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Close-up of the Backside of
…
| Name of Image |
Close-up of the Backside of the Moon |
| Date of Image |
1969-07-20 |
| Full Description |
This is a detailed view of the back side of Moon in the vicinity of Crater No. 308 taken during the Apollo 11 mission. Apollo 11, the first manned lunar mission, launched from The Kennedy Space Center, Florida via a Saturn V launch vehicle on July 16, 1969 and safely returned to Earth on July 24, 1969. The Saturn V vehicle was developed by the Marshall Space Flight Center (MSFC) under the direction of Dr. Wernher von Braun. The 3-man crew aboard the flight consisted of Neil A. Armstrong, commander, Michael Collins, Command Module pilot, and Edwin E. Aldrin Jr., Lunar Module pilot. The Lunar Module (LM), named ?Eagle, carrying astronauts Neil Armstrong and Edwin Aldrin, was the first crewed vehicle to land on the Moon. Meanwhile, astronaut Collins piloted the Command Module in a parking orbit around the Moon. Armstrong was the first human to ever stand on the lunar surface, followed by Edwin (Buzz) Aldrin. The crew collected 47 pounds of lunar surface material which was returned to Earth for analysis. The surface exploration was concluded in 2½ hours. With the success of Apollo 11, the national objective to land men on the Moon and return them safely to Earth had been accomplished. |
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Apollo 11: East Crater Panor
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| Title |
Apollo 11: East Crater Panorama |
| Explanation |
On July 20, 1969 [ http://history.nasa.gov/ap11ann/introduction.htm ], Apollo 11 astronauts Neil Armstrong [ http://history.nasa.gov/ap11ann/kippsphotos/ 5528.jpg ] and Edwin "Buzz" Aldrin [ http://history.nasa.gov/ap11ann/kippsphotos/ 5390.jpg ] became the first to walk on the Moon [ http://www.hq.nasa.gov/alsj/a11/a11.html ]. This panorama of their landing site [ http://www.boulder.swri.edu/~durda/Apollo/ landing_sites.html ] sweeps across the magnificent desolation [ http://antwrp.gsfc.nasa.gov/apod/ap031109.html ] of the Moon's Sea [ http://www.fourmilab.ch/earthview/lunarform/ maria.html ] of Tranquility, with their Lunar Module, the Eagle, in the background at the far left. East Crater, about 30 meters wide and 4 meters deep, is on the right (scroll right), and was so named because it is about 60 meters east of the Lunar Module. Armstrong had piloted the Eagle safely over the crater. Near the end of his stay on the lunar surface [ http://antwrp.gsfc.nasa.gov/apod/ap040417.html ] Armstrong strayed far enough from the Lunar Module [ http://antwrp.gsfc.nasa.gov/apod/ap020628.html ] to take the pictures used to construct this wide-angle view, his shadow appearing at the panorama's left edge. The object near the middle foreground is a stereo close-up camera. |
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1st Manned Lunar Landing and
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PIA03902
Sol (our sun)
Thermal Emission Imaging Sys
…
| Title |
1st Manned Lunar Landing and 1st Robotic Mars Landing Commemorative Release: Viking 1 Landing Site in Chryse Planitia - Visible Image |
| Original Caption Released with Image |
(Released 20 July 2002) The date July 20 marks two major milestones in humanity's grand push to explore the frontier of space. On this date, in 1969, the Apollo 11 lunar module Eagle landed the first men (Neil Armstrong and Edwin "Buzz" Aldrin) on another celestial body, the Moon . In 1976, seven years to the day, the robotic Viking 1 Lander made the first successful landing on the ruddy rock strewn surface of Mars . To commemorate these milestones the THEMIS Team is releasing both an IR (Infra-Red) and Visible image of the Viking 1 landing site. THEMIS is currently imaging landing sites for future robotic missions including the twin Mars Exploration Rovers set to touchdown in January 2004. All of these missions anticipate the day when, hopefully in the not too distant future, astronauts will land on the red planet. So as we reflect on our rich tradition of space exploration let us also dream and plan on a wondrous future exploring the mysterious red planet. Viking 1 landed on a relatively smooth plain in Chryse Planitia (Plains of Gold), which is a low region of the northern hemisphere of Mars. The reported landing site is 22.48° N, 49.97° W. The landing site is marked with an X in the images. This region of Mars is dominated by plains, wrinkle ridges, and impact craters. This 4 framelet image is part of a 5 band image sequence. This image primarily contains plains, wrinkle ridges and craters. Some craters have ripples on their floors, which are probably dunes while other craters have some type of deposit on their floors. These deposits are most likely aeolian in nature. In places the wrinkle ridges appear to be buried or mantled with material that may be either volcanic and or fluvial in origin. The lander's view of the surface shows an undulating rocky surface with some finer grained materials present, and distant crater rims and wrinkle ridges. |
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1st Manned Lunar Landing and
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PIA03902
Sol (our sun)
Thermal Emission Imaging Sys
…
| Title |
1st Manned Lunar Landing and 1st Robotic Mars Landing Commemorative Release: Viking 1 Landing Site in Chryse Planitia - Visible Image |
| Original Caption Released with Image |
(Released 20 July 2002) The date July 20 marks two major milestones in humanity's grand push to explore the frontier of space. On this date, in 1969, the Apollo 11 lunar module Eagle landed the first men (Neil Armstrong and Edwin "Buzz" Aldrin) on another celestial body, the Moon . In 1976, seven years to the day, the robotic Viking 1 Lander made the first successful landing on the ruddy rock strewn surface of Mars . To commemorate these milestones the THEMIS Team is releasing both an IR (Infra-Red) and Visible image of the Viking 1 landing site. THEMIS is currently imaging landing sites for future robotic missions including the twin Mars Exploration Rovers set to touchdown in January 2004. All of these missions anticipate the day when, hopefully in the not too distant future, astronauts will land on the red planet. So as we reflect on our rich tradition of space exploration let us also dream and plan on a wondrous future exploring the mysterious red planet. Viking 1 landed on a relatively smooth plain in Chryse Planitia (Plains of Gold), which is a low region of the northern hemisphere of Mars. The reported landing site is 22.48° N, 49.97° W. The landing site is marked with an X in the images. This region of Mars is dominated by plains, wrinkle ridges, and impact craters. This 4 framelet image is part of a 5 band image sequence. This image primarily contains plains, wrinkle ridges and craters. Some craters have ripples on their floors, which are probably dunes while other craters have some type of deposit on their floors. These deposits are most likely aeolian in nature. In places the wrinkle ridges appear to be buried or mantled with material that may be either volcanic and or fluvial in origin. The lander's view of the surface shows an undulating rocky surface with some finer grained materials present, and distant crater rims and wrinkle ridges. |
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1st Manned Lunar Landing and
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PIA03902
Sol (our sun)
Thermal Emission Imaging Sys
…
| Title |
1st Manned Lunar Landing and 1st Robotic Mars Landing Commemorative Release: Viking 1 Landing Site in Chryse Planitia - Visible Image |
| Original Caption Released with Image |
(Released 20 July 2002) The date July 20 marks two major milestones in humanity's grand push to explore the frontier of space. On this date, in 1969, the Apollo 11 lunar module Eagle landed the first men (Neil Armstrong and Edwin "Buzz" Aldrin) on another celestial body, the Moon . In 1976, seven years to the day, the robotic Viking 1 Lander made the first successful landing on the ruddy rock strewn surface of Mars . To commemorate these milestones the THEMIS Team is releasing both an IR (Infra-Red) and Visible image of the Viking 1 landing site. THEMIS is currently imaging landing sites for future robotic missions including the twin Mars Exploration Rovers set to touchdown in January 2004. All of these missions anticipate the day when, hopefully in the not too distant future, astronauts will land on the red planet. So as we reflect on our rich tradition of space exploration let us also dream and plan on a wondrous future exploring the mysterious red planet. Viking 1 landed on a relatively smooth plain in Chryse Planitia (Plains of Gold), which is a low region of the northern hemisphere of Mars. The reported landing site is 22.48° N, 49.97° W. The landing site is marked with an X in the images. This region of Mars is dominated by plains, wrinkle ridges, and impact craters. This 4 framelet image is part of a 5 band image sequence. This image primarily contains plains, wrinkle ridges and craters. Some craters have ripples on their floors, which are probably dunes while other craters have some type of deposit on their floors. These deposits are most likely aeolian in nature. In places the wrinkle ridges appear to be buried or mantled with material that may be either volcanic and or fluvial in origin. The lander's view of the surface shows an undulating rocky surface with some finer grained materials present, and distant crater rims and wrinkle ridges. |
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1st Manned Lunar Landing and
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PIA03901
Sol (our sun)
Thermal Emission Imaging Sys
…
| Title |
1st Manned Lunar Landing and 1st Robotic Mars Landing Commemorative Release: Viking 1 Landing Site in Chryse Planitia - Infrared Image |
| Original Caption Released with Image |
(Released 20 July 2002) The date July 20 marks two major milestones in humanity's grand push to explore the frontier of space. On this date, in 1969, the Apollo 11 lunar module Eagle landed the first men (Neil Armstrong and Edwin "Buzz" Aldrin) on another celestial body, the Moon . In 1976, seven years to the day, the robotic Viking 1 Lander made the first successful landing on the ruddy rock strewn surface of Mars . To commemorate these milestones the THEMIS Team is releasing both an IR (Infra-Red) and Visible image of the Viking 1 landing site. THEMIS is currently imaging landing sites for future robotic missions including the twin Mars Exploration Rovers set to touchdown in January 2004. All of these missions anticipate the day when, hopefully in the not too distant future, astronauts will land on the red planet. So as we reflect on our rich tradition of space exploration let us also dream and plan on a wondrous future exploring the mysterious red planet. Viking 1 landed on a relatively smooth plain in Chryse Planitia (Plains of Gold), which is a low region of the northern hemisphere of Mars. The reported landing site is 22.48° N, 49.97° W. The landing site is marked with an X in the images. This region of Mars is dominated by plains, wrinkle ridges, and impact craters. This one band IR (band 9 at 12.6 microns) image shows bright and dark textures, which are primarily due to differences in the abundance of rocks on the surface. The relatively cool (dark) regions during the day are rocky or indurated materials whereas fine sand and dust are warmer (bright). The brightness levels show daytime surface temperatures, which range from about minus 34 degrees to minus 22 degrees Celsius (minus 29 degrees to minus 8 degrees Fahrenheit). Many of the temperature variations are due to slope effects, with sun-facing slopes warmer than shaded slopes. The dark rings around several of the craters are due to the presence of rocky (cool) material ejected from the crater. These rocks are well below the resolution of any existing Mars camera, but THEMIS can detect the temperature variations they produce. Daytime temperature variations are produced by a combination of topographic (solar heating) and thermophysical (thermal inertia and albedo) effects. Due to topographic heating the surface morphologies seen in THEMIS daytime IR images are similar to those seen in previous imagery and MOLA topography. Smooth, undulating, and ridged plains dominate this scene. The major thermophysical variations seen in daytime images are associated with impact craters and the wrinkle ridges. Other than these ejecta deposits and the wrinkle ridges, there is little variation in the thermophysical properties of the surface materials. |
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1st Manned Lunar Landing and
…
PIA03901
Sol (our sun)
Thermal Emission Imaging Sys
…
| Title |
1st Manned Lunar Landing and 1st Robotic Mars Landing Commemorative Release: Viking 1 Landing Site in Chryse Planitia - Infrared Image |
| Original Caption Released with Image |
(Released 20 July 2002) The date July 20 marks two major milestones in humanity's grand push to explore the frontier of space. On this date, in 1969, the Apollo 11 lunar module Eagle landed the first men (Neil Armstrong and Edwin "Buzz" Aldrin) on another celestial body, the Moon . In 1976, seven years to the day, the robotic Viking 1 Lander made the first successful landing on the ruddy rock strewn surface of Mars . To commemorate these milestones the THEMIS Team is releasing both an IR (Infra-Red) and Visible image of the Viking 1 landing site. THEMIS is currently imaging landing sites for future robotic missions including the twin Mars Exploration Rovers set to touchdown in January 2004. All of these missions anticipate the day when, hopefully in the not too distant future, astronauts will land on the red planet. So as we reflect on our rich tradition of space exploration let us also dream and plan on a wondrous future exploring the mysterious red planet. Viking 1 landed on a relatively smooth plain in Chryse Planitia (Plains of Gold), which is a low region of the northern hemisphere of Mars. The reported landing site is 22.48° N, 49.97° W. The landing site is marked with an X in the images. This region of Mars is dominated by plains, wrinkle ridges, and impact craters. This one band IR (band 9 at 12.6 microns) image shows bright and dark textures, which are primarily due to differences in the abundance of rocks on the surface. The relatively cool (dark) regions during the day are rocky or indurated materials whereas fine sand and dust are warmer (bright). The brightness levels show daytime surface temperatures, which range from about minus 34 degrees to minus 22 degrees Celsius (minus 29 degrees to minus 8 degrees Fahrenheit). Many of the temperature variations are due to slope effects, with sun-facing slopes warmer than shaded slopes. The dark rings around several of the craters are due to the presence of rocky (cool) material ejected from the crater. These rocks are well below the resolution of any existing Mars camera, but THEMIS can detect the temperature variations they produce. Daytime temperature variations are produced by a combination of topographic (solar heating) and thermophysical (thermal inertia and albedo) effects. Due to topographic heating the surface morphologies seen in THEMIS daytime IR images are similar to those seen in previous imagery and MOLA topography. Smooth, undulating, and ridged plains dominate this scene. The major thermophysical variations seen in daytime images are associated with impact craters and the wrinkle ridges. Other than these ejecta deposits and the wrinkle ridges, there is little variation in the thermophysical properties of the surface materials. |
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Apollo 11 Lunar Module ascen
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| Title |
Apollo 11 Lunar Module ascent stage photographed from Command Module |
| Description |
The Apollo 11 Lunar Module ascent stage, with Astronauts Neil A. Armstrong and Edwin E. Aldrin Jr. aboard, is photographed from the Command and Service Modules in lunar orbit. This view is looking west with the earth rising above the lunar horizon. Astronaut Michael Collins, command module pilot, remained with the Command/Service Module in lunar orbit while Armstrong and Aldrin explored the Moon. The Lunar Module is approaching from below. The mare area in the background is Smyth's Sea. At right center is International Astronomical Union crater no. 189. |
| Date Taken |
1969-07-21 |
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