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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…

Earth and Planetary Astrophysics · Physics 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

The New Horizons flyby of the cold classical Kuiper Belt object MU69 showed it to be a contact binary. The existence of other contact binaries in the 1-10km range raises the question of how common these bodies are and how they evolved into…

Earth and Planetary Astrophysics · Physics 2020-11-30 Wladimir Lyra , Andrew N. Youdin , Anders Johansen

The New Horizons spacecraft's encounter with the cold classical Kuiper belt object (486958) Arrokoth (formerly 2014 MU69) revealed a contact-binary planetesimal. We investigate how it formed, finding it is the product of a gentle, low-speed…

We report HST lightcurve observations of the New Horizons (NH) spacecraft encounter KBO (486958) 2014 MU69 acquired near opposition in July 2017. In order to plan the optimum flyby sequence the NH mission planners needed to learn as much as…

Earth and Planetary Astrophysics · Physics 2020-02-12 S. D. Benecchi , S. Porter , M. W. Buie , A. M. Zangari , A. J. Verbiscer , K. S. Noll , S. A. Stern , J. R. Spencer , A. Parker

The Cold Classical Kuiper Belt, a class of small bodies in undisturbed orbits beyond Neptune, are primitive objects preserving information about Solar System formation. The New Horizons spacecraft flew past one of these objects, the 36 km…

The New Horizons mission has returned stunning images of the bilobate Kuiper belt object (486958) Arrokoth. It is a contact binary, formed from two intact and relatively undisturbed predecessor objects joined by a narrow contact region. We…

The discovery that many trans-neptunian objects exist in pairs, or binaries, is proving invaluable for shedding light on the formation, evolution and structure of the outer Solar system. Based on recent systematic searches it has been…

Astrophysics · Physics 2007-05-23 Sergey A. Astakhov , Ernestine A. Lee , David Farrelly

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 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…

Using the New Horizons LORRI camera, we searched for satellites near five Kuiper belt objects (KBOs): four cold classicals (CCs: 2011 JY31, 2014 OS393, 2014 PN70, 2011 HZ102) and one scattered disk object (SD: 2011 HK103). These objects…

Earth and Planetary Astrophysics · Physics 2022-01-19 H. A. Weaver , S. B. Porter , J. R. Spencer , The New Horizons Science Team

It appears that at least several percent of large Kuiper belt objects are members of wide binaries. Physical collisions are too infrequent to account for their formation. Collisionless gravitational interactions are more promising. These…

Astrophysics · Physics 2009-11-07 Peter Goldreich , Yoram Lithwick , Re'em Sari

In preparation for the Jan 1/2019 encounter between the New Horizons spacecraft and the Kuiper Belt object 2014 MU69, we provide estimates of the expected impact crater surface density on the Kuiper Belt object. Using the observed crater…

Earth and Planetary Astrophysics · Physics 2019-02-13 Sarah Greenstreet , Brett Gladman , William McKinnon , JJ Kavelaars , Kelsi Singer

A large fraction of 100-km-class low-inclination objects in the classical Kuiper Belt (KB) are binaries with comparable mass and wide separation of components. A favored model for their formation was capture during the coagulation growth of…

Earth and Planetary Astrophysics · Physics 2015-05-19 David Nesvorny , Andrew N. Youdin , Derek C. Richardson

The Pluto-Charon binary system is the best-studied representative of the binary Kuiper-belt population. Its origins are vital to understanding the formation of other Kupier-belt objects (KBO) and binaries, and the evolution of the outer…

Earth and Planetary Astrophysics · Physics 2020-09-02 Mor Rozner , Evgeni Grishin , Hagai B. Perets

Recent observations have revealed an unexpectedly high binary fraction among the Trans-Neptunian Objects (TNOs) that populate the Kuiper-belt. The discovered binaries have four characteristics they comprise a few percent of the TNOs, the…

Astrophysics · Physics 2015-06-24 Yoko Funato , Junichiro Makino , Piet Hut , Eiichiro Kokubo , Daisuke Kinoshita

Observations of the Kuiper Belt indicate that a larger than expected percentage of KBO's (approximately 8 out of 500) are in binary pairs. The formation and survival of such objects presents a conundrum [1]. Two competing theories have been…

Space Physics · Physics 2007-05-23 R. C. Nazzario , T. W. Hyde

Here we present an updated shape model of (486958) Arrokoth, the bilobate Kuiper Belt Object (KBO) which the NASA New Horizons spacecraft flew past in 2019. This updated shape model uses all of the resolved images of Arrokoth obtained by…

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…

The non-resonant Kuiper belt objects (KBOs) between the 3:2 and 2:1 Neptunian mean motion resonances can be largely divided between a cold classical belt (CCB) and a hot classical belt (HCB). A notable difference between these two…

Earth and Planetary Astrophysics · Physics 2021-07-07 Lukas R Stone , Nathan A Kaib

Given the large orbital separation and high satellite-to-primary mass ratio of all known Kuiper Belt Object (KBO) binaries, it is important to reassess their stability as bound pairs with respect to several disruptive mechanisms. Besides…

Astrophysics · Physics 2007-05-23 Jean-Marc Petit , Olivier Mousis
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