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    The Venera program established a number of precedents in space exploration, among them being the first human-made devices to enter the atmosphere of another planet Venera 3 on March 1, , the first to make a soft landing on another planet Venera 7 on December 15, , the first to return images from another planet's surface Venera 9 on June 8, , and the first to perform high-resolution radar mapping scans Venera 15 on June 2, The first Soviet attempt at a flyby probe to Venus was launched on February 4, , but failed to leave Earth orbit.

    In keeping with the Soviet policy at that time of not announcing details of failed missions, the launch was announced under the name Tyazhely Sputnik "Heavy Satellite".

    It is also known as Venera 1VA. As with some of the Soviet Union's other planetary probes, the later versions were launched in pairs with a second vehicle launched soon after the first.

    Venera 1 and Venera 2 were intended to fly past Venus without entering orbit. Venera 1 was launched on February 12, Telemetry on the probe failed seven days after launch.

    Venera 2 launched on November 12, , but also suffered a telemetry failure after leaving Earth orbit. Several other failed attempts at Venus flyby probes were launched by the Soviet Union in the early s, [2] [3] but were not announced as planetary missions at the time, and hence did not officially receive the "Venera" designation.

    The Venera 3 to 6 probes were similar. Weighing approximately one ton, and launched by the Molniya -type booster rocket, they included a cruise "bus" and a spherical atmospheric entry probe.

    The probes were optimised for atmospheric measurements, but not equipped with any special landing apparatus. Although it was hoped they would reach the surface still functioning, the first probes failed almost immediately, thereby disabling data transmission to Earth.

    Venera 3 became the first human-made object to impact another planet's surface as it crash-landed on March 1, However, as the spacecraft's data probes had failed upon atmospheric penetration, no data from within the Venusian boundary were retrieved from the mission.

    On 18 October , Venera 4 became the first spacecraft to measure the atmosphere of another planet. While the Soviet Union initially claimed the craft reached the surface intact, re-analysis including atmospheric occultation data from the American Mariner 5 spacecraft that flew by Venus the day after its arrival demonstrated that Venus's surface pressure was atmospheres, much higher than Venera 4's 25 atm hull strength, and the claim was retracted.

    Realizing the ships would be crushed before reaching the surface, the Soviets launched Venera 5 and Venera 6 as atmospheric probes.

    Designed to jettison nearly half their payload prior to entering the planet's atmosphere, these craft recorded 53 and 51 minutes of data, respectively, while slowly descending by parachute before their batteries failed.

    The Venera 7 probe was the first one designed to survive Venus surface conditions and to make a soft landing. Massively overbuilt to ensure survival, it had few experiments on board, and scientific output from the mission was further limited due to an internal switchboard failure which stuck in the "transmit temperature" position.

    Venera 7's parachute failed shortly before landing very close to the surface. Due to the resultant antenna misalignment, the radio signal was very weak, but was detected with temperature telemetry for 23 more minutes before its batteries expired.

    Thus, it became, on 15 December , the first human-made probe to transmit data from the surface of Venus. Venera 8 , launched in , was equipped with an extended set of scientific instruments for studying the surface gamma-spectrometer etc.

    The cruise bus of Venera 7 and 8 was similar to that of earlier ones, with the design ascending to the Zond 3 mission. The lander transmitted data during the descent and landed in sunlight.

    It measured the light level but had no camera. It transmitted data for almost an hour. Following the failed Kosmos , the Venera 9 and 10 probes and Venera 11 and 12 probes were of a different design.

    They weighed approximately five tons and were launched by the powerful Proton booster. They included a transfer and relay bus that had engines to brake into Venus orbit Venera 9 and 10 , 15 and 16 and to serve as receiver and relay for the entry probe's transmissions.

    The entry probe was attached to the top of the bus in a spherical heat shield. The probes were optimized for surface operations with an unusual looking design that included a spherical compartment to protect the electronics from atmospheric pressure and heat for as long as possible.

    Beneath this was a shock absorbing "crush ring" for landing. Above the pressure sphere was a cylindrical antenna structure and a wide dish shaped structure that resembled an antenna but was actually an aerobrake.

    They were designed to operate on the surface for a minimum of 30 minutes. Instruments varied on different missions, but included cameras and atmospheric and soil analysis equipment.

    All four landers had problems with some or all of their camera lens caps not releasing. The Venera 9 lander operated for at least 53 minutes and took pictures with one of two cameras; the other lens cap did not release.

    The Venera 10 lander operated for at least 65 minutes and took pictures with one of two cameras; the other lens cap did not release. The Venera 11 lander operated for at least 95 minutes but neither cameras' lens caps released.

    The Venera 12 lander operated for at least minutes but neither cameras' lens caps released. The design was similar to the earlier Venera 9—12 landers.

    They carried instruments to take scientific measurements of the ground and atmosphere once landed, including cameras, a microphone, a drill and surface sampler, and a seismometer.

    They also had instruments to record electric discharges during its descent phase through the Venusian atmosphere. The Venera 13 lander survived for minutes, and the Venera 14 lander for 57 minutes, where the planned design life was only 32 minutes.

    The Venera 14 craft had the misfortune of ejecting the camera lens cap directly under the surface compressibility tester arm, and returned information for the compressibility of the lens cap rather than the surface.

    The descent vehicles transmitted data to the buses, which acted as data relays as they flew by Venus. The Venera 15 and 16 spacecraft were orbiter missions; similar to previous probes, but the entry probes were replaced with surface imaging radar equipment.

    Radar imaging was necessary to penetrate the dense cloud of Venus. Venera-D is a proposed mission to Venus that would include a highly capable orbiter and a lander.

    From the standpoint of total mass delivered to Venus, the best launch opportunities occur in and There were many scientific findings about Venus from the data retrieved by the Venera probes.

    For example, after analyzing the radar images returned from Venera 15 and 16, it was concluded that the ridges and grooves on the surface of Venus were the result of tectonic deformations.

    The Venera 9 and 10 landers had two cameras each. However on both these missions, only one functioned because the lens covers failed to separate from the second camera on the landers.

    The design was changed for Venera 11 and 12, but on those missions all cameras failed. Venera 13 and 14 were the only landers on which all cameras worked properly; unfortunately, the titanium lens cap on Venera 14 landed precisely on the area which was targeted by the soil compression probe.

    From Wikipedia, the free encyclopedia. A Soviet program that explored Venus with multiple probes. For other uses, see Venera disambiguation.

    This article has multiple issues. Please help improve it or discuss these issues on the talk page. Learn how and when to remove these template messages.

    This article needs additional citations for verification. Please help improve this article by adding citations to reliable sources.

    Unsourced material may be challenged and removed. This article is a rough translation from Russian. It may have been generated by a computer or by a translator without dual proficiency.

    Please help to enhance the translation. Weighing approximately one ton, and launched by the Molniya -type booster rocket, they included a cruise "bus" and a spherical atmospheric entry probe.

    The probes were optimised for atmospheric measurements, but not equipped with any special landing apparatus. Although it was hoped they would reach the surface still functioning, the first probes failed almost immediately, thereby disabling data transmission to Earth.

    Venera 3 became the first human-made object to impact another planet's surface as it crash-landed on March 1, However, as the spacecraft's data probes had failed upon atmospheric penetration, no data from within the Venusian boundary were retrieved from the mission.

    On 18 October , Venera 4 became the first spacecraft to measure the atmosphere of another planet. While the Soviet Union initially claimed the craft reached the surface intact, re-analysis including atmospheric occultation data from the American Mariner 5 spacecraft that flew by Venus the day after its arrival demonstrated that Venus's surface pressure was atmospheres, much higher than Venera 4's 25 atm hull strength, and the claim was retracted.

    Realizing the ships would be crushed before reaching the surface, the Soviets launched Venera 5 and Venera 6 as atmospheric probes.

    Designed to jettison nearly half their payload prior to entering the planet's atmosphere, these craft recorded 53 and 51 minutes of data, respectively, while slowly descending by parachute before their batteries failed.

    The Venera 7 probe was the first one designed to survive Venus surface conditions and to make a soft landing. Massively overbuilt to ensure survival, it had few experiments on board, and scientific output from the mission was further limited due to an internal switchboard failure which stuck in the "transmit temperature" position.

    Venera 7's parachute failed shortly before landing very close to the surface. Due to the resultant antenna misalignment, the radio signal was very weak, but was detected with temperature telemetry for 23 more minutes before its batteries expired.

    Thus, it became, on 15 December , the first human-made probe to transmit data from the surface of Venus. Venera 8 , launched in , was equipped with an extended set of scientific instruments for studying the surface gamma-spectrometer etc.

    The cruise bus of Venera 7 and 8 was similar to that of earlier ones, with the design ascending to the Zond 3 mission.

    The lander transmitted data during the descent and landed in sunlight. It measured the light level but had no camera.

    It transmitted data for almost an hour. Following the failed Kosmos , the Venera 9 and 10 probes and Venera 11 and 12 probes were of a different design.

    They weighed approximately five tons and were launched by the powerful Proton booster. They included a transfer and relay bus that had engines to brake into Venus orbit Venera 9 and 10 , 15 and 16 and to serve as receiver and relay for the entry probe's transmissions.

    The entry probe was attached to the top of the bus in a spherical heat shield. The probes were optimized for surface operations with an unusual looking design that included a spherical compartment to protect the electronics from atmospheric pressure and heat for as long as possible.

    Beneath this was a shock absorbing "crush ring" for landing. Above the pressure sphere was a cylindrical antenna structure and a wide dish shaped structure that resembled an antenna but was actually an aerobrake.

    They were designed to operate on the surface for a minimum of 30 minutes. Instruments varied on different missions, but included cameras and atmospheric and soil analysis equipment.

    All four landers had problems with some or all of their camera lens caps not releasing. The Venera 9 lander operated for at least 53 minutes and took pictures with one of two cameras; the other lens cap did not release.

    The Venera 10 lander operated for at least 65 minutes and took pictures with one of two cameras; the other lens cap did not release. The Venera 11 lander operated for at least 95 minutes but neither cameras' lens caps released.

    The Venera 12 lander operated for at least minutes but neither cameras' lens caps released. The design was similar to the earlier Venera 9—12 landers.

    They carried instruments to take scientific measurements of the ground and atmosphere once landed, including cameras, a microphone, a drill and surface sampler, and a seismometer.

    They also had instruments to record electric discharges during its descent phase through the Venusian atmosphere.

    The Venera 13 lander survived for minutes, and the Venera 14 lander for 57 minutes, where the planned design life was only 32 minutes.

    The Venera 14 craft had the misfortune of ejecting the camera lens cap directly under the surface compressibility tester arm, and returned information for the compressibility of the lens cap rather than the surface.

    The descent vehicles transmitted data to the buses, which acted as data relays as they flew by Venus. The Venera 15 and 16 spacecraft were orbiter missions; similar to previous probes, but the entry probes were replaced with surface imaging radar equipment.

    Radar imaging was necessary to penetrate the dense cloud of Venus. Venera-D is a proposed mission to Venus that would include a highly capable orbiter and a lander.

    From the standpoint of total mass delivered to Venus, the best launch opportunities occur in and There were many scientific findings about Venus from the data retrieved by the Venera probes.

    For example, after analyzing the radar images returned from Venera 15 and 16, it was concluded that the ridges and grooves on the surface of Venus were the result of tectonic deformations.

    The Venera 9 and 10 landers had two cameras each. However on both these missions, only one functioned because the lens covers failed to separate from the second camera on the landers.

    The design was changed for Venera 11 and 12, but on those missions all cameras failed. Venera 13 and 14 were the only landers on which all cameras worked properly; unfortunately, the titanium lens cap on Venera 14 landed precisely on the area which was targeted by the soil compression probe.

    From Wikipedia, the free encyclopedia. A Soviet program that explored Venus with multiple probes. For other uses, see Venera disambiguation.

    This article has multiple issues. Please help improve it or discuss these issues on the talk page.

    Learn how and when to remove these template messages. This article needs additional citations for verification. Please help improve this article by adding citations to reliable sources.

    Unsourced material may be challenged and removed. This article is a rough translation from Russian. It may have been generated by a computer or by a translator without dual proficiency.

    Please help to enhance the translation. Main articles: Venera 1 and Venera 2. Main articles: Venera 3 , Venera 4 , Venera 5 , and Venera 6.

    Main article: Venera 7. Main article: Venera 8. Main articles: Venera 9 , Venera 10 , Venera 11 , and Venera Main articles: Venera 13 and Venera Main articles: Venera 15 and Venera Main article: Vega program.

    Main article: Venera-D. Encyclopedia Astronautica. Archived from the original on 9 September

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    The Venera 3 to 6 probes were similar. Weighing approximately one ton, and launched by the Molniya -type booster rocket, they included a cruise "bus" and a spherical atmospheric entry probe.

    The probes were optimised for atmospheric measurements, but not equipped with any special landing apparatus.

    Although it was hoped they would reach the surface still functioning, the first probes failed almost immediately, thereby disabling data transmission to Earth.

    Venera 3 became the first human-made object to impact another planet's surface as it crash-landed on March 1, However, as the spacecraft's data probes had failed upon atmospheric penetration, no data from within the Venusian boundary were retrieved from the mission.

    On 18 October , Venera 4 became the first spacecraft to measure the atmosphere of another planet. While the Soviet Union initially claimed the craft reached the surface intact, re-analysis including atmospheric occultation data from the American Mariner 5 spacecraft that flew by Venus the day after its arrival demonstrated that Venus's surface pressure was atmospheres, much higher than Venera 4's 25 atm hull strength, and the claim was retracted.

    Realizing the ships would be crushed before reaching the surface, the Soviets launched Venera 5 and Venera 6 as atmospheric probes.

    Designed to jettison nearly half their payload prior to entering the planet's atmosphere, these craft recorded 53 and 51 minutes of data, respectively, while slowly descending by parachute before their batteries failed.

    The Venera 7 probe was the first one designed to survive Venus surface conditions and to make a soft landing. Massively overbuilt to ensure survival, it had few experiments on board, and scientific output from the mission was further limited due to an internal switchboard failure which stuck in the "transmit temperature" position.

    Venera 7's parachute failed shortly before landing very close to the surface. Due to the resultant antenna misalignment, the radio signal was very weak, but was detected with temperature telemetry for 23 more minutes before its batteries expired.

    Thus, it became, on 15 December , the first human-made probe to transmit data from the surface of Venus. Venera 8 , launched in , was equipped with an extended set of scientific instruments for studying the surface gamma-spectrometer etc.

    The cruise bus of Venera 7 and 8 was similar to that of earlier ones, with the design ascending to the Zond 3 mission.

    The lander transmitted data during the descent and landed in sunlight. It measured the light level but had no camera.

    It transmitted data for almost an hour. Following the failed Kosmos , the Venera 9 and 10 probes and Venera 11 and 12 probes were of a different design.

    They weighed approximately five tons and were launched by the powerful Proton booster. They included a transfer and relay bus that had engines to brake into Venus orbit Venera 9 and 10 , 15 and 16 and to serve as receiver and relay for the entry probe's transmissions.

    The entry probe was attached to the top of the bus in a spherical heat shield. The probes were optimized for surface operations with an unusual looking design that included a spherical compartment to protect the electronics from atmospheric pressure and heat for as long as possible.

    Beneath this was a shock absorbing "crush ring" for landing. Above the pressure sphere was a cylindrical antenna structure and a wide dish shaped structure that resembled an antenna but was actually an aerobrake.

    They were designed to operate on the surface for a minimum of 30 minutes. Instruments varied on different missions, but included cameras and atmospheric and soil analysis equipment.

    All four landers had problems with some or all of their camera lens caps not releasing. The Venera 9 lander operated for at least 53 minutes and took pictures with one of two cameras; the other lens cap did not release.

    The Venera 10 lander operated for at least 65 minutes and took pictures with one of two cameras; the other lens cap did not release.

    The Venera 11 lander operated for at least 95 minutes but neither cameras' lens caps released. The Venera 12 lander operated for at least minutes but neither cameras' lens caps released.

    The design was similar to the earlier Venera 9—12 landers. They carried instruments to take scientific measurements of the ground and atmosphere once landed, including cameras, a microphone, a drill and surface sampler, and a seismometer.

    They also had instruments to record electric discharges during its descent phase through the Venusian atmosphere. The Venera 13 lander survived for minutes, and the Venera 14 lander for 57 minutes, where the planned design life was only 32 minutes.

    The Venera 14 craft had the misfortune of ejecting the camera lens cap directly under the surface compressibility tester arm, and returned information for the compressibility of the lens cap rather than the surface.

    The descent vehicles transmitted data to the buses, which acted as data relays as they flew by Venus.

    The Venera 15 and 16 spacecraft were orbiter missions; similar to previous probes, but the entry probes were replaced with surface imaging radar equipment.

    Radar imaging was necessary to penetrate the dense cloud of Venus. Venera-D is a proposed mission to Venus that would include a highly capable orbiter and a lander.

    From the standpoint of total mass delivered to Venus, the best launch opportunities occur in and There were many scientific findings about Venus from the data retrieved by the Venera probes.

    For example, after analyzing the radar images returned from Venera 15 and 16, it was concluded that the ridges and grooves on the surface of Venus were the result of tectonic deformations.

    The Venera 9 and 10 landers had two cameras each. However on both these missions, only one functioned because the lens covers failed to separate from the second camera on the landers.

    The design was changed for Venera 11 and 12, but on those missions all cameras failed. Venera 13 and 14 were the only landers on which all cameras worked properly; unfortunately, the titanium lens cap on Venera 14 landed precisely on the area which was targeted by the soil compression probe.

    From Wikipedia, the free encyclopedia. A Soviet program that explored Venus with multiple probes. For other uses, see Venera disambiguation.

    This article has multiple issues. Please help improve it or discuss these issues on the talk page. Learn how and when to remove these template messages.

    This article needs additional citations for verification. Please help improve this article by adding citations to reliable sources.

    Unsourced material may be challenged and removed. This article is a rough translation from Russian. It may have been generated by a computer or by a translator without dual proficiency.

    Please help to enhance the translation. Main articles: Venera 1 and Venera 2. Main articles: Venera 3 , Venera 4 , Venera 5 , and Venera 6.

    Main article: Venera 7. Main article: Venera 8. Main articles: Venera 9 , Venera 10 , Venera 11 , and Venera Main articles: Venera 13 and Venera Main articles: Venera 15 and Venera Main article: Vega program.

    Main article: Venera-D. Encyclopedia Astronautica. Instruments varied on different missions, but included cameras and atmospheric and soil analysis equipment.

    All four landers had problems with some or all of their camera lens caps not releasing. The Venera 9 lander operated for at least 53 minutes and took pictures with one of two cameras; the other lens cap did not release.

    The Venera 10 lander operated for at least 65 minutes and took pictures with one of two cameras; the other lens cap did not release. The Venera 11 lander operated for at least 95 minutes but neither cameras' lens caps released.

    The Venera 12 lander operated for at least minutes but neither cameras' lens caps released. The design was similar to the earlier Venera 9—12 landers.

    They carried instruments to take scientific measurements of the ground and atmosphere once landed, including cameras, a microphone, a drill and surface sampler, and a seismometer.

    They also had instruments to record electric discharges during its descent phase through the Venusian atmosphere.

    The Venera 13 lander survived for minutes, and the Venera 14 lander for 57 minutes, where the planned design life was only 32 minutes.

    The Venera 14 craft had the misfortune of ejecting the camera lens cap directly under the surface compressibility tester arm, and returned information for the compressibility of the lens cap rather than the surface.

    The descent vehicles transmitted data to the buses, which acted as data relays as they flew by Venus.

    The Venera 15 and 16 spacecraft were orbiter missions; similar to previous probes, but the entry probes were replaced with surface imaging radar equipment.

    Radar imaging was necessary to penetrate the dense cloud of Venus. Venera-D is a proposed mission to Venus that would include a highly capable orbiter and a lander.

    From the standpoint of total mass delivered to Venus, the best launch opportunities occur in and There were many scientific findings about Venus from the data retrieved by the Venera probes.

    For example, after analyzing the radar images returned from Venera 15 and 16, it was concluded that the ridges and grooves on the surface of Venus were the result of tectonic deformations.

    The Venera 9 and 10 landers had two cameras each. However on both these missions, only one functioned because the lens covers failed to separate from the second camera on the landers.

    The design was changed for Venera 11 and 12, but on those missions all cameras failed. Venera 13 and 14 were the only landers on which all cameras worked properly; unfortunately, the titanium lens cap on Venera 14 landed precisely on the area which was targeted by the soil compression probe.

    From Wikipedia, the free encyclopedia. A Soviet program that explored Venus with multiple probes. For other uses, see Venera disambiguation.

    This article has multiple issues. Please help improve it or discuss these issues on the talk page. Learn how and when to remove these template messages.

    This article needs additional citations for verification. Please help improve this article by adding citations to reliable sources. Unsourced material may be challenged and removed.

    This article is a rough translation from Russian. It may have been generated by a computer or by a translator without dual proficiency. Please help to enhance the translation.

    Main articles: Venera 1 and Venera 2. Main articles: Venera 3 , Venera 4 , Venera 5 , and Venera 6. Main article: Venera 7.

    Main article: Venera 8. Main articles: Venera 9 , Venera 10 , Venera 11 , and Venera Main articles: Venera 13 and Venera Main articles: Venera 15 and Venera Main article: Vega program.

    Main article: Venera-D. Encyclopedia Astronautica. Archived from the original on 9 September Retrieved 28 July Retrieved Journal of Geophysical Research.

    Journal of Geophysical Research March 30, , p. Bibcode : JGR Outline of Venus. Geodynamics Geology Surface features Venus snow Venusquake. Neith hypothetical moon.

    Aspects Orbit Phases. Venus-crosser asteroid VE Akatsuki BepiColombo. Colonization Inspiration Mars flyby Terraforming. Geological mapping of Venus Artificial objects on Venus.

    Book Category Portal. Venera programme. Venera 1 Venera 2. Venera 15 Venera Venera 3 Venera 4 Venera 5 Venera 6 Venera 7.

    Soviet space probes. Luna Lunokhod rovers Zond program. Venera Vega. Mars Fobos. Spacecraft missions to Venus. Vega 1 2. Jupiter Icy Moons Explorer Dragonfly Missions are ordered by launch date.

    Categories : Venera program.

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