SWAP (New Horizons)
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SWAP (Solar Wind Around Pluto) is an science instrument aboard the unmanned ''
New Horizons ''New Horizons'' is an Interplanetary spaceflight, interplanetary space probe that was launched as a part of NASA's New Frontiers program. Engineered by the Johns Hopkins University Applied Physics Laboratory (APL) and the Southwest Research ...
'' space probe, which was designed to flyby dwarf planet
Pluto Pluto (minor-planet designation: 134340 Pluto) is a dwarf planet in the Kuiper belt, a ring of trans-Neptunian object, bodies beyond the orbit of Neptune. It is the ninth-largest and tenth-most-massive known object to directly orbit the S ...
. SWAP was designed to record
Solar Wind The solar wind is a stream of charged particles released from the upper atmosphere of the Sun, called the corona. This plasma mostly consists of electrons, protons and alpha particles with kinetic energy between . The composition of the sola ...
en route, at, and beyond Pluto. At Pluto, SWAP's purpose was to record the relationship between the solarwind and
ion An ion () is an atom or molecule with a net electrical charge. The charge of an electron is considered to be negative by convention and this charge is equal and opposite to the charge of a proton, which is considered to be positive by conve ...
s and/or material entering space from the
atmosphere of Pluto The atmosphere of Pluto is the tenuous layer of gases surrounding Pluto. It consists mainly of nitrogen (N2), with minor amounts of methane (CH4) and carbon monoxide (CO), all of which are vaporized from their ices on Pluto's surface. It contain ...
.


Background

The atmosphere of Pluto was discovered in 1988, but it remained enigmatic and it was hard to understand an atmosphere existing in such low temperatures (45 Kelvin (–380° Fahrenheit)). One of the ideas about Pluto is atmospheric loss, with Pluto being compared to losses from
comets A comet is an icy, small Solar System body that, when passing close to the Sun, warms and begins to release gases, a process that is called outgassing. This produces a visible atmosphere or coma, and sometimes also a tail. These phenomena are ...
. The idea of atmospheric loss was suggested in 1980, even before the atmosphere was discovered. One idea is the
photoionization Photoionization is the physical process in which an ion is formed from the interaction of a photon with an atom or molecule. Cross section Not every interaction between a photon and an atom, or molecule, will result in photoionization. The prob ...
of escaping
neutral particle In physics, a neutral particle is a particle with no electric charge, such as a neutron. The term ''neutral particles'' should not be confused with ''truly neutral particles'', the subclass of neutral particles that are also identical to their ow ...
s might alter the flow solar wind around the dwarf planet. The atmosphere was known to be very tenuous compared to Earth, and one of the questions was how the gases were interacting with the solar wind and sunlight, likewise weaker at Pluto's orbit than at Earth's. One of the ideas was that Pluto's atmosphere would be stripped away by the solar wind over time. By the 2010s, only three other spacecraft besides ''New Horizons'' have collected extensive data about the solar wind beyond 10 AU, ''
Voyager 2 ''Voyager 2'' is a space probe launched by NASA on August 20, 1977, to study the outer planets and interstellar space beyond the Sun's heliosphere. As a part of the Voyager program, it was launched 16 days before its twin, ''Voyager 1'', on a ...
'', ''
Pioneer 10 ''Pioneer 10'' (originally designated Pioneer F) is an American space probe, launched in 1972 and weighing , that completed the first mission to the planet Jupiter. Thereafter, ''Pioneer 10'' became the first of five artificial objects to ach ...
'', and ''
Pioneer 11 ''Pioneer 11'' (also known as ''Pioneer G'') is a robotic space probe launched by NASA on April 5, 1973, to study the asteroid belt, the environment around Jupiter and Saturn, solar winds, and cosmic rays. It was the first probe to encounter ...
''.


Overview

SWAP is designed to be able to detect the sparse solar wind concentration at 32 AU, which is about three orders of magnitude less than near Earth (1 AU). However, at that distance the flow of the Solar Wind is still
supersonic Supersonic speed is the speed of an object that exceeds the speed of sound ( Mach 1). For objects traveling in dry air of a temperature of 20 °C (68 °F) at sea level, this speed is approximately . Speeds greater than five times ...
, and thus liable to create a
bow shock In astrophysics, a bow shock occurs when the magnetosphere of an astrophysical object interacts with the nearby flowing ambient plasma such as the solar wind. For Earth and other magnetized planets, it is the boundary at which the speed of ...
around an obstacle. One of the areas of investigation is the relationship between high altitude atmospheric loss and the solar wind. After the July 2015 flyby of Pluto by ''New Horizons'', data from SWAP was used to study the nature of Pluto's interaction with the solar wind. It was determined that NH entered a Pluto pause and passed through a heavy ion tail. Earlier in the mission SWAP was intended to observe the Solar Wind around Jupiter.http://www.boulder.swri.edu/pkb/ssr/ssr-swap.pdf SWAP was also designed to be used in conjunction with PEPPSI and REX, to study how the solar wind changes with greater distance from the Sun. SWAP took only limited observations before 2012, but after that took a greater amount of data. Starting in 2012, while the rest of the spacecraft was in hibernation most of the time, SWAP was turned on to collect data about the Solar wind as it journeyed out to Pluto at 33 AU. SWAP recorded data about solar wind in the outer solar system and beyond Pluto, and some of the data that is sought about the solar wind are the proton density, speed, and temperature. One of the observations made with SWAP was that Pluto's interaction region on sunward was limited to an area of 6 Pluto radii (about 7000 kilometers); this was smaller than expected.


Design

SWAP is a top-hat
electrostatic analyzer An electrostatic analyzer or ESA is an instrument used in ion optics that employs an electric field to allow the passage of only those ions or electrons that have a given specific energy. It usually also focuses these particles (concentrates the ...
. SWAP has a barrier known as the ''Retarding Potential Analyzer'' (RPA) that can be open or shut depending on the conditions. When closed ions must pass through the RPA before reaching the inner detectors. Beyond the orbit of Jupiter, it was not necessary to have the RPA engaged for measurements to protect the sensors from being overloaded. The RPA can protect the sensors from being overloaded by solar wind intensities that are too strong, as the device is also required to measure much fainter solar wind fluxes at 33 AU from Sun where Pluto would be at the time of the flyby, and even beyond. SWAP can detect ions up to 6.5 kiloelectron volts (keV).http://pluto.jhuapl.edu/Mission/Spacecraft/Payload.php SWAP weighs 3.3 kilograms (7.3 pounds) and uses an average of 2.3 watts of spacecraft electrical power. Overall swap is designed to study the solar wind, including at the distant of 32 AU, and to study atmospheric loss from the atmosphere of Pluto.


See also

*
MAVEN MAVEN is an American spacecraft orbiting Mars to study the loss of its atmospheric gases to space, providing insight into the history of the planet's climate and water. The spacecraft name is an acronym for "Mars Atmosphere and Volatile Evolu ...
(explored the Martian atmospheric loss, Mars orbiter of the 2010s) * SWAP (instrument) (similarly named spacecraft instrument on a Solar space observatory) *
SWEAP SWEAP (Solar Wind Electrons Alphas and Protons) is an instrument on the unmanned space probe to the Sun, the Parker Solar Probe. The spacecraft with SWEAP on board was launched by a Delta IV Heavy on 12 August 2018 from Cape Canaveral, Florida. ...
(instrument on the
Parker Solar Probe The Parker Solar Probe (PSP; previously Solar Probe, Solar Probe Plus or Solar Probe+) is a NASA space probe launched in 2018 with the mission of making observations of the outer corona of the Sun. It will approach to within 9.86 solar radii (6 ...
)


References


External links


''New Horizons'' Swap Pluto Cruise Calibrated V2.0
{{NH1 New Horizons Spacecraft instruments