Venera 8 (russian: Венера-8 meaning ''Venus 8'') was a probe in the Soviet Venera program for the exploration of Venus and was the second robotic space probe to conduct a successful landing on the surface of Venus. Venera 8 was a Venus atmospheric probe and lander. Its instrumentation included temperature, pressure, and light sensors as well as an altimeter, gamma ray spectrometer, gas analyzer, and radio transmitters.

Journey to Venus

The spacecraft took 118 days to reach Venus with one mid-course correction on 6 April 1972, separating from the bus (which contained a cosmic ray detector, solar wind detector, and ultraviolet

spectrometer A spectrometer () is a scientific instrument used to separate and measure spectral components of a physical phenomenon. Spectrometer is a broad term often used to describe instruments that measure a continuous variable of a phenomenon where the ...

) and entering the atmosphere on 22 July 1972 at 08:37 UT. A refrigeration system attached to the bus was used to pre-chill the descent capsule's interior prior to atmospheric entry in order to prolong its life on the surface. Descent speed was reduced from 41,696 km/h to about 900 km/h by aerobraking. The 2.5 meter diameter parachute opened at an altitude of 60 km.

Descent

Venera 8 transmitted data during the descent. A sharp decrease in illumination was noted at 35 to 30 km altitude and wind speeds of less than 1 m/s were measured below 10 km. Venera 8 landed at 09:32 UT in what is now called

Vasilisa Regio This is a list of geological features on Venus. Venus is the second planet from the Sun. Venus is classified as a terrestrial planet and it is sometimes called Earth's "sister planet" owing to their similar size, gravity, and bulk composition (Venu ...

, within 150 km radius of , in sunlight, about 500 km from the morning

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. The lander mass was 495 kg.

Lander

The lander continued to send back data for 50 minutes, 11 seconds after landing before failing due to the harsh surface conditions. The probe confirmed the earlier data on the high Venus surface temperature and pressure (470 degrees Celsius, 90 atmospheres) returned by Venera 7, and also measured the light level as being suitable for surface photography, finding it to be similar to the amount of light on Earth on an overcast day with roughly 1 km visibility. Venera 8's photometer measurements showed for the first time that the Venusian clouds end at a high altitude, and the atmosphere was relatively clear from there down to the surface. The on-board gamma ray spectrometer measured the uranium/ thorium/ potassium ratio of the surface rock, indicating it was similar to Alkali basalt.

Payload experiments

* Temperature and pressure sensors - ITD * Accelerometer - DOU-1M * Cadmium sulfide Photometers - IOV-72 * Ammonia analyser – IAV-72 * Gamma ray

– GS-4 * Radar altimeter

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* Radio Doppler experiment

References

External links