Epilogue: Paradigms, Problems, and Predictions

Author(s):  
John Chambers ◽  
Jacqueline Mitton

This concluding chapter talks about how astronomers and space agencies in dozens of countries are helping to see the solar system as never before, transforming points of light into real worlds, and even bringing samples of those worlds back to Earth. At the same time, the stunning discovery of hundreds of other planetary systems in the galaxy has provided a powerful stimulus to understand how planetary systems form and evolve, and to find out what makes one system different from another. Moreover, in 2010, NASA announced its latest science plan. One of the key goals for NASA's future planetary science program is to learn how the Sun's family began and how it has changed over time. The chapter argues that the rapid pace of recent developments makes now a good time to take stock of what scholars know, even though the story is still incomplete.

Author(s):  
Karel Schrijver

How many planetary systems formed before our’s did, and how many will form after? How old is the average exoplanet in the Galaxy? When did the earliest planets start forming? How different are the ages of terrestrial and giant planets? And, ultimately, what will the fate be of our Solar System, of the Milky Way Galaxy, and of the Universe around us? We cannot know the fate of individual exoplanets with great certainty, but based on population statistics this chapter sketches the past, present, and future of exoworlds and of our Earth in general terms.


2010 ◽  
Vol 6 (S276) ◽  
pp. 304-307
Author(s):  
Melvyn B. Davies

AbstractMany stars are formed in some form of cluster or association. These environments can have a much higher number density of stars than the field of the galaxy. Such crowded places are hostile environments: a large fraction of initially single stars will undergo close encounters with other stars or exchange into binaries. We describe how such close encounters and exchange encounters will affect the properties of a planetary system around a single star. We define singletons as single stars which have never suffered close encounters with other stars or spent time within a binary system. It may be that planetary systems similar to our own solar system can only survive around singletons. Close encounters or the presence of a stellar companion will perturb the planetary system, leading to strong planet-planet interactions, often leaving planets on tighter and more eccentric orbits. Thus, planetary systems which initially resembled our own solar system may later more closely resemble the observed extrasolar planetary systems.


Author(s):  
David A. Rothery

The first definite discovery of a planet around another star—an ‘exoplanet’—was made in 1995. We now know of more than 1,000 stars with exoplanets. In our Solar System, moons are considerably more numerous than planets, so it would be surprising if exomoons did not outnumber exoplanets. Only a few exceptional exoplanets have been seen by direct imaging and any exomoons are presently well below the visibility threshold. ‘Moons in other planetary systems: exomoons’ considers why exomoons matter. If hydrothermal vents on ocean floors really are a good place for life to begin, then icy exomoons with internal oceans throughout the galaxy could host microbial life.


2004 ◽  
Vol 202 ◽  
pp. 458-461 ◽  
Author(s):  
L. V. Ksanfomality

N = RsfpneflfifcL. This well known Drake equation denoting the number N of civilizations in the Galaxy, includes a factor fp that is the fraction of stars that have planetary systems, and another factor ne that is the mean number of planets suitable for life. The latter is usually understood as the number of planets within the habitable zone. When the Solar system remained a unique object of its kind the sense of fp and ne seemed to be clear. There is now a limited statistic in hand about the features of other planetary systems, permitting a rough estimation of fp and ne (based on the list of 32 star companions, compiled by G. Marcy, 14.02.2000).


Author(s):  
Karel Schrijver

Where centuries ago one could be burned at the stake for speculating about distant worlds, the modern scientific method has made us realize that there are planetary systems around most of the over a hundred billion stars in the Galaxy. Learning that the Earth was not the center of the Solar System represented a true revolution in our thinking, but the recent insight that the Solar System is but one of an immense number of similar systems was smoothly adopted by our culture, which had already been exposed to many fictional worlds over the preceding dedades. This introductory chapter describes these changes, woven into the story of how astrophysics has grown from the work of a few isolated individuals into a globe-spanning, fast-publishing enterprise with state-of-the-art observatories, from master–pupil teaching to university-based education, and from learning from often ancient books to modern observation-based investigations.


2021 ◽  
Author(s):  
James Head

<p>The Earth’s Moon is a cornerstone and keystone in the understanding of the origin and evolution of the terrestrial, Earth-like planets.  It is a cornerstone in that most of the other paradigms for the origin, modes of crustal formation (primary, secondary and tertiary), bombardment history, role of impact craters and basins in shaping early planetary surfaces and fracturing and modifying the crust and upper mantle, volcanism and the formation of different types of secondary crust, and petrogenetic models where no samples are available, all have a fundamental foundation in lunar science.  The Moon is a keystone in that knowledge of the Moon holds upright the arch of our understand of the terrestrial planets. It is thus imperative to dedicate significant resources to the continued robotic and human exploration of this most accessible of other terrestrial planetary bodies, and to use this cornerstone and keystone as a way to frame critical questions about the Solar System as a whole, and to explore other planetary bodies to modify and strengthen the lunar paradigm.   </p> <p>What is the legacy, the long-term impact of our efforts? The Apollo Lunar Exploration Program revealed the Earth as a planet, showed the inextricable links of the Earth-Moon system, and made the Solar System our neighborhood. We now ask: What are our origins and where are we heading?: We seek to understand the origin and evolution of the Moon, the Moon’s links to the earliest history of Earth, and its lessons for exploration and understanding of Mars and other terrestrial planets. A basis for our motivation is the innate human qualities of curiosity and exploration, and the societal/species-level need to heed Apollo 16 Commander John Young’s warning that “Single-planet species don’t survive!”. These perspectives impel us to learn the lessons of off-Earth, long-term, long-distance resupply and self-sustaining presence, in order to prepare for the exploration of Mars and other Solar System destinations. </p> <p>Key questions in this lunar exploration endeavor based on a variety of studies and analyses (1-3) include:</p> <p>-How do planetary systems form and evolve over time and when did major events in our Solar System occur?</p> <p>How did planetary interiors differentiate and evolve through time, and how are interior processes expressed through surface-atmosphere interactions?</p> <p>-What processes shape planetary surfaces and how do these surfaces record Solar System history?</p> <p>-How do worlds become habitable and how is habitability sustained over time?</p> <p>-Why are the atmospheres and climates of planetary bodies so diverse, and how did they evolve over time?</p> <p>-Is there life elsewhere in the Solar System?</p> <p>Specific lunar goals and objectives will be outlined in this broad planetary science context.</p> <p> </p> <p>References: 1. Carle Pieters et al. (2018) http://www.planetary.brown.edu/pdfs/5480.pdf, 2. Lunar Exploration Analysis Group, https://www.lpi.usra.edu/leag/. 3) Erica Jawin et al. Planetary Science Priorities for the Moon in the Decade 2023-2033: Lunar Science is Planetary Science.</p>


Author(s):  
John Chambers ◽  
Jacqueline Mitton

Science is a voyage of discovery, a lasting quest to find the truth, with many twists and turns along the way. Planetary science—the study of how planetary systems form and evolve—is no exception. In fact, a great deal has happened in the few short years since we first wrote this book. Many new discoveries have been made by space missions, by astronomers using telescopes, and by researchers in laboratories using computers. These discoveries have naturally influenced the way we think about our solar system and how it formed. Some discoveries have confirmed previous predictions while others have forced researchers to modify their theories. Occasionally, a discovery has thrown open a new window, greatly increasing the range of possible scenarios. This afterword is a brief tour of some recent discoveries and what they might mean....


2015 ◽  
Vol 11 (A29A) ◽  
pp. 3-5
Author(s):  
Alessandro Morbidelli ◽  
Nader Haghighipour

The past few years have witnessed a large increase in the number of extrasolar planets. Thanks to successful surveys from the ground and from space, there are now over 1000 confirmed exoplanets and more then 3000 planetary candidates. More than 130 of these systems host multiple planets. Many of these systems demonstrate physical and orbital characteristics fundamentally different from those of our solar system. The challenges associated with the diversity of planetary systems have raised many interesting questions on planet formation and orbital dynamics.


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