Kennedy Space Center Gearing Up for November 1 launch

Technicians at NASA's Kennedy Space Center in Florida are servicing the solid rocket booster hydraulic power units as the space shuttle Discovery stack is readied for launch. Liftoff remains targeted for Nov. 1 at 4:40 p.m. EDT. The remnants of Tropical Storm Nicole passed well offshore from Kennedy and aren't affecting operations at the center. Discovery's processing at the pad also was not affected by the storm. At NASA's Johnson Space Center in Houston, the STS-133 crew will perform a bench review of flight crew equipment.

New cosmic phenomenon termed Coreshine

Astronomers have discovered a new, cosmic phenomenon, termed "coreshine," which is revealing new information about how stars and planets come to be.

The scientists used data from NASA's Spitzer Space Telescope to measure infrared light deflecting off cores -- cold, dark cocoons where young stars and planetary systems are blossoming. This coreshine effect, which occurs when starlight from nearby stars bounces off the cores, reveals information about their age and consistency. In a new paper, to be published Friday, Sept. 24, in the journal Science, the team reports finding coreshine across dozens of dark cores.

"Dark clouds in our Milky Way galaxy, far from Earth, are huge places where new stars are born. But they are shy and hide themselves in a shroud of dust so that we cannot see what happens inside," said Laurent Pagani of the Observatoire de Paris and the Centre National de la Recherche Scientifique, both in France. "We have found a new way to peer into them. They are like ghosts because we see them but we also see through them."

Pagani and his team first observed one case of the coreshine phenomenon in 2009. They were surprised to see that starlight was scattering off a dark core in the form of infrared light that Spitzer could see. They had thought the grains of dust making up the core were too small to deflect the starlight; instead, they expected the sunlight would travel straight through. Their finding told them that the dust grains were bigger than previously thought -- about 1 micron instead of 0.1 micron (a typical human hair is about 100 microns).

That might not sound like a big difference, but it can significantly change astronomers' models of star and planet formation. For one thing, the larger grain size means that planets -- which form as dust circling young stars sticks together -- might take shape more quickly. In other words, the tiny seeds for planet formation may be forming very early on, when a star is still in its pre-embryonic phase.

But this particular object observed in 2009 could have been a fluke. The researchers did not know if what they found was true of other dark clouds -- until now. In the new study, they examine 110 dark cores, and find that about half of them exhibit coreshine.

The finding amounts to a new tool for not only studying the dust making up the dark cores, but also for assessing their age. The more developed star-forming cores will have larger dust grains, so, using this tool, astronomers can better map their ages across our Milky Way galaxy. Coreshine can also help in constructing three-dimensional models of the cores -- the deflected starlight is scattered in a way that is dependent on the cloud structures.

Said Pagani, "We're opening a new window on the realm of dark, star-forming cores."

Other authors are Aurore Bacmann of the Astrophysics Laboratory of Grenoble, France, and Jürgen Steinacker, Amelia Stutz and Thomas Henning of the Max-Planck Institute for Astronomy, Germany. Steinacker is also with the Observatoire de Paris, and Stutz is also with the University of Arizona, Tucson.

The Spitzer measurements are based on data from the mission's public archive, taken before the telescope ran out of its liquid coolant in May 2009 and began its current warm mission.

New Images of Saturn's Aurora

A new movie and images showing Saturn's shimmering aurora over a two-day period are helping scientists understand what drives some of the solar system's most impressive light shows.

The new, false-color images and video are available online at: http://www.nasa.gov/cassini and http://saturn.jpl.nasa.gov

The movie and images are part of a new study that, for the first time, extracts auroral information from the entire catalogue of Saturn images taken by the visual and infrared mapping spectrometer instrument (VIMS) aboard NASA's Cassini spacecraft. These images and preliminary results are being presented by Tom Stallard, lead scientist on a joint VIMS and Cassini magnetometer collaboration, at the European Planetary Science Congress in Rome on Friday, Sept. 24.

In the movie, the aurora phenomenon clearly varies significantly over the course of a Saturnian day, which lasts around 10 hours 47 minutes. On the noon and midnight sides (left and right sides of the images, respectively), the aurora can be seen to brighten significantly for periods of several hours, suggesting the brightening is connected with the angle of the sun. Other features can be seen to rotate with the planet, reappearing at the same time and the same place on the second day, suggesting that these are directly controlled by the orientation of Saturn's magnetic field.

"Saturn's auroras are very complex and we are only just beginning to understand all the factors involved," Stallard said. "This study will provide a broader view of the wide variety of different auroral features that can be seen, and will allow us to better understand what controls these changes in appearance."

Auroras on Saturn occur in a process similar to Earth's northern and southern lights. Particles from the solar wind are channeled by Saturn's magnetic field toward the planet's poles, where they interact with electrically charged gas (plasma) in the upper atmosphere and emit light. At Saturn, however, auroral features can also be caused by electromagnetic waves generated when the planet's moons move through the plasma that fills Saturn's magnetosphere.

Previous data from Cassini have contributed to a number of detailed snapshots of the aurora. But understanding the overall nature of the auroral region requires a huge number of observations, which can be difficult because Cassini observation time close to Saturn is in high demand, Stallard said.

However, VIMS observations of numerous other scientific targets also include auroral information. Sometimes the aurora can be clearly seen, but sometimes Stallard and colleagues add multiple images together to produce a signal. This wide set of observations allows Cassini scientists to understand the aurora in general, rather than the beautiful specific cases that dedicated auroral observations allow, Stallard said.

Stallard and his colleagues have investigated about 1,000 images from the 7,000 that VIMS has taken to date of Saturn's auroral region.

The new, false-color images show Saturn's aurora glowing in green around the planet's south pole. The auroral information in the two images was extracted from VIMS data taken on May 24, 2007, and Nov. 1, 2008. The video covers about 20 Earth hours of VIMS observations, from Sept. 22 and 23, 2007.

"Detailed studies like this of Saturn's aurora help us understand how they are generated on Earth and the nature of the interactions between the magnetosphere and the uppermost regions of Saturn's atmosphere," said Linda Spilker, Cassini project scientist, based at NASA's Jet Propulsion Laboratory, Pasadena, Calif.

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. JPL manages the mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter was designed, developed and assembled at JPL. The visual and infrared mapping spectrometer team is based at the University of Arizona, Tucson. Stallard's work on Saturn's auroras is funded by the Science and Technologies Facilities Council, Swindon, U.K.

Expedition 24 Crew Successfully Return to Earth

Expedition 24 Commander Alexander Skvortsov and Flight Engineers Tracy Caldwell Dyson and Mikhail Kornienko landed their Soyuz TMA-18 spacecraft in Kazakhstan on Saturday, Sept. 25, wrapping up a six-month stay aboard the International Space Station.

Skvortsov was at the controls of the spacecraft as it undocked at 10:02 p.m. EDT Friday from the Poisk docking port on the station's Zvezda module, a day later than planned because of a Poisk-side hatch sensor problem Thursday night. That problem prevented hooks on the Poisk side of the docking interface from opening, resulting in a one-day landing delay.

Following undocking and a normal descent, the crew landed at 1:23 a.m. near Arkalyk, Kazakhstan, as the station orbited 220 miles above over the Pacific Ocean off the coast of Japan.

Russian recovery teams were on hand to help the crew exit the Soyuz vehicle and adjust to gravity after 176 days in space. Skvortsov and Kornienko will return to the Gagarin Cosmonaut Training Center in Star City, outside of Moscow. Caldwell Dyson will return to Houston aboard a NASA plane.

The trio launched aboard the Soyuz TMA-18 spacecraft from the Baikonur Cosmodrome in Kazakhstan in April. As members of the Expedition 23 and 24 crews, they spent 174 days on the station. Caldwell Dyson and Expedition 25 Commander Doug Wheelock conducted three spacewalks to replace a faulty cooling pump module on the station’s truss structure. Kornienko conducted one spacewalk to perform assembly work on the Russian segment of the complex.

The station is now occupied by Wheelock, who assumed command of the station Wednesday, NASA Flight Engineer Shannon Walker and Russian Flight Engineer Fyodor Yurchikhin, who arrived in mid-June.

A new trio of Expedition 25 crew members, NASA’s Scott Kelly, Alexander Kaleri and Oleg Skripochka, will launch from the Baikonur Cosmodrome on Oct. 7, U.S. time and will arrive on the station about 48 hours later.

The Soyuz TMA-18 spacecraft Landing

The Soyuz TMA-18 spacecraft is seen as it lands with Expedition 24 Commander Alexander Skvortsov and Flight Engineers Tracy Caldwell Dyson and Mikhail Kornienko near the town of Arkalyk, Kazakhstan on Saturday, Sept. 25, 2010. Russian Cosmonauts Skvortsov and Kornienko and NASA Astronaut Caldwell Dyson, are returning from six months onboard the International Space Station where they served as members of the Expedition 23 and 24 crews.

Your Face in Space

NASA wants to put a picture of you on one of the two remaining space shuttle missions and launch it into orbit. To launch your face into space and become a part of history, just follow the link below:
https://faceinspace.nasa.gov/index.aspx

Jupiter is approaching Earth

Been outside at midnight lately? There's something you really need to see. Jupiter is approaching Earth for the closest encounter between the two planets in more than a decade--and it is dazzling.

The night of closest approach is Sept. 20-21st. This is also called "the night of opposition" because Jupiter will be opposite the sun, rising at sunset and soaring overhead at midnight. Among all denizens of the midnight sky, only the moon itself will be brighter.

Earth-Jupiter encounters happen every 13 months when the Earth laps Jupiter in their race around the sun. But because Earth and Jupiter do not orbit the sun in perfect circles, they are not always the same distance apart when Earth passes by. On Sept. 20th, Jupiter will be as much as 75 million km closer than previous encounters and will not be this close again until 2022.

The view through a telescope is excellent. Because Jupiter is so close, the planet's disk can be seen in rare detail--and there is a lot to see. For instance, the Great Red Spot, a cyclone twice as wide as Earth, is bumping up against another storm called "Red Spot Jr." The apparition of two planet-sized tempests grinding against one another must be seen to be believed.

Also, Jupiter's trademark South Equatorial Belt (SEB) recently vanished, possibly submerging itself beneath high clouds. Researchers say it could reappear at any moment. The dramatic resurgence would be accompanied by a globe-straddling profusion of spots and cloudy swirls, clearly visible in backyard telescopes.

And what was that flash? Amateur astronomers have recently reported a surprising number of fireballs in Jupiter's atmosphere. Apparently, many small asteroids or comet fragments are hitting the giant planet and exploding among the clouds. Researchers who have studied these events say visible flashes could be occurring as often as a few times a month.

Finally, we mustn't forget the moons of Jupiter because they are also having a close encounter with Earth. These are planet-sized worlds with active volcanoes (Io), possible underground oceans (Europa), vast fields of craters (Callisto), and mysterious global grooves (Ganymede). When Galileo discovered the moons 400 years ago, they were no more than pinpricks of light in his primitive spy glass. Big, modern amateur telescopes reveal actual planetary disks with colorful markings.

It makes you wonder, what would Galileo think?

Expedition 24 Crew Members Prepare for landing on Friday in Kazakhstan

Expedition 24 Commander Alexander Skvortsov and Flight Engineers Tracy Caldwell Dyson and Mikhail Kornienko spent Monday preparing for their departure Thursday from the International Space Station. They packed items to be returned to Earth in their Soyuz TMA-18 spacecraft, reviewed deorbit and landing procedures and checked out their Sokol launch and entry suits.

Once they undock, Expedition 25 will begin its increment with Commander Doug Wheelock and Flight Engineers Shannon Walker and Fyodor Yurchikhin continuing their stay on the station. Skvortsov will ceremonially hand command of the station over to Wheelock Wednesday afternoon.

NASA Astronaut Scott Kelly and Russian Cosmonauts Alexander Kaleri and Oleg Skripochka will join Expedition 25 as flight engineers when they dock in the new Soyuz TMA-01M spacecraft next month.

Walker set up equipment for the Anomalous Long Term Effects in Astronauts' Central Nervous System experiment. Also known as ALTEA, the experiment uses several diagnostic technologies to measure the effect of the exposure of crew members to cosmic radiation. Specifically, ALTEA was set up Monday to measure the effectiveness of materials on the orbital complex designed to shield the crew from this radiation.

Meanwhile, Kornienko assisted Skvortsov in a session with the Russian Pilot-M experiment. Pilot-M tests piloting skill in simulations on a laptop under stopwatch control and studies the response of cosmonauts to the effects of stress factors in flight.

Yurchikhin worked with the Matryoshka-R experiment. The Russian payload is designed for sophisticated radiation studies and is named after the traditional Russian set of nested dolls.

Wheelock installed a cable that will send power to the Pressurized Multipurpose Module when it is delivered by the STS-133 crew aboard space shuttle Discovery later this year.

Caldwell Dyson set up the U.S. Sound Level Meter and performed an acoustic survey of the station, the data from which she later downloaded to controllers on the ground.

Come to the NASA Goddard Visitor Center for celebrating International Observe the Moon Night

Come to the NASA Goddard Visitor Center on Saturday, September 18, 2010 from 6:30 pm – 10:00 pm for a fun-filled evening celebrating International Observe the Moon Night. Enjoy guest speakers, hands-on activities, laser ranging facility tours*, a public unveiling of Lunar Reconnaissance Orbiter (LRO) images, and of course, Moon observations! Learn why the Moon goes through phases, how it came to look like it does today, and what we’ve discovered as LRO orbits about 30 miles above Moon’s surface. The 2010 International Observe the Moon Night is our opportunity to celebrate the science returned from the Lunar Reconnaissance Orbiter, which was built at NASA Goddard and reached lunar orbit on June 23, 2009.

* Laser ranging facility tours are open to the first 100 people on a first-come, first-served basis, so arrive at 6:30 pm to ensure your space!

Agenda for the International Observe the Moon Night
(Hands-on activities and moon observations from 6:45 pm – 10:00 pm)

6:30 pm - Welcome and introduction
6:45 pm - Remote presentation by a scientist from the Lunar and Planetary Institute in Houston, TX
6:45 pm - Science On a Sphere shows every 15 minutes, hands-on activities begin
7:00 pm - Laser ranging tours begin and run every half hour, moon observation with amateur astronomers begins
7:30 pm - 8:15 pm - Presentation by local lunar expert
8:30 pm - 9:15 pm - Presentation by local lunar expert
9:15 pm - 10:00 pm – Hands-on activities, moon observation with amateur astronomers

NASA's Chandra X-ray Observatory Finds Evidence for Stellar Cannibalism

Evidence that a star has recently engulfed a companion star or a giant planet has been found using NASA's Chandra X-ray Observatory. The likely existence of such a "cannibal" star provides new insight into how stars and the planets around them may interact as they age.

The star in question, known as BP Piscium (BP Psc), appears to be a more evolved version of our Sun, but with a dusty and gaseous disk surrounding it. A pair of jets several light years long blasting out of the system in opposite directions has also been seen in optical data. While the disk and jets are characteristics of a very young star, several clues -- including the new results from Chandra -- suggest that BP Psc is not what it originally appeared to be.

Instead, astronomers have suggested that BP Psc is an old star in its so-called red giant phase. And, rather than being hallmarks of its youth, the disk and jets are, in fact, remnants of a recent and catastrophic interaction whereby a nearby star or giant planet was consumed by BP Psc.

When stars like the Sun begin to run of nuclear fuel, they expand and shed their outer layers. Our Sun, for example, is expected to swell so that it nearly reaches or possibly engulfs Earth, as it becomes a red giant star.

"It appears that BP Psc represents a star-eat-star Universe, or maybe a star-eat-planet one," said Joel Kastner of the Rochester Institute of Technology, who led the Chandra study. "Either way, it just shows it's not always friendly out there."

Several pieces of information have led astronomers to rethink how old BP Psc might be. First, BP Psc is not located near any star-forming cloud, and there are no other known young stars in its immediate vicinity. Secondly, in common with most elderly stars, its atmosphere contains only a small amount of lithium. Thirdly, its surface gravity appears to be too weak for a young star and instead matches up with one of an old red giant.

Chandra adds to this story. Young, low-mass stars are brighter than most other stars in X-rays, and so X-ray observations can be used as a sign of how old a star may be. Chandra does detect X-rays from BP Psc, but at a rate that is too low to be from a young star. Instead, the X-ray emission rate measured for BP Psc is consistent with that of rapidly rotating giant stars.

The spectrum of the X-ray emission -- that is how the amount of X-rays changes with wavelength -- is consistent with flares occurring on the surface of the star, or with interactions between the star and the disk surrounding it. The magnetic activity of the star itself might be generated by a dynamo caused by its rapid rotation. This rapid rotation can be caused by the engulfment process.

"It seems that BP Psc has been energized by its meal," said co-author Rodolfo (Rudy) Montez Jr., also from the Rochester Institute of Technology.

The star's surface is obscured throughout the visible and near-infrared bands, so the Chandra observation represents the first detection at any wavelength of BP Psc itself.

"BP Psc shows us that stars like our Sun may live quietly for billions of years," said co-author David Rodriguez from UCLA, "but when they go, they just might take a star or planet or two with them."

Although any close-in planets were presumably devastated when BP Psc turned into a giant star, a second round of planet formation might be occurring in the surrounding disk, hundreds of millions of years after the first round. A new paper using observations with the Spitzer Space Telescope has reported possible evidence for a giant planet in the disk surrounding BP Psc. This might be a newly formed planet or one that was part of the original planetary system.

"Exactly how stars might engulf other stars or planets is a hot topic in astrophysics today," said Kastner. "We have many important details that we still need to work out, so objects like BP Psc are really exciting to find."

These results appeared in The Astrophysical Journal Letters. Other co-authors on the study were Nicolas Grosso of the University of Strasbourg, Ben Zuckerman from UCLA, Marshall Perrin from the Space Telescope Science Institute, Thierry Forveille of the Grenoble Astrophysics Laboratory in France and James Graham from University of California, Berkeley.

NASA's Marshall Space Flight Center in Huntsville, Ala., manages the Chandra program for NASA's Science Mission Directorate in Washington. The Smithsonian Astrophysical Observatory controls Chandra's science and flight operations from Cambridge, Mass.

A Snapshot of Arctic Sea Ice from NASA's Aqua satellite

Sad news for planet hunters

Bad news for planet hunters: most of the "hot Jupiters" that astronomers have been searching for in star clusters were likely destroyed long ago by their stars. In a paper accepted for publication by the Astrophysical Journal, John Debes and Brian Jackson of NASA's Goddard Space Flight Center in Greenbelt, Md., offer this new explanation for why no transiting planets (planets that pass in front of their stars and temporarily block some of the light) have been found yet in star clusters. The researchers also predict that the planet hunting being done by the Kepler mission is more likely to succeed in younger star clusters than older ones.

"Planets are elusive creatures," says Jackson, a NASA Postdoctoral Program fellow at Goddard, "and we found another reason that they're elusive."

When astronomers began to search for planets in star-packed globular clusters about 10 years ago, they hoped to find many new worlds. One survey of the cluster called 47 Tucanae (47 Tuc), for example, was expected to find at least a dozen planets among the roughly 34,000 candidate stars. "They looked at so many stars, people thought for sure they would find some planets," says Debes, a NASA Postdoctoral Program fellow at Goddard. "But they didn't."

More than 450 exoplanets (short for "extrasolar planets," or planets outside our solar system) have been found, but "most of them have been detected around single stars," Debes notes.

"Globular clusters turn out to be rough neighborhoods for planets," explains Jackson, "because there are lots of stars around to beat up on them and not much for them to eat." The high density of stars in these clusters means that planets can be kicked out of their solar systems by nearby stars. In addition, the globular clusters surveyed so far have been rather poor in metals (elements heavier than hydrogen and helium), which are the raw materials for making planets; this is known as low metallicity.

Debes and Jackson propose that hot Jupiters—large planets that are at least 3 to 4 times closer to their host stars than Mercury is to our sun—are quickly destroyed. In these cramped orbits, the gravitational pull of the planet on the star can create a tide—that is, a bulge—on the star. As the planet orbits, the bulge on the star points a little bit behind the planet and essentially pulls against it; this drag reduces the energy of the planet's orbit, and the planet moves a little closer to the star. Then the bulge on the star gets bigger and saps even more energy from the planet's orbit. This continues for billions of years until the planet crashes into the star or is torn apart by the star's gravity, according to Jackson's model of tidal orbital decay.

"The last moments for these planets can be pretty dramatic, as their atmospheres are ripped away by their stars' gravity," says Jackson. "It has even been suggested recently the hot Jupiter called WASP-12B is close enough to its star that it is currently being destroyed."

Debes and Jackson modeled what would have happened in 47 Tuc if the tidal effect were unleashed on hot Jupiters. They recreated the range of masses and sizes of the stars in that cluster and simulated a likely arrangement of planets. Then they let the stars' tides go to work on the close-in planets. The model predicted that so many of these planets would be destroyed, the survey would come up empty-handed. "Our model shows that you don't need to consider metallicity to explain the survey results," says Debes, "though this and other effects will also reduce the number of planets."

Ron Gilliland, who is at the Space Telescope Science Institute in Baltimore and participated in the 47 Tuc survey, says, "This analysis of tidal interactions of planets and their host stars provides another potentially good explanation—in addition to the strong correlation between metallicity and the presence of planets—of why we failed to detect exoplanets in 47 Tuc."

In general, Debes and Jackson's model predicts that one-third of the hot Jupiters will be destroyed by the time a cluster is a billion years old, which is still juvenile compared to our solar system (about 4-1/2 billion years old). 47 Tuc has recently been estimated to be more than 11 billion years old. At that age, the researchers expect more than 96% of the hot Jupiters to be gone.

The Kepler mission, which is searching for hot Jupiters and smaller, Earth-like planets, gives Debes and Jackson a good chance to test their model. Kepler will survey four open clusters—groups of stars that are not as dense as globular clusters—ranging from less than half a billion to nearly 8 billion years old, and all of the clusters have enough raw materials to form significant numbers of planets, Debes notes. If tidal orbital decay is occurring, Debes and Jackson predict, Kepler could find up to three times more Jupiter-sized planets in the youngest cluster than in the oldest one. (An exact number depends on the brightness of the stars, the planets' distance from the stars, and other conditions.)

"If we do find planets in those clusters with Kepler," says Gilliland, a Kepler co-investigator, "looking at the correlations with age and metallicity will be interesting for shaping our understanding of the formation of planets, as well as their continued existence after they are formed."

If the tidal orbital decay model proves right, Debes adds, planet hunting in clusters may become even harder. "The big, obvious planets may be gone, so we'll have to look for smaller, more distant planets," he explains. "That means we will have to look for a much longer time at large numbers of stars and use instruments that are sensitive enough to detect these fainter planets."

The Kepler mission is managed by NASA's Ames Research Center, Moffett Field, Calif., for the Science Mission Directorate at NASA Headquarters in Washington.

Vote on your favorite song

The wakeup song has been a part of the space program since the days of the Apollo missions, and now NASA is giving you two chances to be a part of this history! We need your help selecting wakeup songs to be played during the final missions of the Space Shuttle Program! Select one or both of the missions below:

Listen to and vote on your favorite song from a list of 40 previously played wakeup songs.

The two songs with the most votes will be played during the STS-133 mission.

Cast your vote now through the mission launch date, currently scheduled for November 1, 2010. Winners will be announced during the STS-133 mission.

To vote Click here

NASA's eyes on Hurricane Earl as it heads for New England

NASA satellites and the International Space Station are keeping eyes on Hurricane Earl as it heads for New England. Watches and Warnings are posted in the U.S. northeast.

Having felt the effects of both increasing wind shear and cooler waters, Hurricane Earl weakened to a Category 2 storm on the Saffir-Simpson scale with winds still powerful at 90 knots (104 mph) as it neared the North Carolina coast. It was at this time that the Tropical Rainfall Measuring Mission (TRMM) satellite captured the data about TRMM's rainfall rates.

The rainfall pattern associated with Earl and was made using data from the TRMM satellite when it flew over the storm on September 3 at 08:22 UTC (4:22 a.m. EDT). Rainbands from Earl were visible over the outer banks, eastern North Carolina, and southeastern Virginia, but the storm no longer has a well-defined eye. TRMM observed moderate rainfall mostly to the north of Earl's center.

Meanwhile, from a second vantage point in space, at the International Space Station, Astronaut Douglas Wheelock caught an image of the eye of the storm on September 3. As the ISS flew over Hurricane Earl Wheelock noted that it looked like magnificent chaos from up there on the Space Station and called it incredibly breathtaking.

At 11 a.m. EDT on Sept. 3, Hurricane Earl's maximum sustained winds were near 85 mph. It was located about 350 miles south-southwest of Nantucket, Mass. near 36.8 North and 73.1 West. Earl's minimum central pressure was 961 millibars, and he was moving north-northeast at 21 mph.

Because Earl is now forecast to track farther away from the coast, many of the watches and warnings have been discontinued, but new watches and warnings are in place. The current watches and warnings in effect include: a hurricane warning is in effect for Woods Hole eastward around Cape Cod to Sagamore Beach Massachusetts, including Marthas Vineyard and Nantucket Island. In addition a Hurricane Watch is now in effect for Nova Scotia, Canada from Ecum Secum westward to Digby.

NASA and ATK Aerospace Systems successfully completed Segment Solid Rocket Motor Test

With a loud roar and mighty column of flame, NASA and ATK Aerospace Systems successfully completed a two-minute, full-scale test of the largest and most powerful solid rocket motor designed for flight. The motor is potentially transferable to future heavy-lift launch vehicle designs.

The stationary firing of the first-stage development solid rocket motor, dubbed DM-2, was conducted by ATK, a division of Alliant Techsystems of Brigham City, Utah. DM-2 is the most heavily instrumented solid rocket motor in NASA history, with a total of 53 test objectives measured through more than 760 instruments.

Prior to the static test, the solid rocket motor was cooled to 40 degrees Fahrenheit to verify the performance of new materials and assess motor performance at low temperatures during the full-duration test. Initial test data showed the motor performance met all expectations.

"For every few degrees the temperature rises, solid propellant burns slightly faster and only through robust ground testing can we understand how material and motor performance is impacted by different operating conditions," said Alex Priskos, first stage manager for Ares Projects at NASA's Marshall Space Flight Center in Huntsville, Ala. "Ground-testing at temperature extremes pushes this system to its limits, which advances our understanding of five-segment solid rocket motor performance."

The first-stage solid rocket motor is designed to generate up to 3.6-million pounds of thrust at launch. Information collected from this test, together with data from the first development motor test last year, will be evaluated to better understand the performance and reliability of the design.

Although similar to the solid rocket boosters that help power the space shuttle to orbit, the five-segment development motor includes several upgrades and technology improvements implemented by NASA and ATK engineers. Motor upgrades from a shuttle booster include the addition of a fifth segment, a larger nozzle throat, and upgraded insulation and liner. The motor cases are flight-proven hardware used on shuttle launches for more than three decades. The cases used in this ground test have collectively launched 59 previous missions.

After more testing, the first-stage solid rocket motor will be certified to fly at temperature ranges between 40-90 degrees Fahrenheit. The solid rocket motor was built as an element of NASA's Constellation Program and is managed by the Ares Projects Office at Marshall. ATK Aerospace Systems is the prime contractor.

NASA has begun to study the sun closer than ever before

NASA has begun development of a mission to visit and study the sun closer than ever before. The unprecedented project, named Solar Probe Plus, is slated to launch no later than 2018.

The small car-sized spacecraft will plunge directly into the sun's atmosphere approximately four million miles from our star's surface. It will explore a region no other spacecraft ever has encountered. NASA has selected five science investigations that will unlock the sun's biggest mysteries.

"The experiments selected for Solar Probe Plus are specifically designed to solve two key questions of solar physics -- why is the sun's outer atmosphere so much hotter than the sun's visible surface and what propels the solar wind that affects Earth and our solar system? " said Dick Fisher, director of NASA's Heliophysics Division in Washington. "We've been struggling with these questions for decades and this mission should finally provide those answers."

As the spacecraft approaches the sun, its revolutionary carbon-composite heat shield must withstand temperatures exceeding 2550 degrees Fahrenheit and blasts of intense radiation. The spacecraft will have an up close and personal view of the sun enabling scientists to better understand, characterize and forecast the radiation environment for future space explorers.

NASA invited researchers in 2009 to submit science proposals. Thirteen were reviewed by a panel of NASA and outside scientists. The total dollar amount for the five selected investigations is approximately $180 million for preliminary analysis, design, development and tests.

The selected proposals are:

-- Solar Wind Electrons Alphas and Protons Investigation: principal investigator, Justin C. Kasper, Smithsonian Astrophysical Observatory in Cambridge, Mass. This investigation will specifically count the most abundant particles in the solar wind -- electrons, protons and helium ions -- and measure their properties. The investigation also is designed to catch some of the particles in a special cup for direct analysis.

-- Wide-field Imager: principal investigator, Russell Howard, Naval Research Laboratory in Washington. This telescope will make 3-D images of the sun's corona, or atmosphere. The experiment actually will see the solar wind and provide 3-D images of clouds and shocks as they approach and pass the spacecraft. This investigation complements instruments on the spacecraft providing direct measurements by imaging the plasma the other instruments sample.

-- Fields Experiment: principal investigator, Stuart Bale, University of California Space Sciences Laboratory in Berkeley, Calif. This investigation will make direct measurements of electric and magnetic fields, radio emissions, and shock waves that course through the sun's atmospheric plasma. The experiment also serves as a giant dust detector, registering voltage signatures when specks of space dust hit the spacecraft's antenna.

-- Integrated Science Investigation of the Sun: principal investigator, David McComas of the Southwest Research Institute in San Antonio. This investigation consists of two instruments that will take an inventory of elements in the sun's atmosphere using a mass spectrometer to weigh and sort ions in the vicinity of the spacecraft.

-- Heliospheric Origins with Solar Probe Plus: principal investigator, Marco Velli of NASA's Jet Propulsion Laboratory in Pasadena, Calif. Velli is the mission's observatory scientist, responsible for serving as a senior scientist on the science working group. He will provide an independent assessment of scientific performance and act as a community advocate for the mission.

"This project allows humanity's ingenuity to go where no spacecraft has ever gone before," said Lika Guhathakurta, Solar Probe Plus program scientist at NASA Headquarters, in Washington. "For the very first time, we'll be able to touch, taste and smell our sun."

The Solar Probe Plus mission is part of NASA's Living with a Star Program. The program is designed to understand aspects of the sun and Earth's space environment that affect life and society. The program is managed by NASA'S Goddard Space Flight Center in Greenbelt, Md., with oversight from NASA's Science Mission Directorate's Heliophysics Division. The Johns Hopkins University Applied Physics Laboratory in Laurel, Md., is the prime contractor for the spacecraft.

NASA's Kepler spacecraft Discovers Two Planets Transiting the Same Star

NASA's Kepler spacecraft has discovered the first confirmed planetary system with more than one planet crossing in front of, or transiting, the same star.

The transit signatures of two distinct planets were seen in the data for the sun-like star designated Kepler-9. The planets were named Kepler-9b and 9c. The discovery incorporates seven months of observations of more than 156,000 stars as part of an ongoing search for Earth-sized planets outside our solar system. The findings will be published in Thursday's issue of the journal Science.

Kepler's ultra-precise camera measures tiny decreases in the stars' brightness that occur when a planet transits them. The size of the planet can be derived from these temporary dips.

The distance of the planet from the star can be calculated by measuring the time between successive dips as the planet orbits the star. Small variations in the regularity of these dips can be used to determine the masses of planets and detect other non-transiting planets in the system.

In June, mission scientists submitted findings for peer review that identified more than 700 planet candidates in the first 43 days of Kepler data. The data included five additional candidate systems that appear to exhibit more than one transiting planet. The Kepler team recently identified a sixth target exhibiting multiple transits and accumulated enough follow-up data to confirm this multi-planet system.

"Kepler's high quality data and round-the-clock coverage of transiting objects enable a whole host of unique measurements to be made of the parent stars and their planetary systems," said Doug Hudgins, the Kepler program scientist at NASA Headquarters in Washington.

Scientists refined the estimates of the masses of the planets using observations from the W.M. Keck Observatory in Hawaii. The observations show Kepler-9b is the larger of the two planets, and both have masses similar to but less than Saturn. Kepler-9b lies closest to the star with an orbit of about 19 days, while Kepler-9c has an orbit of about 38 days. By observing several transits by each planet over the seven months of data, the time between successive transits could be analyzed.

"This discovery is the first clear detection of significant changes in the intervals from one planetary transit to the next, what we call transit timing variations," said Matthew Holman, a Kepler mission scientist from the Harvard-Smithsonian Center for Astrophysics in Cambridge, Mass. "This is evidence of the gravitational interaction between the two planets as seen by the Kepler spacecraft."

In addition to the two confirmed giant planets, Kepler scientists also have identified what appears to be a third, much smaller transit signature in the observations of Kepler-9. That signature is consistent with the transits of a super-Earth-sized planet about 1.5 times the radius of Earth in a scorching, near-sun 1.6 day-orbit. Additional observations are required to determine whether this signal is indeed a planet or an astronomical phenomenon that mimics the appearance of a transit.

NASA's Ames Research Center in Moffett Field, Calif., manages Kepler's ground system development, mission operations and science data analysis. NASA's Jet Propulsion Laboratory in Pasadena, Calif., managed Kepler mission development.

Ball Aerospace and Technologies Corp. in Boulder, Colo., developed the Kepler flight system and supports mission operations with the Laboratory for Atmospheric and Space Physics at the University of Colorado in Boulder. The Space Telescope Science Institute in Baltimore archives, hosts and distributes the Kepler science data.

Build a Life-Sized Model and Real Giant NASA Space Telescope

It takes many years to build a space telescope or a satellite and years to put one together. However, when it comes assembling and disassembling the life-sized model of NASA's James Webb Space Telescope, it takes a couple of days. That's how long it took to assemble the Webb model in New York City recently.

Assembling a Life-Sized Model

The life-sized model is constructed mainly of aluminum and steel, weighs 12,000 lbs., and is approximately 80 feet long, 40 feet wide and 40 feet tall. It was specifically designed for an environment subject to gravity and weather. A specially manufactured material imported from France called "Ferrari recontraint" allows the sunshield to 'breathe.' The model requires 2 trucks to ship it over land, and assembly takes a crew of 12 approximately four days.

How Real Satellites/Space Telescopes Come About

It takes years to bring a real large space telescope from basic concept to hardware reality. First, a scientist comes up with an idea to study some aspect of the Earth or the cosmos. The idea is discussed, reviewed and developed by committees of scientists. It is proposed to NASA, who makes decisions on what missions to go forth on, and which missions to pass on. If a mission is selected for study a timeline is created to develop the mission.

One of the most difficult aspects of creating a new mission is convincing others to fund it. Once a mission is funded, the team of scientists and engineers "pitching" the mission can then investigate how it could come together. Later, NASA usually selects a prime contractor to help design the telescope and other systems that will fly on the satellite. Northrop Grumman was selected to build components for the Webb telescope. The instruments, or cameras, on the telescope are selected as well, with teams of scientists to watch over the design.

The design process usually includes a number of different designs, which are all tested to see which would yield the best result for the type of object the instrument would study. For example, various types of infrared cameras may be developed and tested, and the one that gives a scientist the best result, would be chosen to be built as a test unit.

Engineering Test Units

Engineering test units, or ETUs are created before an actual instrument is built, so that engineers and scientists can make sure it would work properly. ETUs are a replica of the flight unit that can perform certain flight functions for testing purposes. ETUs are also used when engineers are practicing installation of an instrument into a satellite's mainframe or "bus." The outcome of the tests on ETUs may lead to a change in handling procedures of the actual flight instrument, but not a change in its flight construction.

Once the ETUs test successful, then the actual instruments that will fly aboard a satellite or space telescope can be manufactured. Those instruments go through their own set of rigorous tests by the manufacturing contractor, NASA and other partners. On the Webb telescope, NASA is partnering with the European Space Agency and the Canadian Space Agency.

Testing the System

Satellite and space telescope instruments can endure harsh temperature swings as big as 200 degrees Fahrenheit, micro-meteor impacts and exposure to solar radiation. On top of that, before a spacecraft like the Webb can operate in orbit, it has to survive a ride on a rocket to get there. That's where environmental testing chambers like the ones at NASA's Goddard Space Flight Center in Greenbelt, Md., come into play. Hardware gets run through NASA Goddard's centrifuge, acoustics and thermal vacuum chambers to ensure they can endure the rigors of launch.

The centrifuge simulates the increased feeling of gravity's pull during a launch. For astronauts, that's normally a few minutes at two or three times the force of Earth's gravity, measured in Gs. The Webb telescope can experience 6-7 G's due to the Ariane 5 rocket's combined acceleration and vibration. The Webb telescope will be launched on an Ariane 5 ECA rocket. The launch vehicle is part of the European contribution to the mission.

Launching a rocket carrying a satellite or space telescope creates extraordinarily loud noise, so engineers use an Acoustic Test Chamber to make sure an instrument can handle it safely. In Goddard's 42-foot-tall chamber, technicians expose payloads to the noise of a launch. To do that, they rely on 6-foot-tall speakers. The speakers (more accurately called horns) use an altering flow of gaseous nitrogen to produce a sound level as high as 143 decibels for one-minute tests. That's about the level of sound heard standing next to a jet engine during takeoff.

The hardware is also tested in the thermal vacuum which exposes them to conditions they will experience in space. The chamber has massive mechanical vacuum pumps and cryopumps to ensure that the hard vacuum of space is simulated in the test chamber. The cryopumps use gaseous helium to condense remaining gases out of the chamber once the mechanical pumps have done their work. The two types of pumps work together to eliminate all but the tiniest trace of air in the chamber, down to about a billionth of Earth's normal atmospheric pressure.

Because the Webb telescope is operating in the infrared portion of the electromagnetic spectrum it is designed to operate at very cold temperatures. To simulate this environment an additional cooling system, a helium refrigeration system, was added so the thermal vacuum chamber could reach temperatures in the -413 Fahrenheit (F) range. "The ISIM structure was tested in our thermal vacuum chamber down to about 26 Kelvin, or minus 413 F," said Jon F. Lawrence, Webb telescope Mechanical Systems Lead Engineer/Launch Vehicle Liaison at NASA Goddard.

This test program starts at the lowest level of assembly, instrument or spacecraft components and is repeated at each next level of assembly. Once the instruments pass these tests they are all put together into the structure which holds them and the unit is tested again. The instrument structure is connected to the telescope and the whole observatory is tested yet again. There isn't a vacuum chamber large enough to hold the entire Webb observatory at NASA Goddard, so the telescope will travel to NASA's Johnson Space Center in Houston, Texas, to be tested in a chamber that was originally built for testing the Apollo command module to simulate the trip to the moon. The next stop after that is launch into deep space.

Currently, ETUs or actual flight hardware for the Webb telescope are being tested in various ways.

The James Webb Space Telescope is the next-generation premier space observatory, exploring deep space phenomena from distant galaxies to nearby planets and stars. The Webb Telescope will give scientists clues about the formation of the universe and the evolution of our own solar system, from the first light after the Big Bang to the formation of star systems capable of supporting life on planets like Earth.

The Webb Telescope project is managed at NASA's Goddard Space Flight Center in Greenbelt, Md. The telescope is a joint project of NASA, the European Space Agency and the Canadian Space Agency.

NASA Sensors to Guide Spacecraft for Safe Landing

NASA is developing technologies that will allow landing vehicles to automatically identify and navigate to the location of a safe landing site while detecting landing hazards during the final descent to the surface. This is important because future missions -- whether to the Moon, an asteroid, Mars or other location -- will need this capability to land safely near specific resources that are located in potentially hazardous terrain.

Langley Research Center, Hampton, Va., has designed three light detection and ranging (lidar) sensors that together can provide all the necessary data for achieving safe autonomous precision landing.

The sensor suite was flown over varied objects on Rogers Dry Lake to test the system's ability to detect potentially hazardous objects on the surface.

One is a three-dimensional active imaging device, referred to as flash lidar, for detecting hazardous terrain features and identifying safe landing sites. The second is a Doppler lidar instrument for measuring the vehicle velocity and altitude to help land precisely at the chosen site. The third is a high-altitude laser altimeter providing data prior to final approach for correcting the flight trajectory towards the designated landing area.

In conjunction with laser/lidar sensor development at Langley, NASA's Jet Propulsion Laboratory, Pasadena, Calif., is developing algorithms, or mathematical procedures, for analyzing the acquired three-dimensional lidar maps and determining the most suitable landing site. The resulting Doppler lidar and laser altimeter data are used by the navigation system being developed by NASA Johnson Space Center, Houston, and Charles Draper Laboratory, Cambridge, Mass., to control the spacecraft to the identified location.

These technologies have been integrated as part of NASA's Autonomous Landing and Hazard Avoidance Technology (ALHAT) project and are in the process of being demonstrated in a series of flight tests.

The most recent flight tests occurred at NASA's Dryden Flight Research Center, Edwards, Calif., in July.

"These were the first tests where we had all three of our laser systems on board and working together as a complete sensor suite," said Langley's Farzin Amzajerdian, technical lead for development of the sensors. "These tests are being viewed as critical by many within NASA."

Robert Reisse, Langley project manager, added, "We were pleased that the flight tests we've conducted so far have resulted in better than expected performance of these sensors."

The main objective of the first test, carried out in May 2008, was to demonstrate the application of 3-D imaging technology, or 'flash' lidar, for topography mapping and hazard detection.

The second round of flight tests, completed in August 2008, was to evaluate the capabilities of the Doppler lidar. This lidar provides high reliability vehicle velocity vector, altitude and attitude with about two orders of magnitude higher precision than radars.

The third flight test campaign was conducted in June 2009 in which the flash lidar and laser altimeter were integrated and flown onboard a fixed-wing aircraft to assess its performance for terrain relative navigation and altimetry functions. Several flights were performed in areas of Death Valley and in the Nevada Test Site with various flight pro

NASA Langley students: Ping-Pong Balls to Float Crew Capsule Simulator

If ping-pong balls can float a sunken boat, they should be able to keep an uncrewed space capsule simulator from sinking.

Right?

That's what a team of summer students and engineers think at NASA's Langley Research Center in Hampton, Va. Langley is fabricating a proposed design of an astronaut crew module simulator for uncrewed flight-testing as part of the agency's effort to build a vehicle to replace the space shuttle.

The Orion crew exploration vehicle is the nation's next generation spacecraft designed to carry up to four astronauts to low Earth orbit and beyond.

Orion's first suborbital flight test will launch to 400,000 feet, or 75 miles above Earth. Because the crew module will not be pressurized during the test, it will not have the buoyancy of a pressurized spacecraft. This puts the simulated crew module at risk of sinking to the bottom of the Atlantic Ocean after splashdown.

To save the valuable test article for analysis and possible reuse, Langley called on a team of creative minds for a solution.

And as it turned out, inexpensive, lightweight ping-pong balls provided the answer. Langley engineer John DiNonno proposed the idea, and the Orion Flight Test Office told the team to study it.

The idea quickly became "very plausible," said student Caroline Kirk.


Way to go

"At first we didn't really realize that we were going to get so far in proving that it would be possible," said Kirk, a Suffolk, Va., native attending Virginia Tech as an aerospace engineering major. "But when we thought about everything logically, it just seemed like ping-pong balls were the way to go."

She and a team of seven other students worked the project in Langley's Mechanical Systems Branch, where they were assigned for the summer.

DiNonno got the idea from a Discovery Channel program about raising a sunken boat using 27,000 ping-pong balls.

Engineer David Covington said that when DiNonno suggested the ping-pong ball idea, "I just laughed. Not a 'what are you thinking' kind of laugh, but more of a 'that's the most awesome thing I've heard in a long time' laugh. I asked him 'are you serious?' and he said 'yeah, we're authorized to do a four-week study.' So we went straight to work."

Ensuring the outcome would be relatively low-cost was a top priority, said DiNonno.

"Recovering the capsule was not a requirement, but it was a desire," he said. "So there wasn't going to be a lot of investment in it."

Testing process

The students divided the tasks needed to determine if the idea was feasible, each becoming a "principal investigator" for a specific area.

They tested ping-pong balls of varying quality, much the way spacecraft hardware is tested. They studied how the balls would react to the near-vacuum at the edge of space. Using buoyancy tests, they determined how well the balls would float.

The students also subjected the ping-pong balls to mechanical loads using a hydraulic press, and heated them to see how they would react to the high temperatures of descent into the Earth's atmosphere. And they performed electrostatic discharge tests to determine if the balls would produce a static charge that could disrupt the space capsule's electronics.

The ping-pong balls passed all the challenges, said Heather Blount, a materials science engineering student at Virginia Tech.

"Through all our testing and calculations, we figured out that it could be a safe and viable option," said Blount, of Yorktown, Va.

Keeping the crew module afloat would take at least 150,000 ping-pong balls, the students estimate, at a retail price of 50 cents or less each -- a fraction of the cost of traditional options. The students hope to reduce the cost through a bulk purchase.

If the flight test is approved, the ping-pong ball concept would still need to be vetted with the flight test team and reviewed by NASA senior management. If implemented, the ping-pong balls probably will be put into netted bags and secured inside the crew module just prior to launch. They would virtually fill the available space inside the uncrewed capsule.

Then, when the unsealed capsule splashes down, the buoyancy of the ping-pong balls will offset the weight of incoming water and it will float instead of sink.

The ping-pong balls also will reduce the volume of air that needs to be vented from the capsule during ascent - as well as drawn in during descent - as the capsule travels through significant changes in atmospheric pressure.


'Awesome' students

Approval of the flight test, as well as a launch date, has yet to be determined. "Even if it is not used, it's an idea that's out there that someone else could use," said Langley engineer Amanda Cutright, a student mentor.

Cutright said she has been enthused by the students.

"It's awesome working with them," she said. "They bring a different perspective. I've been really impressed with how quickly they pick up new ideas and new technology. It seems each team of students that we mentor learns quicker and is able to provide creative ideas."

Kirk said the ping-pong ball project has been a unique experience. At school, she said, "we do lab experiments but nothing similar to this at all. Being able to develop an experiment that will be used for space flight tests is an opportunity of a lifetime."

NASA employees and contractors involved in the project include engineers Amanda Cutright; Brendan Shaughnessy, Analytical Services and Materials Inc.; David Covington, ATK Space Systems Inc.; and John DiNonno, all of the Mechanical Systems Branch.