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Stars are classified according to their color
Stars are classified according to their color

... between the stars. • Distance that light travels in one year. Its about 9.5 million million kilometers. That is not a typo!  ...
THE STAR - physics.udel.edu
THE STAR - physics.udel.edu

... contemporaneous Persian figure.[2] The two other notably bright stars in Cassiopeia are both variable stars. Gamma Cassiopeiae is a shell star, a type of variable star that has a very high rate of rotation. This causes the star to be somewhat unstable and periodically eject rings of material. ...
Astronomy
Astronomy

... d. both b and c 15. In the HR diagram, stable stars with the smallest mass and lowest temperature are found in the ______ of the diagram. a. center (main sequence) b. upper left corner c. upper right corner d. lower right corner ...
JPL Small-Body Database Browser
JPL Small-Body Database Browser

The Brightness of Stars
The Brightness of Stars

File
File

...  as they orbit the Sun, material ________ forming the tail  the tail _______ points away from the Sun  Halley's comet orbits the Sun every ____ years (1986) Meteors and Meteorites  Earth is bombarded everyday by _____ and ______ fragments from space  when one of the objects _______ up generatin ...
Codes of Life
Codes of Life

... centre gets hotter and hotter until a nuclear fusion reaction begins. ...
Astro 2 - Red Hook Central School District
Astro 2 - Red Hook Central School District

... • http://www.youtube.com/watch?v=jjmjEDY qbCk • From 4:48 ...
Astronomy Toolkit
Astronomy Toolkit

... • The star radiates light in all directions so that its emission is spread over a sphere • To find the intensity, I, of light from a star at the Earth (the intensity is the emission per unit area), divide the star’s luminosity by the area of a sphere, with the star at the centre and radius equal to ...
Jeopardy Questions
Jeopardy Questions

... Q: How do black holes and neutron stars form? A: When a massive star has iron at its core, and can no longer fuse atoms to create energy, gravitational forces take over and the core collapses into either a neutron star or a black hole, depending on if its mass can be supported by neutron degeneracy ...
CHAPTER 2 NOTES (STARS AND GALAXIES)
CHAPTER 2 NOTES (STARS AND GALAXIES)

... Stars moving away from the Earth have light waves from the star that will be expanded and appear longer- red (red shift) Doppler effect- apparent change in the wavelengths of light that occurs when an object is moving toward or away from Earth Every galaxy in the universe is moving away from the Ear ...
1 - WordPress.com
1 - WordPress.com

... 6. What two star characteristics does the Hertzsprung-Russell diagram compare? 7. What is a star’s spectrum? ...
The Family of Stars
The Family of Stars

- hoganshomepage
- hoganshomepage

... Characteristics of Stars The Sun is an average star: it’s not hot or cool it’s not large or small. We can compare stars by colour, temperature, size, brightness and spectrum. P.458 ...
Diapositiva 1
Diapositiva 1

... dinamical study indicates that runaway stllar colosion at an earlier age may have formed a black hole with more than 100 times the mass of the Sun. The presence of a black hole within the cluster could explain the observed high velocities of the Trapezium stars. The Orion Nebula's distance of some 1 ...
Chapter 30
Chapter 30

... seen in the sky during different seasons of the year? A. Stellar motion around Polaris B. Earth’s rotation on its axis C. Earth’s revolution around the sun D. Position north or south of the equator ...
Stellar Evolution: After the Main Sequence
Stellar Evolution: After the Main Sequence

... As a cluster ages, the main sequence is “eaten away” from the upper left as stars of progressively smaller mass evolve into red giants ...
Astronomy Galaxies & The Universe
Astronomy Galaxies & The Universe

... The original mass of the star determines its temperature and the color. (Big – glows blue, medium – glows yellow-orange, small – glows red) Red Giants / Red Super-giants form as H2 fuel is used up and gravity overpowers released energy, center core contracts while outer layer expands (He2 + He2 → C ...
A star is a - Trimble County Schools
A star is a - Trimble County Schools

... __________________ cannot distinguish the distance a star is from earth • Clusters are stars close to each other due to gravitational attraction Binary Stars • _____________________________ – Pairs of stars that revolve around one another – Gravitationally bound & orbiting a common center of mass • ...
25 Study Guide
25 Study Guide

... • Binary stars can be used to determine stellar mass. • The nearest stars have the largest parallax angles, while those of distant stars are too small to measure. • Three factors control the apparent brightness of a star as seen from Earth: how big it is, how hot it is, and how far away it is. • A H ...
Groups of Stars
Groups of Stars

... Describe how the life stages are similar. You will need to choose the life cycle of either a lowmedium mass star OR a high mass star. ...
Day-6
Day-6

Monday, April 15
Monday, April 15

Lifecycle of a Star
Lifecycle of a Star

... much faster than small or medium stars ...
The Life Cycle of Stars Webquest
The Life Cycle of Stars Webquest

... energy that makes stars shine. 3. You will also begin to understand the forces involved in stars that maintain this nuclear reaction and how these forces change as the star ages. 4. You will explore the stages stars progress through from birth to death and how the death of a star depends on its init ...
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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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