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October 2006
OCTOBER 2 0 0 6 �������������� http://www.universetoday.com �������������� TAMMY PLOTNER WITH JEFF BARBOUR 283 SUNDAY, OCTOBER 1 In 1897, the world’s largest refractor (40”) debuted at the University of Chica- go’s Yerkes Observatory. Also today in 1958, NASA was established by an act of Congress. More? In 1962, the 300-foot radio telescope of the National Ra- dio Astronomy Observatory (NRAO) went live at Green Bank, West Virginia. It held place as the world’s second largest radio scope until it collapsed in 1988. Tonight let’s visit with an old lunar favorite. Easily seen in binoculars, the hexagonal walled plain of Albategnius ap- pears near the terminator about one-third the way north of the south limb. Look north of Albategnius for even larger and more ancient Hipparchus giving an almost “figure 8” view in binoculars. Between Hipparchus and Albategnius to the east are mid-sized craters Halley and Hind. Note the curious ALBATEGNIUS AND HIPPARCHUS ON THE relationship between impact crater Klein on Albategnius’ southwestern wall and TERMINATOR CREDIT: ROGER WARNER that of crater Horrocks on the northeastern wall of Hipparchus. Now let’s power up and “crater hop”... Just northwest of Hipparchus’ wall are the beginnings of the Sinus Medii area. Look for the deep imprint of Seeliger - named for a Dutch astronomer. Due north of Hipparchus is Rhaeticus, and here’s where things really get interesting. If the terminator has progressed far enough, you might spot tiny Blagg and Bruce to its west, the rough location of the Surveyor 4 and Surveyor 6 landing area. -
Instruction Manual Meade Instruments Corporation
Instruction Manual 7" LX200 Maksutov-Cassegrain Telescope 8", 10", and 12" LX200 Schmidt-Cassegrain Telescopes Meade Instruments Corporation NOTE: Instructions for the use of optional accessories are not included in this manual. For details in this regard, see the Meade General Catalog. (2) (1) (1) (2) Ray (2) 1/2° Ray (1) 8.218" (2) 8.016" (1) 8.0" Secondary 8.0" Mirror Focal Plane Secondary Primary Baffle Tube Baffle Field Stops Correcting Primary Mirror Plate The Meade Schmidt-Cassegrain Optical System (Diagram not to scale) In the Schmidt-Cassegrain design of the Meade 8", 10", and 12" models, light enters from the right, passes through a thin lens with 2-sided aspheric correction (“correcting plate”), proceeds to a spherical primary mirror, and then to a convex aspheric secondary mirror. The convex secondary mirror multiplies the effective focal length of the primary mirror and results in a focus at the focal plane, with light passing through a central perforation in the primary mirror. The 8", 10", and 12" models include oversize 8.25", 10.375" and 12.375" primary mirrors, respectively, yielding fully illuminated fields- of-view significantly wider than is possible with standard-size primary mirrors. Note that light ray (2) in the figure would be lost entirely, except for the oversize primary. It is this phenomenon which results in Meade 8", 10", and 12" Schmidt-Cassegrains having off-axis field illuminations 10% greater, aperture-for-aperture, than other Schmidt-Cassegrains utilizing standard-size primary mirrors. The optical design of the 4" Model 2045D is almost identical but does not include an oversize primary, since the effect in this case is small. -
Diffuse X-Ray Emission from the Planetary Nebula NGC 7009
A&A 387, L1–L5 (2002) Astronomy DOI: 10.1051/0004-6361:20020330 & c ESO 2002 Astrophysics Diffuse X-ray emission from the planetary nebula NGC 7009? M. A. Guerrero, R. A. Gruendl, and Y.-H. Chu Astronomy Department, University of Illinois, 1002 W. Green Street, Urbana, IL 61801, USA Received 7 February 2002 / Accepted 1 March 2002 Abstract. XMM-Newton EPIC observations of the planetary nebula (PN) NGC 7009, the Saturn Nebula, have detected extended X-ray emission in its central cavity. The diffuse X-ray emission must originate in the shocked fast stellar wind. The spectra show that the temperature of the hot gas is 1.8 × 106 K. The rms density derived from the volume emission measure is a few tens H-atom cm−3. The hot gas does not appear over-pressurized with respect to the nebular shell. NGC 7009 represents an evolutionary stage at which the influence of the hot gas in the PN interior starts to decline due to the diminishing strength of the fast stellar wind and the expansion of the central cavity. Key words. ISM: planetary nebulae: general – ISM: planetary nebulae: individual: NGC 7009 – stars: winds, outflows – X-rays: ISM 1. Introduction Chandra observations of the evolved PN NGC 7293 (the Helix Nebula), on the other hand, does not show any dif- It has been commonly accepted that the shell struc- fuse X-ray emission (Guerrero et al. 2001). These results ture of a planetary nebula (PN) is formed by the cur- suggest that the hot gas content of a PN diminishes as the rent fast stellar wind sweeping up the previous asymp- PN ages. -
Caldwell Catalogue - Wikipedia, the Free Encyclopedia
Caldwell catalogue - Wikipedia, the free encyclopedia Log in / create account Article Discussion Read Edit View history Caldwell catalogue From Wikipedia, the free encyclopedia Main page Contents The Caldwell Catalogue is an astronomical catalog of 109 bright star clusters, nebulae, and galaxies for observation by amateur astronomers. The list was compiled Featured content by Sir Patrick Caldwell-Moore, better known as Patrick Moore, as a complement to the Messier Catalogue. Current events The Messier Catalogue is used frequently by amateur astronomers as a list of interesting deep-sky objects for observations, but Moore noted that the list did not include Random article many of the sky's brightest deep-sky objects, including the Hyades, the Double Cluster (NGC 869 and NGC 884), and NGC 253. Moreover, Moore observed that the Donate to Wikipedia Messier Catalogue, which was compiled based on observations in the Northern Hemisphere, excluded bright deep-sky objects visible in the Southern Hemisphere such [1][2] Interaction as Omega Centauri, Centaurus A, the Jewel Box, and 47 Tucanae. He quickly compiled a list of 109 objects (to match the number of objects in the Messier [3] Help Catalogue) and published it in Sky & Telescope in December 1995. About Wikipedia Since its publication, the catalogue has grown in popularity and usage within the amateur astronomical community. Small compilation errors in the original 1995 version Community portal of the list have since been corrected. Unusually, Moore used one of his surnames to name the list, and the catalogue adopts "C" numbers to rename objects with more Recent changes common designations.[4] Contact Wikipedia As stated above, the list was compiled from objects already identified by professional astronomers and commonly observed by amateur astronomers. -
AHSP Telescope Observing Award
AHSP Telescope Observing Award Compiled by Dan L. Ward • To qualify for the TOA pin, you must see 15 of the following 20 telescope targets. Check off each as you spot them. Seen # Object Const. Type* RA Dec Mag Size Nickname 1. M13 Her GC 16 41.7 +36 28 5.9 16' Great Hercules Globular 2. M57 Lyr PN 18 53.6 +33 02 9.7 86"x62" Ring Nebula 3. NGC 6819 Cyg OC 19 41.3 +40 11 7.3 5’ Fox Head Cluster 4. M27 Vul PN 19 59.6 +22 43 8.1 8’x6’ Dumbbell Nebula 5. NGC 7000 Cyg BN 20 58.8 +44 20 - 120'x100' North America Nebula 6. NGC 7009 Aqr PN 21 04.2 -11 22 8.3 28”x23” Saturn Nebula 7. M15 Peg GC 21 30.0 +12 10 7.5 12’ Great Pegasus Cluster 8. M2 Aqr GC 21 33.5 -00 49 6.3 16’ NGC 7089 9. M39 Cyg OC 21 32.2 +48 26 4.6 32' NGC 7092 10. M30 Cap GC 21 40.4 -23 11 8.4 11’x11’ NGC 7099 11. NGC 7331 Peg Gx 22 37.1 +34 25 10.4 11’x4’ Caldwell 30 12. M31 And Gx 00 42.8 +41 16 4.5 178’ Andromeda Galaxy 13. NGC 253 Scl Gx 00 47.5 -25 18 7.1 25’x7’ Sculptor Galaxy 14. NGC 457 Cas OC 01 19.1 +58 20 6.4 13’ Owl Cluster/ET Cluster 15. M74 Psc Gx 01 36.7 +15 47 10.5 10’x9.5’ The Phantom 16. -
Planetary Nebula: from Messier to Abell (Chart Addendum)
Planetary Nebula: From Messier to Abell (Chart Addendum) Messier Planetary Nebulae: M27 known as the “Dumbbell Nebula”, is located in the summer constellation of Vulpecula, 'The Fox’. Discovered in 1764, it was first planetary nebula ever observed, and is one of the brightest and most impressive, easily visible in binoculars. M27 is about 1360 light years distant, and is estimated to be close to 14,600 years old, and about 3 light- years in size. On summer evenings, it is well placed, almost directly overhead, and can be naked-eye from a dark sky location. Due to its high surface brightness, M27 can even be observable thru a small telescope or binoculars during Full Moon. Its central white dwarf star shines at 12.9+ magnitude and is easily visible at the center of the dumbbell shaped nebula in small telescopes. Distinct structural features can be observed within M27, including bright, sharply defined arcs coming off of either end of the dumbbell, along with striations between the main arcs and the center of the nebula. UHC and OIII filters will enhance the contrast of internal features of the nebula. M57 Located in the summer constellation of Lyra, 'The Lyre (Harp)’, and is known as the ‘Ring Nebula’. It was second planetary nebula discovered by Messier (in 1779, about 15 yrs after M27), and is easy to locate and can be observed with small telescopes, even in suburban skies. It is about 2300 light years distant, and about 6000 years old, and is estimated to have a diameter of about a half-light year, and is expanding at about 12 miles per second. -
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. -
Aquirius Sky Atlas
Aquarius Sternkarten / Star maps Astronomische Daten für diese Karten stammen von frei verfügbaren Datenbanken im Internet Astronomical data for this sky atlas were taken from free database sources on the internet Objektkataloge / Object databases: Centre de Données astronomiques de Strasbourg - http://cdsweb.u-strasbg.fr Saguaro Astronomy Club: SAC Database 7.70 - http://www.saguaroastro.org Sternkatalog / Star database: Star Database: SKY2000 Catalog, Version 4 (Myers+ 2002) http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=V/109 An den Karten haben mitgewirkt / People that have been working on the maps: Fred Van Gestel (author), Dennis Wallace (PDF and data base editing) Alle Sternkarten stehen unter einer Creative Commons – Namensnennung – Nicht-Kommerziell Lizenz All star maps are licensed under a Creative Commons – Attribution – NonCommercial license http://creativecommons.org/licenses/by-nc/4.0/ Aquarius ©2014 by Fred Van Gestel – http://vangestel.de/astro AQUARIUS constellation index (objects up to 12m0) 21 Objects Open clusters Object Const. Name Page(s) Vmag Size Instrument OIII UHC H-β Distance NGC/IC M73 AQR Aqr 1-2 9.00 1' 10x50 2000 Ly 6994 1 open cluster Globular clusters Object Const. Name Page(s) Vmag Size Instrument OIII UHC H-β Distance NGC/IC M2 AQR Aqr 1-2 6.50 6' 8x30 40000 Ly 7089 M72 AQR Aqr 1-2 9.30 3' 10x50 62000 Ly 6981 N7492 AQR Aqr 2-1 11.20 7492 3 globular clusters Galaxies Object Const. Name Page(s) Vmag Size Instrument OIII UHC H-β Distance NGC/IC H393 AQR Aqr 1-1 10.80 4.2' 7606 H396 AQR Aqr 1-1 Aqr 2-1 11.10 3.5' 7723 H397 AQR Aqr 1-1 Aqr 2-1 10.70 4.7' 7727 N7183 AQR Aqr 2-1 11.90 7183 N7184 AQR Aqr 2-1 10.90 7184 N7218 AQR Aqr 2-1 12.00 7218 N7284 AQR Aqr 2-1 11.90 7284 N7285 AQR Aqr 2-1 11.90 7285 N7371 AQR Aqr 1-1 Aqr 2-1 11.50 7371 N7377 AQR Aqr 2-1 11.10 7377 N7391 AQR Aqr 1-1 12.00 7391 N7392 AQR Aqr 2-1 11.90 7392 N7585 AQR Aqr 1-1 11.40 7585 N7600 AQR Aqr 1-1 11.90 7600 N7721 AQR Aqr 1-1 11.60 7721 15 galaxies Planetary nebula Object Const. -
Aquarius, the Watering Can Man by Magda Streicher [email protected]
deepsky delights Aquarius, the Watering Can Man by Magda Streicher [email protected] Aquarius is by no means just another constellation – it’s quite simply something exceptional in its own right. Aquarius the Image source: Stellarium water-bearer spreads out its lanky image just north of Capricornus the sea-goat. Other ier, the French astronomer. Averted vision well-known water constellations are Piscis yields the best view, which sees the object Austrinus the southern fish, Cetus the whale, brightening relatively quickly to a core that Delphinus the dolphin and Hydra the water appears slightly more square than round and snake. The water-bearer was so named due less concentrated than most globulars. Not to the Sun’s entry into the constellation dur- at all easy to resolve, although I can pick up ing the Babylonian monsoon season. The a grainy tangerine skin impression, which image portrays a man pouring water from a makes me suspect partial resolution. pitcher he’s holding in his right hand. Little sprays of brighter stars look like numerous Just 1.2 degrees to the east, arguably one of drops of water and stand out well against the most interesting documented clusters or the fainter background star-field. When star asterisms can be seen. NGC 6994, bet- Aquarius is about appear in the east, Albali, ter known as Messier 73, consists of a cluster or Epsilon Aquarii, at magnitude 3.7, pops of only four stars, which the University of up as the western-most star in the constella- Padua in Italy places at different distances as tion, as if to say “Here I am!” field stars. -
The Age of Aquarius Is an Astrological Term Denoting Either the Current Or Upcoming Astrological Age, Depending on the Method of Calculation
The Age of Aquarius is an astrological term denoting either the current or upcoming astrological age, depending on the method of calculation. Astrologers maintain that an astrological age is a product of the earth's slow precessional rotation and lasts for 2,150 years, on average. In popular culture in the United States, the Age of Aquarius refers to the advent of the New Age movement in the 1960s and 1970s. There are various methods of calculating the length of an astrological age. In sun- sign astrology, the first sign is Aries, followed by Taurus, Gemini, Cancer, Leo, Virgo, Libra, Scorpio, Sagittarius, Capricorn, Aquarius, and Pisces, whereupon the cycle returns to Aries and through the zodiacal signs again. Astrological ages, however, proceed in the opposite direction ("retrograde" in astronomy). Therefore, the Age of Aquarius follows the Age of Pisces. Mythology of the constellation Aquarius This is the eleventh zodiacal sign and one which has always been connected with water. To the Babylonians it represented an overflowing urn, and they associated this with the heavy rains which fell in their eleventh month, whilst the Egyptians saw the constellation as Hapi, the god of the Nile. Greek legend, however, tells of Ganymede, an exceptionally handsome, young prince of Troy. He was spotted by Zeus, who immediately decided that he would make a perfect cup-bearer. The story then differs - one version telling how Zeus sent his pet eagle, Aquila, to carry Ganymede to Olympus, another that it was Zeus, himself, disguised as an eagle, who swept up the youth and carried him to the home of the gods. -
2021-01-22 Weekly Newsletter
rguably one of the best ever sitcoms and certainly Aone of mine and Robbie’s favourites, ‘Allo Allo’ manages to take the mickey out of every side in WWII without causing offence to any of them. When we lived in France we discovered that the French transla�on was every bit as funny. ClickHERE for an hour of the best bits. There can’t be many people who don’t think fresh snow is beau�ful Do you have hidden talents? Do (before it goes grey and you have a man cave or a she shed, slushy and we have to go in which you turn out canvas out in it). masterpieces, wooden wonders, metal marvels or other amazing One scien�st/photographer is so fascinated with things? Does your snow crystals that he has developed a camera par�cular hobby/skill take the which captures images at a microscopic level. form of magic, music or Click HERE to read the ar�cle. mayhem? Our readers would love to read about your (family friendly) pas�mes so please send in your stories. If you can share photos or videos even be�er! Send contribu�ons to the normal email address. To get things started, some of you already know that I sing in a chorus. Click HERE to watch us singing our version of the Who would have thought that a car with so many Turtles’ song ‘Happy Together’. I can’t controversial stories a�ached to it, not to begin to describe the fun and men�on poor owner experiences, could not only challenges we had learning this one. -
November 2014
PRET ORI A CENT RE ASSA - NOVEM BER 2014 PAGE 1 NEWSLETTER NOVEMBER 2 014 Next m eeting Venue: The auditorium behind the main building at Christian Brothers College (CBC), Mount Edmund, Pretoria Road, Silverton, Pretoria. Date and time: Wednesday 26 November at 19h15. Programme: • Beginner’s Corner:.”What is a year?” by Michael Poll.* • What’s Up? by Percy Jacobs. • 10 minute break — library will be open. • Main talk: “The star of Bethlehem” by Prof André Buys, • Socializing over tea/coffee and biscuits. The chairperson at the meeting will be Danie Barnardo. * See page 5 for a summary of his talk. Next observing evening Friday 21 November from sunset onwards at the Pretoria Centre Observatory, which is also situ- ated at CBC. Turn left immediately after entering the main gate and follow the road. Contents of this newsletter Chairman’s Report for the meeting of 22nd October 2014 2 NOTICE BOARD 1 4 NOTICE BOARD 2 N.B. 5 Pretoria ASSA - ASSA "Top 100" Observing list 5 Summary of talk for Beginners Corner 5 Summary of “What’s Up?” to be presented on 26 November 2014 6 One Splendid Deep Sky Object: NGC 7009, a planetary nebula 7 Photograph with caption & Feature of the month: Titan eclipsed by Rhea 8 Report for Observing Evening on October 17th 2014 9 Basics: Stephan’s Quintet 9 Image of Stephan’s Quintet 10 Noteworthy astronomy-related articles on the Internet 10 Sunspot Group AR 2192 12 Pretoria Centre committee & Pretoria Centre committee & Old newsletters & Database 12 PAGE 2 PRET ORI A CENT RE ASSA - NOVEM BER 2014 Chairman’s Report for the meeting of 22nd October 2014 by Percy Jacobs Visitors & members were welcomed to our monthly meeting.