Minggu, 31 Mei 2009

Sailing Stone

Sailing stones

Sailing stone in Racetrack Playa

The sailing stones (sliding rocks, moving rocks) are a geological phenomenon where rocks move in long tracks along a smooth valley floor without human or animal intervention. They have been recorded and studied in a number of playas around Racetrack Playa, Death Valley, where the number and length of travel grooves are notable.
.


Racetrack stones only move every two or three years and most tracks develop over three or four years. Stones with rough bottoms leave straight striated tracks while those with smooth bottoms wander. Stones sometimes turn over, exposing another edge to the ground and leaving a different track in the stone's wake.

Sliding rock trails fluctuate in direction and length. Some rocks which start next to each other start out travelling parallel, but one may abruptly change direction to the left, right, or even back the direction it came from. Length also varies because two similarly size and shaped rocks could travel uniform, then one could burst ahead or stop dead in its track.

Speed is an unknown variable. Since these stones are rarely transported and nobody has witnessed the movement, the speed the rocks travel at are not known.

Description
Tracks are sometimes not linear

Most of the so-called gliding stones originate from an 850 foot (260 m) high hillside made of dark dolomite on the south end of the playa, but some are intrusive igneous rock from adjacent slopes (most of those being tan-colored feldspar-rich syenite). Tracks are often tens to hundreds of feet (low to high tens of meters) long, a few to 12 inches (8 to 30 cm) wide, and typically much less than an inch (2.5 cm) deep.

A balance of specific conditions are thought to be needed for stones to move:

* A saturated yet non-flooded surface,
* Thin layer of clay,
* Very strong gusts as initiating force,
* Strong sustained wind to keep stones going.


Research history
Rocks on Racetrack Playa

Geologists Jim McAllister and Allen Agnew mapped the bedrock of the area in 1948 and made note of the tracks. Naturalists from the National Park Service later wrote more detailed descriptions and Life magazine featured a set of photographs from The Racetrack. Speculation about how the stones may move started at this time. Various and sometimes idiosyncratic possible explanations have been put forward over the years that have ranged from the supernatural to the very complex. Most hypotheses favored by interested geologists posit that strong winds when the mud is wet are at least in part responsible. Some stones weigh as much as a human, which some researchers such as geologist George M. Stanley who published a paper on the topic in 1955 feel is too heavy for the area's wind to move. They maintain that ice sheets around the stones either help to catch the wind or move in ice flows.

Bob Sharp and Dwight Carey started a Racetrack stone movement monitoring program in May 1972. Eventually thirty stones with fresh tracks were labeled and stakes were used to mark their locations. Each stone was given a name and changes in the stones' position were recorded over a seven year period. Sharp and Carey also tested the ice flow hypothesis by corralling selected stones. A corral 5.5 feet (1.7 m) in diameter was made around a 3 inch (7.5 cm) wide, 1 pound (0.5 kg) track-making stone with seven rebar segments placed 25 to 30 inches (64 to 76 cm) apart. If a sheet of ice around the stones either increased wind-catching surface area or helped move the stones by dragging them along in ice flows, then the rebar should at least slow down and deflect the movement. Neither appeared to occur; the stone barely missed a rebar as it moved 28 feet (8.5 m) to the northwest out of the corral in the first winter. Two heavier stones were placed in the corral at the same time; one moved five years later in the same direction as the first but its companion did not move during the study period. This indicated that if ice played a part in stone movement, then ice collars around stones must be small.
Panorama of the Milky Way with the tracks of sailing stones below. Note the stone on the right hand side.

Ten of the initial twenty-five stones moved in the first winter with Mary Ann (stone A) covering the longest distance at 212 feet (64.5 m). Two of the next six monitored winters also saw multiple stones move. No stones were confirmed to have moved in the summer and some winters none or only a few stones moved. In the end all but two of the thirty monitored stones moved during the seven year study. At 2.5 inches (6.5 cm) in diameter Nancy (stone H) was the smallest monitored stone. It also moved the longest cumulative distance, 860 feet (262 m), and the greatest single winter movement, 659 feet (201 m). The largest stone to move was 80 pounds (36 kg).

Karen (stone J) is a 29 by 19 by 20 inch (74 by 48 by 51 cm) block of dolomite and weighs an estimated 700 pounds (about 320 kg). Perhaps not surprisingly Karen didn't move during the monitoring period. The stone may have created its 570 straight and old track from momentum gained from its initial fall onto the wet playa. However, Karen disappeared sometime before May 1994, possibly during the unusually wet winter of 1992 to 1993. Removal by artificial means is considered unlikely due to the lack of associated damage to the playa that the needed truck and winch would have done. A possible sighting of Karen was made in 1994 a half mile (800 m) from the playa.

Professor John Reid led six research students from Hampshire College and the University of Massachusetts in a follow-up study in 1995. They found highly congruent trails from stones that moved in the late 1980s and during the winter of 1992-1993. At least some stones were proved beyond a reasonable doubt to have been moved in ice flows that may be up to half a mile (800 m) wide. Physical evidence included swaths of lineated areas that could only have been created by moving thin sheets of ice. So wind alone as well as in conjunction with ice flows are thought to be motive forces.

Physicists studying the phenomenon in 1995 found that winds blowing on playa surfaces can be compressed and intensified. They also found that boundary layers (the region just above ground where winds are slower due to ground drag) on these surfaces can be as low as 2 inches (5 cm). This means that stones just a few inches high feel the full force of ambient winds and their gusts, which can reach 90 mph (145 km/h) in winter storms. Such gusts are thought to be the initiating force while momentum and sustained winds keep the stones moving, possibly as fast as a moderate run (only half the force required to start a stone sailing is needed to keep it in motion).

Wind and ice both are the favored hypothesis for these mysterious sliding rocks. Noted in Don J. Easterbrook's "Surface Processes and Landforms", he mentioned that because of the lack of parallel paths between some rock paths, this could be caused by the breaking up of ice resulting in alternate routes. Even though the ice breaks up into smaller blocks, it is still necessary for the rocks to slide

Kamis, 07 Mei 2009

Teori Relativitas

Teori relativitas Albert Einstein adalah sebutan untuk kumpulan dua teori fisika: relativitas umum dan relativitas khusus. Kedua teori ini diciptakan untuk menjelaskan bahwa gelombang elektromagnetik tidak sesuai dengan teori gerakan Newton.

Gelombang elektromagnetik dibuktikan bergerak pada kecepatan yang konstan, tanpa dipengaruhi gerakan sang pengamat. Inti pemikiran dari kedua teori ini adalah bahwa dua pengamat yang bergerak relatif terhadap masing-masing akan mendapatkan waktu dan interval ruang yang berbeda untuk kejadian yang sama, namun isi hukum fisika akan terlihat sama oleh keduanya.
Relativitas khusus

Tulisan Einstein tahun 1905, "Tentang Elektrodinamika Benda Bergerak", memperkenalkan teori relativitas khusus. Relativitas khusus menunjukkan bahwa jika dua pengamat berada dalam kerangka acuan lembam dan bergerak dengan kecepatan sama relatif terhadap pengamat lain, maka kedua pengamat tersebut tidak dapat melakukan percobaan untuk menentukan apakah mereka bergerak atau diam. Bayangkan ini seperti saat Anda berada di dalam sebuah kapal selam yang bergerak dengan kecepatan tetap. Anda tidak akan dapat mengatakan apakah kapal selam tengah bergerak atau diam. Teori relativitas khusus disandarkan pada postulat bahwa kecepatan cahaya akan sama terhadap semua pengamat yang berada dalam kerangka acuan lembam.

Postulat lain yang mendasari teori relativitas khusus adalah bahwa hukum fisika memiliki bentuk matematis yang sama dalam kerangka acuan lembam manapun. Dalam teori relativitas umum, postulat ini diperluas untuk mencakup tidak hanya kerangka acuan lembam, namun menjadi semua kerangka acuan.

Relativitas umum

Relativitas umum diterbitkan oleh Einstein pada 1916 (disampaikan sebagai satu seri pengajaran di hadapan "Prussian Academy of Science" 25 November 1915). Akan tetapi, matematikawan Jerman David Hilbert menulis dan menyebarluaskan persamaan sejenis sebelum Einstein. Ini tidak menyebabkan tuduhan pemalsuan oleh Einstein, tetapi kemungkinan mereka merupakan para pencipta relativitas umum.

Teori relativitas umum menggantikan hukum gravitasi Newton. Teori ini menggunakan matematika geometri diferensial dan tensor untuk menjelaskan gravitasi. Teori ini memiliki bentuk yang sama bagi seluruh pengamat, baik bagi pengamat yang bergerak dalam kerangka acuan lembam ataupun bagi pengamat yang bergerak dalam kerangka acuan yang dipercepat. Dalam relativitas umum, gravitasi bukan lagi sebuah gaya (seperti dalam Hukum gravitasi Newton) tetapi merupakan konsekuensi dari kelengkungan (curvature) ruang-waktu. Relativitas umum menunjukkan bahwa kelengkungan ruang-waktu ini terjadi akibat kehadiran massa.






Isaac Newton


Sir Isaac Newton, (4 Januari 1643 - 31 Maret 1727; KJ: 25 Desember 1642 – 20 Maret 1727) adalah seorang fisikawan, matematikawan, ahli astronomi dan juga ahli kimia yang berasal dari Inggris. Beliau merupakan pengikut aliran heliosentris dan ilmuwan yang sangat berpengaruh sepanjang sejarah, bahkan dikatakan sebagai bapak ilmu fisika modern.

Dengan berbagai hasil karya ilmiah yang dicapainya, Newton menulis sebuah buku Philosophiae Naturalis Principia Mathematica, dimana pada buku tersebut dideskripsikan mengenai teori gravitasi secara umum, berdasarkan hukum gerak yang ditemukannya, dimana benda akan tertarik ke bawah karena gaya gravitasi. Bekerja sama dengan Gottfried Leibniz, Newton mengembangkan teori kalkulus. Newton merupakan orang pertama yang menjelaskan tentang teori gerak dan berperan penting dalam merumuskan gerakan melingkar dari hukum Kepler, dimana Newton memperluas hukum tersebut dengan beranggapan bahwa suatu orbit gerakan melingkar tidak harus selalu berbentuk lingkaran sempurna (seperti elipse, hiperbola dan parabola). Newton menemukan spektrum warna ketika melakukan percobaan dengan melewati sinar putih pada sebuah prisma, dia juga percaya bahwa sinar merupakan kumpulan dari partikel-partikel. Newton juga mengembangkan hukum tentang pendinginan yang di dapatkan dari teori binomial, dan menemukan sebuah prinsip momentum dan angular momentum.

Pendapat Kepala Akademi Ilmiah Berlin tentang Newton: "Newton ialah seorang jenius besar yang pernah ada dan paling beruntung, yang tak bisa kita temukan lebih dari suatu sistem dunia untuk didirikan." [See Shapley.]



Albert Einstein


Albert Einstein (14 Maret 1879–18 April 1955) adalah seorang ilmuwan fisika teoretis yang dipandang luas sebagai ilmuwan terbesar dalam abad ke-20. Dia mengemukakan teori relativitas dan juga banyak menyumbang bagi pengembangan mekanika kuantum, mekanika statistik, dan kosmologi. Dia dianugerahi Penghargaan Nobel dalam Fisika pada tahun 1921 untuk penjelasannya tentang efek fotoelektrik dan "pengabdiannya bagi Fisika Teoretis".

Setelah teori relativitas umum dirumuskan, Einstein menjadi terkenal ke seluruh dunia, pencapaian yang tidak biasa bagi seorang ilmuwan. Di masa tuanya, keterkenalannya melampaui ketenaran semua ilmuwan dalam sejarah, dan dalam budaya populer, kata Einstein dianggap bersinonim dengan kecerdasan atau bahkan jenius. Wajahnya merupakan salah satu yang paling dikenal di seluruh dunia.
Albert Einstein, Tokoh Abad Ini (Person of the Century)

Pada tahun 1999, Einstein dinamakan "Tokoh Abad Ini" oleh majalah Time. Kepopulerannya juga membuat nama "Einstein" digunakan secara luas dalam iklan dan barang dagangan lain, dan akhirnya "Albert Einstein" didaftarkan sebagai merk dagang.

Untuk menghargainya, sebuah satuan dalam fotokimia dinamai einstein, sebuah unsur kimia dinamai einsteinium, dan sebuah asteroid dinamai 2001 Einstein.

Rumus Einstein yang paling terkenal adalah (lihat E=mc²):

E = mc^2 \!



Amazon Deals