Skip to main content

Come analyze HEASARC, IRSA, and MAST data in the cloud! The Fornax Initiative is now welcoming all interested beta users.


The Salyut 4 Space Station


Line drawing of Salyut 4

The Salyut 4 space station was launched on 26 December 1974. It was in an orbit with an apogee of 355 km and a perigee of 343 km. The orbital period was 91.3 minutes. It was at an inclination of 51.6 degrees. The X-ray telescope was switched on on 15 January 1975. Salyut-4 reentered the Earth’s atmosphere on 2 February 1977.

Mission Characteristics

Lifetime
Jan 1975–Feb 1977
Special Features
Space station launched and operated by the Soviet Union, which included an X-ray telescope

Payload

Salyut 4 X-ray instrument (Filin telescope)

Energy Range
0.2–10 keV
Effective Area
37 cm2 0.2–2 keV
450 cm2 2–10 keV
Field of View
3° × 10° (FWHM) collimator
The Salyut-4 X-ray instrument, often called the Filin telescope, consisted of four gas flow proportional counters, three of which have a total detection surface of 450 cm2 in the energy range 2–10 keV, and one of which has an effective surface of 37 cm2 for the range 0.2–2 keV. The field of view was limited by a slit collimator. The instrumentation also included optical sensors which were mounted on the outside of the station together with the X-ray detectors, and power supply and measurement units which were inside the station. Ground based calibration of the detectors is considered along with in-flight operation in three modes: inertial orientation, orbital orientation, and survey. Data could be collected in 4 energy channels: 2–3.1 keV, 3.1–5.9 keV, 5.9–9.6 keV, and 2–9.6 keV in the larger detectors. The smaller detector had discriminator levels set at 0.2 keV, 0.55 keV, and 0.95 keV.

Science Highlights

Among others, observations of Sco X-1, Cir X-1, Cyg X-1, and A0620-00 were published from the Filin data. A highly variable low energy (0.6–0.9 keV) flux was detected in Sco X-1. Cir X-1 was not detected at all during a 5 July 1975 observation, providing an upper limit on the emission of 3.5 × 10-11 erg/cm2/s in the 0.2–2.0 keV range. Cyg X-1 was observed on several occasions. Highly variable flux, in both the time and energy domains, was observed.