [ *** = 3 stars = Difficult ] Sat., 4 Dec. —— PUBLIC STAR PARTY @ Tierra del Sol. Tues., 7 Dec. —— MOON occults JUPITER before dawn for those who live well east of the Rockies; here in San Diego the Moon will be a very close 0.3 degrees from Jupiter @ 1:30 a.m. {See below.} Sat., 11 Dec. —— NEW MOON, 5:29 p.m. —— “New Moon Night” @ Tierra del Sol. Tues., 14 Dec. —— GEMINID METEOR SHOWER (the best of the year) peaks this morning. Sat., 18 Dec. —— PUBLIC STAR PARTY @ Tierra del Sol; explore the Moon’s “terminator” (where dark turns to light) for spectacular views of mountains, craters & rills. Tues., 21 Dec. —— WINTER SOLSTICE, 4:42 a.m. Brrrrrr! Sun., 26 Dec. —— FULL MOON, 7:06 p.m. Mon., 29 Dec. —— MERCURY passes just 1.2 degrees from VENUS this morning. {See below.} Sat., 1 Jan. 2005 —— 12:00 a.m.
Recommended publications
  • A Basic Requirement for Studying the Heavens Is Determining Where In
    Abasic requirement for studying the heavens is determining where in the sky things are. To specify sky positions, astronomers have developed several coordinate systems. Each uses a coordinate grid projected on to the celestial sphere, in analogy to the geographic coordinate system used on the surface of the Earth. The coordinate systems differ only in their choice of the fundamental plane, which divides the sky into two equal hemispheres along a great circle (the fundamental plane of the geographic system is the Earth's equator) . Each coordinate system is named for its choice of fundamental plane. The equatorial coordinate system is probably the most widely used celestial coordinate system. It is also the one most closely related to the geographic coordinate system, because they use the same fun­ damental plane and the same poles. The projection of the Earth's equator onto the celestial sphere is called the celestial equator. Similarly, projecting the geographic poles on to the celest ial sphere defines the north and south celestial poles. However, there is an important difference between the equatorial and geographic coordinate systems: the geographic system is fixed to the Earth; it rotates as the Earth does . The equatorial system is fixed to the stars, so it appears to rotate across the sky with the stars, but of course it's really the Earth rotating under the fixed sky. The latitudinal (latitude-like) angle of the equatorial system is called declination (Dec for short) . It measures the angle of an object above or below the celestial equator. The longitud inal angle is called the right ascension (RA for short).
    [Show full text]
  • Astronomical Coordinate Systems
    Appendix 1 Astronomical Coordinate Systems A basic requirement for studying the heavens is being able to determine where in the sky things are located. To specify sky positions, astronomers have developed several coordinate systems. Each sys- tem uses a coordinate grid projected on the celestial sphere, which is similar to the geographic coor- dinate system used on the surface of the Earth. The coordinate systems differ only in their choice of the fundamental plane, which divides the sky into two equal hemispheres along a great circle (the fundamental plane of the geographic system is the Earth’s equator). Each coordinate system is named for its choice of fundamental plane. The Equatorial Coordinate System The equatorial coordinate system is probably the most widely used celestial coordinate system. It is also the most closely related to the geographic coordinate system because they use the same funda- mental plane and poles. The projection of the Earth’s equator onto the celestial sphere is called the celestial equator. Similarly, projecting the geographic poles onto the celestial sphere defines the north and south celestial poles. However, there is an important difference between the equatorial and geographic coordinate sys- tems: the geographic system is fixed to the Earth and rotates as the Earth does. The Equatorial system is fixed to the stars, so it appears to rotate across the sky with the stars, but it’s really the Earth rotating under the fixed sky. The latitudinal (latitude-like) angle of the equatorial system is called declination (Dec. for short). It measures the angle of an object above or below the celestial equator.
    [Show full text]
  • Making a Sky Atlas
    Appendix A Making a Sky Atlas Although a number of very advanced sky atlases are now available in print, none is likely to be ideal for any given task. Published atlases will probably have too few or too many guide stars, too few or too many deep-sky objects plotted in them, wrong- size charts, etc. I found that with MegaStar I could design and make, specifically for my survey, a “just right” personalized atlas. My atlas consists of 108 charts, each about twenty square degrees in size, with guide stars down to magnitude 8.9. I used only the northernmost 78 charts, since I observed the sky only down to –35°. On the charts I plotted only the objects I wanted to observe. In addition I made enlargements of small, overcrowded areas (“quad charts”) as well as separate large-scale charts for the Virgo Galaxy Cluster, the latter with guide stars down to magnitude 11.4. I put the charts in plastic sheet protectors in a three-ring binder, taking them out and plac- ing them on my telescope mount’s clipboard as needed. To find an object I would use the 35 mm finder (except in the Virgo Cluster, where I used the 60 mm as the finder) to point the ensemble of telescopes at the indicated spot among the guide stars. If the object was not seen in the 35 mm, as it usually was not, I would then look in the larger telescopes. If the object was not immediately visible even in the primary telescope – a not uncommon occur- rence due to inexact initial pointing – I would then scan around for it.
    [Show full text]
  • Multiwavelength Observations of the Peculiar Planetary Nebula Ic 2149 R
    The Astrophysical Journal, 576:860–869, 2002 September 10 # 2002. The American Astronomical Society. All rights reserved. Printed in U.S.A. MULTIWAVELENGTH OBSERVATIONS OF THE PECULIAR PLANETARY NEBULA IC 2149 R. Va´zquez,1 L. F. Miranda,2 J. M. Torrelles,3 L. Olguı´n,4 G. Benı´tez,1,5 L. F. Rodrı´guez,6 and J. A. Lo´pez1 Received 2001 August 18; accepted 2002 May 15 ABSTRACT We report high- and low-dispersion spectroscopy, optical imaging, and high-resolution Very Large Array- A 3.6 cm continuum observations of the peculiar planetary nebula IC 2149. These observations show that ‘‘ bipolar ’’ is a suitable morphological classification for IC 2149. Most nebular material is concentrated in a knotty, bright ring seen edge-on, embedded in an apparently oblate ellipsoidal shell from which remnant or incipient bipolar lobes emerge. We confirm the previously reported depletion in heavy elements and deduce a very low ejected nebular mass d0.03 M . All this information indicates that the formation of IC 2149 is the result of the evolution of a low-mass central star. Subject headings: ISM: kinematics and dynamics — planetary nebulae: individual (IC 2149) — stars: AGB and post-AGB 1. INTRODUCTION ula. IC 2149 hosts a very bright central star (V ’ 11:34, Ciardullo et al. 1999) with a stellar wind indicated by the In the last 10 yr, the commonly accepted theory on forma- presence of P Cygni profiles in the UV spectrum that indi- tion of planetary nebulae (PNs), involving the interaction of cate a wind velocity of V 1000–1600 km sÀ1 and a mass- stellar winds (Kwok, Purton, & Fitzgerald 1978), has been w ’ loss rate of M_ 10À8 M yrÀ1 (Perinotto, Benvenuti, & constantly revised in order to take into account a variety of w ’ Cerruti-Sola 1982; Feibelman et al.
    [Show full text]
  • MANUAL Blaze-Grating-Spektroskop/Spektrograph of N.Sommer Introduction
    MANUAL Blaze-Grating-Spektroskop/Spektrograph of N.Sommer Introduction The light of all astronomical objects contains three kinds of important, totally different Information. First the direction can be determined, from where it comes, enabling us to measure the Position and distance of the source. Secondly, its intensity can be investigated, so the luminosity and its eventual variations are evalu- able. Thirdly, looking at the spectrum one can analyse the chemical composition, radial velocity, surface tem- perature and the type and structure of the source of light. Furthermore the spectrum allows us to ascertain the otherwise determined source's distance using a different method. Spectrographs split up the component wavelengths (colors) of light and use either prisms, gratings or combinations of these. Prisms form only one spectrum but with very uneven dispersing power, so spectral lines are more crowded at red wavelengths than at blue. A further disadvantage is the faintness of the spectrum for the important blue region of wave- lengths because of the strong absorption in the glass-substrate and the especially high dispersion of blue light. So determination of specific wavelengths is more complex. On the other side, beneath an unchanged part of light (zero order) gratings deliver several higher order spectra (I1st & higher orders), which show nearly constant dispersion for all colors from red to blue light and high intensity for the shorter wavelengths. The Shortcoming of producing several spectra is greatly lessened by the Special figuring of the grooves, thus directing most of the light into one of two 1st order spectra. This effectively results in much brighter spectra, just like using a telescope of considerably greater aperture.
    [Show full text]
  • 100 Brightest Planetary Nebulae
    100 BRIGHTEST PLANETARY NEBULAE 100 BRIGHTEST PLANETARY NEBULAE 1 100 BRIGHTEST PLANETARY NEBULAE Visual Magnitude (brightest to least bright) Name Common Name Visual Magnitude Stellar Magnitude Angular Size Constellation NGC 7293 Helix Nebula 7 13.5 900 Aquarius NGC 6853 Dumbbell Nebula (M27) 7.5 13.9 330 Vulpecula NGC 3918 Blue Planetary 8 ? 16 Centaurus NGC 7009 Saturn Nebula 8 12.8 28 Aquarius NGC 3132 Eight‐Burst Planetary 8.5 10.1 45 Vela NGC 6543 Cat's Eye Nebula 8.5 11.1 20 Draco NGC 246 Skull Nebula 8.5 12 225 Cetus NGC 6572 Blue Raquetball Nebula 8.5 13.6 14 Ophiuchus NGC 6210 Turtle Nebula 9 12.7 16 Hercules NGC 6720 Ring Nebula (M57) 9 15.3 70 Lyra NGC 7027 Magic Carpet Nebula 9 16.3 14 Cygnus NGC 7662 Blue Snowball Nebula 9 13.2 20 Andromeda NGC 1360 Robin's Egg Nebula 9.5 11.4 380 Fornax NGC 1535 Cleopatra's Eye Nebula 9.5 12.2 18 Eridanus NGC 2392 Eskimo/Clown Face Nebula 9.5 10.5 45 Gemini NGC 2867 Royal Aqua Nebula 9.5 16.6 15 Carina NGC 3242 Ghost of Jupiter Nebula 9.5 12.3 40 Hydra NGC 6826 Blinking Planetary Nebula 9.5 10.4 25 Cygnus IC 418 Spirograph Nebula 10 10.2 12 Lepus NGC 5189 Spiral Planetary Nebula 10 14.9 140 Musca NGC 5882 Green Snowball Nebula 10 13.4 14 Lupus NGC 6818 Little Gem Nebula 10 16.9 18 Sagittarius NGC 40 Bow Tie Nebula 10.5 11.6 36 Cepheus NGC 1514 Crystal Ball Nebula 10.5 9.4 120 Taurus NGC 2346 Butterfly Nebula 10.5 11.5 55 Monoceros NGC 2438 Smoke Ring in M46 10.5 17.7 70 Puppis NGC 2440 Peanut Nebula 10.5 17.7 30 Puppis NGC 4361 Raven's Eye Nebula 10.5 13.2 100 Corvus IC 4406 Retina Nebula
    [Show full text]
  • Desert Skies – Winter 2016
    Tucson Amateur Astronomy Association Observing our Desert Skies since 1954 Volume , Issue Inside this issue: NGC 2170 in Monoceros President’s 2 Letter Outreach 3-6 Members’ News 7 CAC Update 8-10 Feature Articles 11-13 Observing 14-18 Kid’s Page 17 Classifieds 12 Sponsors 12 TAAA member Larry Phillips took this image (above) of NGC 2170. This is both a reflection (blue) Contacts 19 and emission (red) nebulae and star birth area found in the constellation Monoceros (the Unicorn). The black streaks are absorption nebulae. This object is 2400 light years away and the image expands an area 15 light years across. © Larry Take Note! Phillips. Used by permission. Grand Canyon Star Party Larry describes this as a hybrid image combining H- Get Ready! alpha images with regular RGB images. He has 38 CAC Update and Big News! hours of exposure in this image. Astronomy Services Report This area of Orion and Monoceros, contains a large molecular cloud known as R2 Mon to which NGC Planetary Nebulae and 2170 belongs and Barnard’s Loop which Image: NGC 2170 as seen companions encompasses much of Orion. by VISTA (Visible Objects in Canis Minor At right, an infrared image of the same object Infrared Survey Kid’s Page (different orientation). The infrared image Telescope for penetrates the dark nebulosity revealing a stellar Determining Stellar Astronomy) reveals the nursery. Magnitude secrets of the Unicorn. Viewing Black Hole Event For more information about this object, visit http:// Credit: ESO Horizon www.robgendlerastropics.com/NGC2170text.html. Desert Skies Page 2 Volume LXI, Issue 4 Winter 2016 From Our President Our mission is to provide opportunities for members and the public to share the joy and excitement of astronomy through observing, education and fun.
    [Show full text]
  • Interstellarum 17 Starhopper
    interstellarumEditorial fokussiert Wegen der kurzen Zeit, die diesmal zwi- schen dem Erscheinen dieser und der letz- Liebe Beobachterinnen, liebe Beobachter, ten Ausgabe lag, können wir in diesem Heft nur erste Ergebnisse der interstellarum Ein- Wir bedanken uns ganz herzlich bei Ihnen steiger-Aktion zeigen. Wir möchten alle allen für die hervorragende Aufnahme des Leser herzlich aufrufen, an dieser einmali- ersten Heftes der neuen Folge. Ihr gen Initiative teilzunehmen. Bitte informie- Zuspruch, Ihre Ermutigungen und viele ren Sie sich auf Seite 9 ausführlich über neue Bestellungen machten uns klar, dass unser neues Zielobjekt M 13 – unter allen wir auf dem richtigen Weg sind. Wir möch- Einsendern von Einsteiger-Beschreibungen, ten Sie dabei auch weiterhin an unserer Sei- -Zeichnungen und -Fotos verlosen wir drei te haben – beteiligen Sie sich an interstella- Freiabos und einen »Deep Sky Reiseführer«! rum kritisch und aktiv! Übrigens: Wir möchten Sie recht herzlich Unsere Service-Plattform im Internet – auf die Deep-Sky-Tagung 2001 einladen. www.interstellarum.de – wird mehr und Dort können Sie nicht nur in entspannter mehr zu einer Drehscheibe der Informatio- Atmosphäre über Deep-Sky fachsimpeln, nen für unsere Leser, die wir in naher sondern auch persönlichen Kontakt zum Zukunft noch deutlich ausbauen werden. interstellarum-Team knüpfen, wenn Sie Besuchen Sie unsere Website doch regelmä- wollen – wir freuen uns darauf. Mehr ßig und geben Sie auch anderen Stern- Informationen und Anmeldeunterlagen freunden unsere Internet-Seiten als Surf- finden Sie in diesem Heft. tipp weiter! Gefällt Ihnen das neue interstellarum? Wir haben versucht, Ihnen mit dieser Aus- Wenn ja, empfehlen Sie uns doch weiter: gabe abermals mehr zu bieten, als dies Ihren Beobachtungsfreunden, Ihren Ver- schon bei interstellarum 16 der Fall war: ein einskollegen, und warum nicht auch dem angenehmes Layout, noch mehr Farbe und jungen Einsteiger auf dem Beobachtungs- wieder viele interessante Beiträge.
    [Show full text]
  • The Planetary Nebula Club Objects by Month (As Posted by Ted Forte On
    The Planetary Nebula Club objects by month (As posted by Ted Forte on “backbayastro”) August Planetaries As most of you know, I am the coordinator of the Astronomical League’s Planetary Nebula Club. Several members of the BBAA helped me create the Planetary Nebula Club by serving on the object selection committee, serving on the rules committee, providing images, or by authoring parts of the observing manual. The Planetary Nebula Club creation was truly a BBAA effort. I think it’s a shame, therefore, that more BBAA’ers haven’t completed the program and earned the pin. So if you are looking for an observing program to complete, why not our very own? There was never a better time to start. More than half the list is visible right now and no less than 31 of our 110 PNe are optimally placed in August. Hence the title of this epistle. It is my intention to spark an interest in the program and suggest the objects that might be bagged in the coming weeks. Many of you have no doubt observed these objects already, so please chime in and share your impressions of them. As is true of the entire list, our August selection contains both well-known showpieces and some seldom mentioned objects that you might not consider tracking down if not for this program. There are no less than 17 of the 31 August objects that I would describe as “stellar”. I must confess that I am not the biggest fan of these tiny objects and had I been the sole arbiter of the list it would have contained far fewer of these.
    [Show full text]
  • The Homebuilt Telescope
    Patrick Moore’s Practical Astronomy Series For other titles published in the series, go to www.springer.com/series/3192 Make Time for the Stars Fitting Astronomy into Your Busy Life Antony Cooke Antony Cooke Capistrano Beach, CA ISBN 978-0-387-89340-2 e-ISBN 978-0-387-89341-9 DOI: 10.1007/978-0-387-89341-9 Springer Dordrecht Heidelberg London New York © Springer Science+Business Media, LLC 2009 All rights reserved. This work may not be translated or copied in whole or in part without the written permission of the publisher (Springer Science+Business Media, LLC, 233 Spring Street, New York, NY 10013, USA), except for brief excerpts in connection with reviews or scholarly analysis. Use in connection with any form of information storage and retrieval, electronic adaptation, computer software, or by similar or dissimilar methodology now known or hereafter developed is forbidden. The use in this publication of trade names, trademarks, service marks, and similar terms, even if they are not identified as such, is not to be taken as an expression of opinion as to whether or not they are subject to proprietary rights. Printed on acid-free paper Springer is part of Springer Science+Business Media (www.springer.com) This book is dedicated to my mother, Margot Cooke, with love and appreciation for the encouragement, freedom, and opportunities she provided so that I could make the most of everything meaningful to me. About the Author It has often been said that music and astronomy go hand in hand. Antony Cooke’s passion for both fields were clear very early in his life, but music ultimately would claim his career.
    [Show full text]
  • 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.
    [Show full text]
  • Planetary Nebula
    v 2016-06-07 <<< The 110 Best Planetary Nebula >>> Page 1 of 2 ^NGC Common Name Type Mag Size RA DEC 12AM Constellation 40 Red Bow-Tie Nebula PN 10.5 60" x 40" 00:13.0 +72° 31' Oct 09 Cepheus 246 Skull Nebula PN 8.5 4' 00:47.1 -11° 52' Oct 17 Cetus 650 Little Dumbbell - M76 PN 10.1 3' x 2' 01:42.3 +51° 35' Nov 01 Perseus 651 Little Dumbbell - M76 PN 10.1 3' x 2' 01:42.3 +51° 35' Nov 01 Perseus ic 1747 PN 12.0 20" 01:57.6 +63° 19' Nov 03 Cassiopeia ic 289 PN 13.0 40" 03:10.3 +61° 19' Nov 06 Cassiopeia 1360 Robin's Egg Nebula PN 9.5 6" 03:33.2 -25° 52' Nov 12 Fornax ic 351 PN 12.0 7" 03:47.5 +35° 03' Nov 17 Perseus ic 2003 PN 12.0 8" 03:56.4 +33° 53' Nov 19 Perseus 1501 Blue Oyster Nebula PN 12.5 1' 04:07.0 +60° 55 Nov 22 Camelopardalis 1514 Crystal Ball Nebula PN 10.5 2' 04:09.3 +30° 47' Nov 22 Taurus 1535 Cleopatra's Eye Nebula PN 9.5 18" 04:14.3 -12° 44' Nov 24 Eridanus ic 418 Spirograph Nebula PN 10.0 12" 05:27.5 -12° 42' Dec 13 Lepus 2022 White Snowball PN 11.5 20" 05:42.1 +09° 05' Dec 16 Orion ic 2149 Eye of the Charioteer PN 11.0 9" 05:56.4 +46° 06' Dec 20 Auriga ic 2165 PN 12.0 8" 06:21.7 -12° 59' Dec 25 Canis Major 2242 PN 14.5 22" 06:34.1 +44° 46' Dec 29 Auriga 2346 Butterfly Nebula PN 10.5 1' 07:09.4 -00° 48' Jan 06 Monoceros 2371 Candy Wrapper PN 13.0 55" x 30" 07:25.6 +29° 29' Jan 11 Gemini 2372 Candy Wrapper PN 13.0 55" x 30" 07:25.6 +29° 29' Jan 11 Gemini 2392 Eskimo Nebula PN 9.5 45" 07:29.1 +20° 55' Jan 12 Gemini 2438 Smoke Ring Nebula PN 10.5 1' 07:41.8 -14° 44' Jan 15 Puppis 2440 Peanut Nebula PN 10.5 30" 07:41.9 -18°
    [Show full text]