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  1. combined, two stars at the same temperature can be vastly different in brightness because of their sizes. Image: Betelgeuse (Hubble Space Telescope.) It is 950 times bigger than the sun! The basic formula that relates stellar light output (called luminosity) with the surface area of a star, and the temperature of the star, is L = A x F where the

  2. Problem 494: The Close Encounter to the Sun of Barnards Star Students use parametric equations and calculus to determine the linear equation for the path of Barnards Star, and then determine when the minimum distance to the sun occurs [Grade: 12 | Topics: Derivitives and minimization] Problem 490: LL Pegasi - A Perfect Spiral in Space The star LL Persei is ejecting gas like a sprinkler on a ...

  3. Pollux is ≈ 8 times larger than the sun. NB: Thanks to the Stefan-Boltzmann law, astronomers can calculate the radii of the stars. The brightness of a star is: L = 4πσR2T4 L is the brightness, σ is the Stefan-Boltzmann constant, R the radius of the star and T the temperature.

  4. Sep 16, 2020 · When a star that is eight times larger than the sun ends its life, it does not go gentle into that good night. Shifting pressure in its core causes it to collapse and trigger a supernova, the largest explosion in the universe. The initial flash of light, which can outshine the star’s host galaxy, may last only seconds.

  5. 22. According to current knowledge, yes. If the gas cloud is too massive, the pressure of the radiation prevents the collapse and the star formation. The article Stars Have a Size Limit by Michael Schirber, it's about 150 Solar Masses. However, there's the Pistol Star, which is speculated to be 200 SM. In the article 'Das wechselhafte Leben der ...

  6. spacemath.gsfc.nasa.gov › EarthSciSpace Math - NASA

    ( e.g if Star A is 6 times larger than Star B, and Star C is 1/2 the size of Star B, how big is Star C in terms of Star A?) [Grade: 4-6 | Topics: working with fractions; scale models] Problem 158: The Solar Neighborhod within 17 Light Years - Students create a scale model of the local solar neighborhood and determine the shortest travel distances to several stars.

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  8. Jul 4, 2024 · After the main sequence, a high-mass star finishes its life cycle in the following evolutionary stages: Red supergiant → supernova → neutron star (or black hole) The key differences between a lower mass and higher mass star at this stage are: A higher mass star will stay on the main sequence for a shorter time before it becomes a red ...

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