Missile Defense Alarm System

MIDAS Infrared Sensor

The Missile Defense Alarm System (MIDAS) was an American system of 12 early-warning satellites that provided limited notice of Soviet intercontinental ballistic missile launches between 1960 and 1966. Originally 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, which served as a successor 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 built at Thule, Greenland) 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 Scotland), 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.^[1] 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.^[1]

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.”^[2] 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.^[3] 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.^[4] 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.^[3]

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.^[5] 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.^[6]

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.^[7]

Implementing a complete system, estimated in 1959, was put at between $200 million and $600 million ($1.35 billion to $4 billion in 2006 dollars^[8]).^[9] 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.^[9]

In FY1959, ARPA spent US $22.8 million (inflation adjusted US$ 185.4 million in 2016) on MIDAS, and in FY1960, ARPA and Air Force a combined sum of US $94.9 million (inflation adjusted US$760.4 million in 2016).^[10]

Program summary and launch history

The MIDAS program officially 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 the launch went awry when the Agena's range safety destruct charges inadvertently activated during the coasting phase prior to staging, rupturing the Atlas's LOX tank dome and sending the satellite into the Atlantic Ocean.

On May 24, Midas 2 was orbited successfully but suffered a malfunction of the communications system which prevented ground controllers from sending commands to the satellite, and thus the mission had to be abandoned. 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. This time, one solar array failed to deploy and the satellite's batteries ran down after six orbits. Midas 4 (October 21) brought about further frustration when the Atlas's staging electrical disconnect malfunctioned during booster jettison, which caused the programmer to reset itself, and so the booster ended up putting the satellite into a useless orbit.

The MIDAS program was temporarily suspended at this point when a committee headed by ARPA director Jack Ruina recommended that no attempt at an operational missile early warning system be made until the Air Force demonstrated that it was a feasible concept at all. The committee found that program management of MIDAS was "awful" and at the current rate of success, "it would take ten years to develop an operational system". Late in 1961, President Kennedy issued an executive order placing all DoD space programs under strict secrecy, and so MIDAS was given the cover name "Program 461". The development time of the program was also lengthened to give more space to work out problems with the hardware.

Despite these changes, the failures kept coming. After a six-month gap, Midas 5 orbited on April 9, 1962. The Atlas lost roll control at T+186 seconds, however the satellite reached orbit successfully. Once there however, it experienced a massive power failure during the sixth orbit. Eight months later, Midas 6 lifted off (December 17) but never made it to orbit. A malfunction of the launcher equipment at SLC-3 1-2 damaged a hydraulic line on the Atlas booster, which eventually caused the B-2 engine to shut down. The booster drifted off its flight path and the Range Safety destruct command was sent 82 seconds into the launch.

Midas 7 was orbited successfully on May 9, 1963 and detected ten different US ICBM tests in its six-week mission, making the first successful detection of a missile launch from space. Then came another failure when Midas 8 (June 12) ended up in the Pacific Ocean when the Atlas's sustainer engine shut down 102 seconds into launch. Midas 9, six weeks later, was successful. Then there were no more launches in the Midas program for three years. Midas 10-12 were launched during five months in mid-1966, after which the program was officially ended and gave way to its successor, the Defense Support Program.

MIDAS and its successors were declassified in 1998.

MIDAS was at best a qualified success since like many early space programs, it was overly ambitious and had goals beyond the capabilities of contemporary technology. Problems included mistaking sunlight reflected from clouds as an enemy missile launch. The W-17 infrared sensor proved unable to detect the initial heat plume of a missile through the Earth's atmosphere, and only with the introduction of the W-37 sensor was a launch detected from orbit. Even with this success, the MiDAS system was hampered by unsuccessful launches that destroyed satellites and killed any hope of round-the-clock coverage of the Soviet Union. In addition, the lack of a continuous power source such as a nuclear reactor or solar panels meant that the satellites' batteries were exhausted after a few short weeks in orbit.

Though the MiDAS program itself failed to meet expectations, it paved the way for the eventual introduction of the Defense Support Program system of satellites that were first launched in the 1970s and provide early warning of missile launches today.

MiDAS launches

Mission chart from Astronautix^[11] and ^[12]

Photo gallery

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  MIDAS infrared sensor

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  MIDAS infrared sensor installation

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  RTS-1 infrared payload

See also

• Air Force Space Command
• Defense Support Program
• Missile defense
• SM-65 Atlas
• Space-Based Infrared System

References

United States reconnaissance satellites
IMINT	Photographic KH-1 Corona KH-2 Corona KH-3 Corona KH-4A Corona KH-4B Corona KH-5 Argon KH-6 Lanyard KH-7 Gambit KH-8 Gambit 3 KH-9 Hexagon KH-10 Dorian Electro-optical Samos KH-11 Kennan Misty Enhanced Imaging System Synthetic aperture radar Quill Lacrosse FIA Infrared
SIGINT	Low Earth orbit GRAB Poppy White Cloud Samos-F Highly elliptical orbit Jumpseat Trumpet Geosynchronous Earth orbit Canyon Magnum Mentor (Orion) Mercury Rhyolite/Aquacade Vortex
MASINT	Primary mission FORTE GPS DMSP Vela Secondary mission MIDAS DSP SBIRS STSS
Research and development	Primary mission MiTEx Secondary mission
Unknown	USA number USA-193