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  1. Feb 2, 2016 · The stars in our galactic neighbourhood do have a dynamical, gravitational effect on the inner workings of the solar system:. They built the Oort cloud. The Oort cloud is a roughly spherical cloud of icy bodies that is thought to act as a reservoir of long-period comets (and which we speculate exists to explain said comets' existence).

    • Callisto

      Q&A for active researchers, academics and students of...

    • Stellar Evolution
    • The Fate of Medium-Sized Stars
    • The Fate of Massive Stars

    A star is born, lives, and dies, much like everything else in nature. Using observations of stars in all phases of their lives, astronomers have constructed a lifecycle that all stars appear to go through. The fate and life of a star depends primarily on it's mass. All stars begin their lives from the collapse of material in a giant molecular cloud...

    When a medium-sized star (up to about 7 times the mass of the Sun) reaches the red giant phase of its life, the core will have enough heat and pressure to cause helium to fuse into carbon, giving the core a brief reprieve from its collapse. Once the helium in the core is gone, the star will shed most of its mass, forming a cloud of material called ...

    A red giant star with more than 7 times the mass of the Sun is fated for a more spectacular ending. These high-mass stars go through some of the same steps as the medium-mass stars. First, the outer layers swell out into a giant star, but even bigger, forming a red supergiant. Next, the core starts to shrink, becoming very hot and dense. Then, fusi...

  2. 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.

    • Adapted by Jean Creighton
    • 2019
  3. Apr 10, 2022 · Newton’s universal law of gravitation says that the force acting upon (and therefore the acceleration of) an object toward Earth should be inversely proportional to the square of its distance from the center of Earth. Objects like apples at the surface of Earth, at a distance of one Earth-radius from the center of Earth, are observed to ...

  4. Objects like apples at the surface of Earth, at a distance of one Earth-radius from the center of Earth, are observed to accelerate downward at 9.8 meters per second per second (9.8 m/s 2) (9.8 m/s 2). It is this force of gravity on the surface of Earth that gives us our sense of weight.

  5. science.nasa.gov › universe › starsStars - NASA Science

    Stars form in large clouds of gas and dust called molecular clouds. Molecular clouds range from 1,000 to 10 million times the mass of the Sun and can span as much as hundreds of light-years. Molecular clouds are cold which causes gas to clump, creating high-density pockets. Some of these clumps can collide with each other or collect more matter ...

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  7. Jan 6, 2022 · Some things—space probes and satellites spinning over our heads—never come down. And the idea of gravity as a simple up-down force happening purely on Earth is very wrong too. Gravity is like invisible elastic stretched through the whole universe, holding the stars and planets together and pulling them toward one another. Much more ...

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