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<> Like Earth, the sun has an interior and an atmosphere. <>/XObject<>/ProcSet[/PDF/Text/ImageB/ImageC/ImageI] >>/MediaBox[ 0 0 720 540] /Contents 8 0 R/Group<>/Tabs/S/StructParents 1>> Composed of plasma escaping from the Sun that reaches 1.000.000 kelvin, but with a density even lower than the chromosphere. The Sun could fit 109 Earths side-by-side across its diameter, and it has enough volume (takes up enough space) to hold about 1.3 million Earths. Every layer of the Sun is very different , and requires a distinct %���� h�bbd``b`��+A�/��b�X��O)����) �( s H V ���ȴ 2 0 obj Rating: How astronomers study the Sun . Evolution of the Sun on the HR diagram 6. endobj •The sun produces an enormous amount of energy in its core, or central region. 1 0 obj Jeans instability 4. Structure of the sun the core the suns core has a tremendously high temperature and pressure the temperature is roughly 15 million c at this temperature nuclear fusion occurs turning four hydrogen nuclei into a single helium nucleus plus a lot of energy. 4 0 obj endobj 9 0 obj Equations of stellar structure 7. endobj Low (EOC) x�u�Kk1������L��7��d $.' The chromosphere this relatively thin layer of the sun is sculpted by magnetic field lines that restrain the electrically charged solar plasma occasionally larger plasma features called prominences form and extend far into the very tenuous and hot corona sometimes ejecting material away from the sun. Because the sun is so large, its gravity is strong enough to hold all of the planets and other distant objects in orbit. The structure of the sun astrophysicists classify the sun as a star of average size temperature and brightness a typical dwarf star just past middle age it has a power output of about 1026watts and is expected to continue producing energy at that rate for another 5 billion years. endstream endobj 540 0 obj <. The sun… Interior structure of the Sun: Outer layers are not to scale The core is where nuclear fusion takes place.
",#(7),01444'9=82. endstream 7 0 obj Kelvin-Helmholtz stage 5. 539 0 obj <> endobj 562 0 obj <>stream %%EOF endobj Hash File: c98de5ee1c14fd36bd0f2c374f27170a.pdf. endobj SC.8.E.5.6 Create models of solar properties including: rotation, structure of the Sun, convection, sunspots, solar flares, and prominences. stream �b``$@���'@� 2�
the structure of the sun Aug 27, 2020 Posted By Andrew Neiderman Publishing TEXT ID 12466973 Online PDF Ebook Epub Library 1996 volume with a clear and structure of the suns interior at deeper layers inside the sun the weight of the outer layers is larger the sun must have a higher temperature and the structure of the sun By Cao Xueqin FILE ID d5240f Freemium Media Library The Structure Of The Sun PAGE #1 : The Structure Of The Sun By Cao Xueqin - the sun does not have a solid surface or continents like earth nor does it have a solid b�G���CE|l*���ofl˨�. 3 0 obj endobj endstream endobj startxref The Sun, like all stars, is an enormous ball of extremely hot, largely ionized gas, shining under its own power.And we do mean enormous. stream
endstream The energy emitted by the surface repesents energy transported from the core through the radiative zone, the convection zone, and finally the photosphere, which by definition Formation and Evolution of the Sun 1. <>>>
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