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Fires in Southeast Australia
A crippling heat wave and st
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2/6/09
| Description |
A crippling heat wave and strong winds in southeastern Australia contributed to an outbreak of forest and grassland fires in Victoria in late January 2009. By January 30, about 5,500 hectares had burned and at least 10 homes had been destroyed, reported the Australian Broadcasting Corporation (ABC). The homes were located in a small community near the town of Boolara. Nearly surrounded by wildfire, the town had also run out of water and lost power, said ABC News. This image from the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA's Aqua satellite was captured on January 30. A large plume of smoke spreads southward from a fire (outlined in red) that appears to be burning in a small area of forest west of Churchill (a larger town near Boolara) in Victoria's Gippsland region. The forest is dark green in contrast to the surrounding grass or cropland. The fire, says ABC News, started as two blazes in plantation forests in the Strzelecki Ranges. The large version of the scene shows a wider area that includes several other fires. Image credit: Jeff Schmaltz, MODIS Rapid Response Team, NASA's Goddard Space Flight Center Text credit: Rebecca Lindsey, NASA's Earth Observatory |
| Date |
2/6/09 |
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Bushfires in Southeast Austr
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Bushfires in southeastern Au
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2/9/09
| Description |
Bushfires in southeastern Australia turned deadly over the first weekend of February 2009. Out-of-control fires raced into small communities and towns in Victoria, and more than 100 people had died as of February 9, according to news reports. The Australian Broadcasting Corporation (ABC News) reported that many of those who died had remained to protect their homes. Among the most devastated communities were those in the Kinglake area and Marysville. As of February 9, firefighters were expressing concern about the increased activity of the fire around the town of Dederang, southwest of Lake Hume. This image shows the Barry Mountains of central Victoria on February 9, 2009. The image, captured by the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA's Aqua satellite,is shown in false color, using visible, near-infrared and shortwave infrared light. Places where the sensor detected active fire are outlined in red. Burned areas are brick red, and places of intense heat -- often a sign of open flame in this kind of image -- are glowing pink. Smoke turns a transparent blue, which makes it easier to see the ground. Fire is a regular occurrence in the forests and grasslands of southeastern Australia, even in the absence of people. In the hot, dry summer months, vegetation dries out, lightning triggers many natural wildfires. However, in the past decade, the area has experienced several severe droughts, and in late January and early February, parts of South Australia, Victoria, and New South Wales were also paralyzed by an exceptional heatwave. Conditions were primed for devastating fires, some of which appear to have been started by lighting and others, according to news reports, by arson. The event was the worst fire disaster in Australia's history. > Labeled image > Photo-like image Image credit: NASA's Goddard Space Flight Center, MODIS Rapid Response Team Text credit: Rebecca Lindsey, NASA's Earth Observatory |
| Date |
2/9/09 |
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Bushfires in Southeast Austr
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Bushfires in Victoria, Austr
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2/23/09
| Description |
Bushfires in Victoria, Australia, flared up significantly in the last week of February 2009. The state has been battling deadly fires since late January 2009 with only brief periods of calm. According to news reports from the Australian Broadcasting Corporation on February 23, new emergency evacuation warnings over the weekend had forced hundreds of residents from communities across the state into shelters. This image from the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA's Aqua satellite shows the fires on February 23. This image includes visible, shortwave-, and near-infrared light to thin the smoke and highlight the burned areas (brick red). In this type of image, areas of glowing pink often indicate open flame. Among the areas where bushfires were threatening communities were Daylesford, Warburton and Belgrave. The high-resolution images provided above are at MODIS' maximum spatial resolution (level of detail) of 250 meters per pixel. The MODIS Rapid Response Team provides twice-daily images of Victoria in additional resolutions. Image credit: NASA's MODIS Rapid Response Team Text credit: Rebecca Lindsey, NASA's Earth Observatory |
| Date |
2/23/09 |
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Cathedral Fire, Wilson's Pro
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Wilson's Promontory National
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3/18/09
| Description |
Wilson's Promontory National Park, located at the southern tip of Victoria, Australia, was one of many areas scorched by large bushfires in February 2009. The Cathedral Fire, which was sparked by lightning on February 8, burned an estimated 25,200 hectares (62,271 acres) in the park before it was fully contained on March 14, the day this image was captured by the Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) on NASA's Terra satellite. The image combines visible light with near-infrared light, the resulting false-color image makes burned areas more obvious (charcoal-brown). Unburned vegetation is red, and areas where vegetation is naturally sparse or dormant are beige. Beaches and sandy spots are nearly as white as the clouds. North of the park boundary (upper left), the landscape is beige and light red, a rural-agricultural area where people have cleared the natural vegetation. The park has a wide variety of habitats, including beaches, tidal mud flats, grass-covered dunes, marshes and swamps, and upland forests. The burn scar is darker in some places in others, which could be because the amount of burning there was more severe, but it could also be due to differences in the type of vegetation that burned and the characteristics of the soil. For example, the burn scar appears very dark in a swampy area inland of Five Mile Beach. The park was closed for several weeks while managers assessed the damage and made sure it would be safe for visitors to return. Some areas will be reopened to the public beginning March 21. Image credit: NASA/Jesse Allen, based on data from NASA/GSFC/METI/ERSDAC/JAROS and the U.S./Japan ASTER Science Team Text credit: Rebecca Lindsey, NASA's Earth Observatory |
| Date |
3/18/09 |
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Fires in East Gippsland, Vic
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Several bushfires were burni
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4/2/09
| Description |
Several bushfires were burning in state and national parks in the eastern corner of Victoria on March 31, 2009, spreading smoke across a large area of southern Victoria, including Melbourne (visible in large image). This image of the fires (outlined in red) was captured by the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA's Aqua satellite. Clouds were building across the area at the time of this image, and they delivered some rain later that day and evening, according to the April 1 fire status report from the Victoria Department of Sustainability and the Environment. Image credit: NASA's MODIS Rapid Response Team Text credit: Rebecca Lindsey, NASA's Goddard Space Flight Center |
| Date |
4/2/09 |
|
NASA's Mars Team Teaches Old
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Animated route of Spirit's e
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1/2/07
3 Years on Mars: Opportunity
Overview of Mars Exploration
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1/24/07
Opportunity Rover Weathers t
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Mars Exploration Rover, Oppo
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7/23/07
As Martian Skies Brighten, R
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NASA's Mars Exploration Rove
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Cape Verde, Mars
This Mars Exploration Rover
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4/1/08
| Description |
This Mars Exploration Rover Opportunity Pancam "super resolution" mosaic of the approximately 6 meter (20 foot) high cliff face of the Cape Verde promontory was taken by the rover from inside Victoria Crater, during the rover's descent into Duck Bay. Super-resolution is an imaging technique that utilizes information from multiple pictures of the same target in order to generate an image with a higher resolution than any of the individual images. Cape Verde is a geologically rich outcrop and is teaching scientists about how rocks at Victoria crater were modified since they were deposited long ago. This image complements super resolution mosaics obtained at Cape St. Mary and Cape St. Vincent and is consistent with the hypothesis that Victoria crater is located in the middle of what used to be an ancient sand dune field. This image was acquired on sols 1342 and 1356 (Nov. 2 and 17, 2007). Image Credit: NASA/JPL-Caltech/Cornell University |
| Date |
4/1/08 |
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L, C, and X-band Victoria, B
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This three-frequency spacebo
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3/14/96
| Date |
3/14/96 |
| Description |
This three-frequency spaceborne radar image shows the southern end of Vancouver Island on the west coast of Canada. The white area in the lower right is the city of Victoria, the capital of the province of British Columbia. The three radar frequencies help to distinguish different land use patterns. The bright pink areas are suburban regions, the brownish areas are forested regions, and blue areas are agricultural fields or forest clear- cuts. Founded in 1843 as a fur trading post, Victoria has grown to become one of western Canada's largest commercial centers. In the upper right is San Juan Island, in the state of Washington. The Canada/U.S. border runs through Haro Strait, on the right side of the image, between San Juan Island and Vancouver Island. The image was acquired by the Spaceborne Imaging Radar-C/X-band Synthetic Aperture Radar (SIR-C/X-SAR) on October 6, 1994, onboard the space shuttle Endeavour. The area shown is 37 kilometers by 42 kilometers (23 miles by 26 miles) and is centered at 48.5 degrees north latitude, 123.3 degrees west longitude. North is toward the upper left. The colors are assigned to different radar frequencies and polarizations as follows: red is L-band horizontally transmitted and received, green is C-band, vertically transmitted and received, and blue is X-band, vertically transmitted and received. SIR-C/X-SAR, a joint mission of the German, Italian and United States space agencies, is part of NASA's Mission to Planet Earth program. ##### |
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Hong Kong, China X band
This is an X-SAR image spann
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10/9/94
| Date |
10/9/94 |
| Description |
This is an X-SAR image spanning an area of approximately 20 kilometers by 40 kilometers (12 miles by 25 miles) of the island of Hong Kong, the Kowloon Peninsula and the new territories in southern China, taken by the imaging radar on board the space shuttle Endeavour on October 4, 1994. North is toward the top left corner of the image. The Kaitak Airport runway on Kowloon Peninsula (center right of image) was built on reclaimed land and extends almost 3 kilometers (nearly 2 miles) into Victoria Harbor. To the south of the harbor lies the island of Hong Kong. The bright areas around the harbor are the major residential and business districts. Housing more than six million residents, Hong Kong is the most densely populated area in the world. The large number of objects visible in the harbor and surrounding waters are a variety of sea-going vessels, anchored in one of the busiest seaports in the Far East. ----- Spaceborne Imaging Radar-C and X-band Synthetic Aperture Radar (SIR-C/X-SAR) is part of NASA's Mission to Planet Earth. The radars illuminate Earth with microwaves, allowing detailed observations at any time, regardless of weather or sunlight conditions. SIR-C/X-SAR uses three microwave wavelengths: L-band (24 cm), C-band (6 cm) and X-band (3 cm). The multi-frequency data will be used by the international scientific community to better understand the global environment and how it is changing. The SIR-C/X-SAR data, complemented by aircraft and ground studies, will give scientists clearer insights into those environmental changes which are caused by nature and those changes which are induced by human activity. SIR-C was developed by NASA's Jet Propulsion Laboratory. X-SAR was developed by the Dornier and Alenia Spazio companies for the German space agency, Deutsche Agentur fuer Raumfahrtangelegenheiten (DARA), and the Italian space agency, Agenzia Spaziale Italiana (ASI), with the Deutsche Forschungsanstalt fuer Luft und Raumfahrt e.V.(DLR), the major partner in science, operations and data processing of X-SAR. ##### |
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Exploring the Wetlands of Ti
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| Description |
Exploring the Wetlands of Titan |
| Full Description |
Cassini peers through the murky orange haze of Titan to spy what are believed to be bodies of liquid hydrocarbons, two of them as large as seas on Earth, near the moon's north pole. This movie blends a near natural-color view and an infrared glimpse of Titan's surface obtained by the visual cameras, followed by a transition to imagery collected by the radar instrument aboard Cassini, for a dramatic reveal of the north pole of Saturn's largest moon. As the movie zooms in on the north pole, the most readily visible bodies are outlined in blue. The largest of these, on the left, is as big as the Caspian Sea on Earth, the next largest, on the right, is about the size of Lake Superior. When compared to the surface area of Titan however (which is six times smaller than Earth's), these bodies are equivalent in size to the Bay of Bengal and Timor Sea, respectively. Geographically speaking, they are more like seas. The movie continues with a gradual transition to a polar map of the radar imagery taken so far by Cassini of the north polar region. It is clear that one of the radar swaths has intersected a small upper bay of the largest sea, and has almost entirely imaged the second one. The extreme darkness of these regions in the radar data argues strongly for the presence of liquid hydrocarbons, such as methane and ethane, which remain liquid at Titan's frigid temperature of minus 180 degrees Celsius (minus 288 degrees Fahrenheit). See Titan (T25) Viewed by Cassini's Radar - Feb. 22, 2007. The movie continues with a pan across the pole and the radar imagery that has uncovered a multitude of much smaller lakes. Features of strikingly similar morphology to these dark northern seas and smaller lakes were first discovered in Cassini Imaging Science Subsystem images in June 2005, at Titan's south pole (see Land of Lakes?). The lake-like shoreline of the largest of these, called Ontario Lacus, its size (about the size of Lake Victoria), and its proximity to the south pole where the largest field of clouds yet seen on Titan had been observed, earned it the reputation as the best candidate for a body of liquid hydrocarbons on Titan up until that point, though the case for liquids was weak. When adjusted for the size of Titan, Ontario Lacus is equivalent in size to the Black Sea. Now, by inference, scientists are more confident that it, and the smaller features that dot the south pole, are also likely open bodies of liquid, and in aggregate make up a southern wetlands on Titan, similar to the one observed in the north polar movie. The images used to make this movie were taken with the Cassini spacecraft narrow-angle camera on Feb. 25, 2007, at a distance of approximately 1.3 million kilometers (800,000 miles) from Titan. The infrared images were taken with a special filter centered at 938 nanometers that provides the cameras' best view of Titan's surface features. This view was then composited with images taken at 619, 568 and 440 nanometers to, create a near natural color appearance. The radar data were acquired in synthetic aperture radar mode. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging operations center is based at the Space Science Institute in Boulder, Colo. For more information about the Cassini-Huygens mission visit http://saturn.jpl.nasa.gov . The Cassini imaging team homepage is at http://ciclops.org . Credit: NASA/JPL/Space Science Institute |
| Date |
March 15, 2007 |
|
Exploring the Wetlands of Ti
…
| Description |
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn. |
| Full Description |
Cassini peers through the murky orange haze of Titan to spy what are believed to be bodies of liquid hydrocarbons, two of them as large as seas on Earth, near the moon's north pole. This movie blends a near natural-color view and an infrared glimpse of Titan's surface obtained by the visual cameras, followed by a transition to imagery collected by the radar instrument aboard Cassini, for a dramatic reveal of the north pole of Saturn's largest moon. As the movie zooms in on the north pole, the most readily visible bodies are outlined in blue. The largest of these, on the left, is as big as the Caspian Sea on Earth, the next largest, on the right, is about the size of Lake Superior. When compared to the surface area of Titan however (which is six times smaller than Earth's), these bodies are equivalent in size to the Bay of Bengal and Timor Sea, respectively. Geographically speaking, they are more like seas. The movie continues with a gradual transition to a polar map of the radar imagery taken so far by Cassini of the north polar region. It is clear that one of the radar swaths has intersected a small upper bay of the largest sea, and has almost entirely imaged the second one. The extreme darkness of these regions in the radar data argues strongly for the presence of liquid hydrocarbons, such as methane and ethane, which remain liquid at Titan's frigid temperature of minus 180 degrees Celsius (minus 288 degrees Fahrenheit). See Titan (T25) Viewed by Cassini's Radar - Feb. 22, 2007. The movie continues with a pan across the pole and the radar imagery that has uncovered a multitude of much smaller lakes. Features of strikingly similar morphology to these dark northern seas and smaller lakes were first discovered in Cassini Imaging Science Subsystem images in June 2005, at Titan's south pole (see Land of Lakes?). The lake-like shoreline of the largest of these, called Ontario Lacus, its size (about the size of Lake Victoria), and its proximity to the south pole where the largest field of clouds yet seen on Titan had been observed, earned it the reputation as the best candidate for a body of liquid hydrocarbons on Titan up until that point, though the case for liquids was weak. When adjusted for the size of Titan, Ontario Lacus is equivalent in size to the Black Sea. Now, by inference, scientists are more confident that it, and the smaller features that dot the south pole, are also likely open bodies of liquid, and in aggregate make up a southern wetlands on Titan, similar to the one observed in the north polar movie. The images used to make this movie were taken with the Cassini spacecraft narrow-angle camera on Feb. 25, 2007, at a distance of approximately 1.3 million kilometers (800,000 miles) from Titan. The infrared images were taken with a special filter centered at 938 nanometers that provides the cameras' best view of Titan's surface features. This view was then composited with images taken at 619, 568 and 440 nanometers to, create a near natural color appearance. The radar data were acquired in synthetic aperture radar mode. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging operations center is based at the Space Science Institute in Boulder, Colo. For more information about the Cassini-Huygens mission visit http://saturn.jpl.nasa.gov . The Cassini imaging team homepage is at http://ciclops.org . Credit: NASA/JPL/Space Science Institute |
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Land of Lakes?
| Description |
This view of Titan's south polar region reveals an intriguing dark feature |
| Full Description |
NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging operations center is based at the Space Science Institute in Boulder, Colo. For more information about the Cassini-Huygens mission visit http://saturn.jpl.nasa.gov . The Cassini imaging team homepage is at http://ciclops.org . Credit: NASA/JPL/Space Science Institute, This view of Titan's south pole reveals the intriguing dark feature named Ontario Lacus and a host of smaller features dotting the south polar region. The true nature of this feature, seen here at left of center, is not yet known with absolute certainty. However, the feature's darkness, the shore-like smoothness of its perimeter, and its presence in an area where frequent convective storm clouds have been observed by Cassini and Earth-based astronomers made it the best candidate for an open body of liquid on Titan when this image was taken in June 2005. This interpretation has been strengthened by the sighting of features having similar morphologies in Titan's northern polar region during the flyby of Titan in late February (see Exploring the Wetlands of Titan). The possibility that these northern features, the sizes of small seas, are either completely or partially filled with liquid hydrocarbons is significantly strengthened by Cassini radar data that overlap portions of the Imaging Science Subsystem-observed northern bodies, (see Titan (T25) Viewed by Cassini's Radar - Feb. 22, 2007). Previously, scientists had speculated that Ontario Lacus might simply be a broad depression filled by dark, solid hydrocarbons falling from the atmosphere onto Titan's surface. In this case, the smoothed outline might be the result of a process unrelated to rainfall, such as a sinkhole or a volcanic caldera. However, the strong likelihood that the northern polar features are lakes and seas has made imaging scientists more confident that Ontario Lacus, and the smaller dark features dotting the southern polar region of Titan, also hold liquid. If correct, this new revelation would mean that each pole on Titan is a large wetlands area. The feature is named for Lake Ontario because its shape and length are similar, though the Titan feature is much wider. In actual surface area, the feature is roughly the size of Lake Victoria. However, if the relative sizes of Titan and Earth are accounted for, Ontario Lacus covers roughly the same fraction of Titan as does the Black Sea on Earth. A red cross below the center in the scene marks the pole. The brightest features seen here are methane clouds. A movie sequence showing the evolution of bright clouds in the region during the same flyby is also available (see Clouds in the Distance). This view is a composite of three narrow-angle camera images, taken over several minutes during Cassini's distant June 6, 2005, flyby. The images were combined to produce a sharper view of Titan's surface. The images were taken using a combination of spectral filters sensitive to wavelengths of polarized infrared light. The images were acquired from approximately 450,000 kilometers (279,000 miles) from Titan. Resolution in the scene is approximately 3 kilometers (2 miles) per pixel. The view has been contrast enhanced to improve the overall visibility of surface features. The Cassini-Huygens mission is a cooperative project of |
| Date |
June 28, 2005 |
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Getting a Sense of Scale
| title |
Getting a Sense of Scale |
| date |
10.06.2006 |
| description |
This photo composite shows an aerial view of FedEx Field in Landover, Md., home of the Washington Redskins, superimposed on Mars' Victoria Crater to give a sense of the crater's scale. Image Credit: FedEx Field: Screenshot (c) Google Inc. and reproduced with permission. Victoria Crater: NASA/JPL/UA |
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Victoria Crater' at Meridian
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| title |
Victoria Crater' at Meridiani Planum |
| date |
10.06.2006 |
| description |
This image from the High Resolution Imaging Science Experiment on NASA's Mars Reconnaissance Orbiter shows "Victoria crater," an impact crater at Meridiani Planum, near the equator of Mars. The crater is approximately 800 meters (half a mile) in diameter. It has a distinctive scalloped shape to its rim, caused by erosion and downhill movement of crater wall material. Layered sedimentary rocks are exposed along the inner wall of the crater, and boulders that have fallen from the crater wall are visible on the crater floor. The floor of the crater is occupied by a striking field of sand dunes. Since January 2004, the Mars Exploration Rover Opportunity has been operating at Meridiani Planum. Five days before this image was taken, Opportunity arrived at the rim of Victoria crater, after a drive of more than 9 kilometers (over 5 miles). The rover can be seen in this image, at roughly the "ten o'clock" position along the rim of the crater. This view is a portion of an image taken by the High Resolution Imaging Science Experiment (HiRISE) camera onboard the Mars Reconnaissance Orbiter spacecraft on Oct. 3, 2006. The complete image is centered at minus7.8 degrees latitude, 279.5 degrees East longitude. The range to the target site was 297 kilometers (185.6 miles). At this distance the image scale is 29.7 centimeters (12 inches) per pixel (with 1 x 1 binning) so objects about 89 centimeters (35 inches) across are resolved. The image shown here has been map-projected to 25 centimeters (10 inches) per pixel and north is up. The image was taken at a local Mars time of 3:30 PM and the scene is illuminated from the west with a solar incidence angle of 59.7 degrees, thus the sun was about 30.3 degrees above the horizon. At a solar longitude of 113.6 degrees, the season on Mars is northern summer. This is an enhanced-color view generated from images acquired by the HiRISE camera using its red filter and blue-green filter. Images from the High Resolution Imaging Science Experiment and additional information about the Mars Reconnaissance Orbiter are available online at: http://www.nasa.gov/mroor http://HiRISE.lpl.arizona.edu. For information about NASA and agency programs on the Web, visit: http://www.nasa.gov. JPL, a division of the California Institute of Technology in Pasadena, manages the Mars Reconnaissance Orbiter for NASA's Science Mission Directorate, Washington. Lockheed Martin Space Systems is the prime contractor for the project and built the spacecraft. The HiRISE camera was built by Ball Aerospace & Technologies Corporation and is operated by the University of Arizona. Image Credit: NASA/JPL/UA |
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Opportunity's Second Martian
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| title |
Opportunity's Second Martian Birthday at Cape Verde |
| date |
10.20.2007 |
| description |
A promontory nicknamed "Cape Verde" can be seen jutting out from the walls of Victoria Crater in this approximate true-color picture taken by the panoramic camera on NASA's Mars Exploration Rover Opportunity. The rover took this picture on martian day, or sol, 1329 (Oct. 20, 2007), more than a month after it began descending down the crater walls - and just 9 sols shy of its second Martian birthday on sol 1338 (Oct. 29, 2007). Opportunity landed on the Red Planet on Jan. 25, 2004. That's nearly four years ago on Earth, but only two on Mars because Mars takes longer to travel around the sun than Earth. One Martian year equals 687 Earth days. The overall soft quality of the image, and the "haze" seen in the lower right portion, are the result of scattered light from dust on the front sapphire window of the rover's camera. This view was taken using three panoramic-camera filters, admitting light with wavelengths centered at 750 nanometers (near infrared), 530 nanometers (green) and 430 nanometers (violet). Image Credit: NASA/JPL-Caltech/Cornell |
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Hubble Resolves Quasars' Hos
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| Title |
Hubble Resolves Quasars' Host Galaxies |
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Hubble Uncovers Oldest "Cloc
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| Title |
Hubble Uncovers Oldest "Clocks" in Space to Read Age of Universe |
| General Information |
What is a Space Science Update? Major Hubble discoveries on NASA television ... Astronomers explain their Hubble discoveries at a press conference, called a Space Science Update (SSU), broadcast on NASA television. The SSU includes a question and answer session with members of the media. Back to top [ #top ] |
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Hubble Uncovers Oldest "Cloc
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| Title |
Hubble Uncovers Oldest "Clocks" in Space to Read Age of Universe |
| General Information |
What is a Space Science Update? Major Hubble discoveries on NASA television ... Astronomers explain their Hubble discoveries at a press conference, called a Space Science Update (SSU), broadcast on NASA television. The SSU includes a question and answer session with members of the media. Back to top [ #top ] |
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Hubble Uncovers Oldest "Cloc
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| Title |
Hubble Uncovers Oldest "Clocks" in Space to Read Age of Universe |
| General Information |
What is a Space Science Update? Major Hubble discoveries on NASA television ... Astronomers explain their Hubble discoveries at a press conference, called a Space Science Update (SSU), broadcast on NASA television. The SSU includes a question and answer session with members of the media. Back to top [ #top ] |
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Hubble Uncovers Oldest "Cloc
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| Title |
Hubble Uncovers Oldest "Clocks" in Space to Read Age of Universe |
| General Information |
What is a Space Science Update? Major Hubble discoveries on NASA television ... Astronomers explain their Hubble discoveries at a press conference, called a Space Science Update (SSU), broadcast on NASA television. The SSU includes a question and answer session with members of the media. Back to top [ #top ] |
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Hubble Uncovers Oldest "Cloc
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| Title |
Hubble Uncovers Oldest "Clocks" in Space to Read Age of Universe |
| General Information |
What is a Space Science Update? Major Hubble discoveries on NASA television ... Astronomers explain their Hubble discoveries at a press conference, called a Space Science Update (SSU), broadcast on NASA television. The SSU includes a question and answer session with members of the media. Back to top [ #top ] |
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Hubble Uncovers Oldest "Cloc
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| Title |
Hubble Uncovers Oldest "Clocks" in Space to Read Age of Universe |
| General Information |
What is a Space Science Update? Major Hubble discoveries on NASA television ... Astronomers explain their Hubble discoveries at a press conference, called a Space Science Update (SSU), broadcast on NASA television. The SSU includes a question and answer session with members of the media. Back to top [ #top ] |
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Hubble Uncovers Oldest "Cloc
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| Title |
Hubble Uncovers Oldest "Clocks" in Space to Read Age of Universe |
| General Information |
What is a Space Science Update? Major Hubble discoveries on NASA television ... Astronomers explain their Hubble discoveries at a press conference, called a Space Science Update (SSU), broadcast on NASA television. The SSU includes a question and answer session with members of the media. Back to top [ #top ] |
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Hubble Uncovers Oldest "Cloc
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| Title |
Hubble Uncovers Oldest "Clocks" in Space to Read Age of Universe |
| General Information |
What is a Space Science Update? Major Hubble discoveries on NASA television ... Astronomers explain their Hubble discoveries at a press conference, called a Space Science Update (SSU), broadcast on NASA television. The SSU includes a question and answer session with members of the media. Back to top [ #top ] |
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Deepest View of Space Yields
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| Title |
Deepest View of Space Yields Young Stars in Andromeda Halo |
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Deepest View of Space Yields
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| Title |
Deepest View of Space Yields Young Stars in Andromeda Halo |
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Deepest View of Space Yields
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| Title |
Deepest View of Space Yields Young Stars in Andromeda Halo |
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Deepest View of Space Yields
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| Title |
Deepest View of Space Yields Young Stars in Andromeda Halo |
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Deepest View of Space Yields
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| Title |
Deepest View of Space Yields Young Stars in Andromeda Halo |
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Deepest View of Space Yields
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| Title |
Deepest View of Space Yields Young Stars in Andromeda Halo |
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Deepest View of Space Yields
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| Title |
Deepest View of Space Yields Young Stars in Andromeda Halo |
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Deepest View of Space Yields
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| Title |
Deepest View of Space Yields Young Stars in Andromeda Halo |
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Deepest View of Space Yields
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| Title |
Deepest View of Space Yields Young Stars in Andromeda Halo |
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Deepest View of Space Yields
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| Title |
Deepest View of Space Yields Young Stars in Andromeda Halo |
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Deepest View of Space Yields
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| Title |
Deepest View of Space Yields Young Stars in Andromeda Halo |
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Deepest View of Space Yields
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| Title |
Deepest View of Space Yields Young Stars in Andromeda Halo |
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Deepest View of Space Yields
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| Title |
Deepest View of Space Yields Young Stars in Andromeda Halo |
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Astronomers Find Smallest Ex
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| Title |
Astronomers Find Smallest Extrasolar Planet Yet Around Normal Star |
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Hubble Observations Confirm
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| Title |
Hubble Observations Confirm that Planets Form from Disks Around Stars |
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Hubble Observations Confirm
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| Title |
Hubble Observations Confirm that Planets Form from Disks Around Stars |
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Hubble Yields Direct Proof o
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| Title |
Hubble Yields Direct Proof of Stellar Sorting in a Globular Cluster |
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Hubble Yields Direct Proof o
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| Title |
Hubble Yields Direct Proof of Stellar Sorting in a Globular Cluster |
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Hubble Yields Direct Proof o
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| Title |
Hubble Yields Direct Proof of Stellar Sorting in a Globular Cluster |
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Hubble's Advanced Camera for
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| Title |
Hubble's Advanced Camera for Surveys Resumes Exploring the Universe |
| General Information |
What is a News Nugget? News Nuggets are bulletins from the world of astronomy. After a brief hiatus, the Advanced Camera for Surveys aboard NASA?s Hubble Space Telescope is back in business, probing the far reaches of space in a quest to understand the true nature of the universe?s most dominant constituent: dark energy. This is one of the first images of the universe taken after the ACS camera resumed science operation on July 4th. The camera was offline for nearly two weeks as NASA engineers switched to a backup power supply after the camera?s primary power supply failed. Read more: * The Full Story [ http://hubblesite.org/newscenter/archive/releases/2006/36/full/ ] |
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Hubble's Advanced Camera for
…
| Title |
Hubble's Advanced Camera for Surveys Resumes Exploring the Universe |
| General Information |
What is a News Nugget? News Nuggets are bulletins from the world of astronomy. After a brief hiatus, the Advanced Camera for Surveys aboard NASA?s Hubble Space Telescope is back in business, probing the far reaches of space in a quest to understand the true nature of the universe?s most dominant constituent: dark energy. This is one of the first images of the universe taken after the ACS camera resumed science operation on July 4th. The camera was offline for nearly two weeks as NASA engineers switched to a backup power supply after the camera?s primary power supply failed. Read more: * The Full Story [ http://hubblesite.org/newscenter/archive/releases/2006/36/full/ ] |
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Hubble's Advanced Camera for
…
| Title |
Hubble's Advanced Camera for Surveys Resumes Exploring the Universe |
| General Information |
What is a News Nugget? News Nuggets are bulletins from the world of astronomy. After a brief hiatus, the Advanced Camera for Surveys aboard NASA?s Hubble Space Telescope is back in business, probing the far reaches of space in a quest to understand the true nature of the universe?s most dominant constituent: dark energy. This is one of the first images of the universe taken after the ACS camera resumed science operation on July 4th. The camera was offline for nearly two weeks as NASA engineers switched to a backup power supply after the camera?s primary power supply failed. Read more: * The Full Story [ http://hubblesite.org/newscenter/archive/releases/2006/36/full/ ] |
|
Hubble's Advanced Camera for
…
| Title |
Hubble's Advanced Camera for Surveys Resumes Exploring the Universe |
| General Information |
What is a News Nugget? News Nuggets are bulletins from the world of astronomy. After a brief hiatus, the Advanced Camera for Surveys aboard NASA?s Hubble Space Telescope is back in business, probing the far reaches of space in a quest to understand the true nature of the universe?s most dominant constituent: dark energy. This is one of the first images of the universe taken after the ACS camera resumed science operation on July 4th. The camera was offline for nearly two weeks as NASA engineers switched to a backup power supply after the camera?s primary power supply failed. Read more: * The Full Story [ http://hubblesite.org/newscenter/archive/releases/2006/36/full/ ] |
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