Astronomy:Venera 11

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Short description: 1978 Soviet uncrewed spacecraft which successfully landed on Venus
Venera 11
Venus 12.jpg
Seal of Venera 11
OperatorSoviet Academy of Sciences
COSPAR ID1978-084A
1978-084D
SATCAT no.11020
11027
Mission durationTravel: 3 months and 16 days
Lander: 95 minutes
Spacecraft properties
Spacecraft4V-1
Spacecraft type4V-1 No. 360[1]
Bus4MV
Launch mass4,447.3 kg (9,805 lb)[1]
BOL mass4,715 kg (10,395 lb)
Landing mass760 kg (1,680 lb)
Dimensions2.7 m × 2.3 m × 5.7 m (8.9 ft × 7.5 ft × 18.7 ft)
Start of mission
Launch dateSeptember 9, 1978 (1978-09-09), 03:25:39 UTC[1]
RocketProton-K/D-1 8K82K
Launch siteBaikonur 81/23
End of mission
Last contactFebruary 1, 1980[1]
Orbital parameters
Reference systemGeocentric
RegimeLow Earth
Semi-major axis6,569 kilometers (4,082 mi)
Eccentricity0.0312
Perigee altitude177 kilometers (110 mi)
Apogee altitude205 kilometers (127 mi)
Inclination51.5°
Flyby of Venus
Spacecraft componentVenera 11 flight platform
Closest approach25 December 1978
Distance~35,000 kilometers (22,000 mi)
Venus lander
Spacecraft componentVenera 11 descent craft
Landing date25 December 1978, 03:24
Landing site [ ⚑ ] 14°S 299°E / 14°S 299°E / -14; 299 (near Phoebe Regio)
Venera
 

The Venera 11 (Russian: Венера-11 meaning Venus 11) was a Soviet uncrewed space mission which was part of the Venera program to explore the planet Venus. Venera 11 was launched on 9 September 1978 at 03:25:39 UTC.[2]

Separating from its flight platform on December 23, 1978 the lander entered the Venus atmosphere two days later on December 25 at 11.2 km/s. During the descent, it employed aerodynamic braking followed by parachute braking and ending with atmospheric braking. It made a soft landing on the surface at 06:24 Moscow Time (03:24 UT) on 25 December after a descent time of approximately 1 hour. The touchdown speed was 7 to 8 m/s.[3] Information was transmitted to the flight platform for retransmittal to Еarth until it moved out of range 95 minutes after touchdown.[4] Landing coordinates are [ ⚑ ] 14°S 299°E / 14°S 299°E / -14; 299.[3][5]

Flight platform

After ejection of the lander probe, the flight platform continued on past Venus in a heliocentric orbit. Near encounter with Venus occurred on December 25, 1978, at approximately 35,000 km altitude. The flight platform acted as a data relay for the descent craft for 95 minutes until it flew out of range and returned its own measurements on interplanetary space.[6]

Venera 11 flight platform carried solar wind detectors, ionosphere electron instruments and two gamma ray burst detectors – the Soviet-built KONUS and the France -built SIGNE 2. The SIGNE 2 detectors were simultaneously flown on Venera 12 and Prognoz 7 to allow triangulation of gamma ray sources. Before and after Venus flyby, Venera 11 and Venera 12 yielded detailed time-profiles for 143 gamma-ray bursts, resulting in the first ever catalog of such events. The last gamma-ray burst reported by Venera 11 occurred on January 27, 1980.

List of flight platform instruments and experiments:[7]

  • 30–166 nm Extreme UV spectrometer
  • Compound plasma spectrometer
  • KONUS Gamma-ray burst detector
  • SNEG Gamma-ray Burst detector
  • Magnetometer
  • 4 Semiconductor counters
  • 2 Gas-discharge counters
  • 4 Scintillation counters
  • Hemispherical proton telescope

The mission ended in February, 1980. Venera 11 is currently in heliocentric orbit, with perihelion of 0.69 AU, aphelion of 1.01 AU, eccentricity of 0.19, inclination of 2.3 degrees and orbital period of 284 days.

Lander

The lander carried instruments to study the temperature and atmospheric and soil chemical composition. A device called Groza was intended to search for lightning on Venus. Both Venera 11 and Venera 12 had landers with two cameras, each designed for color imaging, though Soviet literature does not mention them. Each failed to return images when the lens covers did not separate after landing due to a design flaw. The soil analyzer also failed. A gas chromatograph was on board to measure the composition of the Venus atmosphere, as well as instruments to study scattered solar radiation. Results reported included some evidence of lightning,[8] a high Ar36/Ar40 ratio, and the discovery of carbon monoxide at low altitudes.[4]

List of lander experiments and instruments:


See also

References

  1. ↑ 1.0 1.1 1.2 1.3 Siddiqi, Asif A. (2018). Beyond Earth: A Chronicle of Deep Space Exploration, 1958–2016. The NASA history series (second ed.). Washington, DC: NASA History Program Office. pp. 127–128. SP2018-4041. ISBN 978-1-62683-042-4. https://www.nasa.gov/sites/default/files/atoms/files/beyond-earth-tagged.pdf. 
  2. ↑ "Venera 11". http://solarsystem.nasa.gov/missions/profile.cfm?MCode=Venera_11. 
  3. ↑ 3.0 3.1 "Venera 11 Descent Craft Launch and Orbital Information". https://nssdc.gsfc.nasa.gov/nmc/spacecraft/displayTrajectory.action?id=1978-084D. 
  4. ↑ 4.0 4.1 "Venera 11 Descent Craft". https://nssdc.gsfc.nasa.gov/nmc/spacecraft/display.action?id=1978-084D. 
  5. ↑ "Venera 11 – Detail". https://solarsystem.nasa.gov/missions/venera-11/in-depth/. 
  6. ↑ "Venera 11". https://nssdc.gsfc.nasa.gov/nmc/spacecraft/display.action?id=1978-084A. 
  7. ↑ Mitchell, Don P.. "Drilling into the Surface of Venus". http://mentallandscape.com/V_Venera11.htm. 
  8. ↑ Lorenz, Ralph D. (2018-06-20). "Lightning detection on Venus: a critical review". Progress in Earth and Planetary Science 5 (1): 34. doi:10.1186/s40645-018-0181-x. ISSN 2197-4284. Bibcode: 2018PEPS....5...34L. 

External links



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