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Three months after flyby, New Horizons team publishes first research paper

Diversity of Pluto's landforms, atmosphere, and moons highlight the first three months of New Horizons data returns

Date:
October 15, 2015
Source:
Southwest Research Institute
Summary:
The New Horizons team described a wide range of findings about the Pluto system in its first research paper, just published. 'The Pluto System: Initial Results from its Exploration by New Horizons' appears in and on the cover of the Oct. 16 issue of the journal Science; the publication comes just three months after NASA's historic first exploration of the Pluto system in mid-July.
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This high-resolution image captured by NASA's New Horizons spacecraft combines blue, red and infrared images taken by the Ralph/Multispectral Visual Imaging Camera (MVIC). Pluto's surface shows a remarkable range of subtle colors, digitally enhanced in this view to a rainbow of pale blues, yellows, oranges, and deep reds. The bright expanse is the western lobe of the "heart," informally known as Tombaugh Regio. The lobe, informally called Sputnik Planum, has been found to be rich in nitrogen, carbon monoxide, and methane ices. Pluto's diameter is 1,473 miles (2,372 kilometers).
Credit: Image Courtesy of NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute

The New Horizons team described a wide range of findings about the Pluto system in its first research paper, published today. "The Pluto System: Initial Results from its Exploration by New Horizons" appears in and on the cover of the Oct. 16 issue of the journal Science; the publication comes just three months after NASA's historic first exploration of the Pluto system in mid-July.

The authors include more than 150 New Horizons project and NASA personnel; Principal Investigator Alan Stern of Southwest Research Institute (SwRI) is first author.

From the variety in Pluto's geological landforms, to Pluto's atmosphere, to its intriguing moons, New Horizons has revealed a degree of diversity and complexity on Pluto and its moons that few expected in the frigid outer reaches of the solar system.

"The New Horizons mission completes our initial reconnaissance of the solar system, giving humanity our first look at this fascinating world and its system of moons," said Jim Green, director of planetary science at NASA Headquarters in Washington. "New Horizons is not only writing the textbook on the Pluto system, it's serving to inspire current and future generations to keep exploring -- to keep searching for what's beyond the next hill."

NASA's New Horizons spacecraft reached a distance of 8,507 miles (13,691 kilometers) from Pluto's surface during its July 14 closest approach, gathering a treasure trove of data that will take almost another year to return to Earth. The data returned so far show a surprisingly wide variety of landforms and terrain ages on Pluto, as well as variations in color, composition, and albedo (surface reflectivity). Team members also discovered evidence for a water-ice rich crust and multiple haze layers in Pluto's atmosphere, and found that Pluto is both larger and more ice rich than expected prior to the flyby.

"The Pluto system surprised us in many ways, most notably teaching us that small planets can remain active billions of years after their formation," said Stern. "We were also taught important lessons by the unexpected degree of geological complexity that both Pluto and its large moon Charon display."

Observations of Pluto's moons show Charon has extensive resurfacing, extensional tectonics, and a puzzling dark terrain at its North Pole. Evidence also points to variations in the composition of its crust.

Although no new satellites were detected, New Horizons provided the first resolved images of Pluto's smaller moons Nix and Hydra, finding Nix is approximately 34 miles (54 kilometers) long and Hydra is 27 miles (43 kilometers) long. Puzzlingly, their surface reflectivities are significantly higher than Charon's.

The spacecraft's science payload collected more than 50 gigabits of data from the Pluto system leading up to and at closest approach. Data were gathered by the suite of science instruments aboard New Horizons, including the Ralph infrared spectrometer/imager, the Long-Range Reconnaissance Imager (LORRI), the Alice ultraviolet spectrograph, twin REX radio science experiments, the Solar Wind Around Pluto (SWAP) detector, the PEPSSI charged-particle spectrometer, and a student-built and operated dust detector.


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Journal Reference:

  1. S. A. Stern, F. Bagenal, K. Ennico, G. R. Gladstone, W. M. Grundy, W. B. McKinnon, J. M. Moore, C. B. Olkin, J. R. Spencer, H. A. Weaver, L. A. Young, T. Andert, J. Andrews, M. Banks, B. Bauer, J. Bauman, O. S. Barnouin, P. Bedini, K. Beisser, R. A. Beyer, S. Bhaskaran, R. P. Binzel, E. Birath, M. Bird, D. J. Bogan, A. Bowman, V. J. Bray, M. Brozovic, C. Bryan, M. R. Buckley, M. W. Buie, B. J. Buratti, S. S. Bushman, A. Calloway, B. Carcich, A. F. Cheng, S. Conard, C. A. Conrad, J. C. Cook, D. P. Cruikshank, O. S. Custodio, C. M. Dalle Ore, C. Deboy, Z. J. B. Dischner, P. Dumont, A. M. Earle, H. A. Elliott, J. Ercol, C. M. Ernst, T. Finley, S. H. Flanigan, G. Fountain, M. J. Freeze, T. Greathouse, J. L. Green, Y. Guo, M. Hahn, D. P. Hamilton, S. A. Hamilton, J. Hanley, A. Harch, H. M. Hart, C. B. Hersman, A. Hill, M. E. Hill, D. P. Hinson, M. E. Holdridge, M. Horanyi, A. D. Howard, C. J. A. Howett, C. Jackman, R. A. Jacobson, D. E. Jennings, J. A. Kammer, H. K. Kang, D. E. Kaufmann, P. Kollmann, S. M. Krimigis, D. Kusnierkiewicz, T. R. Lauer, J. E. Lee, K. L. Lindstrom, I. R. Linscott, C. M. Lisse, A. W. Lunsford, V. A. Mallder, N. Martin, D. J. McComas, R. L. McNutt, D. Mehoke, T. Mehoke, E. D. Melin, M. Mutchler, D. Nelson, F. Nimmo, J. I. Nunez, A. Ocampo, W. M. Owen, M. Paetzold, B. Page, A. H. Parker, J. W. Parker, F. Pelletier, J. Peterson, N. Pinkine, M. Piquette, S. B. Porter, S. Protopapa, J. Redfern, H. J. Reitsema, D. C. Reuter, J. H. Roberts, S. J. Robbins, G. Rogers, D. Rose, K. Runyon, K. D. Retherford, M. G. Ryschkewitsch, P. Schenk, E. Schindhelm, B. Sepan, M. R. Showalter, K. N. Singer, M. Soluri, D. Stanbridge, A. J. Steffl, D. F. Strobel, T. Stryk, M. E. Summers, J. R. Szalay, M. Tapley, A. Taylor, H. Taylor, H. B. Throop, C. C. C. Tsang, G. L. Tyler, O. M. Umurhan, A. J. Verbiscer, M. H. Versteeg, M. Vincent, R. Webbert, S. Weidner, G. E. Weigle, O. L. White, K. Whittenburg, B. G. Williams, K. Williams, S. Williams, W. W. Woods, A. M. Zangari, E. Zirnstein. The Pluto system: Initial results from its exploration by New Horizons. Science, 2015; 350 (6258): aad1815 DOI: 10.1126/science.aad1815

Cite This Page:

Southwest Research Institute. "Three months after flyby, New Horizons team publishes first research paper: Diversity of Pluto's landforms, atmosphere, and moons highlight the first three months of New Horizons data returns." ScienceDaily. ScienceDaily, 15 October 2015. <www.sciencedaily.com/releases/2015/10/151015144810.htm>.
Southwest Research Institute. (2015, October 15). Three months after flyby, New Horizons team publishes first research paper: Diversity of Pluto's landforms, atmosphere, and moons highlight the first three months of New Horizons data returns. ScienceDaily. Retrieved May 23, 2017 from www.sciencedaily.com/releases/2015/10/151015144810.htm
Southwest Research Institute. "Three months after flyby, New Horizons team publishes first research paper: Diversity of Pluto's landforms, atmosphere, and moons highlight the first three months of New Horizons data returns." ScienceDaily. www.sciencedaily.com/releases/2015/10/151015144810.htm (accessed May 23, 2017).

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