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SEPTEMBER 2014 OT H E D Ebn V E R S E R V ESEPTEMBERR 2014
THE DENVER OBSERVER SEPTEMBER 2014 OT h e D eBn v e r S E R V ESEPTEMBERR 2014 FROM THE INSIDE LOOKING OUT Calendar Taken on July 25th in San Luis State Park near the Great Sand Dunes in Colorado, Jeff made this image of the Milky Way during an overnight camping stop on the way to Santa Fe, NM. It was taken with a Canon 2............................. First quarter moon 60D camera, an EFS 15-85 lens, using an iOptron SkyTracker. It is a single frame, with no stacking or dark/ 8.......................................... Full moon bias frames, at ISO 1600 for two minutes. Visible in this south-facing photograph is Sagittarius, and the 14............ Aldebaran 1.4˚ south of moon Dark Horse Nebula inside of the Milky Way. He processed the image in Adobe Lightroom. Image © Jeff Tropeano 15............................ Last quarter moon 22........................... Autumnal Equinox 24........................................ New moon Inside the Observer SEPTEMBER SKIES by Dennis Cochran ygnus the Swan dives onto center stage this other famous deep-sky object is the Veil Nebula, President’s Message....................... 2 C month, almost overhead. Leading the descent also known as the Cygnus Loop, a supernova rem- is the nose of the swan, the star known as nant so large that its separate arcs were known Society Directory.......................... 2 Albireo, a beautiful multi-colored double. One and named before it was found to be one wide Schedule of Events......................... 2 wonders if Albireo has any planets from which to wisp that came out of a single star. The Veil is see the pair up-close. -
Interstellar Extinction in the Direction of Young Open Star Clusters
ISSN (Online) 2393-8021 ISSN (Print) 2394-1588 IARJSET International Advanced Research Journal in Science, Engineering and Technology Vol. 6, Issue 5, May 2019 Interstellar Extinction in the Direction of Young Open Star Clusters Alok K. Durgapal* Center of Advanced Study, Department of Physics, D. S. B. Campus, Kumaun University Nainital, India Abstract: The total to selective extinction law in optical and near-IR wavelengths for twenty young open star clusters namely Berkeley 7, Collinder 69, Hogg 10, NGC 2362, Czernik 43, NGC 6530, NGC 6871, Bochum 10, Haffner 18, IC 4996, NGC 2384, NGC 6193, NGC 6618, NGC 7160, Collinder 232, Haffner 19, NGC 2401, NGC 6231, NGC 6823, NGC 7380 have been studied. It is found that fifteen clusters follow normal extinction law and five clusters show an anomalous behavior. Keywords: Star cluster: Reddening, interstellar dust- Interstellar extinction I. INTRODUCTION The interstellar dust which is remnant of star formation process can transmit and redirect the light of stars ([2]). As a result it becomes very difficult to determine accurate distances and magnitudes of astronomical objects ([11]); to overcome this difficulty we must have knowledge of composition of interstellar dust in every line of sight. The interstellar extinction is caused either by general interstellar medium (ISM) or by localized region of higher mean density ([9], [15]). Study of interstellar extinction provides information about components of the molecular cloud from which a star was formed. Young stars contain dust around them so young open star clusters are the ideal objects for extinction study ([5], [8], [10], [16], [17]). First started with Trumpler in 1920 and then many investigators studied extinction in the Galaxy. -
Photo of the Year by PAS Member Barry Simon Next PAS General
PAS-Times The newsletter of the Pontchartrain Astronomy Society January 2019 visit us online www.astronola.org Volume 60, Issue 1 Photo of the Year Next PAS General Meeting by PAS member Barry Simon Summer Milky Way with Friday, Jan. 19th,2019 at 7:30pm Dark Horse Nebula, UNO Science Bldg. Room 1001 Rho Ophiuchus Nebulosity, M4 and Antares PAS Times Volume 60, Issue 1 Page 2 President’s Message outreach for the public. We will try to PAS Officers for 2019 By: Bill Johnson address several basic skills for the beginners, and a few advanced topics for the our Greetings to all and welcome to 2019! seasoned members. If you have a topic you President: Happy New year to all the PAS members would like to see covered at one of our Bill Johnson and friends. meetings, or if you would like to present a [email protected] subject, please contact an officer and we will Yes, we are now in a New Year, with lots of do our best to address it for you. 1st Vice-President: promise for good things to come. New Year’s Mike Danielson resolutions may include losing weight, giving As a final request to start of the new year, Program Chairman up smoking, and a host of other bad habits I’m asking all members to commit to attending [email protected] that we all seem to have for one reason or one more event than you did last year. One another. My resolution is to get out just a more meeting, one more outreach, one more little more than last year and do some event. -
Young Stars in NGC 6231 and the Sco OB1 Association
Handbook of Star Forming Regions Vol. II Astronomical Society of the Pacific, c 2008 Bo Reipurth, ed. Young Stars in NGC 6231 and the Sco OB1 Association Bo Reipurth Institute for Astronomy, University of Hawaii 640 N. Aohoku Place, Hilo, HI 96720, USA Abstract. NGC 6231 is a young cluster in the southern sky, around 3-5 Myr old, located at a distance of about 1.6 kpc at the near side of the Sagittarius spiral arm. It forms the nucleus of the extended Sco OB1 association. The cluster is very rich, with more than 100 massive stars, among them 15 O-stars. Radial velocity studies have revealed a very large binary fraction among these OB stars. The young low- mass population has recently been identified using deep X-ray observations. Within the large HII region Gum 55 that surrounds NGC 6231 there exists a major elephant trunk, which shows evidence for recent second-generation star formation in the form of young B-stars surrounded by reflection nebulae and a number of low-mass Hα emission stars. 1. Introduction The open cluster NGC 6231 (also known as De Cheseaux No. 9, Lacaille II.13, Dun- lop 499, Melotte 153, and Collinder 315) in Scorpius was first discovered by Giovanni Battista Hodierna, who included it in his 1654 ”De systemate orbis cometici; deque admirandis coeli characteribus” [Of the systematics of the world of comets, and on the admirable objects of the sky]. Subsequently, NGC 6231 was independently discovered by Edmond Halley, who included it as one of three nebulous objects in his 1678 catalog of southern stars (Ashworth 1981). -
E. E. Barnard and His Dark Nebula!
Visible throughout our galaxy are clouds of interstellar matter, thin but widespread wisps of gas and dust. Some of the stars near nebulae are often very massive and their high-energy radiation can excite the gas of the nebula to shine; such nebula is called emission nebula. If the stars are dimmer or further away, their light is reflected by the dust in the nebula and can be seen as reflection nebula. Some nebulae are only visible by the absorption of the light from objects behind them. These are called dark nebula Edward Emerson Barnard was a professor of astronomy at the University of Chicago Yerkes Observatory. As a pioneer in astrophotography, he cataloged a series of dark nebula of the Milky Way. Through this work of studying the structure of the Milky Way, Barnard discovered that certain dark regions of our galaxy are actually clouds of gas and dust that obscured the more distant stars in the background. Today, we’re going to look-back on his life and accomplishments. We’ll also review several of my observations of his dark nebula. Barnard’s Early Years: A: Childhood, Work, and Stargazing Edward Emerson Barnard was born on December 16th, 1857 in Nashville Tennessee, at the cusp of the Civil War. His mother, Elizabeth, (at the age of 42), had moved the family from Cincinnati to Nashville a few months prior to Edward’s birth, when his father, Reuben Barnard had passed away. The family lived in near poverty, with Elizabeth as the sole provider working several small jobs, the most profitable being that of her making wax flowers, which she had a skill at creating. -
Watch This Space for July 2014
Watch this Space for July 2014 Planet Watch Moon Phases The Planets on view this month are: New Moon First Quarter Not visible this month 26 / 07 / 14 05 / 07 / 14 Mercury: Venus: At mag - 3.8 rises at 3am and is low in the Full Moon Last Quarter dawn twilight Mars: In Virgo at mag +0.4, sets around midnight 12 / 07 / 14 19 / 07 / 14 Jupiter: Not visible this month Saturn: In Libra at mag +0.6, sets around 1am The Sun Uranus: In Pisces at mag +5.8, rises around midnight Rises: 05:08, 15th July, Sets: 21:12 Neptune: In Aquarius at mag +7.8, rises around 11pm Constellation of the Month Ophiuchus — The Serpent Bearer 11th in size of the 88 constellations, Ophiuchus is a large but generally faint con- stellation. It is associated with the figure of Asclepius, the famous healer in Greek mythology, whose snake-entwined staff remains a symbol of medicine today. Notable stars: Oph - (Rasalhague) Brightest star in the constellation at mag 2.1. A very fast rotating star (89% of breakup speed) its equatorial radius is 20% larger than its polar radius, resulting in a polar temperature 2000K higher than at the equator. Barnard’s Star Mag 9.5 is the fourth closest star to our sun at 6 ly distance. It has the largest proper motion known at 10.3” per year and will be closest to the Sun at about 3.75l y by the year 9,800. Constellation map credit: Torsten Bronger Some Interesting Objects: Ophiuchus contains 39 NGC objects, including 22 globular clus- ters (7 of which are Messier objects) and 3 planetary nebulae. -
SAA 100 Club
S.A.A. 100 Observing Club Raleigh Astronomy Club Version 1.2 07-AUG-2005 Introduction Welcome to the S.A.A. 100 Observing Club! This list started on the USENET newsgroup sci.astro.amateur when someone asked about everyone’s favorite, non-Messier objects for medium sized telescopes (8-12”). The members of the group nominated objects and voted for their favorites. The top 100 objects, by number of votes, were collected and ranked into a list that was published. This list is a good next step for someone who has observed all the objects on the Messier list. Since it includes objects in both the Northern and Southern Hemispheres (DEC +72 to -72), the award has two different levels to accommodate those observers who aren't able to travel. The first level, the Silver SAA 100 award requires 88 objects (all visible from North Carolina). The Gold SAA 100 Award requires all 100 objects to be observed. One further note, many of these objects are on other observing lists, especially Patrick Moore's Caldwell list. For convenience, there is a table mapping various SAA100 objects with their Caldwell counterparts. This will facilitate observers who are working or have worked on these lists of objects. We hope you enjoy looking at all the great objects recommended by other avid astronomers! Rules In order to earn the Silver certificate for the program, the applicant must meet the following qualifications: 1. Be a member in good standing of the Raleigh Astronomy Club. 2. Observe 80 Silver observations. 3. Record the time and date of each observation. -
Small Wonders: Ophiuchus
Page 1 of 13 Small Wonders: Ophiuchus Small Wonders: Ophiuchus A monthly sky guide for the beginning to intermediate amateur astronomer Tom Trusock - 06/09 Barnard 72 (The Snake Nebula) - One of the many dark nebulae in Ophiuchus: Contributed by Hunter Wilson Tom Trusock June 2009 Page 2 of 13 Small Wonders: Ophiuchus This massive constellation culminates around midnight on June 12th and for me, has always been the harbinger of Summer. As with many constellations, it's mythology is somewhat mixed, but the most prevalent mythos is it's association with Aesculapius, surgeon aboard Jason's Argo. I've been an amateur astronomer for decades now, but I'm still awed by the sheer size of this constellation. Bordered on the north by Hercules and the south by Scorpius and Sagittarius, it reaches from +14 to just beneath -30 declination, and covers nearly three hours in right ascension and splits Serpens neatly in two. Widefield Finder Chart - Looking South, early June around 12pm. It's brightest star is 2nd magnitude Rasalhague located at the top of the constellations distinctive bell shape. The most interesting star within it's borders is probably the mag 9.5 red dwarf named Barnard's Star. Discovered in 1916 by E. E. Barnard, it's six light years away (making it the second closest star) and has a proper motion in our sky of one degree every 350 years. Barnard's star is approaching us rapidly – around 87 miles per second – and will reach closest approach of 3.8 light years around 8000 years from now. -
Caldwell Catalogue - Wikipedia, the Free Encyclopedia
Caldwell catalogue - Wikipedia, the free encyclopedia Log in / create account Article Discussion Read Edit View history Caldwell catalogue From Wikipedia, the free encyclopedia Main page Contents The Caldwell Catalogue is an astronomical catalog of 109 bright star clusters, nebulae, and galaxies for observation by amateur astronomers. The list was compiled Featured content by Sir Patrick Caldwell-Moore, better known as Patrick Moore, as a complement to the Messier Catalogue. Current events The Messier Catalogue is used frequently by amateur astronomers as a list of interesting deep-sky objects for observations, but Moore noted that the list did not include Random article many of the sky's brightest deep-sky objects, including the Hyades, the Double Cluster (NGC 869 and NGC 884), and NGC 253. Moreover, Moore observed that the Donate to Wikipedia Messier Catalogue, which was compiled based on observations in the Northern Hemisphere, excluded bright deep-sky objects visible in the Southern Hemisphere such [1][2] Interaction as Omega Centauri, Centaurus A, the Jewel Box, and 47 Tucanae. He quickly compiled a list of 109 objects (to match the number of objects in the Messier [3] Help Catalogue) and published it in Sky & Telescope in December 1995. About Wikipedia Since its publication, the catalogue has grown in popularity and usage within the amateur astronomical community. Small compilation errors in the original 1995 version Community portal of the list have since been corrected. Unusually, Moore used one of his surnames to name the list, and the catalogue adopts "C" numbers to rename objects with more Recent changes common designations.[4] Contact Wikipedia As stated above, the list was compiled from objects already identified by professional astronomers and commonly observed by amateur astronomers. -
Α. I. First Astronomer to Suggest That the Earth Is Not the Center of The
Α. i. first astronomer to suggest that the Earth is not the center of the Universe? [1] - 2 1.Galileo 2.Aristarchus 3.Copernicus 4.Cassini 5.Zhang Heng 6.al-Biruni 7.Kepler 8.Brahe 9.Aryabhatta ii. The obliquity of the ecliptic in degrees. (one decimal) [3] - 234 iii. The first known and brightest quasar is 3C__. [3] - 273 iv. A relativistic jet moves at 0.83c. If no Doppler shift is observed, how many degrees is the angle between the jet and the line of sight, assuming that the source has negligible velocity? (integer) [3] - 122 v. This nebula is NGC__. [4] – 7000 vi. Choose the names of the layers A, B and C of the Jovian atmosphere, beginning from Layer A. [3] - 195 1.Troposphere 2.Magnetosphere 3.Ionosphere 4.Ozone layer 5.Thermosphere 6.Lithosphere 7.Chromosphere 8.Photosphere 9. Stratosphere B. i. How many AU is one parsec? (integer) [6] - 206265 ii. Jupiter-Sun-Trojan Asteroids angle (degrees). (integer) [2] - 60 iii. This nebula is M__. [2] - 57 th o iv. On the 25 of August, at a latitude of φ>0 and longitude λL =37 W (time zone = GMT – 2hrs), we observe a star with Declination (δ) such that φ+δ=90, and Right Ascension α=67.5ο. What is the local civil time at the hh:mm during the lower culmination of the star? It is given that at 00:00hrs on the 24th of August, hour angle of vernal equinox is 21h 58m. [4] - 1857 v. During a Meteor Shower, in a radius of 100km, an observer counted 600 meteors/min. -
108 Afocal Procedure, 105 Age of Globular Clusters, 25, 28–29 O
Index Index Achromats, 70, 73, 79 Apochromats (APO), 70, Averted vision Adhafera, 44 73, 79 technique, 96, 98, Adobe Photoshop Aquarius, 43, 99 112 (software), 108 Aquila, 10, 36, 45, 65 Afocal procedure, 105 Arches cluster, 23 B1620-26, 37 Age Archinal, Brent, 63, 64, Barkhatova (Bar) of globular clusters, 89, 195 catalogue, 196 25, 28–29 Arcturus, 43 Barlow lens, 78–79, 110 of open clusters, Aricebo radio telescope, Barnard’s Galaxy, 49 15–16 33 Basel (Bas) catalogue, 196 of star complexes, 41 Aries, 45 Bayer classification of stellar associations, Arp 2, 51 system, 93 39, 41–42 Arp catalogue, 197 Be16, 63 of the universe, 28 Arp-Madore (AM)-1, 33 Beehive Cluster, 13, 60, Aldebaran, 43 Arp-Madore (AM)-2, 148 Alessi, 22, 61 48, 65 Bergeron 1, 22 Alessi catalogue, 196 Arp-Madore (AM) Bergeron, J., 22 Algenubi, 44 catalogue, 197 Berkeley 11, 124f, 125 Algieba, 44 Asterisms, 43–45, Berkeley 17, 15 Algol (Demon Star), 65, 94 Berkeley 19, 130 21 Astronomy (magazine), Berkeley 29, 18 Alnilam, 5–6 89 Berkeley 42, 171–173 Alnitak, 5–6 Astronomy Now Berkeley (Be) catalogue, Alpha Centauri, 25 (magazine), 89 196 Alpha Orionis, 93 Astrophotography, 94, Beta Pictoris, 42 Alpha Persei, 40 101, 102–103 Beta Piscium, 44 Altair, 44 Astroplanner (software), Betelgeuse, 93 Alterf, 44 90 Big Bang, 5, 29 Altitude-Azimuth Astro-Snap (software), Big Dipper, 19, 43 (Alt-Az) mount, 107 Binary millisecond 75–76 AstroStack (software), pulsars, 30 Andromeda Galaxy, 36, 108 Binary stars, 8, 52 39, 41, 48, 52, 61 AstroVideo (software), in globular clusters, ANR 1947 -
High-Mass Binaries in the Very Young Open Cluster NGC 6231
A&A 368, 122–136 (2001) Astronomy DOI: 10.1051/0004-6361:20000528 & c ESO 2001 Astrophysics High-mass binaries in the very young open cluster NGC 6231 Implication for cluster and star formation B. Garc´ıa1,?,?? and J. C. Mermilliod2 1 CRICyT- Centro Regional de Investigaciones Cient´ıficas y T´ecnicas, CC 131-5500 Mendoza, Argentina 2 Institut d’Astronomie de l’Universit´e de Lausanne, 1290 Chavannes-des-Bois, Switzerland Received 3 October 2000 / Accepted 20 December 2000 Abstract. New radial-velocity observations of 37 O- and B stars in the very young open cluster NGC 6231 confirm the high frequency of short-period spectroscopic binaries on the upper main sequence. Among the 14 O-type stars, covering all luminosity classes from dwarfs to supergiants, 8 are definitively double-lined systems and all periods but one are shorter than 7 days. Several additional binaries have been detected among the early B-type stars. NGC 6231 is an exceptional cluster to constrain the scenarios of cluster- and binary-star formation over a large range of stellar masses. We discuss the evidences, based on NGC 6231 and 21 other clusters, with a total of 120 O-type stars, for a clear dichotomy in the multiplicity rate and structure of very young open clusters containing O-type stars in function of the number of massive stars. However, we cannot answer the question whether the observed characteristics result from the formation processes or from the early dynamical evolution. Key words. galaxies: open clusters and associations: NGC 6231 – stars: binaries: spectroscopic – stars: early-type – stars: rotation 1.