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Distances to the Stars in Leo
Distances to the Stars in Leo

... matter for astronomers, or anyone else for that matter, to determine the absolute magnitude of the star using the distance-magnitude relation. However, most stars are too far away to have a measurable parallax. In these cases, the distance to the star must be determined by some other method. We can ...
Big Bear Valley Astronomical Society
Big Bear Valley Astronomical Society

... over the Bull, which was then placed in the heavens, but for his sacrilege the gods declared that the life of his best friend, Enkidu, should be taken as a forfeit. The chief star, Aldebaran is the 1st magnitude star referred to by Ptolemy as 'the Torch' on account of its bright, rose-colored lumin ...
Universe Notes - Solon City Schools
Universe Notes - Solon City Schools

... an H-R diagram where most stars spend 90% of their life. i. A diagonal band running from the bright, hot stars on the upper left to the dim, cool stars on the lower right ii. Example: The Sun lies in the main sequence ...
Stars: from Adolescence to Old Age
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... But this new period of stability does not last very long As the helium is quickly used up in the fusion into carbon and oxygen, gravity will once more take over The situation is analogous to the end of the main sequence 4 August 2005 ...
HR Diagram Activity - Mr. Alster`s Science Classes
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... Purpose: In this lab we will investigate the relationship between the temperature, brightness and diameter of stars. Introduction The H-R Diagram is a tool that astronomers use to classify stars based on their luminosity, magnitude, temperature, spectral class and evolutionary stage. The H-R Diagram ...
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... 10.For a main sequence star (a typical star), you can generally say that brighter stars are hotter. (Blue is also acceptable, since it is usually true.) ...
AST 207 Homework 7 Due 4 November 2011
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... c. (3 pts.) You ask the student to write an essay on how the platinum nucleus got from that environment into the nose ring. What are essential elements of the essay? 2. Mizar, the first binary star discovered from the spectrum. Even though Mizar appears to be a single star, Pickering’s spectrum show ...
What is the Zodiac? The Zodiac is defined by 12 constellations
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... Claudius Ptolemy of Alexandria (90 – 168 AD) was a Greek astronomer who borrowed his information from the ancient Babylonian texts and he listed the 48 constellations that are recognized as the Zodiac. The IAU (International Astronomical Union) established in 1919 has identified 88 constellations. T ...
Sermon Notes
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blue_giant
blue_giant

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Our Universe
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Chapter 25 PowerPoint
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ASTR-1020: Astronomy II Course Lecture Notes Section III
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... Example III–7. We measure the trigonometric parallax of a visual binary star as 0.20 arcsec and measure an angular separation between the pair of stars in this binary as 5 arcsec. Over a few years of observations, we determine the orbital period of this pair to be 30 years. What is the combined mass ...
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STAR FORMATION (Ch. 19) - University of Texas Astronomy Home
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... disks, and progressing to evolved massive stars in the young starburst cluster.To the upper right of center is the evolved blue supergiant called Sher 25. The star has a unique circumstellar ring of glowing gas that is a galactic twin to the famous ring around the supernova 1987A--see the image of S ...
1 Ay 124 Winter 2016 – HOMEWORK #3
1 Ay 124 Winter 2016 – HOMEWORK #3

... Problem 1 The nearest spiral galaxy to the Milky Way, M31, has a very concentrated nucleus. At a projected radius of 1 arcsec, stars in the nucleus have a line of sight velocity dispersion of 150 km s−1 , and are also rotating about the nucleus at 150 km s−1 . The total luminosity from within 1 arc ...
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Astronomy Exam #4
Astronomy Exam #4

... 26. An O star is known to be eight times the temperature of the Sun and fivr times its radius. What is its luminosity? You may answer either in Watts or in units of solar luminosity. Note: the radius of the Sun is 696,000 km and the temperature of the Sun is 5,800 K. ...
1. How old is our sun now? How does its present luminosity
1. How old is our sun now? How does its present luminosity

... (b) They were probably present over 3 B yrs ago, but were very common 2 to 2.5 B yrs ago, where microfossils are found and also stromatolites, which are layered rocks formed from sediments trapped by growing mats of cyanobacteria. 11. The scales below indicate the sweep of time before the present in ...
Universe 8e Lecture Chapter 17 Nature of Stars
Universe 8e Lecture Chapter 17 Nature of Stars

... shells. These include carbon fusion, neon fusion, oxygen fusion, and silicon fusion. The Deaths of the Most Massive Stars: A star with an initial mass greater than 8 M dies in a violent cataclysm in which its core collapses and most of its matter is ejected into space at high speeds. The luminosity ...
Universe 8e Lecture Chapter 17 Nature of Stars
Universe 8e Lecture Chapter 17 Nature of Stars

... shells. These include carbon fusion, neon fusion, oxygen fusion, and silicon fusion. The Deaths of the Most Massive Stars: A star with an initial mass greater than 8 M dies in a violent cataclysm in which its core collapses and most of its matter is ejected into space at high speeds. The luminosity ...
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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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