Mission type | Atmospheric Probe |
---|---|
Operator | Rocket Lab / MIT |
Website | |
Spacecraft properties | |
Bus | Photon Explorer [1] |
Manufacturer | Rocket Lab |
Dry mass | Probe:17 kg (37 lb) [2] |
Payload mass | Probe:1 kg (2.2 lb) [2] |
Start of mission | |
Launch date | January 2025 [3] |
Rocket | Electron |
Launch site | Launch Complex 1, Māhia [4] |
Contractor | Rocket Lab |
Flyby of Moon | |
Closest approach | 2025 (planned) |
Venus atmospheric probe | |
Spacecraft component | Probe |
Atmospheric entry | 13 May 2025 (planned) [5] |
Transponders | |
Band | S-band [4] |
Venus Life Finder Missions [6] |
Venus Life Finder is a planned uncrewed spacecraft to Venus designed to detect signs of life in the Venusian atmosphere. [4] Slated to be the first private mission to another planet, [7] the spacecraft is being developed by Rocket Lab in collaboration with a team from the Massachusetts Institute of Technology. [8] The spacecraft will consist of a Photon Explorer cruise stage which will send a small atmospheric probe into Venus with a single instrument,an autofluorescing nephelometer,to search for organic compounds within Venus' atmosphere. [9]
Originally planned for launch in May 2023,the probe is now planned to launch in January 2025, [3] or no earlier than 30 December 2024,with arrival at Venus on 13 May 2025. [5]
Research published in 2020 indicated the presence of phosphine (PH3) in Venus' atmosphere,resulting in a widespread public and academic interest in the possibility of life in the Venusian atmosphere. [10] [11] Although the probe will not directly search for phosphine,it will search for organic compounds in Venus' atmosphere,which would indicate potentially habitable conditions within Venus' cloud layer. [9] [12] Additionally,the mission will demonstrate an inexpensive,deep space mission with a small spacecraft and small launch vehicle,as well as mature the interplanetary Photon spacecraft. [4] Peter Beck,CEO of Rocket Lab commented that the Venus Life Finder represents a "real opportunity in the market for these incremental little missions in between [NASA missions]". [13]
Venus Life Finder is hoped to be the first of a series of small missions to Venus to better understand the planet. [6]
The spacecraft consists of two main components- a Photon Explorer cruise stage,and a small atmospheric probe with a autofluorescing nephelometer. [2]
The Explorer cruise stage,first developed for NASA's CAPSTONE,is the interplanetary variant of the Photon satellite bus. [1] The Explorer cruise stage,a self contained spacecraft with solar arrays for generating power,an attitude control system and a HyperCurie engine for propulsion,will remain attached to the atmospheric probe until 30 minutes prior to atmospheric entry. [4] [2]
The 17 kg (37 lb) cone-shaped atmospheric probe measures just 40 cm (16 in) across,which was chosen to accommodate the electronics and the focal length of the nephelometer. [4] The probe outer mould line is a scaled-down version of the Deep Space 2 probe. Like the Deep Space 2 probe,the probe carries no parachute nor does it eject its heat shield. The nephelometer,flight computer,and radio are housed in a spherical titanium pressure vessel encased within a layer of insulation to protect the electronics and instrument from the corrosive Venusian atmosphere and maintain acceptable temperatures. [2]
The probe contains one scientific instrument:
Venus Life Finder is being developed by a team of less than thirty people,led by Sara Seager of the Massachusetts Institute of Technology. [9] The mission cost is estimate at less than 10 million US dollars,funded by Rocket Lab,MIT and undisclosed philanthropists. Peter Beck,CEO of Rocket Lab,has said that the spacecraft is a "nights-and-weekends project," and that it "gets pushed to the side all the time,but [they are] still working on it." [5]
Venus Life Finder is planned to launch in January 2025 by an Electron launch vehicle from Rocket Lab's Launch Complex 1 on the Māhia Peninsula in New Zealand. After being delivered to low Earth orbit,the Explorer cruise stage will perform a series of burns culminating in a lunar gravity assist which will send the spacecraft to Venus. [5] During the 128 day interplanetary cruise,the spacecraft will make occasional mid-course corrections in preparation for arrival at Venus. [4] [2]
The probe will separate from the Explorer cruise stage 30 minutes before Venus atmospheric entry on 13 May 2025. Entering on the night-side to minimize background light for the autofluorescence nephelometer instrument,the probe will experience a peak g-force of 60 Gs and will descend through the atmosphere without a parachute. [14] The probe will have just five minutes in the cloud layer,between 65 km (40 mi) to 45 km (28 mi) in altitude,to perform its measurements. [9] The probe will directly transmit its data to Earth by S-band until expected loss of signal thirty minutes after atmospheric entry,after which it will impact the Venusian surface. [4] Due to constraints on the power of the transmitter as well as limited transmission time,the data collected will be sent through a neural network to fit within the limited 125 bytes/second bandwidth allotted. [14]
Venus is the second planet from the Sun. It is a terrestrial planet and is the closest in mass and size to its orbital neighbour Earth. Venus has by far the densest atmosphere of the terrestrial planets, composed mostly of carbon dioxide with a thick, global sulfuric acid cloud cover. At the surface it has a mean temperature of 737 K and a pressure 92 times that of Earth's at sea level. These extreme conditions compress carbon dioxide into a supercritical state at Venus's surface.
Mariner 1, built to conduct the first American planetary flyby of Venus, was the first spacecraft of NASA's interplanetary Mariner program. Developed by Jet Propulsion Laboratory, and originally planned to be a purpose-built probe launched summer 1962, Mariner 1's design was changed when the Centaur proved unavailable at that early date. Mariner 1, were then adapted from the lighter Ranger lunar spacecraft. Mariner 1 carried a suite of experiments to determine the temperature of Venus as well to measure magnetic fields and charged particles near the planet and in interplanetary space.
The Venera program was 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.
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).
The Pioneer Venus Multiprobe, also known as Pioneer Venus 2 or Pioneer 13, was a spacecraft launched in 1978 to explore Venus as part of NASA's Pioneer program. This part of the mission included a spacecraft bus which was launched from Earth carrying one large and three smaller probes, which after separating penetrated the Venusian atmosphere at a different location, returning data as they descended into the planet's thick atmosphere. The entry occurred on December 9, 1978.
Venera 7 was a Soviet spacecraft, part of the Venera series of probes to Venus. When it landed the Venusian surface on 15 December 1970, it became the first spacecraft to soft land on another planet and the first to transmit data from there back to Earth.
Venera 13 was part of the Soviet Venera program meant to explore Venus.
Akatsuki, also known as the Venus Climate Orbiter (VCO) and Planet-C, was a Japan Aerospace Exploration Agency (JAXA) space probe tasked with studying the atmosphere of Venus. It was launched aboard an H-IIA 202 rocket on 20 May 2010, but failed to enter orbit around Venus on 6 December 2010. After the craft orbited the Sun for five years, engineers successfully placed it into an alternative Venusian elliptic orbit on 7 December 2015 by firing its attitude control thrusters for 20 minutes and made it the first Japanese satellite orbiting 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.
The atmosphere of Venus is the very dense layer of gases surrounding the planet Venus. Venus's atmosphere is composed of 96.5% carbon dioxide and 3.5% nitrogen, with other chemical compounds present only in trace amounts. It is much denser and hotter than that of Earth; the temperature at the surface is 740 K, and the pressure is 93 bar (1,350 psi), roughly the pressure found 900 m (3,000 ft) under water on Earth. The atmosphere of Venus supports decks of opaque clouds of sulfuric acid that cover the entire planet, preventing optical Earth-based and orbital observation of the surface. Information about surface topography has been obtained exclusively by radar imaging.
Venera-D is a proposed Russian space mission to Venus that would include an orbiter and a lander to be launched in 2031. 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.
Sara Seager is a Canadian-American astronomer and planetary scientist. She is a professor at the Massachusetts Institute of Technology and is known for her work on extrasolar planets and their atmospheres. She is the author of two textbooks on these topics, and has been recognized for her research by Popular Science, Discover Magazine, Nature, and TIME Magazine. Seager was awarded a MacArthur Fellowship in 2013 citing her theoretical work on detecting chemical signatures on exoplanet atmospheres and developing low-cost space observatories to observe planetary transits.
The possibility of life on Venus is a subject of interest in astrobiology due to Venus' proximity and similarities to Earth. To date, no definitive evidence has been found of past or present life there. In the early 1960s, studies conducted via spacecraft demonstrated that the current Venusian environment is extreme compared to Earth's. Studies continue to question whether life could have existed on the planet's surface before a runaway greenhouse effect took hold, and whether a relict biosphere could persist high in the modern Venusian atmosphere.
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 June 2, 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.
SPRITE was a proposed Saturn atmospheric probe mission concept of the NASA. SPRITE is a design for an atmospheric entry probe that would travel to Saturn from Earth on its own cruise stage, then enter the atmosphere of Saturn, and descend taking measurements in situ.
Venus Atmospheric Maneuverable Platform (VAMP) is a mission concept by the aerospace companies Northrop Grumman and LGarde for a powered, long endurance, semi-buoyant inflatable aircraft that would explore the upper atmosphere of planet Venus for biosignatures as well as perform atmospheric measurements. The inflatable aircraft has a trapezoidal shape that is sometimes called delta wing or flying wing, and would have dual electric-driven propellers that would be stowed during atmospheric entry.
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