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Astronomy 103
Astronomy 103

... William Wollaston in England, and Joseph Fraunhofer in Bavaria developed the spectroscope in the early 1800's. Wollaston was the first to see dark lines in the spectrum of the Sun and by 1863, it was known that these dark lines were identical to patterns of spectral lines from particular elements fo ...
Answers
Answers

... stars with different starting masses. ☆ Select a different starting mass for your star in the ‘Star Properties’ banner. ☆ Use the Hertzsprung-Russell diagram tab, click play to watch your new stars evolution. ☆ Try out a few different masses then answer the following questions. 1. Using the Hertzspr ...
The life of Stars
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... • Radius: 10-100 solar radii ...
Introduction to the HR Diagram
Introduction to the HR Diagram

... located in the upper right-hand corner of the H-R diagram. As the central core of a main sequence star with a mass from ~0.8 to 8 solar masses runs out of hydrogen, radiation pressure no longer balances gravity and the star begins to collapse. There is still hydrogen in the outer layers surrounding ...
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... cells told hormones called androgens to turn on during development, causing your body to form male hormones and parts or female hormones and parts. Your brain and spinal cord developed first, and then your cells differentiated (changed) into different organs and parts. By the time your mother was fo ...
Stellar Evolution - Academic Computer Center
Stellar Evolution - Academic Computer Center

The Evolution of Low Mass Stars
The Evolution of Low Mass Stars

... consume that fuel at a much higher rate than less massive stars. As a result, more massive stars exhaust their fuel much faster and have shorter main sequence lifetimes. The lifetimes for the most massive stars are only a few million years while the least massive stars fuse hydrogen for trillions of ...
Life on the Main Sequence + Expansion to Red Giant
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... I. Main-Sequence Stars A. Stellar Models B. Why is there a Main Sequence? C. The Upper End of the Main Sequence D. The Lower End of the Main Sequence E. The Life of a Main-Sequence Star F. The Life Expectancies of Stars II. Post-Main-Sequence Evolution A. Expansion into a Giant ...
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... Canis major represented either a two-headed dog, a dog that was a gift from Zeus to Europa, or Orion’s hunting dog, helping him to fight Taurus. ...
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The Life of a Star

... previous fusion reactions (primary & secondary fusion reactions): Hydrogen →Helium → Carbon → Neon → Silicon → Iron – When ALL fusion reactions stop, gravity takes over and the star collapses inwards. ...
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... It is a system of stars, dust, and gas held together by gravity. There are three basic types: spiral, elliptical, and irregular. A spiral galaxy is a flattened, discus-shaped collection of stars, having a central bulge. Examples include the Milky Way and Andromeda. An elliptical galaxy ranges in sha ...
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... 26. What is the mass range of stars that will create planetary nebulae and white dwarfs? 27. What is the mass of the core that makes a white dwarf and how big is the white dwarf? 28. Click on “White Dwarf”. Read the description and explain how the mass of a spoonful of white dwarf material can weigh ...
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... • The background color in this diagram indicates the temperature of the stars. • The Sun is a yellow-white G2 star. • Most stars including the Sun have properties along the mainsequence strip running from hot high-luminosity stars at upper left to cool low-luminosity stars at lower right. Fig. 9-8, ...
PPT file
PPT file

... “there are more stars in the universe than grains of sand on all the beaches of Earth.” In between stars there is interstellar matter, which is made up of gas (mostly Hydrogen) and dust. Birth of a Star Gravity attracts chunks of gas and dust in a nebula to come ...
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Why is there a main sequence?

... I. Main-Sequence Stars A. Stellar Models B. Why is there a Main Sequence? C. The Upper End of the Main Sequence D. The Lower End of the Main Sequence E. The Life of a Main-Sequence Star F. The Life Expectancies of Stars II. Post-Main-Sequence Evolution A. Expansion into a Giant ...
TY Course Day 2 Friday Constellations v1
TY Course Day 2 Friday Constellations v1

< 1 ... 63 64 65 66 67 68 69 70 71 ... 132 >

Corona Borealis

Corona Borealis /kɵˈroʊnə bɒriˈælɨs/ is a small constellation in the Northern Celestial Hemisphere. It is one of the 48 constellations listed by the 2nd-century astronomer Ptolemy, and remains one of the 88 modern constellations. Its brightest stars form a semicircular arc. Its Latin name, inspired by its shape, means ""northern crown"". In classical mythology Corona Borealis generally represented the crown given by the god Dionysus to the Cretan princess Ariadne and set by him in the heavens. Other cultures likened the pattern to a circle of elders, an eagle's nest, a bear's den, or even a smokehole. Ptolemy also listed a southern counterpart, Corona Australis, with a similar pattern. The brightest star is the magnitude 2.2 Alpha Coronae Borealis. The yellow supergiant R Coronae Borealis is the prototype of a rare class of giant stars—the R Coronae Borealis variables—that are extremely hydrogen deficient, and thought to result from the merger of two white dwarfs. T Coronae Borealis, also known as the Blaze Star, is another unusual type of variable star known as a recurrent nova. Normally of magnitude 10, it last flared up to magnitude 2 in 1946. ADS 9731 and Sigma Coronae Borealis are multiple star systems with six and five components respectively. Five star systems have been found to have Jupiter-sized exoplanets. Abell 2065 is a highly concentrated galaxy cluster one billion light-years from our Solar System containing more than 400 members, and is itself part of the larger Corona Borealis Supercluster.
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