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Triton is the largest moon of the Neptune system and possesses a thin nitrogen atmosphere with trace amounts of carbon monoxide and methane, making it of similar composition to that of the dwarf planet Pluto. Like Pluto and Saturn's moon…

Due to its inclined orbit and the complex geometry of the magnetic field of Neptune, Triton experiences a highly variable magnetic environment. As precipitation of magnetospheric electrons is thought to have a large impact on the Triton…

地球与行星天体物理 · 物理学 2024-07-24 B. Benne , B. Benmahi , M. Dobrijevic , T. Cavalié , J-C. Loison , K. M. Hickson , M. Barthélémy , J. Lilensten

Neptune's largest satellite, Triton, is one of the most fascinating and enigmatic bodies in the solar system. Among its numerous interesting traits, Triton appears to have far fewer craters than would be expected if its surface was…

天体物理学 · 物理学 2009-10-31 S. A. Stern , W. B. McKinnon

This brief review will discuss the current knowledge on the origin and evolution of the nitrogen atmospheres of the icy bodies in the solar system, particularly of Titan, Triton and Pluto. An important tool to analyse and understand the…

地球与行星天体物理 · 物理学 2020-11-03 M. Scherf , H. Lammer , N. V. Erkaev , K. E. Mandt , S. E. Thaller , B. Marty

Neptune remains a mysterious world that deserves further exploration and is a high-priority objective for a future planetary mission in order to better understand the formation and evolution of ice giant planets. We have developed a coupled…

地球与行星天体物理 · 物理学 2020-11-17 M. Dobrijevic , J. C. Loison , V. Hue , T. Cavalié , K. M. Hickson

Neptune's moon Triton shares many similarities with Pluto, including volatile cycles of N2, CH4 and CO, and represents a benchmark case for the study of surface-atmosphere interactions on volatile-rich KBOs. Within the context of New…

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

Comparatively little is known about atmospheric chemistry on Uranus and Neptune, because remote spectral observations of these cold, distant ``Ice Giants'' are challenging, and each planet has only been visited by a single spacecraft during…

地球与行星天体物理 · 物理学 2021-03-03 J. I. Moses , T. Cavalie , L. N. Fletcher , M. T. Roman

The Neptunian satellite system is unusual, comprising Triton, a large ($\sim2700$ km) moon on a close-in, circular, yet retrograde orbit, flanked by Nereid, the largest irregular satellite ($\sim$300 km) on a highly eccentric orbit. Capture…

地球与行星天体物理 · 物理学 2020-04-07 Daohai Li , Apostolos A. Christou

Titan is the only moon with a substantial atmosphere, the only other thick N$_{2}$ atmosphere besides Earth's, the site of extraordinarily complex atmospheric chemistry that far surpasses any other solar system atmosphere, and the only…

地球与行星天体物理 · 物理学 2018-01-10 Sarah M. Hörst

Triton and Pluto are believed to share a common origin, both forming initially in the Kuiper Belt but Triton being later captured by Neptune. Both objects display similar sizes, densities, and atmospheric and surface ice composition, with…

地球与行星天体物理 · 物理学 2024-09-04 Tanguy Bertrand , François Forget , Emmanuel Lellouch

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

The Neptunian satellite system is unusual. The major satellites of Jupiter, Saturn, and Uranus are all in prograde, low-inclination orbits. Neptune on the other hand, has the fewest satellites, and most of the system's mass is within one…

地球与行星天体物理 · 物理学 2017-11-07 Raluca Rufu , Robin M. Canup

Triton possesses a thin atmosphere, primarily composed of nitrogen, sustained by the sublimation of surface ices. The goal is to determine the composition of Triton's atmosphere and to constrain the nature of surface-atmosphere…

地球与行星天体物理 · 物理学 2015-05-18 E. Lellouch , C. de Bergh , B. Sicardy , S. Ferron , H. -U. Käufl

The largest moon of Neptune, Triton, possess a cold and hazy atmosphere. Since the discovery of near-surface haze layer during the Voyager fly in 1989, the haze formation mechanism has not been investigated in detail. Here, we provide the…

地球与行星天体物理 · 物理学 2021-05-12 Kazumasa Ohno , Xi Zhang , Ryo Tazaki , Satoshi Okuzumi

Titan, Saturn's largest satellite, maintains an atmosphere composed primarily of nitrogen (N$_2$) and methane (CH$_4$) that leads to a complex organic chemistry. Some of the nitriles (CN-bearing organics) on Titan are known to have…

地球与行星天体物理 · 物理学 2025-03-14 J. Nosowitz , M. A. Cordiner , C. A. Nixon , A. E. Thelen , Z. Kisiel , N. A. Teanby , P. G. J. Irwin , S. B. Charnley , V. Vuitton

This report arises from an ongoing program to monitor Neptune's largest moon Triton spectroscopically in the 0.8 to 2.4 micron range using IRTF/SpeX. Our objective is to search for changes on Triton's surface as witnessed by changes in the…

地球与行星天体物理 · 物理学 2015-05-13 W. M. Grundy , L. A. Young , J. A. Stansberry , M. W. Buie , C. B. Olkin , E. F. Young

Titan is one of the more distinctive bodies in our solar system. In addition to being the largest of Saturn's moons, its thick atmosphere gene-rates interest because of its similarities and differences with Earth [1, 2]. Like Earth, Titan's…

地球与行星天体物理 · 物理学 2010-10-21 C. C. Harris , L. S. Matthews , T. W. Hyde

Several clues indicate that Titan's atmosphere has been depleted in methane during some period of its history, possibly as recently as 0.5-1 billion years ago. It could also happen in the future. Under these conditions, the atmosphere…

地球与行星天体物理 · 物理学 2015-06-22 Benjamin Charnay , François Forget , Gabriel Tobie , Christophe Sotin , Robin Wordsworth

Triton is a unique moon in our Solar System, being the only large moon to orbit on a retrograde and highly inclined orbit. As a result, it is thought that it did not form around Neptune, but rather was captured from heliocentric orbit. The…

地球与行星天体物理 · 物理学 2024-09-26 Quirijn Benjamin van Woerkom
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