KH-8 Gambit 3: Difference between revisions
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| name = KH-8 GAMBIT |
| name = KH-8 GAMBIT |
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| image = GAMBIT3 Agena.png |
| image = GAMBIT3 Agena.png |
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| image_caption = Schematics of GAMBIT-3 and [[RM- |
| image_caption = Schematics of GAMBIT-3 and [[RM-81 Agena#Agena-D|Agena D]] |
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| mission_type = [[Imagery intelligence]] |
| mission_type = [[Imagery intelligence]] |
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| operator = [[National Reconnaissance Office]] |
| operator = [[National Reconnaissance Office]] |
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| launch_mass = 4100 kg (on orbit) |
| launch_mass = 4100 kg (on orbit) |
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| dimensions = {{cvt|14.75|x|1.52|m}} |
| dimensions = {{cvt|14.75|x|1.52|m}} |
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| launch_rocket = [[ |
| launch_rocket = [[Titan (rocket family)#Titan III|Titan III]] |
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| launch_site = [[Vandenberg Air Force Base]], [[SLC-4E]] |
| launch_site = [[Vandenberg Air Force Base]], [[SLC-4E]] |
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| launch_contractor = [[Martin Marietta]] |
| launch_contractor = [[Martin Marietta]] |
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| disposal_type = |
| disposal_type = |
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| orbit_reference = [[Sun-synchronous orbit]] |
| orbit_reference = [[Sun-synchronous orbit]] |
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| instruments_list = {{Infobox spaceflight/Instruments |
| instruments_list = {{Infobox spaceflight/Instruments |
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| acronym1 = MC | name1 = Main Camera |
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| acronym2 = APTC | name2 = Astro-Position Terrain Camera |
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}} |
}} |
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}} |
}} |
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The '''KH-8''' ([[Byeman Control System|BYEMAN]] codename '''Gambit-3''')<ref>{{cite web |title=GAMBIT 3 KH-8 Reconnaissance Satellite |url=https://www.nationalmuseum.af.mil/Visit/Museum-Exhibits/Fact-Sheets/Display/Article/195922/gambit-3-kh-8-reconnaissance-satellite/ |website=National Museum of the U.S. Air Force |access-date=10 August 2022}}</ref> was a long-lived series of [[reconnaissance satellite]]s of the "[[Key Hole]]" (KH) series used by the [[United States]] from July 1966 to April 1984,<ref>{{cite book |title=American espionage and the Soviet target |first=Jeffrey |last=Richelson |publisher=W. Morrow |year=1987 |isbn=978-0-688-06753-3 |page=[https://archive.org/details/americanespionag00rich/page/195 195] |url-access=registration |url=https://archive.org/details/americanespionag00rich/page/195 }}</ref> and also known as Low Altitude Surveillance Platform.<ref>[http://www.globalsecurity.org/space/systems/imint-overview.htm |
The '''KH-8''' ([[Byeman Control System|BYEMAN]] codename '''Gambit-3''')<ref>{{cite web |title=GAMBIT 3 KH-8 Reconnaissance Satellite |url=https://www.nationalmuseum.af.mil/Visit/Museum-Exhibits/Fact-Sheets/Display/Article/195922/gambit-3-kh-8-reconnaissance-satellite/ |website=National Museum of the U.S. Air Force |access-date=10 August 2022}}</ref> was a long-lived series of [[reconnaissance satellite]]s of the "[[Key Hole]]" (KH) series used by the [[United States]] from July 1966 to April 1984,<ref>{{cite book |title=American espionage and the Soviet target |first=Jeffrey |last=Richelson |publisher=W. Morrow |year=1987 |isbn=978-0-688-06753-3 |page=[https://archive.org/details/americanespionag00rich/page/195 195] |url-access=registration |url=https://archive.org/details/americanespionag00rich/page/195 }}</ref> and also known as Low Altitude Surveillance Platform.<ref>[http://www.globalsecurity.org/space/systems/imint-overview.htm Global Security Space Systems IMINT Overview] LASP</ref> The satellite ejected [[Corona (satellite)#Recovery|"film-bucket" canisters]] of [[photographic film]] that were retrieved as they descended through the [[Atmosphere of Earth|atmosphere]] by [[parachute]]. Ground resolution of the mature satellite system was better than {{convert|4|in|m}}.<ref name="NRO_GAMBITStory"/> There were 54 launch attempts of the 3,000 kilogram satellites, all from [[Vandenberg Air Force Base]], on variants of the [[Titan (rocket family)#Titan III|Titan III]] rocket. Three launches failed to achieve orbit. The first one was satellite #5 on April 26, 1967, which fell into the Pacific Ocean after the Titan second stage developed low thrust. The second was satellite #35 on May 20, 1972, which suffered an Agena pneumatic regulator failure and reentered the atmosphere. A few months later, pieces of the satellite turned up in England and the US managed to arrange for their hasty return. The third failure was satellite #39 on June 26, 1973, which suffered a stuck Agena fuel valve. The Bell 8096 engine failed to start and the satellite burned up in the atmosphere. The KH-8 was manufactured by [[Lockheed Corporation|Lockheed]]. The camera system/satellite was manufactured by [[Eastman Kodak]]'s A&O Division in [[Rochester, New York]]. |
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The Gambit codename was also used by the satellite's predecessor, the [[KH-7 Gambit]]. |
The Gambit codename was also used by the satellite's predecessor, the [[KH-7 Gambit]]. |
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Gambit 3 satellites were the same width as the Gambit 1 models, but also slightly longer – reaching about 29 |
Gambit 3 satellites were the same width as the Gambit 1 models, but also slightly longer – reaching about {{convert|29|ft|m}} in length. They carried {{convert|12,241|ft|m|abbr=off|sp=us}} of film and were designed for longer missions of up to 31 days.<ref name="Space.com">{{cite web|url=http://www.space.com/14394-declassified-spy-satellites-air-force.html|title=Declassified US Spy Satellites from Cold War Land in Ohio|date=January 28, 2012|publisher=Space.com |access-date=2015-10-11}}</ref> |
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While Gambit was primarily designed and operated as a surveillance satellite, capturing high definition images of specific targets at low orbital altitudes, a single Gambit Block 3 mission was operated in 'dual-mode', orbiting first at a higher altitude to capture wide-area search imagery before lowering its perigee to capture normal surveillance imagery. The first film return capsule failed to separate correctly due to a new pyro mechanism failing to perform correctly. The contingency release mechanism separated the film bucket and parachute from its return capsule, and left the film bucket stranded in orbit. In September 2002, the film bucket re-entered over the South Atlantic into deep water. As the film bucket lacked its protective heatshield or the parachute needed to slow its descent, no attempt was made to recover it.<ref>{{Cite web|title=GAMBIT_Dual_Mode|url=https://www.nro.gov/FOIA/Major-NRO-Programs-and-Projects/GAMBIT-Dual-Mode/|access-date=2021-02-19|website=www.nro.gov}}</ref> |
While Gambit was primarily designed and operated as a surveillance satellite, capturing high definition images of specific targets at low orbital altitudes, a single Gambit Block 3 mission was operated in 'dual-mode', orbiting first at a higher altitude to capture wide-area search imagery before lowering its perigee to capture normal surveillance imagery. The first film return capsule failed to separate correctly due to a new pyro mechanism failing to perform correctly. The contingency release mechanism separated the film bucket and parachute from its return capsule, and left the film bucket stranded in orbit. In September 2002, the film bucket re-entered over the South Atlantic into deep water. As the film bucket lacked its protective heatshield or the parachute needed to slow its descent, no attempt was made to recover it.<ref>{{Cite web|title=GAMBIT_Dual_Mode|url=https://www.nro.gov/FOIA/Major-NRO-Programs-and-Projects/GAMBIT-Dual-Mode/|access-date=2021-02-19|website=www.nro.gov}}</ref> |
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The Camera Optics Module of KH-8 consists of four cameras. |
The Camera Optics Module of KH-8 consists of four cameras. |
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The main camera of KH-8B (introduced in 1971) with a focal length of {{convert|175.6|inch|m|abbr=on}} is a single strip camera, designed to gather high-resolution images of ground targets. In the strip camera the ground image is reflected by a steerable flat mirror to a {{convert|1.21|m|in|abbr=on}} diameter stationary [[concave mirror|concave]] primary mirror. The primary mirror reflects the light through an opening in the flat mirror and through a [[Ross (optics)|Ross corrector]]. At periapsis altitude of 75 |
The main camera of KH-8B (introduced in 1971) with a focal length of {{convert|175.6|inch|m|abbr=on}} is a single strip camera, designed to gather high-resolution images of ground targets. In the strip camera the ground image is reflected by a steerable flat mirror to a {{convert|1.21|m|in|abbr=on}} diameter stationary [[concave mirror|concave]] primary mirror. The primary mirror reflects the light through an opening in the flat mirror and through a [[Ross (optics)|Ross corrector]]. At [[periapsis]] altitude of {{convert|75|nmi|km}}, the main camera imaged a 6.3 km wide ground swath on a {{convert|8.811|in|abbr=on}} wide moving portion of film through a small slit aperture, resulting in an image scale of 28 meter / millimeter.<ref name="NRO_KH8Camera">{{cite web|url=http://www.nro.gov/history/csnr/gambhex/index.html|title=KH-8 Camera System|publisher=National Reconnaissance Office|year=1970|access-date=2011-09-26|archive-url=https://web.archive.org/web/20120915093330/http://www.nro.gov/history/csnr/gambhex/index.html|archive-date=2012-09-15|url-status=dead}}</ref><ref name="IkesGambit">{{cite web|url=http://www.thespacereview.com/article/1279/1|title=Ike's gambit: The development and operations of the KH-7 and KH-8 spy satellites|publisher=www.thespacereview.com|first=Dwayne A.|last=Day|access-date=2009-01-25|date=2010-11-29}}</ref> The Astro-Position Terrain Camera (APTC) contains three cameras: a 75mm focal length terrain frame camera, and two 90mm focal length stellar cameras. The terrain frame camera takes exposures of Earth in direction of the vehicle roll position for attitude determination. The stellar cameras observed in 180 degree opposite directions and took images of star fields.<ref name="NRO_KH8Camera"/> |
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[[File:TheGambitStoryPage154.png|thumb|150px|Ground-resolution distance achievable by KH-8]] |
[[File:TheGambitStoryPage154.png|thumb|150px|Ground-resolution distance achievable by KH-8]] |
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The films used by GAMBIT were provided by [[Eastman Kodak]], and evolved through a series of successively higher definition films, starting with Type 3404 with a resolving power of 50 to 100 [[line pairs per mm]].<ref name="KodakType3404">{{cite web|url=http://www.kodak.com/eknec/documents/2e/0900688a802b092e/ti1669.pdf|title=KODAK PLUS-X AERECON II Film 3404|publisher=Kodak|date=2005-11-28|url-status=dead|archive-url=https://web.archive.org/web/20131106013809/http://www.kodak.com/eknec/documents/2e/0900688a802b092e/ti1669.pdf|archive-date=2013-11-06}}</ref> Subsequent films used were Type 1414 high-definition film, SO-217 high-definition fine-grain film, and a series of films with [[Silver halide#Light sensitivity|silver-halide crystals]] of very uniform size and shape. The size of silver-halide crystals decreased from 1,550 angstrom in film Type SO-315, to 1,200 angstrom in SO-312, and ultimately to 900 angstrom in SO-409.<ref name="NRO_GAMBITStory">{{cite web|url=http://www.nro.gov/history/csnr/gambhex/index.html|title=The GAMBIT Story|publisher=National Reconnaissance Office|date=June 1991|access-date=2011-09-26|archive-url=https://web.archive.org/web/20120915093330/http://www.nro.gov/history/csnr/gambhex/index.html|archive-date=2012-09-15|url-status=dead}}</ref> Under optimal conditions GAMBIT would thus have been able to record ground features as small as 0.28 |
The films used by GAMBIT were provided by [[Eastman Kodak]], and evolved through a series of successively higher definition films, starting with Type 3404 with a resolving power of 50 to 100 [[line pairs per mm]].<ref name="KodakType3404">{{cite web|url=http://www.kodak.com/eknec/documents/2e/0900688a802b092e/ti1669.pdf|title=KODAK PLUS-X AERECON II Film 3404|publisher=Kodak|date=2005-11-28|url-status=dead|archive-url=https://web.archive.org/web/20131106013809/http://www.kodak.com/eknec/documents/2e/0900688a802b092e/ti1669.pdf|archive-date=2013-11-06}}</ref> Subsequent films used were Type 1414 high-definition film, SO-217 high-definition fine-grain film, and a series of films with [[Silver halide#Light sensitivity|silver-halide crystals]] of very uniform size and shape. The size of silver-halide crystals decreased from 1,550 angstrom in film Type SO-315, to 1,200 angstrom in SO-312, and ultimately to 900 angstrom in SO-409.<ref name="NRO_GAMBITStory">{{cite web|url=http://www.nro.gov/history/csnr/gambhex/index.html|title=The GAMBIT Story|publisher=National Reconnaissance Office|date=June 1991|access-date=2011-09-26|archive-url=https://web.archive.org/web/20120915093330/http://www.nro.gov/history/csnr/gambhex/index.html|archive-date=2012-09-15|url-status=dead}}</ref> Under optimal conditions GAMBIT would thus have been able to record ground features as small as {{convert|0.28|to|0.56|m|ft|abbr=on}} using the Eastman Kodak Type 3404 film. Using a film with a resolving power equivalent to the Kodak's Type 3409 film of 320 to 630 line pairs per mm, GAMBIT would have been able to record ground features as small as 5 cm to 10 cm (2" to 4").<ref name="KodakType3409">{{cite web|url=http://www.kodak.com/eknec/documents/fe/0900688a802b08fe/ti2344.pdf|title=KODAK AERECON High Altitude Film 3409|publisher=Kodak|date=2005-11-28|url-status=dead|archive-url=https://web.archive.org/web/20140110092741/http://www.kodak.com/eknec/documents/fe/0900688a802b08fe/ti2344.pdf|archive-date=2014-01-10}}</ref> The initial September 2011 release of "The Gambit Story" quotes "The mature system produced examples of imagery better than four inches ground-resolution distance". This number was again redacted in a later release.<ref name="NRO_GAMBITStory"/> Five to ten centimeters corresponds to the resolution limit imposed by atmospheric turbulence as derived by Fried<ref>{{cite journal|last1=Fried|first1=David|title=Limiting Resolution Looking Down Through the Atmosphere|journal=Journal of the Optical Society of America|date=1966|volume=56|issue=10|pages=1380–1384|doi=10.1364/josa.56.001380|bibcode=1966JOSA...56.1380F}}</ref> and, independently, Evvard<ref>{{cite journal|last1=Evvard|first1=John|title=Atmospheric Turbulence Limits on the Observational Capabilities of Aerospacecraft|journal=NASA Technical Note|date=1 December 1968|volume=NASA-TN-D-4940|url=https://ntrs.nasa.gov/search.jsp?R=19690003603|access-date=18 June 2015}}</ref> in the mid-1960s; remarkably, GAMBIT had reached a physical limit on resolution only a few years after the US launched its first reconnaissance satellite. GAMBIT was also able to record objects in orbit. The capability was developed to photograph Soviet spacecraft, but was first used to aid NASA engineers designing repairs for the damaged [[Skylab]] space station in 1973.<ref name="day20120611">{{cite news| url=http://www.thespacereview.com/article/2100/1 | title=Out of the black | work=The Space Review | date=2012-06-11 | access-date=June 11, 2012 | author=Day, Dwayne Allen}}</ref><ref name="day20130520">{{Cite web |last=Day |first=Dwayne |date=2013-05-20 |title=Those magnificent spooks and their spying machine: The spies help rescue Skylab |url=https://www.thespacereview.com/article/2299/1 |access-date=2020-07-10 |website=The Space Review}}</ref> |
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==Missions== |
==Missions== |
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==Notable Missions== |
==Notable Missions== |
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In May |
In May 1973 Gambit KH8-38 was used to observe the crippled [[Skylab]] space station, as part of the preparation for repairing it by the [[Skylab 2]] mission.<ref name="day20130520"/> |
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==Cost== |
==Cost== |
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==References== |
==References== |
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* Mark Wade (August 9, 2003). [https://web.archive.org/web/20040413035819/http://www.astronautix.com/craft/kh8.htm KH-8]. ''Encyclopedia Astronautica''. |
* Mark Wade (August 9, 2003). [https://web.archive.org/web/20040413035819/http://www.astronautix.com/craft/kh8.htm KH-8]. ''Encyclopedia Astronautica''. Accessed April 23, 2004. |
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* [http://www.globalsecurity.org/space/systems/kh-8.htm KH-8 Gambit.] GlobalSecurity.org |
* [http://www.globalsecurity.org/space/systems/kh-8.htm KH-8 Gambit.] GlobalSecurity.org |
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{{reflist|2}} |
{{reflist|2}} |
Latest revision as of 19:10, 9 February 2024
Mission type | Imagery intelligence | ||||||
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Operator | National Reconnaissance Office | ||||||
Spacecraft properties | |||||||
Manufacturer |
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Launch mass | 4100 kg (on orbit) | ||||||
Dimensions | 14.75 m × 1.52 m (48.4 ft × 5.0 ft) | ||||||
Start of mission | |||||||
Rocket | Titan III | ||||||
Launch site | Vandenberg Air Force Base, SLC-4E | ||||||
Contractor | Martin Marietta | ||||||
Orbital parameters | |||||||
Reference system | Sun-synchronous orbit | ||||||
Regime | Low Earth orbit | ||||||
Perigee altitude | 135 km (84 mi) | ||||||
Apogee altitude | 305 km (190 mi) | ||||||
Inclination | 110.5° | ||||||
Main telescope | |||||||
Type | Aspheric reflector with five-element Ross corrector | ||||||
Diameter | 1.1 m (3 ft 7 in) | ||||||
Focal length | 4.46 m (14.6 ft) | ||||||
Focal ratio | f/4.09 | ||||||
Wavelengths | visible light, Near-infrared | ||||||
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The KH-8 (BYEMAN codename Gambit-3)[1] was a long-lived series of reconnaissance satellites of the "Key Hole" (KH) series used by the United States from July 1966 to April 1984,[2] and also known as Low Altitude Surveillance Platform.[3] The satellite ejected "film-bucket" canisters of photographic film that were retrieved as they descended through the atmosphere by parachute. Ground resolution of the mature satellite system was better than 4 inches (0.10 m).[4] There were 54 launch attempts of the 3,000 kilogram satellites, all from Vandenberg Air Force Base, on variants of the Titan III rocket. Three launches failed to achieve orbit. The first one was satellite #5 on April 26, 1967, which fell into the Pacific Ocean after the Titan second stage developed low thrust. The second was satellite #35 on May 20, 1972, which suffered an Agena pneumatic regulator failure and reentered the atmosphere. A few months later, pieces of the satellite turned up in England and the US managed to arrange for their hasty return. The third failure was satellite #39 on June 26, 1973, which suffered a stuck Agena fuel valve. The Bell 8096 engine failed to start and the satellite burned up in the atmosphere. The KH-8 was manufactured by Lockheed. The camera system/satellite was manufactured by Eastman Kodak's A&O Division in Rochester, New York.
The Gambit codename was also used by the satellite's predecessor, the KH-7 Gambit.
Gambit 3 satellites were the same width as the Gambit 1 models, but also slightly longer – reaching about 29 feet (8.8 m) in length. They carried 12,241 feet (3,731 meters) of film and were designed for longer missions of up to 31 days.[5]
While Gambit was primarily designed and operated as a surveillance satellite, capturing high definition images of specific targets at low orbital altitudes, a single Gambit Block 3 mission was operated in 'dual-mode', orbiting first at a higher altitude to capture wide-area search imagery before lowering its perigee to capture normal surveillance imagery. The first film return capsule failed to separate correctly due to a new pyro mechanism failing to perform correctly. The contingency release mechanism separated the film bucket and parachute from its return capsule, and left the film bucket stranded in orbit. In September 2002, the film bucket re-entered over the South Atlantic into deep water. As the film bucket lacked its protective heatshield or the parachute needed to slow its descent, no attempt was made to recover it.[6]
Camera Optics Module
[edit]The Camera Optics Module of KH-8 consists of four cameras.
The main camera of KH-8B (introduced in 1971) with a focal length of 175.6 in (4.46 m) is a single strip camera, designed to gather high-resolution images of ground targets. In the strip camera the ground image is reflected by a steerable flat mirror to a 1.21 m (48 in) diameter stationary concave primary mirror. The primary mirror reflects the light through an opening in the flat mirror and through a Ross corrector. At periapsis altitude of 75 nautical miles (139 km), the main camera imaged a 6.3 km wide ground swath on a 8.811 in (223.8 mm) wide moving portion of film through a small slit aperture, resulting in an image scale of 28 meter / millimeter.[7][8] The Astro-Position Terrain Camera (APTC) contains three cameras: a 75mm focal length terrain frame camera, and two 90mm focal length stellar cameras. The terrain frame camera takes exposures of Earth in direction of the vehicle roll position for attitude determination. The stellar cameras observed in 180 degree opposite directions and took images of star fields.[7]
The films used by GAMBIT were provided by Eastman Kodak, and evolved through a series of successively higher definition films, starting with Type 3404 with a resolving power of 50 to 100 line pairs per mm.[9] Subsequent films used were Type 1414 high-definition film, SO-217 high-definition fine-grain film, and a series of films with silver-halide crystals of very uniform size and shape. The size of silver-halide crystals decreased from 1,550 angstrom in film Type SO-315, to 1,200 angstrom in SO-312, and ultimately to 900 angstrom in SO-409.[4] Under optimal conditions GAMBIT would thus have been able to record ground features as small as 0.28 to 0.56 m (0.92 to 1.84 ft) using the Eastman Kodak Type 3404 film. Using a film with a resolving power equivalent to the Kodak's Type 3409 film of 320 to 630 line pairs per mm, GAMBIT would have been able to record ground features as small as 5 cm to 10 cm (2" to 4").[10] The initial September 2011 release of "The Gambit Story" quotes "The mature system produced examples of imagery better than four inches ground-resolution distance". This number was again redacted in a later release.[4] Five to ten centimeters corresponds to the resolution limit imposed by atmospheric turbulence as derived by Fried[11] and, independently, Evvard[12] in the mid-1960s; remarkably, GAMBIT had reached a physical limit on resolution only a few years after the US launched its first reconnaissance satellite. GAMBIT was also able to record objects in orbit. The capability was developed to photograph Soviet spacecraft, but was first used to aid NASA engineers designing repairs for the damaged Skylab space station in 1973.[13][14]
Missions
[edit]Name | Block[15] | Launch Date | Alt. Name | NSSDC ID No. | Launch Vehicle | Orbit | Decay date |
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KH8-1 | I | 1966-07-29 | OPS-3014 | 1966-069A | Titan IIIB | 158.0 km × 250.0 km, i=94.1° | 1966-08-06[16] |
KH8-2 | I | 1966-09-28 | OPS-4096 | 1966-086A | Titan IIIB | ||
KH8-3 | I | 1966-12-14 | OPS-8968 | 1966-113A | Titan IIIB | ||
KH8-4 | I | 1967-02-24 | OPS-4204 | 1967-016A | Titan IIIB | ||
KH8-5 | I | 1967-04-26 | OPS-4243 | 1967-F04, 1967-003X | Titan IIIB | no stable orbit | 1967-04-26 |
KH8-6 | I | 1967-06-20 | OPS-4282 | 1967-064A | Titan IIIB | ||
KH8-7 | I | 1967-08-16 | OPS-4886 | 1967-079A | Titan IIIB | ||
KH8-8 | I | 1967-09-19 | OPS-4941 | 1967-090A | Titan IIIB | ||
KH8-9 | I | 1967-10-25 | OPS-4995 | 1967-103A | Titan IIIB | ||
KH8-10 | I | 1967-12-05 | OPS-5000 | 1967-121A | Titan IIIB | ||
KH8-11 | I | 1968-01-18 | OPS-5028 | 1968-005A | Titan IIIB | ||
KH8-12 | I | 1968-03-13 | OPS-5057 | 1968-018A | Titan IIIB | ||
KH8-13 | I | 1968-04-17 | OPS-5105 | 1968-031A | Titan IIIB | ||
KH8-14 | I | 1968-06-05 | OPS-5138 | 1968-047A | Titan IIIB | ||
KH8-15 | I | 1968-08-06 | OPS-5187 | 1968-064A | Titan IIIB | ||
KH8-16 | I | 1968-09-10 | OPS-5247 | 1968-074A | Titan IIIB | ||
KH8-17 | I | 1968-11-06 | OPS-5296 | 1968-099A | Titan IIIB | ||
KH8-18 | I | 1968-12-04 | OPS-6518 | 1968-108A | Titan IIIB | ||
KH8-19 | I | 1969-01-22 | OPS-7585 | 1969-007A | Titan IIIB | ||
KH8-20 | I | 1969-03-04 | OPS-4248 | 1969-019A | Titan IIIB | ||
KH8-21 | I | 1969-04-15 | OPS-5310 | 1969-039A | Titan IIIB | ||
KH8-22 | I | 1969-06-03 | OPS-1077 | 1969-050A | Titan IIIB | ||
KH8-23 | II | 1969-08-23 | OPS-7807 | 1969-074A | Titan 23B | ||
KH8-24 | II | 1969-10-24 | OPS-8455 | 1969-095A | Titan 23B | ||
KH8-25 | II | 1970-01-14 | OPS-6531 | 1970-002A | Titan 23B | ||
KH8-26 | II | 1970-04-15 | OPS-2863 | 1970-031A | Titan 23B | ||
KH8-27 | II | 1970-06-25 | OPS-6820 | 1970-048A | Titan 23B | ||
KH8-28 | II | 1970-08-18 | OPS-7874 | 1970-061A | Titan 23B | ||
KH8-29 | II | 1970-10-23 | OPS-7568 | 1970-090A | Titan 23B | ||
KH8-30 | II | 1971-01-21 | OPS-7776 | 1971-005A | Titan 23B | 139.0 km × 418.0 km, i=110.8° | 1971-02-09[17] |
KH8-31 | II | 1971-04-22 | OPS-7899 | 1971-033A | Titan 23B | 132.0 km × 401.0 km, i=110.9° | 1971-05-13[18] |
KH8-32 | II | 1971-08-12 | OPS-8607 | 1971-070A | Titan 24B | 137.0 km × 424.0 km, i=111.0° | 1971-09-03[19] |
KH8-33 | II | 1971-10-23 | OPS-7616 | 1971-092A | Titan 24B | 134.0 km × 416.0 km, i=110.9° | 1971-11-17[20] |
KH8-34 | II | 1972-03-17 | OPS-1678 | 1972-016A | Titan 24B | 131.0 km × 409.0 km, i=111.0° | 1972-04-11[21] |
KH8-35 | II | 1972-05-20 | OPS-6574 | 1972-F03 | Titan 24B | failed to reach orbit | |
KH8-36 | II | 1972-09-01 | OPS-8888 | 1972-068A | Titan 24B | 140.0 km × 380.0 km, i=110.5° | 1972-09-30[22] |
KH8-37 | III | 1972-12-21 | OPS-3978 | 1972-103A | Titan 24B | 139.0 km × 378.0 km, i=110.5° | 1973-01-23[23] |
KH8-38 | III | 1973-05-16 | OPS-2093 | 1973-028A | Titan 24B | 139.0 km × 399.0 km, i=110.5° | 1973-06-13[24] |
KH8-39 | III | 1973-06-26 | OPS-4018 | 1973-F04 | Titan 24B | failed to reach orbit | (mix-up with KH8-38 in NSSDC) |
KH8-40 | III | 1973-09-27 | OPS-6275 | 1973-068A | Titan 24B | 131.0 km × 385.0 km, i=110.5° | 1973-10-29[25] |
KH8-41 | III | 1974-02-13 | OPS-6889 | 1974-007A | Titan 24B | 134.0 km × 393.0 km, i=110.4° | 1974-03-17[26] |
KH8-42 | III | 1974-06-06 | OPS-1776 | 1974-042A | Titan 24B | 136.0 km × 394.0 km, i=110.5° | 1974-07-24[27] |
KH8-43 | III | 1974-08-14 | OPS-3004 | 1974-065A | Titan 24B | 135.0 km × 402.0 km, i=110.5° | 1974-09-29[28] |
KH8-44 | III | 1975-04-18 | OPS-4883 | 1975-032A | Titan 24B | 134.0 km × 401.0 km, i=110.5° | 1975-06-05[29] |
KH8-45 | III | 1975-10-09 | OPS-5499 | 1975-098A | Titan 24B | 125.0 km × 356.0 km, i=96.4° | 1975-11-30[30] |
KH8-46 | III | 1976-03-22 | OPS-7600 | 1976-027A | Titan 24B | 125.0 km × 347.0 km, i=96.4° | 1976-05-18[31] |
KH8-47 | III | 1976-09-15 | OPS-8533 | 1976-094A | Titan 24B | 135.0 km × 330.0 km, i=96.4° | 1976-11-05[32] |
KH8-48 | IV | 1977-03-13 | OPS-4915 | 1977-019A | Titan 24B | 124.0 km × 348.0 km, i=96.4° | 1977-05-26[33] |
KH8-49 | IV | 1977-09-23 | OPS-7471 | 1977-094A | Titan 24B | 125.0 km × 352.0 km, i=96.5° | 1977-12-08[34] |
KH8-50 | IV | 1979-05-28 | OPS-7164 | 1979-044A | Titan 24B | 124.0 km × 305.0 km, i=96.4° | 1979-08-26[35] |
KH8-51 | IV | 1981-02-28 | OPS-1166 | 1981-019A | Titan 24B | 138.0 km × 336.0 km, i=96.4° | 1981-06-20[36] |
KH8-52 | IV | 1982-01-21 | OPS-2849 | 1982-006A | Titan 24B | 630.0 km × 641.0 km, i=97.4° | 1982-05-23[37] |
KH8-53 | IV | 1983-04-15 | OPS-2925 | 1983-032A | Titan 24B | 124.0 km × 254.0 km, i=96.5° | 1983-08-21[38] |
KH8-54 | IV | 1984-04-17 | OPS-8424 | 1984-039A | Titan 24B | 127.0 km × 235.0 km, i=96.4° | 1984-08-13[39] |
(NSSDC ID Numbers: See COSPAR)
Notable Missions
[edit]In May 1973 Gambit KH8-38 was used to observe the crippled Skylab space station, as part of the preparation for repairing it by the Skylab 2 mission.[14]
Cost
[edit]The total cost of the 54 flight KH-8 program from FY1964 to FY1985, without non-recurring costs, was US$2.3 billion in respective year dollars.[15]
Other U.S. imaging spy satellites
[edit]- Corona series: KH-1, KH-2, KH-3, KH-4
- KH-5 ARGON, KH-6 LANYARD
- KH-7 Gambit and KH-8 GAMBIT
- KH-9 Hexagon "Big Bird"
- MOL – KH-10
- KH-11 Kennen, Misty (classified project), Enhanced Imaging System
References
[edit]- Mark Wade (August 9, 2003). KH-8. Encyclopedia Astronautica. Accessed April 23, 2004.
- KH-8 Gambit. GlobalSecurity.org
- ^ "GAMBIT 3 KH-8 Reconnaissance Satellite". National Museum of the U.S. Air Force. Retrieved August 10, 2022.
- ^ Richelson, Jeffrey (1987). American espionage and the Soviet target. W. Morrow. p. 195. ISBN 978-0-688-06753-3.
- ^ Global Security Space Systems IMINT Overview LASP
- ^ a b c "The GAMBIT Story". National Reconnaissance Office. June 1991. Archived from the original on September 15, 2012. Retrieved September 26, 2011.
- ^ "Declassified US Spy Satellites from Cold War Land in Ohio". Space.com. January 28, 2012. Retrieved October 11, 2015.
- ^ "GAMBIT_Dual_Mode". www.nro.gov. Retrieved February 19, 2021.
- ^ a b "KH-8 Camera System". National Reconnaissance Office. 1970. Archived from the original on September 15, 2012. Retrieved September 26, 2011.
- ^ Day, Dwayne A. (November 29, 2010). "Ike's gambit: The development and operations of the KH-7 and KH-8 spy satellites". www.thespacereview.com. Retrieved January 25, 2009.
- ^ "KODAK PLUS-X AERECON II Film 3404" (PDF). Kodak. November 28, 2005. Archived from the original (PDF) on November 6, 2013.
- ^ "KODAK AERECON High Altitude Film 3409" (PDF). Kodak. November 28, 2005. Archived from the original (PDF) on January 10, 2014.
- ^ Fried, David (1966). "Limiting Resolution Looking Down Through the Atmosphere". Journal of the Optical Society of America. 56 (10): 1380–1384. Bibcode:1966JOSA...56.1380F. doi:10.1364/josa.56.001380.
- ^ Evvard, John (December 1, 1968). "Atmospheric Turbulence Limits on the Observational Capabilities of Aerospacecraft". NASA Technical Note. NASA-TN-D-4940. Retrieved June 18, 2015.
- ^ Day, Dwayne Allen (June 11, 2012). "Out of the black". The Space Review. Retrieved June 11, 2012.
- ^ a b Day, Dwayne (May 20, 2013). "Those magnificent spooks and their spying machine: The spies help rescue Skylab". The Space Review. Retrieved July 10, 2020.
- ^ a b "The GAMBIT story". National Reconnaissance Office. June 1991. Archived from the original on October 7, 2017. Retrieved September 25, 2011.
- ^ "KH 8-01". NASA National Space Science Data Center. October 8, 2010.
- ^ "KH 8-30". NASA National Space Science Data Center. October 8, 2010.
- ^ "KH 8-31". NASA National Space Science Data Center. October 8, 2010.
- ^ "KH 8-32". NASA National Space Science Data Center. October 8, 2010.
- ^ "KH 8-33". NASA National Space Science Data Center. October 8, 2010.
- ^ "KH 8-34". NASA National Space Science Data Center. October 8, 2010.
- ^ "KH 8-36". NASA National Space Science Data Center. October 8, 2010.
- ^ "KH 8-37". NASA National Space Science Data Center. October 8, 2010.
- ^ "KH 8-38". NASA National Space Science Data Center. October 8, 2010.
- ^ "KH 8-40". NASA National Space Science Data Center. October 8, 2010.
- ^ "KH 8-41". NASA National Space Science Data Center. October 8, 2010.
- ^ "KH 8-42". NASA National Space Science Data Center. October 8, 2010.
- ^ "KH 8-43". NASA National Space Science Data Center. October 8, 2010.
- ^ "KH 8-44". NASA National Space Science Data Center. October 8, 2010.
- ^ "KH 8-45". NASA National Space Science Data Center. October 8, 2010.
- ^ "KH 8-46". NASA National Space Science Data Center. October 8, 2010.
- ^ "KH 8-47". NASA National Space Science Data Center. October 8, 2010.
- ^ "KH 8-48". NASA National Space Science Data Center. October 8, 2010.
- ^ "KH 8-49". NASA National Space Science Data Center. October 8, 2010.
- ^ "KH 8-50". NASA National Space Science Data Center. October 8, 2010.
- ^ "KH 8-51". NASA National Space Science Data Center. October 8, 2010.
- ^ "KH 8-52". NASA National Space Science Data Center. October 8, 2010.
- ^ "KH 8-53". NASA National Space Science Data Center. October 8, 2010.
- ^ "KH 8-54". NASA National Space Science Data Center. October 8, 2010.