Earth's Rotating Inner Core Shifts Its Speed
NASA/NOAA/GSFC/Suomi NPP/VIIRS/Norman Kuring
Western Hemisphere Feb. 24, 2012 -- We at Discovery News are loving the new photos of Earth coming in from VIIRS, the biggest and most important instrument of the five aboard NASA's Earth-observing satellite - Suomi NPP. These composite images are put together using a number of swaths of the Earth's surface taken with the Visible/Infrared Imager Radiometer Suite (VIIRS) over the course of a day as the Suomi NPP satellite orbits the planet from pole to pole. Here we see the western hemisphere from swaths taken on Jan. 4, 2012.
NASA/NOAA/GSFC/Suomi NPP/VIIRS/Norman Kuring
Eastern Hemisphere The Suomi NPP satellite flew over the eastern hemisphere six times during an eight hour time period on Jan 23, 2012. NASA scientist Norman Kuring took those six sets of data and combined them into this image shown here.
NASA/NOAA/GSFC/Suomi NPP/VIIRS/Norman Kuring
Australian View Here NASA scientist Norman Kuring has done the same with the VIIRS data sets taken on Feb. 8, 2012.
Arctic View The newly launched Suomi National Polar-orbiting Partnership (S-NPP) satellite, which was blasted into space on Oct. 28, 2011, circled the Earth 15 times to capture the visual data used for the stunning picture.
BIG PIC: White Marble View Over Arctic
Hot and Cold Here we see the results of the Clouds and the Earth's Radiant Energy System (CERES) instrument at work on the Suomi NPP satellite. "In the longwave image, heat energy radiated from Earth (in watts per square meter) is shown in shades of yellow, red, blue and white. The brightest-yellow areas are the hottest and are emitting the most energy out to space, while the dark blue areas and the bright white clouds are much colder, emitting the least energy. Increasing temperature, decreasing water vapor, and decreasing clouds will all tend to increase the ability of Earth to shed heat out to space," the NASA CERES team explained.
Image by NASA’s NPP Land Product Evaluation
Keeping Up with the Sun From its vantage 824 kilometers (512 miles) above Earth, the Visible Infrared Imager Radiometer Suite (VIIRS) on the NPOESS Preparatory Project (NPP) satellite gets a complete view of our planet every day. This image from Nov. 24, 2011, was the first complete global image from VIIRS. Rising from the south and setting in the north on the daylight side of Earth, VIIRS images the surface in long wedges measuring 3,000 kilometers (1,900 miles) across. The swaths from each successive orbit overlap one another, so that at the end of the day, the sensor has a complete view of the globe. The Arctic is missing because it is too dark to view in visible light during the winter. The NPP satellite was placed in a Sun-synchronous orbit, a unique path that takes the satellite over the equator at the same local (ground) time in every orbit. So, when NPP flies over Kenya, it is about 1:30 p.m. on the ground. When NPP reaches Gabon—about 3,000 kilometers to the west—on the next orbit, it is close to 1:30 p.m. on the ground. This orbit allows the satellite to maintain the same angle between the Earth and the Sun so that all images have similar lighting. The consistent lighting is evident in the daily global image. Stripes of sunlight (sunglint) reflect off the ocean in the same place on the left side of every swath. The consistent angle is important because it allows scientists to compare images from year to year without worrying about extreme changes in shadows and lighting. PHOTOS: Sunsets and Other Sky Wonders
Final Checks Electro Magnetic Interference testing of the Suomi NPP satellite at the Ball Aerospace facility.
Behind the Scenes By stitching six swaths together, NASA scientist Norman Kuring takes the Suomi NPP satellite perspective from its polar orbit around Earth at an altitude of 512 miles (about 824 kilometers), and changes it to a 'Blue Marble' view as though it were seen from 7,918 miles (about 12,743 kilometers).
NEWS: Earth's Mugshot Explained
Earth's solid-metal inner core is a key component of the planet, helping to give rise to the magnetic field that protects us from harmful space radiation, but its remoteness from the planet's surface means that there is much we don't know about what goes on down there. But some secrets of the inner core are being revealed by acoustic waves passing through the planet's heart and iron squeezed to enormous pressures in the lab.
Two new studies, both detailed online May 12 in the journal Nature Geoscience, reveal that Earth’s inner core may actually be softer than previously thought, and that the speed at which it spins can fluctuate over time.
Under the liquid-metal outer layer of the Earth's core is a solid ball of superhot iron and nickel alloy about 760 miles (1,220 kilometers) in diameter. Scientists recently discovered the inner core is, at 10,800 degrees Fahrenheit (6,000 degrees Celsius), as hot as the surface of the sun.
Churning in the liquid outer core results in the dynamo that generates Earth's magnetic field. Geoscientists think interactions between the inner and outer cores may help explain the nature of the planet's dynamo, the details of which remain largely unknown.
"The Earth's inner core is the most remote part of our planet, and so there is a lot we don't know about it because we can't go down and collect samples," said Arianna Gleason, a geoscientist at Stanford University in California. (Infographic: Tallest Mountain to Deepest Ocean Trench)
One way scientists can learn more about the inner core is by analyzing acoustic waves from earthquakes that ripple through the inner core as they pass through the planet. Hrvoje Tkalcic, a geophysicist at the Australian National University in Canberra, and his colleagues relied on earthquake doublets — earthquakes that occur in pairs and generate extraordinarily similar acoustic waves — to investigate the inner core. Because these waves are so alike, the data they return are readily comparable, and because they are separated relatively briefly in time, they can help the researchers image subtle changes that might occur in that time frame.
Seismic observations and computer models of the Earth's innards suggested the inner core spins at a different rate than the mantle does, but there were conflicting estimates for how fast the inner core actually rotated. By analyzing 24 earthquake doublets, Tkalcic and his collaborators found the speed at which the inner core spun apparently fluctuated over the course of approximately decades between 1961 and 2007.
"It is the first observational evidence that the inner core rotates at a variety of speeds with respect to the mantle...It also reconciles old discrepancies," Tkalcic told OurAmazingPlanet. (Past analyses of how fast the inner core rotated came up with different speeds.)
The inner core, on average, rotates eastward. At the speeds it travels, it might, on average, complete a revolution every 750 to 1,440 years. However, these speeds appear unstable, which makes it uncertain just how long it actually takes to finish a turn on its axis, Tkalcic said.
It remains unknown exactly why these fluctuations in speed happen. Gravitational and magnetic forces likely both play a part, Tkalcic said.
In another study, Gleason and her colleagues sought to learn more about the inner core by mimicking its conditions in the lab. They measured the strength of iron by squeezing it within a diamond anvil at room temperature while scanning it with X-rays.
"We know the Earth's inner core is composed mostly of iron, but we don't really know too much about the behavior of iron under the pressure and temperature at conditions in the core," Gleason said.
The metal was subjected to more than 200 billion pascals of pressure, or about 180,000 times the pressure of the average human bite.
"We found the inherent mechanical strength of iron under those conditions is quite low, surprisingly weak," Gleason said.
These findings may help explain why material within Earth's inner core is apparently distributed in a lopsided way, Gleason said. The weakness of iron might lead crystallites in the inner core to flow and line up a certain way, she explained.
Gleason noted that the researchers did not mimic the extreme temperatures found in the inner core, nor did the metal they experimented with match the composition of the inner core. In future experiments, they hope to use lasers to heat the metal to the proper temperatures, and test various iron-nickel alloys.
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