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The formation and evolution of haze layers in planetary atmospheres play a critical role in shaping their chemical composition, radiative balance, and optical properties. In the outer solar system, the atmospheres of Titan and the giant…

地球与行星天体物理 · 物理学 2025-08-06 David Dubois

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

Titan's abundant atmospheric N2 and CH4 gases are notable characteristics of the moon that may help constrain its origins and evolution. Previous work suggests that atmospheric CH4 is lost on geologically short timescales and may be…

地球与行星天体物理 · 物理学 2024-12-19 Kelly E. Miller , Dionysis I. Foustoukos , George Cody , Conel M. O'D. Alexander

Titan, the largest satellite of Saturn, has an atmosphere chiefly made up of N2 and CH4 and includes traces of many simple organic compounds. This atmosphere also partly consists of haze and aerosol particles which during the last 4.5…

地球与行星天体物理 · 物理学 2009-06-22 S. Pilling , D. P. P. Andrade , Alvaro C. Neto , R. Rittner , A. Naves de Brito

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…

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

Organic aerosols accumulated in Titan's orange haze start forming in its ionosphere. This upper part of the atmosphere is highly reactive and complex ion chemistry takes place at altitudes from 1200 to 900 km. The ionosphere is a nitrogen…

地球与行星天体物理 · 物理学 2020-11-17 Audrey Chatain , Nathalie Carrasco , Nathalie Ruscassier , Thomas Gautier , Ludovic Vettier , Olivier Guaitella

The organic haze of aerosols that shrouds the Saturnian moon Titan has previously been studied by both observations and laboratory simulation experiments. Here we report the abiotic formation of amino acid precursors in complex organic…

地球与行星天体物理 · 物理学 2013-09-26 Toshinori Taniuchi , Yoshinori Takano , Kensei Kobayashi

Chemistry in Titan's N2-CH4 atmosphere produces complex organic aerosols. The chemical processes and the resulting organic compounds are still far from understood, although extensive observations, laboratory, and theoretical simulations…

地球与行星天体物理 · 物理学 2022-09-26 Chao He , Joseph Serigano , Sarah M. Horst , Michael Radke , Joshua A. Sebree

Titan has a climate system with similarities to Earth, including the presence of a thick atmosphere made up of several atmospheric layers. As on Earth, Titan's climate is influenced by several factors: the gaseous species making up the…

地球与行星天体物理 · 物理学 2025-03-17 Zoé Perrin , Nathalie Carrasco , Thomas Gautier , Nathalie Ruscassier , Julien Maillard , Carlos Afonso , Ludovic Vettier

Thermochemical modeling and shock-tube experiments show that shocks applied to N$_2$/CH$_4$ gas mixtures can synthesize organic molecules. Sufficiently large, hypersonic meteoroids entering the atmosphere of Saturn's moon Titan should…

地球与行星天体物理 · 物理学 2023-07-21 Erin E. Flowers , Christopher F. Chyba

Titan's atmosphere possesses thick haze layers, but their formation mechanisms remain poorly understood, including the influence of oxygen-containing gas components on organic matter synthesis. As the most abundant oxygen-containing gas,…

化学物理 · 物理学 2025-06-19 Zhengbo Yang , Yu Liu , Chao He , Pengcheng Yu , Rong Jin , Xiangqun Liu , Jinpu Zhang , Jiuhou Lei

The origin of Titan's atmospheric methane is a key issue for understanding the origin of the Saturnian satellite system. It has been proposed that serpentinization reactions in Titan's interior could lead to the formation of the observed…

Titan's organic aerosols are formed in the ionosphere, a layer ionized by solar VUV photons and energetic particles from the magnetosphere of Saturn, forming a natural N2-CH4-H2 plasma. Previous works showed some chemical evolution…

地球与行星天体物理 · 物理学 2023-09-06 Audrey Chatain , Nathalie Carrasco , Ludovic Vettier , Olivier Guaitella

Thanks to the \textit{Cassini} spacecraft onboard instruments, it has been known that Titan's ionospheric chemistry is complex and the molecular growth is initiated through the photolysis of the most abundant species directly in the upper…

地球与行星天体物理 · 物理学 2020-01-08 Jérémy Bourgalais , Nathalie Carraso , Ludovic Vettier , Pascal Pernot

Saturn's largest satellite, Titan, has a thick atmosphere dominated by nitrogen and methane. The dense orange-brown smog hiding the satellite's surface is produced by photochemical reactions of methane, nitrogen and their dissociation…

天体物理学 · 物理学 2009-11-13 Olivier Mousis , Bernard Schmitt

The aerosols present in the atmosphere of the Saturn s moon Titan are of particular planetary science interest and several spacecraft missions already allowed to gather spectroscopic data. Titan haze s analogs, so-called tholins, were…

With the Cassini-Huygens Mission in orbit around Saturn, the large moon Titan, with its reducing atmosphere, rich organic chemistry, and heterogeneous surface, moves into the astrobiological spotlight. Environmental conditions on Titan and…

生物物理 · 物理学 2007-05-23 D. Schulze-Makuch , D. Grinspoon

Titan's thick atmosphere is primarily composed of nitrogen and methane. Complex chemistry happening in Titan's atmosphere produces optically thick organic hazes. These hazes play significant roles in Titan's atmosphere and on its surface,…

地球与行星天体物理 · 物理学 2021-12-17 Chao He , Sarah M. Horst , Michael Radke , Marcella Yant

We present results of an investigation into the formation of nitrogen-bearing molecules in the atmosphere of Titan. We extend a previous model (Li et al. 2015, 2016) to cover the region below the tropopause, so the new model treats the…

地球与行星天体物理 · 物理学 2016-10-05 Karen Willacy , Mark Allen , Yuk Yung
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