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相关论文: Beyond the New Horizon: The Future of Pluto

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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…

地球与行星天体物理 · 物理学 2018-10-17 S. Alan Stern , William Grundy , William B. McKinnon , Harold A. Weaver , Leslie A. Young

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…

地球与行星天体物理 · 物理学 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 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…

Many of the unusual properties of Pluto's orbit are widely accepted as evidence for the orbital migration of the giant planets in early solar system history. However, some properties remain an enigma. Pluto's long term orbital stability is…

地球与行星天体物理 · 物理学 2022-04-19 Renu Malhotra , Takashi Ito

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:…

地球与行星天体物理 · 物理学 2015-05-28 Hector Javier Durand-Manterola , Hector Perez-de-Tejada

The number of planets in the solar system over the last three centuries has, perhaps surprisingly, been less of a fixed value than one would think it should be. In this paper, we look at the specific case of Vulcan, which was both a planet…

地球与行星天体物理 · 物理学 2024-04-01 Michael B. Lund

Since the last Pluto volatile transport models were published (Hansen and Paige 1996), we have (i) new stellar occultation data from 2002 and 2006-2012 that have roughly twice the pressure as the discovery occultation of 1988, (ii) new…

地球与行星天体物理 · 物理学 2015-06-11 Leslie A. Young

The first exploration of Pluto was motivated by (i) the many intriguing aspects of this body, its atmosphere, and its giant impact binary-planet formation; as well as (ii) the scientific desire to initiate the reconnaissance of the…

天体物理仪器与方法 · 物理学 2021-03-18 Stuart J. Robbins , S. Alan Stern , Richard Binzel , Will Grundy , Doug Hamilton , Rosaly Lopes , Bill McKinnon , Cathy Olkin

During 2005-2012, images from Hubble Space Telescope (HST) revealed four moons orbiting Pluto-Charon (Weaver et al 2006, Showalter et al 2011, 2012). Although their orbits and geometric shapes are well-known, the 2$\sigma$ uncertainties in…

地球与行星天体物理 · 物理学 2019-07-24 Scott J. Kenyon , Benjamin C. Bromley

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…

地球与行星天体物理 · 物理学 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

Pluto's first known moon, Charon, was discovered in 1978 (Christy 1978) and has a diameter about half that of Pluto (Buie 1992,Young 1994, Sicardy 2005), which makes it larger relative to its primary than any other moon in the Solar System.…

The goal of this chapter is to review hypotheses for the origin of the Pluto system in light of observational constraints that have been considerably refined over the 85-year interval between the discovery of Pluto and its exploration by…

地球与行星天体物理 · 物理学 2021-07-20 Robin M. Canup , Kaitlin M. Kratter , Marc Neveu

The Pluto system provides a unique local laboratory for the study of binaries with multiple low mass companions. In this paper, we study the orbital stability of P4, the most recently discovered moon in the Pluto system. This newfound…

地球与行星天体物理 · 物理学 2015-06-05 Andrew N. Youdin , Kaitlin M. Kratter , Scott J. Kenyon

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…

The Pluto system is an archetype for the multitude of icy dwarf planets and accompanying satellite systems that populate the vast volume of the solar system beyond Neptune. New Horizons' exploration of Pluto and its five moons gave us a…

地球与行星天体物理 · 物理学 2022-01-26 Alex H. Parker

The search for habitable planets like Earth around other stars fulfils an ancient imperative to understand our origins and place in the cosmos. The past decade has seen the discovery of hundreds of planets, but nearly all are gas giants…

天体物理学 · 物理学 2009-11-13 Eric Gaidos , Nader Haghighipour , Eric Agol , David Latham , Sean Raymond , John Rayner

Several trace constituents can reach saturation vapor pressure in Pluto's present day atmosphere. As such, we describe a search for discrete could features in Pluto's atmosphere using New Horizons data obtained on 14-15 July 2015, during…

The study of the differences detected between the observed and the predicted positions of Uranus taking only the ancient planets into account led to the discovery of planet Neptune in 1846. This event remains one of the best accomplishments…

地球与行星天体物理 · 物理学 2024-05-13 Gabriel Rodríguez-Moris , José A. Docobo
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