{"id":221913,"date":"2017-06-21T21:56:58","date_gmt":"2017-06-22T01:56:58","guid":{"rendered":"http:\/\/www.euvolution.com\/futurist-transhuman-news-blog\/uncategorized\/revisiting-the-ice-giants-nasa-considers-missions-to-uranus-and-neptune-the-planetary-society-blog.php"},"modified":"2017-06-21T21:56:58","modified_gmt":"2017-06-22T01:56:58","slug":"revisiting-the-ice-giants-nasa-considers-missions-to-uranus-and-neptune-the-planetary-society-blog","status":"publish","type":"post","link":"https:\/\/www.euvolution.com\/futurist-transhuman-news-blog\/nasa\/revisiting-the-ice-giants-nasa-considers-missions-to-uranus-and-neptune-the-planetary-society-blog.php","title":{"rendered":"Revisiting the ice giants: NASA considers missions to Uranus and Neptune &#8211; The Planetary Society (blog)"},"content":{"rendered":"<p><p>    Jason    Davis  June21,2017  <\/p>\n<p>    If you look up Uranus and Neptune in an encyclopedia, there's a    good chance the pictures you see will be about 30 years old.  <\/p>\n<p>    In the late 1970s, the twin Voyager spacecraft launched on a    grand tour of the solar system, taking advantage of a rare planetary alignment that only happens every    175 years. Voyager 2 flew past Uranus in January 1986, and    Neptune in August 1989. The probe was traveling too fast, and    lacked the fuel, to slow down and enter orbit.  <\/p>\n<p>    We haven't been back since.  <\/p>\n<p>    Every 10 years, NASA releases a report called the decadal survey outlining    top priorities for planetary exploration. The current    iteration, covering 2013 through 2022, identifies three top    missions: Mars sample return, the Europa Clipper, and a return to Uranus    or Neptune (Uranus was favored due to more convenient planetary    alignments, which affects travel times).  <\/p>\n<p>    With the next decadal survey just five years away, scientists    are revisiting the plan to send a spacecraft to our outermost    planets, known as the ice giants. A new NASA report, officially    a \"pre-decadal\" mission study, describes the reasons to go and    the spacecraft that could take us there.  <\/p>\n<p>        NASA \/ JPL      <\/p>\n<p>    Like most planets, our understanding of Uranus and Neptune has    greatly evolved since the early days of planetary science.  <\/p>\n<p>    Before photographic imagery became a common tool for studying    the universe, astronomers spent long, cold nights hunched over    telescope eyepieces, hand-drawing what their eyes saw.  <\/p>\n<p>    Heidi Hammel, a Planetary Society board member and the    executive vice president of AURA, a consortium of universities    that operates astronomical observatories, told me some early    Uranus drawings portrayed the planet with distinct atmospheric    features. The advent of photography changed that, revealing the    planet as a featureless, pale-green orb. This led to a theory    that planets farther from the Sun exhibited less atmospheric    activity.  <\/p>\n<p>    Intuitively, this made sense: Jupiter has vibrant bands and    swirls, Saturn is stormy but muted, and Uranus was featureless    (Neptune was too far away to discern much of anything).  <\/p>\n<p>    \"When Voyager flew by Uranus, it was like, 'Well, okay, we were    right,'\" Hammel said. \"There were no clouds to look at there.    It was very bland, with maybe 10 discrete cloud features.\"  <\/p>\n<p>    Neptune was expected to be equally dull. But when Voyager    arrived three years later, that wasn't the case.  <\/p>\n<p>    \"Neptune was a huge shock,\" she said. \"There was this huge dark    spot, like a quarter of the size of the planetreally    monstrous. And then all of these bright features, and    eventually a second dark feature, and all sorts of clouds. I    mean, this planet was just absolutely covered with storm    systems.\"  <\/p>\n<p>    Why, then, was Uranus so bland? The question went unaddressed    for years, until Hammel saw an academic poster at a conference    with long-exposure images of Uranus captured by the Hubble    Space Telescope. The images, taken in support of a search for    new moons, inadvertently revealed a set of features not seen by    Voyager 2.  <\/p>\n<p>    \"I said, what is that?\" Hammel recalled. The poster author    replied, \"Well, that's Uranus.\"  <\/p>\n<p>    Uranus, famously, orbits the Sun tipped on its side. When    Voyager flew past, the planet's pole was facing the Sun. Since    then, Uranus' 84-year orbit around the sun has progressed    enough to illuminate more of the equator. This has apparently    had a drastic effect on the planet's atmosphere, activating a    host of swirls and storms.  <\/p>\n<p>    Follow-up observations with adaptive optics-equipped ground    telescopes continued to reveal new features. As for the early    Uranus photographs, Hammel said atmospheric distortion likely    smeared out discernible features, meaning those original    astronomical drawings may have been correct all along.  <\/p>\n<p>    \"Only now do we have the technology to reproduce what the human    eye was able to see back in the eighteen hundreds,\" she said.  <\/p>\n<p>        Heidi Hammel, Imke de Pater, W. M. Keck        Observatory      <\/p>\n<p>    The most pressing question to be solved by a mission to either    of the ice giants is figuring out what lies beneath the    planets' outer layers of clouds. This is similar to the    question NASA's Juno spacecraft is trying to answer at Jupiter.  <\/p>\n<p>    Figuring out these planets' basic compositions and interior    structures would fill an important gap in our knowledge of how    solar systems form. Among the exoplanets we've discovered,    worlds weighing the same as Uranus and Neptune appear more    common than gas giants like Jupiter and Saturn. Yet ice giants    seem to require a very specific set of conditions to form    during the birth of a solar system.  <\/p>\n<p>    \"Based on the current models, it looks like there's only a    really narrow time window when you can get these sort of    planets to form,\" said Amy Simon, a senior scientist at NASA's    Goddard Space Flight Center. \"You need to have a big enough    core, but on the other hand, you need to have the solar nebula    dissipating so that you can get these gas and ices in there at    the same time.\"  <\/p>\n<p>    Simon co-chaired the science team for the new ice giants    report. She told me the reasons to go back, as well as the top    science priorities, have not drastically changed since the last    decadal survey.  <\/p>\n<p>    \"There weren't a ton of changes,\" she said. \"The focus was on a    more detailed study of all the mission trades, to look at the    technology you might need, and what type of mission you'd like    to fly.\"  <\/p>\n<p>    All of the mission concepts envision detachable probes that    would be sent hurtling into the ice giants' atmospheres. The    main spacecraft would remain in orbit at least two or three    years, and be nuclear-powered, owing to the small amount of    sunlight reaching that far into space.  <\/p>\n<p>    The basic set of proposed science instruments include a camera,    magnetometers and a doppler imager. The doppler imager, Simon    said, was a particularly innovative example of how the planets'    interior structures could be revealed.  <\/p>\n<p>    \"The idea behind it is that you're essentially looking for    seismic waves on the planet,\" she said. \"You're looking to see    the planet oscillate. And the idea behind that is similar to    studies they've done on the Sun, where you can see the Sun    oscillating and you can determine its interior structure.\"  <\/p>\n<p>        NASA \/ JPL-Caltech \/ Justin Cowart      <\/p>\n<p>    The Voyager 2 mission also captured one-sided glimpses of    Uranus' and Neptune's major moons.  <\/p>\n<p>    One of the most interesting moons turned out to be Triton.    Triton is believed to be a Kuiper Belt object captured by    Neptune's gravitational pull. In the process, Triton either    smacked into the rest of Neptune's moons or flung them out of    the system entirely.  <\/p>\n<p>    Voyager images revealed a relatively young surface that looked    like the skin of a cantaloupe, with nitrogen-spewing geysers in    the southern hemisphere.  <\/p>\n<p>    \"And again,\" said Simon, \"We've only seen part of Triton. Who    knows what's on the other side?\"  <\/p>\n<p>    \"With Triton, you can do comparative planetology to Pluto,\"    Hammel said. \"They're a matched set of Kuiper Belt objects,    like fraternal twins who were separated at birth and took on    completely different life stories.\"  <\/p>\n<p>    Uranus, on the other hand, has five large moons: Miranda,    Ariel, Umbriel, Titania, and Oberon. Unlike Triton, they are    likely native to the planet's system, making them our only    chance to study large worlds leftover from an ice giant's    formation.  <\/p>\n<p>    The new report does not single out a preference for visiting    either Uranus or Neptune. Both are \"equally compelling as a    scientific target,\" it said.  <\/p>\n<p>    \"Each planet has something important to teach us that the other    cannot,\" said Hammel. \"I think the deciding factor will    probably have to do with what launch vehicles are available,    and what trajectories are most favorable to get us to those    planets in a reasonable amount of time. Scientifically, your    bounty is going to be fabulous for either planet.\"  <\/p>\n<p>        Hubble \/ Ted Stryk, Roane State CC      <\/p>\n<p>    What, exactly, constitutes a reasonable amount of time for    getting to Uranus or Neptune?  <\/p>\n<p>    Simon said the report assumes a spacecraft life of about 15    years, even though missions like Voyager, as well as the    Cassini spacecraft at Saturn, have exceeded that.  <\/p>\n<p>    \"There are reliability limitations on the hardware,\" she said.    \"Even though we've seen propulsion tanks last longer than that,    that's just not how they're rated. We didn't want to be pushing    the reliability too hard.\"  <\/p>\n<p>    The travel time to Uranus, using an Atlas V with five solid    rocket boosters, is 12 years for an orbiter. It takes 13 years    to get to Neptune using a Delta IV Heavy launcherand that's    with an extra solar-electric propulsion stage to add additional    thrust. All missions require Jupiter gravity assists, as well    as likely flybys of Venus and Earth.  <\/p>\n<p>    NASA's heavy lift Space Launch System, SLS, could potentially    shave four years off the transit time. But there's a catch: a    spacecraft can't go too fast, because it still has to slow down    to enter orbit upon arrival. The report notes aerocapture    techniquesbasically, skimming the planet's atmosphere to shave    speedcould allow for higher cruising velocities.  <\/p>\n<p>    A vehicle like SLS could, however, launch two missions at once.    But that's assuming NASA spends what could end up being $2    billion per mission.  <\/p>\n<p>    Good launch windows are available for Uranus between 2030 and    2034, while Neptune trajectories are favorable around 2029.    That means we might not get to see the ice giants again until    the late 30s or early 40s.  <\/p>\n<p>    That's still okay with both Hammel and Simon.  <\/p>\n<p>    \"I kind of hope this excites younger scientists, because this    will be their mission,\" said Simon, who recalls seeing Voyager    2 images on TV as a child. \"We might get it off the ground for    them, but they are going to be the scientists doing the    activities. So I really hope it does generate a lot of interest    in early career folks, and in the public.\"  <\/p>\n<p>        Become a member of The Planetary Society and together we        will create the future of space exploration.      <\/p>\n<p>        Join Today      <\/p>\n<p>        Support enables our dedicated journalists to research        deeply and bring you original space exploration articles.      <\/p>\n<p>                Donate      <\/p>\n<p>        Empowering the world's citizens to advance space science        and exploration.      <\/p>\n<p>                Member Login         2017 The Planetary Society. All rights reserved.                Terms of Use The Planetary Society is a registered        501(c)(3) nonprofit organization.      <\/p>\n<p><!-- Auto Generated --><\/p>\n<p>Original post: <\/p>\n<p><a target=\"_blank\" href=\"http:\/\/www.planetary.org\/blogs\/jason-davis\/2017\/20170621-revisiting-ice-giants.html\" title=\"Revisiting the ice giants: NASA considers missions to Uranus and Neptune - The Planetary Society (blog)\">Revisiting the ice giants: NASA considers missions to Uranus and Neptune - The Planetary Society (blog)<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p> Jason Davis June21,2017 If you look up Uranus and Neptune in an encyclopedia, there's a good chance the pictures you see will be about 30 years old. In the late 1970s, the twin Voyager spacecraft launched on a grand tour of the solar system, taking advantage of a rare planetary alignment that only happens every 175 years.  <a href=\"https:\/\/www.euvolution.com\/futurist-transhuman-news-blog\/nasa\/revisiting-the-ice-giants-nasa-considers-missions-to-uranus-and-neptune-the-planetary-society-blog.php\">Continue reading <span class=\"meta-nav\">&rarr;<\/span><\/a><\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"limit_modified_date":"","last_modified_date":"","_lmt_disableupdate":"","_lmt_disable":"","footnotes":""},"categories":[20],"tags":[],"class_list":["post-221913","post","type-post","status-publish","format-standard","hentry","category-nasa"],"modified_by":null,"_links":{"self":[{"href":"https:\/\/www.euvolution.com\/futurist-transhuman-news-blog\/wp-json\/wp\/v2\/posts\/221913"}],"collection":[{"href":"https:\/\/www.euvolution.com\/futurist-transhuman-news-blog\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.euvolution.com\/futurist-transhuman-news-blog\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.euvolution.com\/futurist-transhuman-news-blog\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/www.euvolution.com\/futurist-transhuman-news-blog\/wp-json\/wp\/v2\/comments?post=221913"}],"version-history":[{"count":0,"href":"https:\/\/www.euvolution.com\/futurist-transhuman-news-blog\/wp-json\/wp\/v2\/posts\/221913\/revisions"}],"wp:attachment":[{"href":"https:\/\/www.euvolution.com\/futurist-transhuman-news-blog\/wp-json\/wp\/v2\/media?parent=221913"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.euvolution.com\/futurist-transhuman-news-blog\/wp-json\/wp\/v2\/categories?post=221913"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.euvolution.com\/futurist-transhuman-news-blog\/wp-json\/wp\/v2\/tags?post=221913"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}