• Study Resource
  • Explore
    • Arts & Humanities
    • Business
    • Engineering & Technology
    • Foreign Language
    • History
    • Math
    • Science
    • Social Science

    Top subcategories

    • Advanced Math
    • Algebra
    • Basic Math
    • Calculus
    • Geometry
    • Linear Algebra
    • Pre-Algebra
    • Pre-Calculus
    • Statistics And Probability
    • Trigonometry
    • other →

    Top subcategories

    • Astronomy
    • Astrophysics
    • Biology
    • Chemistry
    • Earth Science
    • Environmental Science
    • Health Science
    • Physics
    • other →

    Top subcategories

    • Anthropology
    • Law
    • Political Science
    • Psychology
    • Sociology
    • other →

    Top subcategories

    • Accounting
    • Economics
    • Finance
    • Management
    • other →

    Top subcategories

    • Aerospace Engineering
    • Bioengineering
    • Chemical Engineering
    • Civil Engineering
    • Computer Science
    • Electrical Engineering
    • Industrial Engineering
    • Mechanical Engineering
    • Web Design
    • other →

    Top subcategories

    • Architecture
    • Communications
    • English
    • Gender Studies
    • Music
    • Performing Arts
    • Philosophy
    • Religious Studies
    • Writing
    • other →

    Top subcategories

    • Ancient History
    • European History
    • US History
    • World History
    • other →

    Top subcategories

    • Croatian
    • Czech
    • Finnish
    • Greek
    • Hindi
    • Japanese
    • Korean
    • Persian
    • Swedish
    • Turkish
    • other →
 
Profile Documents Logout
Upload
Stellar Evolution
Stellar Evolution

Main Sequence stars
Main Sequence stars

Lecture 6: Stellar Distances and Brightness
Lecture 6: Stellar Distances and Brightness

The Birth of Stars and Planets
The Birth of Stars and Planets

Lecture 10: Stellar Evolution
Lecture 10: Stellar Evolution

Summer Triangle (Winter in the south hemisphere) Lyra
Summer Triangle (Winter in the south hemisphere) Lyra

... brightest star in the sky. It is three times larger than our Sun, and 60 times more luminous. Vega was the first star to be photographed in the 1850's. It was also one of the first stars discovered to have a disk of proto-planetary dust orbiting around it, by the IRAS satellite in 1983. This discove ...
Slide 1 - Personal.psu.edu
Slide 1 - Personal.psu.edu

... When looking at just a few atoms, the gravitational force is nowhere near strong enough to overcome the random thermal motion: ...
Unit 11: Stellar Evolution
Unit 11: Stellar Evolution

Stellar Physics - Craigie High School
Stellar Physics - Craigie High School

... The development of what we know about the Earth, Solar System and Universe is a fascinating study in its own right. From earliest times Man has wondered at and speculated over the ‘Nature of the Heavens’. It is hardly surprising that most people (until around 1500 A.D.) thought that the Sun revolved ...
The Hertzsprung-Russell Diagram
The Hertzsprung-Russell Diagram

... The orbital period comes from watching the stars, or the periodic variation of their velocity or brightness. To get orbital semimajor axis, you need either the parallax to a visual system or the velocity from a spectroscopic system. In a spectroscopic system, you only have a lower limit unless you k ...
New light on our Sun`s fate - Space Telescope Science Institute
New light on our Sun`s fate - Space Telescope Science Institute

Plotting Supernova Light Curves
Plotting Supernova Light Curves

Study Guide for the Comprehensive Final Exam
Study Guide for the Comprehensive Final Exam

... Describe or identify changes in a star during its main sequence lifetime. Describe how shell fusion in a star causes the star to become giants. Identify the “ashes” of H-burning and He-burning Mass loss and Death of Low-Mass Stars Match the stage of the Sun’s future evolution with the mechanism of e ...
The Classification of Stellar Spectra
The Classification of Stellar Spectra

Star Birth - Sierra College Astronomy Home Page
Star Birth - Sierra College Astronomy Home Page

REGIONAL exam 2013
REGIONAL exam 2013

Chapter 17 Star Stuff
Chapter 17 Star Stuff

14-1 Reading Questions: Neutron Stars
14-1 Reading Questions: Neutron Stars

... 1. A neutron star, containing a little more than _________ solar mass, compressed to a radius of about __________, can be left as a remnant after a type ______ supernova explosion. A neutron star’s density is so high that physicists calculate that this material is stable only as a __________________ ...
EF Eri: Its White Dwarf Primary and L Dwarf Secondary
EF Eri: Its White Dwarf Primary and L Dwarf Secondary

... nova, nova-like (IP). These binaries contain an accretion disk. • If the white dwarf has a ~10 to 250MG field --> Polar or AM Herculis type. These contain no accretion disk. ...
Sample Stellar Evolution TEST QUESTIONS
Sample Stellar Evolution TEST QUESTIONS

... 11. The Orion region contains young main sequence stars and an emission nebula. 12. The thermal motions of the atoms in a gas cloud can make it collapse to form a protostar. 13. The pressure of a gas generally depends on its temperature and its density. 14. Stars swell into giants when hydrogen is e ...
Neutron Stars
Neutron Stars

... Novae: white dwarf re-ignition in binary system • Nova is a faint star suddenly brightens by a factor of 104 to 108 over a few days or hours • It reaches a peak luminosity of about 105 Lsun • A nova is different from supernova (luminosity of 109 Lsun) • Material from an ordinary star in a close bin ...
Building the Hertzsprung
Building the Hertzsprung

Nature of Stars 2
Nature of Stars 2

ASTR-264-Lecture
ASTR-264-Lecture

... moons. Solar systems, planets, moons, and asteroids and comets are all in it Nebula-an interstellar cloud of gas and/or dust Galaxy- a great island of stars in space, held together by gravity and orbiting a common center Universe-the sum total of all matter and energy; that is, everything within it ...
Chapter 10. Stellar Spectra
Chapter 10. Stellar Spectra

< 1 ... 46 47 48 49 50 51 52 53 54 ... 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.
  • studyres.com © 2025
  • DMCA
  • Privacy
  • Terms
  • Report