Sunday, September 22, 2013

Energy Storage


DLR energy, transport and materials research on German Aerospace Day
We all want energy to be available when we need it. During German Aerospace Day, energy researchers at the German Aerospace Center (Deutsches Zentrum für Luft- und Raumfahrt; DLR) will demonstrate how innovative storage devices can be used to efficiently harness energy. DLR solar researchers will show the public how much power is available from the Sun, and how they can put this energy to use in solar power plants. When people move from A to B, they want to do so quickly and easily; DLR transport researchers will show how this could be achieved in future, perhaps with fewer traffic jams. DLR materials scientists have their sights set on using 22 September to demonstrate how a 15-ton truck can remain suspended in the air for over an hour, bonded by an adhesive surface no larger than credit card. Visitors can also get to know ultra-lightweight and extremely stable materials at the Institute of Materials Research.


Wednesday, September 18, 2013

Signs of Change in our Atmosphere and Climate



The American Southwest is broiling in triple-digit temperatures for the fourth consecutive day as a result of a record-breaking heat wave that is smothering the region.
In Death Valley, California, the temperature reached 128° Fahrenheit (53° Celsius) on Sunday—just a few degrees shy of the July 10, 1913, record of 134° Fahrenheit (57° Celsius).
The heat wave has also been partly blamed for a wildfire that killed 19 firefighterson Sunday in Yarnell Hill, Arizona.
So what's behind the heat wave? Is global warming a factor? And how does it compare with past events? We talked to Martin Tingley, a climatologist at Harvard University, to find out.
In April, Tingley and his colleague Peter Huybers published a study in the journalNature that concluded that the years 2005, 2007, 2010 and 2011 were warmer than any year going back 600 years, to 1400.
Do scientists know what's behind the current heat wave?
Looking at the meteorological charts, it looks to be a blocking event. That happens when there's a particular configuration of the jet stream that's quite stable. So there's a big high-pressure ridge on the West Coast and a low-pressure trough in the East Coast. That's why it's quite rainy here [in Cambridge, Massachusetts] and very hot on the West Coast.
Have you or other scientists had a chance to analyze this current heat wave and determine how it compares to past years?
No ... because 2013 is not over yet. One very hot week will have some signature on the seasonal average, but how large that signature will be depends on what happens for the rest of the summer.
Also, the study that Peter [Huybers] and I did made use of paleoclimate records—things like tree rings and ice cores. One of the limitations of that study is we can't really think of week-long heat waves like what's going on. We were limited to seasonal averages—hot summers versus cool summers—and we found that recent warm extremes in terms of summer average conditions at the high northern latitudes are unprecedented in the last 600 years.
You reached those conclusions after performing a statistical analysis on the paleoclimate data. Do you have an analogy that helps explain how that analysis works?
One imperfect analogy: Even though you and I have never met, I would bet that I'm taller than you because I'm 6-foot-4-inches (1.9 meters), and that puts me in a high percentile of the distribution of heights. But if I were to walk into a room of 1,000 people, I probably wouldn't be the tallest.
It's the same when we're addressing the question of was 2011 the hottest year in the last 600 years. It's a different statistical question to ask was it warmer than one particular year in the past—that's like me saying I'm taller than you—and it's a much different question to ask whether 2011 was the hottest year amongst all of the past 600 years.
To deal with this, what we do is instead of coming up with a single best estimate ... we use a simple statistical model to simulate 4,000 equally likely realizations of the climate [based on the paleoclimate data]. Then we can ask in how many of these 4,000 possible climate histories was 2011 the warmest year? So instead of having a single best estimate, we have 4,000 possible realizations.
Climate scientists often compare the effects of global warming to loaded dice: Not every roll of a loaded die will come up six—but sixes will occur more often than if the die had not been tampered with. Is that still the thinking?
Can we attribute this particular heat wave to an anthropogenic impact on the climate? The only safe answer is, well, probably not. It's like if I flip one coin and it comes up heads, that doesn't mean the coin is loaded.
But what we're seeing now, there seems to be a trend toward more hot extremes and fewer cold extremes. That's a pattern that's consistent with an anthropogenically-forced increase in temperatures.
What can people expect from future extreme heat waves that are affected by global warming? Will they be anything like the current heat wave affecting the West Coast?
I think that's a really big open question right now: Given rising mean temperatures, how will the extremes change, in both magnitude and frequency? It's actually one of the research projects we are tackling at the moment: How are extremes in temperature on daily timescales changing with respect to the mean temperature?
If the mean temperature goes up by half a degree, do the extremes simply track that half-degree increase? Or are the extremes being amplified in some sense so that they are becoming hotter with respect to the mean?
As a climate scientist, are you doing anything personally to prepare for the hotter summers that will result from global warming?
Well, I like to ski a lot in the winter, and I'm concerned that ski conditions are becoming more variable, especially on the East Coast.
That's not really something that I've done in my life to prepare, but it's something that's given me a lot of pause. Will the slopes have consistent snow cover for the next generation of skiers, and will the tradition of East Coast skiing survive a warming climate?


Tuesday, September 10, 2013

Ceres classified as Dwarf planet, has icy surface


Dwarf Planet Ceres May Have Underground Ice, Scientists Say
In March of 2015, NASA's Dawn mission will arrive at the dwarf planet Ceres, the first of the smaller class of planets to be discovered and the closest to Earth.
The dwarf planet Ceres, which orbits the sun in the asteroid belt between Mars and Jupiter, is a unique body in the solar system, bearing many similarities to Jupiter's moon Europa and Saturn's moon Enceladus, both considered to be potential sources for harboring life.
On Thursday, August 15, Britney Schmidt, science team liaison for the Dawn Mission, and Julie Castillo-Rogez, planetary scientist from JPL, spoke in an Google Plus Hangout titled 'Ceres: Icy World Revealed?' about the growing excitement related to the innermost icy body. [Dwarf Planets of Our Solar System (Infographic)]
"I think of Ceres actually as a game changer in the solar system," Schmidt said.
"Ceres is arguably the only one of its kind."
The dwarf planet Ceres as seen by the Hubble Space Telescope.
The innermost icy body
When Ceres was discovered in 1801, astronomers first classified it as a planet. The massive body traveled between Mars and Jupiter, where scientists had mathematically predicted a planet should lie. Further observations revealed that a number of small bodies littered the region, and Ceres was downgraded to just another asteroid within the asteroid belt. It wasn't until Pluto was classified as a dwarf planet in 2006 that Ceres was upgraded to the same level.
Ceres is the most massive body in the asteroid belt, and larger than some of the icy moons scientists consider ideal for hosting life. It is twice the size of Enceladus, Saturn's geyser-spouting moon that may hide liquid water beneath its surface.
Unlike other asteroids, the Texas-sized Ceres has a perfectly rounded shape that hints toward its origins.
"The fact that Ceres is so round tells us that it almost certainly had to form in the early solar system," Schmidt said. She explained that a later formation would have created a less rounded shape.
The shape of the dwarf planet, combined with its size and total mass, reveal a body of incredibly low density.
"Underneath this dusty, dirty, clay-type surface, we think that Ceres might be icy," Schmidt said. "It could potentially have had an ocean at one point in its history."
"The difference between Ceres and other icy bodies [in the solar system] is that it's the closest to the sun," Castillo-Rogez said.
Less than three times as far as Earth from the sun, Ceres is close enough to feel the warmth of the star, allowing ice to melt and reform.
Investigating the interior of the dwarf planet could provide insight into the early solar system, especially locations where water and other volatiles might have existed.
"Ceres is like the gatekeeper to the history of water in the middle solar system," Schmidt said.


NASA Footage with unusual objects streaking by


While most of the objects streaking by are probably space junk or shooting stars, it
is interesting that there is so much movement near our planet. :)


Monday, September 9, 2013

Moon Launch images, impressive.

NASA's latest mission to the moon is notable not only for what it will accomplish, but also for how widely its start was seen. The fact that the Lunar Atmosphere and Dust Environment Explorer, or LADEE, was launched from Virginia's Mid-Atlantic Regional Spaceport after dark on Friday meant that the mission's Minotaur 5 rocket blast had a potential audience of millions of people.

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Friday, September 6, 2013

JWST'S NEAR INFRARED SPECTROGRAPH (NIRSPEC)

The Near InfraRed Spectrograph (NIRSpec) is one of four instruments on the James Webb Space Telescope (JWST). NIRSpec is a multi-object spectrograph capable of observing more than 100 astronomical objects simultaneously in a large field of view of ~ 3 arcminutes × 3 arcminutes. It will support JWST's four main science themes by providing low (R~100), medium (R~1000), and high-resolution (R~2700) spectroscopic observations.
NIRSpec measures 1.9m × 1.3m × 0.7 m and weighs approximately 200 kg. It is an all-reflective system with a total of 14 mirrors, seven interchangeable dispersive elements and eight interchangeable filters.
The black dome and horn-shaped assembly in the centre foreground is the calibration assembly. This will be used for on-orbit calibration and monitoring the performance of the instrument.
To the left, with one silver- and three gold-coloured squares arranged around a cylinder, is the grating wheel.
The filter wheel can just be seen at the centre, towards the back of the shot, with two of the eight interchangeable filters showing.
The camera, which focuses the light beam onto the focal plane assembly (not visible), is in the large silver box at the back left of the shot.
NIRSpec is developed by ESA with EADS Astrium Germany GmbH as the prime contractor.



Wednesday, September 4, 2013

Close up Video of International Space Station

Impressive video, although there is quite a bit of lint? or something on the camera outer cover.


WAIT FOR THE CLOSEUP, IT'S IMPRESSIVE. :)