Solar System Exploration: a Vision for the Next Hundred Years
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The Space Launch System for Exploration and Science. K
45th Lunar and Planetary Science Conference (2014) 2234.pdf THE SPACE LAUNCH SYSTEM FOR EXPLORATION AND SCIENCE. K. Klaus1, M. S. Elsperman1, B. B. Donahue1, K. E. Post1, M. L. Raftery1, and D. B. Smith1, 1The Boeing Company, 13100 Space Center Blvd, Houston TX 77059, [email protected], [email protected], [email protected], mi- [email protected], [email protected], [email protected]. Introduction: The Space Launch System (SLS) is same time which will simplify mission design and re- the most powerful rocket ever built and provides a duce launch costs. One of the key features of the SLS critical heavy-lift launch capability enabling diverse in cislunar space is performance to provide “dual-use”, deep space missions. This exploration class vehicle i.e. Orion plus 15t of any other payload. launches larger payloads farther in our solar system An opportunity exists to deliver payload to the lu- and faster than ever before. Available fairing diameters nar surface or lunar orbit on the unmanned 2017 range from 5 m to 10 m; these allow utilization of ex- MPCV/ SLS test flight (~4.5t of mass margin exists for isting systems which reduces development risks, size this flight). Concepts of this nature can be done for limitations and cost. SLS injection capacity shortens less than Discovery class mission budgets (~$450M) mission travel time. Enhanced capabilities enable a and may be done as a joint venture by the NASA Sci- variety of missions including human exploration, plan- ence Mission Directorate and Human Exploration Op- etary science, astrophysics, heliophysics, planetary erations Mission Directorate using the successful Lu- defense, Earth observaton and commercial space en- nar Reconnaissance Orbiter as a program model. -
Breakthrough Propulsion Study Assessing Interstellar Flight Challenges and Prospects
Breakthrough Propulsion Study Assessing Interstellar Flight Challenges and Prospects NASA Grant No. NNX17AE81G First Year Report Prepared by: Marc G. Millis, Jeff Greason, Rhonda Stevenson Tau Zero Foundation Business Office: 1053 East Third Avenue Broomfield, CO 80020 Prepared for: NASA Headquarters, Space Technology Mission Directorate (STMD) and NASA Innovative Advanced Concepts (NIAC) Washington, DC 20546 June 2018 Millis 2018 Grant NNX17AE81G_for_CR.docx pg 1 of 69 ABSTRACT Progress toward developing an evaluation process for interstellar propulsion and power options is described. The goal is to contrast the challenges, mission choices, and emerging prospects for propulsion and power, to identify which prospects might be more advantageous and under what circumstances, and to identify which technology details might have greater impacts. Unlike prior studies, the infrastructure expenses and prospects for breakthrough advances are included. This first year's focus is on determining the key questions to enable the analysis. Accordingly, a work breakdown structure to organize the information and associated list of variables is offered. A flow diagram of the basic analysis is presented, as well as more detailed methods to convert the performance measures of disparate propulsion methods into common measures of energy, mass, time, and power. Other methods for equitable comparisons include evaluating the prospects under the same assumptions of payload, mission trajectory, and available energy. Missions are divided into three eras of readiness (precursors, era of infrastructure, and era of breakthroughs) as a first step before proceeding to include comparisons of technology advancement rates. Final evaluation "figures of merit" are offered. Preliminary lists of mission architectures and propulsion prospects are provided. -
Congress of the United States Congressional Budget Office May 1988
CONGRESS OF THE UNITED STATES CONGRESSIONAL BUDGET OFFICE MAY 1988 A SPECIAL STUDY THE NASA PROGRAM IN THE 1990s AND BEYOND The Congress of the United States Congresssional Budget Of'f'ice NOTES All costs are expressed in 1988 dollars of budget authority, unless otherwise noted. All years are fiscal years, except when applied to launch schedules. PREFACE The United States space program stands at a crossroads. The momentum of the National Aeronautics and Space Administration (NASA) program over the last 20 years has brought NASA to a point where new activities will require substantial increases in the agency's budget. Critics of the NASA program have called for even more ambi- tious goals, most prominently an expansion of manned space flight to the Moon or Mars. Fiscal concerns, however, may limit even the more modest set of activities envisioned by NASA. This special study, requested by the Senate Committee on Commerce, Science, and Trans- portation, examines the broad options for the U.S. space program in the 1990s. In keeping with the mandate of the Congressional Budget Office (CBO) to provide objective nonpartisan analysis, the report makes no recommendations. David H. Moore, of CBO's Natural Resources and Commerce Division, prepared the report under the supervision of Everett M. Ehrlich. Frances M. Lussier of CBO's National Security Division and Michael Sieverts of CBO's Budget Analysis Division provided valu- able comments and assistance. Many outside reviewers made useful comments and criticisms. Amanda Balestrieri edited the manuscript. Margaret Cromartie prepared early drafts of the report, and Kathryn Quattrone prepared the final draft for publication. -
Electric Propulsion System Modeling for the Proposed Prometheus 1 Mission
NASA/TM—2005-213892 AIAA–2005–3891 Electric Propulsion System Modeling for the Proposed Prometheus 1 Mission Douglas Fiehler QSS Group, Inc., Cleveland, Ohio Ryan Dougherty Jet Propulsion Laboratory, Pasadena, California David Manzella Glenn Research Center, Cleveland, Ohio September 2005 The NASA STI Program Office . in Profile Since its founding, NASA has been dedicated to • CONFERENCE PUBLICATION. Collected the advancement of aeronautics and space papers from scientific and technical science. The NASA Scientific and Technical conferences, symposia, seminars, or other Information (STI) Program Office plays a key part meetings sponsored or cosponsored by in helping NASA maintain this important role. NASA. The NASA STI Program Office is operated by • SPECIAL PUBLICATION. Scientific, Langley Research Center, the Lead Center for technical, or historical information from NASA’s scientific and technical information. The NASA programs, projects, and missions, NASA STI Program Office provides access to the often concerned with subjects having NASA STI Database, the largest collection of substantial public interest. aeronautical and space science STI in the world. The Program Office is also NASA’s institutional • TECHNICAL TRANSLATION. English- mechanism for disseminating the results of its language translations of foreign scientific research and development activities. These results and technical material pertinent to NASA’s are published by NASA in the NASA STI Report mission. Series, which includes the following report types: Specialized services that complement the STI • TECHNICAL PUBLICATION. Reports of Program Office’s diverse offerings include completed research or a major significant creating custom thesauri, building customized phase of research that present the results of databases, organizing and publishing research NASA programs and include extensive data results . -
Comet/Asteroid Protection System (CAPS): Preliminary Space-Based System Concept and Study Results
NASA/TM-2005-213758 Comet/Asteroid Protection System (CAPS): Preliminary Space-Based System Concept and Study Results Daniel D. Mazanek, Carlos M. Roithmayr, and Jeffrey Antol Langley Research Center, Hampton, Virginia Sang-Young Park, Robert H. Koons, and James C. Bremer Swales Aerospace, Inc., Hampton, Virginia Douglas G. Murphy, James A. Hoffman, Renjith R. Kumar, and Hans Seywald Analytical Mechanics Associates, Inc., Hampton, Virginia Linda Kay-Bunnell and Martin R. Werner Joint Institute for Advancement of Flight Sciences (JIAFS) The George Washington University, Hampton, Virginia Matthew A. Hausman Colorado Center for Astrodynamics Research The University of Colorado, Boulder, Colorado Jana L. Stockum San Diego State University, San Diego, California May 2005 The NASA STI Program Office . in Profile Since its founding, NASA has been dedicated to the • CONFERENCE PUBLICATION. Collected advancement of aeronautics and space science. The papers from scientific and technical NASA Scientific and Technical Information (STI) conferences, symposia, seminars, or other Program Office plays a key part in helping NASA meetings sponsored or co-sponsored by NASA. maintain this important role. • SPECIAL PUBLICATION. Scientific, The NASA STI Program Office is operated by technical, or historical information from NASA Langley Research Center, the lead center for NASA’s programs, projects, and missions, often scientific and technical information. The NASA STI concerned with subjects having substantial Program Office provides access to the NASA STI public interest. Database, the largest collection of aeronautical and space science STI in the world. The Program Office is • TECHNICAL TRANSLATION. English- also NASA’s institutional mechanism for language translations of foreign scientific and disseminating the results of its research and technical material pertinent to NASA’s mission. -
982-R120461 October 1, 2005
982-R120461 October 1, 2005 PROMETHEUS PROJECT National Aeronautics and Space Administration Final Report Jet Propulsion Laboratory California Institute of Technology Pasadena, California [This page intentionally left blank] 982-R120461 PROMETHEUS PROJECT OCTOBER 1, 2005 FINAL REPORT Signature Page Name Title Date Signature Randall Taylor Prometheus Project Closeout Manager i 982-R120461 PROMETHEUS PROJECT OCTOBER 1, 2005 FINAL REPORT [This page intentionally left blank] ii 982-R120461 PROMETHEUS PROJECT OCTOBER 1, 2005 FINAL REPORT Acknowledgement The Jet Propulsion Laboratory (JPL), a division of the California Institute of Technology, manages the Prometheus Project for the National Aeronautics and Space Administration’s Prometheus Nuclear Systems Program. iii 982-R120461 PROMETHEUS PROJECT OCTOBER 1, 2005 FINAL REPORT [This page intentionally left blank] iv 982-R120461 PROMETHEUS PROJECT OCTOBER 1, 2005 FINAL REPORT TABLE OF CONTENTS 1. INTRODUCTION..............................................................................................................1 1.1 Project Identification................................................................................................1 1.2 Project Summary......................................................................................................1 1.3 Project History .........................................................................................................2 1.4 Scope of Final Report ..............................................................................................4 -
Interstellar Travel Or Even 1.3 Mlbs at Launch
Terraforming Mars: By Aliens? Astronomy 330 •! Sometime movies are full of errors. •! But what can you do? Music: Rocket Man– Elton John Online ICES Question •! ICES forms are available online, so far 39/100 Are you going to fill out an ICES form before the students have completed it. deadline? •! I appreciate you filling them out! •! Please make sure to leave written comments. I a)! Yes, I did it already. find these comments the most useful, and typically b)! Yes, sometime today that’s where I make the most changes to the c)! Yes, this weekend course. d)! Yes, I promise to do it before the deadline of May6th! e)! No, I am way too lazy to spend 5 mins to help you or future students out. Final Final •! In this classroom, Fri, May 7th, 0800-1100. •! A normal-sized sheet of paper with notes on both •! Will consist of sides is allowed. –! 15 question on Exam 1 material. •! Exam 1and 2 and last year’s final are posted on –! 15 question on Exam 2 material. class website (not Compass). –! 30 questions from new material (Lect 20+). –! +4 extra credit questions •! I will post a review sheet Friday. •! A total of 105 points, i.e. 5 points of extra credit. •! Final Exam grade is based on all three sections. •! If Section 1/2 grade is higher than Exam 1/2 grade, then it will replace your Exam 1/2 grade. Final Papers Outline •! Final papers due at BEGINNING of discussion •! Rockets: how to get the most bang for the buck. -
Entire Issue in PDF Format
AMERICAN RANDONNEUR VOLUME 23 • ISSUE #3 FALL 2020 IN THIS Bikepacking the WestX Trail, 2020 — JAY FICHIALOS Cycling During the Novel Coronavirus Pandemic — MARY FOLEY ISSUE High Hopes Dashed but a Silver Lining Emerges — DAVID NALL NEW, Northern Transcontinental Mid July to Mid August 34 days, 3,700 miles, 110 miles per day We changed 1,000 miles of this route and added two more days across the midwestern states. This tour begins in Everett, Washington and crosses the northern states of Washington, Idaho, Montana, Pacific Atlantic Cycling Tour Wyoming, South Dakota, Minnesota, Wisconsin, Illinois, Indiana, Ohio, Pennsylvania, New York, www.pactour.com Vermont, Massachusetts before ending in Portsmouth, Lon Haldeman and Susan Notorangelo New Hampshire. This tour is almost filled with Contact us... 262-736-2453 50 riders on the waiting list [email protected] Southern Transcontinental Planning Ahead for 2021 Celebrating Lon and Susan’s 100th Cycling Event Across America Due to the ever changing Covid-19 virus Early September to early October This will be a 27 day tour from San Diego, California to restrictions all tours and dates are subject Tybee Island (Savannah) Georgia. Most days average to change. 110 miles. We will cross the country through a variety of terrain and visit many historical sites along the way. PAC tour will have a full schedule of popular tours for the 2021 season including our Arizona Desert Cycling Camp. Many of these tours have been filling up one year in advance. We are listing these tours now so you can Andes to the Amazon in Peru prepare to sign up when registration opens. -
The Challenge of Interstellar Travel the Challenge of Interstellar Travel
The challenge of interstellar travel The challenge of interstellar travel ! Interstellar travel - travel between star systems - presents one overarching challenge: ! The distances between stars are enormous compared with the distances which our current spacecraft have travelled ! Voyager I is the most distant spacecraft, and is just over 100 AU from the Earth ! The closest star system (Alpha Centauri) is 270,000 AU away! ! Also, the speed of light imposes a strict upper limit to how fast a spacecraft can travel (300,000 km/s) ! in reality, only light can travel this fast How long does it take to travel to Alpha Centauri? Propulsion Ion drive Chemical rockets Chemical Nuclear drive Solar sail F = ma ! Newton’s third law. ! Force = mass x acceleration. ! You bring the mass, your engine provides the force, acceleration is the result The constant acceleration case - plus its problems ! Let’s take the case of Alpha Centauri. ! You are provided with an ion thruster. ! You are told that it provides a constant 1g of acceleration. ! Therefore, you keep accelerating until you reach the half way point before reversing the engine and decelerating the rest of the way - coming to a stop at Alpha Cen. ! Sounds easy? Relativity and nature’s speed limit ! What does it take to maintain 1g of accelaration? ! At low velocities compared to light to accelerate a 1000kg spacecraft at 1g (10ms-2) requires 10,000 N of force. ! However, as the velocity of the spacecraft approaches the velocity of light relativity starts to kick in. ! The relativistic mass can be written as γ x mass, where γ is the relativistic Lorentz factor. -
The HARPS Search for Earth-Like Planets in the Habitable Zone I
A&A 534, A58 (2011) Astronomy DOI: 10.1051/0004-6361/201117055 & c ESO 2011 Astrophysics The HARPS search for Earth-like planets in the habitable zone I. Very low-mass planets around HD 20794, HD 85512, and HD 192310, F. Pepe1,C.Lovis1, D. Ségransan1,W.Benz2, F. Bouchy3,4, X. Dumusque1, M. Mayor1,D.Queloz1, N. C. Santos5,6,andS.Udry1 1 Observatoire de Genève, Université de Genève, 51 ch. des Maillettes, 1290 Versoix, Switzerland e-mail: [email protected] 2 Physikalisches Institut Universität Bern, Sidlerstrasse 5, 3012 Bern, Switzerland 3 Institut d’Astrophysique de Paris, UMR7095 CNRS, Université Pierre & Marie Curie, 98bis Bd Arago, 75014 Paris, France 4 Observatoire de Haute-Provence/CNRS, 04870 St. Michel l’Observatoire, France 5 Centro de Astrofísica da Universidade do Porto, Rua das Estrelas, 4150-762 Porto, Portugal 6 Departamento de Física e Astronomia, Faculdade de Ciências, Universidade do Porto, Portugal Received 8 April 2011 / Accepted 15 August 2011 ABSTRACT Context. In 2009 we started an intense radial-velocity monitoring of a few nearby, slowly-rotating and quiet solar-type stars within the dedicated HARPS-Upgrade GTO program. Aims. The goal of this campaign is to gather very-precise radial-velocity data with high cadence and continuity to detect tiny signatures of very-low-mass stars that are potentially present in the habitable zone of their parent stars. Methods. Ten stars were selected among the most stable stars of the original HARPS high-precision program that are uniformly spread in hour angle, such that three to four of them are observable at any time of the year. -
Interstellar Spaceflight
SPACEFLIGHT TOMORROW Interstellar Can We Travel to Other Stars? Small self-replicating probes could be launched on interstellar journeys. Creating a galactic Internet may yield even greater benefits by Timothy Ferris iving as we do in technologically triumphant times, we are inclined to NEAREST STARS to the solar system view interstellar spaceflight as a technical challenge, like breaking the are depicted in this view of the Milky Way galaxy as seen from 500 light- Lsound barrier or climbing Mount Everest—something that will no years above the galactic plane. The doubt be difficult but feasible, given the right resources and resourcefulness. green lines between the stars (inset) represent high-bandwidth radio This view has much to recommend it. Unmanned interstellar travel has, in a sense, beams in a hypothetical communi- already been achieved, by the Pioneer 10 and 11 and Voyager 1 and 2 probes, which cations network linking alien civiliza- were accelerated by their close encounters with Jupiter to speeds in excess of the sun’s tions. Such an interstellar network escape velocity and are outward-bound forever. By interstellar standards, these space- would allow intelligent species to craft are slow: Voyager 1, the speediest of the four at 62,000 kilometers per hour share knowledge without incurring (39,000 miles per hour), will wander for several tens of thousands of years before it the tremendous expense of traveling encounters another star. But the Wright brothers’ first airplane wasn’t particularly to other stars. speedy either. A manned interstellar spacecraft that improved on Voyager’s velocity by the same 1,000-fold increment by which Voyager improved on the Kitty Hawk flights could reach nearby stars in a matter of decades, if a way could be found to pay its exorbitant fuel bill. -
Another Unit of Distance (I Like This One Better): Light Year
How far away are the nearest stars? Last time: • Distances to stars can be measured via measurement of parallax (trigonometric parallax, stellar parallax) • Defined two units to be used in describing stellar distances (parsec and light year) Which stars are they? Another unit of distance (I like this A new unit of distance: the parsec one better): light year A parsec is the distance of a star whose parallax is 1 arcsecond. A light year is the distance a light ray travels in one year A star with a parallax of 1/2 arcsecond is at a distance of 2 parsecs. A light year is: • 9.460E+15 meters What is the parsec? • 3.26 light years = 1 parsec • 3.086 E+16 meters • 206,265 astronomical units The distances to the stars are truly So what are the distances to the stars? enormous • If the distance between the Earth and Sun were • First measurements made in 1838 (Friedrich Bessel) shrunk to 1 cm (0.4 inches), Alpha Centauri • Closest star is Alpha would be 2.75 km (1.7 miles) away Centauri, p=0.75 arcseconds, d=1.33 parsecs= 4.35 light years • Nearest stars are a few to many parsecs, 5 - 20 light years 1 When we look at the night sky, which So, who are our neighbors in space? are the nearest stars? Altair… 5.14 parsecs = 16.8 light years Look at Appendix 12 of the book (stars nearer than 4 parsecs or 13 light years) The nearest stars • 34 stars within 13 light years of the Sun • The 34 stars are contained in 25 star systems • Those visible to the naked eye are Alpha Centauri (A & B), Sirius, Epsilon Eridani, Epsilon Indi, Tau Ceti, and Procyon • We won’t see any of them tonight! Stars we can see with our eyes that are relatively close to the Sun A history of progress in measuring stellar distances • Arcturus … 36 light years • Parallaxes for even close stars • Vega … 26 light years are tiny and hard to measure • From Abell “Exploration of the • Altair … 17 light years Universe”, 1966: “For only about • Beta Canum Venaticorum .