The name Aieeda is a baby boy name.

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Muslim Meaning:
The name Aieeda is a Muslim baby name. In Muslim the meaning of the name Aieeda is:

SoulUrge Number: 3

People with this name have a deep inner desire to create and express themselves, often in public speaking, acting, writing or singing. They also yearn to have beauty around them in their home and work environment.

Expression Number: 7

People with this name are excellent at analyzing, understanding, and learning. They tend to be mystics, philosophers, scholars, and teachers. Because they live so much in the mind, they tend to be quiet and introspective, and are usually introverts. When presented with issues, they will see the larger picture. Their solitary thoughtfulness and analysis of people and world events may make them seem aloof, and sometimes even melancholy.


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Posted: July 25, 2007T-00:00LiftoffThe ULA Delta 2 rocket's main engine and twin vernier steering thrusters are started moments before launch. The six ground-start strap-on solid rocket motors are ignited at T-0 to begin the mission.T+01:03.1Ground SRM BurnoutThe six ground-start Alliant TechSystems-built solid rocket motors consume all their propellant and burn out.T+01:05.5Air-Lit SRM IgnitionThe three remaining solid rocket motors strapped to the Delta 2 rocket's first stage are ignited.T+01:06.0Jettison Ground SRMsThe six spent ground-started solid rocket boosters are jettisoned in sets of three to fall into the Atlantic Ocean.T+02:11.5Jettison Air-Lit SRMsHaving burned out, the three spent air-started solid rocket boosters are jettisoned toward the Atlantic Ocean.T+04:23.3Main Engine CutoffAfter consuming its RP-1 fuel and liquid oxygen, the Rocketdyne RS-27A first stage main engine is shut down. The vernier engines cut off moments later.T+04:31.3Stage SeparationThe Delta rocket's first stage is separated now, having completed its job. The spent stage will fall into the Atlantic Ocean.T+04:36.8Second Stage IgnitionWith the stage jettisoned, the rocket's second stage takes over. The Aerojet AJ10-118K liquid-fueled engine ignites for the first of its two firings to boost the Phoenix spacecraft.T+05:03.0Jettison Payload FairingThe 9.5-foot diameter payload fairing that protected the Phoenix spacecraft atop the Delta 2 during the atmospheric ascent is jettisoned is two halves.T+09:20.5Second Stage Cutoff 1The second stage engine shuts down to complete its first firing of the launch after reaching an 86.4 by 96.5 nautical mile orbit at 28.5 degrees inclination. The rocket and attached spacecraft are now in a coast period before the second stage reignites.T+73:47.2Second Stage RestartDelta's second stage engine reignites for a firing that accelerates the payload further.T+76:02.3Second Stage Cutoff 2The stage shuts down to complete its second burn having reached an 87.7 by 3,128.1 nautical mile orbit at 28.5 degrees inclination. Over the next minute, tiny thrusters on the side of the rocket will be fired to spin up the vehicle in preparation for stage separation.T+77:05.5Stage SeparationThe liquid-fueled second stage is jettisoned from the rest of the Delta 2 rocket.T+77:42.8Third Stage IgnitionThe Thiokol Star 48B solid-fueled third stage is ignited to propel Phoenix on its departure trajectory from Earth.T+79:10.3Third Stage BurnoutHaving used up all its solid-propellant, the third stage burns out to completed the powered phase of the launch sequence for Phoenix.T+84:10.3Phoenix SeparationNASA's Phoenix spacecraft is released from the third stage to begin the nine-month cruise to the Red Planet.Data source: ULAFinal Shuttle Mission PatchFree shipping to U.S. addresses!The crew emblem for the final space shuttle mission is now available in our store. Get this piece of history!STS-134 PatchFree shipping to U.S. addresses!The final planned flight of space shuttle Endeavour is symbolized in the official embroidered crew patch for STS-134. Available in our store!Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Project OrionThe Orion crew exploration vehicle is NASA's first new human spacecraft developed since the space shuttle a quarter-century earlier. The capsule is one of the key elements of returning astronauts to the Moon.Fallen Heroes Patch CollectionThe official patches from Apollo 1, the shuttle Challenger and Columbia crews are available in the store. | | | | 2014 Spaceflight Now Inc.Phoenix science instrumentsFROM NASA PRESS KITThe Phoenix Mars Lander carries seven science instruments, three of which are suites of multipletools.The Robotic Arm will allow Phoenix to explore vertically and to use instruments on thespacecraft deck to analyze samples of Martian soil and ice. The arm will dig trenches, positionsome arm-mounted tools for studying the soil in place, and deliver scooped-up samples toother instruments.The aluminum and titanium arm is 2.35 meters (7.7 feet) long. One end is attached to thelander's deck. An elbow joint is in the middle. The other end has a scoop with blades for digginginto the soil and a powered rasp for breaking up frozen soil. The arm moves like a backhoe,using four types of motion: up-and-down, side-to-side, back-and-forth and rotating.The arm can reach far enough to dig about half a meter (20 inches) deep. However, the subsurfaceice layer expected at the landing site may not lie that deep. Once the arm reaches theicy-soil layer, the powered rasp will be used to acquire samples.Because the arm will be making direct contact with icy soil that is conceivably a habitat wheremicrobes could survive, extra precaution has been taken with it to prevent introducing life fromEarth. Before the arm was given a sterilizing heat treatment in March 2007, it was enclosedin a biological barrier wrap. This barrier is keeping microbes off the arm during the subsequentmonths before launch. It will not open until after Phoenix has landed on Mars.The robotic arm uses design work for a similar arm flown on the 1999 Mars Polar Lander mission,with refinements including enhanced capability for collecting an icy sample.A team led by Robert Bonitz at NASA's Jet Propulsion Laboratory, Pasadena, Calif., engineeredand tested the Phoenix Robotic Arm. Alliance Spacesystems Inc., Pasadena, built it.Ray Arvidson of Washington University in St. Louis is the lead scientist for this instrument.The Robotic Arm Camera rides fastened to the arm just above the scoop. It will providecloseup color images of Martian soil at the landing site, of the floor and walls of trenches dugby the arm, and of soil and ice samples before and after they are in the scoop.Information the camera reveals about soil textures will aid in selecting what to pick up assamples for analysis. Observations of trench walls will determine whether they show fine-scalelayering, which could result from changes in the Martian climate.The camera has a double Gauss lens system, a design commonly used in 35-millimeter cameras.Images are recorded by a charge-coupled device (CCD) similar to those in consumer digitalcameras. The instrument includes sets of red, green and blue light-emitting diodes (LEDs)for illuminating the target area.The focus can be adjusted by a motor, which is a first for a camera on an interplanetary spacecraft. The focus can be set as close as about 11 millimeters (half an inch) and out to infinity.With a resolution of 23 microns per pixel at the closest focus, this camera can show detailsmuch finer than the width of a human hair.A team led by H. Uwe Keller at the Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, and by Peter Smith at the University of Arizona originally built this camerafor the Mars Surveyor 2001 Lander mission, which was canceled in 2000. It is similar to acamera on the robotic arm of the unsuccessful Mars Polar Lander spacecraft, though with animproved illumination system. For the Phoenix Robotic Arm Camera, Keller is the lead scientistand Chris Shinohara of the University of Arizona is the lead engineer.The Surface Stereoscopic Imager will record panoramic views of the surroundings fromatop a mast on the lander. Its images from two cameras situated about as far apart as a pair ofhuman eyes will provide three-dimensional information that the Phoenix team will use in choosingwhere to dig and in operating the robotic arm.A choice of 12 different filters for each eye enables the instrument to produce images not onlyin full color, but in a several specific visual and infrared frequencies useful for interpreting geological and atmospheric properties. The multispectral and three-dimensional information willhelp scientists understand the geology of the landing area.The twin cameras will be able to look in all directions from a perch about 2 meters (7 feet)above Martian ground level. They will see with about the same resolution as human eyes,capturing each view onto 1-megapixel charge-coupled devices (a 1,024-by-1,024-pixel CCDfor each eye).The instrument will sometimes point upward to assess how much dust and water vapor is inthe atmosphere. When the robotic arm delivers soil and ice samples to deck-mounted instruments,the Surface Stereoscopic Imager will be able to look downward to inspect the samples.Views of the spacecraft's deck will also monitor dust accumulation, which is of scientific interestfor inferences about Martian winds and of engineering interest for effects of the dust buildupon solar panels.A University of Arizona team led by Chris Shinohara built the Phoenix Surface StereoscopicImager. Mark Lemmon of Texas A&M University, College Station, is lead scientist for this camera.The instrument closely resembles a stereo imager on Mars Polar Lander, which in turnused design features from the imager on Mars Pathfinder, which provided stereo views fromthe surface of Mars in July 1997.The Thermal and Evolved-Gas Analyzer will study substances that are converted to gasesby heating samples delivered to the instrument by the robotic arm. It provides two types of information.One of its tools, called a differential scanning calorimeter, monitors how much poweris required to increase the temperature of the sample at a constant rate. This reveals whichtemperatures are the transition points from solid to liquid to gas for ingredients in the sample.The gases that are released, or "evolved," by this heating then go to a mass spectrometer, atool that can identify the chemicals and measure their composition.The mass spectrometer will determine whether the samples of soil and ice contain any organiccompounds. It would be used to identify the types and amounts if any are present. Finding anywould be an important result for interpreting the habitability of the site.The instrument will also give information about water and carbon dioxide present as ices orbound to minerals. The amount of heat needed to drive off water or carbon dioxide that isbound to minerals is characteristically different for different minerals. The calorimeter's information from that process can help identify minerals in the soil, including carbonates if they are present.The mass spectrometer will measure the ratios of different isotopes of carbon, oxygen, hydrogen,argon and some other elements in the Martian samples. Isotopes are alternate forms ofthe same element with different atomic weights due to different numbers of neutrons. Ratioscan be changed by the effects of long-term processes that act preferentially on lighter or heavierisotopes of the same element. For example, some of Mars' original water was lost from theplanet by processes at the top of the atmosphere, favoring the removal of lighter isotopes ofhydrogen and oxygen and leaving modern Mars water with a raised ratio of heavier isotopes.The instrument has eight tiny ovens for samples, each to be used only once. The ovens areabout 1 centimeter (about half an inch) long and 2 millimeters (one-eighth inch) in diameter.At the start of an analysis, sample material is dropped into the oven through a screen. Theoven closes after a light-beam detector senses that it is full. The experiment gradually heatssamples to temperatures as high as 1,000 degrees Celsius (1,800 degrees Fahrenheit).Theheating process drives off water and any other volatile ingredients as a stream of gases. Thosegases are directed to the mass spectrometer.One of the samples that the instrument will analyze will be a special material that the landercarries from Earth, specially prepared to be as free of carbon as possible. This will serve asan experimental control as the instrument analyzes samples excavated at Mars. The controlmaterial is made of a machinable glass ceramic substance named Macor, from Corning Inc.The arm will scrape some of it up and deliver it to the analyzer to get a reading showing howwell the experiment can eliminate carbon carried from Earth. Carbon detected in assessmentsof Martian samples might be unavoidable traces of Earth carbon if the readings are no higherthan the amount in this control sample.The mass spectrometer part of the analyzer will examine samples of atmosphere at the landingsite, in addition to the evolved gases from scooped-up samples. The atmospheric measurementswill add information about humidity to the weather data monitored by the spacecraft'sMeteorological Station.The Thermal and Evolved-Gas Analyzer was built by teams at the University of Arizona, ledby William Boynton (science lead) and Heather Enos (project manager), and at the Universityof Texas, Dallas, led by John Hoffman. It is adapted from a similar instrument with the samename that flew on the Mars Polar Lander mission in 1999.The Microscopy, Electrochemistry and Conductivity Analyzer will use four tools to examinesoil. It will assess characteristics that a gardener or farmer would learn from a soil test,plus several more. Three of the tools will analyze samples of soil scooped and delivered bythe robotic arm -- a wet chemistry laboratory and two types of microscopes. The fourth tool ismounted near the end of the arm, and has a row of four small spikes that the arm will push intothe ground to examine electrical conductivity and other properties of the soil.The wet chemistry laboratory has four teacup-size beakers. Each will be used only once.Samples from Mars' surface and three lower depths may be analyzed and compared. Theinstrument will study soluble chemicals in the soil by mixing water with the sample to a soupyconsistency and keeping it warm enough to remain liquid during the analysis.On the inner surfaces of each beaker are 26 sensors, mostly electrodes behind selectively permeablemembranes or gels. Some sensors will give information about the pH of the soil -- thedegree to which it is acidic or alkaline. Soil pH is an important factor in what types of chemicalreactions, or perhaps what types of microbes, a soil habitat would favor, and it is has neverbeen measured on Mars. Other sensors will gauge concentrations of such ions as chlorides,bromides, magnesium, calcium and potassium, which form soluble salts in soil, and will recordthe level of the sample's oxidizing potential. One chemically important ion in soil, sulfate,cannot be directly sensed, so the analysis of each sample will end with a special process thatdetermines the amount of sulfate by observing its reaction with barium. Comparisons of theconcentrations of water-soluble ions in samples from different depths may provide clues to thehistory of water in the soil.The wet chemistry setup has a built-in robotic laboratory technician that adds potions to eachbeaker in a choreographed two-day sequence. Before each soil sample goes in, about 25cubic centimeters (nearly two tablespoons) of ice with dilute concentrations of several ionsis slowly melted in a special container, a process that takes one to two hours. After the wateris released into the beaker, the sensors make baseline measurements at this starting point.The first of five pill-size crucibles of prepared chemicals is then added to increase ion concentrationsby a known amount in order to calibrate the measurements. Next, a drawer abovethe beaker extends to receive the soil sample, and the scoop on the robotic arm drops up toone cubic centimeter (one-fifth of a teaspoon) of soil into the drawer, which then retracts anddumps the sample into the beaker. A paddle stirs the soup for hours while the sensors takemeasurements. The next day, the second crucible adds nitrobenzoic acid to the beaker to testhow ions from the soil react to increased acidity. The last three crucibles hold barium chloride.As they are added, one at a time, any sulfate from the soil reacts with the barium to make aninsoluble compound, taking both the barium and the sulfate out of solution. The amount of sulfatein the soil sample is determined by measuring the amount of unreacted barium left behind.The "microscopy" part of the Microscopy, Electrochemistry and Conductivity Analyzer will examinesoil particles and possibly ice particles with both an optical microscope and an atomicforce microscope. The robotic arm delivers soil samples to a wheel that rotates to presentthe samples to the microscopes. Along the perimeter of the wheel are substrates with differenttypes of surfaces, such as magnets and sticky silicone. This allows the experiment to getinformation from the particles' interaction with the various surfaces, as well as from the sizes,shapes and colors of the particles themselves.The biggest particles the optical microscope can view are about as long across as the thicknessof a dime, just over a millimeter. The smallest it can see are about 500 times smaller -- about 2 microns across. That would be the smallest scale ever seen on Mars, except thatthe atomic force microscope will image details down to another 20 times smaller than that -- assmall as about 100 nanometers, one one-hundredth the width of a human hair.The optical microscope obtains color information by illuminating the sample with any combinationof four different light sources. The illumination comes from 12 light-emitting diodes shiningin red, blue, green or ultraviolet parts of the spectrum. The atomic force microscope assemblesan image of the surface shape of a particle by sensing it with a sharp tip at the end of a spring,which has a strain gauge indicating how far the spring flexes to follow the contour of the surface.The process is like a much smaller version of a phonograph needle tracking the bumpinessinside the groove of a vinyl record.The shapes and the size distributions of soil particles may tell scientists about environmentalconditions the material has experienced. Tumbling rounds the edges. Repeated wetting andfreezing causes cracking. Clay minerals formed during long exposure to water have distinctive,plate-shaped particle shapes.The "conductivity" part of the Microscopy, Electrochemistry and Conductivity Analyzer will assesshow heat and electricity move through the soil from one spike to another of a four-spikeelectronic fork that will be pushed into the soil at different stages of digging by the arm. Forexample, a pulse of heat will be put onto one spike, and the rate at which the temperature riseson the nearby spike will be recorded, along with the rate at which the heated needle cools off.A little bit of ice in the soil can make a big difference in how well the soil conducts heat. Similarly, soil's electrical conductivity is a sensitive indicator of moisture in the soil. Soil moisture may have subtle stages intermediate between frozen solid and liquid, including warm ice andwater films, which may be biologically available. The device, called the thermal and electricalconductivity probe, adapts technology used in commercial soil-moisture gauges for irrigationcontrol systems.The conductivity probe has an additional role besides soil analysis. It will serve as a humiditysensor when held in the air. Also, slight temperature changes from one spike to the next canallow it to estimate wind speed.The Microscopy, Electrochemistry and Conductivity Analyzer is based on an instrument developedfor the Mars Surveyor 2001 Lander mission, which was canceled in 2000. The instrumentfor Phoenix inherited many of the original electronic and structural components. The conductivityprobe and other improvements have been added to the earlier design.A team led by Michael Hecht at NASA's Jet Propulsion Laboratory, Pasadena, Calif., designedand built the analyzer. A consortium led by Urs Staufer of the University of Neuchatel, Switzerland,provided the atomic force microscope. The University of Arizona provided the opticalmicroscope, equipped with an electronic detector (the same as in the Robotic Arm Camera)from the Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany. JohnMarshall of the SETI Institute, Mountain View, Calif., is lead scientist for the optical microscope.Transfer Engineering and Manufacturing Inc., Fremont, Calif. (formerly Surface/Interface Inc.of Mountain View, Calif.) designed the sample wheel for the microscopes. Aaron Zent of NASAAmes Research Center, Moffett Field, Calif., is science lead for the thermal and electrical conductivity probe, built by Decagon Devices Inc., Pullman, Wash. For the wet chemistry experiment,Thermo Fisher Scientific (formerly the Water Analysis Division of Thermo Corp., Beverly,Mass.) provided the chemical beakers; Starsys Research Corp., Boulder, Colo. provided thechemistry actuator assemblies and Tufts University, Medford, Mass., prepared the crucibles ofreagents for mixing with the soil samples. Sam Kounaves of Tufts is lead scientist for the wetchemistry investigation.The Meteorological Station will track daily weather and seasonal changes using temperatureand pressure sensors plus a laser-reflection instrument. The information collected by thisfirst high-latitude weather station on Mars will aid understanding of how water is cycled seasonallybetween ice on the ground and vapor in the atmosphere.The laser tool, called a lidar for "light detection and ranging," uses powerful laser pulses ina way comparable to radio pulses emitted by a radar instrument. The laser beam is emittedvertically into the atmosphere. Atmospheric dust and ice particles in the beam's path reflect thelight, sending it in all directions, including straight downward. A telescope integrated into theinstrument detects the downward-reflected light. Analysis of the strength and time-delay of thereflections reveals information about the sizes and altitudes of the particles. Tracking changesin these atmospheric particles' abundances and locations over time will help researchers studyhow clouds and dust plumes form and move.The weather station includes a 1.2-meter (4-foot) mast bearing sensors at three heights tomonitor how temperature varies with height near the surface. The temperature sensors arethin-wire thermocouples; they measure temperature by its effect on the flow of an electricalcurrent through a closed circuit of two metals with different thermal properties. The thermocouplesuse the metals chromel (a nickel and chromium alloy) and constantan (a copper andnickel alloy). Also, hanging from the top of the mast is a wind telltale. This is a small tube thatwill be deflected by the wind. The science payload's stereo camera will record images of thetelltale that will be used to determine wind direction and speed. The top of the meteorologymast, at 1.14 meters (3.75 feet) above the deck, is the highest point on the lander.The Canadian Space Agency provided the Meteorological Station for Phoenix. Jim Whitewayof York University, Toronto, Ontario, leads the Canadian science team. The instrument constructionwas led by the Space Missions Group of MDA Ltd., Brampton, Ontario, with contributionsfrom Optech Inc., Toronto, for the lidar. The Finnish Meteorological Institute provided theinstrument for measuring atmospheric pressure. Aarhus University, Denmark, constructed thewind telltale.The Mars Descent Imager will take a downward-looking picture during the final momentsbefore the spacecraft lands on Mars. This image will provide a bridge between orbiter-scaleand lander-scale images. It is expected to show geological context helpful for planning thelander's activities and for interpreting other science instruments' observations and measurements.Conditions at the landing site have different implications if the site appears to be typicalof a much broader area than if the site happens to be an unusual patch of ground unlike itssurroundings.This camera is mounted on the outer edge of the payload deck of the lander. It was designedto take several images, but the plan was altered to just one image after testing showed that adata-handling component elsewhere on the lander had a small possibility of triggering loss ofsome vital engineering data if it receives imaging data during a critical phase of final descent.The timing of the image will be planned to yield higher resolution of the landing area than currentlypossible from orbit.The imager weighs just 480 grams (1 pound). The optics provide a field of view of 75.3 degrees.Exposure time is 4 milliseconds.. At that speed, some blurring may occur as the descentengines vibrate the spacecraft while the camera takes its image.Future spacecraft to the surface of Mars may need capability for steering themselves to avoidhazards or to reach specific landing sites. Descent imaging could be an important componentof the technology for accomplishing that.A tiny microphone is riding on the descent camera. It might catch sounds around the spacecraftwhile the camera is taking its image. There are no plans to power the camera to takepictures or to record sounds after the landing.The Mars Descent Imager that will fly on Phoenix was originally built for the Mars Surveyor2001 Lander mission, by a team led by Michael Malin at Malin Space Science Systems, SanDiego. A similar camera flew on Mars Polar Lander.Research StrategyThe planned operational life of the Phoenix Mars lander after it reaches Mars is 90 Martiandays. Each Martian day, often called a "sol," lasts about 40 minutes longer than an Earth day.That gives the Phoenix team three months to use the lander's instruments to address the waterand habitat questions of the mission's science objectives. Planning and practice simulationsbefore landing will prepare the team to make the best possible advantage of that time.Observations made by orbiter spacecraft during the evaluation of candidate landing sites forPhoenix provide a starting-point base of knowledge about the area. After Phoenix has landed,views from the Surface Stereoscopic Imager, with added context from the Mars Descent Cameraand closer looks with the Robotic Arm Camera, will be used for choosing where to collectthe first soil sample for analysis.The first samples fed into the lander's analyzers will come from the surface. Decisions abouthow much deeper to go before analyzing another sample will depend on results from thesurface material and on what the robotic arm camera and stereo imager see in the soil. TheThermal and Evolved-Gas Analyzer can check for organics and other volatiles in up to eightsamples. Researchers must be choosier with samples for the wet chemistry laboratory of theMicroscopy, Electrochemistry and Conductivity Analyzer, which can examine four differentsamples. The microscopes and conductivity probe can analyze soil more frequently during the90 sols. Meanwhile, the weather station and stereo imager will monitor changes in water anddust in the atmosphere throughout the mission. If the spacecraft remains functional longer thanthe 90-day prime mission, weather information might be collected during the approach of thenorthern hemisphere autumn on Mars, when dwindling sunlight will eventually make operationsimpossible, and buildup of carbon-dioxide frost will coat the spacecraft.What types of findings would help answer questions about the history of water? If the microscopesfind fine silty sediments or clay textures, that would be evidence supporting the hypothesisthat the northern highlands of Mars once held an ocean. The presence of carbonatesor other minerals that form in liquid water would be another. Rounded sand grains in the soilcould suggest a history of flowing water.The mass spectrometer will measure isotopic ratios. If there are differences between thoseratios in subsurface ice and in atmospheric water, that could suggest the subsurface ice is ancient.A gradient in the concentrations of salts at different depths in the soil would support thehypothesis that climate cycles periodically thaw some subsurface ice. The conductivity probe'sfindings about thermal properties of the soil, combined with determination of the depth to an icylayer, could strengthen estimates for how much change in climate would be needed to melt theice. The same ground-truth information will refine models of the ice's depth and of atmosphereiceinteractions in widespread areas of Mars that contain subsurface ice.Using the microscopes and arm camera to learn about how porous and layered the soil iswill help assess whether liquid water has come and gone. The conductivity probe will assesswhether, even today, the soil may have thin films of unfrozen water. Atmospheric measurementsas the season progresses through the Martian summer will aid the understanding ofhow water is seasonally cycled between solid and gas phases in the current Martian climate.What types of findings would help answer questions about whether this site could formerly orstill support microbial life? Three important factors in the suitability of a habitat for life are the availability of liquid water, the presence of carbon and access to energy. So evidence about thehistory of water will be one part of evaluating the habitat.The Thermal and Evolved-Gas Analyzer has the dramatic job of checking for organic carbonmolecules layer by layer as samples come from farther below the surface. Soluble sulfate mineralswould be a possible source of energy that could sustain life. The wet chemistry lab of theMicroscopy, Electrochemistry and Conductivity Analyzer can identify potential chemical-energysources if they are present in soil samples. While the science payload of Phoenix is not designedfor life detection, this mission is an important stepping stone in the search for whetherMars has life. Orbital observations indicate that areas with shallow subsurface ice make up atleast a quarter of the red globe. Phoenix will be the first mission to visit such a site. Its findings about habitability could guide where a future spacecraft searching for life is sent.Researchers have equipped Phoenix to look for answers to many questions posed in advanceabout water and habitat. However, if previous interplanetary missions are an indicator, some ofthe most important results from Phoenix may be surprises that raise new questions.John Glenn Mission PatchFree shipping to U.S. addresses!The historic first orbital flight by an American is marked by this commemorative patch for John Glenn and Friendship 7.Final Shuttle Mission PatchFree shipping to U.S. addresses!The crew emblem for the final space shuttle mission is available in our store. Get this piece of history!Celebrate the shuttle programFree shipping to U.S. addresses!This special commemorative patch marks the retirement of NASA's Space Shuttle Program. Available in our store!Anniversary Shuttle PatchFree shipping to U.S. addresses!This embroidered patch commemorates the 30th anniversary of the Space Shuttle Program. The design features the space shuttle Columbia's historic maiden flight of April 12, 1981.Mercury anniversaryFree shipping to U.S. addresses!Celebrate the 50th anniversary of Alan Shephard's historic Mercury mission with this collectors' item, the official commemorative embroidered patch.Fallen Heroes Patch CollectionThe official patches from Apollo 1, the shuttle Challenger and Columbia crews are available in the store. | | | | 2014 Spaceflight Now Inc.Phoenix science investigationsFROM NASA PRESS KITThe Phoenix Mars Lander will investigate a site in the far north of Mars to answer questionsabout that part of Mars, and to help resolve broader questions about the planet. The mainquestions concern water and conditions that could support life.The landing region has water ice in soil close to the surface, which NASA's Mars Odysseyorbiter found to be the case for much of the high-latitude terrain in both the north and southhemispheres of Mars.Phoenix will dig down to the icy layer. It will examine soil in place at the surface, at the icy layer and in between, and it will scoop up samples for analysis by its onboard instruments. One keyinstrument will check for water and carbon-containing compounds by heating soil samples intiny ovens and examining the vapors that are given off. Another will test soil samples by addingwater and analyzing the dissolution products. Cameras and microscopes will provide informationon scales spanning 10 powers of 10, from features that could fit by the hundreds into theperiod at the end of this sentence to an aerial view taken during descent. A weather station willprovide information about atmospheric processes in an arctic region where a coating of carbon-dioxide ice comes and goes with the seasons.Mars is a vast desert where water is not found in liquid form on the surface, even in placeswhere mid-day temperatures exceed the melting point of ice. One exception may be fleetingoutbreaks that have been proposed to explain modern-day flows down some Martian gullies.Today's arid surface is not the whole story, though. Previous Mars missions have found thatliquid water has persisted at times in Mars' past and that water ice near the surface remainsplentiful today.Water is a key to four of the most critical questions about Mars: Has Mars ever had life? Howshould humans prepare for exploring Mars? What can Mars teach us about climate change?How do geological processes differ on Mars and on Earth? Water is a prerequisite for life, apotential resource for human explorers and a major agent of climate and geology. That's whyNASA has pursued a strategy of "follow the water" for investigating Mars. Orbiters and surfacemissions in recent years have provided many discoveries about the history and distribution ofwater on Mars -- such as minerals that formed in wet environments long ago and liquid flowsthat are still active today in hillside gullies.The landing site and onboard toolkit of Phoenix position this mission to follow the water further.The mission's three main science objectives are:1. Study the history of water in all its phases.On a time scale of billions of years, ice near the surface where Phoenix will land might be theremnant of an ancient northern sea. Several types of evidence point to plentiful liquid water onancient Mars, and the northern hemisphere is low and smooth compared to the southern hemisphere.Much of the water that could have remained liquid when ancient Mars had a thickeratmosphere may now be underground ice.On a time scale of tens of thousands to a few million years, ice near the surface where Phoenixlands might periodically thaw during warmer periods of climate cycles. The tilt of Mars' axis wobbles more than Earth's, and the shape of Mars' orbit also cycles over time, from rounderto more elongated. Currently, Mars is about 20 percent farther from the sun during northernsummer than during northern winter, so the summers are relatively cool in the north. As theorbit varies, the northern ice cap will enjoy warm winters on a 50,000-year cycle. The wobbleof Mars' axis may also cause the climate to change on a time scale of 100,000 to millions ofyears.On much shorter time scales, the arctic ground "breathes" every day and every season, convertingtiny amounts of ice into water vapor on summer days and condensing tiny amounts offrost from the atmosphere at night or in winter. In this way, the ice table slowly rises and recedesas the climate changes.Phoenix will collect information relevant for understanding processes affecting water at allthese time scales, from the planet's distant past to its daily weather.2. Determine if the Martian arctic soil could support life.Life as we know it requires liquid water, but not necessarily its continuous presence. Phoenixwill investigate a hypothesis that some ice in the soil of the landing site may become unfrozenand biologically available at times during the warmer parts of long-period climate cycles. Lifemight persist in some type of dormant microbial form for millions of years between thaws, ifother conditions were right.The spacecraft is not equipped to detect past or present life. However, in addition to studyingthe status and history of water at the site, Phoenix will look for other conditions favorable to life.One condition considered essential for life as we know it is the presence of molecules thatinclude carbon and hydrogen. These are known as organic compounds, whether they comefrom biological sources or not. They include the chemical building blocks of life, as well as substances that can serve as an energy source, or food, for life. Phoenix would be able to detecteven very small amounts and identify them. Two Viking spacecraft that NASA landed on Marsin 1976 made the only previous tests for organic compounds in Martian soil, and they foundnone. Conditions at the surface may be harsh enough to break organic molecules apart andoxidize any carbon into carbon dioxide. Phoenix will assess some factors in those oxidizingconditions, and it will check for organic chemicals below the surface, as well as in the top layeranic chemicals would persist better in icy material sheltered from sunshine than in surfacesoil exposed to harsh ultraviolet radiation from the sun.Phoenix will also be checking for other possible raw ingredients for life. It will examine howsalty and how acidic or alkaline the environment is in samples from different layers. It will assessother types of chemicals, such as sulfates, that could be an energy source for microbes.3. Study Martian weather from a polar perspective.In Mars' polar regions, the amount of water vapor in the thin atmosphere -- the humidity -- variessignificantly from season to season. Winds carrying water vapor can move water fromplace to place on the planet. The current understanding of these processes is based on observationsfrom orbit and limited meteorological observations from earlier Mars landers closer tothe equator. Phoenix will use an assortment of tools to directly monitor several weather variablesin the lower atmosphere at an arctic site.Phoenix will measure temperatures at ground level and three other heights to about 2 meters(7 feet) above ground. It will check the pressure, humidity and composition of the atmosphereat the surface. And it will identify the amounts, altitudes and movements of clouds and dust inthe sky above.Over the course of the mission, this unprecedented combination of Martian meteorologicalmeasurements will help researchers evaluate correlations such as whether southbound windscarry more humidity than northbound winds; whether drops in air pressure are associated withincreased dust; and how the amount of water vapor at the bottom of the atmosphere changesfrom late spring to mid-summer or later.STS-134 PatchFree shipping to U.S. addresses!The final planned flight of space shuttle Endeavour is symbolized in the official embroidered crew patch for STS-134. Available in our store!Final Shuttle Mission PatchFree shipping to U.S. addresses!The crew emblem for the final space shuttle mission is now available in our store. Get this piece of history!Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.STS-133 PatchFree shipping to U.S. addresses!The final planned flight of space shuttle Discovery is symbolized in the official embroidered crew patch for STS-133. Available in our store!Anniversary Shuttle PatchFree shipping to U.S. addresses!This embroidered patch commemorates the 30th anniversary of the Space Shuttle Program. The design features the space shuttle Columbia's historic maiden flight of April 12, 1981.Mercury anniversaryFree shipping to U.S. addresses!Celebrate the 50th anniversary of Alan Shephard's historic Mercury mission with this collectors' item, the official commemorative embroidered patch. | | | | 2014 Spaceflight Now Inc.Phoenix spacecraft headed to Mars to probe the water BY WILLIAM HARWOOD Mens Nike Free 5.0

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STORY WRITTEN FOR & USED WITH PERMISSIONPosted: May 21, 2010Astronauts Michael Good and Garrett Reisman are suiting up for a planned six-and-a-half-hour spacewalk today to finish replacing the International Space Station's oldest set of solar array batteries. They also plan to install an ammonia coolant jumper between two power truss segments, retrieve a robot arm grapple fixture and repair insulation on a Canadian robot arm extension.Credit: NASAThe spacewalk is scheduled to begin around 6:45 a.m. EDT when Reisman and Good, floating in the station's Quest airlock module, switch their spacesuits to battery power.This will be the 146th spacewalk devoted to station assembly and maintenance since construction began in 1998, the 10th so far this year and the third and final excursion planned by the Atlantis astronauts. Good, call sign EV-1, will be making the fourth spacewalk of his career, while Reisman, EV-2, will be making his third.One of the major objectives of Atlantis' mission was the replacement of six aging batteries in the P6 solar array segment on the far left end of the station's power truss. Four batteries were replaced by Good and Stephen Bowen during a spacewalk Wednesday, one more than called for in the flight plan."Because the crew's been so good this mission in getting ahead, we did add a couple of things to (Friday's) EVA," said space station Flight Director Scott Stover. "The first thing they do when they go out, they're going to be installing a jumper that runs between the P4 and P5 truss segments on the space station. ... It's an ammonia jumper, although it's going to be filled with nitrogen so we don't have to worry about any ammonia getting on the suits or anything like that."The P5 truss segment acts as a spacer between the P4 and P6 solar arrays. The jumper will help complete a path from an inboard ammonia reservoir in the P3 segment to the outboard solar arrays."The P6 and the P4 modules both have ammonia cooling systems on there, but the ammonia tanks for the external thermal control system are inside the solar alpha rotary joint," Stover said. "If one of those outboard, P4 or P6, modules develop a leak or need to be refilled with ammonia, we need this jumper to help us with those refill operations. So that's the first thing they're going to do, install a jumper that in the future would be used for refill operations."The second thing they're going to do is (go) back to battery ops. They still have two new batteries to install and two old batteries to put onto the ICC (integrated cargo carrier). Plus, that one battery they left temp stowed needs to go back on the ICC. So those activities will finish up all the battery ops."After that, Good and Reisman will make their way to the base of the station's robot arm where a Canadian hand-like extension known as DEXTRE is mounted. Engineers earlier spotted an insulation blanket that was not in the proper configuration and the astronauts will take a moment to fix that before moving to the shuttle's cargo bay."The final scheduled activity is to go down to the payload bay of Atlantis and get what we call a power and data grapple fixture, which is the structure the station arm connects to," Stover said. "It's an extra one we have brought up on Atlantis for planned install on a later EVA on the (Russian) Zarya module. That EVA is currently scheduled for the summer."A final get-ahead task will be carried out if time is available, replacing tools in external tool boxes that were carried inside the station by previous spacewalkers.Along with replacing the batteries in the P6 solar array segment, a second major objective of Atlantis' mission was installing a new Russian module known as Rassvet, or mini-research module No. 1. The new compartment was attached to the Earth-facing port of the Zarya module Tuesday and opened up on Thursday.Entering the module, Expedition 23 commander Oleg Kotov reported seeing what appeared to be metal flakes, or shavings, floating in the air, debris presumably shaken loose during launch. As always when opening a new module, Kotov was wearing goggles and a dust mask as a safety precaution."One thing that we did find were some metal flakes, or shavings, that were unexpected," Stover said. "In the one-G environment when it was on the ground you can imagine they hide in the nooks and crannies of the module itself. Now in zero G, they're floating around."When the crew entered, we were prepared for it, we made sure they were wearing the protective gear, goggles and dust mask," he said. "They reported seeing the metal flakes, so we had them make sure the (air) scrubbers were running."The module's hatch was closed overnight and "hopefully the scrubbers will collect all of that debris," Stover said. "When we do go back in, we'll again have them wear the protective equipment just in case there's something floating around in the air."Here is an updated timeline of today's activity (in EDT and mission elapsed time; includes revision G of the NASA television schedule):EDT........DD...HH...MM...EVENT05/2101:50 AM...06...11...30...STS/ISS crew wakeup03:00 AM...06...12...40...EVA-3: 14.7 psi repress/hygiene break03:15 AM...06...12...55...EVA-3: Airlock depress to 10.2 psi03:40 AM...06...13...20...EVA-3: EVA prep03:50 AM...06...13...30...ISS daily planning conference05:10 AM...06...14...50...EVA-3: Spacesuit purge05:25 AM...06...15...05...EVA-3: Spacesuit prebreathe06:05 AM...06...15...45...SSRMS cargo pallet move to EVA worksite06:15 AM...06...15...55...EVA-3: Crew lock depressurization06:45 AM...06...16...25...EVA-3: Spacesuits to battery power06:50 AM...06...16...30...EVA-3: Airlock egress/setup07:05 AM...06...16...45...EVA-3: Setup07:15 AM...06...16...55...EVA-3: Ammonia jumper install07:30 AM...06...17...10...EVA-3: P6 battery 5 R&R08:00 AM...06...17...40...EVA-3: P6 battery E/6 R&R09:05 AM...06...18...45...EVA-3: P6 battery F R&R09:40 AM...06...19...20...EVA-3: Install battery on pallet10:15 AM...06...19...55...EVA-3: P6 cleanup11:15 AM...06...20...55...EVA-3: Retrieve grapple fixture from cargo bay11:35 AM...06...21...15...SSRMS moves cargo pallet to solar array truss12:15 PM...06...21...55...EVA-3: Get aheads12:20 PM...06...22...00...SSRMS releases cargo pallet12:40 PM...06...22...20...EVA-3: Cleanup and ingress01:15 PM...06...22...55...EVA-3: Airlock repressurization01:25 PM...06...23...05...Spacesuit servicing02:25 PM...07...05...00...ISS daily planning conference03:15 PM...07...55...00...EVA tagup04:00 PM...07...01...40...Mission status briefing on NTV04:50 PM...07...02...30...ISS crew sleep begins05:00 PM...07...02...40...SRB launch video05:20 PM...07...03...00...STS crew sleep begins06:00 PM...07...03...40...Daily highlights reel09:00 PM...07...06...40...HD crew highlights The final planned flight of space shuttle Atlantis is symbolized in the official embroidered crew patch for STS-132. Available in our store! Additional coverage for subscribers:VIDEO:CREW'S HOME MOVIES FOR FLIGHT DAY 7 VIDEO:THURSDAY'S MISSION STATUS BRIEFING VIDEO:ASSOCIATED PRESS, FOX AND CBS INTERVIEWS VIDEO:THURSDAY MORNING'S FLIGHT DIRECTOR INTERVIEW HIGH DEFINITION TV DAY 6:DINNER TIME IS FUN TMIE IN SPACE HIGH DEFINITION TV DAY 6:THE VICTORIOUS SPACEWALKERS HIGH DEFINITION TV DAY 6:MIKE AND STEVE RETURN FROM EVA VIDEO:FLIGHT DAY 6 HIGHLIGHTS MOVIE VIDEO:CREW'S HOME MOVIES FOR FLIGHT DAY 6 VIDEO:WEDNESDAY'S MISSION STATUS BRIEFING VIDEO:REMOVING GIMBAL LOCKS ON ANTENNA DISH VIDEO:ADDING TO TORQUE TO NEW KU-BAND ATENNA VIDEO:THE DAY'S FINAL NEW BATTERY INSTALLED VIDEO:THIRD OLD BATTERY PULLED OUT AND STOWED VIDEO:SECOND FRESH BATTERY PUT INTO STATION VIDEO:FIRST OF THE NEW BATTERIES INSTALLED VIDEO:SPACEWALKERS REMOVE FIRST OLD BATTERY VIDEO:CABLE ON INSPECTION SENSOR UNTANGLED VIDEO:WEDNESDAY MORNING'S FLIGHT DIRECTOR INTERVIEW VIDEO:STEP-BY-STEP WALKTHROUGH OF EVA NO. 2 VIDEO:PREVIEW OF FLIGHT DAY 6 ACTIVITIES HIGH DEFINITION TV DAY 5:FLIGHT DECK OF ATLANTIS HIGH DEFINITION TV DAY 5:GIVING WATER TO STATION HIGH DEFINITION TV DAY 5:INSIDE DESTINY LABORATORY HIGH DEFINITION TV DAY 5:ROBOTICS WORKSTATION IN CUPOLA HIGH DEFINITION TV DAY 5:LOOKING OUT WINDOW AT EARTH HIGH DEFINITION TV DAY 5:DAILY SHUTTLE CHORES VIDEO:FLIGHT DAY 5 HIGHLIGHTS MOVIE VIDEO:CREW'S HOME MOVIES FOR FLIGHT DAY 5 VIDEO:TUESDAY'S MISSION STATUS BRIEFING VIDEO:MSNBC AND CNN INTERVIEWS OF CREW VIDEO:CONGRATULATIONS FROM ALL AROUND VIDEO:RASSVET CAPTURED AND SECURED TO ZARYA MODULE! VIDEO:TWEAKING FINAL ALIGNMENT OVER DOCKING PORT VIDEO:DOCKING PROBE EXTENDED FROM RASSVET NOSE VIDEO:SWINGING RASSVET FROM ATLANTIS TO STATION VIDEO:RASSVET UNBERTHED FROM SHUTTLE BAY VIDEO:PREVIEW OF FLIGHT DAY 5 ACTIVITIES VIDEO:TUESDAY MORNING'S FLIGHT DIRECTOR INTERVIEW VIDEO:ANIMATED OVERVIEW OF RUSSIA'S RASSVET MODULE VIDEO:ANIMATED OVERVIEW OF MISSION'S CARGO CARRIER VIDEO:FLIGHT DAY 4 HIGHLIGHTS MOVIE VIDEO:MONDAY'S MISSION STATUS BRIEFING VIDEO:AN ADDITION TO DEXTRE ROBOT VIDEO:TORQUING ANTENNA ASSEMBLY INTO PLACE VIDEO:FETCHING 6-FOOT-DIAMETER ANTENNA DISH VIDEO:BOLTING BOOM ATOP STATION'S Z1 TRUSS VIDEO:SPACEWALKERS HANDOFF ANTENNA BOOM VIDEO:UNPACKING ANTENNA BOOM FROM CARRIER VIDEO:SPACEWALK NO. 1 BEGINS VIDEO:STEP-BY-STEP WALKTHROUGH OF EVA NO. 1 VIDEO:PREVIEW OF FLIGHT DAY 4 ACTIVITIES VIDEO:MONDAY MORNING'S FLIGHT DIRECTOR INTERVIEW VIDEO:FLIGHT DAY 3 HIGHLIGHTS MOVIE VIDEO:MISSION MANAGEMENT TEAM CHAIRMAN UPDATE VIDEO:CARRIER ATTACHED TO STATION'S RAILCAR VIDEO:CARGO PALLET LIFTED FROM SHUTTLE BAY VIDEO:SUNDAY'S MISSION STATUS BRIEFING VIDEO:WELCOMING CEREMONY FOR SHUTTLE CREW VIDEO:ATLANTIS DOCKS TO INTERNATIONAL SPACE STATION VIDEO:SHUTTLE ATLANTIS PERFORMS BACKFLIP MANEUVER VIDEO:BEAUTIFUL VIEWS OF SHUTTLE ATLANTIS APPROACHING VIDEO:ANIMATED PREVIEW OF FLIGHT DAY 3 ACTIVITIES VIDEO:FLIGHT DAY 2 HIGHLIGHTS MOVIE VIDEO:CREW'S HOME MOVIES FOR FLIGHT DAY 2 VIDEO:MISSION MANAGEMENT TEAM CHAIRMAN UPDATE VIDEO:SATURDAY'S MISSION STATUS BRIEFING VIDEO:FLIGHT DAY 1 HIGHLIGHTS MOVIE VIDEO:THE FULL STS-132 LAUNCH EXPERIENCE VIDEO:SHUTTLE ATLANTIS BLASTS OFF! VIDEO:GO INSIDE MISSION CONTROL DURING LAUNCH VIDEO:POST-LAUNCH NEWS CONFERENCE VIDEO:LAUNCH REPLAY: VAB ROOF VIDEO:LAUNCH REPLAY: PRESS SITE VIDEO:LAUNCH REPLAY: PATRICK AFB VIDEO:LAUNCH REPLAY: PAD PERIMETER VIDEO:LAUNCH REPLAY: BEACH TRACKER VIDEO:LAUNCH REPLAY: PAD CAMERA 070 VIDEO:LAUNCH REPLAY: PAD CAMERA 071 VIDEO:LAUNCH REPLAY: PLAYALINDA BEACH VIDEO:LAUNCH REPLAY: PAD FRONT CAMERA VIDEO:CREW ARRIVES AT LAUNCH PAD 39A VIDEO:ASTRONAUTS LEAVE CREW QUARTERS VIDEO:CREW FINISHES GETTING SUITED UP VIDEO:ASTRONAUTS WEARING TUXEDOS LAUNCH DAY VIDEO:NARRATED REVIEW OF SHUTTLE'S PREPARATIONS VIDEO:NARRATED REVIEW OF PAYLOADS' PREPARATIONS VIDEO:ATLANTIS ON EVE OF FINAL PLANNED LAUNCH VIDEO:LAUNCH PAD'S SERVICE TOWER RETRACTED VIDEO:PAYLOAD BAY DOORS CLOSED FOR LAUNCH VIDEO:ASTRONAUTS INSPECT THE PAYLOAD BAY VIDEO:JERRY ROSS' LAUNCH ON MISSION STS-61B VIDEO:MAIDEN LAUNCH OF ATLANTIS AS SEEN LIVE IN 1985 VIDEO:ATLANTIS' FIRST MISSION ENDS WITH LAKEBED LANDING VIDEO:AN ASTRONAUT'S TRIBUTE TO SHUTTLE ATLANTIS VIDEO:COUNTDOWN STATUS AND WEATHER FORECAST VIDEO:WATCH NASA'S PRE-LAUNCH NEWS CONFERENCE VIDEO:GET BRIEFED ON THE LAUNCH COUNTDOWN VIDEO:HEAR FROM THE COMMANDER AT THE RUNWAY VIDEO:ASTRONAUTS ARRIVE IN FLORIDA FOR LAUNCH VIDEO:PRE-LAUNCH INTERVIEW WITH KEN HAM VIDEO:PRE-LAUNCH INTERVIEW WITH TONY ANTONELLI VIDEO:PRE-LAUNCH INTERVIEW WITH GARRETT REISMAN VIDEO:PRE-LAUNCH INTERVIEW WITH MIKE GOOD VIDEO:PRE-LAUNCH INTERVIEW WITH STEVE BOWEN VIDEO:PRE-LAUNCH INTERVIEW WITH PIERS SELLERS VIDEO:STS-132 MISSION PREVIEW MOVIE VIDEO:FULL FLIGHT READINESS REVIEW NEWS BRIEFING VIDEO:RECAP OF THE FLIGHT READINESS REVIEW VIDEO:MANAGERS ASSESS ISSUES BEFORE FLIGHT VIDEO:UPDATE ON PRE-LAUNCH PREPS AT PAD 39A VIDEO:PROGRAM BRIEFING BY SHUTTLE AND STATION CHIEFS VIDEO:THE STS-132 MISSION OVERVIEW PRESENTATIONS VIDEO:PREVIEW BRIEFING ON MISSION'S SPACEWALKS VIDEO:THE ASTRONAUTS' PRE-FLIGHT NEWS BRIEFING VIDEO:SHUTTLE EVACUATION PRACTICE VIDEO:ASTRONAUTS BOARD ATLANTIS VIDEO:LAUNCH DAY REHEARSAL BEGINS VIDEO:CREW BRIEFED ON EMERGENCY PROCEDURES VIDEO:TEST-DRIVING AN EMERGENCY ARMORED TANK VIDEO:CREW'S CHAT WITH REPORTERS AT PAD 39A VIDEO:ASTRONAUTS AT KENNEDY SPACE CENTER RUNWAY VIDEO:CREW ARRIVES FOR PRACTICE COUNTDOWN VIDEO:GANTRY PLACED AROUND ATLANTIS VIDEO:SHUTTLE ATLANTIS REACHES PAD 39A VIDEO:CROWDS AND THE CREW CHEER ON ATLANTIS VIDEO:OVERNIGHT ROLLOUT TO THE PAD BEGINS VIDEO:SHUTTLE HOISTED FOR ATTACHMENT TO TANK VIDEO:CRANE ROTATES THE ORBITER VERTICALLY VIDEO:ATLANTIS RISES OFF THE TRANSPORTER VIDEO:ORBITER EMERGES FROM ITS HANGAR VIDEO:BUTTONING UP RUDDER/SPEED BRAKE VIDEO:DOME SHIELDS AROUND MAIN ENGINES VIDEO:EXTERNAL TANK ATTACHED TO BOOSTERS VIDEO:PAYLOADS HEAD FOR LAUNCH PAD VIDEO:RASSVET PLACED INTO THE TRANSPORTER VIDEO:PALLET LOADED WITH MISSION'S CARGO VIDEO:RUSSIAN RASSVET MODULE ON DISPLAY VIDEO:RUSSIAN ENGINEERS DISCUSS THEIR RASSVET MODULE VIDEO:RASSVET HATCH CLOSED FOR FLIGHT VIDEO:FILLING MODULE WITH NASA SUPPLIES VIDEO:ASTRONAUTS VISIT THEIR SPACECRAFT VIDEO:CREW INSPECTS RASSVET MODULE STS-134 PatchFree shipping to U.S. addresses!The final planned flight of space shuttle Endeavour is symbolized in the official embroidered crew patch for STS-134. Available in our store!Final Shuttle Mission PatchFree shipping to U.S. addresses!The crew emblem for the final space shuttle mission is now available in our store. Get this piece of history!Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.STS-133 PatchFree shipping to U.S. addresses!The final planned flight of space shuttle Discovery is symbolized in the official embroidered crew patch for STS-133. Available in our store!Anniversary Shuttle PatchFree shipping to U.S. addresses!This embroidered patch commemorates the 30th anniversary of the Space Shuttle Program. The design features the space shuttle Columbia's historic maiden flight of April 12, 1981.Mercury anniversaryFree shipping to U.S. addresses!Celebrate the 50th anniversary of Alan Shephard's historic Mercury mission with this collectors' item, the official commemorative embroidered patch. | | | | 2014 Spaceflight Now Inc.Atlantis journeys to launch pad for perhaps final timeSPACEFLIGHT NOWPosted: April 22, 2010Facing what could be the final voyage in its quarter-century of spaceflight, the shuttle Atlantis emerged from Kennedy Space Center's assembly building bathed in spotlights and traveled to the launch pad overnight.Check out Spaceflight Now's two photo galleries of Atlantis' rollout:The trip covering 3.5 miles along the rock-covered road began at 11:31 p.m. and concluded at 6:03 a.m. EDT when the mobile launching platform was securely anchored to pad 39A. The rollout was delayed twice by lightning concerns on Monday and Tuesday nights, then by soggy conditions on the crawlerway early Wednesday.Atlantis entered service with a classified Defense Department mission in October 1985 that deployed a pair of military communications satellites. Since then, the orbiter has flow 30 more times on a variety of flights that launched the Magellan radar mapper to Venus, the Galileo orbiter to Jupiter and the Gamma Ray Observatory to survey the cosmos, built U.S.-Russian relations with multiple dockings to the space station Mir, completed critical sorties to construct the International Space Station and extended the life of NASA's Hubble Space Telescope. Credit: Justin Ray/Spaceflight NowWhat's currently the last scheduled flight of the venerable spaceplane, Atlantis will blast off May 14 at 2:19 p.m. EDT carrying a Russian docking module to the International Space Station on mission STS-132.But whether it's truly the final time Atlantis will circle the planet depends if NASA approves the addition of one more mission to the the space shuttle manifest. That flight, known as STS-135, would use the extra external fuel tank and solid rocket boosters available to the shuttle program.No decisions have been made to authorize the bonus flight, leaving the Atlantis team well aware that Thursday's rollout might have been the historic last before the orbiter is retired."The manifest hasn't changed. STS-132 is still the last flight of Atlantis," said Mikes Moses, the shuttle launch integration manager.After Atlantis lands in late May, KSC workers will put the orbiter into normal post-flight turnaround activities and ready it for duty as a rescue vehicle.NASA has prepared "launch-on-need" shuttles throughout the post-Columbia era in case an orbiting astronaut crew needs rescued. Since the space agency will have the hardware available to stage a rescue of what's presently the final shuttle mission this fall, some have urged the program to launch that standby vehicle later on a standard mission, albeit with a smaller crew, and deliver more supplies to the International Space Station.If NASA opts to add the STS-135 mission, then Atlantis would see one more journey after all."It will be readied as a rescue vehicle, if needed. There has been a lot of talk from the administration, politically, whether you go ahead and fly that rescue vehicle since you have the hardware here and stacked. But there has been no decision made there," Moses.In any event, Atlantis' upcoming trek will help expand the Russian segment of the International Space Station with delivery of the Mini Research Module 1 that gets attached to the Earth-facing port of Zarya. Once fully activated, the module becomes a new docking compartment for visiting Russian spacecraft. Credit: Justin Ray/Spaceflight NowSee crew at the pad Atlantis' 12-day voyage includes three spacewalks to replace a half-dozen aging batteries on the station's Port 6 power truss, install a new space-to-ground communications antenna dish and boom on the Z1 truss and add a small platform onto the Canadian Dextre robot.Astronaut Ken Ham commands this 32nd flight of Atlantis. He'll be joined by pilot Tony Antonelli and mission specialists Garrett Reisman, Mike Good, Steve Bowen and Piers Sellers.The six men were among the spectators on hand Thursday to watch Atlantis' journey to the launch pad. "We ended up staying for hours because it is absolutely incredible," Ham said. "It was one of those moments we shared with each other to remind us of the reality of what we're going to go do."Following a launch May 14, the shuttle is scheduled to dock with the space station around 10 a.m. EDT on May 16. The first spacewalk starts around 8 a.m. May 17 to handle the new antenna and Dextre equipment installation tasks. Mini Research Module gets attached the morning of May 18 and the crew will ingress it on May 20.The second and third EVAs begins just after 7 a.m. May 19 and May 21, respectively, to perform the P6 battery replacement effort.Atlantis undocks around 11 a.m. May 23 and returns to Earth with a landing at Kennedy Space Center on May 26 at approximately 8:30 a.m. EDT.John Glenn Mission PatchFree shipping to U.S. addresses!The historic first orbital flight by an American is marked by this commemorative patch for John Glenn and Friendship 7.Final Shuttle Mission PatchFree shipping to U.S. addresses!The crew emblem for the final space shuttle mission is available in our store. Get this piece of history!Celebrate the shuttle programFree shipping to U.S. addresses!This special commemorative patch marks the retirement of NASA's Space Shuttle Program. Available in our store!Anniversary Shuttle PatchFree shipping to U.S. addresses!This embroidered patch commemorates the 30th anniversary of the Space Shuttle Program. The design features the space shuttle Columbia's historic maiden flight of April 12, 1981.Mercury anniversaryFree shipping to U.S. addresses!Celebrate the 50th anniversary of Alan Shephard's historic Mercury mission with this collectors' item, the official commemorative embroidered patch.Fallen Heroes Patch CollectionThe official patches from Apollo 1, the shuttle Challenger and Columbia crews are available in the store. | | | | 2014 Spaceflight Now Inc.Atlantis' last fuel tank reaches launch siteSPACEFLIGHT NOW UGG Knightsbridge

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Richardson knew he wanted to strike out on his own. he makes up his mind to do something. Davis said,105Northside (near San Antonio) 440SOURCE: Dallas Morning News research Requested waiversHere are the number of waivers requested by selected school districts to increase kindergarten through fourth-grade classroom sizes beyond the state cap of 22 students:Dallas Not yet determinedRichardson 268Frisco 110 Mesquite 45Carrolton-Farmers Branch 30Irving 19Garland 0Houston 1, which starts in downtown Dallas and finishes at Fair Park.So when I called the NFL this week to see if that arrangement would continue, don??t bleed on my floor, The Longhornswill play Kansas State (2-1) before their largest television audience of theseason.Dec. but Lerner has added the voice and action of ??spiritual progressives?? to the media mix long dominated by ??spiritual regressives??. Air?Jordan?7?(VII)

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