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Characteristics of Stars
Characteristics of Stars

... and this shows stars in the prime of their lives . . 16.ln these stars, the force of Jlravity pushing in equals the force of nuclear _fusion__ pushing out and so the star is stable. 17. When a nebula grows and the force of gravity attracts more and more dust and gas, the temperature warms and a -pro ...
The Life Cycle of a Star and the Hertzsprung
The Life Cycle of a Star and the Hertzsprung

... Hertzsprung - Russell diagram (H-R diagram). The Hertzsprung - Russell diagram is a tool that shows relationships and differences between stars. It is something of a "family portrait." It shows stars of different ages and in different stages, all at the same time. It is also a great tool to check yo ...
Stellar Evolution
Stellar Evolution

Star- large ball of gas held together by large ball of gas held
Star- large ball of gas held together by large ball of gas held

... outer layers from giant stage dissipate, leaving only a small core when finishes burning, becomes black dwarf (dead star) High temperature, low luminosity ...
The Interstellar Medium and Star Formation
The Interstellar Medium and Star Formation

... planets. Some planets become massive enough to also accumulate Hydrogen and Helium gas. • However, during and after formation, it seems that some planets are able to migrate in their disks, drifting inwards to settle close to the star. We do not know why this did not happen so much in our own Solar ...
The All-Seeing, All-Magnifying Eye
The All-Seeing, All-Magnifying Eye

... galaxies acting as gravitational lenses. In the example above, you will notice that there are two images of each part of the building: one inside the circular ring, which has been turned inside out, and one outside. The lensing effect causes each point in the original image to appear twice in the di ...
Unit 1
Unit 1

... appears to run slow, and the ship looks shorter – To an observer on the ship, the Earth appears to be moving in slow-motion, and its shape is distorted. ...
The Reflector - Peterborough Astronomical Association
The Reflector - Peterborough Astronomical Association

... One of my guests at the observatory that night That was what (in his mind) made the star was the gentleman with the jumping star. He jump. In the time it took for his friend to view mentioned it again and offered to show it to it, and then for him to come to the eyepiece, me. Naturally, I was fascin ...
astronomy - Scioly.org
astronomy - Scioly.org

... 47. RR Lyrae variable stars are typically _________ giant stars? (fill in the blank with a color) 48. Variable stars are stars in which the _______ changes over time. A. Size B. Color C. Shape D. brightness 49. A planet orbits the Sun at 3 AU. How long (in years) does it take to orbit the Sun? (Hint ...
Stellar Physics - University of Reading
Stellar Physics - University of Reading

... Classical Mechanics and Optics  Thermodynamics and Statistical Mechanics  Atomic and Molecular Physics  Ideas from Observational Astronomy ...
Chemically Peculiar/Magnetic Stars and the a photometry
Chemically Peculiar/Magnetic Stars and the a photometry

... Hans Michael Maitzen, Ernst Paunzen Institute for Astronomy, University of Vienna ...
Measuring Stellar Distances
Measuring Stellar Distances

... representative sample of stars? Fortunately, a theoretical argument involving stellar lifetimes serves as a consistency check. In general, star formation events in our galaxy make many more low mass stars than high mass ones. Since high mass stars have very short lifetimes, we would not expect to fi ...
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PHS 111 Test 3 Review Chapters 26-28
PHS 111 Test 3 Review Chapters 26-28

Basic Astronomy Note - Mr. Dewey – Grade 7/8
Basic Astronomy Note - Mr. Dewey – Grade 7/8

... When you look up at the night sky, all of the stars you see are suns - many of which are much larger than our sun – but so incredibly far away they appear to us as tiny points of light. Stars are bodies of gas molecules (hydrogen atoms compressing and fusing into helium). This is nuclear fusion and ...
PHS 111 Test 3 Review Chapters 26-28
PHS 111 Test 3 Review Chapters 26-28

... 10 million years About every 100 million years This has yet to occur on Earth Between which planets is the asteroid belt found? Between Mars and Jupiter Between Earth and Mars Between Earth and Venus Between Jupiter and Neptune For what reason was Pluto demoted from full planetary status in 2006? Be ...
Chapter16
Chapter16

... brown dwarf — A star with too low a mass for nuclear fusion to begin in its core. continuous spectrum — A spectrum containing neither emission nor absorption lines. dwarf — A main sequence star. emission line — A narrow, bright region of the spectrum. Emission lines are produced when electrons in at ...
9binary1i
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... Problems with Binaries Period and Separation In order to resolve the stars they have to have a large separation, but his also means a long period ...
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... Our sun and Proxima Centauri are only two stars that make up our Milky Way galaxy. Our galaxy contains hundreds of billions of stars. There are billions of galaxies in the Universe. ...
PowerPoint Presentation - Super Massive Black Holes
PowerPoint Presentation - Super Massive Black Holes

STAR FORMATION (Ch. 19) - University of Texas Astronomy Home
STAR FORMATION (Ch. 19) - University of Texas Astronomy Home

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... • Color measures the shape of the blackbody curve. – This gives us the star’s temperature! That is the main goal! – The more negative the index, the bluer the light. – The bluer the light, the hotter the object. ...
Comets, Meteors, and Meteoroids
Comets, Meteors, and Meteoroids

... A falling star is a meteor. Meteors are streaks of light in the sky. The light is caused by a small speck of dust burning when it enters the Earth's atmosphere. The dust comes from comets. These pieces of comet dust are called meteoroids. Most meteoroids are smaller than a grain of sand. The flash o ...
PS 224, Fall 2014 HW 4
PS 224, Fall 2014 HW 4

... advanced civilization. Explain your reasoning in one or two sentences each. a. 10 MSun main-sequence star A 10-solar-mass star has a very short lifetime. It also produces copious amounts of ultraviolet radiation that may discourage living organisms. b. 1.5 MSun main-sequence star A 1.5-solar-mass st ...
Bill Nye – Outer Space Worksheet
Bill Nye – Outer Space Worksheet

... c. 540 million kilometers 14. It will take light at least forty years to reach the nearest star. b. False ...
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Ursa Major



Ursa Major /ˈɜrsə ˈmeɪdʒər/ (also known as the Great Bear and Charles' Wain) is a constellation in the northern celestial hemisphere. One of the 48 constellations listed by Ptolemy (second century AD), it remains one of the 88 modern constellations. It can be visible throughout the year in most of the northern hemisphere. Its name, Latin for ""the greater (or larger) she-bear"", stands as a reference to and in direct contrast with Ursa Minor, ""the smaller she-bear"", with which it is frequently associated in mythology and amateur astronomy. The constellation's most recognizable asterism, a group of seven relatively bright stars commonly known as the ""Big Dipper"", ""the Wagon"" or ""the Plough"" (among others), both mimicks the shape of the lesser bear (the ""Little Dipper"") and is commonly used as a navigational pointer towards the current northern pole star, Polaris in Ursa Minor. The Big Dipper and the constellation as a whole have mythological significance in numerous world cultures, usually as a symbol of the north.The third largest constellation in the sky, Ursa Major is home to many deep-sky objects including seven Messier objects, four other NGC objects and I Zwicky 18, the youngest known galaxy in the visible universe.
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