Comunidade ODS dos participantes do curso "Astronomia Hands-On: Descobrir o Cosmos" promovido pelo Centro de Formação do NUCLIO. Este curso está acreditado pelo Conselho Científico-Pedagógico da Formação Contínua com o registo nºCCPFC/ACC-69425/12, tem uma duração de 25 horas presenciais, dando acesso a 1 crédito. A ação releva para efeitos de progressão em carreira de Professores dos Ensinos Básico e Secundário de acordo com o artigo 5º do Regime Jurídico da Formação Contínua de Professores e
As children, we’re taught to paint cold things blue and hot things red. In science we learn that blue things are actually far hotter than red things! In this lesson, we will learn how hot objects radiate energy as light of many colors following what is called a black body curve. This community is part of the ISE hangouts series devoted to Astronomy and Space Science. Each community has an associated hangout where Dr. Pamela Gay, renowed astronomer and educator interviews scientists involved in
This subcommunity is dedicated to explore the topic of comets and their probable importance for life on Earth. This space will be populated with relevant tools and resources to help the construction of innovative and engaging scenarios related to comets and its exploration. This community is part of the ISE hangouts series devoted to Astronomy and Space Science. Each community has an associated hangout where Dr. Pamela Gay, renowed astronomer and educator interviews scientists involved in
This community brings together teachers who are using resources, virtual experiments and online labs from the fields of Astronomy and High Energy Physics (HEP). Among other activities, it offers access training, resources and to a network of robotic telescopes and the major CERN experiments, ATLAS and CMS. Transit of Mercury 2016 Live at: http://ustre.am/1vYJ6 The organisers of the recent projects IYA2009 - Shape of the Earth, ERATOSTHENES experiment and IYA2009 - Distance to the Moon and
Today, we are able to study the universe in many colors that can’t be seen with our eyes. From detecting X-rays, to listening to the radio universe, we are able to use digital detectors to “see” hidden aspects of distant objects. In this Hangout, we will review the electromagnetic spectrum... This community is part of the collection of communities devoted to the Inspiring Science Educaiton Hangout Series. Each community has an associated hangout where Dr. Pamela Gay, renowed astronomer and
Much of the evolution of the universe can be described through the pull of gravity and push of pressure. Gravity condenses gas, it heats up, and if it can, it expands, and if it can’t, stars are formed. In this Hangout, we will consider the gas laws, and look at different kinds of nebulae. This community is part of the collection of communities devoted to the Inspiring Science Educaiton Hangout Series. Each community has an associated hangout where Dr. Pamela Gay, renowed astronomer and educator
This community will enable teachers, students and researchers involved in extended collaborative activities. It introducesthem to the field of science through the use of resources and tools bringing together a network of educational communities, eLearning tools and resources and relevant partners of the field. Through the Inspiring Science Education website and the activities organised by the partners, teachers can help students make their own scientific discoveries, witness and understand
In this community all digital ISE-Demonstrators are available: Demonstrators show you how the the ISE pedagogical approach can be implemented in practice. You can use Demonstrators as they are or clone it and adapt it to your own requirements.
Our universe started as a fog of particles, but slight variations in density allowed the formation of stars, galaxies, and the large-scale structures of the universe. In this Hangout we’ll discuss early structure formation and fast forward to today’s stars with planets. This community is part of the collection of communities created in the framework of Inspiring Science Education Hangout Series. Each community has an associated hangout where Dr. Pamela Gay, renowed astronomer and educator
The Earth is warm because energy created in the core of the Sun is able to travel from the Sun’s Core to its surface, and then shine through space all the way to Earth. As it travels, the light is transformed from deadly high-energy particles to the nice warm light that keeps us alive. In this Hangout, we will discuss the primary ways energy is transported: convection, conduction, and radiation. This community is part of the collection of communities devoted to the Inspiring Science Education
We can’t observer how the universe formed, but scientists are still willing to say that we know the universe was created through a Big Bang. In this scenario, students will learn the three main lines of evidence for the Big Bang: the universe is expanding, the Cosmic Microwave Radiation, and the mixture of chemical elements. This community is part of the ISE hangouts series devoted to Astronomy and Space Science. Each community has an associated hangout where Dr. Pamela Gay, renowed astronomer
Everything in our universe is made up of a very small numbers of particles, and is controlled by just four forces. In this community, we will discuss these basic building blocks of everything. This community is part of the ISE hangouts series devoted to Astronomy and Space Science. Each community has an associated hangout where Dr. Pamela Gay, renowed astronomer and educator interviews scientists involved in research related to the topic being addressed by the hangout. You can find the hangout
