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相关论文: Is Interstellar travel to an exoplanet Possible?

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The existence of a positive and possibly varying Lambda-term opens a much wider field of possibilities for the future of our Universe than it was usually thought before. Definite predictions may be made for finite (though very large)…

天体物理学 · 物理学 2008-11-26 A. A. Starobinsky

Today, we know ~4330 exoplanets orbiting their host stars in ~3200 planetary systems. The diversity of these exoplanets is large, and none of the known exoplanets is a twin to any of the solar system planets, nor is any of the known…

地球与行星天体物理 · 物理学 2021-12-15 Christiane Helling

Thousands of planets beyond our solar system have been discovered to date, dozens of which are rocky in composition and are orbiting within the circumstellar habitable zone of their host star. The next frontier in life detection beyond our…

It is commonly asserted that superluminal particle motion can enable backward time travel, but little has been written providing details. It is shown here that the simplest example of a "closed loop" event -- a twin paradox scenario where a…

科普物理 · 物理学 2015-09-10 Robert J. Nemiroff , David M. Russell

Two decades ago, astronomers began detecting planets orbiting stars other than our Sun, so-called exoplanets. Since that time, the rate of detections and the sensitivity to ever-smaller planets has improved dramatically with several…

地球与行星天体物理 · 物理学 2014-05-08 David M. Kipping

Hot giant exoplanets are very exotic objects with no equivalent in the Solar System that allow us to study the behavior of atmospheres under extreme conditions. Their thermal and chemical day--night dichotomies associated with extreme wind…

地球与行星天体物理 · 物理学 2023-01-31 William Pluriel

With the discovery of hundreds of exoplanets and a potentially huge number of Earth-like planets waiting to be discovered, the conditions for their habitability have become a focal point in exoplanetary research. The classical picture of…

地球与行星天体物理 · 物理学 2015-06-22 M. Guedel , R. Dvorak , N. Erkaev , J. Kasting , M. Khodachenko , H. Lammer , E. Pilat-Lohinger , H. Rauer , I. Ribas , B. E. Wood

Extrasolar planets and belts of debris orbiting post-main-sequence single stars may become unbound as the evolving star loses mass. In multiple star systems, the presence or co-evolution of the additional stars can significantly complicate…

地球与行星天体物理 · 物理学 2015-06-04 Dimitri Veras , Christopher A. Tout

Exoplanet surveys have confirmed one of humanity's (and all teenagers') worst fears: we are weird. If our Solar System were observed with present-day Earth technology -- to put our system and exoplanets on the same footing -- Jupiter is the…

地球与行星天体物理 · 物理学 2022-02-23 Sean N. Raymond , Andre Izidoro , Alessandro Morbidelli

The potential existence of a distant planet ("Planet Nine") in the Solar system has prompted a re-think about the evolution of planetary systems. As the Sun transitions from a main sequence star into a white dwarf, Jupiter, Saturn, Uranus…

地球与行星天体物理 · 物理学 2016-09-07 Dimitri Veras

Given the fact that Earth is so far the only place in the Milky Way galaxy known to harbor life, the question arises of whether the solar system is in any way special. To address this question, I compare the solar system to the many…

太阳与恒星天体物理 · 物理学 2018-01-17 Mario Livio

The importance of understanding the current and historical galactic environments of cool stars is discussed. The penetration of interstellar gas into a stellar astrosphere is a function of the interaction of the star with the interstellar…

天体物理学 · 物理学 2007-05-23 Priscilla C. Frisch

This paper outlines astrophysical issues related to the long term fate of the universe. We consider the evolution of planets, stars, stellar populations, galaxies, and the universe itself over time scales which greatly exceed the current…

天体物理学 · 物理学 2008-11-26 Fred C. Adams , Gregory Laughlin

The habitability of the surface of any planet is determined by a complex evolution of its interior, surface, and atmosphere. The electromagnetic and particle radiation of stars drive thermal, chemical and physical alteration of planetary…

Given the inexorable increase in the Sun's luminosity, Earth will exit the habitable zone in ~1 Gyr. There is a negligible chance that Earth's orbit will change during that time through internal Solar System dynamics. However, there is a…

地球与行星天体物理 · 物理学 2023-11-22 Sean N. Raymond , Nathan A. Kaib , Franck Selsis , Herve Bouy

Stars do not form in isolation but together with other stars, and often in a clustered environment. Depending on the initial conditions in these environments, such as initial density and substructure, the distances of encounters between…

地球与行星天体物理 · 物理学 2024-08-01 Christina Schoettler , James E. Owen

The majority of stars form in star clusters and many are thought to have planetary companions. We demonstrate that multi-planet systems are prone to instabilities as a result of frequent stellar encounters in these star clusters much more…

地球与行星天体物理 · 物理学 2015-06-15 W. Hao , M. B. N. Kouwenhoven , R. Spurzem

Atmospheric mass loss is thought to have strongly shaped the sample of close-in exoplanets. These atmospheres should be lost isotropically, leading to no net migration on the planetary orbit. However, strong stellar winds can funnel the…

地球与行星天体物理 · 物理学 2024-12-02 Benjamin Hanf , Will Kincaid , Hilke Schlichting , Livan Cappiello , Daniel Tamayo

The possibility that extraterrestrial intelligences (ETIs) could be hostile to humanity has been raised as a reason to avoid even trying to contact ETIs. However, there is a distinct shortage of analytical discussion about the risks of an…

科普物理 · 物理学 2013-02-05 Janne M. Korhonen