Friday, November 20, 2009

Robotics and Spacewalk Today

False depressurization caution alarms sounded on the International Space Station last night just after 8:30 p.m. EST waking the shuttle and station crew. The flight control teams on the ground were able to determine there was no depressurization occurring. The crew was never in any danger and ventilation fans were shutoff as a precaution. That shutoff kicked up dust that resulted in a fire alarm in the European Columbus laboratory also sounding.

By 9:15 p.m., the flight control teams in Houston were working to bring the station back into its normal configuration, and Atlantis’ crew was told it could go back to sleep. The space station crew members were required to stay up a bit longer as the station’s ventilation system was reactivated. That work took a little over an hour, after which the station crew was able to resume its sleep period as well. Flight control teams are looking into the cause of the initial false alarm.

Thursday, November 19, 2009

A Partial View - Nasa Space Station


Backdropped by the blackness of space, a partial view of Space Shuttle Atlantis' payload bay, vertical stabilizer, orbital maneuvering system pods and docking mechanism are featured in this image photographed by the STS-129 crew from an aft flight deck window.

The spacewalk began

Astronauts Busy Inside and Outside Station Today
Atlantis’ crew was awakened at 4:28 a.m. EST to the sound of The Newsboys’ song “In Wonder.” It was played for Mission Specialist Randy Bresnik, who is choreographing today’s spacewalk from inside the station.

The spacewalk began at 9:24 a.m. and is scheduled to last 6.5 hours. Mission Specialists Mike Foreman and Robert Satcher installed a spare S-band antenna structural assembly brought up in Atlantis’ cargo bay. The equipment is being stored on the Z1 segment of the station’s truss system, and to get it there Satcher rode the station’s robotic arm, driven by Mission Specialist Leland Melvin, Commander Charles Hobaugh and Pilot Barry Wilmore.

Meanwhile, inside the station, further work is going on to prepare the station for the arrival of the Tranquility node. Station Commander Frank De Winne and Flight Engineer Jeff Williams will be working at the port hatch of the Harmony node to rewire data, power and cooling lines and air flow connections that will be connected to Tranquility. Their task is also scheduled to take about 6.5 hours today. De Winne and Williams will continue working on the project over several days during the STS-129 mission.

Wednesday, November 18, 2009

Space shuttle Atlantis

Space shuttle Atlantis docked with the station at 11:51 a.m. EST.

After a series of leak checks that should take about two hours, the hatches between the two vehicles will be opened and the two crews will start their joint operations.

Space shuttle Atlantis is scheduled to dock to the station at 11:53 a.m. EST and deliver two pallets carrying more than 20,000 pounds worth of spare equipment too large to be launched into space aboard any other vehicle.

The morning focused on preparations for the rendezvous and docking to the station. Commander Charles Hobaugh and Pilot Barry Wilmore performed a few final corrective jet firings to refine the orbiter’s path to the station and position the vehicle for its rendezvous pitch maneuver 600 feet beneath the station.

Hobaugh will fly Atlantis ahead of the space station and slowly back it in for the docking to the station’s Harmony node. After a series of leak checks that should take about two hours, the hatches between the two vehicles will be opened and the two crews will start their joint operations.

Hatch opening will mark the end of Flight Engineer Nicole Stott’s two-and-a-half-month stint with the space station’s crew.

Tuesday, November 17, 2009

All 'SMILES' Aboard International Space Station in Wake of New Experiment

There's a new way to look at environmental issues on Earth -- from 210 miles up aboard the International Space Station -- and investigators are all "SMILES" with early results.

The SMILES experiment, more properly known as the Superconducting Submillimeter-wave Limb-emission Sounder, is investigating issues such as ozone depletion and air quality problems.

The experiment launched on the Japanese Aerospace Exploration Agency’s H-II Transfer Vehicle in September -- an unmanned cargo ship for station resupply. Housed on the Japanese Experiment Module's Exposed Facility, SMILES is gathering data on trace gases known to cause ozone depletion, such as chlorine and bromine compounds. The Exposed Facility provides a multipurpose platform where science experiments can be deployed and operated in open space. The observations are taken in the stratosphere, the region of the atmosphere six to 30 miles above the Earth's surface.

"Measurements of ozone and trace gases in the stratosphere from instruments such as SMILES are important for understanding the dynamics of Earth’s atmosphere," said Julie Robinson, International Space Station program scientist at Johnson Space Center in Houston.

The advantage of this experiment is the space station's power and payload resources, which enable researchers to test out new technologies. As a result, SMILES can measure precise molecules of trace atmospheric gases and obtain data about elements in quantities too small to be measured until now.

SMILES observations taken in October show that ozone amounts are greater around Earth's equatorial region than at higher latitudes, illustrating the characteristics of stratospheric ozone in its global distribution.

"This is just the beginning," said Takuki Sano, a member of the SMILES science team with the Japan Aerospace Exploration Agency. "In due course, SMILES, with its full-scale observation, will contribute to the prediction of ozone depletion through analyses of the accumulated observation data, thus clarifying the influence the stratosphere has on the troposphere -- the lowest and most dense layer of the atmosphere 10 to 12 miles above the Earth’s surface."

Monitoring the Launch


NASA mission managers monitor the launch of the space shuttle Atlantis from Firing Room Four of the NASA Kennedy Space Center, Monday, Nov. 16, 2009. Shuttle Atlantis and its six-member crew are on an 11-day STS-129 mission to the International Space Station to transport spare hardware to the outpost and return a station crew member who spent more than two months in space.

Space Station Assembly



Russian Progress Spacecraft

The Progress resupply vehicle is an automated, unpiloted version of the Soyuz spacecraft that is used to bring supplies and fuel to the International Space Station. The Progress also has the ability to raise the Station's altitude and control the orientation of the Station using the vehicle's thrusters.

Image to right: A Progress spacecraft sits atop a Soyuz rocket at Baikonur Cosmodrome. Credit: NASA

Both the Progress M and M1 versions have a pressurized Cargo Module to carry supplies, a Refueling Module that holds fuel tanks containing propellant and pressurized gases, and an Instrumentation/Propulsion Module where the Progress systems equipment and thrusters are located.

The Progress spacecraft is launched to the Space Station from the Baikonur Cosmodrome in Kazakhstan aboard a Soyuz rocket. It normally docks to the end of the Station's Zvezda Service Module, but it can also dock to the bottom of the Pirs Docking Compartment.

Cargo Module

The Progress Cargo Module -- which is similar in construction to the Soyuz Orbital Module -- can carry up to 1,700 kilograms (3,748 pounds) of supplies to the Space Station in a pressurized volume of about 6 cubic meters (212 cubic feet). Once the Progress docks with the Space Station, the crew enters the Cargo Module through the docking hatch.

After the cargo is removed and before the Progress undocks, the crew refills it with trash, unneeded equipment and wastewater, which will burn up with the spacecraft when it re-enters the Earth's atmosphere. The Cargo Module can hold 1,000 to 1,700 kilograms (2,205 to 3,748 pounds) of trash.


Refueling Module
In place of the Soyuz Descent Module, the Progress has a Refueling Module. The Progress M1 Refueling Module has eight propellant tanks that can hold up to 1,740 kilograms (3,836 pounds) of fuel, depending on how much weight is carried in the Cargo Module. Four of the tanks contain fuel, while the other four contain the fuel's oxidizer. The Progress M has four tanks -- two for fuel and two for oxidizer -- and two water tanks. The M1 has no water tanks.

The contents of the fuel and oxidizer tanks can be transferred to the Space Station's own propulsion system through fluid connectors in the docking ring. This propellant can also be used by the Progress' thrusters to boost the Station altitude or to change its orientation, or attitude, in space.

Instrumentation/Propulsion Module

This module contains the electronic equipment, or avionics, for the Progress' systems and sensors. It is similar in design to the Soyuz Instrumentation/Propulsion Module. Any fuel in this module that is not used to get the Progress to the Station or for undocking and deorbit can be used to boost the altitude of the Space Station. Surplus fuel amounts can vary from 185 to 250 kilograms (408 to 551 pounds).

Rendezvous, Docking and Undocking

The Progress normally takes two days to reach the Space Station. The rendezvous and docking are both automated, although once the spacecraft is within 150 meters (492 feet) of the Station, the Russian Mission Control Center just outside Moscow and the Station crew monitor the approach and docking.

The Progress uses an automated, radar-based system called Kurs to dock to the Station. The active portion of the Kurs is on the Progress and the passive equipment is on the Station. The Station crew can also dock the Progress using the TORU system, a backup remote control docking system in the Station's Zvezda Service Module.

Once the Progress is filled with trash, usually a day before the launch of the next Progress vehicle, the Station crew closes the hatches and initiates the undocking process. Once the Progress has undocked, the vehicle's thrusters are fired to maneuver it into an orbit that will send it into the Earth's atmosphere, where it will burn up on re-entry over the Pacific Ocean.

NASA Moon Mission Wins Second-Best of 'What's New' Award by Popular Science

The Lunar Reconnaissance Orbiter (LRO) is cited as one of the best innovations in aviation in the December issue of Popular Science.

"It is an honor to be selected by Popular Science for Best of What’s New in aviation," said Craig Tooley, LRO project manager from NASA’s Goddard Space Flight Center in Greenbelt, Md. "There was tremendous excitement about the United States returning to the moon after many years. I believe our selection is a result of that excitement."

Each year, the editors of Popular Science review thousands of products in search of the top 100 tech innovations of the year; breakthrough products and technologies that represent a significant leap in their categories. The winners -- the Best of What's New -- are awarded inclusion in the much-anticipated December issue of Popular Science, the most widely read issue of the year since the debut of Best of What's New in 1987. Best of What's New awards are presented to 100 new products and technologies in 11 categories: Automotive, Aviation and Space, Computing, Engineering, Gadgets, Green Technology, Home Entertainment, Security, Home Technology, Personal Health and Recreation.

"For 22 years, Popular Science has honored the innovations that surprise and amaze us -- those that make a positive impact on our world today and challenge our views of what’s possible in the future." said Mark Jannot, editor-in-chief of Popular Science. "The Best of What’s New Award is the magazine’s top honor, and the 100 winners -- chosen from among thousands of entrants -- represent the highest level of achievement in their fields."

LRO launched from Kennedy Space Center, Fla. on June 18, 2009. Since that time the spacecraft has completed calibration and commissioning. LRO has already begun its detailed survey of the moon. First results from the mission included -- new looks at the Apollo landing sites; indications that permanently shadowed and nearby regions may harbor water and hydrogen; observations that large areas in the permanently shadowed regions are colder than Pluto; and detailed information on terrain roughness.

LRO is scheduled for a one year exploration mission in a polar orbit about 31 miles above the lunar surface. During the next year, LRO will produce a complete map of the lunar surface in unprecedented detail, search for resources and potential safe landing sites for human explorers and measure lunar temperatures and radiation levels.

NASA’s Goddard Space Flight Center built and manages the mission for the Exploration Systems Mission Directorate at NASA Headquarters in Washington. The Institute for Space Research, Moscow, provided the neutron detector aboard the spacecraft.

Monday, November 16, 2009

Ares I-X Flight Test

The Ares I-X Flight Test blasts off from the launch pad at NASA’s Kennedy Space Center. Image Credit: Thilo Kranz, Deutsches Zentrum fur Luft-und Raumhahrt (German Space Agency)


Ares I-X, including the Upper Stage Simulator (USS) built at NASA’s Glenn Research Center, is illuminated the night before launch. Image Credit: Thilo Kranz, Deutsches Zentrum fur Luft-und Raumhahrt (German Space Agency)

NASA's Ares I-X Rocket Completes Successful Flight Test

CAPE CANAVERAL, Fla. -- NASA's Ares I-X test rocket lifted off at 11:30 a.m. EDT Wednesday from NASA's Kennedy Space Center in Florida for a two-minute powered flight. The test flight lasted about six minutes from its launch from the newly-modified Launch Complex 39B until splash down of the rocket's booster stage nearly 150 miles down range.

"This is a huge step forward for NASA's exploration goals," said Doug Cooke, associate administrator for the Exploration Systems Mission Directorate at NASA Headquarters in Washington. "Ares I-X provides NASA with an enormous amount of data that will be used to improve the design and safety of the next generation of American spaceflight vehicles -- vehicles that could again take humans beyond low Earth orbit."

The 327-foot tall Ares I-X test vehicle produced 2.6 million pounds of thrust to accelerate the rocket to nearly 3 g's and Mach 4.76, just shy of hypersonic speed. It capped its easterly flight at a sub-orbital altitude of 150,000 feet after the separation of its first stage, a four-segment solid rocket booster.

Parachutes deployed for recovery of the booster and the solid rocket motor will be recovered at sea for later inspection. The simulated upper stage, Orion crew module, and launch abort system will not be recovered.

"The most valuable learning is through experience and observation," said Bob Ess, Ares I-X mission manager. "Tests such as this -- from paper to flight -- are vital in gaining a deeper understanding of the vehicle, from design to development."

Wednesday's flight offered an early opportunity to test and prove hardware, facilities, and ground operations - important data for future space vehicles. During the flight, a range of performance data was relayed to the ground and also stored in the onboard flight data recorder. The 700 sensors mounted on the vehicle provide flight test engineering data to correlate with computer models and analysis. The rocket's sensors gathered information in several areas, including assembly and launch operations, separation of the vehicle's first and second stages, controllability and aerodynamics, the re-entry and recovery of the first stage and new vehicle design techniques.

The Ares I-X efforts are led by the Ares I-X mission management office of the Constellation Program, based at NASA's Johnson Space Center in Houston, and NASA's Exploration Systems Mission Directorate in Washington. NASA's Glenn Research Center in Cleveland designed and built the vehicle's upper stage mass simulator. NASA's Langley Research Center in Hampton, Va., provided aerodynamic characterization, flight test vehicle integration and the crew module/launch abort system mass simulator. NASA's Marshall Space Flight Center in Huntsville, Ala., with contractor support, provided management for the development of Ares I-X avionics, roll control, and first stage systems. The Kennedy Space Center provided operations and associated ground activities and launch operations.

Contractors for Ares I-X include Alliant Techsystems, or ATK, of Salt Lake City for the first stage solid rocket booster and Teledyne Brown Engineering of Huntsville for the roll control system. Jacobs Engineering of Tullahoma, Tenn., supported by Lockheed Martin of Denver, provided the avionics systems. United Space Alliance of Houston and ATK Launch Systems support the ground systems and launch operations.

Hosting Destruction


This artist's concept illustrates the two types of spiral galaxies that populate our universe: those with plump middles, or central bulges (upper left), and those lacking the bulge (foreground).

New observations from NASA's Spitzer Space Telescope provide strong evidence that the slender, bulgeless galaxies can, like their chubbier counterparts, harbor supermassive black holes at their cores. Previously, astronomers thought that a galaxy without a bulge could not have a supermassive black hole. In this illustration, jets shooting away from the black holes are depicted as thin streams.

The findings are reshaping theories of galaxy formation, suggesting that a galaxy's "waistline" does not determine whether it will be home to a big black hole.

Friday, November 13, 2009

NASA finds water on the moon




WASHINGTON (AFP) – A "significant amount" of frozen water has been found on the moon, the US space agency said Friday heralding a giant leap forward in space exploration and boosting hopes of a permanent lunar base.

Preliminary data from a dramatic experiment on the moon "indicates the mission successfully uncovered water in a permanently shadowed lunar crater," NASA said in a statement.

"The discovery opens a new chapter in our understanding of the moon," it added, as ecstatic scientists celebrated the landmark discovery.

"Yes indeed we found water and we did not find only a little bit but a significant amount," said Anthony Colaprete, project scientist and principal investigator for the 79-million-dollar LCROSS mission.

The data was found after NASA sent two spacecraft crashing into the lunar surface last month in a dramatic experiment to probe Earth's nearest neighbor for water.

One rocket slammed into the Cabeus crater, near the lunar southern pole, at around 5,600 miles (9,000 kilometers) per hour.

Moon holds key to solar system's secrets

The rocket was followed four minutes later by a spacecraft equipped with cameras to record the impact which sent a huge plume of material billowing up from the bottom of the crater, untouched by sunlight for billions of years.

"In the 20 to 30 meter crater we found maybe about a dozen, at least, two-gallon buckets of water. This is an initial result," Colaprete told reporters.

"We are ecstatic," he added in a statement.

"Multiple lines of evidence show water was present in both the high angle vapor plume and the ejecta curtain created by the LCROSS Centaur impact.

"The concentration and distribution of water and other substances requires further analysis, but it is safe to say Cabeus holds water," Colaprete said.

Scientists had previously theorized that, except for the possibility of ice at the bottom of craters, the moon was totally dry.

Finding water on Earth's natural satellite is a major breakthrough in space exploration.

"It's very exciting, it is painting a new image of the moon," said Gregory Deloy, from the University of California hailing it as "an extraordinary discovery."

He theorized that "one of the possible source of water is a comet."

"We're unlocking the mysteries of our nearest neighbor and, by extension, the solar system," said Michael Wargo, chief lunar scientist at NASA headquarters in Washington.

"The full understanding of the LCROSS data may take some time. The data is that rich," Colaprete cautioned.

"Along with the water in Cabeus, there are hints of other intriguing substances. The permanently shadowed regions of the moon are truly cold traps, collecting and preserving material over billions of years."

Only 12 men, all Americans, have ever walked on the moon, and the last to set foot there were in 1972, at the end of the Apollo missions.

But NASA's ambitious plans to put US astronauts back on the moon by 2020 to establish manned lunar bases for further exploration to Mars under the Constellation project are increasingly in doubt.

NASA's budget is currently too small to pay for Constellation's Orion capsule, a more advanced and spacious version of the Apollo lunar module, as well as the Ares I and Ares V launchers needed to put the craft in orbit.

A key review panel appointed by President Barack Obama said existing budgets are not large enough to fund a return mission before 2020.


soucre : news.yahoo.com

Hosting Destruction


This artist's concept illustrates the two types of spiral galaxies that populate our universe: those with plump middles, or central bulges (upper left), and those lacking the bulge (foreground).

New observations from NASA's Spitzer Space Telescope provide strong evidence that the slender, bulgeless galaxies can, like their chubbier counterparts, harbor supermassive black holes at their cores. Previously, astronomers thought that a galaxy without a bulge could not have a supermassive black hole. In this illustration, jets shooting away from the black holes are depicted as thin streams.

The findings are reshaping theories of galaxy formation, suggesting that a galaxy's "waistline" does not determine whether it will be home to a big black hole.

Thursday, November 12, 2009

Skirting an Obstacle


This view from the navigation camera on NASA's Mars Exploration Rover Opportunity shows tracks left by backing out of a wind-formed ripple after the rover's wheels had started to dig too deeply into the dust and sand of the ripple.

The frames combined into this view were taken on the 1,867th Martian day, or sol, of Opportunity's mission on Mars (April 25, 2009). The scene spans 120 degrees, from southeastward on the left to westward on the right.

Two sols earlier, Opportunity drove 310 feet south-southwestward before stopping when the rover detected that its wheels were slipping more than the limit that engineers had set for the drive. That Sol 1865 (April 23, 2009) drive created the tracks that enter this scene from the left and ended with wheels on the left side of the rover partially embedded in the ripple. On Sol 1866, Opportunity began to back away from this potential trap, but moved only about 11 inches. On Sol 1867, the rover backed up 12 feet before taking this picture. Subsequently, Opportunity proceeded on a path avoiding the ripple where the wheel slippage occurred.

For scale, the distance between the parallel wheel tracks is about about 40 inches). This view is presented as a cylindrical projection with geometric seam correction.

International Space Station

In a project known as Butterflies in Space, the Atlantis space shuttle will next week carry a butterfly habitat containing monarch and painted lady adults and larvae to the International Space Station.

The idea is that thousands of schoolkids across the US will be able to study the effects of space travel on the little astronauts, comparing them with examples reared in their own classroms. The children will be able to monitor their progress via still and video images.

"One of the most exciting things about this project is that we can use the International Space Station to bring spaceflight experiments into classrooms around the country," said BioServe Director Louis Stodieck, principal investigator on the project. "Our continuing goal is to inspire K-12 students around the country in science, technology, engineering and math."

The butterfly payload has been designed and built by BioServe Space Technologies in CU-Boulder's aerospace engineering department and will carry two butterfly habitats containing monarch and painted lady butterfly larvae and enough nectar and other food to support them as they develop.

Wednesday, November 11, 2009

Atlantis space Station.

At NASA's Kennedy Space Center in Florida, technicians at Launch Pad 39A begin work today to get space shuttle Atlantis' propulsion systems ready for flight to the International Space Station.
The shuttle's three main engines, as well as the orbital maneuvering system and reaction control system, which will be used to steer Atlantis in space, will start being pressurized for flight.

Techs also will complete installation of sensors and microphones in Atlantis' aft section today for the acoustic environment testing. Final systems checks in the shuttle's aft section are complete.

The STS-129 astronauts will fly to Kennedy tomorrow in NASA's Shuttle Training Aircraft. Landing at the Shuttle Landing Facility is expected around 12 p.m. EST. NASA TV will air the crew's arrival live on the Web at www.nasa.gov/ntv.

The countdown to launch begins 1 p.m. Friday.

Liftoff of Atlantis' 11-day cargo mission to the space station is set for 2:28 p.m. EST Nov. 16.

Atlantis and Crew Prepare for Flight

The STS-129 mission will be commanded by Charles O. Hobaugh and piloted by Barry E. Wilmore. Mission Specialists are Robert L. Satcher Jr., Mike Foreman, Randy Bresnik and Leland Melvin. Wilmore, Satcher and Bresnik will be making their first trips to space.

Atlantis and its crew will deliver two control moment gyroscopes, equipment and EXPRESS Logistics Carrier 1 and 2 to the International Space Station. The mission will feature three spacewalks.

Atlantis also will return station crew member Nicole Stott to Earth and is slated to be the final space shuttle crew rotation flight.

Tuesday, November 10, 2009

Observatories Celebrate International Year of Astronomy

A never-before-seen view of the turbulent heart of our Milky Way galaxy is being unveiled by NASA on Nov. 10. This event will commemorate the 400 years since Galileo first turned his telescope to the heavens in 1609.

In celebration of this International Year of Astronomy, NASA is releasing images of the galactic center region as seen by its Great Observatories to more than 150 planetariums, museums, nature centers, libraries and schools across the country.

The sites will unveil a giant, 6-foot-by-3-foot print of the bustling hub of our galaxy that combines a near-infrared view from the Hubble Space Telescope, an infrared view from the Spitzer Space Telescope and an X-ray view from the Chandra X-ray Observatory into one multi-wavelength picture. Experts from all three observatories carefully assembled the final image from large mosaic photo surveys taken by each telescope. This composite image provides one of the most detailed views ever of our galaxy's mysterious core.

Participating institutions also will display a matched trio of Hubble, Spitzer and Chandra images of the Milky Way's center on a second large panel measuring 3 feet by 4 feet. Each image shows the telescope's different wavelength view of the galactic center region, illustrating not only the unique science each observatory conducts, but also how far astronomy has come since Galileo.

Monday, November 09, 2009

Kennedy Space Center Runway Than Shuttle Ops

Space shuttle Endeavour rolls down the Shuttle Landing Facility runway past the air traffic control tower. The tower is about 100 feet above the 3-mile-long runway and affords controllers working inside a clear view of the SLF and much of the Kennedy Space Center area. They also have radar and other technology to watch the airspace around the center


The Shuttle Landing Facility was the takeoff point for Steve Fossett's record-setting solo flight aboard the Virgin Atlantic GlobalFlyer.


Part of an air traffic controllers duties during launch and landing operations is coordinating the search-and-rescue teams and landing convoy that are on hand for potential shuttle work.


Air shows bring in the biggest variety of aircraft at once for the Shuttle Landing Facility. Here, an F-104 from Starfighters Inc., from bottom, two F-16s, an F-4 Phantom II and a pair of F-18s share the ramp at the SLF before a recent air show.

Since there is no weight limit on the SLF runway, it can host any aircraft in the world, no matter how big. Here, a European transport brings a module for the International Space Station so it can be processed and taken to the orbital laboratory by the space shuttle lear view of the SLF and much of the Kennedy Space Center area. They also have radar and other technology to watch the airspace around the center

Friday, November 06, 2009

Space Shuttle News

Less Than Two Weeks to Launch

At NASA's Kennedy Space Center in Florida, Launch Pad 39A technicians are loading space shuttle Atlantis' two, mass-memory units today. Located in the middeck's two avionics bays, each reel-to-reel digital magnetic tape storage device holds basic flight software for the shuttle's general purpose computers and can store additional data.

Preparations for final ordnance installations and connections at the pad will begin today and are expected to wrap up this weekend.

At NASA's Johnson Space Center in Houston, the STS-129 mission's six astronauts will be given their L-10 physicals today. They'll also practice integrated entry procedures in Johnson's motion base simulator.

The STS-129 mission will be commanded by Charles O. Hobaugh and piloted by Barry E. Wilmore. Mission Specialists are Robert L. Satcher Jr., Mike Foreman, Randy Bresnik and Leland Melvin. Wilmore, Satcher and Bresnik will be making their first trips to space.

Atlantis and its crew will deliver two control moment gyroscopes, equipment and EXPRESS Logistics Carrier 1 and 2 to the International Space Station. The mission will feature three spacewalks.

Atlantis also will return station crew member Nicole Stott to Earth and is slated to be the final space shuttle crew rotation flight.

Thursday, November 05, 2009

A Feel for Astronomy

The field of astronomy is very visual and can be challenging to teach to people who are visually impaired. For more than a decade, David Hurd has embraced this challenge as a space science professor at Edinboro University of Pennsylvania. Hurd and his wife Robin have worked through his university and with NASA to develop tactile, or textured, products that can be used in teaching about space to students who are visually impaired.

"So much of space is still so visual and so out of reach for them," Hurd said.

Hurd and tactile engineer John Matelock began creating tactile astronomy tools because a student with a visual impairment signed up for Hurd's introductory astronomy course. The course was primarily visual and auditory -- students used the university's planetarium, where Hurd pointed to and described what was there. Hurd and Matelock created a tactile star chart and a planisphere, which is used for determining the positions of the stars at a given time. Over the years Hurd has built a library of tactile charts, graphs and models.

Robin Hurd said it helped that her husband and Matelock shared a passion about astronomy. "I have a feeling John (Matelock) stayed up till midnight some nights making tactiles because he was so excited to be doing something astronomy-related," she said.

One of the Hurds' star products is a Tactile Guide to the Solar System. The guide is based on an earlier version that originated with NASA scientist Steve Dwornik and was developed by Ball Aerospace & Technologies Corp. and Cass Runyon, a professor at the College of Charleston in Charleston, S.C. The guide illustrates the comparative size and distance of the planets in the solar system. It also details the individual characteristics of each planet. The objects in the guide are not smooth, like a ball, but textured so students can understand that planets have unique surface features.

"One of our passions is to make these things feel like they look," said David. "The easy way to do tactile material is to outline it, make dots for sun spots or solar flares, but it really doesn't feel like it really looks. So we try to come up with creative ways to make our tactiles feel like the images look."

The Hurds used materials such as cork and sand to produce a three-dimensional mold, called a master, to make objects "feel as they look." For example, satellite pictures of the sun show the sun as fibrous and bubbly, Robin described. The Hurds created a sun out of Spanish moss to give it that fibrous, bubbly feel. "So that when you feel the sun, you actually perceive the texture and can relate it to the actual image of the sun. This helps 'viewers' realize it is not like a smooth ball," Robin said.

The Tactile Guide to the Solar System includes a CD with digital talking text. The CD works with text readers, which convert text to speech, and refreshable Braille technology, which converts text to Braille. The digital talking text allows users to access detailed information about each planet and NASA missions. The guide is part of the Lunar Nautics Toolkit, available through NASA's Central Operations of Resources for Educators, or CORE.

In addition to working with students with visual impairments at Edinboro University, Hurd has four sons, none of whom are blind but three of whom have other disabilities. The youngest two are identical twins with physical disabilities that affect their walking and speech. The Hurds' middle son has mild autism and problems with auditory processing, social cues and non-verbal signals. "On a personal level, our passion for meeting the needs of people with disabilities comes partially because of the learning differences we see in our own kids," Robin said.

The development of tactile materials is just another way of inspiring the next generation of explorers, David Hurd said. "The difference is we're inspiring explorers who were overlooked in the past, and that's what's really exciting about what we're doing."

Hurd and Matelock's early products were created through the university. Matelock has since retired from the university, and David and Robin Hurd now develop tactile products and teaching materials through AAC Core Concepts. AAC stands for Alternative and Augmentative Communication. The Tactile Guide to the Solar System was developed in cooperation with NASA in support of the agency's goal of engaging Americans in NASA's missions.

In May, David and Robin Hurd were invited to attend a NASA Education forum in conjunction with the launch of the STS-125 Hubble Servicing Mission. The STS-125 mission carried into space two Louis Braille Bicentennial Silver Dollar coins to recognize the critical role Braille plays in the pursuit of careers in math and science by the visually impaired. This commemorative coin, only available until Dec. 11, 2009, is the first U.S. coin to have readable Braille. As authorized by Congress, the United States Braille coin will fund efforts by the National Federation of the Blind to reverse the Braille literacy crisis in America. After Dec. 11, any unsold coins will be melted.

It was Hurd's first time to see a space shuttle launch in person. "Even though I'm in the fringe -- and most people are in the fringe when you go to something like that -- you feel like such a part," Hurd said about participating in the launch. "It takes everybody to make that happen, from the engineers to the astronauts themselves, from the business people to those involved with education and public outreach, from the school administration to the school teachers to the students.

"It was so neat to feel that kinship. Even though we couldn't be on board, we were part of that launch."

Space Shuttle Overview: Atlantis (OV-104)

NASA's fourth space-rated space shuttle, OV-104 "Atlantis," was named after the two-masted boat that served as the primary research vessel for the Woods Hole Oceanographic Institute in Massachusetts from 1930 to 1966. The boat had a 17-member crew and accommodated up to five scientists who worked in two onboard laboratories, examining water samples and marine life. The crew also used the first electronic sounding devices to map the ocean floor.


Construction of the orbiter Atlantis began on March 3, 1980. Thanks to lessons learned in the construction and testing of orbiters Enterprise, Columbia and Challenger, Atlantis was completed in about half the time in man-hours spent on Columbia. This is largely attributed to the use of large thermal protection blankets on the orbiter's upper body, rather than individual tiles requiring more attention.

Weighing in at 151,315 pounds when it rolled out of the assembly plant in Palmdale, Calif., Atlantis was nearly 3.5 tons lighter than Columbia. The new orbiter arrived at NASA's Kennedy Space Center in Florida on April 9, 1985, and over the next seven months was prepared for her maiden voyage.

Like her seafaring predecessor, orbiter Atlantis has carried on the spirit of exploration with several important missions of her own. On Oct. 3, 1985, Atlantis launched on her first space flight, STS-51-J, with a classified payload for the U.S. Department of Defense. The vehicle went on to carry four more DOD payloads on later missions.


Atlantis 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.

Construction Milestones - OV-104

Jan. 29, 1979 Contract Award
March 30, 1980 Start structural assembly of crew module
Nov. 23, 1981 Start structural assembly of aft-fuselage
June 13, 1983 Wings arrive at Palmdale from Grumman
Dec. 2, 1983 Start of Final Assembly
April 10, 1984 Completed final assembly
March 6, 1985 Rollout from Palmdale
April 3, 1985 Overland transport from Palmdale to Edwards
April 9, 1985 Delivery to Kennedy Space Center
Sept. 5, 1985 Flight Readiness Firing
Oct. 3, 1985 First Flight (STS-51-J)

Upgrades and Features

By early 2005, Atlantis had undergone two overhauls known as Orbiter Maintenance Down Periods. Some of the most significant upgrades and new features included:
  • Installation of the drag chute
  • New plumbing lines and electrical connections configuring the orbiter for extended duration missions
  • New insulation for the main landing gear doors
  • Improved nosewheel steering
  • Preparations for the Mir Orbiter Docking System unit later installed at Kennedy
  • Installation of the International Space Station airlock and Orbiter Docking System
  • Installation of the Multifunction Electronic Display System, or "glass cockpit"

Prelaunch Preps Continue at Kennedy and Johnson

Final system checks on space shuttle Atlantis' aft, or back, section continue on Launch Pad 39A at NASA's Kennedy Space Center today. Technicians also will install several cameras in the shuttle's payload bay.

Workers finished attaching the orbiter midbody umbilical unit from the pad's rotating service structure to the shuttle, and then leak checks were conducted and completed.

Atlantis' cargo, consisting of Express Logistics Carrier 1 and 2, holding about 28,000 pounds of supplies and spare parts for the International Space Station, were moved from the pad's changeout room into the shuttle's payload bay yesterday.

Meanwhile, at NASA's Johnson Space Center in Houston, the six STS-129 astronauts are participating in a final prelaunch meeting with the Mission Control Center's flight director team today, and they’ll also be reviewing final flight data.

Enceladus' Icy Surface


Cassini captured this raw image on its Nov. 02, 2009, flyby of Enceladus. The camera was pointing toward Enceladus from approximately 10,000 kilometers (6,000 miles) away.

This image has not been validated or calibrated. A validated/calibrated image will be archived with the NASA Planetary Data System in 2010.

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, D.C. 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.

Image Credit: NASA/JPL/Space Science Institute

Spring Bloom in New Zealand Waters



Off the east coast of New Zealand, cold rivers of water that have branched off from the Antarctic Circumpolar Current flow north past the South Island and converge with warmer waters flowing south past the North Island. The surface waters of this meeting place are New Zealand's most biologically productive. This image of the area on October 25, 2009, from the MODIS sensor on NASA’s Aqua satellite shows the basis for that productivity: large blooms of plantlike organisms called phytoplankton.

Phytoplankton use chlorophyll and other pigments to absorb sunlight for photosynthesis, and when they grow in large numbers, they change the way the ocean surface reflects sunlight. Caught up in eddies and currents, the blooms create intricate patterns of blues and greens that spread across thousands of square kilometers of the sea surface.

Especially bright blue areas may indicate the presence of phytoplankton called coccolithophores, which are coated with calcium-carbonate (chalk) scales that are very reflective. The duller greenish-brown areas of the bloom may be diatoms, which have a silica-based covering.

In addition to their importance as the foundation of the ocean food web, phytoplankton play a key role in the climate because, like plants on land, they absorb carbon dioxide from the atmosphere. When they die, they sink to the ocean floor where the carbon they took from the atmosphere is stored for thousands of years.

X-38 Crew Return Vehicle Finds New Home



One of NASA's three X-38 Crew Return Vehicle technology demonstrators that flew at NASA's Dryden Flight Research Center at Edwards Air Force Base, Calif., a decade ago has found a new home in America's heartland.

In this image from test flights in 1999, the X-38 research vehicle drops away from NASA's B-52 mothership immediately after being released from the B-52's wing pylon. More than 30 years earlier, this same B-52 launched the original lifting-body vehicles flight tested by NASA and the Air Force at what is now called the Dryden Flight Research Center and the Air Force Flight Test Center.

The wingless lifting body craft was transferred this past weekend from NASA's Johnson Space Center in Houston to the Strategic Air and Space Museum, located just off Interstate 80 at Ashland, Neb., about 20 miles southeast of Omaha. The X-38 adds to the museum's growing collection of aerospace vehicles and other historical artifacts.

The move of the second X-38 built to the museum has a fitting connection, as the X-38 vehicles were air-launched from NASA's famous B-52B 008 mothership. The B-52 bomber served as the backbone of the Air Force's Strategic Air Command during the command's history.

Prior to cancellation, the X-38 program was developing the technology for proposed vehicles that could return up to seven International Space Station crewmembers to Earth in case of an emergency. These vehicles would have been carried to the space station in the cargo bay of a space shuttle and attached to station docking ports. If an emergency arose that forced the ISS crew to leave the space station, a Crew Return Vehicle would have undocked and returned them to Earth much like the space shuttle, although the vehicle would have deployed a parafoil for the final descent and landing.