{"id":14089,"date":"2018-01-06T19:32:01","date_gmt":"2018-01-06T11:32:01","guid":{"rendered":"https:\/\/wp-productionenv-bjg9h2g2bgg5b8aa.southeastasia-01.azurewebsites.net\/news\/plot-thickens-as-new-horizons-moves-within-year-of-next-flyby\/"},"modified":"2018-01-06T19:32:01","modified_gmt":"2018-01-06T11:32:01","slug":"plot-thickens-as-new-horizons-moves-within-year-of-next-flyby","status":"publish","type":"post","link":"https:\/\/starpath.global\/news\/plot-thickens-as-new-horizons-moves-within-year-of-next-flyby\/","title":{"rendered":"Plot thickens as New Horizons moves within year of next flyby"},"content":{"rendered":"
\"\"
Artist\u2019s concept of the New Horizons spacecraft\u2019s flyby of 2014 MU69. Credit: NASA\/Johns Hopkins University Applied Physics Laboratory\/Southwest Research Institute\/Steve Gribben<\/figcaption><\/figure>\n

The final days before NASA\u2019s New Horizons probe barrels in on its next destination on Jan. 1, 2019, should prove eventful, with scientists trying to sort out whether a distant mini-world detected by the Hubble Space Telescope more than three years ago may actually be a swarm of icy objects.<\/p>\n

New Horizons\u2019 sharp-eyed camera will serve as a look-out as the spacecraft makes a speedy approach toward 2014 MU69, the official name for the mission\u2019s next target. Scientists will search for moons and icy debris, discoveries which could add intrigue to the one-shot encounter on New Year\u2019s Day 2019.<\/p>\n

2014 MU69 is poised to become the most distant object ever visited, and New Horizons\u2019 science team know little about the spacecraft\u2019s next destinations, which lurks in the dark reaches of the Kuiper Belt a billion miles (1.6 billion kilometers) beyond Pluto.<\/p>\n

\u201cBesides being the farthest exploration in the history of humankind, this flyby is also going to the most primitive and pristine object ever explored,\u201d said Alan Stern, principal investigator on the New Horizons mission from the Southwest Research Institute in Boulder, Colorado. \u201cWe\u2019ve really never been to anything like this.\u201d<\/p>\n

The nuclear-powered spacecraft made the first close-up exploration of Pluto and its moons in July 2015, and NASA has approved a new flight plan to fly past 2014 MU69, which scientists say is 100 times smaller than Pluto.<\/p>\n

But new evidence suggests 2014 MU69, which NASA says will get a new nickname in the coming months, could consist of multiple objects bound together by tenuous gravity.<\/p>\n

Using precise tracking data from Hubble and an updated star catalog provided by the European Space Agency\u2019s Gaia mission, astronomers found three opportunities last June and July when 2014 MU69 would pass between the Earth and another star. On each occasion, the star\u2019s light was briefly blocked by the object\u2019s passage.<\/p>\n

Scientists deployed an array of telescopes to Argentina and South Africa in June, but they saw nothing when they expected to see a star temporarily wink out. It turns out the astronomers put the telescopes in the wrong place.<\/p>\n

Another chance came July 10, when the U.S.-German SOFIA airborne observatory flew to a point where 2014 MU69\u2019s shadow was projected to again blot out a star. Again, astronomers saw nothing.<\/p>\n

But the New Horizons team hit a jackpot July 17, said Marc Buie, a co-investigator on the mission from SWRI.<\/p>\n

\u201c(For) just the barest brief bit of time the star winked out,\u201d Buie said in a press briefing last month at the American Geophysical Union\u2019s fall meeting in New Orleans. \u201cI have to say this was very reassuring. Up to now, we\u2019re looking at a really faint little blip from Hubble, and you can wonder, \u2018Is this really real?\u2019 But, boy, when it blots out the star you know you\u2019ve got something.\u201d<\/p>\n

Astronomers plotted observations from dozens of telescopes, showing exactly when and for how long each telescope saw 2014 MU69 block, or occult, the light from a background star.<\/p>\n

\"\"
Scientists plotted the occultation measurements from 22 telescopes July 10, revealing an outline of 2014 MU69\u2019s expected shape. Credit: NASA\/JHUAPL\/SWRI\/Marc Buie<\/figcaption><\/figure>\n

The occultations observed by each telescope varied in time and length, immediately telling Buie and his team that 2014 MU69 was not perfectly round world. The object is probably a dual-lobe world, with its two segments either orbiting one another or a contact binary stuck together \u201clike two globs of ice cream,\u201d Buie said.<\/p>\n

But there\u2019s more to the story.<\/p>\n

Astronomers took a closer look at data from SOFIA\u2019s attempt July 10 to catch 2014 MU69\u2019s shadow, and the airborne telescope did see a momentary blip in the star the object was predicted to block, but not at the expected time and location.<\/p>\n

While stressing the results are still preliminary, Buie said his team, which led last year\u2019s occultation observations, believes SOFIA saw a moonlet orbiting 2014 MU69 that has, so far, escaped detection by even the sharpest telescopes, like Hubble. The hypothesized moon also went undetected during the following ground-based campaign July 17.<\/p>\n

\u201cWhat we think is we\u2019ve got a contact binary, orbiting around a common center of mass with another moon that sits out there, so now it\u2019s almost like we\u2019ve got three objects in one here,\u201d Buie said.<\/p>\n

\u201cThis is very exciting,\u201d he said. \u201cIf you ever thought why are we going to this little chunk of rock out in the middle of nowhere out in the outer solar system, this is going to have a lot of surprises. We think that this is probably a sign that the object itself was not a collisional fragment. We think it was made like this, and we really are going to see something that dates back to the birth of our solar system.\u201d<\/p>\n

\u201cThis might be the harbinger, it might be a hint that there is actually a swarm of satellites around MU69,\u201d Stern said.<\/p>\n

With less than a year left until New Horizons\u2019 arrival, scientists have limited time to learn more about 2014 MU69.<\/p>\n

Buie\u2019s team has identified one more occultation opportunity, on Aug. 4, when telescopes could again be deployed to map 2014 MU69\u2019s shape, and perhaps confirm the presence of a moon.<\/p>\n

2014 MU69 will blot out the light from a star in a swath extending from South America, across the Atlantic Ocean, into North Africa. Buie said the New Horizons science team is discussing a field campaign with partners in Colombia and Senegal, where a network of mobile telescopes could be placed to try and find the shadow of 2014 MU69 and its potential moon.<\/p>\n

After that, the next chance for scientists to learn more about 2014 MU69 will come in the final weeks and days before New Horizons speeds by the object.<\/p>\n

\u201cWe won\u2019t resolve the object until the week of the flyby, and it\u2019s going to be a very exciting, almost overnight experience in which MU69 will go from a point of light to a real place in the sky, a new world that humans have explored,\u201d Stern said.<\/p>\n

\u201cMU69 will appear as a point of light, or if there are satellites, multiple points of light, until literally the last day or two, and then it will be just a couple of pixels across, and it will only be after the flyby on Jan. 1, 2 and 3, that spectacular images will start to come to the ground.\u201d<\/p>\n

The Kuiper Belt is made up of hundreds of thousands of frozen rocks and dwarf planets that orbit the sun beyond Neptune. Pluto is the largest of the group, but scientists think the city-sized 2014 MU69 is more representative of the Kuiper Belt\u2019s population.<\/p>\n

Objects orbiting in the Kuiper Belt are the leftovers from the solar system\u2019s formation, when dust came together to form protoplanets, and collisions eventually led to the genesis of the planets themselves.<\/p>\n

2014 MU69, which appears reddish in Hubble imagery, has likely remained in its primordial state since the solar system\u2019s early history 4.5 billion years ago. Comets that come from the far outer solar system originated in the same frozen, faint environment, but repeated passes near the sun have erased their ancient characteristics.<\/p>\n

\u201cThis object has always been in this very low collisional environment, very cold \u2014 basically 40 degrees above absolute zero (minus 387 degrees Fahrenheit) \u2014 so it should have preserved a record of that accretionary time better than anything that\u2019s ever been observed by any spacecraft mission in history,\u201d Stern said.<\/p>\n

\"\"
New Horizons\u2019s trajectory to its next target, the Kuiper Belt object 2014 MU69. Credit: NASA<\/figcaption><\/figure>\n

Running on a plutonium power source and traveling with enough speed to eventually escape the sun\u2019s gravitational grip, New Horizons is set to make its closest approach to 2014 MU69 at 12:33 a.m. EST (0533 GMT) on Jan. 1, 2019.<\/p>\n

The flyby will occur late on New Year\u2019s Eve in the other U.S. time zones, when New Horizons will pass by its distant target at a relative velocity of more than 31,000 mph (14 kilometers per second).<\/p>\n

Ground controllers placed the spacecraft into hibernation mode last month, and an on-board timer is due to wake up the probe June 4 for an instrument checkout ahead of the formal start of the 2014 MU69 encounter phase in mid-August.<\/p>\n

One of New Horizons\u2019 first jobs will be to locate 2014 MU69 with its on-board camera, a milestone expected in August or September. The spacecraft\u2019s navigation team will use the observations to ensure New Horizons is on the right approach trajectory.<\/p>\n

Mission planners have built in nine opportunities for New Horizons to fine-tune its course with minor thruster firings, beginning in mid-October and extending through Dec. 22, according to Alice Bowman, the mission operations manager at the Johns Hopkins University Applied Physics Laboratory.<\/p>\n

All of the course corrections may not be required.<\/p>\n

\u201cOnce we detect (2014 MU69), we\u2019ll be looking for the moon that we have the hints of from the occulation data,\u201d said John Spencer, New Horizons\u2019 deputy project scientist from SWRI. \u201cWe\u2019ll be looking for maybe additional moons that might be there, trying to map their orbits. We\u2019ll be surveying the region around MU69 for hazardous material, and we\u2019ll also be refining our navigation of where MU69 is.\u201d<\/p>\n

The best guess for the potential moon\u2019s size is roughly 3 miles (5 kilometers) across, and nearly 200 miles (300 kilometers) could separate 2014 MU69\u2019s main body from its companion, assuming it exists, according to Buie.<\/p>\n

Officials want to know whether any smaller moons surround the object to ensure New Horizons does not collide with any debris during its high-speed encounter.<\/p>\n

Scientists have established a preferred flyby trajectory that will take New Horizons around 2,175 miles (3,500 kilometers) from 2014 MU69, but managers could decide as late as mid-December to re-target an aim point more than 6,000 miles (10,000 kilometers) away if they find debris, sacrificing some scientific data and high-resolution imagery for safety.<\/p>\n

If New Horizons takes the preferred route, the spacecraft will produce sharper images of 2014 MU69 than it did at Pluto, thanks to a flyby distance less than one-third the range of New Horizons\u2019 visit to Pluto.<\/p>\n

\u201cIt\u2019s pretty hard to beat what New Horizons did during the Pluto flyby, but one way that the MU69 flyby will actually do better is with spatial resolution,\u201d said Hal Weaver, New Horizons\u2019 project scientist at the Johns Hopkins University Applied Physics Laboratory. \u201cFor those of us who are interested in studying the geology of the surface of MU69, and seeing what it really looks like instead of this pinpoint of light \u2026 spatial resolution is everything.\u201d<\/p>\n

The probe\u2019s other instruments will search for a coma, or gas cloud, surrounding 2014 MU69, and scan the object for water, ammonia, carbon monoxide and methane ices. Scientists also want to know what makes the miniature world so red and dark.<\/p>\n

It will take nearly two years for New Horizons to beam back all its data on 2014 MU69 back to Earth, transmitting through the vast black gulf of space at a glacial at 1 to 2 kilobits per second.<\/p>\n

But broad strokes will land sooner, beginning in late December and extending through the first few days of January 2019, when the first high-resolution views will arrive on Earth.<\/p>\n

\u201cSpend your Christmas in the Kuiper Belt,\u201d Stern said. \u201cIt\u2019s going to be exciting, and there\u2019s not going to be anything like it again. There\u2019s no planned further exploration of the Kuiper Belt.\u201d<\/p>\n

One journalist asked scientists if they expect to get a lump of coal for Christmas in 2018.<\/p>\n

\u201cMaybe two of three lumps of coal,\u201d Spencer joked.<\/p>\n

Email the author.<\/i><\/b><\/p>\n

Follow Stephen Clark on Twitter: @StephenClark1.<\/strong><\/em><\/p>\n","protected":false},"excerpt":{"rendered":"

Artist\u2019s concept of the New Horizons spacecraft\u2019s flyby of 2014 MU69. Credit: NASA\/Johns Hopkins University Applied Physics Laboratory\/Southwest Research Institute\/Steve Gribben The final days before NASA\u2019s New Horizons probe barrels in on its next destination on Jan. 1, 2019, should prove eventful, with scientists trying to sort out whether a distant mini-world detected by the […]<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"_acf_changed":false,"inline_featured_image":false,"footnotes":"","_links_to":"","_links_to_target":""},"categories":[2],"tags":[2337,3077,1861,2173,2174,1561,2612],"class_list":["post-14089","post","type-post","status-publish","format-standard","hentry","category-news","tag-2014-mu69","tag-agu-2017","tag-jhuapl","tag-kuiper-belt","tag-new-horizons","tag-planetary-science","tag-swri"],"acf":[],"_links":{"self":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/posts\/14089"}],"collection":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/comments?post=14089"}],"version-history":[{"count":0,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/posts\/14089\/revisions"}],"wp:attachment":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/media?parent=14089"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/categories?post=14089"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/tags?post=14089"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}