(aerospace engineering) An instrumented vehicle, the payload of a rocket-launching system designed specifically for flight missions to other planets or the moon and into deep space, as distinguished from earth-orbiting satellites.
| Sci-Tech Dictionary: space probe |
(aerospace engineering) An instrumented vehicle, the payload of a rocket-launching system designed specifically for flight missions to other planets or the moon and into deep space, as distinguished from earth-orbiting satellites.
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| Sci-Tech Encyclopedia: Space probe |
An automated, crewless vehicle, the payload of a rocket-launching system, designed for flight missions to other planets, to the Moon, and into interplanetary space, as distinguished from Earth-orbiting satellites (see table).
Name | Launch date | Comments |
|---|---|---|
Luna 1 | Jan. 2, 1959 | Lunar probe; now in solar orbit; passed within 3278 mi (5275 km) of the Moon |
Pioneer 4 | Mar. 3, 1959 | Cosmic rays; passed 37,300 mi (60,000 km) from Moon |
Luna 2 | Sept. 2, 1959 | Impacted Moon |
Luna 3 | Oct. 4, 1959 | Photographed far side of Moon |
Pioneer 5 | Mar. 11, 1960 | First deep-space probe; magnetic fields and cosmic rays |
Mariner 2 | Aug. 26, 1962 | First planetary flyby; Venus probe |
Ranger 7 | July 28, 1964 | Lunar impact and approach photography |
Mariner 4 | Nov. 28, 1964 | Mars encounter; photography, magnetic fields, cosmic rays |
Ranger 8 | Feb. 17, 1965 | Lunar impact and approach photographs |
Ranger 9 | Mar. 21, 1965 | Lunar impact and Alphonsus; approach photography |
Zond 3 | July 18, 1965 | Photographs from lunar encounter |
Pioneer 6 | Dec. 16, 1965 | Solar orbit |
Luna 9 | Jan. 31, 1966 | First photographs from lunar surface |
Luna 10 | Mar. 31, 1966 | Lunar and interplanetary data |
Surveyor 1 | May 30, 1966 | Soft landing on Moon: environmental data and photography |
Lunar Orbiter 1 | Aug. 10, 1966 | Lunar photographs |
Pioneer 7 | Aug. 17, 1966 | Solar orbit |
Luna 11 | Aug. 24, 1966 | Lunar data |
Luna 12 | Oct. 22, 1966 | Lunar orbital photography and other data |
Lunar Orbiter 2 | Nov. 6, 1966 | Lunar orbital photography |
Luna 13 | Dec. 21, 1966 | Lunar surface photography and soil information |
Lunar Orbiter 3 | Feb. 5, 1967 | Lunar orbital photography |
Surveyor 3 | Apr. 17, 1967 | Lunar surface photography and surface properties |
Lunar Orbiter 4 | May 4, 1967 | Lunar orbital photography |
Venera 4 | June 12, 1967 | Analysis of Venus atmosphere; first instrumented landing on another planet |
Mariner 5 | June 14, 1967 | Venus probe; atmospheric and magnetospheric data |
Lunar Orbiter 5 | Aug. 1, 1967 | Lunar orbital photography |
Surveyor 5 | Sept. 8, 1967 | Lunar surface photography and surface properties, including elemental analysis of surface |
Surveyor 6 | Nov. 7, 1967 | Same as Surveyor 5; landing in Sinus Medii |
Pioneer 8 | Dec. 13, 1967 | Solar orbit |
Surveyor 7 | Jan. 7, 1968 | Same as Surveyor 5 |
Zond 5 | Sept. 14, 1968 | Circled Moon; recovered Sept. 21, 1968 |
Pioneer 9 | Nov. 8, 1968 | Solar orbit |
Zond 6 | Nov. 10, 1968 | Circled Moon; recovered Nov. 17, 1968 |
Venera 5 | Jan. 5, 1969 | Same as Venera 4 |
Venera 6 | Jan. 10, 1969 | Same as Venera 4 |
Mariner 6 | Feb. 25, 1969 | Photography and analysis of surface and atmosphere of Mars |
Mariner 7 | Mar. 27, 1969 | Same as Mariner 6 |
Luna 15 | July 14, 1969 | Lunar reconnaissance (crashed during attempted lunar landing) |
Zond 7 | Aug. 8, 1969 | Reentered Aug. 14, 1969; third uncrewed circumlunar flight; recovered in the Soviet Union |
Venera 7 | Aug. 17, 1970 | Lander capsule transmitted 23 min from surface of Venus, Dec. 15, 1970 |
Luna 16 | Sept. 12, 1970 | Reentered Sept. 24, 1970; uncrewed Moon lander touched down on Sea of Fertility Sept. 20, 1970; returned lunar soil samples |
Zond 8 | Oct. 20, 1970 | Circled Moon; recovered Oct. 27, 1970 |
Luna 17 | Nov. 10, 1970 | Landed on Moon Nov. 17, 1970; uncrewed Moon rover |
Mars 2 | May 19, 1971 | First Soviet Mars landing |
Mars 3 | May 28, 1971 | Mars probe |
Mariner 9 | May 30, 1971 | Mars probe |
Luna 18 | Sept. 2, 1971 | Impacted Moon Sept. 11, 1971 |
Luna 19 | Sept. 28, 1971 | Lunar photography mission |
Luna 20 | Feb. 14, 1972 | Recovered Feb. 25, 1972; returned lunar sample |
Pioneer 10 | Mar. 2, 1972 | Jupiter encounter; transjovian interplanetary probe |
Venera 8 | Mar. 27, 1972 | Venus landing July 22, 1972 |
Luna 21 | Jan. 8, 1972 | Moon landing Jan. 16, 1972, with Lunikhod rover |
Pioneer 11 | Apr. 5, 1973 | Jupiter encounter and transjovian interplanetary probe; also Saturn encounter |
Mars 4 | July 21, 1973 | Mars orbiter |
Mars 5 | July 25, 1973 | Mars orbiter |
Mars 6 | Aug. 5, 1973 | Mars lander |
Mars 7 | Aug. 9, 1973 | Mars lander |
Mariner 10 | Nov. 3, 1973 | Venus and Mercury encounter |
Luna 22 | May 29, 1974 | Lunar probe |
Helios 1 | Dec. 10, 1974 | Inner solar system, solar wind exploration |
Venera 9 | June 8, 1975 | Venus probe |
Venera 10 | June 14, 1975 | Venus probe |
Viking 1 | Aug. 20, 1975 | Mars lander and orbiter |
Viking 2 | Sept. 9, 1975 | Mars lander and orbiter |
Helios 2 | Jan. 15, 1976 | Interplanetary; similar objectives to those of Helios 1 |
Luna 24 | Aug. 9, 1976 | Recovered Aug. 25, 1976; returned lunar sample |
Voyager 2 | Aug. 20, 1977 | Jupiter, Saturn, Uranus, and Neptune encounters; also satellites and ring systems |
Voyager 1 | Sept. 5, 1977 | Same objectives as Voyager 2 with some orbital differences giving differing encounter trajectories |
Pioneer Venus Orbiter | May 20, 1978 | Returning atmospheric, surface, and particle and field information |
Pioneer Venus Multi-Probe Bus | Aug. 8, 1978 | Penetration of Venus atmosphere by four probes; returned atmospheric data |
Venera 11 | Sept. 8, 1978 | Venus lander; returned information on surface properties; detection of lightning and thunderlike sounds |
Venera 12 | Sept. 14, 1978 | Similar mission to Venera 11 |
Venera 13 | Oct. 30, 1981 | Venus lander |
Venera 14 | Nov. 4, 1981 | Venus lander |
Venera 15 | June 2, 1983 | Venus lander; surface topography |
Venera 16 | June 7, 1983 | Similar mission to Venera 15 |
International | — | Originally International Sun-Earth Explorer 3 (ISEE 3) Earth satellite, redirected using a lunar swingby on Dec. 22, 1983, to encounter with Comet Giacobini-Zinner; plasma and magnetic field |
Cometary | ||
Explorer (ICE) | ||
Vega 1 | Dec. 15, 1984 | Venus probe-Halley intercept |
Vega 2 | Dec. 21, 1984 | Venus probe-Halley intercept |
Sokigake | Jan. 8, 1985 | Halley intercept; precursor to Suisei, upgraded to full mission |
Giotto | July 2, 1985 | Halley intercept |
Suisei | Aug. 19, 1985 | Halley intercept; plasma and magnetic field measurements |
Phobos 1 | July 7, 1988 | Mars/Phobos probe, lost by command error |
Phobos 2 | July 12, 1988 | Mars/Phobos probe; some data but communications lost |
Magellan | May 4, 1989 | Venus radar mapper |
Galileo | Oct. 18, 1989 | Jupiter orbiter and atmospheric probe |
Muses | Jan. 24, 1990 | Moon orbiter and relay probe; orbiter transmitter malfunctioned |
Ulysses | Oct. 6, 1990 | Solar polar orbiter |
Mars Observer | Sept. 25, 1992 | Contact lost 3 days before Mars arrival |
Clementine | Jan. 25, 1994 | Orbited Moon; thruster malfunction prevented asteroid flyby |
Solar and Heliospheric Observatory (SOHO) | Dec. 2, 1995 | Orbits L1 libration point to study the Sun |
NEAR-Shoemaker | Feb. 17, 1996 | Asteroid orbiter |
Mars Global Surveyor | Nov. 7, 1996 | Mars orbiter |
Mars 96 | Nov. 16, 1996 | Mars orbiter and landers; launch vehicles failed |
Mars Pathfinder | Dec. 4, 1996 | Mars lander and rover |
Advanced Composition Explorer | Aug. 25, 1997 | Orbits L1 libration point to study charged particles |
Cassini | Oct. 15, 1997 | Saturn orbiter/Titan descent probe |
Lunar Prospector | Jan. 6, 1998 | Lunar orbiter |
Nozomi (Planet-B) | July 4, 1998 | Mars orbiter; orbit insertion failed |
Deep Space 1 | Oct. 24, 1998 | Test of ion engine and 11 other advanced technologies; asteroid flyby |
Mars Climate Orbiter | Dec. 11, 1998 | Lost during Mars arrival |
Mars Polar Lander | Jan. 3, 1999 | Lost during Mars arrival |
Stardust | Feb. 7, 1999 | Comet flyby, dust sample return |
Mars Odyssey | April 7, 2001 | Mars orbiter |
Wilkinson Microwave Anisotropy Probe | June 30, 2001 | Orbits L2 libration point to study cosmic background radiation |
Genesis | August 8, 2001 | Orbits L1 libration point to collect solar wind samples and return them |
Hyabusa (Muses-C) | May 9, 2003 | Asteroid sample return mission |
Mars Express | June 2, 2003 | Mars orbiter and lander; orbiter was successful but Beagle 2 lander failed |
MER-A/Spirit | June 10, 2003 | Mars rover |
MER-B/Opportunity | July 7, 2003 | Mars rover |
Spitzer Space Telescope (Space Infrared Telescope Facility) | August 25, 2003 | Infrared observatory in Earth-trailing orbit |
MESSENGER | August 3, 2004 | Mercury orbiter |
The space probe is used primarily for scientific purposes, which are stated as the mission objectives. Missions generally fall into three categories according to destination: those to the rocky bodies in the inner solar system, including the Earth-like planets, asteroids, and comets; those to the giant gaseous planets in the outer solar system; and those designed to study solar physics and the properties of interplanetary space. Most spacecraft launched to a planet or other body also study the environment of charged particles and electromagnetic fields in interplanetary space during their cruise phase en route to the destination. See also Asteroid; Solar system.
Missions may also be categorized by complexity. The simplest are flyby spacecraft, which study their target body during a relatively brief encounter period from a distance of hundreds to thousands of miles as they continue past. Next are orbiters, which circle a planet or other body for extended study; some may carry atmospheric descent probes. Even more complex are lander missions, which touch down on a planet or other body for the collection of on-site data; some may bear exploration rovers designed to range beyond the immediate landing site. Finally, the most complex space probes envisaged are sample-return missions, which would collect specimen material from a target body and return it to Earth for detailed study.
Spacecraft subsystems
In the broadest terms, a space probe may be considered a vehicle that transports a payload of sensing instruments to the vicinity of a target body. Thus, the spacecraft must include a number of subsystems to provide power, to communicate with Earth, to maintain and modify attitude and perform maneuvers, to maintain acceptable on-board temperature, and to manage the spacecraft overall. See also Space technology.
Scientific instruments
The scientific payload may be divided into remote-sensing instruments, such as cameras, and direct-sensing instruments, such as magnetometers or dust detectors. They may be classified as passive instruments, which detect radiance given off by a target body, or active ones, which emit energy such as radar pulses to characterize a target body. See also Remote sensing.
Power subsystem
Electrical power is required for all spacecraft functions. The total required power ranges from about 300 to 2500 W for current missions, depending on the complexity of the spacecraft. The power subsystem must generate, store, and distribute electrical power. All space probes launched so far have generated power either via solar panels or via radioisotope thermoelectric generators (RTGs). See also Nuclear battery; Solar cell; Space power systems.
Telecommunications subsystem
In order to accomplish its mission, the spacecraft must maintain communications with Earth, such as receiving commands sent from ground controllers, and transmitting scientific data and routine engineering “housekeeping” data. All of these transmissions are made in various segments of the microwave spectrum. The design of the telecommunications subsystem takes into account the volume of data to be transmitted and the distance from Earth at which the spacecraft will operate, dictating such considerations as the size of antennas and the power of the on-board transmitters. See also Microwave.
Advanced planetary probes have carried a dish-shaped high-gain antenna which is the chief antenna used to both transmit and receive. These antennas typically consist of a large parabolic reflector, with a subreflector mounted at the main reflector's focus in a Cassegrain-type configuration. In the interest of redundancy and in the event that Earth pointing is lost, spacecraft virtually always carry other on-board antennas. These may be low-gain antennas, which typically offer nearly omnidirectional coverage except for blind spots shadowed by the spacecraft body, or medium-gain antennas, which provide a beam width of perhaps 20–30°. See also Antenna (electromagnetism).
Attitude-control subsystem
It would be impossible to navigate the spacecraft successfully or point its scientific instruments or antennas without closely controlling its orientation in space, or attitude. Some spacecraft, particularly earlier ones, have been spin-stabilized; during or shortly after launch, the spacecraft is set spinning at a rate on the order of a few revolutions per minute. Much like a rotating toy top, the spacecraft's orientation is stabilized by the gyroscopic action of its spinning mass. Most planetary spacecraft, however, are three-axis-stabilized, meaning that their attitude is fixed in relation to space. The spacecraft's attitude is maintained and changed via onboard thruster jets or reaction wheels, or a combination of both.
Propulsion subsystem
Most spacecraft are outfitted with a series of thruster jets, each of which produces approximately 0.2–2 pounds-force (1–10 newtons) of thrust. Thrusters are usually fueled with a monopropellant, hydrazine, which decomposes explosively when it contacts an electrically heated metallic catalyst within the thruster. In addition to maintaining the spacecraft's attitude, on-board thrusters are used for trajectory-correction maneuvers. Spacecraft designed to orbit a planet or similar target body must carry a larger propulsion element capable of decelerating the spacecraft into orbit upon arrival. See also Spacecraft propulsion.
Thermal control subsystem
In order to minimize the impact of temperature variations on the electronics on board, spacecraft nearly always incorporate some form of thermal control. Mechanical louvers, controlled by bimetallic strips similar to those in terrestrial thermostats, are often used to selectively radiate heat from the interior of the spacecraft into space. Other thermal strategies include painting exterior surfaces. In some cases, spacecraft may also carry one or more active forms of heating to maintain temperature at required minimums.
Command and data subsystem
This designation is given to the main computer that oversees management of spacecraft functions and handling of collected data. Blocks of commands transmitted from Earth are stored in memory in the command and data subsystem and are executed at prescribed times. This subsystem also contains the spacecraft clock in order to accurately pace its activities, as well as all the activities of the spacecraft.
Structure subsystem
The spacecraft's physical structure is considered a subsystem itself for the purposes of planning and design. Usually the heart of this structure is a spacecraft bus, often consisting of a number of bays, which houses the spacecraft's main subsystems. See also Spacecraft structure.
| Wikipedia: Space probe |
A space probe is a scientific space exploration mission in which a robotic spacecraft leaves the gravity well of Earth and approaches the Moon or enters interplanetary or interstellar space (see list of probes by operational status for a list of active probes); The space agencies of the USSR (now Russia and Ukraine), the United States, the European Union, Japan, India and China have in the aggregate launched probes to several planets and moons of the solar system as well as to a number of asteroids and comets.
Contents |
Once a probe has left the vicinity of Earth, its trajectory will likely take it along an orbit around the Sun similar to the Earth's orbit. To reach another planet, the conceptually simplest means is to execute a Hohmann transfer orbit maneuver. More complex techniques, such as gravitational slingshots, can be more efficient, though they may require the probe to spend more time in transit. A technique using very little propulsion, but possibly requiring a considerable amount of time, is to follow a trajectory on the Interplanetary Transport Network.
Mariner 9:
Upon its arrival at Mars on November 13, 1971 Mariner 9 became the first space probe to orbit another planet. After 349 days in orbit, Mariner 9 had transmitted 7,329 images covering over 80% of the Martian surface, and with the depletion of its supply of propellant the spacecraft was turned off on October 27, 1972.
Huygens probe:
The Huygens probe was a lander constructed by the European Space Agency (ESA) and launched as part of the Cassini-Huygens mission to Saturn's moon Titan. Huygens separated from the Cassini orbiter on December 25, 2004, and landed on Titan on January 14, 2005. It returned 350 pictures from the surface.
Spirit and Opportunity:
The Mars Exploration Rovers, Spirit and Opportunity landed on Mars to explore the Martian surface and geology, and searched for clues to past water activity on Mars. They were each launched in 2003 and landed in 2004. As of January 24, 2007, both Spirit and Opportunity have lasted for more than three years on Mars—when they were intended to last only three months. On February 6, 2007, Opportunity had traversed more than 10 km (6 mi) on the surface of Mars.[1]
Voyager 1:
Voyager 1 is a 733-kilogram probe launched September 5, 1977. It is currently[update] still operational, making it the longest-lasting mission of the U.S. National Aeronautics and Space Administration (NASA). It visited Jupiter and Saturn and was the first probe to provide detailed images of the moons of these planets.
Voyager 1 is the farthest human-made object from Earth, traveling away from both the Earth and the Sun at a relatively faster speed than any other probe. As of May 9, 2008, Voyager 1 is over 15.89 terameters (15.89 × 1012 meters, or 15.89 × 109 km, 106.26 AU, 14.72 light-hours, or 9.87 billion miles) from the Sun. At this distance, signals from Voyager 1 take more than fourteen hours to reach its control center at the Jet Propulsion Laboratory. Voyager 1 and Voyager 2 have both achieved solar escape velocity, meaning that its trajectory will not return it to the solar system.
Along with Pioneer 10, Pioneer 11, and its sister ship Voyager 2, Voyager 1 is an interstellar probe.
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