|
|
Final RTF SSME test at A2 te
…
The Space Shuttle's Main Eng
…
8/19/04
| Description |
The Space Shuttle's Main Engine (SSME) reached another milestone Aug. 19, 2004, when a successful flight acceptance test was conducted at NASA Stennis Space Center (SSC). The engine tested was the final of three engines that will carry the next Space Shuttle into orbit. The engine will be shipped to NASA Kennedy Space Center in Florida for installation on Space Shuttle Discovery for STS-114, NASA's Return to Flight mission. The engine test, which began about 8:10 p.m. CDT, ran for 520 seconds (8 minutes), the length of time it takes for the Space Shuttle to reach orbit. |
| Date |
8/19/04 |
|
Galaxies Gather at Great Dis
…
| Title |
Galaxies Gather at Great Distances |
| Description |
Astronomers have discovered nearly 300 galaxy clusters and groups, including almost 100 located 8 to 10 billion light-years away, using the space-based Spitzer Space Telescope and the ground-based Mayall 4-meter telescope at Kitt Peak National Observatory in Tucson, Ariz. The new sample represents a six-fold increase in the number of known galaxy clusters and groups at such extreme distances, and will allow astronomers to systematically study massive galaxies two-thirds of the way back to the Big Bang. A mosaic portraying a bird's eye view of the field in which the distant clusters were found is shown at upper left. It spans a region of sky 40 times larger than that covered by the full moon as seen from Earth. Thousands of individual images from Spitzer's infrared array camera instrument were stitched together to create this mosaic. The distant clusters are marked with orange dots. Close-up images of three of the distant galaxy clusters are shown in the adjoining panels. The clusters appear as a concentration of red dots near the center of each image. These images reveal the galaxies as they were over 8 billion years ago, since that's how long their light took to reach Earth and Spitzer's infrared eyes. These pictures are false-color composites, combining ground-based optical images captured by the Mosaic-I camera on the Mayall 4-meter telescope at Kitt Peak, with infrared pictures taken by Spitzer's infrared array camera. Blue and green represent visible light at wavelengths of 0.4 microns and 0.8 microns, respectively, while red indicates infrared light at 4.5 microns. Kitt Peak National Observatory is part of the National Optical Astronomy Observatory in Tuscon, Ariz. |
|
Galaxies Gather at Great Dis
…
| Title |
Galaxies Gather at Great Distances |
| Description |
Astronomers have discovered nearly 300 galaxy clusters and groups, including almost 100 located 8 to 10 billion light-years away, using the space-based Spitzer Space Telescope and the ground-based Mayall 4-meter telescope at Kitt Peak National Observatory in Tucson, Ariz. The new sample represents a six-fold increase in the number of known galaxy clusters and groups at such extreme distances, and will allow astronomers to systematically study massive galaxies two-thirds of the way back to the Big Bang. A mosaic portraying a bird's eye view of the field in which the distant clusters were found is shown at upper left. It spans a region of sky 40 times larger than that covered by the full moon as seen from Earth. Thousands of individual images from Spitzer's infrared array camera instrument were stitched together to create this mosaic. The distant clusters are marked with orange dots. Close-up images of three of the distant galaxy clusters are shown in the adjoining panels. The clusters appear as a concentration of red dots near the center of each image. These images reveal the galaxies as they were over 8 billion years ago, since that's how long their light took to reach Earth and Spitzer's infrared eyes. These pictures are false-color composites, combining ground-based optical images captured by the Mosaic-I camera on the Mayall 4-meter telescope at Kitt Peak, with infrared pictures taken by Spitzer's infrared array camera. Blue and green represent visible light at wavelengths of 0.4 microns and 0.8 microns, respectively, while red indicates infrared light at 4.5 microns. Kitt Peak National Observatory is part of the National Optical Astronomy Observatory in Tuscon, Ariz. |
|
Galaxies Gather at Great Dis
…
| Title |
Galaxies Gather at Great Distances |
| Description |
Astronomers have discovered nearly 300 galaxy clusters and groups, including almost 100 located 8 to 10 billion light-years away, using the space-based Spitzer Space Telescope and the ground-based Mayall 4-meter telescope at Kitt Peak National Observatory in Tucson, Ariz. The new sample represents a six-fold increase in the number of known galaxy clusters and groups at such extreme distances, and will allow astronomers to systematically study massive galaxies two-thirds of the way back to the Big Bang. A mosaic portraying a bird's eye view of the field in which the distant clusters were found is shown at upper left. It spans a region of sky 40 times larger than that covered by the full moon as seen from Earth. Thousands of individual images from Spitzer's infrared array camera instrument were stitched together to create this mosaic. The distant clusters are marked with orange dots. Close-up images of three of the distant galaxy clusters are shown in the adjoining panels. The clusters appear as a concentration of red dots near the center of each image. These images reveal the galaxies as they were over 8 billion years ago, since that's how long their light took to reach Earth and Spitzer's infrared eyes. These pictures are false-color composites, combining ground-based optical images captured by the Mosaic-I camera on the Mayall 4-meter telescope at Kitt Peak, with infrared pictures taken by Spitzer's infrared array camera. Blue and green represent visible light at wavelengths of 0.4 microns and 0.8 microns, respectively, while red indicates infrared light at 4.5 microns. Kitt Peak National Observatory is part of the National Optical Astronomy Observatory in Tuscon, Ariz. |
|
Galaxies Gather at Great Dis
…
| Title |
Galaxies Gather at Great Distances |
| Description |
Astronomers have discovered nearly 300 galaxy clusters and groups, including almost 100 located 8 to 10 billion light-years away, using the space-based Spitzer Space Telescope and the ground-based Mayall 4-meter telescope at Kitt Peak National Observatory in Tucson, Ariz. The new sample represents a six-fold increase in the number of known galaxy clusters and groups at such extreme distances, and will allow astronomers to systematically study massive galaxies two-thirds of the way back to the Big Bang. A mosaic portraying a bird's eye view of the field in which the distant clusters were found is shown at upper left. It spans a region of sky 40 times larger than that covered by the full moon as seen from Earth. Thousands of individual images from Spitzer's infrared array camera instrument were stitched together to create this mosaic. The distant clusters are marked with orange dots. Close-up images of three of the distant galaxy clusters are shown in the adjoining panels. The clusters appear as a concentration of red dots near the center of each image. These images reveal the galaxies as they were over 8 billion years ago, since that's how long their light took to reach Earth and Spitzer's infrared eyes. These pictures are false-color composites, combining ground-based optical images captured by the Mosaic-I camera on the Mayall 4-meter telescope at Kitt Peak, with infrared pictures taken by Spitzer's infrared array camera. Blue and green represent visible light at wavelengths of 0.4 microns and 0.8 microns, respectively, while red indicates infrared light at 4.5 microns. Kitt Peak National Observatory is part of the National Optical Astronomy Observatory in Tuscon, Ariz. |
|
Galaxies Gather at Great Dis
…
| Title |
Galaxies Gather at Great Distances |
| Description |
Astronomers have discovered nearly 300 galaxy clusters and groups, including almost 100 located 8 to 10 billion light-years away, using the space-based Spitzer Space Telescope and the ground-based Mayall 4-meter telescope at Kitt Peak National Observatory in Tucson, Ariz. The new sample represents a six-fold increase in the number of known galaxy clusters and groups at such extreme distances, and will allow astronomers to systematically study massive galaxies two-thirds of the way back to the Big Bang. A mosaic portraying a bird's eye view of the field in which the distant clusters were found is shown at upper left. It spans a region of sky 40 times larger than that covered by the full moon as seen from Earth. Thousands of individual images from Spitzer's infrared array camera instrument were stitched together to create this mosaic. The distant clusters are marked with orange dots. Close-up images of three of the distant galaxy clusters are shown in the adjoining panels. The clusters appear as a concentration of red dots near the center of each image. These images reveal the galaxies as they were over 8 billion years ago, since that's how long their light took to reach Earth and Spitzer's infrared eyes. These pictures are false-color composites, combining ground-based optical images captured by the Mosaic-I camera on the Mayall 4-meter telescope at Kitt Peak, with infrared pictures taken by Spitzer's infrared array camera. Blue and green represent visible light at wavelengths of 0.4 microns and 0.8 microns, respectively, while red indicates infrared light at 4.5 microns. Kitt Peak National Observatory is part of the National Optical Astronomy Observatory in Tuscon, Ariz. |
|
Galaxies Gather at Great Dis
…
| Title |
Galaxies Gather at Great Distances |
| Description |
Astronomers have discovered nearly 300 galaxy clusters and groups, including almost 100 located 8 to 10 billion light-years away, using the space-based Spitzer Space Telescope and the ground-based Mayall 4-meter telescope at Kitt Peak National Observatory in Tucson, Ariz. The new sample represents a six-fold increase in the number of known galaxy clusters and groups at such extreme distances, and will allow astronomers to systematically study massive galaxies two-thirds of the way back to the Big Bang. A mosaic portraying a bird's eye view of the field in which the distant clusters were found is shown at upper left. It spans a region of sky 40 times larger than that covered by the full moon as seen from Earth. Thousands of individual images from Spitzer's infrared array camera instrument were stitched together to create this mosaic. The distant clusters are marked with orange dots. Close-up images of three of the distant galaxy clusters are shown in the adjoining panels. The clusters appear as a concentration of red dots near the center of each image. These images reveal the galaxies as they were over 8 billion years ago, since that's how long their light took to reach Earth and Spitzer's infrared eyes. These pictures are false-color composites, combining ground-based optical images captured by the Mosaic-I camera on the Mayall 4-meter telescope at Kitt Peak, with infrared pictures taken by Spitzer's infrared array camera. Blue and green represent visible light at wavelengths of 0.4 microns and 0.8 microns, respectively, while red indicates infrared light at 4.5 microns. Kitt Peak National Observatory is part of the National Optical Astronomy Observatory in Tuscon, Ariz. |
|
Great Galactic Buddies
| Title |
Great Galactic Buddies |
| Description |
Like great friends, galaxies stick together. Astronomers using NASA's Spitzer Space Telescope have spotted a handful of great galactic pals bonding back when the universe was a mere 4.6 billion years old. The universe is believed to be 13.7 billion years old. Collectively, these great galactic buddies are called galaxy clusters. A typical galaxy cluster can contain hundreds of galaxies and trillions of stars. In this false-color composite, some of the oldest galaxy clusters in the universe pose for Spitzer's Infrared Array Camera. The individual galaxies that make up the distant clusters are shown as red dots in all four images. The green blobs are Milky Way stars along the line of sight, and the blue specks are faint galaxies at various distances along the line of sight. The green and blue data are from a visible-light, ground-based telescope. The cluster at 9.1 billion light-years away (lower right panel) is currently the most distant galaxy cluster ever detected. These images are three-color composites, in which blue represents visible light with a wavelength of 0.4 microns, and green indicates visible light of 0.8 microns. The visible data were captured by the ground-based Mosaic-1 camera at the Kitt Peak National Observatory in Tucson, Ariz. Red represents infrared light of 4.5 microns, captured by Spitzer's infrared array camera. |
|
Great Galactic Buddies
| Title |
Great Galactic Buddies |
| Description |
Like great friends, galaxies stick together. Astronomers using NASA's Spitzer Space Telescope have spotted a handful of great galactic pals bonding back when the universe was a mere 4.6 billion years old. The universe is believed to be 13.7 billion years old. Collectively, these great galactic buddies are called galaxy clusters. A typical galaxy cluster can contain hundreds of galaxies and trillions of stars. In this false-color composite, some of the oldest galaxy clusters in the universe pose for Spitzer's Infrared Array Camera. The individual galaxies that make up the distant clusters are shown as red dots in all four images. The green blobs are Milky Way stars along the line of sight, and the blue specks are faint galaxies at various distances along the line of sight. The green and blue data are from a visible-light, ground-based telescope. The cluster at 9.1 billion light-years away (lower right panel) is currently the most distant galaxy cluster ever detected. These images are three-color composites, in which blue represents visible light with a wavelength of 0.4 microns, and green indicates visible light of 0.8 microns. The visible data were captured by the ground-based Mosaic-1 camera at the Kitt Peak National Observatory in Tucson, Ariz. Red represents infrared light of 4.5 microns, captured by Spitzer's infrared array camera. |
|
Great Galactic Buddies
| Title |
Great Galactic Buddies |
| Description |
Like great friends, galaxies stick together. Astronomers using NASA's Spitzer Space Telescope have spotted a handful of great galactic pals bonding back when the universe was a mere 4.6 billion years old. The universe is believed to be 13.7 billion years old. Collectively, these great galactic buddies are called galaxy clusters. A typical galaxy cluster can contain hundreds of galaxies and trillions of stars. In this false-color composite, some of the oldest galaxy clusters in the universe pose for Spitzer's Infrared Array Camera. The individual galaxies that make up the distant clusters are shown as red dots in all four images. The green blobs are Milky Way stars along the line of sight, and the blue specks are faint galaxies at various distances along the line of sight. The green and blue data are from a visible-light, ground-based telescope. The cluster at 9.1 billion light-years away (lower right panel) is currently the most distant galaxy cluster ever detected. These images are three-color composites, in which blue represents visible light with a wavelength of 0.4 microns, and green indicates visible light of 0.8 microns. The visible data were captured by the ground-based Mosaic-1 camera at the Kitt Peak National Observatory in Tucson, Ariz. Red represents infrared light of 4.5 microns, captured by Spitzer's infrared array camera. |
|
Great Galactic Buddies
| Title |
Great Galactic Buddies |
| Description |
Like great friends, galaxies stick together. Astronomers using NASA's Spitzer Space Telescope have spotted a handful of great galactic pals bonding back when the universe was a mere 4.6 billion years old. The universe is believed to be 13.7 billion years old. Collectively, these great galactic buddies are called galaxy clusters. A typical galaxy cluster can contain hundreds of galaxies and trillions of stars. In this false-color composite, some of the oldest galaxy clusters in the universe pose for Spitzer's Infrared Array Camera. The individual galaxies that make up the distant clusters are shown as red dots in all four images. The green blobs are Milky Way stars along the line of sight, and the blue specks are faint galaxies at various distances along the line of sight. The green and blue data are from a visible-light, ground-based telescope. The cluster at 9.1 billion light-years away (lower right panel) is currently the most distant galaxy cluster ever detected. These images are three-color composites, in which blue represents visible light with a wavelength of 0.4 microns, and green indicates visible light of 0.8 microns. The visible data were captured by the ground-based Mosaic-1 camera at the Kitt Peak National Observatory in Tucson, Ariz. Red represents infrared light of 4.5 microns, captured by Spitzer's infrared array camera. |
|
Great Galactic Buddies
| Title |
Great Galactic Buddies |
| Description |
Like great friends, galaxies stick together. Astronomers using NASA's Spitzer Space Telescope have spotted a handful of great galactic pals bonding back when the universe was a mere 4.6 billion years old. The universe is believed to be 13.7 billion years old. Collectively, these great galactic buddies are called galaxy clusters. A typical galaxy cluster can contain hundreds of galaxies and trillions of stars. In this false-color composite, some of the oldest galaxy clusters in the universe pose for Spitzer's Infrared Array Camera. The individual galaxies that make up the distant clusters are shown as red dots in all four images. The green blobs are Milky Way stars along the line of sight, and the blue specks are faint galaxies at various distances along the line of sight. The green and blue data are from a visible-light, ground-based telescope. The cluster at 9.1 billion light-years away (lower right panel) is currently the most distant galaxy cluster ever detected. These images are three-color composites, in which blue represents visible light with a wavelength of 0.4 microns, and green indicates visible light of 0.8 microns. The visible data were captured by the ground-based Mosaic-1 camera at the Kitt Peak National Observatory in Tucson, Ariz. Red represents infrared light of 4.5 microns, captured by Spitzer's infrared array camera. |
|
Leaving Earth
| title |
Leaving Earth |
| date |
06.10.2003 |
| description |
This spectacular shot of solid rocket motors separating from a Delta II rocket over Florida was captured during the June 10 liftoff of the Mars Exploration Rover, Spirit. The rover and its twin, Opportunity, will arrive at Mars in January 2004. |
|
Hurricane Charley Hammers Fl
…
| title |
Hurricane Charley Hammers Florida |
| date |
08.13.2004 |
| description |
Hurricane Charley makes landfall at 3:45 p.m. (EDT) on Friday, Aug. 13. Maximum sustained winds were near 140 mph with higher gusts. Hurricane force winds extended outward up to 25 miles from the center, and tropical storm force winds extend outward up to 85 miles. The storm cut a swatch across the state. *Image Credit*: NOAA |
|
Inspecting Cassini's nuclear
…
| Title |
Inspecting Cassini's nuclear power source |
| Full Description |
Environmental Health Specialist Jamie A. Keeley of EG&G Florida Inc., KSC's base operations contractor, uses an ion chamber dose rate meter to measure radiation levels in one of the three radioisotope thermoelectric generators (RTGs) that will provide electrical power to the Cassini spacecraft. Technicians tested and monitored four RTGs, including one spare, in the Radioisotope Thermoelectric Generator Storage building in KSC's Industrial Area. The RTGs use heat from the natural decay of plutonium to generate electric power. This nuclear powered system enables the spacecraft to operate far from the Sun, where solar power systems are not feasible. Similar RTGs powered the Galileo and Ulysses spacecraft. A close-up study of Saturn and its moons, the Cassini/Huygens mission launched from Cape Canaveral Air Station in October 1997 and reached the Saturnian system in July 2004 for four years of observation. Scientific instruments carried aboard the Cassini orbiter will study Saturn's atmosphere, magnetic field, rings, and several moons, while the Huygens probe will separate and land on the surface of Titan, Saturn's largest moon. The Cassini-Huygens mission owes its name to the Dutch astronomer Christiaan Huygens and Italian astronomer Giovanni Domenico Cassini. Both had spectacular careers as observers of the heavens, which included important discoveries about Saturn and its satellites. Huygens (1629-1695) discovered Saturn's largest moon, Titan, in 1655 and in 1656 described the shape and phase changes of Saturn's rings. Cassini (1625-1712) was the first to observe four of Saturn's moons, Iapetus, Rhea, Tethys, and Dione, in the 1670s and 1680s. He also, in 1675, discovered the gap in Saturn's rings, now called the Cassini Division, and proposed that the rings were formed from many tiny particles. Cassini-Huygens is a joint mission of NASA, the European Space Agency (ESA), and the Italian Space Agency, Agenzia Spaziale Italiana (ASI). JPL is managing the Cassini project for NASA. The mission was proposed in November 1982 by a group of European and American scientists from the European Science Foundation and the National Academy of Sciences. The Solar System Exploration Committee of the NASA Advisory Council endorsed the idea in April 1983, and NASA and ESA began a joint assessment study in 1984. ESA officially adopted the project in November 1988, and Congress approved funding for NASA's portion of the mission in FY 89. |
| Date |
06/17/1997 |
| NASA Center |
Kennedy Space Center |
|
NASA Finds Direct Proof of D
…
| Title |
NASA Finds Direct Proof of Dark Matter |
| General Information |
What is a News Nugget? News Nuggets are bulletins from the world of astronomy. Dark matter and normal matter have been wrenched apart by the tremendous collision of two large clusters of galaxies. This composite image shows the galaxy cluster 1E 0657-56, also known as the "bullet cluster." The hot gas detected by Chandra in X-rays is seen as two pink clumps in the image and contains most of the "normal" matter in the two clusters. The bullet-shaped clump on the right is the hot gas from one cluster, which passed through the hot gas from the other larger cluster during the collision. An optical image from Magellan and the Hubble Space Telescope shows the galaxies in orange and white. The blue areas in this image show where astronomers find most of the mass in the clusters. For more information about this research on the Web, visit: http://chandra.harvard.edu/press/06_releases/press_082106.html [ http://chandra.harvard.edu/press/06_releases/press_082106.html ] |
|
Hurricane Jeanne on Septembe
…
| Title |
Hurricane Jeanne on September 23, 2004 |
| Abstract |
After days of hammering Haiti, Hurricane Jeanne heads toward the United States. |
| Completed |
2004-09-24 |
|
TRMM Tropical Microwave Imag
…
| Title |
TRMM Tropical Microwave Imager (TMI) sees the power of Hurricane Jeanne On September 25, 2004 |
| Abstract |
NASA's TRMM spacecraft is used by meteorologists to understand Hurricane Jeanne. TRMM saw this view of Hurricane Jeanne on September 25, 2004, just before it made landfall. The cloud cover is taken by TRMM's Visible and Infrared Scanner (VIRS). It looks underneath of the storm's clouds to reveal the underlying rain structure. Blue represents areas with at least 0.25 inches of rain per hour. Green shows at least 0.5 inches of rain per hour. Yellow is at least 1.0 inches of rain and red is at least 2.0 inches of rain per hour. |
| Completed |
2004-09-30 |
|
TRMM Tropical Microwave Imag
…
| Title |
TRMM Tropical Microwave Imager (TMI) sees the power of Hurricane Jeanne On September 25, 2004 |
| Abstract |
NASA's TRMM spacecraft is used by meteorologists to understand Hurricane Jeanne. TRMM saw this view of Hurricane Jeanne on September 25, 2004, just before it made landfall. The cloud cover is taken by TRMM's Visible and Infrared Scanner (VIRS). It looks underneath of the storm's clouds to reveal the underlying rain structure. Blue represents areas with at least 0.25 inches of rain per hour. Green shows at least 0.5 inches of rain per hour. Yellow is at least 1.0 inches of rain and red is at least 2.0 inches of rain per hour. |
| Completed |
2004-09-30 |
|
TRMM Tropical Microwave Imag
…
| Title |
TRMM Tropical Microwave Imager (TMI) sees the power of Hurricane Jeanne On September 25, 2004 |
| Abstract |
NASA's TRMM spacecraft is used by meteorologists to understand Hurricane Jeanne. TRMM saw this view of Hurricane Jeanne on September 25, 2004, just before it made landfall. The cloud cover is taken by TRMM's Visible and Infrared Scanner (VIRS). It looks underneath of the storm's clouds to reveal the underlying rain structure. Blue represents areas with at least 0.25 inches of rain per hour. Green shows at least 0.5 inches of rain per hour. Yellow is at least 1.0 inches of rain and red is at least 2.0 inches of rain per hour. |
| Completed |
2004-09-30 |
|
TRMM Tropical Microwave Imag
…
| Title |
TRMM Tropical Microwave Imager (TMI) sees the power of Hurricane Jeanne On September 25, 2004 |
| Abstract |
NASA's TRMM spacecraft is used by meteorologists to understand Hurricane Jeanne. TRMM saw this view of Hurricane Jeanne on September 25, 2004, just before it made landfall. The cloud cover is taken by TRMM's Visible and Infrared Scanner (VIRS). It looks underneath of the storm's clouds to reveal the underlying rain structure. Blue represents areas with at least 0.25 inches of rain per hour. Green shows at least 0.5 inches of rain per hour. Yellow is at least 1.0 inches of rain and red is at least 2.0 inches of rain per hour. |
| Completed |
2004-09-30 |
|
TRMM Tropical Microwave Imag
…
| Title |
TRMM Tropical Microwave Imager (TMI) sees the power of Hurricane Jeanne On September 25, 2004 |
| Abstract |
NASA's TRMM spacecraft is used by meteorologists to understand Hurricane Jeanne. TRMM saw this view of Hurricane Jeanne on September 25, 2004, just before it made landfall. The cloud cover is taken by TRMM's Visible and Infrared Scanner (VIRS). It looks underneath of the storm's clouds to reveal the underlying rain structure. Blue represents areas with at least 0.25 inches of rain per hour. Green shows at least 0.5 inches of rain per hour. Yellow is at least 1.0 inches of rain and red is at least 2.0 inches of rain per hour. |
| Completed |
2004-09-30 |
|
TRMM Tropical Microwave Imag
…
| Title |
TRMM Tropical Microwave Imager (TMI) sees the power of Hurricane Jeanne On September 25, 2004 |
| Abstract |
NASA's TRMM spacecraft is used by meteorologists to understand Hurricane Jeanne. TRMM saw this view of Hurricane Jeanne on September 25, 2004, just before it made landfall. The cloud cover is taken by TRMM's Visible and Infrared Scanner (VIRS). It looks underneath of the storm's clouds to reveal the underlying rain structure. Blue represents areas with at least 0.25 inches of rain per hour. Green shows at least 0.5 inches of rain per hour. Yellow is at least 1.0 inches of rain and red is at least 2.0 inches of rain per hour. |
| Completed |
2004-09-30 |
|
Hurricane Frances Progressio
…
| Title |
Hurricane Frances Progression with Fixed View |
| Abstract |
Hurricane Frances races towards Florida and both the Terra and Aqua satellite are spectators. |
| Completed |
2004-09-03 |
|
Hurricane Frances Progressio
…
| Title |
Hurricane Frances Progression with Fixed View |
| Abstract |
Hurricane Frances races towards Florida and both the Terra and Aqua satellite are spectators. |
| Completed |
2004-09-03 |
|
Hurricane Frances Progressio
…
| Title |
Hurricane Frances Progression with Fixed View |
| Abstract |
Hurricane Frances races towards Florida and both the Terra and Aqua satellite are spectators. |
| Completed |
2004-09-03 |
|
Hurricane Frances Progressio
…
| Title |
Hurricane Frances Progression with Fixed View |
| Abstract |
Hurricane Frances races towards Florida and both the Terra and Aqua satellite are spectators. |
| Completed |
2004-09-03 |
|
Hurricane Frances Progressio
…
| Title |
Hurricane Frances Progression with Fixed View |
| Abstract |
Hurricane Frances races towards Florida and both the Terra and Aqua satellite are spectators. |
| Completed |
2004-09-03 |
|
Hurricane Frances Progressio
…
| Title |
Hurricane Frances Progression with Fixed View |
| Abstract |
Hurricane Frances races towards Florida and both the Terra and Aqua satellite are spectators. |
| Completed |
2004-09-03 |
|
Hurricane Frances Progressio
…
| Title |
Hurricane Frances Progression with a Fixed View |
| Abstract |
A fixed view of the Atlantic Ocean with Hurricane Frances sprinting towards Florida |
| Completed |
2004-09-07 |
|
Hurricane Frances Progressio
…
| Title |
Hurricane Frances Progression with a Fixed View |
| Abstract |
A fixed view of the Atlantic Ocean with Hurricane Frances sprinting towards Florida |
| Completed |
2004-09-07 |
|
Hurricane Frances Progressio
…
| Title |
Hurricane Frances Progression with a Fixed View |
| Abstract |
A fixed view of the Atlantic Ocean with Hurricane Frances sprinting towards Florida |
| Completed |
2004-09-07 |
|
Hurricane Frances Progressio
…
| Title |
Hurricane Frances Progression with a Fixed View |
| Abstract |
A fixed view of the Atlantic Ocean with Hurricane Frances sprinting towards Florida |
| Completed |
2004-09-07 |
|
Hurricane Frances Progressio
…
| Title |
Hurricane Frances Progression with a Fixed View |
| Abstract |
A fixed view of the Atlantic Ocean with Hurricane Frances sprinting towards Florida |
| Completed |
2004-09-07 |
|
Hurricane Frances Progressio
…
| Title |
Hurricane Frances Progression with a Fixed View |
| Abstract |
A fixed view of the Atlantic Ocean with Hurricane Frances sprinting towards Florida |
| Completed |
2004-09-07 |
|
Hurricane Frances Progressio
…
| Title |
Hurricane Frances Progression with a Fixed View |
| Abstract |
A fixed view of the Atlantic Ocean with Hurricane Frances sprinting towards Florida |
| Completed |
2004-09-07 |
|
Hurricane Frances Progressio
…
| Title |
Hurricane Frances Progression with a Fixed View |
| Abstract |
A fixed view of the Atlantic Ocean with Hurricane Frances sprinting towards Florida |
| Completed |
2004-09-07 |
|
Hurricane Frances Progressio
…
| Title |
Hurricane Frances Progression with a Fixed View |
| Abstract |
A fixed view of the Atlantic Ocean with Hurricane Frances sprinting towards Florida |
| Completed |
2004-09-07 |
|
Hurricane Dennis
| Title |
Hurricane Dennis |
| Abstract |
The formation of Hurricane Dennis on July 5 made that the earliest date on record that four named storms formed in the Atlantic basin. Dennis proved to be a powerful and destructive storm in the Caribbean Sea and the Gulf of Mexico. It crossed over Cuba on July 8 and 9, leaving at least 10 dead, and caused additional deaths in Haiti. After re-emerging over open water, Dennis re-strengthened into a dangerous Category 4 hurricane with top wind speeds of 233 kilometers per hour (145 mph). The storm passed within 90 kilometers (55 miles) of Pensacola, Florida, and hit land about 80 kilometers (50 miles) east of where Hurricane Ivan struck in September, 2004. A large storm surge of more than 10 feet was created in certain areas, and many homes and businesses in low-lying areas were flooded. |
| Completed |
2005-07-11 |
|
Hurricane Dennis
| Title |
Hurricane Dennis |
| Abstract |
The formation of Hurricane Dennis on July 5 made that the earliest date on record that four named storms formed in the Atlantic basin. Dennis proved to be a powerful and destructive storm in the Caribbean Sea and the Gulf of Mexico. It crossed over Cuba on July 8 and 9, leaving at least 10 dead, and caused additional deaths in Haiti. After re-emerging over open water, Dennis re-strengthened into a dangerous Category 4 hurricane with top wind speeds of 233 kilometers per hour (145 mph). The storm passed within 90 kilometers (55 miles) of Pensacola, Florida, and hit land about 80 kilometers (50 miles) east of where Hurricane Ivan struck in September, 2004. A large storm surge of more than 10 feet was created in certain areas, and many homes and businesses in low-lying areas were flooded. |
| Completed |
2005-07-11 |
|
Hurricane Dennis
| Title |
Hurricane Dennis |
| Abstract |
The formation of Hurricane Dennis on July 5 made that the earliest date on record that four named storms formed in the Atlantic basin. Dennis proved to be a powerful and destructive storm in the Caribbean Sea and the Gulf of Mexico. It crossed over Cuba on July 8 and 9, leaving at least 10 dead, and caused additional deaths in Haiti. After re-emerging over open water, Dennis re-strengthened into a dangerous Category 4 hurricane with top wind speeds of 233 kilometers per hour (145 mph). The storm passed within 90 kilometers (55 miles) of Pensacola, Florida, and hit land about 80 kilometers (50 miles) east of where Hurricane Ivan struck in September, 2004. A large storm surge of more than 10 feet was created in certain areas, and many homes and businesses in low-lying areas were flooded. |
| Completed |
2005-07-11 |
|
Hurricane Dennis
| Title |
Hurricane Dennis |
| Abstract |
The formation of Hurricane Dennis on July 5 made that the earliest date on record that four named storms formed in the Atlantic basin. Dennis proved to be a powerful and destructive storm in the Caribbean Sea and the Gulf of Mexico. It crossed over Cuba on July 8 and 9, leaving at least 10 dead, and caused additional deaths in Haiti. After re-emerging over open water, Dennis re-strengthened into a dangerous Category 4 hurricane with top wind speeds of 233 kilometers per hour (145 mph). The storm passed within 90 kilometers (55 miles) of Pensacola, Florida, and hit land about 80 kilometers (50 miles) east of where Hurricane Ivan struck in September, 2004. A large storm surge of more than 10 feet was created in certain areas, and many homes and businesses in low-lying areas were flooded. |
| Completed |
2005-07-11 |
|
Hurricane Dennis
| Title |
Hurricane Dennis |
| Abstract |
The formation of Hurricane Dennis on July 5 made that the earliest date on record that four named storms formed in the Atlantic basin. Dennis proved to be a powerful and destructive storm in the Caribbean Sea and the Gulf of Mexico. It crossed over Cuba on July 8 and 9, leaving at least 10 dead, and caused additional deaths in Haiti. After re-emerging over open water, Dennis re-strengthened into a dangerous Category 4 hurricane with top wind speeds of 233 kilometers per hour (145 mph). The storm passed within 90 kilometers (55 miles) of Pensacola, Florida, and hit land about 80 kilometers (50 miles) east of where Hurricane Ivan struck in September, 2004. A large storm surge of more than 10 feet was created in certain areas, and many homes and businesses in low-lying areas were flooded. |
| Completed |
2005-07-11 |
|
TRMM Tropical Microwave Imag
…
| Title |
TRMM Tropical Microwave Imager (TMI) sees the power of Hurricane Jeanne On September 26, 2004 |
| Abstract |
NASA's TRMM spacecraft is used by meteorologists to understand It looks underneath of the storm's clouds to reveal the underlying rain structure. Blue represents areas with at least 0.25 inches of rain per hour. Green shows at least 0.5 inches of rain per hour. Yellow is at least 1.0 inches of rain and red is at least 2.0 inches of rain per hour. |
| Completed |
2004-09-27 |
|
TRMM Tropical Microwave Imag
…
| Title |
TRMM Tropical Microwave Imager (TMI) sees the power of Hurricane Jeanne On September 26, 2004 |
| Abstract |
NASA's TRMM spacecraft is used by meteorologists to understand It looks underneath of the storm's clouds to reveal the underlying rain structure. Blue represents areas with at least 0.25 inches of rain per hour. Green shows at least 0.5 inches of rain per hour. Yellow is at least 1.0 inches of rain and red is at least 2.0 inches of rain per hour. |
| Completed |
2004-09-27 |
|
TRMM Tropical Microwave Imag
…
| Title |
TRMM Tropical Microwave Imager (TMI) sees the power of Hurricane Jeanne On September 26, 2004 |
| Abstract |
NASA's TRMM spacecraft is used by meteorologists to understand It looks underneath of the storm's clouds to reveal the underlying rain structure. Blue represents areas with at least 0.25 inches of rain per hour. Green shows at least 0.5 inches of rain per hour. Yellow is at least 1.0 inches of rain and red is at least 2.0 inches of rain per hour. |
| Completed |
2004-09-27 |
|
TRMM Tropical Microwave Imag
…
| Title |
TRMM Tropical Microwave Imager (TMI) sees the power of Hurricane Jeanne On September 26, 2004 |
| Abstract |
NASA's TRMM spacecraft is used by meteorologists to understand It looks underneath of the storm's clouds to reveal the underlying rain structure. Blue represents areas with at least 0.25 inches of rain per hour. Green shows at least 0.5 inches of rain per hour. Yellow is at least 1.0 inches of rain and red is at least 2.0 inches of rain per hour. |
| Completed |
2004-09-27 |
|
TRMM Tropical Microwave Imag
…
| Title |
TRMM Tropical Microwave Imager (TMI) sees the power of Hurricane Jeanne On September 26, 2004 |
| Abstract |
NASA's TRMM spacecraft is used by meteorologists to understand It looks underneath of the storm's clouds to reveal the underlying rain structure. Blue represents areas with at least 0.25 inches of rain per hour. Green shows at least 0.5 inches of rain per hour. Yellow is at least 1.0 inches of rain and red is at least 2.0 inches of rain per hour. |
| Completed |
2004-09-27 |
|
TRMM Tropical Microwave Imag
…
| Title |
TRMM Tropical Microwave Imager (TMI) sees the power of Hurricane Jeanne On September 26, 2004 |
| Abstract |
NASA's TRMM spacecraft is used by meteorologists to understand It looks underneath of the storm's clouds to reveal the underlying rain structure. Blue represents areas with at least 0.25 inches of rain per hour. Green shows at least 0.5 inches of rain per hour. Yellow is at least 1.0 inches of rain and red is at least 2.0 inches of rain per hour. |
| Completed |
2004-09-27 |
|
TRMM Looks at the Rain Fueli
…
| Title |
TRMM Looks at the Rain Fueling Hurricane Ivan on September 15, 2004 |
| Abstract |
NASA's TRMM spacecraft is used by meteorologists to understand Hurricane Ivan. TRMM snapped this view of Hurricane Ivan on September 15, 2004 just before the storm strikes land. The cloud cover is taken by TRMM's Visible and Infrared Scanner (VIRS). The rain structure is taken by TRMM's Precipitation Radar (PR). It looks underneath of the storm's clouds to reveal the underlying rain structure. Blue represents areas with at least 0.25 inches of rain per hour. Green shows at least 0.5 inches of rain per hour. Yellow is at least 1.0 inches of rain and Red is at least 2.0 inches of rain per hour. High vertical bands on the outside of the storm indicated that Hurricane Ivan was very likely to spawn tornados in Florida and Georgia. |
| Completed |
2004-09-15 |
|
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