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Birth of Planets with Alma

Astronomers have captured the best image ever of planet formation around an infant star as part of the testing and verification process for the Atacama Large Millimeter/submillimeter Array’s (ALMA) new high-resolution capabilities.

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Black Body Radiation

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.
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CERN's supercollider by Brian Cox - TED talk

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CERNland

CERNland is the virtual theme park developed to bring the excitement of CERN's research to a young audience aged between 7 and 12. CERNland is designed to show children what we do at CERN and inspire them with some physics at the same time. CERNland contains games on all topics related to the CERN activity.

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Comets - A physical model

Instructions on how to build a model of a comet

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Cooking a Comet

Comets are considered to be time capsules containing information about the conditions of the early Solar System. In order to understand what they are, where they come from, and their influence on the evolution of Earth, it is necessary to find out what material they contain. This demonstration and practical activity, along with the resulting discussion, gives an insight into the chemical constituents of comets. An additional activity (extension), which looks at the impact processes on Earth as well as calculations of the kinetic energy involved, is included.

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Digging Into Comets

The solar system is littered with Ice. The bulk of this material orbits quietly in the outer Solar System, but sometimes something disturbs the ice and it comes plunging in toward the Sun. In this lesson, we will discuss comets, how we explore them, and how they brought water to worlds like Earth.
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Eagle Nebula - Pilars of Creation

NASA's Hubble Space Telescope has revisited the famous Pillars of Creation, revealing a sharper and wider view of the structures in this visible-light image.

Astronomers combined several Hubble exposures to assemble the wider view. The towering pillars are about 5 light-years tall. The dark, finger-like feature at bottom right may be a smaller version of the giant pillars. The new image was taken with Hubble's versatile and sharp-eyed Wide Field Camera 3.

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Earth & the Formation of Our Solar System

This activity asks you to explore how planet formation is connected to star formation. Although you learned about star formation in Unit 3, you haven’t yet studied the process of planet formation. The purpose of this activity is to give you an opportunity to use your intuition and logic to make deductions about what might happen next to the matter that is left over after a star has formed.  

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Electromagnetic Spectrum

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 lesson, we will review the electromagnetic spectrum.
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Energy Forms and Changes

Topics

  • Energy
  • Conservation of Energy
  • Energy Systems
  • Energy Forms
  • Energy Changes
  • Thermal Energy

Description

Explore how heating and cooling iron, brick, and water adds or removes energy. See how energy is transferred between objects. Build your own system, with energy sources, changers, and users. Track and visualize how energy flows and changes through your system.

Sample Learning Goals

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Forces Governing Atomic Interactions

Topics

  • Atomic Interactions
  • Interaction Potential
  • Van der Waals Force
  • Atomic Bonding

Description

Explore the interactions between various combinations of two atoms. Turn on the force arrows to see either the total force acting on the atoms or the individual attractive and repulsive forces. Try the "Adjustable Attraction" atom to see how changing the parameters affects the interaction.

Sample Learning Goals

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Gas Laws with Stars and Nebulae

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.
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Gravity Force Lab

Topics

  • Force
  • Gravity
  • Newton's Third Law

Description

Visualize the gravitational force that two objects exert on each other. Change properties of the objects in order to see how it changes the gravity force.

Sample Learning Goals

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