The Evening Sky Map a SEPTEMBER 2021 E

Total Page:16

File Type:pdf, Size:1020Kb

The Evening Sky Map a SEPTEMBER 2021 E 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 e o t u a n t o d r O N t o h t e Z r N a I e o C p r t p R h I a R C s O e r C a l H e t L s s t , E E i s a e l H ( d P T F u o t O l i e NORTH D t R a ( l N N M E A n C X r O P e A ) H h . M C T t r . I P o N L S n E E P Z m “ o E r A N F H O NORTHERN HEMISPHERE M T R LYNX T Y N H E ” K E ) W S . T Capella T E W U B R N W D E T W T H The Evening Sky Map A SEPTEMBER 2021 E C T FREE* EACH MONTH FOR YOU TO EXPLORE, LEARN & ENJOY THE NIGHT SKY O S h L K e Y E CAMELOPARDALIS b R M r i A g A h S SKY MAP SHOWS HOW Get Sky Calendar on Twitter P T t URSA MAJOR URSA C A s E R t . J a r Sky Calendar – September 2021 http://twitter.com/skymaps O r a B THE NIGHT SKY LOOKS U s t O S N o L D f h A t NE C r I I a T EARLY SEPT PM T o 9 M81 s S S N 2 Moon near Castor at 23h UT (morning sky). s E i NW C o e L E p “ h E N T t e M82 O C LATE SEPT 8 PM T i , P . a E O 3 Moon near Pollux at 5h UT (morning sky). s (Add 1 Hour For Daylight Saving) L i N R PERSEUS A f r R o O a I ( S l Z r SKY MAP DRAWN FOR J ” m I o T U R H P S 4 Moon near Beehive cluster M44 at 7h UT (morning sky). E a O A LATITUDE OF 40° T N d H O W n R A Dipper i T E - NORTH AND IS f H S Algol s H The Big The S h 5 at 21h UT (evening sky). Mags. –4.1 & 1.0. o Venus 1.6° NNE of Spica T Y T t A M94 a SUITABLE FOR O R CANES VENATICI p S ) U I e h Cluster LATITUDES UP g A E 7 at 0:51 UT. Start of lunation 1221. t New Moon Double h u Polaris L R a C o E TO 15° NORTH l & Alcor & NCP t R P Mizar Caroli D I MINOR i Cor C r s OR SOUTH O M51 9 Moon near Mercury at 2h UT (evening sky). Mag. 0.1. URSA o I e R ( N CASSIOPEIA a Thuban E OF THIS M64 r G s T e y U N p 9 Moon near Spica at 22h UT (evening sky). CEPHEUS t O O p o γ i Dipper W E D r ANDROMEDA ) e H Little g T 10 Moon near Venus at 6h UT (evening sky). Mag. –4.1. c i S o O B D g η M3 N n ARIES e T β DRACO H i A h z 10 Asteroid 2 Pallas at opposition at 17h UT (evening t E e ) . Hamal E e H C s T sky). Mag. 8.6. O C I U M33 M L N M31 P I E A P Z ( 11 Moon at perigee (closest to Earth) at 9:53 UT S δ T S D I γ ν D C μ A Arcturus I E (distance 368,461 km; angular size 32.4'). T ε R h H E e R C E a T 13 Moon near Antares at 3h UT (evening sky). V n I O O c N i Etamin Y e M39 L n Deneb T 13 First Quarter Moon at 20:40 UT. M92 BOÖTES T t H C PISCES A c E M13 o T R R CORONA Gemma n I EAST 14 Mercury at greatest elongation east at 4h UT BOREALIS A Great Square Great s D P of Pegasus of t ε e P Y CYGNUS Vega l (27° from Sun, evening sky). Mag. 0.2 E K l 61 a A S t R i E S o WEST β H 14 Neptune at opposition at 9h UT. Mag. 7.8. n A T L o F LYRA . O f M57 χ ” O N s 17 Moon near Saturn at 5h UT (evening sky). Mag. 0.4. A T G Summer Triangle d q Albireo o R u PEGASUS HERCULES T g A a H VIRGO P r M27 18 Moon near Jupiter at 10h UT (evening sky). Mag. –2.8. e E i u h E M5 B s t H α SERPENS (CAPUT) O r f T e 20 Full Moon at 23:54 UT. T o S T p Cr 399 I O Circlet d r γ e a M P s o M15 A 21 Mercury 1.4° SSW of Spica at 15h UT (25° from e DELPHINUS r O n “ M F t Enif e s E T Sun, evening sky). Mags. 0.4 and 1.0. h H a Altair IC 4665 t H T E y s CETUS o a F M AQUARIUS 6633 u O 22 September equinox at 19:22 UT. The time when the t A n M12 i R P g d E OPHIUCHUS I m e T Sun reaches the point along the ecliptic where it S i M2 M10 f N a η LIBRA i E T n t H SERPENS C n crosses into the southern celestial hemisphere marking E p (CAUDA) e E o AQUILA d H S u i A T r Diphda s the start of autumn in the Northern Hemisphere and M i . n M11 t E e S g E o A w p M spring in the Southern Hemisphere. S I a 7009 M16 t T T t β n H e Jupiter e r i D E f c N 26 Moon near the Pleiades at 3h UT (morning sky). r n A D o I m M17 A S R CAPRICORNUS . E E a 7293 M23 y T 26 Moon near Aldebaran at 21h UT (morning sky). C k A T j M25 s D I a Saturn M21 e O r M20 N N i th I Symbols n A 26 Moon at apogee (farthest from Earth) at 22h UT (distance T t Antares s T H o Fomalhaut Nunki M4 s R A t M22 M8 ro E Galaxy T h c C 404,640 km; angular size 29.5'). Y e AUSTRINUSPISCIS a O m s N U SE The e O o Teapot h S Double Star F u c R 29 Last Quarter Moon at 1:57 UT. A th SW et A CE o tr E . f s P Variable Star B a SAGITTARIUS M6 y P E l SCORPIUS a A 30 Moon near Castor at 8h UT (morning sky). G ar W IT IN g y S Diffuse Nebula e lk A B fi M7 i Y sh M N 30 Moon near Pollux at 13h UT (morning sky). U , e ZO SI P Th I Planetary Nebula N isc CORONA OR G is H More sky events and links at http://Skymaps.com/skycalendar/ TH A GRUS AUSTRALIS O- Open Star Cluster E us -T SK tri ON Y nu IZ All times in Universal Time (UT). (USA Eastern Summer Time = UT – 4 hours.) MA s. OR Globular Star Cluster P T H O OM FIN FR SAVE ON RECOMMENDED PRODUCTS • http://Skymaps.com/store D A The SKY B Sum . T RIG me head IGH Star Magnitudes HT r Tria SOUTH over E N -1 0 1 2 3 4 • Star Atlases & Planispheres • Star Charts & Astro Posters STA ngle stars TIR R PA – Vega, bright E EN TTER Altair, and Deneb – three S TH Copyright © 2000–2021 Kym Thalassoudis. All Rights Reserved. • Books for Sky Watchers • Telescopes & Binoculars 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. Mag varies between 3.5 & 4.4 over 5.366 days.
Recommended publications
  • Planet Positions: 1 Planet Positions
    Planet Positions: 1 Planet Positions As the planets orbit the Sun, they move around the celestial sphere, staying close to the plane of the ecliptic. As seen from the Earth, the angle between the Sun and a planet -- called the elongation -- constantly changes. We can identify a few special configurations of the planets -- those positions where the elongation is particularly noteworthy. The inferior planets -- those which orbit closer INFERIOR PLANETS to the Sun than Earth does -- have configurations as shown: SC At both superior conjunction (SC) and inferior conjunction (IC), the planet is in line with the Earth and Sun and has an elongation of 0°. At greatest elongation, the planet reaches its IC maximum separation from the Sun, a value GEE GWE dependent on the size of the planet's orbit. At greatest eastern elongation (GEE), the planet lies east of the Sun and trails it across the sky, while at greatest western elongation (GWE), the planet lies west of the Sun, leading it across the sky. Best viewing for inferior planets is generally at greatest elongation, when the planet is as far from SUPERIOR PLANETS the Sun as it can get and thus in the darkest sky possible. C The superior planets -- those orbiting outside of Earth's orbit -- have configurations as shown: A planet at conjunction (C) is lined up with the Sun and has an elongation of 0°, while a planet at opposition (O) lies in the opposite direction from the Sun, at an elongation of 180°. EQ WQ Planets at quadrature have elongations of 90°.
    [Show full text]
  • Phobos, Deimos: Formation and Evolution Alex Soumbatov-Gur
    Phobos, Deimos: Formation and Evolution Alex Soumbatov-Gur To cite this version: Alex Soumbatov-Gur. Phobos, Deimos: Formation and Evolution. [Research Report] Karpov institute of physical chemistry. 2019. hal-02147461 HAL Id: hal-02147461 https://hal.archives-ouvertes.fr/hal-02147461 Submitted on 4 Jun 2019 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Phobos, Deimos: Formation and Evolution Alex Soumbatov-Gur The moons are confirmed to be ejected parts of Mars’ crust. After explosive throwing out as cone-like rocks they plastically evolved with density decays and materials transformations. Their expansion evolutions were accompanied by global ruptures and small scale rock ejections with concurrent crater formations. The scenario reconciles orbital and physical parameters of the moons. It coherently explains dozens of their properties including spectra, appearances, size differences, crater locations, fracture symmetries, orbits, evolution trends, geologic activity, Phobos’ grooves, mechanism of their origin, etc. The ejective approach is also discussed in the context of observational data on near-Earth asteroids, main belt asteroids Steins, Vesta, and Mars. The approach incorporates known fission mechanism of formation of miniature asteroids, logically accounts for its outliers, and naturally explains formations of small celestial bodies of various sizes.
    [Show full text]
  • Experiencing Hubble
    PRESCOTT ASTRONOMY CLUB PRESENTS EXPERIENCING HUBBLE John Carter August 7, 2019 GET OUT LOOK UP • When Galaxies Collide https://www.youtube.com/watch?v=HP3x7TgvgR8 • How Hubble Images Get Color https://www.youtube.com/watch? time_continue=3&v=WSG0MnmUsEY Experiencing Hubble Sagittarius Star Cloud 1. 12,000 stars 2. ½ percent of full Moon area. 3. Not one star in the image can be seen by the naked eye. 4. Color of star reflects its surface temperature. Eagle Nebula. M 16 1. Messier 16 is a conspicuous region of active star formation, appearing in the constellation Serpens Cauda. This giant cloud of interstellar gas and dust is commonly known as the Eagle Nebula, and has already created a cluster of young stars. The nebula is also referred to the Star Queen Nebula and as IC 4703; the cluster is NGC 6611. With an overall visual magnitude of 6.4, and an apparent diameter of 7', the Eagle Nebula's star cluster is best seen with low power telescopes. The brightest star in the cluster has an apparent magnitude of +8.24, easily visible with good binoculars. A 4" scope reveals about 20 stars in an uneven background of fainter stars and nebulosity; three nebulous concentrations can be glimpsed under good conditions. Under very good conditions, suggestions of dark obscuring matter can be seen to the north of the cluster. In an 8" telescope at low power, M 16 is an impressive object. The nebula extends much farther out, to a diameter of over 30'. It is filled with dark regions and globules, including a peculiar dark column and a luminous rim around the cluster.
    [Show full text]
  • 5 the Orbit of Mercury
    Name: Date: 5 The Orbit of Mercury Of the five planets known since ancient times (Mercury, Venus, Mars, Jupiter, and Saturn), Mercury is the most difficult to see. In fact, of the 6 billion people on the planet Earth it is likely that fewer than 1,000,000 (0.0002%) have knowingly seen the planet Mercury. The reason for this is that Mercury orbits very close to the Sun, about one third of the Earth’s average distance. Therefore it is always located very near the Sun, and can only be seen for short intervals soon after sunset, or just before sunrise. It is a testament to how carefully the ancient peoples watched the sky that Mercury was known at least as far back as 3,000 BC. In Roman mythology Mercury was a son of Jupiter, and was the god of trade and commerce. He was also the messenger of the gods, being “fleet of foot”, and commonly depicted as having winged sandals. Why this god was associated with the planet Mercury is obvious: Mercury moves very quickly in its orbit around the Sun, and is only visible for a very short time during each orbit. In fact, Mercury has the shortest orbital period (“year”) of any of the planets. You will determine Mercury’s orbital period in this lab. [Note: it is very helpful for this lab exercise to review Lab #1, section 1.5.] Goals: to learn about planetary orbits • Materials: a protractor, a straight edge, a pencil and calculator • Mercury and Venus are called “inferior” planets because their orbits are interior to that of the Earth.
    [Show full text]
  • Field Astronomy Circumpolar Star at Elongation ➢ at Elongation a Circumpolar Star Is at the Farthest Position from the Pole Either in the East Or West
    Field Astronomy Circumpolar Star at Elongation ➢ At elongation a circumpolar star is at the farthest position from the pole either in the east or west. ➢ When the star is at elongation (East or West), which is perpendicular to the N-S line. ➢ Thus the ZMP is 90° as shown in the figure below. Distances between two points on the Earth’s surface ➢ Direct distance From the fig. above, in the spherical triangle APB P = Difference between longitudes of A and B BP = a = co-latitude of B = 90 – latitude of B AP = b = co-latitude of A = 90 – latitude of A Apply the cosine rule: cosp− cos a cos b CosP = sinab sin Find the value of p = AB Then the distance AB = arc length AB = ‘p’ in radians × radius of the earth ➢ Distance between two points on a parallel of latitude Let A and B be the two points on the parallel latitude θ. Let A’ and B’ be the corresponding points on the equator having the same longitudes (ФB, ФA). Thus from the ∆ O’AB AB = O’B(ФB - ФA) From the ∆ O’BO o O’B = OB’ sin (90- θ) Since =BOO ' 90 = R cos θ where R=Radius of the Earth. AB= (ФB - ФA) R cos θ where ФB , ФA are longitudes of B and A in radians. Practice Problems 1. Find the shortest distance between two places A and B on the earth for the data given below: Latitude of A = 14° N Longitude of A = 60°30‘E Latitude of B = 12° N Longitude of A = 65° E Find also direction of B from A.
    [Show full text]
  • Observing Project
    Observing Project Objectives: • Learn how to “practically” measure angles on the sky • How to take data and assess measurement errors • How to plot and interpret graphs • Geometry of Earth-Moon-Sun system • Measure the orbital period of the Moon • Predict the phase of the moon of a future date th • First 3 Observations Due May 29 !!!! Moon Moves Across the Constellations Could measure the movement against the background stars The Moon moves at an angle (difficult to measure) The stars themselves move over days due to our revolution around the Sun Measure with respect to the sun! Moon’s Elongation: Separation of the Moon and Sun in the sky. Moon’s Elongation Angle Moon’s Orbit • Fix the Moon-Sun geometry • Elongation angle changes as the Moon orbits • So do the Moon phases 315° 225° 270° Moon Phase Number TPS At what Elongation angle is the Moon visible during the day? 315° A. 100 B. 45 225° C. 180 270° D. 225 TPS What Moon phase could you directly measure the Moon’s Elongation Angle? 315° A. Waxing Gibbous 225° B. Waxing Crescent 270° C. Full Moon D. Depends on the time of year *Don’t Look Directly into the SUN!!! • How do we measure the Moon’s elongation angle at night??? • Hour Angle: angle of object from your local Meridian • What is the time of day of the “little cowboy”? • A: Midnight Meridian • How do we measure the Sun’s HA at night??? • Our clocks are based of the Sun’s Position. • Noon: when the Sun crosses our Meridian • What is the HA of the Sun at Midnight? • A: 180 degrees Meridian Moon Elongation = Sun HA – Moon HA Daylight Savings Time Artificially move the clocks forward by 1 hour How does this change Astronomical Noon??? Would this affect your measurement??? Mountain Standard Time (MST) • The Sun is closer to the Meridian Mountain Daylight Time (MDT) MST = MDT – 1 hour Hours to Degrees Earth rotates once every 24 hours • 360 degrees per 24 hours • 360/24 = 15 (degrees/hour) Sun’s HA (degrees) = [ MST – 12 (noon) ] * 15 What is the HA of a first quarter Moon at midnight? A.
    [Show full text]
  • Binocular Observing Olympics Stellafane 2018
    Binocular Observing Olympics Stellafane 2018 Compiled by Phil Harrington www.philharrington.net • To qualify for the BOO pin, you must see 15 of the following 20 binocular targets. Check off each as you spot them. Seen # Object Const. Type* RA Dec Mag Size Nickname 1. M4 Sco GC 16 23.6 -26 32 6.0 26' Cat’s Eye Globular 2. M13 Her GC 16 41.7 +36 28 5.9 16' Great Hercules Globular 3. M6 Sco OC 17 40.1 -32 13 4.2 15' Butterfly Cluster 4. IC 4665 Oph OC 17 46.3 +05 43 4.2 41' Summer Beehive 5. M7 Sco OC 17 53.9 -34 49 3.3 80' Ptolemy’s Cluster 6. M20 Sgr BN/OC 18 02.6 -23 02 8.5 29'x27' Trifid Nebula 7. M8 Sgr BN/OC 18 03.8 -24 23 5.8 90'x40' Lagoon Nebula 8. M17 Sgr BN 18 20.8 -16 11 7 46'x37' Swan or Omega Nebula 9. M22 Sgr GC 18 36.4 -23 54 5.1 24' Great Sagittarius Cluster 10. M11 Sct OC 18 51.1 -06 16 5.8 14' Wild Duck Cluster 11. M57 Lyr PN 18 53.6 +33 02 9.7 70"x150" Ring Nebula 12. Collinder 399 Vul AS 19 25.4 +20 11 3.6 60' Coathanger/Brocchi’s Cluster 13. PK 64+5.1 Cyg PN 19 34.8 +30 31 9.6p 8" Campbell's Hydrogen Star 14. M27 Vul PN 19 59.6 +22 43 8.1 8’x6’ Dumbbell Nebula 15.
    [Show full text]
  • Astronomy Lab: Planets
    Phys 102 Astronomy Name ____________________Key POSITIONS OF THE PLANETS PLANETARY POSITIONS WITH RESPECT TO THE SUN: 23 Use appendix 11 in the Field Guide for February 1, 2021 to complete the following table: Object Planetary Longitude Atlas Chart # Constellation Elongation Sol () 313 32 Capricornus ZERO! Planets ☿ in order Mercury ( ) 326 32 Capricornus 13° E of orbit Venus(♀) 300 43 Capricornus 13° W distance from the Mars (♂) 43 22 Aries 90° E Sun. Jupiter (♃) 310 31/43 Capricornus 3° W Saturn (♄) 305 31/43 Capricornus 8° W PLANETARY POSITIONS IN THE SKY The digram below shows an observer looking south at sunset. From the planetary longitude of the sun and planets abovee, show where the planets will be in the observer’s sky (some may be below the horizon). Discuss how these positions correspond to the times the planets will be visible to this observer (eg. after sunset, before sunrise or most of the night). 11 Sun’s PL + 90° _______43° ♂ At E. Quadrature! Observer’s meridian Come look for the planets with me! ☿ Sun’s PL ± 180 Sun’s PL _______133° _______ E observer W ♃ 313° Sun setting on looking ♄ western horizon south ♀ Sun’s PL - 90°: _______223° Phys. 102: Astronomy Spring 2021 PLANETARY POSITIONS IN THE SOLAR SYSTEM A view of the solar system as seen FROM ABOVE THE NORTH ECLIPTIC POLE with the sun in the center is shown below. The line from the Earth ( ) to the Sun ( ) represents the planetary longitude of the sun. For each of the five visible planets, 1) Center a protractor on the Earth, measure the elongation angle from the sun's longitude.
    [Show full text]
  • Introduction No. 104 July 2020
    No. 104 July 2020 Introduction I hope you are in good health as July’s Binocular Sky Newsletter reaches you. Although it is primarily targeted at binocular (and small telescope) observers in the UK, this particular community extends well south of the Equator. So welcome! Astronomical darkness, albeit short, return for locations south of about 53.5°N this month and, as binocular observers with our combination of maximum portability and minimal set-up time, we are well suited to take advantage of what this darkness reveals. I hesitate to write this, given recent history of our dashed expectations of “promising” comets, but we have another one, C/2020 F3 (NEOWISE). It’s visible in SOHO images and might just live up to expectations. (But it might not!) The binocular planets, Uranus and Neptune are becoming visible in the pre-dawn sky, as is Ceres but the short darkness means that there is only one suitable lunar occultations of a star, a dark-limb reappearance. If you would like to receive the newsletter automatically each month, please complete and submit the subscription form. You can get “between the newsletters” alerts, etc. via and . Binocular Sky Newsletter – July 2020 The Deep Sky (Hyperlinks will take you to finder charts and more information on the objects.) The all-sky chart on the next page reveals a lot about the structure of the Milky Way galaxy. Running in a strip down the middle, coinciding with the Milky Way itself, is the orange band of open clusters. Here, we are looking along the plane of the spiral arms which, of course, is where the star-forming (and, hence, open cluster forming) regions are.
    [Show full text]
  • Summer Sp Target Information
    SUMMER SP TARGET INFORMATION ALGIEBA (g LEO) BASIC INFORMATION OBJECT TYPE: Binary Star CONSTELLATION: Leo BEST VIEW: Late April DISCOVERY: Known to Ancients DISTANCE: 131 ly BINARY SEPARATION: 4” (170 AU) ORBITAL PERIOD: ~500 yr. APPARENT MAGNITUDE: 1.98 DISTANCE DETERMINATION After measuring the shift in position of the star relative to background stars as Earth orbits the Sun, simple trigonometry can yield the distance. The Hipparcos satellite was launched in 1989 to create a comprehensive catalog of trigonometric parallax measurements from space. The distance quoted above is from this catalog. NOTABLE FEATURES/FACTS • William Herschel discovered Algieba’s binary nature in 1782. • Both components of Algieba have evolved beyond the main sequence. They began their lives as B-type stars, and they will end their lives as white dwarfs. • In 2010, a team including former UT astronomer Arte Hatzes discovered a planet orbiting Algieba A. The planet is nine times the mass of Jupiter and orbits the star in 1.2 years at an average distance of 1.2 AU. SUMMER SP TARGET INFORMATION MESSIER 97 (THE OWL NEBULA) BASIC INFORMATION OBJECT TYPE: Planetary Nebula CONSTELLATION: Ursa Major BEST VIEW: Early May DISCOVERY: Pierre Mechain, 1781 DISTANCE: ~2000 ly DIAMETER: 1.8 ly APPARENT MAGNITUDE: +9.9 APPARENT DIMENSIONS: 3.3’ DISTANCE DETERMINATION The distances to most planetary nebulae are very poorly known. A variety of methods can be used, providing mixed results. In many cases, astronomers resort to statistical methods to estimate the distances to planetary nebulae. Although we don’t have accurate distances for most of the planetary nebulae in the Milky Way, we do know exactly how far away the Large Magellanic Cloud is.
    [Show full text]
  • Contents 2 Jan
    By Martin Ratcliffe and Richard Talcott Sky Guide 2018 Mars shines brilliantly and looms large through telescopes this year as it puts on its finest show since 2003. NASA/JPL-CALTECH contents 2 Jan. 2018 Eclipse of the Blue Moon 3 Feb. 2018 Target galaxies these cool winter nights 4 March 2018 Catch Mercury at dusk 5 April 2018 The Lyre plays a sweet meteor song 6 May 2018 Jupiter rules spring nights 7 June 2018 Saturn’s rings on gorgeous display 8 July 2018 Red Planet renaissance 9 Aug. 2018 Prime time for the Perseids 10 Sept. 2018 Venus blazes in the evening twilight 11 Oct. 2018 An ice giant butts into the Ram Martin Ratcliffe provides professional 12 Nov. 2018 Juno at its best in 35 years planetarium development for Sky-Skan, Inc. Richard Talcott is a senior editor of Astronomy. 13 Dec. 2018 Making a swing past Earth 14 2019 Preview Looking ahead to next year ... A supplement to Astronomy magazine 618364 2018 Jan. S M T W T F S Eclipse of the 2 3 4 5 6 7 9 10 11 12 13 14 15 17 18 19 20 Blue Moon 21 22 23 25 26 27 28 29 30 anuary features two third of the country experience Full Moons, both of only the initial partial phases. which command our The Moon dips into Earth’s attention. The first dark umbral shadow at 1 Mercury is at great- comes New Year’s 6:48 a.m. EST (3:48 a.m. PST), est western elonga- night and arrives less than five but the Moon sets before total- tion (23°), 3 P.M.
    [Show full text]
  • Messier Object Mapping System
    Messier Object Mapping System Messier Object Constellation Map# Messier Object Constellation Map# M1 Taurus 1-6 M56 Lyra 3 M2 Aquarius 8 M57 Lyra 3 M3 Canes Venatici 4-10 M58 Virgo IN2-5 M4 Scorpius 2 M59 Virgo IN2 M5 Scorpius 10 M60 Virgo IN2-5-9-10 M6 Scorpius 2 M61 Virgo IN2-5-8 M7 Scorpius 2 M62 Ophiuchus 2 M8 Sagittarius 2-IN1 M63 Canes Venatici 4 M9 Ophiuchus 2 M64 Coma Berenices 4-5 M10 Ophiuchus 2 M65 Leo 5 M11 Scutum 2 M66 Leo 5 M12 Ophiuchus 2 M67 Cancer 6 M13 Hercules 3 M68 Hydra 9 M14 Ophiuchus 2 M69 Sagittarius 2-IN1-8 M15 Pegasus 8 M70 Sagittarius 2-IN1-8 M16 Serpens 2-IN1 M71 Sagittarius 2 M17 Sagittarius 2-IN1 M72 Aquarius 8 M18 Sagittarius 2-IN1 M73 Aquarius 8 M19 Ophiuchus 2 M74 Pisces 11 M20 Sagittarius 2-IN1-8 M75 Sagittarius 8 M21 Sagittarius 2-IN1-8 M76 Perseus 7 M22 Sagittarius 2-IN1-8 M77 Cetus 11 M23 Sagittarius 2-IN1 M78 Orion 1 M24 Sagittarius 2-IN1 M79 Lepus 1 M25 Sagittarius 2-IN1-8 M80 Scorpius 2 M26 Scutum 2 M81 Ursa Major 4 M27 Vupecula 3 M82 Ursa Major 4 M28 Sagittarius 2-IN1-8 M83 Hydra 9 M29 Cygnus 3 M84 Virgo IN2-5 M30 Capricornus 8 M85 Coma Berenices 4-5 M31 Andromeda 7-11 M86 Virgo IN2-5 M32 Andromeda 7-11 M87 Virgo IN2-5 M33 Triangulum 7-11 M88 Coma Berenices IN2-5 M34 Perseus 7-11 M89 Virgo IN2 M35 Gemini 1-6 M90 Virgo IN2-5 M36 Auriga 1-6 M91 Virgo IN2-5 M37 Auriga 1-6 M92 Hercules 3 M38 Auriga 1 M93 Puppis 1-6 M39 Cygnus 3-7 M94 Canes Venatici 4-5 M40 Ursa Major 4 M95 Leo 5 M41 Canis Major 1 M96 Leo 5 M42 Orion 1 M97 Ursa Major 4 M43 Orion 1 M98 Coma Berenices IN2-4-5 M44 Sagittarius 6 M99 Coma Berenices IN2-4-5 M45 Taurus 1-11 M100 Coma Berenices IN2-4-5 M46 Puppis 1-6 M101 Ursa Major 4 M47 Puppis 1-6 M102 Draco 4 M48 Hydra 6 M103 Cassiopeia 7 M49 Virgo 2-IN1-8 M104 Virgo 5-9-10 M50 Monoceros 1-6 M105 Leo 5 M51 Canes Venatici 4-10 M106 Canes Venatici 4-5 M52 Cassiopeia 7 M107 Ophiuchus 2 M53 Coma Berenices 4-5-10 M108 Ursa Major 4 M54 Sagittarius 2-IN1-8 M109 Ursa Major 4-5 M55 Sagittarius 2-8 M110 Andromeda 7-11 Messier Object List # NGC# Constellation Type Name, If Any Mag.
    [Show full text]