Ozone Success Story: NASA Video of Enviro Action That Worked

Ozone layer hole. Image credit: NASA
Ozone layer hole. Image credit: NASA

[/caption]

Imagine the year 2065. Two-thirds of Earth’s ozone is gone. The infamous ozone hole over Antarctica is a year-round fixture with a twin over the North Pole. People living in mid-latitude cities like Washington, D.C., get sunburned after five minutes. DNA-mutating UV radiation is up 650 percent, with likely harmful effects on plants, animals and human skin cancer rates.

Such is the world we would have inherited if 193 nations had not agreed to ban ozone-depleting substances, according to atmospheric chemists at NASA, Johns Hopkins University in Baltimore and the Netherlands Environmental Assessment Agency in Bilthoven. The researchers have unveiled new computer simulations this week of a worldwide disaster that humans managed to avoid.

In retrospect, the researchers say, the Montreal Protocol was a “remarkable international agreement that should be studied by those involved with global warming and the attempts to reach international agreement on that topic.”

ozone-simulation
This time series from the ozone "World Avoided" model shows the concentration of ozone over the South Pole at four key times. Reds represent normal to high concentrations; blues show depleted areas. Credit: NASA Goddard's Scientific Visualization Studio

Ozone is Earth’s natural sunscreen, absorbing and blocking most of the incoming UV radiation from the sun and protecting life from DNA-damaging radiation. The gas is naturally created and replenished by a photochemical reaction in the upper atmosphere where UV rays break oxygen molecules into individual atoms that then recombine into three-part molecules (O3). As it is moved around the globe by upper level winds, ozone is slowly depleted by naturally occurring atmospheric gases. It is a system in natural balance.

But chlorofluorocarbons — invented in 1928 as refrigerants and as inert carriers for chemical sprays — upset that balance. Researchers discovered in the 1970s and 1980s that while CFCs are inert at Earth’s surface, they are quite reactive in the stratosphere (10 to 50 kilometers altitude, or 6 to 31 miles), where roughly 90 percent of the planet’s ozone accumulates. UV radiation causes CFCs and similar bromine compounds in the stratosphere to break up into elemental chlorine and bromine that readily destroy ozone molecules. 

In the 1980s, ozone-depleting substances opened a wintertime “hole” over Antarctica and opened the eyes of the world to the effects of human activity on the atmosphere.  In January 1989, the Montreal Protocol went into force, the first-ever international agreement on regulation of chemical pollutants.

In the new study, published online in the journal Atmospheric Chemistry and Physics, Goddard scientist Paul Newman and his team simulated “what might have been” if chlorofluorocarbons (CFCs) and similar chemicals were not banned. The simulation used a comprehensive model that included atmospheric chemical effects, wind changes, and radiation changes. The “World avoided” video can be viewed here in Quicktime (for more formats, go here).

By the simulated year 2020, 17 percent of all ozone is depleted globally. An ozone hole starts to form each year over the Arctic, which was once a place of prodigious ozone levels.

By 2040, global ozone concentrations fall below the same levels that currently comprise the “hole” over Antarctica. The UV index in mid-latitude cities reaches 15 around noon on a clear summer day, giving a perceptible sunburn in about 10 minutes. Over Antarctica, the ozone hole becomes a year-round fixture.

By the end of the model run in 2065, global ozone drops 67 percent compared to 1970s levels. The intensity of UV radiation at Earth’s surface doubles; at certain shorter wavelengths, intensity rises by as much as 10,000 times. Skin cancer-causing radiation soars.

“Our world avoided calculation goes a little beyond what I thought would happen,” said Goddard scientist and study co-author Richard Stolarski, who was among the pioneers of atmospheric ozone chemistry in the 1970s. “The quantities may not be absolutely correct, but the basic results clearly indicate what could have happened to the atmosphere.”

“We simulated a world avoided,” added Newman, “and it’s a world we should be glad we avoided.”

As it is, production of ozone-depleting substances was mostly halted about 15 years ago, though their abundance is only beginning to decline because the chemicals can reside in the atmosphere for 50 to 100 years. The peak abundance of CFCs in the atmosphere occurred around 2000, and has decreased by roughly 4 percent to date. Stratospheric ozone was depleted by 5 to 6 percent at middle latitudes, but has somewhat rebounded in recent years.

Disappearing Stars Confirm Supernova Origins

Artist's rendering of SN 1993J, where a red supergiant supernova progenitor star (left) is exploding after having transferred about 10 solar masses of hydrogen gas to the blue companion star (right). Credit: ESA

Artist’s rendering of SN 1993J, where a red supergiant supernova progenitor star (left) is exploding after having transferred about seven solar masses of hydrogen gas to the blue companion star (right). Credit: ESA

Astronomers have caught two stars in the disappearing acts that link them to type II supernova events.

Type II supernovae are widely believed to result from the internal collapse and explosion of massive stars, about nine times the size of our sun. But precious few observations have actually confirmed the relationship.

Now, researchers have spotted two parent stars that showed up in supernovae “before” images — but not in images taken after the blasts. 

“The disappearance of the progenitors confirms that these two supernovae were produced by Red Supergiants,” write co-authors Justyn Maund and Stephen Smartt. Their new paper is out in this week’s issue of Science.


sn2003gd

SN 2003gd. Credit: Gemini Observatory

So far only one star has been shown to have disappeared after it exploded — the star that exploded as SN 1987A in the Local Group of galaxies. Seven other stars have been spotted in the neighborhoods of type II supernovae before they went off, but none of them has been shown to have disappeared, Maund and Smartt write.

Maund is affiliated with both the University of Copenhagen in Denmark and the University of California at Santa Cruz, and Smartt is from Queen’s University Belfast in the UK. They used the Hubble Space Telescope and the Gemini Telescope to observe the two supernovae.

The progenitor of SN 2003gd, an M-supergiant star in the galaxy M74, “is no longer observed at the SN location,” they found. They estimated 2003gd is seven times the mass of the sun, which they acknowledge “is at the lower end of the mass range considered theoretically possible to produce core-collapse events.” They said there’s enough uncertainty in the object’s mass that it could be greater than seven solar masses — but even if it’s not, several other stars in the low end of the range are suspected of exploding as supernovae.

The co-authors are also careful to point out that dust from the supernova is still visible, and, “One could argue that the star identified as the progenitor was a neighboring star that is now obscured by dust formation.” But their work indicates that the explosion wasn’t dusty enough to obscure a star as luminous as SN 2003gd’s parent. They believe the progenitor star has truly disappeared — although further confirmation will come as the dust continues to clear.

SN 1993J is a truly exceptional case. The K-supergiant star that exploded in that supernova is also no longer present, the authors report — but its B-supergiant binary companion is still observed. 

The model for the binary system was of a progenitor star 15 times the mass of the sun, with a slightly less massive binary companion. The progenitor star evolved faster, and transferred some of its mass onto the binary companion, including a substantial amount of its hydrogen envelope. The binary companion grew to 22 times the mass of the sun. The interaction happened over about 250 years and affected the supernova explosion to such an extent that SN 1993J became known as one of the most peculiar supernovae ever seen.

The site of SN 1993J was imaged several times over the 2 to 13 years after the explosion with Hubble and a handful of other telescopes. By the 2004 observation, the red portion of the SN spectral energy distribution had faded below the level of the red spectral energy of the binary progenitor system, “ruling out the continued presence of the K-supergiant star and, hence, confirming it as the progenitor of SN 1993J,” the authors wrote.

They said soon the blue part of the supernova’s spectrum will fade, opening up a window for observations of the remaining companion star.

The authors conclude that their “simple, but time-consuming” method “leaves no doubt that the two stars were the progenitors of the supernovas, SN 2003gd and SN 1993J, and confirms that type II supernovas are birthed from Red Supergiants, as predicted.”

New Particle Throws Monkeywrench in Particle Physics

[/caption]

The hits just keep on coming from Department of Energy’s Fermi National Accelerator Laboratory. So far this month, the lab has announced the discovery of a rare single top quark, and then narrowed the gaptwice, actually — for the mass of the elusive Higgs Boson particle, or “God particle,” thought to give all other particles their mass. 

Now, scientists have detected a new, completely untheorized particle that challenges what physicists thought they knew about how quarks combine to form matter. They’re calling it Y(4140), reflecting its measured mass of 4140 Mega-electron volts. 

“It must be trying to tell us something,” said Jacobo Konigsberg of the University of Florida, a spokesman for Fermilab’s collider detector team. “So far, we’re not sure what that is, but rest assured we’ll keep on listening.”

particles
The Standard Model of elementary particles and forces includes six quarks, which bind together to form composite particles. Credit: Fermilab

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Matter as we know it comprises building blocks called quarks. Quarks fit together in various well-established ways to build other particles: mesons, made of a quark-antiquark pair, and baryons, made of three quarks. 

But recently, electron-positron colliders at Stanford’s SLAC National Accelerator Laboratory and the Japanese laboratory KEK have revealed examples of composite quark structures — named X and particles — that are not the usual mesons and baryons. And now, the Collider Detector at Fermilab (CDF) collaboration has found evidence for the Y(4140) particle.

The Y(4140) particle decays into a pair of other particles, the J/psi and the phi, suggesting to physicists that it might be a composition of charm and anticharm quarks. However, the characteristics of this decay do not fit the conventional expectations for such a make-up. Other possible interpretations beyond a simple quark-antiquark structure are hybrid particles that also contain gluons, or even four-quark combinations.

The Fermilab scientists observed Y(4140) particles in the decay of a much more commonly produced particle containing a bottom quark, called the B+ meson. Sifting through trillions of proton-antiproton collisions from Fermilab’s Tevatron, they identified a small sampling of B+ mesons that decayed in an unexpected pattern. Further analysis showed that the B+ mesons were decaying into Y(4140).

The Y(4140) particle is the newest member of a family of particles of similar unusual characteristics observed in the last several years by experimenters at Fermilab’s Tevatron as well as at KEK and the SLAC lab, which operates at Stanford through a partnership with the U.S. Department of Energy.

“We congratulate CDF on the first evidence for a new unexpected Y state that decays to J/psi and phi,” said Japanese physicist Masanori Yamauchi, a KEK spokesperson. “This state may be related to the Y(3940) state discovered by Belle and might be another example of an exotic hadron containing charm quarks. We will try to confirm this state in our own Belle data.”

Theoretical physicists are trying to decode the true nature of these exotic combinations of quarks that fall outside our current understanding of mesons and baryons. Meanwhile, experimentalists happily continue to search for more such particles.

“We’re building upon our knowledge piece by piece,” said Fermilab spokesperson Rob Roser, “and with enough pieces, we’ll understand how this puzzle fits together.”

The Y(4140) observation is the subject of an article submitted by CDF to Physical Review Letters this week. Besides announcing Y(4140), the CDF experiment collaboration is presenting more than 40 new results at the Moriond Conference on Quantum Chromodynamics in Europe this week, including the discovery of electroweak top-quark production and a new limit on the Higgs boson, in concert with experimenters from Fermilab’s DZero collaboration. 

Source: Fermilab

At Last: Successful Launch for European Climate Satellite

[/caption]

Europe’s Gravity field and steady-state Ocean Circulation Explorer (GOCE) is headed into orbit, after a successful launch at 10:21 a.m. EDT (14:21 GMT) on Tuesday from the Plesetsk Cosmodrome in northern Russia. 

The successful liftoff came after delays stretching back to last September, but Tuesday’s launch went off without any complications.

“It was a nice liftoff,” said Mission Scientist Mark Drinkwater.

Monday’s launch failed to progress when the doors of the launch service tower simply did not open. That after a previous failure last September, when problems cropped up with the guidance and navigation subsystems on the Russian Breeze KM rocket. 

GOCE is the first of a new family of ESA satellites, called Earth Explorers, designed to study our planet and its environment in order to improve our knowledge and understanding of Earth-system processes and their evolution, to characterize the challenges of global climate change. Its specific mission is to map Earth’s gravity field with unprecedented accuracy, providing insight into ocean circulation, sea-level change, climate change, volcanism and earthquakes.

Source: ESA

Hubble Snaps Rare Moon Parade Across Saturn

[/caption]

Once every 15 years, Saturn flashes its paper-thin rings in edge-on formation relative to Earth. 

Because the orbits of Saturn’s major satellites are in the ring plane, too, this alignment gives astronomers a rare opportunity to capture a spectacular parade of celestial bodies crossing Saturn’s surface.

Leading this moon train is Titan – larger than the planet Mercury. The frigid moon’s thick nitrogen atmosphere is tinted orange with the smoggy byproducts of sunlight interacting with methane and nitrogen. Several of the much smaller icy moons that are closer in to the planet line up along the upper edge of the rings. 

In the image, snapped by the Hubble Space Telescope on February 24, the giant orange moon Titan casts a large shadow onto Saturn’s north polar hood. Below Titan, near the ring plane and to the left is the moon Mimas, casting a much smaller shadow onto Saturn’s equatorial cloud tops. Farther to the left, and off Saturn’s disk, are the bright moon Dione and the fainter moon Enceladus.

Hubble’s exquisite sharpness also reveals Saturn’s banded cloud structure, which is similar to Jupiter’s.

hs-2009-12-b-print
The top frame captures the giant moon Titan and its shadow near Saturn's northern polar hood. Dione, the brightest of the icy moons in this view – which are closer in to Saturn – can easily be traced crossing the disk from far left to image center. In the center frame, the smaller moon Enceladus can be seen near the western limb of Saturn. Credit: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)

At the time, Saturn was at a distance of roughly 775 million miles (1.25 billion kilometers) from Earth. Hubble can see details as small as 190 miles (300 km) across on Saturn. The dark band running across the face of the planet slightly above the rings is the shadow of the rings cast on the planet.

Early 2009 was a favorable time for viewers with small telescopes to watch moon and shadow transits crossing the face of Saturn. Titan, Saturn’s largest moon, crossed Saturn on four separate occasions: January 24, February 9, February 24, and March 12, although not all events were visible from all locations on Earth.

 This “ring plane crossing” occurs every 14-15 years. In 1995-96 Hubble witnessed the ring plane crossing event, as well as many moon transits, and even helped discover several new moons of Saturn.

Source (and more images!): HubbleSite

Indian Balloon Experiment Nets Three New Bacteria

[/caption]

Indian scientists flying a giant balloon experiment have announced the discovery of three new species of bacteria from the stratosphere.

In all, 12 bacterial and six fungal colonies were detected, nine of which, based on gene sequencing, showed greater than 98 percent similarity with reported known species on earth. Three bacterial colonies, however, represented totally new species. All three boast significantly higher UV resistance compared to their nearest phylogenetic neighbors on Earth.

The experiment was conducted using a balloon that measures 26.7 million cubic feet  (756,059 cubic meters) carrying 1,000 pounds (459 kg) of scientific payload soaked in liquid Neon. It was flown from the National Balloon Facility in Hyderabad, operated by the Tata Institute of Fundamental Research (TIFR). 

An onboard cryosampler contained sixteen evacuated and sterilized stainless steel probes. Throughout the flight, the probes remained immersed in liquid Neon to create a cryopump effect. The cylinders, after collecting air samples from different heights ranging from 20 km to 41 km (12 to 25 miles) above the Earth’s surface, were parachuted down and retrieved. The samples were analyzed by scientists at the Center for Cellular and Molecular Biology in Hyderabad as well as the National Center for Cell Science in Pune for independent confirmation.

One of the new species has been named as Janibacter hoylei, after the astrophysicist Fred Hoyle, the second as Bacillus isronensis recognizing the contribution of ISRO in the balloon experiments which led to its discovery, and the third as Bacillus aryabhata after India’s celebrated ancient astronomer Aryabhata (also the name of ISRO’s first satellite).

The researchers have pointed out in a press release that precautionary measures and controls operating in the experiment inspire confidence that the new species were picked up in the stratosphere.

“While the present study does not conclusively establish the extra-terrestrial origin of microorganisms, it does provide positive encouragement to continue the work in our quest to explore the origin of life,” they added.

This was the second such experiment conducted by ISRO, with the first one in 2001. Even though the first experiment had yielded positive results, the researchers decided to repeat the experiment while exercising extra care to ensure that it was totally free from any terrestrial contamination.

Source: Indian Space Research Organisation

Additional links: Center for Cellular and Molecular BiologyNational Center for Cell Science, Tata Institute of Fundamental Research

ESO Image Reveals Galaxy Duo in Explosive Dance

The ‘peculiar galaxy’ Arp 261 has been imaged in unprecedented detail, revealing two galaxies in a slow motion — but highly chaotic and disruptive — close encounter. 

Arp 261 lies about 70 million light-years distant in the constellation of Libra, the Scales. The new close-up was captured by the ESO’s Very Large Telescope, at the Paranal Observatory in Chile.

Although individual stars are very unlikely to collide in such an interaction, the huge clouds of gas and dust certainly do crash into each other at high speed, leading to the formation of bright new clusters of very hot stars that are clearly seen in the picture. The paths of the existing stars in the galaxies are also dramatically disrupted, creating the faint swirls extending to the upper left and lower right of the image. Both interacting galaxies were probably dwarfs not unlike the Magellanic Clouds orbiting our own galaxy.

Arp 261 is listed in Halton Arp’s catalogue of Peculiar Galaxies that appeared in the 1960s, with the goal of chronicling objects in the sky that appear strange and may tell rewarding science stories. 

The images used to create the new picture of Arp 261 were not actually taken to study the interacting galaxies at all, but to investigate the properties of the inconspicuous object just to the right of the brightest part of Arp 261 and close to the center of the image. This is an unusual exploding star, called SN 1995N, that is thought to be the result of the final collapse of a massive star at the end of its life, a so-called core collapse supernova. SN 1995N is unusual because it has faded very slowly — and still shows clearly more than seven years after the explosion took place.

SN 1995N is also one of the few supernovae to have been observed to emit X-rays. It is thought that these unusual characteristics are a result of the exploding star being in a dense region of space so that the material blasted out from the supernova plows into it and creates X-rays.

Apart from the interacting galaxy and its supernova, the image also contains several other objects at wildly different distances from us. Starting very close to home, two small asteroids, in our Solar System between the orbits of Mars and Jupiter, happened to cross the images as they were being taken and show up as the red-green-blue trails at the left and top of the picture. The trails arise as the objects are moving during the exposures and also between the exposures through different colored filters. The asteroid at the top is number 14670 and the one to the left number 9735. They are probably less than 5 km (3 miles) across. The reflected sunlight from these small bodies takes about 15 minutes to reach Earth.

The next closest object is probably the apparently bright star at the bottom. It may look bright, but it is still about one hundred times too faint to be seen with the unaided eye. It is most likely a star rather like the Sun and about 500 light-years from us — 20 million times further away than the asteroids. Arp 261 itself, and the supernova, are about 140,000 times farther away than this star, but still in what astronomers would regard as our cosmic neighborhood. Much more distant still, perhaps some fifty to one hundred times further away than Arp 261, lies the cluster of galaxies visible on the right of the picture.

Videos of the unusual system are available here and here.

Source: ESO

Europe’s Climate Satellite Fails to Leave Pad

[/caption]

Europe’s Gravity field and steady-state Ocean Circulation Explorer (GOCE) seems to be stuck on the pad.

The climate change satellite was expected to launch out of Russia at 14:21 GMT (10:21 EDT) today, from the Plesetsk Cosmodrome in northern Russia. The weather was fine and mission managers were optimistic with seconds to liftoff — and then, everything froze. With seven seconds left on the countdown clock, an unexpected hold went into place and ESA broadcasters simply stopped talking.

Update, 12:30 p.m. EDT: The ESA has announced that launch failed when the doors of the launch service tower did not open. The tower was held in position and did not move back as required for a launch. An investigation is under way, and the agency intends to try again tomorrow at the same time (15:21 CET; 14:21 GMT; 10:21 a.m. EDT).

GOCE is the first of a new family of ESA satellites, called Earth Explorers, designed to study our planet and its environment in order to improve our knowledge and understanding of Earth-system processes and their evolution, to characterize the challenges of global climate change.

The satellite is supposed to launch into a Sun-synchronous, near-circular polar orbit by a Russian Rockot vehicle – a converted SS-19 ballistic missile. Its specific mission is to map Earth’s gravity field with unprecedented accuracy, providing insight into ocean circulation, sea-level change, climate change, volcanism and earthquakes.

GOCE has been undergoing preparations for launch since it was taken out of storage around three weeks ago. Launch campaign activities included a series of mechanical and electrical tests, mating to the Upper Stage and finally encapsulation in the launcher fairing. A video of the anticipated fairing separation was produced pre-launch, and is available here.

Today’s go-ahead followed a successful countdown rehearsal conducted by ESA’s Mission Control Team, the Russian Mission Control Centre and the international tracking station network on Friday.

“We’ve been in this room for many hours and many days in the past. We want to do the real thing now,” said Paolo Laberinti, head of verification and testing, just moments before the seemingly foiled launch.

This isn’t the first time GOCE has encountered problems. The craft had to stand down from launch in September 2008 when problems were discovered with the guidance and navigation subsystems on the Russian Breeze KM rocket. GOCE had to be de-mated from the rocket and brought back into the clean room.

Stay tuned for updates to this post as the ESA releases details about the failure.

Source: ESA

Liftoff! Discovery Finally Leaves Earth for ISS

[/caption]

NASA’s space shuttle discovery launched successfully from Cape Canaveral Air Force Base at 7:43 p.m. (EDT) on Sunday, under flawless skies and without a single significant complication, despite past issues that had postponed the launch no less than five times.

Less than a minute after leaving the launch pad, Discovery was traveling 365 miles (578 kilometers) per hour. Less than two minutes after that, the craft was speeding away at 1,100 miles (17,000 kilometers) per hour and climbing, toward the International Space Station.

All three main engines performed perfectly throughout Discovery’s flight. Eight minutes after launch,  the twin solid rocket boosters burned out and fell away as the craft was traveling 17,500 miles (28,000 kilometers) an hour. 

Now that it’s orbiting Earth, it will take Discovery about two days to catch up to the International Space Station. 

Early Sunday afternoon, Launch Director Mike Leinbach sent a “red team” to launch pad 39A to manually correct a valve issue that caused a drop in helium pressure. But following that minor adjustment, NASA encountered no issues to delay the launch. 

In fact, the weather improved as the day went on. Original weather predictions had been 80 percent favorable for launch, but by 6 p.m. that prediction had been upgraded to 100 percent. 

Discovery’s payload includes technology to boost the station’s power capacity in line with doubling the size of the ISS crew from three to six in May.

The set of solar arrays that the STS-119 crew will be bringing up includes two solar array wings, each of which has two 115-foot-long arrays, for a total wing span of 240 feet, including the equipment that connects the two halves and allows them to twist as they track the sun. Altogether, the four sets of arrays can generate 84 to 120 kilowatts of electricity – enough to provide power for more than 40 average homes. Since the three existing arrays can handle the majority of the station’s day-to-day operational and life support needs, the newest solar array will double the amount of power available for scientific research. 

The Discovery crew has been bouncing between NASA’s Kennedy Space Center, in Florida, and the Johnson Space Center in Houston since late January; the first launch attempt was scheduled for early February. But four times, managers rescheduled the launch based on their concern following a hydrogen control valve malfunction on the shuttle Endeavour last fall. They wanted to rule out any similar glitches on Discovery.

Things were looking good for the fifth attempt on Wednesday — when skies would have been clear across much of the east coast — but a leak during refueling led to another cancellation.

Fueling of Discovery’s tank — with nearly 500,000 gallons of chilled liquid oxygen and hydrogen propellants  — went off Sunday morning without a hitch. 

Discovery’s flight is STS-119, but NASA has actually flown 131 missions with shuttles. Under the Obama administration, the shuttle program is expected to retire next year.

Discovery Launch: Sixth Attempt a Charm?

[/caption]

With just over four hours to go before launch, NASA is 80 percent optimistic that tonight’s Discovery launch will be a go — with the weather holding the only foreseeable wild card. Launch time is 7:43 p.m. local time (EDT) from the Cape Canaveral Air Force Station. 

Unfortunately for east coast skywatchers, a storm system that’s been dumping rain all weekend will obstruct a view of the launch that would otherwise be a beauty, as the shuttle will cruise northeast over the ocean nearly parallel to the shore. Without the clouds, the launch would have been visible as far west as the Appalachian Mountains, and as far north as the southern tip of Nova Scotia. 

But Florida’s weather is looking promising, partly cloudy (and 80 degrees at the time of this post) with an 80 percent chance of cooperating with the launch.

7:20 p.m. (EDT) update: With less than a half hour to go, daylight is fading under clear skies in Florida. Earlier, the weather forecast improved from 80 percent to 100 percent favorable for launch. NASA is reporting no problems.

The Discovery crew members are set to fly a new truss segment to the International Space Station and install the final set of power-generating solar arrays, boosting the station’s power capacity and paving the way for doubling the size of the ISS crew from three to six.

The Discovery crew has been bouncing between NASA’s Kennedy Space Center, in Florida, and the Johnson Space Center in Houston since late January; the first launch attempt was scheduled for early February. But four times, managers rescheduled the launch based on their concern following a hydrogen control valve malfunction on the shuttle Endeavour last fall. They wanted to rule out any similar glitches on Discovery.

Things were looking good for the fifth attempt on Wednesday — when skies would have been clear across much of the east coast — but a leak during refueling sent up another red flag. 

Understandably, this morning’s fueling was a bit tense. But for three hours beginning at 10:20 EDT, nearly 500,000 gallons of chilled liquid oxygen and hydrogen propellants flowed into Discovery’s external tank without incident. 

Two irregularities have been reported so far this afternoon: a bat was found clinging to Discovery’s external tank, and Launch Director Mike Leinbach sent a “red team” to launch pad 39A to manually correct a valve issue that caused a drop in helium pressure. 

Neither issue is expected to interfere with launch.

Stay tuned for updates, either to this post or a new one.

LEAD IMAGE CAPTION: NASA’s Discovery shuttle pictured under a full moon on Wednesday, when its fifth launch attempt was scrapped. Tonight marks the sixth. NASA/Bill Ingalls

Source: NASA