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Project “COLOR” due TODAY
Project “COLOR” due TODAY

Chapter 27.1
Chapter 27.1

...  Other differences include composition, temperature, brightness, and distance from earth. ...
How Far is far ?
How Far is far ?

... All galaxies are Red -Shifted • Their light is shifted lower in frequency, meaning they are moving away from us. • The farther away they are, the more they’re red-shifted, the faster they’re moving. • This was the first strong piece of evidence that the universe is expanding. ...
Pistol Star - University of Dayton
Pistol Star - University of Dayton

... •Made from granules caused by convection currents that carry energy to the surface •These dark spots are the cooler areas of descending gas, which may be small and last a few days, or they can be 150,000km and last for months •Sunspots are 1000 degrees cooler than surrounding area and put off half ...
1. Which of the following statements is incorrect concerning sidereal
1. Which of the following statements is incorrect concerning sidereal

... A. Cepheid variables obey a period luminosity relationship but RR-Lyra stars do not B. Cepheid variables are much more luminous than RR-Lyra variables because they have much larger surface areas C. RR-Lyra stars have a variation period that is so short it cannot be measured as accurately as for Ceph ...
Astronomy Assignment #1
Astronomy Assignment #1

... 12. Star C and star D are at the same distance from us, but star D is 10,000 times more luminous than star C. How do their brightness levels compare? Star D will appear brighter by a factor of 10,000 over star C. 13. How do the magnitudes of stars C and D in problem 4 compare? (Problem 4 synopsis: ...
Stellar Nucleosynthesis
Stellar Nucleosynthesis

... into space (supernovae), the processed material can be incorporated into gas clouds that will later form stars and planets. • The material that formed our solar system incorporated some of the remains of previous stars. • All of the atoms on the Earth except hydrogen and most of the helium are recyc ...
Matariki-Maori New Year
Matariki-Maori New Year

... Looking west this shows the Sun setting - from mid-winter through the equinox to mid-summer (Northern Hemisphere view). What dates are these? ...
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Lesson Plan - ScienceA2Z.com

... The International Astronomical Union (IAU) divides the sky into 88 official constellations with exact boundaries, so that every direction or place in the sky belongs within one constellation. In the northern hemisphere, these are mostly based upon the constellations of the ancient Greek tradition, p ...
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The Magnitude Scale

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Simple Winter Star - Dark Sky Discovery

Wednesday, November 7, 2007
Wednesday, November 7, 2007

... pressure to resist gravity. • A hotter interior results in thermonuclear fusion proceeding more efficiently. Conversion of (stored) energy from mass into heat & light proceeds faster, so the star has a higher luminosity. We’re talking about the theory of the structure of a star here, because we are us ...
Earth`s Motion and Seasons
Earth`s Motion and Seasons

... The light from street lights, businesses, and signs make it difficult to objects in the night sky. This is known as light pollution. Round table brainstorm how our community could develop a plan to reduce light pollution. ...
September 2013 - astronomy for beginners
September 2013 - astronomy for beginners

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... The size and location of the HZ depends on the nature of the star The situation becomes even more extreme in the case of a red dwarf, such as Barnard's Star (M4: about 2,000 times less luminous than the Sun), the HZ of which would extend only between about 750,000 and 2 million km (0.02 to 0.06 AU) ...
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... ______ 8. large, cool star in third stage of its life cycle 9. Explain how energy is generated in the core of a star during the second stage of its life cycle. _______________________________________________________________________________________________________ ____________________________________ ...
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... It is the tiniest star, having collapsed into a superdense state. It is thought to have formed when a large star exploded as a supernova. ...
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... • Outside measuring the sun or the stars: Many possible conditions --clouds, fog, water vapor, air pollution, smoke. All absorb or scatter light which decreases the amount that comes through. • Also, sunlight and starlight reflect off the “top” of the atmosphere and never reach the Earth. For the su ...
The life and times of stars
The life and times of stars

... White light is made up from light of many colours – a rainbow Light can be thought of a made of particles called photons, but also as waves! The different colours represent different energy levels of the photons – e.g. a blue photon is more energetic than a red photon A blue photon has a shorter wav ...
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... 5. As the disk of dust and gas cools, the material within it begins to clump together. The young star can react quite violently, and produce a very strong stellar wind. Some of the clumps are large and dense enough to avoid being blown away by this wind, they likely become planets. 6. A star spends ...
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SGL 9 NGC Galaxy magnitude 9/10 observing challenge Up for

... It is Friday the 4th April. It is 9.30pm and its dark and the sky is clear. Time to start. Due South, almost overhead is Lynx. Use the TAKI charts and detailed CDC charts attached to find the objects. Object 1 – NGC 2683 (Taki page 53) A lovely edge of spiral galaxy some 30 million light years away. ...
16SolMW - NMSU Astronomy
16SolMW - NMSU Astronomy

Aspire: Star Life Cycle - Easy Peasy All-in
Aspire: Star Life Cycle - Easy Peasy All-in

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CH29 The Life of a Star

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Perseus (constellation)



Perseus, named after the Greek mythological hero Perseus, is a constellation in the northern sky. It was one of 48 listed by the 2nd-century astronomer Ptolemy and among the 88 modern constellations defined by the International Astronomical Union (IAU). It is located in the northern celestial hemisphere near several other constellations named after legends surrounding Perseus, including Andromeda to the west and Cassiopeia to the north. Perseus is also bordered by Aries and Taurus to the south, Auriga to the east, Camelopardalis to the north, and Triangulum to the west.The galactic plane of the Milky Way passes through Perseus but is mostly obscured by molecular clouds. The constellation's brightest star is the yellow-white supergiant Alpha Persei (also called Mirfak), which shines at magnitude 1.79. It and many of the surrounding stars are members of an open cluster known as the Alpha Persei Cluster. The best-known star, however, is Algol (Beta Persei), linked with ominous legends because of its variability, which is noticeable to the naked eye. Rather than being an intrinsically variable star, it is an eclipsing binary. Other notable star systems in Perseus include X Persei, a binary system containing a neutron star, and GK Persei, a nova that peaked at magnitude 0.2 in 1901. The Double Cluster, comprising two open clusters quite near each other in the sky, was known to the ancient Chinese. The constellation gives its name to the Perseus Cluster (Abell 426), a massive galaxy cluster located 250 million light-years from Earth. It hosts the radiant of the annual Perseids meteor shower—one of the most prominent meteor showers in the sky.
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