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Red Giant Structure There are two important characteristics for the
Red Giant Structure There are two important characteristics for the

Orion - Starry Starry Night!
Orion - Starry Starry Night!

... Canis Major is a constellation in the southern celestial hemisphere. Visible : Jan, Feb, Mar, Apr, Dec Winter - Spring 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 s ...
Classification_of_Stars_By_Luminosity
Classification_of_Stars_By_Luminosity

... The systemisation of apparent magnitude In the nineteenth century systems were developed for measuring exactly how much light was arriving from a star. The intensity of the light (the energy arriving every second per metre 2 at Earth) was calculated. This is sometimes referred to as the apparent br ...
File - the ridgeway ASTRONOMY page
File - the ridgeway ASTRONOMY page

The University of Sydney Page
The University of Sydney Page

... However, if the star is not massive enough, it will never reach high enough temperatures to fuse carbon: this is true for the Sun. So for low mass stars, this is the end of the line. We will now look at the fate of different mass stars: very low mass (< 0.4 solar masses), medium mass (0.4 – about 6 ...
AAVSO: Mu Cephei, October 2002 Variable Star Of The Month
AAVSO: Mu Cephei, October 2002 Variable Star Of The Month

... Mu Cephei is really big. It is so big that it is one of the largest stars known; estimated to be the third largest star in the sky after its neighbor VV Cephei and the even larger Epsilon Aurigae (both are eclipsing binaries). If you were so inclined, you could fit one billion suns inside mu cephei ...
Chapter 17 Star Stuff Agenda How does a star`s mass affect nuclear
Chapter 17 Star Stuff Agenda How does a star`s mass affect nuclear

An interesting nebular object in LDN 288
An interesting nebular object in LDN 288

Mid-infrared imaging of the dust shell around the post
Mid-infrared imaging of the dust shell around the post

Stars III The Hertzsprung
Stars III The Hertzsprung

educator guide - Michigan Science Center
educator guide - Michigan Science Center

... universe. Recent discoveries have shown, however, that there are many more red dwarf stars than expected. This makes our star brighter than about 85% of all stars. This shouldn’t be taken to mean it is close to the brightest stars out there. In fact, the brightest (and most massive) known star, R136 ...
The Prospective Aspect of the Cosmogonic Models in Laozi and T
The Prospective Aspect of the Cosmogonic Models in Laozi and T

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Far Ultraviolet Spectroscopic Explorer

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Astronomical Distance Determination • etc.
Astronomical Distance Determination • etc.

Publisher: Emily Barrosse Acquisitions Editor: Kelley Tyner
Publisher: Emily Barrosse Acquisitions Editor: Kelley Tyner

What units are used in astronomical photometry?
What units are used in astronomical photometry?

... Distance: Distance is an easy concept to understand: it is just a length in some units such as in feet, km, light years, parsecs etc. It has been excrutiatingly difficult to measure astronomical distances until this century. Unfortunately most stars are so far away that it is impossible to directly ...
Project 4: The HR diagram. Open clusters
Project 4: The HR diagram. Open clusters

... This site has collected almost all the available data on open clusters and you can call up a plot showing the cluster you have measured. You can scale this plot to show the stars you see in your image, and then, by just clicking on a particular star, get its published values of V and (B-V) – provide ...
2900 K micrometers T
2900 K micrometers T

After the ZAMS - Lincoln-Sudbury Regional High School
After the ZAMS - Lincoln-Sudbury Regional High School

... matter-to-energy conversion in their cores. However the stellar winds are a much more serious source of mass loss. These winds commence as soon as a molecular cloud starts to heat up. But the effect really becomes important when fusion starts in the core. ...
Chapter 9 Circular Motion Dynamics
Chapter 9 Circular Motion Dynamics

... the rim, a distance R from the center. The turntable turns at constant angular speed ω and the coin rides without slipping. Suppose the coefficient of static friction between the turntable and the coin is given by µ . Let g be the gravitational constant. What is the maximum angular speed ω max such ...
MS Word
MS Word

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charts_set_7

... End product is 100’s or 1000’s of dense clumps each destined to form star, binary star, etc. Hence a cloud gives birth to a cluster of stars. ...
Visual Double Star Measurements with Equatorial - Alt
Visual Double Star Measurements with Equatorial - Alt

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Dyson sphere

A Dyson sphere is a hypothetical megastructure that completely encompasses a star and hence captures most or all of its power output. It was first described by Olaf Stapledon in his science fiction novel, ""Star Maker"". The concept was later popularly adopted by Freeman Dyson. Dyson speculated that such structures would be the logical consequence of the long-term survival and escalating energy needs of a technological civilization, and proposed that searching for evidence of the existence of such structures might lead to the detection of advanced intelligent extraterrestrial life. Different types of Dyson spheres correlate with information on the Kardashev scale.Since then, other variant designs involving building an artificial structure or series of structures to encompass a star have been proposed in exploratory engineering or described in science fiction under the name ""Dyson sphere"". These later proposals have not been limited to solar-power stations. Many involve habitation or industrial elements. Most fictional depictions describe a solid shell of matter enclosing a star, which is considered the least plausible variant of the idea (see below). In May 2013, at the Starship Century Symposium in San Diego, Dyson repeated his comments that he wished the concept had not been named after him.
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