Love Has No Language ~2008~ Promo[EXCLUSIVE]
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The Other End Of Line (2008) Exclusive Theatrical Promo
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Rab Ne Bana Di Jodi (2008) - Haule Haule Exclusive Proper DVD Promo
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Cheenti Cheenti Bang Bang (2008) Bollyood OST
Director : Shantanu Pal
Producer : Sushil Bahety, Rajiv Bahety, R.D. Mallik, N.D. Nagpal & Anivan Ghose
Cast : Aashish Vidyarti, Anjan Srivastava, Asrani & Mahesh Manjrekar
Music Director :Jeet, Ibrahim Ashq, Javed AkhtarSalim Sulaiman, Vishal & Shekhar
Lyricists : Nida Fazli, Joy, Raag Megh, Irfan Siddiquie, Vishal, Shekhar & Pravin Mani
Cassettes and CD’s on : Sa Re Ga Ma Music Records
Singers : Shaan, Joy, Sudesh Bhosle, Ustad Rashid Khan, Kunal Ganjawala, Udit Narayan & Alka Yagnik
Audio Release Date : September 2008
Tracklist
01 - Shaan - Cham Cham
02 - Joy - Chirongo Pitti
03 - Sudesh Bhosle - Baje Bigul
04 - Ustad Rashid Khan - Ghanana Ghanana
05 - Shaan & Shreya - Jhil Mil (Hindi)
06 - Kunal Ganjawala - Lets Be One (Hindi)
07 - Kunal Ganjawala - Chain Kulli Ki Main Kulli
08 - Abhishek Bachchan & Sunidhi Chauhan - Right Here Right Now (Hip Hop Mix)
09 - Udit Narayan & Alka Yagnik - Idhar Chala Main Udhar Chala
10 - Srinivas & Sujatha - Hey Hey Tum Ho
Download Free Cheenti Cheenti Bang Bang (2008) Indian Bollywood OST Mp3 Songs Music Album
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01. Cheenti Cheenti Bang Bang - Cham Cham [GLOOMX.com].mp3
02. Cheenti Cheenti Bang Bang - Chirongo Pitti [GLOOMX.com].mp3
03. Cheenti Cheenti Bang Bang - Baje Bigul [GLOOMX.com].mp3
04. Cheenti Cheenti Bang Bang - Ghanana Ghanana [GLOOMX.com].mp3
05. Cheenti Cheenti Bang Bang - Jhil Mil (Hindi) [GLOOMX.com].mp3
06. Cheenti Cheenti Bang Bang - Lets Be One (Hindi) [GLOOMX.com].mp3
07. Cheenti Cheenti Bang Bang - Chain Kulli Ki Main Kulli [GLOOMX.com].mp3
08. Cheenti Cheenti Bang Bang - Right Here Right Now (Hip Hop Mix) [GLOOMX.com].mp3
09. Cheenti Cheenti Bang Bang - Idhar Chala Main Udhar Chala [GLOOMX.com].mp3
10. Cheenti Cheenti Bang Bang - Hey Hey Tum Ho [GLOOMX.com].mp3
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[b]Rapidshare Links:~[/b]
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Movie Name : Drona
Year of Release : 2008
Release Date : 2 October 2008
Genre : Action, Drama, Thriller, Fantasy
Banner : Rose Movies
Producer : Sunil Lulla, Shrishti Arya
Executive Producer : Iqbal Kidwai
Director : Goldie Behl
Music Director : Dhruv Ghanekar
Lyricist : Vaibhav Modi
Cinematographer : Sameer Arya
Story Writer : Goldie Behl
Dialogue Writer : Jaydeep Sarkar
Screenplay Writer : Rohini Killough, Jaydeep Sarkar, Goldie Behl
Editor : Shyam Salgaonkar
Production Designer : Tania R. Behl
Action Director : Sham Kaushal, Tom Delmar
Costume Designer : Anaita Shroff Adajania
Sound Designer : Baylon Fonseca
Still Photographer : Amit Asher
Visual Effects : David Bush
Playback Singer : Nandini Srikar, Roop Kumar Rathod, Sunidhi Chauhan, Sadhana Sargam, Shaan, Suzanne D’Mello, Dean Devlin, Sunaina
Part I:
http://rapidshare.com/files/150689489/Drona.2008.DaDa.www.amaderforum.com.1.rar.001
http://rapidshare.com/files/150689491/Drona.2008.DaDa.www.amaderforum.com.1.rar.002
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Part 2:
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The unprecedented image quality of the High Resolution Imaging Science Experiment (HiRISE) carried by NASA’s Mars Reconnaissance Orbiter is helping scientists make leaps forward in understanding both the ongoing and ancient processes that shaped the surface of Mars.
3D view of a few scallops. The ridges are asymmetrical with a steeper, shorter, scarp-facing-slope and form steps on the scallop floor (HiRISE image PSP_001938_2265 overlaid on a HiRISE DEM). (Credit: NASA/JPL/University of Arizona)
Professor Alfred McEwen, HiRISE’s Principal Investigator, highlighted some of the most recent results at the European Planetary Science Congress in Münster on September 24th.
A study of the nature and distribution of ancient megabreccia, led by McEwen at the University of Arizona, suggests that this bedrock was formed during the late heavy bombardment period. Megabreccia consists of angular, randomly-orientated blocks that formed suddenly in energetic events such as meteorite impacts. It is thought to contain fragments of the oldest and deepest bedrock exposed on the surface of Mars.
“We think that the megabreccia was formed during a period of heightened meteorite activity about 3.9 billion years ago. This is around the time life appears to have begun on Earth, but we have very little record of that era in our terrestrial geology because ancient rocks are heavily metamorphosed. Mars preserves a much better record of the heavy bombardment and, unlike the dry lunar surface, it shows the environmental effects in a water-rich crust,” said McEwen.
The HiRISE team has identified megabreccia in more than 50 locations consistent with the most ancient terrains on Mars. These include the central uplifts of large craters and deep exposures such as the floor of parts of Valles Marineris. Well-exposed rock outcrops are needed to identify megabreccia, in particular from the diversity of colours and textures indicating diverse rock types.
Megabreccia contains rock fragments from the earliest geological period on Mars, the Noachian era, which is more than 3.8 billion years ago.
The megabreccia blocks vary in size from relatively small (1-5 metres) to larger than 10 metres in diameter. The blocks are cemented in a matrix of finer material. The small blocks were probably formed by post Noachian cratering, particularly when found in material filling crater floors. The large blocks are only found in locations consistent with hard, deep bedrock, such as the central uplifts. McEwen suggests that the blocks are largely cemented by melt from impacts and hydrothermal alteration.
“We are in the midst of a paradigm shift in understanding the Noachian crust of Mars, thanks to the high-resolution data from the Mars Express and MRO missions. The spectrometers on these missions found evidence of alteration due to water in the bedrock in many, if not most Noachian aged places. However, the younger Noachian era may have been relatively dry, so we may need to study the oldest outcrops of megabreccia to understand this era.”
McEwen will also be presenting results of processes that may be shaping the surface of Mars today. A study led by Dr Alexandra Lefort, a researcher in the team of Professor Nicolas Thomas of the University of Bern, has shown that scallop-shaped features found in mid-latitudes on Mars are likely to be formed by the sublimation of shallow ice.
HiRISE imagery shows the scallops have steep polar-facing scaps and gentle equatorial-facing rises. Groups of scallops appear to be separated by areas of knobbly ground. Lefort and colleagues studied scallops in the western part of a region called Utopia Planitia, between 40-55 degrees north.
Lefort said, “We have developed a model where a small hummock on the landscape becomes warmer on the equatorial-facing side. As the fraction of ice in the subsurface sublimates, the ground slumps leaving an asymmetric scallop-shaped hollow. The equatorial-facing slope continues to erode, lengthening out the shape. Near the polar-facing scarp, the depression is deepest and coldest and the underlying ice is most stable. Higher ice concentrations near the scarp leads to the development of a fine network of polygonal-shaped cracks across the floor and this may make the scarp more fragile and prone to landslides. Eventually, neighbouring scallops can coalesce”
Large parts of the mid and high-latitudes of Mars are covered by an erosion-resistant mantle deposit perhaps metres thick in places. This layer consists of ice and dust, with concentrations equivalent to around 4 percent water at 40 degree latitudes, ranging to 20 percent water at 60 degree latitudes. It is unclear as yet whether the scallops form in the ice-rich mantle or in ground that is rich in ice due to some other process
Unlike Earth, Mars has a significant variation in the angle at which its rotational axis is tilted relative to the plane of its orbital axis, known as its obliquity. Over periods of tens of millions of years, this angle can vary from nearly vertical to almost 60 degrees. Models have shown that ice is most stable at lower latitudes during periods of high obliquity. The axis of Mars is currently tilted at an angle of 25.2 degrees, an intermediate obliquity, which means that it is possible that these scallop-forming erosion processes are continuing today.
Dr Kathryn Fishbaugh presented results suggesting that the presence of thick, erosion resistant layers called marker beds, which are found at regular intervals through the north polar layered deposits, are linked to changes caused by periodic fluctuations in the planet’s orbital orientation.
The marker beds are separated by 20-30 metres and are 5-10 metres thick, without any evidence of finer-scale layering within them. This suggests that they have either been deposited quickly or that a coating layer is shrouding evidence of fine layering. Between the marker beds are thinner layers with a thickness of a metre or less.
Fishbaugh and colleagues have found an intriguing resonance between the ratio of marker beds to fine layers (20,30:1) and the ratio of the orbital inclination to the precessional period of Mars’s axis (23:1).
“From our observations, it looks like marker beds are formed on Mars when its orbit is relatively flat with respect to the equatorial plane and its axis is relatively upright. But this makes it hard to explain why these layers are so tough. It’s easier to explain the resistance to erosion of they were formed during periods of high obliquity. With more observations, we hope to answer this question.”
Scientists detect a mysterious flow of galactic clusters
Galaxy clusters and CMBGalaxy clusters across the sky (white spots, shown here on an all-sky survey of the cosmic microwave background) appear to move, on average, in one direction toward the southern sky (purple patch). NASA, WMAP, Kashlinsky et al.
A newly discovered “dark flow” appears to carry clusters of galaxies toward a point in the southern sky, a new study suggests.
As if dark matter and dark energy weren’t confusing enough, researchers detected what they have dubbed dark flow while surveying 700 galaxy clusters — each containing hundreds to thousands of galaxies — within a radius of approximately 1 billion light-years. On average, the clusters appeared to move in a uniform direction at about 1,000 kilometers per second.
While no one knows the cause of the motion, the scientists suggest that whatever it is may no longer lie within the visible universe. The work appears online in two separate papers, one to appear in the Oct. 20 Astrophysical Journal Letters and the other in an upcoming Astrophysical Journal.
“We expected to find something completely different,” says Alexander Kashlinsky, an astrophysicist at NASA’s
The result flies in the face of one of cosmologists’ most cherished assumptions — backed by a vast wealth of data — that the universe is uniform. That is, its structure and the density of matter in it are about the same in all regions of the sky.
But the findings further complicate the picture of cosmology, comments cosmologist Glenn Starkman of
Harald Ebeling, an astronomer at the
The researchers’ work built upon a survey of the entire sky in the X-ray spectrum taken by the orbiting telescope ROSAT in the early 1990s. Galaxy clusters are usually suffused in a thin but very hot plasma, which emits X-rays. Back then, Ebeling and others used the ROSAT data to identify hundreds of large galaxy clusters by their X-ray halos, and matched that with optical-telescope data to estimate the clusters’ distance from Earth.
In the new study, the researchers estimated the motion of each cluster with respect to the CMB radiation, which is believed to be “the ultimate reference” of movement on a cosmological scale, says Ebeling.
As CMB radiation crosses a galaxy cluster, it gets scattered by electrons in the intergalactic plasma, Ebeling says. The scattering affects the radiation’s frequency. The frequency goes up if the cluster is moving toward Earth, and down if it’s moving away. This is called the kinetic Sunyaev-Zeldovich effect, analogous to the familiar Doppler shift of sound waves. The Doppler shift explains why the pitch of an ambulance’s siren sounds different depending on whether the ambulance is approaching or moving away from the listener.
The researchers looked for the kinetic Sunyaev-Zeldovich effect in CMB data released two years ago by NASA’s Wilkinson Microwave Anisotropy Probe mission. The effect was extremely small — comparable to a temperature change of millionths of a kelvin, Ebeling says.
For a single cluster, a variation this small easily drowns in the much larger experimental errors. Moreover, each cluster tends to move in its own direction, tugged by clusters nearby. But on average, the velocities showed a clear trend. “The velocity is not only high,” Kashlinsky says, “but it also remains the same velocity as far as you can see.”
“People will be inherently skeptical of any such results,” Starkman says, since they call into question the standard, homogeneous model of the universe. “Even those who have doubts about the model don’t have better alternatives.” But, he adds, researchers should still take the results seriously.
Kashlinsky says that random energy fluctuations in the earliest split second of the Big Bang — the epoch of stupendous expansion called inflation — could have created a large imbalance in the distribution of matter. While the denser regions of the universe would now be forever out of sight, the imbalance could have left its mark on the overall structure of spacetime. Like a dining room table tipped so that all the dinner plates slide off in the same direction, the imbalance may have put the local corner of the universe on a slope.
Such a large-scale imbalance is “absolutely possible,” says cosmologist Andrei Linde of
The results are something that people will “scratch their heads over,” says Ethan Vishniac of
Fossil find uncovers new species of meat-eating dinosaur that had birdlike lungs
AVIAN AIRWAYS.The new dinosaur species Aerosteon riocoloradensis had lungs (red) and air sacs (other colors) similar to those of modern birds. Full StoryTodd Marshall, Project Exploration
Unlike mammals, birds have evolved a highly efficient system of breathing in which multiple bellows, or air sacs, in the rib cage push oxygen-rich air through a fixed lung.
The fossils from this new dinosaur — called Aerosteon riocoloradensis, which means air bones from the Río Colorado, the Argentine river near where they were found — show characteristically avian features, including air-filled bones in the rib cage that show the hallmark imprints of air sacs, the team reports online September 30 in PLoS ONE.
Scientists are left to wonder why a birdlike system of breathing would be used both by a 10-meter long predatory dinosaur that weighed as much as an Indian elephant, and by a chicken.
In birds, air goes in one end of a lung and comes out the other, a system called flow-through lungs. This allows more oxygen to be absorbed than the mammalian way of breathing, in which air comes in and goes out the same way, leaving some stale air behind after each breath. Birds’ small, lightweight lungs are also a big benefit for flying.
“The real trick is understanding how the air sac is useful to both birds and dinosaurs,” says study coauthor Jeffrey Wilson of the
Soft tissues, like lungs, disintegrate long before scientists can find them, but can leave imprints, or “stamps,” on hard bones, explains
“Since generally all we have is bones in the fossil record, we hit the jackpot with Aerosteon, which shows the presence of these air sacs,” explains study lead author Paul Sereno of the University of Chicago.
The idea of birds and dinosaurs sharing breathing styles has been around for a while. In 2005, a team led by Patrick O’Connor of
In addition to shedding light on the mysterious beginnings of modern bird features, this newly discovered dinosaur unravels some deeper questions about dinosaur lineages.
“Aerosteon represents a surviving lineage never before found and possibly existing in the Late Cretaceous only on the isolated continent of
Title……………….. …………: Welcome to Sajjanpur
Release year………………… ….: 2008
Language…………….. …………: Hindi
Runtime……………… …………: 2 Hour & 13 Minutes & 18 Sec.
Resolution…………… …………: 640×288
English Subtitles……………. ….: YES
Sample:
Genre……………….. …………: N/A
Color……………….. …………: Color
Source………………. …………: DVD-5
