Project Echo was the first passive communications satellite experiment. Each of the two American spacecraft, launched in 1960 and 1964, were metalized balloon satellites acting as passive reflectors of microwave signals. Communication signals were transmitted from one location on Earth and bounced off the surface of the satellite to another Earth location.[1]
![]() Echo 1 sits fully inflated at a Navy hangar in Weeksville, North Carolina. | |
Names | ECHO 1 NASA A-11 |
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Mission type | Communications |
Operator | NASA |
Harvard designation | 1960 Alpha 11 |
COSPAR ID | 1960-009A |
SATCAT no. | 00049 |
Mission duration | 7.75 years (achieved) |
Spacecraft properties | |
Bus | ECHO |
Manufacturer | Bell Labs |
Launch mass | 180 kg (400 lb) |
Dimensions | 30.48 m (100.0 ft) diameter sphere when inflated |
Start of mission | |
Launch date | 12 August 1960, 03:39:43 GMT |
Rocket | Thor DM-19 Delta (Thor 270 / Delta 2) |
Launch site | Cape Canaveral, LC-17A |
Contractor | Douglas Aircraft Company |
End of mission | |
Decay date | 25 May 1968 |
Orbital parameters | |
Reference system | Geocentric orbit |
Regime | Low Earth orbit |
Perigee altitude | 1,524 km (947 mi) |
Apogee altitude | 1,684 km (1,046 mi) |
Inclination | 47.2° |
Period | 118.3 minutes |
![]() Echo 2 undergoing tensile stress test in a dirigible hangar at Weeksville, North Carolina. | |
Names | NASA A-12 |
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Mission type | Communications |
Operator | NASA |
COSPAR ID | 1964-004A |
SATCAT no. | 00740 |
Mission duration | 5.5 years (achieved) |
Spacecraft properties | |
Bus | ECHO |
Manufacturer | Bell Labs |
Dimensions | 41 m (135 ft) diameter sphere when inflated |
Start of mission | |
Launch date | 25 January 1964, 13:59:04 GMT |
Rocket | Thor-Agena B (Thor 397 / Agena 6301 / TA-2) |
Launch site | Vandenberg, LC-75-1-1 (SLC-2E) |
Contractor | Douglas Aircraft Company (Thor) Lockheed Martin (Agena) |
End of mission | |
Decay date | 7 June 1969 |
Orbital parameters | |
Reference system | Geocentric orbit |
Regime | Low Earth orbit |
Perigee altitude | 1,029 km (639 mi) |
Apogee altitude | 1,316 km (818 mi) |
Inclination | 81.5° |
Period | 108.95 minutes |
The first transmissions using Echo were sent from Goldstone, California to Holmdel, New Jersey on 12 August 1960. The last Echo satellite deorbited and burned up in the atmosphere on 7 June 1969.[2]
The concept of using orbital satellites to relay communications predated space travel, first being advanced by Arthur C. Clarke in 1945. Experiments using the moon as a passive reflecting way station for messages began as early as 1946.[3] With the launching of Sputnik 1, Earth's first artificial satellite, in 1957, interest quickly developed in orbiting communications satellites.
In July 1958, at a US Air Force sponsored meeting on communications satellites, Bell Telephone Laboratories engineer John R. Pierce put forth a presentation on passive satellite relay, describing how a reflective orbiting body could be used to bounce transmissions from one point on the Earth to another. William H. Pickering, director of Jet Propulsion Laboratory (JPL), also attended the conference and suggested that JPL facilities, specifically a 26 m (85 ft) diameter polar-mounted antenna installed near Goldstone Dry Lake in the Mojave Desert, might be used as a ground facility for experiments with such a satellite.[4]
In October 1958, Pierce, along with fellow Bell engineer Rudolf Kompfner, designed an experiment to observe atmospheric refractive effects using reflective balloon satellites. Believing the experiment would advance research toward transoceanic communications via satellites, the two engineers presented a paper advocating for the launch of balloon satellites to be used as passive communications reflectors to the National Symposium on Extended Range and Space Communication on 6 and 7 October 1958.
That same month, the National Aeronautics and Space Administration (NASA) was formed, and two months later JPL was transferred from the United States Army to the new agency. Project Echo, NASA's first communications satellite project, was officially laid out in a 22 January 1959 meeting with representatives from NASA, JPL, and Bell Telephone Laboratories setting the initial launch for September 1959.[5]
Project Echo was a pathfinder mission with the objective of testing new technologies and preparing for future missions. Spaceflight engineers used Echo to prove new ideas and test limits in aerodynamics, satellite shape and size, construction materials, temperature control and satellite tracking.[6] Echo was designed as an experiment to demonstrate the potential of satellite communications, not to function as a global communications system.
Echo was designed, approved and built with the following objectives:[5]
All of these objectives were accomplished with Project Echo. Further experiments used the satellite to engage a two-way telephone conversation on 15 August 1960 and to relay a live television transmission in April 1962.
Two ground stations were used for testing Project Echo. The Goldstone facility located at Goldstone Dry Lake in the Mojave Desert, California and the Holmdel facility located at Holmdel, New Jersey. Both sites used separate antennas for transmitting and receiving. West-to-east transmissions were sent from Goldstone by a 26 m (85 ft) dish antenna built for Project Echo by JPL. The signals were received at Holmdel by a 6 × 6 m (20 × 20 ft) aperture horn-reflector antenna. Horn antennas were known to have low-noise properties. A transmission frequency of 2390 megahertz was selected, as this was the planned frequency band for future satellite experiments. East-to-west transmissions were sent from Holmdel using a 18 m (59 ft) diameter parabolic antenna and received at Goldstone using the existing Pioneer program antenna. A transmission frequency of 960.05 megahertz was used for westbound communications because the JPL receiver was already tuned to this frequency from the Pioneer lunar program.[5]
Satellite acquisition and tracking were accomplished by three methods: optical, digital slave, and automatic radar. Optical tracking was the easiest method but could only be used at night when the Sun illuminated the satellite. Broad and narrow field telescopes with a television camera were mounted to the structure of the antenna at each site. The camera images were displayed to a servo operator who would control the position of the antenna to track the satellite. When optical tracking could not be used, a computer system called digital slave could acquire and track Echo. Digital slave worked by receiving primary tracking data from the NASA Minitrack network of stations. The computer would then issue antenna-pointing commands to control the antenna. The third tracking method was a continuous-wave radar subsystem. Radar was not suitable for acquisition of the satellite, but once Echo was acquired by optical, or digital slave, radar signals could be used to automatically maintain tracking.[5]
The Echo spacecraft (Echo 1, Echo 1A, and Echo 2) were large thin skinned spheres that were inflated in orbit after leaving the atmosphere. These balloon satellites were approximately 30 m (98 ft) in diameter with a thin skin made of Mylar (a trade name for stretched polyethylene terephthalate or BoPET), and were built by Gilmore Schjeldahl's G.T. Schjeldahl Company in Northfield, Minnesota. The satellites functioned as a reflector, not a transceiver; after being placed in low Earth orbit, signals could be sent from a ground station, reflected by its surface, and returned to Earth.[7]
As its shiny surface was also reflective in the range of visible light, Echo was easily visible to the unaided eye over most of the Earth. The spacecraft was nicknamed a "satelloon" by those involved in the project (a portmanteau combining satellite and balloon). It was used to redirect transcontinental and intercontinental telephone, radio, and television signals.[8] During the latter portion of its life, it was used to evaluate the technical feasibility of satellite triangulation.
Echo 1 was 30 m (98 ft) in diameter, had a non-rigid skin made of 12.7 μm (0.00050 in)-thick Mylar, and had a total mass of 180 kg (400 lb), weighing 71 kg (157 lb) at launch. During ground inflation tests, 18,000 kg (40,000 lb) of air were needed to fill the balloon, but while in orbit, several pounds of gas were all that was required to fill the sphere. To address the problem of meteorite punctures and keep the sphere inflated, Echo 1 included a 15.12 kg (33.3 lb) make-up gas system using two types of sublimating powders – 9.1 kg (20 lb) of anthraquinone and 4.6 kg (10 lb) of benzoic acid.[9] It also had 107.9 MHz telemetry beacons, powered by five nickel-cadmium batteries that were charged by 70 solar cells mounted on the balloon. The spacecraft was useful to the calculation of atmospheric density and solar pressure, due to its large area-to-mass ratio.[8]
Echo 2 was a 41.1 m (135 ft)-diameter balloon satellite, the last launched by Project Echo. A revised inflation system was used for the balloon, to improve its smoothness and sphericity. Echo 2's skin was rigidizable, unlike that of Echo 1. Therefore, the balloon was capable of maintaining its shape without a constant internal pressure; a long-term supply of inflation gas was not needed, and it could easily survive strikes from micrometeoroids. The balloon was constructed from a 9 μm (0.00035 in)-thick mylar film sandwiched between and bonded with two layers of 4.5 μm (0.00018 in)-thick aluminum foil.[10] It was inflated to a pressure that caused the metal layers of the laminate to plastically deform slightly, while the polymer was still in the elastic range. This resulted in a rigid and very smooth spherical shell. A beacon telemetry system provided a tracking signal, monitored spacecraft skin temperature between −120 and +16 °C (−184 and 61 °F), and measured the internal pressure of the spacecraft between 0.00005 mm of mercury and 0.5 mm of mercury, especially during the initial inflation stages. The system consisted of two beacon assemblies powered by solar cell panels and had a minimum power output of 45 mW at 136.02 MHz and 136.17 MHz.[11]
Five suborbital ballistic tests to determine whether the launch, deploy, and expansion mechanisms would work were flown using the Shotput test vehicle. The first Shotput flew at 5:40 pm on 27 October 1959. Shotput 1 successfully delivered the Echo prototype to the desired altitude, but a small amount of residual gas in the folds of the balloon violently expanded, bursting the test article. People up and down the Atlantic coast witnessed what looked like distant fireworks as thousands of pieces of shredded Mylar reflected sunlight in a display that lasted for about 10 minutes.[6] Four more Shotput tests were flown on 16 January, 27 February, 1 April, and 31 May 1960.[12]
On 13 May 1960, the first attempt to orbit an Echo satellite was made. The mission, which was also the maiden voyage of the Thor-Delta launch vehicle, failed before deployment of the payload. Echo 1 lifted off from Cape Canaveral's LC-17A, and the Thor stage performed properly, but during the coasting phase, the attitude control jets on the unproven Delta stage failed to ignite, sending the payload into the Atlantic Ocean instead of into orbit.
On 12 August 1960, Echo 1A (commonly referred to as Echo 1) was successfully put into an orbit of 944 to 1,048 mi (1,519 to 1,687 km) by another Thor-Delta.[2][13] A microwave transmission from the JPL Goldstone facility in California, was relayed by the satellite to Bell Laboratories in Holmdel, New Jersey, that same day.[8] It was originally expected that Echo 1A would not survive long after its fourth dip into the atmosphere in July 1963, although estimates allowed the possibility that it would continue to orbit until 1964 or beyond.[8] It ended up surviving much longer than expected, and finally reentered Earth's atmosphere and burned up on 24 May 1968.
On 25 January 1964, Echo 2 was launched on a Thor Agena launch vehicle. In addition to passive communications experiments, it was used to investigate the dynamics of large spacecraft and for global geometric geodesy. Since it was larger than Echo 1A and orbiting in a near-polar orbit, Echo 2 was conspicuously visible to the unaided eye over all of the Earth. It reentered Earth's atmosphere and burned up on 7 June 1969.
Both Echo 1A and Echo 2 experienced a solar sail effect due to their large size and low mass.[14] Later passive communications satellites, such as OV1-08 PasComSat, solved the problems associated with this by using a grid-sphere design instead of a covered surface. Later yet, NASA abandoned passive communications systems altogether, in favor of active satellites.
Project Echo facilitated the first successful satellite transmission and first two way communications between the JPL Goldstone facility and Bell Telephone Laboratories facility in Holmdel, New Jersey. Other groups participated in experiments including the Collins Radio Company and the Naval Research laboratory. Because Echo was only a passive system, it was primarily useful in demonstrating the future potential of satellite communications and became obsolete before it deorbited in 1968. Echo was most known to the general public for its visibility as it could be seen at night with the naked eye.[5]
The Echo satellite program also provided the astronomical reference points required to accurately locate Moscow. This improved accuracy was sought by the U.S. military for the purpose of targeting intercontinental ballistic missiles.[15]
The large horn antenna at Holmdel constructed by Bell Labs for the Echo project was later used by Arno Penzias and Robert Woodrow Wilson for their Nobel Prize-winning discovery of the cosmic microwave background radiation.[16]
On 15 December 1960, the U.S. Post Office issued a postage stamp depicting Echo 1.
The observed variations of the Echo orbit - due primarily to the effects of the pressure of sunlight - are in excellent agreement with our theoretical results. The perigee altitude has an oscillation of large amplitude (approximately equal to 600 km (370 mi)) and long period (approximately equal to 300 days), which has a decisive influence on the lifetime of Echo I. Our present best estimate is that the balloon will perish in the summer of 1963.
← 1959 · Orbital launches in 1960 · 1961 → | |
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Discoverer 9 | Discoverer 10 | Midas 1 | Pioneer 5 | S-46 | TIROS-1 | Transit 1B · Solrad mass simulator | Discoverer 11 | Luna E-3 No.1 | Luna E-3 No.2 | Echo 1 | Korabl-Sputnik 1 | Midas 2 | Transit 2A · SOLRAD 1 | Discoverer 12 | Vostok-1K No.1 | Discoverer 13 | Echo 1A | Courier 1A | Discoverer 14 | Korabl-Sputnik 2 | Discoverer 15 | Pioneer P-30 | Courier 1B | Mars 1M No.1 | Samos 1 | Mars 1M No.2 | Discoverer 16 | Explorer 8 | Discoverer 17 | TIROS-2 | Transit 3A · SOLRAD 2 | Korabl-Sputnik 3 | Explorer S-56 | Discoverer 18 | Pioneer P-31 | Discoverer 19 | Vostok-1K No.4 | |
Payloads are separated by bullets ( · ), launches by pipes ( | ). Uncatalogued launch failures are listed in italics. Payloads deployed from other spacecraft are denoted in brackets. |
← 1963 · Orbital launches in 1964 · 1965 → | |
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Poppy 3 · GGSE-1 · SOLRAD 7A · SECOR 1 | OPS 3367A · OPS 3367B | Relay 2 | Echo 2 | Jupiter Nosecone | Elektron 1 · Elektron 2 | Ranger 6 | OPS 3444 | Zond 3MV-1 No.2 | Kosmos 25 | OPS 2423 | OPS 3722 | OPS 3435 | Kosmos 26 | BE-A | Luna E-6 No.6 | OPS 3467 | Kosmos 27 | Ariel 2 | Zond 1 | Kosmos 28 | Gemini 1 | Polyot 2 | Luna E-6 No.5 | Transit 5BN-3 · Transit 5E-4 | OPS 3743 | Kosmos 29 | OPS 2921 | Kosmos 30 | OPS 3592 | Apollo AS-101 | OPS 4412 | OPS 3483 | Molniya-1 No.2 | Kosmos 31 | Kosmos 32 | OPS 3236 | OPS 4467A · OPS 4467B | OPS 3754 | Kosmos 33 | ESRS | Atlas-Centaur 3 | Kosmos 34 | OPS 3395 | OPS 3684 · OPS 4923 | Elektron 3 · Elektron 4 | OPS 3491 | Kosmos 35 | Vela 2A · Vela 2B · ERS-13 | Ranger 7 | Kosmos 36 | OPS 3042 | Kosmos 37 | OPS 3802 · OPS 3216 | Kosmos 38 · Kosmos 39 · Kosmos 40 | Syncom 3 | OPS 2739 | Kosmos 41 | Kosmos 42 · Kosmos 43 | Kosmos 44 | Titan 3A-2 | OGO-1 | Kosmos 45 | OPS 3497 | Apollo AS-102 | OPS 4262 | Kosmos 46 | Explorer 21 | OPS 3333 | Kosmos 47 | OPS 5798 · Dragsphere 1 · Dragsphere 2 | OPS 4036 | Explorer 22 | Voskhod 1 | Kosmos 48 | OPS 3559 | Strela-1 No.6 · Strela-1 No.7 · Strela-1 No.8 | OPS 4384 · OPS 5063 | Kosmos 49 | Kosmos 50 | OPS 5434 | OPS 3062 | Mariner 3 | Explorer 23 | OPS 3360 | Explorer 24 · Explorer 25 | Mariner 4 | Zond 2 | DS-2 No.2 | OPS 4439 | Kosmos 51 | Titan 3A-1 | Surveyor Mass Model | OPS 6582 · Transit 5E-5 | San Marco 1 | OPS 3358 | Explorer 26 | OPS 3762 | |
Payloads are separated by bullets ( · ), launches by pipes ( | ). Crewed flights are indicated in underline. Uncatalogued launch failures are listed in italics. Payloads deployed from other spacecraft are denoted in brackets. |