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12 Introduction to Cepheid Variable Stars Exercise
12 Introduction to Cepheid Variable Stars Exercise

Leaving the Main Sequence
Leaving the Main Sequence

... • Degenerate-electron pressure is independent of temperature. • He heats up, He burning happens faster. • Without having a “ pressure safety valve”, temperature becomes too high to make the ...
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Measuring Distances - Stockton University
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Slide 1
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June - Magic Valley Astronomical Society
June - Magic Valley Astronomical Society

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... • Stars “move” East to West over the course of one Night (in circle about the North Star) • Stars “move” East to West by 2 hours per month and “return” to the same position after one Year • It’s just caused by Earth’s daily spin and yearly orbit about the Sun • Star wheel depends on latitude: northe ...
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... At their maximum brightness, supernovae are as bright as an entire galaxy. ...
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... They showed a photometric variability as large as ∼0.36 mag between series, so the system was monitored for a single, 4-hour interval on the night of September 2, 2009, and an orbital period was determined. Another similar 4-hour time-series was covered in the Johnson B-band with the SAAO 1m telesco ...
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... C. It is moving away from the Earth. D. It will live longer than a B spectral class main sequence star. E. It is the same size as a red giant star of the same temperature. 28. There are reported to be about 6,000 stars visible to the naked eye. How many of those stars would you expect to be part of ...
January 2015 - Newbury Astronomical Society
January 2015 - Newbury Astronomical Society

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... 16. What do these super large stars produce? 17. What happens when 2 neutron stars collide? What is produced? 18. What is the chance of a collision between the sun and another star? Failed Stars (After 5th intro frame) 19. What are “blue stragglers”? 20. Which types of stars are known as “failed sta ...
10.1 Introduction
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... Figure 10.6). At a distance of only 2.4 pc, Wolf 359 is the fifth closest star to the Sun, after the three stars that make up the α Centauri system and Barnard’s star. Its spectral type is M6.0 V and its luminosity is 0.001L ; ...
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... Meteors: Pieces of this dust or debris that enter the atmosphere and burns up. These are also known as ‘shooting stars’ or ‘falling stars’. Most burn up and never land at the surface. Fireball: Is simply a very bright meteor, generated by a larger chunk or rock. Fireballs can make it to the ground, ...
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... • Red galaxies have lots of red stars (both giants and main sequence). • Blue galaxies have both blue and red main sequence… but probably not a lot of red giants yet. – Blue MS are much more luminous than red MS so a population with both would appear mostly blue. ...
PARALLAX EXERCISE1 The goal of this exercise is to introduce the
PARALLAX EXERCISE1 The goal of this exercise is to introduce the

... The measurements that you made above are quite similar to those made by astronomers in order to measure the distances to nearby stars. The big difference is that even the nearest stars are quite far away compared to the diameter of the Earth’s orbit around the Sun. Because the stars are so far away, ...
parallax
parallax

... The measurements that you made above are quite similar to those made by astronomers in order to measure the distances to nearby stars. The big difference is that even the nearest stars are quite far away compared to the diameter of the Earth’s orbit around the Sun. Because the stars are so far away, ...
Patterns in the Night Sky
Patterns in the Night Sky

... Although we can mark out the same constellations our ancient ancestors saw thousands of years ago, their component stars are not in exactly the same location as they were then. Precise observations of stars reveal that they move relative to each other in space, but these changes in position occur s ...
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Boötes



Boötes /boʊˈoʊtiːz/ is a constellation in the northern sky, located between 0° and +60° declination, and 13 and 16 hours of right ascension on the celestial sphere. The name comes from the Greek Βοώτης, Boōtēs, meaning herdsman or plowman (literally, ox-driver; from βοῦς bous “cow”). The ""ö"" in the name is a diaeresis, not an umlaut, meaning that each 'o' is to be pronounced separately.One of the 48 constellations described by the 2nd century astronomer Ptolemy, Boötes is now one of the 88 modern constellations. It contains the fourth brightest star in the night sky, the orange-hued Arcturus. Boötes is home to many other bright stars, including eight above the fourth magnitude and an additional 21 above the fifth magnitude, making a total of 29 stars easily visible to the naked eye.
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