KH-9 Hexagon

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KH-9 HEXAGON
KH9 Hexagon integration.png
A KH-9 HEXAGON during assembly by Lockheed
Mission type Imagery intelligence
Operator National Reconnaissance Office
Spacecraft properties
Manufacturer
Launch mass11400 kg to 13300 kg (with mapping camera)
Dimensions16.2 m × 3.05 m (53.1 ft × 10.0 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 170 km (110 mi)
Apogee altitude 260 km (160 mi)
Inclination 97°
Main telescope
Typefolded Wright camera
Diameter0.91 m (3 ft 0 in)
Focal length1.52 m (5 ft 0 in)
Focal ratiof/3.0
Wavelengths visible light, Near-infrared
A KH-9 HEXAGON main features KH-9 HEXAGON.jpg
A KH-9 HEXAGON main features

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 (NRO), 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 2 ft (0.61 m), [3] though another source says "images in the "better-than-one-foot" category" for the last "Gambit" missions. [4]

Contents

They are also officially known as the Broad Coverage Photo Reconnaissance satellites (Code 467), built by Lockheed Corporation for the 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). [5]

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. [6] [7] [8]

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. [9]

Development

KH-9 was, according to many who worked on it, the most sophisticated mechanical satellite in history. [10] It was 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 70 ft (21 m) 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. [11] In the mid 1970s, over 1,000 people in the Danbury, Connecticut area worked on the secret project. [12]

A reentry vehicle from the first Hexagon satellite sank to 16,000 ft (4,900 m) below the Pacific Ocean after its parachute failed. The USS Trieste II (DSV-1) retrieved its payload in April 1972 after a lengthy search, but the film had disintegrated during the nine months underwater, leaving no usable photographs. [13]

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 13,300 and 11,400 kg (29,300 and 25,100 lb), respectively.

NRO intended to replace HEXAGON with ZEUS, later DAMON—HEXAGON's camera flown on the Space Shuttle—but DAMON was canceled in December 1980. [10] [14] In December 1976 NRO launched the first KH-11 KENNEN. While its electro-optical digital imaging had a smaller field of view than HEXAGON, by not needing film KENNEN was usable for years. [10]

Main KH-9 components

Satellite Control Section

Satellite Control Section HexagonSatelliteControlSection.png
Satellite Control Section

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 10 ft (3.0 m) (compared to 5 ft (1.5 m) for the Agena) and a length of 6 ft (1.8 m). 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". [15] SCS was equipped with deployable solar panels and an unfurlable parabolic antenna for high data rate communication. [16]

Main camera

A main camera optical path HEXAGON MainCameraOpticalPath.png
A main camera optical path
A achieved ground resolution of Satellite Vehicles (SV) 1 to 18 main cameras. KH9 resolution maincamera.png
A achieved ground resolution of Satellite Vehicles (SV) 1 to 18 main cameras.
A KH-9 image of the Soviet Kubinka airfield Kubinka3.jpg
A KH-9 image of the Soviet Kubinka airfield

The main camera system was designed by Perkin-Elmer to take stereo images, [17] 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 90–200 mi (480,000–1,060,000 ft; 140–320 km). The camera optical layout is an f/3.0 folded Wright camera, with a focal length of 60 in (1,500 mm). The system aperture is defined by a 20 in (510 mm) 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 0.91 m (3 ft 0 in)-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 2 ft (0.61 m) during the later phase of the project. [3] [18] Dwayne Allen Day calculated, using disclosed specifications, that HEXAGON was capable of 0.2 m (7.9 in) at nadir, and 0.4 m (1 ft 4 in) at apogee. [10]

Mapping camera

Missions 1205 to 1216 carried a "mapping camera" (also known as a "frame camera") that used 9 in (230 mm) film and had a moderately low resolution of initially 30 ft (9.1 m), which improved to 20 ft (6.1 m) on later missions [19] (somewhat better than LANDSAT). Intended for mapmaking, photos this camera took cover the entire Earth with images between 1973 and 1981. [20] Almost all the imagery from this camera, amounting to 29,000 images, each covering 3,400 km2 (1,300 sq mi), was declassified in 2002 as a result of Executive order 12951, [21] 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. [22]

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. [23]

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. [15]

Reentry vehicles

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. [15]

High-altitude atmospheric density

Missions 1205 to 1207 carried Doppler beacons [24] to help map the atmospheric density at high altitudes in an effort to understand the effect on ephemeris predictions. [25] [26] The measurements of the atmospheric density were released through NASA. [27]

ELINT subsatellites

Stereo pair of KH-9 imagery (Los Angeles-1968/06) D3C1217-200676A005.jpg
Stereo pair of KH-9 imagery (Los Angeles-1968/06)

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. [28] [29] [30] [31] [32] [33] [34] [35] [36]

IRCB (S73-7)

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. [37] [38]

KH-9 missions

NameBlock [11] Mission no.Launch date NSSDC ID
NORAD #
Other NameLaunch vehicleOrbitDecay date
KH9-1I120115 June 19711971-056A [39]
05297
OPS 7809 Titan IIID 184.0 km × 300.0 km, i=96.4°6 August 1971 [39]
KH9-2I120220 January 19721972-002A [40]
05769
OPS 1737Titan IIID157.0 km × 331.0 km, i=97.0°29 February 1972 [40]
KH9-3I12037 July 19721972-052A [41]
06094
OPS 7293Titan IIID174.0 km × 251.0 km, i=96.9°13 September 1972 [41]
KH9-4I120410 October 19721972-079A [42]
06227
OPS 8314Titan IIID160.0 km × 281.0 km, i=96.5°8 January 1973 [42]
KH9-5I12059 March 19731973-014A [43]
06382
OPS 8410Titan IIID152.0 km × 270.0 km, i=95.7°19 May 1973 [43]
KH9-6I120613 July 19731973-046A [44]
06727
OPS 8261Titan IIID156.0 km × 269.0 km, i=96.2°12 October 1973 [44]
KH9-7II120710 November 19731973-088A [45]
06928
OPS 6630Titan IIID159.0 km × 275.0 km, i=96.9°13 March 1974 [45]
KH9-8II120810 April 19741974-020A [46]
07242
OPS 6245Titan IIID153.0 km × 285.0 km, i=94.5°28 July 1974 [46]
KH9-9II120929 October 19741974-085A [47]
07495
OPS 7122Titan IIID162.0 km × 271.0 km, i=96.7°19 March 1975 [47]
KH9-10II12108 June 19751975-051A [48]
07918
OPS 6381Titan IIID157.0 km × 234.0 km, i=96.3°5 November 1975 [48]
KH9-11II12114 December 19751975-114A [49]
08467
OPS 4428Titan IIID157.0 km × 234.0 km, i=96.7°1 April 1976 [49]
KH9-12II12128 July 19761976-065A [50]
09006
OPS 4699Titan IIID159.0 km × 242.0 km, i=97.0°13 December 1976 [50]
KH9-13III121327 June 19771977-056A [51]
10111
OPS 4800Titan IIID155.0 km × 239.0 km, i=97.0°23 December 1977 [51]
KH9-14III121416 March 19781978-029A [52]
10733
OPS 0460Titan IIID172.0 km × 218.0 km, i=96.4°11 September 1978 [52]
KH9-15III121516 March 19791979-025A [53]
11305
OPS 3854Titan IIID177.0 km × 256.0 km, i=96.3°22 September 1979 [53]
KH9-16III121618 June 19801980-052A [54]
11850
OPS 3123Titan IIID169.0 km × 265.0 km, i=96.5°6 March 1981 [54]
KH9-17III121711 May 19821982-041A [55]
13170
OPS 5642Titan IIID177.0 km × 262.0 km, i=96.4°5 December 1982 [55]
KH9-18III121820 June 19831983-060A [56]
14137
OPS 0721 Titan 34D 163.0 km × 224.0 km, i=96.4°21 March 1984 [56]
KH9-19IV121925 June 19841984-065A [57]
15063
USA 2Titan 34D170.0 km × 230.0 km, i=96.5°18 October 1984 [57]
KH9-20IV122018 April 19861986-F03Launch failed [2] Titan 34D

(NSSDC ID Numbers: See COSPAR)

Cost

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 17.47 billion in 2023, with an average reference year of 1976). [11]

Specifications

Data source: The Encyclopedia of US Spacecraft [1] and NSSDC

Declassification

The HEXAGON images have been declassified in 2011 as a continuation of Executive Order 12951. [59] [60] The declassified imagery has since been used by a team of scientists from Dartmouth College to detect Roman forts in Syria, [61] and the Catalan Institute of Classical Archaeology (ICAC) to detect qanat irrigation systems. [62]

See also

Other U.S. imaging spy satellites:

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