The Sky This Month – Oct 11 to Nov 15, 2017 (Times in EDT & EST) by Chris Vaughan
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Security & Defence European
a 7.90 D 14974 E D European & Security ES & Defence 6/2019 International Security and Defence Journal COUNTRY FOCUS: AUSTRIA ISSN 1617-7983 • Heavy Lift Helicopters • Russian Nuclear Strategy • UAS for Reconnaissance and • NATO Military Engineering CoE Surveillance www.euro-sd.com • Airborne Early Warning • • Royal Norwegian Navy • Brazilian Army • UAS Detection • Cockpit Technology • Swiss “Air2030” Programme Developments • CBRN Decontamination June 2019 • CASEVAC/MEDEVAC Aircraft • Serbian Defence Exports Politics · Armed Forces · Procurement · Technology ANYTHING. In operations, the Eurofighter Typhoon is the proven choice of Air Forces. Unparalleled reliability and a continuous capability evolution across all domains mean that the Eurofighter Typhoon will play a vital role for decades to come. Air dominance. We make it fly. airbus.com Editorial Europe Needs More Pragmatism The elections to the European Parliament in May were beset with more paradoxes than they have ever been. The strongest party which will take its seats in the plenary chambers in Brus- sels (and, as an expensive anachronism, also in Strasbourg), albeit only for a brief period, is the Brexit Party, with 29 seats, whose programme is implicit in their name. Although EU institutions across the entire continent are challenged in terms of their public acceptance, in many countries the election has been fought with a very great deal of emotion, as if the day of reckoning is dawning, on which decisions will be All or Nothing. Some have raised concerns about the prosperous “European Project”, which they see as in dire need of rescue from malevolent sceptics. Others have painted an image of the decline of the West, which would inevitably come about if Brussels were to be allowed to continue on its present course. -
Archons (Commanders) [NOTICE: They Are NOT Anlien Parasites], and Then, in a Mirror Image of the Great Emanations of the Pleroma, Hundreds of Lesser Angels
A R C H O N S HIDDEN RULERS THROUGH THE AGES A R C H O N S HIDDEN RULERS THROUGH THE AGES WATCH THIS IMPORTANT VIDEO UFOs, Aliens, and the Question of Contact MUST-SEE THE OCCULT REASON FOR PSYCHOPATHY Organic Portals: Aliens and Psychopaths KNOWLEDGE THROUGH GNOSIS Boris Mouravieff - GNOSIS IN THE BEGINNING ...1 The Gnostic core belief was a strong dualism: that the world of matter was deadening and inferior to a remote nonphysical home, to which an interior divine spark in most humans aspired to return after death. This led them to an absorption with the Jewish creation myths in Genesis, which they obsessively reinterpreted to formulate allegorical explanations of how humans ended up trapped in the world of matter. The basic Gnostic story, which varied in details from teacher to teacher, was this: In the beginning there was an unknowable, immaterial, and invisible God, sometimes called the Father of All and sometimes by other names. “He” was neither male nor female, and was composed of an implicitly finite amount of a living nonphysical substance. Surrounding this God was a great empty region called the Pleroma (the fullness). Beyond the Pleroma lay empty space. The God acted to fill the Pleroma through a series of emanations, a squeezing off of small portions of his/its nonphysical energetic divine material. In most accounts there are thirty emanations in fifteen complementary pairs, each getting slightly less of the divine material and therefore being slightly weaker. The emanations are called Aeons (eternities) and are mostly named personifications in Greek of abstract ideas. -
Redalyc.Status and Trends of Smallsats and Their Launch Vehicles
Journal of Aerospace Technology and Management ISSN: 1984-9648 [email protected] Instituto de Aeronáutica e Espaço Brasil Wekerle, Timo; Bezerra Pessoa Filho, José; Vergueiro Loures da Costa, Luís Eduardo; Gonzaga Trabasso, Luís Status and Trends of Smallsats and Their Launch Vehicles — An Up-to-date Review Journal of Aerospace Technology and Management, vol. 9, núm. 3, julio-septiembre, 2017, pp. 269-286 Instituto de Aeronáutica e Espaço São Paulo, Brasil Available in: http://www.redalyc.org/articulo.oa?id=309452133001 How to cite Complete issue Scientific Information System More information about this article Network of Scientific Journals from Latin America, the Caribbean, Spain and Portugal Journal's homepage in redalyc.org Non-profit academic project, developed under the open access initiative doi: 10.5028/jatm.v9i3.853 Status and Trends of Smallsats and Their Launch Vehicles — An Up-to-date Review Timo Wekerle1, José Bezerra Pessoa Filho2, Luís Eduardo Vergueiro Loures da Costa1, Luís Gonzaga Trabasso1 ABSTRACT: This paper presents an analysis of the scenario of small satellites and its correspondent launch vehicles. The INTRODUCTION miniaturization of electronics, together with reliability and performance increase as well as reduction of cost, have During the past 30 years, electronic devices have experienced allowed the use of commercials-off-the-shelf in the space industry, fostering the Smallsat use. An analysis of the enormous advancements in terms of performance, reliability and launched Smallsats during the last 20 years is accomplished lower prices. In the mid-80s, a USD 36 million supercomputer and the main factors for the Smallsat (r)evolution, outlined. -
By Sara Bridges
Pag. 001 By Sara Bridges Astronomy is one of the oldest sciences in the world; even the cavemen saw that the patterns and shapes of the stars were predictable and cyclical. But what about you, have you ever looked up at the night sky to see all the millions of stars twinkling back down at you? On first sight it can just look like a mass of stars with no meaning or direction, but if you look again you will notice that these stars make particular pat- terns which are known as constellations. There are eighty eight modern constellations recognised by The International Astro- nomical Union and each of these constellations have a name and an accompanying legend that makes looking at the night sky one of the most interesting and satisfying things you can do for both adults and children of all ages. People throughout the ages have used constellations for a whole manner of different rea- sons. Some farmers used them to help them determine when to plant and harvest in the days before there were calendars. The shapes that the stars seemed to form made it very easy for early farmers to remem- ber their positions in the sky and therefore helped to them recognise when certain seasons were approaching. When they could see Orion high in the sky they knew it was winter, the ancient Egyp- tians prepared for the flooding of the Nile when they saw Sirius rise with the sun. In South Africa the Pleiades star cluster was known as the ‘digging stars’, when they re- appeared in the early morning sky it was time to start digging the ground in order to plant crops. -
Accurate Positions of Pluto and Asteroids Observed in Bucharest During the Year 1932
ACCURATE POSITIONS OF PLUTO AND ASTEROIDS OBSERVED IN BUCHAREST DURING THE YEAR 1932 GHEORGHE BOCŞA, PETRE POPESCU, MIHAELA LICULESCU Astronomical Institute of the Romanian Academy Str. Cuţitul de Argint 5, 040557 Bucharest, Romania E-mail: [email protected] Abstract. The paper contains the observations of minor planets performed in Bucharest Astronomical Observatory in the year 1932 with the 380/6000 mm astrograph. Both Turner’s (constants) and Schlesinger’s (dependences) methods were used in the computation of the normal coordinates of the objects. Keywords: photographic astrometry – minor planets. 1. INTRODUCTION The article is a continuation of the complete investigation of Bucharest Wide-Field Plates Archive initiated in 2010; it contains the plates with asteroids observed in 1932. That year 185 plates were exposed and were stored in the archive, but were not reduced. After analysing them, 98 plates were detected to contain measurable minor planets. The first observed positions in this year were of planet Pluto. They were exposed on 1318cm plates, with 52 minutes exposure .The observations were performed by the famous Romanian astronomer Professor Gheorghe Demetrescu. The most difficult problem was the identification of the planet, the three plates obtained in 1932 having dozens of stars with up to 15 magnitudes. As all the observations were performed in the same month and the planet did not have a great proper motion, it was possible to superpose two plates and to identify Pluto. The values (O–C)α and (O–C)δ were calculated by M. Svechnikov from the Institute of Applied Astronomy in Sankt Petersburg on the basis of precise positions obtained in Bucharest, which we integrated in Pluto’s orbit. -
Revisitfrom2012
A Revisit From Near-Earth Object (NEO) 2012 TC4 Eight days after its discovery, near-Earth object (NEO) 2012 TC4 approached our planet to within 95,000 km, or 25% of the Moon's distance, when it reached perigee at 05:29 UT on 12 October 2012. In this close flyby, 2012 TC4 crossed Earth's orbit travelling inbound toward perihelion on 25.0 November 2012 UT, when it was about 91% of our distance from the Sun. Even in the Earth's night sky before perigee, 2012 TC4 was difficult to observe. Its absolute magnitude H = 26.525 placed its diameter somewhere in the 7.5-30 m range, depending on its unknown surface reflectivity, making observations possible only at very close range. Upon entering Earth's daytime sky as it passed through perigee, 2012 TC4's orbit condition code (OCC) stood at 4 thanks to 281 visible light telescopic observations spanning a 7-day arc. At OCC = 4, 2012 TC4 along-track heliocentric position uncertainty would increase at rates up to 382 arc- seconds per decade.1 Predicted position precision, together with knowledge of 2012 TC4's size and shape, can be vastly improved with radar observations. Although observations were attempted with the Goldstone, California DSS-14 planetary radar in 2012, no echoes were obtained before pointing uncertainties quickly exceeded the precision required to detect 2012 TC4. As it was lost to further observations in 2012, Earth gravity perturbations to 2012 TC4 had increased the NEO's heliocentric orbit period from 1.455 years to 1.667 years. -
Aqueous Alteration on Main Belt Primitive Asteroids: Results from Visible Spectroscopy1
Aqueous alteration on main belt primitive asteroids: results from visible spectroscopy1 S. Fornasier1,2, C. Lantz1,2, M.A. Barucci1, M. Lazzarin3 1 LESIA, Observatoire de Paris, CNRS, UPMC Univ Paris 06, Univ. Paris Diderot, 5 Place J. Janssen, 92195 Meudon Pricipal Cedex, France 2 Univ. Paris Diderot, Sorbonne Paris Cit´e, 4 rue Elsa Morante, 75205 Paris Cedex 13 3 Department of Physics and Astronomy of the University of Padova, Via Marzolo 8 35131 Padova, Italy Submitted to Icarus: November 2013, accepted on 28 January 2014 e-mail: [email protected]; fax: +33145077144; phone: +33145077746 Manuscript pages: 38; Figures: 13 ; Tables: 5 Running head: Aqueous alteration on primitive asteroids Send correspondence to: Sonia Fornasier LESIA-Observatoire de Paris arXiv:1402.0175v1 [astro-ph.EP] 2 Feb 2014 Batiment 17 5, Place Jules Janssen 92195 Meudon Cedex France e-mail: [email protected] 1Based on observations carried out at the European Southern Observatory (ESO), La Silla, Chile, ESO proposals 062.S-0173 and 064.S-0205 (PI M. Lazzarin) Preprint submitted to Elsevier September 27, 2018 fax: +33145077144 phone: +33145077746 2 Aqueous alteration on main belt primitive asteroids: results from visible spectroscopy1 S. Fornasier1,2, C. Lantz1,2, M.A. Barucci1, M. Lazzarin3 Abstract This work focuses on the study of the aqueous alteration process which acted in the main belt and produced hydrated minerals on the altered asteroids. Hydrated minerals have been found mainly on Mars surface, on main belt primitive asteroids and possibly also on few TNOs. These materials have been produced by hydration of pristine anhydrous silicates during the aqueous alteration process, that, to be active, needed the presence of liquid water under low temperature conditions (below 320 K) to chemically alter the minerals. -
The Sky This Month – March 25 to April 22, 2015 by Chris Vaughan
RASC Toronto Centre – www.rascto.ca The Sky This Month – March 25 to April 22, 2015 by Chris Vaughan NEWS Space Exploration – Public and Private Ref. http://www.spaceflightnow.com/tracking/index.html Launches March 25 afternoon - Delta 4 rocket from Cape Canaveral Air Force Station, Florida, payload USAF’s 9th Block 2F GPS navsat. March 25 pm - Dnepr rocket from Dombarovsky, Russia, payload Kompsat 3A high-resolution Earth observation sat for Korea. March 25 pm - H-2A rocket from Tanegashima Space Center, Japan, payload Japanese optical reconnaissance sat. March 27 afternoon - Soyuz rocket from Baikonur Cosmodrome, Kazakhstan, payload manned Soyuz spacecraft to ISS (capsule to remain at ISS for about six months as escape pod). March 27 pm - Soyuz rocket from Sinnamary, French Guiana, payload two Galileo full operational capability sats for Europe’s Galileo navigation constellation. March 28 am - PSLV rocket from Satish Dhawan Space Center, Sriharikota, India, payload IRNSS 1D navsat, 4th in the Indian Regional System. TBD - Soyuz 2-1v rocket from Plesetsk Cosmodrome, Russia, payload Kanopus ST Earth observation satellite. April 10 pm - Falcon 9 rocket from Cape Canaveral Air Force Station, Florida, payload 8th Dragon spacecraft on the 6th operational commercial cargo delivery mission to ISS. April 15 TBD - Ariane 5 rocket from Kourou, French Guiana, payload Thor 7 and Sicral 2 satellites. April TBD - Rockot rocket from Plesetsk Cosmodrome, Russia, payload three Gonets M comsats. New Horizons Mission to Pluto-Charon The New Horizons spacecraft is scheduled to fly through the Pluto-Charon system on July 14, 2015, travelling approx. 13.78 km per second (49,600 kph), then head out into the Kuiper Belt. -
Michael W. Busch Updated June 27, 2019 Contact Information
Curriculum Vitae: Michael W. Busch Updated June 27, 2019 Contact Information Email: [email protected] Telephone: 1-612-269-9998 Mailing Address: SETI Institute 189 Bernardo Ave, Suite 200 Mountain View, CA 94043 USA Academic & Employment History BS Physics & Astrophysics, University of Minnesota, awarded May 2005. PhD Planetary Science, Caltech, defended April 5, 2010. JPL Planetary Science Summer School, July 2006. Hertz Foundation Graduate Fellow, September 2007 to June 2010. Postdoctoral Researcher, University of California Los Angeles, August 2010 – August 2011. Jansky Fellow, National Radio Astronomy Observatory, August 2011 – August 2014. Visiting Scholar, University of Colorado Boulder, July – August 2012. Research Scientist, SETI Institute, August 2013 – present. Current Funding Sources: NASA Near Earth Object Observations. Research Interests: • Shapes, spin states, trajectories, internal structures, and histories of asteroids. • Identifying and characterizing targets for both robotic and human spacecraft missions. • Ruling out potential future asteroid-Earth impacts. • Radio and radar astronomy techniques. Selected Recent Papers: Marshall, S.E., and 24 colleagues, including Busch, M.W., 2019. Shape modeling of potentially hazardous asteroid (85989) 1999 JD6 from radar and lightcurve data, Icarus submitted. Reddy, V., and 69 colleagues, including Busch, M.W., 2019. Near-Earth asteroid 2012 TC4 campaign: results from global planetary defense exercise, Icarus 326, 133-150. Brozović, M., and 16 colleagues, including Busch, M.W., 2018. Goldstone and Arecibo radar observations of (99942) Apophis in 2012-2013, Icarus 300, 115-128. Brozović, M., and 19 colleagues, including Busch, M.W., 2017. Goldstone radar evidence for short-axis mode non-principal axis rotation of near-Earth asteroid (214869) 2007 PA8. Icarus 286, 314-329. -
Near-Earth Asteroid 2012 TC4 Observing Campaign Results From
Icarus 326 (2019) 133–150 Contents lists available at ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Near-Earth asteroid 2012 TC4 observing campaign: Results from a global T planetary defense exercise ⁎ Vishnu Reddya, , Michael S. Kelleyb, Davide Farnocchiac, William H. Ryand, Cristina A. Thomase, Lance A.M. Bennerc, Jessie Dotsonf, Marco Michelig, Melissa J. Bruckera, Schelte J. Bush, Marina Brozovicc, Lorien Wheeleri, Viqar Abbasij, James M. Bauerk, Amber Bonsalll, Zarah L. Browna, Michael W. Buschm, Paul Chodasc, Young-Jun Choin,o, Nicolas Erasmusp, Kelly E. Fastb, John P. Faucherq, Rachel B. Fernandesa, Frank D. Ghigol, David G. Gilbankp, Jon D. Giorginic, Annika Gustafssone, Olivier Hainautr, Walter M. Harrisa, Joseph S. Jaoc, Lindley S. Johnsonb, Theodore Karetaa, Myung-Jin Kimn, Detlef Koschnys, Emily A. Kramerc, Rob R. Landisb, Denis G. Laurinj, Jeffrey A. Larsenq, Clement G. Leec, Cassandra Lejolya, Tim Listert, Robert McMillana, Joseph R. Masieroc, Donovan Mathiasu, Michael Mommertv, Hong-Kyu Moonw, Nicholas A. Moskovitzx, Shantanu P. Naiduc, Ravi Teja Nallapuy, Haris Khan Niaziz, John W. Noonana, David Polishookaa, Eileen V. Ryand, Lauren Schatzab, James V. Scottia, Benjamin Sharkeya, Boris M. Shustovac, Amanda A. Sickafoosep,ad, Marc A. Silvaae, Martin A. Sladec, Lindsay R. Slicka, Lawrence G. Snedekerae, Alessondra Springmanna, David Tholenaf, David E. Trillinge,p, Alberto Q. Vodnizaag, Richard Wainscoataf, Robert Werykaf, Makoto Yoshikawaah a Lunar and Planetary Laboratory, University of Arizona, 1629 E University Blvd, Tucson, AZ 85721, USA b Planetary Defense Coordination Office, Planetary Science Division, NASA Headquarters, 300 E St SW, Washington, DC20546,USA c Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA d Magdalena Ridge Observatory, New Mexico Tech, 801 Leroy Place, Socorro, NM 87801, USA e Dept. -
Close Approach of Asteroid 2012 TC4 Poses No Danger to Earth 10 October 2017, by Tomasz Nowakowski, Astrowatch.Net
Close approach of asteroid 2012 TC4 poses no danger to Earth 10 October 2017, by Tomasz Nowakowski, Astrowatch.net 1.67 years at a distance of about 1.4 AU. Astronomers estimate that 2012 TC4 has a diameter between 26 to 85 feet (8 to 26 meters). Calculations revealed by JPL in July 2017 indicated that 2012 TC4 could pass as close as 4,200 miles (6,800 kilometers). These results were based on only seven days of tracking of this asteroid after it was discovered. However, new observations of this space rock conducted at the European Southern Observatory (ESO) by Olivier Hainaut, Detlef Koschny and Marco Micheli of the European Space Agency (ESA) in July and August 2017, show different estimates. "The new calculations indicate that TC4 will fly The house-sized asteroid 2012 TC4 is slated to safely past our planet on Oct. 12, at a distance of give Earth a close shave on Thursday, October 12, about 43,500 kilometers (27,000 miles) above the swooshing by our planet at approximately 5:41 surface, or about one-eighth of the distance to the UTC (1:41 a.m. EDT) at a distance of about 31,000 moon," JPL reported. miles (50,000 kilometers). Although there were some worries that this rocky object could hit the Therefore, new data provided by the latest Earth, latest observations confirm that it poses no observational campaign exclude the possibility of danger to our home planet at all. 2012 TC4 hitting our planet. Harris emphasizes that even if this asteroid crashed into Earth, it would not "The actual miss distance is pinned down to cause any major damage. -
Exercise – Exercise - Exercise
EXERCISE – EXERCISE - EXERCISE Update for Close Approach of Asteroid 2012 TC4 Observations continue for the small asteroid designated 2012 TC4 that is predicted to safely pass close by the Earth in about two weeks - on Thursday, 12 October 2017. Multiple teams of astronomers have now measured the asteroid’s motion and will observe for physical properties as part of the characterization campaign as the object gets closer. Orbit predictions using the new observations from observatories around the world have refined the time of closest approach to 1:42 AM EDT at a distance of 27,211 miles (43,793 kilometers) from Earth’s surface. This notification is provided as part of an exercise of the recovery, characterization, and reporting of a close approach object, as outlined in NPD 8740.1 - Notification and Communications Regarding Potential Near-Earth Object Threats. Exercise input by the Pan-STARRS near-Earth object survey project in Hawaii indicate that 2012 TC4 could have only been picked up by routine survey operations just last Monday, 25 Sept - only 18 days before closest approach. Only the targeted search for 2012 TC4 as a known approaching asteroid with a larger, 8 meter telescope resulted in its recovery in early August. Also as part of this exercise scientists funded by NASA’s Planetary Defense Coordination Office will use the observed physical properties of the asteroid to model potential impact effects if this asteroid were to impact Earth. Models will be updated with the latest observations as would happen in a real-world potential impact scenario in order to inform emergency response planning.