Venera 9
| Mission type | Venus orbiter/lander |
|---|---|
| COSPAR ID |
Orbiter: 1975-050A Lander: 1975-050D |
| SATCAT № |
Orbiter: 7915 Lander: 100000 |
| Spacecraft properties | |
| Spacecraft | 4V-1 No.660 |
| Manufacturer | Lavochkin |
| Launch mass | 2,015 kilograms (4,442 lb) |
| Power | 10000Template:Missing unit |
| Start of mission | |
| Launch date | June 8, 1975, 02:38:00 UTC[1] |
| Rocket | Proton-K/D[1] |
| Launch site | Baikonur 81/24 |
| End of mission | |
| Last contact |
Lander: October 22, 1975 Orbiter: 25 December 1975 |
| Orbital parameters | |
| Reference system | Cytherocentric |
| Eccentricity | 0.89002 |
| Pericytherion | 7,625 kilometres (4,738 mi) |
| Apocytherion | 118,072 kilometres (73,367 mi) |
| Inclination | 29.5 degrees |
| Period | 48.3 hours |
| Venus orbiter | |
| Spacecraft component | Orbiter |
| Orbital insertion | October 20, 1975 |
| Venus lander | |
| Spacecraft component | Lander |
| Landing date | October 22, 1975, 05:13 UTC |
| Landing site | 31°01′N 291°38′E / 31.01°N 291.64°E |
Venera 9 (Russian: Венера-9 meaning Venus 9), manufacturer's designation: 4V-1 No. 660,[2] was a USSR unmanned space mission to Venus. It consisted of an orbiter and a lander. It was launched on June 8, 1975 02:38:00 UTC and had a mass of 4,936 kg (10,884 lb).[3] The orbiter was the first spacecraft to orbit Venus, while the lander was the first to return images from the surface of another planet.[4]
Orbiter
The orbiter consisted of a cylinder with two solar panel wings and a high gain parabolic antenna attached to the curved surface. A bell-shaped unit holding propulsion systems was attached to the bottom of the cylinder, and mounted on top was a 2.4 meter sphere which held the lander.
The orbiter entered Venus orbit on October 20, 1975. Its mission was to act as a communications relay for the lander and to explore cloud layers and atmospheric parameters with several instruments and experiments. It performed 17 survey missions from October 26, 1975 to December 25, 1975.
List of orbiter instruments and experiments
- 1.6-2.8 μm IR Spectrometer
- 8-28 μm IR Radiometer
- 352 nm UV Photometer
- 2 Photo-polarimeters (335-800 nm)
- 300-800 nm Spectrometer
- . Lyman-α H/D Spectrometer
- Bistatic Radar Mapping
- CM, DM Radio Occultations
- Triaxial Magnetometer
- 345-380 nm UV Camera
- 355-445 nm Camera
- 6 Electrostatic Analyzers
- 2 Modulation Ion Traps
- Low-Energy Proton / Alpha detector
- Low-Energy Electron detector
- 3 Semiconductor Counters
- 2 Gas-Discharge Counters
- Cherenkov Detector
Lander
On October 20, 1975, the lander spacecraft was separated from the orbiter, and landing was made with the Sun near zenith at 05:13 UTC on October 22. Venera 9 landed within a 150 km radius of 31°01′N 291°38′E / 31.01°N 291.64°E, near Beta Regio, on a steep (20°) slope covered with boulders (suspected to be the slope of the tectonic rift valley, Aikhulu Chasma). The entry sphere weighed 1,560 kg (3,440 lb) and the surface payload 660 kg (1,455 lb).[6]
It was the first spacecraft to return an image from the surface of another planet.
A system of circulating fluid was used to distribute the heat load. This system, plus pre-cooling prior to entry, permitted operation of the lander for 53 minutes after landing, at which time radio contact with the orbiter was lost as the orbiter moved out of radio range.[5] During descent, heat dissipation and deceleration were accomplished sequentially by protective hemispheric shells, three parachutes, a disc-shaped drag brake, and a compressible, metal, doughnut-shaped landing cushion. The landing was about 2,200 km from the Venera 10 landing site.
Venera 9 measured clouds that were 30–40 km thick with bases at 30–35 km altitude. It also measured atmospheric chemicals including hydrochloric acid, hydrofluoric acid, bromine, and iodine. Other measurements included surface pressure of about 90 atmospheres (9 MPa), temperature of 485 °C (905 °F), and surface light levels comparable to those at Earth mid-latitudes on a cloudy summer day. Venera 9 was the first probe to send back black and white television pictures from the Venusian surface showing shadows, no apparent dust in the air, and a variety of 30 to 40 cm rocks which were not eroded. Planned 360-degree panoramic pictures could not be taken because one of two camera lens covers failed to come off, limiting pictures to 180 degrees. This failure recurred with Venera 10.
Lander payload[5]
- Temperature and pressure sensors
- Accelerometer
- Visible / IR photometer - IOV-75
- Backscatter and multi-angle nephelometers - MNV-75
- P-11 Mass spectrometer - MAV-75
- Panoramic telephotometers (2, with lamps)
- Anemometer - ISV-75
- Gamma ray spectrometer - GS-12V
- Gamma ray densitometer - RP-75
Image processing
Don P. Mitchell recently came across the original Venera imaging data while researching the Soviet Venus program, and reconstructed the images using modern image processing software.
See also
References
- 1 2 McDowell, Jonathan. "Launch Log". Jonathan's Space Page. Retrieved 11 April 2013.
- ↑ RussianSpaceWeb.com
- ↑ "NSSDC Master Catalog - Venera 9". NASA National Science Data Center. Retrieved 13 April 2013.
- ↑ Solar System Exploration Multimedia Gallery: Venera 9, NASA website, accessed August 7, 2009.
- 1 2 3 Mitchell, Don P. "First Pictures of the Surface of Venus". Retrieved 13 April 2013.
- ↑ Interplanetary Spacecraft
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