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L = σAT 4
L = σAT 4

... order OBAFGKM. This is the same as a scale of decreasing temperature. Once again the scale is not a ...
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Astronomy 20 Homework # 2

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Lecture 19 - Stellar Lifecycles
Lecture 19 - Stellar Lifecycles

... • The pressures of the surrounding layers are so high that the atoms of the iron core are crushed, smashing the electrons into the protons forming neutrons. • Once neutrons are formed the collapse stops, the surrounding gas is heated and explodes off the core. This is a supernova explosion. • The ex ...
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Lesson Plan - ScienceA2Z.com

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Crux The Southern Cross

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Astronomy Final Study Guide – Name: **This will be the biggest test

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The Ultraluminous X-ray Source in Holmberg IX and its Environment

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Photometric Surveys and Variable stars

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Sample Exam 1

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Final Exam Review

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Candles in the Dark

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Types of Stars http://space.about.com/od/stars/tp/What-Are

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Chapter 5 Galaxies and Star Systems

... that spiral outward, like pinwheels. The spiral arms contain many bright, young stars as well as gas and dust. Most new stars in the spiral galaxies form in theses spiral arms. Relatively few new stars form in the central bulge. Some spiral galaxies, called barred-spiral galaxies, have a huge bar-sh ...
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... far. Choose the correct response from those listed, along with at least a one (1) sentence justification for your answer. Alternate justification techniques include math calculations and labeled sketches. Each question is worth 5 points: 2 for the letter response and 3 for the justification. Collabo ...
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Science Olympiad 2008 Reach for the Stars Division B

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August 2015 - Shasta Astronomy Club

... In the past, such star clusters would have been mistaken for foreground stars because of their brightness. But when these clusters are examined more closely, the single point of light resolves into a fuzzy cluster, and spectrum data reveal it’s much farther away. The width of one of the ultracompact ...
Physics 2028: Great Ideas in Science II: The Changing Earth Module
Physics 2028: Great Ideas in Science II: The Changing Earth Module

... one of these eddies as shown in Figure I-4. 3. As the cloudlet contracts, it spins faster due to the conservation of angular momentum L = M R2 ω, where ω is the angular velocity of the protostellar cloudlet =⇒ since M is constant, as R gets smaller, ω gets larger. This increased spin causes the equa ...
Grade 9 Academic Science – Unit 3 Space
Grade 9 Academic Science – Unit 3 Space

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Cygnus (constellation)



Cygnus /ˈsɪɡnəs/ is a northern constellation lying on the plane of the Milky Way, deriving its name from the Latinized Greek word for swan. The swan is one of the most recognizable constellations of the northern summer and autumn, it features a prominent asterism known as the Northern Cross (in contrast to the Southern Cross). Cygnus was among the 48 constellations listed by the 2nd century astronomer Ptolemy, and it remains one of the 88 modern constellations.Cygnus contains Deneb, one of the brightest stars in the night sky and one corner of the Summer Triangle, as well as some notable X-ray sources and the giant stellar association of Cygnus OB2. One of the stars of this association, NML Cygni, is one of the largest stars currently known. The constellation is also home to Cygnus X-1, a distant X-ray binary containing a supergiant and unseen massive companion that was the first object widely held to be a black hole. Many star systems in Cygnus have known planets as a result of the Kepler Mission observing one patch of the sky, the patch is the area around Cygnus. In addition, most of the eastern part of Cygnus is dominated by the Hercules–Corona Borealis Great Wall, a giant galaxy filament that is the largest known structure in the observable universe; covering most of the northern sky.
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