{"id":15753,"date":"2016-01-29T19:01:43","date_gmt":"2016-01-29T11:01:43","guid":{"rendered":"https:\/\/wp-productionenv-bjg9h2g2bgg5b8aa.southeastasia-01.azurewebsites.net\/news\/water-ice-abounds-in-plutos-frigid-bedrock\/"},"modified":"2016-01-29T19:01:43","modified_gmt":"2016-01-29T11:01:43","slug":"water-ice-abounds-in-plutos-frigid-bedrock","status":"publish","type":"post","link":"https:\/\/starpath.global\/news\/water-ice-abounds-in-plutos-frigid-bedrock\/","title":{"rendered":"Water ice abounds in Pluto\u2019s frigid bedrock"},"content":{"rendered":"
\"This
This false-color image, derived from observations in infrared light by the Ralph\/Linear Etalon Imaging Spectral Array (LEISA) instrument, shows where the spectral features of water ice are abundant on Pluto\u2019s surface. It is based on two LEISA scans of Pluto obtained on July 14, 2015, from a range of about 67,000 miles (108,000 kilometers). The map on the right incorporates a more sensitive model accounting for the contributions of Pluto\u2019s various ices all together, revealing more water ice deposits. Credit: NASA\/Johns Hopkins University Applied Physics Laboratory\/Southwest Research Institute<\/figcaption><\/figure>\n

New maps produced from data gathered during the New Horizons spacecraft\u2019s flyby of Pluto last year reveal surprisingly widespread water ice shaping mountains capped by methane snow and forming an underlying bedrock that blankets the distant world.<\/p>\n

The latest results indicate Pluto has more water ice than previously thought, scientists said.<\/p>\n

\u201cEverywhere we look, from mountains to tectonics to the impact features, it\u2019s pretty clear that the water ice crust is near the surface of Pluto,\u201d said Alan Stern, the New Horizons mission\u2019s principal investigator at the Southwest Research Institute in Boulder, Colorado.<\/p>\n

The New Horizons team analyzed data collected by an infrared spectral imager within the probe\u2019s Ralph instrument, which measures the composition of Pluto based on light reflected off its surface.<\/p>\n

A first look at the spectral data showed muted deposits of water ice. The initial analysis compared the sensor\u2019s raw measurements with the reference spectrum of pure water ice, and scientists said that technique was susceptible to masking by reflections from other ices \u2014 such as nitrogen, methane and carbon monoxide \u2014 hiding the water ice underneath.<\/p>\n

Scientists devised a new model to analyze the data incorporating all of Pluto\u2019s various ices, producing a more sensitive map, officials wrote on the New Horizons mission\u2019s website.<\/p>\n

It turns out water ice is more prevalent on Pluto than expected, but it is still absent from large regions such as the vast plains informally named Sputnik Planum on the western lobe of the dwarf planet\u2019s famous heart-shaped feature.<\/p>\n

Sputnik Planum likely formed when another object slammed into Pluto billions of years ago, carving a basin that filled with nitrogen ice. Images of Sputnik Planum showed apparent glacial flows descending from an adjacent mountain range, and cellular patterns that scientists think are caused by convection from a heat source deep inside Pluto.<\/p>\n

The geologic activity came as a surprise to many on New Horizons\u2019 science team. Pluto lurks more than 30 times farther from the sun than Earth, it is smaller than the moon, and it is not tidally locked to a large nearby planet, leaving little energy to drive its and climate and geologic movements.<\/p>\n

Like Sputnik Planum, another expanse near Pluto\u2019s north pole, informally called Lowell Regio, also has a weak water ice signature.<\/p>\n

\"This
This image of the boundary of Sputnik Planum and neighboring mountains is seen in exaggerated color to distinguish compositional differences. Credit: NASA\/Johns Hopkins University Applied Physics Laboratory\/Southwest Research Institute<\/figcaption><\/figure>\n

\u201cThis indicates that at least in these regions, Pluto\u2019s icy bedrock is well hidden beneath a thick blanket of other ices such as methane, nitrogen and carbon monoxide,\u201d scientists wrote on the New Horizons website.<\/p>\n

Stern told scientists Wednesday in a meeting of NASA\u2019s Small Bodies Assessment Group that the New Horizons team assumed towering mountain ranges discovered during the July 14 flyby were made of water ice, which behaves much like rock at Pluto\u2019s frigid temperatures near minus 390 degrees Fahrenheit (minus 235 degrees Celsius).<\/p>\n

\u201cWater ice has a lower density than nitrogen ice, and many of these mountain ranges actually appear to be completely chaotic in terms of their structure,\u201d Stern said. \u201cSo it appears that there are lot of water ice cubes measuring (many) kilometers across floating in an ocean of frozen nitrogen.\u201d<\/p>\n

Before New Horizons zipped by Pluto last year, telescopic observations from Earth showed the faraway world to be rich in nitrogen. But nitrogen is not strong enough to form mountains like the peaks discovered on Pluto.<\/p>\n

\u201cNitrogen can\u2019t support steep topography because it\u2019s a very weak material, and it slumps under its own weight, even in Pluto\u2019s low gravity,\u201d Stern said Wednesday.<\/p>\n

The rugged landscapes of water ice found on Pluto are covered in a thin veneer of other frozen materials that hid the water\u2019s presence from ground-based observatories, and even the Hubble Space Telescope, Stern said.<\/p>\n

Despite the lack of a water ice detection from Earth, many scientists still predicted the material would be found on Pluto. But the new maps show much more water ice than known before.<\/p>\n

\u201cIt really makes you wonder, when we\u2019re doing studies of other small Kuiper Belt planets, or other objects in the deep outer solar system, what we really know about them,\u201d Stern said. \u201cWater ice is very widespread on Pluto, and there\u2019s no hint of it in any ground-based data set, from any telescope, by any author, anywhere in the literature, but it\u2019s there.\u201d<\/p>\n

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

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

This false-color image, derived from observations in infrared light by the Ralph\/Linear Etalon Imaging Spectral Array (LEISA) instrument, shows where the spectral features of water ice are abundant on Pluto\u2019s surface. It is based on two LEISA scans of Pluto obtained on July 14, 2015, from a range of about 67,000 miles (108,000 kilometers). 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":[2173,2174,1561,2848],"class_list":["post-15753","post","type-post","status-publish","format-standard","hentry","category-news","tag-kuiper-belt","tag-new-horizons","tag-planetary-science","tag-pluto"],"acf":[],"_links":{"self":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/posts\/15753"}],"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=15753"}],"version-history":[{"count":0,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/posts\/15753\/revisions"}],"wp:attachment":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/media?parent=15753"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/categories?post=15753"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/tags?post=15753"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}