| KH-9 HEXAGON | |||||||||||||||||
| Mission Type: | Imagery intelligence | ||||||||||||||||
| Operator: | National Reconnaissance Office | ||||||||||||||||
| Manufacturer: |
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| Launch Mass: | 11400 kg to 13300 kg (with mapping camera) | ||||||||||||||||
| Launch Rocket: | Titan III | ||||||||||||||||
| Launch Site: | Vandenberg Air Force Base, SLC-4E | ||||||||||||||||
| Launch Contractor: | Martin Marietta | ||||||||||||||||
| Orbit Reference: | Sun-synchronous orbit | ||||||||||||||||
| Orbit Regime: | Low Earth orbit | ||||||||||||||||
| Orbit Inclination: | 97° | ||||||||||||||||
| Apsis: | gee | ||||||||||||||||
| Telescope Type: | folded Wright camera | ||||||||||||||||
| Telescope Wavelength: | visible light, Near-infrared | ||||||||||||||||
| Instruments List: |
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KH-9 (BYEMAN codename HEXAGON), commonly known as Big Bird or KeyHole-9,[1] was a series of photographic reconnaissance satellites launched by the United States between 1971 and 1986. Of twenty launch attempts by the National Reconnaissance Office, all but one were successful.[2] Photographic film aboard the KH-9 was stored on RCA Astro Electronic Division take up reel system then sent back to Earth in recoverable film return capsules for processing and interpretation. The highest ground resolution achieved by the main cameras of the satellite was, though another source says "images in the "better-than-one-foot" category" for the last "Gambit" missions.[3]
They are also officially known as the Broad Coverage Photo Reconnaissance satellites (Code 467), built by Lockheed Corporation for the National Reconnaissance Office (NRO).[1]
The satellites were an important factor in determining Soviet military capabilities and in the acquisition of accurate intelligence for the formulation of U.S. national policy decisions as well as deployment of U.S. forces and weapon systems. The satellites were instrumental in U.S. National Technical Means of Verification of Strategic Arms Limitation Talks (SALT) and the Anti-Ballistic Missile Treaty (ABMT).[4]
The KH-9 was declassified in September 2011 and an example was put on public display for a single day on 17 September 2011 in the parking lot of the Steven F. Udvar-Hazy Center of the National Air and Space Museum.[5] [6] [7]
On 26 January 2012, the National Museum of the United States Air Force put a KH-9 on public display along with its predecessors the KH-7 and KH-8.[8]
The KH-9 was originally conceived in the early 1960s as a replacement for the CORONA search satellites. The goal was to search large areas of the Earth with a medium resolution camera. The KH-9 carried two main cameras, although a mapping camera was also carried on several missions. The photographic film from the cameras was sent to recoverable re-entry vehicles and returned to Earth, where the capsules were caught in mid-air by an aircraft. Four re-entry vehicles were carried on most missions, with a fifth added for missions that included a mapping camera.
Between September 1966 and July 1967, the contractors for the Hexagon subsystems were selected. Lockheed Missiles and Space Company (LMSC) was awarded the contract for the Satellite Basic Assembly (SBA), Perkin Elmer for the primary Sensor Subsystem (SS), McDonnell for the Reentry Vehicle (RV), RCA Astro-Electronics Division for the Film Take-Up system, and Itek for the Stellar Index camera (SI). Integration and ground-testing of Satellite Vehicle-1 (SV-1) were completed in May 1971, and it was subsequently shipped to Vandenberg Air Force Base in a container. Ultimately, four generations ("blocks") of KH-9 HEXAGON reconnaissance satellites were developed. KH9-7 (missions 7 to 12) was the first to fly a Block-II panoramic camera and SBA. Block-III (missions 13 to 18) included upgrades to electrical distribution and batteries. Two added tanks with ullage control for the Orbit Adjust System (OAS) and new thrusters for the Reaction Control System (RCS) served to increase KH-9's operational lifetime. In addition, the nitrogen supply for the film transport system and the camera vessel was increased. Block-IV (missions 19 and 20) was equipped with an extended command system using plated-wire memory. In the mid 1970s, over 1,000 people in the Danbury, Connecticut area worked on the secret project.[9]
A reentry vehicle from the first Hexagon satellite sank to below the Pacific Ocean after its parachute failed. The retrieved its payload in April 1972 after a lengthy search, but the film had disintegrated during the nine months underwater, leaving no usable photographs.[10]
Over the duration of the program, the lifetime of the individual satellites increased steadily. The final KH-9 operated for 275 days. The satellite mass with and without the Mapping Camera System was, respectively.
The Satellite Control Section (SCS), which forms the aft part of the SBA, started as Air Force Project 467. SCS was intended as a more capable replacement for the on-orbit propulsion, which had been provided by the Agena upper stage for previous generations of reconnaissance satellites. The SCS featured an increased diameter of (compared to for the Agena) and a length of . It housed hydrazine propellant tanks for the pressure fed Orbital Adjust System (OAS) and the Reaction Control System (RCS). OAS and RCS were connected by a transfer line to facilitate propellant exchange. The tank pressure was maintained within the operational range by additional high pressure nitrogen tanks. The SCS incorporated a freon gas system for backup attitude control inherited from the Agena, commonly referred to as "lifeboat".[11] SCS was equipped with deployable solar panels and an unfurlable parabolic antenna for high data rate communication.[12]
The main camera system was designed by Perkin-Elmer to take stereo images,[13] with a forward looking camera on the port side, and an aft looking camera on the starboard side. Images were taken at altitudes ranging from . The camera optical layout is an f/3.0 folded Wright camera, with a focal length of . The system aperture is defined by a diameter aspheric corrector plate, which corrects the spherical aberration of the Wright design. In each of the cameras the ground image passes through the corrector plate to a 45°-angle flat mirror, which reflects the light to a -diameter concave main mirror. The main mirror directs the light through an opening in the flat mirror and through a four-element lens system onto the film platen. The cameras could scan contiguous areas up to 120° wide, and achieved a ground resolution better than during the later phase of the project.[14] [15]
Missions 1205 to 1216 carried a "mapping camera" (also known as a "frame camera") that used film and had a moderately low resolution of initially, which improved to on later missions [16] (somewhat better than LANDSAT). Intended for mapmaking, photos this camera took cover the entire Earth with images between 1973 and 1981.[17] Almost all the imagery from this camera, amounting to 29,000 images, each covering, was declassified in 2002 as a result of Executive order 12951,[18] the same order which declassified CORONA, and copies of the films were transferred to the U.S. Geological Survey's Earth Resources Observation Systems office.[19]
Scientific analysis of declassified KH-9 satellite images continues to reveal historic trends and changes in climate and terrestrial geology. A 2019 study of glacial melt in the Himalayas over the past half-century used data collected by KH-9 satellites throughout the 1970s and 1980s to demonstrate that melt rates had doubled since 1975.[20]
The KH-9 was never a backup project for the KH-10 Manned Orbital Laboratory. It was developed solely as a replacement for the Corona search system.[11]
The forward section of KH-9 housed four McDonnell Douglas Mark 8 satellite reentry vehicles (RV), which were fed film exposed by the main cameras. Each RV had an empty mass of 434 kg. It housed a film take-up assembly (built by RCA Astro Electronic Division) with a mass of 108 kg, and could store about 227 kg of film. The twelve mapping missions were equipped with an additional General Electrics Mark V RV, which could store about 32 kg of film for a total mass of 177 kg.[11]
Missions 1205 to 1207 carried Doppler beacons[21] to help map the atmospheric density at high altitudes in an effort to understand the effect on ephemeris predictions.[22] [23] The measurements of the atmospheric density were released through NASA.[24]
Missions 1203, 1207, 1208, 1209, and 1212 to 1219 included Ferret ELINT sub-satellites, which were launched into a high Earth orbit to catalogue Soviet air defence radars, eavesdrop on voice communications, and tape missile and satellite telemetry. Missions 1210 to 1212 also included scientific subsatellites.[25] [26] [27] [28] [29] [30] [31] [32] [33]
IRCB (Infra-Red Calibration Balloon) was an 66 cm diameter inflatable calibration sphere orbited in the Space Test Program. It was a piggy-back payload on KH9-8 (1208) boosting it to a 500 mile (800 kilometers) circular orbit. It disappeared from ground-based sensors in the 1990s, and was found again in 2024.[34] [35]
| Name | Block [36] | Mission no. | Launch date | NSSDC ID NORAD # | Other Name | Launch vehicle | Orbit | Decay date | |
|---|---|---|---|---|---|---|---|---|---|
| KH9-1 | I | 1201 | 15 June 1971 | 1971-056A 05297 | OPS 7809 | Titan IIID | 184.0 km × 300.0 km, i=96.4° | 6 August 1971 [37] | |
| KH9-2 | I | 1202 | 20 January 1972 | 1972-002A 05769 | OPS 1737 | Titan IIID | 157.0 km × 331.0 km, i=97.0° | 29 February 1972 [38] | |
| KH9-3 | I | 1203 | 7 July 1972 | 1972-052A 06094 | OPS 7293 | Titan IIID | 174.0 km × 251.0 km, i=96.9° | 13 September 1972 [39] | |
| KH9-4 | I | 1204 | 10 October 1972 | 1972-079A 06227 | OPS 8314 | Titan IIID | 160.0 km × 281.0 km, i=96.5° | 8 January 1973 [40] | |
| KH9-5 | I | 1205 | 9 March 1973 | 1973-014A 06382 | OPS 8410 | Titan IIID | 152.0 km × 270.0 km, i=95.7° | 19 May 1973 [41] | |
| KH9-6 | I | 1206 | 13 July 1973 | 1973-046A 06727 | OPS 8261 | Titan IIID | 156.0 km × 269.0 km, i=96.2° | 12 October 1973 [42] | |
| KH9-7 | II | 1207 | 10 November 1973 | 1973-088A 06928 | OPS 6630 | Titan IIID | 159.0 km × 275.0 km, i=96.9° | 13 March 1974 [43] | |
| KH9-8 | II | 1208 | 10 April 1974 | 1974-020A 07242 | OPS 6245 | Titan IIID | 153.0 km × 285.0 km, i=94.5° | 28 July 1974 [44] | |
| KH9-9 | II | 1209 | 29 October 1974 | 1974-085A 07495 | OPS 7122 | Titan IIID | 162.0 km × 271.0 km, i=96.7° | 19 March 1975 [45] | |
| KH9-10 | II | 1210 | 8 June 1975 | 1975-051A 07918 | OPS 6381 | Titan IIID | 157.0 km × 234.0 km, i=96.3° | 5 November 1975 [46] | |
| KH9-11 | II | 1211 | 4 December 1975 | 1975-114A 08467 | OPS 4428 | Titan IIID | 157.0 km × 234.0 km, i=96.7° | 1 April 1976 [47] | |
| KH9-12 | II | 1212 | 8 July 1976 | 1976-065A 09006 | OPS 4699 | Titan IIID | 159.0 km × 242.0 km, i=97.0° | 13 December 1976 [48] | |
| KH9-13 | III | 1213 | 27 June 1977 | 1977-056A 10111 | OPS 4800 | Titan IIID | 155.0 km × 239.0 km, i=97.0° | 23 December 1977 [49] | |
| KH9-14 | III | 1214 | 16 March 1978 | 1978-029A 10733 | OPS 0460 | Titan IIID | 172.0 km × 218.0 km, i=96.4° | 11 September 1978 [50] | |
| KH9-15 | III | 1215 | 16 March 1979 | 1979-025A 11305 | OPS 3854 | Titan IIID | 177.0 km × 256.0 km, i=96.3° | 22 September 1979 [51] | |
| KH9-16 | III | 1216 | 18 June 1980 | 1980-052A 11850 | OPS 3123 | Titan IIID | 169.0 km × 265.0 km, i=96.5° | 6 March 1981 [52] | |
| KH9-17 | III | 1217 | 11 May 1982 | 1982-041A 13170 | OPS 5642 | Titan IIID | 177.0 km × 262.0 km, i=96.4° | 5 December 1982 [53] | |
| KH9-18 | III | 1218 | 20 June 1983 | 1983-060A 14137 | OPS 0721 | Titan 34D | 163.0 km × 224.0 km, i=96.4° | 21 March 1984 [54] | |
| KH9-19 | IV | 1219 | 25 June 1984 | 1984-065A 15063 | USA 2 | Titan 34D | 170.0 km × 230.0 km, i=96.5° | 18 October 1984 [55] | |
| KH9-20 | IV | 1220 | 18 April 1986 | 1986-F03 | Launch failed | Titan 34D | — | — |
The total cost of the 20 flights KH-9 program from FY1966 to FY1986 was US$3.262 billion in respective year dollars (equivalent to billion in, with an average reference year of 1976).[36]
Data source: The Encyclopedia of US Spacecraft [1] and NSSDC
Other U.S. imaging spy satellites: