Observing Log Leyland Observatory

Total Page:16

File Type:pdf, Size:1020Kb

Observing Log Leyland Observatory Observing Log and commentary Leyland Observatory Len Adam November 2012 1 Thursday 1st November 2012 Thursday 1st November 2012 Will this really be a daylight comet? I have just downloaded the image of the field of Comet C/2012 S1 (ISON) that is predicted to be a naked eye object in Autumn 2013. I used the 32 inch Mount Lemmon Telescope belonging to the November 2012 University of Arizona that is part of the Sierra Stars network to make the exposure. It was a 5 minute Observations exposure taken yesterday at 11:26 U.T. There is an object at the precise spot indicated by the SKyX chart for the comet that I have circled in the image below. Reference magnitudes would indicate that Len Adam the comet is around mag 17. I plate solved the image in the SKy6 and measured the magnitude using the CCDSoft/Sky6 photometry facility at mag 17.55. (See the image on the next page - bottom left - taken a few days later (very close to the moon) that confirms this is the comet showing exact positions corresponding to predictions) 159 170 163 Comet C\2012 S1 ISON 2012 31 Oct. 11: 26 U.T. Remote image from Schulman 0.81-m. Mt Lemmon Arizona 300s exp. SBIG STX KAF-16803 binned 2x2 0.65 arcsec /pixel. FOV 22.5’X22.5’ UCAC3 Reference Magnitudes Unfiltered mag measured at 17.55 Len Adam 2 Thursday 1st November 2012 Including Magnified view By the 5th November 2012 the comet had moved to here Location on 31 Oct 2012 Image Courtesy of the University of Arizona The Schulman telescope 3 Thursday 1st November 2012 The orbit of the comet is shown below - it is heading for the Sun at a sharp angle to the plane of the ecliptic. Courtesy NASA/JPL-Caltech. It is currently 5.6 AU from the Earth – i.e. Over 5 times further away from us than the Sun itself. Not surprising then that it is very faint at the moment . When it gets closer it will get brighter – the warmth of the Sun will begin to melt some of the icy content and a tail will develop. At its closest to the Earth it will be at a distance of about 0.43 AU - around 13 times nearer than it is now. It is predicted to be a daytime comet as bright as the full Moon and could be a good Christmas Comet. 4 Courtesy NASA/JPL-Caltech. Thursday 1st November 2012 I realised that on 26th October I had also carried out a supernova search on 38 galaxies in Auriga that I had omitted from my October log. (No supernovae found) .This is the first image – PGC 16158. PGC 16158 Courtesy of Software Bisque This is the solved image placed behind the SkyX star chart – meaning that labels e.g. Magnitudes are superimposed on the image – an excellent feature. 5 Thursday 1st November 2012 Plate solution for another Auriga galaxy – PGC 16918 showing magnitudes of stars superimposed on the image by the solution. Courtesy of Software Bisque The corresponding DSS image 85s exposure Courtesy of The Oschin Schmidt Telescope operated by the California Institute of Technology and Palomar Observatory. 6 Thursday 1st November 2012 PGC 17954 image superimposed on the SkyX chart and the C14/ST9XE Field of View Indicator. Courtesy of Software Bisque The image of PGC 17954 in Auriga 7 Friday 2nd November 2012 Friday 2nd November 2012 An image of M52 was attempted using the iTelescope.net T20 telescope. T20 Courtesy of iTelescope.net Unfortunately the image was greyed out so I will try for this object on another occasion. (See Wednesday 21st November) 8 Friday 2nd November 2012 SJ O’Meara Hidden Treasures Target NGC 6503 – The Lost in Space Nebula Having purchased the above author’s excellent Hidden Treasures book on Sunday in Manchester , I am locating images that I have previously taken that correspond to some of his targets and finding out more about them. This is a 30 second image taken on 20th April 2011. There was no cooling for some reason as the FITS header shows a 12 degree temperature. The plate solution above shows a plate scale of 2-02 arcseconds per pixel and a Field of View of 17 minutes X 17 minutes. Courtesy of ESA/Hubble and NASA A Hubble view of NGC 6503. The pink glowing areas are starbirth regions . The galaxy is called the “Lost in Space” galaxy by Stephen O’Meara because it is located at the edge of a void (shades of Star Trek). It is only one third the major axis size of our Galaxy and is a Dwarf Spiral Galaxy. Arthur Auwers the German astronomer discovered the galaxy in 1854. It lies at a distance of 17 million Light Years. 9 Friday 2nd November 2012 The location of NGC 6503 in Draco Courtesy of Cartes du Ciel 10 Telescope Image Courtesy of iTelescope .net Friday 2nd November 2012 This is the same M42 image that I previously showed the luminance file for – P44 October Log. 11 Friday 2nd November 2012 This is the “Running Man” nebula – taken from the M42 image above. The images below are interesting sections of the above image for further study. 12 Colour variation of theM42 image. Friday 2nd November 2012 13 Sunday 4th November 2012 Sunday 4th November 2012 A busy morning and evening with observations and images of NGC 1499, 2 comets , 38 galaxies in Auriga, 20 galaxies in Cassiopeia, 42 galaxies in Cygnus and 4 galaxies in Triangulum. I used the T20 iTelescope.net telescope to image the California Nebula (well part of it) in Perseus. I was looking for an emission nebula to image that was well away from the Moon to get further practice using IRIS This is the SkyX chart of the California Nebula showing the Field of View of the T20 Telescope with the solved plate superimposed. North is up in this image The final image after processing in IRIS is shown below Courtesy of Software Bisque Courtesy of Software Bisque Courtesy of Software Bisque 14 The final image with North towards the top to correspond to the solved image in the chart above is shown on the next page. Sunday 4th November 2012 15 Sunday 4th November 2012 Comet C/2010 S1 (Linear) in Cygnus A series of images of Comet C/2010 S1 (Linear) were taken on Sunday night. The first is shown below Photometry I solved the plate in SkyX and measured the magnitude in CCDSoft at 13.91 using a 14th magnitude UCAC3 reference star. Astrometry The position was measured at RA 20h 36m 57s DEC 41d 31m 05s at the date and time shown from the FITS Header. Position of the Comet today – it is almost 6 times the distance to the Sun from Earth. 16 Courtesy NASA/JPL-Caltech. Sunday 4th November 2012 Comet 168P Hergenrother in Andromeda 168P has a period of 6.89 years. It was discovered by Carl W. Hergenrother on November 22nd 1998. Its last Perihelion (before this year) was in 1995. It was at Perihelion this year (2012) on October 1st Other Astrometry Designations The position was measured at RA 23h 40m 30s P/1998 W2 P/2005 N2 DEC 37d 08m 51s This means that This means that it was the at the date and time shown it was the second comet discovered on the FITS Header. This is for second comet in the first half of July the head of the comet. No discovered in 2005. Of course in fact it photometry was attempted. the second half was a rediscovery of of November P/1998 W2 1998. Because this is a short period comet (<250 years) and it HAS returned since discovery it is given the designation 168P Hergenrother. 17 Sunday 4th November 2012 During the Supernova Patrol an image was obtained of three galaxies in Cygnus all within 3 minutes of arc PGC 67235 was the target PGC 67239 PGC 67243 PGC 67235 PGC 67235 18 Courtesy of Software Bisque Plate solution for NGC 6946 Sunday 4th November 2012 Courtesy of Software Bisque NGC 6946 was imaged as part of the Supernova Patrol tonight in Cygnus. 19 Sunday 4th November 2012 NGC 6946 is known as the “Fireworks” Galaxy . 5 Supernovae that have occurred in this galaxy are shown in the above image. Stellar magnitudes in the region are also shown 20 Wednesday 7th November 2012 Wednesday 7th November 2012 The T20 iTelescope.net telescope in New Mexico was given the task of imaging NGC 2264 “The Christmas Tree Nebula” with a 300 second exposure. Image Courtesy of iTelescope .com The SkyX New Mexico Skies site document was opened to check that the choice of field of view was appropriate and that the object was in an appropriate position for imaging at that site. (Altitude) The SkyX report is shown on the left. At 59 degrees altitude it is in a good position. 21 Wednesday 7th November 2012 NGC 2264 22 Wednesday 7th November 2012 As soon as the NGC 2264 run was complete on T20 I started a run on M38 Courtesy of iTelescope.net Courtesy of Software Bisque 23 Wednesday 7th November 2012 M38 is at an altitude of almost 87 degrees. It has dimensions 15’ X 15’ so will certainly not fill the 112’ X 84’ T20 FOV. However the FOV will include Herschel H39-7 which has a FO V of 5 minutes square. Telescope Image courtesy of iTelescope.net 24 Messier 38 including H39-7 Wednesday 7th November 2012 25 Wednesday 7th November 2012 M38 itself from the full image H39-7 from the full image This is also known as NGC 1907 26 A stretched view brings out the red nebulosity in the region Wednesday 7th November 2012 27 Wednesday 7th November 2012 Supernova 2012fm This is an image that I took that missed the supernova – although it had already been discovered.
Recommended publications
  • Meeting Announcement Upcoming Star Parties And
    CVAS Executive Committee Pres – Bruce Horrocks Night Sky Network Coordinator – [email protected] Garrett Smith – [email protected] Vice Pres- James Somers Past President – Dell Vance (435) 938-8328 [email protected] [email protected] Treasurer- Janice Bradshaw Public Relations – Lyle Johnson - [email protected] [email protected] Secretary – Wendell Waters (435) 213-9230 Webmaster, Librarian – Tom Westre [email protected] [email protected] Vol. 7 Number 6 February 2020 www.cvas-utahskies.org The President’s Corner Meeting Announcement By Bruce Horrocks – CVAS President Our next meeting will be held on Wed. I don’t know about most of you, but I for February 26th at 7 pm in the Lake Bonneville Room one would be glad to at least see a bit of sun and of the Logan City Library. Our presenter will be clear skies at least once this winter. I believe there Wendell Waters, and his presentation is called was just a couple of nights in the last 2 months that “Charles Messier and the ‘Not-Comet’ Catalogue”. I was able to get out and do some observing and so I The meeting is free and open to the public. am hoping to see some clear skies this spring. I Light refreshments will be served. COME AND have watched all the documentaries I can stand on JOIN US!! Netflix, so I am running out of other nighttime activities to do and I really want to get out and test my new little 72mm telescope. Upcoming Star Parties and CVAS Events We made a change to our club fees at our last meeting and if you happened to have missed We have four STEM Nights coming up in that I will just quickly explain it to you now.
    [Show full text]
  • Messier Objects
    Messier Objects From the Stocker Astroscience Center at Florida International University Miami Florida The Messier Project Main contributors: • Daniel Puentes • Steven Revesz • Bobby Martinez Charles Messier • Gabriel Salazar • Riya Gandhi • Dr. James Webb – Director, Stocker Astroscience center • All images reduced and combined using MIRA image processing software. (Mirametrics) What are Messier Objects? • Messier objects are a list of astronomical sources compiled by Charles Messier, an 18th and early 19th century astronomer. He created a list of distracting objects to avoid while comet hunting. This list now contains over 110 objects, many of which are the most famous astronomical bodies known. The list contains planetary nebula, star clusters, and other galaxies. - Bobby Martinez The Telescope The telescope used to take these images is an Astronomical Consultants and Equipment (ACE) 24- inch (0.61-meter) Ritchey-Chretien reflecting telescope. It has a focal ratio of F6.2 and is supported on a structure independent of the building that houses it. It is equipped with a Finger Lakes 1kx1k CCD camera cooled to -30o C at the Cassegrain focus. It is equipped with dual filter wheels, the first containing UBVRI scientific filters and the second RGBL color filters. Messier 1 Found 6,500 light years away in the constellation of Taurus, the Crab Nebula (known as M1) is a supernova remnant. The original supernova that formed the crab nebula was observed by Chinese, Japanese and Arab astronomers in 1054 AD as an incredibly bright “Guest star” which was visible for over twenty-two months. The supernova that produced the Crab Nebula is thought to have been an evolved star roughly ten times more massive than the Sun.
    [Show full text]
  • Guide Du Ciel Profond
    Guide du ciel profond Olivier PETIT 8 mai 2004 2 Introduction hjjdfhgf ghjfghfd fg hdfjgdf gfdhfdk dfkgfd fghfkg fdkg fhdkg fkg kfghfhk Table des mati`eres I Objets par constellation 21 1 Androm`ede (And) Andromeda 23 1.1 Messier 31 (La grande Galaxie d'Androm`ede) . 25 1.2 Messier 32 . 27 1.3 Messier 110 . 29 1.4 NGC 404 . 31 1.5 NGC 752 . 33 1.6 NGC 891 . 35 1.7 NGC 7640 . 37 1.8 NGC 7662 (La boule de neige bleue) . 39 2 La Machine pneumatique (Ant) Antlia 41 2.1 NGC 2997 . 43 3 le Verseau (Aqr) Aquarius 45 3.1 Messier 2 . 47 3.2 Messier 72 . 49 3.3 Messier 73 . 51 3.4 NGC 7009 (La n¶ebuleuse Saturne) . 53 3.5 NGC 7293 (La n¶ebuleuse de l'h¶elice) . 56 3.6 NGC 7492 . 58 3.7 NGC 7606 . 60 3.8 Cederblad 211 (N¶ebuleuse de R Aquarii) . 62 4 l'Aigle (Aql) Aquila 63 4.1 NGC 6709 . 65 4.2 NGC 6741 . 67 4.3 NGC 6751 (La n¶ebuleuse de l’œil flou) . 69 4.4 NGC 6760 . 71 4.5 NGC 6781 (Le nid de l'Aigle ) . 73 TABLE DES MATIERES` 5 4.6 NGC 6790 . 75 4.7 NGC 6804 . 77 4.8 Barnard 142-143 (La tani`ere noire) . 79 5 le B¶elier (Ari) Aries 81 5.1 NGC 772 . 83 6 le Cocher (Aur) Auriga 85 6.1 Messier 36 . 87 6.2 Messier 37 . 89 6.3 Messier 38 .
    [Show full text]
  • Injunction Sought to Delay J.C. Penney
    Injunction sought to delay J.C. Penney and meaningful consideration of en­ the town’s Economic Development original complaint but not in the By Scot French Manchester law firm of Beck & new,” since it has been part of the vironmental factors.” Commission, said this morning he complaint for a new trial. He Herald Reporter Pagano, said the coalition has coalition’s plans for several years. ’The environmentalists, organized The justices ruled that the lower had not yet seen a copy of the injunc­ speculated that the motion was filed already proved that the lack of a tion motion and therefore could not to correct that oversight. A Manchester enviromnmeiital mass transit system to serve the by local pharmacist Michael court had followed improper Dworkin, won a major victory last procedures in rejecting the en­ comment. The J.C. Penney vvarehouse, a coalition fighting for a mass transit site will dangerously increase air regional distribution center for system to serve the Buckiand In- May when the state Supreme Court vironmentalists case and ordered a Bourke G. Spellacy, an attorney pollution in the area. who has represented J.C. Penney catalogue sales in the northeast, dustriai Park has formally asked He said the injunction is the “only struck down a lower court ruling new trial. against the coalition and ordered a since the originai suit was filed in began accepting applications for 1,- the courts to block the J.C. Penney relief avaiiable” while the coalition I’AGANO SAID PROCEDURAL 500 full-time jobs last month. warehouse from opening this fall. new trial.
    [Show full text]
  • February 2019 These Pages Are Intended to Help You Find Your Way Around the Sky
    WHAT'S UP THIS MONTH – FEBRUARY 2019 THESE PAGES ARE INTENDED TO HELP YOU FIND YOUR WAY AROUND THE SKY The chart above shows the night sky as it appears on 15th February at 21:00 (9 o’clock) in the evening Greenwich Mean Time (GMT). As the Earth orbits the Sun and we look out into space each night the stars will appear to have moved across the sky by a small amount. Every month Earth moves one twelfth of its circuit around the Sun, this amounts to 30 degrees each month. There are about 30 days in each month so each night the stars appear to move about 1 degree. The sky will therefore appear the same as shown on the chart above at 10 o’clock GMT at the beginning of the month and at 8 o’clock GMT at the end of the month. The stars also appear to move 15º (360º divided by 24) each hour from east to west, due to the Earth rotating once every 24 hours. The centre of the chart will be the position in the sky directly overhead, called the Zenith. First we need to find some familiar objects so we can get our bearings. The Pole Star Polaris can be easily found by first finding the familiar shape of the Great Bear ‘Ursa Major’ that is also sometimes called the Plough or even the Big Dipper by the Americans. Ursa Major is visible 1 of 13 pages throughout the year from Britain and is always easy to find. This month it is in the North East.
    [Show full text]
  • 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]
  • March 2021 These Pages Are Intended to Help You Find Your Way Around the Sky
    WHAT'S UP THIS MONTH – MARCH 2021 THESE PAGES ARE INTENDED TO HELP YOU FIND YOUR WAY AROUND THE SKY The chart above shows the whole night sky as it appears on 15th March at 21:00 (9 o’clock) Greenwich Mean Time (GMT). As the Earth orbits the Sun and we look out into space each night the stars will appear to have moved across the sky by a small amount. Every month Earth moves one twelfth of its circuit around the Sun, this amounts to 30 degrees each month. There are about 30 days in each month so each night the stars appear to move about 1 degree. The sky will therefore appear the same as shown on the chart above at 8 o’clock GMT at the beginning of the month and at 10 o’clock GMT at the end of the month. The stars also appear to move 15º (360º divided by 24) each hour from east to west, due to the Earth rotating once every 24 hours. The centre of the chart will be the position in the sky directly overhead, called the Zenith. First we need to find some familiar objects so we can get our bearings. The Pole Star Polaris can be easily found by first finding the familiar shape of the Great Bear ‘Ursa Major’ that is also sometimes called the Plough or even the Big Dipper by the Americans. Ursa Major is visible throughout the year from Britain and is always quite easy to find. This month it is high in the North East.
    [Show full text]
  • OBSERVING BASICS by GUY MACKIE
    OBSERVING BASICS by GUY MACKIE Observing Reports The colorful and detailed photographs we see of celestial objects are not at all like the ubiquitous "fuzzy blobs" we see at the eyepiece. Nevertheless, you are freezing your buns off and loosing much needed sleep for work, the next day so why not make a description of your observations that will make the hunt worthwhile. Here are some suggestions to fill the empty spaces in your logbook and to imprint the observing experience more deeply in your memory. The Basics Your website www.m51.ca has a downloadable log sheet template that is just super, but you can also make up one for yourself or customize the website version to your own needs. The main things to start your report should be the circumstances under which you observed: Observing Location Time (of observing session and of the observation of each object) Optics (type of instrument, eyepiece, filters, power of magnification) Transparency (page 56 of the Observers Handbook) Seeing (for me this is a subjective rating of the atmospheric stability based on Planet features and double star observations) It is good to know the field of view (FOV) of each of your eyepieces in minutes of degree, then you can estimate the approximate size of the object. The sketchpad I use has the FOV for every eyepiece I use taped to the back, a handy reference. To calculate your field of view there are websites that will punch out the both the magnification and the FOV for most eyepieces. You can do it yourself: With any motor drives turned off, place a star near the celestial equator just outside the field of view in the eyepiece so that it will drift across the middle of the field of view.
    [Show full text]
  • Core-Collapse Supernovae Overview with Swift Collaboration
    Publications Spring 2015 Core-Collapse Supernovae Overview with Swift Collaboration Kiranjyot Gill Embry-Riddle Aeronautical University, [email protected] Michele Zanolin Embry-Riddle Aeronautical University, [email protected] Marek Szczepańczyk Embry-Riddle Aeronautical University, [email protected] Follow this and additional works at: https://commons.erau.edu/publication Part of the Astrophysics and Astronomy Commons, and the Physics Commons Scholarly Commons Citation Gill, K., Zanolin, M., & Szczepańczyk, M. (2015). Core-Collapse Supernovae Overview with Swift Collaboration. , (). Retrieved from https://commons.erau.edu/publication/3 This Report is brought to you for free and open access by Scholarly Commons. It has been accepted for inclusion in Publications by an authorized administrator of Scholarly Commons. For more information, please contact [email protected]. Core-Collapse Supernovae Overview with Swift Collaboration∗ Kiranjyot Gill,y Dr. Michele Zanolin,z and Marek Szczepanczykx Physics Department, Embry Riddle Aeronautical University (Dated: June 30, 2015) The Core-Collapse supernovae (CCSNe) mark the dynamic and explosive end of the lives of massive stars. The mysterious mechanism, primarily focused with the shock revival phase, behind CCSNe explosions could be explained by detecting the corresponding gravitational wave (GW) emissions by the laser interferometer gravitational wave observatory, LIGO. GWs are extremely hard to detect because they are weak signals in a floor of instrument noise. Optical observations of CCSNe are already used in coincidence with LIGO data, as a hint of the times where to search for the emission of GWs. More of these hints would be very helpful. For the first time in history a Harvard group has observed X-ray transients in coincidence with optical CCSNe.
    [Show full text]
  • The Messier Catalog
    The Messier Catalog Messier 1 Messier 2 Messier 3 Messier 4 Messier 5 Crab Nebula globular cluster globular cluster globular cluster globular cluster Messier 6 Messier 7 Messier 8 Messier 9 Messier 10 open cluster open cluster Lagoon Nebula globular cluster globular cluster Butterfly Cluster Ptolemy's Cluster Messier 11 Messier 12 Messier 13 Messier 14 Messier 15 Wild Duck Cluster globular cluster Hercules glob luster globular cluster globular cluster Messier 16 Messier 17 Messier 18 Messier 19 Messier 20 Eagle Nebula The Omega, Swan, open cluster globular cluster Trifid Nebula or Horseshoe Nebula Messier 21 Messier 22 Messier 23 Messier 24 Messier 25 open cluster globular cluster open cluster Milky Way Patch open cluster Messier 26 Messier 27 Messier 28 Messier 29 Messier 30 open cluster Dumbbell Nebula globular cluster open cluster globular cluster Messier 31 Messier 32 Messier 33 Messier 34 Messier 35 Andromeda dwarf Andromeda Galaxy Triangulum Galaxy open cluster open cluster elliptical galaxy Messier 36 Messier 37 Messier 38 Messier 39 Messier 40 open cluster open cluster open cluster open cluster double star Winecke 4 Messier 41 Messier 42/43 Messier 44 Messier 45 Messier 46 open cluster Orion Nebula Praesepe Pleiades open cluster Beehive Cluster Suburu Messier 47 Messier 48 Messier 49 Messier 50 Messier 51 open cluster open cluster elliptical galaxy open cluster Whirlpool Galaxy Messier 52 Messier 53 Messier 54 Messier 55 Messier 56 open cluster globular cluster globular cluster globular cluster globular cluster Messier 57 Messier
    [Show full text]
  • The Night Sky February 2021. Auriga Constellation
    Binocular Observing February 2021 by Andrew Lohfink. The Night Sky February 2021. Auriga Constellation. Auriga Constellation. The constellation Auriga lies high in the February night sky near the zenith. Look for the bright star Capella which forms part of a lop sided hexagon asterism. Auriga contains two large binocular asterisms best viewed at low power with wide field views. The first is called The Cheshire Cat and can be seen arrowed opposite. The Cheshire Cat Asterism. Just to the west of M38 lies a chance line of sight asterism – The Cheshire cat or Smiley Face. There are a curved line of stars forming the mouth and 2 bright stars forming the eyes. See if you can tease out the differing colours of the stars. The Leaping Minnow Asterism. Just to the west of The Cheshire Cat lies another binocular asterism called The Leaping Minnow. Seen opposite, the bright stars in the centre of the image form a fish shape. When observed directly in the night sky you may be able to see a small pool of stars where the minnow splashes into the water. The differing star colours are a beautiful sight in any size binoculars but look best at about 15x70. You will not see the nebulosity either side of the asterism as seen in the opposite image with binoculars. The Three Messier Clusters in Auriga. Auriga is home to the famous trio of open star clusters – M36, 37 & 38. Each can be seen with binoculars of all sizes. The key to finding them is imagine a line from Theta to Gamma Aurigae (also known as Beta Tauri).
    [Show full text]
  • Volume 74 Nos 11 & 12 December 2015 News Notes
    Volume 74 Nos 11 & 12 December 2015 In this issue News Notes – Number of Research Astronomers in SA Fireball Observations- Blaauwberg Meridian Marker AGM – Colloquia and Seminars – Sky Delights EDITORIAL Mr Case Rijsdijk (Editor, MNASSA ) BOARD Mr Auke Slotegraaf (Editor, Sky Guide Africa South ) Mr Christian Hettlage (Webmaster) Prof M.W. Feast (Member, University of Cape Town) Prof B. Warner (Member, University of Cape Town) MNASSA Mr Case Rijsdijk (Editor, MNASSA ) PRODUCTION Dr Ian Glass (Assistant Editor) Ms Lia Labuschagne (Book Review Editor) Willie Koorts (Consultant) EDITORIAL MNASSA, PO Box 9, Observatory 7935, South Africa ADDRESSES Email: [email protected] Web page: http://mnassa.saao.ac.za MNASSA Download Page: www.mnassa.org.za SUBSCRIPTIONS MNASSA is available for free download on the Internet ADVERTISING Advertisements may be placed in MNASSA at the following rates per insertion: full page R400, half page R200, quarter page R100. Small advertisements R2 per word. Enquiries should be sent to the editor at [email protected] CONTRIBUTIONS MNASSA mainly serves the Southern African astronomical community. Articles may be submitted by members of this community or by those with strong connections. Else they should deal with matters of direct interest to the community . MNASSA is published on the first day of every second month and articles are due one month before the publication date. RECOGNITION Articles from MNASSA appear in the NASA/ADS data system. Cover picture : While observing dwarf novae in the Large Magellanic Cloud, Petri Vaisanen and Fred Marang captured a set of images through 3 of the Sloan filters (u, g & r).
    [Show full text]