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相关论文: Mars, a Post-Habitable Planet?

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Mars is the Solar System's canonical small, rocky planet that transitioned from early geologic activity and surface liquid water to a cold and arid planet with a thin, cold, CO$_2$-dominated atmosphere. The evolution of Mars, in the context…

Habitability is a measure of an environment's potential to support life, and a habitable exoplanet supports liquid water on its surface. However, a planet's success in maintaining liquid water on its surface is the end result of a complex…

地球与行星天体物理 · 物理学 2021-12-15 Ravi kumar Kopparapu , Eric T. Wolf , Victoria S. Meadows

The climate of early Mars remains a topic of intense debate. Ancient terrains preserve landscapes consistent with stream channels, lake basins, and possibly even oceans, and thus the presence of liquid water flowing on the Martian surface 4…

地球与行星天体物理 · 物理学 2018-10-05 Ramses M. Ramirez , Robert A. Craddock

In the past 15 years, astronomers have revealed that a significant fraction of the stars should harbor planets and that it is likely that terrestrial planets are abundant in our galaxy. Among these planets, how many are habitable, i.e.…

地球与行星天体物理 · 物理学 2013-05-09 Francois Forget

Earth has a unique surface character among Solar System worlds. Not only does it harbor liquid water, but also large continents. An exoplanet with a similar appearance would remind us of home, but it is not obvious whether such a planet is…

地球与行星天体物理 · 物理学 2015-11-20 Nicolas B. Cowan

The climate of Mars likely evolved from a warmer, wetter early state to the cold, arid current state. However, no solutions for this evolution have previously been found to satisfy the observed geological features and isotopic measurements…

地球与行星天体物理 · 物理学 2015-12-03 Renyu Hu , David M. Kass , Bethany L. Ehlmann , Yuk L. Yung

Planet Mars past environmental conditions were similar to the early Earth, but nowadays they are similar to those of a very cold desert, irradiated by intense solar UV light. However, some terrestrial lifeform showed the capability to adapt…

地球与行星天体物理 · 物理学 2011-02-23 Giuseppe Galletta , Giulio Bertoloni , Maurizio D'Alessandro

The frequently discovered flooding structure on Mars and other planets has long been an intriguing mystery remained un-disclosed so far. Considering that on Earth, quite a few low melting point liquid metals or their alloy can be candidates…

综合物理 · 物理学 2014-03-18 Jing Liu , Yunxia Gao , Huangde Li

Our present-day atmosphere is often used as an analog for potentially habitable exoplanets, but Earth's atmosphere has changed dramatically throughout its 4.5 billion year history. For example, molecular oxygen is abundant in the atmosphere…

地球与行星天体物理 · 物理学 2018-12-05 Stephanie L. Olson , Edward W. Schwieterman , Christopher T. Reinhard , Timothy W. Lyons

A habitable exoplanet is a world that can maintain stable liquid water on its surface. Techniques and approaches to characterizing such worlds are essential, as performing a census of Earth-like planets that may or may not have life will…

地球与行星天体物理 · 物理学 2024-01-22 Tyler D. Robinson

According to the standard liquid-water definition, the Earth is only partially habitable. We reconsider planetary habitability in the framework of energy-balance models, the simplest seasonal models in physical climatology, to assess the…

天体物理学 · 物理学 2009-11-13 David S. Spiegel , Kristen Menou , Caleb A. Scharf

Whereas the Solar System has Mars and Europa as the best candidates for finding fossil/extant life as we know it - based on complex carbon compounds and liquid water - the 263 (non-pulsar) planetary systems around other stars as known at 15…

地球与行星天体物理 · 物理学 2018-12-05 Barrie W Jones

Earth is the only planet known to harbor life and, as a result, the search for habitable and inhabited planets beyond the Solar System commonly focuses on analogs to our planet. However, Earth's atmosphere and surface environment have…

地球与行星天体物理 · 物理学 2019-10-17 Tyler D. Robinson , Christopher T. Reinhard

Understanding the concept of habitability is related to an evolutionary knowledge of the particular planet-in-question. Additional indications so-called "systemic aspects" of the planetary system as a whole governs a particular planet's…

Mars' wet-to-dry transition is a major environmental catastrophe, yet the spatial pattern, tempo, and cause of drying are poorly constrained. We built a globally-distributed database of constraints on Mars late-stage paleolake size relative…

地球与行星天体物理 · 物理学 2023-01-11 Edwin S. Kite , Axel Noblet

Ongoing and future space missions aim to identify potentially habitable planets in our Solar System and beyond. Planetary habitability is determined not only by a planet's current stellar insolation and atmospheric properties, but also by…

地球与行星天体物理 · 物理学 2018-09-12 Jun Yang , Feng Ding , Ramses M. Ramirez , W. R. Peltier , Yongyun Hu , Yonggang Liu

Here, we evaluate our nearest planetary neighbor, Venus, as an exemplar of the runaway greenhouse state that bounds the inner edge of the habitable zone. Despite its current hellish surface environment, Venus may once have been habitable…

地球与行星天体物理 · 物理学 2018-04-18 Giada Arney , Stephen Kane

Two habitable planetary states are proposed: an aqua planet like the Earth and a land planet that has a small amount of water. Land planets keep liquid water under larger solar radiation compared to aqua planets. Water loss may change an…

地球与行星天体物理 · 物理学 2015-10-28 T. Kodama , H. Genda , Y. Abe , K. J. Zahnle

The aim of my dissertation is to investigate habitability in extra-Solar Systems. Most of the time, only planets are considered as possible places where extraterrestrial life can emerge and evolve, however, their moons could be inhabited,…

地球与行星天体物理 · 物理学 2017-04-26 Vera Dobos
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