Conference Program August 10-12, 2011
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10. Scientific Programme 10.1
10. SCIENTIFIC PROGRAMME 10.1. OVERVIEW (a) Invited Discourses Plenary Hall B 18:00-19:30 ID1 “The Zoo of Galaxies” Karen Masters, University of Portsmouth, UK Monday, 20 August ID2 “Supernovae, the Accelerating Cosmos, and Dark Energy” Brian Schmidt, ANU, Australia Wednesday, 22 August ID3 “The Herschel View of Star Formation” Philippe André, CEA Saclay, France Wednesday, 29 August ID4 “Past, Present and Future of Chinese Astronomy” Cheng Fang, Nanjing University, China Nanjing Thursday, 30 August (b) Plenary Symposium Review Talks Plenary Hall B (B) 8:30-10:00 Or Rooms 309A+B (3) IAUS 288 Astrophysics from Antarctica John Storey (3) Mon. 20 IAUS 289 The Cosmic Distance Scale: Past, Present and Future Wendy Freedman (3) Mon. 27 IAUS 290 Probing General Relativity using Accreting Black Holes Andy Fabian (B) Wed. 22 IAUS 291 Pulsars are Cool – seriously Scott Ransom (3) Thu. 23 Magnetars: neutron stars with magnetic storms Nanda Rea (3) Thu. 23 Probing Gravitation with Pulsars Michael Kremer (3) Thu. 23 IAUS 292 From Gas to Stars over Cosmic Time Mordacai-Mark Mac Low (B) Tue. 21 IAUS 293 The Kepler Mission: NASA’s ExoEarth Census Natalie Batalha (3) Tue. 28 IAUS 294 The Origin and Evolution of Cosmic Magnetism Bryan Gaensler (B) Wed. 29 IAUS 295 Black Holes in Galaxies John Kormendy (B) Thu. 30 (c) Symposia - Week 1 IAUS 288 Astrophysics from Antartica IAUS 290 Accretion on all scales IAUS 291 Neutron Stars and Pulsars IAUS 292 Molecular gas, Dust, and Star Formation in Galaxies (d) Symposia –Week 2 IAUS 289 Advancing the Physics of Cosmic -
Proxima B: the Alien World Next Door - Is Anyone Home?
Proxima b: The Alien World Next Door - Is Anyone Home? Edward Guinan Biruni Observatory Dept. Astrophysics & Planetary Science th 40 Anniversary Workshop Villanova University 12 October, 2017 [email protected] Talking Points i. Planet Hunting: Exoplanets ii. Living with a Red Dwarf Program iii. Alpha Cen ABC -nearest Star System iv. Proxima Cen – the red dwarf star v. Proxima b Nearest Exoplanet vi. Can it support Life? vii. Planned Observations / Missions Planet Hunting: Finding Exoplanets A brief summary For citizen science projects: www.planethunters.org Early Thoughts on Extrasolar Planets and Life Thousands of years ago, Greek philosophers speculated… “There are infinite worlds both like and unlike this world of ours...We must believe that in all worlds there are living creatures and planets and other things we see in this world.” Epicurius c. 300 B.C First Planet Detected 51 Pegasi – November 1995 Mayer & Queloz / Marcy & Butler Credit: Charbonneau Many Exoplanets (400+) have been detected by the Spectroscopic Doppler Motion Technique (now can measure motions as low as 1 m/s (3.6 km/h = 2.3 mph)) Exoplanet Transit Eclipses Rp/Rs ~ [Depth of Eclipse] 1/2 Transit Eclipse Depths for Jupiter, Neptune and Earth for the Sun 0.01% (Earth-Sun) 0.15% (Neptune-Sun) 1.2% (Jupiter-Sun) Kepler Mission See: kepler.nasa.gov Has so far discovered 6000+ Confirmed & Candidate Exoplanets The Search for Planets Outside Our Solar System Exoplanet Census May 2017 Exoplanet Census (May-2017) Confirmed exoplanets: 3483+ (Doppler / Transit) 490+ Multi-planet Systems [April 2017] Exoplanet Candidates: 7900+ orbiting 2600+ stars (Mostly from the Kepler Mission) [May 2017] Other unconfirmed (mostly from CoRot)Exoplanets ~186+ Potentially Habitable Exoplanets: 51 (April 2017) Estimated Planets in the Galaxy ~ 50 -100 Billion! Most expected to be hosted by red dwarf stars Nomad (Free-floating planets) ~ 25 - 50 Billion Known planets with life: 1 so far. -
IAU Symp 269, POST MEETING REPORTS
IAU Symp 269, POST MEETING REPORTS C.Barbieri, University of Padua, Italy Content (i) a copy of the final scientific program, listing invited review speakers and session chairs; (ii) a list of participants, including their distribution on gender (iii) a list of recipients of IAU grants, stating amount, country, and gender; (iv) receipts signed by the recipients of IAU Grants (done); (v) a report to the IAU EC summarizing the scientific highlights of the meeting (1-2 pages). (vi) a form for "Women in Astronomy" statistics. (i) Final program Conference: Galileo's Medicean Moons: their Impact on 400 years of Discovery (IAU Symposium 269) Padova, Jan 6-9, 201 Program Wednesday 6, location: Centro San Gaetano, via Altinate 16.0 0 – 18.00 meeting of Scientific Committee (last details on the Symp 269; information on the IYA closing ceremony program) 18.00 – 20.00 welcome reception Thursday 7, morning: Aula Magna University 8:30 – late registrations 09.00 – 09.30 Welcome Addresses (Rector of University, President of COSPAR, Representative of ESA, President of IAU, Mayor of Padova, Barbieri) Session 1, The discovery of the Medicean Moons, the history, the influence on human sciences Chair: R. Williams Speaker Title 09.30 – 09.55 (1) G. Coyne Galileo's telescopic observations: the marvel and meaning of discovery 09.55 – 10.20 (2) D. Sobel Popular Perceptions of Galileo 10.20 – 10.45 (3) T. Owen The slow growth of human humility (read by Scott Bolton) 10.45 – 11.10 (4) G. Peruzzi A new Physics to support the Copernican system. Gleanings from Galileo's works 11.10 – 11.35 Coffee break Session 1b Chair: T. -
To Boldly Go? Interstellar Destinations: Nearby Potentially Habitable Worlds
To Boldly Go? Interstellar Destinations: Nearby Potentially Habitable Worlds AAPT Regional Meeting March 21, 2014 Edward Guinan Dept. Astrophysics & Planetary Science. With Scott Engle, Larry Dewarf & Gal Matijevic Students: Evan Kullberg, Allyn Durbin, Anna Marion, Connor Hause & Scott Michener Talking Points • Introduction: Finding Exoplanets & Planet Census • Living with a Red Dwarf Program: Summary • of Findings • • Nearby Stars and Exoplanetary Systems • The red dwarf / planetary system GJ 581 Habitable Planets? So far best choice. • To Boldly go? Interstellar Travel: Summary & Prospects Planet Hunting Finding Exoplanets very short summary For student projects: www.planethunters.org Many Exoplanets (400+) have been detected by the Spectroscopic Doppler Motion Technique (now can measure motions as low 1 m/s (3.6 km/h = 2.3 mph)) Reflex Radial Velocity Motion 20 of Sun Produced by Jupiter Typical 10 Error K 13 m/s 0 i = 90è -10 (orbit seen Radial Velocity (m/s) 11.86 yrs edge-on) -20 0 5 10 15 20 Time (Years) Semi-Amplitude, K, of 2pG ⅓ m sin i 1 _ K = p Radial Velocity induced P (M + m )⅔ √1 – e2 by a companion: * p Exoplanet Transit Eclipses Rp/Rs ~ [Depth of Eclipse] 1/2 Kepler Mission See: kepler.nasa.gov February 2014: Kepler Mission Discovers 715 New Planets (in multiple Planetary systems) Total confirmed Exoplanets: 1700 (Mar 2014) New Large Earth-size Planets discovered Around Nearby Red Dwarf Stars March 2014 Toumi et al. 2014 MNRAS Study indicates that 1/5 red dwarfs host Habitable planets Breaking News: March 2014 Habitable planets common around red dwarf stars (Toumi et al. -
1 Report on the 29Th International School for Young Astronomers
Report on the 29th International School for Young Astronomers (ISYA) Malaysia, 5 - 23 March 2007, Kuala Lumpur and Langkawi Island Prof. Dr. Mazlan Othman Chairman of National Committee on organizing ISYA2007 Mr. Mhd Fairos Asillam Science Officer in ANGKASA, Secretary of the National Committee on organizing ISYA2007 Dr. Michele Gerbaldi Chairperson for the ISYA programme (IAU) I – Introduction Dr. Mazlan Othman, Director General of the Malaysian National Space Agency (ANGKASA), sent a letter of intent, in February 2005 to the IAU Executive Committee offering to host the ISYA in 2007. The IAU Executive Committee selected Malaysia for the venue of the 29th ISYA between the 5th March and the 23rd March 2007. The IAU agreed to provide transportation to students and professors and Malaysia agreed to cover accommodation and catering expenses for the School, local transportation and facilities for education. This 29th ISYA was organised by the University Kebangsaan Malaysia (UKM) with the cooperation of the National Space Agency of Malaysia (ANGKASA), the Ministry of Science Technology and Innovation (MOSTI) and the University Malaya (UM). The School took place: ● at the University Kebangsaan Malaysia (UKM), Selangor - 5 to 9 March 2007 ● and then at the MARA Junior Science College, Langkawi Island where is located the National Observatory.- 10 to 23 March 2007. Objective: The objective of ISYA 2007 is as follows: i) To encourage the young scientist especially from the Asia Pacific region to get involved deeply in astronomy research and explore the future development of space science while building a strong network within the countries of this region; 1 ii) To train and expose the participants to the latest knowledge in the astronomical research arena; and iii) To present a unique opportunity for participants to have informal discussions among their peers and with recognised experts in the selected fields of research over a period of three weeks. -
Helium Burning of 22Ne: Targets, Detectors, and Initial Measurements
HELIUM BURNING OF 22NE: TARGETS, DETECTORS, AND INITIAL MEASUREMENTS Sean Hunt A dissertation submitted to the faculty of the University of North Carolina at Chapel Hill in partial fulfillment of the requirements for the degree of Doctor of Philosophy in the Department of Physics and Astronomy. Chapel Hill 2019 Approved by: Christian Iliadis Art Champagne Tom Clegg Richard Longland Fabian Heitsch c 2019 Sean Hunt ALL RIGHTS RESERVED ii ABSTRACT SEAN HUNT: Helium Burning of 22Ne: Targets, Detectors, and Initial Measurements. (Under the direction of Christian Iliadis) The goal of the work in this dissertation is to advance the understanding of nuclear astrophysics by remeasuring a reaction vital to the stellar synthesis of heavy elements. The 22Ne(↵,γ)26Mg and 22Ne(↵,n)25Mg reactions are of great importance to the s-process which takes place in asymptotic giant branch and massive stars, and produces half of all elements heavier than iron. The low energy resonances in these reactions have the greatest impact on the s-process, but have poorly understood resonance strengths. The ↵-particle beam necessary to measure the 22Ne(↵,n)25Mg and 22Ne(↵,γ)26Mg reac- tions are very damaging to solid targets. In this study, three types of targets made of glass, sintered metal, and evaporated metal were designed and fabricated. All three targets are capable of withstanding the effects of ↵-particle bombardment. Previous measurements of the 22Ne(↵,n)25Mg reaction saw significant contamination from the 13C(↵,n)16O reaction. A significant effort was made in this dissertation to de- velop new capture-gated detector technologies to differentiate between low energy neu- trons of interest and high energy contaminant neutrons. -
NL#121 August
AAS NEWSLETTER A Publication for the members of the American Astronomical Society August 2004 Issue 121 Inside 2 AAS Elections Preliminary Slate 4 2005 AAS Prize Nomination Form Left: Arlo with Wykescha Young, who has served as Arlo’s Administrative Secretary since 1999, 5 holding awards presented at the AAS Members Meeting in Denver. Right: Arlo received a framed print Climate Change Statement Report of meeting covers from 1995-2004 at the AAS Banquet in Denver. 6-7 2003 AAS ARLO PASSES THE QUILL Fiscal Report An important milestone was passed at the Denver meeting with the ending of Arlo Landolt’s unprecedented second nine-year stint as Secretary of the AAS. Arlo served 1980-1989 and again 1995- 2004. The AAS thanks and salutes Arlo for a total of eighteen years incumbency in this extremely important office. The AAS also appreciates the support provided by Louisiana State University which 14-15 Highlights hosted the Secretary’s office for each of his nine-year terms. from Denver Arlo is succeeded by John Graham of the Carnegie Institution’s Department of Terrestrial Magnetism, Washington, DC. 20 O’Keefe at Denver Meeting ASTRONOMY EDUCATION: GADGETS AND GIZMOS For the San Diego meeting, a room will be available for demonstrations of instructional technology in astronomy education. The facility will have power and high speed Internet at about twelve stations and will be open throughout the week to give everyone the opportunity for a hands-on experience. Suitable demonstrations would include interactive web tools (applets, immersive experiences, touch screens), instructional software, remote observing tools, audience response systems (or “clickers”), and wireless delivery of content to handheld devices or web phones. -
Cycle 11 Abstract Catalog
Cycle 11 Abstract catalog (based on Phase I submissions) Generated on: Mon Dec 10 08:39:48 EST 2001 ============================================================================= Proposal Category: GO Scientific Category: Quasar Absorption Lines and IGM ID: 9350 Title: Intergalactic HeII absorption in CSO 118 = HS 1157+3143 PI: Dieter Reimers PI Institution: Hamburger Sternwarte We propose to observe the HeII Gunn-Peterson effect in the z = 3 quasar CSO 118, which has been discovered in our SNAPSHOT survey to have a transparent line of sight. The aim is in particular to extend our knowledge about HeII reionization which has been observed to take place in the range z = 3.1 to z = 2.8. While existing and future FUSE observations will cover the redshift range z < 2.9, redshifts above 2.9 have been covered by HST with only 2 lines of sights. ================================================================================ Proposal Category: GO Scientific Category: Cosmology ID: 9351 Title: Determining Hubble's Constant from Observations of Cepheids in the Host Galaxy of SN Ia 1994ae PI: Adam Riess PI Institution: Space Telescope Science Institute We propose to determine the luminosity of the type Ia supernova (SN Ia) 1994ae by observing Cepheids in the host spiral galaxy NGC 3370. Modern CCD photometry has yielded an extremely tight Hubble diagram for SNe Ia with a precisely determined intercept (i.e., Delta H_0/H_0 ~ 1) measurement of the true Hubble constant is still limited by the calibration. The HST calibration of all but a few SNe Ia observed to date is significantly compromised by the systematics of photographic photometry and host galaxy extinction, as well as by the photometric uncertainties associated with WFPC2. -
100Th Anniversary Edition
Volume 40 Number 1 JAAVSO 2012 The Journal of the American Association of Variable Star Observers Part A of two parts pages 1–266 100th Anniversary Edition • History • Associations • Science • Review Papers 49 Bay State Road Cambridge, MA 02138 U. S. A. The Journal of the American Association of Variable Star Observers Editor Editorial Board John R. Percy Geoffrey C. Clayton Matthew R. Templeton University of Toronto Louisiana State University AAVSO Toronto, Ontario, Canada Baton Rouge, Louisiana Douglas L. Welch Associate Editor Edward F. Guinan McMaster University Elizabeth O. Waagen Villanova University Hamilton, Ontario, Canada Villanova, Pennsylvania Assistant Editor David B. Williams Matthew R. Templeton Pamela Kilmartin Whitestown, Indiana University of Canterbury Production Editor Christchurch, New Zealand Thomas R. Williams Michael Saladyga Houston, Texas Laszlo Kiss Konkoly Observatory Lee Anne Willson Budapest, Hungary Iowa State University Ames, Iowa Paula Szkody University of Washington Seattle, Washington The Council of the American Association of Variable Star Observers 2011–2012 Director Arne A. Henden President Mario E. Motta Past President Jaime R. García 1st Vice President Jennifer Sokoloski Secretary Gary Walker Treasurer Gary W. Billings (term ended May 2012) Treasurer Timothy Hager Councilors Edward F. Guinan John Martin Roger S. Kolman Donn R. Starkey Chryssa Kouveliotou Robert J. Stine Arlo U. Landolt David G. Turner ISSN 0271-9053 JAAVSO The Journal of The American Association of Variable Star Observers Volume 40 Number 1 2012 Part A of two parts: pages 1–266 100th Anniversary Edition History Associations Science Review Papers 49 Bay State Road Cambridge, MA 02138 ISSN 0271-9053 U. S. A.