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Mock Exam 2013 Paper 2
Mock Exam 2013 Paper 2

Great Observatories Origins Deep Survey (GOODS) Observation
Great Observatories Origins Deep Survey (GOODS) Observation

... • The goal is to discuss modern astronomical facilities and practice, as well as the state of current research so that if you choose astronomy as a profession, you know what is going on in today’s research (at least in extragalactic astronomy). It probably is the first time you are exposed to what i ...
What is light?
What is light?

... You observe a very large and very hot star in the constellation Orion. On the same night, you observe another star in Orion that is much smaller but has the same temperature. Which star is more luminous? a) the larger star b) the smaller star c) They have the same temperature. d) There is insuffici ...
The Warburton`s Challenge
The Warburton`s Challenge

Stars and Temperature and Color
Stars and Temperature and Color

... spectrum is in the ranges covered by the different cones. ...
AST 301 Introduction to Astronomy - University of Texas Astronomy
AST 301 Introduction to Astronomy - University of Texas Astronomy

... Astronomers measure the temperatures and luminosities of many stars and plot them on a diagram called the Hertzsprung-Russell (or H-R) diagram. The horizontal axis is surface temperature and the vertical axis is luminosity. Each star is a dot on the diagram. For historical reasons they plot temperat ...
AST 301 Introduction to Astronomy - University of Texas Astronomy
AST 301 Introduction to Astronomy - University of Texas Astronomy

THE LIFE CYCLE OF STARS
THE LIFE CYCLE OF STARS

Spectroscopy
Spectroscopy

Astronomy news
Astronomy news

... The tight upper limit on the pulsed fraction (<1.3% at 2) obtained for periods between 0.02 and 1000s and another upper limit on the pulsed fraction of 2.1% (at 1) was reported for periods in the range 1-20 ms. ...
ppt file
ppt file

Name: Notes – #51 Our Suns Brilliant Future 1. In the core of our
Name: Notes – #51 Our Suns Brilliant Future 1. In the core of our

Stars: Properties and Classification
Stars: Properties and Classification

... (LSun=4 x 1026 Watts). Only about 10-9 of this actually hits the Earth. Yet, the power of sunlight that illuminates a patch of desert 100 km x 100 km is equal to the total power consumption of the US. 4 x 1026 Watts radiated over entire surface ...
Problem Set No. 5
Problem Set No. 5

astr100_finalexam
astr100_finalexam

... space travel within, and ouside of, the solar system. List some of the issues that make human space travel within the Solar System difficult. What are the factors that make human interstellar space travel unlikely - even in the distant future? If they exist, what implications does this have for cont ...
Life Cycles of Stars
Life Cycles of Stars

... • Equivalent to entire Earth’s nuclear arsenal going off one km away - every second • This energy output would last for days ...
Planetarium Key Points
Planetarium Key Points

Stellar Evolution: the Death of Stars
Stellar Evolution: the Death of Stars

... expel most stellar material outward • Shock wave produces a series of nuclear reaction, the only place elements heavier than iron (such as silver, gold) are produced in the universe ...
Star Light, Star Bright: Exploring how stars are classified
Star Light, Star Bright: Exploring how stars are classified

The Evolution of Stars - hrsbstaff.ednet.ns.ca
The Evolution of Stars - hrsbstaff.ednet.ns.ca

... keeps us safely planted here on Earth, but it is more that just that. Gravity, or gravitation, is the natural phenomenon by which all objects with mass attract other objects. Without gravity the universe would be a very different place. ...
Homework 5 (stellar properties)
Homework 5 (stellar properties)

Space Exploration
Space Exploration

... • Eg. When you have an object that you view from your right eye, then your left eye. It appears to have moved but really, the viewing angle is just slightly different. • Astronomers use a star’s parallax (angles) to triangulate the star’s distance from earth • Measurements of stars can be taken mont ...
The Ever Expanding Universe: Part II
The Ever Expanding Universe: Part II

HW8 - UCSB Physics
HW8 - UCSB Physics

Star Types
Star Types

... sun, an O star, a white dwarf, or a red giant? Which of these star is the hottest? What are Sun-like stars (0.4 Msun < M < 8 Msun) in common? What about red dwarfs (0.08 Msun < M < 0.4 Msun) ? Where do stars spend most of their 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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