January 2019 | Page 1
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Bolden Testimony
HOLD FOR RELEASE UNTIL PRESENTED BY WITNESS November 17, 2011 Statement of The Honorable Charles F. Bolden, Jr. Administrator National Aeronautics and Space Administration before the Subcommittee on Science and Space Committee on Commerce, Science and Transportation U. S. Senate Mr. Chairman and Members of the Subcommittee, thank you for the opportunity to appear before you today to discuss the outlook for NASA’s human space flight program. This has been a remarkable year, as we have completed assembling and outfitting of the U.S. On-orbit Segment (USOS) of the International Space Station (ISS), allowing us to focus on full utilization of the Station’s research capabilities; taken key steps in moving forward into the future of exploration beyond Low-Earth Orbit (LEO); celebrated the 50 th anniversary of human spaceflight; and witnessed the successful conclusion of the historic Space Shuttle Program. We are also pleased with the progress our industry partners have made in developing an American capability to transport cargo and eventually astronauts to the ISS, and end the outsourcing of this work to foreign governments. More importantly, this will add a critical level of redundancy for transporting cargo and crew to the ISS. A robust transportation architecture is important to ensuring full utilization of this amazing research facility. Enabling commercial crew and cargo transportation systems in LEO allows NASA to focus on developing its own systems for sending astronauts on missions of exploration beyond LEO. This split between commercial and Government systems allows for a cost effective approach to promote a broad base for human exploration by the United States. -
Through Astronaut Eyes: Photographing Early Human Spaceflight
Purdue University Purdue e-Pubs Purdue University Press Book Previews Purdue University Press 6-2020 Through Astronaut Eyes: Photographing Early Human Spaceflight Jennifer K. Levasseur Follow this and additional works at: https://docs.lib.purdue.edu/purduepress_previews This document has been made available through Purdue e-Pubs, a service of the Purdue University Libraries. Please contact [email protected] for additional information. THROUGH ASTRONAUT EYES PURDUE STUDIES IN AERONAUTICS AND ASTRONAUTICS James R. Hansen, Series Editor Purdue Studies in Aeronautics and Astronautics builds on Purdue’s leadership in aeronautic and astronautic engineering, as well as the historic accomplishments of many of its luminary alums. Works in the series will explore cutting-edge topics in aeronautics and astronautics enterprises, tell unique stories from the history of flight and space travel, and contemplate the future of human space exploration and colonization. RECENT BOOKS IN THE SERIES British Imperial Air Power: The Royal Air Forces and the Defense of Australia and New Zealand Between the World Wars by Alex M Spencer A Reluctant Icon: Letters to Neil Armstrong by James R. Hansen John Houbolt: The Unsung Hero of the Apollo Moon Landings by William F. Causey Dear Neil Armstrong: Letters to the First Man from All Mankind by James R. Hansen Piercing the Horizon: The Story of Visionary NASA Chief Tom Paine by Sunny Tsiao Calculated Risk: The Supersonic Life and Times of Gus Grissom by George Leopold Spacewalker: My Journey in Space and Faith as NASA’s Record-Setting Frequent Flyer by Jerry L. Ross THROUGH ASTRONAUT EYES Photographing Early Human Spaceflight Jennifer K. -
Espinsights the Global Space Activity Monitor
ESPInsights The Global Space Activity Monitor Issue 2 May–June 2019 CONTENTS FOCUS ..................................................................................................................... 1 European industrial leadership at stake ............................................................................ 1 SPACE POLICY AND PROGRAMMES .................................................................................... 2 EUROPE ................................................................................................................. 2 9th EU-ESA Space Council .......................................................................................... 2 Europe’s Martian ambitions take shape ......................................................................... 2 ESA’s advancements on Planetary Defence Systems ........................................................... 2 ESA prepares for rescuing Humans on Moon .................................................................... 3 ESA’s private partnerships ......................................................................................... 3 ESA’s international cooperation with Japan .................................................................... 3 New EU Parliament, new EU European Space Policy? ......................................................... 3 France reflects on its competitiveness and defence posture in space ...................................... 3 Germany joins consortium to support a European reusable rocket......................................... -
Deep Space Atomic Clock
National Aeronautics and Space Administration Deep Space Atomic Clock tion and radio science. Here are some examples of how one-way deep-space tracking with DSAC can improve navigation and radio science that is not supported by current two-way tracking. Ground-based 1. Simultaneously track two spacecraft on a atomic clocks are downlink with the Deep Space Network (DSN) the cornerstone of at destinations such as Mars, and nearly dou- spacecraft navigation ble a space mission’s tracking data because it for most deep-space missions because of their use no longer has to “time-share” an antenna. in generating precision two-way tracking measure- ments. These typically include range (the distance 2. Improve tracking data precision by an order of between two objects) and Doppler (a measure of magnitude using the DSN’s Ka-band downlink the relative speed between them). A two-way link (a tracking capability. signal that originates and ends at the ground track- ing antenna) is required because today’s spacecraft 3. Mitigate Ka-band’s weather sensitivity (as clocks introduce too much error for the equivalent compared to two-way X-band) by being able one-way measurements to be useful. Ground atom- to switch from a weather-impacted receiving ic clocks, while providing extremely stable frequen- antenna to one in a different location with no cy and time references, are too large for hosting on tracking outages. a spacecraft and cannot survive the harshness of space. New technology is on the horizon that will 4. Track longer by using a ground antenna’s en- change this paradigm. -
Celebrating the Wonder of the Night Sky
Celebrating the Wonder of the Night Sky The heavens proclaim the glory of God. The skies display his craftsmanship. Psalm 19:1 NLT Celebrating the Wonder of the Night Sky Light Year Calculation: Simple! [Speed] 300 000 km/s [Time] x 60 s x 60 m x 24 h x 365.25 d [Distance] ≈ 10 000 000 000 000 km ≈ 63 000 AU Celebrating the Wonder of the Night Sky Milkyway Galaxy Hyades Star Cluster = 151 ly Barnard 68 Nebula = 400 ly Pleiades Star Cluster = 444 ly Coalsack Nebula = 600 ly Betelgeuse Star = 643 ly Helix Nebula = 700 ly Helix Nebula = 700 ly Witch Head Nebula = 900 ly Spirograph Nebula = 1 100 ly Orion Nebula = 1 344 ly Dumbbell Nebula = 1 360 ly Dumbbell Nebula = 1 360 ly Flame Nebula = 1 400 ly Flame Nebula = 1 400 ly Veil Nebula = 1 470 ly Horsehead Nebula = 1 500 ly Horsehead Nebula = 1 500 ly Sh2-106 Nebula = 2 000 ly Twin Jet Nebula = 2 100 ly Ring Nebula = 2 300 ly Ring Nebula = 2 300 ly NGC 2264 Nebula = 2 700 ly Cone Nebula = 2 700 ly Eskimo Nebula = 2 870 ly Sh2-71 Nebula = 3 200 ly Cat’s Eye Nebula = 3 300 ly Cat’s Eye Nebula = 3 300 ly IRAS 23166+1655 Nebula = 3 400 ly IRAS 23166+1655 Nebula = 3 400 ly Butterfly Nebula = 3 800 ly Lagoon Nebula = 4 100 ly Rotten Egg Nebula = 4 200 ly Trifid Nebula = 5 200 ly Monkey Head Nebula = 5 200 ly Lobster Nebula = 5 500 ly Pismis 24 Star Cluster = 5 500 ly Omega Nebula = 6 000 ly Crab Nebula = 6 500 ly RS Puppis Variable Star = 6 500 ly Eagle Nebula = 7 000 ly Eagle Nebula ‘Pillars of Creation’ = 7 000 ly SN1006 Supernova = 7 200 ly Red Spider Nebula = 8 000 ly Engraved Hourglass Nebula -
Brisbane South - Logan -Gold Coast - Tweed Heads
Southern Astronomical Society - Brisbane South - Logan -Gold Coast - Tweed Heads - www.sas.org.au SEPTEMBER 2019 Greg Bock ~ IC5332 - face on spiral 2 SEPTEMBER 2019 Mark Boothman ~ Andromeda Galaxy 3 SEPTEMBER 2019 ~ SAS Facebook Page Image Credit & Copyright: Michael Miller, Jimmy Walker https://apod.nasa.gov/apod/ ap190824.html Explanation: Globular star cluster Omega Centauri, also known as NGC 5139, is some 15,000 light-years away. http:// www.remarkableheavens.com/ http://jwalk.smugmug.com/ 4 SEPTEMBER 2019 Glenn Burgess ~ Jupiter 5 OCTOBER 2019 Tony Kim ~ Fornax barred galaxy and friends. 6 OCTOBER 2019 Mark Boothman ~ Pleiades aka Seven Sisters, Subaru. 7 OCTOBER 2019 ~ SAS FACEBOOK PAGE Chandra X-ray Observatory "Mystic Mountain" shows the glow of oxygen in blue, hydrogen & nitrogen in green, and sulphur in red. 8 OCTOBER 2019 ~ In the News [ 50 years since the Murchison Meteorite landed in the Victorian countryside. A total of 4 kilograms of Murchison meteorite sits in the Melbourne Museum collection. ABC Science: Fiona Pepper 9 OCTOBER 2019 David Bainbridge ~ Casper the Friendly Ghost Nebula 10 NOVEMBER 2019 John McLennan ~ ORION NEBULA 11 NOVEMBER 2019 Ray Suckling ~ Horse Head NebulaB33, Horse Head Nebu- 12 NOVEMBER 2019 , Mark Boothman ~ Orion Nebula / Orion 13 NOVEMBER 2019 ~ SAS FACEBOOK PAGE The Skeptics' Guide to the Universe This is the clearest picture of Mars to date. 14 NOVEMBER 2019 Tony Kim ~ Horse Head Nebula 15 DECEMBER 2019 ~ Combined Societies Meeting Pat Pearl, Peter Marples and Greg Bock (members of the BOSS team) receiving their awards for supernova discoveries from SAS President, Brendan Junge. 16 DECEMBER 2019 Mike Geisel ~ M42 the Great Nebulae in Orion 17 DECEMBER 2019 Tony Kim ~ Andromeda 18 DECEMBER 2019 ~ SAS FACEBOOK PAGE NASA Solar System Exploration Danielson Crater, an impact crater about 42 miles or 67 kilometres in diameter, located in the southwest Arabia Terra region of Mars. -
SAMENA TRENDS Bocar A
Volume 10, August, 2019 A SAMENA Telecommunications Council Publication www.samenacouncil.org S AMENA TRENDS FOR SAMENA TELECOMMUNICATIONS COUNCIL'S MEMBERS BUILDING DIGITAL ECONOMIES Tech Mahindra: The Rise of the DX-Organization ... 59 Loon: Overcoming the Infrastructure Challenge in Broadband ... 74 Featured Eng. Nezar Banbeela Chief Executive Officer VIVA Bahrain THIS MONTH MATERIALIZING THE DIGITAL AGENDA 7441_Et_Business Mobile App_SAMENA Magazine_A4.indd 1 5/21/19 1:36 PM VOLUME 10, AUGUST, 2019 Contributing Editors Knowledge Contributions Subscriptions Izhar Ahmad Alfa [email protected] SAMENA Javaid Akhtar Malik Huawei Loon Advertising TRENDS Syniverse [email protected] Tech Mahindra Editor-in-Chief SAMENA TRENDS Bocar A. BA Publisher [email protected] SAMENA Telecommunications Tel: +971.4.364.2700 Council CONTENTS 05 EDITORIAL FEATURED 10 REGIONAL & MEMBERS UPDATES Members News Regional News 62 SATELLITE UPDATES Satellite News 77 WHOLESALE UPDATES Wholesale News 83 TECHNOLOGY UPDATES The SAMENA TRENDS newsletter is wholly Technology News 06 Eng. Nezar Banabeela owned and operated by The SAMENA Chief Executive Officer Telecommunications Council (SAMENA 92 REGULATORY & POLICY UPDATES VIVA Bahrain Council). Information in the newsletter is not Regulatory News intended as professional services advice, and SAMENA Council disclaims any liability for A Snapshot of Regulatory use of specific information or results thereof. Activities in the SAMENA Region Articles and information contained in this publication -
The Observer Battle Point Astronomical Association
September 2021 VOL. 13 THE OBSERVER BATTLE POINT ASTRONOMICAL ASSOCIATION WWW.BPASTRO.ORG BAINBRIDGE ISLAND, WA CALL TO ACTION: Oppose Soccer Lights at James Webb Space Telescope Event at KiDiMu Battle Point Park! As was mentioned in the last newsletter, the Bainbridge Island As you have likely heard, there is a proposal to light the soccer Kids Discovery Museum (KiDiMu) has been selected by NASA to fields for nighttime soccer practice and play, Monday through be an official host of the Webb Telescope Community Events Friday 5 to 9 PM from October to March, but could expand to Initiative. Based on the BPAA’s agreement to partner with include longer hours, weekends, and other fields (pickle ball, KiDiMu, planning has begun to assist them in this event. tennis, field hockey, baseball). The James Webb Space Telescope (JWST) launch has slipped from October 31st, based on the shipment of the telescope, the Opposition has arisen to this proposal for all kinds of reasons, top readiness of the Ariane 5 rocket, and the readiness of the of the list is the impact lights will have on the Ritchie Observatory. spaceport in South America. Therefore, KiDiMu is planning a Other reasons are traffic and safety, as well as impacts to wildlife. one-day event on November 20th (the Saturday before We’re doing our best to stop it at Battle Point Park and identify an Thanksgiving), at which we would participate with activities and alternative location. exhibits (a few telescopes that the kids can touch, for example). We are also planning to have some BPAA members each A neighborhood group --- the Battle Point Alliance --- has joined spending an hour or two at KiDiMu during the week leading up to with the Battle Point Astronomical Association to resist any plan the event to discuss space science, telescopes, and launches. -
Asteroid Redirect Mission (ARM) Formulation Assessment and Support Team (FAST) Final Report
NASA/TM–2016-219011 Asteroid Redirect Mission (ARM) Formulation Assessment and Support Team (FAST) Final Report Daniel D. Mazanek and David M. Reeves, Langley Research Center, Hampton, Virginia Paul A. Abell, Johnson Space Center, Houston, Texas Erik Asphaug, Arizona State University, Tempe, Arizona Neyda M. Abreu, Penn State DuBois, DuBois, Pennsylvania James F. Bell, Arizona State University, Tempe, Arizona William F. Bottke, Southwest Research Institute, Boulder, Colorado Daniel T. Britt and Humberto Campins, University of Central Florida, Orlando, Florida Paul W. Chodas, Jet Propulsion Laboratory, Pasadena, California Carolyn M. Ernst, John Hopkins University, Laurel, Maryland Marc D. Fries, Johnson Space Center, Houston, Texas Leslie S. Gertsch, Missouri University of Science and Technology, Rolla, Missouri Daniel P. Glavin, Goddard Space Flight Center, Greenbelt, Maryland Christine M. Hartzell, University of Maryland, College Park, Maryland Amanda R. Hendrix, Planetary Science Institute, Niwot, Colorado Joseph A. Nuth, Goddard Space Flight Center, Greenbelt, Maryland Daniel J. Scheeres, University of Colorado, Boulder, Colorado Joel C. Sercel, TransAstra Corporation, Lake View Terrace, California Driss Takir, United States Geological Survey, Flagstaff, Arizona Kris Zacny, Honeybee Robotics, Pasadena, California February 2016 NASA STI Program ... in Profile Since its founding, NASA has been dedicated to the CONFERENCE PUBLICATION. advancement of aeronautics and space science. The Collected papers from scientific and technical NASA scientific and technical information (STI) conferences, symposia, seminars, or other program plays a key part in helping NASA maintain meetings sponsored or this important role. co-sponsored by NASA. The NASA STI program operates under the auspices SPECIAL PUBLICATION. Scientific, technical, or of the Agency Chief Information Officer. -
How the 'Pillars of Creation' Were Created 26 June 2014, by Dr Robert Massey
How the 'Pillars of Creation' were created 26 June 2014, by Dr Robert Massey During their most stable phase on the so-called main sequence, they have surface temperatures of more than 30,000 degrees Celsius (on the Sun the surface is about 5500 degrees), are strong sources of ultraviolet light and emit copious material in a powerful wind. All of this shapes their surroundings. The O-type stars heat any interstellar gas in their vicinity, creating bubbles which act like snow ploughs sweeping up surrounding colder material. In these regions, where gas is compressed, large numbers of new stars are seen forming so many scientists argue that the O stars drive star formation. The famous Hubble Space Telescope image of the 'Pillars of Creation', from 1995. Credit: NASA / ESA / STScI / J. Hester and P. Scowen (Phys.org) —The 'Pillars of Creation', an image made with the Hubble Space Telescope in 1995, is one of the most famous astronomical views. It shows how 'elephant trunks' of cooler interstellar gas are eroded by the intense radiation and winds from nearby massive stars. Now Scott Balfour, an astronomer at Cardiff University, has run a new simulation where similar structures appear with a remarkably close appearance to their real life counterparts. He also An image from the simulation, showing a slice of space suggests that the stars that make these structures 25 x 25 light years across and 0.2 light years thick (for are of little help in forming new siblings. On reference 1 light year is about 9.6 million million km or a Thursday 26 June Scott will present his results in a bit more than 63000 times the distance from the Earth to talk at the National Astronomy Meeting in the Sun). -
Writing Successful Proposals: OBSERVATIONS from NASA
Writing Successful Proposals: OBSERVATIONS FROM NASA Dr. Thomas H. Zurbuchen Associate Administrator Science Mission Directorate @Dr_ThomasZ Context for Today's Talk • Only focused on Announcements of Opportunity, not ROSES selections • Large and increasing number of NASA science missions led by PIs • Proven high rates of mission success across science disciplines resulting from PI-class missions management methodology • Process of becoming a PI is complex and involves many stakeholders, with more than 80% of all submitted mission proposals failing at Step 1 • Will use historical data to discuss our view of process and philosophy, questioning how we can do better • Already changed proposal process and will without doubt, do it again • Note, some comments reflect views of the current NASA Science Associate Administrator and leadership team • Today’s talk is being webcast and recorded; all content will be made available on science.nasa.gov/researchers/new-pi-resources 2 Imagine Being a PI… • You receive a call from me informing you that your mission was selected for development • Your life changes in a heartbeat; you have already invested a significant fraction of at least two years with your project, and know strengths and weaknesses of your partners and team • You have survived two major down-selects; you have managed to raise support measured in millions of dollars and in work-years from your team • You know you have lots of autonomy, but you have lots of responsibility as well; you will represent your mission, NASA, and an entire science -
A Great Successor to the Hubble Space Telescope
Astro2020 APC White Paper Title: A Great Successor to the Hubble Space Telescope Type of Activity: Space Based Project Principal Author: Name: B. Scott Gaudi Institution: The Ohio State University Email: [email protected] Phone: 614-292-1914 Co-authors: Shawn Domagal-Goldman, GSFC, [email protected], Debra Fischer, Yale University, [email protected], Alina Kiessling, JPL, [email protected], Bertrand Mennesson, JPL, [email protected], Bradley M. Peterson, Ohio State University/STScI, [email protected], Aki Roberge, GSFC, [email protected], Dan Stern, JPL, [email protected], Keith Warfield, JPL, [email protected] The Legacy of the Hubble Space Telescope (HST) There is perhaps no more iconic and immediately recognizable image of a space telescope than that of HST (Figure 1). HST was launched on April 24, 1990, and is approaching its 30th anniversary. HST has inspired generations of scientists, with such iconic images at the “Pillars of Creation”, the “Hubble eXtreme Deep Field”, and extraordinary images of resolved stellar populations (Figure 2). HST has made important contributions to nearly every area of astronomy and planetary science, resulting in over 16,000 refereed publications. While these contributions are too numerous to Figure 1. The Hubble Space Telescope from list here, it is worth highlighting a few notable orbit. NASA/ESA examples uniquely enabled by space-based observations at wavelengths short than 600nm. We will also highlight how improved UV/Optical capabilities, such as will be available with HabEx or LUVOIR, would substantially or dramatically improve these science cases.