559-1221 Partial Eclipse at Houge Park SJAA Activities Calendar

Total Page:16

File Type:pdf, Size:1020Kb

559-1221 Partial Eclipse at Houge Park SJAA Activities Calendar Partial Eclipse at Houge Park Bob Havner The June 10th eclipse at Houge Park was a huge success. The telescopes on telescope row were packed together as tight as possible. I don’t know if there was an exact count but I would guess at least 30 scopes were set up throughout the park. I want to thank everyone who brought out their equipment and a special thanks to Juanita Ryan and her 5th grade class who brought a ton of food and drinks to share with the observers. Quite a crowd gathered at Houge Park for the June 10 partial solar eclipse. Photo by Alex Crichton. — Bob Havner, [email protected] SJAA Activities Calendar Jim Van Nuland July 3 Deep-Sky weekend. Sunset 8:10 5-6 Glacier Point Star Parties. p.m., 24% moon rises 2:00 a.m. 6 Deep-Sky weekend. Sunset 8:28 10 Deep-Sky weekend. Sunset 8:04 p.m., 12% moon rises 3:26 a.m. p.m., 8% moon sets 9:48 p.m. 10-15 Shingletown Star Party 16 Houge Park star party. Sunset 13 Deep-Sky weekend. Sunset 8:27 7:58 p.m., 69% moon sets 1:19 p.m.,18% moon sets 11:16 p.m. a.m. 19 Houge Park star party. Sunset 17 ATM Class XIII — Houge Park, 8:21 p.m., 81% moon sets 2:36 7:30 p.m. a.m. 24 General Meeting: Juanita Ryan, Above: A family studies the solar projection from 20 ATM Class XI — Houge Park, Antarctica Meteor Trip the long focus heliograph provided by Dwight Elvey and Chris Angelos. Below is the objective 7:30 p.m. 29 ATM Class XIII — Houge Park, part of the heliograph, set up 115 feet away 27 General Meeting: Dr. Ken Lum, 7:30 p.m. from the projection screen. Photos by Alex Optical Designer Bernhard V. 30 Astronomy Class IX —Houge Crichton. Schmidt Park, 7:30 p.m. 30 Houge Park star party. Sunset August 7:39 p.m., 50% moon rises 11:54 1 ATM Class XII — Houge Park, a.m. 7:30 p.m. 31 Deep-Sky weekend. 2 Astronomy class VIII 2 Houge Park star party. Sunset September Meeting: Slide and 8:14 p.m., 33% moon rises 1:22 Equipment Night a.m. 24 Hour News and Information Hotline: (408) 559-1221 www.sjaa.net Copyright © 2002 San Jose Astronomical Association, Inc. Volume 13 Number 7 Official Publication of the San Jose Astronomical Association, July 2002 Mooning Things To Do Dave North I suppose a dedicated Loonie shouldn’t admit to such a thing, but sometimes the full Moon just isn’t all that interesting. Sure, you can do the “ray tracing” thang, and sometimes you’re picking up “good librations,” but even so such observations rarely take more than a half hour or so. What to do? This is a problem also faced by the Terminally Lunaphobic crowd (deepsky weasels), but we needn’t concern ourselves about their con- stant whining. I’m convinced the first thing you have to do in order to be a The main telescope field at this year’s RTMC, with its notable features, direct sun and dust. Photo proficient deepsky observer is learn to by the author. complain about every little thing, then use it as an excuse to stand around which is nowhere near Riverside. and a great opportunity to visit with and gossip. I think the idea originally involved many of the wonderful folks who make But the full Moon can be a great amateur builders showing off their up our hobby. time to travel, if you’re also interested craft, but increasingly this is less in Oh, there were a few commercial in things other than astronomy, but evidence, but boatloads of profes- innovations to check out this year. One who around here is? And what kind of sional builders show up — so the side of the telescope field seemed astronomy trip can you make at the full Telescope Makers part certainly literally littered with Coronado solar Moon? works. filters, and they are a great product. This May offered an interesting My personal favorite for this year opportunity: RTMC. And I’m sure many was the new Rigel Skylight/Starlight. SJAA members are curious about it, ... The full Moon can be a I’m sure you’ve seen these flashlights since it takes place on one of the worst great time to travel, if you’re in their original incarnation. The new travel weekends of the year, and is a version is completely redesigned, with long way to go. interested in things other a Great Big Knob for adjusting bright- At one time in the hazy past (a than astronomy. ness, very easily used with gloves on. couple of years ago) RTMC stood for Great stuff! It’s also water-resistant, Riverside Telescope Makers Confer- which is certainly useful in heavy dew ence. It takes place at Camp Oakes, And it is a Conference. or the middle of a lake (such as the which is just above Big Bear Lake, But now it’s called something Big Bear Lake solar observatory). else, I think RTMC Astronomy Expo — There were probably some and the RTMC doesn’t actually stand things I missed, but it seemed like not for anything officially any more. And it’s that much had happened in the incorporated or something. And it commercial world, and perhaps even costs a little more than it used to. less in the amateur world. Many great Otherwise, same old thing. scopes from previous RTMCs were You might think the major reason there, but not much that was both new to go is getting a look at all the cool and remarkable. At the height of the new telescopes various manufacturers event on Saturday afternoon, the are offering, and to see what amateurs telescope field where one usually sees are up to these days. And, to some new amateur work was nearly empty, extent, you’d be right. and there were also significant gaps in But the real point of going to the line of vendor booths. RTMC is to hang out with all the other Still, I’m told attendance was One of the many vendors at the 2002 RTMC folks from all over the country who Astronomy Expo. Photo by the author. attend: it’s a Gathering Of The Clans, Continued on next page SJAA EPHEMERIS Page 2 July 2002 Mooning at RTMC It gets everywhere. In your eyes, Alex Filippenko, ASP President, Continued from previous page ears, nose and throat. And in your University of California, Berkeley scope, if you take one — we never do Geoff Marcy, University of about normal, and there were about anymore (or leave it in the car). California, Berkeley the usual number of entries in the So that’s basically what RTMC is Chris McKay, NASA’s Ames telescope maker’s competition. all about. Give ‘em your 20 bucks and Research Center It may just be that they were hang out in a windy (often hot) David Morrison, NASA’s Ames spread out all over the place rather dustbowl. Research Center than in “the field,” as some folks claim. Or, more accurately, get in touch Jill Tarter, SETI Institute I can easily understand, how- with some of the nicest — and most Chris Impey, University of ever, why someone would avoid interesting — folks in the world. Arizona setting up there (or, for that matter, It’s the latter that brings us back, Ben Zuckerman, University of bringing any nice optics to RTMC). year after year. California, Los Angeles The dust. ps: The devoted Loonie also has Seth Shostak, SETI Institute There are three things you’ll a problem of what to do at new Moon. After the lectures, we will hold a probably remember about RTMC if In June, that was no problem. Just panel discussion. The panel will take you ever go there: all the great people, watch the eclipse! questions from the audience, and the the uncomfortable direct sun, and the Informally, hundreds of folks various speakers will debate issues dust. Definitely the dust. showed up at Houge Park, and it was discussed during their lectures. The entire area is covered wth a great fun. Especially since the day Seating is limited for the lecture series, fine grit, and tends to have winds was hot, and the eclipse gave us some so we encourage early registration. anywhere from a gentle zephyr (with cooling relief for a while. Admission for the lecture series occasional dust devils) to gale-force Plus, it was a rare opportunity to is: $35 general public, $30 ASP blows that topple scopes. And those look at the Dark Side Of The Moon. members, $25 students. winds carry some of the finest abra- Fun few weeks there! If you are an ASP member, we sives known to man. — Dave North, [email protected] invite you to attend our annual member’s meeting, which follows the panel discussion. Admission is free. If that’s not enough, from 7:00 to The ASP’s 2002 Annual Meeting 10:00 p.m. the ASP will be hosting a reception at the UC-Berkeley Faculty The Cosmic Thread: From Stars to Life Club, followed by a dinner banquet in Robert Naeye the Heyns Room. Award-winning author and journalist Timothy Ferris Is life widespread through the You Had to Design a Universe?” A free will speak at the banquet. Following cosmos, or is Earth a lonely oasis? public star party, sponsored by the Ferris’s talk, the ASP will present its The Astronomical Society of the San Francisco Amateur Astronomers 2002 Annual Awards, including the Pacific cordially invites you to learn (SFAA), follows Levy’s talk.
Recommended publications
  • ___... -.:: GEOCITIES.Ws
    __ __ _____ _____ _____ _____ ____ _ __ / / / / /_ _/ / ___/ /_ _/ / __ ) / _ \ | | / / / /__/ / / / ( ( / / / / / / / /_) / | |/ / / ___ / / / \ \ / / / / / / / _ _/ |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ersion 1.21 By K. Bradley Washburn "The Historian" ______________ | __ | | \| /\ / | | |/_/ / | | |\ \/\ / | | |_\/ \/ | |______________| K. Bradley Washburn HISTORY OF THE FUTURE Page 2 of 2 FOREWARD Relevant Notes WARNING: THIS FILE IS HAZARDOUS TO YOUR PRINTER'S INK SUPPLY!!! [*Story(Time Before:Time Transpired:Time After)] KEY TO ABBREVIATIONS AS--The Amazing Stories AST--Animated Star Trek B5--Babylon 5 BT--The Best of Trek DS9--Deep Space Nine EL--Enterprise Logs ENT--Enterprise LD--The Lives of Dax NE--New Earth NF--New Frontier RPG--Role-Playing Games S.C.E.--Starfleet Corps of Engineers SA--Starfleet Academy SNW--Strange New Worlds sQ--seaQuest ST--Star Trek TNG--The Next Generation TNV--The New Voyages V--Voyager WLB—Gateways: What Lay Beyond Blue italics - Completely canonical. Animated and live-action movies, episodes, and their novelizations. Green italics - Officially canonical. Novels, comics, and graphic novels. Red italics – Marginally canonical. Role-playing material, source books, internet sources. For more notes, see the AFTERWORD K. Bradley Washburn HISTORY OF THE FUTURE Page 3 of 3 TIMELINE circa 13.5 billion years ago * The Big Bang.
    [Show full text]
  • Arxiv:2010.13762V1 [Astro-Ph.EP] 26 Oct 2020
    Draft version October 27, 2020 Typeset using LATEX default style in AASTeX63 A Framework for Relative Biosignature Yields from Future Direct Imaging Missions Noah W. Tuchow 1 and Jason T. Wright 1 1Department of Astronomy & Astrophysics and Center for Exoplanets and Habitable Worlds and Penn State Extraterrestrial Intelligence Center 525 Davey Laboratory The Pennsylvania State University University Park, PA, 16802, USA ABSTRACT Future exoplanet direct imaging missions, such as HabEx and LUVOIR, will select target stars to maximize the number of Earth-like exoplanets that can have their atmospheric compositions charac- terized. Because one of these missions' aims is to detect biosignatures, they should also consider the expected biosignature yield of planets around these stars. In this work, we develop a method of computing relative biosignature yields among potential target stars, given a model of habitability and biosignature genesis, and using a star's habitability history. As an illustration and first application of this method, we use MESA stellar models to calculate the time evolution of the habitable zone, and examine three simple models for biosignature genesis to calculate the relative biosignature yield for different stars. We find that the relative merits of K stars versus F stars depend sensitively on model choice. In particular, use of the present-day habitable zone as a proxy for biosignature detectability favors young, luminous stars lacking the potential for long-term habitability. Biosignature yields are also sensitive to whether life can arise on Cold Start exoplanets that enter the habitable zone after formation, an open question deserving of more attention. Using the case study of biosignature yields calculated for θ Cygni and 55 Cancri, we find that robust mission design and target selection for HabEx and LUVOIR depends on: choosing a specific model of biosignature appearance with time; the terrestrial planet occurrence rate as a function of orbital separation; precise knowledge of stellar properties; and accurate stellar evolutionary histories.
    [Show full text]
  • Guidance Equations
    o Jo o z E (J t-u¡ l! LLO o l¡t l- GUIDANCE, NAVIGATION f AND CONTR t l-= vt Approved: .7/ "tu, /,f_t> G. M. LEVINE, DIREÇTO CE ANALYSIS APOLLO GUIDANCE AND NAVIGATION PROGRAM vl= - F Approvedr oate: ts Ü:l l- t2Z/ l¡t S.L PPS, SKYLARK MANAGER rrt APOLLO GUIDANCE AND NAVIGATION PROGRAM Ð T Approved Date: ,/1-orl7t (J R. H. BATT DEVELOPMENT APOLLO CE ATION PROGRAM rt) vt Approved: oate, / iZ)ci7 I D. G. HOAG, f APOLLO GUTDAN N TION PROGRAM Approved: ø,// Q, ,A-,-**- Date í ô.( R. R. RAGAN, #epurv DIREC{oR INSTRUMENTATION LABORATORY R- 693 GUIDANCE SYSTEM OPERATIONS PLAN FOR MANNED CSM EARTH ORB ITAL MISS IONS USING PROGRAM SKYLARK 1 SECTION 5 GUIDANCE EQUATIONS OCTOBER 19?1 Itl II. cHARrEs STAR,K DR.APER CAMBRIÓGE, MASSACHUSETTS, O2139 LABORATORY INOEXI¡{Ê DATA SIGTIATOR r0c T PCH sus,lfgf'i -ll ¡ r 4., DATE OPR L,, t&-w ,0-3f "11 ¡{ ¡f Ê-åE3 -æLW * Mtr { '-)¡:, ;tÍi't, f*ti')t'/.15'¿¡ ACKNOWLEDGEMENT This |eport was p|epared under DSR Project 55-23890, sponsored by the ìlanned Spacecraft Center of the National Aeronautics and Space Administration thlough Contlact NAS 9-4065. 'ì, 11 R- 693 GUIDANCE SYSTEM OPERATIONS PLAN FOR MANNED CM EARTH ORBITAL MISSIONS USING PROGRAM SKYLARK 1 SECTION 5 GUIDANCE EQUATIONS ) Signatures appearing on this page designate approval of this document by NASA/MSC. Approved Date: '2/ John R. Ga Section Chief, Guidance Program Section Manned Spacecraft Center, NASA Approved: f Date /a/ z ohn E. Williams, J Chief, Simulation and Flight Software Branch Manned Spacecraft Center, N ApproverJ: Date ,{r es C, Stokes, Jr.
    [Show full text]
  • Using Asteroseismology to Characterise Exoplanet Host Stars
    Using asteroseismology to characterise exoplanet host stars Mia S. Lundkvist, Daniel Huber, Victor Silva Aguirre, and William J. Chaplin Abstract The last decade has seen a revolution in the field of asteroseismology – the study of stellar pulsations. It has become a powerful method to precisely characterise exoplanet host stars, and as a consequence also the exoplanets themselves. This syn- ergy between asteroseismology and exoplanet science has flourished in large part due to space missions such as Kepler, which have provided high-quality data that can be used for both types of studies. Perhaps the primary contribution from aster- oseismology to the research on transiting exoplanets is the determination of very precise stellar radii that translate into precise planetary radii, but asteroseismology has also proven useful in constraining eccentricities of exoplanets as well as the dy- namical architecture of planetary systems. In this chapter, we introduce some basic principles of asteroseismology and review current synergies between the two fields. Mia S. Lundkvist Zentrum fur¨ Astronomie der Universitat¨ Heidelberg, Landessternwarte, Konigstuhl¨ 12, 69117 Hei- delberg, DE, and Stellar Astrophysics Centre, Aarhus University, Ny Munkegade 120, 8000 Aarhus C, DK, e-mail: [email protected] Daniel Huber Institute for Astronomy, University of Hawai‘i, 2680 Woodlawn Drive, Honolulu, HI 96822, US and Sydney Institute for Astronomy, School of Physics, University of Sydney, NSW 2006, Aus- tralia, e-mail: [email protected] Victor Silva Aguirre arXiv:1804.02214v2 [astro-ph.SR] 9 Apr 2018 Stellar Astrophysics Centre, Aarhus University, Ny Munkegade 120, 8000 Aarhus C, DK, e-mail: [email protected] William J.
    [Show full text]
  • Isabelle Boisse WORK EXPERIENCE EDUCATION MAIN
    Isabelle Boisse [email protected]; [email protected] date and place of birth: 28/06/1982, Talence (France) 65 rue des dames 75017 Paris, France +33 (0)6 28 32 33 78 38 rua da Fàbrica, Centro de Astrofìsica da Universidade do Porto apartamento 51/52, Porto, Portugal Rua das Estrelas, 4150-762 Porto, Portugal +351 925104420 +351 226 089 822 WORK EXPERIENCE Oct. 2010 - ... : Post-doctorat with N.C. Santos at the Centro de Astrofìsica da Universidade do Porto (CAUP), Porto, Portugal Sept. 2007- Sept. 2010 : PhD thesis : Doppler spectroscopy diagnostics for research and characterization of exoplanets with Pr. Bouchy F. and Pr. Hébrard G., at the Institut d’Astrophysique de Paris (IAP), Paris, France Teaching assistant (pratical work and tutorial) in physics to L1 and L2 students at University Pierre & Marie Curie, Paris, France, 64 hours/year (3 years) April - June 2007 : Research training period : Characterization of stellar activity and metallicity in the search for exoplanets with high-precision radial velocimetry with Pr. Bouchy F. and Pr. Hébrard G., IAP, Paris, France April - July 2006 : Research training period : Image processing of adaptive optics applied to the research of the Neptune’s arcs with Pr. Dumas C., ESO Santiago, Chile, and Pr. Sicardy B., LESIA, Observatoire de Meudon, France Oct. 2005 - Feb. 2006 : Teaching training period in a high school: Lycée Voltaire, Paris (weekly prepa- ration and instruction of physics classes to high school students) with M.Verdon May - June 2005 : Research training period : Looking for sources for UHECRs (Ultra high energy cos- mic rays) with Pr.
    [Show full text]
  • Pos(BASH2015)007
    Precision Stellar Astrophysics in the Kepler Era PoS(BASH2015)007 Daniel Huber∗ Sydney Institute for Astronomy, School of Physics, University of Sydney, NSW 2006, Australia E-mail: [email protected] The study of fundamental properties (such as temperatures, radii, masses, and ages) and interior processes (such as convection and angular momentum transport) of stars has implications on var- ious topics in astrophysics, ranging from the evolution of galaxies to understanding exoplanets. In this contribution I will review the basic principles of two key observational methods for con- straining fundamental and interior properties of single field stars: the study stellar oscillations (asteroseismology) and optical long-baseline interferometry. I will highlight recent breakthrough discoveries in asteroseismology such as the measurement of core rotation rates in red giants and the characterization of exoplanet systems. I will furthermore comment on the reliability of inter- ferometry as a tool to calibrate indirect methods to estimate fundamental properties, and present a new angular diameter measurement for the exoplanet host star HD 219134 which demonstrates that diameters for stars which are relatively well resolved (& 1 mas for the K band) are consistent across different instruments. Finally I will discuss the synergy between asteroseismology and interferometry to test asteroseismic scaling relations, and give a brief outlook on the expected impact of space-based missions such as K2, TESS and Gaia. Frank N. Bash Symposium 2015 18-20 October The University of Texas at Austin, USA ∗Speaker. c Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0).
    [Show full text]
  • Extrasolar Planets and Their Host Stars
    Kaspar von Braun & Tabetha S. Boyajian Extrasolar Planets and Their Host Stars July 25, 2017 arXiv:1707.07405v1 [astro-ph.EP] 24 Jul 2017 Springer Preface In astronomy or indeed any collaborative environment, it pays to figure out with whom one can work well. From existing projects or simply conversations, research ideas appear, are developed, take shape, sometimes take a detour into some un- expected directions, often need to be refocused, are sometimes divided up and/or distributed among collaborators, and are (hopefully) published. After a number of these cycles repeat, something bigger may be born, all of which one then tries to simultaneously fit into one’s head for what feels like a challenging amount of time. That was certainly the case a long time ago when writing a PhD dissertation. Since then, there have been postdoctoral fellowships and appointments, permanent and adjunct positions, and former, current, and future collaborators. And yet, con- versations spawn research ideas, which take many different turns and may divide up into a multitude of approaches or related or perhaps unrelated subjects. Again, one had better figure out with whom one likes to work. And again, in the process of writing this Brief, one needs create something bigger by focusing the relevant pieces of work into one (hopefully) coherent manuscript. It is an honor, a privi- lege, an amazing experience, and simply a lot of fun to be and have been working with all the people who have had an influence on our work and thereby on this book. To quote the late and great Jim Croce: ”If you dig it, do it.
    [Show full text]
  • Turn Left at Orion
    This page intentionally left blank Turn Left at Orion A hundred night sky objects to see in a small telescope — and how to find them Third edition Guy Consolmagno Vatican Observatory, Tucson Arizona and Vatican City State Dan M. Davis State University ofNew York at Stony Brook illustrations by Karen Kotash Sepp, Anne Drogin, and Mary Lynn Skirvin CAMBRIDGE UNIVERSITY PRESS Cambridge, New York, Melbourne, Madrid, Cape Town, Singapore, São Paulo Cambridge University Press The Edinburgh Building, Cambridge CB2 8RU, UK Published in the United States of America by Cambridge University Press, New York www.cambridge.org Information on this title: www.cambridge.org/9780521781909 © Cambridge University Press 1989, 1995, 2000 This publication is in copyright. Subject to statutory exception and to the provision of relevant collective licensing agreements, no reproduction of any part may take place without the written permission of Cambridge University Press. First published in print format 2000 ISBN-13 978-0-511-33717-8 eBook (EBL) ISBN-10 0-511-33717-5 eBook (EBL) ISBN-13 978-0-521-78190-9 hardback ISBN-10 0-521-78190-6 hardback Cambridge University Press has no responsibility for the persistence or accuracy of urls for external or third-party internet websites referred to in this publication, and does not guarantee that any content on such websites is, or will remain, accurate or appropriate. How Do You Get to Albireo? .............................4 How to Use This Book ....................................... 6 Contents The Moon ......................................................... 12 Lunar Eclipses Worldwide, 2004–2020 ........................... 23 The Planets ......................................................26 Approximate Positions of the Planets, 2004–2019.......... 28 When to See Mercury in the Evening Sky, 2004–2019 ...
    [Show full text]
  • Asteroseismology of Red Giant Stars
    1 Asteroseismology of red giant stars Rafael A. Garc´ıa1 & Dennis Stello2 1Laboratoire AIM, CEA/DSM – CNRS - Univ. Paris Diderot – IRFU/SAp, Centre de Saclay, 91191 Gif-sur-Yvette Cedex, France 2Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney, NSW 2006, Australia 1.1 Introduction If appropriately excited, a star will oscillate like a giant spherical instrument. In most stars, including the Sun, surface convection provides the excitation mechanism (Goldreich and Keeley, 1977). With turbulent velocities reaching speeds comparable to the local sound speed near the surface of the star, the vigorous convective motions can excite standing acoustic waves. These are known as pressure or p modes because the restoring force arises from the pressure gradient. The broad frequency spectrum of this excitation mechanism gives rise to many oscillation modes, both radial and non-radial, excited simultaneously. These stochastically excited and intrinsically damped oscillations were first detected in the Sun (Leighton et al., 1962), and hence are commonly known as solar-like oscillations. Oscillation modes can be characterised by the number of nodes, n, in the radial direction, called the radial order, and a non-radial part described by spherical harmonics, each with an angular degree, l, which equals the number of nodal lines on the surface, and an azimuthal order, m, which is the number of those nodal lines crossing the equator of the star. Except for the Sun, we can genrally not resolve these oscillations on the surfaces of cool stars and so the surface displacements of modes with high angular degree (l & 4) cannot be observed because regions of opposite phase tend to cancel out.
    [Show full text]
  • Precision Stellar Astrophysics in the Kepler Era Daniel Huber
    Precision Stellar Astrophysics in the Kepler Era Daniel Huber∗ Sydney Institute for Astronomy, School of Physics, University of Sydney, NSW 2006, Australia E-mail: [email protected] The study of fundamental properties (such as temperatures, radii, masses, and ages) and interior processes (such as convection and angular momentum transport) of stars has implications on var- ious topics in astrophysics, ranging from the evolution of galaxies to understanding exoplanets. In this contribution I will review the basic principles of two key observational methods for con- straining fundamental and interior properties of single field stars: the study stellar oscillations (asteroseismology) and optical long-baseline interferometry. I will highlight recent breakthrough discoveries in asteroseismology such as the measurement of core rotation rates in red giants and the characterization of exoplanet systems. I will furthermore comment on the reliability of inter- ferometry as a tool to calibrate indirect methods to estimate fundamental properties, and present a new angular diameter measurement for the exoplanet host star HD219134 which demonstrates that diameters for stars which are relatively well resolved (& 1mas for the K band) are consistent across different instruments. Finally I will discuss the synergy between asteroseismology and interferometry to test asteroseismic scaling relations, and give a brief outlook on the expected impact of space-based missions such as K2, TESS and Gaia. arXiv:1604.07442v1 [astro-ph.SR] 25 Apr 2016 Frank N. Bash Symposium 2015 18-20 October The University of Texas at Austin, USA ∗Speaker. c Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0).
    [Show full text]
  • Kuruluşundan Günümüze Istanbul Üniversitesi Fen Fakültesi Astronomi
    KURULUŞUNDAN GÜNÜMÜZE İSTANBUL ÜNİVERSİTESİ FEN FAKÜLTESİ ASTRONOMİ VE UZAY BİLİMLERİ BÖLÜMÜ 1933-2000 Prof.Dr. H.Hüseyin Menteşe Dr. Hasan H. Esenoğlu Doç.Dr. Hülya Çalõşkan İSTANBUL ARALIK 2002 İÇİNDEKİLER SUNUŞ.…......................................................................…….....….........................……………......…...iii ÖNSÖZ.…......................................................................…….....….........................…………….…........iv I. GİRİŞ.....…......................................................................…….....….................................1 II. İ.Ü. FEN FAKÜLTESİ ASTRONOMİ VE UZAY BİLİMLERİ BÖLÜMÜ’NÜN KISA TARİHÇESİ...……………..................................……….........4 II.1. 1933 Üniversite Reformu’ndan Günümüze Kadar İstanbul Üniversitesi Fen Fakültesi Astronomi ve Uzay Bilimleri Bölümü ve Astronomi..........……...........5 II.2. 1933–2000 Yõllarõ Arasõnda Astronomi ve Uzay Bilimleri Bölümü’nde Okutulan Astronomi Derslerinin Tarih Sõrasõna Göre Listesi…………………………..........20 II.3. 1933–2000 Yõllarõ Arasõnda Astronomi ve Uzay Bilimleri Bölümü’nde Okutulan Astronomi Derslerinin Ömür Süresine Göre Listesi……………………….....…....21 II.4. 1933–2000 Yõllarõ Arasõnda Astronomi ve Uzay Bilimleri Bölümü’nde Okutulan Astronomi Derslerinin Tarih Sõrasõna Göre Ayrõntõlõ Listesi.....……........….…....22 III. ASTRONOMİ VE UZAY BİLİMLERİ BÖLÜMÜ’NDE ÇALIŞANLARIN ÖZ GEÇMİŞLERİ...……....................................……………......28 IV. KURULUŞUNDAN GÜNÜMÜZE ASTRONOMİ VE UZAY BİLİMLERİ BÖLÜMÜ’NDE ÇALIŞMIŞ YERLİ VE YABANCI
    [Show full text]
  • November 28Th
    Io – November2014 p.1 IO - November 2014 Issue 2014-11 PO Box 7264 Eugene Astronomical Society Annual Club Dues $25 Springfield, OR 97475 President: Sam Pitts - 688-7330 www.eugeneastro.org Secretary: Jerry Oltion - 343-4758 Additional Board members: EAS is a proud member of: Jacob Strandlien, Tony Dandurand, John Loper. Next Meeting Thursday, November 20th What I Want For Christmas by Jerry Oltion, Mel Bartels, Jon Schwartz, and YOU Our November 20th meeting will be an opportunity to talk about equipment in an informal setting. Jerry, Mel, and Jon will lead the discussion, but everyone is encouraged to join in as we talk about what’s available for amateur astronomers today, what’s essential and what’s just a nice luxury. Have a favorite something you can’t do without? Bring it and tell us why you like it so much. If you’re thinking of buying new gear for Christmas, ei- ther for yourself or for someone else, now’s your chance to talk to people who might already have and use it. Learn whether it’s as good as advertised and find out if it’s what you really want. The meeting is at 7:00 on Thursday, November 20th at the Science Factory planetarium. Come early to visit before the program starts. Next First Quarter Friday: November 28th Our October 31st First Quarter Friday wasn’t exactly mobbed with costumed kids seeking the treat of photons older then they were, but on the other hand we did have mostly clear sky for a couple of hours and a dozen or so people to show the sights to.
    [Show full text]