Wednesday, 18 February 2009

Outer Space

By:
Arip Nurahman
Department of Physics
Faculty of Sciences and Mathematics, Indonesia University of Education

and

Follower Open Course Ware at Massachusetts Institute of Technology
Cambridge, USA
Department of Physics
http://web.mit.edu/physics/
http://ocw.mit.edu/OcwWeb/Physics/index.htm
&
Aeronautics and Astronautics Engineering
http://web.mit.edu/aeroastro/www/
http://ocw.mit.edu/OcwWeb/Aeronautics-and-Astronautics/index.htm
















From: Wikipedia

Outer space, often simply called space, comprises the relatively empty regions of the universe outside the atmospheres of celestial bodies. Outer space is used to distinguish it from airspace (and terrestrial locations). Contrary to popular understanding, outer space is not completely empty (i.e. a perfect vacuum) but contains a low density of particles, predominantly hydrogen plasma, as well as electromagnetic radiation. Hypothetically, it also contains dark matter and dark energy.

The term "outer space" was first recorded by H. G. Wells in 1901. The shorter term space is actually older, being first used to mean the region beyond Earth's sky in John Milton's Paradise Lost in 1667.

Contents


See also


References

  1. ^ "Etymonline : Outer". Retrieved on 2008-03-24.
  2. ^ "Etymonline: Space". Retrieved on 2008-03-24.
  3. ^ NASA Human Body in a Vacuum
  4. ^ a b c d e Harding, Richard M. (1989), Survival in Space: Medical Problems of Manned Spaceflight, London: Routledge, ISBN 0-415-00253-2 .
  5. ^ Billings, Charles E. (1973). "Barometric Pressure", in edited by James F. Parker and Vita R. West: Bioastronautics Data Book, Second Edition, NASA. NASA SP-3006.
  6. ^ "Human Exposure to Vacuum". Retrieved on 2006-03-25.
  7. ^ Webb P. (1968). "The Space Activity Suit: An Elastic Leotard for Extravehicular Activity". Aerospace Medicine 39: 376–383.
  8. ^ Czarnik, Tamarack R.. "EBULLISM AT 1 MILLION FEET: Surviving Rapid/Explosive Decompression". Retrieved on 2006-03-25.
  9. ^ Linda Shiner. "X-15 Walkaround: A short guide to the fastest airplane ever.". Air & Space Magazine. Retrieved on 2007-01-19.
  10. ^ "Report of the Living With a Star Geospace Mission Definition Team". NASA (September, 2002).
  11. ^ "LWS Geospace Missions". NASA.
  12. ^ Davidson, Keay & Smoot, George. Wrinkles in Time. New York: Avon, 1993: 158-163
  13. ^ Silk, Joseph. Big Bang. New York: Freeman, 1977: 299.
  14. ^ NASA COBE website
  15. ^ FAR 91.211, http://www.airweb.faa.gov/Regulatory_and_Guidance_Library/rgFAR.nsf/0/ba9afbf96dbc56f0852566cf006798f9!OpenDocument&ExpandSection=-3

Tuesday, 17 February 2009

Indonesian Space Sciences & Technology School

Prototyping Avionics

Level:

Undergraduate

Instructors:

Dr. Alvar Saenz-Otero



The F-15E Strike Eagle: An array of avionics and electronics systems gives it the capability to fight at low altitude, day or night, and in all weather. (Image courtesy of Armchair Aviator on Flickr.)

Course Features

Course Description

In the past building prototypes of electronic components for new projects/products was limited to using protoboards and wirewrap. Manufacturing a printed-circuit-board was limited to final production, where mistakes in the implementation meant physically cutting traces on the board and adding wire jumpers - the final products would have these fixes on them! Today that is no longer the case, while you will still cut traces and use jumpers when debugging a board, manufacturing a new final version without the errors is a simple and relatively inexpensive task. For that matter, manufacturing a prototype printed circuit board which you know is likely to have errors but which will get the design substantially closer to the final product than a protoboard setup is not only possible, but desirable. In this class, you'll learn to design, build, and debug printed-circuit-boards.

Avionics are the electronic systems used on aircraft, artificial satellites and spacecraft. Avionic systems include communications, navigation, the display and management of multiple systems and the hundreds of systems that are fitted to aircraft to meet individual roles. These can be as simple as a searchlight for a police helicopter or as complicated as the tactical system for an airborne early warning platform.



References

  • Avionics: Development and Implementation by Cary R. Spitzer (Hardcover - Dec 15, 2006)
  • Principles of Avionics, 4th Edition by Albert Helfrick, Len Buckwalter, and Avionics Communications Inc. (Paperback - Jul 1, 2007)
  • Avionics Training: Systems, Installation, and Troubleshooting by Len Buckwalter (Paperback - Jun 30, 2005)



Added & Edited

By: Arip Nurahman
Department of Physics Education, Faculty of Sciences and Mathematics
Indonesia University of Education

and

Follower Open Course Ware at Massachusetts Institute of Technology
Cambridge, USA
Department of Physics 
http://web.mit.edu/physics/
http://ocw.mit.edu/OcwWeb/Physics/index.htm
&
Aeronautics and Astronautics Engineering
http://web.mit.edu/aeroastro/www/
http://ocw.mit.edu/OcwWeb/Aeronautics-and-Astronautics/index.htm

















Sumber:

1. MIT Open Course Ware
2. Wikipedia

 

Thursday, 12 February 2009

Nobel Fisika Indonesia

Central for Research and Development for Winning

Nobel Prize in Physics at Indonesia

 "Untuk investigasinya dalam kepadatan gas yang terpenting dan untuk penemuan argon olehnya."

John William Strutt, 3rd Baron Rayleigh

The Lord Rayleigh

John William Strutt, 3rd Baron Rayleigh
Born 12 November 1842(1842-11-12)
Langford Grove, Maldon, Essex, England
Died 30 June 1919(1919-06-30) (aged 76)
Terling Place, Witham, Essex, England
Nationality United Kingdom
Fields Physics
Institutions University of Cambridge
Alma mater University of Cambridge
Doctoral advisor Edward John Routh
Doctoral students J. J. Thomson
George Paget Thomson
Jagdish Chandra Bose
Known for Discovery of argon
Rayleigh waves
Rayleigh scattering
Rayleigh criterion
Duplex Theory
Theory of Sound
Rayleigh flow
Notable awards Nobel Prize for Physics (1904)
Copley Medal (1899)
Signature
John William Strutt, 3rd Baron Rayleigh (12 November 1842-30 Juni 1919) adalah fisikawan Inggris yang menurunkan sebuah persamaan untuk menghitung variasi sebaran cahaya dengan panjang gelombang. Ia juga mengembangkan sebuah persamaan yang menggambarkan penyebaran panjang gelombang pada radiasi badan hitam, namun hanya diterapkan pada panjang gelombang yang panjang. Rayleigh mencatat bahwa nitrogen di udara lebih padat daripada yang diperoleh dari mineral. Ia menulis jurnal Nature yang meminta usulan. Sir William Ramsay tertarik, dan penelitiannya memuncak pada 1894 dengan penemuan argon. Rayleigh dianugerahi Penghargaan Nobel dalam Fisika 1904.

Nobel Lecture

Nobel Lecture, December 12, 1904

The Density of Gases in the Air and the Discovery of Argon


From Nobel Lectures, Physics 1901-1921, Elsevier Publishing Company, Amsterdam, 1967
In order to read the text you need Acrobat Reader.

Award Ceremony Speech

Presentation Speech by Professor J.E. Cederblom, President of the Royal Swedish Academy of Sciences, on December 10, 1904
Your Majesty, Your Royal Highnesses, Ladies and Gentlemen.

The Royal Academy of Sciences has decided that the Nobel Prize for Physics for the present year is to be awarded to Lord Rayleigh, Professor at the Royal Institution, London, for his investigations on the density of the most important gases, and for his discovery of argon, one of the results of those investigations.

Among the problems in physico-chemical science that have more especially taken up the attention of scientists, the nature and composition of atmospheric air has always held a prominent position. For centuries this problem has been the object of both keen enquiry and extensive experimental investigation, consequently its history affords a very striking picture of the gradual development of those sciences in their entirety, closely connected as it is with the progress made in the various departments of physics and chemistry.

The retarding influence, which in former times was continuously exercised not only by incorrect opinions that had become firmly established but also by insufficient experimental groundwork, is plainly observable, and this explains the fact that during the seventeenth century the solution of the problem was not, and could not, be arrived at by such scientists as Boyle, Mayow, and Hales; it was only obtained a hundred years later, after the discoveries of Priestley, Black, Cavendish, and above all Lavoisier, in a manner which not only then, but up to quite a recent date, was considered final.

Under such circumstances it is but natural that the discovery of a new component of the air, one that is present to the considerable amount of about one per cent, excited great and justifiable astonishment. How was it possible, people asked, that in the face of all the improvements in both physical and chemical methods of observation of the present day this gas should for so long have remained unobserved? The answer to this question lies not only in the strange indifference to chemical investigations by which the age is characterized, but also in the investigations on the physical properties of atmospheric gases not having then reached that high degree of accuracy which Lord Rayleigh has since succeeded in attaining.

This is specially the case in determining densities. It has been shown that nitrogen, when separated from the air, is invariably heavier than when produced from its chemical compounds. As the difference is no less than one half per cent, there is no doubt as to the existence of this divergence, since the accuracy of the weigher was such that the possible fault could only be 1/50 thereof. Since between these two kinds of nitrogen- on the one hand the atmospheric, on the other that obtained from chemical compounds - there is a definite difference in density, the question arose: What could be the cause of this peculiar state of things? All the circumstances of the investigation which might be supposed to have any influence in this respect having been carefully examined, and their influence being found insufficient to explain the difference observed, there remained, in Lord Rayleigh's opinion, but one possibility, viz. that the atmospheric nitrogen was not a simple element, but was a combination of pure nitrogen and some new, hitherto unknown, heavier gas.

If so, this gas could be isolated in some way or other. The methods, physical or chemical, available for this isolation were already known in principle, and the problem now was to obtain the new gas not only in the purest form possible, but also in a sufficient quantity to allow of a thorough investigation of its essential properties. These both difficult and tedious tests have been carried out conjointly by Lord Rayleigh and Sir William Ramsay, and have resulted not only in completely proving that the new gas occurs in a ready state in the air, but also in establishing a thorough knowledge of its chief physical and chemical characteristics.

The time at my disposal does not permit of my giving a detailed account of these questions, interesting and important as they undoubtedly are, but I venture to call attention to the fact that besides the great importance always adherent to the proving of the existence of a new element, this one is of special interest owing to the purely physical investigations on which it is based, investigations which - embracing not only nitrogen but several other important gases-are characterized by a delicacy and precision that is very rarely met with in the history of physical research.

Considering also that to the discovery of argon we may trace one of the causes of Sir William Ramsay's brilliant discovery of helium and the other so-called "noblegases" which followed shortly after, we may truly aver that Lord Rayleigh's work is of that fundamental character that the award to him of the Nobel Prize in Physics must be greeted with sincere and fully justified satisfaction, more especially since this section of his work is but a single link in a long chain of remarkable investigations with which from various points of view he has enriched Physical Science, and which are of such a nature that they will ensure him a prominent position in its history for all time to come.

From Nobel Lectures, Physics 1901-1921, Elsevier Publishing Company, Amsterdam, 1967

Copyright © The Nobel Foundation 1904
Ucapan Terima Kasih;
1. DEPDIKNAS Republik Indonesia
2. Kementrian Riset dan Teknologi Indonesia
3. Lembaga Ilmu Pengetahuan Indonesia (LIPI)
4. Akademi Ilmu Pengetahuan Indonesia
5. Tim Olimpiade Fisika Indonesia
Sumber:

1. Wikipedia

2. Nobel Prize Org.

Disusun Ulang Oleh;

Arip Nurahman

Pendidikan Fisika, FPMIPA. Universitas Pendidikan Indonesia
&
Follower Open Course Ware at MIT-Harvard University, Cambridge. USA.

Semoga Bermanfaat dan Terima Kasih