• Title/Summary/Keyword: Saturn V

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The Review of Saturn V 1st Stage (S-IC) Propulsion System (Saturn V 발사체 1단(S-IC) 추진기관 시스템 연구)

  • Hong, Yonggi;Kim, Cheulwoong
    • Journal of the Korean Society of Propulsion Engineers
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    • v.19 no.2
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    • pp.73-80
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    • 2015
  • It had been almost a half century since Apollo Mission was ended. However, in these days, a lot of researches are being conducted for restoration and making improvements in technologies used in Saturn V rocket's development. This study reviews the first stage of Saturn V rocket(S-IC), from development history to technologies in various subsystems such as engine purge system, POGO suppression system, hydraulic and pneumatic control system, propellant dispersion system, telemetry system and retrorocket system. Understandings of S-IC stage's operation systems would be helpful in understanding of launch vehicle system and reduction of time and cost in future development process.

Electromagnetic Electron-Cyclotron Wave for Ring Distribution with Alternating Current (AC) Electric Field in Saturn Magnetosphere

  • Haridas, Annex Edappattu;Kanwar, Shefali;Pandey, Rama Shankar
    • Journal of Astronomy and Space Sciences
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    • v.39 no.2
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    • pp.35-42
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    • 2022
  • During their respective missions, the spacecraft Voyager and Cassini measured several Saturn magnetosphere parameters at different radial distances. As a result of information gathered throughout the journey, Voyager 1 discovered hot and cold electron distribution components, number density, and energy in the 6-18 Rs range. Observations made by Voyager of intensity fluctuations in the 20-30 keV range show electrons are situated in the resonance spectrum's high energy tail. Plasma waves in the magnetosphere can be used to locate Saturn's inner magnetosphere's plasma clusters, which are controlled by Saturn's spin. Electromagnetic electron cyclotron (EMEC) wave ring distribution function has been investigated. Kinetic and linear approaches have been used to study electromagnetic cyclotron (EMEC) wave propagation. EMEC waves' stability can be assessed by analyzing the dispersion relation's effect on the ring distribution function. The primary goal of this study is to determine the impact of the magnetosphere parameters which is observed by Cassini. The magnetosphere of Saturn has also been observed. When the plasma parameters are increased as the distribution index, the growth/damping rate increases until the magnetic field model affects the magnetic field at equator, as can be seen in the graphs. We discuss the outputs of our model in the context of measurements made in situ by the Cassini spacecraft.

Analysis of Thrust Misalignments and Offsets of Lateral Center of Gravity Effects on Guidance Performance of a Space Launch Vehicle (추력비정렬 및 횡방향 무게중심 오프셋에 의한 우주발사체 유도 성능 영향성 분석)

  • Song, Eun-Jung;Cho, Sangbum;Sun, Byung-Chan
    • Journal of the Korean Society for Aeronautical & Space Sciences
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    • v.47 no.8
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    • pp.574-581
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    • 2019
  • This paper investigates the effects of thrust misalignments and offsets of the lateral center of gravity of a space launch vehicle on its guidance performance. Sensitivity analysis and Monte Carlo simulations are applied to analyze their effects by computing changes in orbit injection errors when including the error sources. To compensate their effects, the attitude controller including an integrator additionally and the Steering Misalignment Correction (SMC) routine of the Saturn V are considered, and then Monte Carlo simulations are performed to evaluate their performances.

새로운 에너지물질 분자의 설계기술 동향

  • Lee, Jun-Ung
    • Defense and Technology
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    • no.4 s.290
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    • pp.18-29
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    • 2003
  • 냉전의 또 하나의 부산물은 우주경쟁인데, 인공위성 등 발사체의 추진기관은 거의 예외 없이 액체연료를 사용하는 액체추진로켓이고, 이것의 연료가 되는 액체산소, 액체수소 등은 발사체에 저장된 상태로 보관 할 수 없다는 단점 때문에 거의 군사용으로 적용되고 있지 않다. 지금은 SATURN-V와 같은 거대한 액체 추진 로켓을 대신해서 부분적으로 재활용이 가능한 우주왕복선이 사용되고 있는데, 여기에는 처음 이륙단계 대부분의 추력을 고체추진제에 의존하고 있기 때문에 이들의 성능 향상을 위한 좀 더 강역하고, 안전성을 높일 수 있는 에너지 물질에 대한 요구가 증대되고 있는 실정이다.

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Structural Dynamic Analysis of a Space Launch Vehicle using an Axisymmetric Two-dimensional Shell Element

  • Sim, JiSoo;Lee, SangGu;Kim, JunBeom;Shin, SangJoon;Park, SeungSoo;Ohm, WonSuk
    • International Journal of Aeronautical and Space Sciences
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    • v.18 no.3
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    • pp.485-497
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    • 2017
  • The pogo phenomenon refers to a type of multidiscipline-related instability found in space launch vehicles. It is caused by coupling between the fuselage structure and other structural propulsion components. To predict the pogo phenomenon, it is essential to undertake adequate structural modeling and to understand the characteristics of the feedlines and the propulsion system. To do this, a modal analysis is conducted using axisymmetric two-dimensional shell elements. The analysis is validated using examples of existing launch vehicles. Other applications and further plans for pogo analyses are suggested. In addition, research on the pogo phenomenon of Saturn V and the space shuttle is conducted in order to constitute a pogo stability analysis using the results of the present modal analysis.