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PRELIMS Academy for Civil Services PRESS SCIENCE & Powered by: TECHNOLOGY https://t.me/joinchat/AAAAAFYrI5kpQsEAKqmo-A SCIENCE AND TECH TABLE OF CONTENTS 1. 5G 2. MCR 1 Gene 3. Ebola 4. Gaganyaan 5. Digital North East Vision 2022 6. Repurpose used cooking oil (RUCO) 7. Thermal Battery Plant 8. Bacteria Wolbachia 9. Green Propellants by ISRO 10. Electric Propulsion System 11. NASA Developing First Asteroid Deflection Mission 12. Petya Ransomware Attack 13. NISAR Mission 14. China Launches The First Quantum Communications Satellite 15. Cryo-electron Microscopy 16. World First AI News Anchor Debuts In China 17. SpiNNaker : World’s largest brain-like supercomputer 18. RISECREEK 19. National Digital Communications Policy 2018 20. Ensemble Prediction Systems (EPS) 21. Remove DEBRIS Mission To Tackle Space Junk 22. NASA’s New Planet Hunting Probe – TESS 23. World’s First Wind-Sensing Satellite 24. ICESAT-2 25. Planetary Nebula 26. NASA’s Dawn asteroid mission 27. China’s Artificial Moon 28. Hyperion Proto-super cluster Page | 1 https://t.me/joinchat/AAAAAFYrI5kpQsEAKqmo-A 29. DNA Profiling Bill 30. Genome Valley 2.0 31. CRISPR Technology 32. Earth Bio-genome Project 33. WHO Recommends Quadrivalent Influenza Vaccine 34. Hepatitis E Virus 35. Trans Fatty Acids 36. Formalin 37. Acinetobacter Junii 38. World’s First Hydrogen Train 39. New form of matter ‘excitonium’ discovered 40. A New State Of Matter Created 41. NASA’s HAMMER To Deal With Asteroids Heading For Earth 42. GSAT-6A 43. InSight Mission 44. Interstitium 45. Copernicus programme 46. ‘P NULL’ PHENOTYPE 47. AIR - BREATHING ELECTRIC THRUSTER 48. Cold Fusion Reactor 49. -
TOI-1634 B: an Ultra-Short-Period Keystone Planet Sitting Inside the M-Dwarf Radius Valley
The Astronomical Journal, 162:79 (21pp), 2021 August https://doi.org/10.3847/1538-3881/ac0157 © 2021. The American Astronomical Society. All rights reserved. TOI-1634 b: An Ultra-short-period Keystone Planet Sitting inside the M-dwarf Radius Valley Ryan Cloutier1,43 , David Charbonneau1 , Keivan G. Stassun2 , Felipe Murgas3 , Annelies Mortier4 , Robert Massey5 , Jack J. Lissauer6 , David W. Latham1 , Jonathan Irwin1, Raphaëlle D. Haywood7 , Pere Guerra8 , Eric Girardin9, Steven A. Giacalone10 , Pau Bosch-Cabot8, Allyson Bieryla1 , Joshua Winn11 , Christopher A. Watson12 , Roland Vanderspek13 , Stéphane Udry14 , Motohide Tamura15,16,17 , Alessandro Sozzetti18 , Avi Shporer19 , Damien Ségransan14 , Sara Seager19,20,21 , Arjun B. Savel10,22 , Dimitar Sasselov1 , Mark Rose6 , George Ricker13 , Ken Rice23,24 , Elisa V. Quintana25 , Samuel N. Quinn1 , Giampaolo Piotto26 , David Phillips1 , Francesco Pepe14, Marco Pedani27 , Hannu Parviainen3,28 , Enric Palle3,28 , Norio Narita16,29,30,31 , Emilio Molinari32 , Giuseppina Micela33 , Scott McDermott34, Michel Mayor14 , Rachel A. Matson35 , Aldo F. Martinez Fiorenzano27, Christophe Lovis14, Mercedes López-Morales1 , Nobuhiko Kusakabe16,17 , Eric L. N. Jensen36 , Jon M. Jenkins6 , Chelsea X. Huang19 , Steve B. Howell6 , Avet Harutyunyan27, Gábor Fűrész19, Akihiko Fukui37,38 , Gilbert A. Esquerdo1 , Emma Esparza-Borges28 , Xavier Dumusque14 , Courtney D. Dressing10 , Luca Di Fabrizio27, Karen A. Collins1 , Andrew Collier Cameron39 , Jessie L. Christiansen40 , Massimo Cecconi27, Lars A. Buchhave41 , Walter Boschin3,27,28 , and Gloria Andreuzzi27,42 1 Center for Astrophysics ∣ Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USA; [email protected] 2 Department of Physics & Astronomy, Vanderbilt University, 6301 Stevenson Center Lane, Nashville, TN 37235, USA 3 Instituto de Astrofísica de Canarias, C/ Vía Láctea s/n, E-38205 La Laguna, Spain 4 Astrophysics Group, Cavendish Laboratory, University of Cambridge, J.J. -
Road Map of HEAPA-Related Future Missions HEAPA 4Th Future Plan Review Committee 2020/10-2022/9 Lead: Kazuhiro Nakazawa (Nagoya-U/KMI)
20th HEAPA WS 2021/3/8-10 Road map of HEAPA-related future missions HEAPA 4th Future Plan Review Committee 2020/10-2022/9 Lead: Kazuhiro Nakazawa (Nagoya-U/KMI) JAXA Summary of the 3rd committee outcome Vision Preface Astronomical X-ray and Gamma-ray observations are directly related with understanding the how matter and energy exits within the Universe, not only celestial objects, but also the volume itself. They are also key enablers to dig into the extreme physics. In the two broadest aims of astrophysical research, understand the Universe as of now, and understand how it came to be as such, high-energy astrophysics plays an essential role. Summary of the 3rd committee outcome Vision: three big goals Understand our Universe; matter, energy and spacetime, and its origin Dark matter : LSS/clusters to see where DM are, and search for DM direct signal Missing baryon : how the baryon and metals are distributed in the Universe Origins of the large diversity in Universe and celestial objects Galaxy and SMBH co-evolution and their impact on re-ionization Metal synthesis in the Universe Relativistic high-energy phenomena in the Universe Verifying fundamental physics in extreme condition Extreme gravitation : stellar-mass BH, SMBH Extreme high-density matter EoS : Neutron star, quark star Extreme magnetism : Magnetar Diffusive shock : wide variety of yet to be known interactions therein Dark Matter (Re): search for its direct signal Summary of the 3rd committee outcome Mission Categories by JAXA class How to launch Definition and budget Strategic H-IIA, H-III Top science. Flagship mission of Large class each community. -
Arxiv:1809.07242V1 [Astro-Ph.EP] 19 Sep 2018
Draft version September 20, 2018 Preprint typeset using LATEX style emulateapj v. 12/16/11 TESS DISCOVERY OF AN ULTRA-SHORT-PERIOD PLANET AROUND THE NEARBY M DWARF LHS 3844 Roland K. Vanderspek1, Chelsea X. Huang1,2, Andrew Vanderburg3, George R. Ricker1, David W. Latham4, Sara Seager1,17, Joshua N. Winn5, Jon M. Jenkins4, Jennifer Burt1,2, Jason Dittmann1,17, Elisabeth Newton1, Samuel N. Quinn6, Avi Shporer1, David Charbonneau6, Jonathan Irwin6, Kristo Ment6, Jennifer G. Winters6, Karen A. Collins6, Phil Evans7, Tianjun Gan8, Rhodes Hart9, Eric L.N. Jensen10, John Kielkopf11, Shude Mao8, William Waalkes13, Franc¸ois Bouchy12, Maxime Marmier12, Louise D. Nielsen12, Gael¨ Ottoni12, Francesco Pepe12, Damien Segransan´ 12, Stephane´ Udry12, Todd Henry20, Leonardo A. Paredes18, Hodari-Sadiki James18, Rodrigo H. Hinojosa19, Michele L. Silverstein18, Enric Palle21, Zachory Berta-Thompson13, Misty D. Davies4, Michael Fausnaugh1, Ana W. Glidden1, Joshua Pepper14, Edward H. Morgan1, Mark Rose15, Joseph D. Twicken16, Jesus Noel S. Villasenor~ 1, and the TESS Team Draft version September 20, 2018 ABSTRACT Data from the newly-commissioned Transiting Exoplanet Survey Satellite (TESS) has revealed a \hot Earth" around LHS 3844, an M dwarf located 15 pc away. The planet has a radius of 1:32 ± 0:02 R⊕ and orbits the star every 11 hours. Although the existence of an atmosphere around such a strongly irradiated planet is questionable, the star is bright enough (I = 11:9, K = 9:1) for this possibility to be investigated with transit and occultation spectroscopy. The star's brightness and the planet's short period will also facilitate the measurement of the planet's mass through Doppler spectroscopy. -
Arcus: the X-Ray Grating Spectrometer Explorer R
Arcus: The X-ray Grating Spectrometer Explorer R. K. Smith*a, M. Abrahamb, R. Allureda, M. Bautzc, J. Bookbinderd, J. Bregmane, L. Brennemana, N. S. Brickhousea, D. Burrowsf, V. Burwitzg, P. N. Cheimetsa, E. Costantinih, S. Dawsonc, C. DeRooa, A. Falconef, A. R. Fostera, L. Galloi, C. E. Grantc, H. M. Güntherc, R. K. Heilmannc, E. Hertza, B. Hined, D. Huenemoerderc, J. S. Kaastrah, I. Kreykenbohmj, K. K. Madsenk, R. McEntafferf, E. Millerc, J. Millere, E. Morsel, R. Mushotzkym, K. Nandrag, M. Nowakc, F. Paerelsn, R. Petreo, K. Poppenhaegerp, A. Ptako, P. Reida, J. Sandersg, M. Schattenburgc, N. Schulzc, A. Smaleo, P. Temid, L. Valencicq, S. Walkerd, R. Willingaler, J. Wilmsj, S. J. Wolka aSmithsonian Astrophysical Observatory, 60 Garden St, Cambridge, MA, US; bThe Aerospace Corp, Pasadena, CA, US, cMassachusetts Institute of Technology, Cambridge, MA, US; dNASA Ames Research Center, Moffet Field, CA US; eUniversity of Michigan, Ann Arbor, MI, US; fThe Pennsylvania State University, University Park, PA, US; gMax-Planck-Institut für extraterrestrische Physik, Garching, DE; hS- RON Netherlands Institute for Space Research, Utrecht, NL; iSaint Mary’s University, Halifax, Canada; jFrie- drich-Alexander-Universitaet, Erlangen-Nürnberg, DE; kCalifornia Institute of Technology, Pasadena, CA, US; lOrbital ATK, Dulles, VA, US; mUniversity of Maryland, College Park, MD, US; nColumbia University, New York, NY, US; oNASA Goddard Space Flight Center, Greenbelt, MD, US, pQueen’s University, Belfast, UK; qJohns Hopkins University, Baltimore, MD, US; rUniversity of Leicester, Leicester, UK 1. ABSTRACT Arcus, a Medium Explorer (MIDEX) mission, was selected by NASA for a Phase A study in August 2017. The observatory provides high-resolution soft X-ray spectroscopy in the 12-50Å bandpass with unprecedent- ed sensitivity: effective areas of >450 cm2 and spectral resolution >2500. -
16Th HEAD Meeting Session Table of Contents
16th HEAD Meeting Sun Valley, Idaho – August, 2017 Meeting Abstracts Session Table of Contents 99 – Public Talk - Revealing the Hidden, High Energy Sun, 204 – Mid-Career Prize Talk - X-ray Winds from Black Rachel Osten Holes, Jon Miller 100 – Solar/Stellar Compact I 205 – ISM & Galaxies 101 – AGN in Dwarf Galaxies 206 – First Results from NICER: X-ray Astrophysics from 102 – High-Energy and Multiwavelength Polarimetry: the International Space Station Current Status and New Frontiers 300 – Black Holes Across the Mass Spectrum 103 – Missions & Instruments Poster Session 301 – The Future of Spectral-Timing of Compact Objects 104 – First Results from NICER: X-ray Astrophysics from 302 – Synergies with the Millihertz Gravitational Wave the International Space Station Poster Session Universe 105 – Galaxy Clusters and Cosmology Poster Session 303 – Dissertation Prize Talk - Stellar Death by Black 106 – AGN Poster Session Hole: How Tidal Disruption Events Unveil the High 107 – ISM & Galaxies Poster Session Energy Universe, Eric Coughlin 108 – Stellar Compact Poster Session 304 – Missions & Instruments 109 – Black Holes, Neutron Stars and ULX Sources Poster 305 – SNR/GRB/Gravitational Waves Session 306 – Cosmic Ray Feedback: From Supernova Remnants 110 – Supernovae and Particle Acceleration Poster Session to Galaxy Clusters 111 – Electromagnetic & Gravitational Transients Poster 307 – Diagnosing Astrophysics of Collisional Plasmas - A Session Joint HEAD/LAD Session 112 – Physics of Hot Plasmas Poster Session 400 – Solar/Stellar Compact II 113 -
Table of Contents
TABLE OF CONTENTS 1. ART AND CULTURE 1-3 2. SOCIAL ISSUES 4-25 a. Education b. Health and Sanitation c. Women d. Child e. Vulnerable Groups 3. POLITY AND GOVERNANCE 26-33 4. ECONOMY AND INFRASTRUCTURE 34-51 a. Indian Economy b. Banking And Finance c. Agriculture d. Industry e. Infrastructure f. Human Resource Development 5. INTERNATIONAL AFFAIRS AND BILATERAL ISSUES 52-63 6. SUMMITS AND ORGANISATION 64-71 7. DEFENCE AND SECURITY 72-76 8. ENVIRONMENT AND ECOLOGY 77-106 9. SCIENCE AND TECHNOLOGY 107-133 a. IT And ICT b. Space c. Defence Technology d. Biotechnology e. Health And Medicines 10. MISCELLANEOUS 134-151 VAJIRAM AND RAVI Quick Revision For Prelims (Jun-Nov 2018) ART AND CULTURE ➢ Aadi Mahotsav • Aadi Mahotsav, a National Tribal Festival, is being organized in New Delhi by the Ministry of Tribal Affairs and TRIFED to celebrate, cherish and promote the spirit of tribal craft, culture, cuisine and commerce. • Theme of The Festival: “A Celebration of the Spirit of Tribal Culture, Craft, Cuisine and Commerce”. • The Mahotsav will comprise of display and sale of items of tribal art and craft, tribal medicine & healers, tribal cuisine and display of tribal folk performance, in which tribal artisans, chefs, folk dancers/musicians from 23 States of the country shall participate and provide glimpse of their rich traditional culture. ➢ International Buddhist Conclave 2018 • The International Buddhist Conclave (IBC) 2018 held in India saw participation from 29 countries having significant Buddhist population. Japan was the partner country. • The 4 days Conclave was held at New Delhi and Ajanta (Maharashtra), followed by site visits to Rajgir, Nalanda and Bodhgaya (Bihar) and Sarnath (UP). -
The Future of X-Rayastronomy
The Future of X-rayAstronomy Keith Arnaud [email protected] High Energy Astrophysics Science Archive Research Center University of Maryland College Park and NASA’s Goddard Space Flight Center Themes Politics Efficient high resolution spectroscopy Mirrors Polarimetry Other missions Interferometry Themes Politics Efficient high resolution spectroscopy Mirrors Polarimetry Other missions Interferometry How do we get a new X-ray astronomy experiment? A group of scientists and engineers makes a proposal to a national (or international) space agency. This will include a science case and a description of the technology to be used (which should generally be in a mature state). In principal you can make an unsolicited proposal but in practice space agencies have proposal rounds in the same way that individual missions have observing proposal rounds. NASA : Small Explorer (SMEX) and Medium Explorer (MIDEX): every ~2 years alternating Small and Medium, three selected for study for one year from which one is selected for launch. RXTE, GALEX, NuSTAR, Swift, IXPE Arcus, a high resolution X-ray spectroscopy mission was a finalist in the latest MIDEX round but was not selected. Missions of Opportunity (MO): every ~2 years includes balloon programs, ISS instruments and contributions to foreign missions. Suzaku, Hitomi, NICER, XRISM Large missions such as HST, Chandra, JWST are not selected by such proposals but are decided as national priorities through the Astronomy Decadal process. Every ten years a survey is run by the National Academy of Sciences to decide on priorities for both land-based and space-based astronomy. 1960: HST; 1970: VLA; 1980: VLBA; 1990: Chandra and SIRTF; 2000: JWST and ALMA; 2010 WFIRST and LSST. -
Astronomy and Astrophysics Advisory Committee for 2017
Director’s Office 933 North Cherry Avenue Steward Observatory P.O. Box 210065 URL: www.as.arizona.edu Tucson, AZ 85721-0065 Telephone: (520) 621-6524 [email protected] March 15, 2018 Dr. France A. Córdova, Director National Science Foundation 2415 Eisenhower Avenue, Suite 19000 Alexandria, VA 22314 Mr. Robert M. Lightfoot, Jr., Acting Administrator Office of the Administrator NASA Headquarters Washington, DC 20546-0001 Mr. Richard Perry, Secretary of Energy U.S. Department of Energy 1000 Independence Ave., SW Washington, DC 20585 The Honorable John Thune, Chairman Committee on Commerce, Science and Transportation United States Senate Washington, DC 20510 The Honorable Lisa Murkowski, Chairwoman Committee on Energy & Natural Resources United States Senate Washington, DC 20510 The Honorable Lamar Smith, Chairman Committee on Science, Space and Technology United States House of Representatives Washington, DC 20515 Dear Dr. Córdova, Mr. Lightfoot, Secretary Perry, Chairman Thune, Chairwoman Murkowski, and Chairman Smith: I am pleased to transmit to you the annual report of the Astronomy and Astrophysics Advisory Committee for 2017. The Astronomy and Astrophysics Advisory Committee was established under the National Science Foundation Authorization Act of 2002 Public Law 107-368 to: (1) assess, and make recommendations regarding, the coordination of astronomy and astrophysics programs of the Foundation and the National Aeronautics and Space Administration, and the Department of Energy; Arizona’s First University – Since 1885 Dr. -
New Type of Black Hole Detected in Massive Collision That Sent Gravitational Waves with a 'Bang'
New type of black hole detected in massive collision that sent gravitational waves with a 'bang' By Ashley Strickland, CNN Updated 1200 GMT (2000 HKT) September 2, 2020 <img alt="Galaxy NGC 4485 collided with its larger galactic neighbor NGC 4490 millions of years ago, leading to the creation of new stars seen in the right side of the image." class="media__image" src="//cdn.cnn.com/cnnnext/dam/assets/190516104725-ngc-4485-nasa-super-169.jpg"> Photos: Wonders of the universe Galaxy NGC 4485 collided with its larger galactic neighbor NGC 4490 millions of years ago, leading to the creation of new stars seen in the right side of the image. Hide Caption 98 of 195 <img alt="Astronomers developed a mosaic of the distant universe, called the Hubble Legacy Field, that documents 16 years of observations from the Hubble Space Telescope. The image contains 200,000 galaxies that stretch back through 13.3 billion years of time to just 500 million years after the Big Bang. " class="media__image" src="//cdn.cnn.com/cnnnext/dam/assets/190502151952-0502-wonders-of-the-universe-super-169.jpg"> Photos: Wonders of the universe Astronomers developed a mosaic of the distant universe, called the Hubble Legacy Field, that documents 16 years of observations from the Hubble Space Telescope. The image contains 200,000 galaxies that stretch back through 13.3 billion years of time to just 500 million years after the Big Bang. Hide Caption 99 of 195 <img alt="A ground-based telescope&amp;#39;s view of the Large Magellanic Cloud, a neighboring galaxy of our Milky Way. -
NAC Astrophysics Advisory Committee Teleconference Minutes, October 18-19, 2017
NAC Astrophysics Advisory Committee Teleconference Minutes, October 18-19, 2017 NASA ADVISORY COUNCIL ASTROPHYSICS ADVISORY COUNCIL October 18-19, 2017 Teleconference MEETING MINUTES This image cannot currently be displayed. 1/14/2018 _____________________________________________________________ B. Scott Gaudi, Chair 1/14/2018 _____________________________________________________________ Hashima Hasan, Executive Secretary 1 NAC Astrophysics Advisory Committee Teleconference Minutes, October 18-19, 2017 Table of Contents Introductions and Announcements 3 Astrophysics Division Update 3 Summary of Hubble/Chandra Senior Reviews 7 Webb Telescope Update 8 Spitzer Update 10 ExoPAG/PhysPAG/COPAG Updates 10 Community Comment Period 12 Discussion 12 R&A Update 13 Internal Scientist Funding Model 14 Discussion 15 SMD Cubesats Program Update 16 HEO Future Exploration Plans 17 Technology Gap Update 18 NASA Airborne Astronomy Ambassadors Program 19 Public Comment Period 19 Discussion, Recommendations, Actions 19 Adjourn 21 Appendix A- Attendees Appendix B-Membership roster Appendix C-Presentations Appendix D-Agenda Prepared by Elizabeth Sheley Ingenicomm 2 NAC Astrophysics Advisory Committee Teleconference Minutes, October 18-19, 2017 Wednesday, October 18, 2017 Introduction and Announcements Dr. Hashima Hasan, Executive Secretary of the Astrophysics Advisory Committee (APAC), opened the meeting by welcoming the Committee members. Dr. Hasan then reviewed the Federal Advisory Committee Act (FACA) rules. She noted that a few APAC members had conflicts of interest with specific topics on the agenda. Known conflicts of interest included Dr. Jason Kalirai (STScI) on the James Webb Space Telescope and Hubble Space Telescope; Drs. Mark Bautz (MIT) and Patricia Boyd (NASA GSFC) for the Transiting Exoplanet Survey Satellite (TESS); Dr. Bautz for the Chandra X-ray Observatory; Drs. -
Space Science Acronyms
Space Science Acronyms AA Auroral radio Absorption AACGM Altitude Adjusted Corrected GeoMagnetic ABI Auroral Boundary Index ACCENT Atmospheric Chemistry of Combustion Emissions Near the Tropopause ACE Advanced Composition Explorer ACF Auto Correlation Functions ACR Anomalous Cosmic Rays ADCS Attitude Determination and Control Subsystem ADEOS ADvanced Earth Observation Satellite (Japan) ADEP ARTIST Data Editing and Printing ADMS Atmospheric Density Mass Spectrometer AE Atmosphere Explorer AE Auroral Electrojet index AEPI Atmospheric Emissions Photometric Imager AES Auger Electron Spectroscopy AEU Antenna Element Unit AFB Air Force Base AFGL Air Force Geophysical Laboratory AFIT Air Force Institute of Technology AFOSR Air Force Office of Scientific Research AFRL Air Force Research Lab AFSCN Air Force Satellite Control Network AFSPC Air Force SPace Command AFWA Air Force Weather Agency AGILE Astrorivelatore Gamma a Immagini Leggero AGU American Geophysical Union AGW Atmospheric Gravity Waves AI Asymmetry Index AIDA Arecibo Initiative in Dynamics of the Atmosphere AIM Aeronomy of Ices in the Mesosphere AKR Auroral Kilometric Radiation AL Auroral Electrojet Lower Limit Index ALF Absorption Limiting Frequency ALIS Airglow Limb Imaging System ALOMAR Arctic Lidar Observatory for Middle Atmospheric Research ALOS Advanced Land Observing Satellite ALSP Apollo Lunar Surface Probe ALTAIR ARPA Long-Range Tracking and Identification Radar AMBER African Meridian B-field Educational Research Array AMCSR Advanced Modular Coherent Scatter Radar AMI Aeronomic