The Comet's Tale
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Density Profiles of Populous Star Clusters in the Magellanic Clouds
Density profiles of populous star clusters in the Magellanic Clouds Grigor Nikolov,1,2 Anastasos Dapergolas,3 Mary Kontizas,2 Valeri Golev,1 Maya Belcheva2 1 Department of Astronomy, Faculty of Physics, Sofia University, BG-1164 Sofia, Bulgaria 2 Department of Astrophysics, Astronomy & Mechanics, Faculty of Physics, University of Athens, GR-15783 Athens, Greece 3 IAA, National Observatory of Athens, GR-11810 Athens, Greece [email protected] (Conference poster) Abstract. The Large Magellanic Cloud (LMC) and the Small Magellanic Cloud (SMC) provide the unique opportunity to study young and populous star clusters. Some of them are elliptical in shape, or are members of a multiple systems, which are almost absent in the Milky Way. We have selected a sample of Magellanic Clouds’ star clusters, some of them candidates of a multiple system components, to investigate them by means of their number density profiles. This approach allows us to determine the radial distribution of the stars of different magnitude. Since the brighter stars have larger masses than the fainter stars, the profiles can be used to trace mass-segregation in the clusters. We have fitted a theoretical model by Elson, Fall & Freeman [1987] to determine the core radius and the concentration of the stars for each magnitude range. Key words: star clusters Профили на плътността на населени звездни купове в Магелановите облаци Григор Николов, Анастасос Даперголас, Мери Контизас, Валери Голев, Мая Белчева Големият и Малкият Магеланови облаци предлагат уникалната възможност за изуча- ване на млади богато населени звездни купове. Някои от тях имат елиптична форма или са членове на двойни системи, каквито се срещат много рядко в Млечния път. -
Projekt Brána Do Vesmíru
Projekt Brána do vesmíru Hvězdárna Valašské Meziříčí, p. o. Krajská hvezdáreň v Žiline Súčasnosť a budúcnosť výskumu medziplanetárnej hmoty RNDr. Peter Vereš, PhD. University of Hawaii / Univerzita Komenského Ako sa objavila MPH ● Pôvodne iba nehybná hviezdna sféra ● Mesiac a Slnko ● Bludné planéty viditeľné voľným okom Starovek => novovek Piazzi ● 1.1.1801 ● Objekt pozorovaný 41 dní ● Stratený...predpoklad, medzi Marsom a Jupiterom ● Laplace – nemožné nájsť ● Gauss (24) vynašiel metódu, vypočítal, Ceres bol nájdený... Halley ● Kométy, odjakživa považované za poslov zlých správ, vysvetlené ako atmosferické javy ● ● ● ● Názov Kometes (dlhovlasá) ● 1577 Brahe = paralaxa, ďalej ako Mesiac ● Edmond Halley si všimol periodicitu kométy 1531, 1607, 1682 = návrat v 1758 Meteory ● Zaznamenané v -1809, - 687 (Lyridy) ● Ernst Chladni 1794 Kniha o pôvode Pallasovho železa ● 1798 Brandes, Benzenberg, paralaxa 400 meteorov, 22 spoločných ● 1803 dážď / Paríž, priznanie kozmického pôvodu ● 1833 USA dážď 20/s, LEO ● 1845/46 rozpad kométy Biela, dažde Andromedíd (72, 85, 93, 99) ● 1861 = Kirkwood, súvis rojov s kométami ● 1866 Schiaparelli: Swift-Tuttle (Perzeidy), Tempel (Leonidy) ● 1899 Adams vypočítal, že Jupiter narušil dráhu kométy, dážď nebol 1833, rytina, Leonidy 1998, foto, Leonidy, AGO Modra MPH a Slnečná sústava ● Slnko ● planéty (8) ● trpasličie planéty /Ceres, Pluto, Haumea, Makemake, Eris ● MPH = asteroidy, kométy, prach, plyn, .... Vznik a vývoj asteroidov ● -4571mil. rokov – vznik Sl. sús. ● Akrécia hmoty – nehomogenity, planetesimály, „viskózna -
Ice& Stone 2020
Ice & Stone 2020 WEEK 41: OCTOBER 4-10 Presented by The Earthrise Institute # 41 Authored by Alan Hale This week in history OCTOBER 4 5 6 7 8 9 10 OCTOBER 4, 2020: The main-belt asteroid (1679) Nevanlinna will occult the 7th-magnitude star HD 224945 in Pisces. The predicted path of the occultation crosses Newfoundland, part of the Maritime Provinces of Canada, the northeastern through the south-central U.S. (including Houston, Texas), north-central Mexico (including the northern regions of Monterrey, Nuevo Leon), and the southern Pacific Ocean. OCTOBER 4 5 6 7 8 9 10 OCTOBER 7, 2008: Twenty hours after its discovery by Richard Kowalski during the course of the Mount Lemmon Survey in Arizona, the tiny asteroid 2008 TC3 enters Earth’s atmosphere above Sudan, explodes, and drops meteorite fragments – the Almahata Sitta meteorite – on the Nubian Desert. This is the first instance of an impacting asteroid being discovered in space while still inbound to an impact, and it is the subject of this week’s “Special Topics” presentation. OCTOBER 7, 2009: Astronomers using the Infrared Telescope Facility in Hawaii announce that the surface of the large main-belt asteroid (24) Themis appears to be completely covered with water ice. The significance of this discovery is discussed in a previous “Special Topics” presentation. OCTOBER 4 5 6 7 8 9 10 OCTOBER 8, 1769: Comet Messier C/1769 P1 passes through perihelion at a heliocentric distance of 0.123 AU. This was the brightest comet discovered by the 18th-Century French comet hunter Charles Messier and is a previous “Comet of the Week.” OCTOBER 4 5 6 7 8 9 10 OCTOBER 9, 1933: A brief but strong “storm” of Draconid meteors is seen over Europe. -
NASA Ames Jim Arnold, Craig Burkhardt Et Al
The re-entry of artificial meteoroid WT1190F AIAA SciTech 2016 1/5/2016 2008 TC3 Impact October 7, 2008 Mohammad Odeh International Astronomical Center, Abu Dhabi Peter Jenniskens SETI Institute Asteroid Threat Assessment Project (ATAP) - NASA Ames Jim Arnold, Craig Burkhardt et al. Michael Aftosmis - NASA Ames 2 Darrel Robertson - NASA Ames Next TC3 Consortium http://impact.seti.org Mission Statement: Steve Larson (Catalina Sky Survey) “Be prepared for the next 2008 TC3 John Tonry (ATLAS) impact” José Luis Galache (Minor Planet Center) Focus on two aspects: Steve Chesley (NASA JPL) 1. Airborne observations of the reentry Alan Fitzsimmons (Queen’s Univ. Belfast) 2. Rapid recovery of meteorites Eileen Ryan (Magdalena Ridge Obs.) Franck Marchis (SETI Institute) Ron Dantowitz (Clay Center Observatory) Jay Grinstead (NASA Ames Res. Cent.) Peter Jenniskens (SETI Institute - POC) You? 5 NASA/JPL “Sentry” early alert October 3, 2015: WT1190F Davide Farnocchia (NASA/JPL) Catalina Sky Survey: Richard Kowalski Steve Chesley (NASA/JPL) Marco Michelli (ESA NEOO CC) 6 WT1190F Found: October 3, 2015: one more passage Oct. 24 Traced back to: 2013, 2012, 2011, …, 2009 Re-entry: Friday November 13, 2015 10.61 km/s 20.6º angle Bill Gray 11 IAC + UAE Space Agency chartered commercial G450 Mohammad Odeh (IAC, Abu Dhabi) Support: UAE Space Agency Dexter Southfield /Embry-Riddle AU 14 ESA/University Stuttgart 15 SETI Institute 16 Dexter Southfield team Time UAE Camera Trans-Lunar Insertion Stage Leading candidate (1/13/2016): LUNAR PROSPECTOR T.L.I.S. Launch: January 7, 1998 UT Lunar Prospector itself was deliberately crashed on Moon July 31, 1999 Carbon fiber composite Spin hull thrusters Titanium case holds Amonium Thiokol Perchlorate fuel and Star Stage 3700S HTPB binder (both contain H) P.I.: Alan Binder Scott Hubbard 57-minutes later: Mission Director Separation of TLIS NASA Ames http://impact.seti.org 30 . -
Ice& Stone 2020
Ice & Stone 2020 WEEK 33: AUGUST 9-15 Presented by The Earthrise Institute # 33 Authored by Alan Hale About Ice And Stone 2020 It is my pleasure to welcome all educators, students, topics include: main-belt asteroids, near-Earth asteroids, and anybody else who might be interested, to Ice and “Great Comets,” spacecraft visits (both past and Stone 2020. This is an educational package I have put future), meteorites, and “small bodies” in popular together to cover the so-called “small bodies” of the literature and music. solar system, which in general means asteroids and comets, although this also includes the small moons of Throughout 2020 there will be various comets that are the various planets as well as meteors, meteorites, and visible in our skies and various asteroids passing by Earth interplanetary dust. Although these objects may be -- some of which are already known, some of which “small” compared to the planets of our solar system, will be discovered “in the act” -- and there will also be they are nevertheless of high interest and importance various asteroids of the main asteroid belt that are visible for several reasons, including: as well as “occultations” of stars by various asteroids visible from certain locations on Earth’s surface. Ice a) they are believed to be the “leftovers” from the and Stone 2020 will make note of these occasions and formation of the solar system, so studying them provides appearances as they take place. The “Comet Resource valuable insights into our origins, including Earth and of Center” at the Earthrise web site contains information life on Earth, including ourselves; about the brighter comets that are visible in the sky at any given time and, for those who are interested, I will b) we have learned that this process isn’t over yet, and also occasionally share information about the goings-on that there are still objects out there that can impact in my life as I observe these comets. -
The Comet's Tale
THE COMET’S TALE Journal of the Comet Section of the British Astronomical Association Number 33, 2014 January Not the Comet of the Century 2013 R1 (Lovejoy) imaged by Damian Peach on 2013 December 24 using 106mm F5. STL-11k. LRGB. L: 7x2mins. RGB: 1x2mins. Today’s images of bright binocular comets rival drawings of Great Comets of the nineteenth century. Rather predictably the expected comet of the century Contents failed to materialise, however several of the other comets mentioned in the last issue, together with the Comet Section contacts 2 additional surprise shown above, put on good From the Director 2 appearances. 2011 L4 (PanSTARRS), 2012 F6 From the Secretary 3 (Lemmon), 2012 S1 (ISON) and 2013 R1 (Lovejoy) all Tales from the past 5 th became brighter than 6 magnitude and 2P/Encke, 2012 RAS meeting report 6 K5 (LINEAR), 2012 L2 (LINEAR), 2012 T5 (Bressi), Comet Section meeting report 9 2012 V2 (LINEAR), 2012 X1 (LINEAR), and 2013 V3 SPA meeting - Rob McNaught 13 (Nevski) were all binocular objects. Whether 2014 will Professional tales 14 bring such riches remains to be seen, but three comets The Legacy of Comet Hunters 16 are predicted to come within binocular range and we Project Alcock update 21 can hope for some new discoveries. We should get Review of observations 23 some spectacular close-up images of 67P/Churyumov- Prospects for 2014 44 Gerasimenko from the Rosetta spacecraft. BAA COMET SECTION NEWSLETTER 2 THE COMET’S TALE Comet Section contacts Director: Jonathan Shanklin, 11 City Road, CAMBRIDGE. CB1 1DP England. Phone: (+44) (0)1223 571250 (H) or (+44) (0)1223 221482 (W) Fax: (+44) (0)1223 221279 (W) E-Mail: [email protected] or [email protected] WWW page : http://www.ast.cam.ac.uk/~jds/ Assistant Director (Observations): Guy Hurst, 16 Westminster Close, Kempshott Rise, BASINGSTOKE, Hampshire. -
PYTS/ASTR 206 – Comets 1
PYTS/ASTR 206 – Comets 1 Announcements HW6 available today, due in a week Use Kevin as the TA for this one 2 In-class assignments left in 3 lectures PYTS/ASTR 206 – Comets 2 Comets PTYS/ASTR 206 – The Golden Age of Planetary Exploration Shane Byrne – [email protected] PYTS/ASTR 206 – Comets 3 In this lecture… Observations of comets What are comets? Composition and structure Cometary tails Ion and dust tails Where do comets come from? Orbits of comets Oort cloud Scattered Kuiper Belt PYTS/ASTR 206 – Comets 4 Observations of comets Comets have been known from ancient times Thought to foreshadow disasters and major battles Pre-telescopes the known solar system was a pretty empty place Moon and the Sun Mercury, Venus, Mars, Jupiter, Saturn And COMETS No Uranus No Neptune No planetary Moons (except ours) No Asteroids No Kuiper Belt Objects PYTS/ASTR 206 – Comets 5 People have recorded comet sightings for millennia 167 BC 687 AD 1986 AD PYTS/ASTR 206 – Comets 6 Ancient Greeks thought comets were atmospheric phenomena In the west this went unchallenged until telescopes came along Tycho Brahe’s parallax measurements proved this wrong Comets were much further away than the Moon Renaissance astronomers thought comets moved in straight lines through the solar system Even Kepler argued they shouldn’t follow elliptical orbits like the planets In the 1680s astronomers tracked a comet and showed it had an elliptical orbit Comets were solar system objects – just like planets PYTS/ASTR 206 – Comets 7 Newton finally -
THE GREAT CHRIST COMET CHRIST GREAT the an Absolutely Astonishing Triumph.” COLIN R
“I am simply in awe of this book. THE GREAT CHRIST COMET An absolutely astonishing triumph.” COLIN R. NICHOLL ERIC METAXAS, New York Times best-selling author, Bonhoeffer The Star of Bethlehem is one of the greatest mysteries in astronomy and in the Bible. What was it? How did it prompt the Magi to set out on a long journey to Judea? How did it lead them to Jesus? THE In this groundbreaking book, Colin R. Nicholl makes the compelling case that the Star of Bethlehem could only have been a great comet. Taking a fresh look at the biblical text and drawing on the latest astronomical research, this beautifully illustrated volume will introduce readers to the Bethlehem Star in all of its glory. GREAT “A stunning book. It is now the definitive “In every respect this volume is a remarkable treatment of the subject.” achievement. I regard it as the most important J. P. MORELAND, Distinguished Professor book ever published on the Star of Bethlehem.” of Philosophy, Biola University GARY W. KRONK, author, Cometography; consultant, American Meteor Society “Erudite, engrossing, and compelling.” DUNCAN STEEL, comet expert, Armagh “Nicholl brilliantly tackles a subject that has CHRIST Observatory; author, Marking Time been debated for centuries. You will not be able to put this book down!” “An amazing study. The depth and breadth LOUIE GIGLIO, Pastor, Passion City Church, of learning that Nicholl displays is prodigious Atlanta, Georgia and persuasive.” GORDON WENHAM, Adjunct Professor “The most comprehensive interdisciplinary of Old Testament, Trinity College, Bristol synthesis of biblical and astronomical data COMET yet produced. -
Three Decades of Small-Telescope Science
Three Decades of Small-Telescope Science A Report on the 2011 Society for Astronomical Sciences 30th Annual Sym- posium on Telescope Science Robert K. Buchheim For three decades, the Society for Astronomical Sciences has supported small telescope sci- ence, encouraged amateur research, and facilitated pro-am collaboration. On May 24-26, more than one hundred participants in the 30th anniversary SAS Symposium heard presentations cov- ering a wide range of astronomical topics, reaching from the laboratory to the distant cosmos. From Planets to Galaxies Sky & Telescope Editor-in-Chief Bob Naeye opened the technical session with a review of the amateur contributions to exoplanet discovery and research through monitoring of transits and micro-lensing events. R. Jay GaBany described his participation as an astro-imager in the search for evidence of galactic mergers. His exquisite deep images taken with his 24-inch telescope displayed the di- verse patterns of star streams that can be left behind when a dwarf galaxy is disrupted and ab- sorbed by a larger galaxy. He also noted that not all faint structures are evidence of galactic mergers: the faint ”loop” structure near M-81 is actually foreground “galactic cirrus” in our own Milky Way masquerading as a faux tidal loop. Education and Outreach Several papers related to education and outreach were presented. Debra Ceravolo applied her expertise in the generation and perception of colors, to describe a new method of merging narrow-band (e.g. Hα) and broad-band (e.g. RGB) images into a natural-color image that displays enhanced detail without glaring false colors. -
THE MAGELLANIC CLOUDS NEWSLETTER an Electronic Publication Dedicated to the Magellanic Clouds, and Astrophysical Phenomena Therein
THE MAGELLANIC CLOUDS NEWSLETTER An electronic publication dedicated to the Magellanic Clouds, and astrophysical phenomena therein No. 141 — 1 June 2016 http://www.astro.keele.ac.uk/MCnews Editor: Jacco van Loon Editorial Dear Colleagues, It is my pleasure to present you the 141st issue of the Magellanic Clouds Newsletter. There is a lot of interest in massive stars, star clusters, supernova remnants and binaries, but also several exciting new results about the large-scale structure of the Magellanic Clouds System. The next issue is planned to be distributed on the 1st of August 2016. Editorially Yours, Jacco van Loon 1 Refereed Journal Papers Non-radial pulsation in first overtone Cepheids of the Small Magellanic Cloud R. Smolec1 and M. Sniegowska´ 2 1Nicolaus Copernicus Astronomical Center, Warsaw, Poland 2Warsaw University Observatory, Warsaw, Poland We analyse photometry for 138 first overtone Cepheids from the Small Magellanic Cloud, in which Optical Gravitational Lensing Experiment team discovered additional variability with period shorter than first overtone period, and period ratios in the (0.60,0.65) range. In the Petersen diagram, these stars form three well-separated sequences. The additional variability cannot correspond to other radial mode. This form of pulsation is still puzzling. We find that amplitude of the additional variability is small, typically 2–4 per cent of the first overtone amplitude, which corresponds to 2–5 mmag. In some stars, we find simultaneously two close periodicities corresponding to two sequences in the Petersen diagram. The most important finding is the detection of power excess at half the frequency of the additional variability (at subharmonic) in 35 per cent of the analysed stars. -
Richard C. Hoagland - Summary Bibliography
Richard C. Hoagland - Summary Bibliography Search the database Advanced Search Not Logged In Log In Help Navigating Other Pages: Home Page ISFDB Wiki ISFDB FAQ Magazines Awards Recent Edits Recent Verifications Other Bibliographies For This Author: Summary Awards Alphabetical Chronological Editing Tools: Moderator Edit Author Data Make/Remove a Pseudonym Show All Titles Check for Duplicate Titles Add New Data: Add New Anthology Add New Chapterbook Add New Collection Add New Fanzine Add New Magazine Add New Nonfiction Add New Novel Add New Omnibus Policies: Disclaimer Privacy Policy Banner Art Credits License: This work is licensed under a Creative Commons License. Used These Alternate Names: Dick Hoagland Interviews: Interview: Richard Hoagland Biography: Bio:Richard C. Hoagland Bibliographic Comments: Author:Richard C. Hoagland Nonfiction The Monuments of Mars: A City on the Edge of Forever (1989) Dark Mission: The Secret History of NASA (2007) with Mike Bara Essay Series Science Fact (Analog) o Why We WON'T Find Life on Mars (1974) o Rendezvous in 1985 (1975) o Return to Mars: A Mission for the Enterprise (1977) o The Blivit in the B-Ring (Part 1 of 2) (1982) o The Blivit in the B-Ring (Part 2 of 2) (1983) o The Curious Case of the Humanoid Face ... On Mars (1986) (R)evolution o Torchships Now! (If, July-August 1974) (1974) with Robert D. Enzmann o Torchships Now! (If, September-October 1974) (1974) with Robert D. Enzmann o Following Yonder Star (1974) Essays Forum: Television: Never-Never Land and Clarke's Third Law (1974) [only as by Dick Hoagland ] The Origin of the Solar System (1977) with Ben Bova Space: The El Chichon Incident (1983) Richard C. -
Stellar Rotation the Missing Piece in Stellar Physics
Stellar rotation the missing piece in Stellar physics Collaborators: Richard de Grijs (MQ), Licai Deng (NAOC), Chengyuan Li (SYSU), Michael Albrow (UC), Petri Vaisanen (SAAO), Zara Randriamanakoto (SAAO) Weijia Sun (PKU) 07/14/2021 Why stellar rotation is important? Why stellar rotation is important? • Dynamo-driven magnetic activity • Stellar winds • Surface abundances • Chemical yields • Internal structure • External structure Why stellar rotation is important? • Dynamo-driven magnetic activity • Stellar winds • Surface abundances • Chemical yields • Internal structure • External structure Matt & Pudritz 2005 Why stellar rotation is important? • Dynamo-driven magnetic activity • Stellar winds • Surface abundances • Chemical yields • Internal structure • External structure Maeder & Meynet 2011 Why stellar rotation is important? • Dynamo-driven magnetic activity • Stellar winds • Surface abundances • Chemical yields • Internal structure • External structure Rivinius+2013 extended MSTO and split MS Found in Magellanic Clouds clusters rMS bMS NGC 1846 NGC 1856 1.5 Gyr 350 Myr Mackey et al. 2008 Milone et al. 2015 Not only in MC clusters Niederhofer et al. 2015 But also in Galactic OCs Pattern NGC 5822 0.9 Gyr Sun et al. 2019a Cordoni et al. 2018 What causes eMSTO and split MS? • Extended star formation history (eSFH) • Variability • A wide range of stellar rotations What causes eMSTO and split MS? Stellar rotation 300 0.0 250 Gravity darkening 0.5 1.0 200 (mag) 1.5 150 G M 2.0 100 2.5 50 pole-on (i = 0) 3.0 0.2 0.4 0.6 G G (mag) BP ° RP edge-on (i = 90) It’s mainly v sin i that affects the locus of a star in the CMD Georgy et al.