Astrophysics Implementation Plan: 2018 Update
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The Early Explorers by Andrew J
The Early Explorers by Andrew J. LePage August 8, 1999 Among these programs were the next generation of Introduction Explorer satellites the ABMA was planning. In the chaos that swept the United States after the launching of the first Soviet Sputniks, a variety of The First New Explorers satellite programs was sponsored by the Department The first of the new series of larger Explorer satellites of Defense (DoD) to supplement (and in some cases was the 39.7 kilogram (87.5 pound) satellite NASA supplant) the country's flagging "official" satellite designated as S-1. Built by JPL, the spin stabilized program, Vanguard. One of the stronger programs S-1 consisted of a pair of fiberglass cones joined at was sponsored by the ABMA (Army Ballistic Missile their bases with a diameter and height of 76 Agency) with its engineering team lead by the centimeters each. The scientific payload consisted of German rocket expert, Wernher von Braun. Using instruments to study cosmic rays, solar X-ray and the Juno I launch vehicle, the ABMA team launched ultraviolet emissions, micrometeorites, as well as the America's first satellite, Explorer 1, which was built globe's heat balance. This was all powered by a bank by Caltech's Jet Propulsion Laboratory (JPL) (see of 15 nickel-cadmium batteries recharged by 3,000 Explorer: America's First Satellite in the February solar cells mounted on the satellite's exterior. This 1998 issue of SpaceViews). advanced payload was equipped with a timer to turn itself off after a year in orbit. While these first satellites returned a wealth of new data, they were limited by the tiny 11 kilogram (25 Explorer S-1 was launched from Cape Canaveral on pound) payload capability of the Juno I. -
Monte Carlo Simulacija Protojata Galaksija U Cosmos Pregledu Neba
SVEUILITE U ZAGREBU PRIRODOSLOVNO-MATEMATIKI FAKULTET FIZIKI ODSJEK Neven Tomi£i¢ MONTE CARLO SIMULACIJA PROTOJATA GALAKSIJA U COSMOS PREGLEDU NEBA Diplomski rad Zagreb, 2015 SVEUILITE U ZAGREBU PRIRODOSLOVNO-MATEMATIKI FAKULTET FIZIKI ODSJEK SMJER: ISTRAIVAKI Neven Tomi£i¢ Diplomski rad MONTE CARLO SIMULACIJA PROTOJATA GALAKSIJA U COSMOS PREGLEDU NEBA Voditelj diplomskog rada: doc. dr. sc. Vernesa Smol£i¢ Ocjena diplomskog rada: ____________________ Povjerenstvo: 1. _________________________ 2. _________________________ 3. _________________________ Datum polaganja: _____________ Zagreb, 2015 ZAHVALA Zahvalio bih se mentorici doc. dr. sc. Vernesi Smol£i¢, na mentorstvu i voenju kroz ovaj rad. Posebno bih se zahvalio asistentu dipl. ing. Nikoli Baranu za tehni£ku pomo¢ i savjetovanje pri izvedbi simulacija i rada u programskom jeziku IDL. Zahvalio bih se dr. sc. Oskariu Miettinenu i kolegici Niki Jurlin, za pomo¢ i savjetovanje pri analizi protojata. Takoer se zahvaljujem dr. sc. Jacinti Delhaize, mag. phys. Mladenu Novaku i kolegi Kre²imiru Tisani¢u za savjetovanje i pomo¢ pri radu. Zahvalio bih se svojim roditeljima na savjetima za ºivot i za potporu koju mi cijeli ºivot pruºaju na mom putu u znanost. Takoer bih se zahvalio svim svojim profesorima, prija- teljima i kolegama u mom osnovno²kolskom, srednjo²kolskom i fakultetskom obrazovanju, a pogotovo prof. Ankici Ben£ek, prof. Andreji Pehar, prof. Ana-Mariji Kukuruzovi¢ i prof. Josipu Matijevi¢u koji su me usmjeravali prema znanosti. Saºetak Jata tj. skupovi galaksija su veliki virializirani skupovi galaksija. Galaksije do- prinose oko 5% mase jata, unutar-klasterski medij oko 10% mase i tamna tvar do 85% mase. Te strukture su nastale iz protojata galaksija. Protojato je rani oblik jata sa manje galaksija i sa uo£enom ve¢om gusto¢om broja galaksija u odnosu na ostale dijelove promatranog neba. -
XIII Publications, Presentations
XIII Publications, Presentations 1. Refereed Publications E., Kawamura, A., Nguyen Luong, Q., Sanhueza, P., Kurono, Y.: 2015, The 2014 ALMA Long Baseline Campaign: First Results from Aasi, J., et al. including Fujimoto, M.-K., Hayama, K., Kawamura, High Angular Resolution Observations toward the HL Tau Region, S., Mori, T., Nishida, E., Nishizawa, A.: 2015, Characterization of ApJ, 808, L3. the LIGO detectors during their sixth science run, Classical Quantum ALMA Partnership, et al. including Asaki, Y., Hirota, A., Nakanishi, Gravity, 32, 115012. K., Espada, D., Kameno, S., Sawada, T., Takahashi, S., Ao, Y., Abbott, B. P., et al. including Flaminio, R., LIGO Scientific Hatsukade, B., Matsuda, Y., Iono, D., Kurono, Y.: 2015, The 2014 Collaboration, Virgo Collaboration: 2016, Astrophysical Implications ALMA Long Baseline Campaign: Observations of the Strongly of the Binary Black Hole Merger GW150914, ApJ, 818, L22. Lensed Submillimeter Galaxy HATLAS J090311.6+003906 at z = Abbott, B. P., et al. including Flaminio, R., LIGO Scientific 3.042, ApJ, 808, L4. Collaboration, Virgo Collaboration: 2016, Observation of ALMA Partnership, et al. including Asaki, Y., Hirota, A., Nakanishi, Gravitational Waves from a Binary Black Hole Merger, Phys. Rev. K., Espada, D., Kameno, S., Sawada, T., Takahashi, S., Kurono, Lett., 116, 061102. Y., Tatematsu, K.: 2015, The 2014 ALMA Long Baseline Campaign: Abbott, B. P., et al. including Flaminio, R., LIGO Scientific Observations of Asteroid 3 Juno at 60 Kilometer Resolution, ApJ, Collaboration, Virgo Collaboration: 2016, GW150914: Implications 808, L2. for the Stochastic Gravitational-Wave Background from Binary Black Alonso-Herrero, A., et al. including Imanishi, M.: 2016, A mid-infrared Holes, Phys. -
Information Summaries
TIROS 8 12/21/63 Delta-22 TIROS-H (A-53) 17B S National Aeronautics and TIROS 9 1/22/65 Delta-28 TIROS-I (A-54) 17A S Space Administration TIROS Operational 2TIROS 10 7/1/65 Delta-32 OT-1 17B S John F. Kennedy Space Center 2ESSA 1 2/3/66 Delta-36 OT-3 (TOS) 17A S Information Summaries 2 2 ESSA 2 2/28/66 Delta-37 OT-2 (TOS) 17B S 2ESSA 3 10/2/66 2Delta-41 TOS-A 1SLC-2E S PMS 031 (KSC) OSO (Orbiting Solar Observatories) Lunar and Planetary 2ESSA 4 1/26/67 2Delta-45 TOS-B 1SLC-2E S June 1999 OSO 1 3/7/62 Delta-8 OSO-A (S-16) 17A S 2ESSA 5 4/20/67 2Delta-48 TOS-C 1SLC-2E S OSO 2 2/3/65 Delta-29 OSO-B2 (S-17) 17B S Mission Launch Launch Payload Launch 2ESSA 6 11/10/67 2Delta-54 TOS-D 1SLC-2E S OSO 8/25/65 Delta-33 OSO-C 17B U Name Date Vehicle Code Pad Results 2ESSA 7 8/16/68 2Delta-58 TOS-E 1SLC-2E S OSO 3 3/8/67 Delta-46 OSO-E1 17A S 2ESSA 8 12/15/68 2Delta-62 TOS-F 1SLC-2E S OSO 4 10/18/67 Delta-53 OSO-D 17B S PIONEER (Lunar) 2ESSA 9 2/26/69 2Delta-67 TOS-G 17B S OSO 5 1/22/69 Delta-64 OSO-F 17B S Pioneer 1 10/11/58 Thor-Able-1 –– 17A U Major NASA 2 1 OSO 6/PAC 8/9/69 Delta-72 OSO-G/PAC 17A S Pioneer 2 11/8/58 Thor-Able-2 –– 17A U IMPROVED TIROS OPERATIONAL 2 1 OSO 7/TETR 3 9/29/71 Delta-85 OSO-H/TETR-D 17A S Pioneer 3 12/6/58 Juno II AM-11 –– 5 U 3ITOS 1/OSCAR 5 1/23/70 2Delta-76 1TIROS-M/OSCAR 1SLC-2W S 2 OSO 8 6/21/75 Delta-112 OSO-1 17B S Pioneer 4 3/3/59 Juno II AM-14 –– 5 S 3NOAA 1 12/11/70 2Delta-81 ITOS-A 1SLC-2W S Launches Pioneer 11/26/59 Atlas-Able-1 –– 14 U 3ITOS 10/21/71 2Delta-86 ITOS-B 1SLC-2E U OGO (Orbiting Geophysical -
Page 1 of 5 Second Stand Alone Missions of Opportunity
Second Stand Alone Missions Of Opportunity Notice (SALMON-2) Program Element Appendix (PEA) Q Heliophysics Explorers Mission of Opportunity Program Library Step-2 Change Log The current version of this document may be found in the Program Library, at https://explorers.larc.nasa.gov/HPSMEX/MO/programlibrary.html, by selecting the “View Step-2 Change Log” link. Updates to the Program Library are represented in reverse-chronological order. Latest revisions are indicated via highlighting. May 4, 2018: CFR-2014-title2-vol1-sec200-466.pdf posted to NASA and Federal Documents item “2 CFR 200.466, “Scholarships and Student Aid Costs” (NOTE: Step-2 addition.)” April 11, 2018: 2017_LSP_Advisory_Services_Overview_for_2016_Heliophysics_Explorer.pdf reposted as an update to Program Specific Documents item “29. 2017 LSP Advisory Services Overview (NOTE: Step-2 addition.)”. Typo corrected on title slide. March 9, 2018: tailored-Class-D-guidance-for-AOs-updated-redact.pdf (dated 12 February 2018) posted as an update to Program Specific Documents item “34. Guidance on the Application of NASA Science Mission Directorate (SMD) Class-D Tailoring/Streamlining Decision Memorandum (signed 07 December 2017) to Currently Active Explorers Program AO Competitions (NOTE: Step-2 addition.)” March 5, 2018: Explorers-Program-Plan-Signed-2014.09.09_Redacted.pdf posted to Program Specific Documents item “32. Explorers Program Plan (NOTE: Step-2 addition.)” March 5, 2018: tailored-Class-D-guidance-for-AOs-redact.pdf (dated 12 February 2018) posted as Program Specific Documents item “31. Guidance on the Application of NASA Science Mission Directorate (SMD) Class-D Tailoring/Streamlining Decision Memorandum (signed [7] December 2017) to Currently Active Explorers Program AO Competitions (NOTE: Step-2 addition.)” March 5, 2018: SMD-Class-D-Policy-redact.pdf (dated 17 December 2017) posted as Program Specific Documents item “30. -
Science: Planetary Science Outyears Are Notional
Science: Planetary Science Outyears are notional ($M) 2019 2020 2021 2022 2023 Planetary Science $2,235 $2,200 $2,181 $2,162 $2,143 Ø Creates a robotic Lunar Discovery and Exploration program, that supports commercial partnerships and innovative approaches to achieving human and science exploration goals. Ø Continues development of Mars 2020 and Europa Clipper. Ø Establishes a Planetary Defense program, including the Double Asteroid Redirection Test (DART) and Near-Earth Object Observations. Ø Studies a potential Mars Sample Return mission incorporating commercial partnerships. Ø Formulates the Lucy and Psyche missions. Ø Selects the next New Frontiers mission. Ø Invests in CubeSats/SmallSats that can achieve entirely new science at lower cost. Ø Operates 10 Planetary missions. § OSIRIS-REx will map asteroid Bennu. § New Horizons will fly by its Kuiper belt target. Dawn Image of Ceres on January 13, 2015 20 Science: Astrophysics Outyears are notional ($M) 2019 2020 2021 2022 2023 Astrophysics $1,185 $1,185 $1,185 $1,185 $1,185 Ø Launches the James Webb Space Telescope. Ø Moves Webb into the Cosmic Origins Program within the Astrophysics Account. Ø Terminates WFIRST due to its significant cost and higher priorities elsewhere within NASA. Increases funding for future competed missions and research. Ø Supports the TESS exoplanet mission following launch by June 2018. Ø Formulates or develops, IXPE, GUSTO, XARM, Euclid, and a new MIDEX mission to be selected in FY 2019. Ø Operates ten missions and the balloon project. Ø Invests in CubeSats/SmallSats that can achieve entirely new science at lower cost. Ø All Astrophysics missions beyond prime operations (including SOFIA) will be subject to senior review in 2019. -
Progress with Litebird
LiteBIRD Lite (Light) Satellite for the Studies of B-mode Polarization and Inflation from Cosmic Background Radiation Detection Progress with LiteBIRD Masashi Hazumi (KEK/Kavli IPMU/SOKENDAI/ISAS JAXA) for the LiteBIRD working group 1 LiteBIRD JAXA Osaka U. Kavli IPMU Kansei U. Tsukuba APC Paris T. Dotani S. Kuromiya K. Hattori Gakuin U. M. Nagai R. Stompor H. Fuke M. Nakajima N. Katayama S. Matsuura H. Imada S. Takakura Y. Sakurai TIT Cardiff U. I. Kawano K. Takano H. Sugai Kitazato U. S. Matsuoka G. Pisano UC Berkeley / H. Matsuhara T. Kawasaki R. Chendra LBNL T. Matsumura Osaka Pref. U. KEK Paris ILP D. Barron K. Mitsuda M. Inoue M. Hazumi Konan U. U. Tokyo J. Errard J. Borrill T. Nishibori K. Kimura (PI) I. Ohta S. Sekiguchi Y. Chinone K. Nishijo H. Ogawa M. Hasegawa T. Shimizu CU Boulder A. Cukierman A. Noda N. Okada N. Kimura NAOJ S. Shu N. Halverson T. de Haan A. Okamoto K. Kohri A. Dominjon N. Tomita N. Goeckner-wald S. Sakai Okayama U. M. Maki T. Hasebe McGill U. P. Harvey Y. Sato T. Funaki Y. Minami J. Inatani Tohoku U. M. Dobbs C. Hill K. Shinozaki N. Hidehira T. Nagasaki K. Karatsu M. Hattori W. Holzapfel H. Sugita H. Ishino R. Nagata S. Kashima MPA Y. Hori Y. Takei A. Kibayashi H. Nishino T. Noguchi Nagoya U. E. Komatsu O. Jeong S. Utsunomiya Y. Kida S. Oguri Y. Sekimoto K. Ichiki NIST R. Keskitalo T. Wada K. Komatsu T. Okamura M. Sekine T. Kisner G. Hilton R. Yamamoto S. Uozumi N. -
Updated Design of the CMB Polarization Experiment Satellite Litebird
Journal of Low Temperature Physics (2020) 199:1107–1117 https://doi.org/10.1007/s10909-019-02329-w Updated Design of the CMB Polarization Experiment Satellite LiteBIRD H. Sugai, et al. [full author details at the end of the article] Received: 30 August 2019 / Accepted: 26 December 2019 / Published online: 27 January 2020 © The Author(s) 2020 Abstract Recent developments of transition-edge sensors (TESs), based on extensive experi- ence in ground-based experiments, have been making the sensor techniques mature enough for their application on future satellite cosmic microwave background (CMB) polarization experiments. LiteBIRD is in the most advanced phase among such future satellites, targeting its launch in Japanese Fiscal Year 2027 (2027FY) with JAXA’s H3 rocket. It will accommodate more than 4000 TESs in focal planes of refective low-frequency and refractive medium-and-high-frequency telescopes in order to detect a signature imprinted on the CMB by the primordial gravitational waves predicted in cosmic infation. The total wide frequency coverage between 34 and 448 GHz enables us to extract such weak spiral polarization patterns through the precise subtraction of our Galaxy’s foreground emission by using spectral dif- ferences among CMB and foreground signals. Telescopes are cooled down to 5 K for suppressing thermal noise and contain polarization modulators with transmis- sive half-wave plates at individual apertures for separating sky polarization signals from artifcial polarization and for mitigating from instrumental 1/f noise. Passive cooling by using V-grooves supports active cooling with mechanical coolers as well as adiabatic demagnetization refrigerators. Sky observations from the second Sun– Earth Lagrangian point, L2, are planned for 3 years. -
The Hot and Energetic Universe
The Hot And Energetic Universe The Universe was always the final frontier of the Human quest for knowledge Through all its history, humanity has observed the sky trying to understand the Cosmos outside the limits of our planet Today, this effort has yielded significant results. Now we know that our sun is a typical star, which does not differ significantly from the other stars of the starry sky. We have discovered the planets of our Solar System and we have studied the conditions prevailing in them. We studied asteroids and comets and found their important role in the formation of planets. We understand the basic principles of the formation, the life and the death of stars. We have also discovered thousands of exoplanets orbiting other stars. We studied giant star clusters. We have discovered dense clouds of interstellar dust and gas where new stars are born continuously. We have managed to describe the gigantic complex of stars to which we belong. Our Galaxy. We realized that our Galaxy is not alone in the universe and that there are hundreds of billions of galaxies. We discovered that the universe of galaxies is extremely violent and in constant motion. Finally we found that the whole universe is in accelerating expansion and we are searching urgently for its origin. This quest is an epic journey towards knowledge, which abolish superstitions and defines human existence. Vehicles for the journey of humanity in the universe are scientific instruments called telescopes, which are installed at various observatories. Telescopes collect light. Their performance depends on the diameter of the lens or mirror used. -
Arxiv:2006.06594V1 [Astro-Ph.CO]
Mitigating the optical depth degeneracy using the kinematic Sunyaev-Zel'dovich effect with CMB-S4 1, 2, 2, 1, 3, 4, 5, 6, 5, 6, Marcelo A. Alvarez, ∗ Simone Ferraro, y J. Colin Hill, z Ren´eeHloˇzek, x and Margaret Ikape { 1Berkeley Center for Cosmological Physics, Department of Physics, University of California, Berkeley, CA 94720, USA 2Lawrence Berkeley National Laboratory, One Cyclotron Road, Berkeley, CA 94720, USA 3Department of Physics, Columbia University, New York, NY, USA 10027 4Center for Computational Astrophysics, Flatiron Institute, New York, NY, USA 10010 5Dunlap Institute for Astronomy and Astrophysics, University of Toronto, 50 St George Street, Toronto ON, M5S 3H4, Canada 6David A. Dunlap Department of Astronomy and Astrophysics, University of Toronto, 50 St George Street, Toronto ON, M5S 3H4, Canada The epoch of reionization is one of the major phase transitions in the history of the universe, and is a focus of ongoing and upcoming cosmic microwave background (CMB) experiments with im- proved sensitivity to small-scale fluctuations. Reionization also represents a significant contaminant to CMB-derived cosmological parameter constraints, due to the degeneracy between the Thomson- scattering optical depth, τ, and the amplitude of scalar perturbations, As. This degeneracy subse- quently hinders the ability of large-scale structure data to constrain the sum of the neutrino masses, a major target for cosmology in the 2020s. In this work, we explore the kinematic Sunyaev-Zel'dovich (kSZ) effect as a probe of reionization, and show that it can be used to mitigate the optical depth degeneracy with high-sensitivity, high-resolution data from the upcoming CMB-S4 experiment. -
Astrophysics
National Aeronautics and Space Administration Astrophysics Committee on NASA Science Paul Hertz Mission Extensions Director, Astrophysics Division NRC Keck Center Science Mission Directorate Washington DC @PHertzNASA February 1-2, 2016 Why Astrophysics? Astrophysics is humankind’s scientific endeavor to understand the universe and our place in it. 1. How did our universe 2. How did galaxies, stars, 3. Are We Alone? begin and evolve? and planets come to be? These national strategic drivers are enduring 1972 1982 1991 2001 2010 2 Astrophysics Driving Documents http://science.nasa.gov/astrophysics/documents 3 Astrophysics Programs Physics of the Cosmos Cosmic Origins Exoplanet Exploration Program Program Program 1. How did our universe 2. How did galaxies, stars, 3. Are We Alone? begin and evolve? and planets come to be? Astrophysics Explorers Program Astrophysics Research Program James Webb Space Telescope Program (managed outside of Astrophysics Division until commissioning) 4 Astrophysics Programs and Missions Physics of the Cosmos Cosmic Origins Exoplanet Exploration Program Program Program Chandra Hubble Spitzer Kepler/K2 XMM-Newton (ESA) Herschel (ESA) WFIRST Fermi SOFIA Planck (ESA) LISA Pathfinder (ESA) Astrophysics Explorers Program Euclid (ESA) NuSTAR Swift Suzaku (JAXA) Athena (ESA) ASTRO-H (JAXA) NICER TESS L3 GW Obs (ESA) 3 SMEX and 2 MO in Phase A James Webb Space Telescope Program: Webb 5 Astrophysics Programs and Missions Physics of the Cosmos Cosmic Origins Exoplanet Exploration Program Program Program Missions in extended phase Chandra Hubble Spitzer Kepler/K2 XMM-Newton (ESA) Herschel (ESA) WFIRST Fermi SOFIA Planck (ESA) LISA Pathfinder (ESA) Astrophysics Explorers Program Euclid (ESA) NuSTAR Swift Suzaku (JAXA) Athena (ESA) ASTRO-H (JAXA) NICER TESS L3 GW Obs (ESA) 3 SMEX and 2 MO in Phase A James Webb Space Telescope Program: Webb 6 Astrophysics Mission Portfolio • NASA Astrophysics seeks to advance NASA’s strategic objectives in astrophysics as well as the science priorities of the Decadal Survey in Astronomy and Astrophysics. -
Photographs Written Historical and Descriptive
CAPE CANAVERAL AIR FORCE STATION, MISSILE ASSEMBLY HAER FL-8-B BUILDING AE HAER FL-8-B (John F. Kennedy Space Center, Hanger AE) Cape Canaveral Brevard County Florida PHOTOGRAPHS WRITTEN HISTORICAL AND DESCRIPTIVE DATA HISTORIC AMERICAN ENGINEERING RECORD SOUTHEAST REGIONAL OFFICE National Park Service U.S. Department of the Interior 100 Alabama St. NW Atlanta, GA 30303 HISTORIC AMERICAN ENGINEERING RECORD CAPE CANAVERAL AIR FORCE STATION, MISSILE ASSEMBLY BUILDING AE (Hangar AE) HAER NO. FL-8-B Location: Hangar Road, Cape Canaveral Air Force Station (CCAFS), Industrial Area, Brevard County, Florida. USGS Cape Canaveral, Florida, Quadrangle. Universal Transverse Mercator Coordinates: E 540610 N 3151547, Zone 17, NAD 1983. Date of Construction: 1959 Present Owner: National Aeronautics and Space Administration (NASA) Present Use: Home to NASA’s Launch Services Program (LSP) and the Launch Vehicle Data Center (LVDC). The LVDC allows engineers to monitor telemetry data during unmanned rocket launches. Significance: Missile Assembly Building AE, commonly called Hangar AE, is nationally significant as the telemetry station for NASA KSC’s unmanned Expendable Launch Vehicle (ELV) program. Since 1961, the building has been the principal facility for monitoring telemetry communications data during ELV launches and until 1995 it processed scientifically significant ELV satellite payloads. Still in operation, Hangar AE is essential to the continuing mission and success of NASA’s unmanned rocket launch program at KSC. It is eligible for listing on the National Register of Historic Places (NRHP) under Criterion A in the area of Space Exploration as Kennedy Space Center’s (KSC) original Mission Control Center for its program of unmanned launch missions and under Criterion C as a contributing resource in the CCAFS Industrial Area Historic District.