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mnogo vuce na black u odnosu na prethodne stvari

na svasta covek naleti :)

Ajmo dgb! :)

to je to

milan-fiora gg3+ siti-tham gg3+ volfs-lever gg3+ (u 90+1 lever daje pocasni, cim je volfs krenuo sa centra sudija svira kraj :D) abilbao-sevilja gg3+ atalanta-inter gg3+ 200>10600 A E AE! na main tiketu (najjaca uplata) me zajebala zvezda dvojka, jebo me pas u dupe... ko me jebe kada sam subjektivan, idiot retardirani :)

Ne, pošto je CPU nešto malo jači u igrama (nećeš to ni osetiti) al je grafička dosta slabija, tako da se ne isplati.

stutgart sa 2 - 0 do 2- 4. pa koliko je namestena utakmica :D?

Odlična stvar za elektroniku, samo rokajte

lenght:)

Sta je ovo gde se nalazim

HD talasi za opustanje...

:p bak u epizodi "teško je"

Dawn Sees "Young" Surface on Giant Asteroid Like a Hollywood starlet constantly retouching her makeup, the giant asteroid Vesta is constantly stirring its outermost layer to present a young face. Data from NASA's Dawn mission show that a form of weathering that occurs on the moon and other airless bodies we've visited in the inner solar system does not alter Vesta's outermost layer in the same way. Carbon-rich asteroids have also been splattering dark material on Vesta's surface over a long span of the body's history. The results are described in two papers released today in the journal Nature. "Dawn's data allow us to decipher how Vesta records fundamental processes that have also affected Earth and other solar system bodies," said Carol Raymond, Dawn deputy principal investigator at NASA's Jet Propulsion Laboratory, Pasadena, Calif. "No object in our solar system is an island. Throughout solar system history, materials have exchanged and interacted." Over time, soils on Earth's moon and asteroids such as Itokawa have undergone extensive weathering in the space environment. Scientists see this in the accumulation of tiny metallic particles containing iron, which dulls the fluffy outer layer. Dawn's visible and infrared mapping spectrometer (VIR) and framing camera detected no accumulation of such tiny particles on Vesta, and this particular protoplanet, or almost-planet, remains bright and pristine. Nevertheless, the bright rays of the youngest features on Vesta are seen to degrade rapidly and disappear into background soil. Scientists know frequent, small impacts continually mix the fluffy outer layer of broken debris. Vesta also has unusually steep topography relative to other large bodies in the inner solar system, which leads to landslides that further mix surface material. "Getting up close and familiar with Vesta has reset our thinking about the character of the uppermost soils of airless bodies," said Carle Pieters, one of the lead authors and a Dawn team member based at Brown University, Providence, R.I. "Vesta 'dirt' is very clean, well mixed and highly mobile." Early pictures of Vesta showed a variety of dramatic light and dark splotches on Vesta's surface. These light and dark materials were unexpected and now show the brightness range of Vesta is among the largest observed on rocky bodies in our solar system. Dawn scientists suspected early on that bright material is native to Vesta. One of their first hypotheses for the dark material suggested it might come from the shock of high-speed impacts melting and darkening the underlying rocks or from recent volcanic activity. An analysis of data from VIR and the framing camera has revealed, however, that the distribution of dark material is widespread and occurs both in small spots and in diffuse deposits, without correlation to any particular underlying geology. The likely source of the dark material is now shown to be the carbon-rich material in meteoroids, which are also believed to have deposited hydrated minerals from other asteroids on Vesta. To get the amount of darkening we now see on Vesta, scientists on the Dawn team estimate about 300 dark asteroids with diameters between 0.6 to 6 miles (1 and 10 kilometers) likely hit Vesta during the last 3.5 billion years. This would have been enough to wrap Vesta in a blanket of mixed material about 3 to 7 feet (1 to 2 meters) thick. "This perpetual contamination of Vesta with material native to elsewhere in the solar system is a dramatic example of an apparently common process that changes many solar system objects," said Tom McCord, the other lead author and a Dawn team member based at the Bear Fight Institute, Winthrop, Wash. "Earth likely got the ingredients for life - organics and water - this way." Launched in 2007, Dawn spent more than a year investigating Vesta. It departed in September 2012 and is currently on its way to the dwarf planet Ceres. JPL manages the Dawn mission for NASA's Science Mission Directorate in Washington. Dawn is a project of the directorate's Discovery Program, managed by NASA's Marshall Space Flight Center in Huntsville, Ala. The University of California at Los Angeles (UCLA) is responsible for overall Dawn mission science. Orbital Sciences Corp. in Dulles, Va., designed and built the spacecraft. The German Aerospace Center, the Max Planck Institute for Solar System Research, the Italian Space Agency and the Italian National Astrophysical Institute are international partners on the mission team. The California Institute of Technology in Pasadena manages JPL for NASA. For more information about Dawn, visit: http://www.nasa.gov/dawn and http://dawn.jpl.nasa.gov . Jia-Rui Cook Jet Propulsion Laboratory, Pasadena, Calif. 818-354-0850 jccook@jpl.nasa.gov 2012-342 Izvinjavam se sto je na Engleskom, ne bih da prevodim jer bi bilo previse smesno.. Continuing Work With Scoops at 'Rocknest' The Mars Hand Lens Imager (MAHLI) on the arm of NASA's Mars rover Curiosity took this image of a rock called "Et-Then" during the mission's 82nd sol, or Martian day (Oct. 29, 2012.) Image Credit: NASA/JPL-Caltech/MSSS › Full image and caption › Latest images › Curiosity gallery › Curiosity videos NASA's Mars Rover Curiosity on Sol 82 (Oct. 29, 2012) used its Mars Hand Lens Imager (MAHLI) to photograph the diverse rocks in the "Rocknest" area and prepared for an overnight analysis of a soil sample by the Chemistry and Mineralogy (CheMin) instrument. On the preceding sol, the rover completed its third round of using vibration of scooped Martian soil to scrub the interior surfaces of the sample-processing mechanisms on the rover's arm. Also on Sol 81, the rover's Sample Analysis at Mars (SAM) instrument completed an analysis of a sample of Martian atmosphere. The rover continues regular monitoring of the surrounding environment using the other instruments of its science payload. Sol 82, in Mars local mean solar time at Gale Crater, ended at 1:35 p.m. Oct. 29, PDT (4:35 p.m., EDT). Guy Webster 818-354-6278 Jet Propulsion Laboratory, Pasadena, Calif. guy.webster@jpl.nasa.gov 2012-339

ти из прве филијале су радили свој посао како треба, а друге је твој брат слагао и налази се у девизном прекршају. шта да ти кажем... мислим, надам се да овде ико разуме потребу да се прате токови новца. мени је јасно колико то неком рендом лику изгледа као иживљавање троме администрације, али то је будалаштина. контрола има свој смисао.

drale ne kapira jednu stvar. Ovde pricamo o malim projektima. Recimo sad mohi i recimo ja nesto uradimo i treba da naplatimo 1000 eura. Vec umorni i izakani pripremom i ivodjenjem projekata, treba da se zlopatimo po salterima, bankama, birokratijom i da se osecamo kao mali edni crvi koji mole za siroinju, a posteno su zaradili i sebe skinuli sa grbace ovoj usranoj drzavi. Mislis da nas to nece demoralisati. Ti koji sad radis u ogromnom sistemu i birokratija ti je prirodno okruzenje, to ofc ne mozes da shvatis kao prepreku.

svasta po nesto :D

hvala, bas si strucnjak. jos malo pa mozes i kod olje beckovic.

naravno da postoji duša, masa joj je tačno 21 gram.

Resio si da se zenis, hoces zivot da promenis ili ? :D

800 kinti, poslednji novci

Ne mozes samnom tako da pricas ja sam cetnicki vojvoda !

Pricaju dva cigana...oces da idemo na JAGODINsko!? OFK-ors!!!!