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Chapter 19 Notes Stars Stars are bright balls of gas that are trillions
Chapter 19 Notes Stars Stars are bright balls of gas that are trillions

... i. While many stars become white dwarves as they get older, very massive stars can become strange objects like pulsars, supernovas, black holes and neutron stars. ii. Supernovas 1. Massive stars use their hydrogen much faster than stars like the sun do. 2. At the end of their lives they may explode ...
chapter10
chapter10

... • Sun will expand to a red giant in ~ 5 billion years • Expands to ~ Earth’s orbit • Earth will then be incinerated! • Sun may form a planetary nebula (but uncertain) • Sun’s C,O core will become a white dwarf ...
Brichler-powerpoint
Brichler-powerpoint

... –When the most massive stars die, they become black holes – an object with gravity so strong that not ...
HR Diagram
HR Diagram

... H-R Diagram Scientists began to learn about stars by observing properties of stars, including brightness and color. Astronomers tried to make sense of the star data by grouping together stars with similar properties. The Hertzsprung-Russell diagram provides a way to group similar stars. The H-R dia ...
Astronomy ANSWER KEY KEEP SECURE
Astronomy ANSWER KEY KEEP SECURE

Module G - U1_ L3 - Life Cycle of Stars
Module G - U1_ L3 - Life Cycle of Stars

... • The densest regions, called dense cores, form new stars. • The temperature within dense cores increases for millions of years. • At about 10 million °C, the process of hydrogen nuclear fusion begins, marking the birth of a star. • A star can remain actively fusing hydrogen into helium for billions ...
Introduction to Astronomy
Introduction to Astronomy

... (temperature)4 For a given size, hotter implies brighter. A bright, cool star must be unusually large (“red giant”). A faint, hot star must be unusually small (“white dwarf”). ...
Star Light, Star Bright: Exploring how stars are classified
Star Light, Star Bright: Exploring how stars are classified

Stellar Evolution Notes
Stellar Evolution Notes

... It takes about 10 billion years for a star with the mass of the Sun to convert all of the hydrogen in its ...
Stellar Evolution Notes
Stellar Evolution Notes

Properties of Stars in general
Properties of Stars in general

The Milky Way Galaxy
The Milky Way Galaxy

... Globular clusters must orbit around the center of mass of the galaxy! Thus, assuming the clusters are distributed uniformly around the galaxy, he measured the 3D distribution of clusters (using Cepheid variables) and then assumed that the center of that distribution was where the center of the galax ...
- Stevenson High School
- Stevenson High School

... 4. Are there any stars that are not part of a constellation? Explain. 5. How is astrology and astronomy different? 6. How is astrology and astronomy related? 7. What is the significance of the zodiac? 8. If your zodiac sign is Virgo, what does that mean about the position of the earth, sun, and the ...
Friday, August 28 - Otterbein University
Friday, August 28 - Otterbein University

... • Their positions are related because – the direction of Polaris defines the rotation axis of the celestial sphere – The sun is somewhere on the sphere – From a “skewed” perspective everything on the sphere culminates on the meridian ...
Slide 1
Slide 1

ReviewQuestionsForClass
ReviewQuestionsForClass

Wednesday, April 2 - Otterbein University
Wednesday, April 2 - Otterbein University

... • If the Sun = a golf ball, then ...
eneb_form
eneb_form

Chapter 28 – Stars and Galaxies
Chapter 28 – Stars and Galaxies

Superwind - The University of Sydney
Superwind - The University of Sydney

... Astronomers at The University of Manchester believe they have found the answer to the mystery of a powerful ‘superwind’ which causes the death of stars. Writing in Nature, the team of researchers, lead by Barnaby Norris from the University of Sydney in Australia, used new techniques which allowed th ...
What is a Scientist? - Cockeysville Middle School
What is a Scientist? - Cockeysville Middle School

STUDY GUIDE FOR CHAPTER 1
STUDY GUIDE FOR CHAPTER 1

Stellar Evolution
Stellar Evolution

Word
Word

Astronomy Unit Period
Astronomy Unit Period

< 1 ... 90 91 92 93 94 95 96 97 98 ... 132 >

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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