Challenges for a South Texas Spaceport
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Rsos/Fsos. Personnel Directly Supporting Or Interacting with an RSO/FSO During NASA Range Flight Operations
Range Flight Safety Operations Course: GSFC-RFSO Duration: 24 hours This introductory course focuses on the roles and responsibilities of the Range Safety Officer (RSO) or Flight Safety Officer (FSO) during Range Flight Safety activities and real-time support including pre- launch/flight, launch/flight, and recovery/landing for NASA Sounding Rocket, Unmanned Aircraft System, and Expendable Launch Vehicle operations. Range Flight Safety policies, guidelines, and requirements applicable to the duties of an RSO for each vehicle type are reviewed. Launch/Flight constraints and commit criteria, mission rules, day of launch/flight activities, and display techniques are presented. Tracking and telemetry, post-flight operations, lessons learned, and the use and importance of contingency plans are discussed. This course includes several classroom exercises to reinforce techniques and procedures utilized during Range Flight Safety operations. Due to the unique interaction with real-world equipment, this course is conducted at Wallops Flight Facility and class size is limited to a maximum of twelve (12) students. Prerequisites: SMA-AS-WBT-410, Range Flight Safety Orientation, or equivalent experience and/or training, is required. SMA-AS-WBT-335, Flight Safety Systems, or equivalent experience and/or training, is required. SMA-AS-WBT-435, NASA Range Flight Safety Analysis, or equivalent experience and/or training, is required. Target Audience: Anyone identified as needing initial training for personnel performing RSO/FSO functions during NASA range flight operations. Personnel in the management chain responsible for oversight of RSOs/FSOs. Personnel directly supporting or interacting with an RSO/FSO during NASA range flight operations. RELEASED - Printed documents may be obsolete; validate prior to use.. -
Centaur Dl-A Systems in a Nutshell
NASA Technical Memorandum 88880 '5 t I Centaur Dl-A Systems in a Nutshell (NASA-TM-8888o) CElTAUR D1-A SYSTEBS IN A N87- 159 96 tiljTSBELL (NASA) 29 p CSCL 22D Andrew L. Gordan Lewis Research Center Cleveland, Ohio January 1987 . CENTAUR D1-A SYSTEMS IN A NUTSHELL Andrew L. Gordan National Aeronautics and Space Administration Lewis Research Center Cleveland, Ohio 44135 SUMMARY This report identifies the unique aspects of the Centaur D1-A systems and subsystems. Centaur performance is described in terms of optimality (pro- pellant usage), flexibility, and airborne computer requirements. Major I-. systems are described narratively with some numerical data given where it may 03 CJ be useful. v, I W INTRODUCT ION The Centaur D1-A launch vehicle continues to be a key element in the Nation's space program. The Atlas/Centaur and Titan/Centaur combinations have boosted into orbit a variety of spacecraft on scientific, lunar, and planetary exploration missions and Earth orbit missions. These versatile, reliable, and accurate space booster systems will contribute to many significant space pro- grams well into the shuttle era. Centaur D1-A is the latest version of the Nation's first high-energy cryogenic launch vehicle. Major improvements in avionics and payload struc- ture have enhanced mission flexibility and mission success reliability. The liquid hydrogen and liquid oxygen propellants and the pressurized stainless steel structure provide a top-performance vehicle. Centaur's primary thrust comes from two Pratt 8, Whitney constant- thrust, turbopump-fed, regeneratively cooled, liquid-fueled rocket engines. Each RL10A-3-3a engine can generate 16 500 lb of thrust, for a total thrust of 33 000 lb. -
NTI Day 9 Astronomy Michael Feeback Go To: Teachastronomy
NTI Day 9 Astronomy Michael Feeback Go to: teachastronomy.com textbook (chapter layout) Chapter 3 The Copernican Revolution Orbits Read the article and answer the following questions. Orbits You can use Newton's laws to calculate the speed that an object must reach to go into a circular orbit around a planet. The answer depends only on the mass of the planet and the distance from the planet to the desired orbit. The more massive the planet, the faster the speed. The higher above the surface, the lower the speed. For Earth, at a height just above the atmosphere, the answer is 7.8 kilometers per second, or 17,500 mph, which is why it takes a big rocket to launch a satellite! This speed is the minimum needed to keep an object in space near Earth, and is called the circular velocity. An object with a lower velocity will fall back to the surface under Earth's gravity. The same idea applies to any object in orbit around a larger object. The circular velocity of the Moon around the Earth is 1 kilometer per second. The Earth orbits the Sun at an average circular velocity of 30 kilometers per second (the Earth's orbit is an ellipse, not a circle, but it's close enough to circular that this is a good approximation). At further distances from the Sun, planets have lower orbital velocities. Pluto only has an average circular velocity of about 5 kilometers per second. To launch a satellite, all you have to do is raise it above the Earth's atmosphere with a rocket and then accelerate it until it reaches a speed of 7.8 kilometers per second. -
Up, Up, and Away by James J
www.astrosociety.org/uitc No. 34 - Spring 1996 © 1996, Astronomical Society of the Pacific, 390 Ashton Avenue, San Francisco, CA 94112. Up, Up, and Away by James J. Secosky, Bloomfield Central School and George Musser, Astronomical Society of the Pacific Want to take a tour of space? Then just flip around the channels on cable TV. Weather Channel forecasts, CNN newscasts, ESPN sportscasts: They all depend on satellites in Earth orbit. Or call your friends on Mauritius, Madagascar, or Maui: A satellite will relay your voice. Worried about the ozone hole over Antarctica or mass graves in Bosnia? Orbital outposts are keeping watch. The challenge these days is finding something that doesn't involve satellites in one way or other. And satellites are just one perk of the Space Age. Farther afield, robotic space probes have examined all the planets except Pluto, leading to a revolution in the Earth sciences -- from studies of plate tectonics to models of global warming -- now that scientists can compare our world to its planetary siblings. Over 300 people from 26 countries have gone into space, including the 24 astronauts who went on or near the Moon. Who knows how many will go in the next hundred years? In short, space travel has become a part of our lives. But what goes on behind the scenes? It turns out that satellites and spaceships depend on some of the most basic concepts of physics. So space travel isn't just fun to think about; it is a firm grounding in many of the principles that govern our world and our universe. -
Multisatellite Determination of the Relativistic Electron Phase Space Density at Geosynchronous Orbit: Methodology and Results During Geomagnetically Quiet Times Y
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 110, A10210, doi:10.1029/2004JA010895, 2005 Multisatellite determination of the relativistic electron phase space density at geosynchronous orbit: Methodology and results during geomagnetically quiet times Y. Chen, R. H. W. Friedel, and G. D. Reeves Los Alamos National Laboratory, Los Alamos, New Mexico, USA T. G. Onsager NOAA, Boulder, Colorado, USA M. F. Thomsen Los Alamos National Laboratory, Los Alamos, New Mexico, USA Received 10 November 2004; revised 20 May 2005; accepted 8 July 2005; published 20 October 2005. [1] We develop and test a methodology to determine the relativistic electron phase space density distribution in the vicinity of geostationary orbit by making use of the pitch-angle resolved energetic electron data from three Los Alamos National Laboratory geosynchronous Synchronous Orbit Particle Analyzer instruments and magnetic field measurements from two GOES satellites. Owing to the Earth’s dipole tilt and drift shell splitting for different pitch angles, each satellite samples a different range of Roederer L* throughout its orbit. We use existing empirical magnetic field models and the measured pitch-angle resolved electron spectra to determine the phase space density as a function of the three adiabatic invariants at each spacecraft. Comparing all satellite measurements provides a determination of the global phase space density gradient over the range L* 6–7. We investigate the sensitivity of this method to the choice of the magnetic field model and the fidelity of the instrument intercalibration in order to both understand and mitigate possible error sources. Results for magnetically quiet periods show that the radial slopes of the density distribution at low energy are positive, while at high energy the slopes are negative, which confirms the results from some earlier studies of this type. -
FY2009 NRO Congressional Budget Justification Book
NATIONAL RECONNAISSANCE OFFICE 14675 Lee Road Chantilly, VA 20151-1715 6 July 2009 Mr. Steven Aftergood Senior Research Analyst Federation of American Scientists 1725 DeSales St NW, 6th Floor Washington, D.C. 20036 Dear Mr. Aftergood: This is in response to your faxed letter, dated 5 March 2008, received in the Information Management Services Center of the National Reconnaissance Office (NRO) on 7 March 2008. Pursuant to the Freedom of Information Act (FOIA), you requested "a copy of all unclassified portions of the NRO Congressional Budget Justification Book (CBJB) for Fiscal Year 2009.° Your request was processed in accordance with the Freedom of Information Act, 5 U.S.C. § 552, as amended. A thorough search of our files and databases located one record, consisting of 465 pages that is responsive to your request. This record is being released to you in part. Material withheld is denied pursuant to FOIA exemption(b) (3) which applies to information specifically exempt by statute, 50 U.S.C. § 403-1(i) which protects intelligence sources and methods from unauthorized disclosure. AS you are aware, the FOIA authorizes federal agencies to assess fees for record services. Based upon the information provided, you have been placed in the "other" category of requesters, which means that a requester is responsible for charges incurred for the cost of search time exceeding two hours and duplication in excess of the first 100 pages of document reproduction in the processing of this request. In your request, you expressed a willingness to pay fees up to the amount of $50.00. -
Minotaur I User's Guide
This page left intentionally blank. Minotaur I User’s Guide Revision Summary TM-14025, Rev. D REVISION SUMMARY VERSION DOCUMENT DATE CHANGE PAGE 1.0 TM-14025 Mar 2002 Initial Release All 2.0 TM-14025A Oct 2004 Changes throughout. Major updates include All · Performance plots · Environments · Payload accommodations · Added 61 inch fairing option 3.0 TM-14025B Mar 2014 Extensively Revised All 3.1 TM-14025C Sep 2015 Updated to current Orbital ATK naming. All 3.2 TM-14025D Sep 2018 Branding update to Northrop Grumman. All 3.3 TM-14025D Sep 2020 Branding update. All Updated contact information. Release 3.3 September 2020 i Minotaur I User’s Guide Revision Summary TM-14025, Rev. D This page left intentionally blank. Release 3.3 September 2020 ii Minotaur I User’s Guide Preface TM-14025, Rev. D PREFACE This Minotaur I User's Guide is intended to familiarize potential space launch vehicle users with the Mino- taur I launch system, its capabilities and its associated services. All data provided herein is for reference purposes only and should not be used for mission specific analyses. Detailed analyses will be performed based on the requirements and characteristics of each specific mission. The launch services described herein are available for US Government sponsored missions via the United States Air Force (USAF) Space and Missile Systems Center (SMC), Advanced Systems and Development Directorate (SMC/AD), Rocket Systems Launch Program (SMC/ADSL). For technical information and additional copies of this User’s Guide, contact: Northrop Grumman -
Three Events Occurred During This Period Which Together Constitute a Major Milestone in the Way Meteorological Data Are Pr
6.1 DESIGNING WEATHER SUPPORT FOR FUTURE RANGES – RESULTS FROM THE ADVANCED RANGE TECHNOLOGY WORKING GROUP WEATHER SUBGROUP William P. Roeder1 and John T. Madura2 145th Weather Squadron, Patrick Air Force Base, FL 2Weather Office, Kennedy Space Center, FL 1. INTRODUCTION 2. ARTWG WEATHER TECHNOLOGY ROADMAP The Advanced Range Technology Working Group The ARTWG Weather Subgroup, which included (ARTWG) was formed to identify the technologies government, industry and university participants, prepared required for the best performing, most cost-effective future a technology roadmap summarizing desired major space launch and test Ranges, and the R&D required to capabilities for optimal meteorological support to space achieve those technologies. The ARTWG resulted from a ranges for 25 years into the future. The 25-year planning White House Office of Science and Technology Policy time was further divided into three sub-periods (Table-2). (2000) report on the future of America’s space program. The near term requirements can be met with technology The White House tasked NASA and the U.S. Air Force to that is currently available and implementation can begin cooperatively identify the R&D requirements necessary to immediately. The mid term requirements are those that ensure the future competitiveness of U.S. ranges. Two will likely be available in 5-10 years or will require a small parallel initiatives resulted, the ARTWG (2004) co-chaired amount of development. The far term requirements are by NASA and the Air Force, and the companion Advanced advanced capabilities that will require considerable time Spaceport Technology Working Group (ASTWG) (2003), for research and development. -
Geosynchronous Orbit Determination Using Space Surveillance Network Observations and Improved Radiative Force Modeling
Geosynchronous Orbit Determination Using Space Surveillance Network Observations and Improved Radiative Force Modeling by Richard Harry Lyon B.S., Astronautical Engineering United States Air Force Academy, 2002 SUBMITTED TO THE DEPARTMENT OF AERONAUTICS AND ASTRONAUTICS IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF MASTER OF SCIENCE IN AERONAUTICS AND ASTRONAUTICS AT THE MASSACHUSETTS INSTITUTE OF TECHNOLOGY JUNE 2004 0 2004 Massachusetts Institute of Technology. All rights reserved. Signature of Author: Department of Aeronautics and Astronautics May 14, 2004 Certified by: Dr. Pa1 J. Cefola Technical Staff, the MIT Lincoln Laboratory Lecturer, Department of Aeronautics and Astronautics Thesis Supervisor Accepted by: Edward M. Greitzer H.N. Slater Professor of Aeronautics and Astronautics MASSACHUSETTS INS E OF TECHNOLOGY Chair, Committee on Graduate Students JUL 0 1 2004 AERO LBRARIES [This page intentionally left blank.] 2 Geosynchronous Orbit Determination Using Space Surveillance Network Observations and Improved Radiative Force Modeling by Richard Harry Lyon Submitted to the Department of Aeronautics and Astronautics on May 14, 2004 in Partial Fulfillment of the Requirements for the Degree of Master of Science in Aeronautics and Astronautics ABSTRACT Correct modeling of the space environment, including radiative forces, is an important aspect of space situational awareness for geostationary (GEO) spacecraft. Solar radiation pressure has traditionally been modeled using a rotationally-invariant sphere with uniform optical properties. This study is intended to improve orbit determination accuracy for 3-axis stabilized GEO spacecraft via an improved radiative force model. The macro-model approach, developed earlier at NASA GSFC for the Tracking and Data Relay Satellites (TDRSS), models the spacecraft area and reflectivity properties using an assembly of flat plates to represent the spacecraft components. -
Federal Register/Vol. 84, No. 72/Monday, April 15, 2019
15296 Federal Register / Vol. 84, No. 72 / Monday, April 15, 2019 / Proposed Rules DEPARTMENT OF TRANSPORTATION Docket: Background documents or FSS—Flight safety system comments received may be read at PC—Probability of casualty Federal Aviation Administration http://www.regulations.gov at any time. PI—Probability of impact Follow the online instructions for RLV—Reusable launch vehicle 14 CFR Parts 401, 404, 413, 414, 415, accessing the docket or go to the Docket Table of Contents 417, 420, 431, 433, 435, 437, 440, and Operations in Room W12–140 of the 450 I. Overview of Proposed Rule West Building Ground Floor at 1200 II. Background [Docket No.: FAA–2019–0229; Notice No. New Jersey Avenue SE, Washington, A. History 19–01] DC, between 9 a.m. and 5 p.m., Monday B. Licensing Process through Friday, except Federal holidays. C. National Space Council RIN 2120–AL17 FOR FURTHER INFORMATION CONTACT: For D. Streamlined Launch and Reentry Licensing Requirements Aviation Streamlined Launch and Reentry questions concerning this action, contact Randy Repcheck, Office of Rulemaking Committee Licensing Requirements III. Discussion of the Proposal Commercial Space Transportation, A. The FAA’s Approach To Updating and AGENCY: Federal Aviation Federal Aviation Administration, 800 Streamlining Launch and Reentry Administration (FAA), Department of Independence Avenue SW, Washington, Regulations Transportation (DOT). DC 205914; telephone (202) 267–8760; B. Single Vehicle Operator License ACTION: Notice of proposed rulemaking email [email protected]. C. Performance-Based Requirements and (NPRM). SUPPLEMENTARY INFORMATION: Means of Compliance D. Launch From a Federal Launch Range SUMMARY: This rulemaking would Authority for This Rulemaking E. -
Addendum to the 2019 Written Re-Evaluation of the 2014 Final Environmental Impact Statement for the Spacex Texas Launch Site
ADDENDUM TO THE 2019 WRITTEN RE-EVALUATION OF THE 2014 FINAL ENVIRONMENTAL IMPACT STATEMENT FOR THE SPACEX TEXAS LAUNCH SITE Introduction and Background Introduction This written re-evaluation (WR) evaluates whether supplemental environmental analysis is needed to address changes to Space Exploration Technologies Corporation’s (SpaceX) ongoing program of experimental test flights of a reusable suborbital launch vehicle from SpaceX’s Boca Chica Launch Site (formerly referred to as the Texas Launch Site). This program is being conducted pursuant to the licensed test program (LRLO 20-119A) the Federal Aviation Administration (FAA) Office of Commercial Space Transportation issued on May 28, 2020. The affected environment and environmental impacts of construction and operation of the Boca Chica site in Cameron County, Texas were analyzed in the 2014 Final Environmental Impact Statement for the SpaceX Texas Launch Site (2014 EIS; FAA 2014a). The FAA’s Record of Decision (ROD) was issued for this action on July 9, 2014. This WR describes modifications to SpaceX’s Security Plan, specifically its intention to limit public access to the closure area defined in the 2014 EIS for an increased number of hours, and evaluates whether the impacts of the proposed increase in closures1 fall within the scope of impacts analyzed in the 2014 EIS. To accommodate the existing licensed test program (LRLO 20-119A), the 180 hours of closures per year would need to be increased to up to 300 hours of closures per year. Due to the nature of the testing, there have been two instances where closures extended overnight following unplanned test anomalies to ensure public safety prior to opening the road the next morning. -
10/2/95 Rev EXECUTIVE SUMMARY This Report, Entitled "Hazard
10/2/95 rev EXECUTIVE SUMMARY This report, entitled "Hazard Analysis of Commercial Space Transportation," is devoted to the review and discussion of generic hazards associated with the ground, launch, orbital and re-entry phases of space operations. Since the DOT Office of Commercial Space Transportation (OCST) has been charged with protecting the public health and safety by the Commercial Space Act of 1984 (P.L. 98-575), it must promulgate and enforce appropriate safety criteria and regulatory requirements for licensing the emerging commercial space launch industry. This report was sponsored by OCST to identify and assess prospective safety hazards associated with commercial launch activities, the involved equipment, facilities, personnel, public property, people and environment. The report presents, organizes and evaluates the technical information available in the public domain, pertaining to the nature, severity and control of prospective hazards and public risk exposure levels arising from commercial space launch activities. The US Government space- operational experience and risk control practices established at its National Ranges serve as the basis for this review and analysis. The report consists of three self-contained, but complementary, volumes focusing on Space Transportation: I. Operations; II. Hazards; and III. Risk Analysis. This Executive Summary is attached to all 3 volumes, with the text describing that volume highlighted. Volume I: Space Transportation Operations provides the technical background and terminology, as well as the issues and regulatory context, for understanding commercial space launch activities and the associated hazards. Chapter 1, The Context for a Hazard Analysis of Commercial Space Activities, discusses the purpose, scope and organization of the report in light of current national space policy and the DOT/OCST regulatory mission.