Juno (spacecraft)

Juno's name comes from Greek and Roman mythology. The god Jupiter drew a veil of clouds around himself to hide his mischief, and his wife, the goddess Juno, was able to peer through the clouds and reveal Jupiter's true nature.

— NASA ^[11]

A NASA compilation of mission names and acronyms referred to the mission by the backronym Jupiter Near-polar Orbiter. ^[12] However the project itself has consistently described it as a name with mythological associations ^[13] and not an acronym. The spacecraft's current name is in reference to the Roman goddess Juno. ^[11] Juno is sometimes called the New Frontiers 2 as the second mission in the New Frontiers program, ^{[14] [15]} but is not to be confused with New Horizons 2, a proposed but unselected New Frontiers mission.

Overview

Juno's interplanetary trajectory; tick marks at 30-day intervals.

Juno spacecraft trajectory animation

Animation of Juno's trajectory from August 5, 2011
  Juno ·   Earth  ·   Mars  ·   Jupiter

Juno was selected on June 9, 2005, as the next New Frontiers mission after New Horizons . ^[16] The desire for a Jupiter probe was strong in the years prior to this, but there had not been any approved missions. ^{[17] [18]} The Discovery Program had passed over the somewhat similar but more limited Interior Structure and Internal Dynamical Evolution of Jupiter (INSIDE Jupiter) proposal, ^[18] and the turn-of-the-century era Europa Orbiter was canceled in 2002. ^[17] The flagship-level Europa Jupiter System Mission was in the works in the early 2000s, but funding issues resulted in it evolving into ESA's Jupiter Icy Moons Explorer. ^[19]

Juno completed a five-year cruise to Jupiter, arriving on July 5, 2016. ^[7] The spacecraft traveled a total distance of roughly 2.8×10^⁹ km (19 AU; 1.7×10^⁹ mi) to reach Jupiter. ^[20] The spacecraft was designed to orbit Jupiter 37 times over the course of its mission. This was originally planned to take 20 months. ^{[4] [5]}

Juno's trajectory used a gravity assist speed boost from Earth, accomplished by an Earth flyby in October 2013, two years after its launch on August 5, 2011. ^[21] The spacecraft performed an orbit insertion burn to slow it enough to allow capture. It was expected to make three 53-day orbits before performing another burn on December 11, 2016, that would bring it into a 14-day polar orbit called the Science Orbit. Because of a suspected problem in Juno's main engine, the burn scheduled on December 11, 2016, was cancelled and Juno remained in its 53-day orbit until the first Ganymede encounter of its Extended Mission. ^[22] This extended mission began with a flyby of Ganymede on June 7, 2021. ^{[23] [24]} Subsequent flybys of Europa and then Io will further decrease the orbital period to 33 days by February 2024. ^[25]

During the science mission, infrared and microwave instruments will measure the thermal radiation emanating from deep within Jupiter's atmosphere. These observations will complement previous studies of its composition by assessing the abundance and distribution of water, and therefore oxygen. This data will provide insight into Jupiter's origins. Juno will also investigate the convection that drives natural circulation patterns in Jupiter's atmosphere. Other instruments aboard Juno will gather data about its gravitational field and polar magnetosphere. The Juno mission was planned to conclude in February 2018 after completing 37 orbits of Jupiter, but now has been commissioned through 2025 to do a further 42 additional orbits of Jupiter as well as close flybys of Ganymede, Europa and Io. ^[26] The probe was then intended to be deorbited and burnt up in Jupiter's outer atmosphere ^{[4] [5]} to avoid any possibility of impact and biological contamination of one of its moons. ^[27]

Flight trajectory

Juno awaiting its launch in 2011

Launch

Juno was launched atop an Atlas V (551 configuration) at Cape Canaveral Air Force Station (CCAFS), Florida on August 5, 2011, 16:25:00 UTC. The Atlas V (AV-029) used a Russian-built RD-180 main engine, powered by kerosene and liquid oxygen. The main engine ignited and underwent checkout then, 3.8 seconds later, the five strap-on solid rocket boosters (SRBs) ignited. Following the SRB burnout, about 93 seconds into the flight, two of the spent boosters fell away from the vehicle, followed 1.5 seconds later by the remaining three. When heating levels had dropped below predetermined limits, the payload fairing that protected Juno during launch and transit through the thickest part of the atmosphere separated, about 3 minutes 24 seconds into the flight. The Atlas V main engine cut off 4 minutes 26 seconds after liftoff. Sixteen seconds later, the Centaur second stage ignited, and it burned for about 6 minutes, putting the satellite into an initial parking orbit. ^[28] The vehicle coasted for about 30 minutes, and then the Centaur was reignited for a second firing of 9 minutes, placing the spacecraft on an Earth escape trajectory in a heliocentric orbit. ^[28]

Prior to separation, the Centaur stage used onboard reaction engines to spin Juno up to 1.4 r.p.m. About 54 minutes after launch, the spacecraft separated from the Centaur and began to extend its solar panels. ^[28] Following the full deployment and locking of the solar panels, Juno's batteries began to recharge. Deployment of the solar panels reduced Juno's spin rate by two-thirds. The probe is spun to ensure stability during the voyage and so that all instruments on the probe are able to observe Jupiter. ^{[27] [29]}

The voyage to Jupiter took five years, and included two orbital maneuvers in August and September 2012 and a flyby of the Earth on October 9, 2013. ^{[30] [31]} When it reached the Jovian system, Juno had traveled approximately 19 astronomical units (2.8 billion kilometres). ^[32]

• 
  Atlas V on launch pad
• 
  Lift-off
• Launch video

Flyby of the Earth

South America ^[33] as seen by JunoCam on its October 2013 Earth flyby

Video of Earth and Moon taken by the Juno spacecraft

After traveling for about a year in an elliptical heliocentric orbit, Juno fired its engine twice in 2012 near aphelion (beyond the orbit of Mars) to change its orbit and return to pass by the Earth at a distance of 559 kilometers in October 2013. ^[30] It used Earth's gravity to help slingshot itself toward the Jovian system in a maneuver called a gravity assist. ^[34] The spacecraft received a boost in speed of more than 3.9 km/s (8,700 mph), and it was set on a course to Jupiter. ^{[34] [35] [36]} The flyby was also used as a rehearsal for the Juno science team to test some instruments and practice certain procedures before the arrival at Jupiter. ^{[34] [37]}

Insertion into Jovian orbit

Jupiter's gravity accelerated the approaching spacecraft to around 210,000 km/h (130,000 mph). ^[38] On July 5, 2016, between 03:18 and 03:53 UTC Earth-received time, an insertion burn lasting 2,102 seconds decelerated Juno by 542 m/s (1,780 ft/s) ^[39] and changed its trajectory from a hyperbolic flyby to an elliptical, polar orbit with a period of about 53.5 days. ^[40] The spacecraft successfully entered Jovian orbit on July 5, 2016, at 03:53 UTC. ^[3]

Orbit and environment

Juno's elliptical orbit and the Jovian radiation belts

Juno's highly elliptical initial polar orbit takes it within 4,200 km (2,600 mi) of the planet and out to 8.1×10^⁶ km (5.0×10^⁶ mi), far beyond Callisto's orbit. An eccentricity-reducing burn, called the Period Reduction Maneuver, was planned that would drop the probe into a much shorter 14 day science orbit. ^[41] Originally, Juno was expected to complete 37 orbits over 20 months before the end of its mission. Due to problems with helium valves that are important during main engine burns, mission managers announced on February 17, 2017, that Juno would remain in its original 53-day orbit, since the chance of an engine misfire putting the spacecraft into a bad orbit was too high. ^[22] Juno completed only 12 science orbits before the end of its budgeted mission plan, ending July 2018. ^[42] In June 2018, NASA extended the mission through July 2021, as described below.

The orbits were carefully planned in order to minimize contact with Jupiter's dense radiation belts, which can damage spacecraft electronics and solar panels, by exploiting a gap in the radiation envelope near the planet, passing through a region of minimal radiation. ^{[8] [43]} The "Juno Radiation Vault", with 1-centimeter-thick titanium walls (three times as thick as the Galileo spacecraft body's), also aids in protecting Juno's electronics by reducing the incoming radiation by a factor of 800. ^[44] Despite the intense radiation, JunoCam and the Jovian Infrared Auroral Mapper (JIRAM) are expected to endure at least eight orbits, while the Microwave Radiometer (MWR) should endure at least eleven orbits. ^[45] Although the flux of electrons close to Jupiter is about ten times as high as it is around Jupiter's moon Europa, ^[46] Juno will still receive a lower total dose of radiation in its polar orbit (20 mrad through end of mission) ^[47] than the Galileo orbiter received in its equatorial orbit. Galileo's subsystems were damaged by radiation during its mission, including an LED in its data recording system. ^[48]

Orbital operations

Animation of Juno's trajectory around Jupiter from June 1, 2016, to October 25, 2025
  Juno ·   Jupiter

Ganymede, photographed on 7 June 2021 by Juno during its extended mission

The spacecraft completed its first flyby of Jupiter (perijove 1) on August 26, 2016, and captured the first images of the planet's north pole. ^[49]

On October 14, 2016, days prior to perijove 2 and the planned Period Reduction Maneuver, telemetry showed that some of Juno's helium valves were not opening properly. ^[50] On October 18, 2016, some 13 hours before its second close approach to Jupiter, Juno entered into safe mode, an operational mode engaged when its onboard computer encounters unexpected conditions. The spacecraft powered down all non-critical systems and reoriented itself to face the Sun to gather the most power. Due to this, no science operations were conducted during perijove 2. ^[51]

On December 11, 2016, the spacecraft completed perijove 3, with all but one instrument operating and returning data. One instrument, JIRAM, was off pending a flight software update. ^[52] Perijove 4 occurred on February 2, 2017, with all instruments operating. ^[22] Perijove 5 occurred on March 27, 2017. ^[53] Perijove 6 took place on May 19, 2017. ^{[53] [54]}

Although the mission's lifetime is inherently limited by radiation exposure, almost all of this dose was planned to be acquired during the perijoves. As of 2017 ^[update] , the 53.4 day orbit was planned to be maintained through July 2018 for a total of twelve science-gathering perijoves. At the end of this prime mission, the project was planned to go through a science review process by NASA's Planetary Science Division to determine if it will receive funding for an extended mission. ^[22]

In June 2018, NASA extended the mission operations plan to July 2021. ^[55]

In January 2021, NASA extended the mission operations to September 2025. ^[56] In this phase Juno began to examine Jupiter's inner moons, Ganymede, Europa and Io. A flyby of Ganymede occurred on June 7, 2021, 17:35 UTC, coming within 1,038 km (645 mi), the closest any spacecraft has come to the moon since Galileo in 2000. ^{[23] [24] [57]} A flyby of Europa took place on September 29, 2022, at a distance of 352 km (219 mi). ^{[58] [59]} Juno performed two flybys of Io on December 30, 2023, and February 3, 2024, gathering observational data on volcanic activity. From April 2024, Juno will begin a series of experiments to learn more about Jupiter's interior shape and structure. ^[60]

Planned deorbit and disintegration

NASA originally planned to deorbit the spacecraft into the atmosphere of Jupiter after completing 32 orbits of Jupiter, but has since extended the mission to September 2025. ^{[61] [56]} The controlled deorbit is intended to eliminate space debris and risks of contamination in accordance with NASA's planetary protection guidelines. ^{[62] [63] [64]}

Team

Scott Bolton of the Southwest Research Institute in San Antonio, Texas is the principal investigator and is responsible for all aspects of the mission. The Jet Propulsion Laboratory in California manages the mission and the Lockheed Martin Corporation was responsible for the spacecraft development and construction. The mission is being carried out with the participation of several institutional partners. Coinvestigators include Toby Owen of the University of Hawaii, Andrew Ingersoll of California Institute of Technology, Frances Bagenal of the University of Colorado at Boulder, and Candy Hansen of the Planetary Science Institute. Jack Connerney of the Goddard Space Flight Center served as instrument lead. ^{[65] [66]}

Cost

Juno was originally proposed at a cost of approximately US$700 million (fiscal year 2003) for a launch in June 2009 (equivalent to US$1159 million in 2023). NASA budgetary restrictions resulted in postponement until August 2011, and a launch on board an Atlas V rocket in the 551 configuration. As of 2019 ^[update] the mission was projected to cost US$1.46 billion for operations and data analysis through 2022. ^[67]

Scientific objectives

Jupiter imaged using the VISIR instrument on the VLT. These observations will inform the work to be undertaken by Juno.

The Juno spacecraft's suite of science instruments will: ^[69]

• Determine the ratio of oxygen to hydrogen, effectively measuring the abundance of water in Jupiter, which will help distinguish among prevailing theories linking Jupiter's formation to the Solar System.
• Obtain a better estimate of Jupiter's core mass, which will also help distinguish among prevailing theories linking Jupiter's formation to the Solar System.
• Precisely map Jupiter's gravitational field to assess the distribution of mass in Jupiter's interior, including properties of its structure and dynamics.
• Precisely map Jupiter's magnetic field to assess the origin and structure of the field, and the depth at which the planet's magnetic field is created. This experiment will also help scientists understand the fundamental physics of dynamo theory.
• Map the variation in atmospheric composition, temperature, structure, cloud opacity and dynamics to pressures far greater than 100 bar (10 MPa; 1,500 psi) at all latitudes.
• Characterize and explore the three-dimensional structure of Jupiter's polar magnetosphere and auroras. ^[69]
• Measure the orbital frame-dragging, known also as Lense–Thirring precession caused by the angular momentum of Jupiter, ^{[70] [71]} and possibly a new test of general relativity effects connected with the Jovian rotation. ^[72]

Scientific instruments

The Juno mission's scientific objectives are being achieved with a payload of nine instruments on board the spacecraft: ^{[73] [74] [75] [76] [77]}

Microwave radiometer (MWR)

Main article: Microwave Radiometer (Juno)

Microwave Radiometer

The microwave radiometer comprises six antennas mounted on two of the sides of the body of the probe. They will perform measurements of electromagnetic waves on frequencies in the microwave range: 600 MHz, 1.2, 2.4, 4.8, 9.6 and 22 GHz, the only microwave frequencies which are able to pass through the thick Jovian atmosphere. The radiometer will measure the abundance of water and ammonia in the deep layers of the atmosphere up to 200 bar (20 MPa; 2,900 psi) pressure or 500–600 km (310–370 mi) deep. The combination of different wavelengths and the emission angle should make it possible to obtain a temperature profile at various levels of the atmosphere. The data collected will determine how deep the atmospheric circulation is. ^{[78] [79]} The MWR is designed to function through orbit 11 of Jupiter. ^[80]
(Principal investigator: Mike Janssen, Jet Propulsion Laboratory)

Jovian Infrared Auroral Mapper (JIRAM)

Main article: Jovian Infrared Auroral Mapper

Jovian Infrared Auroral Mapper

The spectrometer mapper JIRAM, operating in the near infrared (between 2 and 5 μm), conducts surveys in the upper layers of the atmosphere to a depth of between 50 and 70 km (31 and 43 mi) where the pressure reaches 5 to 7 bar (500 to 700 kPa). JIRAM will provide images of the aurora in the wavelength of 3.4 μm in regions with abundant H₃⁺ ions. By measuring the heat radiated by the atmosphere of Jupiter, JIRAM can determine how clouds with water are flowing beneath the surface. It can also detect methane, water vapor, ammonia and phosphine. It was not required that this device meets the radiation resistance requirements. ^{[81] [82] [83]} The JIRAM instrument is expected to operate through the eighth orbit of Jupiter. ^[80]
(Principal investigator: Alberto Adriani, Italian National Institute for Astrophysics)

JIRAM's spin-compensation mirror is stuck since PJ44, but the instrument is operational. ^[84]

Magnetometer (MAG)

Main article: Magnetometer (Juno)

MAG

The magnetic field investigation has three goals: mapping of the magnetic field, determining the dynamics of Jupiter's interior, and determination of the three-dimensional structure of the polar magnetosphere. The magnetometer experiment consists of the Flux Gate Magnetometer (FGM), which will observe the strength and direction of the magnetic field lines, and the Advanced Stellar Compass (ASC), which will monitor the orientation of the magnetometer sensors. ^[75]
(Principal investigator: Jack Connerney, NASA's Goddard Space Flight Center)

Gravity Science (GS)

Main article: Gravity Science (Juno)

Gravity Science

The purpose of measuring gravity by radio waves is to establish a map of the distribution of mass inside Jupiter. The uneven distribution of mass in Jupiter induces small variations in gravity all along the orbit followed by the probe when it runs closer to the surface of the planet. These gravity variations drive small probe velocity changes. The purpose of radio science is to detect the Doppler effect on radio broadcasts issued by Juno toward Earth in Ka-band and X-band, which are frequency ranges that can conduct the study with fewer disruptions related to the solar wind or Jupiter's ionosphere. ^{[85] [86] [74]}
(Principal investigator: John Anderson, Jet Propulsion Laboratory; Principal investigator (Juno's Ka-band Translator): Luciano Iess, Sapienza University of Rome)

Jovian Auroral Distributions Experiment (JADE)

Main article: Jovian Auroral Distributions Experiment

JADE

The energetic particle detector JADE will measure the angular distribution, energy, and the velocity vector of ions and electrons at low energy (ions between 13 eV and 20 KeV, electrons of 200 eV to 40 KeV) present in the aurora of Jupiter. On JADE, like JEDI, the electron analyzers are installed on three sides of the upper plate which allows a measure of frequency three times higher. ^{[74] [87]}
(Principal investigator: David McComas, Southwest Research Institute)

Jovian Energetic Particle Detector Instrument (JEDI)

Main article: Jovian Energetic Particle Detector Instrument

JEDI

The energetic particle detector JEDI will measure the angular distribution and the velocity vector of ions and electrons at high energy (ions between 20 keV and 1 MeV, electrons from 40 to 500 keV) present in the polar magnetosphere of Jupiter. JEDI has three identical sensors dedicated to the study of particular ions of hydrogen, helium, oxygen and sulfur. ^{[74] [88]}
(Principal investigator: Barry Mauk, Applied Physics Laboratory)

Radio and Plasma Wave Sensor (Waves)

Main article: Waves (Juno)

Radio and Plasma Wave Sensor

This instrument will identify the regions of auroral currents that define Jovian radio emissions and acceleration of the auroral particles by measuring the radio and plasma spectra in the auroral region. It will also observe the interactions between Jupiter's atmosphere and magnetosphere. The instrument consists of two antennae that detect radio and plasma waves. ^[75]
(Principal investigator: William Kurth, University of Iowa)

Ultraviolet Spectrograph (UVS)

Main article: UVS (Juno)

Ultraviolet Spectrograph

UVS will record the wavelength, position and arrival time of detected ultraviolet photons during the time when the spectrograph slit views Jupiter during each turn of the spacecraft. The instrument will provide spectral images of the UV auroral emissions in the polar magnetosphere. ^[75]
(Principal investigator: G. Randall Gladstone, Southwest Research Institute)

JunoCam (JCM)

Main article: JunoCam

JunoCam

A visible light camera/telescope, included in the payload to facilitate education and public outreach; later re-purposed to study the dynamics of Jupiter's clouds, particularly those at the poles. ^[89] It was anticipated that it would operate through only eight orbits of Jupiter ending in September 2017 ^[90] due to the planet's damaging radiation and magnetic field, ^[80] but as of October 2023 (55 orbits), JunoCam remains operational. ^[91]
(Principal investigator: Michael C. Malin, Malin Space Science Systems)

Locations of Juno's science instruments

Interactive 3D model of Juno

Operational components

Solar panels

Illumination test on one of Juno's solar panels

Juno is the first mission to Jupiter to use solar panels instead of the radioisotope thermoelectric generators (RTG) used by Pioneer 10 , Pioneer 11 , the Voyager program, Ulysses , Cassini–Huygens , New Horizons , and the Galileo orbiter. ^[92] It is also the farthest solar-powered trip in the history of space exploration. ^[93] Once in orbit around Jupiter, Juno receives only 4% as much sunlight as it would on Earth, but the global shortage of plutonium-238 at the time, ^{[94] [95] [96] [97]} as well as advances made in solar cell technology over the past several decades, makes it economically preferable to use solar panels of practical size to provide power at a distance of 5 a.u. from the Sun. ^[98]

The Juno spacecraft uses three solar panels symmetrically arranged around the spacecraft. Shortly after it cleared Earth's atmosphere, the panels were deployed. Two of the panels have four hinged segments each, and the third panel has three segments and a magnetometer. Each panel is 2.7 by 8.9 m (8 ft 10 in by 29 ft 2 in) ^[99] providing 50 square metres (540 sq ft) of active cells ^{[100] [101]} – the largest on any NASA deep-space probe at the time of launching. ^[102]

The combined mass of the three panels is nearly 340 kg (750 lb). ^[103] If the panels were optimized to operate at Earth, they would produce 12 to 14 kilowatts of power. Only about 486 watts were generated when Juno arrived at Jupiter, projected to decline to near 420 watts as radiation degrades the cells. ^[104] The solar panels will remain in sunlight continuously from launch through the end of the mission, except for short periods during the operation of the main engine and eclipses by Jupiter. A central power distribution and drive unit monitors the power that is generated by the solar panels and distributes it to instruments, heaters, and experiment sensors, as well as to batteries that are charged when excess power is available. Two 55 Ah lithium-ion batteries that are able to withstand the radiation environment of Jupiter provide power when Juno passes through eclipse. ^[105]

Telecommunications

Juno's high-gain antenna dish being installed

Juno uses in-band signaling ("tones") for several critical operations as well as status reporting during cruise mode, ^[106] but it is expected to be used infrequently. Communications are via the 34 m (112 ft) and 70 m (230 ft) antennas of the NASA Deep Space Network (DSN) utilizing an X-band direct link. ^[105] The command and data processing of the Juno spacecraft includes a flight computer capable of providing about 50 Mbit/s of instrument throughput. Gravity science subsystems use the X-band and K_a-band Doppler tracking and autoranging. ^[107]

Due to telecommunications constraints, Juno will only be able to return about 40 megabytes of JunoCam data during each 11-day orbital period, limiting the number of images that are captured and transmitted during each orbit to somewhere between 10 and 100 depending on the compression level used. ^{[108] [ needs update ]} The overall amount of data downlinked on each orbit is significantly higher and used for the mission's scientific instruments; JunoCam is intended for public outreach and is thus secondary to the science data. This is comparable to the previous Galileo mission that orbited Jupiter, which captured thousands of images ^[109] despite its slow data rate of 1000 bit/s (at maximum compression level) due to the failure of its high gain antenna.

The communication system is also used as part of the Gravity Science experiment. ^[110]

Propulsion

Juno uses a LEROS 1b main engine with hypergolic propellant, manufactured by Moog Inc in Westcott, Buckinghamshire, England. ^[111] It uses approx. 2,000 kg (4,400 lb) of hydrazine and nitrogen tetroxide for propulsion, including 1,232 kg (2,716 lb) available for the Jupiter Orbit Insertion plus subsequent orbital maneuvers. The engine provides a thrust of 645 newtons. The engine bell is enclosed in a debris shield fixed to the spacecraft body, and is used for major burns. For control of the vehicle's orientation (attitude control) and to perform trajectory correction maneuvers, Juno utilizes a monopropellant reaction control system (RCS) consisting of twelve small thrusters that are mounted on four engine modules. ^[105]

Galileo plaque and minifigures

Galileo Galilei plaque

Juno carries a plaque to Jupiter, dedicated to Galileo Galilei. The plaque was provided by the Italian Space Agency (ASI) and measures 7.1 by 5.1 cm (2.8 by 2.0 in). It is made of flight-grade aluminum and weighs 6 g (0.21 oz). ^[112] The plaque depicts a portrait of Galileo and a text in Galileo's own handwriting, penned in January 1610, while observing what would later be known to be the Galilean moons. ^[112] The text translates as:

On the 11th it was in this formation – and the star closest to Jupiter was half the size than the other and very close to the other so that during the previous nights all of the three observed stars looked of the same dimension and among them equally afar; so that it is evident that around Jupiter there are three moving stars invisible till this time to everyone.

The spacecraft also carries three Lego minifigures representing Galileo Galilei, the Roman god Jupiter, and his sister and wife, the goddess Juno. In Roman mythology, Jupiter drew a veil of clouds around himself to hide his mischief. Juno was able to peer through the clouds and reveal Jupiter's true nature. The Juno minifigure holds a magnifying glass as a sign of searching for the truth, and Jupiter holds a lightning bolt. The third Lego crew member, Galileo Galilei, has his telescope with him on the journey. ^[113] The figurines were produced in partnership between NASA and Lego as part of an outreach program to inspire children's interest in science, technology, engineering, and mathematics (STEM). ^[114] Although most Lego toys are made of plastic, Lego specially made these minifigures of aluminum to endure the extreme conditions of space flight. ^[115]

Scientific results

Among early results, Juno gathered information about Jovian lightning that revised earlier theories. ^[116] Juno provided the first views of Jupiter's north pole, as well as providing insight about Jupiter's aurorae, magnetic field, and atmosphere. ^[117]

In 2021, analysis of the frequency of interplanetary dust impacts (primarily on the backs of the solar panels), as Juno passed between Earth and the asteroid belt, indicated that this dust, which causes the Zodiacal light, comes from Mars, rather than from comets or asteroids that come from the outer solar system, as was previously thought. ^[118]

Juno made many discoveries that are challenging existing theories about Jupiter's formation. When Juno flew over the poles of Jupiter it imaged clusters of stable cyclones that exist at the poles. ^[119] It found that the magnetosphere of Jupiter is uneven and chaotic. Using its Microwave Radiometer, Juno found that the red and white bands that can be seen on Jupiter extend hundreds of kilometers into the Jovian atmosphere, yet the interior of Jupiter is not evenly mixed. This has resulted in the theory that Jupiter does not have a solid core as previously thought, but a "fuzzy" core made of pieces of rock and metallic hydrogen. This peculiar core may be a result of a collision that happened early on in Jupiter's formation. ^[120]

In April 2020, Juno detected a meteor impact on Jupiter, with estimated mass of 250-5000 kg. ^[121]

Results from Juno on storms suggests that they are far taller than expected, with some extending 60 miles (100 kilometers) below the cloud tops and others, including the Great Red Spot, extending over 200 miles (350 kilometers). With Juno traveling low over Jupiter's cloud deck at about 130,000 mph (209,000 kph) Juno scientists were able to measure velocity changes as small 0.01 millimeter per second using a NASA's Deep Space Network tracking antenna, from a distance of more than 400 million miles (650 million kilometers). This enabled the team to constrain the depth of the Great Red Spot to about 300 miles (500 kilometers) below the cloud tops. The new results show that the cyclones are warmer on top, with lower atmospheric densities, while they are colder at the bottom, with higher densities. Anticyclones, which rotate in the opposite direction, are colder at the top but warmer at the bottom. ^[122]

Juno

Artist's rendering of the Juno spacecraft
Names	New Frontiers 2
Mission type	Jupiter orbiter
Operator	NASA  / Jet Propulsion Laboratory
COSPAR ID	2011-040A
SATCAT no.	37773
Website	www.nasa.gov/mission_pages/juno/main/index.html (NASA) www.missionjuno.swri.edu (SwRI)
Mission duration	Planned: 7 years Elapsed: 13 years, 1 month, 14 days Cruise: 4 years, 10 months, 29 days Science phase: 3 years, 1 month and 21 days (in progress; extended until September 2025)
Spacecraft properties
Manufacturer	Lockheed Martin Space
Launch mass	3,625 kg (7,992 lb) [1]
Dry mass	1,593 kg (3,512 lb) [2]
Dimensions	20.1 × 4.6 m (66 × 15 ft) [2]
Power	14 kW at Earth, [2] 435 W at Jupiter [1] 2 × 55-ampere hour lithium-ion batteries [2]
Start of mission
Launch date	August 5, 2011, 16:25:00 UTC
Rocket	Atlas V 551 (AV-029)
Launch site	Cape Canaveral, SLC-41
Contractor	United Launch Alliance
Flyby of Earth
Closest approach	October 9, 2013
Distance	559 km (347 mi)

Date (UTC)	Event	Latitude (centric) [123]	Longitude (Sys. III) [123]
August 5, 2011, 16:25:00	Launched [124]
August 5, 2012, 06:57:00	Deep Space Maneuvers [125] (total dV: 345 m/s + 385 m/s) [126]
September 3, 2012, 06:30:00
October 9, 2013, 19:21:00	Earth gravity assist (from 126,000 to 150,000 km/h (78,000 to 93,000 mph)) [127] — Gallery
July 5, 2016, 03:53:00	Arrival at Jupiter and polar orbit insertion (1st orbit). [4] [5]	3°	30°
August 27, 2016, 12:50:44	Perijove 1 [128] — Gallery	4°	100°
October 19, 2016, 18:10:53	Perijove 2: Planned Period Reduction Maneuver, but the main engine's fuel pressurisation system did not operate as expected. [129]	5°	350°
December 11, 2016, 17:03:40	Perijove 3 [130] [131]	6°	10°
February 2, 2017, 12:57:09	Perijove 4 [131] [132]	7°	270°
March 27, 2017, 08:51:51	Perijove 5 [53]	8°	180°
May 19, 2017, 06:00:47	Perijove 6 [54]	8°	140°
July 11, 2017, 01:54:42	Perijove 7: Flyover of the Great Red Spot [133] [134]	9°	50°
September 1, 2017, 21:48:50	Perijove 8 [135]	10°	320°
October 24, 2017, 17:42:31	Perijove 9 [136]	11°	230°
December 16, 2017, 17:56:59	Perijove 10 [137] [138]	12°	300°
February 7, 2018, 13:51:49	Perijove 11 [124]	13°	210°
April 1, 2018, 09:45:57	Perijove 12 [124]	14°	110°
May 24, 2018, 05:40:07	Perijove 13 [124]	15°	20°
July 16, 2018, 05:17:38	Perijove 14 [124]	16°	70°
September 7, 2018, 01:11:55	Perijove 15 [124]	17°	340°
October 29, 2018, 21:06:15	Perijove 16 [124]	17°	250°
December 21, 2018, 17:00:25	Perijove 17 [139] [124]	18°	160°
February 12, 2019, 16:19:48	Perijove 18 [124]	19°	240°
April 6, 2019, 12:13:58	Perijove 19 [124]	20°	100°
May 29, 2019, 08:08:13	Perijove 20 [124]	20°	10°
July 21, 2019, 04:02:44	Perijove 21 [140] [124]	21°	280°
September 12, 2019, 03:40:47	Perijove 22 [140] [124]	22°	320°
November 3, 2019, 23:32:56	Perijove 23 [124]	22°	190°
December 26, 2019, 16:58:59	Perijove 24: Distant Ganymede flyby [124] [141]	23°	70°
February 17, 2020, 17:51:36	Perijove 25 [124]	23°	140°
April 10, 2020, 14:24:34	Perijove 26 [124]	24°	50°
June 2, 2020, 10:19:55	Perijove 27 [124]	25°	340°
July 25, 2020, 06:15:21	Perijove 28 [124]	25°	250°
September 16, 2020, 02:10:49	Perijove 29 [124]	26°	160°
November 8, 2020, 01:49:39	Perijove 30 [124]	27°	210°
December 30, 2020, 21:45:12	Perijove 31 [124]	27°	120°
February 21, 2021, 17:40:31	Perijove 32 [124]	28°	30°
April 15, 2021, 13:36:26	Perijove 33 [124] [142]	29°	300°
June 8, 2021, 07:46:00	Perijove 34: Ganymede flyby, coming within 1,038 km (645 mi) of the moon's surface. [23] Orbital period reduced from 53 days to 43 days. [143] [124] [123]	28°	290°
July 21, 2021, 08:15:05	Perijove 35: End of first mission extension. [143] Originally scheduled for July 30, 2021, prior to approval of second mission extension. [144]	29°	300°
September 2, 2021	Perijove 36 [124]	30°	100°
October 16, 2021	Perijove 37 [124]	31°	40°
November 29, 2021	Perijove 38 [124]	31°	80°
January 12, 2022	Perijove 39 [124]	32°	90°
February 25, 2022	Perijove 40 [124]	33°	280°
April 9, 2022	Perijove 41 [124]	34°	60°
May 23, 2022	Perijove 42 [124]	35°	70°
July 5, 2022	Perijove 43 [124]	36°	310°
August 17, 2022	Perijove 44 [124]	37°	150°
September 29, 2022, 09:36	Perijove 45: Europa flyby. Closest approach: 352 km (219 mi). Orbital period reduced from 43 days to 38 days. [58] [59] [123]	37°	230°
November 6, 2022	Perijove 46 [124]	38°	350°
December 15, 2022	Perijove 47: Io flyby on Dec 14, 2022. Closest approach: 64,000 km (40,000 mi). [124]	39°	160°
January 22, 2023	Perijove 48 [124]	40°	200°
March 1, 2023	Perijove 49 [124]	41°	170°
April 8, 2023	Perijove 50 [124]	42°	210°
May 16, 2023	Perijove 51 [124]	43°	140°
June 23, 2023	Perijove 52 [124]	44°	80°
July 31, 2023	Perijove 53: Io flyby on July 30, 2023. Closest approach: 22,000 km (14,000 mi). [145]	45°	120°
September 7, 2023	Perijove 54 [124]	45°	190°
October 15, 2023	Perijove 55 [124]	46°	110°
November 22, 2023	Perijove 56 [124]	47°	120°
December 30, 2023	Perijove 57: Io flyby. Closest approach: 1,500 km (930 mi). [146]	47°	90°
February 3, 2024	Perijove 58: Io flyby. Closest approach: 1,500 km (930 mi). [146] Orbital period reduced from 38 to 33 days. [143] [123]	48°	290°
March 7, 2024	Perijove 59 [123]	49°	0°
April 9, 2024	Perijove 60 [123]	50°	40°
May 12, 2024	Perijove 61 [123]	51°	250°
June 14, 2024	Perijove 62 [123]	52°	60°
July 17, 2024	Perijove 63 [123]	53°	260°
August 18, 2024	Perijove 64 [123]	54°	40°
September 20, 2024	Perijove 65 [123]	55°	240°
October 23, 2024	Perijove 66 [123]	56°	20°
November 25, 2024	Perijove 67 [123]	57°	120°
December 28, 2024	Perijove 68 [123]	57°	310°
January 30, 2025	Perijove 69 [123]	58°	110°
March 4, 2025	Perijove 70 [123]	59°	0°
April 5, 2025	Perijove 71 [123]	60°	210°
May 8, 2025	Perijove 72 [123]	61°	50°
June 10, 2025	Perijove 73 [123]	62°	320°
July 13, 2025	Perijove 74 [123]	63°	180°
August 15, 2025	Perijove 75 [123]	63°	80°
September 17, 2025	Perijove 76: End of second mission extension. [143] [123]	64°	320°

Gallery

Jupiter

• 
  Perijove 26 image
• 
  Image from about 94,500 km (58,700 mi) of Jupiter's southern polar region (27 August 2016)
• 
  Jupiter growing and shrinking in apparent size before and after the spacecraft made its closest approach (27 August 2016)
• 
  Infrared view of the southern aurora of Jupiter (27 August 2016)
• 
  Southern storms of Jupiter
• 
  Area of Jupiter where multiple atmospheric conditions appear to collide (27 March 2017)
• 
  Retreating from Jupiter, about 46,900 km (29,100 mi) above the cloud tops (19 May 2017)
• 
  Image taken from 16,535 km (10,274 mi) above the atmosphere at a latitude of −36.9° (10 July 2017)
• 
  Closeup of the Great Red Spot taken from about 8,000 km (5,000 mi) above it (11 July 2017)
• 
  The Great Red Spot as seen by JunoCam in April 2018
• 
  Jupiter viewed by Juno
  (12 February 2019)
• Jupiter flyover
  (Juno; 05:07; 2 June 2020)
• 
  Photograph taken at the end of Perijove 15 (September 6, 2018)

Moons

• 
  Ganymede, taken by the JunoCam instrument during Juno's flyby on 7 June 2021 ^[147]
• 
  Infrared view of Ganymede during the anniversary flyby by Juno
• 
  View of Europa taken during Juno's flyby on 29 September 2022

• 
  Low resolution view of Io captured by JunoCam (September 2017)
• 
  Io, as recorded by JunoCam
  (2 September 2017)
• 
  Plume near Io's terminator
  (21 December 2018) ^[148]
• 
  Io, viewed by JunoCam
  Several Volcanos
  (15 October 2023)
• 
  Io, viewed by JunoCam
  Volcanic plume
  (15 October 2023)
• 
  Io, taken by the JunoCam instrument during Juno's flyby
  (30 December 2023) ^[149]

See also

• Atmosphere of Jupiter
• Comet Shoemaker–Levy 9
• Europa Clipper
• Exploration of Jupiter
• Jupiter Icy Moons Explorer
• List of missions to the outer planets
• Moons of Jupiter

References

1. "Juno Mission to Jupiter" (PDF). NASA FACTS. NASA. April 2009. p. 1. Archived (PDF) from the original on April 6, 2020. Retrieved April 5, 2011. This article incorporates text from this source, which is in the public domain.
2. "Jupiter Orbit Insertion Press Kit" (PDF). NASA. 2016. Archived (PDF) from the original on August 14, 2016. Retrieved July 7, 2016. This article incorporates text from this source, which is in the public domain.
3. Foust, Jeff (July 5, 2016). "Juno enters orbit around Jupiter". SpaceNews. Archived from the original on December 31, 2016. Retrieved August 25, 2016.
4. Chang, Kenneth (July 5, 2016). "NASA's Juno Spacecraft Enters Jupiter's Orbit". The New York Times. Archived from the original on May 2, 2019. Retrieved July 5, 2016.
5. Greicius, Tony (September 21, 2015). "Juno – Mission Overview". NASA. Archived from the original on September 7, 2018. Retrieved October 2, 2015. This article incorporates text from this source, which is in the public domain.
6. Dunn, Marcia (August 5, 2011). "NASA probe blasts off for Jupiter after launch-pad snags". NBC News. Archived from the original on September 14, 2019. Retrieved August 31, 2011.
7. Chang, Kenneth (June 28, 2016). "NASA's Juno Spacecraft Will Soon Be in Jupiter's Grip". The New York Times. Archived from the original on August 14, 2018. Retrieved June 30, 2016.
8. Riskin, Dan (July 4, 2016). Mission Jupiter (Television documentary). Science Channel.
9. Cheng, Andrew; Buckley, Mike; Steigerwald, Bill (May 21, 2008). "Winds in Jupiter's Little Red Spot Almost Twice as Fast as Strongest Hurricane". NASA. Archived from the original on May 13, 2017. Retrieved August 9, 2017. This article incorporates text from this source, which is in the public domain .
10. "Juno's Solar Cells Ready to Light Up Jupiter Mission". NASA. July 15, 2011. Archived from the original on February 16, 2017. Retrieved October 4, 2015. This article incorporates text from this source, which is in the public domain .
11. "NASA's Juno Spacecraft Launches to Jupiter". NASA. August 5, 2011. Archived from the original on April 26, 2020. Retrieved August 5, 2011. This article incorporates text from this source, which is in the public domain.
12. "Mission Acronyms & Definitions" (PDF). NASA. Archived (PDF) from the original on September 25, 2020. Retrieved April 30, 2016. This article incorporates text from this source, which is in the public domain .
13. "Juno Launch Press Kit, Quick Facts" (PDF). jpl.nasa.gov. Jet Propulsion Lab. August 2011. Archived (PDF) from the original on June 17, 2019. Retrieved May 23, 2019. This article incorporates text from this source, which is in the public domain .
14. Leone, Dan (February 23, 2015). "NASA Sets Next US$1 Billion New Frontiers Competition for 2016". SpaceNews. Retrieved January 2, 2017.
15. Hillger, Don; Toth, Garry (September 20, 2016). "New Frontiers-series satellites". Colorado State University. Archived from the original on November 30, 2016. Retrieved January 2, 2017.
16. "Juno Mission to Jupiter". Astrobiology Magazine. June 9, 2005. Archived from the original on June 20, 2018. Retrieved December 7, 2016.
17. Ludwinski, Jan M.; Guman, Mark D.; Johannesen, Jennie R.; Mitchell, Robert T.; Staehle, Robert L. (1998). The Europa Orbiter Mission Design. 49th International Astronautical Congress, September 28 – October 2, 1998, Melbourne, Australia. hdl:2014/20516.
18. Zeller, Martin (January 2001). "NASA Announces New Discovery Program Awards". NASA and University of Southern California. Archived from the original on March 5, 2017. Retrieved December 25, 2016. This article incorporates text from this source, which is in the public domain .
19. Dougherty, M. K.; Grasset, O.; Bunce, E.; Coustenis, A.; Titov, D. V.; et al. (2011). JUICE (JUpiter ICy moon Explorer): a European-led mission to the Jupiter system (PDF). EPSC-DPS Joint Meeting 2011, October 2–7, 2011, Nantes, France. Bibcode:2011epsc.conf.1343D. Archived (PDF) from the original on November 21, 2011. Retrieved December 25, 2016.
20. Dunn, Marcia (August 1, 2011). "NASA going green with solar-powered Jupiter probe". USA Today. Archived from the original on April 26, 2020. Retrieved October 24, 2015.
21. "NASA's Shuttle and Rocket Launch Schedule". NASA. Archived from the original on September 13, 2008. Retrieved February 17, 2011. This article incorporates text from this source, which is in the public domain .
22. Brown, Dwayne; Cantillo, Laurie; Agle, D. C. (February 17, 2017). "NASA's Juno Mission to Remain in Current Orbit at Jupiter" (Press release). NASA. Archived from the original on February 20, 2017. Retrieved March 13, 2017. This article incorporates text from this source, which is in the public domain .
23. Greicius, Tony (June 3, 2021). "NASA's Juno to Get a Close Look at Jupiter's Moon Ganymede". NASA. Archived from the original on June 3, 2021. Retrieved June 4, 2021.
24. "See the First Images NASA's Juno Took as It Sailed by Ganymede | NASA". June 8, 2021. Archived from the original on June 9, 2021. Retrieved June 9, 2021.
25. "NASA's Juno Mission Expands Into the Future" (Press release). NASA. January 13, 2021. Archived from the original on January 23, 2021. Retrieved January 21, 2021. This article incorporates text from this source, which is in the public domain .
26. Carter, Jamie. "Self-Destruction Of $1.4 Billion Spacecraft At Jupiter Scrubbed By NASA As It Returns More Stunning Images". Forbes. Retrieved November 11, 2022.
27. Juno Mission Profile & Timeline Archived November 25, 2011, at the Wayback Machine
28. "Atlas/Juno launch timeline". Spaceflight Now. July 28, 2011. Archived from the original on March 17, 2021. Retrieved July 29, 2011.
29. "Juno's Solar Cells Ready to Light Up Jupiter Mission". NASA. June 27, 2016. Archived from the original on April 26, 2020. Retrieved July 5, 2016. This article incorporates text from this source, which is in the public domain .
30. Whigham, Nick (July 7, 2016). "The success of Juno's Jupiter mission has its origins in a famous idea from more than 50 years ago". news.com.au. Archived from the original on January 6, 2019. Retrieved January 5, 2019.
31. Wall, Mike (October 9, 2013). "NASA Spacecraft Slingshots By Earth On Way to Jupiter, Snaps Photos". Space.com. Archived from the original on January 6, 2019. Retrieved January 5, 2019.
32. Agle, D. C. (August 12, 2013). "NASA's Juno is Halfway to Jupiter". NASA/JPL. Archived from the original on August 2, 2020. Retrieved August 12, 2013. This article incorporates text from this source, which is in the public domain .
33. Greicius, Tony, ed. (March 25, 2014). "Earth Triptych from NASA's Juno Spacecraft". NASA. Archived from the original on November 13, 2016. Retrieved November 26, 2017. This article incorporates text from this source, which is in the public domain.
34. "Earth Flyby – Mission Juno". missionjuno.swri.edu. Archived from the original on October 3, 2015. Retrieved October 2, 2015.
35. "NASA's Juno Gives Starship-Like View of Earth Flyby". February 13, 2015. Archived from the original on March 3, 2020. Retrieved October 2, 2015. This article incorporates text from this source, which is in the public domain .
36. Greicius, Tony (August 26, 2013). "Juno Earth Flyby". NASA. Archived from the original on April 26, 2020. Retrieved October 8, 2015. This article incorporates text from this source, which is in the public domain .
37. Greicius, Tony (February 13, 2015). "NASA's Juno Gives Starship-Like View of Earth Flyby". Archived from the original on March 3, 2020. Retrieved July 5, 2016. This article incorporates text from this source, which is in the public domain .
38. Chang, Kenneth (July 5, 2016). "NASA's Juno Spacecraft Enters Jupiter's Orbit". The New York Times. Archived from the original on May 2, 2019. Retrieved July 5, 2016.
39. "NASA's Juno Spacecraft in Orbit Around Mighty Jupiter". NASA. July 4, 2016. Archived from the original on July 6, 2016. Retrieved July 5, 2016. This article incorporates text from this source, which is in the public domain .
40. Clark, Stephen (July 4, 2016). "Live coverage: NASA's Juno spacecraft arrives at Jupiter". Spaceflight Now. Archived from the original on July 5, 2016. Retrieved July 5, 2016.
41. Gebhardt, Chris (September 3, 2016). "Juno provides new data on Jupiter; readies for primary science mission". NASASpaceflight.com. Archived from the original on October 20, 2016. Retrieved October 23, 2016.
42. Clark, Stephen (February 21, 2017). "NASA's Juno spacecraft to remain in current orbit around Jupiter". Spaceflight Now. Archived from the original on February 26, 2017. Retrieved April 26, 2017.
43. Moomaw, Bruce (March 11, 2007). "Juno Gets A Little Bigger With One More Payload For Jovian Delivery". Space Daily. Archived from the original on January 26, 2021. Retrieved August 31, 2011.
44. "Juno Armored Up to Go to Jupiter". NASA. July 12, 2010. Archived from the original on August 13, 2016. Retrieved July 11, 2016. This article incorporates text from this source, which is in the public domain .
45. "Understanding Juno's Orbit: An Interview with NASA's Scott Bolton". universetoday.com. January 8, 2016. Archived from the original on February 7, 2016. Retrieved February 6, 2016.
46. "Armored Spacecraft Sets Course for Jupiter - IEEE Spectrum".
47. "Juno's risky rendezvous with Jupiter". July 2016.
48. Webster, Guy (December 17, 2002). "Galileo Millennium Mission Status". NASA – Jet Propulsion Laboratory. Archived from the original on November 24, 2020. Retrieved February 22, 2017. This article incorporates text from this source, which is in the public domain .
49. Firth, Niall (September 5, 2016). "NASA's Juno probe snaps first images of Jupiter's north pole". New Scientist. Archived from the original on September 6, 2016. Retrieved September 5, 2016.
50. Agle, D. C.; Brown, Dwayne; Cantillo, Laurie (October 15, 2016). "Mission Prepares for Next Jupiter Pass". NASA. Archived from the original on June 17, 2019. Retrieved October 19, 2016. This article incorporates text from this source, which is in the public domain .
51. Grush, Loren (October 19, 2016). "NASA's Juno spacecraft went into safe mode last night". The Verge. Archived from the original on March 5, 2017. Retrieved October 23, 2016.
52. "NASA Juno Mission Completes Latest Jupiter Flyby". NASA /Jet Propulsion Laboratory. December 9, 2016. Archived from the original on May 17, 2017. Retrieved February 4, 2017. This article incorporates text from this source, which is in the public domain .
53. Agle, D. C.; Brown, Dwayne; Cantillo, Laurie (March 27, 2017). "NASA's Juno Spacecraft Completes Fifth Jupiter Flyby". NASA. Archived from the original on March 29, 2017. Retrieved March 31, 2017. This article incorporates text from this source, which is in the public domain .
54. Anderson, Natali (May 20, 2017). "NASA's Juno Spacecraft Completes Sixth Jupiter Flyby". Sci-News. Archived from the original on May 25, 2017. Retrieved June 4, 2017.
55. Agle, D. C.; Wendel, JoAnna; Schmid, Deb (June 6, 2018). "NASA Re-plans Juno's Jupiter Mission". NASA/JPL. Archived from the original on July 24, 2020. Retrieved January 5, 2019.
56. Talbert, Tricia (January 8, 2021). "NASA Extends Exploration for Two Planetary Science Missions". NASA. Archived from the original on January 11, 2021. Retrieved January 11, 2021.
57. "NASA spacecraft captures first closeups of Jupiter's largest moon in decades | Jupiter | the Guardian". www.theguardian.com. Archived from the original on June 9, 2021. Retrieved February 2, 2022.
58. "NASA's Juno Shares First Image From Flyby of Jupiter's Moon Europa". NASA . September 29, 2022. Retrieved September 30, 2022.
59. Chang, Kenneth (September 30, 2022). "New Europa Pictures Beamed Home by NASA's Juno Spacecraft" . The New York Times . Retrieved September 30, 2022.
60. "NASA's Juno Orbiter Captures Stunning Images of Jupiter's Moon Io". February 9, 2024. Retrieved March 7, 2024.
61. "Mission Name: Juno". NASA's Planetary Data System. July 2020. Archived from the original on January 11, 2021. Retrieved January 9, 2021. This article incorporates text from this source, which is in the public domain .
62. Bartels, Meghan (July 5, 2016). "To protect potential alien life, NASA will destroy its US$1 billion Jupiter spacecraft on purpose". Business Insider. Archived from the original on January 8, 2018. Retrieved January 7, 2018.
63. Dickinson, David (February 21, 2017). "Juno Will Stay in Current Orbit Around Jupiter". Sky and Telescope. Archived from the original on January 8, 2018. Retrieved January 7, 2018.
64. "NASA Juno Spacecraft to remain in Elongated Capture Orbit around Jupiter". Spaceflight101.com. February 18, 2017. Archived from the original on October 31, 2017. Retrieved January 7, 2018.
65. "Juno Institutional Partners". University of Wisconsin–Madison. 2008. Archived from the original on November 15, 2009. Retrieved August 8, 2009.
66. "NASA Sets Launch Coverage Events For Mission To Jupiter". NASA. July 27, 2011. Archived from the original on September 17, 2011. Retrieved July 27, 2011. This article incorporates text from this source, which is in the public domain .
67. "The Planetary Exploration Budget Dataset". The Planetary Society. Archived from the original on April 12, 2020. Retrieved April 12, 2020.
68. "Jupiter Awaits Arrival of Juno". Archived from the original on June 28, 2016. Retrieved June 28, 2016.
69. "Juno Science Objectives". University of Wisconsin–Madison. Archived from the original on September 19, 2015. Retrieved October 13, 2008.
70. Iorio, L. (August 2010). "Juno, the angular momentum of Jupiter and the Lense–Thirring effect". New Astronomy. 15 (6): 554–560. arXiv: 0812.1485 . Bibcode:2010NewA...15..554I. doi:10.1016/j.newast.2010.01.004.
71. Helled, R.; Anderson, J.D.; Schubert, G.; Stevenson, D.J. (December 2011). "Jupiter's moment of inertia: A possible determination by Juno". Icarus. 216 (2): 440–448. arXiv: 1109.1627 . Bibcode:2011Icar..216..440H. doi:10.1016/j.icarus.2011.09.016. S2CID   119077359.
72. Iorio, L. (2013). "A possible new test of general relativity with Juno". Classical and Quantum Gravity. 30 (18): 195011. arXiv: 1302.6920 . Bibcode:2013CQGra..30s5011I. doi:10.1088/0264-9381/30/19/195011. S2CID   119301991.
73. "Instrument overview". Wisconsin University-Madison. Archived from the original on October 16, 2008. Retrieved October 13, 2008.
74. Dodge, R.; Boyles, M. A.; Rasbach, C. E. (September 2007). "Key and driving requirements for the Juno payload suite of instruments" (PDF). NASA. GS, p. 8; JADE and JEDI, p. 9. Archived from the original (PDF) on July 21, 2011. Retrieved December 5, 2010. This article incorporates text from this source, which is in the public domain .
75. "Juno Spacecraft: Instruments". Mission Juno. Southwest Research Institute. Archived from the original on April 26, 2012. Retrieved December 20, 2011.
76. "Juno launch: press kit August 2011" (PDF). NASA. pp. 16–20. Archived (PDF) from the original on October 25, 2011. Retrieved December 20, 2011. This article incorporates text from this source, which is in the public domain .
77. "More and Juno Ka-band transponder design, performance, qualification and in-flight validation" (PDF). Laboratorio di Radio Scienza del Dipartimento di Ingegneria Meccanica e Aerospaziale, università "Sapienza". 2013. Archived (PDF) from the original on March 4, 2016. Retrieved July 10, 2015.
78. Owen, T.; Limaye, S. (October 23, 2008). "Instruments : microwave radiometer". University of Wisconsin–Madison. Archived from the original on March 28, 2014.
79. "Juno spacecraft MWR". University of Wisconsin–Madison. Archived from the original on August 21, 2015. Retrieved October 19, 2015.
80. "After Five Years in Space, a Moment of Truth". Mission Juno. Southwest Research Institute. Archived from the original on April 17, 2016. Retrieved October 18, 2016.
81. "About JIRAM". IAPS (Institute for Space Astrophysics and Planetology of the Italian INAF). Archived from the original on August 9, 2016. Retrieved June 27, 2016.
82. Owen, T.; Limaye, S. (October 23, 2008). "Instruments : the Jupiter Infrared Aural Mapper". University of Wisconsin–Madison. Archived from the original on March 3, 2016.
83. "Juno spacecraft JIRAM". University of Wisconsin–Madison. Archived from the original on August 21, 2015. Retrieved October 19, 2015.
84. Rogers, John. "JunoCam at PJ57: Part I: Io" (PDF). britastro.org. Retrieved April 2, 2024.
85. Anderson, John; Mittskus, Anthony (October 23, 2008). "Instruments: Gravity Science Experiment". University of Wisconsin–Madison. Archived from the original on February 4, 2016.
86. "Juno spacecraft GS". University of Wisconsin–Madison. Archived from the original on August 21, 2015. Retrieved December 31, 2015.
87. "Juno spacecraft JADE". University of Wisconsin–Madison. Archived from the original on August 21, 2015. Retrieved December 31, 2015.
88. "Juno spacecraft JEDI". University of Wisconsin–Madison. Archived from the original on August 21, 2015. Retrieved October 19, 2015.
89. Agle, D. C.; Brown, Dwayne; Wendel, JoAnna; Schmid, Deb (December 12, 2018). "NASA's Juno Mission Halfway to Jupiter Science". NASA/JPL. Archived from the original on December 14, 2018. Retrieved January 5, 2019. This article incorporates text from this source, which is in the public domain .
90. "Understanding Juno's Orbit: An Interview with NASA's Scott Bolton". Universe Today. January 8, 2016. Archived from the original on February 7, 2016. Retrieved February 6, 2016.
91. "Ganymede in True (RGB) and False (GRB) Colour". JunoCam Image Processing. NASA, SwRI, MSSS. June 12, 2021. Retrieved June 13, 2021.
92. "Cruising to Jupiter: A Powerful Math Lesson – Teachable Moments". NASA/JPL Edu. Archived from the original on March 20, 2021. Retrieved June 10, 2021.
93. "NASA's Juno Mission to Jupiter to Be Farthest Solar-Powered Trip". Space.com . August 4, 2011. Archived from the original on October 3, 2015. Retrieved October 2, 2015.
94. David Dickinson (March 21, 2013). "U.S. to restart plutonium production for deep space exploration". Universe Today. Archived from the original on March 17, 2021. Retrieved February 15, 2015.
95. Greenfieldboyce, Nell. "Plutonium Shortage Could Stall Space Exploration". NPR.org. NPR. Archived from the original on August 3, 2020. Retrieved December 10, 2013.
96. Greenfieldboyce, Nell. "The Plutonium Problem: Who Pays For Space Fuel?". NPR.org. NPR. Archived from the original on May 3, 2018. Retrieved December 10, 2013.
97. Wall, Mike (April 6, 2012). "Plutonium Production May Avert Spacecraft Fuel Shortage". Space.com . Archived from the original on July 3, 2013. Retrieved December 10, 2013.
98. "NASA's Juno Spacecraft Breaks Solar Power Distance Record". NASA. January 13, 2016. Retrieved April 29, 2023.
99. "Juno Solar Panels Complete Testing". NASA. June 24, 2016. Archived from the original on March 23, 2021. Retrieved July 5, 2016. This article incorporates text from this source, which is in the public domain .
100. "JPL: Calculating solar power in space". Jet Propulsion Laboratory . Retrieved October 15, 2023.
101. "Lockheed Martin: Looking at Jupiter like never before" . Retrieved October 15, 2023.
102. NASA's Juno Spacecraft Launches to Jupiter Archived April 26, 2020, at the Wayback Machine "... and that its massive solar arrays, the biggest on any NASA deep-space probe, have deployed and are generating power". This article incorporates text from this source, which is in the public domain .
103. "Juno's Solar Cells Ready to Light Up Jupiter Mission". Archived from the original on December 25, 2014. Retrieved June 19, 2014.
104. "Juno prepares for mission to Jupiter". Machine Design. Archived from the original on October 31, 2010. Retrieved November 2, 2010.
105. "Juno Spacecraft Information – Power Distribution". Spaceflight 101.com. 2011. Archived from the original on November 25, 2011. Retrieved August 6, 2011.
106. "Key Terms". Mission Juno. Southwest Research Institute. Section TONES. Archived from the original on May 5, 2016.
107. Asmar, Sami W.; Bolton, Scott J.; Buccino, Dustin R.; Cornish, Timothy P.; Folkner, William M.; Formaro, Roberto; Iess, Luciano; Jongeling, Andre P.; Lewis, Dorothy K.; Mittskus, Anthony P.; Mukai, Ryan; Simone, Lorenzo (2017). "The Juno Gravity Science Instrument". Space Science Reviews. 213 (1–4): 205. Bibcode:2017SSRv..213..205A. doi:10.1007/s11214-017-0428-7. S2CID   125973393. Doppler measurements at X-band (~8 GHz) are supported by the spacecraft telecommunications subsystem for command and telemetry and are used for spacecraft navigation as well as Gravity Science. The spacecraft also includes a Ka-band (~32 GHz) translator and amplifier specifically for the Gravity Science investigation contributed by the Italian Space Agency.
108. "Junocam will get us great global shots down onto Jupiter's poles". Archived from the original on January 23, 2013. Retrieved July 6, 2016.
109. "Overview | Galileo". solarsystem.nasa.gov. NASA. Archived from the original on February 15, 2017. Retrieved May 14, 2021.
110. "Planetary Data System – Gravity Science Experiment". nmsu.edu. Retrieved April 29, 2023.
111. Amos, Jonathan (September 4, 2012). "Juno Jupiter probe gets British boost". BBC News. Archived from the original on July 17, 2018. Retrieved September 4, 2012.
112. "Juno Jupiter Mission to Carry Plaque Dedicated to Galileo". NASA. August 3, 2011. Archived from the original on May 8, 2020. Retrieved August 5, 2011.
113. "Juno Spacecraft to Carry Three Lego minifigures to Jupiter Orbit". NASA. August 3, 2011. Archived from the original on May 8, 2020. Retrieved August 5, 2011. This article incorporates text from this source, which is in the public domain .
114. "Juno Spacecraft to Carry Three Figurines to Jupiter Orbit". NASA. August 3, 2011. Archived from the original on December 22, 2016. Retrieved December 25, 2016. This article incorporates text from this source, which is in the public domain .
115. Pachal, Peter (August 5, 2011). "Jupiter Probe Successfully Launches With Lego On Board". PC Magazine. Archived from the original on July 4, 2017. Retrieved September 2, 2017.
116. Connerney, John; et al. (June 2018). "Prevalent lightning sferics at 600 megahertz near Jupiter's poles". Nature. 558 (7708): 87–90. Bibcode:2018Natur.558...87B. doi:10.1038/s41586-018-0156-5. PMID   29875484. S2CID   46952214.
117. "Overview | Juno". NASA . Archived from the original on May 19, 2021. Retrieved May 19, 2021.
118. Shekhtman, Lonnie (March 9, 2021). "Serendipitous Juno Detections Shatter Ideas About Origin of Zodiacal Light". Jet Propulsion Laboratory . NASA. Archived from the original on March 18, 2021. Retrieved March 19, 2021.
119. "NASA's Juno Navigators Enable Jupiter Cyclone Discovery". NASA Jet Propulsion Laboratory (JPL). Retrieved May 14, 2022.
120. Crockett, Christopher (June 8, 2020). "What has the Juno spacecraft taught us about Jupiter?". Astronomy.com. Retrieved May 14, 2022.
121. "Meteor in Jupiter's atmosphere, observed by Juno UVS". Mission Juno. Retrieved August 17, 2023.
122. Margetta, Robert (October 28, 2021). "NASA's Juno: Science Results Offer First 3D View of Jupiter Atmosphere". NASA. Retrieved August 17, 2023. This article incorporates text from this source, which is in the public domain .
123. "Mission Perijoves". Mission Juno. Retrieved September 1, 2023.
124. "PDS: Mission Information". Planetary Data System . NASA. March 2022. Archived from the original on June 21, 2022. Retrieved June 21, 2022.
125. Agle, D. C.; Martinez, Maria (September 17, 2012). "Juno's Two Deep Space Maneuvers are 'Back-To-Back Home Runs'". NASA/JPL. Archived from the original on August 2, 2020. Retrieved October 12, 2015. This article incorporates text from this source, which is in the public domain .
126. "Juno Mission & Trajectory Design – Juno".
127. "Juno Earth Flyby – 9 October 2013". NASA. August 26, 2013. Archived from the original on April 26, 2020. Retrieved July 4, 2016.
128. Agle, D. C.; Brown, Dwayne; Cantillo, Laurie (August 27, 2016). "NASA's Juno Successfully Completes Jupiter Flyby". NASA. Archived from the original on March 9, 2021. Retrieved October 1, 2016. This article incorporates text from this source, which is in the public domain .
129. "Mission Prepares for Next Jupiter Pass". Mission Juno. Southwest Research Institute. October 14, 2016. Archived from the original on March 17, 2021. Retrieved October 15, 2016.
130. Agle, D. C.; Brown, Dwayne; Cantillo, Laurie (December 12, 2016). "NASA Juno Mission Completes Latest Jupiter Flyby". NASA – Jet Propulsion Laboratory. Archived from the original on May 17, 2017. Retrieved December 12, 2016. This article incorporates text from this source, which is in the public domain .
131. Thompson, Amy (December 10, 2016). "NASA's Juno Spacecraft Preps for Third Science Orbit". Inverse. Archived from the original on March 17, 2021. Retrieved December 12, 2016.
132. "It's Never 'Groundhog Day' at Jupiter". NASA – Jet Propulsion Laboratory. February 1, 2017. Archived from the original on September 22, 2020. Retrieved February 4, 2017. This article incorporates text from this source, which is in the public domain .
133. Witze, Alexandra (May 25, 2017). "Jupiter's secrets revealed by NASA probe". Nature. doi:10.1038/nature.2017.22027. Archived from the original on June 4, 2017. Retrieved June 14, 2017.
134. Lakdawalla, Emily (November 3, 2016). "Juno update: 53.5-day orbits for the foreseeable future, more Marble Movie". The Planetary Society. Archived from the original on April 26, 2020. Retrieved June 14, 2017.
135. "Photos from Juno's Seventh Science Flyby of Jupiter". Spaceflight101.com. September 8, 2017. Archived from the original on February 13, 2018. Retrieved February 12, 2018.
136. Mosher, Dave (November 7, 2017). "NASA's US$1 billion Jupiter probe just sent back stunning new photos of the gas giant". Business Insider. Archived from the original on March 4, 2018. Retrieved March 4, 2018.
137. "Juno's Perijove-10 Jupiter Flyby, Reconstructed in 125-Fold Time-Lapse". NASA / JPL / SwRI / MSSS / SPICE / Gerald Eichstädt. December 25, 2017. Archived from the original on February 13, 2018. Retrieved February 12, 2018.
138. "Overview of Juno's Perijove 10". The Planetary Society. December 16, 2017. Archived from the original on February 13, 2018. Retrieved February 12, 2018.
139. Boyle, Alan (December 26, 2018). "Ho, ho, Juno! NASA orbiter delivers lots of holiday goodies from Jupiter's north pole". geekwire.com. Archived from the original on April 26, 2019. Retrieved February 7, 2019.
140. Lakdawalla, Emily (November 3, 2016). "Juno update: 53.5-day orbits for the foreseeable future, more Marble Movie". Planetary Society. Archived from the original on April 26, 2020. Retrieved December 25, 2018.
141. "Ganymede". Mission Juno. Retrieved February 11, 2022.
142. Greicius, Tony (May 18, 2021). "Juno Returns to "Clyde's Spot" on Jupiter". NASA. Archived from the original on May 27, 2021. Retrieved June 4, 2021.
143. "NASA's Juno Mission Expands Into the Future". NASA. January 13, 2021. Archived from the original on January 13, 2021. Retrieved January 13, 2021.
144. Wall, Mike (June 8, 2018). "NASA Extends Juno Jupiter Mission Until July 2021". Space.com. Archived from the original on June 23, 2018. Retrieved June 23, 2018.
145. "NASA's Juno Is Getting Ever Closer to Jupiter's Moon Io". July 26, 2023. Retrieved July 28, 2023.
146. "NASA's Juno to Get Close Look at Jupiter's Volcanic Moon Io on Dec. 30". NASA . December 27, 2023. Retrieved December 27, 2023.
147. "See the First Images NASA's Juno Took as It Sailed by Ganymede". Jet Propulsion Laboratory .
148. "Juno mission captures images of volcanic plumes on Jupiter's moon Io". Southwest Research Institute. December 31, 2018. Archived from the original on January 3, 2019. Retrieved January 2, 2019.
149. "NASA's Juno to Get Close Look at Jupiter's Volcanic Moon Io on Dec. 30".

External links

• Official website
• Juno mission at Southwest Research Institute
• Juno Mission at NASA's Solar System Exploration
• Why With Nye playlist on YouTube, Bill Nye discussing the science behind NASA's Juno mission to Jupiter
• JunoCam image processing web site
• Animation of perijove 15 flyby by Gerald Eichstädt (see channel for more)
• Animation of perijove 16 flyby by Gerald Eichstädt and Seán Doran (see albums 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16, 17, 18, 20 21, 23, 24 and 25 for more)
• Juno image album by Kevin M. Gill