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  1. Using the chalk, the students will draw lines connecting the stars. On the bottom of the paper, the students will write the name of the constellation they chose. Allow the students about 15 minutes to complete the activity. Reconvene and review when the students are finished. Closure/Assessment.

  2. 30 de may. de 2019 · Updated on May 30, 2019. Stellar nucleosynthesis is the process by which elements are created within stars by combining the protons and neutrons together from the nuclei of lighter elements. All of the atoms in the universe began as hydrogen. Fusion inside stars transforms hydrogen into helium, heat, and radiation.

  3. Wetenschappelijke onderwerpen helder uitgelegd op een niveau dat bij je past.

  4. 3 de may. de 2023 · Betelgeuse is a red supergiant star with a distinctive orange-red hue. Stars in this class are nearing the end of their lives. They are the largest stars in the universe because they puff up and expand out into space in their old age. A 2020 image from the Heliospheric Imager aboard NASA’s STEREO spacecraft shows the star Betelgeuse, circled.

  5. 21 de dic. de 2023 · Theorists believe that first-generation stars, known as population III, were made of only the ingredients left over from the big bang, mostly hydrogen and helium. As they burned, they fused those ingredients into heavier elements that astronomers lump together as “metals.”. When the stars exploded as supernovae after lifetimes as short as a ...

  6. 8 de nov. de 2023 · Sandy Ong &. Chris Woolston. Among the fastest-rising researchers in the Nature Index, these four scientists are ones to watch. From investigating strategies for reducing greenhouse-gas emissions ...

  7. 18 de ene. de 2024 · Science. 19 Jan 2024. Astrophysical compact objects come in two varieties: neutron stars and black holes. Created when massive stars die and their cores collapse, neutron stars consist of protons and neutrons, whereas black holes are too heavy and dense to be described by anything other than gravity. These entities have uncertain mass limits.