Tag Archives: extreme

25ft space simulator

This chamber is used to test unmanned spacecraft in environments similar to what they will experience in space and on other planets. It is designed to simulate extreme cold, high vacuuum, and intense solar radiation.

The stainless steel chamber is 27′ in diameter and 85′ high. It operates at a pressure equivalent to an altitude of 125 miles. It has a temperature range of -320–250° Fahrenheit. The sun is simulated by an array of 37 30kW compact arc lamps. The light from these lamps is focused through a lens and passes into the chamber through a quartz window. The light is focused on the mirrored ceiling of the simulator and is reflected down towards the chamber floor.

NASA Jet Propulsion Laboratory
California Institute of Technology, Pasadena

By: kara brugman

Sounding Rockets Study How Winds In Space Drive Currents in the Upper Atmosphere

NASA release July 5, 2011

Some 50 miles up in the sky begins a dynamic region of the atmosphere known as the ionosphere. The region is filled with charged particles created by extreme ultraviolet radiation from the sun. At the base of the ionosphere, charged particle motions create a global current called the "atmospheric dynamo." Generally moving in loops from the equator to the poles, the dynamo changes daily based on solar heating and magnetic activity – but what keeps it moving isn’t well understood.

This July, scientists will launch four rockets from NASA’s Wallops Flight Facility, Va., for a five-minute journey some 100 miles up into the atmosphere. The rockets will collect data on the charged particles as well as winds of neutral particles that sweep through the lower ionosphere and how each affects the other, ultimately causing these dynamo currents.

A chemical trail like the one here – this one deployed from a sounding rocket at night as opposed to in the daytime – will help researchers track wind movement to determine how it affects the movement of charged particles in the atmosphere.

Credit: NASA

To read more go to: www.nasa.gov/mission_pages/sunearth/news/rockets-atmosphe…

NASA Goddard Space Flight Center enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission.

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By: NASA Goddard Photo and Video

Deep Space LIVE / Adrenalin

Deep Space LIVE was the place to go for a real live adrenalin rush on November 11, 2010. The screening featured incredible images of extreme athletes whose daredevil stunts took them to the physical and mental limits. BASE jumping from the south face of Austria’s Dachstein, ice climbing in Japan, Canada and Italy, or trial biking over the rooftops of Linz—visitors were in for some pure excitement! With photos by Hermann Erber (AT).

credit: rubra

By: Ars Electronica

Extreme Stars Found Thriving in Galaxies "Death Zones"

           space  Extreme Stars Found Thriving in Galaxies "Death Zones"

“I was dumbfounded. These stars are truly ‘living on the edge. ‘

Don Neil, CalTech

“We’re finding stars in extreme galactic environments where star formation isn’t supposed to happen,” explains NASA GALEX project scientist Susan Neff of the Goddard Space Flight Center. “This is a very surprising development.”

The image above shows long octopus-like arms of star formation stretching far away from the main disk of spiral galaxy M83. Like our own Milky Way Galaxy. M83, is a prominent member of a group of galaxies that includes Centaurus A and NGC 5253, all of which lie about 15 million light years distant. To date, six supernova explosions have been recorded in M83. An intriguing double circumnuclear ring has been discovered at the center of M83.GALEX, which stands for “Galaxy Evolution Explorer,” is an ultraviolet space telescope with a special ability: It is super-sensitive to the kind of UV rays emitted by the youngest stars.  This means the observatory can detect stars being born at very great distances from Earth, more than halfway across the Universe.  The observatory was launched in 2003 on a mission to study how galaxies change and evolve as new stars coalesce inside them.

“In some GALEX images, we see stars forming outside of galaxiesin places where we thought the gas density would be too low for star birth to occur,” says GALEX team member Don Neil of Caltech. Stars are born when interstellar clouds of gas collapse and contract under the pull of their own gravity.  If a cloud gets dense and hot enough as it collapses, nuclear fusion will kick in and—voila!–a star is born. The spiral arms of the Milky Way are a “goldilocks zone” for this process.  ”Here in the Milky Way we have plenty of gas.  It’s a cozy place for stars to form,” says Neil.

But when GALEX looks at other more distant spiral galaxies, it sees stars forming far outside the gassy spiral disk. 

The observatory has also found stars being born:

–in elliptical and irregular galaxies thought to be gas-poor (e.g., 1, 2)–in the gaseous debris of colliding galaxies (1, 2)–in vast “comet-like” tails that trail behind some fast-moving galaxies (1, 2)–in cold primordial gas clouds, which are small and barely massive enough to hang together.

According to GALEX, stellar extremophiles populate just about every nook and cranny of the cosmos where a wisp of gas can get together to make a new sun.

“This could be telling us something profound about the star-forming process,” says Neff.  “There could be ways to make stars in extreme environments that we haven’t even thought of yet.”

The Daily Galaxy via Science@NASA
Image credits:

FORS Team, 8.2-meter VLT, ESO
 

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