Baby It’S Cold Outside!

During those chilly winter nights, bundle up your bump with one of these stylish maternity outerwear options. Now’s the perfect time to snag a jacket on sale for a killer deal.

If you’re in your second or third trimester during the winter months, chances are your old standby warm coats are feeling a little snug. Sure, you can pick up a regular overcoat in a larger size, but it’ll likely add extra bulk since it’s not cut to fit a pregnant body – the last thing you probably want right now. Instead, check out one of these stylish maternity jackets. January is a great time to pick up a coat since most are on sale.

Here are looks we love:

Wool peacoat from A Pea in the Pod

A classic

This Double Breasted Wool Peacoat is a classic outwear choice that will take you from work to play. The simple silhouette goes with anything from work pants to jeans, and the brass buttons jazz it up with a little bling. (A Pea In The Pod Maternity, regularly $180; on sale for $160)

Maternity jacket from Topshop

Feisty fur

For a little extra pizzazz, check out the Maternity Emmie Fur Lined Coat. The removable fur color is a fun accessory when the temperatures are low, but can be removed for a new look when you need to spice things up. Plus, the buckle clip fronts are super cute. (Topshop, $150)

Maternity jacket from Sears

Military style

Military accents and outerwear continue to be big this year and just because you’re expecting doesn’t mean that you can’t indulge in the latest looks. With brass buttons and pleated detailing, the Momo Maternity Military Style Coat is so stylish you’ll want to wear it long after you give birth. (Sears, regularly $160; on sale for $70)

Maternity jacket from Destination Maternity

Casually chic

If you’re looking for a more casual spin on outerwear, this Tie Front Faux Fur Maternity Jacket is just the ticket! The olive shade is a nice alternative to black or grey. Pair with skinny black pants and heeled boots to dress it up or keep it casual with jeans and a pair of comfy kicks. The front tie is designed to accent your waistline and the removable fur color makes it easy to clean. (Destination Maternity, regularly $170; on sale for $80)

Liz Lange for Target maternity coat

Budget find

On sale for a mere $30 this Liz Lange for Target Maternity Tweed Coat is a steal! The front pockets will help keep your hands warm (pregnant women often have poor circulation) and the short length is perfect for busy moms-to-be on the go. Plus, the purple lining is a fun pop of color for dreary winter days. (Target, regularly $60; on sale for $30) 

More maternity style

Maternity wear for parties
Dress your bump for cold weather
Find your perfect pregnancy style


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Assess movements National football league lawsuit listening to about Aug. 26

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STORY WRITTEN FOR & USED WITH PERMISSIONPosted: November 17, 2008The combined crews of the shuttle Endeavour and the international space station are gearing up for a busy day in space, moving a 27,000-pound cargo module loaded with critical equipment and supplies from the shuttle to a docking port on the lab's Harmony module. The astronauts also will also make final preparations for the mission's first spacewalk Tuesday.The morning wakup call from mission control came at 9:35 a.m., with a recording of "London Calling" for astronaut Stephen Bowen."I guess my family really wanted to wake me up this morning," Bowen called down. "And we're all up and ready to go today."Overnight, shuttle astronaut Sandra Magnus officially joined the Expedition 18 crew of the space station, replacing Gregory Chamitoff, who was launched to the outpost on May 31. The transfer was completed at 9:50 p.m. Sunday when Magnus' custom-fitted Soyuz seat liner was installed in the station's Soyuz lifeboat."The Soyuz now becomes Sandy's vehicle in case of an emergency," station flight director Brian Smith said early today. "The seat liners are custom fit to each astronaut and cosmonaut. So Sandy carried hers up with her on the shuttle and very shortly after docking, she took that and installed it in the Soyuz. Greg's came out of the Soyuz and was put in the shuttle for return home. So that marked the official transfer. Sandy is now an ISS crew member, Greg is now a member of STS-126 crew."Also overnight, engineers completed a quick assessment of heat shield components on the extreme outer regions of Endeavour's right wing. That area of the wing could not be easily inspected after the cargo module is mounted on the station if problems were discovered later."If we needed to do any inspection in that area, we'd have to modify some of the planning," Smith said. "With the MPLM (multi-purpose logistics module) installed on node 2 (the Harmony module), we would not be able to access that area for inspection. So we were anxiously awaiting those results. The meeting was held overnight and the debris assessment team came back and said the wing looks great and no further inspection required and we were able to leave the plans (for today's cargo module transfer) in place."Engineers are continuing to evaluate photos and other data to determine the overall health of the shuttle's thermal protection system. There have been no obvious signs of trouble, but analysis of digital photos shot during Endeavour's final approach to the station Sunday is not yet complete.The Italian-built MPLM is loaded with a record amount of cargo, more than 14,000 pounds, including two complex racks of gear designed to convert urine into potable water, a new galley, a second toilet and two crew sleep stations. The equipment is needed to boost the station's crew size from three to six next year.Carried into orbit at the back of Endeavour's cargo bay, the cylindrical cargo module will be picked up by the station's robot arm starting around 11:25 a.m. and attached to the Harmony module's downward-facing, or nadir, port. This will be the first time a cargo module has been attached to Harmony, which was launched to the station last year."This is one of the heaviest MPLMs to fly to the ISS," Smith said. "We've got Don Pettit and Sandy Magnus as the folks assigned to unload the MPLM and then load it back up with the cargo that's going to come back home. And of course, those two are veterans. Sandy's been to the ISS once before, on STS-112 back in 2002, and of course, Don was on ISS as an expedition crew member on Expedition 6. So the veterans are going to do an excellent job and I've got no concerns about all the transfers being completed."While the cargo module is being secured to the station, spacewalkers Bowen, Heidemarie Stefanyshyn-Piper and Robert "Shane" Kimbrough will move equipment needed for upcoming spacewalks into the lab complex. The first spacewalk, by Stefanyshyn-Piper and Bowen, is scheduled to get underway at 1:45 p.m. Tuesday. To prevent the bends after working in their low-pressure suits, both astronauts will spend the night inside the station's Quest airlock at a reduced air pressure.Spacewalk preparations today "will consist of some tool configurations and some equipment transfers, equipment and tools that were flown up with the shuttle will be transferred over to the ISS," Smith said. "The remaining tools required and equipment for this EVA were already on ISS and configured by the ISS crew ahead of time."So the crew is also going to prepare the grease gun that they're going to use on the solar array rotary joint on the starboard side of the ISS during EVA-1. They're going to also take a last-minute review of the procedures and make sure there are no more questions. Then they'll go into the physiological preparations for EVA-1. And that consists of getting set up in the airlock and going on a breathing protocol and then sleeping in the airlock overnight."Today's mission status briefing is scheduled for 3:30 p.m. and the first in a series of media crew interviews is planned for 5:25 p.m. Mission Management Team Chairman LeRoy Cain will update reporters in a 6 p.m. briefing.Here is an updated timeline of today's activity (in EST and mission elapsed time; includes revision B of the NASA television schedule):EST........DD...HH...MM...EVENT09:35 AM...02...13...30...Crew wakeup11:25 AM...02...15...30...ISS daily planning conference11:25 AM...02...15...30...Station arm (SSRMS) grapples cargo module (MPLM)11:55 AM...02...16...00...SSRMS unberths MPLM12:55 PM...02...17...00...Post-docking spacewalk transfers01:15 PM...02...17...20...MPLM installation01:15 PM...02...17...20...Middeck transfers01:45 PM...02...17...50...First stage bolts tightened for MPLM berthing01:55 PM...02...18...00...Crew meals begin02:05 PM...02...18...10...Second stage bolts tightened02:35 PM...02...18...40...REBA checkout02:50 PM...02...18...55...EVA-1: Tools configured02:50 PM...02...18...55...Soyuz pressure suit drying02:55 PM...02...19...00...SSRMS ungrapples MPLM03:30 PM...02...19...05...Mission status briefing on NASA TV03:35 PM...02...19...40...MPLM vestibule pressurization04:50 PM...02...20...55...MPLM vestibule ingress and configuration04:50 PM...02...20...55...Grease gun preps for spacewalk05:25 PM...02...21...30...WXIA-TV, WAGA-TV, WHDH-TV crew interviews06:00 PM...02...22...05...Post-MMT briefing on NASA TV06:20 PM...02...22...25...MPLM activation (part 1)07:55 PM...03...00...00...Equipment airlock preps08:15 PM...03...00...20...MPLM activation (part 2)08:35 PM...03...00...40...MPLM ingress08:50 PM...03...00...55...EVA-1: Procedures review11:20 PM...03...03...25...EVA-1: Mask pre-breathe11/18/0812:05 AM...03...04...10...EVA-1: Airlock depress to 10.2 psi12:25 AM...03...04...30...ISS crew sleep begins12:55 AM...03...05...00...STS crew sleep begins01:00 AM...03...05...05...Flight day 4 highlights reel on NASA TV07:30 AM...03...11...35...Flight director update on NASA TV08:55 AM...03...13...00...Crew wakeupAdditional coverage for subscribers:VIDEO:CREW OPENS HATCH AND ENTERS LEONARDO VIDEO:ATLANTA AND BOSTON TV STATIONS INTERVIEW CREW VIDEO:MONDAY'S MISSION MANAGEMENT TEAM UPDATE VIDEO:MONDAY'S MISSION STATUS BRIEFING VIDEO:LEONARDO MODULE SUCCESSFULLY MOUNTED TO STATION VIDEO:MONDAY MORNING FLIGHT DIRECTOR INTERVIEW VIDEO:PREVIEW ANIMATION OF LEONARDO MODULE ATTACHMENT VIDEO:SUMMARY OF CARGO BEING DELIVERED TO SPACE STATION VIDEO:FLIGHT DAY 3 HIGHLIGHTS MOVIE VIDEO:SUNDAY'S MISSION STATUS BRIEFING VIDEO:SHUTTLE CREW WELCOMED ABOARD STATION VIDEO:SPACE SHUTTLE ENDEAVOUR DOCKS TO SPACE STATION VIDEO:ENDEAVOUR PERFORMS THE 360-DEGREE BACKFLIP VIDEO:VIEWS OF THE SHUTTLE APPROACHING FROM BELOW VIDEO:FLIGHT DIRECTOR'S SUMMARY OF FLIGHT DAY 3 VIDEO:PREVIEW ANIMATION OF RENDEZVOUS AND DOCKING VIDEO:FLIGHT DAY 2 HIGHLIGHTS MOVIE VIDEO:SATURDAY'S MISSION STATUS BRIEFING VIDEO:SATURDAY'S MISSION MANAGEMENT TEAM UPDATE VIDEO:FLIGHT DIRECTOR'S SUMMARY OF FLIGHT DAY 2 VIDEO:PREVIEW ANIMATION OF HEAT SHIELD INSPECTIONS VIDEO:NARRATED TOUR OF ENDEAVOUR'S PAYLOAD BAY VIDEO:FLIGHT DAY 1 HIGHLIGHTS MOVIE VIDEO:SPACE SHUTTLE ENDEAVOUR BLASTS OFF! VIDEO:SPACEFLIGHT NOW'S LAUNCH PAD CAMERA VIDEO:THE FULL STS-126 LAUNCH EXPERIENCE VIDEO:INSIDE MISSION CONTROL DURING LAUNCH VIDEO:POST-LAUNCH NEWS BRIEFING VIDEO:FINAL PRE-LAUNCH POLLS GIVE "GO" FOR LIFTOFF VIDEO:SHUTTLE'S CREW MODULE HATCH CLOSED FOR FLIGHT VIDEO:MISSION SPECIALIST DON PETTIT BOARDS VIDEO:MISSION SPECIALIST SHANE KIMBROUGH BOARDS VIDEO:PILOT ERIC BOE BOARDS ENDEAVOUR VIDEO:COMMANDER CHRIS FERGUSON BOARDS ENDEAVOUR VIDEO:ASTROVAN TAKES CREW TO LAUNCH PAD 39A VIDEO:CREW DEPARTS QUARTERS FOR LAUNCH PAD VIDEO:ASTRONAUTS DON SPACESUITS FOR LAUNCH VIDEO:NARRATED RECAP OF ENDEAVOUR'S PRE-FLIGHT CAMPAIGN VIDEO:NARRATED RECAP OF PAYLOADS' PRE-FLIGHT CAMPAIGN VIDEO:PAD 39A SERVICE GANTRY RETRACTED FOR LAUNCH VIDEO:THURSDAY'S COUNTDOWN STATUS AND WEATHER UPDATE VIDEO:WEDNESDAY'S PRE-LAUNCH NEWS CONFERENCE VIDEO:ENDEAVOUR ASTRONAUTS ARRIVE FOR LAUNCH VIDEO:TUESDAY'S COUNTDOWN STATUS AND WEATHER UPDATE VIDEO:STATION ASTRONAUTS PREPARE FOR SHUTTLE ARRIVAL VIDEO:ENDEAVOUR'S PAYLOADS READIED FOR TREK TO SPACE VIDEO:UPDATE ON SHUTTLE AND STATION PROGRAMS VIDEO:STS-126 MISSION OVERVIEW VIDEO:PREVIEW BRIEFING ON MISSION'S SPACEWALKS VIDEO:THE ASTRONAUTS' PRE-FLIGHT NEWS BRIEFING VIDEO:INTERVIEW WITH COMMANDER CHRIS FERGUSON VIDEO:INTERVIEW WITH PILOT ERIC BOE VIDEO:INTERVIEW WITH MS1 HEIDEMARIE PIPER VIDEO:INTERVIEW WITH MS2 STEPHEN BOWEN VIDEO:INTERVIEW WITH MS3 DON PETITT VIDEO:INTERVIEW WITH MS4 SHANE KIMBROUGH VIDEO:INTERVIEW WITH MS5 SANDY MAGNUS VIDEO:INTERVIEW WITH SPACE STATION'S EXPEDITION 17 CREW VIDEO:ENDEAVOUR COMMANDER AND PILOT PRACTICE LANDINGS VIDEO:ISS PROGRAM MANAGER UPDATES SOYUZ INVESTIGATION VIDEO:ISS PROGRAM MANAGER DESCRIBES SARJ REPAIR PLAN VIDEO:ISS PROGRAM MANAGER DISCUSSES RADIATOR DAMAGE VIDEO:EXPEDITION 18 PRE-FLIGHT MISSION BRIEFING VIDEO:AERIAL VIEWS OF ATLANTIS AND ENDEAVOUR VIDEO:ENDEAVOUR AT SUNRISE ON LAUNCH PAD 39B VIDEO:AERIAL VIEWS OF ENDEAVOUR AFTER ROLLOUT VIDEO:ENDEAVOUR ROLLS FROM VAB TO LAUNCH PAD VIDEO:TIME-LAPSE MOVIE OF ARRIVAL AT PAD 39B VIDEO:TIME-LAPSE MOVIE OF ENDEAVOUR LEAVING VAB VIDEO:SHUTTLE HOISTED FOR ATTACHMENT TO TANK VIDEO:ENDEAVOUR'S DEPARTURE FROM HANGAR VIDEO:TIME-LAPSE MOVIE OF ENDEAVOUR GOING VERTICAL VIDEO:TIME-LAPSE MOVIE OF BEING HOISTED OFF TRANSPORTER VIDEO:TIME-LAPSE MOVIE OF ENDEAVOUR MOVING TO VAB MORE: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. 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STORY WRITTEN FOR & USED WITH PERMISSIONPosted: June 23, 2004NASA unveiled a spectacular high-resolution mosaic of Saturn's enigmatic moon Phoebe today, along with other data from the Saturn-bound Cassini probe showing the moon formed in the extreme outer solar system and later was captured by the ringed planet's gravity. During its historic close encounter with Phoebe, the Cassini spacecraft captured a series of high resolution images of the small moon, six of which have been put together to create this mosaic. Credit: NASA/JPL/Space Science InstituteDownload larger image version "The data that we gathered with the Cassini spacecraft have now given us our first look at this very strange object," said Torrence Johnson, a senior scientist and Cassini team member at the Jet Propulsion Laboratory in Pasadena, Calif. "And what it's told us is that it's a collection of ice and rock and probably carbonaceous compounds."We believe this object has many characteristics in common with things like Pluto and (Neptune's moon) Triton in the outer solar system. In other words, it's a first look at one of these denizens of the outer solar system that we've (seen previously) only from afar."The $3.3 billion Cassini probe, launched in 1997, is scheduled to brake into orbit around Saturn the night of June 30. On June 11, it made a close flyby of Phoebe, giving scientists their first close-up look at the strange moon since Voyager 2 captured a few grainy images in 1981. Voyager 2 imaged Phoebe from a distance of 1.4 million miles. Cassini passed within about 1,285 miles."The Phoebe encounter was a tremendous success scientifically, but also all the instruments worked great, the spacecraft performed beautifully, the nav team put us in exactly the right place and we have wonderful data from all of the experiments," Johnson said. "It's a great warm up for Saturn."Discovered in 1898, Phoebe measures just 137 miles or so across, orbits Saturn at a distance of about nine million miles and circles the planet in the opposite direction from its other moons. Because of that, and the tilt of its orbit, scientists long suspected Phoebe was a captured asteroid or an outer solar system Kuiper belt object left over from the birth of the solar system.The Cassini data indicate the moon almost certainly did, in fact, originate in the Kuiper belt in the extreme outer solar system.Roger Clark, a Cassini researcher with the U.S. Geological Survey said in a new release that "all our evidence leads us to conclude Phoebe's surface is made of water ice, water-bearing minerals, carbon dioxide, possible clays and primitive organic chemicals in patches at different locations on the surface."Cassini also detected as-yet-unknown compounds. But the presence of carbon dioxide provides clear evidence of Phoebe's origin."Phoebe is definitely not an asteroid," said Bonnie Buratti, a member of the Cassini visual and infrared mapping spectrometer team. "It did not form in the asteroid belt because you don't see CO2 in the asteroid belt."It formed some place in the outer solar system beyond the orbit of Jupiter. We believe this is evidence that it came from the Kuiper belt and that it was dragged into the Saturnian system early in the formation of the solar system. So what we see is a very diverse body."With a density of 1.6 grams per cubic centimeter, Phoebe is heavier than pure ice but lighter than most rocks. Johnson said the ratio of water ice to rocky material is similar to that of Pluto and Triton."We believe that four-and-a-half billion years ago, when the solar system was forming, that there were a lot of bodies like Phoebe in the outer solar system," Johnson said. "Since then, most of those bodies have either been accreted in the planets, they have become part of Jupiter, Saturn, Uranus and Neptune, or been gravitationally flung out of the system, out into the outer solar system. 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The must-see pictures show in great detail the cratered surface of the tiny moon. Credit: NASA/JPL/Space Science InstituteDownload larger image version FIRST IMAGE: Phoebe's true nature is revealed in startling clarity in this mosaic of two images taken during Cassini's flyby on June 11, 2004. The image shows evidence for the emerging view that Phoebe may be an ice-rich body coated with a thin layer of dark material. Small bright craters in the image are probably fairly young features. This phenomenon has been observed on other icy satellites, such as Ganymede at Jupiter. When impactors slammed into the surface of Phoebe, the collisions excavated fresh, bright material -- probably ice -- underlying the surface layer. Further evidence for this can be seen on some crater walls where the darker material appears to have slid downwards, exposing more light-colored material. Some areas of the image that are particularly bright - especially near lower right - are over-exposed. An accurate determination of Phoebe's density - a forthcoming result from the flyby - will help Cassini mission scientists understand how much of the little moon is comprised of ices. This spectacular view was obtained at a phase, or Sun-Phoebe-spacecraft, angle of 84 degrees, and from a distance of approximately 32,500 kilometers (20,200 miles). The image scale is approximately 190 meters (624 feet) per pixel. No enhancement was performed on this image. Credit: NASA/JPL/Space Science InstituteDownload larger image version SECOND IMAGE: Phoebe delivers on its promise to reveal new wonders to Cassini by showing probable evidence of an ice-rich body overlain with a thin layer of dark material. The sharply-defined crater at above center exhibits two or more layers of alternating bright and dark material. Imaging scientists on the Cassini mission have hypothesized that the layering might occur during the crater formation, when ejecta thrown out from the crater buries the pre-existing surface that was itself covered by a relatively thin, dark lag deposit over an icy mantle. The lower thin dark layer on the crater wall appears to define the base of the ejecta blanket. The ejecta blanket itself appears to be mantled by a more recent dark surface lag.This image was obtained on June, 11 2004 at a phase, or Sun-Phoebe-spacecraft, angle of 79 degrees, and from a distance of 13,377 kilometers (8,314 miles). The image scale is approximately 80 meters (263 feet) per pixel. No enhancement was performed on this image. Credit: NASA/JPL/Space Science InstituteDownload larger image version THIRD IMAGE:This eye-popping high-resolution image of Phoebe's pitted surface taken very near closest approach shows a 13-kilometer (8-mile) diameter crater with a debris-covered floor. 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The image scale is approximately 18.5 meters (60.5 feet) per pixel. The illumination is from the right. No enhancement was performed on this image.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.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle's last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Saturn's outer rings may be eroding, Cassini data shows UNIVERSITY OF SOUTHERN CALIFORNIA NEWS RELEASEPosted: December 18, 2004A massive eruption of atomic oxygen from Saturn's outer rings, seen by Cassini's ultraviolet camera as the spacecraft neared its destination, may be an indication that the planet's wispy E ring is eroding so fast that it could disappear within 100 million years if not replenished. An artist's concept shows the Cassini space probe at Saturn. Credit: NASA/JPLCassini's Ultraviolet Imaging Spectrograph (UVIS) detected the oxygen atoms spewing into a huge cloud on the dark side of Saturn's rings as Cassini prepared to enter orbit around Saturn in January 2004, said Donald Shemansky, professor of aerospace and mechanical engineering in the USC Viterbi School of Engineering. Data indicated that about 275 million pounds (125 million kilograms) of oxygen was abruptly released in a short period of time. "This was our first surprise in the ultraviolet," said Shemansky, who will analyze ultraviolet data during Cassini's four-year tour of Saturn and its rings with Janet Hallett, a postdoctoral aerospace research associate in the USC Viterbi School. "We aren't sure yet whether this was a transient event or part of a routine recycling process in Saturn's magnetosphere," he said. "Right now scientists are speculating that the oxygen eruption may have been caused by a collision of ice particles from the planet's distant E ring with material in one of the main ring systems, A, B or C. Or it could have been a meteorite collision or an eruption of icy slush on Enceladus, a moon that orbits in the E ring." Shemansky, a co-investigator on the 16-member Cassini ultraviolet imaging team, reported their findings in the Dec. 16 issue of Science Express . Despite Saturn's placid appearance from Earth, the planet is anything but that. The first detailed UV images from the Cassini mission show that Saturn commands a dynamic world of complex, braided ice rings, cannibalistic moons, 1,100 mile-per-hour planetary winds and electrifying auroral displays high in the night skies. Saturn, its moons and highly structured rings live inside a huge cavity in the solar wind created by the planet's strong magnetic field. The magnetosphere is a bubble of particles including electrons, various species of ions, neutral atoms and molecules, several populations of very energetic charged particles like those found in Earth's Van Allen Belts, and charged dust grains. The ionized (electrically charged) gases are called plasmas. However, unlike Jupiter's magnetosphere, Shemansky said Saturn's magnetic cocoon, which is smaller, is filled primarily with neutral gas rather than ions. "Saturn's magnetosphere is turning out to be very different from Jupiter's," he said. "It's dominated by neutral gas and water-rich ingredients produced by its rings, as icy moon debris collides, or by the more energetic collisions of incoming meteorites. It doesn't have nearly as many charged particles, and many of them are absorbed by the rings, so the plasma processes we are observing are entirely different." Two months after his initial observations, Shemansky and his ultraviolet team reported that the large cloud of escaping oxygen atoms had dissipated just as rapidly as it had appeared. Shemansky discounted theories that the rapid loss of material could be explained by "satellite sweeping," a process whereby tiny shepherding moons gobble up debris or deflect it as they clean out gaps between the rings. "The rate at which we saw material escaping from Saturn's outer rings implies that mass equivalent to the entire E ring, even including larger fragments and parent bodies, would be consumed in a period of about 100 million years if no replenishment processes are at work," he said. The rings of gas giants are made up of rocky debris from moons that have been torn apart by tidal waves or by an asteroid or comet collision during heavy bombardment periods. Rings are considered ephemeral and thought to disappear over time spans of billions of years. But Saturn's colorful rings appear to be younger than the planet itself, said scientists ? perhaps only 100 million years old, which is young in cosmological time. They also suspect that Saturn has had several ring systems in its history, although they have never had direct evidence on which to base their assumptions. "These observations are a first in solar system exploration," Shemansky said. "We have direct evidence now that the rings are made up of pure ice and that they are shaped by processes that happen fast," he added. "They aren't the same processes that shaped our solar system 4.5 billion years ago. "Given the fact that the outer rings are present at this time means that the system is being replenished by interactive plasma processes," Shemansky continued. "Clearly, the fact that something is eating up micron-sized grains in the outer ring zones at a high rate tells us that some sort of recycling process must be going on to rebuild them." Cassini's UV imaging spectrograph has made other significant observations. In the ultraviolet, scientists were able to see dust on the rings. Data showed variations in the amount of water-ice contained in the surfaces of ring particles, suggesting that darkened portions had been dusted with powder from pulverized moons or incoming meteoroids. The Cassini UVIS team also obtained ultraviolet images of Phoebe, Saturn's most distant large moon, during the inbound flight to Saturn. Data showed the absorption lines of water-ice on Phoebe's dark surface, which gave scientists more clues about its origins. The only moon in the Saturnian system to orbit in a retrograde, or backward, direction, Phoebe is similar to a common C-type carbonaceous asteroid. Scientists theorize that it was flung out of the Kuiper Belt, a region well beyond Neptune's orbit where thousands of small, icy comets reside, and sucked up by Saturn's strong gravitational field, but no one is absolutely sure of its origin. The Cassini-Huygens spacecraft and science instruments are part of an international mission by NASA, the European Space Agency and the Italian Space Agency to explore Saturn and its many moons and rings. 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.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle's last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Saturn's rotation is a puzzle NASA/JPL NEWS RELEASEPosted: June 28, 2004On approach to Saturn, data obtained by the Cassini spacecraft are already posing a puzzling question: How long is the day on Saturn? Credit: NASA/JPL/Space Science InstituteDownload larger image version Cassini took readings of the day-length indicator regarded as most reliable -- the rhythm of natural radio signals from the planet. The results give 10 hours, 45 minutes, 45 seconds (plus or minus 36 seconds) as the length of time it takes Saturn to complete each rotation. Here's the puzzle: That is about 6 minutes, or one percent, longer than the radio rotational period measured by the Voyager 1 and Voyager 2 spacecraft, which flew by Saturn in 1980 and 1981.Cassini scientists are not questioning Voyager's careful measurements. And they definitely do not think the whole planet of Saturn is actually rotating that much slower than it did two decades ago. Instead, they are looking for an explanation based on some variability in how the rotation deep inside Saturn drives the radio pulse.The radio sounds of Saturn's rotation, which are also the first sounds from Saturn studied by Cassini, are like a heartbeat and can be heard by visiting "The rotational modulation of radio emissions from distant astronomical objects has long been used to provide very accurate measurements of their rotation period," said Dr. Don Gurnett, principal investigator for the Cassini Radio and Plasma Wave Science instrument, University of Iowa, Iowa City. "The technique is particularly useful for the giant gas planets, such as Jupiter and Saturn, which have no surfaces and are covered by clouds that make direct visual measurements impossible."The first hint of something strange about that type of measurement at Saturn was in 1997, when a researcher from Observatoire de Paris reported that Saturn's radio rotation period differed substantially from Voyager. Dr. Michael D. Desch, Cassini Radio Plasma Wave Science team member, and scientist at NASA's Goddard Space Flight Center in Greenbelt, Md., has analyzed Saturn radio data collected by Cassini from April 29, 2003, to June 10, 2004. "We all agree that the radio rotation period of Saturn is longer today than it was in during the Voyager flyby in 1980," he said.Gurnett said, "Although Saturn's radio rotation period has clearly shifted substantially since the Voyager measurements, I don't think any of us could conceive of any process that would cause the rotation of the entire planet to actually slow down. So it appears that there is some kind of slippage between the deep interior of the planet and the magnetic field, which controls the charged particles responsible for the radio emission." He suggests the solution may be tied to the fact that Saturn's rotational axis is nearly identical to its magnetic axis. Jupiter, with a more substantial difference between its magnetic axis and its rotational axis, shows no comparable irregularities in its radio rotation period."This finding is very significant. It demonstrates that the idea of a rigidly rotating magnetic field is wrong," said Dr. Alex Dessler, a senior research scientist at the University of Arizona, Tucson. In that way, the magnetic fields of gas giant planets may resemble that of the Sun. The Sun's magnetic field does not rotate uniformly. Instead, its rotation period varies with latitude. "Saturn's magnetic field has more in common with the Sun than the Earth. The measurement can be interpreted as showing that the part of Saturn's magnetic field that controls the radio emissions has moved to a higher latitude during the last two decades," said Dressler."I think we will be able to unravel the puzzle, but it's going to take some time," said Gurnett. "With Cassini in orbit around Saturn for four years or more, we will be in an excellent position to monitor long-term variations in the radio period, as well as investigate the rotational period using other techniques."Cassini, carrying 12 scientific instruments, is just two days from its planetary rendezvous with Saturn. On June 30 it will become the first spacecraft to orbit Saturn, when it begins a four-year study of the planet, its rings and its 31 known moons. The spacecraft recently flew past Saturn's cratered moon Phoebe, where it captured spectacular images as well as data on its mass and composition.The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Office of Space Science, Washington, D.C. JPL designed, developed and assembled the Cassini orbiter.?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.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle's last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Saturn's swirl imaged CASSINI PHOTO RELEASEPosted: June 15, 2004 Credit: NASA/JPL/Space Science InstituteOn its approach to Saturn orbit insertion, the narrow angle camera on the Cassini spacecraft snapped this image of a turbulent swirl in the high clouds of Saturn's atmosphere. The disturbance occurs in the southern edge of the equatorial band. The image was taken on May 21, 2004, from a distance of 22 million kilometers (13.7 million miles) from Saturn through a filter centered at 889 nanometers. The image scale is 131 kilometers (81 miles) per pixel. Contrast in the image was enhanced to aid visibility. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Office of Space Science, Washington, D.C. The Cassini orbiter and its two onboard cameras, were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. 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.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle's last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Scientists await descent BY WILLIAM HARWOOD
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Page views was initially sent straight in the region with no motors ended up being allowed with Freeway 48 close Verona. Thursday any time your woman came across various law enforcement officials vehicles on the agenda powering the girl's. The lady pulled over to allow these folks go away, your woman claimed, as well as autos ceased once or t <a href=>canada goose chilliwack bomber price </a> wice just before ultimately preventing just about all targeted traffic during the sou <a href=>manitoba canada goose </a> thbound street on the Verona depart.

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Some people are dealing with charges after a pair of gentlemen ended up being in pain throughout an episode for a legitimate health develop operations in Pine Grove Weekend afternoon. The path is often a stalemate highway northern part of Telegraph Trail.

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ce need me personally to have the dying punishment,Inch he explained. "I want people to understand that I personally didn really want this particular to happen."

Your neighbors, Whilst gary Orvis, explained Mr. Bartlett resides alone as part of his property, they mentioned was initially designed over the last partners ages.

Mr. Brabant survivors consist of his particular mom and dad, Kenneth as well as Beat Brabant, involving 608 Webb E., Clayton. They couldn't become attained Friday with regard to opinion.

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Arizona Your FBI unveiled soin video recording in addition to images associated with Deep blue Backyard shooting Aaron Alexis regarding Sunday in addition to stated the guy imagined electromagnetic lake have been curbing him or her to get many weeks until the rampage in which killed 10 people today.

There are no signals that will Alexis, 24, had been targeting any individual inside October. 07 shooting within the Deep blue Lawn during south east Wa, reported Valerie Parlave, the particular Federal bureau of investigation associate movie director in charge of any Wa discipline office environment.

have realized relevant devices about their electrical mass media, which in turn referenced the actual delusional thought that he / she had been governed or maybe affected by particularly lower frequency electromagnetic waves within the past with three months, Parlave advised the headlines office meeting. Lugging some sort of back pack, droped straight enter <a href=>canada goose wear </a> ed your Naval Seashore Systems Demand constructing, website from the shootings, using a entrance.

This brief video recording additionally indicates Alexis, with a new Remington shotgun plus dressed in darkish clothes, climbing down any staircase and taking walks along passages in a crouch place, gun organised ready.

Men and women could be glimpsed at the conclusion of one particular arena. Alexis peeks all around four corners as well as, in some point, seeks the actual shotgun right room but isn't going to fire.

Parlave said Alexis, a federal modern technology specialist, had in his thing any shotgun, that had a new sawed off lens barrel and also stock, including a gun he or she attained during the taking pictures.

ELF System on the shotgun ended up any words and phrases, for the torment, precisely what b declare, out this way

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Additional coverage for subscribers:VIDEO:POST-LANDING NEWS CONFERENCE VIDEO:TRACKING CAMERAS FIRST SPOT CAPSULE DURING DESCENT VIDEO:GENESIS CAPSULE TUMBLES TO A HIGH-SPEED IMPACT VIDEO:SLOW-MOTION VIEW OF CAPSULE SLAMMING INTO GROUND VIDEO:AERIAL VIEWS OF CAPSULE HALF BURIED IN IMPACT CRATER VIDEO:RECOVERY HELICOPTERS TAKE OFF EARLIER IN THE DAY VIDEO:NARRATED ANIMATION SHOWS ORIGINAL RETURN PLAN THURSDAY, SEPTEMBER 9, 20040345 GMT (11:45 p.m. EDT Wed.)This collection of pictures recaps the Genesis solar wind sample return capsule making a high-speed impact into the Utah desert floor after its chutes failed to deploy during atmospheric descent from space on Wednesday. See gallery .0305 GMT (11:05 p.m. EDT Wed.)Genesis' science canister loaded with the solar wind samples was transported by helicopter from the impact site to a holding area next to a specially constructed cleanroom on the Utah base, NASA announced late Wednesday.Foil wrapping was removed from the canister and dirt brushed off before the canister was moved into the cleanroom for analysis of the contents. The Genesis team will begin examining the canister on Thursday morning.The capsule plunged into Earth's atmosphere at 1552:47 GMT (11:52:47 a.m. EDT) and entered the preplanned entry ellipse in the Utah Test & Training Range as predicted. However, the drogue chute and parafoil failed to deploy, causing the craft to smack the ground at a speed of 193 miles per hour. The impact occurred near Granite Peak on a remote portion of the range. No people or structures were anywhere near the area, NASA said.Meanwhile, NASA Administrator Sean O'Keefe released a statement on Wednesday's landing mishap:"We're encouraged by the news out of Utah, despite the hard impact landing of the Genesis Sample Return capsule. The spacecraft was designed in a way to give us the best chance at salvaging the valuable science payload should we suffer a landing like the one we witnessed today."Our re-entry plan was based on safety, and the choice of Dugway was intentional. While today's developments may be disappointing to some, I know the entire NASA family is thankful no one was injured."Exploration of the heavens is not an easy task. Our ability to travel throughout our solar system is limited, whether by human tended or robotic craft. Genesis was an experiment to journey far from home and return with new clues and possible answers to some of the fundamental questions regarding the origin of our universe."With each new mission, we push the frontiers of our knowledge and technology, and we're hopeful that what appears to be a setback, will eventually return some impressive results. After all, this isn't an Olympic event where we're awarded a medal for a perfect landing. Our final achievement will be measured by what we've learned over the entire three-year mission."Our scientists and engineers across NASA and our Jet Propulsion Laboratory are the best in the world. We will find out what happened to Genesis, and we'll continue our quest to accomplish the goals spelled out in our Vision for Space Exploration."WEDNESDAY, SEPTEMBER 8, 2004A small spacecraft carrying priceless samples of the sun crashed into the Utah desert today when its stabilizing parachute failed to deploy, bringing an innovative $264 million mission, NASA's first sample return flight since the Apollo moonshots, to a disappointing end. The Genesis sample return canister, carrying atoms from the sun that were blown into space as part of the solar wind, was to have been plucked out of mid air by a helicopter flown by a Hollywood stunt pilot over the Utah Test and Training Range. But a drogue chute needed to stabilize the craft before deployment of its large parafoil never fired and the craft slammed into the ground at about 193 mph. Video showed the canister half buried in the Utah desert, largely intact. It was carrying 20 to 30 micrograms of solar wind material, the equivalent of a few grains of salt. The atoms were embedded in fragile glass-like wafers. Read our full .2004 GMT (3:04 p.m. EDT)The recovery lead official says the 420-pound capsule is expected to be dug out by shovels and returned to the cleanroom later today.Workers will try to man-handle the craft into a cargo net for transport. If that is unsuccessful, they will attempt to extract the solar wind canister out of the capsule.1859 GMT (2:59 p.m. EDT)The project manager says there shouldn't be a total loss of mission science.1856 GMT (2:56 p.m. EDT)A spacecraft official says none of the pyrotechnics have fired. Therefore, the fault could involve the system used to sense the G-loads to trigger an onboard timer for deployment of chutes, or the electronics that sent commands to fire the pyros or loss of Genesis' battery power.1853 GMT (2:53 p.m. EDT)Teams at the impact site are working to safe and secure the unfired pyrotechnics and an onboard battery that could release sulfur dioxide.The capsule must be dug out of the ground. It will be decided later whether to remove the internal science canister holding the solar wind samples or attempt to keep the capsule in one piece to be ferried to nearby facilities.1850 GMT (2:50 p.m. EDT)With science canister cracked open, it remains unknown how useful the solar wind samples will be given the contamination from the Earth environment. Plans had called for the capsule to be recovered in mid-air and flown to a cleanroom to prevent contamination.1847 GMT (2:47 p.m. EDT)The director of helicopter flight operations was one of the people to inspect the capsule at the impact site. He says the capsule hit on its side and is half way buried into the desert floor. It is leaning 10 degrees from vertical.The chute deployment mortar did not fire.The capsule is "slightly breached" by a few inches from the impact, he said. The science portion of the capsule containing the solar wind samples appeared breach too.1843 GMT (2:43 p.m. EDT)The impact speed is estimated at 193 mph. The capsule landed within the targeted ellipse-shaped entry zone.1841 GMT (2:41 p.m. EDT)The news conference underway. NASA says an investigation board will be appointed within 72 hours. Precautions are being taken to handle the capsule because the ordnance used to deploy the chute and parafoil has not yet fired.1730 GMT (1:30 p.m. EDT)Soon after Genesis was launched in August 2001, engineers noticed potential problems with a battery in the probe's sample return canister. The canister crashed today in the Utah desert when it's stabilizing parachute failed to deploy. The cause of the mishap is not yet known and it may have nothing to do with the battery problem noted early in the mission. But for the record, here is part of a November 15, 2001, news release from the Jet Propulsion Laboratory that addressed the issue:Project managers are monitoring the temperature of the battery inside Genesis' sample return capsule to make sure that long-term heating does not impair its performance when the capsule returns to Earth in September 2004. Although the battery is likely to become hotter than originally expected, the flight team has a number of options for managing the battery's temperature, and they do not expect the issue to affect the mission.The mission's science requirements call for 22 months of solar wind particle collection. "In our current plan Genesis will meet and exceed that goal, collecting up to 26 months' worth of solar wind particles," said Chet Sasaki, Genesis project manager at NASA's Jet Propulsion Laboratory, Pasadena, Calif.The temperature of the lithium-dioxide battery is currently at 23 degrees Celsius (73 degrees Fahrenheit), within the range anticipated by spacecraft designers. A radiator device intended to shield the battery is not working as well as expected, however, and the battery is likely to heat up to 42 degrees Celsius (108 degrees Fahrenheit). Mission managers consider this temperature to be within acceptable limits. They note that similar batteries have been maintained at 60 degrees Celsius (140 degrees Fahrenheit) for 15 months without impairing their performance. Ground tests are being conducted on lithium batteries to measure their durability at various temperatures.The Genesis project team has been attempting to bake potential contaminants off the battery's radiator by heating the area. They are doing this with the spacecraft's sample return backshell opened just enough to allow gas trapped inside the capsule to escape, while still avoiding exposure to the Sun.1722 GMT (1:22 p.m. EDT)The NASA news conference from the Utah landing site is scheduled to begin at 1830 GMT (2:30 p.m. EDT).1633 GMT (12:33 p.m. EDT)A small spacecraft carrying priceless samples of the sun crashed into the Utah desert today when its stabilizing parachute failed to deploy, bringing an innovative $264 million mission, NASA's first sample return flight since the Apollo moonshots, to a disappointing end. Read our .NASA has ended its live video feed from the landing site. We will post additional information as it becomes available. A news conference is coming up later today.1630 GMT (12:30 p.m. EDT)Mission control reports the navigation and targeting of the capsule for reentry was on the mark. However, a failure aboard the capsule prevented the chute and parafoil to deploy. That resulted in the capsule's impact.NASA plans to hold a news conference later this afternoon.1627 GMT (12:27 p.m. EDT)Additional personnel are en route. They will safe the capsule for its removal from the impact crater.1625 GMT (12:25 p.m. EDT)There is nine people at the impact site now to survey the situation. One is taking up-close imagery.1624 GMT (12:24 p.m. EDT)Tracking teams are preserving all of their data for the failure investigation.1622 GMT (12:22 p.m. EDT)The recovery forces at the impact site report the chute never deployed. Therefore, they are treating the capsule as a "hot" craft since the mortar could still be armed. 1620 GMT (12:20 p.m. EDT)Here is what should have happened:Just over two minutes since entry interface the capsule would be at an altitude of 108,000 feet as a mortar aboard the capsule fired, releasing the 6.7-foot drogue parachute to provide stability to the capsule until the main chute is released. The capsule's heat shield will rapidly cool during this subsonic portion of the descent.About four minutes later, three pyrotechnic bolts were to release the drogue chute from the capsule at an altitude of about 22,000 feet. As the drogue chute moved away, it would extract the capsule's main chute, a 34.6- by 12.1-foot parafoil. Full inflation of the parafoil would occur in about 6 seconds. Once inflation is complete, the parafoil and its payload will begin a slow, loose spiral descent through the skies of the Utah Test & Training Range.However, the capsule was in a tumble and none of the chutes deployed to slow the capsule. That thwarted any mid-air recovery.1618 GMT (12:18 p.m. EDT)Mission control says the mortar may still be armed, having failed to fire during descent. Another scenario is the mortar fired and the drogue chute deployed only to break off as the craft plunged back to Earth.1617 GMT (12:17 p.m. EDT)Personnel are walking toward the capsule but keeping their distance due to concerns about the mortar being live.1615 GMT (12:15 p.m. EDT)The chopper crews have been told to be cautious. The mortar that should have fired on the capsule to deploy the chute may still be armed.1615 GMT (12:15 p.m. EDT)The recovery helicopters that were supposed to snag the returning Genesis capsule have now landed next to the capsule.1614 GMT (12:14 p.m. EDT)NASA officials hope there is enough of the capsule intact to determine what caused the chute deployment failure. Whether the solar wind samples will yield any science value remains to be seen. Scientists had said the samples had to be kept in ultra-clean conditions to preserve the information. However, the capsule is significantly broken as it sits on the desert floor after a high-speed impact.1610 GMT (12:10 p.m. EDT)Recovery forces are moving toward the capsule, which has made a very spectacular crater. 1609 GMT (12:09 p.m. EDT)An overhead view of the impact point shows the capsule half-buried on its side. The craft appears to be badly damaged.1605 GMT (12:05 p.m. EDT)There is no indication what might have caused Genesis' problem. NASA says there will be an investigation to determine why the speed-slowing chute and parafoil failed to deploy.1604 GMT (12:04 p.m. EDT)Mission control says without the drogue chute and subsequent parafoil, the capsule would hit the ground at about 100 mph.1602 GMT (12:02 p.m. EDT)NASA's Genesis sample return capsule has suffered a major anomaly during its homecoming today, failing to release its chute and parafoil to slow the descent for a mid-air recovery. The craft plunged into ground a high rate of speed. The status of the solar wind samples is not yet known.1601 GMT (12:01 p.m. EDT)The impact point is 40.07 degrees by 113.30 degrees in Utah.1559 GMT (11:59 a.m. EDT)The capsule is half buried into the ground. But it appears to be mainly intact.1558 GMT (11:58 a.m. EDT)IMPACT! The capsule has slammed into the Utah desert after failing to deploy its chute and parafoil.1557 GMT (11:57 a.m. EDT)The Genesis sample return capule is rapidly tumbling with no chute.1557 GMT (11:57 a.m. EDT)The capsule appears to be tumbling!1555 GMT (11:55 a.m. EDT)After one minute of atmospheric descent, the capsule should be at an altitude of 197,000 feet as the heat shield temperature reaches a peak temperature of 4,500 degrees F.Slightly over 10 seconds later, the capsule will be exposed to about 30 G's, the greatest deceleration it will endure during Earth entry. During this time period, the capsule's heat shield will lose an estimated about 7 pounds, or about 6 percent of its weight, as a small amount of the ablative material erodes away with the heat generated during entry through the atmosphere.1554 GMT (11:54 a.m. EDT)The capsule has been spotted high over the planet!The Genesis sample return capsule has hit the upper fringes of Earth's atmosphere 400,000 feet above the planet for its trek home. The capsule contains samples of the solar wind that were collected a million miles from Earth during the three-year Genesis mission.About 45 seconds after entry interface, the capsule will be exposed to a deceleration force threetimes the force of Earth gravity, or 3 G's. This arms a timer that is started when thedeceleration force passes back down through 3 G's. All of the parachute releases areinitiated from this timer. 1550 GMT (11:50 a.m. EDT)Tracking systems are operating to acquire the capsule as it falls back to Earth.As the capsule descends through the atmosphere, it will be "painted" by powerfulradars located on the Utah Test & Training Range. This will provide tracking informationallowing ground-based cameras to spot the capsule.Backup tracking is providedby a Global Positioning System unit on the Genesis capsule that transmitsposition data to a ground station, which in turn relays the information to the missioncontrol center.The radar, visual and GPS data will provide an accurate plot in threedimensions for the capsule's location. This plot is generated at the mission control centerlocated about 100 miles away from the range at Hill Air ForceBase. A ground control intercept officer based at the Hill Air Force Base mission controlwill direct helicopter flight crews towards the capsule.1545 GMT (11:45 a.m. EDT)Now 10 minutes from the time Genesis will begin atmospheric entry over northern Oregon. The capsule plunge to the atmosphere at a velocity of approximately 24,700 miles per hour. The only human-madeobject to re-enter Earth's atmosphere at a higher speed was the Apollo 10 commandmodule, which reached 24,861 mph.Genesis will be stabilize with its nose down because of the location of its center of gravity, its spin rate and its aerodynamic shape.1542 GMT (11:42 a.m. EDT)The primary capsule recovery chopper, called Vertigo, reports it is three minutes from reaching its standby position in the sky over Utah.1537 GMT (11:37 a.m. EDT)The helicopters are now 6,200 feet in altitude.1535 GMT (11:35 a.m. EDT)"The lead helicopter will deploy an 18-1/2-foot pole with what you could best describe as anoversized, space-age fishing hook on its end," said Roy Haggard, chief executive officerof Elsinore, Calif.-based Vertigo Inc. and director of helicopter flight operations. "When we make the approach we wantthe helicopter skids to be about eight feet above the top of the parafoil. If for some reasonthe capture is not successful, the second helicopter is 1,000 feet behind the firstone and setting up for its approach. We estimate we will have five opportunities toachieve capture."1533 GMT (11:33 a.m. EDT)A military Blackhawk helicopter is escorting the primary and backup capture helicopters. The three choppers are flying toward a spot 7.5 miles away from the recovery position at an altitude of 10,000 feet where they will wait for Genesis.1530 GMT (11:30 a.m. EDT)The capsule is currently high above the Pacific Ocean between Hawaii and the U.S. West Coast, mission control says. It is scheduled to hit the atmosphere for reentry in about 25 minutes.1525 GMT (11:25 a.m. EDT)Both the primary red-colored "Vertigo" helicopter and the backup blue-painted "South Coast" choppers have just taken off from their staging point in Utah. They will fly into position for the upcoming retrieval of Genesis. It is a beautiful, clear morning at the recovery zone.1520 GMT (11:20 a.m. EDT)The choppers have started up. Each specially outfitted helicopter has a three-person crew.1518 GMT (11:18 a.m. EDT)The pilots are making final preparations for takeoff. There are two helicopters ready to retrieve the Genesis capsule -- one primary and one backup. They will have time to make about 5 tries to grab the descending capsules.1515 GMT (11:15 a.m. EDT)To recap the events that occurred earlier this morning, here is NASA's overview:Sept. 8, 2004, will be a busy one for the Genesis team. It begins around 0800 GMTwhen NASA's Deep Space Network transmits a command to the spacecraft to initiate acomputer sequence that will later release the sample return capsule.About 1030 GMT, pyro devices will fire to sever two cable bundles connecting thespacecraft to the capsule, and the hinge connecting the two vehicles will retract.Starting about 1045 GMT, the spacecraft spins itself up to 10 revolutions perminute. The spinning will provide the unguided sample return capsule with additionalstability during entry. The spacecraft then rotates to the proper orientation for releaseand spins up to 15 revolutions per minute. Shortly thereafter, six push-off springs willpush the sample return capsule away from the spacecraft at a rate of 0.914 meters persecond (3 feet per second, or slightly over 2 miles per hour). Capsule release will takeplace at approximately 1153 GMT at an altitude of about 65,896 kilometers(40,946 miles).Approximately 22 minutes after separation, the Genesis spacecraft will fire its thrustersto reorient itself for a divert burn. This time lapse allows the sample return capsule tomove away from the spacecraft to avoid re-contact between the two.1500 GMT (11:00 a.m. EDT)The sample return capsule is barrelling toward Earth's atmosphere having successfully separated from the main body of the Genesis spacecraft earlier this morning. The capsule, which contains the precious collection of solar wind samples, has no propulsion system -- it is simply aimed to the precise trajectory "keyhole" for entry into the atmosphere with no way to abort the homecoming now.Mission navigators expect the capsule to hit the top of Earth's atmosphere at an altitude of 400,000 feet around 1555 GMT (11:55 a.m. EDT). The target "keyhole" is roughly 20.5 miles long and 6.2 miles wide over the Pacific Ocean. If the capsule enters the atmosphere anywhere inside this corridor, it will come down over the designated spot on the Utah Test & Training Range, NASA says.After its fiery plunge through the atmosphere, a series of chute and a large parafoil will slow the capsule in preparation for a mid-air recovery by a helicopter.TUESDAY, SEPTEMBER 7, 2004NASA's Genesis satellite completes its three-year, 20-million mile voyage through space in dramatic fashion Wednesday when a capsule containing samples of solar wind returns to Earth for a mid-air capture by Hollywood helicopter stunt pilots.The $260 million mission will bring back tiny particles that streamed from the Sun, allowing scientists to determine what was in the cloud of gas and dust from which the solar system formed 4.5 billion years ago.The Genesis sample return capsule will enter Earth's atmosphere at 1555 GMT (11:55 a.m. EDT) over Oregon. Two minutes and one time zone later, the capsule will deploy its drogue parachute at 108,000 feet over the vast alkali flats and sagebrush of the U.S. Air Force's Utah Test and Training Range. Waiting 97,000 feet below will be two helicopters and crew bearing the space-age equivalent of a fisherman's rod-and-reel, as NASA puts it."From the time the drogue deploys it will take about 18 minutes for the capsule to reach a height where we can get to it," said Genesis prime pilot Cliff Fleming of South Coast Helicopters, Santa Ana, Calif. "When we are up there that may feel like a long 18 minutes but we have been training for this moment since 1999, so in the grand scheme of things another quarter-hour or so shouldn't matter much."An important milestone in the mission was met Monday, when the Genesis spacecraft performed its final trajectory maneuver before capsule release. The spacecraft passed the Earth-Moon orbit at about 0900 GMT (8 a.m. EDT) Monday, traveling at about 2,700 miles per hour."Our Deep Space Network is allowing us to keep a close eye on our spacecraft and its samples of the Sun," said Genesis project manager Don Sweetnam of NASA's Jet Propulsion Laboratory in Pasadena, Calif. "It is right where we planned it to be. Everything is go. The navigators and engineers here at JPL are go, and the recovery team out in Utah is go, too."Genesis is NASA's first sample return mission since Apollo 17 returned the last of America's lunar samples to Earth in December 1972.According to current models, the solar system formed when a massive cloud of gas and dust collapsed under its own gravity. Most of this mass went into what became the Sun, while other gravitational disturbances in the collapsing nebula led to the formation of smaller bodies that eventually became planets, moons, asteroids, and comets. For years, scientists have sought to determine the composition of that original nebula and compare it to the composition of other solar system bodies to see how those bodies have evolved over time. The best way to do this is to study the composition of the Sun which, given its huge mass, is the body most likely to have retained its original composition. Scientists have already determined the Sun's composition to some by looking for the unique spectral signatures of elements embedded in sunlight. However, even the best spectroscopic observations do not provide planetary scientists with the precision they need to compare the Sun's composition with that of other solar system bodies. To accomplish this scientists need actual samples of the Sun they can study in the lab. While a mission to the Sun itself to obtain samples is not technically feasible, there is a far easier and less expensive alternative. The Sun emits a steady stream of particles known as the solar wind, made of material from the Sun's upper atmosphere. By collecting samples of the solar wind, one is essentially capturing the same material that made up the protosolar nebula. To accomplish this, Genesis launched in August 2001 and flew to the Earth-Sun L1 Lagrange point, about 1 million miles sunward of the Earth. This location, a common place for stationing spacecraft that study the Sun, is also free of the Earth's magnetic field, allowing Genesis to study the solar wind without interference. Genesis spent about two and a half years there, completing wide, looping halo orbits of L1. While there, the spacecraft deployed several ultra-pure wafers of gold, sapphire, silicon and diamond that were designed to capture particles entrained in the solar wind. Different collectors were to be used depending on whether the solar wind is fast or slow, or if a coronal mass ejection -- a type of solar storm -- is taking place. Ion and electron detectors on the spacecraft categorized the nature of the solar wind and determined what collector arrays should be deployed at a given time. In addition to the collector arrays, Genesis also carried a solar wind concentrator. This concentrator was designed to increase the concentration of oxygen and nitrogen ions collected by the spacecraft. Oxygen is of particular interest to scientists because they have measured different ratios of the most common oxygen isotope, O16, to two heavier versions, O17 and O18, on different solar system bodies, but do not know what the original oxygen isotope ratios were in the protosolar nebula. After completing its collection of the solar wind, Genesis left its L1 halo orbit in April. The spacecraft performed a distant flyby of the Earth and then circled the Earth-Sun L2 point, behind the Earth, to set up for a daytime reentry over the western U.S.Before it could touch down on Earth, however, the capsule will be captured in mid-air by helicopter so that the impact of landing does not damage the solar wind samples. Once on Earth, the samples will be taken to a special facility at NASA's Johnson Space Center, where scientists will study them with advanced laboratory equipment to determine their composition and draw conclusions about what was in the protosolar nebula. Scientists have high hopes that the solar wind returned by Genesis will help them resolve some key mysteries about the solar system."Genesis will return a small but precious amount of data crucial to our knowledge of the Sun and the formation of our solar system," said Donald Burnett, principal investigator of Genesis. 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STORY WRITTEN FOR & USED WITH PERMISSIONPosted: September 14, 2006Running behind schedule because of software problems, flight controllers early today began a slow, careful process to unfurl a new set of solar arrays aboard the international space station. The plan called for first deploying the huge panels just a few feet to let them warm up and decompress after years in storage. Later today, the Atlantis astronauts will send commands to fully extend the new arrays. The first section of solar wing was unfurled this morning. Credit: NASA TV/Spaceflight NowThe initial deployment had been planned for Wednesday night, but software problems held up checkout of a large rotary drive mechanism designed to rotate the new arrays 360 degrees to stay face on to the sun as the station circles the globe.One of two drive lock assembly - DLA - motors in the solar alpha rotary joint worked properly in an initial test, rotating the still-stowed arrays 180 degrees. But the drive gear in a redundant DLA appeared to be misaligned and testing was put on hold. Late last night, engineers traced the problem to a software commanding issue and after implementing a workaround, DLA-2 eventually moved the arrays through a 360-degree rotation as planned.Finally, at 5 a.m., the first set of arrays - 4A - began slowly unfurling on ground command as its self-assembling mast pulled the top few feet of folded solar cell blankets from its box. The other array, 2A, followed suit at 5:46 a.m.The Atlantis astronauts hope to complete solar array deployment later today in stages, sending commands to unfurl the panels first to 49 percent and then to a full 100 percent in what promises to be the most visually dramatic moment of the ongoing space station assembly mission.Here is an updated timeline of today's activities (NOTE: solar array deploy times are uncertain and not included; in EDT and mission elapsed time):12:15 AM041300STS/ISS crew wakeup03:35 AM041620EVA tool config05:40 AM041825ERCA troubleshooting06:10 AM041855Station robot arm reconfig06:45 AM041930Crew meals begin11:25 AM050010Canadian PAO event with Jett, MacLean11:45 AM050030Transfer tagup11:50 AM050035CNN, NPR interview Jett, Vinogradov, Williams11:50 AM050035Infrared camera setup12:10 PM050055EVA-3: Procedures review02:20 PM050305EVA-3: Campout mask pre-breathe (Tanner, Piper)03:05 PM050350EVA-3: Crew lock 10.2 depress03:45 PM050430ISS crew sleep begins04:15 PM050500STS crew sleep begins (Tanner, Piper in airlock)Each solar array wing is 15 feet wide and 115 feet long. Extending in opposite directions, the wings will stretch more than 240 feet from tip to tip when fully deployed. The so-called P4 array, or port 4 segment of the station's main power truss, is bolted to the SARJ mechanism on the outboard side of the P3 truss segment that also serves to route power and data to and from the solar panels.When completed, the space station's power truss will stretch more than a football field from end to end. Two huge solar arrays on each end of the truss will track the sun as the station circles the globe, rotating and changing pitch as required to maximize electrical generation.Finishing the main truss and wiring in the new arrays is a major element of near-term station assembly missions.One set of arrays, P6, is already attached to the station, providing power for the U.S. segment of the outpost. It is attached to the Z1 truss that extends upward from the Unity module at right angles to the main solar array truss. It will be moved next August to its final position next to the P4 arrays that were attached to the station Tuesday by Atlantis' crew.Two other sets of identical arrays will be mounted on the right side of the truss during shuttle assembly flights in February 2007 and June 2008.Designed by Boeing, the newly attached P4 truss features two motor-driven self-assesmbling masts designed to pull out a pair of solar blankets. For launch, the arrays are folded like venetian blinds in blanket boxes measuring 15 feet long but just 20 inches thick.The P3 truss was delivered to the Kennedy Space Center in November 1999. P4 followed suit in July 2000. The solar array blankets have not been unfolded since they were originally stowed for launch.Prior to Columbia's launch in January 2003, the arrays were certified to operate and deploy normally when stowed for up to 45 months. Because of the extended downtime after the Columbia accident, one of the blanket boxes on P4 was removed and shipped to California for deployment tests. A replacement blanket was installed aboard P4.As it turned out, the deployment tests went well and the blanket, which had been stowed 39 months at that point, worked normally. As a result, the certification age limit was boosted to 82 months. As of launch aboard Atlantis, the P4 blankets had been stowed for 67 and 73 months respectively.One other consequence of the Columbia recovery and subsequent launch delays was a decision to replace all 12 batteries in P4. The 372-pound batteries were swapped out in March and August of 2005.The solar array wings were designed by Lockheed Martin. They weigh more than 2,400 pounds and feature some 33,000 solar cells per blanket. They are designed to produce more power than the station actually needs to compensate for normal degradation as the outpost ages.The blankets must face the sun directly for maximum electrical generation and two mechanisms are in place to do just that. The wings can be rotated about their long axis by beta gimbal joints, much like the pitch of an airplane propeller can be adjusted. The SARJ, on the other hand, rotates the arrays through 360 degrees like a waterwheel around the axis of the main truss.The P4 integrated equipment assembly, or IEA, is a cube measuring 16 feet on a side and weighing nearly 17,000 pounds. It includes direct current converters, 12 batteries, battery chargers, control computers and an ammonia cooling system to keep the electronic gear at the proper temperature. A single set of folding radiator panels will extend 44 feet when fully deployed.Most of the work to ready the new P4 arrays for extension "is done by the flight control team," Jett said. "The EVA crew does the physical work, in terms of, positioning the arrays and releasing all the bolts and the launch restraints. But then the preparation to actually make the deployment happen, all the activation sequence and the activation of the rotary joint, is all performed by the ground team."The P4 arrays are identical to P6, which was attached to the space station during shuttle mission STS-97 in December 2000. When the first blanket was deployed, engineers were surprised to see several of the blanket panels had stuck together. When they jerked free, a tensioning cable jumped its guides and required repairs on a subsequent spacewalk. For the second array's deployment, the crew let the sun warm up the array and deployed it in a so-called high-tension mode. That technique worked, and the array unfurled without incident.For the P4 deploy, the arrays will first be extended the length of a single bay of each mast - a few feet worth - to relieve compression and to begin warming up the panels."The one-bay deploy is basically to start the relaxation of the blankets and to get ahead," station flight director John McCullough said Wednesday. "The time we're in an inertial attitude, the attitude where we continuously point the arrays at the sun, is limited because the rest of the space station doesn't really like that atitude."For this deploy, we want to have the sun in a certain cone to warm the back of the blankets and there's a limit to that. We can only be there for three revs around the Earth."Working in stages, the astronauts will extend the 4A mast to a distance of 49 percent early Thursday, wait a half hour or so for additional solar heating, and then the rest of the way to full extension. They will repeat that process for the 2A mast. It will take about 90 minutes for each panel to fully deploy."We're not too terribly concerned about stiction on the deploy," said Tanner, a veteran of the STS-97 mission. "We know it might happen in certain panels. The team went hard to work after STS-97 to figure out the mechanism of stiction and what we can do to reduce it. They came up with a good operational plan to nominally deploy."Now if for some reason one or two panels sticks after all that, then we can go out EVA, it would be on EVA 3, and actually manually peel the panels apart for the first 40 inches or so and doing a nominal deploy after that. All of our tests say they will peel open very easily. So we're not too terribly concerned about that."Space station Program Manager Mike Suffredini agreed that experience gained during the STS-97 mission in 2000 should result in a smooth deploy."The good news is we've done it twice before," Suffredini said. "The first time we deployed one of these arrays, we learned about a stiction issue that existed. After quite a bit of work during that mission, we deployed the second array in a little bit different technique, which allowed us to be successful. We learned a lot about techniques to get these arrays out without having the tension wire come loose, which is what happened when we tried to deploy the first one. It turns out after a lot of work ... we figured out a fix to go back in there to put it back in its original condition. And of course, the arrays have been fine ever since.Using an engineering model, "we did quite a bit of testing on this stiction issue and how these arrays can stick together based on the silicon bead that's on the arrays and then we compress them for long periods of time before they go fly. And that was basically the cause of the problem. Over a long period of time this silicon would tend to attach itself to the back part of the array. And so we've done a number of things, largely operational changes but also on how we dealt with the arrays."While the arrays were compressed for shipment to Florida, that pressure was relaxed until shortly before final preparations."Probably the largest changes were operational," Suffredini said. "We will partially deploy the array about one bay's worth and we'll let it warm up and sort of expand a little bit. Then the actual deploy process a little bit later will have us deploy the array halfway and then you'll see us sit for about 30 minutes as we warm it up and then we'll go the rest of the way."In addition to that, we're using what we call a high-tension mode. Instead of leaving the lower part of the array free to move up and down as the array gets deployed, we learned we need to hold it down against the bottom of the blanket box. So the new technique holds it down and then this particular deploy lets the heat warm things up, to allow the silicon to free itself, is the process we'll use to deploy. I have a lot of confidence in the deployment of the arrays."The new solar arrays will not be rotated on the SARJ because of interference with the port wing of the P6 array and they will not provide any power to the space station until reconfigurations during the next shuttle mission in December.For readers interested in a bit more detail, here is an overview provided by Boeing, the prime contractor.Source: BoeingElectrical power is the most critical resource for the ISS because it allows astronauts to live comfortably, safely operate the station, and perform complex scientific experiments. Since the only readily available source of energy for spacecraft is sunlight, technologies were developed to efficiently convert solar energy to electrical power. One way to do this is by using large numbers of solar cells assembled into arrays to produce high power levels. The cells are made from purified crystal ingots of silicon that directly convert light to electricity through a process called photovoltaics. Solar cells do the job, but a spacecraft orbiting the Earth is not always in direct sunlight so energy has to be stored. Storing power in rechargeable batteries provides a continuous source of electricity while the spacecraft is in the Earth's shadow.NASA and Lockheed Martin developed a method of mounting the solar arrays on a "blanket" that can be folded like an accordion for delivery to space. Once in orbit, astronauts deploy the blankets to their full size. Gimbals are used to rotate the arrays so that they face the Sun to provide maximum power to the Space Station. The solar arrays track the sun in two axes: beta and alpha.P4 is the second of four PVMs that will eventually be brought up to the International Space Station, converting sunlight to electricity. The first one, named P6, was brought on orbit by the STS-97 crew in November 2000. The primary functions of the P4 photovoltaic module are to collect, store, convert and distribute electrical power to loads within the segment and to other ISS segments. The P4 PVM consists of two beta gimbal/PV array assemblies, two beta gimbal transition structures, one integrated equipment assembly and associated cabling and tubing. The P4 PVM components were assembled by Boeing in Tulsa, Okla. and Lockheed Martin in Sunnyvale, Calif. prior to final assembly and testing by Boeing at Kennedy Space Center, Fla.There are two solar array wings (SAW) designed, built and tested by Lockheed Martin in Sunnyvale, Calif. on the P4 module, each deployed in the opposite direction from each other. Each SAW is made up of two solar blankets mounted to a common mast. Prior to deployment, each panel is folded accordion style into a solar array blanket box (SABB) measuring 20 inches high and 15 feet in length. Each blanket is only about two inches thick while in this stored position. The mast consists of interlocking battens which are stowed for launch inside a mast canister assembly (MCA) designed, built and tested by ATK-Able. When deployed by the astronauts, the SAW deploys like an erector set as it unfolds. It has two arms like a human torso when mounted on P4 which are rotated outwards by astronauts during a spacewalk so they can be fully deployed. Because these blankets were stored for such a long time, NASA, Boeing and Lockheed Martin conducted extensive testing to ensure they would unfold properly once on orbit to ensure there would be no problems with the blankets sticking together. This testing was completed in July 2003.When fully deployed, the SAW extends 115 feet and spans 38 feet across and extends out to each side of the integrated equipment assembly. Since the second SAW is deployed in the opposite direction, the total wing span is over 240 feet.Each solar array wing weighs over 2,400 pounds and use nearly 33,000 (32,800 per wing) solar array cells, each measuring 8-cm square with 4,100 diodes. The individual cells were made by Spectrolab and ASEC. There are 400 solar array cells to a string and there are 82 strings per wing. Each SAW is capable of generating nearly 32.8 kilowatts (kW) of direct current power. There are two SAWs on the P4 module yielding a total power generation capability approaching 66 kW, enough power to meet the needs of 30 average homes without air conditioning (based on an average 2kW of power).Additional coverage for subscribers:VIDEO:PORT 3/PORT 4 TRUSS KEEL PIN REMOVED AND STOWED VIDEO:HELMETCAM OF BURBANK REMOVING SARJ RESTRAINT VIDEO:SPACEWALKERS PAUSE FOR PICTURE TIME VIDEO:STEVE MACLEAN REPORTS LOST BOLT VIDEO:ROTARY JOINT LOCK REMOVED BY SPACEWALKER VIDEO:STEP-BY-STEP PREVIEW OF SPACEWALK NO. 2 VIDEO:POST-EVA 1 STATUS BRIEFING VIDEO:TANNER LOSES BOLT DURING ROTARY JOINT WORK VIDEO:PIPER UNFOLDS SOLAR BLANKET BOXES VIDEO:SECOND WING'S STRUCTURE DEPLOYED BY PIPER VIDEO:FIRST SOLAR WING'S STRUCTURE DEPLOYED BY TANNER VIDEO:STEP-BY-STEP PREVIEW OF SPACEWALK NO. 1 VIDEO:TRUSS HANDED FROM SHUTTLE ARM TO STATION ARM VIDEO:ARM MANEUVERS TRUSS OVER SHUTTLE WING VIDEO:TRUSS SLOWLY LIFTED OUT OF PAYLOAD BAY VIDEO:ATLANTIS' ARM GRAPPLES THE TRUSS VIDEO:MONDAY'S MISSION STATUS BRIEFING VIDEO:ATLANTIS WELCOMED ABOARD THE STATION VIDEO:DOCKING REPLAY FROM CAMERA ON SHUTTLE ARM VIDEO:SHUTTLE ATLANTIS DOCKS TO THE STATION VIDEO:ATLANTIS' BREATH-TAKING FLIP MANEUVER VIDEO:CREW'S CAMCORDER FOOTAGE OF EXTERNAL TANK VIDEO:NARRATED ANIMATION PREVIEWING TRUSS UNBERTHING VIDEO:NARRATED ANIMATION PREVIEWING THE DOCKING VIDEO:NARRATED ANIMATION OF PAYLOAD BAY CONFIGURATION MORE: VIDEO:BRIEFING ON TANK'S PERFORMANCE VIDEO:TANK'S ONBOARD CAMERA LIFTOFF TO SEPARATION VIDEO:FLIGHT DIRECTOR EXPLAINS INSPECTIONS VIDEO:SUNDAY'S MISSION STATUS BRIEFING VIDEO:LAUNCH OF ATLANTIS! VIDEO:SHEDDING FOAM MAY HAVE HIT ATLANTIS VIDEO:ONBOARD VIEW OF EXTERNAL TANK SEPARATION VIDEO:INSIDE MISSION CONTROL DURING LAUNCH VIDEO:STATION CREW TOLD VISITORS EN ROUTE VIDEO:HOUSTON RADIOS DEBRIS REPORT TO CREW VIDEO:POST-LAUNCH NEWS CONFERENCE VIDEO:QUICK-LOOK BRIEFING ON DEBRIS LAUNCH REPLAYS:VIDEO:BEACH MOUND TRACKER VIDEO:CAMERA IN FRONT OF PAD VIDEO:BANANA CREEK VIEWING SITE VIDEO:VEHICLE ASSEMBLY BUILDING ROOF VIDEO:PAD 39B SIDE PERIMETER VIDEO:PLAYALINDA BEACH TRACKER VIDEO:PLAYALINDA BEACH ZOOM VIDEO:UCS 23 TRACKER VIDEO:UCS 11 TRACKER VIDEO:MISSION SPECIALIST 4 STEVE MACLEAN BOARDS ATLANTIS VIDEO:MISSION SPECIALIST 3 HEIDE PIPER BOARDS VIDEO:MISSION SPECIALIST 2 DAN BURBANK BOARDS VIDEO:MISSION SPECIALIST 1 JOE TANNER BOARDS VIDEO:PILOT CHRIS FERGUSON BOARDS VIDEO:COMMANDER BRENT JETT BOARDS VIDEO:ASTRONAUTS EMERGE FROM CREW QUARTERS VIDEO:CREW SUITS UP FOR LAUNCH TO SPACE VIDEO:FINAL INSPECTION TEAM CHECKS ATLANTIS VIDEO:ASTRONAUTS READY FOR SECOND LAUNCH TRY MORE: STS-115 patchThe official crew patch for the STS-115 mission of space shuttle Atlantis to resume orbital construction of the International Space Station.Choose your 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. 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Discovery's external fuel tank, the subject of extensive insulation design changes in the wake of the 2003 Columbia disaster, is scheduled to arrive at the spaceport around Jan. 5.Columbia was destroyed because of wing leading edge damage caused by a chunk of insulating foam that broke off the ship's external fuel tank during launch. During entry, hot gas ate its way into the left wing's interior, triggering structural failure 37 miles above Texas.The foam in question, used to insulate the fittings that help attach a shuttle's nose to the tank, has been removed and replaced with heaters to prevent dangerous ice buildups. Other changes have been implemented to minimize roam shedding from other areas of the huge tank."I think we have done a very thorough job of working our way through the understanding of how debris is liberated, understanding what sizes will come off, how that debris is transported through the air stream and how it might impact the orbiter," William Parsons, shuttle program manager at the Johnson Space Center in Houston, told reporters today. "So I'm feeling very confident we have our arms around this."But what we have to do is, we have to verify that. And the best way to verify that is to fly a mission. So we're going to go fly a couple of test missions and we're going to take a lot of imagery and we're going to do a lot of inspections and we're going to have sensors in place so that we can verify what we feel very confident that we've accomplished."Wayne Hale, a former flight director who now serves as Parsons' deputy and chairman of the mission management team, said today the requirement is for nothing to come off the tank that weighs more than 0.03 pounds."All our investigations of the foam indicate we will not get a piece of foam coming off bigger than .008, eight one thousandths (of a pound), or almost an order of magnitude smaller than the requirement," he said. "Now, does that mean we won't see a chip in a tile here or there? I would say we'd be optimistic if we said that."But we're clearly moving toward an area where we expect to see much less damage in the tile and no critical damage that will require a repair. So that's our goal in this and it's beginning to look very positive that we'll be able to accomplish that level of control on the ET foam."Parsons said engineers are still wrestling with one aspect of the tank's redesigned insulation - an area around a bellows in a liquid oxygen feed line - but he is optimistic the tank will ship on time. He said any additional work in that area can be performed at Kennedy.Along with minimizing potential debris, NASA has installed sensors behind the shuttle's wing leading edge panels that will detect any significant impacts. Upgraded cameras on the ground and aboard the shuttle will document whatever foam shedding does occur and the astronauts will carry out an exhaustive leading edge inspection in space using cameras and laser sensors mounted on a long boom.But NASA is struggling to perfect techniques for spacewalking astronauts to repair tile or leading edge damage in space in the event such damage actually occurs.Agency managers earlier said certified repair techniques for reinforced carbon carbon leading edge panels likely would not be available in time for STS-114. Such repair techniques were not considered a requirement for flight. That was due in large part to a new capability for the crew of a stricken shuttle to use the space station as a "safe haven" until a rescue flight could be launched.Today, Parsons and Hale said the same philosophy will apply to tile repair. While engineers are continuing efforts to perfect repair techniques, and while two astronauts will carry out tests of those procedures, a certified methodology is not a pre-launch requirement for STS-114."When we started this, we knew it would be extremely difficult to do a repair technique both on tile and on RCC," Parsons said. "I think we said that from the very beginning. The CAIB (Columbia Accident Investigation Board) said to do the best that we could to come up with some technique to repair RCC and repair tile. We have done that. We have continued to put the best and brightest this agency has to offer on this, we've used every resource this agency and this nation has to work on this, we've made a lot of progress."In recent weeks, engineers have raised questions about the possibility of air bubbles forming in the tile repair material that could degrade its performance during entry."We think there are some issues that we still need to resolve, but we still have some time to go resolve that," Parsons said. "And then we're going to go fly a test mission. We're going to have a detailed (repair demonstration spacewalk) in the payload bay of the orbiter. ... We can do a lot of things on the ground, but we have to take them on orbit, put them in work on orbit, bring them back and then see if they work as well as we think they'll work."In a state of emergency, we would have a technique that we would be ready to perform (during STS-114)," he said. "But right at this moment, we're still working through some of the technical details on how to do good tile repair and RCC repair."Pressed to say whether on-orbit repair capability of both RCC and tile were, or were not, launch constraints, Hale said "The Columbia Accident Investigation Board did not say it was a requirement."Parsons added, "but they did say to work on it and they did say to do the best that we could and I think what Wayne's telling you is we have done the best that we could. We have made a lot of progress and we think we'll have something there that we can use and test on STS-114."For the record, the Columbia Accident Investigation Board said that for missions to the international space station, NASA should "develop a practicable capability to inspect and effect emergency repairs to the widest possible range of damage to the thermal protection system, including both tile and reinforced carbon carbon, taking advantage of the additional capabilities available when near to or docked at the international space station."Hale stressed that NASA will not be driven by target launch dates and that Discovery will not fly until the agency's management team is convinced it is safe to do so."We are going to fly when we have determined that the vehicle is ready to fly, when it is safe to fly," he stressed. "We're not being driven by a calendar date, we're being driven by our readiness to go fly. So when we are convinced the external tank is in a good situation, when we are convinced we have the warning devices, the OBSS (inspection boom) and all those other things, wing leading edge sensors, all installed, checked out and ready to go, when we are convinced we have an adequate repair capability, then we'll go fly."The date will kind of be what the date is," he added. 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Find out how to get your . Test firingA full-scale space shuttle solid rocket booster is fired in Utah to conduct 76 test objectives, including a modification that slightly changes the shape of the propellant in a segment of the motor. (2min 11sec file)Side shotThis side-view shows the entire duration firing of the shuttle SRB. (2min 19sec file) Front viewA camera mounted near the booster's nose provides this stunning view of the test firing. (2min 21sec file)Nozzle viewThis remarkable footage shows a close-up view of the booster nozzle as it moves during the firing. (2min 22sec file) Long-range viewA more picturesque view of the firing is captured by this camera located away from the firing site. 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