Prime Focuss

Total Page:16

File Type:pdf, Size:1020Kb

Prime Focuss Highlights of the March Sky. -- -- -- 2nd -- -- -- The Moon passes 4º southsouth of Jupiter, 8 pm. PPrime Focuss -- -- -- 3rd -- -- -- A Publication of the Kalamazoo Astronomical Society Mercury is at greatest western elongation (27º), 6 am. March 2008 -- -- -- 5th -- -- -- The Moon passes 0.2º south of Mercury, 9 am. ThisThis MonthsMonths KAS EventsEvents The Moon passes 0.2º north of Venus, 2 pm. General Meeting: Friday, March 7 @ 7:00 pm -- -- -- 6th -- -- -- Venus passes 0.6º southsouth ofof Kalamazoo Math & Science Center - See Page 16 for Details Neptune, 3 pm. Observing Session: Saturday, March 8 @ 7:00 pm th -- -- -- 7th -- -- -- New Moon Messier Marathon - Richland Township Park - See Page 13 for Map -- -- -- 10thth -- -- -- Special Lecture: Tuesday, March 25 @ 7:00 pm Mars 1.7º northnorth ofof M35.M35. WMU Main Campus, Rood Hall, Room 1104 - See Page 3 for Details th -- -- -- 14 -- -- -- First Quarter Moon First Quarter Moon Full Moon Theater: Saturday, March 29 @ 7:00 pm The Moon passes 1º northnorth WMU Main Campus, Rood Hall, Room 1110 - See Page 3 for Details of Mars near midnight. -- -- -- 19th -- -- -- The Moon passes 0.8º south of Regulus, 4 am. InsideInside thethe Newsletter.Newsletter. .. .. The Moon passes 3º southsouth February Meeting Minutes.................... p. 2 of Saturn, 11 am. Board Meeting Minutes......................... p. 2 -- -- -- 21st -- -- -- Full Moon Harlow Shapely Lecture........................p. 3 Full Moon Theater Preview................. p. 3 -- -- -- 23rd -- -- -- Mercury passes 1.0º southsouth Lunar Eclipse Captured......................... p. 4 of Venus, 6 am. Charles Messier...................................... p. 5 -- -- -- 27thth -- -- -- Guide to the Messier Marathon.......... p. 7 The Moon passes 0.5º Messier Marathon Search List............. p. 11 south of Antares, 6 a.m. NASA Space Place.................................. p. 12 -- -- -- 29thth -- -- -- Last Quarter Moon Messier Marathon Location Map........ p. 13 March Night Sky..................................... p. 14 -- -- -- 30thth -- -- -- The Moon passes 3º southsouth KAS Officers & Announcements........ p. 15 of Jupiter, 1 p.m. www.kasonline.org February Meeting Minutes Board Meeting Minutes The general meeting of the KAS was brought to order by The KAS Board met on February 17th at Sunnyside Church President Jack Price on February 1st at 7:15 pm EST. Thirty (following a one-week weather delay). President Jack Price members and guests were in attendance at the Kalamazoo brought the meeting to order at 5:15 pm. Other board mem- Area Math & Science Center (KAMSC). bers present include Richard Bell, Jean DeMott, Dan Morgan, Rich Mather, and Roger Williams. The guest speaker for the evening was fellow KAS member and Associate Professor of Astronomy at WMU, Dr. Kirk Rich delivered a treasurer’s report showing a current balance Korista. Kirk’s called his latest presentation Pluto - What’s in of $13,423.58. As directed by the board at the last meeting, a Name?. Kirk stated that our ancestors began naming objects Rich had invested much of the assets in certificates of deposit, in the heavens because it gave them a sense of power over $5,800 for the Land Acquisition Fund money and $5,000 for them. He then gave a brief history of the discovery of Pluto part of the cash balance. The CD’s will mature in one year, at by Clyde Tombaugh in 1930. Tombaugh was, in a sense, which time a decision can be made about reinvestment. hired by the ghost of Percival Lowell, who began the search for “Planet X” before his death in 1916. Events planned for March were summarized. The Messier Marathon is scheduled for March 8th at Richland Township Kirk then gave a detailed overview of the layout of the solar Park. Rich had not yet checked on the availability of the park, system and how Pluto fits in to it all. In short, Pluto lies in a but promised to do so immediately. After some discussion, region called the Kuiper Belt and Neptune marks the inner Full Moon Theater was set for March 29th, since the logical boundary of the Kuiper Belt swarm. Pluto’s eccentric orbit March 22nd date is on Easter weekend (see page 3). carries it between 30 - 49 AU from the Sun and actually crosses Neptune’s orbit on occasion. The two bodies will Old Business included the search for a display-table drape never collide due to Pluto’s 17º inclination and a 3:2 reso- printed with the KAS logo. Richard had contacted a number nance. In fact, due to this resonance, Pluto gets closer to Ura- of potential suppliers, finding that the first one contacted nus than it ever does to Neptune. Kirk then described some of quoted by far the lowest price of $150. The Board agreed that Pluto’s characteristics such as its small size (seven moons are Richard should be authorized to buy one of the drapes, pro- larger in diameter) and Pluto’s own family of three moons. vided that inspection of a sample showed the quality to be acceptable. Jean agreed to assist with quality control. The decision of the International Astronomical Union (IAU) in August 2006 was then discussed and Kirk covered the fall- In other old business, the general meeting schedule was out and controversy, including comments made by Alan Stern firmed up, with Mark Miller speaking on large telescopes on (director of the New Horizons mission to Pluto). Kirk then March 7th, Dan Morgan describing telescope construction on went into the physics of what makes a body round and what it April 4th, and Dr. Arunav Kundu of MSU speaking about means to for an object to “clear its neighborhood”. Kirk dis- comet tails on June 6th. September and November have yet to played a graph that was in a paper written in 2002 written by be determined. Astronomy Day is set for April 19th at KNC. Alan Stern and Harold Levison. It showed a body of mass M The topics this year will be the Sun and Mercury. versus the mean distance of the Sun, with the lines of constant gravitational scattering parameter, lambda (Λ). All the eight In new business, the Vicksburg Middle School science night major planets were above the Λ = 1000 line, while ALL other appearance is scheduled again on Wednesday, March 12th. bodies were below the Λ = 0.003 line. Kirk then explained Dr. Christine Jones will speak on March 25th at 7 pm as part that Pluto may ultimately help tell us how the solar system of the Harlow Shapley visiting lecture program, jointly spon- formed 4.5 billion years ago and how it evolved over time. sored by KAS and WMU (see page 3 for program details). So, Pluto may no longer be considered a planet (as Mike Regarding the KAS web site, Richard reported having been Sinclair FINALLY admitted in public), but it may turn out to thinking for some time about how it could be improved be one of the most important bodies in the solar system. through redesign and having recently found a template design that already contains most of the desired features. The tem- After the snack break, we discussed the limited opportunities plate can be purchased for $140, and the redesign could be for observing as of late due to persistent cloud cover and bitter completed when time allows. The Board voted to authorize cold. The 5th anniversary of the Columbia diaster was buying the template. mentioned along with the 50th anniversary of the launch of Explorer I. The new images of Mercury by the MESSENGER The meeting was adjourned at 6:55 pm. The next meeting spacecraft were mentioned. Jean DeMott presented an $1,100 was set for March 9th, same time and place. check to President Jack Price. This brings the land acquisition fund to $8,000 now! The meeting concluded at 9:21 pm. Respectfully submitted by Roger Williams Prime Focus Page 2 March 2008 American Astronomical Society Harlow Shapley Visiting Lecture Program Join us for our next Full Moon Theater Reflections from Outbursts of Supermassive Friday, March 29 @ 7:00 pm Black Holes at the Centers of Galaxies WMU Main Campus - Rood Hall - Room 1110 Presented by Dr. Christine Jones Center for Astrophysics, Harvard University Are you a bored astronomer? Answer: of course you are, but what did you expect? It’s too cold and cloudy this time of year to observe. Not to mention that big, bright nasty Moon is in the way (Yes, it’s only a Waxing Gibbous Moon Galaxies don't like to be alone. Their gravitational pull — on March 15th, but that’s just a technicality). So, if you can’t even across the vast distances of space — causes galaxies to observe and you’re tired of watching the same old drivel on form clusters that can contain hundreds or even thousands of T.V., then join us for the next Full Moon Theater. The KAS individual galaxies. Clusters of galaxies are, in fact, the will provide the popcorn and all the soft drinks. You just largest structures in the Universe that are held together by need to show up and have a great time! gravity. Because of their immense size and mass, galaxy clusters are extremely useful as tools to probe a variety of Our feature presentation... questions about the Universe, including how much mass is luminous matter and how much is dark matter. In addition to being massive, clusters are so luminous that they can be observed back to when the Universe was only half its present age. Comparing the properties of distant clusters with nearby ones allows us to see both how clusters grow over time as smaller clusters fall into them, and also lets us constrain In the Shadow of the Moon important cosmological parameters.
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]
  • 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]
  • Astronomy Magazine Special Issue
    γ ι ζ γ δ α κ β κ ε γ β ρ ε ζ υ α φ ψ ω χ α π χ φ γ ω ο ι δ κ α ξ υ λ τ μ β α σ θ ε β σ δ γ ψ λ ω σ η ν θ Aι must-have for all stargazers η δ μ NEW EDITION! ζ λ β ε η κ NGC 6664 NGC 6539 ε τ μ NGC 6712 α υ δ ζ M26 ν NGC 6649 ψ Struve 2325 ζ ξ ATLAS χ α NGC 6604 ξ ο ν ν SCUTUM M16 of the γ SERP β NGC 6605 γ V450 ξ η υ η NGC 6645 M17 φ θ M18 ζ ρ ρ1 π Barnard 92 ο χ σ M25 M24 STARS M23 ν β κ All-in-one introduction ALL NEW MAPS WITH: to the night sky 42,000 more stars (87,000 plotted down to magnitude 8.5) AND 150+ more deep-sky objects (more than 1,200 total) The Eagle Nebula (M16) combines a dark nebula and a star cluster. In 100+ this intense region of star formation, “pillars” form at the boundaries spectacular between hot and cold gas. You’ll find this object on Map 14, a celestial portion of which lies above. photos PLUS: How to observe star clusters, nebulae, and galaxies AS2-CV0610.indd 1 6/10/10 4:17 PM NEW EDITION! AtlAs Tour the night sky of the The staff of Astronomy magazine decided to This atlas presents produce its first star atlas in 2006.
    [Show full text]
  • Completely Understand Before It Can Work Effectively for Not Only Himself but Also for the Membership
    EDITOR: Judy Butcher Send all articles to- (313) 254-1786 45200 Keding Apt. 102 Utica, MI 48087 The W.A.S.P. is the official publication of the Warren Astronomical Society and is available free to all club members. Requests by other clubs to receive the W.A.S.P. and all other correspondence should be addressed to the editor. Articles should be submitted at least one week prior to the general meeting. Warren Astronomical Society President: Frank McCullough 254-1786 P.O. Box 474 1st V.P.: Roger Tanner 981-0134 East Detroit, MI 48021 2nd V.P.: Ken Strom 977-9489 Secretary: Ken Kelly 839-7250 Treasurer: Bob Lennox 689-6139 Librarian: John Wetzel 882-6816 The Warren Astronomical Society is a local, non-profit organization of amateur astronomers. The Society holds meetings on the first and third Thursdays of each month. The meeting locations are as follows: 1st Thursday – Cranbrook Institute of Science 3rd Thursday – Macomb County Community 500 Lone Pine Road College – South Campus Bloomfield Hills, MI K Building (Student Activities), 14500 Twelve Mile Rd., Warren, MI Membership is open to those interested in astronomy and its related fields. Dues are as follows and include a year’s subscription to Sky and Telescope. Student ................... $21.00 College ........................ $25.00 Senior Citizen ................... $25.00 Individual ............... $30.00 Family......................... $35.00 Observatory Chairman: Ken Strom 977-9489 Stargate Observatory is owned and operated by the Warren Astronomical Society in conjunction with Rotary International. Located on the grounds of Camp Rotary, Stargate features a 12½” club-built Cassegrainian telescope under an aluminum dome.
    [Show full text]
  • Eagle Nebula Star Formation Region
    Eagle Nebula Star Formation Region AST 303: Chapter 17 1 The Formation of Stars (2) • A cloud of gas and dust must collapse if stars are to be formed. • The self-gravity of the cloud will tend to cause it to collapse. • Radiation pressure from nearby hot stars may do the same. • The passage of a shock wave from a nearby supernova blast or some other source (such as galactic shock waves) may do the same. – Note: The “sonic boom” of a jet plane is an example of a shock wave. • When two clouds collide, they may cause each other to collapse. AST 303: Chapter 17 2 Trifid Nebula AST 303: Chapter 17 3 Trifid Nebula Stellar Nursery Revealed AST 303: Chapter 17 4 Young Starburst Cluster Emerges from Cloud AST 303: Chapter 17 5 The Formation of Stars (3) • The gas in the collapsing cloud probably becomes turbulent. • This would tend to fragment the collapsing gas, producing condensations that would be the nuclei of new stars. • There is abundant evidence that shows that the stars in a cluster are all about the same age. For a young cluster, many stars have not yet reached the main sequence: ! Isochron Luminosity "Temperature AST 303: Chapter 17 6 The Formation of Stars (4) • The evolutionary paths of young stars on the H-R diagram look like this. Note the T Tauri stars, long thought to be young stars. • Theory says that these stars use convection as the main method of transporting energy to their surfaces. ! T Tauri Stars Luminosity "Temperature AST 303: Chapter 17 7 The Search for Stellar Precursors • Astronomers have long been fascinated by very dark, dense regions seen outlined against bright gas, called globules.
    [Show full text]
  • Desert Skies – October
    Desert Skies Tucson Amateur Astronomy Association Volume LIV, Number 10 October, 2008 Mount Lemmon SkyCenter Learn about: ♦ Progress on TIMPA Observatory ♦ The new electronic newsletter! ♦ TAAA Astronomy Complex Update ♦ Volunteer for School star parties ♦ Articles from our members ♦ Websites: Trips On The Internet ♦ Constellation of the month Super-Skyway Desert Skies: October, 2008 2 Volume LIV, Number 10 Cover Photos: Upper left: The 24-inch telescope is enclosed atop Mount Lemmon within the dome at the left. Lower left: A 24-inch telescope was installed in the newly remodeled dome at the Mount Lemmon Sky Center in April. Right: The 24-inch Mount Lemmon Sky- Center telescope is the one the public uses in programs offered through the UA's College of Science and Steward Observatory. All pho- tos by Adam Block. TAAA Web Page: http://www.tucsonastronomy.org TAAA Phone Number: (520) 792-6414 Office/Position Name Phone E-mail Address President Ken Shaver 762-5094 [email protected] Vice President Keith Schlottman 290-5883 [email protected] Secretary Luke Scott 749-4867 [email protected] Treasurer Terri Lappin 977-1290 [email protected] Member-at-Large George Barber 822-2392 [email protected] Member-at-Large John Kalas 620-6502 [email protected] Member-at-Large Teresa Plymate 883-9113 [email protected] Chief Observer Dr. Mary Turner 586-2244 [email protected] AL Correspondent (ALCor) Nick de Mesa 797-6614 [email protected] Astro-Imaging SIG Steve
    [Show full text]
  • Probing Physical Conditions in the Crab Nebula with Emission Line Analysis
    University of Kentucky UKnowledge Theses and Dissertations--Physics and Astronomy Physics and Astronomy 2016 PROBING PHYSICAL CONDITIONS IN THE CRAB NEBULA WITH EMISSION LINE ANALYSIS Xiang Wang University of Kentucky, [email protected] Digital Object Identifier: http://dx.doi.org/10.13023/ETD.2016.109 Right click to open a feedback form in a new tab to let us know how this document benefits ou.y Recommended Citation Wang, Xiang, "PROBING PHYSICAL CONDITIONS IN THE CRAB NEBULA WITH EMISSION LINE ANALYSIS" (2016). Theses and Dissertations--Physics and Astronomy. 36. https://uknowledge.uky.edu/physastron_etds/36 This Doctoral Dissertation is brought to you for free and open access by the Physics and Astronomy at UKnowledge. It has been accepted for inclusion in Theses and Dissertations--Physics and Astronomy by an authorized administrator of UKnowledge. For more information, please contact [email protected]. STUDENT AGREEMENT: I represent that my thesis or dissertation and abstract are my original work. Proper attribution has been given to all outside sources. I understand that I am solely responsible for obtaining any needed copyright permissions. I have obtained needed written permission statement(s) from the owner(s) of each third-party copyrighted matter to be included in my work, allowing electronic distribution (if such use is not permitted by the fair use doctrine) which will be submitted to UKnowledge as Additional File. I hereby grant to The University of Kentucky and its agents the irrevocable, non-exclusive, and royalty-free license to archive and make accessible my work in whole or in part in all forms of media, now or hereafter known.
    [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]
  • Universe Discovery Guides: December — Crab Nebula
    National Aeronautics and Space Administration UNIVERSE DISCOVERY GUIDES December CRAB NEBULA In this Hubble close-up of the Crab Nebula, various chemical elements have been detected in the expanding gas, including hydrogen (orange), nitrogen (red), sulfur (pink), and oxygen (green). Some of these elements are newly generated during the life and the explosive death of the star and now blasted back into space. These chemical elements will eventually be incorporated into new stars and planets. Credit: NASA, STScI/AURA More details: http://hubblesite.org/ newscenter/archive/releases/2000/15/ image/a/ The Crab Nebula: The remains of a star that exploded as a supernova about one thousand years ago. Credit: European Southern Observatory (ESO) IN THIS GUIDE » CHILDREN OF THE STARS » SKY FEATURE: CRAB NEBULA » TRY THIS! » ACTIVITY: A UNIVERSE WITHOUT SUPERNOVAE » CONNECT TO NASA SCIENCE » Acknowledgements » Appendix: December Star Map Published 2013. The universe is a place of change. NASA missions advance our understanding of the changing universe. www.nasa.gov 2 CHILDREN OF THE STARS Where did the calcium to build your bones come from? How about the iron in your blood or the oxygen in the air we breathe? You may have seen the table of the elements — these are the atoms which are the building blocks that make up everything we see, including us. Some of those atoms combine to make molecules, like water (consisting of hydrogen and oxygen) and sugars (consisting of carbon, hydrogen and oxygen) — ingredients for supporting life. The number of protons in the atom’s nucleus determine which element it is. For example, hydrogen has one proton; helium has two protons; carbon has six protons; iron has twenty-six protons.
    [Show full text]
  • MESSIER 15 RA(2000) : 21H 29M 58S DEC(2000): +12° 10'
    MESSIER 15 RA(2000) : 21h 29m 58s DEC(2000): +12° 10’ 01” BASIC INFORMATION OBJECT TYPE: Globular Cluster CONSTELLATION: Pegasus BEST VIEW: Late October DISCOVERY: Jean-Dominique Maraldi, 1746 DISTANCE: 33,600 ly DIAMETER: 175 ly APPARENT MAGNITUDE: +6.2 APPARENT DIMENSIONS: 18’ FOV:Starry 1.00Night FOV: 60.00 Vulpecula Sagitta Pegasus NGC 7009 (THE SATURN NEBULA) Delphinus NGC 7009 RA(2000) : 21h 04m 10.8s DEC(2000): -11° 21’ 48.6” Equuleus Pisces Aquila NGC 7009 FOV: 5.00 Aquarius Telrad Capricornus Sagittarius Cetus Piscis Austrinus NGC 7009 Microscopium BASIC INFORMATION OBJECT TYPE: Planetary Nebula CONSTELLATION: Aquarius Sculptor BEST VIEW: Early November DISCOVERY: William Herschel, 1782 DISTANCE: 2000 - 4000 ly DIAMETER: 0.4 - 0.8 ly Grus APPARENT MAGNITUDE: +8.0 APPARENT DIMENSIONS: 41” x 35” Telescopium Telrad Indus NGC 7662 (THE BLUE SNOWBALL) RA(2000) : 23h 25m 53.6s DEC(2000): +42° 32’ 06” BASIC INFORMATION OBJECT TYPE: Planetary Nebula CONSTELLATION: Andromeda BEST VIEW: Late November DISCOVERY: William Herschel, 1784 DISTANCE: 1800 – 6400 ly DIAMETER: 0.3 – 1.1 ly APPARENT MAGNITUDE: +8.6 APPARENT DIMENSIONS: 37” MESSIER 52 RA(2000) : 23h 24m 48s DEC(2000): +61° 35’ 36” BASIC INFORMATION OBJECT TYPE: Open Cluster CONSTELLATION: Cassiopeia BEST VIEW: December DISCOVERY: Charles Messier, 1774 DISTANCE: ~5000 ly DIAMETER: 19 ly APPARENT MAGNITUDE: +7.3 APPARENT DIMENSIONS: 13’ AGE: 50 million years FOV:Starry 1.00Night FOV: 60.00 Auriga Cepheus Andromeda MESSIER 31 (THE ANDROMEDA GALAXY) M 31 RA(2000) : 00h 42m 44.3Cassiopeias DEC(2000): +41° 16’ 07.5” Perseus Lacerta AndromedaM 31 FOV: 5.00 Telrad Triangulum Taurus Orion Aries Andromeda M 31 Pegasus Pisces BASIC INFORMATION OBJECT TYPE: Galaxy CONSTELLATION: Andromeda Telrad BEST VIEW: December DISCOVERY: Abd al-Rahman al-Sufi, 964 Eridanus CetusDISTANCE: 2.5 million ly DIAMETER: ~250,000 ly* APPARENT MAGNITUDE: +3.4 APPARENT DIMENSIONS: 178’ x 63’ (3° x 1°) *This value represents the total diameter of the disk, based on multi-wavelength measurements.
    [Show full text]
  • GTO Keypad Manual, V5.001
    ASTRO-PHYSICS GTO KEYPAD Version v5.xxx Please read the manual even if you are familiar with previous keypad versions Flash RAM Updates Keypad Java updates can be accomplished through the Internet. Check our web site www.astro-physics.com/software-updates/ November 11, 2020 ASTRO-PHYSICS KEYPAD MANUAL FOR MACH2GTO Version 5.xxx November 11, 2020 ABOUT THIS MANUAL 4 REQUIREMENTS 5 What Mount Control Box Do I Need? 5 Can I Upgrade My Present Keypad? 5 GTO KEYPAD 6 Layout and Buttons of the Keypad 6 Vacuum Fluorescent Display 6 N-S-E-W Directional Buttons 6 STOP Button 6 <PREV and NEXT> Buttons 7 Number Buttons 7 GOTO Button 7 ± Button 7 MENU / ESC Button 7 RECAL and NEXT> Buttons Pressed Simultaneously 7 ENT Button 7 Retractable Hanger 7 Keypad Protector 8 Keypad Care and Warranty 8 Warranty 8 Keypad Battery for 512K Memory Boards 8 Cleaning Red Keypad Display 8 Temperature Ratings 8 Environmental Recommendation 8 GETTING STARTED – DO THIS AT HOME, IF POSSIBLE 9 Set Up your Mount and Cable Connections 9 Gather Basic Information 9 Enter Your Location, Time and Date 9 Set Up Your Mount in the Field 10 Polar Alignment 10 Mach2GTO Daytime Alignment Routine 10 KEYPAD START UP SEQUENCE FOR NEW SETUPS OR SETUP IN NEW LOCATION 11 Assemble Your Mount 11 Startup Sequence 11 Location 11 Select Existing Location 11 Set Up New Location 11 Date and Time 12 Additional Information 12 KEYPAD START UP SEQUENCE FOR MOUNTS USED AT THE SAME LOCATION WITHOUT A COMPUTER 13 KEYPAD START UP SEQUENCE FOR COMPUTER CONTROLLED MOUNTS 14 1 OBJECTS MENU – HAVE SOME FUN!
    [Show full text]