EYESAT A (AO-27)

NORAD 22825· COSPAR 1993-061C· Active satellite· Amateur Radio· SSO
Launch
Launched on Sep 26, 1993 from Ariane Launch Area 2, French Guiana aboard a Ariane 40.
Ariane 40 | SPOT 3
Live · TLE epoch 2026-07-25 10:59 UTC
Orbit class
SSO — Sun-Synchronous (LEO at 96–102° inclination)
Operator
United States Government
Country
United States
Manufacturer
Launched
Sep 26, 1993
Mass
Apogee
799 km
Perigee
787 km
Inclination
98.69°
Period
1.68 h

About EYESAT A (AO-27)

EYESAT A, also catalogued under the amateur radio designation AO-27 (AMSAT Oscar 27), is a small American satellite that has occupied a sun-synchronous low Earth orbit since its launch in September 1993. Assigned NORAD catalog number 22825 and international designator 1993-061C, it represents an early example of cooperative small-satellite development in the United States during the post-Cold War era of expanding access to space. More than three decades after its deployment, the spacecraft remains in orbit, a testament to the durability of well-placed low Earth orbit objects even as their operational lives remain uncertain.

Mission and Purpose

EYESAT A was developed under the auspices of the United States Government, though the specific operational details of its mission are not publicly recorded in standard satellite catalogs. The satellite is perhaps best known within the amateur radio community, where it earned the Oscar-27 designation through the AMSAT numbering system — a sequence traditionally reserved for satellites carrying amateur radio payloads or otherwise serving the amateur community. The "AO-27" callsign became the identifier through which many ground station operators around the world first made contact with the spacecraft, and it is under that name that many tracking enthusiasts continue to reference it today.

The "Eyesat" name suggested an imaging or observation role, and the satellite was part of a broader wave of small experimental payloads that rode piggyback on larger commercial or scientific launches during the early 1990s. This period saw a growing recognition that useful scientific and communications work could be accomplished by compact, relatively inexpensive satellites sharing a rocket with a primary payload. The specific instruments aboard EYESAT A and the precise nature of its data-return objectives are not confirmed in publicly available catalog records, so any detailed characterization of its science mission would be speculative.

What is well documented is the satellite's association with amateur radio operations. AO-27 was used by licensed operators to make voice and data contacts by transmitting signals up to the satellite and receiving the retransmitted downlink — a mode of operation that brought satellite communication within reach of hobbyists and educators worldwide. At its peak operational activity, the satellite served as a demonstration that small, low-cost spacecraft could provide real, usable communication links on a global scale.

Orbit and Tracking

EYESAT A occupies a sun-synchronous orbit (SSO), a specialized class of near-polar orbit in which the satellite's orbital plane precesses at a rate that keeps it aligned with the incoming sunlight from the Sun in a roughly constant geometry throughout the year. Sun-synchronous orbits are widely favored for Earth-observation and remote-sensing missions because they ensure that a given ground track is overflown at approximately the same local solar time on every pass, providing consistent illumination conditions for imaging or sensing instruments.

The satellite's current orbital parameters reflect a well-maintained altitude: an apogee of approximately 800 kilometers and a perigee of approximately 786 kilometers place it in a nearly circular orbit with a relatively modest eccentricity. This near-circular geometry is consistent with an intentional design choice, as circular orbits simplify ground contact scheduling and reduce variation in signal strength during passes. The orbital inclination of 98.7 degrees confirms the sun-synchronous character of the orbit — slightly retrograde relative to the equator, as is typical for such trajectories.

With an orbital period of approximately 100.6 minutes, EYESAT A completes roughly 14 to 15 revolutions around the Earth each day. At an inclination of 98.7 degrees, each successive ground track is shifted westward relative to the previous one, meaning the satellite sweeps over different portions of the globe on each orbit while still maintaining that regular solar geometry. From a tracking perspective, the combination of high inclination and low altitude makes the satellite accessible from ground stations at virtually any latitude, including high northern and southern latitudes where equatorial satellites never rise above the horizon.

The satellite has demonstrated remarkable orbital longevity. At altitudes between roughly 786 and 800 kilometers, atmospheric drag is extremely low, and without significant perturbations, objects in such orbits can remain aloft for very long periods — in some cases centuries. EYESAT A has shown no indication of imminent reentry, and as of the time of writing it remains catalogued as still in orbit.

Design and Operator

The satellite is listed as a payload operated by the United States Government. Beyond that attribution, the manufacturer of EYESAT A is not recorded in publicly available catalog data, and its mass is similarly unconfirmed in official sources. The absence of these details is not unusual for small experimental satellites of the era, particularly those developed through university partnerships, government research programs, or quasi-commercial arrangements that did not receive the same level of public documentation as flagship missions.

The "Eyesat" project was part of a broader philosophy that gained significant traction in the early 1990s: that smaller, faster, and cheaper spacecraft could complement — or in some cases replace — larger, more expensive platforms for certain mission types. This approach, sometimes described under the umbrella of the "faster, better, cheaper" ethos that was gaining currency in American civil and defense space programs at the time, encouraged the development of microsatellites and small payloads that could be bundled onto existing launch vehicles at relatively low cost.

EYESAT A was launched aboard an Ariane 4 rocket from the Guiana Space Centre located near Kourou in French Guiana, which serves as the primary launch facility for the European Ariane family of rockets. The launch took place on September 26, 1993, with EYESAT A riding as a secondary payload alongside a notable collection of co-passengers: SPOT-3, the French Earth-observation satellite that served as the primary payload, along with STELLA, Healthsat-2, KITSAT-2, and PoSAT-1. This cluster of secondary passengers illustrated the efficiency of rideshare launches and the international character of early 1990s small-satellite development, with payloads from France, the United Kingdom, South Korea, Portugal, and the United States all sharing a single rocket.

Significance and Current Status

The enduring legacy of EYESAT A lies largely in its role within the amateur satellite community. Under the AO-27 designation, it introduced a generation of radio operators to satellite-based communication, offering a practical and accessible platform that required no specialized ground infrastructure beyond a modest antenna and a radio transceiver. Educational institutions and amateur radio clubs used passes of AO-27 to demonstrate orbital mechanics in a tangible way, tracking the satellite's position in real time and making contact during the brief windows — typically ten minutes or less — when the spacecraft was above the local horizon.

The satellite also contributes, in a small way, to the broader picture of orbital population management and space situational awareness. Objects at EYESAT A's altitude are tracked continuously by ground-based radar networks, and its catalog entry (NORAD 22825) is updated regularly to reflect current two-line element sets. This continuous monitoring ensures that the satellite's position is known with sufficient accuracy for conjunction analysis — the process of assessing whether a tracked object poses a collision risk to operational spacecraft or other debris.

Whether EYESAT A's original mission systems remain functional is not confirmed in available records. Satellites of this class and vintage frequently outlast the operational lifetimes of their electronics, remaining physically intact in orbit long after active communication has ceased. Reports from the amateur community over the years have varied regarding the satellite's responsiveness, and its current operational status cannot be stated definitively based on catalog information alone.

How to Spot It

Despite its small size, EYESAT A is tracked precisely enough that dedicated satellite observers can attempt visual observations under the right conditions. At altitudes of roughly 786 to 800 kilometers, the satellite moves relatively quickly across the sky — a typical overhead pass lasts only a few minutes — and it will appear as a steadily moving point of light, distinguishable from aircraft by the absence of blinking navigation lights.

For the best chance of a visual sighting, observers should look during the twilight hours after sunset or before sunrise, when the ground below is in darkness but the satellite at altitude is still illuminated by direct sunlight. Passes where the satellite climbs to a high elevation above the horizon (approaching or exceeding 60 degrees) will generally be brightest and longest in duration. Satellite-tracking applications and websites — including the real-time tools available on this platform — can generate precise rise, culmination, and set times for any given observer location using current orbital elements. Because EYESAT A's orbit is sun-synchronous, observers at mid- to high latitudes may find that passes cluster predictably in the morning or evening sky depending on the season and the current orientation of the orbital plane.

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