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The early start to life naively suggests that abiogenesis is a rapid process on Earth-like planets. However, if evolution typically takes ~4Gyr to produce intelligent life-forms like us, then the limited lifespan of Earth's biosphere…

地球与行星天体物理 · 物理学 2025-04-09 David Kipping

Life emerged on the Earth within the first quintile of its habitable window, but a technological civilization did not blossom until its last. Efforts to infer the rate of abiogenesis, based on its early emergence, are frustrated by the…

地球与行星天体物理 · 物理学 2022-06-08 David Kipping

One of the most interesting unsolved questions in science today is the question of life on other planets. At the present time it is safe to say that we do not have much of an idea as to whether life is common or exceedingly rare in the…

科普物理 · 物理学 2008-08-21 Brendon J. Brewer

Over the past two decades, enormous advances in the detection of exoplanets have taken place. Currently, we have discovered hundreds of earth-sized planets, several of them within the habitable zone of their star. In the coming years, the…

地球与行星天体物理 · 物理学 2018-12-05 Enric Palle

A habitable zone of a star is defined as a range of orbits within which a rocky planet can support liquid water on its surface. The most intriguing question driving the search for habitable planets is whether they host life. But is the age…

地球与行星天体物理 · 物理学 2016-03-24 M. Safonova , J. Murthy , Yu. A. Shchekinov

Life arose on Earth sometime in the first few hundred million years after the young planet had cooled to the point that it could support water-based organisms on its surface. The early emergence of life on Earth has been taken as evidence…

地球与行星天体物理 · 物理学 2015-03-19 David S. Spiegel , Edwin L. Turner

A simple stochastic model for evolution, based upon the need to pass a sequence of n critical steps (Carter 1983, Watson 2008) is applied to both terrestrial and extraterrestrial origins of life. In the former case, the time at which humans…

地球与行星天体物理 · 物理学 2011-04-22 Michael McCabe , Holly Lucas

Solar X-ray and UV radiation (0.1-320 nm) received at Earth's surface is an important aspect of the circumstances under which life formed on Earth. The quantity that is received depends on two main variables: the emission of radiation by…

天体物理学 · 物理学 2008-11-26 I. Cnossen , J. Sanz-Forcada , F. Favata , O. Witasse , T. Zegers , N. F. Arnold

Despite great advances in our understanding of the formation of the Solar System, the evolution of the Earth, and the chemical basis for life, we are not much closer than the ancient Greeks to an answer of whether life has arisen and…

天体物理学 · 物理学 2007-05-23 Eric Gaidos , Franck Selsis

An extrapolation of the genetic complexity of organisms to earlier times suggests that life began before the Earth was formed. Life may have started from systems with single heritable elements that are functionally equivalent to a…

综合物理 · 物理学 2013-04-12 Alexei A. Sharov , Richard Gordon

Is life most likely to emerge at the present cosmic time near a star like the Sun? We consider the habitability of the Universe throughout cosmic history, and conservatively restrict our attention to the context of "life as we know it" and…

宇宙学与河外天体物理 · 物理学 2016-11-28 Abraham Loeb

The biosignatures of life on Earth do not remain static, but change considerably over the planet's habitable lifetime. Earth's future biosphere, much like that of the early Earth, will consist of predominantly unicellular microorganisms due…

地球与行星天体物理 · 物理学 2015-06-17 Jack T. O'Malley-James , Charles S. Cockell , Jane S. Greaves , John. A. Raven

A recent study reported that there is evidence life may have originated prior to the formation of the Earth. That conclusion was based on a regression analysis of a certain data set involving evolution of functional genome size across major…

种群与进化 · 定量生物学 2013-06-04 Caren Marzban , Raju Viswanathan , Ulvi Yurtsever

Life appears to have emerged relatively quickly on the Earth, a fact sometimes used to justify a high rate of spontaneous abiogenesis ($\lambda$) among Earth-like worlds. Conditioned upon a single datum - the time of earliest evidence for…

地球与行星天体物理 · 物理学 2018-12-26 Jingjing Chen , David Kipping

With recent observations confirming exoplanets orbiting white dwarfs, there is growing interest in exploring and quantifying the habitability of temperate rocky planets around white dwarfs. In this work, the limits of the habitable zone of…

地球与行星天体物理 · 物理学 2024-12-02 Caldon T. Whyte , L. H. Quiroga-Nuñez , Manasvi Lingam , Paola Pinilla

Planet Earth has evolved from an entirely anoxic planet with possibly a different tectonic regime to the oxygenated world with horizontal plate tectonics that we know today. For most of this time, Earth has been inhabited by a purely…

地球与行星天体物理 · 物理学 2024-04-25 Eva E. Stüeken , Stephanie L. Olson , Eli Moore , Bradford J. Foley

The habitable zone is the circumstellar region in which a terrestrial-mass planet with an atmosphere can sustain liquid water on its surface. However, despite the usefulness of this concept, it is being found to be increasingly limiting in…

科普物理 · 物理学 2020-08-05 Ian von Hegner

The probability that life spontaneously emerges in a suitable environment (abiogenesis) is one of the major unknowns in astrobiology. Assessing its value is impeded by the lack of an accepted theory for the origin of life, and is further…

地球与行星天体物理 · 物理学 2023-05-10 Amedeo Balbi , Manasvi Lingam

Any search for present or past life beyond Earth should consider the initial processes and related environmental controls that might have led to its start. As on Earth, such an understanding lies well beyond how simple organic molecules…

The oxygenation of Earth's atmosphere 2.3 billion years ago, which on exoplanets is expected to be most detectable via the UV ozone feature at $\sim$0.25 $\mu$m, is often regarded as a sign of the emergence of photosynthetic life. On…

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