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Chapter 16 Lesson 2: What is a Star
Chapter 16 Lesson 2: What is a Star

Document
Document

... • After the supernova explosion, a high mass star will become a neutron star. • After a supernova explosion, in a very high mass star the core that remains will be so massive, that without the energy created by nuclear fusion to support it, the core is swallowed by its own gravity. • The gravity of ...
- hoganshomepage
- hoganshomepage

... chemical composition of the stars. (also temperature and direction the star is moving in relation to the Earth.) How? Set up a spectroscope with different tubes; each gas has different spectras – light patterns. ...
How Stars Evolve
How Stars Evolve

Stars
Stars

... •With Newton’s modifications to Kepler’s laws, the period and size of the orbits yield the sum of the masses, while the relative distance of each star from the center of mass yields the ratio of the masses. •The ratio and sum provide each mass individually. ...
Astronomy Library wk 6.cwk (WP)
Astronomy Library wk 6.cwk (WP)

Stellar Evolution
Stellar Evolution

Properties of Stars
Properties of Stars

... matter in space from which no light or matter can escape. ...
Chapter 29 Review
Chapter 29 Review

... gravity so immense that nothing—not even light—can escape it ...
Star Properties and Stellar Evolution
Star Properties and Stellar Evolution

... different distances be compared? Use their brightness if they were all an equal distance from Earth = 32 ly. Absolute Magnitude ...
(AU): Average distance from Earth to Sun
(AU): Average distance from Earth to Sun

... if all stars same distance from Earth.  Apparent Magnitude: How bright a star appears to be to an observer on Earth. - Depends on distance. Closer = brighter ...
15 - Edmodo
15 - Edmodo

Morning Announcements
Morning Announcements

... neatly. You can draw it or create a model out of pipe cleaners and construction paper.  Every page must be titled with the stage of the life cycle  Sign the back of each card you create. Each team r will create pages individually or together and sign that it is there work for verification. This is ...
Final Exam - Practice questions for Unit V
Final Exam - Practice questions for Unit V

Cosmology, galaxies, stars and the sun
Cosmology, galaxies, stars and the sun

File - We All Love Science
File - We All Love Science

Stellar Evolution and the HR Diagram – Study Guide
Stellar Evolution and the HR Diagram – Study Guide

... 10. Draw the evolutionary path of our Sun. Start by locating it’s present position on the graph and then indicate where it will be as it ages, and finally what part of the graph it ends in. It would start above Red Dwarfs, but below Giants; it would move down and left to the main sequence (where it ...
Can you write numbers in scientific notation
Can you write numbers in scientific notation

... How well you understand what processes are going on during the proto-star stage of a star’s life? What needs to happen for a proto-star to become a main sequence star? What are the properties of a main sequence star? How does a star’s mass affect the Luminosity, Temperature, Size, and lifespan of a ...
neutron star - The University of Chicago
neutron star - The University of Chicago

... In the first lecture we learned that the fate of stars with masses more than 8 times the mass of the sun is different than that of sun-line stars. ...
solutions 3
solutions 3

Stages in the Life of a Star
Stages in the Life of a Star

The most important questions to study for the exam
The most important questions to study for the exam

... • Our eyes are mounted horizontally about 10 cm apart in our heads, and the brain uses the relative look angles of these eyes to estimate distance to the object viewed. • We are always moving our heads slightly from side to side, and the brain compares look angles from each of these positions to obt ...
Motions of the Celestial Sphere
Motions of the Celestial Sphere

Stefan-Boltzmann Law Problems
Stefan-Boltzmann Law Problems

... 1. A star with the same color as the Sun is found to produces a luminosity 81 times larger. What is its radius compared to the Sun? Since we are asked to compare this star to the Sun we will use a ratio technique that saves a lot of numerical work. Below I will decode the problem by writing out ht g ...
astr221lect2x
astr221lect2x

... day changes during the year because Earth’s orbit is slightly elliptical. • Mean solar time is based on the average length of a day. • Noon is average time at which Sun crosses meridian • It is a local definition of time ...
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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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