Where am I? > Home > News > Astronomy

Key process for space outpost proved on 'vomit comet' ride

Science Centric | 26 September 2009 10:36 GMT
Printable version A clip for your blog or website E-mail the story to a friend
Bookmark or share the story on your social network Vote for this article Leave a comment Decrease text size Increase text size
DON'T MISS —
Ghostly 'spokes' puff out from Saturn's ring's
Ghostly 'spokes' puff out from Saturn's ring's — [15 Nov 2009] — Massive, bright clouds of tiny ice particles hover above the darkened rings of Saturn in an image captured by the Cassini...
Exoplanets clue to sun's curious chemistry
Exoplanets clue to sun's curious chemistry — [12 Nov 2009] — 'For almost 10 years we have tried to find out what distinguishes stars with planetary systems from their barren cousins,'...
Opening up a colourful cosmic jewel box
Opening up a colourful cosmic jewel box — [29 Oct 2009] — Star clusters are among the most visually alluring and astrophysically fascinating objects in the sky. One of the most spectacular...
32 new exoplanets found
32 new exoplanets found — [20 Oct 2009] — 'HARPS is a unique, extremely high precision instrument that is ideal for discovering alien worlds,' says Stephane Udry,...
More Astronomy...

Flying high over the Gulf of Mexico, researchers from NASA and Case Western Reserve University found a key to unlocking oxygen from the surface of the moon.

The celestial body has no atmosphere like Earth's, holding the precious element just a breath away. But, oxygen to breathe, grow food, create water and burn rocket fuel - to make a space outpost a reality - is trapped in its soils.

Scientists from NASA and Case Western Reserve are designing and testing components of an oxygen generator that would extract the element from silicon dioxide and metal oxides in the ground. They have designed sifters needed to produce a consistent supply of oxides. But, how would the sifters work in the moon's gravity, which is about one-sixth as strong as the Earth's?

To find out, Katie Fromwiller, a senior civil engineering student, and Julie Kleinhenz, an assistant research professor of aerospace and mechanical engineering, spent two days flying in high arcs off the Texas coast last month.

This was Fromwiller's first trip on the plane, which space researchers refer to as the 'vomit comet,' due to the unsettling ride. Inside the plane, the pull of gravity approximated the moon's weak gravity during the rapid drop in each arc. The riders felt twice the pull of the Earth's gravity on the way back up. During two runs, they floated in zero gravity.

'Not in a million years would I have ever expected to do something like this with NASA,' said Fromwiller, who is also a member of the Case Western Reserve women's soccer team and the Voices of Glory chorus.

But, the space agency wants to learn how to work with the soils, and Fromwiller's focus is geotechnical engineering. She teamed with Kleinhenz, a veteran of more than 1,000 hours on the vomit comet.

'It was as if they were working on the moon, 20 seconds at a time,' said David Zeng, Frank H. Neff Professor and Chair of Civil Engineering from the Case School of Engineering and one of the principal investigators of the study.

NASA engineers were testing other components of the oxygen generator on the same flight.

NASA, Kleinhenz explained, has plans to build a system that includes a rover that would dig, carry and dump moon soil into a hopper or holding vessel. Sifters would separate particles by size, collecting those that can be converted most efficiently. The particles can also be separated by composition. For example, an electrostatic charger can be used to isolate iron oxides from other soil materials.

The wanted particles would then be blown into a reactor with hydrogen and heated to 2,000 degrees Fahrenheit. At this time, the oxygen released from the oxides would attach to the hydrogen and be collected.

While in flight, the pair tested two kinds of devices, a vibro-sieve and a sifter. As the plane reached lunar gravity, Fromwiller switched on a vibration table that shook a sieve, similar to a perforated pan used to pan for gold. As on Earth, the process worked.

Kleinhenz worked a sifter that operates much like a flour sifter. It, too, was able to separate particles in low gravity.

Zeng and his team are continuing to analyse data produced over the two days. Ultimately, NASA will decide which kind of device to use in the oxygen generator.

Funding for the continued project may be in jeopardy now that a White House advisory panel concluded NASA would need an additional $3 billion annually to return to the moon by 2020 and the funding might be better used elsewhere. But, the panel also said Mars should be the ultimate destination for manned missions.

'The technology is useful outside the lunar system,' Kleinhenz said. 'It's applicable to Mars.'

Source: Case Western Reserve University

This image shows an artist's conception of the bubble around our solar system moving through the interstellar medium, the matter that fills the local region of our galaxy. New observations from the Cassini spacecraft orbiting Saturn suggest the shape resembles something like a slippery ball moving through smoke, (c) NASA/JPL-Caltech/JHUAPLCassini data help redraw shape of solar system

— 16 October 2009

Images from the Ion and Neutral Camera on NASA's Cassini spacecraft suggest that the heliosphere, the region of the sun's influence, may not have the comet-like shape predicted by existing... — full story

Astronomers obtained this portrait of Barnard's Galaxy using the Wide Field Imager attached to the 2.2-metre MPG/ESO telescope at ESO's La Silla Observatory in northern Chile. Also known as NGC 6822, this dwarf irregular galaxy is one of the Milky Way's galactic neighbours. The dwarf galaxy has no shortage of stellar splendour and pyrotechnics. Reddish nebulae in this image reveal regions of active star formation, wherein young, hot stars heat up nearby gas clouds. Also prominent in the upper left of this new image is a striking bubble-shaped nebula. At the nebula's centre, a clutch of massive, scorching stars send waves of matter smashing into surrounding interstellar material, generating a glowing structure that appears ring-like from our perspective. Other similar ripples of heated matter thrown out by feisty young stars are dotted across Barnard's Galaxy, (c) ESOThe Milky Way's tiny but tough galactic neighbour

— 14 October 2009

In the new ESO image, Barnard's Galaxy glows beneath a sea of foreground stars in the direction of the constellation of Sagittarius (the Archer). At the relatively close distance of... — full story

Not surprisingly, interacting galaxies have a dramatic effect on each other. Studies have revealed that as galaxies approach one another massive amounts of gas are pulled from each galaxy towards the centre of the other, until ultimately, the two merge into one massive galaxy. NGC 2623 is in the late stages of the merging process, with the centres of the original galaxy pair now merged into one nucleus, but stretching out from the centre are two tidal tails of young stars, a strong indicator that a merger has taken place. During such a collision, the dramatic exchange of mass and gases initiates star formation, seen here in both the tails. The prominent lower tail is richly populated with bright star clusters - 100 of them have been found in these observations. These star clusters may have formed as part of a loop of stretched material associated with the northern tail, or they may have formed from debris falling back onto the nucleus. In addition to this active star-forming region, both galactic arms harbour very young stars in the early stages of their evolutionary journey, (c) NASA, ESA and A. Evans (Stony Brook University, New York)Sky merger yields sparkling dividends

— 13 October 2009

A recent NASA/ESA Hubble Space Telescope image captures what appears to be one very bright and bizarre galaxy, but is actually the result of a pair of spiral galaxies that resemble... — full story

This artist's conception shows a nearly invisible ring around Saturn - the largest of the giant planet's many rings. It was discovered by NASA's Spitzer Space Telescope, (c) NASA, JPL-Caltech, KeckSpitzer discovers an enormous ring around Saturn

— 8 October 2009

NASA's Spitzer Space Telescope has discovered an enormous ring around Saturn - by far the largest of the giant planet's many rings. The new belt lies at the far reaches of the Saturnian... — full story


Popular tags in Astronomy: Cassini · galaxies · Hubble · Mars