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  1. Science Year 4Unit 9: Earth (The gravitational pull on Earth, the rotation of Earth on its axis and the revolution of Earth around the Sun ) The extra note a...

    • 8 min
    • 5.9K
    • CikguDila Juhan
  2. Stars, Planets, and the Earth | Science for Kids | Grade 4 | PeriwinkleWatch our other videos:English Stories for Kids: https://www.youtube.com/playlist?list...

    • 14 min
    • 64.4K
    • Periwinkle
  3. Feb 8, 2023 · Perhaps you’ve seen videos of how the planets of the solar system move through the universe in this cool helix. Not only are these misleading, but the Earth’s real motion - YOUR motion through ...

    • 16 min
  4. Move the sun, earth, moon and space station to see how it affects their gravitational forces and orbital paths. Visualize the sizes and distances between different heavenly bodies, and turn off gravity to see what would happen without it!

    • Clues from Our Past
    • Looking to Our Future
    • Building Our Knowledge of How Stars and Planets Begin

    In cosmic phenomena, we see echoes of our distant past. Massive clouds of gas and dust condense into centralized protostars, that in turn emit powerful solar wind and bursts of radiation. A newborn star emerges from its molecular cloud nursery. Material left over from the star’s formation collapses into protoplanets. Each of these observations—now ...

    Stars follow different paths as they age, determined by their mass, with the most massive burning their fuel exponentially faster. Smaller stars, like our Sun, live long lives. As they start to run out of hydrogen fuel in their core, they expand and turn red, becoming red giants. The byproducts of fusion collect in the core and, if the star is mass...

    Our current understanding of how, when, and where stars and planets form and evolve is advanced through theory and observation. Data from current and next-generation telescopes will inform new computational models for stellar and planetary life cycles. These models are refined and may yield new theoretical discoveries which are in turn tested again...

  5. 3.3 Newton’s Universal Law of Gravitation. By the end of this section, you will be able to: Newton’s laws of motion show that objects at rest will stay at rest and those in motion will continue moving uniformly in a straight line unless acted upon by a force. Thus, it is the straight line that defines the most natural state of motion.

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  7. Jul 23, 2019 · The life and death of stars form the ingredients that make up Earth, making stars critical to life as we know it. The early universe contained nothing but the chemical elements hydrogen, helium, and tiny amounts of lithium and beryllium. During their life cycles, stars create elements with low atomic masses. These are the first 26 elements in ...