Assembling aliens to explore the Solar System

2021 ◽  
Author(s):  
Catarina Leote ◽  
Sérgio Pereira ◽  
João Retrê ◽  
Pedro Machado ◽  
Gabriella Gilli ◽  
...  

<p><strong>Assembling aliens to explore the Solar System</strong></p> <p>After analysing the school curricula until 7th grade (13 years old), we concluded that, at least in Portugal, there is a limited coverage of astronomy subjects. This situation is also often accompanied by limited training of primary and medium school teachers and limited availability of resources in their mother tongues, as language can also be a barrier for the use of existing resources. In addition, some astronomy concepts require a level of abstract thinking that might be discouraging for some children. The end result is that some children will have a low interest in astronomy, not only because of their personal preferences but as a consequence of low exposure to the subject or a negative perception towards it. To address this situation, the Science Communication Group of Instituto de Astrofísica e Ciências do Espaço (IA) developed a board game about the Solar System, aimed at children from 6 to 12 years old, and adapted to both formal and informal educational contexts. This project, “Help your Alien – A Solar System Game”, was funded in 2019 by the Europlanet Society through its Public Engagement Funding Scheme.</p> <p><strong>Why a board game?</strong></p> <p>By opting for a board game instead of a digital platform, we made the conscious decision of valuing the power of storytelling and social interaction as engaging and focus-promoting learning strategies, unlike the information and stimuli overload sometimes present in digital environments. Another choice made to make the game as appealing and relatable to our target public as possible was to start with a more familiar perspective, biology, as children of this age group will certainly be familiar with “animals” and their characteristics. We made a leap forward towards astrobiology, and created imaginary aliens somehow adapted to their planets and moons. While trying to assemble these imaginary creatures, in a 3-piece puzzle, the game players have to gather information about different objects of the Solar System and discover the home planet of their assembled aliens.  Another reason for creating a board game was the possibility of reaching different publics, in particular those perhaps not immediately interested in astronomy. With “ET – A Solar System Adventure”, we hope to engage children but also their families (parents, grandparents, siblings…), just for the sake of playing, while exposing them to knowledge about the Solar System.</p> <p><strong>Development of the game</strong></p> <p>The game was developed in a collaborative creative process by members of the Science Communication Group and researchers in Planetary Sciences of the IA, combining knowledge in science communication and different publics with scientific knowledge. Even though the game mechanics was inspired in already existing and well-tested games, the whole process of creating this game involved many challenges, from defining the level of complexity while keeping the game engaging, to the adventure of “creating” aliens somehow physiologically adapted to different planets and moons of the Solar System. Mistakes were made and the team had to adapt to the unexpected challenging situation of a pandemic. This resulted in many lessons learned that we hope to share with the community. The game is now at its final stages of production, with the prototype being converted into a polished version with professional illustration and design. A “Print and Play” version in Portuguese and English will soon be made available online on our website. Physical copies will also be produced depending on funding.</p> <p>In our presentation, we will present our game, as well as the premises and goals behind it, its development process, the challenges found along the way, the lessons learned and some strategies to cope with the “new normality” imposed by Covid-19, while advancing the project. We hope the presentation of “ET – A Solar System Adventure” in the EPSC2021 will help to promote this tool for planetary science education among formal and informal educators and to find international collaborations for the translation and local promotion of the game, as well as additional funding for the production of physical copies in different languages.</p>

2016 ◽  
Vol 6 (4) ◽  
pp. 17 ◽  
Author(s):  
Nina Feldmann ◽  
Raphael Kurz ◽  
Cornelia Böhmer ◽  
Eva Maria Beck-Meuth

This paper reports on the development of e-learning material for a blended-learning part-time study program in electrical engineering and information technology. It is focused on the entire process of creation, from the perspective of instructors and higher education professionals supporting the production. In the design of the program, the development of effective study material including e-learning content for the target group was one of the main objectives. Associated with the development of this material, various challenges had to be overcome. In the following, we describe the development and implementation process of the material using results from a survey among lecturers who were contributing e-learning to the program. Different manifestations of e-learning are discussed, and the whole process of production is reviewed. In the current efforts for digitizing higher education in Europe, the findings may be relevant for universities’ e-learning strategies.


Science ◽  
2004 ◽  
Vol 306 (5700) ◽  
pp. 1302-1304 ◽  
Author(s):  
A. Morbidelli

2021 ◽  
Author(s):  
Marco Delbo ◽  
Laurent Galluccio ◽  
Francesca De Angeli ◽  
Paolo Tanga ◽  
Alberto Cellino ◽  
...  

<div class="">Asteroids reflectance spectra in the visible light will be one of the novel products of the Gaia Data Release 3 (DR3). These spectra are produced from Gaia observations obtained by means of the blue and red photometers — the so-called BP and RP, respectively. We will review the strategy adopted to produce asteroid reflectance spectra from BP-RP data, focusing on the choice of spectro-photometric calibrations computed taking into account solar system object astrometry and suitable lists of solar-analog stars.</div> <div class=""> </div> <div class="">Our preliminary investigation shows that we will be able to obtain reflectance spectra for asteroids as small as some km in the main belt, by exploiting the fact that each object has been observed multiple times by Gaia. We will show the capability of Gaia to probe the detailed compositional gradient of the main belt down to small sizes and to study correlations between spectral classes and other asteroid physical parameters, such as albedo and size.</div> <div class=""> </div> <div class="">Concerning the brightest asteroids, we expect to have substantial signal at wavelengths shorter than 450 nm, allowing Gaia to examine this region of the spectrum that has been poorly investigated by ground-based asteroid spectroscopic surveys. This region is characterised by the presence of a reflectance downturn that is diagnostic for the composition of classes of primitive asteroids, for instance those including the parent bodies of carbonaceous chondrites. These asteroids may have played an important role for the delivery of prebiotic compounds to Earth during the early phases of solar system' s history and, as such, are at the center of attention of the planetary science community. </div>


2021 ◽  
Author(s):  
Loïc Rossi

<p>First published in 1887 by Ludwik Lejzer Zamenhof, Esperanto is the most successful constructed language, with speakers all around the globe and even native speakers.</p> <p>The relationship between Esperanto and science starts very early: the scientific journal <em>Internacia Scienca Revuo</em> was created in 1904 and the International Esperantist Science Association (ISAE) was founded in 1907 (Wera Blanke, <em>Scienca Revuo</em> 206, 2006). Many publications and books about scientific topics have since been written or translated in Esperanto. </p> <p>Esperanto has initially been envisioned as a lingua franca to be used in international communication, both in general and for scientific purposes. While English has since taken this role, there is still a desire to maintain and develop the scientific culture and the related terminology in Esperanto. Science outreach is one way to achieve this goal, and new projects have appeared in the last few years.</p> <p>Esperanto represents an interesting challenge for outreach : being a more neutral language, not related to a specific country or ethnic group, the community of speakers (albeit small) is by essence more international and more diverse than in national languages. This is an opportunity, but also comes with some difficulties.</p> <p>In this work, I’ll discuss the advantages and obstacles of communicating science in Esperanto. I’ll present various projects of science communication in Esperanto, with a focus on my personal experience with my YouTube channel <em>D-ro Loĉjo</em>, where I do videos about science and in particular about planetary science.</p>


Author(s):  
Izaskun IRIARTE IRURETA

LABURPENA: Gaur egun Bulego Judizial Berriaren (BJB) ezarpenaren prozesua abian da Euskal Autonomia Erkidegoko barruti judizialetan. «Bulego Judizial Berria»-tzat ezagutzen den Justizia Administrazioaren eraldaketa sakona dakarrenez, berrantolaketa hau gradualki egingo da Euskadin. Testu honen helburua da aurkeztea Bulego Judizial Berria zer den eta zer suposatzen duen, nola antolatu eta gauzatu den Euskadin Bulego Judizial Berriaren ezarpena horretarako propio Eusko Jaurlaritzak onartu zuen planaren eremuan, aurreikusita duen kalitate-sistema, lehen Bulegoen ezarpenaren ondorioak zeintzuk izan diren eta prozesu osoaren erronkak. RESUMEN: En estos momentos está en marcha el proceso implantación de la Oficina Judicial en los partidos judiciales de Euskadi. Dado que lo que se conoce como «Nueva Oficina Judicial» supone una profunda reforma en la Administración de Justicia, esta reestructuración, en Euskadi, se llevará a cabo de forma gradual. Este texto pretende presentar el alcance de la Nueva Oficina Judicial y en qué consiste, cómo se ha organizado y se está llevando a cabo la implantación de la Nueva Oficina Judicial en Euskadi en el marco del plan que aprobó el Gobierno Vasco con ese fin, el sistema de calidad que se ha previsto, las conclusiones extraídas de las primeras Oficinas Judiciales implantadas y los retos del conjunto del proceso. ABSTRACT: Nowadays the implementation process of the Judicial Office in the Judicial Districts of the Basque Country is taking place. This new «Judicial Office» brings about a deep and thorough reform in the Administration of Justice and its functioning. Therefore this reorganisation process will be implemented gradually. This article aims to discuss the meaning and the implications of the New Judicial Office, to describe how the implementation of the New Judicial Office in the Basque Country has been organized and applied within the framework of the Implementation Plan adopted by the Basque Government, including the qualitysystem for the Judicial Office, and finally to draw the lessons learned from the process of implementation as it has been taking place within the first Judicial Offices. The challenges of the whole process are thus brought to the fore.


Author(s):  
Bryan Holler

This is an advance summary of a forthcoming article in the Oxford Research Encyclopedia of Planetary Science. Please check back later for the full article. The International Astronomical Union (IAU) officially recognizes five objects as dwarf planets: Ceres in the main asteroid belt between Mars and Jupiter; and Pluto, Eris, Haumea, and Makemake in the trans-Neptunian region beyond the orbit of Neptune. However, the definition used by the IAU applies to many other trans-Neptunian objects (TNOs) and can be summarized as any nonsatellite large enough to be rounded by its own gravity. Practically speaking, this means any nonsatellite with a diameter >400 km. In the trans-Neptunian region, there are more than 100 objects that satisfy this definition, based on published results and diameter estimates. The dynamical structure of the trans-Neptunian region records the migration history of the giant planets in the early days of the solar system. The semi-major axes, eccentricities, and orbital inclinations of TNOs across various dynamical classes provide constraints on different aspects of planetary migration. For many TNOs, the orbital parameters are all that is known about them, due to their large distances, small sizes, and low albedos. The TNO dwarf planets are a different story. These objects are large enough to be studied in more detail from ground- and space-based observatories. Imaging observations can be used to detect satellites and measure surface colors, while spectroscopy can be used to constrain surface composition. In this way, TNO dwarf planets not only help provide context for the dynamical evolution of the outer solar system, but also reveal the composition of the primordial solar nebula as well as the physical and chemical processes at work at very cold temperatures. The largest TNO dwarf planets, those officially recognized by the IAU, plus others such as Sedna, Quaoar, and Gonggong, are large enough to support volatile ices on their surfaces in the present day. These ices are able to exist as solids and gases on some TNOs, due to their sizes and surface temperatures (similar to water ice on Earth) and include N2 (nitrogen), CH4 (methane), and CO (carbon monoxide). A global atmosphere composed of these three species has been detected around Pluto, the largest TNO dwarf planet, with the possibility of local atmospheres or global atmospheres at perihelion for Eris and Makemake. The presence of nonvolatile species, such as H2O (water), NH3 (ammonia), and organics provide valuable information on objects that may be too small to retain volatile ices over the age of the solar system. In particular, large quantities of H2O mixed with NH3 points to ancient cryovolcanism caused by internal differentiation of ice from rock. Organic material, formed through radiation processing of surface ices such as CH4, records the radiation histories of these objects as well as providing clues to their primordial surface compositions. The dynamical, physical, and chemical diversity of the >100 TNO dwarf planets are key to understanding the formation of the solar system and subsequent evolution to its current state. Most of our knowledge comes from a small handful of objects, but we are continually expanding our horizons as additional objects are studied in more detail.


Life ◽  
2020 ◽  
Vol 10 (5) ◽  
pp. 52 ◽  
Author(s):  
Alex Longo ◽  
Bruce Damer

Two widely-cited alternative hypotheses propose geological localities and biochemical mechanisms for life’s origins. The first states that chemical energy available in submarine hydrothermal vents supported the formation of organic compounds and initiated primitive metabolic pathways which became incorporated in the earliest cells; the second proposes that protocells self-assembled from exogenous and geothermally-delivered monomers in freshwater hot springs. These alternative hypotheses are relevant to the fossil record of early life on Earth, and can be factored into the search for life elsewhere in the Solar System. This review summarizes the evidence supporting and challenging these hypotheses, and considers their implications for the search for life on various habitable worlds. It will discuss the relative probability that life could have emerged in environments on early Mars, on the icy moons of Jupiter and Saturn, and also the degree to which prebiotic chemistry could have advanced on Titan. These environments will be compared to ancient and modern terrestrial analogs to assess their habitability and biopreservation potential. Origins of life approaches can guide the biosignature detection strategies of the next generation of planetary science missions, which could in turn advance one or both of the leading alternative abiogenesis hypotheses.


2015 ◽  
Vol 95 (2) ◽  
pp. 203-214 ◽  
Author(s):  
M.G. Kleinhans ◽  
A.J. Verkade ◽  
T. van Wessel ◽  
M.A.S. Bastings ◽  
W.A. Marra ◽  
...  

AbstractLike earth and planetary scientists, most children are curious about the world, the solar system and the rest of the universe. However, for various reasons primary schools emphasise language and calculus rather than natural sciences. When science is taught, examination systems often favour knowledge of the ‘right’ answer over the process of investigation and logical reasoning towards that answer. In order to continue to spark children's curiosity and their motivation to learn and discover, science education hubs at universities and science museums could collaborate more with schools and teachers, and are beginning to do so. The objective of this position paper is to report on recent experiences in earth and planetary science education for pupils in primary and secondary education, to provide examples and inspiration for scientists. We report three examples of initiation and consolidation of science education in primary schools in the Netherlands: (1) a focus on asking questions and seeking information to reason towards the answer, initiated with a classroom game, Expedition Mundus, (2) bringing pupils and teachers together outside their school in the science museum to gain confidence and self-efficacy, and (3) having children ask their own questions and do their own research guided by the empirical cycle, for example on experimentation on sandbox scale models of channels and crater lake deltas as found on Mars. The focus on other planets, fictitious and real, stimulates pupils to ask questions about planet Earth. Finally, we argue that involvement of more scientists in science education would not only benefit primary and secondary schools and future students but also university education and science communication with society.


Author(s):  
Cesar Orsini ◽  
Veena Rodrigues ◽  
Jorge Tricio

This study presents the design, implementation, and lessons learned from 2 fit-for-purpose online interprofessional faculty development programs for educational practice improvement in the health professions in Chile and the United Kingdom from 2018 to 2021. Both programs were designed to enhance teaching and learning practices in an interprofessional environment based on 4 pillars: professional diversity, egalitarianism, blended/online learning, and active learning strategies. A multidisciplinary mix of educators participated, showing similar results. The 3 main lessons learned were that the following factors facilitated an interprofessional environment: a professions-inclusive teaching style, a flexible learning climate, and interprofessional peer work. These lessons may be transferable to other programs seeking to enhance and support interprofessionality. Faculty development initiatives preparing educators for interprofessional practice should be an integral component of health professions education, as delivering these courses within professional silos is no longer justifiable. As the relevance of interprofessional education grows, an effective way of promoting interprofessonal education is to train the trainers in formal interprofessional settings.


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