Part 6 of 9 COSMO; The Infinity; the entirety; the dimension; the center; the temperature; the elements; the galaxy, the star, and the celestial objects
Part 6 of 9 Article: Cosmic Knowledges
My Blog Title: COSMO; The Infinity; the entirety; the dimension; the center; the temperature; the elements; the galaxy, the star, and the celestial objects
| [Refer to Part 1 of 9 combined references] |
Star is a hot dense gas of mostly hydrogen and some helium and other elements. Stellar classification is based on star spectral compound color temperature from hottest to the least hot. Color code of star is based on the spectral class of red, orange, yellow, green, white and blue. The temperature fluctuates from 2,000 Kelvin to 50,000 Kelvin. The least hot is red; medium hot is orange, yellow and green; hotter and hottest is white and blue. The hotter the surface of a star, the blazing the light becomes. Dimmer light is red light, Infrared and near infrared light. Ultraviolet has a predominant color of purple mixture of red and blue. The violet is purpler and so-called ultraviolet, when violet color is paired with other colors.
Red, green and blue light combined in equal measure radiates white light, when light is cosmological constant. A fraction strand of white light is split into rainbow color, a reverse prism. Rainbow is the spectral code reflection of our sun surface temperature. From TRACE telescope observation and analysis, the sun core is a plasma fission from hydrogen to helium at above 15 million Kelvins. The sun flare is between 10 million Kelvins to 100 million Kelvins. Scientists predict that our sun will become white dwarf star in the next 5 billion years. The biggest star in the universe is UY-Scuti, 1700 times the width of the sun, 2.4 billion kilometers in diameter, a hypergiant near the center of the Milky Way galaxy. Astronomers estimate that there are 1 septillion stars in the universe, which is 1 followed by 24 zeros; and our Milky Way galaxy contains more than 100 billion stars. Some low-mass stars can shine trillions of years longer than the universe has existed, while some massive stars will live only a few million years and our sun is a medium age yellow dwarf star. The surface temperature of the sun is on average 6,000 Kelvin, and the scorching sun's surface radiates photonic light in all colors from red to yellow, orange, green, white, blue, and ultraviolet. Earth's atmospheric layers and magnetic field shield off most of the photonic color element from solar radiation; that is why our atmosphere, so-called sky is blue in day time; aurora is deflected in red, green, ultraviolet, blue at night time; and rainbow is reflected in all color bands of light.
Sound Sources and Titles: Pixabay
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Picture sources: Pixabay and Pexels in PowerDirector and other websites:
3:https://people.com/northern-lights-united-states-2023-everything-to-know-7559020
4:https://svs.gsfc.nasa.gov/11418
5:https://solar-center.stanford.edu/SID/activities/GreenSun.html
6:https://webbtelescope.org/contents/media/images/4190-Image
7:https://www.pablocarlosbudassi.com/2021/02/the-infographic-and-artistic-work-named.html?m=1
8:https://alldimensions.fandom.com/wiki/UY_Scuti
9:https://www.pablocarlosbudassi.com/2021/02/atlas-of-universe-is-linear-version-of_15.html?m=1
10:https://byjus.com/physics/life-cycle-of-stars/
11:https://science.nasa.gov/mission/trace/
12:https://science.nasa.gov/sun/exploration/
13:https://www.snexplores.org/article/explainer-rainbows-fogbows-and-cousins
14:https://wallpapers.com/images/featured-full/rainbow-pictures-povwnf60sljd1snu.jpg
15:https://www.usatoday.com/story/news/nation/2013/05/14/sun-halo-rainbow/2159577/
16:https://wonderopolis.org/wonder/what-are-prisms
17:https://ux.byu.edu/cmyk-and-rgb-understanding-your-color-modes
19:https://www.nasa.gov/image-article/field-of-stars/
20:https://esahubble.org/images/opo1801a/
21:https://svs.gsfc.nasa.gov/vis/a030000/a030900/a030948/omega_cen_core-hst-6310x3225_print.jpg
Video Sources:
1:Pixabay and Pexels in PowerDirector
2:https://svs.gsfc.nasa.gov/11418
3:https://svs.gsfc.nasa.gov/vis/a000000/a000200/a000298/a000298.mp4
Consulted references [Refer to Part 1 of 9 combined references]


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