Mar 2016 Newsletter
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
The Skyscraper 2009 04.Indd
A Better Galaxy Guide: Early Spring M67: One of the most ancient open clusters known and Craig Cortis is a great novelty in this regard. Located 1.7° due W of mag NGC 2419: 3.25° SE of mag 6.2 66 Aurigae. Hard to find 4.3 Alpha Cancri. and see; at E end of short row of two mag 7.5 stars. Highly NGC 2775: Located 3.7° ENE of mag 3.1 Zeta Hydrae. significant and worth the effort —may be approximately (Look for “Head of Hydra” first.) 300,000 light years distant and qualify as an extragalactic NGC 2903: Easily found at 1.5° due S of mag 4.3 Lambda cluster. Named the Intergalactic Wanderer. Leonis. NGC 2683: Marks NW “crook” of coathanger-type triangle M95: One of three bright galaxies forming a compact with easy double star mag 4.2 Iota Cancri (which is SSW by triangle, along with M96 and M105. All three can be seen 4.8°) and mag 3.1 Alpha Lyncis (at 6° to the ENE). together in a low power, wide field view. M105 is at the NE tip of triangle, midway between stars 52 and 53 Leonis, mag Object Type R.A. Dec. Mag. Size 5.5 and 5.3 respectively —M95 is at W tip. Lynx NGC 3521: Located 0.5° due E of mag 6.0 62 Leonis. M65: One of a pair of bright galaxies that can be seen in NGC 2419 GC 07h 38.1m +38° 53’ 10.3 4.2’ a wide field view along with M66, which lies just E. -
April 14 2018 7:00Pm at the April 2018 Herrett Center for Arts & Science College of Southern Idaho
Snake River Skies The Newsletter of the Magic Valley Astronomical Society www.mvastro.org Membership Meeting President’s Message Tim Frazier Saturday, April 14th 2018 April 2018 7:00pm at the Herrett Center for Arts & Science College of Southern Idaho. It really is beginning to feel like spring. The weather is more moderate and there will be, hopefully, clearer skies. (I write this with some trepidation as I don’t want to jinx Public Star Party Follows at the it in a manner similar to buying new equipment will ensure at least two weeks of Centennial Observatory cloudy weather.) Along with the season comes some great spring viewing. Leo is high overhead in the early evening with its compliment of galaxies as is Coma Club Officers Berenices and Virgo with that dense cluster of extragalactic objects. Tim Frazier, President One of my first forays into the Coma-Virgo cluster was in the early 1960’s with my [email protected] new 4 ¼ inch f/10 reflector and my first star chart, the epoch 1960 version of Norton’s Star Atlas. I figured from the maps I couldn’t miss seeing something since Robert Mayer, Vice President there were so many so closely packed. That became the real problem as they all [email protected] appeared as fuzzy spots and the maps were not detailed enough to distinguish one galaxy from another. I still have that atlas as it was a precious Christmas gift from Gary Leavitt, Secretary my grandparents but now I use better maps, larger scopes and GOTO to make sure [email protected] it is M84 or M86. -
The Fixed Stars Report Frederic Chopin
The Fixed Stars Report by Tara Cochrane for Frederic Chopin March 1, 1810 6:00 PM Warsaw, Poland Calculated for: Local Mean Time, Time Zone 0 hours West Latitude: 52 N 15 Longitude: 21 E 00 Your Company Name 1234 N. Your Address City, State 123456 Phone: 1-555-555-5555 [email protected] Introduction Report and Text Copyright 2009 Cosmic Patterns Software, Inc. The contents of this report are protected by Copyright law. By purchasing this report you agree to comply with this Copyright. This report interprets conjunctions of nearly every fixed star that has been given an astrological name to the planets, Asc, MC, 7th house cusp, and 4th cusp. Each interpretation given in this report is based on extensive research on the historical astrological meanings and myths associated with the fixed stars. A list of notable people who have the same conjunction aspect as you do is also given. This comprehensive analysis of the influence of the fixed stars combined with a list of notable people who also have this aspect provides you with extensive information, and hopefully astrologers who use this report can use this information to develop an even more refined and clearer understanding of the meaning of every fixed stars. Interpretations of the Fixed Stars Moon conjunct Dheneb, Orb: 0 deg 55 min Bold, willful, courageous, combative, astute, focused and unyielding characteristics may be indicated. Ascension to a position of leadership and renown is possible. There may be a great deal of personal charisma and emotional intensity, as well as an inclination towards obsession. -
Double and Multiple Star Measurements in the Northern Sky with a 10” Newtonian and a Fast CCD Camera in 2006 Through 2009
Vol. 6 No. 3 July 1, 2010 Journal of Double Star Observations Page 180 Double and Multiple Star Measurements in the Northern Sky with a 10” Newtonian and a Fast CCD Camera in 2006 through 2009 Rainer Anton Altenholz/Kiel, Germany e-mail: rainer.anton”at”ki.comcity.de Abstract: Using a 10” Newtonian and a fast CCD camera, recordings of double and multiple stars were made at high frame rates with a notebook computer. From superpositions of “lucky images”, measurements of 139 systems were obtained and compared with literature data. B/w and color images of some noteworthy systems are also presented. mented double stars, as will be described in the next Introduction section. Generally, I used a red filter to cope with By using the technique of “lucky imaging”, seeing chromatic aberration of the Barlow lens, as well as to effects can strongly be reduced, and not only the reso- reduce the atmospheric spectrum. For systems with lution of a given telescope can be pushed to its limits, pronounced color contrast, I also made recordings but also the accuracy of position measurements can be with near-IR, green and blue filters in order to pro- better than this by about one order of magnitude. This duce composite images. This setup was the same as I has already been demonstrated in earlier papers in used with telescopes under the southern sky, and as I this journal [1-3]. Standard deviations of separation have described previously [1-3]. Exposure times varied measurements of less than +/- 0.05 msec were rou- between 0.5 msec and 100 msec, depending on the tinely obtained with telescopes of 40 or 50 cm aper- star brightness, and on the seeing. -
Korotangi (The Dove)
Korotangi (The Dove) The legend of the korotangi is that it came in the Tainui waka as one of the heirlooms which had been blessed by the high priests in Hawaiiki and which in the new country, would ensure good hunting for the tribe. It was said that the Kawhia and Waikato tribes, who descended from Tainui stock, took the korotangi into battle with them, setting it up on a hill and consulting it as an oracle. The "korotangi" can mean "to roar and rush as the sound of water" in either Maori, Hawaiian or Samoan has been used to support the legend that it was bought on the Tainui waka from afar. The expression “Korotangi” is still used as a term of endearment, or as a simile for any object treasured or loved. A mother lamenting the death of a child will, in her lament, refer to her lost one as her “Korotangi.” 1 No doubt the simile has its origin in the above tradition, which also seems to be a fea- sible explanation of the waiata. It certainly explains the reference to the eat- ing of the pohata leaves and the huahua from Rotorua, as well as the allu- sion to the taumata (hill-top or ridge). The Korotangi, Tawhio Throne, and the art work depicting The Lost Child TeManawa and Korotangi, arrived at Turangawaewae Marae on the same day. The Heart of Heaven is in part the sharing of the walk of TeManawa who lives these things, has fulfilled prophesy. Her journey has been documented since 1992 to current. -
AYOSH Demo Chapter
DEMO CHAPTER Winter - January We start the year of Star Hopping at its beginning, in chilly January. By this point, I was 14 episodes into the Star Hopping series on YouTube, which was started in September. So that’s why we’re starting with Episode 14. We’ll roll over to Episode 1, nine months from now; in September. The months of Winter give rise to the brightest stars in the sky, anchored in the constellations of Orion, Canis Major, Canis Minor, and Gemini. In the northern climes, the weather may be frigid, but on those cold, clear nights, the stars shine more steadily, as the cold dry air makes for spectacular “seeing”. Chapter 4 - Leo We’ll be looking into the constellation of Leo for our Star Hopping targets in this chapter. I’ll be keeping you up a little later to around 11:30 PM, to see Leo the Lion appearing up over the eastern horizon. Even though we’re in January, we are A YEAR OF STAR HOPPING DAVID HEARN PAGE !1 OF !7 DEMO CHAPTER starting to get hints of the constellations of Spring starting to appear late in the evenings. This begins the time to see galaxies! The constellation of Leo portrays the great Lion, with the head of the lion appearing as a very recognizable backwards question mark, and the tail shaped like a large triangle. Leo rises with the head of the lion facing straight up, and within it’s borders lie many deep sky objects, most of which are as I mentioned, galaxies. -
The Electric Sun Hypothesis
Basics of astrophysics revisited. II. Mass- luminosity- rotation relation for F, A, B, O and WR class stars Edgars Alksnis [email protected] Small volume statistics show, that luminosity of bright stars is proportional to their angular momentums of rotation when certain relation between stellar mass and stellar rotation speed is reached. Cause should be outside of standard stellar model. Concept allows strengthen hypotheses of 1) fast rotation of Wolf-Rayet stars and 2) low mass central black hole of the Milky Way. Keywords: mass-luminosity relation, stellar rotation, Wolf-Rayet stars, stellar angular momentum, Sagittarius A* mass, Sagittarius A* luminosity. In previous work (Alksnis, 2017) we have shown, that in slow rotating stars stellar luminosity is proportional to spin angular momentum of the star. This allows us to see, that there in fact are no stars outside of “main sequence” within stellar classes G, K and M. METHOD We have analyzed possible connection between stellar luminosity and stellar angular momentum in samples of most known F, A, B, O and WR class stars (tables 1-5). Stellar equatorial rotation speed (vsini) was used as main parameter of stellar rotation when possible. Several diverse data for one star were averaged. Zero stellar rotation speed was considered as an error and corresponding star has been not included in sample. RESULTS 2 F class star Relative Relative Luminosity, Relative M*R *eq mass, M radius, L rotation, L R eq HATP-6 1.29 1.46 3.55 2.950 2.28 α UMi B 1.39 1.38 3.90 38.573 26.18 Alpha Fornacis 1.33 -
Adrian Zielonka's December 2020 Astronomy and Space News
Astronomy News Night Sky 2020 - December Sunrise Sunset Mercury Venus Rises 1st – 7:53am 1st – 4:07pm 1st – 5:19am 10th – 8:04am 10th – 4:04pm Not Visible 10th – 5:46am 20th – 8:12am 20th – 4:06pm this month. 20th – 6:16am 30th – 8:15am 30th – 4:13pm 30th – 6:43am Moon Rise Moon Set Moon Rise Moon Set - - - - - - - 1st – 8:54am 20th – 12:16pm (ESE) 20th – 10:46pm 1st – 4:52pm 2nd – 9:56am 21st – 12:33pm 21st – 11:55pm 2nd – 5:36pm 3rd – 10:50am 22nd – 12:48pm (E) 23rd – 1:02am (W) 3rd – 6:31pm 4th – 11:35am 23rd – 1:03pm 24th – 2:09am 4th – 7:37pm 5th – 12:10pm 24th – 1:18pm 25th – 3:16am 5th – 8:50pm 6th – 12:38pm 25th – 1:35pm (ENE) 26th – 4:24am (WNW) 6th – 10:07pm (ENE) 7th – 1:01pm (WNW) 26th – 1:55pm 27th – 5:33am 7th – 11:26pm 8th – 1:21pm 27th – 2:19pm 28th – 6:41am 9th – 12:46am 9th – 1:39pm (W) 28th – 2:50pm 29th – 7:46am 10th – 2:08am (E) 10th – 1:58pm 29th – 3:31pm 30th – 8:44am 11th – 3:32am 11th – 2:18pm 30th – 4:23pm 31st – 9:33am 12th – 4:58am (ESE) 12th – 2:42pm (WSW) 31st – 5:27pm - - - - - - - 13th – 6:26am 13th – 3:13pm - - - - - - - Moon Phases 14th – 7:51am 14th – 3:53pm All times Last Quarter – 8th 15th – 9:07am 15th – 4:45pm in notes are set New Moon – 14th 16th – 10:09am 16th – 5:50pm for First Quarter – 21st 17th – 10:56am 17th – 7:03pm Somerton Full Moon – 30th 18th – 11:30am 18th – 8:19pm unless stated 19th – 11:56am +4.5 19th – 9:34pm (WSW) A useful site: www.heavens- A S Zielonka above.com There is a planned launch (no earlier than December) of SpaceX CRS-21 Cargo mission to the International Space Station (ISS). -
CALENDARIO ASTRONOMICO Per L'anno
CALENDARIO ASTRONOMICO per l’anno 2015 (Anno Internazionale della Luce) con tabelle di Cronologia comparata con i Calendari Ortodosso, Copto, Israelita, Musulmano e Cinese Elaborato da LUCIANO UGOLINI Astrofilo di PRATO (Toscana) Componente dell’ASSOCIAZIONE ASTRONOMICA QUASAR presso CENTRO DI SCIENZE NATURALI di GALCETI – PRATO La pubblicazione di questo Calendario è stata curata dal C.A.A.T. - Coordinamento delle Associazioni Astrofile della Toscana – www.astrocaat.it – [email protected] Il C.A.A.T. è: ollaoazioe ta gli astofili tosai, attività ossevativa, poozioe dell’astooia aatoiale ella osta egioe, incontri e seminari di aggiornamento, sesiilizzazioe sul polea dell’iuiaeto luioso. Differenza ET-UT adottata per l’ao 15 = +68 secondi. Gli orari delle congiunzioni fra Luna, Pianeti e Stelle e la loro separazione angolare, si riferiscono all’istate della loro iia distanza e sono indicati per il centro della Terra. Gli orari del sorgere, culminare e tramontare del Sole e della Luna soo espressi per l’orizzote astrooico di Prato Piazza del Coue - Latitudine: ° ’ 8” Nord - Logitudie: ° ’ ” Est da Greewich). Le correzioni da apportare unicamente agli istanti del sorgere, culminare e tramontare degli astri, rispetto a quelle indicate, per altre città della Toscana, sono minime e riconducibili, al massimo, a pochi minuti in più o in meno. Gli altri orari idicati el presete Caledario o ecessitao di alcua correzioe e valgoo per tutta l’Italia. Tutti i tepi soo espressi i T.M.E.C. Tepo Medio dell’Europa Cetrale che è il Tepo Civile segato dai ostri orologi. Non viene tenuto conto dell’aueto di iuti dovuto all’ora estiva, attualete i vigore i Italia dall’ultia Doeica di Marzo all’ultia Doeica di Ottobre. -
Double Star Astronomy: Orbital & Dynamic Elements
double star astronomy: orbital & dynamic elements https://www.handprint.com/ASTRO/bineye3.html Double Star Astronomy Part 4: Orbital & Dynamic Elements Gravitational Dynamics Building a Binary Orbit Kepler's "Laws" Newton's Mechanics Double Star Orbital Elements The Dynamical Equations Diagramming a Double Star Relative Orbit The Solar Standard Formulas Historically, the orbital motions of double stars provided the first evidence that Newton's description of gravitational attraction and the laws of motion (in the Principia mathematica, 1687) applied not just to the planets and periodic comets of the solar system but equally to the celestial motions of the stars around each other and around the Galaxy. The 19th century analysis of the orbits of a small number of nearby, short period binary stars, many of them eclipsing variable and spectroscopic stars, revealed the variety of stellar masses and dimensions, which laid the foundation for theories of stellar structure and evolution. I first present the classical view of Kepler and Newton, then how to "build" a binary star from mass, orbital radius and orbital energy. The orbital elements are defined and illustrated in the graphical construction of the relative orbit and the method used to recreate the inclination. Gravitational Dynamics Kepler's Laws. The effects of gravity within the solar system were first presented in the Epitome of Copernican Astronomy, Books IV & V (1621) by Johannes Kepler. By analyzing measurements of the motion of Mars made by Tycho Brahe, Kepler deduced his three principles of planetary motion (diagram, below): First Law. The orbit of every planet is an ellipse with the Sun at one of the two focal points of the ellipse. -
June 2021 BRAS Newsletter
A JPL Image of surface of Mars, and JPL Ingenuity Helicioptor illustration. Monthly Meeting June 14th at 7:00 PM, in person at last!!! (Monthly meetings are on 2nd Mondays at Highland Road Park Observatory) You can also join this meeting via meet.jit.si/BRASMeet PRESENTATION: a demonstration on how to clean the optics of an SCT or refracting telescope. What's In This Issue? President’s Message Member Meeting Minutes Business Meeting Minutes Outreach Report Asteroid and Comet News Light Pollution Committee Report Globe at Night SubReddit and Discord BRAS Member Astrophotos Messages from the HRPO REMOTE DISCUSSION American Radio Relay League Field Day Observing Notes: Coma Berenices – Berenices Hair Like this newsletter? See PAST ISSUES online back to 2009 Visit us on Facebook – Baton Rouge Astronomical Society BRAS YouTube Channel Baton Rouge Astronomical Society Newsletter, Night Visions Page 2 of 23 June 2021 President’s Message Spring is just flying by it seems. Already June, galaxy season is peeking and the nebulous treasures closer to the Milky Way are starting to creep into the late evening sky. And as a final signal of Spring, we have a variety of life creeping up at the observatory on Highland Road (and not just the ample wildlife that’s been pushed out of the bayou by the rising flood waters, either). Astronomy Day was pretty big success (a much larger crowd than showed up last spring, at any rate) and making good on the ancient prophecy, we began having meetings at HRPO once again. Thanks again to Melanie for helping us score such a fantastic speaker for our homecoming, too. -
O Personenregister
O Personenregister A alle Zeichnungen von Sylvia Gerlach Abbe, Ernst (1840 – 1904) 100, 109 Ahnert, Paul Oswald (1897 – 1989) 624, 808 Airy, George Biddell (1801 – 1892) 1587 Aitken, Robert Grant (1864 – 1951) 1245, 1578 Alfvén, Hannes Olof Gösta (1908 – 1995) 716 Allen, James Alfred Van (1914 – 2006) 69, 714 Altenhoff, Wilhelm J. 421 Anderson, G. 1578 Antoniadi, Eugène Michel (1870 – 1944) 62 Antoniadis, John 1118 Aravamudan, S. 1578 Arend, Sylvain Julien Victor (1902 – 1992) 887 Argelander, Friedrich Wilhelm August (1799 – 1875) 1534, 1575 Aristarch von Samos (um −310 bis −230) 627, 951, 1536 Aristoteles (−383 bis −321) 1536 Augustus, Kaiser (−62 bis 14) 667 Abbildung O.1 Austin, Rodney R. D. 907 Friedrich W. Argelander B Baade, Wilhelm Heinrich Walter (1893 – 1960) 632, 994, 1001, 1535 Babcock, Horace Welcome (1912 – 2003) 395 Bahtinov, Pavel 186 Baier, G. 408 Baillaud, René (1885 – 1977) 1578 Ballauer, Jay R. (*1968) 1613 Ball, Sir Robert Stawell (1840 – 1913) 1578 Balmer, Johann Jokob (1825 – 1898) 701 Abbildung O.2 Bappu, Manali Kallat Vainu (1927 – 1982) 635 Aristoteles Barlow, Peter (1776 – 1862) 112, 114, 1538 Bartels, Julius (1899 – 1964) 715 Bath, KarlLudwig 104 Bayer, Johann (1572 – 1625) 1575 Becker, Wilhelm (1907 – 1996) 606 Bekenstein, Jacob David (*1947) 679, 1421 Belopolski, Aristarch Apollonowitsch (1854 – 1934) 1534 Benzenberg, Johann Friedrich (1777 – 1846) 910, 1536 Bergh, Sidney van den (*1929) 1166, 1576, 1578 Bertone, Gianfranco 1423 Bessel, Friedrich Wilhelm (1784 – 1846) 628, 630, 1534 Bethe, Hans Albrecht (1906 – 2005) 994, 1010, 1535 Binnewies, Stefan (*1960) 1613 Blandford, Roger David (*1949) 723, 727 Blazhko, Sergei Nikolajewitsch (1870 – 1956) 1293 Blome, HansJoachim 1523 Bobrovnikoff, Nicholas T.