Kizimen
Volcano, which
erupted for the first time in 81 years in December 2010, continues to emit gas and ash. TheModerate Resolution Imaging
Spectroradiometer (MODIS) on NASA’s Terra satellite captured these natural-color
(top) and false-color (bottom) views of the eruption on November 1, 2012.
Though the plume is difficult to detect in true color, it shows up clearly in
false color because of the different
combination of bands used to create the two images. In the false-color image,
snow and ice appears bright red and vegetation looks green.
در تاریخ سیاره ی زمین ، گونه ی انسان دیر ، - بسیار دیر- پدید آمد؛ اما در همین زمان کوتاهی که بر روی زمین بوده است ، " دست آدمی" ، تغییرات ژرفی در هوا، در آب و خاک ، در دیگر موجودات زنده و در همه ی نظامی که بخش های گونه گون آن در پیوند بهم فشرده با یکدیگر ، بر هم کنش دارند و محیط زندگی او را می سازند، پدید آورده است . همه ی این ها در آخرین لحظه ی " زمان زمین شناسی " ، روی داده است .
۱۳۹۱ آبان ۱۶, سهشنبه
42-Foot High Tsunami Hit Geneva 1,500 Years Ago; Could Happen Again, Scientists Warn
We usually associate tsunamis with beachside property and the
seaboard, but what about the mountains? More importantly, how about the
postcard-worthy Swiss Alps? It may come as a shocker, but it seems that a
tsunami hit Geneva, Switzerland around 1,500 years ago inundating the shores
with up to 42 feet of water.
Historical accounts have mentioned the tsunami before, but this is the first time scientists have turned up geological evidence to support the claim. The findings, published in the journal Nature Geoscience, state that there is still a risk of this happening to inhabitants around Lake Geneva.
"It's certainly happened before and I think we can expect that it will probably happen again sometime," says one of the researchers, geologist Guy Simpson, from the University of Geneva.
Almost 200,000 people live in the city of Geneva, and somewhere around one million live around the shores of Lake Geneva. A tsunami with the magnitude of the 563 A.D. version would have devastating consequences on such a population density.
"Our numerical simulations with a shallow water model show that delta collapse in the lake generates a large tsunami at various locations along the shore, where a wave of 13 metres (42 feet) is observed after only 15 minutes, and at Geneva where a wave of eight metres (26 feet) arrives 70 minutes after the mass movement is initiated," said the researchers.
Historical accounts have mentioned the tsunami before, but this is the first time scientists have turned up geological evidence to support the claim. The findings, published in the journal Nature Geoscience, state that there is still a risk of this happening to inhabitants around Lake Geneva.
"It's certainly happened before and I think we can expect that it will probably happen again sometime," says one of the researchers, geologist Guy Simpson, from the University of Geneva.
Almost 200,000 people live in the city of Geneva, and somewhere around one million live around the shores of Lake Geneva. A tsunami with the magnitude of the 563 A.D. version would have devastating consequences on such a population density.
"Our numerical simulations with a shallow water model show that delta collapse in the lake generates a large tsunami at various locations along the shore, where a wave of 13 metres (42 feet) is observed after only 15 minutes, and at Geneva where a wave of eight metres (26 feet) arrives 70 minutes after the mass movement is initiated," said the researchers.
The 563
A.D. tsunami is believed to have come from a rock slide three miles from where
the River Rhone enters Lake Geneva in the east.
The team of researchers used radar to find a pile of sediment that is six miles long, five miles wide, and 16 feet thick in the deepest part of Lake Geneva. The scientists dated the sediment to between 381 A.D. and 612 A.D.
"Since the AD 563 event is the only significant natural event recorded in historical accounts within our calculated age interval, we consider our dating results to be a strong indication that the deposit is linked to the AD 563 rockfall and tsunami," wrote Katrina Kremer, according to the AFP.
In essence, it looks like nobody is really safe from Mother Nature, and towns and cities that live in a peaceful lull like some of those in the Alps should have emergency precautions at hand in case such a disasterous scenario occurs.
Read more at http://www.latinospost.com/articles/6284/20121031/42-foot-high-tsunami-hit-geneva-1.htm#El3mYU7ytTSMGedm.99
The team of researchers used radar to find a pile of sediment that is six miles long, five miles wide, and 16 feet thick in the deepest part of Lake Geneva. The scientists dated the sediment to between 381 A.D. and 612 A.D.
"Since the AD 563 event is the only significant natural event recorded in historical accounts within our calculated age interval, we consider our dating results to be a strong indication that the deposit is linked to the AD 563 rockfall and tsunami," wrote Katrina Kremer, according to the AFP.
In essence, it looks like nobody is really safe from Mother Nature, and towns and cities that live in a peaceful lull like some of those in the Alps should have emergency precautions at hand in case such a disasterous scenario occurs.
Read more at http://www.latinospost.com/articles/6284/20121031/42-foot-high-tsunami-hit-geneva-1.htm#El3mYU7ytTSMGedm.99
Asteroid Belts at Just the Right Place are Friendly to Life
This illustration
shows our solar-system model: a Jupiter-size planet moves slightly inward but
is just outside the asteroid belt. Image credit: NASA/ESA/STScI
November 01, 2012
PASADENA, Calif. -- Solar
systems with life-bearing planets may be rare if they are dependent on the
presence of asteroid belts of just the right mass, according to a study by
Rebecca Martin, a NASA Sagan Fellow from the University of Colorado in Boulder,
and astronomer Mario Livio of the Space Telescope Science Institute in
Baltimore, Md.
They suggest that the size and location of an asteroid belt, shaped by the evolution of the sun's planet-forming disk and by the gravitational influence of a nearby giant Jupiter-like planet, may determine whether complex life will evolve on an Earth-like planet.
This might sound surprising because asteroids are considered a nuisance due to their potential to impact Earth and trigger mass extinctions. But an emerging view proposes that asteroid collisions with planets may provide a boost to the birth and evolution of complex life.
Asteroids may have delivered water and organic compounds to the early Earth. According to the theory of punctuated equilibrium, occasional asteroid impacts might accelerate the rate of biological evolution by disrupting a planet's environment to the point where species must try new adaptation strategies.
The astronomers based their conclusion on an analysis of theoretical models and archival observations, including infrared data from NASA's Spitzer Space Telescope.
"Our study shows that only a tiny fraction of planetary systems observed to date seem to have giant planets in the right location to produce an asteroid belt of the appropriate size, offering the potential for life on a nearby rocky planet," said Martin, the study's lead author. "Our study suggests that our solar system may be rather special."
The findings will appear today in the Monthly Notices of the Royal Astronomical Society: Letters.
Martin and Livio suggest that the location of an asteroid belt relative to a Jupiter-like planet is not an accident. The asteroid belt in our solar system, located between Mars and Jupiter, is a region of millions of space rocks that sits near the "snow line," which marks the border of a cold region where volatile material such as water ice is far enough from the sun to remain intact. When Jupiter formed just beyond the snow line, its powerful gravity prevented nearby material inside its orbit from coalescing and building planets.
Instead, Jupiter's influence caused the material to collide and break apart. These fragmented rocks settled into an asteroid belt around the sun.
They suggest that the size and location of an asteroid belt, shaped by the evolution of the sun's planet-forming disk and by the gravitational influence of a nearby giant Jupiter-like planet, may determine whether complex life will evolve on an Earth-like planet.
This might sound surprising because asteroids are considered a nuisance due to their potential to impact Earth and trigger mass extinctions. But an emerging view proposes that asteroid collisions with planets may provide a boost to the birth and evolution of complex life.
Asteroids may have delivered water and organic compounds to the early Earth. According to the theory of punctuated equilibrium, occasional asteroid impacts might accelerate the rate of biological evolution by disrupting a planet's environment to the point where species must try new adaptation strategies.
The astronomers based their conclusion on an analysis of theoretical models and archival observations, including infrared data from NASA's Spitzer Space Telescope.
"Our study shows that only a tiny fraction of planetary systems observed to date seem to have giant planets in the right location to produce an asteroid belt of the appropriate size, offering the potential for life on a nearby rocky planet," said Martin, the study's lead author. "Our study suggests that our solar system may be rather special."
The findings will appear today in the Monthly Notices of the Royal Astronomical Society: Letters.
Martin and Livio suggest that the location of an asteroid belt relative to a Jupiter-like planet is not an accident. The asteroid belt in our solar system, located between Mars and Jupiter, is a region of millions of space rocks that sits near the "snow line," which marks the border of a cold region where volatile material such as water ice is far enough from the sun to remain intact. When Jupiter formed just beyond the snow line, its powerful gravity prevented nearby material inside its orbit from coalescing and building planets.
Instead, Jupiter's influence caused the material to collide and break apart. These fragmented rocks settled into an asteroid belt around the sun.
"To have such
ideal conditions you need a giant planet like Jupiter that is just outside the
asteroid belt [and] that migrated a little bit, but not through the belt,"
Livio explained. "If a large planet like Jupiter migrates through the
belt, it would scatter the material. If, on the other hand, a large planet did
not migrate at all, that, too, is not good because the asteroid belt would be
too massive. There would be so much bombardment from asteroids that life may
never evolve."
Using our solar system as a model, Martin and Livio proposed that asteroid belts in other solar systems would always be located approximately at the snow line. To test their proposal, Martin and Livio created models of planet-forming disks around young stars and calculated the location of the snow line in those disks based on the mass of the central star.
They then looked at all the existing space-based infrared observations from the Spitzer Space Telescope of 90 stars having warm dust, which could indicate the presence of an asteroid belt-like structure. The temperature of the warm dust was consistent with that of the snow line. "The warm dust falls right onto our calculated snow lines, so the observations are consistent with our predictions," Martin said.
The duo then studied observations of the 520 giant planets found outside our solar system. Only 19 of them reside outside the snow line. This suggests that most of the giant planets that may have formed outside the snowline have migrated too far inward to preserve the kind of slightly dispersed asteroid belt needed to foster enhanced evolution of life on an Earth-like planet near the belt. Apparently, less than four percent of the observed systems may actually harbor such a compact asteroid belt.
Using our solar system as a model, Martin and Livio proposed that asteroid belts in other solar systems would always be located approximately at the snow line. To test their proposal, Martin and Livio created models of planet-forming disks around young stars and calculated the location of the snow line in those disks based on the mass of the central star.
They then looked at all the existing space-based infrared observations from the Spitzer Space Telescope of 90 stars having warm dust, which could indicate the presence of an asteroid belt-like structure. The temperature of the warm dust was consistent with that of the snow line. "The warm dust falls right onto our calculated snow lines, so the observations are consistent with our predictions," Martin said.
The duo then studied observations of the 520 giant planets found outside our solar system. Only 19 of them reside outside the snow line. This suggests that most of the giant planets that may have formed outside the snowline have migrated too far inward to preserve the kind of slightly dispersed asteroid belt needed to foster enhanced evolution of life on an Earth-like planet near the belt. Apparently, less than four percent of the observed systems may actually harbor such a compact asteroid belt.
"Based on our scenario, we should concentrate our efforts to look for complex life in systems that have a giant planet outside of the snow line," Livio said.
The Sagan Fellowship Program is administered by the NASA Exoplanet Science Institute at the California Institute of Technology in Pasadena, Calif., whose purpose is to advance the scientific and technical goals of NASA's Exoplanet Exploration Program. The Exoplanet Exploration Program is managed for NASA by NASA's Jet Propulsion Laboratory in Pasadena, Calif. Caltech manages JPL for NASA.
More information about exoplanets and NASA's planet-finding program is at http://planetquest.jpl.nasa.gov .
JPL manages the Spitzer Space Telescope mission for NASA's Science Mission Directorate, Washington. Science operations are conducted at the Spitzer Science Center at Caltech. Data are archived at the Infrared Science Archive housed at the Infrared Processing and Analysis Center at Caltech.
For more information about Spitzer, visit http://spitzer.caltech.edu and http://www.nasa.gov/spitzer .
A Changed Coastline in Jersey
On October 29, 2012, lives were changed forever along the shores
of New Jersey, New York, Connecticut, and in the two dozen United States
affected by what meteorologists are calling Superstorm Sandy. The landscape of the East Coast was
also changed, though no geologist would ever use the word “forever” when
referring to the shape of a barrier island.
The two aerial photographs above show a portion of the New
Jersey coastal town of Mantoloking, just north of where Hurricane Sandy made
landfall. The top photograph was taken by the Remote Sensing Division of the National Oceanic and
Atmospheric Administration (NOAA) on October 31, 2012; the lower image was
acquired by the same group on March 18, 2007. The images were acquired from an
altitude of roughly 7,500 feet, using a Trimble Digital Sensor System.
The Mantoloking Bridge cost roughly $25 million when it was opened
in 2005 to replace a bridge built in 1938. After Sandy passed through on
October 29, 2012, the bridge was covered in water, sand, and debris from
houses; county officials closed it because they considered it unstable.
On the barrier island, entire blocks of houses along Route 35
(also called Ocean Boulevard) were damaged or completely washed
away by the storm
surge and wind. Fires raged in the town from natural gas lines that had
ruptured and ignited. A new inlet was cut across the island, connected the
Atlantic Ocean and the Jones Tide Pond.
1. References
2.
The Asbury Park
Press (2012, October 29) Update: Floating homes close
Mantoloking Bridge. Accessed
November 2, 2012.
3.
NOAA National Geodetic
Survey (2012) Hurricane Sandy Response Imagery. Accessed November 2, 2012.
4.
Point Pleasant
Patch (2012, October 31) Mantoloking Bridge Considered
Unstable; Fires Raging Nearby. Accessed
November 2, 2012.
Aerial photography courtesy of the NOAA Remote Sensing Division.
Caption by Mike Carlowicz.
Instrument:
Aircraft Sensors - Camera
۱۳۹۱ آبان ۱۲, جمعه
Sediment from Hurricane Sandy
As Hurricane Sandy moved north along the East Coast of the
United States, its waves churned up sediments from the continental shelf and
left turbid water in its wake. By midday October 30, 2012, the skies over
coastal Florida, Georgia, and South Carolina had cleared enough to reveal that
turbidity to the Visible Infrared Imaging Radiometer Suite (VIIRS) on the Suomi NPP satellite. Meanwhile, the remnants of
the storm were battering the northeastern states.
Note that the image is rotated so that you are looking south
from Canada, with north toward the bottom.
Europe's oldest prehistoric town unearthed in Bulgaria
Archaeologists in Bulgaria say they have
uncovered the oldest prehistoric town found to date in Europe.
The walled fortified settlement, near the
modern town of Provadia, is thought to have been an important centre for salt
production.
Its discovery in north-east Bulgaria may
explain the huge gold hoard found nearby 40 years ago.
Archaeologists believe that the town was home
to some 350 people and dates back to between 4700 and 4200 BC.
That is about 1,500 years before the start of
ancient Greek civilisation.
The residents boiled water from a local spring
and used it to create salt bricks, which were traded and used to preserve meat.
Salt was a hugely valuable commodity at the
time, which experts say could help to explain the huge defensive stone walls which
ringed the town.
'Extremely
interesting'
Excavations at the site, beginning in 2005,
have also uncovered the remains of two-storey houses, a series of pits used for
rituals, as well as parts of a gate and bastion structures.
A small necropolis, or burial ground, was
discovered at the site earlier this year and is still being studied by
archaeologists.
"We are not talking about a town like the
Greek city-states, ancient Rome or medieval settlements, but about what
archaeologists agree constituted a town in the fifth millennium BC," Vasil
Nikolov, a researcher with Bulgaria's National Institute of Archaeology, told
the AFP news agency.
Archaeologist Krum Bachvarov from the
institute said the latest find was "extremely interesting".
"The huge walls around the settlement,
which were built very tall and with stone blocks... are also something unseen
in excavations of prehistoric sites in south-east Europe so far," he told
AFP.
Similar salt mines near Tuzla in Bosnia and
Turda in Romania help prove the existence of a series of civilisations which
also mined copper and gold in the Carpathian and Balkan mountains during the
same period.
BBC Europe correspondent Nick Thorpe says this
latest discovery almost certainly explains the treasure found exactly 40 years
ago at a cemetery on the outskirts of Varna, 35km (21 miles) away, the oldest
hoard of gold objects found anywhere in the world.
A View Inside Sandy
Satellite instruments captured numerous
images of
Hurricane Sandy—using both daylight and moonlight—as
the enormous storm approached the heavily-populated East Coast of the United
States in late October 2012. In most cases, these instruments observed just the
uppermost layer of clouds at the top of the storm.
However, one satellite—Cloudsat—peered
inside the storm and observed its vertical structure. It did so with a cloud-profiling radar that sent pulses of energy toward
Earth and recorded the strength of the signal that bounced off ice and water
particles.
The bottom map shows the storm as observed by Cloudsat around 2
p.m. local time (18:00 Universal Time) on October 29, 2012. The image shows a
cross-section—what the storm would look like if it had been sliced near the
middle and viewed from the side. (Watch this animation to see how Cloudsat collects data).
The top image, acquired the same day by the Moderate Resolution Imaging
Spectroradiometer on
the Aqua satellite,
is shown for reference. The yellow line is the north-to-south track that
CloudSat took over the storm.
In the Cloudsat data, the darkest blues represent areas where
clouds and raindrops reflected the strongest signal back to the satellite
radar. These areas had the heaviest precipitation and the largest water
droplets. The blue line in the center of the image is the freezing line; ice
particles formed above it, raindrops below it. Though they look similar from
above, the thin clouds on the far left of the image at an altitude between
about 6 and 10 kilometers (4 and 6 miles) are cirrus clouds producing little or
no precipitation.
Another clue to the intensity and concentration of precipitation
is visible at the bottom of the image. In areas with fewer clouds and less
vigorous precipitation, enough radar signals made it all the way to the ground
to create the blue line along the bottom. In areas with heavy precipitation,
the line is absent because so much of the radar’s signal was scattered before
reaching the ground.
Sandy was an unusual hybrid
storm that
included features of both a tropical
cyclone and
an extratropical winter
storm. The offshore tropical storm merged with a storm system approaching from
the west, giving Sandy a cloud structure that was different than most
hurricanes and typhoons.
Sandy’s clouds, for instance, reached about 10 kilometers (6
miles) at their highest point—not as high as the clouds of many tropical
cyclones. For comparison, Hurricane
Earl and Super
Typhoon Choi-Wan’s both
reached about 15 kilometers (9 miles).
Sandy’s cloud field was also unusually wide—about 1,200
kilometers (750 miles) from one end to the other—because the storm was in the
process of becoming an extratropical cyclone. Tropical cyclones tend to have tight,
circular cloud bands that are about 400 kilometers (250 miles) from edge to
edge (or end to end). Extratropical cyclone bands often stretch more than 800
kilometers (500 miles).
Scientists are creating a database of Cloudsat overpasses in order to
better understand how storms work. Natalie
Tourville, a
research meteorologist at Colorado State University who studies tropical
cyclones, explained some of the ways that Cloudsat has proven useful since it
launched in 2006.
“CloudSat is providing exceptional views of the internal
structure of
tropical cyclones, with at least 30 eye
overpassesglobally,” she said. “We’ve been able to sample eye
wall slope
and view the vertical details of the convective
core regions. This
includes where and how large these cores are and how high the cloud tops are.
We've also sampledovershooting
cloud tops (some
extend over 17 kilometers into the atmosphere) and provide detailed analysis of
exactly what is underneath the cirrus clouds of these storm systems.”
Scientists have also developed an innovative technique that uses
Cloudsat measurements, in conjunction with data from other satellites, to
estimate storm intensity—something that has proven challenging to do from
space. A team of researchers first described the technique in an article published
in IEEE
Geoscience and Remote Sensing Letters in 2008. Tourville is currently
working on a follow-up project that aims to improve the technique by using more
recent Cloudsat data.
1.
Further Reading
2.
Durden, S. (2009) Cloudsat
and A-Train Observations of Tropical Cyclones. The Open Atmospheric Journal.
5.
Posselt, D. (2008,
May) Cloudsat Adding a New Dimension to a Classical View of
Extratropical Cyclones. Bulletin of the American
Meteorological Society.
6.
Stephens, G.L.
(2008, January) On the Use of CloudSat and
MODIS Data for Estimating Hurricane Intensity.Geosciences
and Remote Sensing Letters.
NASA Earth Observatory image by Jesse Allen, using CloudSat
FirstLook data provided courtesy of the CloudSat
team at Colorado State University. Caption by Adam Voiland.
Instrument:
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