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Journal articles on the topic 'Life on other planets – drama'

Author: Grafiati

Published: 25 July 2024

Last updated: 31 July 2025

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1

Trzcionka, Joanna. "„Monologami są rozmowy” . Liryczność w Pierścieniu Wielkiej Damy Cypriana Norwida." Colloquia Litteraria 7, no. 2 (2016): 7. http://dx.doi.org/10.21697/cl.2009.2.01.

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“Dialogues are Monologues”. Lyricism in Cyprian Norwid’s The Ring of a Great Lady The article attempts to show how lyricism as an essential component of Cyprian Norwid’s The Ring of a Great Lady affects the artistic shape of the work. This issue is shown by the observation of selected structural elements of the drama, such as time, space and the construction of the main character. In the work the space of the drama and time of the action have been used as metaphors and moved into the sphere of the protagonists’ spiritual experiences. Both time and space planes undergo subjectivism which is the

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Skubnevsky, V. A. "Everyday Life of Barnaul during the Great Patriotic War." Bulletin of Irkutsk State University. Series History 44 (2023): 43–52. http://dx.doi.org/10.26516/2222-9124.2023.44.43.

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The article’s purpose is to analyze the everyday life of the administrative center of the Altai Territory Barnaul during the Great Patriotic War. The question is not yet explored in the literature. The city became one of the major centers for the location of evacuated industrial enterprises from Leningrad, Stalingrad, Kharkov, Lugansk and other cities of the European part of the USSR, as well as hospitals, cultural and educational institutions. On the arrived equipment basis, defense plants as Transmash, Machine-tool, Boiler, Mechanical presses and others were built and put into operation in a

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3

Angel, J. Roger P., and Neville J. Woolf. "Searching for Life on Other Planets." Scientific American 274, no. 4 (1996): 60–66. http://dx.doi.org/10.1038/scientificamerican0496-60.

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Stern, Steve J. "Paradigms of Conquest: History, Historiography, and Politics." Journal of Latin American Studies 24, S1 (1992): 1–34. http://dx.doi.org/10.1017/s0022216x00023750.

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The Quandary of 1492The year 1492 evokes a powerful symbolism.1The symbolism is most charged, of course, among peoples whose historical memory connects them directly to the forces unleashed in 1492. For indigenous Americans, Latin Americans, minorities of Latino or Hispanic descent, and Spaniards and Portuguese, the sense of connection is strong. The year 1492 symbolises a momentous turn in historical destiny: for Amerindians, the ruinous switch from independent to colonised history; for Iberians, the launching of a formative historical chapter of imperial fame and controversy; for Latin Ameri

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Snellen, Ignas. "Planets orbiting other stars: the search for extraterrestrial life." Europhysics News 51, no. 1 (2020): 23–25. http://dx.doi.org/10.1051/epn/2020102.

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Since the Nobel-prize-winning discovery of a planet orbiting a sun-like star, the field of extrasolar planets is undergoing a true revolution. Thousands of planets have been found, of which some may be like Earth. Could there be biological activity on any of these, and how do we find out?

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Jakosky, Bruce, and Andrew H. Knoll. "The Search for Life on Other Planets." Physics Today 53, no. 4 (2000): 63. http://dx.doi.org/10.1063/1.2405460.

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Anonymous. "The Search for Life on Other Planets." Eos, Transactions American Geophysical Union 80, no. 21 (1999): 239. http://dx.doi.org/10.1029/eo080i021p00239-01.

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8

Beichman, Ch. "The Search for Other Planets and Life." EAS Publications Series 41 (2010): 3–23. http://dx.doi.org/10.1051/eas/1041001.

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9

Wackett, Lawrence P. "Microbial life on early earth (and other planets?)." Environmental Microbiology Reports 3, no. 6 (2011): 807–8. http://dx.doi.org/10.1111/j.1758-2229.2011.00307.x.

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Wandel, Amri. "Bio-habitability and life on planets of M-G-type stars." Proceedings of the International Astronomical Union 14, S345 (2018): 189–93. http://dx.doi.org/10.1017/s1743921319001984.

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AbstractThe recent detection of Earth-sized planets in the habitable zone of Proxima Centauri, Trappist-1, and many other nearby M-type stars (which consist some 75% of the stars) has led to speculations, whether liquid water and life actually exist on these planets. Defining the bio-habitable zone, where liquid water and complex organic molecules can survive on at least part of the planetary surface, we suggest that planets orbiting M-type stars may have life-supporting conditions for a wide range of atmospheric properties (Wandel2018). We extend this analysis to synchronously orbiting planet

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Schulze-Makuch, Dirk, and Alberto G. Fairén. "Evaluating the Microbial Habitability of Rogue Planets and Proposing Speculative Scenarios on How They Might Act as Vectors for Panspermia." Life 11, no. 8 (2021): 833. http://dx.doi.org/10.3390/life11080833.

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There are two types of rogue planets, sub-brown dwarfs and “rocky” rogue planets. Sub-brown dwarfs are unlikely to be habitable or even host life, but rocky rogue planets may have a liquid ocean under a thick atmosphere or an ice layer. If they are overlain by an insulating ice layer, they are also referred to as Steppenwolf planets. However, given the poor detectability of rocky rogue planets, there is still no direct evidence of the presence of water or ice on them. Here we discuss the possibility that these types of rogue planets could harbor unicellular organisms, conceivably based on a va

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Somnath, Chakraborty. "Mass gaining of planets and finding life." Akashganga science magazine issn-24567663 2, no. 1 (2019): 8. https://doi.org/10.5281/zenodo.3239467.

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Claudi, Riccardo, and Eleonora Alei. "Biosignatures Search in Habitable Planets." Galaxies 7, no. 4 (2019): 82. http://dx.doi.org/10.3390/galaxies7040082.

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The search for life has had a new enthusiastic restart in the last two decades thanks to the large number of new worlds discovered. The about 4100 exoplanets found so far, show a large diversity of planets, from hot giants to rocky planets orbiting small and cold stars. Most of them are very different from those of the Solar System and one of the striking case is that of the super-Earths, rocky planets with masses ranging between 1 and 10 M ⊕ with dimensions up to twice those of Earth. In the right environment, these planets could be the cradle of alien life that could modify the chemical comp

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Lunine, J. I. "In search of planets and life around other stars." Proceedings of the National Academy of Sciences 96, no. 10 (1999): 5353–55. http://dx.doi.org/10.1073/pnas.96.10.5353.

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Gross, Michael. "The search for life on Earth and other planets." Current Biology 22, no. 7 (2012): R207—R211. http://dx.doi.org/10.1016/j.cub.2012.03.040.

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McGregor, Debra, Sarah Frodsham, and Clarysly Deller. "Participatory Inquiries That Promote Consideration of Socio-Scientific Issues Related to Sustainability within Three Different Contexts: Agriculture, Botany and Palaeontology." Sustainability 15, no. 8 (2023): 6895. http://dx.doi.org/10.3390/su15086895.

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The involvement of students in dramatised inquiries, through participatory activity, offers opportunities to act in-role as scientists. The inquiries can ‘set-the-scene’, provide context and challenges for students to consider possibilities within and beyond everyday life. This approach can engage students in thinking about sustainability and developing citizenship competencies, such as thinking scientifically and critiquing ideas, interrogating evidence and assessing the validity of information, as well as decision making and problem solving. In this paper, adopting stories from the history o

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Paliwal, Ishita, and Caitlin Reintjes. "Origins of Life Lab at McMaster University." Sciential - McMaster Undergraduate Science Journal, no. 2 (March 29, 2019): 21–23. http://dx.doi.org/10.15173/sciential.v1i2.2104.

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One of the many novel scientific studies being conducted at McMaster University focuses on uncovering the origins of life, specifically, how the first cells were formed. Dr. Maikel Rheinstadter, from the Department of Physics and Astronomy, has developed a planetary simulator that effectively replicates environmental conditions both on Earth and other potentially habitable planets in the solar system. His team works to discern how the first cells may have developed on these planets by investigating the idea that water-based life was formed in warm, volcanic ponds. The following interview provi

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Gale, Joseph, and Amri Wandel. "The potential of planets orbiting red dwarf stars to support oxygenic photosynthesis and complex life." International Journal of Astrobiology 16, no. 1 (2016): 1–9. http://dx.doi.org/10.1017/s1473550415000440.

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AbstractWe review the latest findings on extra-solar planets and their potential of having environmental conditions that could support Earth-like life. Focusing on planets orbiting red dwarf (RD) stars, the most abundant stellar type in the Milky Way, we show that including RDs as potential life supporting host stars could increase the probability of finding biotic planets by a factor of up to a thousand, and reduce the estimate of the distance to our nearest biotic neighbour by up to 10. We argue that binary and multiple star systems need to be taken into account when discussing habitability

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Schubotz, Florence, Mark A. Sephton, and Sylvie Derenne. "Biomarkers in Extreme Environments on Earth and the Search for Extraterrestrial Life in Our Solar System." Elements 18, no. 2 (2022): 100–106. http://dx.doi.org/10.2138/gselements.18.2.100.

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Our appreciation of the potential distribution of life in the Solar System has been impacted by the discovery that organisms are able to occupy the most extreme environments on Earth. The persistence of life in the deepest parts of oceans, the deep sedimentary and crustal biosphere accessed by deep drill holes, hot springs, deserts, and polar regions has led to diverse hypotheses regarding the potential for extraterrestrial life on other planets. This chapter provides an overview on how scientists explore the habitability of other planets and moons of our Solar System and far away in outer spa

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Namazova, F. "CHARACTERISTICS OF DRAMA GENRE AND DRAMA LANGUAGE." BULLETIN Series of Philological Sciences 75, no. 1 (2021): 77–82. http://dx.doi.org/10.51889/2021-1.1728-7804.13.

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Addressing the specific problems of dramatic creativity, we must first determine the basic meaning of the term "drama". As we know, the word "drama" has different meanings. We also call a certain range of real events, for example, the drama of life, one of the genres of the dramatic type of literature (the noble drama of the eighteenth century) and the dramatic theater, which is the leading type of performing arts. Dramatic works are fundamentally different from other genres. As early as the 19th century, the great thinker MFAkhundov distinguished the genre of drama he brought to our literatur

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Palhares, Dario, and Íris Almeida dos Santos. "Astronomic Bioethics: Terraforming X Planetary protection." Bangladesh Journal of Bioethics 8, no. 2 (2017): 1–10. http://dx.doi.org/10.3329/bioethics.v8i2.34474.

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A hard difficulty in Astrobiology is the precise definition of what life is. All living beings have a cellular structure, so it is not possible to have a broader concept of life hence the search for extraterrestrial life is restricted to extraterrestrial cells. Earth is an astronomical rarity because it is difficult for a planet to present liquid water on the surface. Two antagonistic bioethical principles arise: planetary protection and terraforming. Planetary protection is based on the fear of interplanetary cross-infection and possible ecological damages caused by alien living beings. Terra

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Shorttle, Oliver, Natalie R. Hinkel, and Cayman T. Unterborn. "Why Geosciences and Exoplanetary Sciences Need Each Other." Elements 17, no. 4 (2021): 229–34. http://dx.doi.org/10.2138/gselements.17.4.229.

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The study of planets outside our Solar System may lead to major advances in our understanding of the Earth and may provide insight into the universal set of rules by which planets form and evolve. To achieve these goals requires applying geoscience’s wealth of Earth observations to fill in the blanks left by the necessarily minimal exoplanetary observations. In turn, many of Earth’s one-offs—plate tectonics, surface liquid water, a large moon, and life: long considered as “Which came first?” conundrums for geoscientists—may find resolution in the study of exoplanets that possess only a subset

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Lorenz, Ralph D. "Planets, life and the production of entropy." International Journal of Astrobiology 1, no. 1 (2002): 3–13. http://dx.doi.org/10.1017/s1473550402001027.

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Two thermodynamic principles offer considerable insight into the climatic and geological settings for life on other planets, namely (1) that natural systems tend to actually achieve the ideal (‘Carnot’) limit of conversion of heat into work and (2) if a fluid system such as an atmosphere has sufficient degrees of freedom, it will choose the degree of heat transport that maximizes the generation of work (equivalently, that which offers maximum entropy production). The first principle agrees well with results on terrestrial cumulus convection, and the mechanical energy released by tectonic activ

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Rossmo, D. Kim. "Bernoulli, Darwin, and Sagan: the probability of life on other planets." International Journal of Astrobiology 16, no. 2 (2016): 185–89. http://dx.doi.org/10.1017/s1473550416000148.

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AbstractThe recent discovery that billions of planets in the Milky Way Galaxy may be in circumstellar habitable zones has renewed speculation over the possibility of extraterrestrial life. The Drake equation is a probabilistic framework for estimating the number of technological advanced civilizations in our Galaxy; however, many of the equation's component probabilities are either unknown or have large error intervals. In this paper, a different method of examining this question is explored, one that replaces the various Drake factors with the single estimate for the probability of life exist

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Cacaj, Drinor, Daniel Angerhausen, Prabal Saxena, et al. "Photobombing for the Large Interferometer For Exoplanets (LIFE). A New Criterion for Target Confusion and Application to a Mid-infrared Rotating Nulling Interferometer." Astronomical Journal 169, no. 5 (2025): 244. https://doi.org/10.3847/1538-3881/adbe6c.

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Abstract One of the primary objectives in modern astronomy is to discover and study planets with characteristics similar to Earth. This pursuit involves analyzing the spectra of exoplanets and searching for biosignatures. Contamination of spectra by nearby objects (e.g., other planets and moons in the same system) is a significant concern and must be addressed for future exo-Earth searching missions. The aim is to estimate, for habitable planets, the probability of spectral contamination by other planets within the same star system. This investigation focuses on the Large Interferometer For Ex

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Mayor, Michel, Stephane Udry, Francesco Pepe, and Christophe Lovis. "Exoplanets: the quest for Earth twins." Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 369, no. 1936 (2011): 572–81. http://dx.doi.org/10.1098/rsta.2010.0245.

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Today, more than 400 extra-solar planets have been discovered. They provide strong constraints on the structure and formation mechanisms of planetary systems. Despite this huge amount of data, we still have little information concerning the constraints for extra-terrestrial life, i.e. the frequency of Earth twins in the habitable zone and the distribution of their orbital eccentricities. On the other hand, these latter questions strongly excite general interest and trigger future searches for life in the Universe. The status of the extra-solar planets field—in particular with respect to very-l

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Lazcano, Antonio. "Astrobiology: Towards an Understanding of the Emergence of Life in the Universe." Symposium - International Astronomical Union 213 (2004): 245–54. http://dx.doi.org/10.1017/s0074180900193350.

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Long before the idea of spontaneous generation was incorporated by JeanBaptiste de Lamarck into evolutionary biology to explain the first emergence of life, the possibility that other planets were inhabited had been discussed, sometimes in considerable detail, by scientists and philosophers alike (Lazcano 2001). More often than not, these were speculations that rested on the idea of a uniform universe but with little or no empirical basis. Today our approaches to the issue of life in the Universe have changed dramatically; neither the formation of planets nor the origin of life are seen as the

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Rimmer, Paul B., Sukrit Ranjan, and Sarah Rugheimer. "Life’s Origins and the Search for Life on Rocky Exoplanets." Elements 17, no. 4 (2021): 265–70. http://dx.doi.org/10.2138/gselements.17.4.265.

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The study of the origin(s) of life on Earth and the search for life on other planets are closely linked. Prebiotic chemical scenarios can help priori-tize target planets for the search for life (as we know it) and can provide informative prior probabilities to help us assess the likelihood that particular spectroscopic features are evidence of life. The prerequisites for origins scenarios themselves predict characteristic spectral signatures. The interplay between origins research and the search for extraterrestrial life starts with laboratory work to guide exploration within our own Solar Sys

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Kashefi, Kazem. "Living hell: Life at high temperatures." Biochemist 27, no. 1 (2005): 6–10. http://dx.doi.org/10.1042/bio02701006.

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Modern hot environments, such as those found in hydrothermal vents, are of great interest to the scientific community because they resemble those ancient environments where life first arose on Earth and also share many characteristics with environments in other planets where life may have actually existed. Evidence to date strongly indicates that Fe(III) respiration may have been one of the first, if not the first, forms of respiration in a hot, early Earth. The abundance of Fe(III) minerals in many modern and ancient hot environments suggests that studies of Fe(III)-reducing hyperthermophilic

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Schmitt, Harrison H. "Life among the Craters." Symposium - International Astronomical Union 213 (2004): 199–202. http://dx.doi.org/10.1017/s0074180900193271.

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The Moon forms one end-member in the planetary mass series Earth-Venus-Mars-Mercury-Asteroids-Moon (Weissman 1999). Having a detailed understanding of the nature and evolution of the two end-members of this series, rather than of just the Earth, has increased the value of other data and inferences by orders of magnitude. As a consequence of obtaining an understanding of the evolution of a second planet, we now can look at other terrestrial planets with far greater insight than ever would have been possible otherwise (Fig. 1).

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Ramirez, Ramses. "A More Comprehensive Habitable Zone for Finding Life on Other Planets." Geosciences 8, no. 8 (2018): 280. http://dx.doi.org/10.3390/geosciences8080280.

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The habitable zone (HZ) is the circular region around a star(s) where standing bodies of water could exist on the surface of a rocky planet. Space missions employ the HZ to select promising targets for follow-up habitability assessment. The classical HZ definition assumes that the most important greenhouse gases for habitable planets orbiting main-sequence stars are CO2 and H2O. Although the classical HZ is an effective navigational tool, recent HZ formulations demonstrate that it cannot thoroughly capture the diversity of habitable exoplanets. Here, I review the planetary and stellar processe

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Doyle, Charlotte L. "Multiple Realities: The Changing Life Worlds of Actors." Journal of Phenomenological Psychology 47, no. 2 (2016): 107–33. http://dx.doi.org/10.1163/15691624-12341310.

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This is an empirical phenomenological interview study into the experiences of professional actors as they create and perform roles for the stage. Prior research was inadequate for capturing actors’ changing life worlds over time. Analyzing the interviews using the descriptive phenomenological method yielded general structural descriptions and pointed to the relevance of Schütz’s description of multiple realities. Being cast in a role changes the pace and goals of actors’ everyday worlds and leads the actors intermittently and with intention to enter other realities—fictional, theoretical, and/

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Rees, Martin. "From Mars to the Multiverse." European Review 26, no. 1 (2017): 1–12. http://dx.doi.org/10.1017/s1062798717000345.

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Unmanned spacecraft have visited the other planets of our Solar System (and some of their moons), beaming back pictures of varied and distinctive worlds – but none propitious for life. However, prospects are far more interesting when we extend our gaze to other stars. Most stars are orbited by retinues of planets. Our home Galaxy contains a billion planets like the Earth. Do some of these have biospheres? Moreover, our Galaxy is one of billions visible with a large telescope – all the aftermath of a cosmic ‘big bang’ 13.8 billion years ago. More astonishing still, ‘our’ big bang may not have b

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Sandora, McCullen, Vladimir Airapetian, Luke Barnes, Geraint F. Lewis, and Ileana Pérez-Rodríguez. "Multiverse Predictions for Habitability: Element Abundances." Universe 8, no. 12 (2022): 651. http://dx.doi.org/10.3390/universe8120651.

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We investigate the dependence of elemental abundances on physical constants, and the implications this has for the distribution of complex life for various proposed habitability criteria. We consider three main sources of abundance variation: differing supernova rates, alpha burning in massive stars, and isotopic stability, and how each affects the metal-to-rock ratio and the abundances of carbon, oxygen, nitrogen, phosphorus, sulfur, silicon, magnesium, and iron. Our analysis leads to several predictions for which habitability criteria are correct by determining which ones make our observatio

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Pilat-Lohinger, Elke. "The ultimate cataclysm: the orbital (in)stability of terrestrial planets in exoplanet systems including planets in binaries." International Journal of Astrobiology 8, no. 3 (2009): 175–82. http://dx.doi.org/10.1017/s1473550409990164.

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AbstractThere is no doubt that stability studies are of great importance in the fascinating research of extrasolar planetary systems. Even if most of the more than 300 extrasolar planets orbit their host stars as single giant planet and build simple two-body systems, we should not exclude the possibility that these systems could host other (small) planets that have not yet been detected due to obsevational limits. Another aspect to carry out stability studies is the growing interest in the search for extraterrestrial life in the universe. The long-term stability of a planetary system is one of

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Higdon, Rachel Delta, and Kate Chapman. "A dramatic existence: Undergraduate preparations for a creative life in the performance industries." Industry and Higher Education 34, no. 4 (2020): 272–83. http://dx.doi.org/10.1177/0950422220912979.

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This article focuses specifically on drama and theatre higher education (HE) programmes and preparation for potential graduate work. The article investigates working in the creative industries and in the performing arts (particularly within acting) and how HE students in the United Kingdom prepare for this life. The growth of the creative industries and successful applied drama in the public and private sectors has also brought business interest in how drama and theatre processes can benefit other workplaces, outside of the creative arts. The article addresses current policy, initiatives and p

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Holmes, Brooke. "Antigone at Colonus and the End(s) of Tragedy." Ramus 42, no. 1-2 (2013): 23–43. http://dx.doi.org/10.1017/s0048671x00000059.

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Sophocles' Oedipus at Colonus, it would seem, is an exercise in closure. In the opening scene, Oedipus, worn down by years of wandering blind and hungry, arrives at the borders of Athens. Here is where his legendary sufferings—his murder of his father, his incestuous marriage to his mother, his betrayal by his sons, his exile from Thebes—are fated to end. Following his miraculous death, his body will become a sacred gift to the city that receives him, protecting it against future attack. In the closing moments of the play, everything unfolds according to plan. Oedipus disappears offstage and m

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Meadows, Victoria, and David Crisp. "The Virtual Planetary Laboratory: Towards Characterization of Extrasolar Terrestrial Planets." Symposium - International Astronomical Union 213 (2004): 129–38. http://dx.doi.org/10.1017/s0074180900193131.

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NASA and ESA are currently undertaking mission studies for space-based observatories designed to search for life on other worlds. To optimize the designs of these missions, and to ultimately interpret the data sent back by them, we need to recognize habitable worlds and to discriminate between planets with and without life based only on remotely-sensed information. This paper provides an overview of the characteristics we would look for on an extrasolar terrestrial planet that might indicate habitability or the presence of life. It also describes a new NASA Astrobiology Institute research proj

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Sari, Lusi Komala, and Bede Blaise Chukwunyere Onwuagboke. "Pragmatic/Religious and Moral Values in Hermana HMT’s Drama Script “Robohnya Surau Kami” (“The Collapse of Our Mosque”)." International Journal of Evaluation and Research in Education (IJERE) 4, no. 4 (2015): 207. http://dx.doi.org/10.11591/ijere.v4i4.4513.

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<span style="line-height: 107%; font-family: 'Times New Roman','serif'; font-size: 9pt; mso-fareast-font-family: 'Times New Roman'; mso-ansi-language: EN; mso-fareast-language: EN-US; mso-bidi-language: AR-SA;" lang="EN">Life in heaven is the hope of all religious human. Yet, to reach the paradise as promised to all faithful is not an easy road. It needs the balance of earthly life and hereafter’s life to reach the place which is promised by God. The drama Robohnya Surau Kami (RSK) created by dramatist Hermana HTM which is adapted from a short story written by A.A. Navis conveys the afor

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Tuchow, Noah W., and Jason T. Wright. "The Abundance of Belatedly Habitable Planets and Ambiguities in Definitions of the Continuously Habitable Zone." Astrophysical Journal 944, no. 1 (2023): 71. http://dx.doi.org/10.3847/1538-4357/acb054.

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Abstract A planet’s history dictates its current potential to host habitable conditions and life. The concept of the continuously habitable zone (CHZ) has been used to define the region around a star most likely to host planets with long-term habitability. However, definitions of the CHZ vary in the literature and often conflict with each other. Calculating the fraction of habitable zone planets in the CHZ as a function of stellar properties, we find that the quality of a star as a host for planets with long-term habitability and biosignatures depends strongly on the formulation of the CHZ use

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Nasution, Melinda. "Nilai-Nilai Kehidupan dalam Naskah Drama Kibar Bendera Si Sarto di Halaman Rumah Karya Rodli TL (Kajian Pragmatik)." RUANG KATA: Journal of Language and Literature Studies 3, no. 01 (2023): 58–72. http://dx.doi.org/10.53863/jrk.v3i01.734.

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Drama as a genre of literature, has its own characteristics compared to other genres, namely poetry and fiction. Drama is unique from the point of view of using language and conveying its message and useful values ??for its readers. However, often the delivery of messages and values ??through character conversations is often not caught by the reader because dialogue in drama often uses connotative words that have ambiguity or indirectness of expression. The presentation of language in drama literary works is in the form of using behavioral instructions that describe the atmosphere and using th

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Anderson, Mark. "Microbes survive meteorite smashes and so could seed life on other planets." New Scientist 197, no. 2649 (2008): 15. http://dx.doi.org/10.1016/s0262-4079(08)60763-0.

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Raulin Cerceau, Florence. "What Possible Life Forms Could Exist on Other Planets: A Historical Overview." Origins of Life and Evolution of Biospheres 40, no. 2 (2010): 195–202. http://dx.doi.org/10.1007/s11084-010-9200-7.

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Arnold, Luc. "Earthshine Observation of Vegetation and Implication for Life Detection on Other Planets." Space Science Reviews 135, no. 1-4 (2007): 323–33. http://dx.doi.org/10.1007/s11214-007-9281-4.

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Beichman, Charles. "The Search for Terrestrial Planets: What Do we Need to Know?" Symposium - International Astronomical Union 202 (2004): 432–41. http://dx.doi.org/10.1017/s0074180900218433.

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The goal of finding and characterizing habitable planets in other solar systems represents one of humanity's greatest scientific challenges. NASA and ESA have initiated studies of missions that could accomplish this goal within the next ten years. What precursor knowledge do we need before we can initiate such a mission? How large should the first steps be in a program whose ultimate aim is to detect life on other planets? This talk describes different concepts for NASA's Terrestrial Planet Finder and discusses potential precursors in a program that balances scientific return, technological ad

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Sandora, McCullen. "Multiverse Predictions for Habitability:Fraction of Planets that Develop Life." Universe 5, no. 7 (2019): 171. http://dx.doi.org/10.3390/universe5070171.

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In a multiverse context, determining the probability of being in our particular universe depends on estimating its overall habitability compared to other universes with different values of the fundamental constants. One of the most important factors in determining this is the fraction of planets that actually develop life, and how this depends on planetary conditions. Many proposed possibilities for this are incompatible with the multiverse: if the emergence of life depends on the lifetime of its host star, the size of the habitable planet, or the amount of material processed, the chances of b

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Nelyubin, N. I. "Theoretical and methodological foundations for the inclusion of the concept of "cogital identity" in the conceptual apparatus of post-non-classical psychology of thinking." Sibirskiy Psikhologicheskiy Zhurnal, no. 88 (2023): 6–20. http://dx.doi.org/10.17223/17267080/88/1.

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In modern psychological discourse there is an increase in anthropologically oriented concepts and methodological tools that contribute to the comprehension of multidimensional human existence in a rapidly becoming more complex and changing world. The conceptosphere of post-non-classical psychology is replenished with interdisciplinary concepts and metaphors necessary to comprehend the multilevel dynamics of the human life world. The relevance of this work is determined by the need to comprehend the phenomenon of actualization by a person in his own thinking of stable subject-thematic dominants

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Gao, Chuling. "Cultural Relics Dance Drama." International Journal of Education and Humanities 17, no. 1 (2024): 112–15. http://dx.doi.org/10.54097/8tjw0382.

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In recent years, the upsurge of Chinese traditional culture has hit. The museum cultural relics and dance drama have achieved a perfect combination. The use of new scientific and technological means has not only given new life to cultural relics, but also opened up new ideas for the vast number of cultural and museum workers and literary creators. The two interact and achieve each other, bringing visual enjoyment to the audience and promoting the development of cultural and museum undertakings.

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Page, Thornton. "Detecting Distant Planets with Space Telescope." Symposium - International Astronomical Union 112 (1985): 85–89. http://dx.doi.org/10.1017/s0074180900146388.

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In 1981 and in 1984, I offered at the University of Houston, CLC, a course on Space Telescope, the first of its kind. The 22 graduate students were assigned research projects of their own choosing designed for ST. Several chose the detection of planets of other stars, showing the popularity of the search for extraterrestrial life. Space Telescope's six instruments can be used for this purpose in several ways, and the students, most of them scientists and engineers at the NASA Johnson Space Center, proposed to use most of these after ST is launched in 1986 or 1987. The student proposals require

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Crowe, Michael J. "Book Review: Planets of other Stars: Strange New Worlds: The Search for Alien Planets and Life beyond Our Solar System." Journal for the History of Astronomy 43, no. 1 (2012): 125–26. http://dx.doi.org/10.1177/002182861204300112.

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