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相关论文: Volatile evolution and atmospheres of Trans-Neptun…

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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

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…

地球与行星天体物理 · 物理学 2023-08-29 Patryk Sofia Lykawka , Takashi Ito

We used N-body simulations to model the 4.5 Gyr orbital evolution of the early Kuiper Belt, incorporating a massive protoplanetary disk, the four giant planets, and 1500 primordial Pluto-class bodies ("Plutos") that drove Neptune's grainy…

地球与行星天体物理 · 物理学 2026-02-20 Patryk Sofia Lykawka , Jonathan Horner , Pedro Bernardinelli

The goal of this work is to determine the physical characteristics of resonant, detached and scattered disk objects in the transneptunian region, observed mainly in the framework of the "TNOs are Cool!" Herschel Open Time Key Program. Based…

地球与行星天体物理 · 物理学 2020-07-01 A. Farkas-Takács , Cs. Kiss , E. Vilenius , G. Marton , T. G. Müller , M. Mommert , J. Stansberry , E. Lellouch , P. Lacerda , A. Pál

Recent observations (Burnes et al 2002,Veillet et al 2002, Margot et al 2002a) have revealed an unexpectedly high binary fraction among the Trans-Neptunian Objects (TNOs) that populate the Kuiper Belt. The TNO binaries are strikingly…

天体物理学 · 物理学 2007-05-23 Yoko Funato , Junichiro Makino , Piet Hut , Eiichiro Kokubo , Daisuke Kinoshita

We present observations of thermal emission from fifteen transneptunian objects (TNOs) made using the Spitzer Space Telescope. Thirteen of the targets are members of the Classical population: six dynamically hot Classicals, five dynamically…

天体物理学 · 物理学 2009-01-22 M. J. Brucker , W. M. Grundy , J. A. Stansberry , J. R. Spencer , S. S. Sheppard , E. I. Chiang , M. W. Buie

Kuiper belt object (KBO) Eris is exceptionally bright with a greater visible geometric albedo than any other known KBO. Its infrared reflectance spectrum is dominated by methane, which should form tholins that darken the surface on…

地球与行星天体物理 · 物理学 2018-11-08 Jason D. Hofgartner , Bonnie J. Buratti , Paul O. Hayne , Leslie A. Young

A stellar occultation by Neptune's main satellite, Triton, was observed on 5 October 2017 from Europe, North Africa, and the USA. We derived 90 light curves from this event, 42 of which yielded a central flash detection. We aimed at…

地球与行星天体物理 · 物理学 2022-04-20 J. Marques Oliveira , B. Sicardy , A. R. Gomes-Júnior , J. L. Ortiz , D. F. Strobel , T. Bertrand , F. Forget , E. Lellouch , J. Desmars , D. Bérard , A. Doressoundiram , J. Lecacheux , R. Leiva , E. Meza , F. Roques , D. Souami , T. Widemann , P. Santos-Sanz , N. Morales , R. Duffard , E. Fernández-Valenzuela , A. J. Castro-Tirado , F. Braga-Ribas , B. E. Morgado , M. Assafin , J. I. B. Camargo , R. Vieira-Martins , G. Benedetti-Rossi , S. Santos-Filho , M. V. Banda-Huarca , F. Quispe-Huaynasi , C. L. Pereira , F. L. Rommel , G. Margoti , A. Dias-Oliveira , F. Colas , J. Berthier , S. Renner , R. Hueso , S. Pérez-Hoyos , A. Sánchez-Lavega , J. F. Rojas , W. Beisker , M. Kretlow , D. Herald , D. Gault , K. -L. Bath , H. -J. Bode , E. Bredner , K. Guhl , T. V. Haymes , E. Hummel , B. Kattentidt , O. Klös , A. Pratt , B. Thome , C. Avdellidou , K. Gazeas , E. Karampotsiou , L. Tzouganatos , E. Kardasis , A. A. Christou , E. M. Xilouris , I. Alikakos , A. Gourzelas , A. Liakos , V. Charmandaris , M. Jelínek , J. Štrobl , A. Eberle , K. Rapp , B. Gährken , B. Klemt , S. Kowollik , R. Bitzer , M. Miller , G. Herzogenrath , D. Frangenberg , L. Brandis , I. Pütz , V. Perdelwitz , G. M. Piehler , P. Riepe , K. von Poschinger , P. Baruffetti , D. Cenadelli , J. -M. Christille , F. Ciabattari , R. Di Luca , D. Alboresi , G. Leto , R. Zanmar Sanchez , P. Bruno , G. Occhipinti , L. Morrone , L. Cupolino , A. Noschese , A. Vecchione , C. Scalia , R. Lo Savio , G. Giardina , S. Kamoun , R. Barbosa , R. Behrend , M. Spano , E. Bouchet , M. Cottier , L. Falco , S. Gallego , L. Tortorelli , S. Sposetti , J. Sussenbach , F. Van Den Abbeel , P. André , M. Llibre , F. Pailler , J. Ardissone , M. Boutet , J. Sanchez , M. Bretton , A. Cailleau , V. Pic , L. Granier , R. Chauvet , M. Conjat , J. L. Dauvergne , O. Dechambre , P. Delay , M. Delcroix , L. Rousselot , J. Ferreira , P. Machado , P. Tanga , J. -P. Rivet , E. Frappa , M. Irzyk , F. Jabet , M. Kaschinski , A. Klotz , Y. Rieugnie , A. N. Klotz , O. Labrevoir , D. Lavandier , D. Walliang , A. Leroy , S. Bouley , S. Lisciandra , J. -F. Coliac , F. Metz , D. Erpelding , P. Nougayrède , T. Midavaine , M. Miniou , S. Moindrot , P. Morel , B. Reginato , E. Reginato , J. Rudelle , B. Tregon , R. Tanguy , J. David , W. Thuillot , D. Hestroffer , G. Vaudescal , D. Baba Aissa , Z. Grigahcene , D. Briggs , S. Broadbent , P. Denyer , N. J. Haigh , N. Quinn , G. Thurston , S. J. Fossey , C. Arena , M. Jennings , J. Talbot , S. Alonso , A. Román Reche , V. Casanova , E. Briggs , R. Iglesias-Marzoa , J. Abril Ibáñez , M. C. Díaz Martín , H. González , J. L. Maestre García , J. Marchant , I. Ordonez-Etxeberria , P. Martorell , J. Salamero , F. Organero , L. Ana , F. Fonseca , V. Peris , O. Brevia , A. Selva , C. Perello , V. Cabedo , R. Gonçalves , M. Ferreira , F. Marques Dias , A. Daassou , K. Barkaoui , Z. Benkhaldoun , M. Guennoun , J. Chouqar , E. Jehin , C. Rinner , J. Lloyd , M. El Moutamid , C. Lamarche , J. T. Pollock , D. B. Caton , V. Kouprianov , B. W. Timerson , G. Blanchard , B. Payet , A. Peyrot , J. -P. Teng-Chuen-Yu , J. Françoise , B. Mondon , T. Payet , C. Boissel , M. Castets , W. B. Hubbard , R. Hill , H. J. Reitsema , O. Mousis , L. Ball , G. Neilsen , S. Hutcheon , K. Lay , P. Anderson , M. Moy , M. Jonsen , I. Pink , R. Walters , B. Downs

Surface modification on Jupiter's volcanically active moon, Io, has to date been attributed almost exclusively to lava emplacement and volcanic plume deposits. Here we demonstrate that wind-blown transport of sediment may also be altering…

地球与行星天体物理 · 物理学 2022-04-20 George D. McDonald , Joshua Méndez Harper , Lujendra Ojha , Paul Corlies , Josef Dufek , Ryan C. Ewing , Laura Kerber

Ocean worlds, or icy bodies in the outer solar system that have or once had subsurface liquid water oceans, are among the most compelling topics of astrobiology. Typically, confirming the existence of a subsurface ocean requires close…

地球与行星天体物理 · 物理学 2023-12-13 Kathleen Mandt , Adrienn Luspay-Kuti , Olivier Mousis , Sarah E. Anderson

Trans-Neptunian objects (TNOs) contain the most primitive and thermally least-processed materials from the early accretional phase of the solar system. They allow us to study interrelations between various classes of small bodies, their…

天体物理学 · 物理学 2009-11-13 S. Bagnulo , I. Belskaya , K. Muinonen , G. P. Tozzi , M. A. Barucci , L. Kolokolova , S. Fornasier

Despite the low solar irradiation it receives, Neptune shows a very active atmosphere with some of the most intense dynamics observed in Solar System atmospheres. Characterizing the atmospheric temperature profiles of the planet is a key to…

Most known trans-Neptunian objects (TNOs) gravitationally scattering off the giant planets have orbital inclinations consistent with an origin from the classical Kuiper belt, but a small fraction of these "scattering TNOs" have inclinations…

A distant, massive planet in the outer solar system has recently been proposed to explain some observed features of extreme trans-Neptunian objects (TNOs). Here we use N-body simulations of the formation of the Kuiper belt and Oort cloud as…

地球与行星天体物理 · 物理学 2021-10-13 Kalee E. Anderson , Nathan A. Kaib

Trans-Neptunian objects (TNOs) with diameter greater than 100 km currently moving in not too eccentric orbits could be formed directly by the contraction of large rarefied condensations. Along with the gravitational influence of planets,…

天体物理学 · 物理学 2007-05-23 Sergei I. Ipatov , Leonid M. Ozernoy

JWST observations provide for the first time evidence for an atmosphere on a rocky exoplanet - 55 Cnc e. The atmosphere of 55 Cnc e is hot with $\text{T}_{\text{eq}}>2000$K and shows strong variability, for which cloud formation above a…

地球与行星天体物理 · 物理学 2026-01-23 Leoni J. Janssen , Yamila Miguel , Michiel Min , Helong Huang , Mantas Zilinskas , Christiaan P. A. van Buchem

Over the last decade, precise exoplanet transmission spectroscopy has revealed the atmospheres of dozens of exoplanets, driven largely by observatories like the Hubble Space Telescope. One major discovery has been the ubiquity of…

Recent observations (Burnes2002,Veillet2002,Margot2002a) have revealed an unexpectedly high binary fraction among the Trans-Neptunian Objects (TNOs) that populate the Kuiper Belt. The TNO binaries are strikingly different from asteroid…

天体物理学 · 物理学 2007-05-23 Yoko Funato , Junichiro Makino , Piet Hut , Eiichiro Kokubo , Daisuke Kinoshita

Context - Around the year 2000, Triton's south pole experienced an extreme summer solstice that occurs every about 650 years, when the subsolar latitude reached about 50{\deg}. Bracketing this epoch, a few occultations probed Triton's…

Understanding the planetary envelope composition of sub-Neptune-type exoplanets is challenging due to the inherent degeneracy in their interior composition scenarios. Particularly, the planetary envelope's H2O/H2 ratio, which can also be…

地球与行星天体物理 · 物理学 2024-08-21 Jeehyun Yang , Renyu Hu