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Cos-B: 30 Years On

Cos-B: 30 Years On

17 August 2005

On 9 August 1975 ESA's first scientific satellite, Cos-B, was launched. Cos-B was ESA's first foray into producing a spacecraft with a single payload: a high-energy gamma-ray telescope. The mission was a remarkable success and returned the first detailed observations of gamma-ray emission from within our galaxy.

The Last Recorded Gamma-Ray

Just three days after launch, 12 August the first data was returned and on 17 August 1975 routine science operations commenced. The mission had a 1-year design life, yet, like many missions, survived far in excess of this and was finally deactivated on 25 April 1982 when the attitude control gas finally ran out.

The final detection was recorded for posterity and signed by all project members present in the control room at the time including: project scientist Kevin Bennett, who now works on ESA's Planck mission, and Giovanni Bignami, the current chair of the Space Science Advisory Committee.

Launch and Orbit

The spacecraft was launched on a Delta 2913 rocket from the Vandenburg Air Force Western Test Range in California. The orbit of Cos-B was roughly 100 000 km with a period of 37 hours. This eccentric orbit was chosen to ensure that for most of the time the satellite was outside the Earth's radiation belts. This led to an efficient viewing programme at the price of high cosmic-ray background.

The orbital plane was inclined at roughly 90 degrees to the Earth's equator and the argument of perigee was placed in the fourth quadrant to ensure that the satellite was in sight of one of the ESTRACK ground stations.

The Spacecraft

Cos-B was configured as a cylinder 1.40 m in diameter and 1.13 m long, with the main experiment package occupying the central region. The total height, including antennas and other structural supports, was 1.71 m. The total mass at launch was 278 kg, of which the experiment was 118 kg.

The satellite was spin-stabilised at about 10 rpm about its axis of symmetry, which coincided with the optical axis of the gamma-ray detector. Sun and Earth sensors were used for attitude measurements from which the pointing direction could be reconstituted with a precision of about 0.5 deg. The timing accuracy was 0.5 ms or better.

Cos-B Spark Chamber

The Cos-B carried a single large experiment, the design and provision of which was the responsibility of a group of research laboratories known as the Caravane Collaboration. The gamma-ray detector features a magnetic-core, wire-matrix spark chamber, SC, triggered by a three-element (B1, B2, C) scintillation counter telescope. For gamma-ray selection a plastic scintillator guard counter (A) surrounding these two units is placed in anti-coincidence to reject triggers due to incident charged particles. Beneath the telescope is an energy calorimeter (E) consisting of a caesium iodide scintillator, which absorbs the secondary particles produced by the incident photons.

Science Summary

The main achievement of Cos-B was the 2CG catalogue of point sources. This early catalogue was based on the selected data from only 30 observations made during the first three years of operation. It was searched for the presence of discrete, or localised, sources of gamma radiation under the assumption of a flat, or smoothly varying background. Thus 25 candidate sources were reported. In view of the availability of the total mission data as well as more realistic background models, the interpretation of these enhancements has evolved rapidly.

Most of the observations performed with Cos-B were devoted to the study of the galactic disc. A detailed and complete intensity map of the galaxy seen in the light of gamma radiation is shown below.

Map of the Milky Way

Light curves and spectra were derived for both the Crab and Vela pulsars. A major discovery resulted from comparing the light curves of the Vela and Crab pulsars for the different epochs. It is seen that while during several years the light curve of Vela remains unchanged the Crab's light curve varies.

Geminga, or 2CG195+4 is one of the brightest sources in the 2CG catalogue. First discovered by SAS2, the source stands out brightly in a low background region of the galactic disc. As a consequence of the favourable signal to noise, an accurate spectrum was determined.

The quasar 3C273 was subjected to repeated observations and the source appeared in three independent data sets. The combined data yielded an energy spectrum, which when combined with data from other wavelengths demonstrated for the first time that the luminosity of 3C273 peaks in the gamma-ray region.


High-energy astrophysics has played a fundamental role in the activities of the Agency with EXOSAT, XMM-Newton and the INTEGRAL mission all building on the work of COS-B.

Last Update: 1 September 2019
14-Jun-2024 18:18 UT

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