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Solar System Project
Solar System Project

Classifying Stars
Classifying Stars

Chapter 11 - USD Home Pages
Chapter 11 - USD Home Pages

... 35. a. What is the approximate mass of a main sequence star that is 10,000 times as luminous as the Sun? b. What is the approximate lumniosuty of a main-sequence star whose mass is one-tenth that of the Sun? Answer: a. Reading Fig 11-14: Find 104 L on the vertical scale; trace horizontally until yo ...
Stellar Evolution
Stellar Evolution

For each statement or question, select the word or expression that
For each statement or question, select the word or expression that

... B. titanium and hydrogen C. hydrogen and helium D. helium and iron ____ 15. Red giants that lose their atmospheres leave faint, Earth-sized stars called A. Cepheid variables B. blue superiants C. white dwarfs D. proton stars ____ 16. Cepheid variable stars have been used to determine the A. ages of ...
Microsoft Word Document
Microsoft Word Document

Extension worksheet – Topic 6 - Cambridge Resources for the IB
Extension worksheet – Topic 6 - Cambridge Resources for the IB

... A large, cool cloud of gas may collapse under gravity to form a star. State where the energy comes from to heat up the star so that nuclear fusion may take place. In this question assume a mass–luminosity relation of L  M 3.5 . a ...
An Introduction to the Night Sky Stars and Constellations
An Introduction to the Night Sky Stars and Constellations

... An Introduction to the Night Sky Stars and Constellations 1. What is the Latin root word of star? 2. Why do stars “twinkle”? 3. Why do planets “shine”? ...
Almach or Alberio
Almach or Alberio

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Spectroscopy Assignment

... ...
Section 2
Section 2

Understanding Stars
Understanding Stars

... Stefan-Boltzman Law A dense hot object emits light of all colors – More of one color than others • “peak” color – The peak color is determined by the temperature • Hotter = bluer! – demo Stellar Spectroscopy Astronomers can tell what elements are in a star by the lines in its spectrum Peak color det ...
Chapter 25 Study guide Answer Key
Chapter 25 Study guide Answer Key

... 3) Which property of a star can be determined by its color? Temperature 4) About how many stars are estimated to occur in pairs or multiples? 50% ...
The Evolutionary Cycle of Stars
The Evolutionary Cycle of Stars

AST 443
AST 443

Study Guide Astronomy
Study Guide Astronomy

... 2. What 2 factors does the brightness of stars depend on? ...
Earth
Earth

... standard distance from Earth) from 20 pc. • Since the star will be “closer”, it will be brighter. • A brighter star has a smaller magnitude • Thus, we expect an absolute magnitude less than ...
18.3 NOTES What is magnitude? Objective: Compare apparent
18.3 NOTES What is magnitude? Objective: Compare apparent

Answers Universe Cornell Notes Chapter 8, Sec 2
Answers Universe Cornell Notes Chapter 8, Sec 2

... and size. Supergiant star, giant star, medium-sized star, white dwarf star, neutron star A star’s color reveals its temperature. Red, yellow - white, blue - white Brightness depends on the star’s size and temperature. It’s brightness as seen from Earth. Apparent brightness is how bright it appears t ...
A Brief History of Planetary Science
A Brief History of Planetary Science

... Each spectral type is divided into 10 sub classes 0 - 9 (from high to low T) ...
Chapter 8 lesson 4 Notes
Chapter 8 lesson 4 Notes

... Stars form when matter comes together and starts to give off energy. ...
Astronomy Learning Objectives and Study Questions for Chapter 12
Astronomy Learning Objectives and Study Questions for Chapter 12

Amazing Stars
Amazing Stars

... ...
Astronomy Problems – Color Index Nov. 2011
Astronomy Problems – Color Index Nov. 2011

Weekly Homework Questions #3, Sep. 14, 2010
Weekly Homework Questions #3, Sep. 14, 2010

... 1. How can one measure the mass of a star other than the Sun? (a) measuring the color of the star and using a color-mass relationship (b) the apparent magnitude of a star tells its mass (c) the gravitational force on a companion star in a double star (d) the mass of a star is determined by its locat ...
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Corona Borealis

Corona Borealis /kɵˈroʊnə bɒriˈælɨs/ is a small constellation in the Northern Celestial Hemisphere. It is one of the 48 constellations listed by the 2nd-century astronomer Ptolemy, and remains one of the 88 modern constellations. Its brightest stars form a semicircular arc. Its Latin name, inspired by its shape, means ""northern crown"". In classical mythology Corona Borealis generally represented the crown given by the god Dionysus to the Cretan princess Ariadne and set by him in the heavens. Other cultures likened the pattern to a circle of elders, an eagle's nest, a bear's den, or even a smokehole. Ptolemy also listed a southern counterpart, Corona Australis, with a similar pattern. The brightest star is the magnitude 2.2 Alpha Coronae Borealis. The yellow supergiant R Coronae Borealis is the prototype of a rare class of giant stars—the R Coronae Borealis variables—that are extremely hydrogen deficient, and thought to result from the merger of two white dwarfs. T Coronae Borealis, also known as the Blaze Star, is another unusual type of variable star known as a recurrent nova. Normally of magnitude 10, it last flared up to magnitude 2 in 1946. ADS 9731 and Sigma Coronae Borealis are multiple star systems with six and five components respectively. Five star systems have been found to have Jupiter-sized exoplanets. Abell 2065 is a highly concentrated galaxy cluster one billion light-years from our Solar System containing more than 400 members, and is itself part of the larger Corona Borealis Supercluster.
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