Jin Kazama
Xitizen-X,video tourney T5DR(AUG2K7)
Video2 dari tourney T5DR di Xitizen-X yg bulan Agustus kemaren..
diupload kesini... (baru sebagian)
http://www.youtube.com/profile?user=andymrb


Link dari video2 ini bakal dipost di TZ...
Tapi, kalau loe keberatan videonya loe dipost di TZ,(karena nga pede atau apa gitu.)
please kasih tau disini.....


Nanti gw bakal ngepost video2 nya kayak dulu lagi...

Dulu waktu ngepost link2 nya video tourney @ Kentang's.
gw cuma masukin beberapa video ke playlist.
trus playlistnya itu gw post di TZ...

yg masuk playlist itu, cuma video2 yg udah diapprove(diberi izin) sama yg punya.



btw, ini report tourneynya
http://indotekken.com/forum/showthread.php?t=880


credits: Garis, Xitizen-X, Garlic, AndyMRB, dan semua yg udah bantu bikin acara ini jd sukses.

By Lizanias

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STORY WRITTEN FOR & USED WITH PERMISSIONPosted: June 23, 2004NASA unveiled a spectacular high-resolution mosaic of Saturn's enigmatic moon Phoebe today, along with other data from the Saturn-bound Cassini probe showing the moon formed in the extreme outer solar system and later was captured by the ringed planet's gravity. During its historic close encounter with Phoebe, the Cassini spacecraft captured a series of high resolution images of the small moon, six of which have been put together to create this mosaic. Credit: NASA/JPL/Space Science InstituteDownload larger image version "The data that we gathered with the Cassini spacecraft have now given us our first look at this very strange object," said Torrence Johnson, a senior scientist and Cassini team member at the Jet Propulsion Laboratory in Pasadena, Calif. "And what it's told us is that it's a collection of ice and rock and probably carbonaceous compounds."We believe this object has many characteristics in common with things like Pluto and (Neptune's moon) Triton in the outer solar system. In other words, it's a first look at one of these denizens of the outer solar system that we've (seen previously) only from afar."The $3.3 billion Cassini probe, launched in 1997, is scheduled to brake into orbit around Saturn the night of June 30. On June 11, it made a close flyby of Phoebe, giving scientists their first close-up look at the strange moon since Voyager 2 captured a few grainy images in 1981. Voyager 2 imaged Phoebe from a distance of 1.4 million miles. Cassini passed within about 1,285 miles."The Phoebe encounter was a tremendous success scientifically, but also all the instruments worked great, the spacecraft performed beautifully, the nav team put us in exactly the right place and we have wonderful data from all of the experiments," Johnson said. "It's a great warm up for Saturn."Discovered in 1898, Phoebe measures just 137 miles or so across, orbits Saturn at a distance of about nine million miles and circles the planet in the opposite direction from its other moons. Because of that, and the tilt of its orbit, scientists long suspected Phoebe was a captured asteroid or an outer solar system Kuiper belt object left over from the birth of the solar system.The Cassini data indicate the moon almost certainly did, in fact, originate in the Kuiper belt in the extreme outer solar system.Roger Clark, a Cassini researcher with the U.S. Geological Survey said in a new release that "all our evidence leads us to conclude Phoebe's surface is made of water ice, water-bearing minerals, carbon dioxide, possible clays and primitive organic chemicals in patches at different locations on the surface."Cassini also detected as-yet-unknown compounds. But the presence of carbon dioxide provides clear evidence of Phoebe's origin."Phoebe is definitely not an asteroid," said Bonnie Buratti, a member of the Cassini visual and infrared mapping spectrometer team. "It did not form in the asteroid belt because you don't see CO2 in the asteroid belt."It formed some place in the outer solar system beyond the orbit of Jupiter. We believe this is evidence that it came from the Kuiper belt and that it was dragged into the Saturnian system early in the formation of the solar system. So what we see is a very diverse body."With a density of 1.6 grams per cubic centimeter, Phoebe is heavier than pure ice but lighter than most rocks. Johnson said the ratio of water ice to rocky material is similar to that of Pluto and Triton."We believe that four-and-a-half billion years ago, when the solar system was forming, that there were a lot of bodies like Phoebe in the outer solar system," Johnson said. "Since then, most of those bodies have either been accreted in the planets, they have become part of Jupiter, Saturn, Uranus and Neptune, or been gravitationally flung out of the system, out into the outer solar system. Apparently, Phoebe managed to hang around to be captured around Saturn."Cassini project scientist Dennis Matson said Cassini had provided more data about Phoebe in two weeks than scientists on the ground had been able to collect over the past century.Additional coverage for subscribers:VIDEO:WATCH TODAY'S PHOEBE FLYBY SCIENCE RESULTS BRIEFING VIDEO:ANIMATION SHOWS CASSINI'S ENCOUNTER WITH PHOEBE Ferryflight Shuttle PatchFree shipping to U.S. addresses!"The Final Mission" - NASA emblem developed for the Shuttle Carrier Aircraft crew and their support teams to deliver the orbiters to their final destinations at museums.Final Shuttle Mission PatchFree shipping to U.S. addresses!The crew emblem for the final space shuttle mission is now available in our store. Get this piece of history!STS-134 PatchFree shipping to U.S. addresses!The final planned flight of space shuttle Endeavour is symbolized in the official embroidered crew patch for STS-134. Available in our store!Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Project OrionThe Orion crew exploration vehicle is NASA's first new human spacecraft developed since the space shuttle a quarter-century earlier. The capsule is one of the key elements of returning astronauts to the Moon.Fallen Heroes Patch CollectionThe official patches from Apollo 1, the shuttle Challenger and Columbia crews are available in the store.Apollo 12 tribute DVD setNew!Featuring the jovial crew of Pete Conrad, Dick Gordon and Alan Bean, the Apollo 12 mission was struck by lightning shortly after liftoff but proceeded on the second successful exploration voyage to the lunar surface. This three-disc DVD brings the mission to life with extraordinary detail.Choose your store: - - - Fallen Heroes special patchThis special 12-inch embroidered patch commemorates the U.S. astronauts who made the ultimate sacrifice, honoring the crews of Apollo 1, Challenger and Columbia.Choose your store: - - - Women in SpaceWomen of Space: Cool Careers on the Final Frontier is for girls, young women, and anyone else interested in learning about exciting careers in space exploration. Includes CD-ROM.Choose your store: - - - Mars rover posterThis new poster features some of the best pictures from NASA's amazing Mars Exploration Rovers Spirit and Opportunity.Choose your store:Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle's last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Saturn's moon Phoebe revealed in stunning detail CASSINI PHOTO RELEASEPosted: June 13, 2004Extraordinary new images taken by the Cassini spacecraft during its close encounter with Saturn's mysterious moon Phoebe were released by scientists Sunday. The must-see pictures show in great detail the cratered surface of the tiny moon. Credit: NASA/JPL/Space Science InstituteDownload larger image version FIRST IMAGE: Phoebe's true nature is revealed in startling clarity in this mosaic of two images taken during Cassini's flyby on June 11, 2004. The image shows evidence for the emerging view that Phoebe may be an ice-rich body coated with a thin layer of dark material. Small bright craters in the image are probably fairly young features. This phenomenon has been observed on other icy satellites, such as Ganymede at Jupiter. When impactors slammed into the surface of Phoebe, the collisions excavated fresh, bright material -- probably ice -- underlying the surface layer. Further evidence for this can be seen on some crater walls where the darker material appears to have slid downwards, exposing more light-colored material. Some areas of the image that are particularly bright - especially near lower right - are over-exposed. An accurate determination of Phoebe's density - a forthcoming result from the flyby - will help Cassini mission scientists understand how much of the little moon is comprised of ices. This spectacular view was obtained at a phase, or Sun-Phoebe-spacecraft, angle of 84 degrees, and from a distance of approximately 32,500 kilometers (20,200 miles). The image scale is approximately 190 meters (624 feet) per pixel. No enhancement was performed on this image. Credit: NASA/JPL/Space Science InstituteDownload larger image version SECOND IMAGE: Phoebe delivers on its promise to reveal new wonders to Cassini by showing probable evidence of an ice-rich body overlain with a thin layer of dark material. The sharply-defined crater at above center exhibits two or more layers of alternating bright and dark material. Imaging scientists on the Cassini mission have hypothesized that the layering might occur during the crater formation, when ejecta thrown out from the crater buries the pre-existing surface that was itself covered by a relatively thin, dark lag deposit over an icy mantle. The lower thin dark layer on the crater wall appears to define the base of the ejecta blanket. The ejecta blanket itself appears to be mantled by a more recent dark surface lag.This image was obtained on June, 11 2004 at a phase, or Sun-Phoebe-spacecraft, angle of 79 degrees, and from a distance of 13,377 kilometers (8,314 miles). The image scale is approximately 80 meters (263 feet) per pixel. No enhancement was performed on this image. Credit: NASA/JPL/Space Science InstituteDownload larger image version THIRD IMAGE:This eye-popping high-resolution image of Phoebe's pitted surface taken very near closest approach shows a 13-kilometer (8-mile) diameter crater with a debris-covered floor. Part of another crater of similar size is visible at left, as is part of a larger crater at top and many scattered smaller craters. The radial streaks in the crater are due to downslope movements of loose fragments from impact ejecta. Also seen are boulders ranging from about 50 to 300 meters (160 to 990 feet) in diameter. The building-sized rocks may have been excavated by large impacts, perhaps from some other region of Phoebe rather than the craters seen here. There is no visible evidence for layering of ice and regolith or a hardened crust in this region, as on other parts of this moon. Some of the relatively bright spots are from small impacts that excavated bright material from beneath the dark surface. Images like this provide information about impact and regolith processes on Phoebe. This image was obtained at a phase, or Sun-Phoebe-spacecraft, angle of 78 degrees, and from a distance of 11,918 kilometers (7,407 miles). The image scale is approximately 18.5 meters (60.5 feet) per pixel. The illumination is from the right. No enhancement was performed on this image.Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle's last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Saturn's outer rings may be eroding, Cassini data shows UNIVERSITY OF SOUTHERN CALIFORNIA NEWS RELEASEPosted: December 18, 2004A massive eruption of atomic oxygen from Saturn's outer rings, seen by Cassini's ultraviolet camera as the spacecraft neared its destination, may be an indication that the planet's wispy E ring is eroding so fast that it could disappear within 100 million years if not replenished. An artist's concept shows the Cassini space probe at Saturn. Credit: NASA/JPLCassini's Ultraviolet Imaging Spectrograph (UVIS) detected the oxygen atoms spewing into a huge cloud on the dark side of Saturn's rings as Cassini prepared to enter orbit around Saturn in January 2004, said Donald Shemansky, professor of aerospace and mechanical engineering in the USC Viterbi School of Engineering. Data indicated that about 275 million pounds (125 million kilograms) of oxygen was abruptly released in a short period of time. "This was our first surprise in the ultraviolet," said Shemansky, who will analyze ultraviolet data during Cassini's four-year tour of Saturn and its rings with Janet Hallett, a postdoctoral aerospace research associate in the USC Viterbi School. "We aren't sure yet whether this was a transient event or part of a routine recycling process in Saturn's magnetosphere," he said. "Right now scientists are speculating that the oxygen eruption may have been caused by a collision of ice particles from the planet's distant E ring with material in one of the main ring systems, A, B or C. Or it could have been a meteorite collision or an eruption of icy slush on Enceladus, a moon that orbits in the E ring." Shemansky, a co-investigator on the 16-member Cassini ultraviolet imaging team, reported their findings in the Dec. 16 issue of Science Express . Despite Saturn's placid appearance from Earth, the planet is anything but that. The first detailed UV images from the Cassini mission show that Saturn commands a dynamic world of complex, braided ice rings, cannibalistic moons, 1,100 mile-per-hour planetary winds and electrifying auroral displays high in the night skies. Saturn, its moons and highly structured rings live inside a huge cavity in the solar wind created by the planet's strong magnetic field. The magnetosphere is a bubble of particles including electrons, various species of ions, neutral atoms and molecules, several populations of very energetic charged particles like those found in Earth's Van Allen Belts, and charged dust grains. The ionized (electrically charged) gases are called plasmas. However, unlike Jupiter's magnetosphere, Shemansky said Saturn's magnetic cocoon, which is smaller, is filled primarily with neutral gas rather than ions. "Saturn's magnetosphere is turning out to be very different from Jupiter's," he said. "It's dominated by neutral gas and water-rich ingredients produced by its rings, as icy moon debris collides, or by the more energetic collisions of incoming meteorites. It doesn't have nearly as many charged particles, and many of them are absorbed by the rings, so the plasma processes we are observing are entirely different." Two months after his initial observations, Shemansky and his ultraviolet team reported that the large cloud of escaping oxygen atoms had dissipated just as rapidly as it had appeared. Shemansky discounted theories that the rapid loss of material could be explained by "satellite sweeping," a process whereby tiny shepherding moons gobble up debris or deflect it as they clean out gaps between the rings. "The rate at which we saw material escaping from Saturn's outer rings implies that mass equivalent to the entire E ring, even including larger fragments and parent bodies, would be consumed in a period of about 100 million years if no replenishment processes are at work," he said. The rings of gas giants are made up of rocky debris from moons that have been torn apart by tidal waves or by an asteroid or comet collision during heavy bombardment periods. Rings are considered ephemeral and thought to disappear over time spans of billions of years. But Saturn's colorful rings appear to be younger than the planet itself, said scientists ? perhaps only 100 million years old, which is young in cosmological time. They also suspect that Saturn has had several ring systems in its history, although they have never had direct evidence on which to base their assumptions. "These observations are a first in solar system exploration," Shemansky said. "We have direct evidence now that the rings are made up of pure ice and that they are shaped by processes that happen fast," he added. "They aren't the same processes that shaped our solar system 4.5 billion years ago. "Given the fact that the outer rings are present at this time means that the system is being replenished by interactive plasma processes," Shemansky continued. "Clearly, the fact that something is eating up micron-sized grains in the outer ring zones at a high rate tells us that some sort of recycling process must be going on to rebuild them." Cassini's UV imaging spectrograph has made other significant observations. In the ultraviolet, scientists were able to see dust on the rings. Data showed variations in the amount of water-ice contained in the surfaces of ring particles, suggesting that darkened portions had been dusted with powder from pulverized moons or incoming meteoroids. The Cassini UVIS team also obtained ultraviolet images of Phoebe, Saturn's most distant large moon, during the inbound flight to Saturn. Data showed the absorption lines of water-ice on Phoebe's dark surface, which gave scientists more clues about its origins. The only moon in the Saturnian system to orbit in a retrograde, or backward, direction, Phoebe is similar to a common C-type carbonaceous asteroid. Scientists theorize that it was flung out of the Kuiper Belt, a region well beyond Neptune's orbit where thousands of small, icy comets reside, and sucked up by Saturn's strong gravitational field, but no one is absolutely sure of its origin. The Cassini-Huygens spacecraft and science instruments are part of an international mission by NASA, the European Space Agency and the Italian Space Agency to explore Saturn and its many moons and rings. Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle's last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Saturn's rotation is a puzzle NASA/JPL NEWS RELEASEPosted: June 28, 2004On approach to Saturn, data obtained by the Cassini spacecraft are already posing a puzzling question: How long is the day on Saturn? Credit: NASA/JPL/Space Science InstituteDownload larger image version Cassini took readings of the day-length indicator regarded as most reliable -- the rhythm of natural radio signals from the planet. The results give 10 hours, 45 minutes, 45 seconds (plus or minus 36 seconds) as the length of time it takes Saturn to complete each rotation. Here's the puzzle: That is about 6 minutes, or one percent, longer than the radio rotational period measured by the Voyager 1 and Voyager 2 spacecraft, which flew by Saturn in 1980 and 1981.Cassini scientists are not questioning Voyager's careful measurements. And they definitely do not think the whole planet of Saturn is actually rotating that much slower than it did two decades ago. Instead, they are looking for an explanation based on some variability in how the rotation deep inside Saturn drives the radio pulse.The radio sounds of Saturn's rotation, which are also the first sounds from Saturn studied by Cassini, are like a heartbeat and can be heard by visiting "The rotational modulation of radio emissions from distant astronomical objects has long been used to provide very accurate measurements of their rotation period," said Dr. Don Gurnett, principal investigator for the Cassini Radio and Plasma Wave Science instrument, University of Iowa, Iowa City. "The technique is particularly useful for the giant gas planets, such as Jupiter and Saturn, which have no surfaces and are covered by clouds that make direct visual measurements impossible."The first hint of something strange about that type of measurement at Saturn was in 1997, when a researcher from Observatoire de Paris reported that Saturn's radio rotation period differed substantially from Voyager. Dr. Michael D. Desch, Cassini Radio Plasma Wave Science team member, and scientist at NASA's Goddard Space Flight Center in Greenbelt, Md., has analyzed Saturn radio data collected by Cassini from April 29, 2003, to June 10, 2004. "We all agree that the radio rotation period of Saturn is longer today than it was in during the Voyager flyby in 1980," he said.Gurnett said, "Although Saturn's radio rotation period has clearly shifted substantially since the Voyager measurements, I don't think any of us could conceive of any process that would cause the rotation of the entire planet to actually slow down. So it appears that there is some kind of slippage between the deep interior of the planet and the magnetic field, which controls the charged particles responsible for the radio emission." He suggests the solution may be tied to the fact that Saturn's rotational axis is nearly identical to its magnetic axis. Jupiter, with a more substantial difference between its magnetic axis and its rotational axis, shows no comparable irregularities in its radio rotation period."This finding is very significant. It demonstrates that the idea of a rigidly rotating magnetic field is wrong," said Dr. Alex Dessler, a senior research scientist at the University of Arizona, Tucson. In that way, the magnetic fields of gas giant planets may resemble that of the Sun. The Sun's magnetic field does not rotate uniformly. Instead, its rotation period varies with latitude. "Saturn's magnetic field has more in common with the Sun than the Earth. The measurement can be interpreted as showing that the part of Saturn's magnetic field that controls the radio emissions has moved to a higher latitude during the last two decades," said Dressler."I think we will be able to unravel the puzzle, but it's going to take some time," said Gurnett. "With Cassini in orbit around Saturn for four years or more, we will be in an excellent position to monitor long-term variations in the radio period, as well as investigate the rotational period using other techniques."Cassini, carrying 12 scientific instruments, is just two days from its planetary rendezvous with Saturn. On June 30 it will become the first spacecraft to orbit Saturn, when it begins a four-year study of the planet, its rings and its 31 known moons. The spacecraft recently flew past Saturn's cratered moon Phoebe, where it captured spectacular images as well as data on its mass and composition.The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Office of Space Science, Washington, D.C. JPL designed, developed and assembled the Cassini orbiter.?Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle's last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Saturn's swirl imaged CASSINI PHOTO RELEASEPosted: June 15, 2004 Credit: NASA/JPL/Space Science InstituteOn its approach to Saturn orbit insertion, the narrow angle camera on the Cassini spacecraft snapped this image of a turbulent swirl in the high clouds of Saturn's atmosphere. The disturbance occurs in the southern edge of the equatorial band. The image was taken on May 21, 2004, from a distance of 22 million kilometers (13.7 million miles) from Saturn through a filter centered at 889 nanometers. The image scale is 131 kilometers (81 miles) per pixel. Contrast in the image was enhanced to aid visibility. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Office of Space Science, Washington, D.C. The Cassini orbiter and its two onboard cameras, were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle's last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Scientists await descent BY WILLIAM HARWOOD
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