 | |
| Mission type | Astrophysics |
|---|---|
| Operator | ESRO |
| COSPAR ID | 1968-041A[1] |
| SATCATno. | 03233 |
| Spacecraft properties | |
| Launch mass | 89.8 kilograms (198 lb) |
| Start of mission | |
| Launch date | 17 May 1968, 02:06:00 (1968-05-17UTC02:06Z) UTC[2][1] |
| Rocket | Scout B |
| Launch site | VandenbergSLC-5 |
| End of mission | |
| Decay date | 8 May 1971, shortly after 03:00 UT |
| Orbital parameters | |
| Reference system | Geocentric |
| Regime | Low Earth |
| Perigee altitude | 326 kilometres (203 mi)[2] |
| Apogee altitude | 1,086 kilometres (675 mi)[2] |
| Inclination | 97.2 degrees[2] |
| Period | 98.9 minutes[2] |
| Epoch | 16 May 1968, 22:09:00 UTC[3] |
ESRO-2B orIris (International Radiation Investigation Satellite; sometimesIris 2[4]) or sometimesESRO II (orESRO 2), was a Europeanastrophysical spin-stabilised researchsatellite which was launched in 1968. Operated by theEuropean Space Research Organisation, ESRO 2B madeastronomical surveys primarily inx-ray andsolar particles detectors.[5]
ESRO-2B was an 89 kg (196 lb) cylindricalspacecraft with a length of 85 cm and a diameter of 76 cm. On 10 December 1968 (approx 195 days since mission start) the on-boardtape recorder suffered a mechanical failure. This effectively ended the two X-ray experiments as they did not provide any significant data return from then on. Other experiments could still be operated through ground radio links.
ESRO-2B was launched on aScout B rocket into ahighly ellipticalnear-polar orbit on 17 May 1968. Its predecessor satellite,ESRO-2A (sometimesIris 1) failed to reach orbit on 29 May 1967,[6] launching on a Scout B rocket fromVandenberg AFB SLC-5. The cause of failure was malfunction of the third stage of the rocket, preventing the satellite from reaching orbit. ESRO-2A was similar to ESRO-2B except it weighed a little less (74 kg).[4]
Spin-stabilised, ESRO-2B had a spin rate of approximately 40rpm and re-entered Earth's atmosphere on 8 May 1971 after completing 16,282 orbits.[4]
Seven instruments were carried aboard EROS 2B[2] designed to detect high energy cosmic rays, determine the total flux of solar X-rays and to measureVan Allen belt protons andcosmic ray protons.[5] While designed for solar observations ESRO-2B is credited with the detection of X-rays from non-solar sources.[2] The instruments were: