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Big-Bang
Big-Bang

... validity of the data. It appears that redshift quantization – the phenomenon itself, not the theories trying to explain it – has survived a quarter-century of peer review.” Dr. D. Russell Humpries, “Our galaxy is the centre of the universe, ...
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... Astronomy – Interpreting Main Sequence Star Data The classification of stars by surface temperature and spectral pattern is a painstaking process requiring the efforts of many scientists from hundreds of observatories around the world. To make it easier to refer to the different types of main sequen ...
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... As far as we know, there are nine planets locked in orbit around the Sun. Only one, our own Earth, supports life. But there are countless other suns throughout countless galaxies scattered across the expanse of the universe. We still don’t know if life exists on another planet in some ...
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... Eventually the star will get even smaller than an atom. When matter gets so dense that light cannot escape from it, the region that it is in becomes a black hole. ...
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Questions for The Elements: Forged in Stars

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PowerPoint Template

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Universe of Learning Science Briefing: Our Home, the Milky Way

... But there are types of stars called Red Clump Giants for which we know the intrinsic brightness. They are also fairly common and bright and can be used to trace the structure of the Galaxy. These can be used to measure distances; stars twice as far away are four times fainter. ...
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Stellar evolution, I

... of a plant, or whether a vast number of specimens, selected from every stage through which the plant passes in the course of its existence, be brought at once to our view?” Our knowledge of stellar evolution comes from a combination of data on stars in clusters, plus theoretical models based on the ...
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... Everything you ever wanted to know about where the electrons hang out! ...
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... What are sunspots? Why do they appear dark in pictures of the Sun? Sunspots are dark patches on the Solar photosphere that mark regions where the magnetic field is strong. They are dark because the sunspot is cooler than the rest of the photosphere. Cool gases emit less thermal radiation than hot ga ...
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File - Mr. LaFranca`s Earth Science Class

... produced by nuclear reactions at its core. Nebula: is a huge, diffuse cloud of gas and dust in space Planet: A celestial body moving in an elliptical orbit around a star. Comet: A small, frozen mass of dust and gas revolving around the sun. Moon: small rocky bodies that orbit a planet Asteroid: smal ...
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... Pre Main Sequence – young, low mass stars that are contracting as they evolve toward their main sequence stage. Mostly made of Hydrogen, some Helium, and some trace elements. Of the trace elements, Lithium appears which is an indicator of stellar youth. Often have large protoplanetary accretion disk ...
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... the trampoline is pushing the marble in certain directions. This shows that a large mass warps space (and time). How did observations taken during a solar eclipse help to prove Einstein’s theory of general relativity? Pictures taken before, during, and after an eclipse show that light from stars was ...
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... • Nebulae are the basic building blocks of the universe • They contain the elements from which stars and solar systems are built. • Most nebulae are composed of about 90% hydrogen, 10% helium, and 0.1% heavy elements such as carbon, nitrogen, magnesium, potassium, calcium, iron. ...
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Astronomical spectroscopy



Astronomical spectroscopy is the study of astronomy using the techniques of spectroscopy to measure the spectrum of electromagnetic radiation, including visible light, which radiates from stars and other hot celestial objects. Spectroscopy can be used to derive many properties of distant stars and galaxies, such as their chemical composition, temperature, density, mass, distance, luminosity, and relative motion using Doppler shift measurements.
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