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Related papers: Pluto Follow On Missions: Background, Rationale, a…

200 papers

A statistical study of the environment around Polar Ring Galaxies is presented. Two kinds of search are performed: 1) a study of the concentration and diameters of all the objects surrounding the Polar Rings, within a search field 5 times…

Astrophysics · Physics 2007-05-23 Chiara Brocca , Daniela Bettoni , Giuseppe Galletta

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

Predicting the rate of escape and thermal structure of Pluto's upper atmosphere in preparation for the New Horizons Spacecraft encounter in 2015 is important for planning and interpreting the expected measurements. Having a moderate Jeans…

Earth and Planetary Astrophysics · Physics 2015-06-12 Justin T. Erwin , O. J. Tucker , Robert E. Johnson

Discovering other worlds the size of our own has been a long-held dream of astronomers. The transiting planets Kepler-20e and Kepler-20f, which belong to a multi-planet system, hold a very special place among the many groundbreaking…

Earth and Planetary Astrophysics · Physics 2019-05-14 Guillermo Torres , Francois Fressin

Simple theoretical calculations have suggested that small body impacts onto Pluto's newly discovered small satellites, Nix and Hydra, are capable of generating time-variable rings or dust sheets in the Pluto system. Using HST/ACS data…

Astrophysics · Physics 2008-11-26 A. J. Steffl , S. A. Stern

On July 14th 2015, NASA's New Horizons mission gave us an unprecedented detailed view of the Pluto system. The complex compositional diversity of Pluto's encounter hemisphere was revealed by the Ralph/LEISA infrared spectrometer on board of…

The very recent discovery of planets orbiting very low mass stars sheds light on these exotic objects. Planetary systems around low-mass stars and brown dwarfs are very different from our solar system: the planets are expected to be much…

Earth and Planetary Astrophysics · Physics 2019-02-06 Emeline Bolmont

During its departure from Pluto, New Horizons used its LORRI camera to image a portion of Pluto's southern hemisphere that was in a decades-long seasonal winter darkness, but still very faintly illuminated by sunlight reflected by Charon.…

The aim of my dissertation is to investigate habitability in extra-Solar Systems. Most of the time, only planets are considered as possible places where extraterrestrial life can emerge and evolve, however, their moons could be inhabited,…

Earth and Planetary Astrophysics · Physics 2017-04-26 Vera Dobos

Using a large suite of n-body simulations, we explore the discovery space for new satellites in the Pluto-Charon system. For the adopted masses and orbits of the known satellites, there are few stable prograde or polar orbits with semimajor…

Earth and Planetary Astrophysics · Physics 2019-09-11 Scott J. Kenyon , Benjamin C. Bromley

Many science missions require an unobstructed view of space and a stable thermal environment but lack the technical or programmatic resources to reach orbits that satisfy these needs. This paper presents a high Earth orbit in 2:1 resonance…

Earth and Planetary Astrophysics · Physics 2013-08-09 Joseph W. Gangestad , Gregory A. Henning , Randy R. Persinger , George R. Ricker

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 orbits of trans-Neptunian objects (TNOs) can indicate the existence of an undiscovered planet in the outer solar system. Here, we used N-body computer simulations to investigate the effects of a hypothetical Kuiper Belt planet (KBP) on…

Earth and Planetary Astrophysics · Physics 2023-08-29 Patryk Sofia Lykawka , Takashi Ito

A stellar occultation by Pluto on 5 September 2019 yielded positive detections at two separate stations. Using an approach consistent with comparable studies, we derived a surface pressure of $11.478 \pm 0.55~\mathrm{\mu bar}$ for Pluto's…

Earth and Planetary Astrophysics · Physics 2023-12-06 Ye Yuan , Fan Li , Yanning Fu , Jian Chen , Wei Tan , Shuai Zhang , Wei Zhang , Chen Zhang , Qiang Zhang , Jiahui Ye , Delai Li , Yijing Zhu , Zhensen Fu , Ansheng Zhu , Yue Chen , Jun Xu , Yang Zhang

The New Horizons mission to the Kuiper Belt has recently revealed intriguing features on the surface of Charon, including a network of chasmata, cutting across or around a series of high topography features, conjoining to form a belt. It is…

Earth and Planetary Astrophysics · Physics 2017-05-16 Uri Malamud , Hagai B. Perets , Gerald Schubert

The CoRoT and Kepler satellites were the first space platforms designed to perform high-precision photometry for a large number of stars. Multiple systems display a wide variety of photometric variability, making them natural benefactors of…

Solar and Stellar Astrophysics · Physics 2016-03-15 John Southworth

The orbital distribution of transneptunian objects (TNOs) in the distant Kuiper Belt (with semimajor axes beyond the 2:1 resonance, roughly $a$=50-100 au) provides constraints on the dynamical history of the outer solar system. Recent…

Earth and Planetary Astrophysics · Physics 2022-10-27 Yukun Huang , Brett Gladman , Matthew Beaudoin , Kevin Zhang

The lunar geological record has much to tell us about the earliest history of the Solar System, the origin and evolution of the Earth-Moon system, the geological evolution of rocky planets, and the near-Earth cosmic environment throughout…

Earth and Planetary Astrophysics · Physics 2015-06-05 I. A. Crawford , M. Anand , C. S. Cockell , H. Falcke , D. A. Green , R. Jaumann , M. A. Wieczorek

The small bodies in the Kuiper Belt region of the distant Solar System are leftovers from planet formation. Their orbital distribution today tells us about how giant planets migrated, while their surface properties, shapes, and sizes tell…

Earth and Planetary Astrophysics · Physics 2024-10-08 Samantha M. Lawler , Rosemary E. Pike

Most detected transiting planets have orbits which would fit within the one of Mercury, exposing them to intense stellar irradiation and interactions that significantly alter their properties. In contrast, colder planets with longer orbital…

Earth and Planetary Astrophysics · Physics 2026-04-13 Solène Ulmer-Moll , Babatunde Akinsanmi , Simon Müller