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Cloud Streets in the Bering Sea: Ice, wind, cold temperatures and ocean waters combined to created dramatic cloud formations over the Bering Sea in late January 2015. The Moderate Resolution Imaging Spectroradiometer (MODIS) aboard NASA's Aqua satellite passed over the region and captured this true-color image on Jan. 23. The frozen tundra of Russia lies in the northwest of the image, and snow-covered Alaska lies in the northeast. Sea ice extends from the land well into the Bering Sea. Over the dark water bright white clouds line in up close, parallel rows. These formations are known as "cloud streets". Air blowing over the cold, snowy land and then over ice becomes both cold and dry. When the air then moves over relatively warmer and much moister water and lead to the development of parallel cylinders of spinning air. On the upper edge of these cylinders of air, where the air is rising, small clouds form. Where air is descending, the skies are clear. This clear/cloudy pattern, formed in parallel rows, gives the impression of streets. Image Credit: NASA/Jeff Schmaltz, MODIS Land Rapid Response Team, NASA GSFC #nasa #earth #earthrightnow #beringsea #modis #aqua #satellite #clouds #science; -
Meanwhile, 20,000 light years this Supernova Sunday, one of only three supernova remnants in the Milky Way known to contain large amounts of oxygen. These oxygen-rich supernovas are of great interest to astronomers because they are one of the primary sources of the heavy elements (that is, everything other than hydrogen and helium) necessary to form planets and people. The X-ray image from Chandra shows a rapidly expanding, intricately structured, debris field that contains, along with oxygen (yellow and orange), other elements such as magnesium (green) and silicon and sulfur (blue) that were forged in the star before it exploded. Image credit: NASA/CXC/SAO #supernovasunday #supernova #nasa #space #science #chandra #superbowl #sb49; -
Echoes of a Stellar Ending on Supernova Sunday: Over 11,000 years ago, a massive, supergiant star came to the end of its life. The star's core collapsed to form an incredibly dense ball of neutrons, and its exterior was blasted away in an immense release of energy astronomers call a supernova. The light from this supernova first reached Earth from the direction of the constellation Cassiopeia around 1667 A.D. If anyone alive at the time saw it, they left no records. It is likely that large amounts of dust between the dying star and Earth dimmed the brightness of the explosion to the point that it was barely, if at all, visible to the unaided eye. The remnant of this supernova was discovered in 1947 from its powerful radio emission. Listed as Cassiopeia A, it is one of the brightest radio sources in the whole sky. More recently, the Wide-field Infrared Survey Explorer (WISE), detected infrared echoes of the flash of light rippling outwards from the supernova. In the image, the central bright cloud of dust is the blast wave moving through interstellar space heating up dust as it goes. The colors used in this image represent specific wavelengths of infrared light. Blue and cyan (blue-green) represent light emitted predominantly from stars at wavelengths of 3.4 and 4.6 microns. Green and red represent light mostly emitted by dust at 12 and 22 microns, respectively. Image credit: NASA/JPL-Caltech/UCLA #supernovasunday #supernova #nasa #space #science #chandra #superbowl #sb49; -
A Supernova Remnant on Supernova Sunday! 3C58 is the remnant of a supernova observed in the year 1181 AD by Chinese and Japanese astronomers. This new Chandra image shows the center of 3C58, which contains a rapidly spinning neutron star surrounded by a thick ring, or torus, of X-ray emission. The pulsar also has produced jets of X-rays blasting away from it to both the left and right, and extending trillions of miles. These jets are responsible for creating the elaborate web of loops and swirls revealed in the X-ray data. These features, similar to those found in the Crab, are evidence that 3C58 and others like it are capable of generating both swarms of high-energy particles and powerful magnetic fields. In this image, low, medium, and high-energy X-rays detected by Chandra are red, green, and blue respectively. Image credit: NASA/CXC/SAO #supernovasunday #supernova #nasa #space #science #chandra #superbowl #sb49; -
A Supernova Remnant on Supernova Sunday! 3C58 is the remnant of a supernova observed in the year 1181 AD by Chinese and Japanese astronomers. This new Chandra image shows the center of 3C58, which contains a rapidly spinning neutron star surrounded by a thick ring, or torus, of X-ray emission. The pulsar also has produced jets of X-rays blasting away from it to both the left and right, and extending trillions of miles. These jets are responsible for creating the elaborate web of loops and swirls revealed in the X-ray data. These features, similar to those found in the Crab, are evidence that 3C58 and others like it are capable of generating both swarms of high-energy particles and powerful magnetic fields. In this image, low, medium, and high-energy X-rays detected by Chandra are red, green, and blue respectively. Image credit: NASA/CXC/SAO #supernovasunday #supernova #nasa #space #science #chandra #superbowl #sb49;
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A Superstar on this #SupernovaSunday! The Eta Carinae does not lack for superlatives. Not only does it contain one of the biggest and brightest stars in our galaxy, weighing at least 90 times the mass of the sun, it is also extremely volatile and is expected to have at least one supernova explosion in the future. Astronomers reported extremely volatile behavior from Eta Carinae in the 19th century, when it became very bright for two decades, outshining nearly every star in the entire sky. This event became known as the "Great Eruption." Data from modern telescopes reveal that Eta Carinae threw off about ten times the sun's mass during that time. Surprisingly, the star survived this tumultuous expulsion of material, adding "extremely hardy" to its list of attributes. Today, astronomers are trying to learn more about the two stars in the Eta Carinae system and how they interact with each other. The heavier of the two stars is quickly losing mass through wind streaming away from its surface at over a million miles per hour. While not the giant purge of the Great Eruption, this star is still losing mass at a very high rate that will add up to the sun's mass in about a millennium. Image Credit: NASA, ESA, and the Hubble SM4 ERO Team #supernova #nasa #space #science #chandra #superbowl #sb49; -
Supernova Sunday! It’s our second annual #SupernovaSunday! Let’s kick off w/ some crab, crab nebula: This image shows a composite view of the Crab nebula, an iconic supernova remnant in our Milky Way galaxy, as viewed by the Herschel Space Observatory and the Hubble Space Telescope. A wispy and filamentary cloud of gas and dust, the Crab nebula is the remnant of a supernova explosion that was observed by Chinese astronomers in the year 1054. The image combines Hubble's view of the nebula at visible wavelengths, obtained using three different filters sensitive to the emission from oxygen and sulphur ions and is shown here in blue. Herschel's far-infrared image reveals the emission from dust in the nebula and is shown here in red. Image credit: ESA/Herschel/PACS/MESS Key Programme Supernova Remnant Team; NASA, ESA and Allison Loll/Jeff Hester (Arizona State University) #supernova #nasa #space #science #chandra #superbowl #sb49; -
Did you know the International Space Station, including its large solar arrays, spans the area of a U.S. football field, including the end zones, and weighs over 900,000 pounds? The complex has more livable room than a conventional six-bedroom house, and has two bathrooms, a gymnasium and a 360-degree bay window. The big game on today will be broadcast during the space station astronauts' sleep period. Flight controllers are expected to uplink the game to the crew, and they has the option to watch in real-time or later when time permits. #nasa #iss #space #superbowl #sb49 #spacestation #astronauts; -
Gravitational Waves from Early Universe Remain Elusive : The color scale in this image from the Planck mission represents the emission from dust, a minor but crucial component that pervades our Milky Way galaxy. The texture indicates the orientation of the galactic magnetic field. It is based on measurements of the direction of the polarized light emitted by the dust. The highlighted region shows the position of a small patch of the sky that was observed with two ground-based experiments at the South Pole, BICEP2 and the Keck Array. The image shows that dust emission is strongest along the plane of the galaxy, in the upper part of the image, but that it cannot be neglected even in other regions of the sky. The small cloud visible in red, to the upper right of the BICEP2 field, shows dust emission from the Small Magellanic Cloud, a satellite galaxy of the Milky Way. Image Credit: ESA/Planck Collaboration #nasa #planck #esa #bigbang #galaxy #science; -
Galaxy Arp 230's irregular shape is thought to be the result of a violent collision with another galaxy sometime in the past. The collision could also be held responsible for the formation of the galaxy's polar ring. The outer ring surrounding the galaxy consists of gas and stars and rotates over the poles of the galaxy. It is thought that the orbit of the smaller of the two galaxies that created Arp 230 was perpendicular to the disk of the second, larger galaxy when they collided. In the process of merging the smaller galaxy would have been ripped apart and may have formed the polar ring structure astronomers can observe today. Image Credit: ESA/Hubble & NASA #hst #hubble #hubble25 #space #nasa #galaxy #astronomy #science;
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And We Have Liftoff! A United Launch Alliance Delta II rocket with the Soil Moisture Active Passive (SMAP) observatory onboard launches from Space Launch Complex 2, at 9:22 a.m. EST Saturday, Jan. 31, 2015, Vandenberg Air Force Base, Calif. SMAP is NASA's first Earth-observing satellite designed to collect global observations of surface soil moisture and its freeze/thaw state. SMAP will provide high resolution global measurements of soil moisture from space. The data will be used to enhance scientists' understanding of the processes that link Earth's water, energy, and carbon cycles. Image Credit: (NASA/Bill Ingalls) #nasa #ula #space #deltaii #earth#earthrightnow#science; -
Ready to launch! The moon is seen above the United Launch Alliance Delta II rocket with the Soil Moisture Active Passive (SMAP) observatory onboard shortly after the mobile service tower was rolled back, at the Space Launch Complex 2, Friday, Jan. 30, 2015, Vandenberg Air Force Base, Calif. Scheduled to launch at 9:20 a.m. EST, SMAP is our first Earth-observing satellite designed to collect global observations of surface soil moisture and its freeze/thaw state. SMAP will provide high resolution global measurements of soil moisture from space. The data will be used to enhance scientists' understanding of the processes that link Earth's water, energy, and carbon cycles. Photo Credit: (NASA/Bill Ingalls) #nasa #ula #space #deltaii #earth #earthrightnow#science; -
Sounding Rockets Launch Into an Aurora: The interaction of solar winds and Earth’s atmosphere produces northern lights, or auroras, that dance across the night sky and mesmerize the casual observer. However, to scientists this interaction is more than a light display. It produces many questions about the role it plays in Earth’s meteorological processes and the impact on the planet’s atmosphere. To help answer some of these questions, our suborbital sounding rockets carrying university-developed experiments into auroras from the Poker Flat Research Range in Alaska. The experiments explore the Earth’s atmosphere’s response to auroral, radiation belt and solar energetic particles and associated effects on nitric oxide and ozone. This composite shot of all four sounding rockets for the M-TeX and MIST experiments is made up of 30 second exposures. Image Credit: NASA/Jamie Adkins #nasa #aurora #space #earth #atmosphere #science; -
The United Launch Alliance Delta II rocket with the Soil Moisture Active Passive (SMAP) observatory onboard is seen as the mobile service tower is moved back to help workers service the rocket at Space Launch Complex 2, Thursday, Jan. 29, 2015, Vandenberg Air Force Base, Calif. During inspections following the Jan. 29 launch attempt, minor “debonds” to the booster insulation were identified; a standard repair is being implemented. SMAP is NASA’s first Earth-observing satellite designed to collect global observations of surface soil moisture and its freeze/thaw state. SMAP will provide high resolution global measurements of soil moisture from space. The data will be used to enhance scientists' understanding of the processes that link Earth's water, energy, and carbon cycles. Photo Credit: (NASA/Bill Ingalls) #nasa #ula #space #deltaii #earth #earthrightnow #science; -
Hubble Spies a Loopy Galaxy: This NASA Hubble Space Telescope photo of NGC 7714 presents an especially striking view of the galaxy's smoke-ring-like structure. The golden loop is made of sun-like stars that have been pulled deep into space, far from the galaxy's center. The galaxy is located approximately 100 million light-years from Earth in the direction of the constellation Pisces. The universe is full of such galaxies that are gravitationally stretched and pulled and otherwise distorted in gravitational tug-o'-wars with bypassing galaxies. The companion galaxy doing the "taffy pulling" in this case, NGC 7715, lies just out of the field of view in this image. A very faint bridge of stars extends to the unseen companion. The close encounter has compressed interstellar gas to trigger bursts of star formation seen in bright blue arcs extending around NGC 7714's center. The gravitational disruption of NGC 7714 began between 100 million and 200 million years ago, at the epoch when dinosaurs ruled the Earth. Image Credit: NASA/ESA #hst #hubble #hubble25 #nasa #space #galaxy #science;
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