PPT-The Sun and the Stars
Author : alida-meadow | Published Date : 2017-04-03
The Sun and the Stars Stellar Lifecycle Starbirth Young Stars Globular Clusters Star Death Star Death Star Death Star Death Aims and Objectives To introduce you
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The Sun and the Stars: Transcript
The Sun and the Stars Stellar Lifecycle Starbirth Young Stars Globular Clusters Star Death Star Death Star Death Star Death Aims and Objectives To introduce you to the properties of t he Sun and the stars and their evolution. do not live alone. B. ackground Design E. . Buunk. / S.E. de Mink, . HST image: NASA . Paresce. Selma E. de Mink. Hubble Science Briefing . , . February 7, 2013. Hubble Fellow at Space Telescope Science Institute / Johns Hopkins University. SUN SUN SUN SUN SUN SUN MON MON MON MON MON MON TUE TUE TUE TUE TUE TUE WED WED WED WED WED WED THU THU THU THU THU THU FRI FRI FRI FRI FRI FRI APRIL JUNE AUGUST MAY JULY SEPTEMBER SAT SAT SAT SAT SAT The Sun and the Stars. The Sun and the Stars. Limb darkening. The surface of the sun does not have uniform brightness, it appears bright toward the centre, darker towards the edges, and the colour is redder, an effect known as Limb darkening - why?. The Sun is a Star, but seen close-up. . The Sun is giant ball of very hot, mostly ionized hydrogen gas that shines under its own power.. The Sun . IS NOT . an average, yellow star. . What is the Sun?. Solar Physics. Course structure. My part - 12 lectures: week 1 – week 6. 6 assignments: . 5 (each week) to do at home (5% of final mark). 1 assignment – computational work (10%) ?. Exam: 70% two parts . E.ST.05.23- Explain the apparent movement of the stars (constellations) and sun across the sky. . DAY ONE. Write down everything written in yellow. . CO: I can explain the apparent motion of the stars (constellations) and the sun through the sky. . Elliptical Galaxies. Spiral Galaxies. Barred Spiral. Lenticular. Irregular (. L. arge . M. agellanic . C. loud). Dwarf Spheroidal Galaxy. Isochrone - 2.5x10. 8. yrs. Isochrone - 4x10. 9. yrs. IMF in the ρ Oph Association. Earth Science 11. Chapter 21. Constellations. Constellation:. A groups of stars that appear to form patterns in the sky.. 88 different constellations can be seen from the Northern and Southern hemispheres.. Chapter 2. Stars. Section 1 Vocabulary. Spectrum. Apparent Magnitude. Absolute Magnitude. Light-Year. Parallax. Color of Stars. Red and Yellow. Cool. Blue . Warm. Blue flame hotter than yellow flame. Fairfield Sun focuses on sexual health, offering reviews and guides on penis extenders. It provides discreet and authoritative information, making it a trusted resource for sexual wellness. How do stars work and evolve?. Why do stars shine?. Nuclear reactions. Fusion and fission reactions. How nuclear reactions can create energy. Why is it hard to get fusion nuclear reactions to occur?. A . star is a massive ball of plasma that emits . light and electromagnetic energy . throughout the universe. . While . there is only one star in our solar system, there are billions upon billions of stars throughout our galaxy and exponentially more in the billions of galaxies in the universe. CORE. The sun produces an enormous amount of energy in its core, or central region. The sun's energy comes from nuclear fusion. During nuclear fusion, hydrogen atoms join together to form helium. Nuclear fusion only can take place under conditions of extremely high pressure and temperature. The temperature inside the sun's core reaches 15 million C, high enough for nuclear fusion to take place. . Daisaku Nogami (Kyoto University). 2014/01/23(Thu). Subaru User's Meeting 2013@NAOJ. Collaborators: K. Shibata, H. . Maehara. , S. Honda, T. . Shibayama. ,. S. . Notsu. , Y. .
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