|
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Phoebe's Radiation
| Description |
Phoebe's Radiation |
| Full Description |
This image shows thermal radiation from the day and night sides of Saturn's moon Phoebe, taken by the composite infrared spectrometer onboard Cassini 1.8 hours before the spacecraft's closest approach to Phoebe on June 11, 2004. The left-hand panel displays the image in grayscale format, showing the brightness of Phoebe's radiation in the wavelength range 15-17 microns, which is about 25 times the longest wavelength visible to the naked eye. In the middle panel this brightness is used to estimate the surface temperature distribution across Phoebe. Temperatures are given in degrees Kelvin, and vary from a relatively toasty 107 Kelvin (-267 Fahrenheit), in the late morning near the equator (white, lower right), to less than 75 Kelvin (-324 Fahrenheit) in the northern hemisphere in the pre-dawn hours (dark blue, upper left). The "ragged edge" of Phoebe in this region is an instrumental artifact. Temperatures are affected strongly by topography, as can be seen by comparison with the visible-wavelength image (right). Some of the coldest temperatures are found in the shadowed region inside the large depression in the northern hemisphere (upper right). 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 Cassini-Huygens mission for NASA's Office of Space Science, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The composite infrared spectrometer team is based at NASA's Goddard Space Flight Center, Greenbelt, Md. For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini composite infrared spectrometer home page at http://cirs.gsfc.nasa.gov/ . Image Credit: NASA/JPL/Goddard Space Flight Center |
|
Phoebe Temperature Maps
| Description |
Phoebe Temperature Maps |
| Full Description |
A montage of maps of Saturn's moon Phoebe shows surface temperatures at various times of day as determined by the composite infrared spectrometer onboard Cassini during the June 11, 2004, Phoebe flyby. The asterisk on each map shows the location of the subsolar point, where the Sun is directly overhead. This point moves across the surface as Phoebe rotates. It is morning in regions to the left of the subsolar point, and afternoon in regions to the right. Like a newspaper weather map, different colors indicate different temperatures, though Phoebe's temperatures are distinctly cooler than even the coldest January day on Earth. Equatorial temperatures peak in the early afternoon near 112 Kelvin (-257 Fahrenheit), plunging to 78 Kelvin (-319 Fahrenheit) before dawn, and are even colder at higher latitudes. The large day/night temperature contrasts imply that Phoebe's surface is covered in loose dust or ice particles that store little heat and thus cool off rapidly at night. Regions of Phoebe's surface that were not observed are shown in black. Most of the maps show the effect on surface temperatures of the large crater-like depression seen in Cassini's visible-wavelength images of Phoebe, which is located just left of center in these maps. Crater walls that are shadowed and cold in the early morning in the first map are sunlit and warm in the late afternoon in the final map. 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 Cassini-Huygens mission for NASA's Office of Space Science, Washington, D.C. The Cassini orbiter was designed, developed and assembled at JPL. The composite infrared spectrometer team is based at NASA's Goddard Space Flight Center, Greenbelt, Md. For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini composite infrared spectrometer home page at http://cirs.gsfc.nasa.gov/ . Image Credit: NASA/JPL/Goddard Space Flight Center |
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Hubble Approaches the Final
…
| Title |
Hubble Approaches the Final Frontier: The Dawn of Galaxies |
|
Hubble Approaches the Final
…
| Title |
Hubble Approaches the Final Frontier: The Dawn of Galaxies |
|
Hubble Approaches the Final
…
| Title |
Hubble Approaches the Final Frontier: The Dawn of Galaxies |
|
Hubble Approaches the Final
…
| Title |
Hubble Approaches the Final Frontier: The Dawn of Galaxies |
|
Hubble Approaches the Final
…
| Title |
Hubble Approaches the Final Frontier: The Dawn of Galaxies |
|
Hubble Images of Asteroids H
…
| Title |
Hubble Images of Asteroids Help Astronomers Prepare for Spacecraft Visit |
|
Hubble Images of Asteroids H
…
| Title |
Hubble Images of Asteroids Help Astronomers Prepare for Spacecraft Visit |
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Hubble Images of Asteroids H
…
| Title |
Hubble Images of Asteroids Help Astronomers Prepare for Spacecraft Visit |
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Mount St. Helens
| Title |
Mount St. Helens |
| Description |
Hot lava had broken through the surface of the growing lava dome on Mount St. Helens when the MASTER sensor took this image in the early morning hours of October 13, 2004. MASTER, which stands for MODIS/ASTER Airborne Simulator, is an aircraft- mounted remote sensing device built to simulate the Moderate Resolution Imaging Spectroradiometer (MODIS [ http://modis.gsfc.nasa.gov/ ]) and Advanced Spaceborne Thermal Emission and Reflection Radiometer [ http://asterweb.jpl.nasa.gov/ ] (ASTER) instruments on NASA's Terra [ http://terra.nasa.gov/ ] satellite. The top image was made from MASTER's thermal sensitive bands, and shows the heat in the volcano's crater. A brilliant white spot on the southwest side of the crater is hot lava bubbling to the surface. Smaller, less intense hot spots around the crater have formed where magma near the surface has heated the rock above it. The dark area around the lava dome is the crater. Shielded from the sun and covered with snow, the dark crater floor is cooler than the surrounding landscape, which appears red. A plume of steam rising from the lava dome (colored purple) drifts southeast in this image. The plume and crater floor are more visible in the lower, true color image. Acquired just after dawn, the image has few shadows and low contrast. An image composed of thermal infrared and visible light wavelengths reveals more details around the mountain. The volcanic plume is bright cyan, the cool crater is purple, and snow is light blue. To the north of the volcano, two bright red lines extend from south to north. These are warm-water streams, possibly heated by the active volcano. NASA images courtesy Jeff Myers, MASTER [ http://masterweb.jpl.nasa.gov/ ] instrument team, NASA Ames Research Center |
|
Mount St. Helens
| Title |
Mount St. Helens |
| Description |
Hot lava had broken through the surface of the growing lava dome on Mount St. Helens when the MASTER sensor took this image in the early morning hours of October 13, 2004. MASTER, which stands for MODIS/ASTER Airborne Simulator, is an aircraft- mounted remote sensing device built to simulate the Moderate Resolution Imaging Spectroradiometer (MODIS [ http://modis.gsfc.nasa.gov/ ]) and Advanced Spaceborne Thermal Emission and Reflection Radiometer [ http://asterweb.jpl.nasa.gov/ ] (ASTER) instruments on NASA's Terra [ http://terra.nasa.gov/ ] satellite. The top image was made from MASTER's thermal sensitive bands, and shows the heat in the volcano's crater. A brilliant white spot on the southwest side of the crater is hot lava bubbling to the surface. Smaller, less intense hot spots around the crater have formed where magma near the surface has heated the rock above it. The dark area around the lava dome is the crater. Shielded from the sun and covered with snow, the dark crater floor is cooler than the surrounding landscape, which appears red. A plume of steam rising from the lava dome (colored purple) drifts southeast in this image. The plume and crater floor are more visible in the lower, true color image. Acquired just after dawn, the image has few shadows and low contrast. An image composed of thermal infrared and visible light wavelengths reveals more details around the mountain. The volcanic plume is bright cyan, the cool crater is purple, and snow is light blue. To the north of the volcano, two bright red lines extend from south to north. These are warm-water streams, possibly heated by the active volcano. NASA images courtesy Jeff Myers, MASTER [ http://masterweb.jpl.nasa.gov/ ] instrument team, NASA Ames Research Center |
|
Severe Floods Sweep Across H
…
| Title |
Severe Floods Sweep Across Haiti and the Dominican Republic |
| Description |
Over the past week, both Haiti and the Dominican Republic, the two countries on the island of Hispaniola, have been ravaged by severe flooding after several days of heavy rain. Hundreds have perished in the two countries as a direct result of mud slides and flash flooding. The hardest hit area was in and around the town of Jimani in the southwestern part of the Dominican Republic near the border with Haiti. The Soliel River overflowed its banks before dawn on the morning of the 25th of May 2004 catching the town by surprise. A trough of low pressure across the central Caribbean provided the impetus for the numerous showers and heavy rains. The effect was amplified as moisture-laden low-level southerly winds from the Caribbean interacted with the topography of the island. The Dominican weather service reported that 10 inches of rain fell near Jimani in just 24 hours. The Tropical Rainfall Measuring Mission satellite which was launched in November of 1997 uses both passive and active sensors to measure rainfall over the global tropics from space. The TRMM-based, near-real time Multi-satellite Precipitation Analysis (MPA) at the NASA Goddard Space Flight Center provides quantitative rainfall estimates over the global tropics. The above images show rainfall accumulation between May 18 and May 25, 2004. The first lower shows MPA rainfall totals over the northern Caribbean. The red areas indicate rainfall totals in excess of 14 inches over most of Hispaniola. Darker red areas along the border between Haiti and the Dominican Republic show rainfall totals for the period approaching 24 inches. The second image provides a close-in view of rainfall contours over the same period. It shows that the highest totals are right along the border between Haiti and the Dominican Republic and over the northeastern part of the Dominican Republic and exceed 550 mm (21.7 inches). The above animations show that the bulk of the rain appears to have fallen in a single day on May 23. This graph confirms what the animations show in more detail. It shows the instantaneous average rainfall over a 250-km radius centered at 19N 72W (near the center of the border between Haiti and the Dominican Republic) over the period. It reveals that most of the rain did, in fact, fall on the 23rd of May although significant amounts fell on May 22 and 24 as well. The dates begin at 00Z (midnight Greenwich Mean Time, or 7 pm local time). This graph shows the accumulated rainfall with time for the same area and period. By 00Z on the 25th, an average of 300 mm (11.8 inches) of rain had fallen over the area with a maximum single point accumulation of 598 mm (23.5 inches).TRMM [ http://trmm.gsfc.nasa.gov/ ] is a joint mission between NASA and the Japanese space agency JAXA. Images produced by Hal Pierce (SSAI/NASA GSFC) and caption by Steve Lang |
|
Severe Floods Sweep Across H
…
| Title |
Severe Floods Sweep Across Haiti and the Dominican Republic |
| Description |
Over the past week, both Haiti and the Dominican Republic, the two countries on the island of Hispaniola, have been ravaged by severe flooding after several days of heavy rain. Hundreds have perished in the two countries as a direct result of mud slides and flash flooding. The hardest hit area was in and around the town of Jimani in the southwestern part of the Dominican Republic near the border with Haiti. The Soliel River overflowed its banks before dawn on the morning of the 25th of May 2004 catching the town by surprise. A trough of low pressure across the central Caribbean provided the impetus for the numerous showers and heavy rains. The effect was amplified as moisture-laden low-level southerly winds from the Caribbean interacted with the topography of the island. The Dominican weather service reported that 10 inches of rain fell near Jimani in just 24 hours. The Tropical Rainfall Measuring Mission satellite which was launched in November of 1997 uses both passive and active sensors to measure rainfall over the global tropics from space. The TRMM-based, near-real time Multi-satellite Precipitation Analysis (MPA) at the NASA Goddard Space Flight Center provides quantitative rainfall estimates over the global tropics. The above images show rainfall accumulation between May 18 and May 25, 2004. The first lower shows MPA rainfall totals over the northern Caribbean. The red areas indicate rainfall totals in excess of 14 inches over most of Hispaniola. Darker red areas along the border between Haiti and the Dominican Republic show rainfall totals for the period approaching 24 inches. The second image provides a close-in view of rainfall contours over the same period. It shows that the highest totals are right along the border between Haiti and the Dominican Republic and over the northeastern part of the Dominican Republic and exceed 550 mm (21.7 inches). The above animations show that the bulk of the rain appears to have fallen in a single day on May 23. This graph confirms what the animations show in more detail. It shows the instantaneous average rainfall over a 250-km radius centered at 19N 72W (near the center of the border between Haiti and the Dominican Republic) over the period. It reveals that most of the rain did, in fact, fall on the 23rd of May although significant amounts fell on May 22 and 24 as well. The dates begin at 00Z (midnight Greenwich Mean Time, or 7 pm local time). This graph shows the accumulated rainfall with time for the same area and period. By 00Z on the 25th, an average of 300 mm (11.8 inches) of rain had fallen over the area with a maximum single point accumulation of 598 mm (23.5 inches).TRMM [ http://trmm.gsfc.nasa.gov/ ] is a joint mission between NASA and the Japanese space agency JAXA. Images produced by Hal Pierce (SSAI/NASA GSFC) and caption by Steve Lang |
|
Severe Floods Sweep Across H
…
| Title |
Severe Floods Sweep Across Haiti and the Dominican Republic |
| Description |
Over the past week, both Haiti and the Dominican Republic, the two countries on the island of Hispaniola, have been ravaged by severe flooding after several days of heavy rain. Hundreds have perished in the two countries as a direct result of mud slides and flash flooding. The hardest hit area was in and around the town of Jimani in the southwestern part of the Dominican Republic near the border with Haiti. The Soliel River overflowed its banks before dawn on the morning of the 25th of May 2004 catching the town by surprise. A trough of low pressure across the central Caribbean provided the impetus for the numerous showers and heavy rains. The effect was amplified as moisture-laden low-level southerly winds from the Caribbean interacted with the topography of the island. The Dominican weather service reported that 10 inches of rain fell near Jimani in just 24 hours. The Tropical Rainfall Measuring Mission satellite which was launched in November of 1997 uses both passive and active sensors to measure rainfall over the global tropics from space. The TRMM-based, near-real time Multi-satellite Precipitation Analysis (MPA) at the NASA Goddard Space Flight Center provides quantitative rainfall estimates over the global tropics. The above images show rainfall accumulation between May 18 and May 25, 2004. The first lower shows MPA rainfall totals over the northern Caribbean. The red areas indicate rainfall totals in excess of 14 inches over most of Hispaniola. Darker red areas along the border between Haiti and the Dominican Republic show rainfall totals for the period approaching 24 inches. The second image provides a close-in view of rainfall contours over the same period. It shows that the highest totals are right along the border between Haiti and the Dominican Republic and over the northeastern part of the Dominican Republic and exceed 550 mm (21.7 inches). The above animations show that the bulk of the rain appears to have fallen in a single day on May 23. This graph confirms what the animations show in more detail. It shows the instantaneous average rainfall over a 250-km radius centered at 19N 72W (near the center of the border between Haiti and the Dominican Republic) over the period. It reveals that most of the rain did, in fact, fall on the 23rd of May although significant amounts fell on May 22 and 24 as well. The dates begin at 00Z (midnight Greenwich Mean Time, or 7 pm local time). This graph shows the accumulated rainfall with time for the same area and period. By 00Z on the 25th, an average of 300 mm (11.8 inches) of rain had fallen over the area with a maximum single point accumulation of 598 mm (23.5 inches).TRMM [ http://trmm.gsfc.nasa.gov/ ] is a joint mission between NASA and the Japanese space agency JAXA. Images produced by Hal Pierce (SSAI/NASA GSFC) and caption by Steve Lang |
|
Severe Floods Sweep Across H
…
| Title |
Severe Floods Sweep Across Haiti and the Dominican Republic |
| Description |
Over the past week, both Haiti and the Dominican Republic, the two countries on the island of Hispaniola, have been ravaged by severe flooding after several days of heavy rain. Hundreds have perished in the two countries as a direct result of mud slides and flash flooding. The hardest hit area was in and around the town of Jimani in the southwestern part of the Dominican Republic near the border with Haiti. The Soliel River overflowed its banks before dawn on the morning of the 25th of May 2004 catching the town by surprise. A trough of low pressure across the central Caribbean provided the impetus for the numerous showers and heavy rains. The effect was amplified as moisture-laden low-level southerly winds from the Caribbean interacted with the topography of the island. The Dominican weather service reported that 10 inches of rain fell near Jimani in just 24 hours. The Tropical Rainfall Measuring Mission satellite which was launched in November of 1997 uses both passive and active sensors to measure rainfall over the global tropics from space. The TRMM-based, near-real time Multi-satellite Precipitation Analysis (MPA) at the NASA Goddard Space Flight Center provides quantitative rainfall estimates over the global tropics. The above images show rainfall accumulation between May 18 and May 25, 2004. The first lower shows MPA rainfall totals over the northern Caribbean. The red areas indicate rainfall totals in excess of 14 inches over most of Hispaniola. Darker red areas along the border between Haiti and the Dominican Republic show rainfall totals for the period approaching 24 inches. The second image provides a close-in view of rainfall contours over the same period. It shows that the highest totals are right along the border between Haiti and the Dominican Republic and over the northeastern part of the Dominican Republic and exceed 550 mm (21.7 inches). The above animations show that the bulk of the rain appears to have fallen in a single day on May 23. This graph confirms what the animations show in more detail. It shows the instantaneous average rainfall over a 250-km radius centered at 19N 72W (near the center of the border between Haiti and the Dominican Republic) over the period. It reveals that most of the rain did, in fact, fall on the 23rd of May although significant amounts fell on May 22 and 24 as well. The dates begin at 00Z (midnight Greenwich Mean Time, or 7 pm local time). This graph shows the accumulated rainfall with time for the same area and period. By 00Z on the 25th, an average of 300 mm (11.8 inches) of rain had fallen over the area with a maximum single point accumulation of 598 mm (23.5 inches).TRMM [ http://trmm.gsfc.nasa.gov/ ] is a joint mission between NASA and the Japanese space agency JAXA. Images produced by Hal Pierce (SSAI/NASA GSFC) and caption by Steve Lang |
|
Severe Floods Sweep Across H
…
| Title |
Severe Floods Sweep Across Haiti and the Dominican Republic |
| Description |
Over the past week, both Haiti and the Dominican Republic, the two countries on the island of Hispaniola, have been ravaged by severe flooding after several days of heavy rain. Hundreds have perished in the two countries as a direct result of mud slides and flash flooding. The hardest hit area was in and around the town of Jimani in the southwestern part of the Dominican Republic near the border with Haiti. The Soliel River overflowed its banks before dawn on the morning of the 25th of May 2004 catching the town by surprise. A trough of low pressure across the central Caribbean provided the impetus for the numerous showers and heavy rains. The effect was amplified as moisture-laden low-level southerly winds from the Caribbean interacted with the topography of the island. The Dominican weather service reported that 10 inches of rain fell near Jimani in just 24 hours. The Tropical Rainfall Measuring Mission satellite which was launched in November of 1997 uses both passive and active sensors to measure rainfall over the global tropics from space. The TRMM-based, near-real time Multi-satellite Precipitation Analysis (MPA) at the NASA Goddard Space Flight Center provides quantitative rainfall estimates over the global tropics. The above images show rainfall accumulation between May 18 and May 25, 2004. The first lower shows MPA rainfall totals over the northern Caribbean. The red areas indicate rainfall totals in excess of 14 inches over most of Hispaniola. Darker red areas along the border between Haiti and the Dominican Republic show rainfall totals for the period approaching 24 inches. The second image provides a close-in view of rainfall contours over the same period. It shows that the highest totals are right along the border between Haiti and the Dominican Republic and over the northeastern part of the Dominican Republic and exceed 550 mm (21.7 inches). The above animations show that the bulk of the rain appears to have fallen in a single day on May 23. This graph confirms what the animations show in more detail. It shows the instantaneous average rainfall over a 250-km radius centered at 19N 72W (near the center of the border between Haiti and the Dominican Republic) over the period. It reveals that most of the rain did, in fact, fall on the 23rd of May although significant amounts fell on May 22 and 24 as well. The dates begin at 00Z (midnight Greenwich Mean Time, or 7 pm local time). This graph shows the accumulated rainfall with time for the same area and period. By 00Z on the 25th, an average of 300 mm (11.8 inches) of rain had fallen over the area with a maximum single point accumulation of 598 mm (23.5 inches).TRMM [ http://trmm.gsfc.nasa.gov/ ] is a joint mission between NASA and the Japanese space agency JAXA. Images produced by Hal Pierce (SSAI/NASA GSFC) and caption by Steve Lang |
|
Severe Floods Sweep Across H
…
| Title |
Severe Floods Sweep Across Haiti and the Dominican Republic |
| Description |
Over the past week, both Haiti and the Dominican Republic, the two countries on the island of Hispaniola, have been ravaged by severe flooding after several days of heavy rain. Hundreds have perished in the two countries as a direct result of mud slides and flash flooding. The hardest hit area was in and around the town of Jimani in the southwestern part of the Dominican Republic near the border with Haiti. The Soliel River overflowed its banks before dawn on the morning of the 25th of May 2004 catching the town by surprise. A trough of low pressure across the central Caribbean provided the impetus for the numerous showers and heavy rains. The effect was amplified as moisture-laden low-level southerly winds from the Caribbean interacted with the topography of the island. The Dominican weather service reported that 10 inches of rain fell near Jimani in just 24 hours. The Tropical Rainfall Measuring Mission satellite which was launched in November of 1997 uses both passive and active sensors to measure rainfall over the global tropics from space. The TRMM-based, near-real time Multi-satellite Precipitation Analysis (MPA) at the NASA Goddard Space Flight Center provides quantitative rainfall estimates over the global tropics. The above images show rainfall accumulation between May 18 and May 25, 2004. The first lower shows MPA rainfall totals over the northern Caribbean. The red areas indicate rainfall totals in excess of 14 inches over most of Hispaniola. Darker red areas along the border between Haiti and the Dominican Republic show rainfall totals for the period approaching 24 inches. The second image provides a close-in view of rainfall contours over the same period. It shows that the highest totals are right along the border between Haiti and the Dominican Republic and over the northeastern part of the Dominican Republic and exceed 550 mm (21.7 inches). The above animations show that the bulk of the rain appears to have fallen in a single day on May 23. This graph confirms what the animations show in more detail. It shows the instantaneous average rainfall over a 250-km radius centered at 19N 72W (near the center of the border between Haiti and the Dominican Republic) over the period. It reveals that most of the rain did, in fact, fall on the 23rd of May although significant amounts fell on May 22 and 24 as well. The dates begin at 00Z (midnight Greenwich Mean Time, or 7 pm local time). This graph shows the accumulated rainfall with time for the same area and period. By 00Z on the 25th, an average of 300 mm (11.8 inches) of rain had fallen over the area with a maximum single point accumulation of 598 mm (23.5 inches).TRMM [ http://trmm.gsfc.nasa.gov/ ] is a joint mission between NASA and the Japanese space agency JAXA. Images produced by Hal Pierce (SSAI/NASA GSFC) and caption by Steve Lang |
|
Thunderstorms above the Sier
…
| Title |
Thunderstorms above the Sierra Nevada |
| Description |
On June 14, 2004, a series of thunderstorms swept over the southern Sierra Nevada. Storms during the summer are frequent in the area. Warm air rises up the flanks of the mountains, cooling as it gains altitude. Moisture in the air then condenses, creating clouds and rainfall. This image was acquired by the National Oceanic and Atmospheric Administration?s Geostationary Operational Environmental Satellite Program (GOES)-West satellite on June 14, 2004, at 4:00 PDT. The animations include data from dawn until dusk. Image and animation by Robert Simmon, based on data provided by the GOES Project Science [ http://rsd.gsfc.nasa.gov/goes/ ] office |
|
Thunderstorms above the Sier
…
| Title |
Thunderstorms above the Sierra Nevada |
| Description |
On June 14, 2004, a series of thunderstorms swept over the southern Sierra Nevada. Storms during the summer are frequent in the area. Warm air rises up the flanks of the mountains, cooling as it gains altitude. Moisture in the air then condenses, creating clouds and rainfall. This image was acquired by the National Oceanic and Atmospheric Administration?s Geostationary Operational Environmental Satellite Program (GOES)-West satellite on June 14, 2004, at 4:00 PDT. The animations include data from dawn until dusk. Image and animation by Robert Simmon, based on data provided by the GOES Project Science [ http://rsd.gsfc.nasa.gov/goes/ ] office |
|
Ceres: Asteroid or Planet?
| Title |
Ceres: Asteroid or Planet? |
| Explanation |
Is Ceres [ http://en.wikipedia.org/wiki/Ceres_%28asteroid%29 ] an asteroid [ http://www.nineplanets.org/asteroids.html ] or a planet? Although a trivial designation to some, the recent suggestion by the Planet Definition Committee [ http://www.iau2006.org/mirror/www.iau.org/iau0601/iau0601_committee.html ] of the International Astronomical Union [ http://www.iau2006.org/mirror/www.iau.org/NEWS.55.0.html ] would have Ceres reclassified from asteroid to planet. A change in taxonomy might lead to more notoriety for the frequently overlooked world. Ceres [ http://www.pantheon.org/articles/c/ceres.html ], at about 1000 kilometers across, is the largest object in the main asteroid belt [ http://www.solstation.com/stars/asteroid.htm ] between Mars and Jupiter. Under the newly proposed criteria [ http://www.iau2006.org/mirror/www.iau.org/iau0601/iau0601_release.html ], Ceres would qualify as a planet because it is nearly spherical and sufficiently distant from other planets. Pictured above [ http://hubblesite.org/newscenter/newsdesk/archive/releases/2005/27/image/a ] is the best picture yet of Ceres, taken by the Hubble Space Telescope [ http://antwrp.gsfc.nasa.gov/apod/ap010806.html ] as part of a series of exposures ending in 2004 January. Currently, NASA's Dawn mission [ http://dawn.jpl.nasa.gov/ ] is scheduled to launch in 2007 June to explore Ceres and Vesta [ http://antwrp.gsfc.nasa.gov/apod/ap060820.html ], regardless of their future designations. |
|
Severe Floods Sweep Across H
…
nasa, nasanaturalhazards
* eoimages.gsfc.nasa.gov/ima
…
hispaniola_TRMM18-25may04
| mediatype |
IMAGE |
| mediatype |
image |
| date |
2004-05-25 |
| creator |
NASA -- NASA Image Of The Day |
| identifier |
hispaniola_TRMM18-25may04 |
|
Thunderstorms above the Sier
…
nasa, nasanaturalhazards
* eoimages.gsfc.nasa.gov/ima
…
sierra_goe_2004166
| mediatype |
IMAGE |
| mediatype |
image |
| date |
2004-06-14 |
| creator |
NASA -- NASA Image Of The Day |
| identifier |
sierra_goe_2004166 |
|
Lava on Mount Saint Helens:
…
nasa, nasaimageofthedaygalle
…
* eoimages.gsfc.nasa.gov/ima
…
sthelens_mst_2004287
| mediatype |
IMAGE |
| mediatype |
image |
| date |
2004-10-13 |
| creator |
NASA -- Images courtesy Jeffrey Myers, NASA Ames Research Center |
| identifier |
sthelens_mst_2004287 |
|
Phoebe Temperature Maps
PIA06403
Saturn
Composite Infrared Spectrome
…
| Title |
Phoebe Temperature Maps |
| Original Caption Released with Image |
A montage of maps of Saturn's moon Phoebe shows surface temperatures at various times of day as determined by the composite infrared spectrometer onboard Cassini during the June 11, 2004, Phoebe flyby. The asterisk on each map shows the location of the subsolar point, where the Sun is directly overhead. This point moves across the surface as Phoebe rotates. It is morning in regions to the left of the subsolar point, and afternoon in regions to the right. Like a newspaper weather map, different colors indicate different temperatures, though Phoebe's temperatures are distinctly cooler than even the coldest January day on Earth. Equatorial temperatures peak in the early afternoon near 112 Kelvin (-257 Fahrenheit), plunging to 78 Kelvin (-319 Fahrenheit) before dawn, and are even colder at higher latitudes. The large day/night temperature contrasts imply that Phoebe's surface is covered in loose dust or ice particles that store little heat and thus cool off rapidly at night. Regions of Phoebe's surface that were not observed are shown in black. Most of the maps show the effect on surface temperatures of the large crater-like depression seen in Cassini's visible-wavelength images of Phoebe, which is located just left of center in these maps. Crater walls that are shadowed and cold in the early morning in the first map are sunlit and warm in the late afternoon in the final map. 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 Cassini-Huygens mission for NASA's Office of Space Science, Washington, D.C. The Cassini orbiter was designed, developed and assembled at JPL. The composite infrared spectrometer team is based at NASA's Goddard Space Flight Center, Greenbelt, Md. For more information, about the Cassini-Huygens mission visit, http://saturn.jpl.nasa.gov [ http://saturn.jpl.nasa.gov/ ] and the Cassini imaging team home page, http//cirs.gsfc.nasa.gov/ [ http://cirs.gsfc.nasa.gov/ ]. |
|
Phoebe's Radiation
PIA06402
Saturn
Composite Infrared Spectrome
…
| Title |
Phoebe's Radiation |
| Original Caption Released with Image |
This image shows thermal radiation from the day and night sides of Saturn's moon Phoebe, taken by the composite infrared spectrometer onboard Cassini 1.8 hours before the spacecraft's closest approach to Phoebe on June 11, 2004. The left-hand panel displays the image in grayscale format, showing the brightness of Phoebe's radiation in the wavelength range 15-17 microns, which is about 25 times the longest wavelength visible to the naked eye. In the middle panel this brightness is used to estimate the surface temperature distribution across Phoebe. Temperatures are given in degrees Kelvin, and vary from a relatively toasty 107 Kelvin (-267 Fahrenheit), in the late morning near the equator (white, lower right), to less than 75 Kelvin (-324 Fahrenheit) in the northern hemisphere in the pre-dawn hours (dark blue, upper left). The "ragged edge" of Phoebe in this region is an instrumental artifact. Temperatures are affected strongly by topography, as can be seen by comparison with the visible-wavelength image (right). Some of the coldest temperatures are found in the shadowed region inside the large depression in the northern hemisphere (upper right). 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 Cassini-Huygens mission for NASA's Office of Space Science, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The composite infrared spectrometer team is based at NASA's Goddard Space Flight Center, Greenbelt, Md. For more information, about the Cassini-Huygens mission visit, http://saturn.jpl.nasa.gov [ http://saturn.jpl.nasa.gov/ ] and the Cassini imaging team home page, http//cirs.gsfc.nasa.gov/ [ http://cirs.gsfc.nasa.gov/ ]. |
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Dunes in Twilight
PIA05242
Sol (our sun)
Mars Orbiter Camera
| Title |
Dunes in Twilight |
| Original Caption Released with Image |
17 January 2004 This Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC) image shows frost-covered north polar dunes in early January 2004. When this picture was taken, the dunes were in twilight, just before the late winter dawn that would come a few days later. These dunes spent many of the last several months in complete darkness. In this image, they are illuminated only by sunlight that has been scattered over the horizon by the martian atmosphere. These dunes are located near 77.0°N, 246.2°W. The image covers an area 3 km (1.9 mi) wide and has been expanded by 200% from its original 12 meters (39 ft.) per pixel scale. While the sun had not yet risen when the image was obtained, illumination is mostly from the lower left. |
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Meteor Search by Spirit, Sol
…
PIA03613
Sol (our sun)
Panoramic Camera
| Title |
Meteor Search by Spirit, Sol 643 |
| Original Caption Released with Image |
, and Selsis et al. (2005) Nature, vol 435, p. 581). On Earth, some meteors come in "storms" or "showers" at predictable times of the year, like the famous Perseid meteor shower in August or the Leonid meteor shower in November. These "storms" happen when Earth passes through the same parts of space where comets sometimes pass. The meteors we see at these times are from leftover debris that was shed off of these comets. The same kind of thing is predicted for Mars, as well. Inspired by calculations about Martian meteor storms by meteor scientists from the University of Western Ontario in Canada and the Centre de Recherche en Astrophysique de Lyon in France, and also aided by other meteor research colleagues from NASA's Marshall Space Flight Center, scientists on the rover team planned some observations to try to detect predicted meteor storms in October and November, 2005. The views shown here are a composite of nine 60-second exposures taken with the panoramic camera on Spirit during night hours of sol 643 (Oct. 25, 2005), during a week when Mars was predicted to pass through a meteor stream associated with comet P/2001R1 LONEOS. Many stars can be seen in the images, appearing as curved "dash-dot" streaks. The star trails are curved because Mars is rotating while the camera takes the images. The dash-dot pattern is an artifact of taking an image for 60 seconds, then pausing about 10 seconds while the image is processed and stored by the rover's computer, then taking another image for 60 seconds, etc., for a total of about 10 minutes worth of "staring" at the night sky. Many stars from the southern constellations Octans and Pavonis can be seen in the images. The brightest ones in this view would be easily visible to the naked eye, but the faintest ones are slightly dimmer than the human eye can detect. In addition to the star trails, there are several smaller linear streaks, dots and splotches that are the trails left by cosmic rays hitting the camera detectors. Cosmic rays are high-energy particles that are created in the Sun and in other stars throughout our galaxy and travel through space in all directions. Some of them strike Earth or other planets, and ones that strike a digital camera detector can leave little tracks or splotches like those seen in these images. Because they come from all directions, some strike the detector face-on, and others strike at glancing angles. Some even skip across the detector like flat rocks skipped across a pond. These are very common phenomena to astronomers used to working with sensitive digital cameras like those in the Mars rovers, the Hubble Space Telescope, or other space probes, and while they can be a nuisance when taking pictures, they generally do not cause any lasting damage to the cameras. One streak in the image, crossing at an angle very different from the direction of the stars'"motion," might be a meteor trail or could be the mark of another cosmic ray. While hunting for meteors on Mars, Annotated Meteor Search by Spirit, Sol 643 The panoramic cameras on NASA's Mars Exploration Rovers are about as sensitive as the human eye at night. The cameras can see the same bright stars that we can see from Earth, and the same patterns of constellations dot the night sky. Scientists on the rover team have been taking images of some of these bright stars as part of several different projects. One project is designed to try to capture "shooting stars," or meteors, in the Martian night sky. "Meteoroids" are small pieces of comets and asteroids that travel through space and eventually run into a planet. On Earth, we can sometimes see meteoroids become brilliant, long "meteors" streaking across the night sky as they burn up from the friction in our atmosphere. Some of these meteors survive their fiery flight and land on the surface (or in the ocean) where, if found, they are called "meteorites." The same thing happens in the Martian atmosphere, and Spirit even accidentally discovered a meteor while attempting to obtain images of Earth in the pre-dawn sky back in March, 2004 (see http://marsrovers.jpl.nasa.gov/gallery/press/spirit/20040311a.html [ http://marsrovers.jpl.nasa.gov/gallery/press/spirit/20040311a.html ], is fun, ultimately the team wants to use the images and results for scientific purposes. These include helping to validate the models and predictions for interplanetary meteor storms, providing information on the rate of impacts of small meteoroids with Mars for comparison with rates for the Earth and Moon, assessing the rate and intensity of cosmic ray impact events in the Martian environment, and looking at whether some bright stars are being dimmed occasionally by water ice or dust clouds occurring at night during different Martian seasons. |
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Meteor Search by Spirit, Sol
…
PIA03613
Sol (our sun)
Panoramic Camera
| Title |
Meteor Search by Spirit, Sol 643 |
| Original Caption Released with Image |
, and Selsis et al. (2005) Nature, vol 435, p. 581). On Earth, some meteors come in "storms" or "showers" at predictable times of the year, like the famous Perseid meteor shower in August or the Leonid meteor shower in November. These "storms" happen when Earth passes through the same parts of space where comets sometimes pass. The meteors we see at these times are from leftover debris that was shed off of these comets. The same kind of thing is predicted for Mars, as well. Inspired by calculations about Martian meteor storms by meteor scientists from the University of Western Ontario in Canada and the Centre de Recherche en Astrophysique de Lyon in France, and also aided by other meteor research colleagues from NASA's Marshall Space Flight Center, scientists on the rover team planned some observations to try to detect predicted meteor storms in October and November, 2005. The views shown here are a composite of nine 60-second exposures taken with the panoramic camera on Spirit during night hours of sol 643 (Oct. 25, 2005), during a week when Mars was predicted to pass through a meteor stream associated with comet P/2001R1 LONEOS. Many stars can be seen in the images, appearing as curved "dash-dot" streaks. The star trails are curved because Mars is rotating while the camera takes the images. The dash-dot pattern is an artifact of taking an image for 60 seconds, then pausing about 10 seconds while the image is processed and stored by the rover's computer, then taking another image for 60 seconds, etc., for a total of about 10 minutes worth of "staring" at the night sky. Many stars from the southern constellations Octans and Pavonis can be seen in the images. The brightest ones in this view would be easily visible to the naked eye, but the faintest ones are slightly dimmer than the human eye can detect. In addition to the star trails, there are several smaller linear streaks, dots and splotches that are the trails left by cosmic rays hitting the camera detectors. Cosmic rays are high-energy particles that are created in the Sun and in other stars throughout our galaxy and travel through space in all directions. Some of them strike Earth or other planets, and ones that strike a digital camera detector can leave little tracks or splotches like those seen in these images. Because they come from all directions, some strike the detector face-on, and others strike at glancing angles. Some even skip across the detector like flat rocks skipped across a pond. These are very common phenomena to astronomers used to working with sensitive digital cameras like those in the Mars rovers, the Hubble Space Telescope, or other space probes, and while they can be a nuisance when taking pictures, they generally do not cause any lasting damage to the cameras. One streak in the image, crossing at an angle very different from the direction of the stars'"motion," might be a meteor trail or could be the mark of another cosmic ray. While hunting for meteors on Mars, Annotated Meteor Search by Spirit, Sol 643 The panoramic cameras on NASA's Mars Exploration Rovers are about as sensitive as the human eye at night. The cameras can see the same bright stars that we can see from Earth, and the same patterns of constellations dot the night sky. Scientists on the rover team have been taking images of some of these bright stars as part of several different projects. One project is designed to try to capture "shooting stars," or meteors, in the Martian night sky. "Meteoroids" are small pieces of comets and asteroids that travel through space and eventually run into a planet. On Earth, we can sometimes see meteoroids become brilliant, long "meteors" streaking across the night sky as they burn up from the friction in our atmosphere. Some of these meteors survive their fiery flight and land on the surface (or in the ocean) where, if found, they are called "meteorites." The same thing happens in the Martian atmosphere, and Spirit even accidentally discovered a meteor while attempting to obtain images of Earth in the pre-dawn sky back in March, 2004 (see http://marsrovers.jpl.nasa.gov/gallery/press/spirit/20040311a.html [ http://marsrovers.jpl.nasa.gov/gallery/press/spirit/20040311a.html ], is fun, ultimately the team wants to use the images and results for scientific purposes. These include helping to validate the models and predictions for interplanetary meteor storms, providing information on the rate of impacts of small meteoroids with Mars for comparison with rates for the Earth and Moon, assessing the rate and intensity of cosmic ray impact events in the Martian environment, and looking at whether some bright stars are being dimmed occasionally by water ice or dust clouds occurring at night during different Martian seasons. |
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Meteor Search by Spirit, Sol
…
PIA03615
Sol (our sun)
Panoramic Camera
| Title |
Meteor Search by Spirit, Sol 668 |
| Original Caption Released with Image |
Annotated Meteor Search by Spirit, Sol 668 The panoramic cameras on NASA's Mars Exploration Rovers are about as sensitive as the human eye at night. The cameras can see the same bright stars that we can see from Earth, and the same patterns of constellations dot the night sky. Scientists on the rover team have been taking images of some of these bright stars as part of several different projects. One project is designed to try to capture "shooting stars," or meteors, in the martian night sky. "Meteoroids" are small pieces of comets and asteroids that travel through space and eventually run into a planet. On Earth, we can sometimes see meteoroids become brilliant, long "meteors" streaking across the night sky as they burn up from the friction in our atmosphere. Some of these meteors survive their fiery flight and land on the surface (or in the ocean) where, if found, they are called "meteorites." The same thing happens in the martian atmosphere, and Spirit even accidentally discovered a meteor while attempting to obtain images of Earth in the pre-dawn sky back in March, 2004 (see http://marsrovers.jpl.nasa.gov/gallery/press/spirit/20040311a.html, and Selsis et al. (2005) Nature, vol 435, p. 581). On Earth, some meteors come in "storms" or "showers" at predictable times of the year, like the famous Perseid meteor shower in August or the Leonid meteor shower in November. These "storms" happen when Earth passes through the same parts of space where comets sometimes pass. The meteors we see at these times are from leftover debris that was shed off of these comets. The same kind of thing is predicted for Mars, as well. Inspired by calculations about Martian meteor storms by meteor scientists from the University of Western Ontario in Canada and the Centre de Recherche en Astrophysique de Lyon in France, and also aided by other meteor research colleagues from NASA's Marshall Space Flight Center, scientists on the rover team planned some observations to try to detect predicted meteor storms in October and November, 2005. The views shown here are a composite of nine 60-second exposures taken with the panoramic camera on Spirit during night hours of sol 668 (Nov. 18, 2005), during a week when Mars was predicted to pass through a meteor stream associated with Halley's comet. The south celestial pole is at the center of the frame. Many stars can be seen in the images, appearing as short, curved streaks forming arcs around the center point. The star trails are curved because Mars is rotating while the camera takes the images. The brightest stars in this view would be easily visible to the naked eye, but the faintest ones are slightly dimmer than the human eye can detect. In addition to the star trails, there are several smaller linear streaks, dots and splotches that are the trails left by cosmic rays hitting the camera detectors. Cosmic rays are high-energy particles that are created in the Sun and in other stars throughout our galaxy and travel, through space in all directions. Some of them strike Earth or other planets, and ones that strike a digital camera detector can leave little tracks or splotches like those seen in these images. Because they come from all directions, some strike the detector face-on, and others strike at glancing angles. Some even skip across the detector like flat rocks skipped across a pond. These are very common phenomena to astronomers used to working with sensitive digital cameras like those in the Mars rovers, the Hubble Space Telescope, or other space probes, and while they can be a nuisance when taking pictures, they generally do not cause any lasting damage to the cameras. Three of the streaks in the image, including one spanning most of the distance from the left edge of the frame to the center, might be meteor trails or could be the marks of other cosmic rays. While hunting for meteors on Mars is fun, ultimately the team wants to use the images and results for scientific purposes. These include helping to validate the models and predictions for interplanetary meteor storms, providing information on the rate of impacts of small meteoroids with Mars for comparison with rates for the Earth and Moon, assessing the rate and intensity of cosmic ray impact events in the Martian environment, and looking at whether some bright stars are being dimmed occasionally by water ice or dust clouds occurring at night during different Martian seasons. |
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Meteor Search by Spirit, Sol
…
PIA03615
Sol (our sun)
Panoramic Camera
| Title |
Meteor Search by Spirit, Sol 668 |
| Original Caption Released with Image |
Annotated Meteor Search by Spirit, Sol 668 The panoramic cameras on NASA's Mars Exploration Rovers are about as sensitive as the human eye at night. The cameras can see the same bright stars that we can see from Earth, and the same patterns of constellations dot the night sky. Scientists on the rover team have been taking images of some of these bright stars as part of several different projects. One project is designed to try to capture "shooting stars," or meteors, in the martian night sky. "Meteoroids" are small pieces of comets and asteroids that travel through space and eventually run into a planet. On Earth, we can sometimes see meteoroids become brilliant, long "meteors" streaking across the night sky as they burn up from the friction in our atmosphere. Some of these meteors survive their fiery flight and land on the surface (or in the ocean) where, if found, they are called "meteorites." The same thing happens in the martian atmosphere, and Spirit even accidentally discovered a meteor while attempting to obtain images of Earth in the pre-dawn sky back in March, 2004 (see http://marsrovers.jpl.nasa.gov/gallery/press/spirit/20040311a.html, and Selsis et al. (2005) Nature, vol 435, p. 581). On Earth, some meteors come in "storms" or "showers" at predictable times of the year, like the famous Perseid meteor shower in August or the Leonid meteor shower in November. These "storms" happen when Earth passes through the same parts of space where comets sometimes pass. The meteors we see at these times are from leftover debris that was shed off of these comets. The same kind of thing is predicted for Mars, as well. Inspired by calculations about Martian meteor storms by meteor scientists from the University of Western Ontario in Canada and the Centre de Recherche en Astrophysique de Lyon in France, and also aided by other meteor research colleagues from NASA's Marshall Space Flight Center, scientists on the rover team planned some observations to try to detect predicted meteor storms in October and November, 2005. The views shown here are a composite of nine 60-second exposures taken with the panoramic camera on Spirit during night hours of sol 668 (Nov. 18, 2005), during a week when Mars was predicted to pass through a meteor stream associated with Halley's comet. The south celestial pole is at the center of the frame. Many stars can be seen in the images, appearing as short, curved streaks forming arcs around the center point. The star trails are curved because Mars is rotating while the camera takes the images. The brightest stars in this view would be easily visible to the naked eye, but the faintest ones are slightly dimmer than the human eye can detect. In addition to the star trails, there are several smaller linear streaks, dots and splotches that are the trails left by cosmic rays hitting the camera detectors. Cosmic rays are high-energy particles that are created in the Sun and in other stars throughout our galaxy and travel, through space in all directions. Some of them strike Earth or other planets, and ones that strike a digital camera detector can leave little tracks or splotches like those seen in these images. Because they come from all directions, some strike the detector face-on, and others strike at glancing angles. Some even skip across the detector like flat rocks skipped across a pond. These are very common phenomena to astronomers used to working with sensitive digital cameras like those in the Mars rovers, the Hubble Space Telescope, or other space probes, and while they can be a nuisance when taking pictures, they generally do not cause any lasting damage to the cameras. Three of the streaks in the image, including one spanning most of the distance from the left edge of the frame to the center, might be meteor trails or could be the marks of other cosmic rays. While hunting for meteors on Mars is fun, ultimately the team wants to use the images and results for scientific purposes. These include helping to validate the models and predictions for interplanetary meteor storms, providing information on the rate of impacts of small meteoroids with Mars for comparison with rates for the Earth and Moon, assessing the rate and intensity of cosmic ray impact events in the Martian environment, and looking at whether some bright stars are being dimmed occasionally by water ice or dust clouds occurring at night during different Martian seasons. |
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KENNEDY SPACE CENTER, FLA. -
…
| Description |
KENNEDY SPACE CENTER, FLA. - In the pre-dawn hours on Launch Pad 17-B at Cape Canaveral Air Force Station, the mobile service tower is silhouetted with the Boeing Delta II rocket that will launch NASA?s Deep Impact spacecraft. The Delta II waits for the arrival and mating of the second stage. A NASA Discovery mission, Deep Impact will probe beneath the surface of Comet Tempel 1 on July 4, 2005, when the comet is 83 million miles from Earth, and reveal the secrets of its interior. After releasing an impactor on a course to hit the comet?s sunlit side, Deep Impact?s flyby spacecraft will collect pictures and data of how the crater forms, measure the crater?s depth and diameter, as well as the composition of the interior of the crater and any material thrown out, and determine the changes in natural outgassing produced by the impact. It will send the data back to Earth through the antennas of the Deep Space Network. |
| Release Date |
12/03/2004 |
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