March 2005 Observatory (619) 766-9118 a Non-Profit Educational Association P.O

Total Page:16

File Type:pdf, Size:1020Kb

March 2005 Observatory (619) 766-9118 a Non-Profit Educational Association P.O San Diego Astronomy Association Celebrating Over 40 Years of Astronomical Outreach Office (619) 645-8940 March 2005 Observatory (619) 766-9118 http://www.sdaa.org A Non-Profit Educational Association P.O. Box 23215, San Diego, CA 92193-3215 Combinations Changing at Tierra Del Sol! The combinations for the front gates, pedestrian gate, SDAA Business Meeting power and pump will change on March 13th, the day Next meeting will be held at: SKF Condition Monitoring after the Messier Marathon at Tierra Del Sol. The 5271 Viewridge Court new combination appears on the mailing label of this San Diego, CA 92123 March 8th at 7:00pm newsletter. Volunteers Needed For Beginner Program Next Program Meeting There is a move to start a new Beginner Program within the club. The program would teach people new to astronomy about what’s up there to view, how to find the objects, March 16th 7:00 pm and about the mounts and telescopes to view those objects. We need volunteers to Mission Trails Regional Park make this program happen. If you are interested in helping out with this project and Visitor and Interpretive Center could donate an hour per month of your time, contact Bob Austin at 1 Father Junipero Serra Trail [email protected] or (760) 787-1174 Need to pay your membership dues? Renew your subscription? There are 2 ways. • The easiest way is to go to http://www.sdaa.org and click on the CONTENTS Membership tab on the left. Then scroll down to the bottom and click March 2005 Vol XLI, Issue 03 Renew. This will take you to PayPal. Once you have completed the Published Monthly by the transaction, click the Continue button at the bottom of the screen so San Diego Astronomy Association the Treasurer gets notified of the payment. You will be taken back to 75¢ /$8.00 year the SDAA website. • Incorporated in California in 1963 You can also pay by check made to SDAA (not to a publisher) and mail it to P.O. Box 23215 San Diego, CA 92193-3215. If you are Gate Combinations Changing......................1 renewing a subscription, please include your renewal notice and any Astronomy 101............................................2 envelope the publisher sent you. Calander .....................................................4 Current rates are: • Camp with the Stars .....................................5 Basic Membership $30.00 • Board Minutes ..............................................6 Contributing Membership $50.00 • Treasurer’s Report.......................................6 Astronomy Magazine $29.00 • ASIG ..............................................................7 Sky & Telescope Magazine $32.95 • Sky Watch.......................................................8 Sky Watch $ 5.99 • The Urban Astronomer.............................9 Odyssey Magazine $25.46 • Astronomy Crossword..............................10 Private Pad Lease $35.00 NASA Space Place.....................................12 Please remember, Private Pad Lease fees are due at the same time membership Editors Note................................................13 fees are due. The Back Page...........................................14 SanSan DiegoDiego AstronomyAstronomy AssociationAssociation By Scott Baker Just a little off the top This month’s constellation is Coma Berenices (the hair of Berenices). There are several tales that describe how this constellation came to be, one involving the tail of Leo, but the most famous tale is about a beautiful woman, Berenices, the Queen of Egypt. Berenices, a beautiful woman with extraordinary hair, was married to Ptolemy III, the King of Egypt. Ptolemy had been waging a war, for some time, with the Assyrians, who had killed his sister. When the war was not as ancient as the story would lead as bright. Its companion, almost the nearing its conclusion, Ptolemy was you to believe, but one created and same size and color, circles the star so needed for one last battle. Berenices cataloged by Tycho Brahe (1546- closely, that its separation is measured pleaded with him not to go, but it was 1601). in hundredths of an arc second. If you to no avail, he needed to finish the war. can split this double, at .05 arc Fearing for Ptolemy’s life, Berenices The constellation of Coma Berenices seconds, you better check for a hair prayed to the gods for his safe return, is really unremarkable as far as across your eyepiece! A much more telling them that she would sacrifice prominent stars, containing only a pleasing double, and easy in small her beautiful hair for his safety. The handful of 4th magnitude stars within scopes, is 24 Comae. Much like gods agreed and Ptolemy, victorious its boundaries. However, small and Albireo in Cygnus, 24 Comae is an over the Assyrians, returned home insignificant as it is, it contains no less orange giant of 5th magnitude, which safely. Hearing of his safe return, than eight Messier objects and a HUGE contrasts beautifully with the blue- Berenices cut off her long beautiful number NGC of objects. Within its white 7th magnitude companion. hair and placed it in the temple as borders is a portion of the area known promised. Ptolemy, seeing his wife’s as the Coma-Virgo Supercluster of For open clusters, Coma Berenices has new “do,” was outraged and went to galaxies and galaxies are what you’ll an excellent example, the “Coma Star the temple to retrieve her hair. Upon find here. There are over 2000 Cluster.” Best seen with binoculars, the arriving at the temple he found that her galaxies in the Coma Virgo Superclus- cluster, containing eighty or so stars, hair was missing which only enraged ter, which also encompasses our own covers over five degrees of sky. The him more. Fearing for Berenices life, “Local Group.” cluster was once known as the fuzzy the Greek astronomer Conon of ball of hair at the end of Leo’s tail, until Samos, who was in Egypt at the time, Before we delve into the galaxies it’s the constellations were redrawn by intervened. He told Ptolemy that the famous for, let’s take a look at a few Tycho Brahe, now the cluster forms the Goddess Aphrodite had come and taken other objects first. knot of Berenices hair. the hair into the heavens, where it shown for all to see, and pointed out For double stars, you can try to split, When you were trying to split Diadem, the constellation to Ptolemy. This but I’m sure you won’t succeed, Alpha you may have caught M53 in your field seemed to appease Ptolemy and all Comae. Called Diadem, Alpha Comae, of view. M53, a fine globular cluster, lived happily until the queen’s death in a star much like our own sun, is 62 is the brightest, at magnitude 7.7, of 223BC. Despite the nice tale, the light years away but shines three times the eight Messier objects in Coma. constellation of Coma Berenices is Astro 101 continued on page 3 Page 2 SAN DIEGO ASTRONOMY ASSOCIATION NEWS AND NOTES, MARCH 2005 San Diego Astronomy Association Lying some 65,000 ly away, it takes a Other ID: HIP 61418, SAO 100160 Other ID: NGC4382 larger scope to resolve the mass of stars Magnitude: 5.03 into individual points, but still worth a Equatorial 2000: RA: 12h 35m Object name: NGC 4394 look in any size instrument. A little more 07.758s Dec: +18°22’37.528" Magnitude: 10.9 difficult at 9th magnitude, 1-degree to Flamsteed-Bayer: 24 Comae Berenices Equatorial 2000: RA: 12h 25m 56s Dec: the southwest lays NGC 5053, another Magnitude B: 6.45 +18°12’51" nice, slightly irregular, globular. Magnitude V: 5.11 Size: 3.4 x 3.2 Angular separation: 08°18’11.101" Object type: Spiral Galaxy Now let’s take a look at what Coma is Dreyer description : Pretty bright, little known for, galaxies! We’ll start with Object name: Coma Star Cluster extended, brighter middle. M64, the “Black Eye” Galaxy. It gets its Other ID: SAC Mel 111 nick name of “Black Eye” from the large Equatorial 2000: RA: 12h 25m 00s Dec: Object name: M 88 obscuring dust cloud at the core of the +26°00’00" Magnitude: 9.4 galaxy, giving it the impression of Size: 275.0 x 275.0 Equatorial 2000: RA: 12h 31m 59s Dec: having a “black eye.” The dust cloud is Object type: Open Cluster +14°25’11" only visible with large scopes under Notes: Coma Berenices star cluster Size: 6.8 x 3.7 ideal conditions; however, the galaxy is Number of Stars: 80 Object type: Spiral Galaxy still a nice compact spiral in smaller Other ID: NGC4501 scopes. M85 and M88 are both fairly Object name: M 53 bright spiral galaxies, with M88 showing Magnitude: 7.7 Object name: M 91 multiple spiral arms under good Equatorial 2000: RA: 13h 12m 55s Dec: Magnitude: 10.1 conditions. While looking at M85, try +18°10’11" Equatorial 2000: RA: 12h 35m 26s Dec: and glimpse the fainter NGC4394 in the Size: 13.0 x 13.0 +14°29’47" same field. M91, M98, M99 and M100 Object type: Globular Cluster Size: 5.2 x 4.2 are all nice galaxies of varying sizes and Other ID: NGC4548 types which deserve more space than Object name: NGC 5053 we have in this newsletter. With so Magnitude: 9.0 Object name: M 98 many galaxies in this area, you wonder Equatorial 2000: RA: 13h 16m 27s Dec: Magnitude: 10.1 why Messier, picked these to put on his +17°41’55" Equatorial 2000: RA: 12h 13m 48s Dec: list, when it could have been so easy to Size: 10.0 x 10.0 +14°53’58" create his list of 110 objects in this area Object type: Globular Cluster Size: 9.8 x 2.8 of the sky alone. Dreyer description : Cluster, very faint, Object type: Spiral Galaxy pretty large, irregularly round, very Other ID: NGC4192 Coma Berenices has a wealth of objects, gradually brighter middle, stars of especially on its southern border with magnitude 15.
Recommended publications
  • Mathématiques Et Espace
    Atelier disciplinaire AD 5 Mathématiques et Espace Anne-Cécile DHERS, Education Nationale (mathématiques) Peggy THILLET, Education Nationale (mathématiques) Yann BARSAMIAN, Education Nationale (mathématiques) Olivier BONNETON, Sciences - U (mathématiques) Cahier d'activités Activité 1 : L'HORIZON TERRESTRE ET SPATIAL Activité 2 : DENOMBREMENT D'ETOILES DANS LE CIEL ET L'UNIVERS Activité 3 : D'HIPPARCOS A BENFORD Activité 4 : OBSERVATION STATISTIQUE DES CRATERES LUNAIRES Activité 5 : DIAMETRE DES CRATERES D'IMPACT Activité 6 : LOI DE TITIUS-BODE Activité 7 : MODELISER UNE CONSTELLATION EN 3D Crédits photo : NASA / CNES L'HORIZON TERRESTRE ET SPATIAL (3 ème / 2 nde ) __________________________________________________ OBJECTIF : Détermination de la ligne d'horizon à une altitude donnée. COMPETENCES : ● Utilisation du théorème de Pythagore ● Utilisation de Google Earth pour évaluer des distances à vol d'oiseau ● Recherche personnelle de données REALISATION : Il s'agit ici de mettre en application le théorème de Pythagore mais avec une vision terrestre dans un premier temps suite à un questionnement de l'élève puis dans un second temps de réutiliser la même démarche dans le cadre spatial de la visibilité d'un satellite. Fiche élève ____________________________________________________________________________ 1. Victor Hugo a écrit dans Les Châtiments : "Les horizons aux horizons succèdent […] : on avance toujours, on n’arrive jamais ". Face à la mer, vous voyez l'horizon à perte de vue. Mais "est-ce loin, l'horizon ?". D'après toi, jusqu'à quelle distance peux-tu voir si le temps est clair ? Réponse 1 : " Sans instrument, je peux voir jusqu'à .................. km " Réponse 2 : " Avec une paire de jumelles, je peux voir jusqu'à ............... km " 2. Nous allons maintenant calculer à l'aide du théorème de Pythagore la ligne d'horizon pour une hauteur H donnée.
    [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]
  • The Puzzling Nature of Dwarf-Sized Gas Poor Disk Galaxies
    Dissertation submitted to the Department of Physics Combined Faculties of the Astronomy Division Natural Sciences and Mathematics University of Oulu Ruperto-Carola-University Oulu, Finland Heidelberg, Germany for the degree of Doctor of Natural Sciences Put forward by Joachim Janz born in: Heidelberg, Germany Public defense: January 25, 2013 in Oulu, Finland THE PUZZLING NATURE OF DWARF-SIZED GAS POOR DISK GALAXIES Preliminary examiners: Pekka Heinämäki Helmut Jerjen Opponent: Laura Ferrarese Joachim Janz: The puzzling nature of dwarf-sized gas poor disk galaxies, c 2012 advisors: Dr. Eija Laurikainen Dr. Thorsten Lisker Prof. Heikki Salo Oulu, 2012 ABSTRACT Early-type dwarf galaxies were originally described as elliptical feature-less galax- ies. However, later disk signatures were revealed in some of them. In fact, it is still disputed whether they follow photometric scaling relations similar to giant elliptical galaxies or whether they are rather formed in transformations of late- type galaxies induced by the galaxy cluster environment. The early-type dwarf galaxies are the most abundant galaxy type in clusters, and their low-mass make them susceptible to processes that let galaxies evolve. Therefore, they are well- suited as probes of galaxy evolution. In this thesis we explore possible relationships and evolutionary links of early- type dwarfs to other galaxy types. We observed a sample of 121 galaxies and obtained deep near-infrared images. For analyzing the morphology of these galaxies, we apply two-dimensional multicomponent fitting to the data. This is done for the first time for a large sample of early-type dwarfs. A large fraction of the galaxies is shown to have complex multicomponent structures.
    [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]
  • The Dynamical State of the Coma Cluster with XMM-Newton?
    A&A 400, 811–821 (2003) Astronomy DOI: 10.1051/0004-6361:20021911 & c ESO 2003 Astrophysics The dynamical state of the Coma cluster with XMM-Newton? D. M. Neumann1,D.H.Lumb2,G.W.Pratt1, and U. G. Briel3 1 CEA/DSM/DAPNIA Saclay, Service d’Astrophysique, L’Orme des Merisiers, Bˆat. 709, 91191 Gif-sur-Yvette, France 2 Science Payloads Technology Division, Research and Science Support Dept., ESTEC, Postbus 299 Keplerlaan 1, 2200AG Noordwijk, The Netherlands 3 Max-Planck Institut f¨ur extraterrestrische Physik, Giessenbachstr., 85740 Garching, Germany Received 19 June 2002 / Accepted 13 December 2002 Abstract. We present in this paper a substructure and spectroimaging study of the Coma cluster of galaxies based on XMM- Newton data. XMM-Newton performed a mosaic of observations of Coma to ensure a large coverage of the cluster. We add the different pointings together and fit elliptical beta-models to the data. We subtract the cluster models from the data and look for residuals, which can be interpreted as substructure. We find several significant structures: the well-known subgroup connected to NGC 4839 in the South-West of the cluster, and another substructure located between NGC 4839 and the centre of the Coma cluster. Constructing a hardness ratio image, which can be used as a temperature map, we see that in front of this new structure the temperature is significantly increased (higher or equal 10 keV). We interpret this temperature enhancement as the result of heating as this structure falls onto the Coma cluster. We furthermore reconfirm the filament-like structure South-East of the cluster centre.
    [Show full text]
  • And Ecclesiastical Cosmology
    GSJ: VOLUME 6, ISSUE 3, MARCH 2018 101 GSJ: Volume 6, Issue 3, March 2018, Online: ISSN 2320-9186 www.globalscientificjournal.com DEMOLITION HUBBLE'S LAW, BIG BANG THE BASIS OF "MODERN" AND ECCLESIASTICAL COSMOLOGY Author: Weitter Duckss (Slavko Sedic) Zadar Croatia Pусскй Croatian „If two objects are represented by ball bearings and space-time by the stretching of a rubber sheet, the Doppler effect is caused by the rolling of ball bearings over the rubber sheet in order to achieve a particular motion. A cosmological red shift occurs when ball bearings get stuck on the sheet, which is stretched.“ Wikipedia OK, let's check that on our local group of galaxies (the table from my article „Where did the blue spectral shift inside the universe come from?“) galaxies, local groups Redshift km/s Blueshift km/s Sextans B (4.44 ± 0.23 Mly) 300 ± 0 Sextans A 324 ± 2 NGC 3109 403 ± 1 Tucana Dwarf 130 ± ? Leo I 285 ± 2 NGC 6822 -57 ± 2 Andromeda Galaxy -301 ± 1 Leo II (about 690,000 ly) 79 ± 1 Phoenix Dwarf 60 ± 30 SagDIG -79 ± 1 Aquarius Dwarf -141 ± 2 Wolf–Lundmark–Melotte -122 ± 2 Pisces Dwarf -287 ± 0 Antlia Dwarf 362 ± 0 Leo A 0.000067 (z) Pegasus Dwarf Spheroidal -354 ± 3 IC 10 -348 ± 1 NGC 185 -202 ± 3 Canes Venatici I ~ 31 GSJ© 2018 www.globalscientificjournal.com GSJ: VOLUME 6, ISSUE 3, MARCH 2018 102 Andromeda III -351 ± 9 Andromeda II -188 ± 3 Triangulum Galaxy -179 ± 3 Messier 110 -241 ± 3 NGC 147 (2.53 ± 0.11 Mly) -193 ± 3 Small Magellanic Cloud 0.000527 Large Magellanic Cloud - - M32 -200 ± 6 NGC 205 -241 ± 3 IC 1613 -234 ± 1 Carina Dwarf 230 ± 60 Sextans Dwarf 224 ± 2 Ursa Minor Dwarf (200 ± 30 kly) -247 ± 1 Draco Dwarf -292 ± 21 Cassiopeia Dwarf -307 ± 2 Ursa Major II Dwarf - 116 Leo IV 130 Leo V ( 585 kly) 173 Leo T -60 Bootes II -120 Pegasus Dwarf -183 ± 0 Sculptor Dwarf 110 ± 1 Etc.
    [Show full text]
  • Sky Notes: 2011 April & May
    Sky Notes: 2011 April & May by Callum Potter Spring is one of my favourite times of year occultation of 87 Leo, another 4th mag star. RZ Cassiopeiae has many through the two to observe. Although the nights are starting a The Sun is certainly worth following, as months, and these are detailed in your BAA bit later, the slightly warmer weather makes activity seems to be on the increase. In recent Handbook. Des Loughney wrote an excel- visual observing much more comfortable. months there has been much speculation about lent paper on the technique in the June 2010 As I was researching these Sky Notes, the aurorae being visible from the south of the Journal, and there is another good article in dearth of planets to observe was quite sur- UK. But for such a ‘mid-latitude’ aurora to be the 2011 April Sky & Telescope (in which prising. Only Saturn is well positioned, and visible requires quite a major coronal mass Des gets a mention too). Bright variable stars I started to wonder how often the absence of ejection to hit us ‘face-on’. It is worth signing are probably under-observed, so if you do many of the planets arises. No doubt some- up to alert services though, and you can now make some observations, please send your one with a more ‘computing’ orientation follow @aurorawatchuk on Twitter which will results to the Variable Star Section. could tell, but in my recollection it’s quite a automatically post alerts when their rare event. So, without many of the planets magnetometers indicate a significant distur- around, I thought I would mention a few bance to the Earth’s magnetic field.
    [Show full text]
  • The Brightest Stars Seite 1 Von 9
    The Brightest Stars Seite 1 von 9 The Brightest Stars This is a list of the 300 brightest stars made using data from the Hipparcos catalogue. The stellar distances are only fairly accurate for stars well within 1000 light years. 1 2 3 4 5 6 7 8 9 10 11 12 13 No. Star Names Equatorial Galactic Spectral Vis Abs Prllx Err Dist Coordinates Coordinates Type Mag Mag ly RA Dec l° b° 1. Alpha Canis Majoris Sirius 06 45 -16.7 227.2 -8.9 A1V -1.44 1.45 379.21 1.58 9 2. Alpha Carinae Canopus 06 24 -52.7 261.2 -25.3 F0Ib -0.62 -5.53 10.43 0.53 310 3. Alpha Centauri Rigil Kentaurus 14 40 -60.8 315.8 -0.7 G2V+K1V -0.27 4.08 742.12 1.40 4 4. Alpha Boötis Arcturus 14 16 +19.2 15.2 +69.0 K2III -0.05 -0.31 88.85 0.74 37 5. Alpha Lyrae Vega 18 37 +38.8 67.5 +19.2 A0V 0.03 0.58 128.93 0.55 25 6. Alpha Aurigae Capella 05 17 +46.0 162.6 +4.6 G5III+G0III 0.08 -0.48 77.29 0.89 42 7. Beta Orionis Rigel 05 15 -8.2 209.3 -25.1 B8Ia 0.18 -6.69 4.22 0.81 770 8. Alpha Canis Minoris Procyon 07 39 +5.2 213.7 +13.0 F5IV-V 0.40 2.68 285.93 0.88 11 9. Alpha Eridani Achernar 01 38 -57.2 290.7 -58.8 B3V 0.45 -2.77 22.68 0.57 144 10.
    [Show full text]
  • A Search For" Dwarf" Seyfert Nuclei. VII. a Catalog of Central Stellar
    TO APPEAR IN The Astrophysical Journal Supplement Series. Preprint typeset using LATEX style emulateapj v. 26/01/00 A SEARCH FOR “DWARF” SEYFERT NUCLEI. VII. A CATALOG OF CENTRAL STELLAR VELOCITY DISPERSIONS OF NEARBY GALAXIES LUIS C. HO The Observatories of the Carnegie Institution of Washington, 813 Santa Barbara St., Pasadena, CA 91101 JENNY E. GREENE1 Department of Astrophysical Sciences, Princeton University, Princeton, NJ ALEXEI V. FILIPPENKO Department of Astronomy, University of California, Berkeley, CA 94720-3411 AND WALLACE L. W. SARGENT Palomar Observatory, California Institute of Technology, MS 105-24, Pasadena, CA 91125 To appear in The Astrophysical Journal Supplement Series. ABSTRACT We present new central stellar velocity dispersion measurements for 428 galaxies in the Palomar spectroscopic survey of bright, northern galaxies. Of these, 142 have no previously published measurements, most being rela- −1 tively late-type systems with low velocity dispersions (∼<100kms ). We provide updates to a number of literature dispersions with large uncertainties. Our measurements are based on a direct pixel-fitting technique that can ac- commodate composite stellar populations by calculating an optimal linear combination of input stellar templates. The original Palomar survey data were taken under conditions that are not ideally suited for deriving stellar veloc- ity dispersions for galaxies with a wide range of Hubble types. We describe an effective strategy to circumvent this complication and demonstrate that we can still obtain reliable velocity dispersions for this sample of well-studied nearby galaxies. Subject headings: galaxies: active — galaxies: kinematics and dynamics — galaxies: nuclei — galaxies: Seyfert — galaxies: starburst — surveys 1. INTRODUCTION tors, apertures, observing strategies, and analysis techniques.
    [Show full text]
  • Observing the Night Sky I
    29:50 Astronomy Lab – Evening Sections Stars, Galaxies, and the Universe Fall 2010 Name Date /10 Grade OBSERVING THE NIGHT SKY I INTRODUCTION In this session we will observe the night sky. The idea is to fix some of the concepts discussed in class, such as the celestial coordinate system. However, the main point is to see the night sky and notice some of the properties of stars and some other astronomical objects such as star clusters and galaxies. This will make them seem more real as we discuss them throughout the semester. Part of the activity will consist of finding stars, constellations, or other astronomical objects. To show that you have found an object, you point it out to a teaching assistant or other observer, who will then “sign‐off” on it for you. In going through these exercises, you will have a chance to use the Sky and Telescope star wheel, the SC1 constellation chart, and the Sky and Telescope Pocket Star Atlas. You may also want to use the interactive sky chart on the Sky and Telescope website: www.skyandtelescope.com. In using the pocket star atlas, you will need a pair of binoculars to see objects fainter than the naked eye limit. Also, be sure and notice where the various constellations are in the sky (i.e. constellation X is low in the northwest, constellation Y is about halfway up the eastern sky). 1 OBSERVING EXERCISES 1. Get yourself oriented so you know where N, S, E and W are. Find the Q1 bright star Arcturus, in the constellation of Bootes, and point it out to your TA.
    [Show full text]
  • Three Naked Eye Galaxies? Dave Eagle
    Three Naked Eye Galaxies? Dave Eagle. Eagleseye Observatory. Star hopping to M31, The Great Andromeda Galaxy. In the autumn sky in the northern hemisphere, the constellations of Perseus and Andromeda are very proudly on display, located on the meridian around midnight, and visible from most of the world. The Great Square of Pegasus is a distinct asterism of four stars. Using just your naked eye, find this square of stars. Incidentally, the top left star (all instructions are now as seen from the northern hemisphere) Sirrah, is now actually Alpha Andromedae. From this square of stars take the top edge of the square and carry the line on towards the left (east) and up. Just under half the distance of the top of the square, you should come to another reasonably bright star. Slightly left and up again, taking a slightly longer journey, you will come to another star of similar brightness. This is Mirach or Beta Andromedae. When you have found this star, turn 90 degrees to the right. You will then see two fairly bright stars leading away. Aim for the second star and gaze at this star. If your skies are reasonably dark, just above and to the right of the second star you should be able to see a faint smudge. This marks the location of M31, The Andromeda Galaxy. In five hops we have found our quarry. Figure 1 – Star hopping from Sirrah to The Andromeda Galaxy. This is the most distant object you can see with the naked eye and is almost 2.5 million light years away.
    [Show full text]
  • The Skyscraper 2009 05.Indd
    THE SKYSCRAPER • MAY 2009 A Better Galaxy Guide: Part 2, Late Spring Craig Cortis Those of you who enjoyed my first field eyepieces. the brighter objects listed and use what installment on this subject (in last Many of my choices here can be you’ve got. In closing, you might find month’s issue) will, I hope, find this seen in a 4-inch telescope and some it advisable to take another look at my second part to be even better. Three are doable in 50mm or larger binocu- article in last month’s issue. The intro- constellations are covered on the lars, but in general, I’d suggest using ductory section explains why I chose accompanying list of recommended telescopes of 6-to-8 inch aperture, at to come up with these observing lists objects and two—Virgo and Coma least for the galaxies. If you don’t own and also how they are planned. I hope Berenices-feature the grandest, richest a scope of that size range, just pick-out you’ll find my notes useful for star- assortment of galaxies bright enough to be seen in small-to-medium aperture Object Type R.A. Dec. Mag. Size Burnham’s instruments of all constellations in the sky, period. This “Virgo-Coma” cluster Virgo of galaxies is so crowded with objects M61 Sp Gx 12h 21.9m +04° 28’ 9.7 6.0x5.6’ v3, p. 2089-91 that trying to “zero-in” on only the best *M84 El Gx 12h 25.1m +12° 53’ 9.2 5.1x4.3’ v3, p.
    [Show full text]