|
|
Browse All
:
Advanced Communication Technology Satellite (ACTS) from 2005
|
Printer Friendly |
Bending the Rings
| Description |
Saturn's rings appear strangely warped in this view of the rings seen through the upper Saturn atmosphere |
| Full Description |
Saturn's rings appear strangely warped in this view of the rings seen through the upper Saturn atmosphere. The atmosphere acts like a lens in refracting (bending) the light reflected from the rings. As the rings pass behind the overexposed limb (edge) of Saturn as seen from Cassini, the ring structure appears to curve downward due to the bending of the light as it passes through the upper atmosphere. This image was obtained using a near-infrared filter. The filter samples a wavelength where methane gas does not absorb light, thus making the far-off rings visible through the upper atmosphere. By comparing this image to similar ones taken using filters where methane gas does absorb, scientists can estimate the vertical profile of haze and the abundance of methane in Saturn's high atmosphere. The image was taken in visible light with the Cassini spacecraft narrow-angle camera on April 14, 2005, through a filter sensitive to wavelengths of infrared light centered at 938 nanometers and at a distance of approximately 197,000 kilometers (123,000 miles) from Saturn. The image scale is 820 meters (2,680 feet) per pixel. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. For more information about the Cassini-Huygens mission visit http://saturn.jpl.nasa.gov . For additional images visit the Cassini imaging team homepage http://ciclops.org . Credit: NASA/JPL/Space Science Institute |
| Date |
May 25, 2005 |
|
Astronomers Find One of the
…
| Title |
Astronomers Find One of the Youngest and Brightest Galaxies in the Early Universe |
|
2005 Ozone Hole
| Title |
2005 Ozone Hole |
| Description |
The year 2005 marks the twentieth anniversary of the discovery of the ozone hole and the first full year that NASA's Aura satellite has provided detailed images of the hole. Aura was launched in 2004 to monitor the Earth's atmosphere, including the health of the delicate ozone layer. The Ozone Monitoring Instrument on Aura collected the data used to create this image on September 11, 2005, when the ozone hole covered 27 million square kilometers—its peak size for the season. Deep blue shows where ozone levels were low enough to be considered part of the ozone hole. New research shows that the ozone layer may be slower in recovering than previously thought. Ozone is a highly reactive colorless gas that contains three oxygen atoms. Near the surface of the Earth, ozone is hazardous to human health, causing problems like lung irritation, but high in the atmosphere, ozone acts as a crucial shield that absorbs harmful ultraviolet radiation from the Sun. The ozone hole is not an actual hole, but a place in the atmosphere where the protective layer of ozone has worn thin. In 1985, Joseph Farman, Brian Gardiner, and Jonathan Shanklin discovered in the ozone hole over Antarctica. In the following two years, scientists confirmed that human-produced chemicals, chlorofluorocarbons, used in refrigeration and propellant devices, were causing the hole. Chlorofluorocarbons contain high levels of chlorine, which breaks free from the larger molecules in the bitter cold and darkness of Antarctic and Arctic winter. Through a series of chemical reactions, the free chlorine becomes a two-atom molecule of chlorine gas. When sunlight returns, the chlorine gas disintegrates into separate chlorine atoms, which catalyze the destruction of atmospheric ozone. Though the production of chlorofluorocarbons was restricted in 1987, reservoirs of the chemicals in existing refrigerators and air conditioners are still emitting ozone-depleting chemicals into the atmosphere at higher levels than predicted, new measurements show. The extra chemicals may delay the recovery of the ozone hole until about 2065. Previous models predicted a recovery of the ozone layer by 2050. These results were announced on December 6, 2005, at the fall meeting of the American Geophysical Union. To read more, see Ozone Hole: Prospects for Recovery [ http://www.nasa.gov/centers/goddard/news/topstory/2005/ozone_recovery.html ] on the NASA Goddard News web page. To read more about the ozone hole and NASA's mission to study it, check out Ozone Hole Watch [ http://ozonewatch.gsfc.nasa.gov/facts/hole.html ]. The site also contains daily images of the ozone hole as measured by Aura's Ozone Monitoring Instrument. NASA image and animations courtesy GSFC Ozone Processing Team, [ http://toms.gsfc.nasa.gov/ ] based on data provided by the Ozone Monitoring Instrument [ http://www.knmi.nl/omi/publ-en/news/index.html ] (OMI) |
|
2005 Ozone Hole
| Title |
2005 Ozone Hole |
| Description |
The year 2005 marks the twentieth anniversary of the discovery of the ozone hole and the first full year that NASA's Aura satellite has provided detailed images of the hole. Aura was launched in 2004 to monitor the Earth's atmosphere, including the health of the delicate ozone layer. The Ozone Monitoring Instrument on Aura collected the data used to create this image on September 11, 2005, when the ozone hole covered 27 million square kilometers—its peak size for the season. Deep blue shows where ozone levels were low enough to be considered part of the ozone hole. New research shows that the ozone layer may be slower in recovering than previously thought. Ozone is a highly reactive colorless gas that contains three oxygen atoms. Near the surface of the Earth, ozone is hazardous to human health, causing problems like lung irritation, but high in the atmosphere, ozone acts as a crucial shield that absorbs harmful ultraviolet radiation from the Sun. The ozone hole is not an actual hole, but a place in the atmosphere where the protective layer of ozone has worn thin. In 1985, Joseph Farman, Brian Gardiner, and Jonathan Shanklin discovered in the ozone hole over Antarctica. In the following two years, scientists confirmed that human-produced chemicals, chlorofluorocarbons, used in refrigeration and propellant devices, were causing the hole. Chlorofluorocarbons contain high levels of chlorine, which breaks free from the larger molecules in the bitter cold and darkness of Antarctic and Arctic winter. Through a series of chemical reactions, the free chlorine becomes a two-atom molecule of chlorine gas. When sunlight returns, the chlorine gas disintegrates into separate chlorine atoms, which catalyze the destruction of atmospheric ozone. Though the production of chlorofluorocarbons was restricted in 1987, reservoirs of the chemicals in existing refrigerators and air conditioners are still emitting ozone-depleting chemicals into the atmosphere at higher levels than predicted, new measurements show. The extra chemicals may delay the recovery of the ozone hole until about 2065. Previous models predicted a recovery of the ozone layer by 2050. These results were announced on December 6, 2005, at the fall meeting of the American Geophysical Union. To read more, see Ozone Hole: Prospects for Recovery [ http://www.nasa.gov/centers/goddard/news/topstory/2005/ozone_recovery.html ] on the NASA Goddard News web page. To read more about the ozone hole and NASA's mission to study it, check out Ozone Hole Watch [ http://ozonewatch.gsfc.nasa.gov/facts/hole.html ]. The site also contains daily images of the ozone hole as measured by Aura's Ozone Monitoring Instrument. NASA image and animations courtesy GSFC Ozone Processing Team, [ http://toms.gsfc.nasa.gov/ ] based on data provided by the Ozone Monitoring Instrument [ http://www.knmi.nl/omi/publ-en/news/index.html ] (OMI) |
|
2005 Ozone Hole
| Title |
2005 Ozone Hole |
| Description |
The year 2005 marks the twentieth anniversary of the discovery of the ozone hole and the first full year that NASA's Aura satellite has provided detailed images of the hole. Aura was launched in 2004 to monitor the Earth's atmosphere, including the health of the delicate ozone layer. The Ozone Monitoring Instrument on Aura collected the data used to create this image on September 11, 2005, when the ozone hole covered 27 million square kilometers—its peak size for the season. Deep blue shows where ozone levels were low enough to be considered part of the ozone hole. New research shows that the ozone layer may be slower in recovering than previously thought. Ozone is a highly reactive colorless gas that contains three oxygen atoms. Near the surface of the Earth, ozone is hazardous to human health, causing problems like lung irritation, but high in the atmosphere, ozone acts as a crucial shield that absorbs harmful ultraviolet radiation from the Sun. The ozone hole is not an actual hole, but a place in the atmosphere where the protective layer of ozone has worn thin. In 1985, Joseph Farman, Brian Gardiner, and Jonathan Shanklin discovered in the ozone hole over Antarctica. In the following two years, scientists confirmed that human-produced chemicals, chlorofluorocarbons, used in refrigeration and propellant devices, were causing the hole. Chlorofluorocarbons contain high levels of chlorine, which breaks free from the larger molecules in the bitter cold and darkness of Antarctic and Arctic winter. Through a series of chemical reactions, the free chlorine becomes a two-atom molecule of chlorine gas. When sunlight returns, the chlorine gas disintegrates into separate chlorine atoms, which catalyze the destruction of atmospheric ozone. Though the production of chlorofluorocarbons was restricted in 1987, reservoirs of the chemicals in existing refrigerators and air conditioners are still emitting ozone-depleting chemicals into the atmosphere at higher levels than predicted, new measurements show. The extra chemicals may delay the recovery of the ozone hole until about 2065. Previous models predicted a recovery of the ozone layer by 2050. These results were announced on December 6, 2005, at the fall meeting of the American Geophysical Union. To read more, see Ozone Hole: Prospects for Recovery [ http://www.nasa.gov/centers/goddard/news/topstory/2005/ozone_recovery.html ] on the NASA Goddard News web page. To read more about the ozone hole and NASA's mission to study it, check out Ozone Hole Watch [ http://ozonewatch.gsfc.nasa.gov/facts/hole.html ]. The site also contains daily images of the ozone hole as measured by Aura's Ozone Monitoring Instrument. NASA image and animations courtesy GSFC Ozone Processing Team, [ http://toms.gsfc.nasa.gov/ ] based on data provided by the Ozone Monitoring Instrument [ http://www.knmi.nl/omi/publ-en/news/index.html ] (OMI) |
|
Lena River Delta, Russia: Im
…
nasa, nasaimageofthedaygalle
…
After a 4,400-kilometer (2,7
…
ge_07343
| mediatype |
IMAGE |
| mediatype |
image |
| date |
2005-07-16 |
| creator |
NASA -- Image courtesy of NASA/GSFC/MITI/ERSDAC/JAROS, and the U.S./Japan asterweb.jpl.nasa.gov/ ASTER Science Team. |
| identifier |
ge_07343 |
|
Lena River Delta, Russia: Im
…
nasa, nasaimageofthedaygalle
…
After a 4,400-kilometer (2,7
…
ge_07343
| mediatype |
IMAGE |
| mediatype |
image |
| date |
2005-07-16 |
| creator |
NASA -- Image courtesy of NASA/GSFC/MITI/ERSDAC/JAROS, and the U.S./Japan asterweb.jpl.nasa.gov/ ASTER Science Team. |
| identifier |
ge_07343 |
|
African dust blows across th
…
nasa, nasaimageofthedaygalle
…
On January 10, 2005, the Mod
…
atlantic_tmo_10jan05
| mediatype |
IMAGE |
| mediatype |
image |
| date |
2005-01-10 |
| creator |
NASA -- NASA image created by Jesse Allen, Earth Observatory, using data provided courtesy of the Goddard Land Processes DAAC. |
| identifier |
atlantic_tmo_10jan05 |
|
2005 Ozone Hole: Image of th
…
nasa, nasaimageofthedaygalle
…
* eoimages.gsfc.nasa.gov/ima
…
antarctica_omi_2005254
| mediatype |
IMAGE |
| mediatype |
image |
| date |
2005-09-11 |
| creator |
NASA -- NASA image and animations courtesy GSFC toms.gsfc.nasa.gov/ Ozone Processing Team, based on data provided by the www.knmi.nl/omi/publ-en/news/index.html Ozone Monitoring Instrument (OMI) |
| identifier |
antarctica_omi_2005254 |
|
2005 Ozone Hole: Image of th
…
nasa, nasaimageofthedaygalle
…
* eoimages.gsfc.nasa.gov/ima
…
antarctica_omi_2005254
| mediatype |
IMAGE |
| mediatype |
image |
| date |
2005-09-11 |
| creator |
NASA -- NASA image and animations courtesy GSFC toms.gsfc.nasa.gov/ Ozone Processing Team, based on data provided by the www.knmi.nl/omi/publ-en/news/index.html Ozone Monitoring Instrument (OMI) |
| identifier |
antarctica_omi_2005254 |
|
Dallas, Texas: Image of the
…
nasa, nasaimageofthedaygalle
…
The Dallas-Fort Worth metrop
…
ISS010-E-24596
| mediatype |
IMAGE |
| mediatype |
image |
| date |
2005-04-14 |
| creator |
NASA -- Astronaut photograph eol.jsc.nasa.gov/scripts/sseop/photo.pl?mission=ISS010&roll=E&frame=24596 ISS010-E-24596 was acquired April 14, 2005, with a Kodak 760C digital camera with a 180 mm lens, and is provided by the ISS Crew Earth Observations experiment and the Image Science & Analysis Group, Johnson Space Center. The spaceflight.nasa.gov/home/index.html International Space Station Program supports the laboratory to help astronauts take pictures of Earth that will be of the greatest value to scientists and the public, and to make those images freely available on the Internet. Additional images taken by astronauts and cosmonauts can be viewed at the NASA/JSC eol.jsc.nasa.gov/ Gateway to Astronaut Photography of Earth. |
| identifier |
ISS010-E-24596 |
|
Bending the Rings
PIA06656
Sol (our sun)
Imaging Science Subsystem -
…
| Title |
Bending the Rings |
| Original Caption Released with Image |
Saturn's rings appear strangely warped in this view of the rings seen through the upper Saturn atmosphere. The atmosphere acts like a lens in refracting (bending) the light reflected from the rings. As the rings pass behind the overexposed limb (edge) of Saturn as seen from Cassini, the ring structure appears to curve downward due to the bending of the light as it passes through the upper atmosphere. This image was obtained using a near-infrared filter. The filter samples a wavelength where methane gas does not absorb light, thus making the far-off rings visible through the upper atmosphere. By comparing this image to similar ones taken using filters where methane gas does absorb, scientists can estimate the vertical profile of haze and the abundance of methane in Saturn's high atmosphere. The image was taken in visible light with the Cassini spacecraft narrow-angle camera on April 14, 2005, through a filter sensitive to wavelengths of infrared light centered at 938 nanometers and at a distance of approximately 197,000 kilometers (123,000 miles) from Saturn. The image scale is 820 meters (2,680 feet) per pixel. |
|
| General Description |
International Space Station Imagery |
|
| General Description |
International Space Station Imagery |
|
| General Description |
STS-114 Shuttle Mission Imagery |
|
| General Description |
STS-114 Shuttle Mission Imagery |
|
| General Description |
STS-114 Shuttle Mission Imagery |
|
|
