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South Africa reflects after ANC centenary To see more go to http://www.youtube.com/user/journeymanpictures Follow us on Facebook (http://goo.gl/YRw42) or Twitter (http://www.twitter.com/journeymanvod) As the world reflects on the ANC s struggle since 1912, South Africa also remembers a leader who is often overlooked by the international community: Robert Sobukwe, founder of the Pan-Africanist Congress. Sobukwe would never see his dream of "South Africa s youth, walking tall, in a country they call their own." He is a man with a remarkable legacy. In particular, his monumental call to action against the pass laws, on 21st March 1960. Heeding the call, thousands of black South Africans left their pass books at home and marched to their police stations, demanding arrest. "You had to give non-violence a chance. That was Sobukwe s mission." Protesters paid the price: police opened fire in the Sharpeville massacre and Sobukwe suffered years of imprisonment. But the protest left an indelible mark on international consciousness and helped clear the path for the ANC to change South African politics. October 2011

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Ultimate Factories: Mack Truck :Find out what it takes to produce Mack s massive Titan engine. ➡ Subscribe: http://bit.ly/NatGeoSubscribe About National Geographic: National Geographic is the world s premium destination for science, exploration, and adventure. Through their world-class scientists, photographers, journalists, and filmmakers, Nat Geo gets you closer to the stories that matter and past the edge of what s possible. Get More National Geographic: Official Site: http://bit.ly/NatGeoOfficialSite Facebook: http://bit.ly/FBNatGeo Twitter: http://bit.ly/NatGeoTwitter Instagram: http://bit.ly/NatGeoInsta The Biggest Mack Engine Ever | Ulitmate Factories https://youtu.be/9k08SQcJkUg National Geographic https://www.youtube.com/natgeo

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Hey Everyone, You can find our 4K UHD content and more great space and science shows on: https://www.magellantv.com/genres/space These high-res time-lapse sequences captured by astronauts aboard the International Space Station give us a beautiful and clear view of some well-known coastlines and countries around the world. Get a good look at England, France, Italy, Egypt, Algeria, Tunisia, Greece, the island of Crete, Taiwan, South Korea, Japan, the United States, Mexico, Ecuador, Peru, Chile, Argentina, Cuba, and more. We ve attempted to show as many countries as we would, but inevitably we ve left many out. Please write to the the astronaut photography office at NASA s Johnson Space Center to request inclusion in this amazing series of sequences.

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Black hole extravaganza from ESOcast. Not long ago, watching something being ripped apart as it falls towards a giant black hole would be science fiction. This is now reality. Observers under dark skies, far from the bright city lights, can marvel at the splendor of the Milky Way, arching in an imposing band across the sky. Zooming in towards the center of our galaxy, about 25000 light years away, you can see that it is composed of myriads of stars. This is a pretty impressive sight, but much is hidden from view by interstellar dust, and astronomers need to look using a different wavelength, the infrared, that can penetrate the dust clouds. With large telescopes, astronomers can then see in detail the swarm of stars circling the supermassive black hole, in the same way that the Earth orbits the Sun. The Galactic Center harbors the closest supermassive black hole known, and the one that is also the largest in terms of its angular diameter on the sky, making it the best choice for a detailed study of black holes. This black hole s mass is a hefty four million times that of the Sun, earning it the title of supermassive black hole. Although it is huge, this black hole is currently supplied with little material and is not shining brightly. But this is about to change. Using ESO s Very Large Telescope, a team of astronomers has discovered a new object that is heading almost straight towards the black hole at vertiginous speed. The object is not a star, but a cloud of gas. "The cloud consists mainly of hydrogen gas, gas which we see anyhow in the galactic center all over the place. This particular cloud weighs more or less three times the mass of Earth. So it s a rather small and tiny blob only, but it glows very brightly in the light of the stars which are surrounding it ." As the astronomers watch, the cloud has been picking up pace as it gets closer to the giant black hole. Its speed has doubled in the last seven years and it is now speeding towards the black hole at more than 8 million kilometers per hour. The astronomers have already seen the cloud s outer layers becoming more and more disrupted over the last few years as it approaches the black hole. But the exciting part is yet to come. "The Black hole, imagine it sitting here, has a tremendous gravitational force and the cloud, as it comes in, it will be elongated and stretched, it will become essentially like spaghetti. It will be elongated and falling into the black hole." "The next few years will be really fantastic and exciting because we are probing the territory. Here this cloud comes and gets disrupted, but now it will begin to interact with the hot gas right around the black hole. We have never seen this before." No one knows what will happen next. The cloud will probably heat up and may start to emit powerful X- rays as it gets disrupted. In the end the material will eventually disappear by falling into the black hole. For the scientists, this event is truly a unique chance to probe the hot gas around the black hole. "But this process of how material gets into the black hole really is not clear to us we don t understand it in any detail. And here in the galactic center we have an opportunity so to speak to have a probe of this process. How material really gets added to the black hole, and what the physical processes are, how the interactions happen in this very central region. That s a fantastic opportunity." This is indeed science fiction becoming science fact.

The Mars Science Lab was launched November 26, 2011, and is scheduled to land on Mars at Gale Crater on August 6, 2012. The rover Curiosity, after completing a more precise landing than ever attempted previously, is intended to help assess Mars habitability for future human missions. Its primary mission objective is to determine whether Mars is or has ever been an environment able to support life. Curiosity is five times as large as either of the Mars Exploration Rovers Spirit or Opportunity and carries more than ten times the mass of scientific instruments present on the older vehicles. The rover is expected to operate for at least 686 days as it explores with greater range than any previous Mars rover. Here are some of the specs that help set Curiosity apart from the other rovers: The rover Curiosity is 3 meters in length, and weighs 900 kg, including 80 kg worth of scientific instruments. It is approximately the size of a Mini Cooper automobile. Once on the surface, Curiosity will be able to roll over obstacles approaching 75 cm high. Maximum terrain-traverse speed is estimated to be 90 meters per hour by automatic navigation, however, with average speeds likely to be about 30 meter per hour depending on power levels, difficulty of the terrain, slippage, and visibility. It is expected to traverse a minimum of 12 miles in its two-year mission. Curiosity is powered by a radioisotope thermoelectric generator, as used by the successful Mars landers Viking 1 and Viking 2 in 1976. Radioisotope power systems are generators that produce electricity from the natural decay of plutonium-238, which is a non-fissile isotope of plutonium. Heat given off by the natural decay of this isotope is converted into electricity, providing constant power during all seasons and through the day and night, and waste heat can be used via pipes to warm systems, freeing electrical power for the operation of the vehicle and instruments. The temperatures that Curiosity can encounter vary from +30 to −127 °C. Therefore, the Heat rejection system uses fluid pumped through 60 meters of tubing in the MSL body so that sensitive components are kept at optimal temperatures. The two identical on-board computers contain radiation-hardened memory to tolerate the extreme radiation environment from space and to safeguard against power-off cycles. Curiosity has two means of communication -- an X-band transmitter and receiver that can communicate directly with Earth, and a UHF software-defined radio for communicating with Mars orbiters. Communication with orbiters is expected to be the main method for returning data to Earth, since the orbiters have both more power and larger antennas than the lander. At landing time, 13 minutes, 46 seconds will be required for signals to travel between Earth and Mars. Like previous rovers Mars Exploration Rovers and Mars Pathfinder, Curiosity is equipped with 6 wheels in a rocker-bogie suspension. The suspension system will also serve as landing gear for the vehicle. Its smaller predecessors used airbag-like systems. Curiosity s wheels are significantly larger than those used on the previous rovers. Each wheel has a pattern of grooves that help it maintain traction, while leaving a distinctive track in Martian soil. That pattern, to be photographed by on-board cameras, will be used to judge the distance travelled.

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