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The near drowning of a space-station astronaut from water that had collected in his helmet during a spacewalk stemmed from acceptance of unusual conditions known to increase risks.

Willingness to accept as routine minor amounts of water in a space-walking astronaut's helmet and a misdiagnosis of a previous water leak helped set the stage for an incident last summer that could have cost an International Space Station crew member his life, according to an analysis of the event.

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In a 122-page report released Wednesday, a mishap investigation board identified a range of causes for the near-tragedy, including organizational causes that carried echoes of accident reports that followed the loss of the shuttles Challenger and Columbia and their crews in 1986 and 2003.

About 44 minutes into a 6.5-hour spacewalk last July, Italian astronaut Luca Parmitano noted that water was building up inside his helmet the second consecutive spacewalk during which he reported the problem. Twenty-three minutes later, he and partner Chris Cassidy were ordered to end the spacewalk.

"The good news was that Luca was very close to the air lock when this happened," said Chris Hansen, space-station chiefengineer and head of the board,during a briefing Wednesday that outlined the findings. "When we terminated the EVA, Luca had a pretty close path to the air lock."

Still, as Parmitano worked his way back to the air lock, water covered his eyes, filled his ears, disrupted communications, and eventually began to enter his nose, making it difficult for him to breathe. Later, when crew mates removed his helmet, they found that it contained at least 1.5 quarts of water.

NASA officials immediately set up the five-member mishap investigation board to uncover the broader causes behind the incident, even as a team of engineers at the Johnson Space Center worked to find the precise mechanical cause for the buildup of water.

Engineers traced the leak to a fan-and-pump assembly that is part of a system that extracts moisture from the air inside the suit and returns it to the suit's water-based cooling system. Contaminants clogged holes that would have carried the water to the cooling system after it was extracted from the air. The water backed up and flowed into the suit's air-circulation system, which sent it into Parmitano's helmet. The specific cause of the contamination is still under investigation.

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Near-drowning of astronaut tied to wrong diagnosis, slow response

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Image Caption: European Space Agency astronaut Luca Parmitano, Expedition 36 flight engineer, attired in an Extravehicular Mobility Unit (EMU) spacesuit, participates in a session of extravehicular activity (EVA) as work continues on the International Space Station. A little more than one hour into the spacewalk, Parmitano reported water floating behind his head inside his helmet. The water was not an immediate health hazard for Parmitano, but Mission Control decided to end the spacewalk early. Credit: NASA

Lee Rannals for redOrbit.com Your Universe Online

Last year, European Space Agency (ESA) astronaut Luca Parmitano nearly drowned in space due to a leaky helmet, and yesterday NASA said this isnt the first time this suit model has misbehaved.

On July 16, 2013 two International Space Station crew members exited the US Airlock to begin a spacewalk. About 44 minutes into the spacewalk Parmitano reported water inside his helmet on the back of his head. Slowly the water began to fill up his helmet, and he was just moments away from actually drowning inside his own helmet while in space.

After this incident took place, NASA launched an investigation to help identify factors that may have contributed to the incident and it recommended changes that could be implemented to prevent it from happening again.

The investigation found that the same suit failure occurred a week earlier, and if this event was properly investigated it could have prevented Luca from being placed at risk the following week.

In summary, the causes for this mishap evolved from inorganic materials causing blockage of the drum holes in the EMU water separator resulting in water spilling into the vent loop; the NASA teams lack of knowledge regarding this particular failure mode; and misdiagnosis of this suit failure when it initially occurred on EVA 22, NASA said in its report.

The space agency said the inorganic materials blocking the water separator drum holes had not been seen during a spacewalk before and is still undergoing investigation. It said the investigation does not have the required data yet to determine the root causes of the contamination source.

Essentially, when the helmet first messed up the team misdiagnosed the problem, allowing Luca to be put in a position where he used the helmet. NASA said that had the issue been discussed in more detail at the end of the spacewalk, the team would have likely realized that the water experienced in the helmet needed to be investigated further before pressing ahead.

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Astronaut Nearly Drowning In Space Could Have Been Prevented

Dusty Space Cloud

This image shows the Large Magellanic Cloud galaxy in infrared light as seen by the Herschel Space Observatory, a European Space Agency-led mission with important NASA contributions, and NASA's Spitzer Space Telescope. In the instruments' combined data, this nearby dwarf galaxy looks like a fiery, circular explosion. Rather than fire, however, those ribbons are actually giant ripples of dust spanning tens or hundreds of light-years. Significant fields of star formation are noticeable in the center, just left of center and at right. The brightest center-left region is called 30 Doradus, or the Tarantula Nebula, for its appearance in visible light.

This enhanced-color image shows sand dunes trapped in an impact crater in Noachis Terra, Mars. Dunes and sand ripples of various shapes and sizes display the natural beauty created by physical processes. The area covered in the image is about six-tenths of a mile (1 kilometer) across. Sand dunes are among the most widespread wind-formed features on Mars. Their distribution and shapes are affected by changes in wind direction and wind strength. Patterns of dune erosion and deposition provide insight into the sedimentary history of the surrounding terrain.

This image obtained by the framing camera on NASA's Dawn spacecraft shows the south pole of the giant asteroid Vesta. Scientists are discussing whether the circular structure that covers most of this image originated by a collision with another asteroid, or by internal processes early in the asteroid's history. Images in higher resolution from Dawn's lowered orbit might help answer that question. The image was recorded with the framing camera aboard NASA's Dawn spacecraft from a distance of about 1,700 miles (2,700 kilometers). The image resolution is about 260 meters per pixel.

This undated photo shows a classic type 1a supernova remnant. Researchers Saul Perlmutter and Adam Riess of the United States and US-Australian Brian Schmidt won the 2011 Nobel Physics Prize on October 4, 2011 for their research on supernovae.

A quartet of Saturn's moons, from tiny to huge, surround and are embedded within the planet's rings in this Cassini composition. Saturn's largest moon, Titan, is in the background of the image, and the moon's north polar hood is clearly visible. See PIA08137 to learn more about that feature on Titan (3,200 miles, or 5,150 kilometers across). Next, the wispy terrain on the trailing hemisphere of Dione (698 miles, or 1,123 kilometers across) can be seen on that moon which appears just above the rings at the center of the image. See PIA10560 and PIA06163 to learn more about Dione's wisps. Saturn's small moon Pandora (50 miles, or 81 kilometers across) orbits beyond the rings on the right of the image. Finally, Pan (17 miles, or 28 kilometers across) can be seen in the Encke Gap of the A ring on the left of the image. The image was taken in visible blue light with the Cassini spacecraft narrow-angle camera on Sept. 17, 2011. The view was obtained at a distance of approximately 1.3 million miles (2.1 million kilometers) from Dione and at a Sun-Dione-spacecraft, or phase, angle of 27 degrees. Image scale is 8 miles (13 kilometers) per pixel on Dione.

Combining almost opposite ends of the electromagnetic spectrum, this composite image of the Herschel in far-infrared and XMM-Newton's X-ray images obtained January 20, 2012, shows how the hot young stars detected by the X-ray observations are sculpting and interacting with the surrounding ultra-cool gas and dust, which, at only a few degrees above absolute zero, is the critical material for star formation itself. Both wavelengths would be blocked by Earth's atmosphere, so are critical to our understanding of the lifecycle of stars . (AFP / Getty Images)

Resembling looming rain clouds on a stormy day, dark lanes of dust crisscross the giant elliptical galaxy Centaurus A. Hubble's panchromatic vision, stretching from ultraviolet through near-infrared wavelengths, reveals the vibrant glow of young, blue star clusters and a glimpse into regions normally obscured by the dust. (NASA / ESA / Hubble Heritage)

A bubbling cauldron of star birth is highlighted in this image from NASA's Spitzer Space Telescope. Infrared light that we can't see with our eyes has been color-coded, such that the shortest wavelengths are shown in blue and the longest in red. The middle wavelength range is green. Massive stars have blown bubbles, or cavities, in the dust and gas--a violent process that triggers both the death and birth of stars. The brightest, yellow-white regions are warm centers of star formation. The green shows tendrils of dust, and red indicates other types of dust that may be cooler, in addition to ionized gas from nearby massive stars.

This composite image shows the central region of the spiral galaxy NGC 4151. X-rays (blue) from the Chandra X-ray Observatory are combined with optical data (yellow) showing positively charged hydrogen (H II) from observations with the 1-meter Jacobus Kapteyn Telescope on La Palma. The red ring shows neutral hydrogen detected by radio observations with the NSF's Very Large Array. This neutral hydrogen is part of a structure near the center of NGC 4151 that has been distorted by gravitational interactions with the rest of the galaxy, and includes material falling towards the center of the galaxy. The yellow blobs around the red ellipse are regions where star formation has recently occurred. (NASA / CXC / CfA / J. Wang)

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Nasa 'Could Have Prevented' Astronaut's Near-Drowning In Space Walk