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Friday, September 23, 2011

NASA's Space Shuttle Bus for Satellites

Three satellites stand out for their role in Earth science: the Earth Radiation Budget Satellite, the Upper Atmosphere Research Satellite, and the Laser Geodynamic Satellite 2.

Earth Radiation Budget Satellite

Launched from Challenger in October 1984 (top image), the Earth Radiation Budget Satellite was designed to investigate how energy from the Sun is absorbed and re-radiated by the planet, also known as the energy budget. The mission lasted 21 years, collecting key data on weather and climate, atmospheric ozone depletion, and the effects of fossil fuel burning.



The seven-ton Upper Atmosphere Research Satellite (UARS) (middle photo) was carried into space by shuttle Discovery in September 1991. UARS housed ten instruments to collect data on a variety of chemicals-including carbon dioxide, ozone, chlorine, methane, nitrogen oxides, and chlorofluorocarbons (CFCs)-and the processes that create, destroy, and mix them in the stratosphere, a region scarcely studied before the launch.

Laser Geodynamic Satellite 2

October 1992 brought the launch of the Laser Geodynamic Satellite 2 (LAGEOS) from a spinning solid fuel rocket (bottom image). Follow-on to LAGEOS 1, launched in 1979, the golf-ball shaped satellite was a simple aluminum sphere covered in tiny reflectors. Scientists could flash a pulse of laser light from the ground to the satellite to measure the geoid, or the shape of the Earth, and the movement of the planet’s tectonic plates.


Thursday, September 22, 2011

Six CMEs in 24 Hours

six coronal mass ejectionsThe sun let loose with at least six coronal mass ejections (CMEs) -- solar phenomena that can send solar particles into space and affect electronic systems in satellites -- from 7 PM ET on September 18, 2011 until 1 PM on September 19. The ejections appear to come from points scattered over the surface of the sun. Two CME's dissipated quickly, but four continue to spread outward from the sun. NASA models suggest that the leading edge of one CME will pass by Earth at around 5 PM ET on Sep 21, at which point sky watchers should be on the lookout for auroras.

Wednesday, September 21, 2011

Columbia Tank Found on Lakebed

Columbia Tank Found on LakebedA newly discovered aluminum tank from space shuttle Columbia's STS-107 mission will be recovered from the shoreline of Lake Nacogdoches in east Texas and eventually will likely be made available to researchers as are other parts of the Columbia debris, NASA's project manager for the recovery said.

"It's very important for us to bring all of Columbia home and we've done that since the accident in 2003," said Mike Ciannilli, the project manager for Columbia's recovery.

The sphere was one of 18 cryogenic tanks Columbia carried during its 16-day mission. It had been underwater for the past eight and half years, having landed there Feb. 1, 2003, when the shuttle broke up over east Texas during re-entry. It was uncovered recently when the lake's water level diminished by about 11 feet during an ongoing drought.

"Recently we got a call from the local authorities in Nacogdoches about a metal sphere and we asked the authorities to take a picture for us and send it to us," Ciannilli said. "We analyzed that with our teams here at the Cape and determined it to be a piece of space shuttle Columbia."

Tuesday, September 20, 2011

The Last Launch of Space Shuttle Endeavour

 Space Shuttle Endeavour

Two days ago, powerful yet controlled explosions rocketed the Space Shuttle Endeavour on its final trip into Earth orbit. The above image was taken seconds after liftoff as the massive orbiter and six astronauts began a climb to a height where the atmosphere is so thin it is unbreathable. The shuttle, on mission STS-134, is expected to dock with the International Space Station (ISS) today.

The Endeavour will deliver to the ISS, among other things, an ambitious detector called the Alpha Magnetic Spectrometer 2 (AMS), a detector that over the next few years could detect a significant abundance of specific types of dark matter, charged antimatter, and even a strangely possible variation of familiar matter called strangelets. The very last trip for any space shuttle is currently planned for mid-July when Atlantis will also visit the space station.

Monday, September 19, 2011

Cassini Present Saturn Moon Quintet

A quintet of Saturn's moonsWith the artistry of a magazine cover shoot, NASA's Cassini spacecraft captured this portrait of five of Saturn's moons poised along the planet's rings.
From left to right are Janus, Pandora, Enceladus, Mimas and finally Rhea, bisected by the right side of the frame. The view was acquired at a distance of approximately 684,000 miles (1.1 million kilometers) from Rhea and 1.1 million miles (1.8 million kilometers) from Enceladus.
The image was taken in visible green light with the Cassini spacecraft narrow-angle camera on July 29, 2011. Image scale is about 4 miles (7 kilometers) per pixel on Rhea and 7 miles (11 kilometers) per pixel on Enceladus.
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 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 operations center is based at the Space Science Institute in Boulder, Colo.

Friday, September 16, 2011

Space Shuttle Discovery

Discovery (OV-103), the third of NASA's fleet of reusable, winged spaceships, arrived at Kennedy Space Center in November 1983. It was launched on its first mission, flight 41-D, on August 30, 1984. It carried aloft three communications satellites for deployment by its astronaut crew.

Other Discovery milestones include the deployment of the Hubble Space Telescope on mission STS-31 in April 1990, the launching of the Ulysses spacecraft to explore the sun's polar regions on mission STS-41 in October of that year and the deployment of the Upper Atmosphere Research Satellite (UARS) in September 1991.

Discovery is named for two famous sailing ships; one sailed by Henry Hudson in 1610-11 to search for a northwest passage between the Atlantic and Pacific Oceans, and the other by James Cook on a voyage during which he discovered the Hawaiian Islands.

Thursday, September 15, 2011

Space Shuttle Launch and Landing

Space Shuttle launch and landing
Beginning with space shuttle Columbia's 1979 delivery to NASA's Kennedy Space Center in Florida, the center has been home to each of the five flown shuttle orbiters for the duration of the Space Shuttle Program. Space shuttle Atlantis completed the program on July 21, 2011, wrapping up the STS-135 mission with a predawn touchdown on the same runway where Columbia first arrived more than 30 years earlier.

NASA's shuttle fleet -- Columbia, Challenger, Discovery, Atlantis and Endeavour -- flew a total of 135 missions. Each one began at Kennedy's Launch Complex 39. Of those missions, 78 ended with a Kennedy landing; 54 concluded with a touchdown on the dry lake bed at Edwards Air Force Base in California; and one landed at White Sands Space Harbor in New Mexico.

Each mission began with a thundering liftoff as the shuttle's twin solid rocket boosters ignited, pushing the vehicle with its crew and cargo beyond the bounds of gravity and into the hostile environment of space. Missions typically lasted one to two weeks, concluding with an hourlong reentry descent through Earth's atmosphere and a precision landing. Because a returning shuttle orbiter was essentially an unpowered glider, there were no second chances -- every touchdown had to be perfect.

The shuttle then was towed to the nearby Vehicle Assembly Building, where it was joined to its tank and boosters. Finally, the completed launch vehicle and its mobile launcher platform rolled out to the launch pad atop a sturdy, slow-moving crawler-transporter. A spectacular liftoff was the reward for each processing flow, and upon landing, the sequence began once again.

Wednesday, September 14, 2011

NASA Launches Mission to Study Moon From Crust to Core

CAPE CANAVERAL, Fla. -- NASA's twin lunar Gravity Recovery and Interior Laboratory (GRAIL) spacecraft lifted off from Cape Canaveral Air Force Station in Florida at 9:08 a.m. EDT (6:08 a.m. PDT) Saturday, Sept. 10, to study the moon in unprecedented detail.

GRAIL-A is scheduled to reach the moon on New Year's Eve 2011, while GRAIL-B will arrive New Year's Day 2012. The two solar-powered spacecraft will fly in tandem orbits around the moon to measure its gravity field. GRAIL will answer longstanding questions about the moon and give scientists a better understanding of how Earth and other rocky planets in the solar system formed.

"If there was ever any doubt that Florida's Space Coast would continue to be open for business, that thought was drowned out by the roar of today's GRAIL launch," said NASA Administrator Charles Bolden. "GRAIL and many other exciting upcoming missions make clear that NASA is taking its next big leap into deep space exploration, and the space industry continues to provide the jobs and workers needed to support this critical effort."

The spacecraft were launched aboard a United Launch Alliance Delta II rocket. GRAIL mission controllers acquired a signal from GRAIL-A at 10:29 a.m. EDT (7:29 a.m. PDT). GRAIL-B's signal was received eight minutes later. The telemetry downlinked from both spacecraft indicates they have deployed their solar panels and are operating as expected.

Monday, September 12, 2011

Space Shuttle Atlantis

Space Shuttle Atlantis

Atlantis (OV-104) was delivered to Kennedy Space Center in April 1985. It lifted off on its maiden voyage on Oct. 3, 1985, on mission 51-J, the second dedicated Department of Defense flight. Later missions included the launch of the Galileo interplanetary probe to Jupiter on STS-34 in October 1989, and STS-37, with the Gamma Ray Observatory (GRO) as its primary payload, in April 1991.

Atlantis is named after a two-masted sailing ship that was operated for the Woods Hole Oceanographic Institute from 1930 to 1966.

Space Shuttle AtlantisAtlantis also served as the on-orbit launch site for many noteworthy spacecraft, including planetary probes Magellan and Galileo, as well as the Compton Gamma Ray Observatory. An impressive array of onboard science experiments took place during most missions to further enhance space research in low Earth orbit.

Starting with STS-71, Atlantis pioneered the Shuttle-Mir missions, flying the first seven missions to dock with the Russian space station. When linked, Atlantis and Mir together formed the largest spacecraft in orbit at the time. The missions to Mir included the first on-orbit U.S. crew exchanges, now a common occurrence on the International Space Station. On STS-79, the fourth docking mission, Atlantis ferried astronaut Shannon Lucid back to Earth after her record-setting 188 days in orbit aboard Mir.

In recent years, Atlantis has delivered several vital components to the International Space Station, including the U.S. laboratory module, Destiny, as well as the Joint Airlock Quest and multiple sections of the Integrated Truss structure that makes up the Station's backbone. As NASA seeks to fulfill the Vision for Space Exploration, beginning with the completion of the Station, Atlantis will be called upon for many missions to come.

Thursday, September 08, 2011

NASA's 747 SCAs--Birds of a Feather Flock Together

NASA’s Shuttle carrier aircraft905 and 911

For the first time ever, NASA's two highly modified Boeing 747 Shuttle Carrier Aircraft briefly flew in formation over the Edwards Air Force Base test range Aug. 2. Both aircraft were scheduled to be in the air on the same day, NASA 911 (foreground) on a flight crew proficiency flight, NASA 905 (rear) on a functional check flight following maintenance operations.

NASA’s Shuttle carrier aircraft905 and 911Since both aircraft were scheduled to be in the air at the same time, SCA pilot Jeff Moultrie of Johnson Space Center's Aircraft Operations Directorate took the opportunity to have both SCA's fly in formation for about 20 minutes while NASA photographer Carla Thomas captured still and video imagery from a NASA Dryden F/A-18.

In addition to Moultrie, NASA 905's check flight crew included pilot Arthur "Ace" Beall and flight engineer Henry Taylor while NASA 911 was flown by Larry LaRose, Steve Malarchick and Bob Zimmerman from NASA Johnson and Frank Batteas and Bill Brockett from NASA Dryden.

NASA Orbiter Fleet - Columbia

First Orbiter Fleet,ColumbiaColumbia (OV-102), the first of NASA's orbiter fleet, was delivered to Kennedy Space Center in March 1979. Columbia initiated the Space Shuttle flight program when it lifted off Pad A in the Launch Complex 39 area at KSC on April 12, 1981. It proved the operational concept of a winged, reusable spaceship by successfully completing the Orbital Flight Test Program - missions STS-1 through STS-4.

Other, achievements for Columbia included the recovery of the Long Duration Exposure Facility (LDEF) satellite from orbit during mission STS-32 in January 1990, and the STS-40 Spacelab Life Sciences mission in June 1991 - the first manned Spacelab mission totally dedicated to human medical research.

Columbia was destroyed over east Texas on its landing descent to Kennedy Space Center on Feb. 1, 2003, at 8:59 a.m. EST at the conclusion of a microgravity research mission, STS-107.

Columbia was named after a small sailing vessel that operated out of Boston in 1792 and explored the mouth of the Columbia River. One of the first ships of the U.S. Navy to circumnavigate the globe was named Columbia. The command module for the Apollo 11 lunar mission was also named Columbia.

Thursday, August 25, 2011

Planet X (Nibiru) Is Quickly Approaching 2012

Planet X or Nibiru is passed between the planets Mars and Jupiter a few 7,200 years ago. "It's definitely bigger than Pluto." So says Dr. Mike Brown of the California Institute of Technology who announced today the discovery of a new planet in the outer solar system.

The planet, which hasn't been officially named yet, was found by Brown and colleagues using the Samuel Oschin Telescope at Palomar Observatory near San Diego. It is currently about 97 times farther from the sun than Earth, or 97 Astronomical Units(AU). For comparison, Pluto is 40 AU from the sun.

This places the new planet more or less in the Kuiper Belt, a dark realm beyond Neptune where thousands of small icy bodies orbit the sun. The planet appears to be typical of Kuiper Belt objects--only much bigger. Its sheer size in relation to the nine known planets means that it can only be classified as a planet itself, Brown says.

Backyard astronomers with large telescopes can see the new planet. But don't expect to be impressed: It looks like a dim speck of light, visual magnitude 19, moving very slowly against the starry background.

The planet was discovered by, in addition to Brown, Chad Trujillo, of the Gemini Observatory in Mauna Kea, Hawaii, and David Rabinowitz, of Yale University, New Haven, Connecticut. They first photographed the new planet with the 48-inch Samuel Oschin Telescope on October 31, 2003. The object was so far away, however, that its motion was not detected until they reanalyzed the data in January of this year. In the last seven months, the scientists have been studying the planet to better estimate its size and its motions.

Tohoku Tsunami Created Icebergs In Antarctica

A NASA scientist and her colleagues were able to observe for the first time the power of an earthquake and tsunami to break off large icebergs a hemisphere away.

Kelly Brunt, a cryosphere specialist at Goddard Space Flight Center, Greenbelt, Md., and colleagues were able to link the calving of icebergs from the Sulzberger Ice Shelf in Antarctica following the Tohoku Tsunami, which originated with an earthquake off the coast of Japan in March 2011. The finding, detailed in a paper published online today in the Journal of Glaciology, marks the first direct observation of such a connection between tsunamis and icebergs.

The birth of an iceberg can come about in any number of ways. Often, scientists will see the towering, frozen monoliths break into the polar seas and work backwards to figure out the cause.So when the Tohoku Tsunami was triggered in the Pacific Ocean on March 11 this spring, Brunt and colleagues immediately looked south. All the way south. Using multiple satellite images, Brunt, Emile Okal at Northwestern University and Douglas MacAyeal at University of Chicago were able to observe new icebergs floating off to sea shortly after the sea swell of the tsunami reached Antarctica.

To put the dynamics of this event in perspective: An earthquake off the coast of Japan caused massive waves to explode out from its epicenter. Swells of water swarmed toward an ice shelf in Antarctica, 8,000 miles (13,600 km) away, and about 18 hours after the earthquake occurred, those waves broke off several chunks of ice that together equaled about two times the surface area of Manhattan. According to historical records, this particular piece of ice hadn't budged in at least 46 years before the tsunami came along.

Sunday, July 17, 2011

NASA's Dawn Spacecraft Enters Orbit Around Asteroid Vesta

PASADENA, Calif. -- NASA's Dawn spacecraft on Saturday became the first probe ever to enter orbit around an object in the main asteroid belt between Mars and Jupiter.

Dawn will study the asteroid, named Vesta, for a year before departing for a second destination, a dwarf planet named Ceres, in July 2012. Observations will provide unprecedented data to help scientists understand the earliest chapter of our solar system. The data also will help pave the way for future human space missions.

"Today, we celebrate an incredible exploration milestone as a spacecraft enters orbit around an object in the main asteroid belt for the first time," NASA Administrator Charles Bolden said. "Dawn's study of the asteroid Vesta marks a major scientific accomplishment and also points the way to the future destinations where people will travel in the coming years. President Obama has directed NASA to send astronauts to an asteroid by 2025, and Dawn is gathering crucial data that will inform that mission."

The spacecraft relayed information to confirm it entered Vesta's orbit, but the precise time this milestone occurred is unknown at this time. The time of Dawn's capture depended on Vesta's mass and gravity, which only has been estimated until now. The asteroid's mass determines the strength of its gravitational pull. If Vesta is more massive, its gravity is stronger, meaning it pulled Dawn into orbit sooner. If the asteroid is less massive, its gravity is weaker and it would have taken the spacecraft longer to achieve orbit. With Dawn now in orbit, the science team can take more accurate measurements of Vesta's gravity and gather more accurate timeline information.

Dawn, which launched in September 2007, is on track to become the first spacecraft to orbit two solar system destinations beyond Earth. The mission to Vesta and Ceres is managed by NASA's Jet Propulsion Laboratory in Pasadena, Calif., for the agency's Science Mission Directorate in Washington. Dawn is a project of the directorate's Discovery Program, which is managed by NASA's Marshall Space Flight Center in Huntsville, Ala.

The University of California, Los Angeles, is responsible for the overall Dawn mission science. Orbital Sciences Corp. of 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 part of the mission's team. JPL is a division of the California Institute of Technology in Pasadena.

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Thursday, July 14, 2011

AQUA Mission-NASA



Aqua Mission

Aqua is a major international Earth Science satellite mission centered at NASA. Launched on May 4, 2002, the satellite has six different Earth-observing instruments on board and is named for the large amount of information being obtained about water in the Earth system from its stream of approximately 89 Gigabytes of data a day. The water variables being measured include almost all elements of the water cycle and involve water in its liquid, solid, and vapor forms. Additional variables being measured include radiative energy fluxes, aerosols, vegetation cover on the land, phytoplankton and dissolved organic matter in the oceans, and air, land, and water temperatures.

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Thursday, July 07, 2011

Cassini Spacecraft Captures Images and Sounds of Big Saturn Storm

PASADENA, Calif. – Scientists analyzing data from NASA's Cassini spacecraft now have the first-ever, up-close details of a Saturn storm that is eight times the surface area of Earth.

On Dec. 5, 2010, Cassini first detected the storm that has been raging ever since. It appears at approximately 35 degrees north latitude on Saturn. Pictures from Cassini's imaging cameras show the storm wrapping around the entire planet covering approximately 1.5 billion square miles (4 billion square kilometers).

The storm is about 500 times larger than the biggest storm previously seen by Cassini during several months from 2009 to 2010. Scientists studied the sounds of the new storm's lightning strikes and analyzed images taken between December 2010 and February 2011. Data from Cassini's radio and plasma wave science instrument showed the lightning flash rate as much as 10 times more frequent than during other storms monitored since Cassini's arrival to Saturn in 2004. The data appear in a paper published this week in the journal Nature.

"Cassini shows us that Saturn is bipolar," said Andrew Ingersoll, an author of the study and a Cassini imaging team member at the California Institute of Technology in Pasadena, Calif. "Saturn is not like Earth and Jupiter, where storms are fairly frequent. Weather on Saturn appears to hum along placidly for years and then erupt violently. I'm excited we saw weather so spectacular on our watch."

At its most intense, the storm generated more than 10 lightning flashes per second. Even with millisecond resolution, the spacecraft's radio and plasma wave instrument had difficulty separating individual signals during the most intense period. Scientists created a sound file from data obtained on March 15 at a slightly lower intensity period.

Cassini has detected 10 lightning storms on Saturn since the spacecraft entered the planet's orbit and its southern hemisphere was experiencing summer, with full solar illumination not shadowed by the rings. Those storms rolled through an area in the southern hemisphere dubbed "Storm Alley." But the sun's illumination on the hemispheres flipped around August 2009, when the northern hemisphere began experiencing spring.

"This storm is thrilling because it shows how shifting seasons and solar illumination can dramatically stir up the weather on Saturn," said Georg Fischer, the paper's lead author and a radio and plasma wave science team member at the Austrian Academy of Sciences in Graz. "We have been observing storms on Saturn for almost seven years, so tracking a storm so different from the others has put us at the edge of our seats."

The storm's results are the first activities of a new "Saturn Storm Watch" campaign. During this effort, Cassini looks at likely storm locations on Saturn in between its scheduled observations. On the same day that the radio and plasma wave instrument detected the first lightning, Cassini's cameras happened to be pointed at the right location as part of the campaign and captured an image of a small, bright cloud. Because analysis on that image was not completed immediately, Fischer sent out a notice to the worldwide amateur astronomy community to collect more images. A flood of amateur images helped scientists track the storm as it grew rapidly, wrapping around the planet by late January 2011.

The new details about this storm complement atmospheric disturbances described recently by scientists using Cassini's composite infrared spectrometer and the European Southern Observatory's Very Large Telescope. The storm is the biggest observed by spacecraft orbiting or flying by Saturn. NASA's Hubble Space Telescope captured images in 1990 of an equally large storm.

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. NASA's Jet Propulsion Laboratory in Pasadena manages the mission for the agency's Science Mission Directorate in Washington. The radio and plasma wave science team is based at the University of Iowa, Iowa City, where the instrument was built. The imaging team is based at the Space Science Institute in Boulder, Colo. JPL is a division of the California Institute of Technology, Pasadena.