Exploration of Jupiter
The exploration of Jupiter has to date been conducted via close observations by automated spacecraft. It began with the arrival of Pioneer 10 into the Jovian system in 1973, and, as of 2008[update], has continued with seven further spacecraft missions. All of these missions were undertaken by the National Aeronautics and Space Administration (NASA), and all save one have been flybys that take detailed observations without the probe landing or entering orbit. These probes make Jupiter the most visited of the Solar System's outer planets as all missions to the outer planets must flyby Jupiter to increase the speed of the probe without needing an excessive amount of fuel that will both be expensive and weigh it down. Plans for more missions to the Jovian system are under development, none of which are scheduled to arrive at the planet before 2016. Sending a craft to Jupiter entails many technical difficulties, especially due to the probes' large fuel requirements and the effects of the planet's harsh radiation environment.
The first spacecraft to visit Jupiter was Pioneer 10 in 1973, followed a few months later by Pioneer 11. Aside from taking the first close-up pictures of the planet, the probes discovered its magnetosphere and its largely fluid interior. The Voyager 1 and Voyager 2 probes visited the planet in 1979, and studied its moons and the ring system, discovering the volcanic activity of Io and the presence of water ice on the surface of Europa. Ulysses further studied Jupiter's magnetosphere in 1992 and then again in 2000. The Cassini probe approached the planet in 2000 and took very detailed images of its atmosphere. The New Horizons spacecraft passed by Jupiter in 2007 and made improved measurements of its and its satellites' parameters.
The Galileo spacecraft is the only one to have actually entered an orbit around Jupiter, arriving in 1995 and studying the planet until 2003. During this period Galileo gathered a large amount of information about the Jovian system, making close approaches to all of the four giant Galilean moons and finding evidence for thin atmospheres on three of them, as well as the possibility of liquid water beneath their surfaces. It also discovered a magnetic field around Ganymede. As it approached Jupiter, it also witnessed the impact of Comet Shoemaker–Levy 9. In December 1995, it sent an atmospheric probe into the Jovian atmosphere, so far the only craft to do so.
Future probes planned by NASA include the Juno spacecraft, launched in 2011, which will enter a polar orbit around Jupiter to determine whether it possesses a rocky core, and the Europa Jupiter System Mission, due to launch sometime around 2020, which will engage in an extended study of the planet's moon system, particularly Europa and Ganymede, and settle the long-running scientific debate over whether an ocean of liquid water exists under Europa's icy surface. Some NASA administrators have even speculated as to the possibility of manned exploration of Jupiter, but such missions are not considered feasible with current technology.
- 1 Technical requirements
- 2 Flyby missions
- 3 Galileo orbital mission (1995–2003)
- 4 Current missions
- 5 Proposed missions
- 6 Manned exploration
- 7 References
- 8 External links
Flights from Earth to other planets in the Solar System have a high energy cost. It requires almost the same amount of energy for a spacecraft to reach Jupiter from Earth's orbit as it does to lift it into orbit in the first place. In astrodynamics, this energy expenditure is defined by the net change in the spacecraft's velocity, or delta-V. The energy needed to reach Jupiter from an Earth orbit requires a delta-V of about 9 km/s, compared to the 9.0–9.5 km/s to reach a low Earth orbit from the ground. However, gravity assists through planetary flybys (such as by Earth or Venus) can be used to reduce the energetic requirement (i.e., the fuel) at launch, albeit at the cost of a significantly longer flight duration to reach a target such as Jupiter when compared to the direct trajectory. Ion thrusters capable of a delta v of more than 10 kilometers/s were used on the Dawn spacecraft. This is more than enough delta v to do a Jupiter fly-by mission from a solar orbit of the same radius as earth's orbit without gravity assist.
A major problem in sending space probes to Jupiter is that the planet has no solid surface on which to land, as there is a smooth transition between the planet's atmosphere and its fluid interior. Any probes descending into the atmosphere are eventually crushed by the immense pressures within Jupiter.
Another major issue is the amount of radiation to which a space probe is subjected, due to the harsh charged-particle environment around Jupiter (for a detailed explanation see Magnetosphere of Jupiter). For example, when Pioneer 11 made its closest approach to the planet, the level of radiation was ten times more powerful than Pioneer's designers had predicted, leading to fears that the probes would not survive; however, with a few minor glitches, the probe managed to pass through the radiation belts. It did however lose most of the images of the moon Io, as the radiation had caused Pioneer's imaging photo polarimeter to receive a number of false commands. The subsequent and far more technologically advanced Voyager spacecraft had to be redesigned to cope with the massive radiation levels. Over the eight years the Galileo spacecraft orbited the planet, the probe's radiation dose far exceeded its design specifications, and its systems failed on several occasions. The spacecraft's gyroscopes often exhibited increased errors, and electrical arcs sometimes occurred between its rotating and non-rotating parts, causing it to enter safe mode, which led to total loss of the data from the 16th, 18th and 33rd orbits. The radiation also caused phase shifts in Galileo's ultra-stable quartz oscillator.
Pioneer program (1973 and 1974)
The first spacecraft to explore Jupiter was Pioneer 10, which flew past the planet in December 1973, followed by Pioneer 11 twelve months later. Pioneer 10 obtained the first-ever close-up images of Jupiter and its Galilean moons; the spacecraft studied the planet's atmosphere, detected its magnetic field, observed its radiation belts and determined that Jupiter is mainly fluid. Pioneer 11 made its closest approach, within some 34,000 km of Jupiter's cloud tops, on December 4, 1974. It obtained dramatic images of the Great Red Spot, made the first observation of Jupiter's immense polar regions, and determined the mass of Jupiter's moon Callisto. The information gathered by these two spacecraft helped astronomers and engineers improve the design of future probes to cope more effectively with the environment around the giant planet.
Voyager program (1979)
Voyager 1 began photographing Jupiter in January 1979 and made its closest approach on March 5, 1979, at a distance of 349,000 km from Jupiter's center. This close approach allowed for greater image resolution, though the flyby's short duration meant that most observations of Jupiter's moons, rings, magnetic field, and radiation environment were made in the 48-hour period bracketing the approach, even though Voyager 1 continued photographing the planet until April. It was soon followed by Voyager 2, which made its closest approach on July 9, 1979, 576 thousand km away from the planet's cloud tops. The probe discovered Jupiter's ring, observed intricate vortices in its atmosphere, observed active volcanoes on Io, a process analogous to plate tectonics on Ganymede, and numerous craters on Callisto.
The Voyager missions vastly improved our understanding of the Galilean moons, and also discovered Jupiter's rings. They also took the first close up images of the planet's atmosphere, revealing the Great Red Spot as a complex storm moving in a counter-clockwise direction. An array of other smaller storms and eddies were found throughout the banded clouds (see animation on the right). Two new, small satellites, Adrastea and Metis, were discovered orbiting just outside the ring, making them the first of Jupiter's moons to be identified by a spacecraft. A third new satellite, Thebe, was discovered between the orbits of Amalthea and Io.
The discovery of volcanic activity on the moon Io was the greatest unexpected finding of the mission, as it was the first time an active volcano was observed on a celestial body other than Earth. Together, the Voyagers recorded the eruption of nine volcanoes on Io, as well as evidence for other eruptions occurring between the Voyager encounters.
Europa displayed a large number of intersecting linear features in the low-resolution photos from Voyager 1. At first, scientists believed the features might be deep cracks, caused by crustal rifting or tectonic processes. However, the high-resolution photos from Voyager 2, taken closer to Jupiter, left scientists puzzled as the features in these photos were almost entirely lacking in topographic relief. This led many to suggest that these cracks might be similar to ice floes on Earth, and that Europa might have a liquid water interior. Europa may be internally active due to tidal heating at a level about one-tenth that of Io, and as a result, the moon is thought to have a thin crust less than 30 kilometers (19 mi) thick of water ice, possibly floating on a 50-kilometers-deep (30 mile) ocean.
On February 8, 1992, the Ulysses solar probe flew past Jupiter's north pole at a distance of 451,000 km. This swing-by maneuver was required for Ulysses to attain a very high-inclination orbit around the Sun, increasing its inclination to the ecliptic to 80.2 degrees. The giant planet's gravity bent the spacecraft's flightpath downward and away from the ecliptic plane, placing it into a final orbit around the Sun's north and south poles. The size and shape of the probe's orbit were adjusted to a much smaller degree, so that its aphelion remained at approximately 5 AU (Jupiter's distance from the Sun), while its perihelion lay somewhat beyond 1 AU (Earth's distance from the Sun). During its Jupiter encounter, the probe made measurements of the planet's magnetosphere. Since the probe had no cameras, no images were taken. In February 2004, the probe arrived again at the vicinity of Jupiter. This time the distance from the planet was much greater—about 240 million km—but it made further observations of Jupiter.
In 2000, the Cassini probe, en route to Saturn, flew by Jupiter and provided some of the highest-resolution images ever taken of the planet. It made its closest approach on December 30, 2000, and made many scientific measurements. About 26,000 images of Jupiter were taken during the months-long flyby. It produced the most detailed global color portrait of Jupiter yet, in which the smallest visible features are approximately 60 km (37 mi) across.
A major finding of the flyby, announced on March 6, 2003, was of Jupiter's atmospheric circulation. Dark belts alternate with light zones in the atmosphere, and the zones, with their pale clouds, had previously been considered by scientists to be areas of upwelling air, partly because on Earth clouds tend to be formed by rising air. But analysis of Cassini imagery showed that the dark belts contain individual storm cells of upwelling bright-white clouds, too small to see from Earth. Anthony Del Genio of NASA's Goddard Institute for Space Studies said that "the belts must be the areas of net-rising atmospheric motion on Jupiter, [so] the net motion in the zones has to be sinking".
Other atmospheric observations included a swirling dark oval of high atmospheric-haze, about the size of the Great Red Spot, near Jupiter's north pole. Infrared imagery revealed aspects of circulation near the poles, with bands of globe-encircling winds, with adjacent bands moving in opposite directions. The same announcement also discussed the nature of Jupiter's rings. Light scattering by particles in the rings showed the particles were irregularly shaped (rather than spherical) and likely originated as ejecta from micrometeorite impacts on Jupiter's moons, probably on Metis and Adrastea. On December 19, 2000, the Cassini spacecraft captured a very low resolution image of the moon Himalia, but it was too distant to show any surface details.
New Horizons (2007)
The New Horizons probe, en route to Pluto, flew by Jupiter for a gravity assist and was the first probe launched directly towards Jupiter since the Ulysses in 1990. Its Long Range Reconnaissance Imager (LORRI) took its first photographs of Jupiter on September 4, 2006. The spacecraft began further study of the Jovian system in December 2006, and made its closest approach on February 28, 2007.
While close to Jupiter, New Horizons' instruments made refined measurements of the orbits of Jupiter's inner moons, particularly Amalthea. The probe's cameras measured volcanoes on Io, studied all four Galilean moons in detail, and made long-distance studies of the outer moons Himalia and Elara. The craft also studied Jupiter's Little Red Spot and the planet's magnetosphere and tenuous ring system.
On March 19, 2007 the Command and Data Handling computer experienced an uncorrectable memory error and rebooted itself, causing the spacecraft to go into safe mode. The craft fully recovered within two days, with some data loss on Jupiter's magnetotail. No other data loss events were associated with the encounter. Due to the immense size of the Jupiter system and the relative closeness of the Jovian system to Earth in comparison to the closeness of Pluto to Earth, New Horizons will send back more data to Earth from the Jupiter encounter than the Pluto encounter.
Galileo orbital mission (1995–2003)
So far, the only spacecraft to orbit Jupiter is the Galileo orbiter, which went into orbit around Jupiter on December 7, 1995. It orbited the planet for over seven years, making 35 orbits before it was destroyed during a controlled impact with Jupiter on September 21, 2003. During this period it gathered a large amount of information about the Jovian system, although the amount of information was not as great as intended because the deployment of its high-gain radio transmitting antenna failed. The major events during the eight-year study included multiple flybys of all of the Galilean moons, as well as Amalthea (the first probe to do so). It also witnessed the impact of Comet Shoemaker-Levy 9 as it approached Jupiter in 1994 and the sending of an atmospheric probe into the Jovian atmosphere in December 1995.
Cameras on the Galileo spacecraft observed fragments of the Shoemaker-Levy 9 comet between July 16 and July 22, 1994 as they collided with Jupiter's southern hemisphere at a speed of approximately 60 kilometres per second. This was the first direct observation of an extraterrestrial collision of solar system objects. While the impacts took place on the side of Jupiter hidden from Earth, Galileo, then at a distance of 1.6 AU from the planet, was able to see the impacts as they occurred. Its instruments detected a fireball which reached a peak temperature of about 24,000 K, compared to the typical Jovian cloudtop temperature of about 130 K, with the plume from the fireball reaching a height of over 3,000 km.
An atmospheric probe was released from the spacecraft in July 1995, entering the planet's atmosphere on December 7, 1995. After a high-g descent into the Jovian atmosphere, the probe discarded the remains of its heat shield, and it parachuted through 150 km of the atmosphere, collecting data for 57.6 minutes, before being crushed by the pressure and temperature to which it was subjected (about 22 times Earth normal, at a temperature of 153 °C). It would have melted thereafter, and possibly vaporized. The Galileo orbiter itself experienced a more rapid version of the same fate when it was deliberately steered into the planet on September 21, 2003 at a speed of over 50 km/s, in order to avoid any possibility of it crashing into and contaminating Europa.
- the first observation of ammonia clouds in another planet's atmosphere—the atmosphere creates ammonia ice particles from material coming up from lower depths;
- confirmation of extensive volcanic activity on Io—which is 100 times greater than that found on Earth; the heat and frequency of eruptions are reminiscent of early Earth;
- observation of complex plasma interactions in Io's atmosphere which create immense electrical currents that couple to Jupiter's atmosphere;
- providing evidence for supporting the theory that liquid oceans exist under Europa's icy surface;
- first detection of a substantial magnetic field around a satellite (Ganymede);
- magnetic data evidence suggesting that Europa, Ganymede and Callisto have a liquid-saltwater layer under the visible surface;
- evidence for a thin atmospheric layer on Europa, Ganymede, and Callisto known as a 'surface-bound exosphere';
- understanding of the formation of the rings of Jupiter (by dust kicked up as interplanetary meteoroids which smash into the planet's four small inner moons) and observation of two outer rings and the possibility of a separate ring along Amalthea's orbit;
- identification of the global structure and dynamics of a giant planet's magnetosphere.
NASA has a mission to study Jupiter in detail from a polar orbit; named Juno, the spacecraft was launched on August 5, 2011 and is due to arrive in 2016. The spacecraft will be placed in a polar orbit to study the planet's composition, gravity field, magnetic field, and polar magnetosphere. Juno will also search for clues about how Jupiter formed, including whether the planet has a rocky core, the amount of water present within the deep atmosphere, and how the mass is distributed within the planet. Juno will also study Jupiter's deep winds, which can reach speeds of 600 km/h.
The Europa Jupiter System Mission (EJSM) is a joint NASA/ESA proposal for exploration of Jupiter and its moons. In February 2009 it was announced that ESA/NASA had given this mission priority ahead of the Titan Saturn System Mission. The proposal includes a launch date of around 2020 and consists of the NASA-led Jupiter Europa Orbiter, and the ESA-led Jupiter Ganymede Orbiter. ESA's contribution will still face funding competition from other ESA projects.
Because of the possibility of subsurface liquid oceans on Jupiter's moons Europa, Ganymede and Callisto, there has been great interest in studying the icy moons in detail. Funding difficulties have delayed progress. The Europa Orbiter was a planned NASA mission to Europa, which was canceled in 2002. Its main objectives included determining the presence or absence of a subsurface ocean and identifying candidate sites for future lander missions. Then there was NASA's JIMO (Jupiter Icy Moons Orbiter) that was canceled in 2005. A European Jovian Europa Orbiter mission was also studied. These missions were superseded by the Europa Jupiter System Mission (EJSM) described above.
While scientists require further evidence to determine the extent of a rocky core on Jupiter, its Galilean moons provide the potential opportunity for future manned exploration.
Particular targets are Europa, due to its potential for life, and Callisto, due to its relatively low radiation dose. In 2003, NASA proposed a program called Human Outer Planets Exploration (HOPE) that involved a manned mission to the Galilean moons. NASA has projected a possible attempt some time in the 2040s. In the Vision for Space Exploration policy announced in January 2004, NASA has discussed manned missions beyond Mars, mentioning that a "human research presence" may be desirable on Jupiter's moons. Before the JIMO mission was cancelled, NASA administrator Sean O'Keefe stated that "human explorers will follow."
Potential for colonization
NASA has speculated on the feasibility of mining the atmospheres of the outer planets, particularly for helium-3, an isotope of helium that is rare on Earth and could have a very high value per unit mass as a thermonuclear fuel. Factories stationed in orbit could mine the gas and deliver it to visiting craft. However, the Jovian system in general poses particular disadvantages for colonization because of the severe radiation conditions prevailing in Jupiter's magnetosphere and the planet's particularly deep gravitational well. Jupiter would deliver about 36 Sv (3600 rem) per day to unshielded colonists at Io and about 5.4 Sv (540 rems) per day to unshielded colonists at Europa, which is a decisive aspect due to the fact that already an exposure to about .75 Sv over a period of a few days is enough to cause radiation poisoning, and about 5 Sv over a few days is fatal.
Ganymede is the Solar System's largest moon and the Solar System's only yet known moon that does possess a magnetosphere, but this does not shield it from cosmic radiation, to a noteworthy degree, because it is overshadowed by Jupiter's magnetic field. Ganymede receives about 0.08 Sv (8 rem) of radiation per day. Callisto being further from Jupiter's powerful radiation belt is subject to 0.0001 Sv (0.01 rem) a day. For comparison, the average amount of radiation taken on Earth by a living organism is about 0.024 Sv per year; the highest natural radiation levels on Earth are recorded around Ramsar hot springs at about 0.26 Sv per year.
One of the main targets chosen by the HOPE study was Callisto. The possibility was mooted of building a surface base on Callisto, because of the low radiation levels at the moon's distance from Jupiter and its geological stability. Callisto is the only one of Jupiter's Galilean satellites for which human exploration is feasible. The levels of ionizing radiation on Io, Europa and Ganymede are hostile to human life, and adequate protective measures have yet to be devised.
It could be possible to build a surface base that would produce fuel for further exploration of the Solar System. In 1997, the Artemis Project designed a plan to colonize Europa. According to the plan, explorers would drill down into the Europan ice crust, entering the postulated subsurface ocean, where they would inhabit artificial air pockets.
- Wong, Al (May 28, 1998). "Galileo FAQ – Navigation". NASA. Retrieved 2006-11-28.
- Burton, Rodney L.; Brown, Kevin; Jacobi, Anthony (2006). "Low Cost Launch of Payloads to Low Earth Orbit" (pdf). Journal of Spacecraft and Rockets 43 (3): 696–698. Bibcode:2006JSpRo..43..696B. doi:10.2514/1.16244.
- Fischer, 1999, p.44
- CRC Handbook of Chemistry and Physics, 64th EDITION, (C) 1983, page F-141
- Guillot, Tristan (1999). "A comparison of the interiors of Jupiter and Saturn". Planetary and Space Science 47 (10–11): 1183–1200. arXiv:astro-ph/9907402. Bibcode:1999P&SS...47.1183G. doi:10.1016/S0032-0633(99)00043-4.
- Wolverton, Mark (2004). The Depths of Space. Joseph Henry Press. p. 130. ISBN 978-0-309-09050-6.
- "The Pioneer missions". NASA. 2007. Retrieved 2009-06-28.
- Fieseler, P.D.; Ardalan, S.M.; Frederickson, A.R. (2002). "The radiation effects on Galileo spacecraft systems at Jupiter". IEEE Transactions on Nuclear Science 49 (6): 2739. Bibcode:2002ITNS...49.2739F. doi:10.1109/TNS.2002.805386.
- Andrew P. Ingersoll and Carolyn C. Porco (July 1978). "Solar heating and internal heat flow on Jupiter". Icarus 35 (1): 27–43. Bibcode:1978Icar...35...27I. doi:10.1016/0019-1035(78)90058-1. Retrieved 2009-07-02.
- Michael Mewhinney (2003). "Pioneer spacecraft sends last signal". NASA. Retrieved 2009-06-28.
- "Pioneer 11". NASA. Retrieved 2009-06-28.
- Stone, Ec; Lane, Al (Jun 1979). "Voyager 1 Encounter with the Jovian System". Science 204 (4396): 945–948. Bibcode:1979Sci...204..945S. doi:10.1126/science.204.4396.945. JSTOR 1748134. PMID 17800428.
- "Jupiter". NASA Jet Propulsion Laboratory. January 14, 2003. Retrieved 2006-11-28.
- "First Close-up Image of Jupiter from Voyager 1 (NASA Voyager Jupiter Encounter Images)". Ciclops.org. Retrieved 2009-05-20.
- E. C. Stone and A. L. Lane (October 5, 1979). "Voyager 2 Encounter with the Jovian System". Science 206 (4421): 925–927. Bibcode:1979Sci...206..925S. doi:10.1126/science.206.4421.925. PMID 17733909.
- Smith, Ba; Soderblom, La; Johnson, Tv; Ingersoll, Ap; Collins, Sa; Shoemaker, Em; Hunt, Ge; Masursky, H; Carr, Mh; Davies, Me; Cook, Af, 2Nd; Boyce, J; Danielson, Ge; Owen, T; Sagan, C; Beebe, Rf; Veverka, J; Strom, Rg; Mccauley, Jf; Morrison, D; Briggs, Ga; Suomi, Ve (Jun 1979). "The Jupiter System Through the Eyes of Voyager 1". Science 204 (4396): 951–972. Bibcode:1979Sci...204..951S. doi:10.1126/science.204.4396.951. PMID 17800430.
- Brian G. Marsden (1980-08-26). "Satellites of Jupiter". IAU Circulars 3507.(discovery)
- Synnott, S.P. (1981). "1979J3: Discovery of a Previously Unknown Satellite of Jupiter". Science 212 (4501): 1392. Bibcode:1981Sci...212.1392S. doi:10.1126/science.212.4501.1392. ISSN 0036-8075. PMID 17746259.
- Burns, J.A.; Simonelli; Showalter; Hamilton; Porco; Throop; Esposito; Simonelli, D. P.;Showalter, M.R. et al. (2004). "Jupiter's Ring-Moon System" (PDF). In Bagenal, F.; Dowling, T.E.; McKinnon, W.B. Jupiter: The Planet, Satellites and Magnetosphere. Cambridge University Press. p. 241. Bibcode:2004jpsm.book..241B.
- Strom, R. G.; et al. (1979). "Volcanic eruption plumes on Io". Nature 280 (5725): 733–736. Bibcode:1979Natur.280..733S. doi:10.1038/280733a0.
- Paul M. Schenk and William B. McKinnon (May 1989). "Fault offsets and lateral crustal movement on Europa: Evidence for a mobile ice shell". Icarus 79 (1): 75–100. Bibcode:1989Icar...79...75S. doi:10.1016/0019-1035(89)90109-7.
- Buratti, B; Veverka, Joseph. "Voyager photometry of Europa". Icarus 55 (1): 93. Bibcode:1983Icar...55...93B. doi:10.1016/0019-1035(83)90053-2.
- Smith, Ej; Wenzel, Kp; Page, De (September 1992). "Ulysses at Jupiter: An Overview of the Encounter". Science 257 (5076): 1503–1507. Bibcode:1992Sci...257.1503S. doi:10.1126/science.257.5076.1503. JSTOR 2879932. PMID 17776156.
- K. Chan, E. S. Paredes, M. S. Ryne (2004). "Ulysses Attitude and Orbit Operations: 13+ Years of International Cooperation" (PDF). American Institute of Aeronautics and Astronautics. Retrieved 2006-11-28.
- Mckibben, R; Zhang, M; Heber, B; Kunow, H; Sanderson, T (2007). "Localized "Jets" of Jovian electrons observed during Ulysses' distant Jupiter flyby in 2003–2004". Planetary and Space Science 55 (1–2): 21–31. Bibcode:2007P&SS...55...21M. doi:10.1016/j.pss.2006.01.007.
- "Ulysses – Science – Jupiter Distant Encounter Selected References". NNASA. Retrieved 2008-10-21.
- Hansen C. J., Bolton S. J., Matson D. L., Spilker L. J., Lebreton J. P. (2004). "The Cassini–Huygens flyby of Jupiter". Icarus 172 (1): 1–8. Bibcode:2004Icar..172....1H. doi:10.1016/j.icarus.2004.06.018.
- "Cassini-Huygens: News-Press Releases-2003". NASA. Archived from the original on 2007-11-21. Retrieved 2008-10-21.
- Alexander, Amir (September 27, 2006). "New Horizons Snaps First Picture of Jupiter". The Planetary Society. Retrieved 2006-12-19.
- "New Horizons Web Site". Johns Hopkins University. Retrieved 2008-11-02.
- Stern, S. Alan (2008). "The New Horizons Pluto Kuiper Belt Mission: An Overview with Historical Context". Space Science Reviews 140 (1–4): 3. arXiv:0709.4417. Bibcode:2008SSRv..140....3S. doi:10.1007/s11214-007-9295-y.
- "NASA Spacecraft Gets Boost From Jupiter for Pluto Encounter.". The America's Intelligence Wire. 28-February–07. Retrieved 2009-07-02.
- Cheng, A. F.; Weaver, H. A.; Conard, S. J.; Morgan, M. F.; Barnouin-Jha, O.; Boldt, J. D.; Cooper, K. A.; Darlington, E. H. et al. (2008). "Long-Range Reconnaissance Imager on New Horizons". Space Science Reviews 140 (1–4): 189. arXiv:0709.4278. Bibcode:2008SSRv..140..189C. doi:10.1007/s11214-007-9271-6.
- "Fantastic Flyby". NASA. May 1, 2007. Retrieved 2009-07-02.
- "Galileo Mission to Jupiter". NASA/Jet Propulsion Laboratory. Retrieved 2009-07-09.
- McConnell, Shannon (April 14, 2003). "Galileo: Journey to Jupiter". NASA/Jet Propulsion Laboratory. Retrieved 2006-11-28.
- Thomas, P.C.; Burns, J.A.; Rossier, L.; et al. (1998). "The Small Inner Satellites of Jupiter". Icarus 135 (1): 360–371. Bibcode:1998Icar..135..360T. doi:10.1006/icar.1998.5976.
- Williams, David R. "Ulysses and Voyager 2". Lunar and Planetary Science. National Space Science Data Center. Retrieved 25 August 2008.
- "Comet Shoemaker-Levy 9 Collision with Jupiter". National Space Science Date Center, NASA. February 2005. Retrieved 2008-08-26.
- Martin, Terry Z. (September 1996). "Shoemaker-Levy 9: Temperature, Diameter and Energy of Fireballs". Bulletin of the American Astronomical Society 28: 1085. Bibcode:1996DPS....28.0814M.
- "Galileo Mission to Jupiter" (PDF). NASA. Retrieved 2008-11-01.
- "BBC News | SCI/TECH | Crash plan for Galileo spaceprobe". 220.127.116.11:8080. 2000-03-03. Retrieved 2009-05-20.
- Rosaly M. C. Lopes and John R. Spencer. (2007). Io after Galileo : a new view of Jupiter's volcanic moon. Berlin: Springer. ISBN 978-3-540-34681-4.
- P. Bond. (2004). Stepping stones to the cosmos : the story of planetary exploration. New York ; Berlin: Springer. pp. 166–182. ISBN 978-0-387-40212-3.
- "Galileo Project Information". Nssdc.gsfc.nasa.gov. Retrieved 2009-05-24.
- "Solar System Exploration: Galileo Legacy Site: Discovery Highlights". Solarsystem.nasa.gov. 2007-08-09. Retrieved 2009-05-24.
- Daniel Fischer. (1999). Mission Jupiter : the spectacular journey of the Galileo spacecraft. New York: Copernicus. ISBN 978-0-387-98764-4.
- NASA Selects New Frontiers Concept Study: Juno Mission to Jupiter | Jupiter Today – Your Daily Source of Jupiter News
- "Juno – NASA's Second New Frontiers Mission to Jupiter". Retrieved 2007-10-24.
- Buckley, M. (May 20, 2008). "Storm Winds Blow in Jupiter’s Little Red Spot". Johns Hopkins Applied Physics Laboratory. Retrieved 2008-10-16.
- Steigerwald , Bill (October 10, 2006). "Jupiter's Little Red Spot Growing Stronger". NASA Goddard Space Center. Retrieved 2008-10-16.
- Talevi, Monica; Brown, Dwayne (2009-02-18). "NASA and ESA Prioritize Outer Planet Missions". Retrieved 2009-02-18.
- Rincon, Paul (2009-02-18). "Jupiter in space agencies' sights". BBC News. Retrieved 2009-02-28.
- Tim Brice. "Outer Planet Flagship Mission: Jupiter Ganymede Orbiter (JGO) Concept". Opfm.jpl.nasa.gov. Retrieved 2009-05-24.
- OPF Study Team (2008-08-28). "Outer Planet Flagship Mission: Briefing to the OPAG Steering Committee" (PDF). Outer Planets Assessment Group. Retrieved 2008-10-14.
- "Laplace: A mission to Europa & Jupiter system". ESA. Retrieved 2009-01-23.
- Volonte, Sergio (2007-07-10). "Cosmic Vision 2015-2025 Proposals". ESA. Retrieved 2009-02-18.
- "The Europa Orbiter Mission Design". Hdl.handle.net. Retrieved 2009-05-20.
- "NASA Kills Europa Orbiter". Space.com. 2002-02-04. Retrieved 2009-05-20.
- Berger, Brian (2005-02-07). "White House scales back space plans". MSNBC. Retrieved 2007-01-02.
- Atzei, Alessandro (2007-04-27). "Jovian Minisat Explorer". ESA. Retrieved 2008-05-08.
- Artemis Society International official website
- Kokh, Peter; Kaehny, Mark; Armstrong, Doug; Burnside, Ken (November 1997). "Europa II Workshop Report". Moon Miner's Manifesto (110).
- Pat Troutman, Kristen Bethke (2003). "Revolutionary Concepts for Human Outer Planet Exploration". NASA. Retrieved 2009-07-02.
- Melissa L. McGuire, James Gilland (2003). "High Power MPD Nuclear Electric Propulsion (NEP) for Artificial Gravity HOPE Missions to Callisto". NASA. Retrieved 2009-06-30.
- "Vision for Space Exploration". NASA. 2003. Retrieved 2009-07-02.
- "NASA plans to send new robot to Jupiter". SpaceDaily. 2004. Retrieved 2009-06-30.
- Robert Zubrin, Entering Space: Creating a Spacefaring Civilization, section: Settling the Outer Solar System: The Sources of Power, pp. 158-160, Tarcher/Putnam, 1999, ISBN 1-58542-036-0
- Jeffrey Van Cleve (Cornell University) et al., "Helium-3 Mining Aerostats in the Atmosphere of Uranus", Abstract for Space Resources Roundtable, accessed May 10, 2006
- Bryan Palaszewski (October 2006). "Atmospheric Mining in the Outer Solar System". Glenn Research Center. Retrieved 2009-07-02.
- Frederick A. Ringwald (2000-02-29). "SPS 1020 (Introduction to Space Sciences)". California State University, Fresno. Retrieved 2009-07-04. (Webcite from 2009-09-20)
- Robert Zubrin, Entering Space: Creating a Spacefaring Civilization, section: Colonizing the Jovian System, pp. 166-170, Tarcher/Putnam, 1999, ISBN 1-58542-036-0
- Ringwald, Frederick A. (29 February 2009). "SPS 1020 (Introduction to Space Sciences)". California State University, Fresno. Retrieved 20 September 2009.
- Troutman, P.A.; Bethke, K. et al. (28 January 2003). Revolutionary Concepts for Human Outer Planet Exploration (HOPE) Revolutionary Concepts for Human Outer Planet Exploration (HOPE). "AIP Conference Proceedings". American Institute of Physics Conference Proceedings 654: 821–828. doi:10.1063/1.1541373. Retrieved 10 May 2006.
- "Humans on Europa: A Plan for Colonies on the Icy Moon". Space.com. 6 June 2001. Retrieved 10 May 2006.