Wednesday, 10 August 2011

Nuclear Reactors for Space Applications

"Everything is becoming science fiction. From the margins of an almost invisible literature has sprung the intact reality of the 20th century."

— J. G. Ballard, 1930.






The Martian Surface Reactor: An Advanced Nuclear Power Station for Manned Extraterrestrial Exploration

A. Bushman, D.M. Carpenter, T.S. Ellis, S.P. Gallagher, M.D. Hershcovitch, M.C. Hine, E.D. Johnson, S.C. Kane, M.R. Presley, A.H. Roach, S. Shaikh, M.P. Short, and M.A. Stawicki




Add and Edited By:

Arip Nurahman
Department of Physics, Faculty of Sciences and mathematics

Indonesian University of Education
and
Follower Open Course Ware at MIT-Harvard University. M.A. USA.

Abstract

As part of the 22.033/22.33 Nuclear Systems Design project, this group designed a100 kWe Martian/Lunar surface reactor system to work for 5 EFPY in support of extraterrestrial human exploration efforts. The reactor design was optimized over the following criteria: small mass and size, controllability, launchability/accident safety, and high reliability. The Martian Surface Reactor was comprised of four main systems: the core, power conversion system, radiator and shielding.

The core produces 1.2 MWth and operates in a fast spectrum. Li heat pipes cool the core and couple to the power conversion system. The heat pipes compliment the chosen pin-type fuel geometry arranged in a tri-cusp configuration. The reactor fuel is UN (33.1w/o enriched), the cladding and structural materials in core are Re, and a Hf vessel encases the core. The reflector is Zr3Si2, chosen for its high albedo. Control is achieved by rotating drums, using a TaB2 shutter material. Under a wide range of postulated accident scenarios, this core remains sub-critical and poses minimal environmental hazards.

The power conversion system consists of three parts: a power conversion unit, a transmission system and a heat exchanger. The power conversion unit is a series of cesium thermionic cells, each one wrapped around a core heat pipe. The thermionic emitter is Re at 1800 K, and the collector is molybdenum at 950 K. These units, operating at 10+% efficiency, produce 125 kWe DC and transmit 100 kWe AC. The power transmission system includes 25 separate DC-to-AC converters, transformers to step up the transmission voltage, and 25 km of 22 gauge copper wire for actual electricity transmission. The remaining 900 kWth then gets transmitted to the heat pipes of the radiator via an annular heat pipe heat exchanger that fits over the thermionics. This power conversion system was designed with much redundancy and high safety margins; the highest percent power loss due to a single point failure is 4%.

The radiator is a series of potassium heat pipes with carbon-carbon fins attached. For each core heat pipe there is one radiator heat pipe. The series of heat pipe/fin combinations form a conical shell around the reactor. There is only a 10 degree temperature drop between the heat exchanger and radiator surface, making the radiating temperature 940 K. In the radiator, the maximum cooling loss due to a single point failure is less than 1%.

The shielding system is a bi-layer shadow shield that covers an 80º arc of the core. The inner layer of the shield is a boron carbide neutron shield; the outer layer is a tungsten gamma shield. The tungsten shield is coated with SiC to prevent oxidation in the Martian atmosphere. At a distance of 11 meters from the reactor, on the shielded side, the radiation dose falls to an acceptable 2 mrem/hr; on the unshielded side, an exclusion zone extends to 14 m from the core. The shield is movable to protect crew no matter the initial orientation of the core.

When combined together, the four systems comprise the MSR. The system is roughly conical, 4.8 m in diameter and 3 m tall. The total mass of the reactor is 6.5 MT.

Nuclear Reactors for Space Applications

With the renewed interest in deep space applications, Professor A. Kadak has instituted several studies on nuclear power systems for space applications using the nuclear engineering design course offered for both graduate and undergraduate students. The first such study considered the design of nuclear electric power for propulsion and a terrestrial power station for manned Mars missions. This project was presented to NASA senior project planners in Washington DC in 2003.

Following that meeting and a subsequent meeting with Naval Reactors engineers, feedback was used to redesign the reactor from a highly efficient spent fuel Plutonium core to a highly enriched uranium core by a Master’s thesis student. This year, due to President Bush’s desire to test the new concepts on the Moon, a terrestrial 100 kwe plant was redesigned for use on both Mars and the Moon in the design project in the fall of 2004. As a result of these projects, the nuclear engineering department is gaining valuable experience in nuclear space applications.

Publications

Nuclear Space Applications (NSA) Program

Abstract MIT-NSA-TR-001 V. Dostal, K. Gezelius, J. Horng, J. Koser, J.P. Iv, E. Shwageraus, P. Yarsky, and A.C. Kadak, "Mission to Mars: How to Get People There and Back with Nuclear Energy" (September 2004).
Abstract MIT-NSA-TR-002 P. Yarsky, A.C. Kadak, and M.J. Driscoll, "Design of a Sodium-cooled Epithermal Long-term Exploration Nuclear Engine" (September 2004).
Abstract MIT-NSA-TR-003 A. Bushman, D.M. Carpenter, T.S. Ellis, S.P. Gallagher, M.D. Hershcovitch, M.C. Hine, E.D. Johnson, S.C. Kane, M.R. Presley, A.H. Roach, S. Shaikh, M.P. Short, and M.A. Stawicki, "The Martian Surface Reactor: An Advanced Nuclear Power Station for Manned Extraterrestrial Exploration" (December 2004).



"Aplikasi IPTEK NUKLIR dalam Penjelajahan Angkasa Luar, Akan menjadi Power Utama"
~Arip~

Sources:

1.MIT Nuclear Space Research
2.SPACE POWER REACTORS
3.Nuclear Reactors for Space

Saturday, 6 August 2011

Einstein dan Relativitas Umum yang Legendaris



Dari mekanika klasik menuju relativitas umum Relativitas umum dapat dipahami dengan baik dengan mengevaluasi kemiripannya beserta perbedaannya dari fisika klasik. 

Langkah pertama adalah realisasi bahwa mekanika klasik dan hukum gravitasi Newton mengijinkan adanya deskripsi geometri. 

Kombinasi deskripsi ini dengan hukum-hukum relativitas khusus akan membawa kita kepada penurunan heuristik relativitas umum. 

Generalisasi relativistik

Geometri gravitasi Newton pada dasarnya didasarkan pada mekanika klasik. Ia hanyalah kasus khusus dari mekanika relativitas khusus.

Dalam bahasa simetri: ketika gravitasi dapat diabaikan, fisika yang berlaku bersifat invarian Lorentz pada relativitas khusus daripada invarian Galileo pada mekanika klasik. 

Perbedaan antara keduanya menjadi signifikan apabila kecepatan terlibat di dalamnya mendekati kecepatan cahaya dan berenergi tinggi.

Referensi:

Kunjungi Juga:

Relativitas Umum dan Ke Geniusan Einstein

Sumber:

The University of Cambridge

Wikipedia

The End

Thursday, 4 August 2011

Mekanika Orbit: Bacaan Selanjutnya

Further reading

Many of the options, procedures, and supporting theory are covered in standard works such as:
  • Bate, R.R., Mueller, D.D., White, J.E., (1971). Fundamentals of Astrodynamics. Dover Publications, New York. ISBN 978-0486600611.
  • Vallado, D. A. (2001). Fundamentals of Astrodynamics and Applications, 2nd Edition. Springer. ISBN 978-0792369035.
  • Battin, R.H. (1999). An Introduction to the Mathematics and Methods of Astrodynamics. American Institute of Aeronautics & Ast, Washington, DC. ISBN 978-1563473425.
  • Chobotov, V.A. (ed.) (2002). Orbital Mechanics, 3rd Edition. American Institute of Aeronautics & Ast, Washington, DC. ISBN 978-1563475375.
  • Herrick, S. (1971). Astrodynamics: Orbit Determination, Space Navigation, Celestial Mechanics, Volume 1. Van Nostrand Reinhold, London. ISBN 978-0442033705.
  • Herrick, S. (1972). Astrodynamics: Orbit Correction, Perturbation Theory, Integration, Volume 2. Van Nostrand Reinhold, London. ISBN 978-0442033712.
  • Kaplan, M.H. (1976). Modern Spacecraft Dynamics and Controls. Wiley, New York. ISBN 978-0471457039.
  • Tom Logsdon (1997). Orbital Mechanics. Wiley-Interscience, New York. ISBN 978-0471146360.
  • John E. Prussing and Bruce A. Conway (1993). Orbital Mechanics. Oxford University Press, New York. ISBN 978-0195078343.
  • M.J. Sidi (2000). Spacecraft Dynamics and Control. Cambridge University Press, New York. ISBN 978-0521787802.
  • W.E. Wiesel (1996). Spaceflight Dynamics, 2nd edition. McGraw-Hill, New York. ISBN 978-0070701106.
  • J.P. Vinti (1998). Orbital and Celestial Mechanics. American Institute of Aeronautics & Ast, Reston, VA. ISBN 978-1563472565.
  • P. Gurfil (2006). Modern Astrodynamics. Butterworth-Heinemann. ISBN 978-0123735621.
The most elementary but very widely used reference is Bate, Mueller and White. It has several useful graphs off which one can read the rates of change of perigee and node due to earth oblateness, but there are typographical errors in a few equations. For example, in Eq. (9.7.5) the term in (3/2) J2 needs (re/r) squared and the term in J3 needs it cubed. The coefficient 315 in the J6 term, Eq.(9.7.6.) should be 245 (but the 315 in the J5 term is just fine). Battin's book may be too mathematical for many users.
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