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The flyby of Pluto and Charon by the New Horizons spacecraft provided high-resolution images of cratered surfaces embedded in the Kuiper belt, an extensive region of bodies orbiting beyond Neptune. Impact craters on Pluto and Charon were…

The Kuiper Belt is a distant region of the Solar System. On 1 January 2019, the New Horizons spacecraft flew close to (486958) 2014 MU69, a Cold Classical Kuiper Belt Object, a class of objects that have never been heated by the Sun and are…

地球与行星天体物理 · 物理学 2020-04-03 S. A. Stern , H. A. Weaver , J. R. Spencer , C. B. Olkin , G. R. Gladstone , W. M. Grundy , J. M. Moore , D. P. Cruikshank , H. A. Elliott , W. B. McKinnon , J. Wm. Parker , A. J. Verbiscer , L. A. Young , D. A. Aguilar , J. M. Albers , T. Andert , J. P. Andrews , F. Bagenal , M. E. Banks , B. A. Bauer , J. A. Bauman , K. E. Bechtold , C. B. Beddingfield , N. Behrooz , K. B. Beisser , S. D. Benecchi , E. Bernardoni , R. A. Beyer , S. Bhaskaran , C. J. Bierson , R. P. Binzel , E. M. Birath , M. K. Bird , D. R. Boone , A. F. Bowman , V. J. Bray , D. T. Britt , L. E. Brown , M. R. Buckley , M. W. Buie , B. J. Buratti , L. M. Burke , S. S. Bushman , B. Carcich , A. L. Chaikin , C. L. Chavez , A. F. Cheng , E. J. Colwell , S. J. Conard , M. P. Conner , C. A. Conrad , J. C. Cook , S. B. Cooper , O. S. Custodio , C. M. Dalle Ore , C. C. Deboy , P. Dharmavaram , R. D. Dhingra , G. F. Dunn , A. M. Earle , A. F. Egan , J. Eisig , M. R. El-Maarry , C. Engelbrecht , B. L. Enke , C. J. Ercol , E. D. Fattig , C. L. Ferrell , T. J. Finley , J. Firer , J. Fischetti , W. M. Folkner , M. N. Fosbury , G. H. Fountain , J. M. Freeze , L. Gabasova , L. S. Glaze , J. L. Green , G. A. Griffith , Y. Guo , M. Hahn , D. W. Hals , D. P. Hamilton , S. A. Hamilton , J. J. Hanley , A. Harch , K. A. Harmon , H. M. Hart , J. Hayes , C. B. Hersman , M. E. Hill , T. A. Hill , J. D. Hofgartner , M. E. Holdridge , M. Horányi , A. Hosadurga , A. D. Howard , C. J. A. Howett , S. E. Jaskulek , D. E. Jennings , J. R. Jensen , M. R. Jones , H. K. Kang , D. J. Katz , D. E. Kaufmann , J. J. Kavelaars , J. T. Keane , G. P. Keleher , M. Kinczyk , M. C. Kochte , P. Kollmann , S. M. Krimigis , G. L. Kruizinga , D. Y. Kusnierkiewicz , M. S. Lahr , T. R. Lauer , G. B. Lawrence , J. E. Lee , E. J. Lessac-Chenen , I. R. Linscott , C. M. Lisse , A. W. Lunsford , D. M. Mages , V. A. Mallder , N. P. Martin , B. H. May , D. J. McComas , R. L. McNutt , Jr. D. S. Mehoke , T. S. Mehoke , D. S. Nelson , H. D. Nguyen , J. I. Núñez , A. C. Ocampo , W. M. Owen , G. K. Oxton , A. H. Parker , M. Pätzold , J. Y. Pelgrift , F. J. Pelletier , J. P. Pineau , M. R. Piquette , S. B. Porter , S. Protopapa , E. Quirico , J. A. Redfern , A. L. Regiec , H. J. Reitsema , D. C. Reuter , D. C. Richardson , J. E. Riedel , M. A. Ritterbush , S. J. Robbins , D. J. Rodgers , G. D. Rogers , D. M. Rose , P. E. Rosendall , K. D. Runyon , M. G. Ryschkewitsch , M. M. Saina , M. J. Salinas , P. M. Schenk , J. R. Scherrer , W. R. Schlei , B. Schmitt , D. J. Schultz , D. C. Schurr , F. Scipioni , R. L. Sepan , R. G. Shelton , M. R. Showalter , M. Simon , K. N. Singer , E. W. Stahlheber , D. R. Stanbridge , J. A. Stansberry , A. J. Steffl , D. F. Strobel , M. M. Stothoff , T. Stryk , J. R. Stuart , M. E. Summers , M. B. Tapley , A. Taylor , H. W. Taylor , R. M. Tedford , H. B. Throop , L. S. Turner , O. M. Umurhan , J. Van Eck , D. Velez , M. H. Versteeg , M. A. Vincent , R. W. Webbert , S. E. Weidner , G. E. Weigle , J. R. Wendel , O. L. White , K. E. Whittenburg , B. G. Williams , K. E. Williams , S. P. Williams , H. L. Winters , A. M. Zangari , T. H. Zurbuchen

We extend previous results showing that the surfaces of Edgeworth-Kuiper Belt objects are not primordial and have been moderately to heavily reworked by collisions. Objects smaller than about $r = 2.5$ km have collisional disruption…

天体物理学 · 物理学 2009-10-31 Daniel D. Durda , S. Alan Stern

Pluto and its satellites will be the most distant objects ever reconnoitered when NASA's New Horizons spacecraft conducts its intensive flyby of this system in 2015. The size-frequency distribution (SFD) of craters on the surfaces in the…

地球与行星天体物理 · 物理学 2015-06-23 S. Alan Stern , Simon Porter , Amanda Zangari

NASA's New Horizons spacecraft will conduct a close flyby of the cold classical Kuiper Belt Object (KBO) designated (486958) 2014 MU69 on January 1, 2019. At a heliocentric distance of 44 AU, "MU69" will be the most distant object ever…

Following its flyby and first imaging the Pluto-Charon binary, the New Horizons spacecraft visited the Kuiper-Belt-Object (KBO) (486958) 2014 MU69 (Arrokoth). Imaging showed MU69 to be a contact-binary, made of two individual lobes…

地球与行星天体物理 · 物理学 2020-04-28 Evgeni Grishin , Uri Malamud , Hagai B. Perets , Oliver Wandel , Christoph M. Schaefer

Debris disks are thought to be sculptured by neighboring planets. The same is true for the Edgeworth-Kuiper debris disk, yet no direct observational evidence for signatures of giant planets in the Kuiper belt dust distribution has been…

地球与行星天体物理 · 物理学 2015-06-19 Christian Vitense , Alexander V. Krivov , Torsten Löhne

NASA's New Horizons (NH) Pluto-Kuiper belt (PKB) mission was launched on 19 January 2006 on a Jupiter Gravity Assist (JGA) trajectory toward the Pluto system for a 14 July 2015 closest approach; Jupiter closest approach occurred on 28…

天体物理学 · 物理学 2009-06-23 S. Alan Stern

We combine several constraints provided by the crater records on Arrokoth and the worlds of the Pluto system to compute the size-frequency distribution (SFD) of the crater production function for craters with diameter D<10km. For this…

地球与行星天体物理 · 物理学 2021-01-20 A. Morbidelli , D. Nesvorny , W. F. Bottke , S. Marchi

The New Horizons spacecraft's nominal trajectory crosses the planet's satellite plane at $\sim 10,000\ \rm{km}$ from the barycenter, between the orbits of Pluto and Charon. I have investigated the risk to the spacecraft based on…

地球与行星天体物理 · 物理学 2017-11-08 Henry B. Throop

Pluto's terrains display a diversity of crater retention ages ranging from areas with no identifiable craters to heavily cratered terrains. This variation in crater densities is consistent with geologic activity occurring throughout Pluto's…

地球与行星天体物理 · 物理学 2022-01-26 Kelsi N. Singer , Sarah Greenstreet , Paul M. Schenk , Stuart J. Robbins , Veronica J. Bray

The Hubble Space Telescope (HST) measured the colors of eight Kuiper Belt Objects (KBOs) that will be observed by the New Horizons spacecraft including its 2019 close fly-by target the Cold Classical KBO (486958) 2014 MU69. We find that the…

NASA's New Horizons spacecraft observed (15810) 1994 JR$_1$, a 3:2 resonant Kupier Belt Object (KBO), using the LOng Range Reconnaissance Imager (LORRI) on November 2, 2015 from a distance of 1.85 AU, and again on April 7, 2016 from a…

In this letter we explore the environment of Pluto and Charon in the far infrared with the main aim to identify the signs of any possible dust ring, should it exist in the system. Our study is based on observations performed at 70 um with…

地球与行星天体物理 · 物理学 2015-07-22 Gabor Marton , Csaba Kiss , Zoltan Balog , Emmanuel Lellouch , Erika Verebelyi , Ulrich Klaas

The central objective of the New Horizons prime mission was to make the first exploration of Pluto and its system of moons. Following that, New Horizons has been approved for its first extended mission, which has the objectives of…

地球与行星天体物理 · 物理学 2018-06-25 S. A. Stern , H. A. Weaver , J. R. Spencer , H. A. Elliott , the New Horizons Team

We propose a Roman Space Telescope survey to investigate fundamental properties of the distant solar system in the region of the Kuiper Belt where object characteristics and the size distribution are inaccessible from any other telescope.…

We investigated 634 crater clusters on Mars detected between 2007 and 2021, which represent more than half of all impacts discovered in this period. Crater clusters form when meteoroids in the 10 kg to 10 ton mass range break-up in Mars'…

地球与行星天体物理 · 物理学 2023-05-03 T. Neidhart , E. K. Sansom , K. Miljković , G. S. Collins , J. Eschenfelder , I. J. Daubar

Approach images taken by the LORRI imaging system during the New Horizons spacecraft encounter have been used to determine the mean radii and shapes of Pluto and Charon. The primary observations are limb locations derived using three…

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