Cosmic Archaeology

2017 ◽  
Author(s):  
John Chambers ◽  
Jacqueline Mitton
Keyword(s):  
Solar System ◽  
Interstellar Space ◽  
Human Society ◽  
The Past ◽  
History Of ◽  
Habitable Planet

This chapter discusses the process of how the solar system had to take form from the near nothingness of interstellar space. Scientists pondering the history of the solar system are much like archaeologists sifting through the sands of Egypt. They bring different methods and tools to the job, but both strive to glean as much as possible from precious relics from the past, and combine this with information deduced from the current surroundings. Deciphering the history of the solar system is archaeology on a grand scale. For human society to arise, species needed to evolve from those that went before. Prior to this, life had to appear on a suitably habitable planet orbiting a long-lived star.

Stellar Evolution

1962 ◽  
Vol 11 (02) ◽  
pp. 137-143
Author(s):  
M. Schwarzschild
Keyword(s):  
Solar System ◽  
Stellar Evolution ◽  
Space Craft ◽  
New Techniques ◽  
Substantial Body ◽  
Individual Stars ◽  
The Past ◽  
Evolution Of Galaxies ◽  
History Of ◽  
Fast Flow

It is perhaps one of the most important characteristics of the past decade in astronomy that the evolution of some major classes of astronomical objects has become accessible to detailed research. The theory of the evolution of individual stars has developed into a substantial body of quantitative investigations. The evolution of galaxies, particularly of our own, has clearly become a subject for serious research. Even the history of the solar system, this close-by intriguing puzzle, may soon make the transition from being a subject of speculation to being a subject of detailed study in view of the fast flow of new data obtained with new techniques, including space-craft.

scholarly journals No evidence for interstellar planetesimals trapped in the Solar system

2020 ◽  
Vol 497 (1) ◽  
pp. L46-L49 ◽  
Author(s):  
A Morbidelli ◽  
K Batygin ◽  
R Brasser ◽  
S N Raymond
Keyword(s):  
Solar System ◽  
Oort Cloud ◽  
Giant Planets ◽  
Asteroid Belt ◽  
Interstellar Space ◽  
Fast Decay ◽  
Early Solar System ◽  
The Past ◽  
Solar System Bodies ◽  
Main Asteroid Belt

ABSTRACT In two recent papers published in MNRAS, Namouni and Morais claimed evidence for the interstellar origin of some small Solar system bodies, including: (i) objects in retrograde co-orbital motion with the giant planets and (ii) the highly inclined Centaurs. Here, we discuss the flaws of those papers that invalidate the authors’ conclusions. Numerical simulations backwards in time are not representative of the past evolution of real bodies. Instead, these simulations are only useful as a means to quantify the short dynamical lifetime of the considered bodies and the fast decay of their population. In light of this fast decay, if the observed bodies were the survivors of populations of objects captured from interstellar space in the early Solar system, these populations should have been implausibly large (e.g. about 10 times the current main asteroid belt population for the retrograde co-orbital of Jupiter). More likely, the observed objects are just transient members of a population that is maintained in quasi-steady state by a continuous flux of objects from some parent reservoir in the distant Solar system. We identify in the Halley-type comets and the Oort cloud the most likely sources of retrograde co-orbitals and highly inclined Centaurs.

scholarly journals Hydrogen molecular ions and the violent birth of the Solar System

2019 ◽  
Vol 377 (2154) ◽  
pp. 20180403 ◽  
Author(s):  
Cecilia Ceccarelli ◽  
Cecile Favre ◽  
Ana López-Sepulcre ◽  
Francesco Fontani
Keyword(s):  
Cosmic Rays ◽  
Solar System ◽  
Past History ◽  
Classical Problem ◽  
Galactic Cosmic Rays ◽  
Energetic Particles ◽  
Molecular Ions ◽  
Observational Constraints ◽  
The Past ◽  
History Of

Many pieces of evidence indicate that the Solar System youth was marked by violent processes: among others, high fluxes of energetic particles (greater than or equal to 10 MeV) are unambiguously recorded in meteoritic material, where an overabundance of the short-lived 10 Be products is measured. Several hypotheses have been proposed to explain from where these energetic particles originate, but there is no consensus yet, mostly because of the scarcity of complementary observational constraints. In general, the reconstruction of the past history of the Solar System is best obtained by simultaneously considering what we know of it and of similar systems nowadays in formation. However, when it comes to studying the presence of energetic particles in young forming stars, we encounter the classical problem of the impossibility of directly detecting them toward the emitting source (analogously to what happens to galactic cosmic rays). Yet, exploiting the fact that energetic particles, such as cosmic rays, create H 3 + and that an enhanced abundance of H 3 + causes dramatic changes on the overall gas chemical composition, we can indirectly estimate the flux of energetic particles. This contribution provides an overview of the search for solar-like protostars permeated by energetic particles and the discovery of a protocluster, OMC-2 FIR4, where the phenomenon is presently occurring. This article is part of a discussion meeting issue ‘Advances in hydrogen molecular ions: H 3 + , H 5 + and beyond’.

scholarly journals Comet C/2018 V1 (Machholz–Fujikawa–Iwamoto): dislodged from the Oort Cloud or coming from interstellar space?

2019 ◽  
Vol 489 (1) ◽  
pp. 951-961 ◽  
Author(s):  
C de la Fuente Marcos ◽  
R de la Fuente Marcos
Keyword(s):  
Solar System ◽  
Dynamical Evolution ◽  
Oort Cloud ◽  
Interstellar Space ◽  
The Sun ◽  
The Past ◽  
Using Data ◽  
To Receive ◽  
Practical Feasibility

ABSTRACT The chance discovery of the first interstellar minor body, 1I/2017 U1 (‘Oumuamua), indicates that we may have been visited by such objects in the past and that these events may repeat in the future. Unfortunately, minor bodies following nearly parabolic or hyperbolic paths tend to receive little attention: over 3/4 of those known have data-arcs shorter than 30 d and, consistently, rather uncertain orbit determinations. This fact suggests that we may have observed interstellar interlopers in the past, but failed to recognize them as such due to insufficient data. Early identification of promising candidates by using N-body simulations may help in improving this situation, triggering follow-up observations before they leave the Solar system. Here, we use this technique to investigate the pre- and post-perihelion dynamical evolution of the slightly hyperbolic comet C/2018 V1 (Machholz–Fujikawa–Iwamoto) to understand its origin and relevance within the context of known parabolic and hyperbolic minor bodies. Based on the available data, our calculations suggest that although C/2018 V1 may be a former member of the Oort Cloud, an origin beyond the Solar system cannot be excluded. If extrasolar, it might have entered the Solar system from interstellar space at low relative velocity with respect to the Sun. The practical feasibility of this alternative scenario has been assessed within the kinematic context of the stellar neighbourhood of the Sun, using data from Gaia second data release, and two robust solar sibling candidates have been identified. Our results suggest that comets coming from interstellar space at low heliocentric velocities may not be rare.

scholarly journals Drawing on the Past to Shape the Future of Synthetic Yeast Research

2020 ◽  
Vol 21 (19) ◽  
pp. 7156
Author(s):  
Thomas A. Dixon ◽  
Isak S. Pretorius
Keyword(s):  
History Of Science ◽  
Human Society ◽  
The Past ◽  
Environmental Recovery ◽  
Collaborative Innovation ◽  
The World ◽  
Technological Developments ◽  
History Of ◽  
Synthetic Genomics ◽  
Global Events

Some years inspire more hindsight reflection and future-gazing than others. This is even more so in 2020 with its evocation of perfect vision and the landmark ring to it. However, no futurist can reliably predict what the world will look like the next time that a year’s first two digits will match the second two digits—a numerical pattern that only occurs once in a century. As we leap into a new decade, amid uncertainties triggered by unforeseen global events—such as the outbreak of a worldwide pandemic, the accompanying economic hardship, and intensifying geopolitical tensions—it is important to note the blistering pace of 21st century technological developments indicate that while hindsight might be 20/20, foresight is 50/50. The history of science shows us that imaginative ideas, research excellence, and collaborative innovation can, for example, significantly contribute to the economic, cultural, social, and environmental recovery of a post-COVID-19 world. This article reflects on a history of yeast research to indicate the potential that arises from advances in science, and how this can contribute to the ongoing recovery and development of human society. Future breakthroughs in synthetic genomics are likely to unlock new avenues of impactful discoveries and solutions to some of the world’s greatest challenges.

scholarly journals 15. Physical Study of Comets, Minor Planets and Meteorites

1979 ◽  
Vol 17 (1) ◽  
pp. 73-102
Author(s):  
N.B. Richter
Keyword(s):  
Solar System ◽  
Considerable Increase ◽  
Solar Nebula ◽  
Past History ◽  
Minor Planets ◽  
The Past ◽  
Physical Study ◽  
History Of

Comets, minor planets and meteorites provide us with valuable information about the past history of the solar system. They belong to the most primitive samples of the primordial solar nebula. Over the past years, we can record a considerable increase of interest in these bodies.

Marxist Historiography Today

2007 ◽  
Author(s):  
Eric Hobsbawm
Keyword(s):  
Social Sciences ◽  
Human Activities ◽  
Human Society ◽  
The Past ◽  
The Social ◽  
The World ◽  
History Of ◽  
New Perspective ◽  
Methodology Of Science ◽  
The Way

This chapter discusses Marxist historiography in the present times. In the interpretation of the world nowadays, there has been a rise in the so-called anti-Rankean reaction in history, of which Marxism is an important but not always fully acknowledged element. This movement challenged the positivist belief that the objective structure of reality was self-explanatory, and that all that was needed was to apply the methodology of science to it and explain why things happened the way they did. This movement also brought together history with the social sciences, therefore turning it into part of a generalizing discipline capable of explaining transformations of human society in the course of its past. This new perspective on the past is a return to ‘total history’, in which the focus is not merely on the ‘history of everything’ but history as an indivisible web wherein all human activities are interconnected.

scholarly journals Albania, a Wonderful Example of Coexistence and Religious Tolerance

2015 ◽  
Vol 4 (1) ◽  
pp. 153
Author(s):  
Evalda Jera
Keyword(s):  
Religious Beliefs ◽  
External Factors ◽  
Religious Communities ◽  
Human Society ◽  
Religious Tolerance ◽  
Factors Affecting ◽  
The Past ◽  
National Tradition ◽  
History Of

If we refear to the history of humanity we note that the tolerance of human society is too early, it was born togather with the man. It should be noted that religious beliefs in Albania are and has always been characterized by a strong feeling and a sincere harmony which is reflected in the relations between people with different religious beliefs, as well as between religious people and atheists. Albanians are both Christian and Muslim, Catholic, Orthodox, and Bektashi. For centuries territories populated by Albanians has been remarkable for a unique interfaith tolerance. Religion has never been in the past and is not now a source of conflict in society. In the history of the Albanian religious, communities have always succeeded with a peacefully cooperation. This tolerance stems from the awareness of the Albanians that they belong to the same nation having a strong ethnic identity regardless of external factors affecting the determination of Albanians from other religions. In the Albanian national tradition, religious tolerance is one of the main characteristics of Albanian people morality . The interest of the nation has always been primary in relation to religious matters, it is first of all beeing Albanian. Albanian as well said Pasko Vasa in the nineteenth century "never churches and mosques can separate usbecouse the religion of Albanians is Albanianhood" and so, because of this we create a big example, a wonderful cooperation, a peaceful atmosphere and open the way for peace and friendship between people not only in Albani but worldwide.

scholarly journals Constraining the Evolutionary History of the Moon and the Inner Solar System: A Case for New Returned Lunar Samples

2019 ◽  
Vol 215 (8) ◽  
Author(s):  
Romain Tartèse ◽  
Mahesh Anand ◽  
Jérôme Gattacceca ◽  
Katherine H. Joy ◽  
James I. Mortimer ◽  
...  
Keyword(s):  
Solar System ◽  
Large Scale ◽  
Lunar Regolith ◽  
The Moon ◽  
Planetary Body ◽  
The Past ◽  
Lunar Samples ◽  
History Of ◽  
Magma Oceans ◽  
Robotic Missions

AbstractThe Moon is the only planetary body other than the Earth for which samples have been collected in situ by humans and robotic missions and returned to Earth. Scientific investigations of the first lunar samples returned by the Apollo 11 astronauts 50 years ago transformed the way we think most planetary bodies form and evolve. Identification of anorthositic clasts in Apollo 11 samples led to the formulation of the magma ocean concept, and by extension the idea that the Moon experienced large-scale melting and differentiation. This concept of magma oceans would soon be applied to other terrestrial planets and large asteroidal bodies. Dating of basaltic fragments returned from the Moon also showed that a relatively small planetary body could sustain volcanic activity for more than a billion years after its formation. Finally, studies of the lunar regolith showed that in addition to containing a treasure trove of the Moon’s history, it also provided us with a rich archive of the past 4.5 billion years of evolution of the inner Solar System. Further investigations of samples returned from the Moon over the past five decades led to many additional discoveries, but also raised new and fundamental questions that are difficult to address with currently available samples, such as those related to the age of the Moon, duration of lunar volcanism, the lunar paleomagnetic field and its intensity, and the record on the Moon of the bombardment history during the first billion years of evolution of the Solar System. In this contribution, we review the information we currently have on some of the key science questions related to the Moon and discuss how future sample-return missions could help address important knowledge gaps.

scholarly journals Dynamical History of the Oort Cloud

1989 ◽  
Vol 116 (1) ◽  
pp. 463-486
Author(s):  
Paul R. Weissman
Keyword(s):  
Solar System ◽  
Interstellar Dust ◽  
Temporal Variations ◽  
Galactic Cosmic Rays ◽  
Oort Cloud ◽  
Interstellar Space ◽  
Satellite Systems ◽  
Short Period ◽  
History Of ◽  
The Impact

AbstractDynamical studies during the past decade have resulted in an almost explosive increase in our understanding of the Oort cloud of comets, which surrounds the solar system. Cometary orbits in the cloud evolve under the complex interaction of stellar, galactic, and giant molecular cloud perturbations, as well as planetary and nongravitational perturbations when the orbits re-enter the planetary region. Evidence has continued to build for a dense, inner Oort cloud of comets which acts as a reservoir to replenish the outer cloud as comets there are stripped away. A ring of comets beyond the orbit of Neptune, which may be the source of the short-period comets, is also likely. Both the estimated number and mass of comets in the Oort cloud have grown such that the total mass may be comparable to the mass of the planets. Temporal variations in the flux of comets from the Oort cloud into the planetary region by a factor of 50% are typical, and by factors of 20 to 200 are possible. The most intense cometary “showers” may have serious implications for biological extinction events on Earth as well as for the impact history of planets and satellite systems. Comets in the Oort cloud are processed by galactic cosmic rays, heated by nearby supernovae, eroded by interstellar dust impacts, and disrupted by mutual collisions (in the inner cloud). A detailed estimate of the Oort cloud’s dynamical history is not possible because of the inability to reconstruct the Sun’s varying galactic motion over the history of the solar system, and because of uncertainty over where comets actually formed. However, it is likely that a substantial fraction of the original Oort cloud population has been lost to interstellar space. We are approaching the time when Oort clouds around other stars may be detectable, though searches to date have so far been negative.

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