The pluto system: Initial results from its exploration by New Horizons

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

doi:10.1126/science.aad1815

The pluto system: Initial results from its exploration by New Horizons

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. BeyerS. 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

Research output: Contribution to journal › Article › peer-review

371 Scopus citations

Abstract

The Pluto system was recently explored by NASA's New Horizons spacecraft, making closest approach on 14 July 2015. Pluto's surface displays diverse landforms, terrain ages, albedos, colors, and composition gradients. Evidence is found for a water-ice crust, geologically young surface units, surface ice convection, wind streaks, volatile transport, and glacial flow. Pluto's atmosphere is highly extended, with trace hydrocarbons, a global haze layer, and a surface pressure near 10 microbars. Pluto's diverse surface geology and long-term activity raise fundamental questions about how small planets remain active many billions of years after formation. Pluto's large moon Charon displays tectonics and evidence for a heterogeneous crustal composition; its north pole displays puzzling dark terrain. Small satellites Hydra and Nix have higher albedos than expected.

Original language	English (US)
Article number	aad1815
Journal	Science
Volume	350
Issue number	6258
DOIs	https://doi.org/10.1126/science.aad1815
State	Published - Oct 16 2015
Externally published	Yes

All Science Journal Classification (ASJC) codes

General

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10.1126/science.aad1815

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Stern, S. A., Bagenal, F., Ennico, K., Gladstone, G. R., Grundy, W. M., McKinnon, W. B., Moore, J. M., Olkin, C. B., Spencer, J. R., Weaver, H. A., Young, L. A., Andert, T., Andrews, J., Banks, M., Bauer, B., Bauman, J., Barnouin, O. S., Bedini, P., Beisser, K., ... Zirnstein, E. (2015). The pluto system: Initial results from its exploration by New Horizons. Science, 350(6258), Article aad1815. https://doi.org/10.1126/science.aad1815

@article{8f181a7fa794465f8a3b5e34f244f822,

title = "The pluto system: Initial results from its exploration by New Horizons",

abstract = "The Pluto system was recently explored by NASA's New Horizons spacecraft, making closest approach on 14 July 2015. Pluto's surface displays diverse landforms, terrain ages, albedos, colors, and composition gradients. Evidence is found for a water-ice crust, geologically young surface units, surface ice convection, wind streaks, volatile transport, and glacial flow. Pluto's atmosphere is highly extended, with trace hydrocarbons, a global haze layer, and a surface pressure near 10 microbars. Pluto's diverse surface geology and long-term activity raise fundamental questions about how small planets remain active many billions of years after formation. Pluto's large moon Charon displays tectonics and evidence for a heterogeneous crustal composition; its north pole displays puzzling dark terrain. Small satellites Hydra and Nix have higher albedos than expected.",

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

year = "2015",

month = oct,

day = "16",

doi = "10.1126/science.aad1815",

language = "English (US)",

volume = "350",

journal = "Science",

issn = "0036-8075",

publisher = "American Association for the Advancement of Science",

number = "6258",

}

Stern, SA, Bagenal, F, Ennico, K, Gladstone, GR, Grundy, WM, McKinnon, WB, Moore, JM, Olkin, CB, Spencer, JR, Weaver, HA, Young, LA, Andert, T, Andrews, J, Banks, M, Bauer, B, Bauman, J, Barnouin, OS, Bedini, P, Beisser, K, Beyer, RA, Bhaskaran, S, Binzel, RP, Birath, E, Bird, M, Bogan, DJ, Bowman, A, Bray, VJ, Brozovic, M, Bryan, C, Buckley, MR, Buie, MW, Buratti, BJ, Bushman, SS, Calloway, A, Carcich, B, Cheng, AF, Conard, S, Conrad, CA, Cook, JC, Cruikshank, DP, Custodio, OS, Dalle Ore, CM, Deboy, C, Dischner, ZJB, Dumont, P, Earle, AM, Elliott, HA, Ercol, J, Ernst, CM, Finley, T, Flanigan, SH, Fountain, G, Freeze, MJ, Greathouse, T, Green, JL, Guo, Y, Hahn, M, Hamilton, DP, Hamilton, SA, Hanley, J, Harch, A, Hart, HM, Hersman, CB, Hill, A, Hill, ME, Hinson, DP, Holdridge, ME, Horanyi, M, Howard, AD, Howett, CJA, Jackman, C, Jacobson, RA, Jennings, DE, Kammer, JA, Kang, HK, Kaufmann, DE, Kollmann, P, Krimigis, SM, Kusnierkiewicz, D, Lauer, TR, Lee, JE, Lindstrom, KL, Linscott, IR, Lisse, CM, Lunsford, AW, Mallder, VA, Martin, N, McComas, DJ, McNutt, RL, Mehoke, D, Mehoke, T, Melin, ED, Mutchler, M, Nelson, D, Nimmo, F, Nunez, JI, Ocampo, A, Owen, WM, Paetzold, M, Page, B, Parker, AH, Parker, JW, Pelletier, F, Peterson, J, Pinkine, N, Piquette, M, Porter, SB, Protopapa, S, Redfern, J, Reitsema, HJ, Reuter, DC, Roberts, JH, Robbins, SJ, Rogers, G, Rose, D, Runyon, K, Retherford, KD, Ryschkewitsch, MG, Schenk, P, Schindhelm, E, Sepan, B, Showalter, MR, Singer, KN, Soluri, M, Stanbridge, D, Steffl, AJ, Strobel, DF, Stryk, T, Summers, ME, Szalay, JR, Tapley, M, Taylor, A, Taylor, H, Throop, HB, Tsang, CCC, Tyler, GL, Umurhan, OM, Verbiscer, AJ, Versteeg, MH, Vincent, M, Webbert, R, Weidner, S, Weigle, GE, White, OL, Whittenburg, K, Williams, BG, Williams, K, Williams, S, Woods, WW, Zangari, AM & Zirnstein, E 2015, 'The pluto system: Initial results from its exploration by New Horizons', Science, vol. 350, no. 6258, aad1815. https://doi.org/10.1126/science.aad1815

TY - JOUR

T1 - The pluto system

T2 - Initial results from its exploration by New Horizons

AU - Stern, S. A.

AU - Bagenal, F.

AU - Ennico, K.

AU - Gladstone, G. R.

AU - Grundy, W. M.

AU - McKinnon, W. B.

AU - Moore, J. M.

AU - Olkin, C. B.

AU - Spencer, J. R.

AU - Weaver, H. A.

AU - Young, L. A.

AU - Andert, T.

AU - Andrews, J.

AU - Banks, M.

AU - Bauer, B.

AU - Bauman, J.

AU - Barnouin, O. S.

AU - Bedini, P.

AU - Beisser, K.

AU - Beyer, R. A.

AU - Bhaskaran, S.

AU - Binzel, R. P.

AU - Birath, E.

AU - Bird, M.

AU - Bogan, D. J.

AU - Bowman, A.

AU - Bray, V. J.

AU - Brozovic, M.

AU - Bryan, C.

AU - Buckley, M. R.

AU - Buie, M. W.

AU - Buratti, B. J.

AU - Bushman, S. S.

AU - Calloway, A.

AU - Carcich, B.

AU - Cheng, A. F.

AU - Conard, S.

AU - Conrad, C. A.

AU - Cook, J. C.

AU - Cruikshank, D. P.

AU - Custodio, O. S.

AU - Dalle Ore, C. M.

AU - Deboy, C.

AU - Dischner, Z. J.B.

AU - Dumont, P.

AU - Earle, A. M.

AU - Elliott, H. A.

AU - Ercol, J.

AU - Ernst, C. M.

AU - Finley, T.

AU - Flanigan, S. H.

AU - Fountain, G.

AU - Freeze, M. J.

AU - Greathouse, T.

AU - Green, J. L.

AU - Guo, Y.

AU - Hahn, M.

AU - Hamilton, D. P.

AU - Hamilton, S. A.

AU - Hanley, J.

AU - Harch, A.

AU - Hart, H. M.

AU - Hersman, C. B.

AU - Hill, A.

AU - Hill, M. E.

AU - Hinson, D. P.

AU - Holdridge, M. E.

AU - Horanyi, M.

AU - Howard, A. D.

AU - Howett, C. J.A.

AU - Jackman, C.

AU - Jacobson, R. A.

AU - Jennings, D. E.

AU - Kammer, J. A.

AU - Kang, H. K.

AU - Kaufmann, D. E.

AU - Kollmann, P.

AU - Krimigis, S. M.

AU - Kusnierkiewicz, D.

AU - Lauer, T. R.

AU - Lee, J. E.

AU - Lindstrom, K. L.

AU - Linscott, I. R.

AU - Lisse, C. M.

AU - Lunsford, A. W.

AU - Mallder, V. A.

AU - Martin, N.

AU - McComas, D. J.

AU - McNutt, R. L.

AU - Mehoke, D.

AU - Mehoke, T.

AU - Melin, E. D.

AU - Mutchler, M.

AU - Nelson, D.

AU - Nimmo, F.

AU - Nunez, J. I.

AU - Ocampo, A.

AU - Owen, W. M.

AU - Paetzold, M.

AU - Page, B.

AU - Parker, A. H.

AU - Parker, J. W.

AU - Pelletier, F.

AU - Peterson, J.

AU - Pinkine, N.

AU - Piquette, M.

AU - Porter, S. B.

AU - Protopapa, S.

AU - Redfern, J.

AU - Reitsema, H. J.

AU - Reuter, D. C.

AU - Roberts, J. H.

AU - Robbins, S. J.

AU - Rogers, G.

AU - Rose, D.

AU - Runyon, K.

AU - Retherford, K. D.

AU - Ryschkewitsch, M. G.

AU - Schenk, P.

AU - Schindhelm, E.

AU - Sepan, B.

AU - Showalter, M. R.

AU - Singer, K. N.

AU - Soluri, M.

AU - Stanbridge, D.

AU - Steffl, A. J.

AU - Strobel, D. F.

AU - Stryk, T.

AU - Summers, M. E.

AU - Szalay, J. R.

AU - Tapley, M.

AU - Taylor, A.

AU - Taylor, H.

AU - Throop, H. B.

AU - Tsang, C. C.C.

AU - Tyler, G. L.

AU - Umurhan, O. M.

AU - Verbiscer, A. J.

AU - Versteeg, M. H.

AU - Vincent, M.

AU - Webbert, R.

AU - Weidner, S.

AU - Weigle, G. E.

AU - White, O. L.

AU - Whittenburg, K.

AU - Williams, B. G.

AU - Williams, K.

AU - Williams, S.

AU - Woods, W. W.

AU - Zangari, A. M.

AU - Zirnstein, E.

PY - 2015/10/16

Y1 - 2015/10/16

N2 - The Pluto system was recently explored by NASA's New Horizons spacecraft, making closest approach on 14 July 2015. Pluto's surface displays diverse landforms, terrain ages, albedos, colors, and composition gradients. Evidence is found for a water-ice crust, geologically young surface units, surface ice convection, wind streaks, volatile transport, and glacial flow. Pluto's atmosphere is highly extended, with trace hydrocarbons, a global haze layer, and a surface pressure near 10 microbars. Pluto's diverse surface geology and long-term activity raise fundamental questions about how small planets remain active many billions of years after formation. Pluto's large moon Charon displays tectonics and evidence for a heterogeneous crustal composition; its north pole displays puzzling dark terrain. Small satellites Hydra and Nix have higher albedos than expected.

AB - The Pluto system was recently explored by NASA's New Horizons spacecraft, making closest approach on 14 July 2015. Pluto's surface displays diverse landforms, terrain ages, albedos, colors, and composition gradients. Evidence is found for a water-ice crust, geologically young surface units, surface ice convection, wind streaks, volatile transport, and glacial flow. Pluto's atmosphere is highly extended, with trace hydrocarbons, a global haze layer, and a surface pressure near 10 microbars. Pluto's diverse surface geology and long-term activity raise fundamental questions about how small planets remain active many billions of years after formation. Pluto's large moon Charon displays tectonics and evidence for a heterogeneous crustal composition; its north pole displays puzzling dark terrain. Small satellites Hydra and Nix have higher albedos than expected.

UR - http://www.scopus.com/inward/record.url?scp=84944463363&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84944463363&partnerID=8YFLogxK

U2 - 10.1126/science.aad1815

DO - 10.1126/science.aad1815

M3 - Article

C2 - 26472913

AN - SCOPUS:84944463363

SN - 0036-8075

VL - 350

JO - Science

JF - Science

IS - 6258

M1 - aad1815

ER -

The pluto system: Initial results from its exploration by New Horizons

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