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Related papers: The New Horizons Spacecraft

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The New Horizons mission was launched on 2006 January 19, and the spacecraft is heading for a flyby encounter with the Pluto system in the summer of 2015. The challenges associated with sending a spacecraft to Pluto in less than 10 years…

Astrophysics · Physics 2008-12-25 H. A. Weaver , W. C. Gibson , M. B. Tapley , L. A. Young , S. A. Stern

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…

Astrophysics · Physics 2009-06-23 S. Alan Stern

The New Horizons spacecraft, launched by NASA in 2006, will arrive in the Pluto-Charon system on July 14, 2015. There, it will spend a few hours imaging Pluto and its moons. It will then have a small amount of reserve propellant which will…

Instrumentation and Methods for Astrophysics · Physics 2014-11-14 Stephen D. J. Gwyn

The New Horizons spacecraft will achieve a wide range of measurement objectives at the Pluto system, including color and panchromatic maps, 1.25-2.50 micron spectral images for studying surface compositions, and measurements of Pluto's…

The space probe 'New Horizon' was launched on 19th of January 2006 in order to study Pluto and its moons. Spacecraft will fly by Pluto as close as 12500 km in the middle of July 2015 and will get the most detailed images of Pluto and its…

Earth and Planetary Astrophysics · Physics 2015-05-01 Alexander V. Devyatkin , Ekaterina A. Bashakova , Viacheslav Yu. Slesarenko

Next year, 2015, the New Horizons spacecraft will have a close encounter with Pluto. In the present study we discuss some possibilities regarding what the spacecraft may encounter during its approach to Pluto. Among them we should include:…

Earth and Planetary Astrophysics · Physics 2015-05-28 Hector Javier Durand-Manterola , Hector Perez-de-Tejada

The NASA New Horizons spacecraft flies past Pluto on July 14, 2015, carrying two instruments that detect charged particles. Pluto has a tenuous, extended atmosphere that is escaping the weak gravity of the planet. The interaction of the…

Earth and Planetary Astrophysics · Physics 2015-10-28 F. Bagenal , P. A. Delamere , H. A. Elliott , M. E. Hill , C. M. Lisse , D. J. McComas , R. L McNutt, , J. D. Richardson , C. W. Smith , D. F. Strobel

The New Horizons spacecraft carried three instruments that measured the space environment near Pluto as it flew by on 14 July 2015. The Solar Wind Around Pluto instrument revealed an interaction region confined sunward of Pluto to within…

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…

Earth and Planetary Astrophysics · Physics 2017-11-08 Henry B. Throop

The LOng-Range Reconnaissance Imager (LORRI) is the high resolution imaging instrument for the New Horizons mission to Pluto, its giant satellite Charon, its small moons Nix and Hydra, and the Kuiper Belt, which is the vast region of icy…

The radio tracking apparatus of the New Horizons spacecraft, currently traveling to the Pluto system where its arrival is scheduled for July 2015, should be able to reach an accuracy of 10 m (range) and 0.1 mm s^-1 (range-rate) over…

Earth and Planetary Astrophysics · Physics 2016-02-01 Lorenzo Iorio

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…

Earth and Planetary Astrophysics · Physics 2021-09-06 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 , R. 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 Energetic Particle Spectrometer Science Investigation (PEPSSI) comprises the hardware and accompanying science investigation on the New Horizons spacecraft to measure pick-up ions from Pluto's outgassing atmosphere. To the extent…

The discovery of Pluto in 1930 presaged the discoveries of both the Kuiper Belt and ice dwarf planets, which are the third class of planets in our solar system. From the 1970s to the 19990s numerous fascinating attributes of the Pluto…

Earth and Planetary Astrophysics · Physics 2018-10-17 S. Alan Stern , William Grundy , William B. McKinnon , Harold A. Weaver , Leslie A. Young

The outer solar system provides a unique, quiet vantage point from which to observe the universe around us, where measurements could enable several niche astrophysical science cases that are too difficult to perform near Earth. NASA's New…

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…

Earth and Planetary Astrophysics · Physics 2018-06-25 S. A. Stern , H. A. Weaver , J. R. Spencer , H. A. Elliott , the New Horizons Team

Using Chandra ACIS-S, we have obtained imaging Xray spectrophotometry of the Pluto system in support of the New Horizons flyby on 14 July 2015. 174 ksec of observations were obtained on 4 visits in Feb 2014 to Aug 2015. We measured a net…

We report on a variety of standard techniques used by New Horizons including a solar ultraviolet occultation, ultraviolet airglow observations, and high-phase look-back particulate search imaging to search for an atmosphere around Pluto's…

Context. Pluto's tenuous nitrogen (N2) atmosphere undergoes strong seasonal effects due to high obliquity and orbital eccentricity, and has been recently (July 2015) observed by the New Horizons spacecraft. Goals are (i) construct a well…

Earth and Planetary Astrophysics · Physics 2019-05-15 E. Meza , B. Sicardy , M. Assafin , J. L. Ortiz , T. Bertrand , E. Lellouch , J. Desmars , F. Forget , D. Bérard , A. Doressoundiram , J. Lecacheux , J. Marques Oliveira , F. Roques , T. Widemann , F. Colas , F. Vachier , S. Renner , R. Leiva , F. Braga-Ribas , G. Benedetti-Rossi , J. I. B. Camargo , A. Dias-Oliveira , B. Morgado , A. R. Gomes-Júnior , R. Vieira-Martins , R. Behrend , A. Castro Tirado , R. Duffard , N. Morales , P. Santos-Sanz , M. Jelínek , R. Cunniffe , R. Querel , M. Harnisch , R. Jansen , A. Pennell , S. Todd , V. D. Ivanov , C. Opitom , M. Gillon , E. Jehin , J. Manfroid , J. Pollock , D. E. Reichart , J. B. Haislip , K. M. Ivarsen , A. P. LaCluyze , A. Maury , R. Gil-Hutton , V. Dhillon , S. Littlefair , T. Marsh , C. Veillet , K. -L. Bath , W. Beisker , H. -J. Bode , M. Kretlow , D. Herald , D. Gault , S. Kerr , H. Pavlov , O. Faragó , O. Klös , E. Frappa , M. Lavayssière , A. A. Cole , A. B. Giles , J. G. Greenhill , K. M. Hill , M. W. Buie , C. B. Olkin , E. F. Young , L. A. Young , L. H. Wasserman , M. Devogèle , R. G. French , F. B. Bianco , F. Marchis , N. Brosch , S. Kaspi , D. Polishook , I. Manulis , M. Ait Moulay Larbi , Z. Benkhaldoun , A. Daassou , Y. El Azhari , Y. Moulane , J. Broughton , J. Milner , T. Dobosz , G. Bolt , B. Lade , A. Gilmore , P. Kilmartin , W. H. Allen , P. B. Graham , B. Loader , G. McKay , J. Talbot , S. Parker , L. Abe , Ph. Bendjoya , J. -P. Rivet , D. Vernet , L. Di Fabrizio , V. Lorenzi , A. Magazzù , E. Molinari , K. Gazeas , L. Tzouganatos , A. Carbognani , G. Bonnoli , A. Marchini , G. Leto , R. Zanmar Sanchez , L. Mancini , B. Kattentidt , M. Dohrmann , K. Guhl , W. Rothe , K. Walzel , G. Wortmann , A. Eberle , D. Hampf , J. Ohlert , G. Krannich , G. Murawsky , B. Gährken , D. Gloistein , S. Alonso , A. Román , J. -E. Communal , F. Jabet , S. de Visscher , J. Sérot , T. Janik , Z. Moravec , P. Machado , A. Selva , C. Perelló , J. Rovira , M. Conti , R. Papini , F. Salvaggio , A. Noschese , V. Tsamis , K. Tigani , P. Barroy , M. Irzyk , D. Neel , J. P. Godard , D. Lanoiselée , P. Sogorb , D. Vérilhac , M. Bretton , F. Signoret , F. Ciabattari , R. Naves , M. Boutet , J. De Queiroz , P. Lindner , K. Lindner , P. Enskonatus , G. Dangl , T. Tordai , H. Eichler , J. Hattenbach , C. Peterson , L. A. Molnar , R. R. Howell

Preliminary spacecraft trajectories for 45 Kuiper Belt Objects (KBOs) and Pluto suitable for launch between 2025 and 2040 are presented. These 46 objects comprise all objects with H magnitude < 4.0 or which have received a name from the…

Earth and Planetary Astrophysics · Physics 2018-10-19 Amanda M. Zangari , Tiffany J. Finley , S. Alan Stern , Mark B. Tapley
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