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Big Bang Theory
Big Bang Theory

... by, the pitch of its siren gets lower. This occurs because of the Doppler shift. Sound waves are compressed as the ambulance approaches, causing the pitch to be higher. As the ambulance drives away, the sound waves are spread apart, causing the pitch to be lower. A similar effect occurs if a star or ...
Star Map - Science Centre
Star Map - Science Centre

... The Big Dipper is one of the most famous asterisms (star patterns) throughout history. In some places of the Northern Hemisphere, its seven brightest stars can be seen all year round. Further South near the equator, it is only visible for a few months. Merak and Dubhe are known as The Pointers, poin ...
3P15.pdf
3P15.pdf

... The excess emission is the surface flux obtained by subtracting the contribution of the photosphere to the total surface flux emitted by the star. Fig. 4a to 7a show, for all the stars of the sample, the mean value of the excess emission of the Hα line vs. the mean value of the excess emission of ot ...
Hertzsprung Rusell Diagram KLT
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... Stars that look to us as though they are near each other, may intact be very far away from each other. Distant but very bright stars look similar to close but dim stars. ...
ASTR1102-002 Potentially useful facts and mathematical relations
ASTR1102-002 Potentially useful facts and mathematical relations

... If the star “Alpha Centauri A” (see Table 1) were moved twice as far away from us, how much brighter/fainter would it become as viewed on the night sky? a. “Alpha Centauri A” would become half as bright. b. “Alpha Centauri A” would become one-fourth as bright. c. “Alpha Centauri A” would become twic ...
August 2014 Saguaro Skies
August 2014 Saguaro Skies

... Aquila, Cygnus and Lacerta. Beginning with the western most, in Aquila, is the planetary nebula NGC6804 that is rather faint but has an irregular shape. The next two are the famous Veil Nebulae, in Cygnus, and are NGC6960 the western part and NGC6992 the eastern part. The western part is bright and ...
The Origin, Structure, and Evolution of the Stars
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... believe that some of the small dark globules found throughout the bright nebulous regions (as can be seen in Figure 3) are the initial phases of star formation. As the protostar continues to contract, one-half of the potential energy stored up in the gravitational field is converted to heat and incr ...
Astr 102 Lec 6: Basic Properties of Stars
Astr 102 Lec 6: Basic Properties of Stars

... Which of these stars actually is highly luminous? ...
File
File

...  A star's birth mass is the most important predictor of a star's luminosity. A star born with low mass will have a high luminosity; a star born with high mass will have a significantly lower luminosity.  A star's birth mass is the most important predictor of a star's surface temperature. A star born ...
Lab PDF - NMSU Astronomy
Lab PDF - NMSU Astronomy

... On a clear, dark night, one might see more than two thousand stars. Unlike our distant ancestors, we recognize that each one is a huge ball of hot gas that radiates energy, like our own (very nearby) star, the Sun. Like the Sun, the stars shine by converting hydrogen into helium via nuclear fusion r ...
A) Polaris B) Betelgeuse C) Procyon B D) Sirius 1. Which star has a
A) Polaris B) Betelgeuse C) Procyon B D) Sirius 1. Which star has a

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The Physical Properties of Normal A Stars
The Physical Properties of Normal A Stars

... Binary star studies can lead to masses and also for eclipsing systems radii as well. The following values based on modern binary data from Harmanec (1988). ...
HR Diagram
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DSLR Photometry
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Spatial distribution of stars in the Milky Way
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... galaxy may be 100 billion. Thus, more than 10 billion trillion stars may exist. But if you look at the night sky far from city lights, you can see only about 3,000 of them without using binoculars or a telescope. Stars, like people, have life cycles -- they are born, pass through several phases, and ...
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... An actual HR Diagram is provided in the upper right panel with an active location indicated by a red x. This active location can be dragged around the diagram. The options panel allows you to control the variables plotted on the x-axis: (temperature, BV, or spectral type) and those plotted on the y- ...
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Published in Contemp. Phys. 51, 464-465 (2010).

... it will fade until, in ∼210,000 years time, it will relinquish its title as our brightest star. Sirius would have passed right across the Milky Way during the stone age. One of the Arabic names for Sirius is al-schira al-abur, or “Sirius which has passed across”, raising the fascinating speculation ...
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... of Orion's Belt. It is one of the brightest nebulae, and is visible to the naked eye in the night sky. M42 is located at a distance of 1,344 ± 20 light years and is the closest region of massive star formation to Earth. The M42 nebula is estimated to be 24 light years across. Older texts frequently ...
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... distributed these heavier elements throughout the galaxy so that late-generation stars had small but significant amounts of elements heavier than helium. Our sun, which formed 4.6 billion years ago, is one such star. The Sun: An Average Star After eons of observing the fiery ball they saw in the day ...
LESSON 8: STARS
LESSON 8: STARS

... In composition and size, the Sun is an average star and is in the middle of its hydrogen-burning stage. It will continue to process hydrogen for another few billion years before swelling into a red giant. Although the Sun is an averagesized star, it is still huge by Earthly standards, having a diame ...
PHYS_3380_082615_bw - The University of Texas at Dallas
PHYS_3380_082615_bw - The University of Texas at Dallas

... them to tell what month it is. For example, Scorpius is only visible in the northern hemisphere's evening sky in the summer. - many of the myths associated with the constellations thought to have been invented to help the farmers remember them - made up stories about them ...
Order of Magnitude Icebreaker
Order of Magnitude Icebreaker

... ★ Derive the maximum rate for black hole growth KAS16/MT ...
2-star-life-cycle-and-star-classification
2-star-life-cycle-and-star-classification

... A) to expand as a red giant, undergo a nova outburst and end as a white dwarf B) to shrink to a white dwarf then eventually expand to a red giant C) become hotter and expand into a blue supergiant D) to become a black hole 54. To an observer on Earth, the Sun appears brighter than the star Rigel bec ...
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Canis Major

Canis Major /ˌkeɪnɨs ˈmeɪdʒər/ is a constellation in the southern celestial hemisphere. In the second century, it was included in Ptolemy's 48 constellations, and is counted among the 88 modern constellations. Its name is Latin for ""greater dog"" in contrast to Canis Minor, the ""lesser dog""; both figures are commonly represented as following the constellation of Orion the hunter through the sky. The Milky Way passes through Canis Major and several open clusters lie within its borders, most notably M41.Canis Major contains Sirius, the brightest star in the night sky, known as the ""dog star"". It is bright because of its proximity to our Solar System. In contrast, the other bright stars of the constellation are stars of great distance and high luminosity. At magnitude 1.5, Epsilon Canis Majoris (Adhara) is the second brightest star of the constellation and the brightest source of extreme ultraviolet radiation in the night sky. Next in brightness are the yellow-white supergiant Delta (Wezen) at 1.8, the blue-white giant Beta (Mirzam) at 2.0, blue-white supergiants Eta (Aludra) at 2.4 and Omicron1 at 3.0, and white spectroscopic binary Zeta (Furud), also at 3.0. The red hypergiant VY Canis Majoris is one of the largest stars known, while the neutron star RX J0720.4-3125 has a radius of a mere 5 km.
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