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Asymptotic Giant Branch
Asymptotic Giant Branch

1. Neutron stars 2. Black holes
1. Neutron stars 2. Black holes

Cosmology 20B Homework 2 solutions
Cosmology 20B Homework 2 solutions

... 14. Discuss the controversy between Darwin and Kelvin over the age of the Sun. What were the arguments behind each of their views and who was right in the end? Taking into account Darwin’s authoritative view on the timescales required for evolution, do you think that life in the Universe would be po ...
Test#3
Test#3

... 1. A measurement of the parallax of a star allows us directly to determine the star's a) rotation rate, b) temperature, c) distance, d) age 2. How much brighter would a star be if an observer moved from 3 to 1 parsec from the star? a) 3 times, b) 9 times, c) 27 times, d) 81 times 3. The difference b ...
Unit 1
Unit 1

PowerPoint
PowerPoint

Astronomy 100 Homework #2 Solutions 1, Problem 3‐27 (2 pts
Astronomy 100 Homework #2 Solutions 1, Problem 3‐27 (2 pts

... 5.
Problem
4‐34
(2
pts).
If
Earth
were
twice
as
far
from
the
Sun,
the
force
of
gravity
 attracting
Earth
to
the
sun
would
be
(c)
one‐quarter
as
strong.
Gravity
follows
an
 inverse
square
law
in
proportion
to
distance.
 6.
Problem
4‐36
(2
pts).
If
the
Moon
were
closer
to
the
Earth,
high
tides
would
b ...
Giant Molecular Clouds and Gravitational Stability
Giant Molecular Clouds and Gravitational Stability

Day 2
Day 2

... Once the star is close to hydrostatic equilibrium, the contraction slows down. However, the star must continue to contract until the temperature in the core is high enough that nuclear fusion can begin and support the star! During the contraction the star's temperature stays about the same, but its ...
Astronomy 15 - Homework 3 - Due Wed. April 24 1) As we`ll see
Astronomy 15 - Homework 3 - Due Wed. April 24 1) As we`ll see

PHYS 2421 EXAM #5 Wednesday, November 11
PHYS 2421 EXAM #5 Wednesday, November 11

Life Cycle of Stars - Faulkes Telescope Project
Life Cycle of Stars - Faulkes Telescope Project

Lecture Notes-PPT
Lecture Notes-PPT

... collect together by gravity. During the exchange of energy between the stars, some stars reach escape velocity from the protocluster and become runaway stars. The rest become gravitationally bound, meaning they will exist as collection orbiting each other forever. ...
Astronomy Learning Objectives and Study Questions for Chapter 12
Astronomy Learning Objectives and Study Questions for Chapter 12

Density, Mass and Surface Area
Density, Mass and Surface Area

The Sun
The Sun

Questions for this book (Word format)
Questions for this book (Word format)

... 4. What are the observed properties of a Cepheid variable (or Delta Cephei star)? How are these properties produced? 5. What information about stellar evolution is provided by the properties of comets? Using Kippenhahn’s figure for the mass loss caused by this mechanism, calculate how much mass the ...
The Hubble Space Telescope
The Hubble Space Telescope

Chapter 1 Daily Note Sheets Completed Power Point
Chapter 1 Daily Note Sheets Completed Power Point

... celestial equator. on or about March 21 ...
Study Guide: Chapters 32-‐34 FROSH CHAPTER 32 1. What is
Study Guide: Chapters 32-‐34 FROSH CHAPTER 32 1. What is

Star Name __Direction ___ Degrees
Star Name __Direction ___ Degrees

... 21. Name three stars that are second magnitude or brighter. Give their location in direction and degrees above the horizon on the celestial sphere. Star Name __Direction Example: Polaris North ___________ ____________ ...
Powerpoint for today
Powerpoint for today

... The slowing-down rate is slowing down at a rate of: 0.98 x 10 -31 /sec ...
Measuring the Properties of Stars
Measuring the Properties of Stars

... being radiated by the surface of a particular star. Astronomers call this power Luminosity, and it has dependancy on two properties of a star; it’s surface size (4R2) and its surface temperature (T). These are direct relationships. An increase in either of the properties, results in an increase in ...
Astronomy 2
Astronomy 2

... most stars are made of hydrogen & helium (determined by temperature & composition no two are alike) ...
Test 2 Review Topics
Test 2 Review Topics

< 1 ... 135 136 137 138 139 140 141 142 143 ... 167 >

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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