OAO 3 (COPERNICUS)
Copernicus, also known as OAO-3, was launched in 1972 as a joint U.S.-U.K. ultraviolet and X-ray astronomy observatory. It studied stars and the interstellar medium and helped establish high-resolution ultraviolet spectroscopy as a powerful astronomical tool.
Object identity
- NORAD ID
- 06153
- COSPAR ID
- 1972-065A
- Operator
- Not listed
- Country
- Not listed
- Launch date
- Not listed
Immediate discovery
Why this satellite matters
Spectroscopy turns light into a mathematical fingerprint. By measuring absorption and emission at specific wavelengths, scientists infer composition, temperature, velocity and physical conditions far beyond direct reach.
Understanding the mission
Science and engineering ideas
Spectroscopy turns light into a mathematical fingerprint. By measuring absorption and emission at specific wavelengths, scientists infer composition, temperature, velocity and physical conditions far beyond direct reach.
Mission
Mission and purpose
The current public orbital catalog identifies this object, but verified mission-specific information may be limited. TransitSatellite will expand this page when authoritative information is available.
- Spectroscopy turns light into a mathematical fingerprint. By measuring absorption and emission at specific wavelengths, scientists infer composition, temperature, velocity and physical conditions far beyond direct reach.
Design
Engineering
Spectroscopy turns light into a mathematical fingerprint. By measuring absorption and emission at specific wavelengths, scientists infer composition, temperature, velocity and physical conditions far beyond direct reach.
Real orbital values
The mathematics
The current two-line element set reports approximately 14.601 revolutions per day. Dividing 1,440 minutes by that value gives an estimated orbital period of 98.6 minutes.
Period
98.6 min
Representative speed
27,029 km/h
Representative altitude
700 km
Inclination
35.01°
Launch record
Launch and deployment
Copernicus launched on 21 August 1972 aboard an Atlas-Centaur from Cape Canaveral.
Orbit
LEO orbit explained
Low Earth orbit is the region closest to Earth used by most crewed spacecraft, many science missions, Earth-observation satellites, and large constellations. Objects move quickly and commonly complete an orbit in roughly 90 to 130 minutes.
LEO can provide detailed Earth views, lower communications delay, and easier access than higher orbits, but it covers less area per spacecraft and is more affected by atmospheric drag.
Live TransitSatellite experience
See OAO 3 (COPERNICUS) moving now
Open the live tracker to view its current calculated position, trajectory, orbital information, visibility tools, and Save and Share controls.
Learning
Questions to explore
- What can an orbit tell us before the mission is fully identified?
- Why are stable catalog identifiers important?
Evidence
Sources and data notes
Current identity and orbital elements come from CelesTrak’s public GP data. Calculated orbit values are derived from the current TLE and may change after catalog updates. Mission-history claims are added separately and require authoritative sources.
Catalog updated
Sep 17, 2026, 8:52 AM UTC
Story review
1970-01-01T00:00:00.000Z
