![]() Venera 14 postage stamp | |
Mission type | Venus flyby / lander |
---|---|
Operator | Soviet Academy of Sciences |
COSPAR ID | 1981-110A 1981-110D |
SATCAT no. | 12939 15600 |
Mission duration | Travel: 4 months and 1 day Lander: 57 minutes |
Spacecraft properties | |
Spacecraft type | 4V-1 No. 761 |
Manufacturer | NPO Lavochkin |
Launch mass | 4,394.5 kg (9,688 lb) [1] |
Landing mass | 760 kilograms (1,680 lb) |
Dry mass | 1,632.71 kilograms (3,599.5 lb) |
Dimensions | 2.7 m × 2.3 m × 5.7 m (8.9 ft × 7.5 ft × 18.7 ft) |
Start of mission | |
Launch date | November 4, 1981 , 05:31:00 UTC [1] |
Rocket | Proton-K/D-1 |
Launch site | Baikonur 200/39 |
End of mission | |
Last contact | lander: 5 March 1982 / carrier: 9 April 1983 [2] |
Orbital parameters | |
Reference system | Heliocentric |
Eccentricity | 0.17 |
Perihelion altitude | 0.71 Astronomical units |
Aphelion altitude | 0.99 Astronomical units |
Inclination | 2.3 degrees |
Period | 286 days |
Flyby of Venus | |
Spacecraft component | Venera 14 flight platform |
Closest approach | March 3, 1982 |
Distance | 26,050 km (16,190 mi) |
Venus lander | |
Spacecraft component | Venera 14 descent craft |
Landing date | March 5,1982,07:00:10 UTC |
Landing site | 13°15′S310°00′E / 13.25°S 310°E (east of Phoebe Regio) |
Venera 14 (called Venus 14 in English) was a probe in the Soviet Venera program for the exploration of Venus.
Venera 14 was identical to the Venera 13 spacecraft, built to take advantage of the 1981 Venus launch opportunity. Venera 14 was launched on 4 November 1981 at 05:31:00 UTC, five days after Venera 13 launched on 30 October 1981 at 06:04:00 UTC. Both had an on-orbit dry mass of 760 kg (1,680 lb).
Each mission consisted of a cruise stage and an attached descent craft.
As the cruise stage flew by Venus, the bus acted as a data relay for the lander before continuing on to a heliocentric orbit. Venera 14 was equipped with a gamma-ray spectrometer, UV grating monochromator, electron and proton spectrometers, gamma-ray burst detectors, solar wind plasma detectors, and two-frequency transmitters which made measurements before, during, and after the Venus flyby.
The descent lander was a hermetically sealed pressure vessel that contained most of the instrumentation and electronics. The lander was mounted on a ring-shaped landing platform and topped by an antenna. Designed similar to the earlier Venera 9–12 landers, the Venera 14 lander carried instruments to take chemical and isotopic measurements, monitor the spectrum of scattered sunlight, and record electric discharges during its descent phase through the Venusian atmosphere. The spacecraft used a camera system, an X-ray fluorescence spectrometer, a screw drill and surface sampler, a dynamic penetrometer, and a seismometer to conduct investigations on the surface.
The list of lander experiments and instruments include: [3]
Venera 14 landed at 13°15′S310°00′E / 13.25°S 310°E , about 950 kilometres (590 mi) southwest of Venera 13, near the eastern flank of Phoebe Regio on a basaltic plain.
After launch and following a four-month cruise to Venus, the descent vehicle separated from the bus and plunged into the Venusian atmosphere on 5 March 1982. A parachute deployed after the lander entered the atmosphere. The parachute released once the lander reached an altitude of about 50 kilometres (31 mi); simple air braking was used in the final descent.
Like its predecessors, Venera 14 was equipped with several systems with which to observe and analyse the Venusian surface and atmosphere.
The quartz camera windows were protected by lens covers that popped off after descent, allowing Venera 14 to capture images of the surface.
The Venera 14 lander was also equipped with a surface soil probe designed to measure the compressibility of the Venusian soil. By unfortunate chance, the lens caps came to rest at the exact point the probe was due to enter and analyse the soil. Thus, instead of the soil, the probe measured the compressibility of the Venera 14 lens cap.
The surface soil composition samples were determined by the X-ray fluorescence spectrometer, and were shown to be similar to oceanic tholeiitic basalts.
Additionally, Venera 14 was equipped with acoustic microphones designed to record atmospheric noise. The recordings were later used to calculate the average wind speed on the Venusian surface. Subsequent analysis determined the average surface wind speed to be between 0.3 and 0.5 metres per second (0.98 and 1.64 ft/s). [4]
The Venera 14 lander functioned for at least 57 minutes (the lander's planned lifespan was 32 minutes) in an environment with a temperature of 465 °C (869 °F) and a pressure of 94 Earth atmospheres (9.5 MPa). Telemetry was maintained by means of the Venera 14 bus in orbit, which carried signals from the lander's uplink antenna and then on to Earth. [5]
The spacecraft bus ended up in a heliocentric orbit where it continued to make observations in the X-ray and gamma ray spectrum. [6] The bus activated its engine on the 14th November 1982 to provide data for later Vega program missions. [6] The last published data for the probe is dated 16 March 1983. [6]
American researcher Don P. Mitchell has processed the color images from Venera 13 and 14 using the raw original data. [7] The new images are based on a more accurate linearization of the original 9-bit logarithmic pixel encoding.
The Venera program was the name given to a series of space probes developed by the Soviet Union between 1961 and 1984 to gather information about the planet Venus.
The Pioneer Venus project was part of the Pioneer program consisting of two spacecraft, the Pioneer Venus Orbiter and the Pioneer Venus Multiprobe, launched to Venus in 1978. The program was managed by NASA's Ames Research Center.
Vega 1 was a Soviet space probe, part of the Vega program. The spacecraft was a development of the earlier Venera craft. They were designed by Babakin Space Centre and constructed as 5VK by Lavochkin at Khimki. The name VeGa (ВеГа) combines the first two letters from the Russian words for Venus and Halley.
The Vega program was a series of Venus missions that also took advantage of the appearance of comet 1P/Halley in 1986. Vega 1 and Vega 2 were uncrewed spacecraft launched in a cooperative effort among the Soviet Union and Austria, Bulgaria, France, Hungary, the German Democratic Republic, Poland, Czechoslovakia, and the Federal Republic of Germany in December 1984. They had a two-part mission to investigate Venus and also flyby Halley's Comet.
Vega 2 was a Soviet space probe part of the Vega program to explore Halley's comet and Venus. The spacecraft was a development of the earlier Venera craft. The name VeGa (ВеГа) combines the first two letters Russian words for Venus and Halley They were designed by Babakin Space Centre and constructed as 5VK by Lavochkin at Khimki. The craft was powered by large twin solar panels. Instruments included an antenna dish, cameras, spectrometer, infrared sounder, magnetometers (MISCHA) and plasma probes. The 4,840 kilograms (10,670 lb) craft was launched on top of a Proton 8K82K rocket from Baikonur Cosmodrome, Tyuratam, Kazakh SSR. Both Vega 1 and 2 were three-axis stabilized spacecraft. The spacecraft were equipped with a dual bumper shield for dust protection from Halley's Comet.
Venera 3 was a Venera program space probe that was built and launched by the Soviet Union to explore the surface of Venus. It was launched on 16 November 1965 at 04:19 UTC from Baikonur, Kazakhstan, USSR. The probe comprised an entry probe, designed to enter the Venus atmosphere and parachute to the surface, and a carrier/flyby spacecraft, which carried the entry probe to Venus and also served as a communications relay for the entry probe.
The Phobos program was an uncrewed space mission consisting of two probes launched by the Soviet Union to study Mars and its moons Phobos and Deimos. Phobos 1 was launched on 7 July 1988, and Phobos 2 on 12 July 1988, each aboard a Proton-K rocket.
Phobos 2 was the last space probe designed by the Soviet Union. It was designed to explore the moons of Mars, Phobos and Deimos. It was launched on 12 July 1988, and entered orbit on 29 January 1989.
The Venera 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.
The Venera 12 was an uncrewed Soviet space mission designed to explore the planet Venus. Venera 12 was launched on 14 September 1978 at 02:25:13 UTC.
Venera 9, manufacturer's designation: 4V-1 No. 660, was a Soviet uncrewed space mission to Venus. It consisted of an orbiter and a lander. It was launched on June 8, 1975, at 02:38:00 UTC and had a mass of 4,936 kilograms (10,882 lb). The orbiter was the first spacecraft to orbit Venus, while the lander was the first to return images from the surface of another planet.
Venera 10, or 4V-1 No. 661, was a Soviet uncrewed space mission to Venus. It consisted of an orbiter and a lander. It was launched on June 14, 1975, 03:00:31 UTC and had a mass of 5033 kg (11096 lb).
Venera 6, or 2V (V-69) No.331, was a Soviet spacecraft, launched towards Venus to obtain atmospheric data. It had an on-orbit dry mass of 1,130 kg (2,490 lb).
Venera 4, also designated 4V-1 No.310, was a probe in the Soviet Venera program for the exploration of Venus. The probe comprised a lander, designed to enter the Venusian atmosphere and parachute to the surface, and a carrier/flyby spacecraft, which carried the lander to Venus and served as a communications relay for it.
Venera 5 was a space probe in the Soviet space program Venera for the exploration of Venus.
Venera 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 13 was part of the Soviet Venera program meant to explore Venus.
Observations of the planet Venus include those in antiquity, telescopic observations, and from visiting spacecraft. Spacecraft have performed various flybys, orbits, and landings on Venus, including balloon probes that floated in the atmosphere of Venus. Study of the planet is aided by its relatively close proximity to the Earth, compared to other planets, but the surface of Venus is obscured by an atmosphere opaque to visible light.
Venera-D is a proposed Russian space mission to Venus that would include an orbiter and a lander to be launched in 2029. The orbiter's prime objective is to perform observations with the use of a radar. The lander, based on the Venera design, would be capable of operating for a long duration on the planet's surface. The "D" in Venera-D stands for "dolgozhivuschaya," which means "long lasting" in Russian.
DAVINCI is a planned mission for an orbiter and atmospheric probe to the planet Venus. Together with the separate VERITAS mission, which will also study Venus, it was selected by NASA on 2 June 2021 to be part of their Discovery Program. Its acronym is inspired by Leonardo da Vinci in honor of his scientific innovations, aerial sketches and constructions.