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Related papers: A Search for Temporal Changes on Pluto and Charon

200 papers

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

Jupiter's banded appearance may appear unchanging to the casual observer, but closer inspection reveals a dynamic, ever-changing system of belts and zones with distinct cycles of activity. Identification of these long-term cycles requires…

Earth and Planetary Astrophysics · Physics 2017-08-18 L. N. Fletcher

It is usually taken for granted that mutual synchronisation of a tidal two-body system is attained through tidal recession, assuming the reduced Hill sphere is not reached. However, synchronisation can be achieved also via tidal approach,…

Earth and Planetary Astrophysics · Physics 2026-04-21 Michael Efroimsky , Michaela Walterova , Yeva Gevorgyan , Amirhossein Bagheri , Valeri V. Makarov , Amir Khan

Context: The role of Pluto contributing to the long-term evolution of the trans-Neptunian region has been considered significant only over its neighboring Plutinos. However, it has recently been found that the long-term stability of the…

Earth and Planetary Astrophysics · Physics 2026-03-11 S. Ramírez-Vargas , A. Peimbert , M. A. Muñoz-Gutiérrez , A. Perez-Villegas

Observations from the Hinode/XRT telescope and STEREO/SECCHI/EUVI are utilized to study polar coronal jets and plumes. The study focuses on the temporal evolution of both structures and their relationship. The data sample, spanning April…

Astrophysics · Physics 2009-11-13 N. -E. Raouafi , G. J. D. Petrie , A. A. Norton , C. J. Henney , S. K. Solanki

The most pristine remnants of the Solar system's planet formation epoch orbit the Sun beyond Neptune, the small bodies of the trans-Neptunian object populations. The bulk of the mass is in ~100 km objects, but objects at smaller sizes have…

Earth and Planetary Astrophysics · Physics 2024-02-19 Andrew Shannon , Alain Doressoundiram , Françoise Roques , Bruno Sicardy , Quentin Kral

Neptune Trojans and Plutinos are two subpopulations of trans-Neptunian objects located in the 1:1 and the 3:2 mean motion resonances with Neptune, respectively, and therefore protected from close encounters with the planet. However, the…

Earth and Planetary Astrophysics · Physics 2009-12-02 A. J. C. Almeida , N. Peixinho , A. C. M. Correia

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…

Earth and Planetary Astrophysics · Physics 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

The Solar Wind Around Pluto (SWAP) instrument on New Horizons will measure the interaction between the solar wind and ions created by atmospheric loss from Pluto. These measurements provide a characterization of the total loss rate and…

Transient Lunar Phenomena (TLP) observed on the surface of the moon, are of high rarity, low repetition rate and very short observation times, resulting in that there is little information about this topic. This necessitates the importance…

Earth and Planetary Astrophysics · Physics 2013-03-06 Cruz Roa AF

Since 2013, dense and narrow rings are known around the small Centaur object Chariklo and the dwarf planet Haumea. Dense material has also been detected around the Centaur Chiron, although its nature is debated. This is the first time ever…

Earth and Planetary Astrophysics · Physics 2020-01-22 Bruno Sicardy , Stefan Renner , Rodrigo Leiva , Françoise Roques , Maryame El Moutamid , Pablo Santos-Sanz , Josselin Desmars

Moons tidally interact with their host planets and stars. A close moon is quickly synchronised by the planet, or becomes captured in a higher spin-orbit resonance. However, the planet requires much more time to significantly alter its…

Earth and Planetary Astrophysics · Physics 2025-09-15 Valeri V. Makarov , Michael Efroimsky

Polarization is a powerful remote-sensing method to investigate solar system bodies. It is an especially sensitive diagnostic tool to reveal physical properties of the bodies whose observational characteristics are governed by small…

Astrophysics · Physics 2009-11-11 S. Bagnulo , H. Boehnhardt , K. Muinonen , L. Kolokolova , I. Belskaya , M. A. Barucci

We present three near-infrared spectra of Pluto taken with the IRTF and SpeX, an optical spectrum of Triton taken with the MMT and the Red Channel Spectrograph, and previously published spectra of Pluto, Triton, and Eris. We combine these…

Earth and Planetary Astrophysics · Physics 2015-06-04 S. C. Tegler , W. M. Grundy , C. B Olkin , L. A. Young , W. Romanishin , D. M. Cornelison , R. Khodadadkouchaki

With the recent discoveries of hundreds of extrasolar planets, the search for planets like Earth and life in the universe, is quickly gaining momentum. In the future, large space observatories could directly detect the light scattered from…

Astrophysics · Physics 2009-11-13 E. Palle , Eric B. Ford , S. Seager , P. Montanes-Rodriguez , M. Vazquez

Up to now, most planet search projects have concentrated on F to K stars. In order to considerably widen the view, we have stated a survey for planets of old, nearby brown dwarfs and very low mass stars. Using UVES, we have observed 26…

Astrophysics · Physics 2011-05-23 Eike W. Guenther , Guenther Wuchterl

The orbits of Pluto's four small satellites (Styx, Nix, Kerberos, and Hydra) are nearly circular and coplanar with the orbit of the large satellite Charon, with orbital periods nearly in the ratios 3:1, 4:1, 5:1, and 6:1 with Charon's…

Earth and Planetary Astrophysics · Physics 2015-06-22 W. H. Cheng , S. J. Peale , Man Hoi Lee

Context. The PLAnetary Transits and Oscillations of stars (PLATO) mission will observe the same area of the sky continuously for at least two years in an effort to detect transit signals of an Earth-like planet orbiting a solar-like star.…

Earth and Planetary Astrophysics · Physics 2024-10-29 A. F. Krenn , M. Lendl , S. Sulis , M. Deleuil , S. J. Hofmeister , N. Jannsen , L. Fossati , J. De Ridder , D. Seynaeve , R. Jarolim , A. M. Veronig

The recent discovery of two large trans-Neptunian objects (TNOs) 2003 UB313 and 2005 FY9, with surface properties similar to those of Pluto, provides an exciting new laboratory for the study of processes considered for Pluto and Triton:…

Astrophysics · Physics 2009-11-11 J. Licandro , W. M. Grundy , N. Pinilla-Alonso , J. de Leon

Context. The equatorial region of Cthulhu as revealed by New Horizons appears to be generally dark and largely devoid of volatiles because its surface albedo is low. Localized bright patches, however, which are interpreted as CH4 frost, are…

Earth and Planetary Astrophysics · Physics 2026-01-09 L. Lange , T. Bertrand , V. Belissa , S. Capry , L. A. Young , A. Falco
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