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Ames Faces Great Challenges . . . and Great Opportunities
National Aeronautics and Space Administration, Ames Research Center, Moffett Field, CA February 2005 Ames faces great challenges . and great opportunities As NASA undergoes a major trans- To assist this, Ames has established are astrobiology (the study of the origin, formation and field center budgets get a New Business Office headed by Wendy evolution and distribution of life in the tighter, Ames faces both “a great chal- Dolci. Hubbard said the New Business universe), integrated next generation Office will man- computing systems; intelligent/adap- age all potential tive systems; entry, descent and landing new business as systems (with the Jet Propulsion Labo- though it were a ratory and NASA Langley Research corporate sales Center); and air traffic management sys- portfolio, and tems. Four of the five core competencies will regularly are exclusive to Ames. track and report Hubbard said that the approval of on potential new Ames’ core competencies places the cen- business oppor- ter “in the critical path” for implement- NASA photo by Tom Trower tunities. In addi- ing the agency’s priorities, particularly tion, he said that The Vision for Space Exploration. Em- managers will be phasizing the importance of maintain- required to visit ing a strong, viable work environment, key customers at Hubbard said Ames will conduct a least once a “health assessment” of its core compe- month, and that tencies by the end of March. project principal To deal with a substantially reduced investigators, “core” center budget, Hubbard an- branch chiefs or nounced a “belt-tightening” action plan Ames Center Director G. Scott Hubbard “whoever has ac- for Ames to prevent the loss of as many countability for a as 400 civil servants and 400 contractor lenge and a great opportunity” as it given product” will also be responsible jobs in a worst-case scenario. -
Hubble Space Telescope Observer’S Guide Winter 2021
HUBBLE SPACE TELESCOPE OBSERVER’S GUIDE WINTER 2021 In 2021, the Hubble Space Telescope will celebrate 31 years in operation as a powerful observatory probing the astrophysics of the cosmos from Solar system studies to the high-redshift universe. The high-resolution imaging capability of HST spanning the IR, optical, and UV, coupled with spectroscopic capability will remain invaluable through the middle of the upcoming decade. HST coupled with JWST will enable new innovative science and be will be key for multi-messenger investigations. Key Science Threads • Properties of the huge variety of exo-planetary systems: compositions and inventories, compositions and characteristics of their planets • Probing the stellar and galactic evolution across the universe: pushing closer to the beginning of galaxy formation and preparing for coordinated JWST observations • Exploring clues as to the nature of dark energy ACS SBC absolute re-calibration (Cycle 27) reveals 30% greater • Probing the effect of dark matter on the evolution sensitivity than previously understood. More information at of galaxies http://www.stsci.edu/contents/news/acs-stans/acs-stan- • Quantifying the types and astrophysics of black holes october-2019 of over 7 orders of magnitude in size WFC3 offers high resolution imaging in many bands ranging from • Tracing the distribution of chemicals of life in 2000 to 17000 Angstroms, as well as spectroscopic capability in the universe the near ultraviolet and infrared. Many different modes are available for high precision photometry, astrometry, spectroscopy, mapping • Investigating phenomena and possible sites for and more. robotic and human exploration within our Solar System COS COS2025 initiative retains full science capability of COS/FUV out to 2025 (http://www.stsci.edu/hst/cos/cos2025). -
Chapter 8.Pdf
CHAeTER 8 INFLUENCE OF PULSARS ON SUPERNOVAE In recent years there has been a great deal of effort to understand in detail the observed light curves of type I1 supernovae. In the standard approach, the observed light curve is to be understood in terms of an initial deposition of thermal energy by the blast wave; and a more gradual input of thermal energy due to radioactive decay of iron-peak elements is invoked to explain the behaviour at later times. The consensus is that the light curves produced by these models are in satisfactory agreement with those observed. In this chapter we discuss the characteristics of the expected light curve, if in addition to the abovementioned sources of energy, there is a continued energy input from an active central pulsar. We argue that in those rare cases when the energy loss rate of the pulsar is comparable to the luminosity of the supernova near light maximum, the light curve will be characterized by an extended plateau phase. The essential reason for this is that the pulsar luminosity is expected to decline over timescales which are much longer than the timescale of, say, radioactive decay. The light curve of the recent supernova in the Large Magellanic Cloud is suggestive of continued energy input from an active pulsar. A detection of strong W,X -ray and 1-ray plerion after the ejecta becomes optically thin will be a clear evidence of the pulsar having powered the light curve. CONTENTS CHAPTER 8 INFLUENCE OF PULSARS ON SUPERNOVAE 8.1 INTRODUCTION ................... 8-1 8.2 EARLIER WORK .................. -
THE 1000 BRIGHTEST HIPASS GALAXIES: H I PROPERTIES B
The Astronomical Journal, 128:16–46, 2004 July A # 2004. The American Astronomical Society. All rights reserved. Printed in U.S.A. THE 1000 BRIGHTEST HIPASS GALAXIES: H i PROPERTIES B. S. Koribalski,1 L. Staveley-Smith,1 V. A. Kilborn,1, 2 S. D. Ryder,3 R. C. Kraan-Korteweg,4 E. V. Ryan-Weber,1, 5 R. D. Ekers,1 H. Jerjen,6 P. A. Henning,7 M. E. Putman,8 M. A. Zwaan,5, 9 W. J. G. de Blok,1,10 M. R. Calabretta,1 M. J. Disney,10 R. F. Minchin,10 R. Bhathal,11 P. J. Boyce,10 M. J. Drinkwater,12 K. C. Freeman,6 B. K. Gibson,2 A. J. Green,13 R. F. Haynes,1 S. Juraszek,13 M. J. Kesteven,1 P. M. Knezek,14 S. Mader,1 M. Marquarding,1 M. Meyer,5 J. R. Mould,15 T. Oosterloo,16 J. O’Brien,1,6 R. M. Price,7 E. M. Sadler,13 A. Schro¨der,17 I. M. Stewart,17 F. Stootman,11 M. Waugh,1, 5 B. E. Warren,1, 6 R. L. Webster,5 and A. E. Wright1 Received 2002 October 30; accepted 2004 April 7 ABSTRACT We present the HIPASS Bright Galaxy Catalog (BGC), which contains the 1000 H i brightest galaxies in the southern sky as obtained from the H i Parkes All-Sky Survey (HIPASS). The selection of the brightest sources is basedontheirHi peak flux density (Speak k116 mJy) as measured from the spatially integrated HIPASS spectrum. 7 ; 10 The derived H i masses range from 10 to 4 10 M . -
+ New Horizons
Media Contacts NASA Headquarters Policy/Program Management Dwayne Brown New Horizons Nuclear Safety (202) 358-1726 [email protected] The Johns Hopkins University Mission Management Applied Physics Laboratory Spacecraft Operations Michael Buckley (240) 228-7536 or (443) 778-7536 [email protected] Southwest Research Institute Principal Investigator Institution Maria Martinez (210) 522-3305 [email protected] NASA Kennedy Space Center Launch Operations George Diller (321) 867-2468 [email protected] Lockheed Martin Space Systems Launch Vehicle Julie Andrews (321) 853-1567 [email protected] International Launch Services Launch Vehicle Fran Slimmer (571) 633-7462 [email protected] NEW HORIZONS Table of Contents Media Services Information ................................................................................................ 2 Quick Facts .............................................................................................................................. 3 Pluto at a Glance ...................................................................................................................... 5 Why Pluto and the Kuiper Belt? The Science of New Horizons ............................... 7 NASA’s New Frontiers Program ........................................................................................14 The Spacecraft ........................................................................................................................15 Science Payload ...............................................................................................................16 -
Chapter 2 Spatially Resolved Spitzer Spectroscopy of the Starburst Nucleus in NGC 5253
Interstellar medium conditions in starburst galaxies Beirão, M.P.L. Citation Beirão, M. P. L. (2010, January 13). Interstellar medium conditions in starburst galaxies. Retrieved from https://hdl.handle.net/1887/14559 Version: Not Applicable (or Unknown) License: Leiden University Non-exclusive license Downloaded from: https://hdl.handle.net/1887/14559 Note: To cite this publication please use the final published version (if applicable). Chapter 2 Spatially Resolved Spitzer Spectroscopy of the Starburst Nucleus in NGC 5253 Chapter enhanced from P. Beir˜ao, B. R. Brandl, D. Devost, J. D. Smith, L. Hao & J. R. Houck, Astrophysical Journal Letters, 643, L1 (2006) We present new Spitzer Space Telescope data on the nearby, low-metallicity star- burst galaxy NGC 5253, from the Infrared Array Camera IRAC and the Infrared Spectrograph IRS1. The mid-IR luminosity profile of NGC 5253 is clearly domi- nated by an unresolved cluster near the center, which outshines the rest of the galaxy at longer wavelengths. We find that the [NeIII]/[NeII] ratio decreases from ∼ 8.5 at the center to ∼ 2.5 at a distance of ∼ 250 pc. The [S IV]/[S III] fol- lows the [Ne III]/[Ne II] ratio remarkably well, being about 4 − 5 times lower at all distances. Our spectra reveal for the first time PAH emission features at 11.3µm; their equivalent widths increase significantly with distance from the center. The good anti-correlation between the PAH strength and the product between hard- ness and luminosity of the UV radiation field suggests photo-destruction of the PAH molecules in the central region. -
November-December 2020 Trumpet
TrumpetThe Archangel Michael Church INSIDE THIS ISSUE Nov-Dec 2020 • Issue 52 • Archangel Michael Church • Port Washington, NY 2 Mission Statement 3 Fr. John’s Message 4 Fr. Michael’s Message 5 Worship Services & Sacraments 6 Stewardship Update 7 Parish Council Elections Mail In Ballot Request Form 8 Philoptochos 9 Ordination to the Diaconate 9 Adult Choir 10 Blood Drive 10 Sunday School 11 Preschool 11 Greek Language Institute 12 Greek Dance Troupe 13 GOYA 14 Byzantine Youth Choir 15 Community Photos 16 Calendars 21 Golf Outing Sponsors QUICK NEWS & EVENTS Sat. Nov. 7th Parish Council Nominations Close Sat., Nov. 7th: Vespers:Synaxis of the Archangels Sun., Nov. 8th: Synaxis of the Archangels Wed., Nov. 18th Due date for PC Election Mail-In Ballot Request Form Mon., Dec. 7th Final Post-mark date for PC Election Mail-In Ballots This year’s religious education theme is: “And you shall love the Lord your God Sat., Dec. 19th: Challenge Liturgy with all your heart, with all your soul, with all your mind, & Christmas Party Sundayand with all Themes your strength.” of (MarkGreat 12:30) Lent The art and graphic work donated by Jim Lolis. The Archangel Michael Church The Archangel Michael Greek Orthodox Church is dedicated to the continuation of Trumpet our Lord and Savior Jesus Christ’s ministry of salvation About the Parish through the proclamation Mission Archangel Michael Greek Orthodox Church and teaching of the Gospel. 100 Fairway Drive Statement Port Washington, New York 11050 We are a community of Phone: 516-944-3180 individuals and families who Fax: 516-944-3185 share the traditions and Website: ArchangelMichaelChurch.org Email: [email protected] ageless beliefs of our Holy Archangel Michael Church is a parish of the Direct Archdiocesan District and Orthodox Christian Faith. -
6.3.10 Nn Layout 1
Photo by Tyler Rhodes HONORING THE FALLEN—Veterans lead the procession from the cemetery to Belmont Point during Nome’s Memorial Day celebration May 31. C VOLUME CIX NO. 22 JUNE 3, 2010 Vote tally unkown Recall appears to fail for 4 of 5 school board members, count still unofficial By Tyler Rhodes counts, the most recent conducted By the time Tuesday rolled by hand on May 28, the shifting re- around—a full week after Nome vot- sults appeared as of press time to ers had gone to the ballot box to de- have only succeeded in removing termine the fate of its school one person, Albert McComas, from board—Heather Payenna had spent the five-member board. With razor- a week uncertain of whether or not thin margins between their “yes” she would keep her seat. and “no” votes, Payenna and fellow “I’m just ready, one way or the board member Kirsten Timbers other, to have this election be certi- have oscillated between being re- fied and be in the books,” Payenna called and retained as the succeed- said outside city hall just after noon ing unofficial tallies have come in. on June 1. As of Tuesday after- The most recent numbers—ob- noon, it looked like she would still served by witnesses to the May 28 have to wait. hand recount—would keep both Payenna was on her way to an ex- women on the board with Timbers pected Nome Common Council enjoying a two-vote margin (484 to meeting to canvass and certify the re- retain vs. -
Astronomia E Astrofísica Na Plataforma Scimago Confirma Essa Tendência De Estabilização Da Quantidade De Artigo, Após Um Período De Alta Mais Intenso
UNIVERSIDADE ESTADUAL DE CAMPINAS INSTITUTO DE ESTUDOS DA LINGUAGEM LABORATÓRIO DE ESTUDOS AVANÇADOS EM JORNALISMO GIULIANA MARIA MIRANDA SANTOS DO “ASTRONOMÊS” PARA O PORTUGUÊS: a comunicação entre astrônomos e jornalistas no Brasil CAMPINAS 2015 GIULIANA MARIA MIRANDA SANTOS DO “ASTRONOMÊS” PARA O PORTUGUÊS: a comunicação entre astrônomos e jornalistas no Brasil Dissertação de mestrado apresentada ao Instituto de Estudos da Linguagem e Laboratório de Estudos Avançados em Jornalismo da Universidade Estadual de Campinas para obtenção do título de mestra em Divulgação Científica e Cultural, na área de Divulgação Científica e Cultural Orientador: Prof. Dr. Marcelo Knobel Este exemplar corresponde à versão final da dissertação defendida pela aluna. CAMPINAS 2015 Agência(s) de fomento e nº(s) de processo(s): Não se aplica. Ficha catalográfica Universidade Estadual de Campinas Biblioteca do Instituto de Estudos da Linguagem Crisllene Queiroz Custódio - CRB 8/8624 Miranda, Giuliana, 1987- M672d MirDo 'astronomês' para o português : a comunicação entre astrônomos e jornalistas no Brasil / Giuliana Maria Miranda Santos. – Campinas, SP : [s.n.], 2015. MirOrientador: Marcelo Knobel. MirDissertação (mestrado) – Universidade Estadual de Campinas, Instituto de Estudos da Linguagem. Mir1. Astronomia na comunicação de massa. 2. Comunicação de massa e linguagem. 3. Jornalismo - Brasil. 4. Divulgação científica - Brasil. 5. Pesquisadores - Brasil. 6. Jornalistas - Brasil. 7. Assessores de imprensa - Brasil. I. Knobel, Marcelo,1968-. II. Universidade Estadual -
FIXED STARS a SOLAR WRITER REPORT for Churchill Winston WRITTEN by DIANA K ROSENBERG Page 2
FIXED STARS A SOLAR WRITER REPORT for Churchill Winston WRITTEN BY DIANA K ROSENBERG Page 2 Prepared by Cafe Astrology cafeastrology.com Page 23 Churchill Winston Natal Chart Nov 30 1874 1:30 am GMT +0:00 Blenhein Castle 51°N48' 001°W22' 29°‚ 53' Tropical ƒ Placidus 02' 23° „ Ý 06° 46' Á ¿ 21° 15° Ý 06' „ 25' 23° 13' Œ À ¶29° Œ 28° … „ Ü É Ü 06° 36' 26' 25° 43' Œ 51'Ü áá Œ 29° ’ 29° “ àà … ‘ à ‹ – 55' á á 55' á †32' 16° 34' ¼ † 23° 51'Œ 23° ½ † 06' 25° “ ’ † Ê ’ ‹ 43' 35' 35' 06° ‡ Š 17° 43' Œ 09° º ˆ 01' 01' 07° ˆ ‰ ¾ 23° 22° 08° 02' ‡ ¸ Š 46' » Ï 06° 29°ˆ 53' ‰ Page 234 Astrological Summary Chart Point Positions: Churchill Winston Planet Sign Position House Comment The Moon Leo 29°Le36' 11th The Sun Sagittarius 7°Sg43' 3rd Mercury Scorpio 17°Sc35' 2nd Venus Sagittarius 22°Sg01' 3rd Mars Libra 16°Li32' 1st Jupiter Libra 23°Li34' 1st Saturn Aquarius 9°Aq35' 5th Uranus Leo 15°Le13' 11th Neptune Aries 28°Ar26' 8th Pluto Taurus 21°Ta25' 8th The North Node Aries 25°Ar51' 8th The South Node Libra 25°Li51' 2nd The Ascendant Virgo 29°Vi55' 1st The Midheaven Gemini 29°Ge53' 10th The Part of Fortune Capricorn 8°Cp01' 4th Chart Point Aspects Planet Aspect Planet Orb App/Sep The Moon Semisquare Mars 1°56' Applying The Moon Trine Neptune 1°10' Separating The Moon Trine The North Node 3°45' Separating The Moon Sextile The Midheaven 0°17' Applying The Sun Semisquare Jupiter 0°50' Applying The Sun Sextile Saturn 1°52' Applying The Sun Trine Uranus 7°30' Applying Mercury Square Uranus 2°21' Separating Mercury Opposition Pluto 3°49' Applying Venus Sextile -
Solar Writer Report for Abraham Lincoln
FIXED STARS A Solar Writer Report for Abraham Lincoln Written by Diana K Rosenberg Compliments of:- Stephanie Johnson Seeing With Stars Astrology PO Box 159 Stepney SA 5069 Australia Tel/Fax: +61 (08) 8331 3057 Email: [email protected] Web: www.esotech.com.au Page 2 Abraham Lincoln Natal Chart 12 Feb 1809 12:40:56 PM UT +0:00 near Hodgenville 37°N35' 085°W45' Tropical Placidus 22' 13° 08°ˆ ‡ 17' ¾ 06' À ¿É ‰ 03° ¼ 09° 00° 06° 09°06° ˆ ˆ ‡ † ‡ 25° 16' 41'08' 40' † 01' 09' Œ 29' ‰ 9 10 23° ¶ 8 27°‰ 11 Ï 27° 01' ‘ ‰02' á 7 12 ‘ áá 23° á 23° ¸ 23°Š27' á Š à „ 28' 28' 6 18' 1 10°‹ º ‹37' 13° 05' ‹ 5 Á 22° ½ 27' 2 4 01' Ü 3 07° Œ ƒ » 09' 23° 09° Ý Ü 06° 16' 06' Ê 00°ƒ 13° 22' Ý 17' 08°‚ Page 23 Astrological Summary Chart Point Positions: Abraham Lincoln Planet Sign Position House Comment The Moon Capricorn 27°Cp01' 12th The Sun Aquarius 23°Aq27' 12th read into 1st House Mercury Pisces 10°Pi18' 1st Venus Aries 7°Ar27' 1st read into 2nd House Mars Libra 25°Li29' 8th Jupiter Pisces 22°Pi05' 1st Saturn Sagittarius 3°Sg08' 9th read into 10th House Uranus Scorpio 9°Sc40' 8th Neptune Sagittarius 6°Sg41' 9th read into 10th House Pluto Pisces 13°Pi37' 1st The North Node Scorpio 6°Sc09' 8th The South Node Taurus 6°Ta09' 2nd The Ascendant Aquarius 23°Aq28' 1st The Midheaven Sagittarius 8°Sg22' 10th The Part of Fortune Capricorn 27°Cp02' 12th Chart Point Aspects Planet Aspect Planet Orb App/Sep The Moon Square Mars 1°32' Separating The Moon Conjunction The Part of Fortune 0°00' Applying The Sun Trine Mars 2°02' Applying The Sun Conjunction The Ascendant -
Rodolfo Smiljanic
Rodolfo Smiljanic Contact address: Tel. +48 22 329 6115 Nicolaus Copernicus Astronomical Center E-mail: [email protected] Polish Academy of Sciences http://users.camk.edu.pl/rsmiljanic ul. Bartycka 18 ORCID: 0000-0003-0942-7855 00-716 Warsaw, Poland Researcher ID: A-1789-2008 Employment Since Nov. 2018 Associate Professor Dec. 2015 { Nov. 2018 Assistant Professor Dec. 2012 { Nov. 2015 Postdoctoral Researcher (100% independent research) Nicolaus Copernicus Astronomical Center Polish Academy of Sciences { Poland Oct. 2009 { Sep. 2012 ESO Fellow (75% independent research, 25% functional duties) European Southern Observatory { Germany Functional Duty: User Support Astronomer for UVES@VLT Jan. 2009 { Sep. 2009 Posdoctoral Researcher University of S~aoPaulo { Brazil Education and degrees June 2018 Habilitation Nicolaus Copernicus Astronomical Center { Poland Sep. 2006 { Nov. 2007 Visiting student at ESO { Germany Mar. 2005 { Dec. 2008 Doctor of Sciences (December 8, 2008) Mar. 2003 { Mar. 2005 Master of Sciences (March 8, 2005) University of S~aoPaulo { Brazil PhD and Master's advisor: Beatriz Barbuy Mar. 1998 { Feb. 2003 Astronomer (February 24, 2003) Federal University of Rio de Janeiro { Brazil Prizes and Awards • Sonata Bis research grant from NCN for the research project \Playing CHESS with stars: decoding the Galactic chemical enrichment history with stellar chemical abundances" (awarded in February 2020 for 5 years): 2 204 160,00 PLN • OPUS Grant from the NCN for the research project \Near-UV stellar spectroscopy: uncovering the past and building the future" (awarded in May 2019) for 3 years: 1 239 420 PLN • Financial support to organize a scientific workshop in Poland (awarded by ESO on May 2017): 5 000 EUR.