Roadmap for Astronomy in Switzerland 2007-2016
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Mars Reconnaissance Orbiter
Chapter 6 Mars Reconnaissance Orbiter Jim Taylor, Dennis K. Lee, and Shervin Shambayati 6.1 Mission Overview The Mars Reconnaissance Orbiter (MRO) [1, 2] has a suite of instruments making observations at Mars, and it provides data-relay services for Mars landers and rovers. MRO was launched on August 12, 2005. The orbiter successfully went into orbit around Mars on March 10, 2006 and began reducing its orbit altitude and circularizing the orbit in preparation for the science mission. The orbit changing was accomplished through a process called aerobraking, in preparation for the “science mission” starting in November 2006, followed by the “relay mission” starting in November 2008. MRO participated in the Mars Science Laboratory touchdown and surface mission that began in August 2012 (Chapter 7). MRO communications has operated in three different frequency bands: 1) Most telecom in both directions has been with the Deep Space Network (DSN) at X-band (~8 GHz), and this band will continue to provide operational commanding, telemetry transmission, and radiometric tracking. 2) During cruise, the functional characteristics of a separate Ka-band (~32 GHz) downlink system were verified in preparation for an operational demonstration during orbit operations. After a Ka-band hardware anomaly in cruise, the project has elected not to initiate the originally planned operational demonstration (with yet-to-be used redundant Ka-band hardware). 201 202 Chapter 6 3) A new-generation ultra-high frequency (UHF) (~400 MHz) system was verified with the Mars Exploration Rovers in preparation for the successful relay communications with the Phoenix lander in 2008 and the later Mars Science Laboratory relay operations. -
Thermal Test Campaign of the Solar Orbiter STM
46th International Conference on Environmental Systems ICES-2016-236 10-14 July 2016, Vienna, Austria Thermal Test Campaign of the Solar Orbiter STM C. Damasio1 European Space Agency, ESA/ESTEC, Noordwijk ZH, 2201 AZ, The Netherlands A. Jacobs2, S. Morgan3, M. Sprague4, D. Wild5, Airbus Defence & Space Limited,Gunnels Wood Road, Stevenage, SG1 2AS, UK and V. Luengo6 RHEA System S.A., Av. Pasteur 23, B-1300 Wavre, Belgium Solar Orbiter is the next solar-heliospheric mission in the ESA Science Directorate. The mission will provide the next major step forward in the exploration of the Sun and the heliosphere investigating many of the fundamental problems in solar and heliospheric science. One of the main design drivers for Solar Orbiter is the thermal environment, determined by a total irradiance of 13 solar constants (17500 W/m2) due to the proximity with the Sun. The spacecraft is normally in sun-pointing attitude and is protected from severe solar energy by the Heat Shield. The Heat Shield was tested separately at subsystem level. To complete the STM thermal verification, it was decided to subject to Solar orbiter platform without heat shield to thermal balance test that was performed at IABG test facility in November- December 2015 This paper will describe the Thermal Balance Test performed on the Solar Orbiter STM and the activities performed to correlate the thermal model and to show the verification of the STM thermal design. Nomenclature AU = Astronomical Unit CE = Cold Element FM = Flight Model HE = Hot Element IABG = Industrieanlagen -
LISA, the Gravitational Wave Observatory
The ESA Science Programme Cosmic Vision 2015 – 25 Christian Erd Planetary Exploration Studies, Advanced Studies & Technology Preparations Division 04-10-2010 1 ESAESA spacespace sciencescience timelinetimeline JWSTJWST BepiColomboBepiColombo GaiaGaia LISALISA PathfinderPathfinder Proba-2Proba-2 PlanckPlanck HerschelHerschel CoRoTCoRoT HinodeHinode AkariAkari VenusVenus ExpressExpress SuzakuSuzaku RosettaRosetta DoubleDouble StarStar MarsMars ExpressExpress INTEGRALINTEGRAL ClusterCluster XMM-NewtonXMM-Newton CassiniCassini-H-Huygensuygens SOHOSOHO ImplementationImplementation HubbleHubble OperationalOperational 19901990 19941994 19981998 20022002 20062006 20102010 20142014 20182018 20222022 XMM-Newton • X-ray observatory, launched in Dec 1999 • Fully operational (lost 3 out of 44 X-ray CCD early in mission) • No significant loss of performances expected before 2018 • Ranked #1 at last extension review in 2008 (with HST & SOHO) • 320 refereed articles per year, with 38% in the top 10% most cited • Observing time over- subscribed by factor ~8 • 2,400 registered users • Largest X-ray catalogue (263,000 sources) • Best sensitivity in 0.2-12 keV range • Long uninterrupted obs. • Follow-up of SZ clusters 04-10-2010 3 INTEGRAL • γ-ray observatory, launched in Oct 2002 • Imager + Spectrograph (E/ΔE = 500) + X- ray monitor + Optical camera • Coded mask telescope → 12' resolution • 72 hours elliptical orbit → low background • P/L ~ nominal (lost 4 out 19 SPI detectors) • No serious degradation before 2016 • ~ 90 refereed articles per year • Obs -
Mro High Resolution Imaging Science Experiment (Hirise)
Sixth International Conference on Mars (2003) 3287.pdf MROHIGHRESOLUTIONIMAGINGSCIENCEEXPERIMENT(HIRISE): INSTRUMENTDEVELOPMENT.AlanDelamere,IraBecker,JimBergstrom,JonBurkepile,Joe Day,DavidDorn,DennisGallagher,CharlieHamp,JeffreyLasco,BillMeiers,AndrewSievers,Scott StreetmanStevenTarr,MarkTommeraasen,PaulVolmer.BallAerospaceandTechnologyCorp.,PO Box1062,Boulder,CO80306 Focus Introduction:Theprimaryfunctionalre- Mechanism PrimaryMirror quirementoftheHiRISEimager,figure1isto PrimaryMirrorBaffle 2nd Fold allowidentificationofbothpredictedandun- Mirror knownfeaturesonthesurfaceofMarstoa muchfinerresolutionandcontrastthanprevi- ouslypossible[1],[2].Thisresultsinacam- 1st Fold erawithaverywideswathwidth,6kmat Mirror 300kmaltitude,andahighsignaltonoise ratio,>100:1.Generationofterrainmaps,30 Filters cmverticalresolution,fromstereoimages Focal requiresveryaccurategeometriccalibration. Plane Theprojectlimitationsofmass,costand schedulemakethedevelopmentchallenging. FocalPlane SecondaryMirror Inaddition,thespacecraftstability[3]must Electronics TertiaryMirror SecondaryMirrorBaffle notbeamajorlimitationtoimagequality. Thenominalorbitforthesciencephaseofthe missionisa3pmorbitof255by320kmwith Figure1Cameraopticalpathoptimizedforlowmass periapsislockedtothesouthpole.Thetrack Integration(TDI)tocreateveryhigh(100:1)signalnoise velocityisapproximately3,400m/s. ratioimages. HiRISEFeatures:TheHiRISEinstrumentperformance Theimagerdesignisanall-reflectivethreemirrorastig- goalsarelistedinTable1.Thedesignfeaturesa50cm matictelescopewithlight-weightedZeroduropticsanda -
Darwin in the Press: What the Spanish Dailies Said About the 200Th Anniversary of Charles Darwin’S Birth
CONTRIBUTIONS to SCIENCE, 5 (2): 193–198 (2009) Institut d’Estudis Catalans, Barcelona Celebration of the Darwin Year 2009 DOI: 10.2436/20.7010.01.75 ISSN: 1575-6343 www.cat-science.cat Darwin in the press: What the Spanish dailies said about the 200th anniversary of Charles Darwin’s birth Esther Díez, Anna Mateu, Martí Domínguez Mètode, University of Valencia, Valencia, Spain Resum. El bicentenari del naixement de Charles Darwin, cele- Summary. The bicentenary of Charles Darwin’s birth, cele- brat durant el passat any 2009, va provocar un considerable brated in 2009, caused a surge in the interest shown by the augment de l’interés informatiu de la figura del naturalista an- press in the life and work of the renowned English naturalist. glès. En aquest article s’analitza la cobertura informativa This article analyzes the press coverage devoted to the Darwin d’aquest aniversari en onze diaris generalistes espanyols, i Year in eleven Spanish daily papers during the week of Dar- s’estableix grosso modo quines són les principals postures de win’s birthday and provides a brief synopsis of the positions la premsa espanyola davant de la teoria de l’evolució. D’aques- adopted by the Spanish press regarding the theory of evolu- ta anàlisi, queda ben palès com el creacionisme és encara molt tion. The analysis makes very clear the relatively strong support viu en els mitjans espanyols més conservadors. for creationism by the conservative press in Spain. Paraules clau: Charles Darwin ∙ ciència vs. creacionisme ∙ Keywords: Charles Darwin ∙ science vs. creationism ∙ tractament informatiu científic scientific news coverage “The more we know of the fixed laws of nature the more In this article, we examine to what extent and in what form incredible do miracles become.” this controversy persists in Spanish society, focusing on the print media’s response to the celebration, in 2009, of the 200th Charles Darwin (1887). -
Will the Real Monster Black Hole Please Stand Up? 8 January 2015
Will the real monster black hole please stand up? 8 January 2015 how the merging of galaxies can trigger black holes to start feeding, an important step in the evolution of galaxies. "When galaxies collide, gas is sloshed around and driven into their respective nuclei, fueling the growth of black holes and the formation of stars," said Andrew Ptak of NASA's Goddard Space Flight Center in Greenbelt, Maryland, lead author of a The real monster black hole is revealed in this new new study accepted for publication in the image from NASA's Nuclear Spectroscopic Telescope Astrophysical Journal. "We want to understand the Array of colliding galaxies Arp 299. In the center panel, mechanisms that trigger the black holes to turn on the NuSTAR high-energy X-ray data appear in various and start consuming the gas." colors overlaid on a visible-light image from NASA's Hubble Space Telescope. The panel on the left shows NuSTAR is the first telescope capable of the NuSTAR data alone, while the visible-light image is pinpointing where high-energy X-rays are coming on the far right. Before NuSTAR, astronomers knew that the each of the two galaxies in Arp 299 held a from in the tangled galaxies of Arp 299. Previous supermassive black hole at its heart, but they weren't observations from other telescopes, including sure if one or both were actively chomping on gas in a NASA's Chandra X-ray Observatory and the process called accretion. The new high-energy X-ray European Space Agency's XMM-Newton, which data reveal that the supermassive black hole in the detect lower-energy X-rays, had indicated the galaxy on the right is indeed the hungry one, releasing presence of active supermassive black holes in Arp energetic X-rays as it consumes gas. -
The XMM-Newton SAS - Distributed Development and Maintenance of a Large Science Analysis System: a Critical Analysis
Astronomical Data Analysis Software and Systems XIII ASP Conference Series, Vol. 314, 2004 F. Ochsenbein, M. Allen, and D. Egret, eds. The XMM-Newton SAS - Distributed Development and Maintenance of a Large Science Analysis System: A Critical Analysis Carlos Gabriel1, John Hoar1, Aitor Ibarra1, Uwe Lammers2, Eduardo Ojero1, Richard Saxton1, Giuseppe Vacanti2 XMM-Newton Science Operations Centre, Science Operations and Data Systems Division of ESA, European Space Agency Mike Denby, Duncan Fyfe, Julian Osborne Department of Physics and Astronomy, University of Leicester, Leicester, LE1 7RH, UK Abstract. The XMM-Newton Scientific Analysis System (SAS) is the software used for the reduction and calibration of data taken with the XMM-Newton satellite instruments leading to almost 400 refereed scien- tific papers published in the last 2.5 years. Its maintenance, further devel- opment and distribution is under the responsibility of the XMM-Newton Science Operations Centre together with the Survey Science Centre, rep- resenting a collaborative effort of more than 30 scientific institutes. Developed in C++, Fortran 90/95 and Perl, the SAS makes large use of open software packages such as ds9 for image display (SAO-R&D Software Suite), Grace, LHEASOFT and cfitsio (HEASARC project), pgplot, fftw and the non-commercial version of Qt (TrollTech). The combination of supporting several versions of SAS for multiple platforms (including SunOS, DEC, many Linux flavours and MacOS) in a widely distributed development process which makes use of a suite of ex- ternal packages and libraries presents substantial issues for the integrity of the SAS maintenance and development. A further challenge comes from the necessity of maintaining the flexibility of a software package evolving together with progress made in instrument calibration and anal- ysis refinement, whilst at the same time being the source of all official products of the XMM-Newton mission. -
The Higgs Boson and the Cosmology of the Early Universe Mikhail Shaposhnikov Blois 2018
The Higgs Boson and the Cosmology of the Early Universe Mikhail Shaposhnikov Blois 2018 Rencontres de Blois, June 4, 2018 – p. 1 Almost 6 years with the Higgs boson: July 4, 2012, Higgs at ATLAS and CMS 3500 ATLAS Data Sig+Bkg Fit (m =126.5 GeV) 3000 H Bkg (4th order polynomial) 2500 Events / 2 GeV 2000 1500 s=7 TeV, ∫Ldt=4.8fb-1 1000 s=8 TeV, ∫Ldt=5.9fb-1 γγ→ 500 H (a) 200100 110 120 130 140 150 160 100 0 -100 Events - Bkg (b) -200 100 110 120 130 140 150 160 Data S/B Weighted 100 Sig+Bkg Fit (m =126.5 GeV) H Bkg (4th order polynomial) 80 weights / 2 GeV Σ 60 40 20 (c) 8100 110 120 130 140 150 160 4 0 -4 (d) -8 Σ weights - Bkg 100 110 120 130 140 150 160 m γγ [GeV] Rencontres de Blois, June 4, 2018 – p. 2 What did we learn from the Higgs discovery for particle physics? Rencontres de Blois, June 4, 2018 – p. 3 The ideas of the authors of the BEH mechanism were right Rencontres de Blois, June 4, 2018 – p. 4 The Standard Model is now complete Rencontres de Blois, June 4, 2018 – p. 5 126 125 U U U GeV Triumph of the SM in particle physics No significant deviations from the SM have been observed Rencontres de Blois, June 4, 2018 – p. 6 126 125 U U U GeV Triumph of the SM in particle physics No significant deviations from the SM have been observed The masses of the top quark and of the Higgs boson, the Nature has chosen, make the SM a self-consistent effective field theory all the way up to the quantum gravity Planck scale MP . -
The Most Dangerous Ieos in STEREO
EPSC Abstracts Vol. 6, EPSC-DPS2011-682, 2011 EPSC-DPS Joint Meeting 2011 c Author(s) 2011 The most dangerous IEOs in STEREO C. Fuentes (1), D. Trilling (1) and M. Knight (2) (1) Northern Arizona University, Arizona, USA, (2) Lowell Observatory, Arizona, USA ([email protected]) Abstract (STEREO-B) which view the Sun-Earth line using a suite of telescopes. Each spacecraft moves away 1 from the Earth at a rate of 22.5◦ year− (Figure 1). IEOs (inner Earth objects or interior Earth objects) are ∼ potentially the most dangerous near Earth small body Our search for IEOs utilizes the Heliospheric Imager population. Their study is complicated by the fact the 1 instruments on each spacecraft (HI1A and HI1B). population spends all of its time inside the orbit of The HI1s are centered 13.98◦ from the Sun along the the Earth, giving ground-based telescopes a small win- Earth-Sun line with a square field of view 20 ◦ wide, 1 dow to observe them. We introduce STEREO (Solar a resolution of 70 arcsec pixel− , and a bandpass of TErrestrial RElations Observatory) and its 5 years of 630—730 nm [3]. Images are taken every 40 minutes, archival data as our best chance of studying the IEO providing a nearly continuous view of the inner solar population and discovering possible impactor threats system since early 2007. The nominal visual limit- ing magnitude of HI1 is 13, although the sensitivity to Earth. ∼ We show that in our current search for IEOs in varies somewhat with solar elongation, and asteroids STEREO data we are capable of detecting and char- fainter than 13 can be seen near the outer edges. -
Prime Focus (06-16).Pub
Highlights of the June Sky - - - - - - Saturn at opposition. - - - - - - DAWN: A very thin waning A Publication of the Kalamazoo Astronomical Society crescent Moon is about 2° below Mercury. Look low in east about 20 minutes before sunrise. - - - 4th - - - New Moon 11:00 pm EDT KAS - - - 9th - - - PM: Regulus, the brightest star in Leo, is about 7° to General Meeting: Friday, June 3 @ 7:00 pm the Moon’s upper left. Kalamazoo Area Math & Science Center - See Page 8 for Details - - - 10th - - - PM: The Moon is located about halfway between Observing Session: Saturday, June 11 @ 9:30 pm Regulus and Jupiter. The Moon, Mars, Jupiter & Saturn - Kalamazoo Nature Center - - - 11th - - - PM: The Moon forms a Board Meeting: Sunday, June 12 @ 5:00 pm triangle with Jupiter and Sunnyside Church - 2800 Gull Road - All Members Welcome Sigma () Leonis. - - - 12th - - - Observing Session: Saturday, June 25 @ 9:30 pm First Quarter Moon 4:10 am EDT Grand Globular Clusters - Kalamazoo Nature Center - - - 14th - - - PM: Spica, the brightest star in Virgo, is <5° below a waxing gibbous Moon. - - - 17th → 18th - - - Inside the Newsletter. PM: The Moon, Saturn, and Mars make a wide, flat May Meeting Minutes............................. p. 2 triangle, with the longest side stretching ~18° to Board Meeting Minutes......................... p. 3 connect the two planets. - - - 18th → 19th - - - Learn More About the A.L...................p. 3 PM: The Moon and Saturn are 3° to 4° apart. Observations of the Red Planet.......... p. 4 - - - 20th - - - NASA Space Place.................................. p. 5 Full Moon 7:02 am EDT June Night Sky......................................... p. 6 Summer solstice occurs at KAS Board & Announcements........... -
NASA Program & Budget Update
NASA Update AAAC Meeting | June 15, 2020 Paul Hertz Director, Astrophysics Division Science Mission Directorate @PHertzNASA Outline • Celebrate Accomplishments § Science Highlights § Mission Milestones • Committed to Improving § Inspiring Future Leaders, Fellowships § R&A Initiative: Dual Anonymous Peer Review • Research Program Update § Research & Analysis § ROSES-2020 Updates, including COVID-19 impacts • Missions Program Update § COVID-19 impact § Operating Missions § Webb, Roman, Explorers • Planning for the Future § FY21 Budget Request § Project Artemis § Creating the Future 2 NASA Astrophysics Celebrate Accomplishments 3 SCIENCE Exoplanet Apparently Disappears HIGHLIGHT in the Latest Hubble Observations Released: April 20, 2020 • What do astronomers do when a planet they are studying suddenly seems to disappear from sight? o A team of researchers believe a full-grown planet never existed in the first place. o The missing-in-action planet was last seen orbiting the star Fomalhaut, just 25 light-years away. • Instead, researchers concluded that the Hubble Space Telescope was looking at an expanding cloud of very fine dust particles from two icy bodies that smashed into each other. • Hubble came along too late to witness the suspected collision, but may have captured its aftermath. o This happened in 2008, when astronomers announced that Hubble took its first image of a planet orbiting another star. Caption o The diminutive-looking object appeared as a dot next to a vast ring of icy debris encircling Fomalhaut. • Unlike other directly imaged exoplanets, however, nagging Credit: NASA, ESA, and A. Gáspár and G. Rieke (University of Arizona) puzzles arose with Fomalhaut b early on. Caption: This diagram simulates what astronomers, studying Hubble Space o The object was unusually bright in visible light, but did not Telescope observations, taken over several years, consider evidence for the have any detectable infrared heat signature. -
SUCCESSES of the HUBBLE SPACE TELESCOPE, 18Th February 2005 Astronomical History the Hubble Telescope Has Been a Major Tool for the Last Fifteen Years
SUCCESSES OF THE HUBBLE SPACE TELESCOPE, 18th February 2005 Astronomical History The Hubble telescope has been a major tool for the last fifteen years. However, astronomy is as old as man – the earliest known good star map was by Hipparchus 2500 years ago, and a Roman statue (now in Naples) is of Atlas supporting a celestial globe. In 1610 Galileo made the first telescope, opening up the sky; he was able to see the moons of Jupiter, which clearly orbited Jupiter – not Earth, then considered the absolute centre of the universe… Larger telescopes were soon built, with long tubes to accommodate the low curvature lenses that gave the best results – they were not easily manoeuvred. There is a large 28” Refractor at the Observatory in Greenwich, designated ROG, made in 1893 but on an 1859 mount, which even in London’s atmosphere is useful for planetary observation. In 19thC astronomers began to study not just the location of celestial objects but what types they were. Reflecting Telescopes These use a mirror as the prime element to gather and focus light. Small ones were made in the late 18thC, then in the early 19thC Herschel designed one with an 18” mirror. Mirrors being supported from behind, are easier to mount than lenses can only be held at the edge; they can gather more light and give a brighter, sharper image. In 1948 the 200” (5 m) Hale telescope at Mount Palomar set a new standard, high up above much of the atmosphere for maximum clarity. This was built for traditional observation by eye; then longer exposures were made possible with photographic plates; now CCDs (Charge Coupled Detectors) give higher sensitivity.