India launches GSAT-10 successfully

An Ariane 5 rocket carrying two satellites, ASTRA 2F and GSAT-10, blasts off from the European space centre of Kourou, French Guiana. AFP/CNES/CSG/S Martin
India's advanced communication satellite GSAT-10 that would augment telecommunication, direct-to-home broadcasting and radio navigation services was successfully launched early on Saturday on board Ariane-5 rocket from Europe's spaceport in French Guiana in South America. At the end of a smooth countdown lasting 11 hours and 30 minutes, Ariane-5 ECA rocket injected GSAT-10 into an elliptical Geosynchronous Transfer Orbit (GTO), very close to the intended one, after a flight of 30 minutes and 45 seconds, Indian Space Research Organisation said. At 3,400kg at lift-off, GSAT-10 is the heaviest built by Bangalore-headquartered Isro. GSAT-10 project is a Rs. 750 crore mission that includes the cost of satellite, launch services by the European space consortium Arianespace and insurance. Soon after GSAT-10 was hurtled into space, Isro's Master Control Facility (MCF) at Hassan in Karnataka took over the command and control of the satellite and declared the launch of Indian space agency's 101st space mission a success. "The satellite is in good health," Isro said after checks on various subsystems of the spacecraft, adding all its parameters were satisfactory. Blasting off from the launch pad at 2.48am (IST), Arianespace's rocket first injected European co-passenger ASTRA 2F into orbit followed by GSAT-10. With a 15-year design life, GSAT-10 is expected to be operational by November and will augment telecommunication, DTH and radio navigation services by adding 30 more to the much-in-demand transponder capacity, now hit by a crunch. Isro chairman K Radhakrishnan, who was at MCF at Hassan at the launch, said, "By November 2012, we expect to operationalise GSAT-10 and make it available to the user community. GSAT-10 is fitted with 30 transponders (12 Ku-band, 12 C-band and six Extended C-Band), which will provide vital augmentation to INSAT/GSAT transponder capacity. With a scramble for transponders, India is now managing a significant part of its requirement by leasing foreign transponders to meet the domestic demand. GSAT-10 also has a navigation payload – GAGAN (GPS aided Geo Augmented Navigation) -- that would provide improved accuracy of GPS signals (of better than seven metres) to be used by Airports Authority of India for civil aviation requirements. This is the second satellite in INSAT/GSAT constellation with GAGAN payload after GSAT-8, launched in May 2011. GSAT-10 was originally scheduled for a Sept 22 launch, but was deferred after scientists detected a small glitch --one gram of dust -- in the upper part of the rocket. GSAT-10 project director TK Anuradha, additional secretary of department of Space, S Srinivasan and director of Isro Satellite Centre SK Shivakumar were among key Isro officials who were in French Guiana for the launch. Shivakumar said GSAT-10 would give an impetus to the 'communication revolution' in India.Arianespace chairman & CEO Jean-Yves Le Gall said at the launch base that Isro is a highly loyal customer, as the collaboration with it began more than 30 years ago with its Apple satellite's orbiting by the third flight of an Ariane vehicle – an Ariane 1 version launched in June 1981. In the coming five days, orbit raising manoeuvres will be performed to place the satellite in the Geostationary Orbit with required inclination with reference to the equator, Isro said. The satellite will be moved to the Geostationary Orbit (36,000km above the equator) by using the satellite propulsion system in a three step approach. After the completion of orbit raising operations, the two solar panels and both the dual gridded antenna reflectors of GSAT-10 will be deployed for further tests and operations. It is planned to experimentally turn on the communication payloads in the second week of October, Isro said. After the successful completion of all in-orbit tests, GSAT-10 will be ready for operational use by November. GSAT-10 will be positioned at 83 deg East orbital location along with INSAT-4A and GSAT-12.Source: Hindustan Times
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Juno's Two Deep Space Maneuvers are 'Back-To-Back Home Runs'

NASA's Juno spacecraft successfully executed a second Deep Space Maneuver, called DSM-2 last Friday, September 14. The 30 minute firing of its main engine refined the Jupiter-bound spacecraft's trajectory, setting the stage for a gravity assist from a flyby of Earth on October 9, 2013. Juno will arrive at Jupiter on July 4, 2016. The maneuver began at 3:30 p.m. PDT (6:30 p.m. EDT), when the Leros-1b main engine began to fire. The burn ended at 4 p.m. PDT (7 p.m. EDT). Based on telemetry, the Juno project team believes the burn was accurate, changing the spacecraft's velocity by about 867 mph (388 meters a second) while consuming about 829 pounds (376 kilograms) of fuel. The burn occurred when Juno was more than 298 million miles (480 million kilometers) from Earth. Juno executed its first deep space maneuver (DSM-1), one of comparable duration and velocity change, on August 30. Together, both maneuvers placed Juno on course for its Earth flyby, which will occur as the spacecraft is completing one elliptical orbit around the sun. The Earth flyby will boost Juno's velocity by 16,330 mph (about 7.3 kilometers per second), placing the spacecraft on its final flight path for Jupiter. The closest approach to Earth, on October 9, 2013, will occur when Juno is at an altitude of about 348 miles (560 kilometers). "It feels like we hit back-to-back home runs here with the near-flawless propulsion system performance seen during both DSM-1 and DSM-2." said Juno Project Manager Rick Nybakken of NASA's Jet Propulsion Laboratory in Pasadena, California. "These successes move us closer to being ready for our most critical mission event, the Jupiter Orbit Insertion main engine burn in July 2016. We're not in the playoffs yet, as that will come in 2016 when we arrive at Jupiter, but it does feel fantastic to have hit both of these DSMs out of the park." Juno was launched on August 5, 2011. Once in orbit, the spacecraft will circle Jupiter 33 times, from pole to pole, and use its collection of eight science instruments to probe beneath the gas giant's obscuring cloud cover. Juno's science team will learn about Jupiter's origins, structure, atmosphere and magnetosphere, and look for a potential solid planetary core. Juno's name comes from Greek and Roman mythology. The god Jupiter drew a veil of clouds around himself to hide his mischief, and his wife, the goddess Juno, was able to peer through the clouds and reveal Jupiter's true nature. Illustration credit: NASA/JPL-Caltech, Source: Minsex
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NASA to launch another Mars mission in 2016

WASHINGTON: Encouraged by the success of “Curiosity”, NASA has announced to launch a new Mars mission in 2016 to take a better look into the guts of the Red Planet. The mission called “InSight” will investigate why Mars’ crust is not divided into tectonic plates that drift like Earth’s. Detailed knowledge of the interior of Mars in comparison to Earth will help scientists understand better how terrestrial planets form and evolve, the American space agency said. “The exploration of Mars is a top priority for NASA, and the selection of ‘InSight’ ensures we will continue to unlock the mysteries of the Red Planet and lay the groundwork for a future human mission there,” said NASA administrator Charles Bolden. “The recent successful landing of the Curiosity rover has galvanised public interest in space exploration and today’s announcement makes clear there are more exciting Mars missions to come,” he said referring to the success of Curiosity. The 12th selection in NASA’s series of Discovery-class missions, ‘InSight’ is build on spacecraft technology used in the space agency’s highly successful Phoenix lander mission, which was launched to the Red Planet in 2007 and determined water existed near the surface in the Martian polar regions. “Our Discovery Programme enables scientists to use innovative approaches to answering fundamental questions about our solar system in the lowest cost mission category,” said John Grunsfeld, associate administrator for the Science Mission Directorate at NASA Headquarters. “’InSight’ will get to the ‘core’ of the nature of the interior and structure of Mars, well below the observations we’ve been able to make from orbit or the surface,” Grunsfeld said. Source: Punjab News
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Mapping the Heliosphere

Minsex: Data from NASA's Cassini spacecraft have enabled scientists to create this map of the heliosphere, the bubble of charged particles around our Sun. Charged particles stream out from our Sun in a phenomenon known as solar wind. The solar wind interacts with the matter between stars, which is known as the interstellar medium. The mingling of interstellar medium and solar wind creates particles called energetic neutral atoms, which stream back towards the Sun. The ion and neutral camera on Cassini's magnetospheric imaging instrument detects energetic neutral atoms. This map shows those in the range of 5,200 to 13,500 electron volts. The regions with the highest intensity of particles are red and those with the lowest intensity of particles are blue. Cassini detects a different spectrum of energetic neutral atoms than NASA's Interstellar Boundary Explorer (IBEX) does. The IBEX images show lower-energy particles. NASA's Voyager mission collects data on energetic ions in the region that is the source of the energetic neutral atoms.The area where IBEX found a ribbon of high-intensity particles is outlined in white. The locations of Voyager 1 and Voyager 2 are indicated with the labels "V1" and "V2." The label "nose" indicates the direction that our solar system is traveling through the interstellar medium. The label "tail" indicates the region in the direction opposite the nose. Image credit: NASA/JPL/JHUAPL Source: Minsex
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Cassini Shows Why Jet Streams Cross-Cut Saturn

Image above: A particularly strong jet stream churns through Saturn's northern hemisphere in this false-color view from NASA's Cassini spacecraft. Image credit: NASA/JPL-Caltech/SSI.
Turbulent jet streams, regions where winds blow faster than in other places, churn east and west across Saturn. Scientists have been trying to understand for years the mechanism that drives these wavy structures in Saturn's atmosphere and the source from which the jets derive their energy. In a new study appearing in the June edition of the journal Icarus, scientists used images collected over several years by NASA's Cassini spacecraft to discover that the heat from within the planet powers the jet streams. Condensation of water from Saturn's internal heating led to temperature differences in the atmosphere. The temperature differences created eddies, or disturbances that move air back and forth at the same latitude, and those eddies, in turn, accelerated the jet streams like rotating gears driving a conveyor belt. A competing theory had assumed that the energy for the temperature differences came from the sun. That is how it works in the Earth's atmosphere. "We know the atmospheres of planets such as Saturn and Jupiter can get their energy from only two places: the sun or the internal heating. The challenge has been coming up with ways to use the data so that we can tell the difference," said Tony Del Genio of NASA's Goddard Institute for Space Studies, N.Y., the lead author of the paper and a member of the Cassini imaging team. The new study was possible in part because Cassini has been in orbit around Saturn long enough to obtain the large number of observations required to see subtle patterns emerge from the day-to-day variations in weather. "Understanding what drives the meteorology on Saturn, and in general on gaseous planets, has been one of our cardinal goals since the inception of the Cassini mission," said Carolyn Porco, imaging team lead, based at the Space Science Institute, Boulder, Colo. "It is very gratifying to see that we're finally coming to understand those atmospheric processes that make Earth similar to, and also different from, other planets." Rather than having a thin atmosphere and solid-and-liquid surface like Earth, Saturn is a gas giant whose deep atmosphere is layered with multiple cloud decks at high altitudes. A series of jet streams slice across the face of Saturn visible to the human eye and also at altitudes detectable to the near-infrared filters of Cassini's cameras. While most blow eastward, some blow westward. Jet streams occur on Saturn in places where the temperature varies significantly from one latitude to another. Thanks to the filters on Cassini's cameras, which can see near-infrared light reflected to space, scientists now have observed the Saturn jet stream process for the first time at two different, low altitudes. One filtered view shows the upper part of the troposphere, a high layer of the atmosphere where Cassini sees thick, high-altitude hazes and where heating by the sun is strong. Views through another filter capture images deeper down, at the tops of ammonia ice clouds, where solar heating is weak but closer to where weather originates. This is where water condenses and makes clouds and rain. In the new study, which is a follow-up to results published in 2007, the authors used automated cloud tracking software to analyze the movements and speeds of clouds seen in hundreds of Cassini images from 2005 through 2012. "With our improved tracking algorithm, we've been able to extract nearly 120,000 wind vectors from 560 images, giving us an unprecedented picture of Saturn's wind flow at two independent altitudes on a global scale," said co-author and imaging team associate John Barbara, also at the Goddard Institute for Space Studies. The team's findings provide an observational test for existing
This figure (above) examines a particularly strong jet stream and the eddies that drive it through the atmosphere of Saturn's northern hemisphere. Image credit: NASA/JPL-Caltech/SSI.
models that scientists use to study the mechanisms that power the jet streams. By seeing for the first time how these eddies accelerate the jet streams at two different altitudes, scientists found the eddies were weak at the higher altitudes where previous researchers had found that most of the sun's heating occurs. The eddies were stronger deeper in the atmosphere. Thus, the authors could discount heating from the sun and infer instead that the internal heat of the planet is ultimately driving the acceleration of the jet streams, not the sun. The mechanism that best matched the observations would involve internal heat from the planet stirring up water vapor from Saturn's interior. That water vapor condenses in some places as air rises and releases heat as it makes clouds and rain. This heat provides the energy to create the eddies that drive the jet streams. The condensation of water was not actually observed; most of that process occurs at lower altitudes not visible to Cassini. But the condensation in mid-latitude storms does happen on both Saturn and Earth. Storms on Earth – the low- and high-pressure centers on weather maps – are driven mainly by the sun's heating and do not mainly occur because of the condensation of water, Del Genio said. On Saturn, the condensation heating is the main driver of the storms, and the sun's heating is not important. Images of one of the strongest jet streams and a figure from the paper can be found at http://www.nasa.gov/cassini ,http://saturn.jpl.nasa.gov and http://ciclops.org . 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 Science Mission Directorate, Washington. 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 in Boulder, Colo. Images (mentioned), Credits: NASA's Goddard Space Flight Center / Bill Steigerwald / Nancy Neal Jones / Space Science Institute / Joe Mason / JPL / Jia-Rui C. Cook.Orbiter.ch Space News: Source: Orbiter Chspace
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