Spring Fling: Sun Emits a Mid-Level Flare

<div style="text-align: center;"><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhJxXECAQGCLog8o5MEauTZL5J5huFS1R-buFfxZtwuFa3-BxTFt5EeJjfDJd96GpwxYCT2M6MIKXFs_PFcA3JnGrbA_wXUs620Gpga9ogDaDcaUf2lxlUBXcZiSNjZ_4cvhskI8ReRHmUu/s1600/740798main_20130411-M6flare-orig_full.jpg"><img border="0" height="640" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhJxXECAQGCLog8o5MEauTZL5J5huFS1R-buFfxZtwuFa3-BxTFt5EeJjfDJd96GpwxYCT2M6MIKXFs_PFcA3JnGrbA_wXUs620Gpga9ogDaDcaUf2lxlUBXcZiSNjZ_4cvhskI8ReRHmUu/s640/740798main_20130411-M6flare-orig_full.jpg" width="640" /></a></div><div style="text-align: center;"><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEh5gmGW_IXRhY-PeetQUF3wOU44OwPWCeqw4wJ2AY0I7BcFz_3FJnmsDpPJd5YwWQzbUVmkSVTqIvoOVTzMCGUPBuDtATTlA9-_6l99R8R6a47byIobGFIAyxXM1QUiTkBt0-myCdTglby3/s1600/740854main_20130411-cmeC3-orig_full.jpg"><img border="0" height="320" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEh5gmGW_IXRhY-PeetQUF3wOU44OwPWCeqw4wJ2AY0I7BcFz_3FJnmsDpPJd5YwWQzbUVmkSVTqIvoOVTzMCGUPBuDtATTlA9-_6l99R8R6a47byIobGFIAyxXM1QUiTkBt0-myCdTglby3/s320/740854main_20130411-cmeC3-orig_full.jpg" width="320" /></a><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgHvauu71ukILZwW0H-yrhAeEUQ2yjfx01sqfjIptO-Go_kFBpPX3D3dipsdMqnCY1K1k5_q6t4L0fjrA7rQT3YwT_bbSt2s620IF8uJmeQLgexbAFirwFb2XlQLz0-sGubURpe7KCTmSO4/s1600/740857main_20130411-cmeC2-unlabeled.jpg"><img border="0" height="217" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgHvauu71ukILZwW0H-yrhAeEUQ2yjfx01sqfjIptO-Go_kFBpPX3D3dipsdMqnCY1K1k5_q6t4L0fjrA7rQT3YwT_bbSt2s620IF8uJmeQLgexbAFirwFb2XlQLz0-sGubURpe7KCTmSO4/s320/740857main_20130411-cmeC2-unlabeled.jpg" width="320" /></a></div><div style="text-align: center;"><br /></div><div><div style="text-align: center;">The M6.5 flare on the morning of April 11, 2013, was also associated with an Earth-directed coronal mass ejection (CME), another solar phenomenon that can send billions of tons of solar particles into space and can reach Earth one to three days later. CMEs can affect electronic systems in satellites and on the ground. Experimental NASA research models show that the CME began at 3:36 a.m. EDT on April 11, leaving the sun at over 600 miles per second.</div><div style="text-align: center;"><br /></div><div style="text-align: center;">Earth-directed CMEs can cause a space weather phenomenon called a geomagnetic storm, which occurs when they connect with the outside of the Earth's magnetic envelope, the magnetosphere, for an extended period of time.</div><div style="text-align: center;"><br /></div><div style="text-align: center;">The recent space weather also resulted in a weak solar energetic particle (SEP) event near Earth. These events occur when very fast protons and charged particles from the sun travel toward Earth, sometimes in the wake of a solar flare. These events are also referred to as solar radiation storms. Any harmful radiation from the event is blocked by the magnetosphere and atmosphere, so cannot reach humans on Earth. Solar radiation storms can, however, disturb the regions through which high frequency radio communications travel.</div><div style="text-align: center;"><br /></div><div style="text-align: center;">NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts, alerts, watches and warnings. NASA and NOAA – as well as the US Air Force Weather Agency (AFWA) and others -- keep a constant watch on the sun to monitor for space weather effects such as geomagnetic storms. With advance notification many satellites, spacecraft and technologies can be protected from the worst effects.</div><div style="text-align: center;"><br /></div><div style="text-align: center;">The sun emitted a mid-level flare, peaking at 3:16 a.m. EDT on April 11, 2013.</div><div style="text-align: center;"><br /></div><div style="text-align: center;">Solar flares are powerful bursts of radiation. Harmful radiation from a flare cannot pass through Earth's atmosphere to physically affect humans on the ground, however -- when intense enough -- they can disturb the atmosphere in the layer where GPS and communications signals travel. This disrupts the radio signals for as long as the flare is ongoing, anywhere from minutes to hours.</div><div style="text-align: center;"><br /></div><div style="text-align: center;">This flare is classified as an M6.5 flare, some ten times less powerful than the strongest flares, which are labeled X-class flares. M-class flares are the weakest flares that can still cause some space weather effects near Earth. This flare produced a radio blackout that has since subsided. The blackout was categorized as an R2 on a scale between R1 and R5 on NOAA’s space weather scales.<br /><br /></div><div><div style="text-align: center;">This is the strongest flare seen so far in 2013. Increased numbers of flares are quite common at the moment, since the sun's normal 11-year activity cycle is ramping up toward solar maximum, which is expected in late 2013. Humans have tracked this solar cycle continuously since it was discovered, and it is normal for there to be many flares a day during the sun's peak activity.</div><br />Images Credit: ESA&NASA/SOHO/GSFC<br />Explanation from: http://www.nasa.gov/mission_pages/sunearth/news/News031513-m6flare.html</div></div>

Spring Fling: Sun Emits a Mid-Level Flare

The M6.5 flare on the morning of April 11, 2013, was also associated with an Earth-directed coronal mass ejection (CME), another solar pheno...

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Starburst Galaxy M82

<div style="text-align: center;"><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhcschPpHDqzmEZREnbyNyfBnV251F2QNNAFv1bL-3nEXiydD2pbWHek6cNTQvt4Fo7rFMpD9eklr-axI08IPyCXUPGpnxUDSVxA_V2WAgCe-H6B4_iuqrmx8p9rrgboAv40j_Ysz3HhS8g/s1600/Cigar-Galaxy.jpg" imageanchor="1"><img alt="Cigar Galaxy" border="0" height="498" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhcschPpHDqzmEZREnbyNyfBnV251F2QNNAFv1bL-3nEXiydD2pbWHek6cNTQvt4Fo7rFMpD9eklr-axI08IPyCXUPGpnxUDSVxA_V2WAgCe-H6B4_iuqrmx8p9rrgboAv40j_Ysz3HhS8g/s1600/Cigar-Galaxy.jpg" title="" width="640" /></a></div><div style="text-align: center;"><br /></div><div style="text-align: center;">This mosaic image is the sharpest wide-angle view ever obtained of M82. The galaxy is remarkable for its bright blue disk, webs of shredded clouds, and fiery-looking plumes of glowing hydrogen blasting out of its central regions.</div><div style="text-align: center;"><br /></div><div style="text-align: center;">Throughout the galaxy's center, young stars are being born 10 times faster than they are inside our entire Milky Way Galaxy. The resulting huge concentration of young stars carved into the gas and dust at the galaxy's center. The fierce galactic superwind generated from these stars compresses enough gas to make millions of more stars.</div><div style="text-align: center;"><br /></div><div style="text-align: center;">In M82, young stars are crammed into tiny but massive star clusters. These, in turn, congregate by the dozens to make the bright patches, or "starburst clumps," in the central parts of M82. The clusters in the clumps can only be distinguished in the sharp Hubble images. Most of the pale, white objects sprinkled around the body of M82 that look like fuzzy stars are actually individual star clusters about 20 light-years across and contain up to a million stars.</div><div style="text-align: center;"><br /></div><div style="text-align: center;">The rapid rate of star formation in this galaxy eventually will be self-limiting. When star formation becomes too vigorous, it will consume or destroy the material needed to make more stars. The starburst then will subside, probably in a few tens of millions of years.</div><div style="text-align: center;"><br /></div><div style="text-align: center;">Located 12 million light-years away, M82 appears high in the northern spring sky in the direction of the constellation Ursa Major, the Great Bear. It is also called the "Cigar Galaxy" because of the elliptical shape produced by the oblique tilt of its starry disk relative to our line of sight.</div><div style="text-align: center;"><br /></div><div style="text-align: center;">The observation was made in March 2006, with the Advanced Camera for Surveys' Wide Field Channel. Astronomers assembled this six-image composite mosaic by combining exposures taken with four colored filters that capture starlight from visible and infrared wavelengths as well as the light from the glowing hydrogen filaments.</div><br />Image Credit: NASA, ESA, and The Hubble Heritage Team (STScI/AURA)<br />Explanation from: http://hubblesite.org/newscenter/archive/releases/2006/14/image/a/

Starburst Galaxy M82

This mosaic image is the sharpest wide-angle view ever obtained of M82. The galaxy is remarkable for its bright blue disk, webs of shredded ...

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A Sun Pillar over Sweden

<div style="text-align: center;"><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiJq7fC_y7AhPdOda5MsExgiZCYzBd0zugtOBQ6vtZVyKH58n3mbg2U-RLV3cawl2SSiHaDc4Ow5fNHpW-b9ks9OkJPBpzOMw06SUrmK-12rItW7Ta_IQQ5YTuyqYY1Q3ySUL5wcEMnm0JO/s1600/sunpillar_strand_2000.jpg"><img border="0" height="426" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiJq7fC_y7AhPdOda5MsExgiZCYzBd0zugtOBQ6vtZVyKH58n3mbg2U-RLV3cawl2SSiHaDc4Ow5fNHpW-b9ks9OkJPBpzOMw06SUrmK-12rItW7Ta_IQQ5YTuyqYY1Q3ySUL5wcEMnm0JO/s640/sunpillar_strand_2000.jpg" width="640" /></a></div><div style="text-align: center;"><br /></div><div style="text-align: center;">Have you ever seen a sun pillar? When the air is cold and the Sun is rising or setting, falling ice crystals can reflect sunlight and create an unusual column of light. Ice sometimes forms flat, six-sided shaped crystals as it falls from high-level clouds. Air resistance causes these crystals to lie nearly flat much of the time as they flutter to the ground. Sunlight reflects off crystals that are properly aligned, creating the sun-pillar effect. In this picture taken in December 2012, a sun-pillar reflects light from a Sun setting over Östersund, Sweden.</div><br />Image Credit & Copyright: Göran Strand<div>Explanation from: http://apod.nasa.gov/apod/ap121218.html</div>

A Sun Pillar over Sweden

Have you ever seen a sun pillar? When the air is cold and the Sun is rising or setting, falling ice crystals can reflect sunlight and create...

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Out of This Whirl: the Whirlpool Galaxy (M51) and Companion Galaxy

<div style="text-align: center;"><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiHP96BTOk69e7emKQh6OwTo3KbclTWT6R7om1Kge1Asx6qDqkjaH_4CzVVE6Vfwmms8KdMNLKwUSvGBsAqS69yJynGi4q4augXP-FXPqUdBbvhZb_2J0hJGzwH1efVjPMrDb44KQSDxINp/s1600/hs-2005-12-a-large_web.jpg"><img border="0" height="400" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiHP96BTOk69e7emKQh6OwTo3KbclTWT6R7om1Kge1Asx6qDqkjaH_4CzVVE6Vfwmms8KdMNLKwUSvGBsAqS69yJynGi4q4augXP-FXPqUdBbvhZb_2J0hJGzwH1efVjPMrDb44KQSDxINp/s640/hs-2005-12-a-large_web.jpg" width="640" /></a></div><div style="text-align: center;"><br /></div><div style="text-align: center;">The graceful, winding arms of the majestic spiral galaxy M51 (NGC 5194) appear like a grand spiral staircase sweeping through space. They are actually long lanes of stars and gas laced with dust.</div><div style="text-align: center;"><br /></div><div style="text-align: center;">This sharpest-ever image of the Whirlpool Galaxy, taken in January 2005 with the Advanced Camera for Surveys aboard NASA's Hubble Space Telescope, illustrates a spiral galaxy's grand design, from its curving spiral arms, where young stars reside, to its yellowish central core, a home of older stars. The galaxy is nicknamed the Whirlpool because of its swirling structure.</div><div style="text-align: center;"><br /></div><div style="text-align: center;">The Whirlpool's most striking feature is its two curving arms, a hallmark of so-called grand-design spiral galaxies. Many spiral galaxies possess numerous, loosely shaped arms which make their spiral structure less pronounced. These arms serve an important purpose in spiral galaxies. They are star-formation factories, compressing hydrogen gas and creating clusters of new stars. In the Whirlpool, the assembly line begins with the dark clouds of gas on the inner edge, then moves to bright pink star-forming regions, and ends with the brilliant blue star clusters along the outer edge.</div><div style="text-align: center;"><br /></div><div style="text-align: center;">Some astronomers believe that the Whirlpool's arms are so prominent because of the effects of a close encounter with NGC 5195, the small, yellowish galaxy at the outermost tip of one of the Whirlpool's arms. At first glance, the compact galaxy appears to be tugging on the arm. Hubble's clear view, however, shows that NGC 5195 is passing behind the Whirlpool. The small galaxy has been gliding past the Whirlpool for hundreds of millions of years.</div><div style="text-align: center;"><br /></div><div style="text-align: center;">As NGC 5195 drifts by, its gravitational muscle pumps up waves within the Whirlpool's pancake-shaped disk. The waves are like ripples in a pond generated when a rock is thrown in the water. When the waves pass through orbiting gas clouds within the disk, they squeeze the gaseous material along each arm's inner edge. The dark dusty material looks like gathering storm clouds. These dense clouds collapse, creating a wake of star birth, as seen in the bright pink star-forming regions. The largest stars eventually sweep away the dusty cocoons with a torrent of radiation, hurricane-like stellar winds, and shock waves from supernova blasts. Bright blue star clusters emerge from the mayhem, illuminating the Whirlpool's arms like city streetlights.</div><div style="text-align: center;"><br /></div><div style="text-align: center;">The Whirlpool is one of astronomy's galactic darlings. Located 31 million light-years away in the constellation Canes Venatici (the Hunting Dogs), the Whirlpool's beautiful face-on view and closeness to Earth allow astronomers to study a classic spiral galaxy's structure and star-forming processes.</div><br />Image Credit: NASA, ESA, S. Beckwith (STScI), and The Hubble Heritage Team (STScI/AURA)<div>Explanation from: http://hubblesite.org/newscenter/archive/releases/2005/12/image/a/</div>

Out of This Whirl: the Whirlpool Galaxy (M51) and Companion Galaxy

The graceful, winding arms of the majestic spiral galaxy M51 (NGC 5194) appear like a grand spiral staircase sweeping through space. They ar...

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Stars in NGC 602a

<div style="text-align: center;"><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjgADa2cks3Az0S_pwRgX2vB5yMccFfw1e7mRhOvyRRG03-pfUlNBInbtYS_xTUXxk25vP6xVzQ67s4aHurjB3m4-3PjqIc4tswFMaZAd9GJJzOVPvVdO45JOO_v63y6dFNE_x6yyqlIRRL/s1600/ngc602.jpg"><img border="0" height="640" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjgADa2cks3Az0S_pwRgX2vB5yMccFfw1e7mRhOvyRRG03-pfUlNBInbtYS_xTUXxk25vP6xVzQ67s4aHurjB3m4-3PjqIc4tswFMaZAd9GJJzOVPvVdO45JOO_v63y6dFNE_x6yyqlIRRL/s640/ngc602.jpg" width="640" /></a></div><div style="text-align: center;"><br /></div><div style="text-align: center;">The Small Magellanic Cloud (SMC) is one of the Milky Way's closest galactic neighbors. Even though it is a small, or so-called dwarf galaxy, the SMC is so bright that it is visible to the unaided eye from the Southern Hemisphere and near the equator. Many navigators, including Ferdinand Magellan who lends his name to the SMC, used it to help find their way across the oceans. </div><div style="text-align: center;"><br /></div><div style="text-align: center;">Modern astronomers are also interested in studying the SMC (and its cousin, the Large Magellanic Cloud), but for very different reasons. Because the SMC is so close and bright, it offers an opportunity to study phenomena that are difficult to examine in more distant galaxies. </div><div style="text-align: center;"><br /></div><div style="text-align: center;">New Chandra data of the SMC have provided one such discovery: the first detection of X-ray emission from young stars with masses similar to our Sun outside our Milky Way galaxy. The new Chandra observations of these low-mass stars were made of the region known as the "Wing" of the SMC. In this composite image of the Wing the Chandra data is shown in purple, optical data from the Hubble Space Telescope is shown in red, green and blue and infrared data from the Spitzer Space Telescope is shown in red. </div><div style="text-align: center;"><br /></div><div style="text-align: center;">Astronomers call all elements heavier than hydrogen and helium -- that is, with more than two protons in the atom's nucleus -- "metals." The Wing is a region known to have fewer metals compared to most areas within the Milky Way. There are also relatively lower amounts of gas, dust, and stars in the Wing compared to the Milky Way. </div><div style="text-align: center;"><br /></div><div style="text-align: center;">Taken together, these properties make the Wing an excellent location to study the life cycle of stars and the gas lying in between them. Not only are these conditions typical for dwarf irregular galaxies like the SMC, they also mimic ones that would have existed in the early Universe. </div><div style="text-align: center;"><br /></div><div style="text-align: center;"><br /></div><div style="text-align: center;">Most star formation near the tip of the Wing is occurring in a small region known as NGC 602, which contains a collection of at least three star clusters. One of them, NGC 602a, is similar in age, mass, and size to the famous Orion Nebula Cluster. Researchers have studied NGC 602a to see if young stars -- that is, those only a few million years old -- have different properties when they have low levels of metals, like the ones found in NGC 602a. </div><div style="text-align: center;"><br /></div><div style="text-align: center;">Using Chandra, astronomers discovered extended X-ray emission, from the two most densely populated regions in NGC 602a. The extended X-ray cloud likely comes from the population of young, low-mass stars in the cluster, which have previously been picked out by infrared and optical surveys, using Spitzer and Hubble respectively. This emission is not likely to be hot gas blown away by massive stars, because the low metal content of stars in NGC 602a implies that these stars should have weak winds. The failure to detect X-ray emission from the most massive star in NGC 602a supports this conclusion, because X-ray emission is an indicator of the strength of winds from massive stars. No individual low-mass stars are detected, but the overlapping emission from several thousand stars is bright enough to be observed. </div><div style="text-align: center;"><br /></div><div style="text-align: center;">The Chandra results imply that the young, metal-poor stars in NGC 602a produce X-rays in a manner similar to stars with much higher metal content found in the Orion cluster in our galaxy. The authors speculate that if the X-ray properties of young stars are similar in different environments, then other related properties -- including the formation and evolution of disks where planets form -- are also likely to be similar. </div><div style="text-align: center;"><br /></div><div style="text-align: center;">X-ray emission traces the magnetic activity of young stars and is related to how efficiently their magnetic dynamo operates. Magnetic dynamos generate magnetic fields in stars through a process involving the star's speed of rotation, and convection, the rising and falling of hot gas in the star's interior. </div><div style="text-align: center;"><br /></div><div style="text-align: center;">The combined X-ray, optical and infrared data also revealed, for the first time outside our Galaxy, objects representative of an even younger stage of evolution of a star. These so-called "young stellar objects" have ages of a few thousand years and are still embedded in the pillar of dust and gas from which stars form, as in the famous "Pillars of Creation" of the Eagle Nebula. </div><div style="text-align: center;"><br /></div>Image Credit: X-ray: NASA/CXC/Univ.Potsdam/L.Oskinova et al; Optical: NASA/STScI; Infrared: NASA/JPL-Caltech<br /><div>Explanation from: http://www.nasa.gov/mission_pages/chandra/multimedia/ngc602a.html</div>

Stars in NGC 602a

The Small Magellanic Cloud (SMC) is one of the Milky Way's closest galactic neighbors. Even though it is a small, or so-called dwarf gal...

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Alaskan Mountains Seen During IceBridge Transit

<div style="text-align: center;"><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiFhcrZFWZP0mQ8WSaTP9bP8HcczP6KBz-YgIEKy14h67VSasuySpPeNRDSsBpxdAB-ZfVL5WnN_qLo91ck7ao63BlFGemUrP76-fa1hMWlv0D0eyTCC5DRbjSTwNVA35SVF3JtJ81rhHWu/s1600/738648main_alaska_mountains_full_full.jpg"><img alt="Alaskan mountains seen from high altitude aboard the NASA P-3B during the IceBridge transit flight from Thule to Fairbanks on March 21, 2013. NASA's Operation IceBridge is an airborne science mission to study Earth's polar ice. Image Credit: NASA/Goddard/Christy Hansen" border="0" height="480" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiFhcrZFWZP0mQ8WSaTP9bP8HcczP6KBz-YgIEKy14h67VSasuySpPeNRDSsBpxdAB-ZfVL5WnN_qLo91ck7ao63BlFGemUrP76-fa1hMWlv0D0eyTCC5DRbjSTwNVA35SVF3JtJ81rhHWu/s640/738648main_alaska_mountains_full_full.jpg" title="" width="640" /></a></div><div style="text-align: center;"><br /></div><div style="text-align: center;">Alaskan mountains seen from high altitude aboard the NASA P-3B during the IceBridge transit flight from Thule to Fairbanks on March 21, 2013.</div><div style="text-align: center;"><br /></div><div style="text-align: center;">NASA's Operation IceBridge is an airborne science mission to study Earth's polar ice.</div><div><br />Image Credit: NASA/Goddard/Christy Hansen</div>

Alaskan Mountains Seen During IceBridge Transit

Alaskan mountains seen from high altitude aboard the NASA P-3B during the IceBridge transit flight from Thule to Fairbanks on March 21, 2013...

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Herschel Sees Through Ghostly Pillars

<div style="text-align: center;"><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgTaBo5xOl5PHWLFXekGoCkPfXQcZKGWKfL_xK4HtiiGFTNet_wu5PLNMqeI0Vrzj2jgSixxgdVb0VcH0tf8HcTeyJ-WLbLBDuQFmgH8845pT8GmR5t35kxqbA49JW7POtZ_cQg1R_dm0s1/s1600/616632main_pia15260-full_full.jpg"><img alt="This Herschel image of the Eagle nebula shows the self-emission of the intensely cold nebula’s gas and dust as never seen before. Each color shows a different temperature of dust, from around 10 degrees above absolute zero (10 Kelvin or minus 442 degrees Fahrenheit) for the red, up to around 40 Kelvin, or minus 388 degrees Fahrenheit, for the blue. Herschel reveals the nebula's intricate tendril nature, with vast cavities forming an almost cave-like surrounding to the famous pillars, which appear almost ghostly in this view. The gas and dust provide the material for the star formation that is still under way inside this enigmatic nebula. Far-infrared light has been color-coded to 70 microns for blue and 160 microns for green using the Photodetector Array Camera, and 250 microns for red using the Spectral and Photometric Imaging Receiver. Herschel is a European Space Agency cornerstone mission, with science instruments provided by consortia of European institutes and with important participation by NASA. NASA's Herschel Project Office is based at NASA's Jet Propulsion Laboratory, Pasadena, Calif. JPL contributed mission-enabling technology for two of Herschel's three science instruments. The NASA Herschel Science Center, part of the Infrared Processing and Analysis Center at the California Institute of Technology in Pasadena, supports the United States astronomical community. Caltech manages JPL for NASA. Image Credit: ESA/Herschel/PACS/SPIRE/Hill, Motte, HOBYS Key Programme Consortium Explanation from: http://www.nasa.gov/mission_pages/herschel/multimedia/pia15260.html" border="0" height="640" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgTaBo5xOl5PHWLFXekGoCkPfXQcZKGWKfL_xK4HtiiGFTNet_wu5PLNMqeI0Vrzj2jgSixxgdVb0VcH0tf8HcTeyJ-WLbLBDuQFmgH8845pT8GmR5t35kxqbA49JW7POtZ_cQg1R_dm0s1/s640/616632main_pia15260-full_full.jpg" title="" width="640" /></a></div><div style="text-align: center;"><br /></div><div style="text-align: center;">This Herschel image of the Eagle nebula shows the self-emission of the intensely cold nebula’s gas and dust as never seen before. Each color shows a different temperature of dust, from around 10 degrees above absolute zero (10 Kelvin or minus 442 degrees Fahrenheit) for the red, up to around 40 Kelvin, or minus 388 degrees Fahrenheit, for the blue. </div><div style="text-align: center;"><br /></div><div style="text-align: center;">Herschel reveals the nebula's intricate tendril nature, with vast cavities forming an almost cave-like surrounding to the famous pillars, which appear almost ghostly in this view. The gas and dust provide the material for the star formation that is still under way inside this enigmatic nebula. </div><div style="text-align: center;"><br /></div><div style="text-align: center;">Far-infrared light has been color-coded to 70 microns for blue and 160 microns for green using the Photodetector Array Camera, and 250 microns for red using the Spectral and Photometric Imaging Receiver. </div><div style="text-align: center;"><br /></div><div style="text-align: center;">Herschel is a European Space Agency cornerstone mission, with science instruments provided by consortia of European institutes and with important participation by NASA. NASA's Herschel Project Office is based at NASA's Jet Propulsion Laboratory, Pasadena, Calif. JPL contributed mission-enabling technology for two of Herschel's three science instruments. The NASA Herschel Science Center, part of the Infrared Processing and Analysis Center at the California Institute of Technology in Pasadena, supports the United States astronomical community. Caltech manages JPL for NASA. </div><div style="text-align: center;"><br /></div>Image Credit: ESA/Herschel/PACS/SPIRE/Hill, Motte, HOBYS Key Programme Consortium<br /><div>Explanation from: http://www.nasa.gov/mission_pages/herschel/multimedia/pia15260.html</div>

Herschel Sees Through Ghostly Pillars

This Herschel image of the Eagle nebula shows the self-emission of the intensely cold nebula’s gas and dust as never seen before. Each color...

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