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The study of the origin of life on Earth has been broadened due to panspermia models that suggest that early life may have been transferred between planets. Mars likely once had conditions that could support life, and it is interesting…

地球与行星天体物理 · 物理学 2026-05-18 Gregory M. Davis , Jonathan Horner , Bradley D. Carter , Stephen C Marsden

Aims. An asymmetric dust cloud was detected around the Moon by the Lunar Dust Experiment on board the Lunar Atmosphere and Dust Environment Explorer mission. We investigate the dynamics of the grains that escape the Moon and their…

地球与行星天体物理 · 物理学 2022-04-05 Kun Yang , Jürgen Schmidt , Weiming Feng , Xiaodong Liu

The deep (~100 km) ocean of Europa, Jupiter's moon, covered by a thick icy shell, is one of the most probable places in the solar system to find extraterrestrial life. Yet, its ocean dynamics and its interaction with the ice cover have…

地球与行星天体物理 · 物理学 2022-01-19 Yosef Ashkenazy , Eli Tziperman

Previous estimates of the annual mean surface temperature of Jupiter's moon, Europa, neglected the effect of the eccentricity of Jupiter's orbit around the Sun, the effect of the emissivity and heat capacity of Europa's ice, the effect of…

地球与行星天体物理 · 物理学 2019-06-05 Yosef Ashkenazy

We shortly discuss the observable consequences of the two hypotheses about the origin of life on Earth and Mars: the Lithopanspermia (Mars to Earth or viceversa) and the origin from a unique progenitor, that for Earth is called LUCA (the…

地球与行星天体物理 · 物理学 2010-06-02 Giuseppe Galletta , Giulio Bertoloni , Maurizio D'Alessandro

Jupiter's icy moons are believed to host subsurface liquid oceans, and among them, Europa stands out as one of the most promising candidates for extraterrestrial life. Yet, the processes driving oceanic flows beneath its ice shell, as well…

地球与行星天体物理 · 物理学 2025-09-16 Florentin Daniel , Ludovic Petitdemange , Christophe Gissinger

We explore the likelihood that early remains of Earth, Mars, and Venus have been preserved on the Moon in high enough concentrations to motivate a search mission. During the Late Heavy Bombardment, the inner planets experienced frequent…

天体物理学 · 物理学 2009-11-07 John C. Armstrong , Llyd E. Wells , Guillermo Gonzalez

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

Roth et al (2014a) reported evidence for plumes of water venting from a southern high latitude region on Europa - spectroscopic detection of off-limb line emission from the dissociation products of water. Here, we present Hubble Space…

地球与行星天体物理 · 物理学 2016-10-05 W. B. Sparks , K. P. Hand , M. A. McGrath , E. Bergeron , M. Cracraft , S. E. Deustua

The outer solar system may provide a potential habitat for extraterrestrial life. Remote sensing data from the Galileo spacecraft suggest that the jovian icy moons, Europa, Ganymede, and possibly Callisto, may harbor liquid water oceans…

地球与行星天体物理 · 物理学 2015-06-23 Jun Kimura , Norio Kitadai

We investigate the prospects for the past or current existence of habitable conditions deep underneath the surfaces of the Moon and Mars as well as generic bound and free-floating extrasolar rocky objects. We construct a simple model that…

地球与行星天体物理 · 物理学 2020-09-23 Manasvi Lingam , Abraham Loeb

Europa's subsurface ocean is a potential candidate for life in the outer solar system. It is thought that plumes may exist which eject ocean material out into space, which may be detected by a spacecraft flyby. Previous work on the…

地球与行星天体物理 · 物理学 2023-03-15 Rowan Dayton-Oxland , Hans L. F. Huybrighs , Thomas O. Winterhalder , Arnaud Maheiux , David Goldstein

Aims. Particles ejected from the lunar surface via hypervelocity impacts form a torus between the Earth and the Moon. According to our previous study (Yang et al., A\&A, 659, A120), among them about $2.3\times10^{-4}\,\mathrm{kg/s}$…

地球与行星天体物理 · 物理学 2025-07-22 Kun Yang , Yu Jiang , Youpeng Liang , Xiaodong Liu

Much of the geologic activity preserved on Europa's icy surface has been attributed to tidal deformation, mainly due to Europa's eccentric orbit. Although the surface is geologically young (30 - 80 Myr), there is little information as to…

地球与行星天体物理 · 物理学 2015-06-24 Alyssa R. Rhoden , Terry A. Hurford , Lorenz Roth , Kurt Retherford

Potential microbial contamination of Martian moons, Phobos and Deimos, which can be brought about by transportation of Mars ejecta produced by meteoroid impacts on the Martian surface, has been comprehensively assessed in a statistical…

Recent findings suggest Mars may have been a clement environment for the emergence of life, and may even have compared favorably to Earth in this regard. These findings have revived interest in the hypothesis that prebiotically important…

地球与行星天体物理 · 物理学 2017-08-02 Sukrit Ranjan , Robin D. Wordsworth , Dimitar D. Sasselov

Identification of habitable planets beyond our solar system is a key goal of current and future space missions. Yet habitability depends not only on the stellar irradiance, but equally on constituent parts of the planetary atmosphere. Here…

地球与行星天体物理 · 物理学 2020-06-11 Ian A. Boutle , Manoj Joshi , F. Hugo Lambert , Nathan J. Mayne , Duncan Lyster , James Manners , Robert Ridgway , Krisztian Kohary

Material from the surface of a planet can be ejected into space by a large impact, and could carry primitive life forms with it. We performed n-body simulations of such ejecta to determine where in the Solar System rock from Earth and Mars…

地球与行星天体物理 · 物理学 2015-06-17 R. J. Worth , Steinn Sigurdsson , Christopher H. House

Motivated by recent research of aging in E. coli, we explore the effects of aging on bacterial fitness. The disposable soma theory of aging was developed to explain how differences in lifespans and aging rates could be linked to life…

种群与进化 · 定量生物学 2007-05-23 Leah R. Johnson , Marc Mangel

From modeling the evolution of disks of planetesimals under the influence of planets, it has been shown that the mass of water delivered to the Earth from beyond Jupiter's orbit could be comparable to the mass of terrestrial oceans. A…

地球与行星天体物理 · 物理学 2020-03-24 M. Ya. Marov , S. I. Ipatov
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