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Multi-angle Images of Hudson …
At left is a true-color imag …
Description At left is a true-color image from the downward-looking (nadir) camera on the Multi-angle Imaging SpectroRadiometer (MISR) instrument on NASA's Terra satellite. The false-color image at right is a composite of red band data taken by the MISR forward 45.6-degree, nadir, and aftward 45.6-degree cameras, displayed in blue, green, and red colors, respectively. Color variations in the left image highlight spectral (true-color) differences, whereas those in the right image highlight differences in angular reflectance properties. The purple areas in the right image are low cloud, and light blue at the edge of the bay is due to increased forward scattering by the fast (smooth) ice. The orange areas are rougher ice, which scatters more light in the backward direction. This example illustrates how multi-angle viewing can distinguish physical structures and textures. Data for all channels are presented in a Space Oblique Mercator map projection to facilitate their co- registration. The images are about 400 km (250 miles) wide with a spatial resolution of about 275 meters (300 yards). North is toward the top. MISR was built and is managed by NASA's Jet Propulsion Laboratory, Pasadena, CA, for NASA's Office of Earth Science, Washington, DC. The Terra satellite is managed by NASA's Goddard Space Flight Center, Greenbelt, MD. JPL is a division of the California Institute of Technology. #####
Hubble Follows Rapid Changes …
Title Hubble Follows Rapid Changes in Jupiter's Aurora
Hubble Reveals Invisible Hig …
Title Hubble Reveals Invisible High-Speed Collision around Supernova 1987A
General Information What is an American Astronomical Society Meeting release? A major news announcement issued at an American Astronomical Society meeting, the premier astronomy conference. The highest velocity material expelled in a cataclysmic, stellar explosion 10 years ago has been detected for the first time by the Hubble telescope's imaging spectrograph. The top image, taken with Hubble's visible-light camera, shows the orange-red rings surrounding Supernova 1987A in the Large Magellanic Cloud. The glowing debris of the supernova explosion, which occurred in February 1987, is at the center of the inner ring. The small, white square indicates the location of the imaging spectrograph aperture. The Hubble data in the middle panel [and a schematic representation in the bottom panel] shows the presence of glowing hydrogen expanding at a speed of 33 million mph (15,000 kilometers per second) coming from an extended area inside the inner ring.
NASA Space Observatories Gli …
Title NASA Space Observatories Glimpse Faint Afterglow of Nearby Stellar Explosion
General Information What is Hubble Heritage? A monthly showcase of new and archival Hubble images. Go to the Heritage site. Back to top [ #top ]
Cassiopeia A - The Colorful …
Title Cassiopeia A - The Colorful Aftermath of a Violent Stellar Death
General Information What is Hubble Heritage? A monthly showcase of new and archival Hubble images. Go to the Heritage site. A new image taken with NASA's Hubble Space Telescope provides a detailed look at the tattered remains of a supernova explosion known as Cassiopeia A (Cas A). It is the youngest known remnant from a supernova explosion in the Milky Way. The new Hubble image shows the complex and intricate structure of the star's shattered fragments. The image is a composite made from 18 separate images taken in December 2004 using Hubble's Advanced Camera for Surveys (ACS).
Hubble Finds Mysterious Disk …
Title Hubble Finds Mysterious Disk of Blue Stars Around Black Hole
Western Fires: Fast Approach …
Title Western Fires: Fast Approach with State Lines
Abstract Western Fires. Fast Approach with State Lines. August 6, 2000
Completed 2000-08-07
TRACE Ultraviolet View of Ja …
Title TRACE Ultraviolet View of January 20, 2005 Solar Flare
Completed 2005-05-19
TRACE Ultraviolet View of Ja …
Title TRACE Ultraviolet View of January 20, 2005 Solar Flare
Completed 2005-05-19
TRACE Ultraviolet View of Ja …
Title TRACE Ultraviolet View of January 20, 2005 Solar Flare
Completed 2005-05-19
TRACE Ultraviolet View of Ja …
Title TRACE Ultraviolet View of January 20, 2005 Solar Flare
Completed 2005-05-19
TRACE Ultraviolet View of Ja …
Title TRACE Ultraviolet View of January 20, 2005 Solar Flare
Completed 2005-05-19
January 2005 Solar Flares fr …
Title January 2005 Solar Flares from SOHO/EIT
Completed 2005-05-19
January 2005 Solar Flares fr …
Title January 2005 Solar Flares from SOHO/EIT
Completed 2005-05-19
January 2005 Solar Flares fr …
Title January 2005 Solar Flares from SOHO/EIT
Completed 2005-05-19
MOLA: Seasonal Snow Variatio …
Title MOLA: Seasonal Snow Variations on Mars: Fast Zoom to Martian North Pole: False Color
Abstract This is a visualization of the topography near the Martian north pole as measured with the MOLA instrument. This particular animation shows a fast zoom to the surface of the pole. The surface color is based on the elevation of the topography.
Completed 2001-12-06
MOLA: Seasonal Snow Variatio …
Title MOLA: Seasonal Snow Variations on Mars: Fast Zoom to Martian North Pole: False Color
Abstract This is a visualization of the topography near the Martian north pole as measured with the MOLA instrument. This particular animation shows a fast zoom to the surface of the pole. The surface color is based on the elevation of the topography.
Completed 2001-12-06
RHESSI and TRACE View of Jan …
Title RHESSI and TRACE View of January 20, 2005 Solar Flare
Abstract RHESSI spacecraft images of gamma-rays (blue) and X-rays (red) thrown off by the hottest part of the flare are shown with UV images from the TRACE spacecraft. The gamma rays are made by energetic protons at the Sun. Scientists were surprised that the gamma rays matched the energy spectrum of protons at Earth: the proton storm may have come directly from the Sun and not from the CME as anticipated.
Completed 2005-05-19
RHESSI and TRACE View of Jan …
Title RHESSI and TRACE View of January 20, 2005 Solar Flare
Abstract RHESSI spacecraft images of gamma-rays (blue) and X-rays (red) thrown off by the hottest part of the flare are shown with UV images from the TRACE spacecraft. The gamma rays are made by energetic protons at the Sun. Scientists were surprised that the gamma rays matched the energy spectrum of protons at Earth: the proton storm may have come directly from the Sun and not from the CME as anticipated.
Completed 2005-05-19
Pine Island Iceberg Formatio …
Title Pine Island Iceberg Formation
Abstract This animation is a sequence showing the formation of the Pine Island iceberg and the glacial seaward flow upstream from the crack. It is a series of MISR images from the Terra satellite on top of the continental Radarsat view of Antarctica. The Pine Island Glacier is the largest discharger of ice in Antarctica and the continent's fastest moving glacier. Even so, when a large crack formed across the glacier in mid 2000, it was surprising how fast the crack expanded, 15 meters per day, and how soon the resulting iceberg broke off, mid-November, 2001. This iceberg, called B-21, is 42 kilometers by 17 kilometers and contains seven years of glacier outflow released to the sea in a single event.
Completed 2002-01-15
Pine Island Iceberg Formatio …
Title Pine Island Iceberg Formation
Abstract This animation is a sequence showing the formation of the Pine Island iceberg and the glacial seaward flow upstream from the crack. It is a series of MISR images from the Terra satellite on top of the continental Radarsat view of Antarctica. The Pine Island Glacier is the largest discharger of ice in Antarctica and the continent's fastest moving glacier. Even so, when a large crack formed across the glacier in mid 2000, it was surprising how fast the crack expanded, 15 meters per day, and how soon the resulting iceberg broke off, mid-November, 2001. This iceberg, called B-21, is 42 kilometers by 17 kilometers and contains seven years of glacier outflow released to the sea in a single event.
Completed 2002-01-15
Pine Island Iceberg Formatio …
Title Pine Island Iceberg Formation
Abstract This animation is a sequence showing the formation of the Pine Island iceberg and the glacial seaward flow upstream from the crack. It is a series of MISR images from the Terra satellite on top of the continental Radarsat view of Antarctica. The Pine Island Glacier is the largest discharger of ice in Antarctica and the continent's fastest moving glacier. Even so, when a large crack formed across the glacier in mid 2000, it was surprising how fast the crack expanded, 15 meters per day, and how soon the resulting iceberg broke off, mid-November, 2001. This iceberg, called B-21, is 42 kilometers by 17 kilometers and contains seven years of glacier outflow released to the sea in a single event.
Completed 2002-01-15
Pine Island Iceberg Formatio …
Title Pine Island Iceberg Formation
Abstract This animation is a sequence showing the formation of the Pine Island iceberg and the glacial seaward flow upstream from the crack. It is a series of MISR images from the Terra satellite on top of the continental Radarsat view of Antarctica. The Pine Island Glacier is the largest discharger of ice in Antarctica and the continent's fastest moving glacier. Even so, when a large crack formed across the glacier in mid 2000, it was surprising how fast the crack expanded, 15 meters per day, and how soon the resulting iceberg broke off, mid-November, 2001. This iceberg, called B-21, is 42 kilometers by 17 kilometers and contains seven years of glacier outflow released to the sea in a single event.
Completed 2002-01-15
Pine Island Iceberg Formatio …
Title Pine Island Iceberg Formation
Abstract This animation is a sequence showing the formation of the Pine Island iceberg and the glacial seaward flow upstream from the crack. It is a series of MISR images from the Terra satellite on top of the continental Radarsat view of Antarctica. The Pine Island Glacier is the largest discharger of ice in Antarctica and the continent's fastest moving glacier. Even so, when a large crack formed across the glacier in mid 2000, it was surprising how fast the crack expanded, 15 meters per day, and how soon the resulting iceberg broke off, mid-November, 2001. This iceberg, called B-21, is 42 kilometers by 17 kilometers and contains seven years of glacier outflow released to the sea in a single event.
Completed 2002-01-15
Pine Island Iceberg Formatio …
Title Pine Island Iceberg Formation
Abstract This animation is a sequence showing the formation of the Pine Island iceberg and the glacial seaward flow upstream from the crack. It is a series of MISR images from the Terra satellite on top of the continental Radarsat view of Antarctica. The Pine Island Glacier is the largest discharger of ice in Antarctica and the continent's fastest moving glacier. Even so, when a large crack formed across the glacier in mid 2000, it was surprising how fast the crack expanded, 15 meters per day, and how soon the resulting iceberg broke off, mid-November, 2001. This iceberg, called B-21, is 42 kilometers by 17 kilometers and contains seven years of glacier outflow released to the sea in a single event.
Completed 2002-01-15
Pine Island Iceberg Formatio …
Title Pine Island Iceberg Formation
Abstract This animation is a sequence showing the formation of the Pine Island iceberg and the glacial seaward flow upstream from the crack. It is a series of MISR images from the Terra satellite on top of the continental Radarsat view of Antarctica. The Pine Island Glacier is the largest discharger of ice in Antarctica and the continent's fastest moving glacier. Even so, when a large crack formed across the glacier in mid 2000, it was surprising how fast the crack expanded, 15 meters per day, and how soon the resulting iceberg broke off, mid-November, 2001. This iceberg, called B-21, is 42 kilometers by 17 kilometers and contains seven years of glacier outflow released to the sea in a single event.
Completed 2002-01-15
Pine Island Iceberg Formatio …
Title Pine Island Iceberg Formation
Abstract This animation is a sequence showing the formation of the Pine Island iceberg and the glacial seaward flow upstream from the crack. It is a series of MISR images from the Terra satellite on top of the continental Radarsat view of Antarctica. The Pine Island Glacier is the largest discharger of ice in Antarctica and the continent's fastest moving glacier. Even so, when a large crack formed across the glacier in mid 2000, it was surprising how fast the crack expanded, 15 meters per day, and how soon the resulting iceberg broke off, mid-November, 2001. This iceberg, called B-21, is 42 kilometers by 17 kilometers and contains seven years of glacier outflow released to the sea in a single event.
Completed 2002-01-15
Pine Island Iceberg Formatio …
Title Pine Island Iceberg Formation
Abstract This animation is a sequence showing the formation of the Pine Island iceberg and the glacial seaward flow upstream from the crack. It is a series of MISR images from the Terra satellite on top of the continental Radarsat view of Antarctica. The Pine Island Glacier is the largest discharger of ice in Antarctica and the continent's fastest moving glacier. Even so, when a large crack formed across the glacier in mid 2000, it was surprising how fast the crack expanded, 15 meters per day, and how soon the resulting iceberg broke off, mid-November, 2001. This iceberg, called B-21, is 42 kilometers by 17 kilometers and contains seven years of glacier outflow released to the sea in a single event.
Completed 2002-01-15
Water Vapor Measurements fro …
Title Water Vapor Measurements from HALOE (1992-1997)
Abstract An animated graph showing HALOE measurements of the water vapor amounts in the upper stratosphere, illustrating that it takes about 5 years for CFCs to reach the upper atmosphere. Tropical water vapor changes slowly with seasonal cycles. These changes, shown here as thick bands, were found to slowly ascend. These measurements tell us how fast the CFCs and other pollutants rise into the stratosphere.
Completed 1999-04-09
Galileo Earth Views (WMS)
Title Galileo Earth Views (WMS)
Abstract The Galileo spacecraft was launched from the Space Shuttle Atlantis on October 18, 1989 on a six-year trip to Jupiter. On the way, the trajectory of the spacecraft took it past Venus once and Earth twice. Galileo took the Earth images in this animation just after the first flyby of the Earth, on December 11 and 12, 1990. This six-hour sequence of images taken two minutes apart clearly shows how the Earth looks from space and how fast (or slow) the cloud features change when looked at from a distance. The path of the sun can be seen crossing Australia by its reflection in the nearby ocean, and the terminator region between night and day can be seen moving across the Indian Ocean. In the original images, the Earth's rotation is so dominant that cloud movement is hard to see, but these images have been mapped to the Earth is such a way that a viewer can watch just the clouds move in the ocean around Antarctica or across the Austrailian land mass. In this animation, New Zealand can ony be seen as a stationary disturbance under a moving cloud bank. The black area with the sharp boundary to the north and east of Australia is the side of the Earth that could not be seen from Galileo's position.
Completed 2004-08-06
TRACE Observes Flows over Ac …
Title TRACE Observes Flows over Active Regions (Fast play)
Completed 2002-04-16
TRACE Observes Flows over Ac …
Title TRACE Observes Flows over Active Regions (Fast play)
Completed 2002-04-16
TRACE Observes Flows over Ac …
Title TRACE Observes Flows over Active Regions (Fast play)
Completed 2002-04-16
TRACE Observes Flows over Ac …
Title TRACE Observes Flows over Active Regions (Fast play)
Completed 2002-04-16
Numerical Simulation of Magn …
Title Numerical Simulation of Magnetic Flux Emerging Through a Model Solar Atmosphere: Density Gradient and Velocities
Abstract This animation is one of a series depicting the results of a two-dimensional ideal magnetohydrodynamic simulation of magnetic flux emerging through a solar atmosphere. The simulation has a resolution of 300x500 cells and a length scale of 16 Mm x 6.8 Mm. The simulation depicts 1730 seconds in the evolution of the model.
Completed 1996-12-12
MODIS Mosaic of Antarctica v …
Title MODIS Mosaic of Antarctica view of Pine Island and Thwaites Glacier without ICESat Topography
Abstract NASA has released a digital image map of the Antarctic continent and surrounding islands. The Moderate Resolution Imaging Spectroradiometer (MODIS) Mosaic of Antarctica (MOA) image map is a composite of 260 swaths comprised of both Terra and Aqua MODIS images acquired between November 20, 2003 and February 29, 2004. MOA provides a cloud-free view of the ice sheet, ice shelves, and land surfaces at a grid scale of 125 m and an estimated resolution of 150 m. All land areas south of 60° S that are larger than a few hundred meters are included in the mosaic. Also included are several persistent fast ice areas and grounded icebergs.
Completed 2005-11-30
Bolivian Deforestation 1984- …
Title Bolivian Deforestation 1984-1998: Fast Dissolve without Dates
Abstract These images show deforestation near Santa Cruz, Bolivia from 1984 to 1998. In the initial 1984 scene, some clearing has already occurred in the humid forest and chaparral. The long striped clearings in the center of the scene are predominately from soybean farms created by Mennonite and Japanese farmers. The more circular patterns, appears in a grid pattern to the North (up) and West (left), are government-run and 'national' farms. The scene is roughly 150 miles tall and 200 miles wide. The city of Santa Cruz lies to the west of the river cutting through the scene.
Completed 1999-12-01
Bolivian Deforestation 1984- …
Title Bolivian Deforestation 1984-1998: Fast Dissolve without Dates
Abstract These images show deforestation near Santa Cruz, Bolivia from 1984 to 1998. In the initial 1984 scene, some clearing has already occurred in the humid forest and chaparral. The long striped clearings in the center of the scene are predominately from soybean farms created by Mennonite and Japanese farmers. The more circular patterns, appears in a grid pattern to the North (up) and West (left), are government-run and 'national' farms. The scene is roughly 150 miles tall and 200 miles wide. The city of Santa Cruz lies to the west of the river cutting through the scene.
Completed 1999-12-01
Bolivian Deforestation 1984- …
Title Bolivian Deforestation 1984-1998: Fast Dissolve without Dates
Abstract These images show deforestation near Santa Cruz, Bolivia from 1984 to 1998. In the initial 1984 scene, some clearing has already occurred in the humid forest and chaparral. The long striped clearings in the center of the scene are predominately from soybean farms created by Mennonite and Japanese farmers. The more circular patterns, appears in a grid pattern to the North (up) and West (left), are government-run and 'national' farms. The scene is roughly 150 miles tall and 200 miles wide. The city of Santa Cruz lies to the west of the river cutting through the scene.
Completed 1999-12-01
Bolivian Deforestation 1984- …
Title Bolivian Deforestation 1984-1998: Fast Dissolve without Dates
Abstract These images show deforestation near Santa Cruz, Bolivia from 1984 to 1998. In the initial 1984 scene, some clearing has already occurred in the humid forest and chaparral. The long striped clearings in the center of the scene are predominately from soybean farms created by Mennonite and Japanese farmers. The more circular patterns, appears in a grid pattern to the North (up) and West (left), are government-run and 'national' farms. The scene is roughly 150 miles tall and 200 miles wide. The city of Santa Cruz lies to the west of the river cutting through the scene.
Completed 1999-12-01
Bolivian Deforestation 1984- …
Title Bolivian Deforestation 1984-1998: Fast Dissolve without Dates
Abstract These images show deforestation near Santa Cruz, Bolivia from 1984 to 1998. In the initial 1984 scene, some clearing has already occurred in the humid forest and chaparral. The long striped clearings in the center of the scene are predominately from soybean farms created by Mennonite and Japanese farmers. The more circular patterns, appears in a grid pattern to the North (up) and West (left), are government-run and 'national' farms. The scene is roughly 150 miles tall and 200 miles wide. The city of Santa Cruz lies to the west of the river cutting through the scene.
Completed 1999-12-01
Bolivian Deforestation 1984- …
Title Bolivian Deforestation 1984-1998: Fast Dissolve without Dates
Abstract These images show deforestation near Santa Cruz, Bolivia from 1984 to 1998. In the initial 1984 scene, some clearing has already occurred in the humid forest and chaparral. The long striped clearings in the center of the scene are predominately from soybean farms created by Mennonite and Japanese farmers. The more circular patterns, appears in a grid pattern to the North (up) and West (left), are government-run and 'national' farms. The scene is roughly 150 miles tall and 200 miles wide. The city of Santa Cruz lies to the west of the river cutting through the scene.
Completed 1999-12-01
Bolivian Deforestation 1984- …
Title Bolivian Deforestation 1984-1998: Fast Dissolve without Dates
Abstract These images show deforestation near Santa Cruz, Bolivia from 1984 to 1998. In the initial 1984 scene, some clearing has already occurred in the humid forest and chaparral. The long striped clearings in the center of the scene are predominately from soybean farms created by Mennonite and Japanese farmers. The more circular patterns, appears in a grid pattern to the North (up) and West (left), are government-run and 'national' farms. The scene is roughly 150 miles tall and 200 miles wide. The city of Santa Cruz lies to the west of the river cutting through the scene.
Completed 1999-12-01
Bolivian Deforestation 1984- …
Title Bolivian Deforestation 1984-1998: Fast Dissolve without Dates
Abstract These images show deforestation near Santa Cruz, Bolivia from 1984 to 1998. In the initial 1984 scene, some clearing has already occurred in the humid forest and chaparral. The long striped clearings in the center of the scene are predominately from soybean farms created by Mennonite and Japanese farmers. The more circular patterns, appears in a grid pattern to the North (up) and West (left), are government-run and 'national' farms. The scene is roughly 150 miles tall and 200 miles wide. The city of Santa Cruz lies to the west of the river cutting through the scene.
Completed 1999-12-01
Bolivian Deforestation 1984- …
Title Bolivian Deforestation 1984-1998: Fast Dissolve without Dates
Abstract These images show deforestation near Santa Cruz, Bolivia from 1984 to 1998. In the initial 1984 scene, some clearing has already occurred in the humid forest and chaparral. The long striped clearings in the center of the scene are predominately from soybean farms created by Mennonite and Japanese farmers. The more circular patterns, appears in a grid pattern to the North (up) and West (left), are government-run and 'national' farms. The scene is roughly 150 miles tall and 200 miles wide. The city of Santa Cruz lies to the west of the river cutting through the scene.
Completed 1999-12-01
The fastest CME of Cycle 23 …
Title The fastest CME of Cycle 23 overtakes another fast CME
Abstract On November 4, 2003, the Sun produced its fastest coronal mass ejection (CME) for cycle 23 out of the active region 0486 located near the southwest limb of the Sun. The CME was expelled with a speed of approximately 2700 km/s. At the time of the launch of this CME, there was another ejection in progress from the same region. The previous ejection started about 7 hours earlier with a speed of about 1000 km/s. The fastest CME overtook the previous one within 2 hours and produced a spectacular radio radiation detected by the Wind, Ulysses and Cassini spacecraft. The movie shows the radio emission and the two interacting CMEs as observed by the SOHO spacecraft.
Completed 2004-05-13
The fastest CME of Cycle 23 …
Title The fastest CME of Cycle 23 overtakes another fast CME
Abstract On November 4, 2003, the Sun produced its fastest coronal mass ejection (CME) for cycle 23 out of the active region 0486 located near the southwest limb of the Sun. The CME was expelled with a speed of approximately 2700 km/s. At the time of the launch of this CME, there was another ejection in progress from the same region. The previous ejection started about 7 hours earlier with a speed of about 1000 km/s. The fastest CME overtook the previous one within 2 hours and produced a spectacular radio radiation detected by the Wind, Ulysses and Cassini spacecraft. The movie shows the radio emission and the two interacting CMEs as observed by the SOHO spacecraft.
Completed 2004-05-13
The fastest CME of Cycle 23 …
Title The fastest CME of Cycle 23 overtakes another fast CME
Abstract On November 4, 2003, the Sun produced its fastest coronal mass ejection (CME) for cycle 23 out of the active region 0486 located near the southwest limb of the Sun. The CME was expelled with a speed of approximately 2700 km/s. At the time of the launch of this CME, there was another ejection in progress from the same region. The previous ejection started about 7 hours earlier with a speed of about 1000 km/s. The fastest CME overtook the previous one within 2 hours and produced a spectacular radio radiation detected by the Wind, Ulysses and Cassini spacecraft. The movie shows the radio emission and the two interacting CMEs as observed by the SOHO spacecraft.
Completed 2004-05-13
The fastest CME of Cycle 23 …
Title The fastest CME of Cycle 23 overtakes another fast CME
Abstract On November 4, 2003, the Sun produced its fastest coronal mass ejection (CME) for cycle 23 out of the active region 0486 located near the southwest limb of the Sun. The CME was expelled with a speed of approximately 2700 km/s. At the time of the launch of this CME, there was another ejection in progress from the same region. The previous ejection started about 7 hours earlier with a speed of about 1000 km/s. The fastest CME overtook the previous one within 2 hours and produced a spectacular radio radiation detected by the Wind, Ulysses and Cassini spacecraft. The movie shows the radio emission and the two interacting CMEs as observed by the SOHO spacecraft.
Completed 2004-05-13
The fastest CME of Cycle 23 …
Title The fastest CME of Cycle 23 overtakes another fast CME
Abstract On November 4, 2003, the Sun produced its fastest coronal mass ejection (CME) for cycle 23 out of the active region 0486 located near the southwest limb of the Sun. The CME was expelled with a speed of approximately 2700 km/s. At the time of the launch of this CME, there was another ejection in progress from the same region. The previous ejection started about 7 hours earlier with a speed of about 1000 km/s. The fastest CME overtook the previous one within 2 hours and produced a spectacular radio radiation detected by the Wind, Ulysses and Cassini spacecraft. The movie shows the radio emission and the two interacting CMEs as observed by the SOHO spacecraft.
Completed 2004-05-13
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