Delta IV Parker Solar Probe Mission Booklet
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Arxiv:2006.00776V1 [Physics.Space-Ph] 1 Jun 2020
manuscript submitted to Geophysical Research Letters Dust impact voltage signatures on Parker Solar Probe: influence of spacecraft floating potential S. D. Bale1,2, K. Goetz3, J. W. Bonnell1, A. W. Case4, C. H. K. Chen5,T. Dudok de Wit6, L. C. Gasque1,2, P. R. Harvey1, J. C. Kasper 7,4, P. J. Kellogg3, R. J. MacDowall8, M. Maksimovic9, D. M. Malaspina10, B. F. Page1,2, M. Pulupa1, M. L. Stevens4, J. R. Szalay11, A. Zaslavsky9 1Space Sciences Laboratory, University of California, Berkeley, CA 94720-7450, USA 2Physics Department, University of California, Berkeley, CA 94720-7300, USA 3School of Physics and Astronomy, University of Minnesota, Minneapolis, 55455, USA 4Smithsonian Astrophysical Observatory, Cambridge, MA 02138 USA 5School of Physics and Astronomy, Queen Mary University of London, London E1 4NS, UK 6LPC2E, CNRS and University of Orleans,´ Orleans,´ France 7Climate and Space Sciences and Engineering, University of Michigan, Ann Arbor, MI 48109, USA 8Solar System Exploration Division, NASA/Goddard Space Flight Center, Greenbelt, MD, 20771 9LESIA, Observatoire de Paris, Universit PSL, CNRS, Sorbonne Universit, Universit de Paris, 5 place Jules Janssen, 92195 Meudon, France 10Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, CO, 80303, USA 11Department of Astrophysical Sciences, Princeton University, Princeton, NJ, 08544, USA Key Points: • The Parker Solar Probe (PSP) FIELDS instrument measures millisecond volt- ages impulses associated with dust impacts • The sign of the largest monopole voltage response is a function of the spacecraft floating potential • These measurements are consistent with models of dynamic charge balance following dust impacts Submitted : June 2, 2020 arXiv:2006.00776v1 [physics.space-ph] 1 Jun 2020 Corresponding author: Stuart D. -
Science: Planetary Science Outyears Are Notional
Science: Planetary Science Outyears are notional ($M) 2019 2020 2021 2022 2023 Planetary Science $2,235 $2,200 $2,181 $2,162 $2,143 Ø Creates a robotic Lunar Discovery and Exploration program, that supports commercial partnerships and innovative approaches to achieving human and science exploration goals. Ø Continues development of Mars 2020 and Europa Clipper. Ø Establishes a Planetary Defense program, including the Double Asteroid Redirection Test (DART) and Near-Earth Object Observations. Ø Studies a potential Mars Sample Return mission incorporating commercial partnerships. Ø Formulates the Lucy and Psyche missions. Ø Selects the next New Frontiers mission. Ø Invests in CubeSats/SmallSats that can achieve entirely new science at lower cost. Ø Operates 10 Planetary missions. § OSIRIS-REx will map asteroid Bennu. § New Horizons will fly by its Kuiper belt target. Dawn Image of Ceres on January 13, 2015 20 Science: Astrophysics Outyears are notional ($M) 2019 2020 2021 2022 2023 Astrophysics $1,185 $1,185 $1,185 $1,185 $1,185 Ø Launches the James Webb Space Telescope. Ø Moves Webb into the Cosmic Origins Program within the Astrophysics Account. Ø Terminates WFIRST due to its significant cost and higher priorities elsewhere within NASA. Increases funding for future competed missions and research. Ø Supports the TESS exoplanet mission following launch by June 2018. Ø Formulates or develops, IXPE, GUSTO, XARM, Euclid, and a new MIDEX mission to be selected in FY 2019. Ø Operates ten missions and the balloon project. Ø Invests in CubeSats/SmallSats that can achieve entirely new science at lower cost. Ø All Astrophysics missions beyond prime operations (including SOFIA) will be subject to senior review in 2019. -
Orion Capsule Launch Abort System Analysis
Orion Capsule Launch Abort System Analysis Assignment 2 AE 4802 Spring 2016 – Digital Design and Manufacturing Georgia Institute of Technology Authors: Tyler Scogin Michel Lacerda Jordan Marshall Table of Contents 1. Introduction ......................................................................................................................................... 4 1.1 Mission Profile ............................................................................................................................. 7 1.2 Literature Review ........................................................................................................................ 8 2. Conceptual Design ............................................................................................................................. 13 2.1 Design Process ........................................................................................................................... 13 2.2 Vehicle Performance Characteristics ......................................................................................... 15 2.3 Vehicle/Sub-Component Sizing ................................................................................................. 15 3. Vehicle 3D Model in CATIA ................................................................................................................ 22 3.1 3D Modeling Roles and Responsibilities: .................................................................................. 22 3.2 Design Parameters and Relations:............................................................................................ -
Materials for Liquid Propulsion Systems
https://ntrs.nasa.gov/search.jsp?R=20160008869 2019-08-29T17:47:59+00:00Z CHAPTER 12 Materials for Liquid Propulsion Systems John A. Halchak Consultant, Los Angeles, California James L. Cannon NASA Marshall Space Flight Center, Huntsville, Alabama Corey Brown Aerojet-Rocketdyne, West Palm Beach, Florida 12.1 Introduction Earth to orbit launch vehicles are propelled by rocket engines and motors, both liquid and solid. This chapter will discuss liquid engines. The heart of a launch vehicle is its engine. The remainder of the vehicle (with the notable exceptions of the payload and guidance system) is an aero structure to support the propellant tanks which provide the fuel and oxidizer to feed the engine or engines. The basic principle behind a rocket engine is straightforward. The engine is a means to convert potential thermochemical energy of one or more propellants into exhaust jet kinetic energy. Fuel and oxidizer are burned in a combustion chamber where they create hot gases under high pressure. These hot gases are allowed to expand through a nozzle. The molecules of hot gas are first constricted by the throat of the nozzle (de-Laval nozzle) which forces them to accelerate; then as the nozzle flares outwards, they expand and further accelerate. It is the mass of the combustion gases times their velocity, reacting against the walls of the combustion chamber and nozzle, which produce thrust according to Newton’s third law: for every action there is an equal and opposite reaction. [1] Solid rocket motors are cheaper to manufacture and offer good values for their cost. -
On Parker Solar Probe, NASA Leaves the Driving to Aerojet Rocketdyne
On Parker Solar Probe, NASA Leaves the Driving to Aerojet Rocketdyne August 12, 2018 KENNEDY SPACE CENTER, Fla., Aug. 12, 2018 (GLOBE NEWSWIRE) -- With a big assist from Aerojet Rocketdyne, NASA’s Parker Solar Probe is now on its way to humankind’s closest encounter ever with a star – in this case our solar system’s sun. Parker Solar Probe NASA image Aerojet Rocketdyne provided the full propulsion system on NASA’s Parker Solar Probe, which will venture eight times closer to the Sun than the previous record holderCredit: NASA/Johns Hopkins APL In addition to the RS-68A main engines for the United Launch Alliance Delta IV Heavy rocket that launched the Parker Probe into space, Aerojet Rocketdyne also supplied the RL10B-2 second stage engine and 12 MR-106 reaction control thrusters on the Delta Cryogenic Second Stage, as well as the full propulsion system on the Parker Solar Probe. The nearly 7-year journey will bring the probe to within 6.2 million kilometers of the Sun’s surface. That’s well within the orbit of the Sun’s nearest planet, Mercury, and eight times closer than the previous record holder, the U.S.-German Helios B probe, which made its closest approach in 1976. “Surviving a years-long journey to the corona of the Sun while operating in autonomous mode requires an incredibly high level of reliability,” said Aerojet Rocketdyne CEO and President Eileen Drake. “Aerojet Rocketdyne propulsion plays a critical role in all aspects of the Parker Solar Probe mission, from launch on the Delta IV, to the probe’s safe cruise through space and approach of the Sun’s atmosphere.” The Parker Solar Probe ultimately will dip into the Sun’s corona, carrying instruments to observe and measure the movement and interaction of phenomena including electric and magnetic fields, energetic particles and solar wind. -
The Active Region Source of a Type III Radio Storm Observed by Parker Solar Probe During Encounter 2 Log-Spaced Chunks, Each of 2.56 Mhz Wide
Astronomy & Astrophysics manuscript no. ISSI_E2_Hinode-final ©ESO 2021 February 10, 2021 The active region source of a type III radio storm observed by Parker Solar Probe during Encounter 2 L. Harra1, 2, D. H. Brooks3, S. D. Bale4, C. H. Mandrini5, 6, K. Barczynski1, 2, R. Sharma7, S. T. Badman4, S. Vargas Domínguez8, and M. Pulupa4 1 PMOD/WRC, Dorfstrasse 33 CH-7260 Davos Dorf, Switzerland e-mail: [email protected] e-mail: [email protected] 2 ETH-Zurich, Hönggerberg campus, HIT building, Zürich, Switzerland 3 College of Science, George Mason University, 4400 University Drive, Fairfax, VA 22030 USA e-mail: [email protected] 4 Physics Department and Space Sciences Laboratory, University of California, Berkeley, USA. 94720-7450 e-mail: [email protected] 5 Instituto de Astronomía y Física del Espacio (IAFE), CONICET-UBA, Buenos Aires, Argentina 6 Facultad de Ciencias Exactas y Naturales (FCEN), UBA, Buenos Aires, Argentina e-mail: [email protected] 7 Fachhochschule Nordwestschweiz (FHNW), Bahnhofstrasse 6, 5210 Windisch, Switzerland e-mail: [email protected] 8 Universidad Nacional de Colombia, Observatorio Astronómico Nacional, Bogotá, Colombia e-mail: [email protected] Received September 2020 ABSTRACT Context. To investigate the source of a type III radio burst storm during encounter 2 of NASA’s Parker Solar Probe (PSP) mission. Aims. It was observed that in encounter 2 of NASA’s Parker Solar Probe mission there was a large amount of radio activity, and in particular a noise storm of frequent, small type III bursts from 31st March to 6th April 2019. Our aim is to investigate the source of these small and frequent bursts. -
Interstellar Probe on Space Launch System (Sls)
INTERSTELLAR PROBE ON SPACE LAUNCH SYSTEM (SLS) David Alan Smith SLS Spacecraft/Payload Integration & Evolution (SPIE) NASA-MSFC December 13, 2019 0497 SLS EVOLVABILITY FOUNDATION FOR A GENERATION OF DEEP SPACE EXPLORATION 322 ft. Up to 313ft. 365 ft. 325 ft. 365 ft. 355 ft. Universal Universal Launch Abort System Stage Adapter 5m Class Stage Adapter Orion 8.4m Fairing 8.4m Fairing Fairing Long (Up to 90’) (up to 63’) Short (Up to 63’) Interim Cryogenic Exploration Exploration Exploration Propulsion Stage Upper Stage Upper Stage Upper Stage Launch Vehicle Interstage Interstage Interstage Stage Adapter Core Stage Core Stage Core Stage Solid Solid Evolved Rocket Rocket Boosters Boosters Boosters RS-25 RS-25 Engines Engines SLS Block 1 SLS Block 1 Cargo SLS Block 1B Crew SLS Block 1B Cargo SLS Block 2 Crew SLS Block 2 Cargo > 26 t (57k lbs) > 26 t (57k lbs) 38–41 t (84k-90k lbs) 41-44 t (90k–97k lbs) > 45 t (99k lbs) > 45 t (99k lbs) Payload to TLI/Moon Launch in the late 2020s and early 2030s 0497 IS THIS ROCKET REAL? 0497 SLS BLOCK 1 CONFIGURATION Launch Abort System (LAS) Utah, Alabama, Florida Orion Stage Adapter, California, Alabama Orion Multi-Purpose Crew Vehicle RL10 Engine Lockheed Martin, 5 Segment Solid Rocket Aerojet Rocketdyne, Louisiana, KSC Florida Booster (2) Interim Cryogenic Northrop Grumman, Propulsion Stage (ICPS) Utah, KSC Boeing/United Launch Alliance, California, Alabama Launch Vehicle Stage Adapter Teledyne Brown Engineering, California, Alabama Core Stage & Avionics Boeing Louisiana, Alabama RS-25 Engine (4) -
IAF SPACE PROPULSION SYMPOSIUM (C4) New Missions Enabled by New Propulsion Technology and Systems (6)
70th International Astronautical Congress 2019 Paper ID: 54982 oral IAF SPACE PROPULSION SYMPOSIUM (C4) New Missions Enabled by New Propulsion Technology and Systems (6) Author: Mr. Steven Vernon Johns Hopkins University Applied Physics Laboratory, United States, [email protected] LAUNCH SYSTEM SOLUTIONS FOR INTERSTELLAR TRAVEL Abstract Building on the experience gained from several successful high launch energy NASA exploration mis- sions, a NASA funded study focused on developing a launch system capable of Interstellar travel in the near term is discussed. The NASA funded Interstellar Probe study managed by Johns Hopkins applied Physics Lab focused on the development a set of launch vehicle and upper stage system solution concepts. The configurations discussed are designed to achieve launch energies significantly above the two previous record setting missions, New Horizons and Parker Solar Probe. The launch system configurations dis- cussed will document of several the very high launch energy solutions explored. With the advent of the NASA Space Launch System (SLS) and its significant lift mass capabilities, coupled to the significant volume available inside the fairing, the SLS system is demonstrated to be particularly well suited to the stacking of one or more upper stages in order to improve and minimize space travel mission durations. The system solutions presented are designed to increase the ultimate launch energies, by a factor of 2-3 times above those achieved for the New Horizons (wet mass = 478 kg, C3 =157.75 km**2/s**2) and Parker Solar Probe (wet mass = 643 kg, C3=154 km**2/s**2) missions. While these two separated Spacecraft launch energy examples were significant engineering achievements, incorporating the Atlas V, 551 and Delta IV Heavy launch systems with unique upper stages, the SLS lift capability configurations presented will be coupled to several Oberth maneuvers and passive and gravity assist trajectories studied. -
The New Heliophysics Division Template
NASA Heliophysics Division Update Heliophysics Advisory Committee October 1, 2019 Dr. Nicola J. Fox Director, Heliophysics Division Science Mission Directorate 1 The Dawn of a New Era for Heliophysics Heliophysics Division (HPD), in collaboration with its partners, is poised like never before to -- Explore uncharted territory from pockets of intense radiation near Earth, right to the Sun itself, and past the planets into interstellar space. Strategically combine research from a fleet of carefully-selected missions at key locations to better understand our entire space environment. Understand the interaction between Earth weather and space weather – protecting people and spacecraft. Coordinate with other agencies to fulfill its role for the Nation enabling advances in space weather knowledge and technologies Engage the public with research breakthroughs and citizen science Develop the next generation of heliophysicists 2 Decadal Survey 3 Alignment with Decadal Survey Recommendations NASA FY20 Presidential Budget Request R0.0 Complete the current program Extended operations of current operating missions as recommended by the 2017 Senior Review, planning for the next Senior Review Mar/Apr 2020; 3 recently launched and now in primary operations (GOLD, Parker, SET); and 2 missions currently in development (ICON, Solar Orbiter) R1.0 Implement DRIVE (Diversify, Realize, Implemented DRIVE initiative wedge in FY15; DRIVE initiative is now Integrate, Venture, Educate) part of the Heliophysics R&A baseline R2.0 Accelerate and expand Heliophysics Decadal recommendation of every 2-3 years; Explorer mission AO Explorer program released in 2016 and again in 2019. Notional mission cadence will continue to follow Decadal recommendation going forward. Increased frequency of Missions of Opportunity (MO), including rideshares on IMAP and Tech Demo MO. -
Development of a 10 Kn LOX/HTPB Hybrid Rocket Engine Through Successive Development and Testing of Scaled Prototypes
DOI: 10.13009/EUCASS2017-334 7TH EUROPEAN CONFERENCE FOR AERONAUTICS AND AEROSPACE SCIENCES (EUCASS) Development of a 10 kN LOX/HTPB Hybrid Rocket Engine through Successive Development and Testing of Scaled Prototypes Maximilian Bambauer and Markus Brandl WARR (TUM) c/o TUM Lehrstuhl für Raumfahrttechnik Boltzmannstraße 15 D-85748 Garching bei München [email protected] [email protected] · Abstract The development of a hybrid flight engine for a sounding rocket requires intensive preparation work and pretests. To obtain better understanding of the difficulties in design and operation that occur with LOX/HTPB rocket engines, four rocket engines with increasing size and thrust level are successively developed and manufactured. Listed chronologically, those engines are the demonstrator engine, the sub- scale engine with a cylindrical grain geometry and later a star shaped geometry, the full-scale test engine and the full-scale flight version. At first a small-scale technology demonstrator was developed. It pro- duced a mean thrust of 160N for 5s and had the purpose to validate the design calculations and to gain first experiences with the use of cryogenic propellants, especially regarding cooldown procedures. Based on this test results the so-called sub-scale engine was developed and tested. The engine can be operated with two grain configurations, using either a cylindrical grain or a star shaped grain. The star shaped grain geometries are realized, using an additive manufactured core, outside of which the HTPB is casted. In the low thrust configuration, the engine is operated using a cylindrical single port HTPB grain and it produces a thrust of about 540 N for a duration of 10 s. -
An Investigation of the Performance Potential of A
AN INVESTIGATION OF THE PERFORMANCE POTENTIAL OF A LIQUID OXYGEN EXPANDER CYCLE ROCKET ENGINE by DYLAN THOMAS STAPP RICHARD D. BRANAM, COMMITTEE CHAIR SEMIH M. OLCMEN AJAY K. AGRAWAL A THESIS Submitted in partial fulfillment of the requirements for the degree of Master of Science in the Department of Aerospace Engineering and Mechanics in the Graduate School of The University of Alabama TUSCALOOSA, ALABAMA 2016 Copyright Dylan Thomas Stapp 2016 ALL RIGHTS RESERVED ABSTRACT This research effort sought to examine the performance potential of a dual-expander cycle liquid oxygen-hydrogen engine with a conventional bell nozzle geometry. The analysis was performed using the NASA Numerical Propulsion System Simulation (NPSS) software to develop a full steady-state model of the engine concept. Validation for the theoretical engine model was completed using the same methodology to build a steady-state model of an RL10A-3- 3A single expander cycle rocket engine with corroborating data from a similar modeling project performed at the NASA Glenn Research Center. Previous research performed at NASA and the Air Force Institute of Technology (AFIT) has identified the potential of dual-expander cycle technology to specifically improve the efficiency and capability of upper-stage liquid rocket engines. Dual-expander cycles also eliminate critical failure modes and design limitations present for single-expander cycle engines. This research seeks to identify potential LOX Expander Cycle (LEC) engine designs that exceed the performance of the current state of the art RL10B-2 engine flown on Centaur upper-stages. Results of this research found that the LEC engine concept achieved a 21.2% increase in engine thrust with a decrease in engine length and diameter of 52.0% and 15.8% respectively compared to the RL10B-2 engine. -
The Delta Launch Vehicle- Past, Present, and Future
The Space Congress® Proceedings 1981 (18th) The Year of the Shuttle Apr 1st, 8:00 AM The Delta Launch Vehicle- Past, Present, and Future J. K. Ganoung Manager Spacecraft Integration, McDonnell Douglas Astronautics Co. H. Eaton Delta Launch Program, McDonnell Douglas Astronautics Co. Follow this and additional works at: https://commons.erau.edu/space-congress-proceedings Scholarly Commons Citation Ganoung, J. K. and Eaton, H., "The Delta Launch Vehicle- Past, Present, and Future" (1981). The Space Congress® Proceedings. 7. https://commons.erau.edu/space-congress-proceedings/proceedings-1981-18th/session-6/7 This Event is brought to you for free and open access by the Conferences at Scholarly Commons. It has been accepted for inclusion in The Space Congress® Proceedings by an authorized administrator of Scholarly Commons. For more information, please contact [email protected]. THE DELTA LAUNCH VEHICLE - PAST, PRESENT AND FUTURE J. K. Ganoung, Manager H. Eaton, Jr., Director Spacecraft Integration Delta Launch Program McDonnell Douglas Astronautics Co. McDonnell Douglas Astronautics Co. INTRODUCTION an "interim space launch vehicle." The THOR was to be modified for use as the first stage, the The Delta launch vehicle is a medium class Vanguard second stage propulsion system, was used expendable booster managed by the NASA Goddard as the Delta second stage and the Vanguard solid Space Flight Center and used by the U.S. rocket motor became Delta's third stage. Government, private industry and foreign coun Following the eighteen month development program tries to launch scientific, meteorological, and failure to launch its first payload into or applications and communications satellites.