Artist impression of how Triton, Neptune's largest moon, might look from high above its surface. The distant Sun appears at the upper-left and the blue crescent of Neptune right of center. (ESO/L. Calcada)
NASA, with participation by the European Space Agency, has just completed a concept study for a mission—or missions—to explore our solar system’s least-understood planets, the distant “ice giants” Uranus and Neptune.
Many of us grew up reading textbooks that described Uranus and Neptune as two of the four “gas giant” worlds of our solar system, along with Jupiter and Saturn. We were taught they were colder and smaller—and quite a bit bluer—than their two larger siblings, but were otherwise probably like them in composition and structure.
But telescope observations from Earth, as well as the Voyager 2 data, have led scientists to suspect Uranus and Neptune may be fundamentally different from Jupiter and Saturn—different enough to have their own term: “ice giants.”
An infrared image of the ice giant Uranus and its thin rings, captured by the Hubble Space Telescope. (NASA/ESA/STScI)
Scientists are hoping to learn more about how these planets and their moons formed long ago and, by extension, what conditions prevailed in the earliest times of the solar system’s existence.
Solar System Forensics
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Scientists piece together what the early solar system was like by studying planets, moons, asteroids, and comets as sites of forensic evidence.
Every planet closer to the sun than Uranus—besides Earth, this includes Saturn, Jupiter, Mars, Venus, Mercury, and dwarf planet Ceres—has been explored with flyby missions and at least one long-term orbiter. To some of these planets we have sent atmospheric or surface-landing robots.
We have even investigated the frozen time capsules called comets, which originate far beyond the realm of the ice giants and preserve pristine, undisturbed evidence of the solar system’s earliest years. Even the dwarf planet Pluto and its moons yielded clues to those early times, when the New Horizons spacecraft grabbed a large batch of high quality data during its 2015 flyby encounter.
But we have only a scant few hours’ worth of up-close data for Uranus and Neptune. It was collected by a single spacecraft, Voyager 2, in 1986 and 1989. These planets’ region of the solar system spans well over a billion miles, and we know relatively little about them.
High clouds (left) and the mysterious storm system dubbed the “Great Dark Spot” (right) in Neptune’s atmosphere, captured by Voyager 2 in 1989. (NASA/Voyager)
NASA’s recent concept study examines aspects of a future mission. The study ranges from what scientific questions we want to answer about these worlds and their moons, to what type of instrumentation and spacecraft (flyby probe, orbiter, atmospheric probe, or combination of them) would best achieve those scientific goals, to possible technologies and trajectories for getting the spacecraft to their distant destinations.
A Grander Tour?
I recall the decade of discovery called the “Grand Tour” in the 1980s when Voyagers 1 and 2 made their way through the outer solar system, bringing us the first visions of its giant worlds and their moons. Only Voyager 2 went on to Uranus and Neptune, beaming back close, detailed pictures of those planets and their moons, where before we had seen only fuzzy balls and dots through Earth’s largest telescopes.
The largest moon of either ice giant planet, Triton, imaged by Voyager 2 in 1989. Triton may be one of the coldest spots in the solar system, though it still shows signs of activity as it spews out plumes of nitrogen gas. (NASA/Voyager)
The Voyager 2 encounters gave us glimpses of methane-rich atmospheres, cloud formations, unusually shaped magnetic fields, and a large storm on Neptune dubbed the “Great Dark Spot.”
Voyager also showed us a variety of unexpectedly dynamic moons, including one—Neptune’s large satellite, Triton—actively spewing plumes of nitrogen gas that fall as frost onto its surface.
Ice Giants
The name “ice giants” does not imply that Uranus and Neptune are made of ice, or even contain significant amounts of frozen material. It is a reference both to the frigidly cold region they dwell in, and the expectation that they are composed of materials like water and ammonia and methane—substances we find in frozen form on smaller bodies out there, such as their icy moons.
The differences between gas giants and ice giants: the gas giants Jupiter and Saturn are largely made of light gases such as hydrogen and helium, while Uranus and Neptune (ice giants) consist of heavier substances. The thick mantles of Uranus and Neptune may be massive oceans of water, ammonia, and methane. (NASA)
It is estimated that as much as 60 percent of an ice giant’s mass consists of heavier materials like these—as compared to Jupiter and Saturn, where 85 percent of the gas giants’ bulk is made up of lighter gases such as hydrogen and helium.
It may even be that a huge liquid ocean accounting for as much as two-thirds of each ice giant’s mass lies hidden beneath the upper cloud layers. Perhaps “liquid giant” would be a better term.
A mission to either of these mysterious planets probably wouldn’t get going until sometime in the next decade, with the actual flight to Uranus or Neptune taking several years. But if the thrilling rewards of Voyager 2’s flybys three decades ago are any indication, it will be a mission well worth waiting for.
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"content": "\u003cp>NASA, with participation by the European Space Agency, \u003ca href=\"https://www.jpl.nasa.gov/news/news.php?feature=6877\">has just completed a concept study \u003c/a>for a mission—or missions—to explore our solar system’s least-understood planets, the distant “ice giants” Uranus and Neptune.\u003c/p>\n\u003cp>Many of us grew up reading textbooks that described Uranus and Neptune as two of the four “gas giant” worlds of our solar system, along with Jupiter and Saturn. We were taught they were colder and smaller—and quite a bit bluer—than their two larger siblings, but were otherwise probably like them in composition and structure.\u003c/p>\n\u003cp>But telescope observations from Earth, as well as the Voyager 2 data, have led scientists to suspect Uranus and Neptune may be fundamentally different from Jupiter and Saturn—different enough to have their own term: “ice giants.”\u003c/p>\n\u003cfigure id=\"attachment_1806520\" class=\"wp-caption aligncenter\" style=\"max-width: 800px\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"size-medium wp-image-1806520\" src=\"https://ww2.kqed.org/science/wp-content/uploads/sites/35/2017/07/Uranus-800x515.jpg\" alt=\"An infrared image of the ice giant Uranus and its thin rings, captured by the Hubble Space Telescope. \" width=\"800\" height=\"515\" srcset=\"https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/Uranus-800x515.jpg 800w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/Uranus-160x103.jpg 160w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/Uranus-768x495.jpg 768w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/Uranus.jpg 894w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/Uranus-240x155.jpg 240w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/Uranus-375x242.jpg 375w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/Uranus-520x335.jpg 520w\" sizes=\"(max-width: 800px) 100vw, 800px\">\u003cfigcaption class=\"wp-caption-text\">An infrared image of the ice giant Uranus and its thin rings, captured by the Hubble Space Telescope. \u003ccite>(NASA/ESA/STScI)\u003c/cite>\u003c/figcaption>\u003c/figure>\n\u003cp>Scientists are hoping to learn more about how these planets and their moons formed long ago and, by extension, what conditions prevailed in the earliest times of the solar system’s existence.\u003c/p>\n\u003cp>\u003cstrong>Solar System Forensics\u003c/strong>\u003c/p>\n\u003cp>[ad fullwidth]\u003c/p>\n\u003cp>Scientists piece together what the \u003ca href=\"https://www.windows2universe.org/our_solar_system/formation.html\">early solar system\u003c/a> was like by studying planets, moons, asteroids, and comets as sites of forensic evidence.\u003c/p>\n\u003cp>[contextly_sidebar id=”KA7ngank5A5APfm7m8wMoODrvc7QyK93″]Every planet closer to the sun than Uranus—besides Earth, this includes Saturn, Jupiter, Mars, Venus, Mercury, and dwarf planet Ceres—has been explored with flyby missions and at least one long-term orbiter. To some of these planets we have sent atmospheric or surface-landing robots.\u003c/p>\n\u003cp>We have even investigated the frozen time capsules called comets, which originate far beyond the realm of the ice giants and preserve pristine, undisturbed evidence of the solar system’s earliest years. Even the dwarf planet Pluto and its moons yielded clues to those early times, when the New Horizons spacecraft grabbed a large batch of high quality data during its 2015 flyby encounter.\u003c/p>\n\u003cp>But we have only a scant few hours’ worth of up-close data for \u003ca href=\"https://solarsystem.nasa.gov/planets/uranus\">Uranus \u003c/a>and \u003ca href=\"https://solarsystem.nasa.gov/planets/neptune\">Neptune. \u003c/a>It was collected by a single spacecraft, Voyager 2, in 1986 and 1989. These planets’ region of the solar system spans well over a billion miles, and \u003ca href=\"http://www.planetary.org/blogs/jason-davis/2017/20170621-revisiting-ice-giants.html\">we know relatively little about them\u003c/a>.\u003c/p>\n\u003cfigure id=\"attachment_1806521\" class=\"wp-caption aligncenter\" style=\"max-width: 800px\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"size-medium wp-image-1806521\" src=\"https://ww2.kqed.org/science/wp-content/uploads/sites/35/2017/07/neptune-greatdarkspot-clouds-800x384.jpg\" alt=\"High clouds (left) and the mysterious storm system dubbed the "Great Dark Spot" (right) in Neptune's atmosphere, captured by Voyager 2 in 1989. \" width=\"800\" height=\"384\" srcset=\"https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/neptune-greatdarkspot-clouds-800x384.jpg 800w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/neptune-greatdarkspot-clouds-160x77.jpg 160w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/neptune-greatdarkspot-clouds-768x369.jpg 768w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/neptune-greatdarkspot-clouds-1020x490.jpg 1020w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/neptune-greatdarkspot-clouds-1180x566.jpg 1180w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/neptune-greatdarkspot-clouds-960x461.jpg 960w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/neptune-greatdarkspot-clouds-240x115.jpg 240w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/neptune-greatdarkspot-clouds-375x180.jpg 375w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/neptune-greatdarkspot-clouds-520x250.jpg 520w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/neptune-greatdarkspot-clouds.jpg 1500w\" sizes=\"(max-width: 800px) 100vw, 800px\">\u003cfigcaption class=\"wp-caption-text\">High clouds (left) and the mysterious storm system dubbed the “Great Dark Spot” (right) in Neptune’s atmosphere, captured by Voyager 2 in 1989. \u003ccite>(NASA/Voyager)\u003c/cite>\u003c/figcaption>\u003c/figure>\n\u003cp>NASA’s recent concept study examines aspects of a future mission. The study ranges from what scientific questions we want to answer about these worlds and their moons, to what type of instrumentation and spacecraft (flyby probe, orbiter, atmospheric probe, or combination of them) would best achieve those scientific goals, to possible technologies and trajectories for getting the spacecraft to their distant destinations.\u003c/p>\n\u003cp>\u003cstrong>A Grander Tour?\u003c/strong>\u003c/p>\n\u003cp>I recall the decade of discovery called the “\u003ca href=\"http://www.aljazeera.com/indepth/opinion/2013/09/how-voyager-missions-became-a-grand-tour-solar-system-20139281055101118.html\">Grand Tour\u003c/a>” in the 1980s when Voyagers 1 and 2 made their way through the outer solar system, bringing us the first visions of its giant worlds and their moons. Only Voyager 2 went on to Uranus and Neptune, beaming back close, detailed pictures of those planets and their moons, where before we had seen only fuzzy balls and dots through Earth’s largest telescopes.\u003c/p>\n\u003cfigure id=\"attachment_1806522\" class=\"wp-caption aligncenter\" style=\"max-width: 800px\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"size-medium wp-image-1806522\" src=\"https://ww2.kqed.org/science/wp-content/uploads/sites/35/2017/07/triton5-800x800.jpg\" alt=\"The largest moon of either ice giant planet, Triton, imaged by Voyager 2 in 1989. Triton may be one of the coldest spots in the solar system, though still shows signs of activity as it spews out plumes of nitrogen gas. \" width=\"800\" height=\"800\" srcset=\"https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/triton5-800x800.jpg 800w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/triton5-160x160.jpg 160w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/triton5-768x768.jpg 768w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/triton5-1020x1020.jpg 1020w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/triton5-1180x1180.jpg 1180w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/triton5-960x960.jpg 960w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/triton5-240x240.jpg 240w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/triton5-375x375.jpg 375w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/triton5-520x520.jpg 520w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/triton5-32x32.jpg 32w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/triton5-50x50.jpg 50w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/triton5-64x64.jpg 64w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/triton5-96x96.jpg 96w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/triton5-128x128.jpg 128w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/triton5-150x150.jpg 150w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/triton5.jpg 1200w\" sizes=\"(max-width: 800px) 100vw, 800px\">\u003cfigcaption class=\"wp-caption-text\">The largest moon of either ice giant planet, Triton, imaged by Voyager 2 in 1989. Triton may be one of the coldest spots in the solar system, though it still shows signs of activity as it spews out plumes of nitrogen gas. \u003ccite>(NASA/Voyager)\u003c/cite>\u003c/figcaption>\u003c/figure>\n\u003cp>The Voyager 2 encounters gave us glimpses of methane-rich atmospheres, cloud formations, unusually shaped magnetic fields, and a large storm on Neptune dubbed the “Great Dark Spot.”\u003c/p>\n\u003cp>Voyager also showed us a variety of unexpectedly dynamic moons, including one—\u003ca href=\"https://solarsystem.nasa.gov/planets/triton/indepth\">Neptune’s large satellite, Triton—\u003c/a>actively spewing plumes of nitrogen gas that fall as frost onto its surface.\u003c/p>\n\u003cp>\u003cstrong>Ice Giants\u003c/strong>\u003c/p>\n\u003cp>The name “ice giants” does not imply that Uranus and Neptune are made of ice, or even contain significant amounts of frozen material. It is a reference both to the frigidly cold region they dwell in, and the expectation that they are composed of materials like water and ammonia and methane—substances we find in frozen form on smaller bodies out there, such as their icy moons.\u003c/p>\n\u003cfigure id=\"attachment_1806519\" class=\"wp-caption aligncenter\" style=\"max-width: 800px\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"size-medium wp-image-1806519\" src=\"https://ww2.kqed.org/science/wp-content/uploads/sites/35/2017/07/Gas_Giant_Interiors-800x477.jpg\" alt=\"The differences between gas giants and ice giants: the gas giants Jupiter and Saturn are largely made of light gases, hydrogen and helium, while Uranus and Neptune (ice giants) consist of heavier substances. The thick mantles of Uranus and Neptune may be massive oceans of water, ammonia, and methane. \" width=\"800\" height=\"477\" srcset=\"https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/Gas_Giant_Interiors-800x477.jpg 800w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/Gas_Giant_Interiors-160x95.jpg 160w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/Gas_Giant_Interiors-768x458.jpg 768w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/Gas_Giant_Interiors-1020x608.jpg 1020w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/Gas_Giant_Interiors.jpg 1920w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/Gas_Giant_Interiors-1180x703.jpg 1180w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/Gas_Giant_Interiors-960x572.jpg 960w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/Gas_Giant_Interiors-240x143.jpg 240w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/Gas_Giant_Interiors-375x223.jpg 375w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/Gas_Giant_Interiors-520x310.jpg 520w\" sizes=\"(max-width: 800px) 100vw, 800px\">\u003cfigcaption class=\"wp-caption-text\">The differences between gas giants and ice giants: the gas giants Jupiter and Saturn are largely made of light gases such as hydrogen and helium, while Uranus and Neptune (ice giants) consist of heavier substances. The thick mantles of Uranus and Neptune may be massive oceans of water, ammonia, and methane. \u003ccite>(NASA)\u003c/cite>\u003c/figcaption>\u003c/figure>\n\u003cp>It is estimated that as much as 60 percent of an ice giant’s mass consists of heavier materials like these—as compared to Jupiter and Saturn, where 85 percent of the gas giants’ bulk is made up of lighter gases such as hydrogen and helium.\u003c/p>\n\u003cp>It may even be that a huge liquid ocean accounting for as much as two-thirds of each ice giant’s mass lies hidden beneath the upper cloud layers. Perhaps “liquid giant” would be a better term.\u003c/p>\n\u003cp>\u003c/p>\n\u003cp>A mission to either of these mysterious planets probably wouldn’t get going until sometime in the next decade, with the actual flight to Uranus or Neptune taking several years. But if the thrilling rewards of Voyager 2’s flybys three decades ago are any indication, it will be a mission well worth waiting for.\u003c/p>\n\n",
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"excerpt": "NASA is considering a mission to explore our solar system's least-understood planets, the distant \"ice giants,\" Uranus and Neptune.",
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"bio": "\u003cstrong>Benjamin Burress\u003c/strong> has been a staff astronomer at Chabot Space & Science Center since July 1999. He graduated from Sonoma State University in 1985 with a bachelor’s degree in physics (and minor in astronomy), after which he signed on for a two-year stint in the Peace Corps, where he taught physics and mathematics in the African nation of Cameroon. From 1989-96 he served on the crew of NASA’s Kuiper Airborne Observatory at Ames Research Center in Mountain View, CA. From 1996-99, he was Head Observer at the Naval Prototype Optical Interferometer program at Lowell Observatory in Flagstaff, AZ.\r\n\r\nRead his \u003ca href=\"http://science.kqed.org/quest/author/ben-burress/\">previous contributions\u003c/a> to \u003ca href=\"http://science.kqed.org/quest/\">QUEST\u003c/a>, a project dedicated to exploring the Science of Sustainability.",
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"content": "\u003cdiv class=\"post-body\">\u003cp>\u003cp>NASA, with participation by the European Space Agency, \u003ca href=\"https://www.jpl.nasa.gov/news/news.php?feature=6877\">has just completed a concept study \u003c/a>for a mission—or missions—to explore our solar system’s least-understood planets, the distant “ice giants” Uranus and Neptune.\u003c/p>\n\u003cp>Many of us grew up reading textbooks that described Uranus and Neptune as two of the four “gas giant” worlds of our solar system, along with Jupiter and Saturn. We were taught they were colder and smaller—and quite a bit bluer—than their two larger siblings, but were otherwise probably like them in composition and structure.\u003c/p>\n\u003cp>But telescope observations from Earth, as well as the Voyager 2 data, have led scientists to suspect Uranus and Neptune may be fundamentally different from Jupiter and Saturn—different enough to have their own term: “ice giants.”\u003c/p>\n\u003cfigure id=\"attachment_1806520\" class=\"wp-caption aligncenter\" style=\"max-width: 800px\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"size-medium wp-image-1806520\" src=\"https://ww2.kqed.org/science/wp-content/uploads/sites/35/2017/07/Uranus-800x515.jpg\" alt=\"An infrared image of the ice giant Uranus and its thin rings, captured by the Hubble Space Telescope. \" width=\"800\" height=\"515\" srcset=\"https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/Uranus-800x515.jpg 800w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/Uranus-160x103.jpg 160w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/Uranus-768x495.jpg 768w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/Uranus.jpg 894w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/Uranus-240x155.jpg 240w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/Uranus-375x242.jpg 375w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/Uranus-520x335.jpg 520w\" sizes=\"(max-width: 800px) 100vw, 800px\">\u003cfigcaption class=\"wp-caption-text\">An infrared image of the ice giant Uranus and its thin rings, captured by the Hubble Space Telescope. \u003ccite>(NASA/ESA/STScI)\u003c/cite>\u003c/figcaption>\u003c/figure>\n\u003cp>Scientists are hoping to learn more about how these planets and their moons formed long ago and, by extension, what conditions prevailed in the earliest times of the solar system’s existence.\u003c/p>\n\u003cp>\u003cstrong>Solar System Forensics\u003c/strong>\u003c/p>\n\u003cp>\u003c/p>\u003c/div>",
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"content": "\u003cdiv class=\"post-body\">\u003cp>\u003c/p>\n\u003cp>Scientists piece together what the \u003ca href=\"https://www.windows2universe.org/our_solar_system/formation.html\">early solar system\u003c/a> was like by studying planets, moons, asteroids, and comets as sites of forensic evidence.\u003c/p>\n\u003cp>\u003c/p>\u003cp>\u003c/p>\u003cp>Every planet closer to the sun than Uranus—besides Earth, this includes Saturn, Jupiter, Mars, Venus, Mercury, and dwarf planet Ceres—has been explored with flyby missions and at least one long-term orbiter. To some of these planets we have sent atmospheric or surface-landing robots.\u003c/p>\n\u003cp>We have even investigated the frozen time capsules called comets, which originate far beyond the realm of the ice giants and preserve pristine, undisturbed evidence of the solar system’s earliest years. Even the dwarf planet Pluto and its moons yielded clues to those early times, when the New Horizons spacecraft grabbed a large batch of high quality data during its 2015 flyby encounter.\u003c/p>\n\u003cp>But we have only a scant few hours’ worth of up-close data for \u003ca href=\"https://solarsystem.nasa.gov/planets/uranus\">Uranus \u003c/a>and \u003ca href=\"https://solarsystem.nasa.gov/planets/neptune\">Neptune. \u003c/a>It was collected by a single spacecraft, Voyager 2, in 1986 and 1989. These planets’ region of the solar system spans well over a billion miles, and \u003ca href=\"http://www.planetary.org/blogs/jason-davis/2017/20170621-revisiting-ice-giants.html\">we know relatively little about them\u003c/a>.\u003c/p>\n\u003cfigure id=\"attachment_1806521\" class=\"wp-caption aligncenter\" style=\"max-width: 800px\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"size-medium wp-image-1806521\" src=\"https://ww2.kqed.org/science/wp-content/uploads/sites/35/2017/07/neptune-greatdarkspot-clouds-800x384.jpg\" alt=\"High clouds (left) and the mysterious storm system dubbed the "Great Dark Spot" (right) in Neptune's atmosphere, captured by Voyager 2 in 1989. \" width=\"800\" height=\"384\" srcset=\"https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/neptune-greatdarkspot-clouds-800x384.jpg 800w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/neptune-greatdarkspot-clouds-160x77.jpg 160w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/neptune-greatdarkspot-clouds-768x369.jpg 768w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/neptune-greatdarkspot-clouds-1020x490.jpg 1020w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/neptune-greatdarkspot-clouds-1180x566.jpg 1180w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/neptune-greatdarkspot-clouds-960x461.jpg 960w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/neptune-greatdarkspot-clouds-240x115.jpg 240w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/neptune-greatdarkspot-clouds-375x180.jpg 375w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/neptune-greatdarkspot-clouds-520x250.jpg 520w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/neptune-greatdarkspot-clouds.jpg 1500w\" sizes=\"(max-width: 800px) 100vw, 800px\">\u003cfigcaption class=\"wp-caption-text\">High clouds (left) and the mysterious storm system dubbed the “Great Dark Spot” (right) in Neptune’s atmosphere, captured by Voyager 2 in 1989. \u003ccite>(NASA/Voyager)\u003c/cite>\u003c/figcaption>\u003c/figure>\n\u003cp>NASA’s recent concept study examines aspects of a future mission. The study ranges from what scientific questions we want to answer about these worlds and their moons, to what type of instrumentation and spacecraft (flyby probe, orbiter, atmospheric probe, or combination of them) would best achieve those scientific goals, to possible technologies and trajectories for getting the spacecraft to their distant destinations.\u003c/p>\n\u003cp>\u003cstrong>A Grander Tour?\u003c/strong>\u003c/p>\n\u003cp>I recall the decade of discovery called the “\u003ca href=\"http://www.aljazeera.com/indepth/opinion/2013/09/how-voyager-missions-became-a-grand-tour-solar-system-20139281055101118.html\">Grand Tour\u003c/a>” in the 1980s when Voyagers 1 and 2 made their way through the outer solar system, bringing us the first visions of its giant worlds and their moons. Only Voyager 2 went on to Uranus and Neptune, beaming back close, detailed pictures of those planets and their moons, where before we had seen only fuzzy balls and dots through Earth’s largest telescopes.\u003c/p>\n\u003cfigure id=\"attachment_1806522\" class=\"wp-caption aligncenter\" style=\"max-width: 800px\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"size-medium wp-image-1806522\" src=\"https://ww2.kqed.org/science/wp-content/uploads/sites/35/2017/07/triton5-800x800.jpg\" alt=\"The largest moon of either ice giant planet, Triton, imaged by Voyager 2 in 1989. Triton may be one of the coldest spots in the solar system, though still shows signs of activity as it spews out plumes of nitrogen gas. \" width=\"800\" height=\"800\" srcset=\"https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/triton5-800x800.jpg 800w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/triton5-160x160.jpg 160w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/triton5-768x768.jpg 768w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/triton5-1020x1020.jpg 1020w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/triton5-1180x1180.jpg 1180w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/triton5-960x960.jpg 960w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/triton5-240x240.jpg 240w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/triton5-375x375.jpg 375w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/triton5-520x520.jpg 520w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/triton5-32x32.jpg 32w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/triton5-50x50.jpg 50w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/triton5-64x64.jpg 64w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/triton5-96x96.jpg 96w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/triton5-128x128.jpg 128w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/triton5-150x150.jpg 150w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/triton5.jpg 1200w\" sizes=\"(max-width: 800px) 100vw, 800px\">\u003cfigcaption class=\"wp-caption-text\">The largest moon of either ice giant planet, Triton, imaged by Voyager 2 in 1989. Triton may be one of the coldest spots in the solar system, though it still shows signs of activity as it spews out plumes of nitrogen gas. \u003ccite>(NASA/Voyager)\u003c/cite>\u003c/figcaption>\u003c/figure>\n\u003cp>The Voyager 2 encounters gave us glimpses of methane-rich atmospheres, cloud formations, unusually shaped magnetic fields, and a large storm on Neptune dubbed the “Great Dark Spot.”\u003c/p>\n\u003cp>Voyager also showed us a variety of unexpectedly dynamic moons, including one—\u003ca href=\"https://solarsystem.nasa.gov/planets/triton/indepth\">Neptune’s large satellite, Triton—\u003c/a>actively spewing plumes of nitrogen gas that fall as frost onto its surface.\u003c/p>\n\u003cp>\u003cstrong>Ice Giants\u003c/strong>\u003c/p>\n\u003cp>The name “ice giants” does not imply that Uranus and Neptune are made of ice, or even contain significant amounts of frozen material. It is a reference both to the frigidly cold region they dwell in, and the expectation that they are composed of materials like water and ammonia and methane—substances we find in frozen form on smaller bodies out there, such as their icy moons.\u003c/p>\n\u003cfigure id=\"attachment_1806519\" class=\"wp-caption aligncenter\" style=\"max-width: 800px\">\u003cimg loading=\"lazy\" decoding=\"async\" class=\"size-medium wp-image-1806519\" src=\"https://ww2.kqed.org/science/wp-content/uploads/sites/35/2017/07/Gas_Giant_Interiors-800x477.jpg\" alt=\"The differences between gas giants and ice giants: the gas giants Jupiter and Saturn are largely made of light gases, hydrogen and helium, while Uranus and Neptune (ice giants) consist of heavier substances. The thick mantles of Uranus and Neptune may be massive oceans of water, ammonia, and methane. \" width=\"800\" height=\"477\" srcset=\"https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/Gas_Giant_Interiors-800x477.jpg 800w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/Gas_Giant_Interiors-160x95.jpg 160w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/Gas_Giant_Interiors-768x458.jpg 768w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/Gas_Giant_Interiors-1020x608.jpg 1020w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/Gas_Giant_Interiors.jpg 1920w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/Gas_Giant_Interiors-1180x703.jpg 1180w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/Gas_Giant_Interiors-960x572.jpg 960w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/Gas_Giant_Interiors-240x143.jpg 240w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/Gas_Giant_Interiors-375x223.jpg 375w, https://cdn.kqed.org/wp-content/uploads/sites/35/2017/07/Gas_Giant_Interiors-520x310.jpg 520w\" sizes=\"(max-width: 800px) 100vw, 800px\">\u003cfigcaption class=\"wp-caption-text\">The differences between gas giants and ice giants: the gas giants Jupiter and Saturn are largely made of light gases such as hydrogen and helium, while Uranus and Neptune (ice giants) consist of heavier substances. The thick mantles of Uranus and Neptune may be massive oceans of water, ammonia, and methane. \u003ccite>(NASA)\u003c/cite>\u003c/figcaption>\u003c/figure>\n\u003cp>It is estimated that as much as 60 percent of an ice giant’s mass consists of heavier materials like these—as compared to Jupiter and Saturn, where 85 percent of the gas giants’ bulk is made up of lighter gases such as hydrogen and helium.\u003c/p>\n\u003cp>It may even be that a huge liquid ocean accounting for as much as two-thirds of each ice giant’s mass lies hidden beneath the upper cloud layers. Perhaps “liquid giant” would be a better term.\u003c/p>\n\u003cp>\u003c/p>\n\u003cp>A mission to either of these mysterious planets probably wouldn’t get going until sometime in the next decade, with the actual flight to Uranus or Neptune taking several years. But if the thrilling rewards of Voyager 2’s flybys three decades ago are any indication, it will be a mission well worth waiting for.\u003c/p>\n\n\u003c/div>\u003c/p>",
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"info": "The MindShift podcast explores the innovations in education that are shaping how kids learn. Hosts Ki Sung and Katrina Schwartz introduce listeners to educators, researchers, parents and students who are developing effective ways to improve how kids learn. We cover topics like how fed-up administrators are developing surprising tactics to deal with classroom disruptions; how listening to podcasts are helping kids develop reading skills; the consequences of overparenting; and why interdisciplinary learning can engage students on all ends of the traditional achievement spectrum. This podcast is part of the MindShift education site, a division of KQED News. KQED is an NPR/PBS member station based in San Francisco. You can also visit the MindShift website for episodes and supplemental blog posts or tweet us \u003ca href=\"https://twitter.com/MindShiftKQED\">@MindShiftKQED\u003c/a> or visit us at \u003ca href=\"/mindshift\">MindShift.KQED.org\u003c/a>",
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"tagline": "Politics from a personal perspective",
"info": "Political Breakdown is a new series that explores the political intersection of California and the nation. Each week hosts Scott Shafer and Marisa Lagos are joined with a new special guest to unpack politics -- with personality — and offer an insider’s glimpse at how politics happens.",
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"possible": {
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"info": "Possible is hosted by entrepreneur Reid Hoffman and writer Aria Finger. Together in Possible, Hoffman and Finger lead enlightening discussions about building a brighter collective future. The show features interviews with visionary guests like Trevor Noah, Sam Altman and Janette Sadik-Khan. Possible paints an optimistic portrait of the world we can create through science, policy, business, art and our shared humanity. It asks: What if everything goes right for once? How can we get there? Each episode also includes a short fiction story generated by advanced AI GPT-4, serving as a thought-provoking springboard to speculate how humanity could leverage technology for good.",
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"pri-the-world": {
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"title": "PRI's The World: Latest Edition",
"info": "Each weekday, host Marco Werman and his team of producers bring you the world's most interesting stories in an hour of radio that reminds us just how small our planet really is.",
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"imageSrc": "https://cdn.kqed.org/wp-content/uploads/2024/04/The-World-Podcast-Tile-360x360-1.jpg",
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},
"radiolab": {
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"title": "Radiolab",
"info": "A two-time Peabody Award-winner, Radiolab is an investigation told through sounds and stories, and centered around one big idea. In the Radiolab world, information sounds like music and science and culture collide. Hosted by Jad Abumrad and Robert Krulwich, the show is designed for listeners who demand skepticism, but appreciate wonder. WNYC Studios is the producer of other leading podcasts including Freakonomics Radio, Death, Sex & Money, On the Media and many more.",
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},
"reveal": {
"id": "reveal",
"title": "Reveal",
"info": "Created by The Center for Investigative Reporting and PRX, Reveal is public radios first one-hour weekly radio show and podcast dedicated to investigative reporting. Credible, fact based and without a partisan agenda, Reveal combines the power and artistry of driveway moment storytelling with data-rich reporting on critically important issues. The result is stories that inform and inspire, arming our listeners with information to right injustices, hold the powerful accountable and improve lives.Reveal is hosted by Al Letson and showcases the award-winning work of CIR and newsrooms large and small across the nation. In a radio and podcast market crowded with choices, Reveal focuses on important and often surprising stories that illuminate the world for our listeners.",
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"officialWebsiteLink": "https://www.revealnews.org/episodes/",
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},
"rightnowish": {
"id": "rightnowish",
"title": "Rightnowish",
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