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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…

Earth and Planetary Astrophysics · Physics 2018-01-10 Sarah M. Hörst

The temperature of the cosmic microwave background (CMB) was equal to the surface temperature of Saturn's moon Titan, 94K, at a redshift z=33.5, after the first galaxies formed. Titan-like objects would have maintained this surface…

Cosmology and Nongalactic Astrophysics · Physics 2022-12-06 Abraham Loeb

Thanks to the Cassini-Huygens mission, Titan, the pale orange dot of Pioneer and Voyager encounters has been revealed to be a dynamic, hydrologically-shaped, organic-rich ocean world offering unparalleled opportunities to explore prebiotic…

Is life a common outcome of physical and chemical processes in the universe? Within our own solar system, a successful search for even primitive life, were it to have an origin independent from life on Earth, would dramatically advance a…

Earth and Planetary Astrophysics · Physics 2010-04-13 J. I. Lunine

Saturn's moon Titan exhibits remarkable parallels to the Earth in many geophysical and geological processes not found elsewhere in the solar system at the present day. These include a nitrogen atmosphere with a condensible gas - methane -…

The Cassini-Huygens mission measured the chemical abundances of the major components of Titan's atmosphere, and analyses of the data revealed several as-yet unexplained anomalies in the methane and hydrogen profiles. We model the…

Earth and Planetary Astrophysics · Physics 2021-07-23 Erin E. Flowers , Christopher F. Chyba , Paul J. Thomas

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…

Earth and Planetary Astrophysics · Physics 2010-10-21 C. C. Harris , L. S. Matthews , T. W. Hyde

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…

Earth and Planetary Astrophysics · Physics 2025-08-06 David Dubois

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…

Earth and Planetary Astrophysics · Physics 2015-06-22 Benjamin Charnay , François Forget , Gabriel Tobie , Christophe Sotin , Robin Wordsworth

Saturn's largest moon, Titan, has an Earth-like volatile cycle, but with methane playing the role of water and surface liquid reservoirs geographically isolated at high latitudes. We recreate Titan's characteristic dry hydroclimate at the…

Earth and Planetary Astrophysics · Physics 2022-07-14 Matthew McKinney , J. Mitchell , S. I. Thomson

The history of the Earth has been marked by major ecological transitions, driven by metabolic innovation, that radically reshaped the composition of the oceans and atmosphere. The nature and magnitude of the earliest transitions, hundreds…

Populations and Evolution · Quantitative Biology 2020-06-12 Boris Sauterey , Benjamin Charnay , Antonin Affholder , Stéphane Mazevet , Régis Ferrière

In order to examine how the terrestrial life emerged, a number of laboratory experiments have been conducted since the 1950s. Methane has been one of the key molecules in these studies. In earlier studies, strongly reducing gas mixtures…

The Cassini-Huygens space mission revealed that Titan s thick brownish haze is initiated high in the atmosphere at about 1000 km of altitude, before a slow transportation down to the surface. Close to the surface at altitudes below 130 km,…

Earth and Planetary Astrophysics · Physics 2018-06-26 Nathalie Carrasco , Sarah Tigrine , Lisseth Gavilan , Laurent Nahon , Murthy S. Gudipati

Earth and Titan are two planetary bodies formed far from each other. Nevertheless the chemical composition of their atmospheres exhibits common indications of being produced by the accretion, plus ulterior in-situ processing of cometary…

Earth and Planetary Astrophysics · Physics 2015-05-27 Josep M. Trigo-Rodriguez , F. Javier Martin-Torres

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…

Earth and Planetary Astrophysics · Physics 2025-03-17 Zoé Perrin , Nathalie Carrasco , Thomas Gautier , Nathalie Ruscassier , Julien Maillard , Carlos Afonso , Ludovic Vettier

While Saturn's moon Titan appears to support an active methane hydrological cycle, no direct evidence for surface-atmosphere exchange has yet appeared. It is possible that the identified lake-features could be filled with ethane, an…

Earth and Planetary Astrophysics · Physics 2015-05-14 M. E. Brown , A. L. Smith , C. Chen , M. Adamkovics

After Earth's origin, our host star, the Sun, was shining 20 to 25 percent less brightly than today. Without greenhouse-like conditions to warm the atmosphere, our early planet would have been an ice ball and life may never have evolved.…

This chapter explores the key carbon compounds that shaped the Archean biogeochemical cycle, delineating their substantial impact on Earth's primordial atmospheric and biospheric evolution. At the heart of the Archean carbon cycle were…

Atmospheric and Oceanic Physics · Physics 2025-03-31 Saleheh Ebadirad , Timothy W. Lyons , Gregory P. Fournier

Titan, Saturn's largest moon, supports a dense atmosphere, numerous bodies of liquid on its surface, and as a richly organic world is a primary focus for understanding the processes that support the development of life. In-situ exploration…

Instrumentation and Methods for Astrophysics · Physics 2021-06-18 James McKevitt

We apply previously introduced measures of chemical disequilibrium to Cassini mass spectroscopy data on the atmosphere of Titan. In the analysis presented here, we use an improved description, avoiding the meanfield approximation in…

Earth and Planetary Astrophysics · Physics 2019-07-03 Ben F. M. Intoy , J. Woods Halley
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