Friday, 22 May 2009

How Indonesian People Get Nobel Prize in The Future

Central for Research and Development for Winning


Nobel Prize in Physics at Indonesia

Nobel Fisika Indonesia
 
 

















































"Untuk penemuan difraksi sinar Xnya dengan kristal."


Nobel Prize® medal - registered trademark of the Nobel Foundation

The Nobel Prize in Physics 1914

"for his discovery of the diffraction of X-rays by crystals"
Max von Laue
Germany
Frankfurt-on-the-Main University
Frankfurt-on-the-Main, Germany
b. 1879
d. 1960
Titles, data and places given above refer to the time of the award.
Photos: Copyright © The Nobel Foundation



Max von Laue

Born Max Theodor Felix von Laue
9 October 1879(1879-10-09)
Pfaffendorf, Kingdom of Prussia, German Empire
Died 24 April 1960(1960-04-24) (aged 80)
West Berlin
Nationality German
Fields Physics
Institutions University of Zürich
University of Frankfurt
University of Berlin
Max Planck Institute
Alma mater University of Strasbourg
University of Göttingen
University of Munich
University of Berlin
Doctoral advisor Max Planck
Doctoral students Fritz London
Leó Szilárd
Max Kohler
Erna Weber
Known for Diffraction of X-rays
Notable awards Nobel Prize for Physics (1914)
Max Theodor Felix von Laue (9 October 1879 – 24 April 1960) was a German physicist who won the Nobel Prize in Physics in 1914 for his discovery of the diffraction of X-rays by crystals. In addition to his scientific endeavors with contributions in optics, crystallography, quantum theory, superconductivity, and the theory of relativity, he had a number of administrative positions which advanced and guided German scientific research and development during four decades. He was instrumental in re-establishing and organizing German science after World War II. He was strongly opposed to National Socialism.

Career

In 1906, Laue became a Privatdozent in Berlin and an assistant to Planck. He also met Albert Einstein for the first time; they became friends and Laue went on to contribute to the acceptance and development of Einstein’s theory of relativity. Laue continued as assistant to Planck until 1909. In Berlin, he worked on the application of entropy to radiation fields and on the thermodynamic significance of the coherence of light waves.[7][9]


From 1909 to 1912, Laue was a Privatdozent at the Institute for Theoretical Physics, under Arnold Sommerfeld, at LMU. During the 1911 Christmas recess and in January 1912, Paul Peter Ewald was finishing the writing of his doctoral thesis under Sommerfeld. It was on a walk through the Englischer Garten in Munich in January, that Ewald told Laue about his thesis topic. The wavelengths of concern to Ewald were in the visible region of the spectrum and hence much larger than the spacing between the resonators in Ewald’s crystal model. Laue seemed distracted and wanted to know what would be the effect if much smaller wavelengths were considered. In June, Sommerfeld reported to the Physikalische Gesellschaft of Göttingen on the successful diffraction of x-rays by Laue, Paul Knipping and Walter Friedrich at LMU, for which Laue would be awarded the Nobel Prize in Physics, in 1914. While at Munich, he wrote the first volume of his book on relativity during the period 1910 to 1911.[8][9][10][11]


In 1912, Laue was called to the University of Zurich as an extraordinarius professor of physics. In 1913, his father was raised to the ranks of hereditary nobility; Laue then became 'Max von Laue'.[9]


From 1914 to 1919, Laue was at the University of Frankfurt as ordinarius professor of theoretical physics. From 1916, he was engaged in vacuum tube development, at the University of Würzburg, for use in military telephony and wireless communications.[6][7][8][9]


In 1919, Laue was called to the University of Berlin as ordinarius professor of theoretical physics, a position he held until 1943, when he was declared emeritus, with his consent and one year before the mandatory retirement age. At the university in 1919, other notables were Walther Nernst, Fritz Haber, and James Franck. Laue, as one of the organizers of the weekly Berlin Physics Colloquium, typically sat in the front row with Nernst and Einstein, who would come over from the Kaiser-Wilhelm-Institut für Physik in Berlin-Dahlem, where he was the director. Among Laue’s notable students at the university were Leó Szilárd, Fritz London, Max Kohler, and Erna Weber. In 1921, he published the second volume of his book on relativity.[6][8][12][13]

As a consultant to the Physikalisch-Technische Reichsanstalt (PTR), Laue met Walther Meissner who was working there on superconductivity. Meissner had discovered that a weak magnetic field decays rapidly to zero in the interior of a superconductor, which is known as the Meissner effect. Laue showed in 1932 that the threshold of the applied magnetic field which destroys superconductivity varies with the shape of the body. Laue published a total of 12 papers and a book on superconductivity. One of the papers was co-authored with Fritz London and his brother Heinz.[7][14][15][16] Meissner published a biography on Laue in 1960.[17]

The Kaiser-Wilhelm Gesellschaft zur Förderung der Wissenschaften (Today: Max-Planck Gesellschaft zur Förderung der Wissenschaften) was founded in 1911. Its purpose was to promote the sciences by founding and maintaining research institutes. One such institute was the Kaiser-Wilhelm Institut für Physik (KWIP) founded in Berlin-Dahlem in 1914, with Einstein as director. Laue was a trustee of the institute from 1917, and in 1922 he was appointed deputy director, whereupon Laue took over the administrative duties from Einstein. Einstein was traveling abroad when Adolf Hitler became Chancellor in January 1933, and Einstein did not return to Germany. Laue then became acting director of the KWIP, a position he held until 1946 or 1948, except for the period 1935 to 1939, when Peter Debye was director. In 1943, to avoid casualties to the personnel, the KWIP moved to Hechingen. It was at Hechingen that Laue wrote his book on the history of physics Geschichte der Physik, which was eventually translated into seven other languages.[7][18][19]


Laue was in opposition to National Socialism in general and their Deutsche Physik in particular – the former persecuted the Jews, in general, and the latter, among other things, put down Einstein’s theory of relativity as Jewish physics. Laue secretly helped scientific colleagues persecuted by National Socialist policies to emigrate from Germany, but he also openly opposed them. An address on 18 September 1933 at the opening of the physics convention in Würzburg, opposition to Johannes Stark, an obituary note on Fritz Haber in 1934, and attendance at a commemoration for Haber are examples which clearly illustrate Laue’s courageous, open opposition:
  • Laue, as chairman of the Deutsche Physikalische Gesellschaft, gave the opening address at the 1933 physics convention. In it, he compared the persecution of Galileo and the oppression of his scientific views on the Solar theory of Copernicus to the then conflict and persecution over the theory of relativity by the proponents of Deutsche Physik, against the work of Einstein, labeled “Jewish physics.”
  • Johannes Stark, who had received the Nobel Prize in Physics in 1919, wished to become the Führer of German physics and was a proponent of Deutsche Physik. Against the unanimous advice of those consulted, Stark was appointed President of the PTR in May 1933. However, Laue successfully blocked Stark’s regular membership in the Prussian Academy of Sciences.
  • Haber received the Nobel Prize in Chemistry in 1918. In spite of this and his many other contributions to Germany, he was forced to emigrate from Germany as a result of the Law for the Restoration of the Professional Civil Service, which removed Jews from their jobs. Laue’s obituary note[20] praising Haber and comparing his forced emigration to the expulsion of Themistocles from Athens was a direct affront to the policies of National Socialism.
  • In connection with Haber, Planck and Laue organized a commemoration event held in Berlin-Dahlem on 29 January 1935, the first anniversary of Haber’s death – attendance at the event by professors in the civil service had been expressly forbidden by the government. While many scientific and technical personnel were represented at the memorial by their wives, Laue and Wolfgang Heubner were the only two professors to attend.[21][22] This was yet another blatant demonstration of Laue’s opposition to National Socialism. The date of the first anniversary of Haber’s death was also one day before the second anniversary of National Socialism seizing power in Germany, thus further increasing the affront given by holding the event.
The speech and the obituary note earned Laue government reprimands. Furthermore, in response to Laue blocking Stark’s regular membership in the Prussian Academy of Sciences, Stark, in December 1933, had Laue sacked from his position as advisor to the PTR, which Laue had held since 1925. Chapters 4 and 5, in Welker’s Nazi Science: Myth, Truth, and the Atomic Bomb, present a more detailed account of the struggle by Laue and Planck against the Nazi takeover of the Prussian Academy of Sciences.[14][23][24][25][26][27]


When Nazi Germany invaded Denmark in World War II, the Hungarian chemist George de Hevesy dissolved the gold Nobel Prizes of von Laue and James Franck in aqua regia to prevent the Nazis from stealing them. He placed the resulting solution on a shelf in his laboratory at the Niels Bohr Institute. After the war, he returned to find the solution undisturbed and precipitated the gold out of the acid. The Nobel Society then re–cast the Nobel Prizes using the original gold.[28]


On 23 April 1945, French troops entered Hechingen, followed the next day by a contingent of Operation Alsos – an operation to investigate the German nuclear energy effort, seize equipment, and prevent German scientists from being captured by the Soviets. The scientific advisor to the Operation was the Dutch-American physicist Samuel Goudsmit, who, adorned with a steel helmet, appeared at Laue’s home. Laue was taken into custody and taken to Huntington, England, and interned at Farm Hall, with other scientists thought to be involved in nuclear research and development.[14]


While incarcerated, Laue was a reminder to the other detainees that one could survive the Nazi reign without having “compromised”; this alienated him from others being detained.[29] During his incarceration, Laue wrote a paper on the absorption of x-rays under the interference conditions, and it was later published in Acta Crystallographica.[14] On 2 October 1945, Laue, Otto Hahn, and Werner Heisenberg, were taken to meet with Henry Hallett Dale, president of the Royal Society, and other members of the Society. There, Laue was invited to attend the 9 November 1945 Royal Society meeting in memory of the German physicist Wilhelm Conrad Röntgen, who discovered X-rays; permission was, however, not forthcoming from the military authorities detaining von Laue.[14]


Laue was returned to Germany early in 1946. He went back to being acting director of the KWIP, which had been moved to Göttingen. It was also in 1946 that the Kaiser-Wilhelm Gesellschaft was renamed the Max-Planck Gesellschaft, and, likewise, the Kaiser-Wilhelm Institut für Physik became the Max-Planck Institut für Physik. Laue also became an adjunct professor at the University of Göttingen. In addition to his administrative and teaching responsibilities, Laue wrote his book on superconductivity, Theorie der Supraleitung, and revised his books on electron diffraction, Materiewellen und ihre Interferenzen, and the first volume of his two-volume book on relativity.[8][14][30]


In July 1946, Laue went back to England, only four months after having been interned there, to attend an international conference on crystallography. This was a distinct honor, as he was the only German invited to attend. He was extended many courtesies by the British officer who escorted him there and back, and a well-known English crystallographer as his host; Laue was even allowed to wander around London on his own free will.[14]


After the war, there was much to be done in re-establishing and organizing German scientific endeavors. Laue participated in some key roles. In 1946, he initiated the founding of the Deutsche Physikalische Gesellschaft in only the British Occupation Zone, as the Allied Control Council would not initially allow organizations across occupation zone boundaries. During the war, the PTR had been dispersed; von Laue, from 1946 to 1948, worked on its re-unification across three zones and its location at new facilities in Braunschweig. Additionally, it took on a new name as the Physikalisch-Technische Bundesanstalt, but administration was not taken over by Germany until after the formation of West Germany on 23 May 1949. Circa 1948, the President of the American Physical Society asked Laue to report on the status of physics in Germany; his report was published in 1949 in the American Journal of Physics.[31] In 1950, Laue participated in the creation of the Verband Deutscher Physikalischer Gesellschaften, formerly affiliated under the Nordwestdeutsche Physikalische Gesellschaft.[8][14][30]


In April 1951, Laue became director of the Max-Planck Institut für physikalische Chemie und Elektrochemie, a position he held until 1959. In 1953, at the request of Laue, the Institute was renamed the Fritz Haber Institut für physikalische Chemie und Elektrochemie der Max-Planck Gesellschaft.[14][32]

Presentation

The following account of von Laue's work is by Professor G. Granqvist, Chairman of the Nobel Committee for Physics of the Royal Swedish Academy of Sciences*
Seldom indeed can a discovery in the field of physics have given rise to such intensive research work as did that of Röntgen in 1896, when he proved the existence of a new form of rays which had hitherto been unknown and which, owing to their remarkable characteristics, have since achieved a position of the greatest importance, not only in the field of pure physics but also in connection with research work throughout the other sciences.

Notwithstanding the considerable number of tests which have been carried out since their discovery and directed toward investigation of the true nature of X-rays, it was not until over a decade had passed that their true nature had finally been elucidated.

Already during the first tests it was established that not even the strongest magnetic fields were able to alter the direction of the rays. It was equally impossible to prove the existence of a refraction on transfer of the rays from one medium to another. If the X-rays were of a corpuscular nature they could not, therefore, be carriers of an electrical charge, as is the case with other known rays of corpuscular nature. If, therefore, we wish to disregard matter which has no electrical charge, it is necessary to assume that the particles, whose motion is characteristic for the X-rays, bear two charges of opposite sign, one of which neutralizes the other. On the other hand, from the fact that there was no evidence of refraction of the X-rays, it was possible to assume that, should they consist of a transverse wave motion - as is the case with light waves - the relevant wavelength would have to be very small, as for very small wavelengths, according to the theory of dispersion of light, the refractive index would approach unity.

After hurriedly discarding an hypothesis which had been expounded initially, according to which X-rays were believed to consist of longitudinal wave motions in ether, opinions as to their actual nature were divided according to the above two alternatives. Nevertheless an objective presentation could only describe them as a type of impulse of an unknown nature.

On the basis of an hypothesis expounded as early as 1896 by Stokes and Wiechert this impulse was believed to consist of a disturbance which occurs in the ether when the cathode-ray particle, i.e. a forward-rushing electron, is impeded on colliding with molecules of matter. This disturbance or impulse was believed to propagate in all directions at the speed of light from the ether surrounding the electron. In each part of the space this disturbance was maintained for a period of identical duration to that in which the electron was impeded. This period of time, multiplied by the speed of light, was described as the impulse width, a quantity which, if the nature of the X-rays were the same as that of the light rays, would coincide with the wavelength.

According to that theory the X-ray impulse, which originates perpendicular to the cathode-ray bundle by which it is excited, is alleged to be completely polarized. The evidence of this type of polarization was first produced by Barkla in 1905, but, contrary to the theory, the polarization was not complete but only partial. While it was possible to explain the causative factors of this aberration the characteristics of the polarization were not adequate to prove the existence of a transverse undulation.

Once Dorn had succeeded, in 1897, in determining the fraction of the energy of the impeded electrons which is converted to X-rays, W. Wien was able to calculate the impulse width which, according to his figures, amounted to approximately 10-10 cm, or only one hundred-thousandth of the shortest known wavelengths of light. The short impulse width thus determined could explain the lack of success with previous diffraction tests which had been carried out on slits with X-rays, for even with the narrowest slit the diffraction phenomenon, which is produced by such small impulse widths or wavelengths, would have to lie just about at the limits of possible observation. And it may, in actual fact, only be said even of the most accurate of these tests conducted by Walter and Pohl that they render diffraction highly probable. From the research carried out by these scientists it would meanwhile seem to follow that the upper limit for the impulse width of X-rays lies at 4 x 10-9.

This was the situation when von Laue placed a research medium of the highest import at the disposal of science by virtue of his epoch-making discovery of the interference of X-rays and, at the same time, proved that X-rays, as is the case with light rays, consist of progressive transversal waves.

Previous research had indicated, as is mentioned in the foregoing, that it was highly probable that, if X-rays are wave motions of the same type as light rays, then their wavelengths would have to be of an order of 10-9 cm. In order to obtain clear interference phenomena of the same type as those which are caused when light rays pass a grating it was necessary for the distance between the grating slits to be of an order of 10-8 cm. But this is approximately the distance between the molecules of a solid body and it was in this manner that von Laue arrived at the idea of employing, as a diffraction grating, a solid body with regularly-arranged molecules, e.g. a crystal. As early as 1850 Bravais had introduced into crystallography the assumption that the atoms composing the various crystals are arranged in regular groups, so-called three-dimensional lattices or space-lattices, whose constants could be calculated with the aid of crystallographic data.

However, the theoretical basis of a space-lattice was unknown and thus it was first necessary for von Laue to develop this theory if else the investigation were to have a value. This he did mainly according to the same approximations as those conventional to the science of optics as applied to normal one-dimensional lattices.

Von Laue left the execution of the experimental work in the hands of W. Friedrich and P. Knipping. The apparatus which they employed consisted of a lead box into which they admitted a thin bundle of X-rays which they directed so as to fall upon a precisely oriented crystal. Sensitized film was positioned both behind and at the sides of the crystal. Already the preparatory tests showed that the intensity maxima which had been anticipated by von Laue became evident in the form of blackened spots on the film positioned behind the crystal.

From the grouping shown by these intensity maxima in accordance with the requirements of the theory, as established, for such photograms of various crystals and from the degree of clarity with which they have been reproduced, it follows that they are an interference phenomenon. Absorption tests have shown that the rays which give rise to the points of interference are actually X-rays, and from this von Laue has deduced with a high degree of certainty that the X-rays which cause intensity maxima on irradiation of a crystal have the character of a wave motion. However, the same is required also for those rays employed for irradiation purposes, for, as he says, were they of a corpuscular nature, coherent oscillations could only arise from those atoms set into motion by the identical corpuscle and these atoms would have to form together one whole agglomerate whose dimensions would tee largest in the direction of radiation. However, contrary to what was indicated in the experiment, this would result in the intensity maxima consisting of irregular concentric circles.

As a result of von Laue's discovery of the diffraction of X-rays in crystals proof was thus established that these light waves are of very small wavelengths. However, this discovery also resulted in the most important discoveries in the field of crystallography. It is now possible to determine the position of atoms in crystals and much important knowledge has been gained in this connection. We can anticipate further discoveries of equal note in the future. It is thus rendered likely that experimental research into the influence of temperature upon diffraction will provide the solution to the question of a zero-point energy, or will at least be of some assistance in arriving at a solution to this problem, as the temperature factor assumes a different value according to whether a zero-point energy exists or not. However, the direct results of this discovery of diffraction are of no less importance: it is now possible to subject the X-ray spectra to direct examination, their line spectra can even be photographed, and science has thus been enriched by a method of research whose full implications can not yet be fully appreciated.

If it is permissible to evaluate a human discovery according to the fruits which it bears then there are not many discoveries ranking on a par with that made by von Laue. If one reflects further on the fact that only a few years have passed since his discovery was first published it may surely be said that, when awarding the Nobel Prize for Physics, the Royal Academy of Sciences will presumably seldom, if ever, be in a position of such close agreement with the letter of the Testament as on this occasion in deciding to award the Nobel Prize for Physics for the year 1914 to Professor Max von Laue, for his discovery of the diffraction of X-rays in crystals.

* The Nobel Prize in Physics 1914 was announced on November 11, 1915.
From Nobel Lectures, Physics 1901-1921, Elsevier Publishing Company, Amsterdam, 1967

Copyright © The Nobel Foundation 1914

Sumber:
1. Wikipedia
2. Nobel Prize Org.

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
Disusun Ulang Oleh: 
Arip Nurahman

Pendidikan Fisika, FPMIPA, Universitas Pendidikan Indonesia
&
Follower Open Course Ware at MIT-Harvard University, USA.
Semoga Bermanfaat dan Terima Kasih

Monday, 18 May 2009

Banjar Ciamis Pangandaran Tasikmalaya Rukyatul Hilal Community

Mari Kita Sama-Sama Bangun dan Kembangkan 

Menentukan Visi dan Misi Komunitas

Menentukan Program Kegiatan


Menentukan Tempat Observasi dan Penelitian


Beberapa Pengertian:


Ru’yatul Hilal Ramadhan 1430 H


Pengertian Hilal: Awal Bulan

Ru’yah : Melihat

Hisab : Menghitung

Ijtimak : konjungsi


Terlihatnya hilal bergantung faktor:

1. Kontras antara kecerlangan hilal dgn langit sekitar.

2. Ketebalan hilal, umur hilal.

3. Mata pengamat.

4. Elongasi memadai. Ijtimak / Konjungsi


Awal Ramadhan 1430 H: Kamis n 20 Agustus 2009 Pukul 17:02:48 WIB


Awal Syawal 1430 H: Sabtu 19 September 2009 Pukul 01:45:36 WIB


Garis Ketinggian hilal 0° Awal Ramadhan 1430 H

Visibilitas Hilal 20 Agustus 2009

Visibilitas Hilal 20 Agustus 2009

Visibilitas Hilal 21 Agustus 2009

Visibilitas Hilal 21 Agustus 2009

Garis Ketinggian hilal 0° Awal Syawal 1430 H

Berdasarkan hisab

    Ketika maghrib 20 Agustus 2009 (29 Shaban 1430 H), hilal berada di bawah ufuk.
    Umur <>
    ketinggian: -10 s/d -20
    Bulan Sya’ban digenapkan 30 hari
    1 Ramadhan 1430 H, bertepatan dengan tanggal 22 Agustus 2009.

Berdasarkan hisab

    Ketika maghrib 19 September 2009 (29 Ramadhan 1430 H), hilal berada di atas ufuk.
    Umur > 10 jam
    Ketinggian: 40 s/d 60
    1 Syawal 1430 H, akan bersesuaian dengan tanggal 20 September 2009.

Berdasarkan hisab

Prediksi Awal Bulan Menurut Berbagai Kriteria

    Rukyat Hilal
    Imkanur Rukyat
    Wujudul Hilal
    Rukyat Global (Matla al Badar)

1. Kriteria Ru’yat Hilal (bil Fi'li)

Wajib menggunakan rukyatul hilal bil fi'li, yaitu dengan merukyat hilal secara langsung pada setiap tanggal 29 penanggalan Hijriyah.

Bila tertutup awan atau menurut Hisab hilal di bawah ufuk, tetap merukyat untuk kemudian mengambil keputusan dengan menggenapkan (istikmal) bulan berjalan menjadi 30 hari.

Hisab juga tetap digunakan, namun hanya sebagai alat bantu dan bukan penentu awal bulan Hijriyah.

Jika bulan terlihat maka awal bulan akan jatuh esok harinya.

Jika tidak maka jumlah hari dalam sebulan digenapkan menjadi 30 hari meski menurut metode hisab umur bulan ditetapkan hanya 29 hari.

2. Imkanur Rukyat

Sering disebut juga dengan ijtimak qoblal ghurub, yaitu terjadinya konjungsi (ijtimak) sebelum tenggelamnya matahari.
Konjungsi (ijtimak) telah terjadi sebelum Matahari tenggelam

Bila Bulan tenggelam setelah Matahari, maka keesokan harinya dinyatakan sebagai awal bulan.

Berpuasalah kalian karena melihat hilal dan berbukalah kalian karena melihatnya. Jika ia tertutup awan, maka sempurnakan bilangan syaban menjadi 30 hari. (HR. Bukhari & Muslim)

Berdasarkan pada hadist yang menyatakan: jika satu penduduk negeri melihat bulan, hendaklah mereka semua berpuasa meski yang lain mungkin belum melihatnya.

Memungkinkan posisi hilal yang masih dibawah ufuk, bersamaan dengan tenggelamnya matahari, atau terbenam setelah matahari.

Dipakai oleh sebagian muslim di Indonesia lewat organisasi-organisasi tertentu yang merujuk kepada terlihatnya hilal di negara lain dalam penentuan awal bulan Hijriyah termasuk penentuan awal Ramadhan, Idul Fitri dan Idul Adha.


3. Kriteria Wujudul Hilal

Tarjih Muhammadiyah 1932 menyatakan As-Saumu wa al-Fithru bir ru'yah wa laa man ilaa bil Hisab (berpuasa dan Idul Fitri itu dengan rukyat dan tidak berhalangan dengan hisab)

Muhammadiyah mulai 1969 tidak lagi melakukan Rukyat dan memilih menggunakan Hisab Wujudul Hilal.

Rukyatul hilal adalah pekerjaan yang sangat sulit dan dikarenakan Islam adalah agama yang tidak berpandangan sempit, maka hisab dapat digunakan sebagai penentu awal bulan Hijriyah.

Bukan sekadar untuk memperkirakan hilal mungkin dilihat atau tidak, akan tetapi dijadikan dasar penetapan awal bulan Hijriyah sekaligus jadi bukti bahwa bulan baru sudah masuk atau belum.

Pasca 2002 Persatuan Islam (Persis) mengikuti langkah Muhammadiyah menggunakan Kriteria Wujudul Hilal



4. Rukyat Global (Matla al Badar)

Kurangnya pemahaman terhadap perkembangan dan modernisasi ilmu falak yang dimiliki oleh para perukyat sering menyebabkan terjadinya kesalahan identifikasi hilal.

Sering terjadi klaim terhadap kenampakan hilal oleh seeorang atau kelompok perukyat pada saat hilal masih berada di bawah limit visibilitas.

Tidak hanya di Indonesia bahkan di negara-negara lain kasus ini sering terjadi.

Sudah bukan berita baru lagi bahwa Saudi kerap kali melakukan istbat terhadap laporan rukyat yang kontroversi.

Kesimpulan

Ijtimak awal Ramadhan 1430 terjadi pada hari Kamis tanggal 20 Agustus 2009, 17:02:48 WIB.

Saat maghrib tanggal 22 Agustus 2008, ketinggian Hilal antara -1° sampai -2°.

Bulan telah wujud, berumur <>

Semua kriteria menyimpulkan 1 Ramadhan 1430 pada hari Sabtu 22 September 2009.

Ijtimak awal Syawal 1430 terjadi pada hari Sabtu 19 September 2009, 01:45:36 WIB .

Saat maghrib 19 September 2009 ketinggian Hilal antara 2° sampai 6°.

Bulan sudah wujud, berumur < 8 jam.

Berdasarkan wujudul hilal: Idul Fitri 1430 H pada hari Ahad, 20 September 2009.


Dilema Ru’yah dan Hisab 1

Beberapa negara/ormas berbeda pendapat:

• Satu ru’yah untuk semua negeri

• Satu Ru’yah untuk satu dan negeri yang berdekatan

• Masing-masing negeri memiliki ru’yah

Kata “kalian” pada hadits ru’yah berlaku umum untuk semua orang Islam. Jika ada yang melihat Hilal, jujur, terpercaya dan terbukti, maka persaksian itu harus diterima.

Umat Islam itu satu, karena itu perlu penyeragaman dalam penentuan Hilal.

Insya Allah, pendapat yang paling kuat / mendekati kebenaran juga pendapat yang paling ideal adalah pendapat yang pertama:

Satu ru’yah untuk semua

Dilema Ru’yah dan Hisab 2

Fakta, kebanyakan negeri memilih pendapat ke-3 (sebagian ada yang memilih pendapat ke-2), sehingga masih sering terjadi perbedaan dalam penentuan Hilal.

Ego masing-masing negara/ormas masih terlihat, padahal seharusnya yang terlihat hanyalah rasa persaudaraan sesama muslim dan melepas perbedaan negara/atribut ormas.

Ketika penentuan awal Dzulhijjah, banyak negara-negara yang mengikuti hasil Ru’yah Arab Saudi. Tetapi ketika penentuan awal Ramadhan dan Syawal, masing-masing kukuh berpendapat dengan hasil ru’yah di negerinya masing-masing. Aneh, kan?

Disinilah hisab sebenarnya bisa berperan dengan baik. Dengan ilmu hisab yang semakin dikuasai oleh astronom muslim, ditambah dengan bantuan teknologi astromoni, mereka memakai hisab untuk keperluan umat Muslim di seluruh dunia.

Dilema Ru’yah dan Hisab 3

Jadwal shalat 5 waktu untuk seluruh dunia, dibuat dengan hisab dan dipakai oleh mayoritas muslim di dunia, termasuk di Indonesia.

Jadwal shalat pada awalnya diketahui dengan cara melihat perubahan posisi matahari (dengan kata lain Ru’yah Syamsu/ Melihat matahari), tetapi dengan adanya ilmu hisab, jadwal sholat bisa dibuat untuk seluruh tempat di dunia.

Kenapa hisab jadwal shalat bisa digunakan di seluruh dunia? Karena perhitungan hasil hisab –Insya Allah– sama (setidaknya hanya selisih beberapa menit) dengan hasil melihat langsung posisi matahari.

Dilema Ru’yah dan Hisab 4

Jadwal shalat 5 waktu yang diterima di seluruh dunia dibuat dengan hisab, anehnya ketika ahli hisab (astronom muslim) membuat hisab untuk Hilal Ramadan, Syawal dan Dzulhijjah, banyak negeri muslim yang menolaknya.

Aneh! Aneh! Aneh!

Dalam keseharian hidup mereka memakai hisab (untuk shalat), tetapi ketika menentukan Hilal menolaknya.

Bisa diketahui dengan jelas kapan waktu gerhana bulan atau gerhana matahari, di tempat mana terjadinya, dan sebagainya. Dengan adanya informasi seperti itu, kaum muslimin jadi mengetahui kapan waktu gerhana, dan juga bisa bersiap-siap untuk melakukan shalat gerhana.

Dilema Ru’yah dan Hisab 5

Sebenarnya hisab dan Ru’yah tidak bertentangan, malah sebaliknya hisab bisa menjadi pendukung Ru’yah.

Dengan hisab, bisa ditentukan apakah Hilal kemungkinan besar akan terlihat atau tidak.

Jika ahli hisab mengatakan Ru’yah dapat terlihat di suatu tempat, maka hanya perlu pembuktian dengan Ru’yah, dan biasanya –Insya Allah– memang benar (karena perhitungan hisabnya sudah bagus dan semakin baik).

Jika ahli hisab dan astronom muslim mengatakan dengan ilmu hisab dan astronominya bahwa Hilal kemungkinan tidak akan terlihat, maka tinggal buktikan saja dengan Ru’yah, simpel kan?

Dilema Ru’yah dan Hisab 6

Dengan ilmu hisab, maka Insya Allah persatuan umat Islam di dunia dalam masalah penanggalan tahun hijriyah dapat tercapai lagi.

Tidak akan ada lagi perbedaan waktu shaum, Idul Fitri dan Idul Adha di seluruh dunia. Alangkah indahnya jika hal tersebut bisa terwujudnya.

Jika non muslim bisa bersatu merayakan natal setiap tanggal 25 Desember, kita sebagai muslim lebih berhak untuk bisa bersatu dalam shaum (Ramadhan), Idul Fitri (Syawal), dan Idul Adha (Dzulhijjah).


Alloh menghendaki kemudahan


"Alloh menghendaki kemudahan bagimu, dan tidak menghendaki kesukaran bagimu."

(QS:2:185)


Memasuki bulan yang mulya ini mari kita saling memohon maaf atas segala kesalahan, kealpaan, dan kekurangan yang telah dilakukan. Saling mendo’akan semoga kita dapat menyatukan hati untuk meningkatkan kedekatan pada Alloh SWT.

Tingkatkan amal ibadah kita, tinggalkan perilaku yang tidak sesuai dengan ajaran Islam, untuk menyongsong kehidupan yang kekal di akhirat. Segala puji dan bumi dengan segala isinya,  yang mempergilirkan siang dan malam, yang menghamparkan Bumi dan meninggikan langit tanpa tiang, yang menghidupkan dan mematikan, yang senantiasa memenuhi segala kebutuhan. Tidak ada kebahagiaan hakiki kecuali dengan melaksanakan ketaatan kepada-Nya. Tidak ada rasa cukup, kecuali dengan mengharap rahmat-Nya. Tidak ada kemuliaan, kecuali dengan tunduk kepada keagungan-Nya. Tidak ada kehidupan, kecuali dengan keridhaan-Nya. Bagi Alloh, yang menciptakan serta memelihara langit


Satu kali orbit Bumi keliling Surya bukan 360 derajat tetapi 345 derajat dilaluinya selama 354 hari 8 jam 48 menit dan 36 detik. Dalam satu bulan Qamariah, Bumi bergerak sejauh 28˚ 45’ atau dalam satu hari sejauh 0derajat 58’ 28’’,4.


Perlu dicatat bahwa Bulan mengorbit keliling Bumi sejauh 331˚ 15’, selama 29 hari 12 jam 44,04 menit. Dia bergerak dalam satu hari sejauh 11˚ 12’. Jadi keliling 360˚ - 331˚ 15’ = 28˚ 45’ kalau dikalikan 12 bulan Qamariah maka satu tahun Islam adalah 354 hari 8 jam 48 menit dan 36 detik atau 345 derajat gerak edar Bumi keliling Surya.


Untuk mengitari Surya 360 derajat keliling, maka Bumi memakai waktu selama 370 hari. Dalam pada itu satu tahun musim pada abad 20 Masehi dijalani Bumi sejauh 355˚ 12’ selama 365 hari 6 jam. Hal ini dapat dibuktikan dengan terlambatnya bintang-bintang di angkasa pada waktu tertentu yang sama setiap tahunnya sejauh 4˚ 48’.


Sumber:

Pendidikan Fisika FPMIPA Universitas Pendidikan Indonesia

Bpk. Taufik Ramlan R. dan Bpk. Judhistira Aria Utama

Observatorium Bosscha, FMIPA–ITB, Lembang – Jawa Barat
Bpk. Dr. B. Dermawan, Dr. N. Sopwan, Dr. M. Raharto


Semoga Bermanfaat dan Terima Kasih

Arip Nurahman,

Pendidikan Fisika, FPMIPA. Universitas Pendidikan Indonesia

dan

Follower Open Course Ware at MIT-Harvard University, Cambridge. USA.

Thursday, 14 May 2009

Nobel Fisika Indonesia

Central for Research and Development for Winning


Nobel Prize in Physics at Indonesia

Nobel Fisika Indonesia


(Belajar Kepada Profesor Onnes)

"for his investigations on the properties of matter at low temperatures which led, inter alia, to the production of liquid helium"


"Untuk pemeriksaannya pada sifat zat pada temperatur rendah yang menunjukkan, inter alia, pada pembuatan helium cair"



H. Kamerlingh Onnes
Born Heike Kamerlingh Onnes
21 September 1853(1853-09-21)
Groningen, Netherlands
Died 21 February 1926(1926-02-21) (aged 72)
Leiden, Netherlands
Nationality Netherlands
Fields Physics
Institutions University of Leiden
Alma mater Heidelberg University
University of Groningen
Doctoral advisor Rudolf Adriaan Mees
Other academic advisors Robert Bunsen
Gustav Kirchhoff
Johannes Bosscha
Doctoral students Jacob Clay
Claude Crommelin
Wander de Haas
Gilles Holst
Johannes Kuenen
Remmelt Sissingh
Ewoud van Everdingen
Jules Verschaffelt
Pieter Zeeman
Known for Onnes-effect, Superconductivity
Notable awards Nobel Prize in Physics (1913)



Heike Kamerlingh Onnes (21 September 1853 – 21 February 1926) was a Dutch physicist and Nobel laureate. He pioneered refrigeration techniques, and he explored how materials behaved when cooled to nearly absolute zero. He was the first to liquify helium. His production of extreme cryogenic temperatures led to his discovery of superconductivity in 1911: for certain materials, electrical resistance abruptly vanishes at very low temperatures.

Photos: Copyright © The Nobel Foundation


Heike Kamerlingh Onnes (lahir di Groningen, Belanda, 21 September 1853 – meninggal di Leiden, Belanda, 21 Februari 1926 pada umur 72 tahun) adalah seorang fisikawan Belanda. Karier ilmiah Onnes dihabiskan menjelajah teknik pendinginan dan fenomena terkait.

Tahun-tahun awal

Ia adalah anak industriwan berada yang darinya ia mewarisi kecenderungan mekanis. Ia mewarisi studi prasarjana dalam fisika dan matematika di Universitas Groningen, rumah asalnya. Sebelum memulai karya sarjananya di kota itu pada 1873, ia menghabiskan 3 semester dengan fisikawan Robert Bunsen dan Gustav Kirchhoff di Heidelberg, Jerman. Dari saat itu ia telah memenangkan beberapa hadiah kompetitif. Pada 1879, ia mendapatkan gelar doktor dalam fisika magna cum laude dengan Prof. R.A. Mees di Groningen. Pada 1878, ia diangkat sebagai asisten Johannes Bosscha, Guru Besar Fisika di Sekolah Politeknik Delft. Pada 1881, ia menerbitkan sebuah karya, Algemene Theorie der Vloeistoffen (Teori Umum Cairan), yang menunjukkan hukum keadaan yang berkenaan dapat diturunkan dari uraian tertimbang, berdasarkan pada sifat dan gerakan molekul.

Jabatan profesor

Kamerlingh Onnes diangkat sebagai guru besar di Universitas Leiden pada 1882. Ia mengetuai Bagian Fisika Eksperimental hingga 1923. Dari awal, tujuannya ialah melanjutkan pengetahuan ilmiah dengan eksperimen yang hati-hati. “Door meten tot weten” [Dari mengukur ke ilmu] ialah mottonya. Ia mendirikan sekolah terkenal buat pembuat alat, yang akan menjamin pasokan perajin terlatih yang cukup ke laboratoriumnya sendiri dan lembaga lain di Belanda selama beberapa dasawarsa. Kamerlingh Onnes menerbitkan sebagian besar karyanya di Verslagen, kemudian Proceedings, dari Akademi Sains dan Ilmiah Kerajaan Belanda (KNAW). Namun, dari awal masa jabatan profesornya di Leiden, ia menerbitkan versi semua karya bahasa Inggrisnya dalam Komunikasi Laboratorium Fisika di Universitas Leiden.


Superkonduktivitas

Kamerlingh Onnes mendirikan laboratorium kelas menengah, yang dilengkapi karya kriogenik yang terkait pada liquifaksi gas. 42 tahun di universitas itu terisi dengan penemuan-penemuan luar biasa. Pencapaian puncaknya ialah liquifaksi helium pada 1908, yang membuka bidang baru fisika temperatur rendah dan memungkinkannya menemukan superkonduktivitas pada 1911. Namun, dari 1880-an hingga 1908 ia dan kelompoknya juga membuat studi meluas perilaku campuran fluida, topik yang terliputi di sini.



The Nobel Prize in Physics 1913

Heike Kamerlingh Onnes

Presentation Speech

Presentation Speech by former Councillor Th. Nordstrom, President of the Royal Swedish Academy of Sciences, on December 10, 1913
Your Majesty, Your Royal Highnesses, Ladies and Gentlemen.

At its meeting on the 11th November the Royal Academy of Sciences decided to award the Nobel Prize for Physics for the year 1913 to Dr. Heike Kamerlingh Onnes, Professor at the University of Leyden "for his investigations on the properties of matter at low temperatures which led, inter alia, to the production of liquid helium".

As early as 100 years ago research into the behaviour of gases at various pressures and temperatures gave a great impetus to physics. Since this time the study of the connection between the pressure, the volume and the temperature of gases has played a very important part in physics, and particularly in thermodynamics - one of the most important disciplines of modern physics.

In the years 1873 and 1880 Van der Waals presented his famous laws governing gases which, owing to their great importance for thermodynamics, were rewarded by the Royal Academy of Sciences in 1910 with the Nobel Prize for Physics.

The thermodynamic laws of Van der Waals were laid down on atheoretical basis under the assumption that certain properties could be attributed to molecules and molecular forces. In the case of gases the properties of which are changed by pressure and temperature, or in one way or another do not agree with Van der Waals' hypothesis, deviations from these laws occur.

A systematic experimental study of these deviations and the changes they undergo due to temperature and the molecular structure of the gas must therefore contribute greatly to our knowledge of the properties of the molecules and of the phenomena associated with them.

It was for this research that Kamerlingh Onnes set up his famous laboratory at the beginning of the 1880's, and in it he designed and improved, with unusual success, the physical apparatus needed for his experiments.

It is impossible to report briefly here on the many important results of this work. They embrace the thermodynamic properties at low temperatures of a series of monatomic and diatomic gases and their mixtures, and have contributed to the development of modern thermodynamics and to an elucidation of those associated phenomena which are so difficult to explain. They have also made very important contributions to our knowledge of the structure of matter and of phenomena related to it.

Whilst important on its own account, this research has gained greater significance because it has led to the attainment of the lowest temperatures so far reached. These lie in the vicinity of so-called absolute zero, the lowest temperature in thermodynamics.

The attainment of low temperatures in general was not possible until we learnt to condense the so-called permanent gases, which, since Faraday's pioneer work in this field in the middle of the 1820's, has been one of the most important tasks of thermodynamics.

After Olszewski, Linde, and Hampson had prepared liquid oxygen and air in a variety of ways, and after Dewar, having overcome great experimental difficulties, had succeeded in condensing hydrogen, all temperatures down to -259°C, i.e. all temperatures down to 14° from absolute zero, could be attained.

At these low temperatures all known gases can easily be condensed, except for helium, which was discovered in the atmosphere in the year 1895.

Thus, by condensing this it would be possible to reach still lower temperatures. After both Olszewski and Dewar, Travers, and Jacquerod had tried in vain to prepare liquid helium, using a variety of met hods it was generally assumed that it was impossible.

The question was solved in 1908, however, by Kamerlingh Onnes, who then prepared liquid helium for the first time.

I should have to cover too much ground if I were to report here on the experimental equipment with which Kamerlingh Onnes was at last successful in liquefying helium, and on the enormous experimental difficulties which had to be overcome. I would only mention here that the liquefaction of helium represented a continuation of the long series of investigations into the properties of gases and liquids at low temperatures which Kamerlingh Onnes has carried out in so praiseworthy a manner. These investigations finally led to the determination of the so-called isotherms of helium and the knowledge gained here was the first step towards the liquefaction of helium. Kamerlingh Onnes has constructed cold baths with liquid helium which permit research to be done into the properties of substances at temperatures which lie between 4,3° and 1,15° from absolute zero.

The attainment of these low temperatures is of the greatest importance to physics research, for at these temperatures both the properties of the substances and also the course followed by physical phenomena, are generally quite different from those at our normal and higher temperatures, and a knowledge of these changes is of fundamental importance in answering many of the questions of modern physics.

Let me mention one of these particularly here.

Various principles borrowed from gas thermodynamics have been transferred to the so-called theory of electrons, which is the guiding principle in physics in explaining all electrical, magnetic, optical, and many heat phenomena.

The laws which have been arrived at in this way also seem to be confirmed by measurements at our normal and higher temperatures. That the situation is at very low temperatures not the same, however, has, amongst other things, been shown by Kamerlingh Onnes' experiments on resistance to electrical conduction at helium temperatures and by the determinations which Nernst and his students have carried out in relation to specific heat at liquid temperatures.

It has become more and more clear that a change in the whole theory of electrons is necessary. Theoretical work in this direction has already been begun by a number of research workers, particularly by Planck and Einstein.

In the meantime new supports had to be created for these investigations. These could only be obtained by a continued experimental study of the properties of substances at low temperatures, particularly at helium temperatures, which are the most suitable for throwing light upon phenomena in the world of electrons. Kamerlingh Onnes' merit lies in the fact that he has created these possibilities and at the same time opened up a field of the greatest consequence and significance to physical science.

Owing to the great importance which Kamerlingh Onnes' work has been seen to have for research in physics, the Royal Academy of Sciences has found ample grounds for bestowing upon him the Nobel Prize for Physics for the year 1913.

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

Copyright © The Nobel Foundation 1913

Sumber:
1. Wikipedia
2. Nobel Prize Org.

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
Disusun Ulang Oleh: 
Arip Nurahman

Pendidikan Fisika, FPMIPA, Universitas Pendidikan Indonesia
&
Follower Open Course Ware at MIT-Harvard University, USA.
Semoga Bermanfaat dan Terima Kasih