Microwave Radiometer (Juno)
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Microwave Radiometer (MWR) is an instrument on the ''Juno'' orbiter sent to planet
Jupiter Jupiter is the fifth planet from the Sun and the List of Solar System objects by size, largest in the Solar System. It is a gas giant with a mass more than two and a half times that of all the other planets in the Solar System combined, but ...
.Spacecom - Jupiter's Stripes Go Deep, and Other Surprises from Juno Probe - October 2016
/ref> MWR is a multi-wavelength
microwave radiometer A microwave radiometer (MWR) is a radiometer that measures energy emitted at one millimeter-to-metre wavelengths (frequencies of 0.3–300 GHz) known as microwaves. Microwave radiometers are very sensitive receivers designed to measure thermally- ...
for making observations of
Jupiter Jupiter is the fifth planet from the Sun and the List of Solar System objects by size, largest in the Solar System. It is a gas giant with a mass more than two and a half times that of all the other planets in the Solar System combined, but ...
's deep
atmosphere An atmosphere () is a layer of gas or layers of gases that envelop a planet, and is held in place by the gravity of the planetary body. A planet retains an atmosphere when the gravity is great and the temperature of the atmosphere is low. A s ...
. MWR can observe radiation from 1.37 to 50 cm in
wavelength In physics, the wavelength is the spatial period of a periodic wave—the distance over which the wave's shape repeats. It is the distance between consecutive corresponding points of the same phase on the wave, such as two adjacent crests, tro ...
, from 600 MHz to 22 GHz in frequencies. This supports its goal of observing the previously unseen atmospheric features and chemical abundances hundreds of miles/km into Jupiter's atmosphere. MWR is designed to detect six different frequencies in that range using separate antennas. MWR views Jupiter's microwave radiation so it can see up to hundreds of miles deep into the planet. In August 2016, as ''Juno'' swung closely by the planet MWR achieved a penetration of 200 to 250 miles (350 to 400 kilometers) below the surface cloud layer. MWR is designed to make observations below the cloud-tops, especially detecting the abundances of certain chemicals and determine dynamic features. These depths have not been observed before. MWR was launched aboard the ''Juno'' spacecraft on August 5, 2011 ( UTC) from Cape Canaveral, USA, as part of the
New Frontiers program The New Frontiers program is a series of space exploration missions being conducted by NASA with the purpose of furthering the understanding of the Solar System. The program selects medium-class missions which can provide high science returns. ...
, and after an interplanetary journey that including a swingby of Earth, entered a
polar orbit A polar orbit is one in which a satellite passes above or nearly above both poles of the body being orbited (usually a planet such as the Earth, but possibly another body such as the Moon or Sun) on each revolution. It has an inclination of about ...
of Jupiter on July 5, 2016 (UTC), The electronics for MWR are located inside the ''
Juno Radiation Vault Juno Radiation Vault is a compartment inside the ''Juno (spacecraft), Juno'' spacecraft that houses much of the probe's electronics and computers, and is intended to offer increased protection of radiation to the contents as the spacecraft endur ...
'', which uses
titanium Titanium is a chemical element with the symbol Ti and atomic number 22. Found in nature only as an oxide, it can be reduced to produce a lustrous transition metal with a silver color, low density, and high strength, resistant to corrosion in ...
to protect it and other spacecraft electronics.Key and Driving Requirements for the Juno Payload Suite of Instruments
/ref> The antennas and transmission lines are designed to handle the radiation environment at Jupiter so the instrument can function.


Goals

Determining the features and abundances of
oxygen Oxygen is the chemical element with the symbol O and atomic number 8. It is a member of the chalcogen group in the periodic table, a highly reactive nonmetal, and an oxidizing agent that readily forms oxides with most elements as wel ...
,
nitrogen Nitrogen is the chemical element with the symbol N and atomic number 7. Nitrogen is a nonmetal and the lightest member of group 15 of the periodic table, often called the pnictogens. It is a common element in the universe, estimated at se ...
, and
sulfur Sulfur (or sulphur in British English) is a chemical element with the symbol S and atomic number 16. It is abundant, multivalent and nonmetallic. Under normal conditions, sulfur atoms form cyclic octatomic molecules with a chemical formula ...
at up to 100 Bars of pressure (1451 psi) will shed light on the origins and nature of Jupiter. It is also designed to detect the amount
water Water (chemical formula ) is an inorganic, transparent, tasteless, odorless, and nearly colorless chemical substance, which is the main constituent of Earth's hydrosphere and the fluids of all known living organisms (in which it acts as a ...
and
ammonia Ammonia is an inorganic compound of nitrogen and hydrogen with the formula . A stable binary hydride, and the simplest pnictogen hydride, ammonia is a colourless gas with a distinct pungent smell. Biologically, it is a common nitrogenous was ...
deep inside Jupiter. It should also be able to provide a temperature profile of atmosphere down to 200 bar (2901 psi). Overall MWR is designed to look down as deep as roughly 1,000
atmospheres The standard atmosphere (symbol: atm) is a unit of pressure defined as Pa. It is sometimes used as a ''reference pressure'' or ''standard pressure''. It is approximately equal to Earth's average atmospheric pressure at sea level. History The s ...
(or Bars or kPa) which is about 342 miles (550 kilometers) down inside Jupiter. (1 bar is roughly the pressure at Earth sea level, 14.6 psi) One of the molecules MR is intended to look for inside Jupiter is water, which it is hoped well help explain the formation of the Solar System. By probing the interior, the insights may reveal how and where Jupiter formed, in turn shedding understanding on the formation of the Earth. At the time of its use in the 2010s, it was one of only four microwave radiometers to have been flown on interplanetary spacecraft. The first was
Mariner 2 Mariner 2 (Mariner-Venus 1962), an American space probe to Venus, was the first robotic space probe to conduct a successful planetary encounter. The first successful spacecraft in the NASA Mariner program, it was a simplified version of the Bl ...
, which used a microwave instrument to determine the high surface temperature of Venus was coming from the surface not higher up in the atmosphere. There is also radiometer type instruments on ''
Rosetta Rosetta or Rashid (; ar, رشيد ' ; french: Rosette  ; cop, ϯⲣⲁϣⲓⲧ ''ti-Rashit'', Ancient Greek: Βολβιτίνη ''Bolbitinē'') is a port city of the Nile Delta, east of Alexandria, in Egypt's Beheira governorate. The Ro ...
'' comet probe, and '' Cassini-Huygens''. Previously, the ''Galileo'' probe directly measured Jupiter's atmosphere ''in situ'' as it descended into the atmosphere, but only down to 22 bars of pressure. However, MWR is designed to look down as deep as 1000 bar of pressure. (1000 bar is about 14,500 psi, or 100000 kPa)


Antennas

MWR has six separate antennas of different size that are mounted to the sides of the ''Juno'' spacecraft body. As the spacecraft turns (it is a spin-stabilzed spacecraft) each antenna takes a "swath" of observations of the giant. Five of the six antennas are all on one side of the spacecraft. The sixth and biggest antenna entirely fills another side the ''Juno'' body. MWR antennas: There are two
patch Patch or Patches may refer to: Arts, entertainment and media * Patch Johnson, a fictional character from ''Days of Our Lives'' * Patch (''My Little Pony''), a toy * "Patches" (Dickey Lee song), 1962 * "Patches" (Chairmen of the Board song) ...
array antennas An antenna array (or array antenna) is a set of multiple connected antennas which work together as a single antenna, to transmit or receive radio waves. The individual antennas (called ''elements'') are usually connected to a single receiver ...
, three slot arrays, and one
horn antenna A horn antenna or microwave horn is an antenna that consists of a flaring metal waveguide shaped like a horn to direct radio waves in a beam. Horns are widely used as antennas at UHF and microwave frequencies, above 300 MHz. They are us ...
. *600 MHz/0.6 GHz frequency/50 cm wavelength (biggest antenna takes up one side of spacecraft body and is a patch array antenna) *1.2 GHz (also a patch array antenna, but located with other five antennas on one side) *2.4 GHz (waveguide slot array) *4.8 GHz (waveguide slot array) *9.6 GHz (waveguide slot array) *22 GHz frequency/1.3 cm light wavelength (horn antenna on upper deck of ''Juno'') As ''Juno'' turns the antennas sweep across Jupiter, each frequency/wavelength capable of seeing a certain distance below the visible cloud tops. See also
Reflective array antenna In telecommunications and radar, a reflective array antenna is a class of directive antennas in which multiple driven elements are mounted in front of a flat surface designed to reflect the radio waves in a desired direction. They are a type o ...
and
Slot antenna A slot antenna consists of a metal surface, usually a flat plate, with one or more holes or slots cut out. When the plate is driven as an antenna by an applied radio frequency current, the slot radiates electromagnetic waves in a way similar to a ...


Results

During a close pass in summer of 2017 when MWR was operated at Jupiter, it detected temperature changes deep within the Great Red Spot (GRS) storm. On Perijove 7, which was the sixth science orbit MWR took readings of Jupiter's great red storm down to dozens of kilometers/miles of depth below the surface layers. The distribution of ammonia gas was reported on in 2017, and analyzed. An ammonia rich layer was identified, as well as a belt of ammonia poor atmosphere from 5 to 20 degrees north. During the first eight orbits, WMR detected hundreds of lightning discharges, mostly in the polar regions.


See also

* ''Galileo'' probe (''in situ'' Atmospheric probe for Jupiter, entered and descended in 1995) * Gravity Science *
Jovian Auroral Distributions Experiment Jovian Auroral Distributions Experiment (JADE) is an instrument that detects and measures ions and electrons around the spacecraft. It is a suite of detectors on the ''Juno'' Jupiter orbiter (launched 2011, orbiting Jupiter since 2016). JADE incl ...
* Waves (''Juno'')


References


External links


NASA ''Juno'' Spacecraft and InstrumentsPIA22177: Slices of Jupiter's Great Red Spot
{{Junojupiternav Spacecraft instruments Juno (spacecraft)