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ESRO 2B
Research satellite
Research satellite
| Field | Value |
|---|---|
| name | ESRO 2B |
| image | Esro-2b small.gif |
| mission_type | Astrophysics |
| operator | ESRO |
| COSPAR_ID | 1968-041A |
| SATCAT | 03233 |
| launch_mass | 89.8 kg |
| launch_date | UTC |
| launch_rocket | Scout B |
| launch_site | Vandenberg SLC-5 |
| last_contact | |
| decay_date | 8 May 1971, shortly after 03:00 UT |
| orbit_epoch | 16 May 1968, 22:09:00 UTC |
| orbit_reference | Geocentric |
| orbit_regime | Low Earth |
| orbit_periapsis | 326 km |
| orbit_apoapsis | 1086 km |
| orbit_inclination | 97.2 degrees |
| orbit_period | 98.9 minutes |
| apsis | gee |
ESRO-2B or Iris (International Radiation Investigation Satellite; sometimes Iris 2
Spacecraft
ESRO-2B was an 89 kg cylindrical spacecraft with a length of 85 cm and a diameter of 76 cm. On 10 December 1968 (approx 195 days since mission start) the on-board tape 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 a Scout B rocket into a highly elliptical near-polar orbit on 17 May 1968. Its predecessor satellite, ESRO-2A (sometimes Iris 1) failed to reach orbit on 29 May 1967, launching on a Scout B rocket from Vandenberg 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).
Spin-stabilised, ESRO-2B had a spin rate of approximately 40 rpm and re-entered Earth's atmosphere on 8 May 1971 after completing 16,282 orbits.
Instruments
Seven instruments were carried aboard EROS 2B designed to detect high energy cosmic rays, determine the total flux of solar X-rays and to measure Van Allen belt protons and cosmic ray protons. While designed for solar observations ESRO-2B is credited with the detection of X-rays from non-solar sources. The instruments were:
- Monitor of Energetic Particle Flux
- Solar and Van Allen Belt Protons
- Solar and Galactic Alpha Particles and Protons
- Primary Cosmic Ray Electrons
- Hard Solar X-rays
- Soft Solar X-rays
- Flux and Energy Spectra of Solar and Galactic Cosmic Ray Particles
References
References
- "NASA – NSSDCA – Spacecraft – Details".
- "ESRO 2B". NASA.
- "NASA – NSSDCA – Spacecraft – Trajectory Details".
- "ESRO 2B: May – December 1968". University of Indiana.
- "NASA – NSSDCA – Spacecraft – Details".
- "ESRO 2A, 2B (Iris 1, 2)". Gunters Space Page.
This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page.
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