The Missile Defense Alarm System, or MIDAS, was a United States Air Force Air Defense Command system of 12 early-warning satellites that provided limited notice of Soviet intercontinental ballistic missile launches between 1960 and 1966. Originally it was intended to serve as a complete early-warning system working in conjunction with the Ballistic Missile Early Warning System. Cost and reliability concerns limited the project to a research and development role. Three of the system's 12 launches ended in failure, and the remaining nine satellites provided crude infrared early-warning coverage of the Soviet Union until the project was replaced by the Defense Support Program. MiDAS represented one element of the United States's first generation of reconnaissance satellites that also included the Corona and SAMOS series. Though MIDAS failed in its primary role as a system of infrared early-warning satellites, it pioneered the technologies needed in successor systems.
Origins On October 4, 1957, from the Tyuratam range in the Kazakh SSR, the Soviet Union launched Sputnik 1, the world's first artificial satellite. The event, while a scientific triumph, also signified that the Soviet Union now had the capability to attack the United States with an intercontinental ballistic missile (ICBM). The R-7, the booster rocket that launched Sputnik 1 and Sputnik 2, could be loaded instead with a hydrogen bomb, bringing the threat of a surprise nuclear Pearl Harbor-style attack on the United States and Canada. To give an early warning of any Soviet sneak ICBM attack, the governments of the United States, Canada, and Denmark (with the authority over Greenland, where the main radar station was built at Thule Air Base) agreed to build the Ballistic Missile Early Warning System (BMEWS). This system would use radar to detect incoming ICBM warheads and give about 20 minutes of warning of an ICBM attack.
However, this system was hampered by the inherent limitations of radar systems and the curvature of the Earth. Due to the location of the Soviet Union on the other side of the Northern Hemisphere, the potential Soviet ICBM sites were thousands of miles over the horizon from the BMEWS radar stations that were under construction at Thule and Clear Air Force Station, Alaska (and later on, in England), and the BMEWS stations, as huge as they are, could not detect the ICBM warheads immediately after their launching. Only when the warheads had risen above the horizon could they be detected and warnings passed on by the U.S. Air Force.
Accurate calculations had already shown that the BMEWS system would give just ten to 25 minutes of warning in the case of an ICBM attack. The MIDAS system, as planned, would extend this warning time to about 30 minutes, giving the extra time needed for all of the Strategic Air Command's nuclear-armed heavy bombers to take off from their air bases, and hence proving to the Soviet government that it could not destroy these bombers in a sneak attack. Hence, the Soviets would be deterred from launching such an attack by a valid threat of nuclear retaliation."Draft of a Report on MIDAS", Jack Ruina, DARPA. November 1, 1961. Accessed November 19, 2007. In addition, the MIDAS system should have been able to confirm radar detections from BMEWS of a thermonuclear attack, hence reducing the chances of an accidental nuclear false alarm from the radar system.
Development and costs
On March 16, 1955, the U.S. Air Force had ordered the development of an advanced reconnaissance satellite to provide continuous surveillance of “preselected areas of the Earth” in order “to determine the status of a potential enemy’s war-making capability.”Mark Erickson, Into the Unknown Together - The DOD, NASA, and Early Spaceflight. 1-58566-140-6 The result of this order was the creation of a then-secret USAF program known as WS-117L, which controlled the development of the first generation of American reconnaissance satellites. These included the Corona series of observation satellites and the SAMOS satellite. The company that was to become the Lockheed-Martin Corporation which had been hired to design, develop, and manufacture the two series of satellites, suggested several other satellite programs to fill supporting roles, including a satellite that would use infrared sensors and a telescope to detect the heat produced by heavy bombers and ICBMs."Space-Based Early Warning: From MIDAS to DSP to SBIRS" Jeffery Richelson, National Security Archive Electronic Briefing Book No. 235. November 9, 2007. Accessed November 14, 2007. In response to the Soviet launch of Sputnik and the appearance of the ICBM threat, Subsystem G was added to WS-117L before the end of 1957.Jeffrey T. Richelson, America's Space Sentinels: DSP Satellites and National Security (Lawrence, KS.: University Press of Kansas, 1999), pgs. 8-9. With the creation of the Advanced Research Projects Agency (ARPA), Subsystem G was taken over by that organization and given the codename MiDAS in November 1958.
In February 1959, ARPA submitted an initial project development plan to the Air Force. As defined in the initial proposal, MIDAS would use infrared sensors from high above the Soviet Union to detect ICBM launches and give early warning of a thermonuclear attack. National Air and Space Museum, October 18, 1999. Accessed November 9, 2007. The plan called for a 10-satellite research and development program between November 1959 and May 1961. After that time, a full-scale operational system would be deployed."Draft of a Report on MIDAS", Jack Ruina, DARPA. November 1, 1961, p. IV-1. Accessed November 19, 2007.
Because the information collected by the MIDAS satellites was extraordinarily time-sensitive, the designers of the system could not use the film-canister dropping system that had been pioneered by the Discoverer/Corona/SAMOS series of reconnaissance satellites. In that system, the cameras aboard the satellites used photographic film capsules that physically re-entered the atmosphere before being retrieved mid-air by a military airplane. The MIDAS satellites would instead have to transmit their warning signals earthward via radio waves. Actual infrared images would not be transmitted due to the limited RF channel capacity that was available then. Instead, the satellite would simply send radio messages that it had detected a suspected missile launch as well as the time and location of the launch.
Multiple MIDAS satellites would be needed to provide round-the-clock coverage of the huge landmass of the Soviet Union. A booster rocket capable of sending a satellite into geostationary orbit had not yet been developed, and one or a few of these might not be able to cover all the possible ICBM launch sites within Russia, especially in the far north near the Arctic Circle. Satellites in polar orbits would be needed to detect launches from across the Soviet Union but due to the nature of the polar orbit, each would have only a brief period of time above the Soviet Union. As the planned capabilities of the satellite changed during the design process, so did the plans for their deployment. A plan completed in January 1959 recommended a constellation of twenty MIDAS satellites orbiting at an altitude of 1,000 miles while a revised plan, produced later that year, envisioned a constellation of twelve spacecraft at 2,000-mile altitudes.N.W. Watkins, "The MIDAS Project: Part I Strategic and Technical Origins and Political Evolution 1955-1963," Journal of the British Interplanetary Society Vol. 50, 1997, pp. 215-224.
Implementing a complete system, estimated in 1959, was put at between $200 million and $600 million"Report of the Early Warning Panel" The President's Science Advisory Committee, March 13, 1959. Accessed November 14, 2007. (equivalent to $ and $ in ). Because of this enormous cost and the fact that several "unanswered questions" remained, the scientific advisory council in charge of advising President Dwight D. Eisenhower on Early Warning systems recommended that a program of research be conducted but that final word on implementing a complete system be delayed for at least a year.
In FY1959, ARPA spent $22.8 million (equivalent to $ in ) on MIDAS, and in FY1960, ARPA and the Air Force spent a combined sum of $94.9 million (equivalent to $ in ).
Program summary and launch history
The MIDAS program commenced on February 26, 1960 when MIDAS 1 lifted off on an Atlas-Agena A booster from LC-14 at Cape Canaveral. The Atlas completed its burn successfully, but during the coasting phase prior to staging, the Atlas LOX tank pressure suddenly went to zero followed by missile tumbling while all Agena telemetry ceased. Postflight investigation proposed several causes, but the most likely one was inadvertent activation of the Agena Inadvertent Separation Destruct System (ISDS) charges. The ISDS system was redesigned after this incident, and MIDAS 2's booster did not carry an ISDS while modifications were being made."Postflight Evaluation Report, Atlas 29D" Convair March 14, 1960
On May 24, MIDAS 2 was orbited successfully, but the attitude control system failed. Some data was returned by the infrared sensor before the telemetry system also failed. Several planned experiments such as detection of flares on the ground and a Titan I missile test were abandoned. It remained in orbit until decaying in 1974. The next launch in the series did not take place for over a year and the program now moved to the West Coast, with Point Arguello's SLC-3 1-2 being its base of operations. During this interval, two CORONA satellites also carried and tested MIDAS sensors.
MIDAS 3, the first operational model, was launched on July 24, 1961 using the new, restartable Agena B stage. The Atlas's programmer reset itself due to a malfunction during booster jettison, but the satellite reached orbit successfully. However, one solar panel failed to deploy, starving MIDAS 3 of electrical power and it died after a few orbits. MIDAS 4 (October 21) brought about further frustration when the Atlas lost roll control at T+186 seconds. The satellite was placed into an incorrect trajectory, causing the Agena B to exhaust its attitude control gas trying to compensate during its two burns. By the time MIDAS 4 reached its intended transfer orbit, there was no attitude control gas left and the satellite could not be stabilized. It did manage to detect a Titan I launch from Cape Canaveral before one solar panel failed. A week into the mission, MIDAS 4 died when its batteries ran down. A month later, a similar control problem on SAMOS 4 resulted in the satellite failing to attain orbit. Investigation into the two failures found that the retrorocket package heat shields on both Atlas had broken off during launch, exposing the gyroscope package to aerodynamic heating. A transistor used in the roll output channel was also suspected to be at fault. It was replaced by a different type of transistor and the retrorocket heat shields were redesigned.