Krajská Hvezdáreň V Žiline So Sídlom Horný Val Č.20, 012 42 Žilina

Total Page:16

File Type:pdf, Size:1020Kb

Krajská Hvezdáreň V Žiline So Sídlom Horný Val Č.20, 012 42 Žilina SPRÁVA O ČINNOSTI A HOSPODÁRENÍ KULTÚRNEJ ORGANIZÁCIE V ZRIAĎOVATEĽSKEJ PÔSOBNOSTI ŽILINSKÉHO SAMOSPRÁVNEHO KRAJA ZA ROK 2018 OBSAH 1 ÚLOHY A MIESTO KULTÚRNEJ ORGANIZÁCIE V NÁRODNOM SYSTÉME KULTÚRNYCH ORGANIZÁCIÍ ....... 5 1.1 POSLANIE KULTÚRNEJ ORGANIZÁCIE A FUNKCIE ...................................................................................................................... 5 1.2 PLNENIE PRIORITNÝCH ÚLOH V ROKU 2018 .......................................................................................................................... 5 1.3 SIEŤ VEREJNÝCH ORGANIZÁCIÍ PODOBNÉHO TYPU V REGIÓNE V ZRIAĎOVATEĽSKEJ PÔSOBNOSTI INÝCH SUBJEKTOV .............................. 7 1.4 POTENCIÁLNE POUŽÍVATEĽSKÉ ZÁZEMIE: .............................................................................................................................. 7 2 MAJETOK VO VLASTNÍCTVE ŽSK V SPRÁVE KULTÚRNEJ ORGANIZÁCIE, PRIESTOROVÉ PODMIENKY, VÝSTAVBA, REKONŠTRUKCIE ......................................................................................................................................... 7 2.1 PASPORTIZÁCIA NEHNUTEĽNÉHO MAJETKU VO VLASTNÍCTVE ŽSK V SPRÁVE KULTÚRNEJ ORGANIZÁCIE .............................................. 7 2.2 AKTUÁLNY STAVEBNO-TECHNICKÝ STAV NEHNUTEĽNOSTÍ ......................................................................................................... 7 2.3 SÚPIS SPRAVOVANÝCH NÁRODNÝCH KULTÚRNYCH PAMIATOK ................................................................................................... 9 2.4 PREVÁDZKOVANÉ PRIESTORY VYUŽÍVANÉ NA VLASTNÚ ČINNOSŤ ................................................................................................ 9 2.5 PREVÁDZKOVANÉ PRIESTORY PRENAJATÉ INÝM SUBJEKTOM ...................................................................................................... 9 2.6 PREVÁDZKOVANÉ PRIESTORY PRENAJATÉ OD INÝCH SUBJEKTOV ................................................................................................. 9 2.7 REKONŠTRUKCIE ............................................................................................................................................................ 10 2.8 OPRAVY A ÚDRŽBA CELKOM A Z TOHO RIEŠENIE HAVÁRIÍ........................................................................................................ 10 2.9 VOZOVÝ PARK ............................................................................................................................................................... 10 2.10 POISTENIE MAJETKU – SKUTOČNOSŤ, POŽIADAVKA .......................................................................................................... 10 2.11 POISTENIE ZBIERKOVÉHO FONDU – SKUTOČNOSŤ, POŽIADAVKA .......................................................................................... 10 2.12 PLNENIE ÚLOH NA ÚSEKU BOZP, PO ............................................................................................................................ 10 3 NÁVŠTEVNOSŤ KULTÚRNEJ ORGANIZÁCIE ............................................................................................. 10 4 NÁVŠTEVNOSŤ PRACOVÍSK KRAJSKEJ HVEZDÁRNE V ŽILINE .................................................................. 11 5 ROČNÉ DANE Z NEHNUTEĽNOSTÍ ........................................................................................................... 12 6 RIADIACA A KONTROLNÁ ČINNOSŤ ....................................................................................................... 12 6.1 VÝSLEDKY VNÚTORNEJ KONTROLNEJ ČINNOSTI ..................................................................................................................... 12 6.2 VÝSLEDKY KONTROLNEJ ČINNOSTI KONTROLNÝCH ORGÁNOV ................................................................................................... 12 7 VZÁJOMNÁ KOORDINÁCIA A KOOPERÁCIA ........................................................................................... 12 7.1 SPOLUPRÁCA S KULTÚRNYMI ORGANIZÁCIAMI V ZRIAĎOVATEĽSKEJ PÔSOBNOSTI ŽSK .................................................................. 12 7.2 SPOLUPRÁCA S KULTÚRNYMI ORGANIZÁCIAMI V ZRIAĎOVATEĽSKEJ PÔSOBNOSTI INÝCH SUBJEKTOV ................................................ 13 7.3 SPOLUPRÁCA S MESTAMI A OBCAMI, ORGANIZÁCIAMI 3. SEKTORU .......................................................................................... 13 7.4 MEDZINÁRODNÁ SPOLUPRÁCA – PREHĽAD SUBJEKTOV A AKTIVÍT............................................................................................. 14 7.5 NAJVÝZNAMNEJŠÍ PARTNERI – DOMÁCI, ZAHRANIČNÍ ............................................................................................................ 14 7.6 SPOLUPRÁCA V ODBORNO-POZOROVATEĽSKÝCH PROGRAMOCH .............................................................................................. 14 7.7 PROBLÉMOVÉ OBLASTI, PERSPEKTÍVY ROZVOJA SPOLUPRÁCE .................................................................................................. 15 7.7.1 ZA OBLASŤ MAJETOK A HOSPODÁRENIE ........................................................................................................ 15 7.7.2 ZA OBLASŤ ĽUDSKÉ ZDROJE ............................................................................................................................ 15 7.7.3 ZA OBLASŤ ODBORNÉ ČINNOSTI ..................................................................................................................... 15 7.7.4 ZA OBLASŤ MARKETING, CESTOVNÝ RUCH A SPOLUPRÁCA ........................................................................... 16 7.7.5 Perspektívy rozvoja ......................................................................................................................................... 17 8 OTVÁRACIE HODINY PRE VEREJNOSŤ A VÝŠKA VSTUPNÉHO V ROKU 2018 ............................................ 18 8.1 OTVÁRACIE HODINY ....................................................................................................................................................... 18 8.2 VÝŠKA VSTUPNÉHO V JEDNOTLIVÝCH OBJEKTOCH ................................................................................................................. 18 8.3 ZMENY V OTVÁRACÍCH HODINÁCH A VO VSTUPNOM V ROKU 2018 ......................................................................................... 18 9 ELEKTRONIZÁCIA, AUTOMATIZÁCIA, TECHNICKÉ VYBAVENIE, VÝPOČTOVÁ TECHNIKA ......................... 18 10 PROJEKTOVÁ ČINNOSŤ ORGANIZÁCIE, GRANTY, NADÁCIE, SPONZORSKÉ, FUNDRAISING ................. 19 10.1.1 Názov projektu: NECHAJME HVIEZDY SVIETIŤ ............................................................................................ 19 10.1.2 Názov projektu: SPOLEČNÉ NEBE – PODPORA ZÁŽITKOVÉ A POZNÁVACÍ TURISTIKY V PŘÍHRANIČNÍM REGIONU 19 10.1.3 Názov projektu: DO VESMÍRU .................................................................................................................... 20 10.1.4 Kultúrne poukazy ........................................................................................................................................ 20 11 PERSONÁLNA OBLASŤ, PERSONÁLNE VYBAVENIE ............................................................................. 20 2 11.1 KVALIFIKAČNÁ ŠTRUKTÚRA, ODBORNÁ PRAX ZAMESTNANCOV, VEKOVÁ ŠTRUKTÚRA ZAMESTNANCOV ........................................ 20 11.2 POČET ZAMESTNANCOV NA DOHODY, SEZÓNNYCH ZAMESTNANCOV, CHRÁNENÉ PRACOVNÉ MIESTA .......................................... 20 11.3 POČET A ŠTRUKTÚRA PRACOVNÝCH MIEST NEOBSADENÝCH DLHŠIE AKO 6 MESIACOV + ZDÔVODNENIE ....................................... 21 12 PRÁCA S DOBROVOĽNÍKMI ............................................................................................................... 21 12.1 POČET ZMLUVNÝCH DOBROVOĽNÍKOV, DRUHY A ROZSAH ČINNOSTÍ..................................................................................... 21 12.2 OBČIANSKE ZDRUŽENIA PRACUJÚCE PRI ORGANIZÁCIÁCH (NA PODPORU ČINNOSTI) ................................................................ 21 13 ÚČASŤ PRACOVNÍKOV A RIADITEĽA NA PORADÁCH, ŠKOLENIACH, SEMINÁROCH, ZSC .................... 21 14 PUBLIC RELATIONS ............................................................................................................................ 21 14.1 ODBORNÁ PUBLIKAČNÁ ČINNOSŤ PRACOVNÍKOV ORGANIZÁCIE ........................................................................................... 21 14.2 PUBLIKAČNÁ ČINNOSŤ O ORGANIZÁCII A JEJ ČINNOSTI ...................................................................................................... 21 14.3 VYDANÉ TLAČOVÉ SPRÁVY, PRÍSPEVKY DO TLAČE.............................................................................................................. 22 14.4 OSTATNÁ PREZENTAČNÁ ČINNOSŤ ................................................................................................................................ 24 14.5 WEB STRÁNKA ORGANIZÁCIE, JEJ AKTUALIZÁCIA .............................................................................................................. 25 14.6 FACEBOOK............................................................................................................................................................... 26 14.7 EDIČNÁ ČINNOSŤ – POČET A NÁZVY EDIČNÝCH TITULOV..................................................................................................... 26 14.8 PROPAGÁCIA A PREZENTÁCIA KULTÚRNEJ ORGANIZÁCIE V INÝCH MÉDIÁCH (ROZHLAS, TELEVÍZIA)
Recommended publications
  • New Voyage to Rendezvous with a Small Asteroid Rotating with a Short Period
    Hayabusa2 Extended Mission: New Voyage to Rendezvous with a Small Asteroid Rotating with a Short Period M. Hirabayashi1, Y. Mimasu2, N. Sakatani3, S. Watanabe4, Y. Tsuda2, T. Saiki2, S. Kikuchi2, T. Kouyama5, M. Yoshikawa2, S. Tanaka2, S. Nakazawa2, Y. Takei2, F. Terui2, H. Takeuchi2, A. Fujii2, T. Iwata2, K. Tsumura6, S. Matsuura7, Y. Shimaki2, S. Urakawa8, Y. Ishibashi9, S. Hasegawa2, M. Ishiguro10, D. Kuroda11, S. Okumura8, S. Sugita12, T. Okada2, S. Kameda3, S. Kamata13, A. Higuchi14, H. Senshu15, H. Noda16, K. Matsumoto16, R. Suetsugu17, T. Hirai15, K. Kitazato18, D. Farnocchia19, S.P. Naidu19, D.J. Tholen20, C.W. Hergenrother21, R.J. Whiteley22, N. A. Moskovitz23, P.A. Abell24, and the Hayabusa2 extended mission study group. 1Auburn University, Auburn, AL, USA ([email protected]) 2Japan Aerospace Exploration Agency, Kanagawa, Japan 3Rikkyo University, Tokyo, Japan 4Nagoya University, Aichi, Japan 5National Institute of Advanced Industrial Science and Technology, Tokyo, Japan 6Tokyo City University, Tokyo, Japan 7Kwansei Gakuin University, Hyogo, Japan 8Japan Spaceguard Association, Okayama, Japan 9Hosei University, Tokyo, Japan 10Seoul National University, Seoul, South Korea 11Kyoto University, Kyoto, Japan 12University of Tokyo, Tokyo, Japan 13Hokkaido University, Hokkaido, Japan 14University of Occupational and Environmental Health, Fukuoka, Japan 15Chiba Institute of Technology, Chiba, Japan 16National Astronomical Observatory of Japan, Iwate, Japan 17National Institute of Technology, Oshima College, Yamaguchi, Japan 18University of Aizu, Fukushima, Japan 19Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA 20University of Hawai’i, Manoa, HI, USA 21University of Arizona, Tucson, AZ, USA 22Asgard Research, Denver, CO, USA 23Lowell Observatory, Flagstaff, AZ, USA 24NASA Johnson Space Center, Houston, TX, USA 1 Highlights 1.
    [Show full text]
  • Bennu: Implications for Aqueous Alteration History
    RESEARCH ARTICLES Cite as: H. H. Kaplan et al., Science 10.1126/science.abc3557 (2020). Bright carbonate veins on asteroid (101955) Bennu: Implications for aqueous alteration history H. H. Kaplan1,2*, D. S. Lauretta3, A. A. Simon1, V. E. Hamilton2, D. N. DellaGiustina3, D. R. Golish3, D. C. Reuter1, C. A. Bennett3, K. N. Burke3, H. Campins4, H. C. Connolly Jr. 5,3, J. P. Dworkin1, J. P. Emery6, D. P. Glavin1, T. D. Glotch7, R. Hanna8, K. Ishimaru3, E. R. Jawin9, T. J. McCoy9, N. Porter3, S. A. Sandford10, S. Ferrone11, B. E. Clark11, J.-Y. Li12, X.-D. Zou12, M. G. Daly13, O. S. Barnouin14, J. A. Seabrook13, H. L. Enos3 1NASA Goddard Space Flight Center, Greenbelt, MD, USA. 2Southwest Research Institute, Boulder, CO, USA. 3Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA. 4Department of Physics, University of Central Florida, Orlando, FL, USA. 5Department of Geology, School of Earth and Environment, Rowan University, Glassboro, NJ, USA. 6Department of Astronomy and Planetary Sciences, Northern Arizona University, Flagstaff, AZ, USA. 7Department of Geosciences, Stony Brook University, Stony Brook, NY, USA. 8Jackson School of Geosciences, University of Texas, Austin, TX, USA. 9Smithsonian Institution National Museum of Natural History, Washington, DC, USA. 10NASA Ames Research Center, Mountain View, CA, USA. 11Department of Physics and Astronomy, Ithaca College, Ithaca, NY, USA. 12Planetary Science Institute, Tucson, AZ, Downloaded from USA. 13Centre for Research in Earth and Space Science, York University, Toronto, Ontario, Canada. 14John Hopkins University Applied Physics Laboratory, Laurel, MD, USA. *Corresponding author. E-mail: Email: [email protected] The composition of asteroids and their connection to meteorites provide insight into geologic processes that occurred in the early Solar System.
    [Show full text]
  • Arecibo Radar Observations of 14 High-Priority Near-Earth Asteroids in CY2020 and January 2021 Patrick A
    Arecibo Radar Observations of 14 High-Priority Near-Earth Asteroids in CY2020 and January 2021 Patrick A. Taylor (LPI, USRA), Anne K. Virkki, Flaviane C.F. Venditti, Sean E. Marshall, Dylan C. Hickson, Luisa F. Zambrano-Marin (Arecibo Observatory, UCF), Edgard G. Rivera-Valent´ın, Sriram S. Bhiravarasu, Betzaida Aponte-Hernandez (LPI, USRA), Michael C. Nolan, Ellen S. Howell (U. Arizona), Tracy M. Becker (SwRI), Jon D. Giorgini, Lance A. M. Benner, Marina Brozovic, Shantanu P. Naidu (JPL), Michael W. Busch (SETI), Jean-Luc Margot, Sanjana Prabhu Desai (UCLA), Agata Rozek˙ (U. Kent), Mary L. Hinkle (UCF), Michael K. Shepard (Bloomsburg U.), and Christopher Magri (U. Maine) Summary We propose the continuation of the long-running project R3037 to physically and dynamically characterize the population of near-Earth asteroids with the Arecibo S-band (2380 MHz; 12.6 cm) planetary radar system. The objectives of project R3037 are to: (1) collect high-resolution radar images of and (2) report ultra-precise radar astrometry for the strongest predicted radar targets for the 2020 calendar year plus early January 2021. Such images will be used for three-dimensional shape modeling as the data sets allow. These observations will be carried out as part of the NASA- funded Arecibo planetary radar program, Grant No. 80NSSC19K0523, to PI Anne Virkki (Arecibo Observatory, University of Central Florida) with Patrick Taylor as Institutional PI at the Lunar and Planetary Institute (Universities Space Research Association). Background Radar is arguably the most powerful Earth-based technique for post-discovery physical and dynamical characterization of near-Earth asteroids (NEAs) and plays a crucial role in the nation’s planetary defense initiatives led through the NASA Planetary Defense Coordination Office.
    [Show full text]
  • Detecting the Yarkovsky Effect Among Near-Earth Asteroids From
    Detecting the Yarkovsky effect among near-Earth asteroids from astrometric data Alessio Del Vignaa,b, Laura Faggiolid, Andrea Milania, Federica Spotoc, Davide Farnocchiae, Benoit Carryf aDipartimento di Matematica, Universit`adi Pisa, Largo Bruno Pontecorvo 5, Pisa, Italy bSpace Dynamics Services s.r.l., via Mario Giuntini, Navacchio di Cascina, Pisa, Italy cIMCCE, Observatoire de Paris, PSL Research University, CNRS, Sorbonne Universits, UPMC Univ. Paris 06, Univ. Lille, 77 av. Denfert-Rochereau F-75014 Paris, France dESA SSA-NEO Coordination Centre, Largo Galileo Galilei, 1, 00044 Frascati (RM), Italy eJet Propulsion Laboratory/California Institute of Technology, 4800 Oak Grove Drive, Pasadena, 91109 CA, USA fUniversit´eCˆote d’Azur, Observatoire de la Cˆote d’Azur, CNRS, Laboratoire Lagrange, Boulevard de l’Observatoire, Nice, France Abstract We present an updated set of near-Earth asteroids with a Yarkovsky-related semi- major axis drift detected from the orbital fit to the astrometry. We find 87 reliable detections after filtering for the signal-to-noise ratio of the Yarkovsky drift esti- mate and making sure the estimate is compatible with the physical properties of the analyzed object. Furthermore, we find a list of 24 marginally significant detec- tions, for which future astrometry could result in a Yarkovsky detection. A further outcome of the filtering procedure is a list of detections that we consider spurious because unrealistic or not explicable with the Yarkovsky effect. Among the smallest asteroids of our sample, we determined four detections of solar radiation pressure, in addition to the Yarkovsky effect. As the data volume increases in the near fu- ture, our goal is to develop methods to generate very long lists of asteroids with reliably detected Yarkovsky effect, with limited amounts of case by case specific adjustments.
    [Show full text]
  • Abstract Ems
    abstracts.md A table containing the talk and poster abstracts is posted below, in alphabetical order of last name. The posters themselves can be viewed on ZENODO (click for link), as well as during the gather.town live viewing sessions. Poster identifiers are in a topic.idnumber schema. Categories are as follows: 1. Atmospheres and Interiors . Detection: Transits, RVs, Microlensing, Astrometry, Imaging . Planet Formation (+ Disk) + Evolution . Know Your Star . Population Statistics & Occurrence . Dynamics 3. Instrumentation / Future 4. Habitability & Astrobiology 5. Machine Learning / Techniques / Methods Name (Affiliation). Title. Abstract Where. We present the optical transmission spectrum of the highly inflated Saturn-mass exoplanet WASP- 21b, using three transits obtained with the ACAM instrument on the William Herschel Telescope through the LRG-BEASTS survey (Low Resolution Ground-Based Exoplanet Atmosphere Survey Lili Alderson (University of using Transmission Spectroscopy). Our transmission spectrum covers a wavelength range of 4635- Bristol). LRG-BEASTS: 9000Å, achieving an average transit depth precision of 197ppm compared to one atmospheric scale Ground-bAsed Detection height at 246ppm. Whilst we detect sodium absorption in a bin width of 30Å, at >4 sigma of Sodium And A Steep confidence, we see no evidence of absorption from potassium. Atmospheric retrieval analysis of the OpticAl Slope in the scattering slope indicates that it is too steep for Rayleigh scattering from H2, but is very similar to Atmosphere of the Highly that of HD189733b. The features observed in our transmission spectrum cannot be caused by stellar InflAted Hot-SAturn activity alone, with photometric monitoring and Ca H&K analysis of WASP-21 showing it to be an WASP-21b.
    [Show full text]
  • Impact Excitation of a Seismic Pulse and Vibrational Normal Modes on Asteroid Bennu and Associated Slumping of Regolith
    Impact Excitation of a Seismic Pulse and Vibrational Normal Modes on Asteroid Bennu and Associated Slumping of Regolith Alice C. Quillena,1,∗, Yuhui Zhaob, YuanYuan Chenb, Paul Sánchezc, Randal C. Nelsond, Stephen R. Schwartze;f aDepartment of Physics and Astronomy, University of Rochester, Rochester, NY 14627, USA bKey Laboratory of Planetary Sciences, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China cColorado Center for Astrodynamics Research, The University of Colorado Boulder, UCB 431, Boulder, CO 80309-0431, United States dDepartment of Computer Science, University of Rochester, Rochester, NY 14627, USA eLunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA fLaboratoire Lagrange, Université Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, C.S. 34229, 06304 Nice Cedex 4, France Abstract We consider an impact on an asteroid that is energetic enough to cause resurfacing by seismic reverberation and just below the catastrophic disrup- tion threshold, assuming that seismic waves are not rapidly attenuated. In asteroids with diameter less than 1 km we identify a regime where rare en- ergetic impactors can excite seismic waves with frequencies near those of the asteroid’s slowest normal modes. In this regime, the distribution of seismic reverberation is not evenly distributed across the body surface. With mass- spring model elastic simulations, we model impact excitation of seismic waves with a force pulse exerted on the surface and using three different asteroid shape models. The simulations exhibit antipodal focusing and normal mode excitation. If the impulse excited vibrational energy is long lasting, vibrations arXiv:1804.02058v2 [astro-ph.EP] 23 Sep 2018 are highest at impact point, its antipode and at high surface elevations such as an equatorial ridge.
    [Show full text]
  • CSC 2019 1St Quarter Report RM Edits
    SETI INSTITUTE Activity Report Q1 2019 Image: An artist's impression of GJ 667 Cc, a potentially habitable planet orbiting a red dwarf constituent in a trinary star system. By ESO/L. Calçada - ESO, CC BY 4.0. 1 2 Peer-Reviewed Publications (only in press or published) 1. Abdalla H, Aharonian F, Ait Benkhali F, Anguner EO, Arakawa M, et al., including Huber D (2019). VHE γ-ray discovery and multiwavelength study of the blazar 1ES 2322-409. MNRAS 482, 3011-3022. 2. Abdalla H, Aharonian F, Ait Benkhali F, Anguner EO, Arakawa M, et al., including Huber D (2019). The 2014 TeV γ-Ray Flare of Mrk 501 Seen with H.E.S.S.: Temporal and Spectral Constraints on Lorentz Invariance Violation. Astrophys. J. 870, id.93, 9pp. 3. Abdalla H, Aharonian F, Ait Benkhali F, Anguner EO, Arakawa M, et al., including Huber D (2019). Particle transport within the pulsar wind nebula HESS J1825-137. Astron. Astrophys. 621, id.A116, 18pp. 4. Arentoft T, Grundahl F, WhiteTR, Slumstrup D, Handberg R, et al. including Huber D (2019). Asteroseismology of the Hyades red giant and planet host ɛ Tauri⋆. Astron. Astrophys. 622, id.A190, 12pp. 5. Bacalla XL, Linnartz H, Cox NLJ, Cami J, Roueff E, et al. (2019). The EDIBLES survey. IV. Cosmic ray ionization rates in diffuse clouds from near-ultraviolet observations of interstellar OH+. Astron. Astropys. 622, id.A31, 12pp. 6. Baldi, R.D., Rodriguez-Zaurin, J., Chiaberge, M., Capetti, A., Sparks, W.B., McHardy, I.M., 2019, ApJ, 870, 53. Hubble Space Telescope Emission-line Images of Nearby 3CR Radio Galaxies: Two Photoionization, Accretion, and Feedback Modes, astro-ph/1811.04946.
    [Show full text]
  • Shape of (101955) Bennu Indicative of a Rubble Pile with Internal Stiffness
    Shape of (101955) Bennu indicative of a rubble pile with internal stiffness The MIT Faculty has made this article openly available. Please share how this access benefits you. Your story matters. Citation Barnouin, O.S., et al., "Shape of (101955) Bennu indicative of a rubble pile with internal stiffness." Nature geoscience 12, 4 (April 2019): p. 247-52 doi 10.1038/s41561-019-0330-x ©2019 Author(s) As Published 10.1038/s41561-019-0330-x Publisher Springer Science and Business Media LLC Version Author's final manuscript Citable link https://hdl.handle.net/1721.1/124550 Terms of Use Creative Commons Attribution-Noncommercial-Share Alike Detailed Terms http://creativecommons.org/licenses/by-nc-sa/4.0/ NASA Public Access Author manuscript Nat Geosci. Author manuscript; available in PMC 2019 October 01. Published in final edited form as: NASA Author ManuscriptNASA Author Manuscript NASA Author Nat Geosci. 2019 Manuscript NASA Author April ; 12(4): 247–252. doi:10.1038/s41561-019-0330-x. Users may view, print, copy, and download text and data-mine the content in such documents, for the purposes of academic research, subject always to the full Conditions of use:http://www.nature.com/authors/editorial_policies/license.html#terms Corresponding Author Olivier S. Barnouin ([email protected]). Author contributions: O.S.B. is the OSIRIS-REx Altimetry Working Group (AltWG) lead responsible for generation of all global and local digital terrain models produced during the OSIRIS-REx Mission. He worked with M.G.D., the instrument PI for OLA, as well as E.E.P., R.W.G, and J.R.W., who developed and tested the SPC software, and subsequently made the GDTM.
    [Show full text]
  • Evidence for Widespread Hydrated Minerals on Asteroid (101955) Bennu
    ARTICLES https://doi.org/10.1038/s41550-019-0722-2 Evidence for widespread hydrated minerals on asteroid (101955) Bennu V. E. Hamilton 1*, A. A. Simon2, P. R. Christensen3, D. C. Reuter2, B. E. Clark4, M. A. Barucci 5, N. E. Bowles6, W. V. Boynton7, J. R. Brucato8, E. A. Cloutis9, H. C. Connolly Jr10, K. L. Donaldson Hanna6, J. P. Emery 11, H. L. Enos7, S. Fornasier5, C. W. Haberle3, R. D. Hanna 12, E. S. Howell7, H. H. Kaplan1, L. P. Keller13, C. Lantz14, J.-Y. Li15, L. F. Lim2, T. J. McCoy16, F. Merlin5, M. C. Nolan 7, A. Praet5, B. Rozitis17, S. A. Sandford18, D. L. Schrader 19, C. A. Thomas20, X.-D. Zou15, D. S. Lauretta7 and the OSIRIS-REx Team21 Early spectral data from the Origins, Spectral Interpretation, Resource Identification, and Security-Regolith Explorer (OSIRIS- REx) mission reveal evidence for abundant hydrated minerals on the surface of near-Earth asteroid (101955) Bennu in the form of a near-infrared absorption near 2.7 µm and thermal infrared spectral features that are most similar to those of aque- ously altered CM-type carbonaceous chondrites. We observe these spectral features across the surface of Bennu, and there is no evidence of substantial rotational variability at the spatial scales of tens to hundreds of metres observed to date. In the visible and near-infrared (0.4 to 2.4 µm) Bennu’s spectrum appears featureless and with a blue (negative) slope, confirming previous ground-based observations. Bennu may represent a class of objects that could have brought volatiles and organic chemistry to Earth.
    [Show full text]
  • Small and Micro/Nanoâ•'Satellite Possibilities in Space Science And
    PROCYON ‘14 Hodoyoshiハイブリッド-1 ‘14 ロケット Small and Micro/nano-satellite Possibilities in Space Science and Exploration - Examples from Japan - Shinichi Nakasuka and Ryu Funase University of Tokyo PRISM ‘09 CubeSat 03,05 Nano-JASMINE ‘17 Overview and Contents • Three streamlines of space science and exploration projects in Japan 1. JAXA/ISAS has excellent history of space sciences using small-large(3t) satellites 2. Universities started own contributions using micro/nano/pico-satellites (since 2003) 3. University-JAXA joint missions for space exploration started in 2013 with PROCYON • University of Tokyo’s contributions in micro/nano/pico-satellite fields • Key strategies to pursue science missions using small/micro/nano/pico-satellites Space Science and Exploration - Japanese Missions and Players - Size(kg) Cate Players Project Examples gory >500 Mid- JAXA Science: Ginga, Akari, Suzaku, Hitomi— large Exploration: Hayabusa & 2, Kaguya, Akatsuki-- 100-500 Small JAXA Science: Hisaki (2013), ERG (2016) ---- Engineering: Ikaros (2010) 20-100 Micro JAXA Science: Reimei (Index, 72kg, 2005) University Nano-JASMINE(38kg, 2017), RiseSat (2018) Exploration: PROCYON (58kg, 2014) 2-20 Nano University Science: CUTE-1.7+APD II (3kg 2008) <2 Pico Exploration: ECUULEUS (6U EM-1 2018) REIMEI CUTE1.7 Nano-JASMINE PROCYON JAXA: “Larger than small-satellite” Exploration Projects • Kaguya: Japanese first lunar orbiter. Improved global topography maps, global gravity map and observation of shadowed interior of the crate, etc (2.9t, launch 2007) • Hayabusa :Challenging space technology demonstration leading to the birth of a new pillar in planetary sciences. Returned and asteroid dusts obtained, and samples are under investigation. (510kg, launch 2003, return 2010) • Akatsuki : Understanding the atmospheric dynamics and cloud physics of Venus, Succeed in inserting into Venus orbit in Dec 2015.
    [Show full text]
  • TOI-2076 and TOI-1807: Two Young, Comoving Planetary Systems Within 50 Pc Identified by TESS That Are Ideal Candidates for Further Follow Up
    The Astronomical Journal, 162:54 (22pp), 2021 August https://doi.org/10.3847/1538-3881/ac06cd © 2021. The American Astronomical Society. All rights reserved. TOI-2076 and TOI-1807: Two Young, Comoving Planetary Systems within 50 pc Identified by TESS that are Ideal Candidates for Further Follow Up Christina Hedges1,2 , Alex Hughes3, George Zhou4 , Trevor J. David5,6 , Juliette Becker7 , Steven Giacalone8 , Andrew Vanderburg9 , Joseph E. Rodriguez10 , Allyson Bieryla11 , Christopher Wirth11,12, Shaun Atherton13, Tara Fetherolf14 , Karen A. Collins11 , Adrian M. Price-Whelan5, Megan Bedell5 , Samuel N. Quinn11 , Tianjun Gan15 , George R. Ricker16 , David W. Latham11 , Roland K. Vanderspek16 , Sara Seager16,17,18, Joshua N. Winn19 , Jon M. Jenkins2 , John F. Kielkopf20 , Richard P. Schwarz21 , Courtney D. Dressing8 , Erica J. Gonzales22,41, Ian J. M. Crossfield23, Elisabeth C. Matthews24 , Eric L. N. Jensen25 , Elise Furlan26 , Crystal L. Gnilka2, Steve B. Howell2 , Kathryn V. Lester2 , Nicholas J. Scott2 , Dax L. Feliz27 , Michael B. Lund26 , Robert J. Siverd28 , Daniel J. Stevens29,30,42 , N. Narita31,32,33,34 , A. Fukui31,34 , F. Murgas34,35 , Enric Palle34,35 , Phil J. Sutton36, Keivan G. Stassun27,37 , Luke G. Bouma38 , Michael Vezie16, Jesus Noel Villaseñor16, Elisa V. Quintana39, and Jeffrey C. Smith2,40 1 Bay Area Environmental Research Institute, P.O. Box 25, Moffett Field, CA 94035, USA; [email protected] 2 NASA Ames Research Center, Moffett Field, CA 94035, USA 3 Department of Physics, Loughborough University, Epinal Way,
    [Show full text]
  • Spis Treści Y!
    Spis treści Drodzy Czytelnicy! Te osobliwe obiekty szczególnie intrygują badaczy ze względu na możliwość zderzenia takich planetoid dużą przyjemnością przekazuję z naszą planetą. Państwu ten powakacyjny numer Z„Fizyki w Szkole”. Mam nadzieję, że znajdą Państwo czas, aby do niego zaj- rzeć. Jest w nim duży artykuł poświęcony Edisonowi. Tu pojawia się pytanie czy Tomasz Alva Edison był fizykiem czy nie? Trudno jednoznacznie odpowiedzieć na to pytanie. Był jednak zdecydowanie człowiekiem, który z osiągnięć fizyki umiał twórczo korzystać. Do grona urzą- dzeń, które stworzył należał gramofon. Stworzył więc z jednej strony podstawy przemysłu fonograficznego z drugiej zaś strony pokazał użyteczność akustyki jako nauki. Drugim jego wielkim osiągnię- 44 Osobliwe planetoidy ¢ Krzysztof Ziołkowski ciem, które na prawie sto lat zmieniło obraz naszego świata było ulepszanie i komercjalizacja żarówki, czyli oświetle- Fizyka wczoraj, dziś, jutro nia elektrycznego. Był też współtwórcą 4 Oganesson 118: czy to koniec tablicy Mendelejewa? radiofonii. Zrewolucjonizował też samą ¢ Grzegorz Karwasz metodologię pracy badawczej tworząc 8 Od zdrowych nerek do dializy, pierwsze zinstytucjonalizowane zespoły czyli o biofizyce układu wydalniczego badawcze i tworząc pierwszy nowocze- ¢ Tomasz Kubiak sny instytut naukowy. 16 Termodynamika: główne koncepcje Innym miłośnikom historii nauki chcie- i etapy rozwoju. Cz. 1. libyśmy zaprezentować pierwsze artykuły ¢ Alfred Zmitrowicz z dwóch cyklów, W cyklu poświęconym 22 Od fonografu do elektrowni, czyli krótka termodynamice, autor omawia pojęcia, historia ponad 1000 wynalazków koncepcje i kolejne etapy jej rozwoju. Edisona Thomasa Alvy ¢ Kazimierz Mikulski Dugi cykl poświęcony jest generatorom elektrostatycznym, a rozpoczyna go arty- 28 Generatory elektrostatyczne – różne podejścia do wytwarzania kuł o historii rozwoju metod wytwarzania wysokich napięć stałych – cz. I.
    [Show full text]