The Evening Sky Map 29 = UT – 4 Hours.) Time Eastern Summer (UT)

Total Page:16

File Type:pdf, Size:1020Kb

The Evening Sky Map 29 = UT – 4 Hours.) Time Eastern Summer (UT) I N E D R I A C A S T N E O D I T A C L E O R N I G D S T S H A E P H M O O R C I . Z N O a r o e u t a n t d o r O t N h o e t Z r N a o I e C r p t h R p I a C R O s e r l C e a H t s L s t i E E , a s l e H ( P d T F o u O l t e i D t R NORTH ( a N N M l E C A n X P O r ) A e H . h C M T t . I r P o N S L n E E P Z m “ o E NORTHERN HEMISPHERE A N r H F O M T R LYNX T Y N H E ” K E ) W S . T Capella T E U W B R N The Evening Sky Map W D E T T SEPTEMBER 2008 WH A E C T FREE* EACH MONTH FOR YOU TO EXPLORE, LEARN & ENJOY THE NIGHT SKY O h S L e K Y E CAMELOPARDALIS b R r M i A g A SKY MAP SHOWS HOW h S P RSA MAJOR RSA t T U C A s t E R a . Sky Calendar – September 2008 J O r r THE NIGHT SKY LOOKS B s a U t O o N S f L D h C A NE t I I a r EARLY SEPT 9 PM T T s o M81 S s 1 Moon near Venus at 16h UT (23° from Sun, evening sky). Mag. –3.8. S N i E NW C o L e E p “ E h T N e LATE SEPT 8 PM O M82 C t i T P a , . O 1 Moon near Mercury at 21h UT (evening sky). Mag. +0.0. E (Add 1 Hour For Daylight Saving) s L N R PERSEUS i A f r R o O I a ( r S SKY MAP DRAWN FOR Z l ” m J I T o U H R 2 Moon near Mars at 3h UT (evening sky). Mag. +1.7. P E a S A LATITUDE OF 40° O N T d W O H R n A Dipper T - i NORTH AND IS E H f S s Algol h H S The Big The 3 Moon near Spica at 8h UT (evening sky). T Y o T a A M94 SUITABLE FOR t O R p CANES VENATICI S U ) e I h Cluster LATITUDES UP t A 4 Saturn at conjunction with Sun at 1h UT (not visible). E g h Double L Polaris R u a C TO 15° NORTH E o t & Alcor & l NCP R Mizar D Caroli I P MINOR Saturn passes into the morning sky. i Cor s OR SOUTH C O r M51 URSA e I o R N a CASSIOPEIA ( OF THIS Thuban E M64 s G r 7 Moon very near Antares at 3h UT (evening sky). T y e U N p t CEPHEUS O O o γ p i Dipper W Occultation visible from western South America, E r D ANDROMEDA e ) H Little c T g S o i Australia and New Zealand. O g D B η M3 n N ARIES T e β DRACO i H A z h e t E ) 7 Mercury 2.5° from Mars at 4h UT (27° from Sun, E . Hamal H e C C s T O I L M33 U evening sky). Mags. +0.1 and +1.7. M I N M31 P P E A Z ( S T δ 7 First Quarter Moon at 14:04 UT. S I D γ C ν D μ A Arcturus T I E ε h R H 7 Moon at apogee (farthest from Earth) at 15h UT e E R C E a in T n V (distance 404,214 km; angular size 29.6'). I c O O i N e Etam Y a M39 92 n L Deneb T M BOÖTES T t 9 Moon near Jupiter at 21h UT (evening sky). Mag. –2.5. H C c PISCES A E M13 o T R R CORONA Gemm n I EAST BOREALIS A s 10 Mercury, Venus, and Mars within 3.6° diameter Square Great D t P of Pegasus of ε e P CYGNUS Y Vega l E l K 61 circle at 8h UT (26° from Sun, evening sky). a A S t R i E o S WEST n β H Mags. +0.2, –3.8, and +1.7. A T o L LYRA F f . O M57 χ O ” N A 11 Mercury at greatest elongation, 27° east from s q T G Summer Triangle Albireo d u R PEGASUS HERCULES o T a A g Sun (evening sky) at 4h UT. Mag. +0.2. H r M27 VIRGO P i E e u E s M5 h B t H α SERPENS (CAPUT) r 12 Venus 0.30° from Mars at 2h UT (26° from Sun, O 9 T f e 9 T o p S T Cr 3 r I O Circlet evening sky). Mags. –3.9 and +1.7. e γ d M s a P e o M1 DELPHINUS A O n r 5 “ M F t Enif 15 Full Moon at 9:13 UT. The full Moon of September s e E T a h H IC 4665 H Altair t T E y is called the “Fruit Moon”. It is also called the CETUS s o F M AQUARIUS 6633 a u O A n t M12 i “Harvest Moon”. P g R OPHIUCHUS d E I m e T S M2 M10 i a N LIBRA f T n η i E 19 Venus 2.4° from Spica at 6h UT (evening sky). SERPENS t H C p (CAUDA) n E AQUILA e E o d H S u i A T 20 Moon at perigee (closest to Earth) at 3h UT (368,886 r Diphda M i s . n M11 t E g e S E A o km; 32.4'). w p M S a I t 7009 M16 t T T e β n H r e D i 22 Last Quarter Moon at 5:04 UT. E f c N r A D o 7 n I m M1 A S R CAPRICORNUS . E 22 September equinox at 15:44 UT. The time when the Sun E a 7293 y T C M23 k A T ja M25 21 s s D I r Jupiter M O M20 e N Symbols reaches the point along the ecliptic where it crosses into the N in h I t A T to Antare s T H Fomalhaut Nunki M22 M8 M4 s R southern celestial hemisphere marking the start of autumn in the A th ro E Galaxy T e c C Y AUSTRINUSPISCIS a O m s N Northern Hemisphere and spring in the Southern Hemisphere. U o SE The e O u Teapot h S Double Star F t c R A h SW t A C re E E of t P 23 Mercury 2.1° from Spica at 22h UT (22° from Sun, evening sky). SAGITTARIUS s P Variable Star B a M6 y A E la SCORPIUS a T G r W I 24 Moon near Beehive cluster (M44) at 23h UT (morning sky). IN ge y S Diffuse Nebula B f M7 ilk A Y is M N U h, e O S P h IZ Planetary Nebula 29 New Moon at 8:12 UT. Start of lunation 1061. IN is CORONA T R G ci O T s -H H Au GRUS AUSTRALIS O Open Star Cluster E st -T All times in Universal Time (UT). (USA Eastern Summer Time = UT – 4 hours.) SK rin ON Y us IZ MA . OR Globular Star Cluster P T H O OM FIN FR SAVE ON RECOMMENDED PRODUCTS • http://Skymaps.com/store D The KY A B Sum . T S RIG me SOUTH ead IGH Star Magnitudes HT r Tria verh E N -101234 • Star Atlases & Planispheres • Star Charts & Astro Posters STA ngle stars o TIR R PA – Vega, bright E EN • Books for Sky Watchers • 2009 Astronomy Calendars TTER Altair, and Deneb – three S TH Copyright © 2000–2008 Kym Thalassoudis. All Rights Reserved. N IN SHOW THE SKY KY MAP All sales support the production and free distribution of The Evening Sky Map. INSTRUCTIONS: THE S * TERMS OF USE: FREE FOR NON-COMMERCIAL EDUCATIONAL USE. ASTRONOMY EDUCATION GROUPS MAY FREELY DISTRIBUTE PRINTED HANDOUTS. FULL DETAILS AT http://Skymaps.com/terms.html About the Celestial Objects Easily Seen with the Naked Eye Listed on this page are several of the brighter, more interesting celestial objects Altair Aql Brightest star in Aquila. Name means "the flying eagle". Dist=16.7 ly. visible in the evening sky this month (refer to the monthly sky map). The objects are Capella Aur The 6th brightest star. Appears yellowish in color. Spectroscopic binary. Dist=42 ly. Arcturus Boo Orange, giant K star. Name means "bear watcher". Dist=36.7 ly. grouped into three categories. Those that can be easily seen with the naked eye (that δ Cephei Cep Cepheid prototype.
Recommended publications
  • KELT-14B and KELT-15B: an Independent Discovery of WASP-122B and a New Hot Jupiter
    Swarthmore College Works Physics & Astronomy Faculty Works Physics & Astronomy 5-11-2016 KELT-14b And KELT-15b: An Independent Discovery Of WASP-122b And A New Hot Jupiter J. E. Rodriguez K. D. Colón K. G. Stassun D. Wright P. A. Cargile See next page for additional authors Follow this and additional works at: https://works.swarthmore.edu/fac-physics Part of the Astrophysics and Astronomy Commons Let us know how access to these works benefits ouy Recommended Citation J. E. Rodriguez, K. D. Colón, K. G. Stassun, D. Wright, P. A. Cargile, D. Bayliss, J. Pepper, K. A. Collins, R. B. Kuhn, M. B. Lund, R. J. Siverd, G. Zhou, B. S. Gaudi, C. G. Tinney, K. Penev, T. G. Tan, C. Stockdale, I. A. Curtis, D. James, S. Udry, D. Segransan, A. Bieryla, D. W. Latham, T. G. Beatty, J. D. Eastman, G. Myers, J. Bartz, J. Bento, Eric L.N. Jensen, T. E. Oberst, and D. J. Stevens. (2016). "KELT-14b And KELT-15b: An Independent Discovery Of WASP-122b And A New Hot Jupiter". Astronomical Journal. Volume 151, Issue 6. 138 DOI: 10.3847/0004-6256/151/6/138 https://works.swarthmore.edu/fac-physics/286 This work is brought to you for free by Swarthmore College Libraries' Works. It has been accepted for inclusion in Physics & Astronomy Faculty Works by an authorized administrator of Works. For more information, please contact [email protected]. Authors J. E. Rodriguez, K. D. Colón, K. G. Stassun, D. Wright, P. A. Cargile, D. Bayliss, J. Pepper, K. A. Collins, R.
    [Show full text]
  • The Evening Sky Map a DECEMBER 2018 N
    I N E D R I A C A S T N E O D I T A C L E O R N I G D S T S H A E P H M O O R C I . Z N O n i f d o P t o ) l a h O N r g i u s , o Z l t P h I C e r o N R ( I o r R r O e t p h C H p i L S t D E E a g r i . H ( B T F e O h T NORTH D R t h N e M e E s A G X O U e A H m M C T i . I n P i N d S L E E m P Z “ e E A N Dipper t e H O NORTHERN HEMISPHERE o M T R r T The Big The N Y s H h . E r o ” E K Alcor & e w ) t W S . s e . T u r T Mizar l E U p W C B e R e a N l W D k b E s T u T MAJOR W H o o The Evening Sky Map A DECEMBER 2018 n E C D O t FREE* EACH MONTH FOR YOU TO EXPLORE, LEARN & ENJOY THE NIGHT SKY URSA S e L h K h e t Y E m R d M A n o A a r Thuban S SKY MAP SHOWS HOW P Get Sky Calendar on Twitter n T 1 i n C A 3 E g R M J http://twitter.com/skymaps O Sky Calendar – December 2018 o d B THE NIGHT SKY LOOKS U M13 f n O N i D “ f L D e T DRACO A o c NE O I t I e T EARLY DEC PM T 8 m P t S i 3 Moon near Spica (morning sky) at 9h UT.
    [Show full text]
  • Star Clusters
    Star Clusters • Eventually, photons and stellar winds clear out the remaining gas and dust and leave behind the stars. • Reflection nebulae provide evidence for remaining dust on the far side of the Pleiades Star Clusters • It may be that all stars are born in clusters. • A good question is therefore why are most stars we see in the Galaxy not members of obvious clusters? • The answer is that the majority of newly-formed clusters are very weakly gravitationally bound. Perturbations from passing molecular clouds, spiral arms or mass loss from the cluster stars `unbind’ most clusters. Star Cluster Ages • We can use the H-R Diagram of the stars in a cluster to determine the age of the cluster. • A cluster starts off with stars along the full main sequence. • Because stars with larger mass evolve more quickly, the hot, luminous end of the main sequence becomes depleted with time. • The `main-sequence turnoff’ moves to progressively lower mass, L and T with time. • Young clusters contain short-lived, massive stars in their main sequence • Other clusters are missing the high-mass MSTO stars and we can infer the cluster age is the main-sequence lifetime of the highest mass star still on the main- sequence. 25Mo 3million years 104 3Mo 500Myrs 102 1M 10Gyr L o 1 0.5Mo 200Gyr 10-2 30000 15000 7500 3750 Temperature Star Clusters Sidetrip • There are two basic types of clusters in the Galaxy. • Globular Clusters are mostly in the halo of the Galaxy, contain >100,000 stars and are very ancient. • Open clusters are in the disk, contain between several and a few thousand stars and range in age from 0 to 10Gyr Galaxy Ages • Deriving galaxy ages is much harder because most galaxies have a star formation history rather than a single-age population of stars.
    [Show full text]
  • Introduction to Astronomy from Darkness to Blazing Glory
    Introduction to Astronomy From Darkness to Blazing Glory Published by JAS Educational Publications Copyright Pending 2010 JAS Educational Publications All rights reserved. Including the right of reproduction in whole or in part in any form. Second Edition Author: Jeffrey Wright Scott Photographs and Diagrams: Credit NASA, Jet Propulsion Laboratory, USGS, NOAA, Aames Research Center JAS Educational Publications 2601 Oakdale Road, H2 P.O. Box 197 Modesto California 95355 1-888-586-6252 Website: http://.Introastro.com Printing by Minuteman Press, Berkley, California ISBN 978-0-9827200-0-4 1 Introduction to Astronomy From Darkness to Blazing Glory The moon Titan is in the forefront with the moon Tethys behind it. These are two of many of Saturn’s moons Credit: Cassini Imaging Team, ISS, JPL, ESA, NASA 2 Introduction to Astronomy Contents in Brief Chapter 1: Astronomy Basics: Pages 1 – 6 Workbook Pages 1 - 2 Chapter 2: Time: Pages 7 - 10 Workbook Pages 3 - 4 Chapter 3: Solar System Overview: Pages 11 - 14 Workbook Pages 5 - 8 Chapter 4: Our Sun: Pages 15 - 20 Workbook Pages 9 - 16 Chapter 5: The Terrestrial Planets: Page 21 - 39 Workbook Pages 17 - 36 Mercury: Pages 22 - 23 Venus: Pages 24 - 25 Earth: Pages 25 - 34 Mars: Pages 34 - 39 Chapter 6: Outer, Dwarf and Exoplanets Pages: 41-54 Workbook Pages 37 - 48 Jupiter: Pages 41 - 42 Saturn: Pages 42 - 44 Uranus: Pages 44 - 45 Neptune: Pages 45 - 46 Dwarf Planets, Plutoids and Exoplanets: Pages 47 -54 3 Chapter 7: The Moons: Pages: 55 - 66 Workbook Pages 49 - 56 Chapter 8: Rocks and Ice:
    [Show full text]
  • The Mathematics of the Chinese, Indian, Islamic and Gregorian Calendars
    Heavenly Mathematics: The Mathematics of the Chinese, Indian, Islamic and Gregorian Calendars Helmer Aslaksen Department of Mathematics National University of Singapore [email protected] www.math.nus.edu.sg/aslaksen/ www.chinesecalendar.net 1 Public Holidays There are 11 public holidays in Singapore. Three of them are secular. 1. New Year’s Day 2. Labour Day 3. National Day The remaining eight cultural, racial or reli- gious holidays consist of two Chinese, two Muslim, two Indian and two Christian. 2 Cultural, Racial or Religious Holidays 1. Chinese New Year and day after 2. Good Friday 3. Vesak Day 4. Deepavali 5. Christmas Day 6. Hari Raya Puasa 7. Hari Raya Haji Listed in order, except for the Muslim hol- idays, which can occur anytime during the year. Christmas Day falls on a fixed date, but all the others move. 3 A Quick Course in Astronomy The Earth revolves counterclockwise around the Sun in an elliptical orbit. The Earth ro- tates counterclockwise around an axis that is tilted 23.5 degrees. March equinox June December solstice solstice September equinox E E N S N S W W June equi Dec June equi Dec sol sol sol sol Beijing Singapore In the northern hemisphere, the day will be longest at the June solstice and shortest at the December solstice. At the two equinoxes day and night will be equally long. The equi- noxes and solstices are called the seasonal markers. 4 The Year The tropical year (or solar year) is the time from one March equinox to the next. The mean value is 365.2422 days.
    [Show full text]
  • The Basques of Lapurdi, Zuberoa, and Lower Navarre Their History and Their Traditions
    Center for Basque Studies Basque Classics Series, No. 6 The Basques of Lapurdi, Zuberoa, and Lower Navarre Their History and Their Traditions by Philippe Veyrin Translated by Andrew Brown Center for Basque Studies University of Nevada, Reno Reno, Nevada This book was published with generous financial support obtained by the Association of Friends of the Center for Basque Studies from the Provincial Government of Bizkaia. Basque Classics Series, No. 6 Series Editors: William A. Douglass, Gregorio Monreal, and Pello Salaburu Center for Basque Studies University of Nevada, Reno Reno, Nevada 89557 http://basque.unr.edu Copyright © 2011 by the Center for Basque Studies All rights reserved. Printed in the United States of America Cover and series design © 2011 by Jose Luis Agote Cover illustration: Xiberoko maskaradak (Maskaradak of Zuberoa), drawing by Paul-Adolph Kaufman, 1906 Library of Congress Cataloging-in-Publication Data Veyrin, Philippe, 1900-1962. [Basques de Labourd, de Soule et de Basse Navarre. English] The Basques of Lapurdi, Zuberoa, and Lower Navarre : their history and their traditions / by Philippe Veyrin ; with an introduction by Sandra Ott ; translated by Andrew Brown. p. cm. Translation of: Les Basques, de Labourd, de Soule et de Basse Navarre Includes bibliographical references and index. Summary: “Classic book on the Basques of Iparralde (French Basque Country) originally published in 1942, treating Basque history and culture in the region”--Provided by publisher. ISBN 978-1-877802-99-7 (hardcover) 1. Pays Basque (France)--Description and travel. 2. Pays Basque (France)-- History. I. Title. DC611.B313V513 2011 944’.716--dc22 2011001810 Contents List of Illustrations..................................................... vii Note on Basque Orthography.........................................
    [Show full text]
  • The Midnight Sky: Familiar Notes on the Stars and Planets, Edward Durkin, July 15, 1869 a Good Way to Start – Find North
    The expression "dog days" refers to the period from July 3 through Aug. 11 when our brightest night star, SIRIUS (aka the dog star), rises in conjunction* with the sun. Conjunction, in astronomy, is defined as the apparent meeting or passing of two celestial bodies. TAAS Fabulous Fifty A program for those new to astronomy Friday Evening, July 20, 2018, 8:00 pm All TAAS and other new and not so new astronomers are welcome. What is the TAAS Fabulous 50 Program? It is a set of 4 meetings spread across a calendar year in which a beginner to astronomy learns to locate 50 of the most prominent night sky objects visible to the naked eye. These include stars, constellations, asterisms, and Messier objects. Methodology 1. Meeting dates for each season in year 2018 Winter Jan 19 Spring Apr 20 Summer Jul 20 Fall Oct 19 2. Locate the brightest and easiest to observe stars and associated constellations 3. Add new prominent constellations for each season Tonight’s Schedule 8:00 pm – We meet inside for a slide presentation overview of the Summer sky. 8:40 pm – View night sky outside The Midnight Sky: Familiar Notes on the Stars and Planets, Edward Durkin, July 15, 1869 A Good Way to Start – Find North Polaris North Star Polaris is about the 50th brightest star. It appears isolated making it easy to identify. Circumpolar Stars Polaris Horizon Line Albuquerque -- 35° N Circumpolar Stars Capella the Goat Star AS THE WORLD TURNS The Circle of Perpetual Apparition for Albuquerque Deneb 1 URSA MINOR 2 3 2 URSA MAJOR & Vega BIG DIPPER 1 3 Draco 4 Camelopardalis 6 4 Deneb 5 CASSIOPEIA 5 6 Cepheus Capella the Goat Star 2 3 1 Draco Ursa Minor Ursa Major 6 Camelopardalis 4 Cassiopeia 5 Cepheus Clock and Calendar A single map of the stars can show the places of the stars at different hours and months of the year in consequence of the earth’s two primary movements: Daily Clock The rotation of the earth on it's own axis amounts to 360 degrees in 24 hours, or 15 degrees per hour (360/24).
    [Show full text]
  • The Hypergiants VY Canis Majoris, Eta Carinae, V766 Centauri and The
    Sixteenth Marcel Grossmann Meeting Contribution ID: 967 Type: Talk in the parallel session The hypergiants VY Canis Majoris, Eta Carinae, V766 Centauri and the red supergiants Betelgeuse, Antares and Aldebaran in the 2.5K SGQ AAVSO database Thursday, 8 July 2021 16:35 (7 minutes) I observe variable stars since 1997. The “candidacy” of Mira Ceti as Betlehem Star because close to Jupiter- Saturn triple conjunction of 6-7 b.C. started at Pontifical University of Lateran and continued in Yale (2001- 2004). Maxima correlation function ruled out Mira for having two consecutive bright maxima, but this prop- erty was confirmed in the “oldest” Myra-type: R Leonis, R Hydrae and Chi Cygni, from their almostfour- century-long lightcurves. To a bright maximum normally a dim one follows, as the correlation function of their consecutive maxima shows. These studies were supported by historical and personal visual observations. Since 2011 I observe firstmag- nitude variable stars, with airmass correction to reach 0.01 magnitudes accuracy with naked eye. AAVSO observer Sebastian Otero first claimed this accuracy, as for NovaCentauri 2013, observed by me fromPorto Alegre and Rio de Janeiro. Betelgeuse’s 801 observations in 10 years, include the deep minimum of 2020. My SGQ contributions to AAVSO-database, paralleled with Betelgeuse’s V-band measurements, help to define the “personal equations” present in all 25M visual observations before CCD era (1911-on) going back to 1893 for Betelgeuse. The temporal extension of lightcurves is crucial to understand the stellar behaviour. More complicate cases are Antares and Aldebaran, less variable and with distant comparison stars.
    [Show full text]
  • Educator's Guide: Orion
    Legends of the Night Sky Orion Educator’s Guide Grades K - 8 Written By: Dr. Phil Wymer, Ph.D. & Art Klinger Legends of the Night Sky: Orion Educator’s Guide Table of Contents Introduction………………………………………………………………....3 Constellations; General Overview……………………………………..4 Orion…………………………………………………………………………..22 Scorpius……………………………………………………………………….36 Canis Major…………………………………………………………………..45 Canis Minor…………………………………………………………………..52 Lesson Plans………………………………………………………………….56 Coloring Book…………………………………………………………………….….57 Hand Angles……………………………………………………………………….…64 Constellation Research..…………………………………………………….……71 When and Where to View Orion…………………………………….……..…77 Angles For Locating Orion..…………………………………………...……….78 Overhead Projector Punch Out of Orion……………………………………82 Where on Earth is: Thrace, Lemnos, and Crete?.............................83 Appendix………………………………………………………………………86 Copyright©2003, Audio Visual Imagineering, Inc. 2 Legends of the Night Sky: Orion Educator’s Guide Introduction It is our belief that “Legends of the Night sky: Orion” is the best multi-grade (K – 8), multi-disciplinary education package on the market today. It consists of a humorous 24-minute show and educator’s package. The Orion Educator’s Guide is designed for Planetarians, Teachers, and parents. The information is researched, organized, and laid out so that the educator need not spend hours coming up with lesson plans or labs. This has already been accomplished by certified educators. The guide is written to alleviate the fear of space and the night sky (that many elementary and middle school teachers have) when it comes to that section of the science lesson plan. It is an excellent tool that allows the parents to be a part of the learning experience. The guide is devised in such a way that there are plenty of visuals to assist the educator and student in finding the Winter constellations.
    [Show full text]
  • Lecture Notes 13: Double Stars and the Detection of Planets More Than Half of All Stars Are in Double Star Or in Multiple Star Systems
    Lecture notes 13: Double stars and the detection of planets More than half of all stars are in double star or in multiple star systems. This fact gives important clues on how stars form, but can also has the important consequence that it allows us to measure stellar masses. Double star types Double stars are conveniently subdivided into classes based on how they are observed: Optical double stars are stars that coincidentally lie on the same line of • sight as seen from the Earth. There are actually quite few of these, most stars that seem to lie close to each other are really double stars, they orbit each other. Visual double stars are doubles that can be separated either visually or • with a telescope. Their orbital period can vary from some years to more than a millennium. Spectroscopic double stars are stars that cannot be separated with a • telescope, but are discovered through studies of the stars’ spectral lines which will indicate periodic radial motions through doppler shifts of the spectral lines. Eclipsing binaries are double stars in which the orbital plane of obser- • vation is such that the stars periodically shadow for each other, leading to a periodic variation in the intensity of the combined flux from the stars. A famous naked eye example is the star Algol in Perseus. Astrometric double stars are stars where only one component is visible, • but that component periodically changes position on the sky due to its orbital motion around its companion. A famous example is Sirius in Canis Minor which has a white dwarf as companion, Sirius B, which is only 1/5000 as luminous as Sirius A.
    [Show full text]
  • Andrea Possenti
    UniversidadUniversidad dede ValenciaValencia 1515November November2010 2010 PulsarsPulsars asas probesprobes forfor thethe existenceexistence ofof IMBHsIMBHs ANDREA POSSENTI LayoutLayout ¾¾ KnownKnown BlackBlack HoleHole classesclasses ¾¾ FormationFormation scenariosscenarios forfor thethe IMBHsIMBHs ¾¾ IMBHIMBH candidatescandidates ¾¾ IMBHIMBH candidatescandidates (?)(?) fromfrom RadioRadio PulsarPulsar datadata analysisanalysis ¾¾ PerspectivesPerspectives forfor thethe directdirect observationobservation ofof IMBHsIMBHs fromfrom PulsarPulsar searchessearches ClassesClasses ofof BlackBlack HolesHoles Stellar mass Black Holes resulting from star evolution are supposed to be contained in many X-ray binaries: for solar metallicity, the max mass is of order few 10 Msun Massive Black Holes seen in the nucleus of the galaxies: 6 9 masses of order ≈ 10 Msun to ≈ 10 Msun AreAre IntermediateIntermediate Mass Black Holes ((IMBH)IMBH) ofof massesmasses ≈≈ 100100 -- 10,000 10,000 MMsunsun alsoalso partpart ofof thethe astronomicalastronomical landscapelandscape ?? N.B. ULX in the Globular Cluster RZ2109 of NGC 4472 may be a stellar mass BH likely in a triple system [ Maccarone et al. 2007 - 2010 ] FormationFormation mechanismsmechanisms forfor IMBHsIMBHs 11- - Mass Mass segregationsegregation ofof compactcompact remnantsremnants inin aa densedense starstar cluster 22– – Runaway Runaway collisionscollisions ofof massivemassive starsstars inin aa densedense starstar clustercluster In both cases, the seed IMBH can then grow by capturing other “ordinary”
    [Show full text]
  • 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.
    [Show full text]