• 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
Life Cycle of Stars
Life Cycle of Stars

... compressed so tightly that its atoms are compacted into a dense shell of neutrons. If the remaining mass of the star is more than about three times that of the Sun, it will collapse so completely that it will literally disappear from the universe. What is left behind is an intense region of gravity ...
Introduction to the HR Diagram
Introduction to the HR Diagram

Basic Properties of Stars D • Composition L
Basic Properties of Stars D • Composition L

... temperature (cumulative) Chemical composition ...
File
File

1. How can we detect extra-solar planets?
1. How can we detect extra-solar planets?

... In recent years a growing number of exoplanets have been detected via transits = temporary drop in brightness of parent star as the planet crosses the star’s disk along our line of sight. ...
Chapter 18 Notes - Valdosta State University
Chapter 18 Notes - Valdosta State University

... can detect a regularly occurring radio wave pulse. These stars are then called pulsars. If the remaining mass after a supernova explosion is large enough, a black hole may be formed. In a black hole matter has contracted to the point that it forms a singularity. Anything (even light) coming within a ...
mass_spetral
mass_spetral

Three types of binary stars.
Three types of binary stars.

AmiraPoster3
AmiraPoster3

... • Our raw value for Ko and the corresponding upper limit on the neutron star mass, 1.020.10 M‫סּ‬, are both comparable with those found by van der Meer et al. (2005). • Previous studies assume the giant star is Roche-lobe filling, thus giving only upper limits to the stellar masses. • Effects of X-r ...
source
source

The Fates of Stars Mass-Luminosity Relation: Lifetime Relation:
The Fates of Stars Mass-Luminosity Relation: Lifetime Relation:

... Two simple relations are of extreme importance in stellar evolution. Mass-Luminosity Relation: Lifetime Relation: ...
Investigating the Celestial Sphere
Investigating the Celestial Sphere

Lecture 10 - Concord University
Lecture 10 - Concord University

... Si fusion ...
Stellar Evolution - University of California, Santa Cruz
Stellar Evolution - University of California, Santa Cruz

... very quickly (10,000 years), less massive stars evolve more slowly -- up to 10 million years. • The long `flat’ sections imply contraction. Increasing Teff at constant L means the surface area is decreasing. ...
HW11
HW11

... process is providing the luminosity and why is a proto-star able to shrink. How does convection play a part in the proto-star evolution? 8) Understand all aspects of low mass star evolution off the main-sequence. Why a star leaves the main sequence, what the sub-giant and giant phases are and what ...
Astronomy Fall 2013 Final Exam History of Astronomy Know: speed
Astronomy Fall 2013 Final Exam History of Astronomy Know: speed

... 4.Where was supernova 1987a located? Large Maganellic cloud in a near by galaxy 5. What produces a Type I supernova? Binary star system with a massive star (8 – 12 solar masses) and white dwarf collide 6.What is the Lighthouse model for pulsating stars? A spinning neutron star shooting a beam of lig ...
Assignment 8 - utoledo.edu
Assignment 8 - utoledo.edu

... a. falls inward very slowly, taking billions of years to get really compressed b. makes a planetary nebula, which gently moves outward from the center c. is vaporized by the incredible heat of the dying star and evaporates d. explodes outward as a supernova e. continues regular fusion and returns to ...
Final Exam, Dec. 19, 2015 - Physics@Brock
Final Exam, Dec. 19, 2015 - Physics@Brock

The dying sun/ creation of elements
The dying sun/ creation of elements

... • In a supernova, there are free neutrons made by destroying nuclei. ...
Review: How does a star`s mass determine its life story?
Review: How does a star`s mass determine its life story?

... Two Types of Supernova Massive star supernova: Iron core of massive star reaches white dwarf limit and collapses into a neutron star, causing explosion White dwarf supernova: Carbon fusion suddenly begins as white dwarf in close binary system reaches white dwarf limit, causing total explosion ...
sc_examII_fall_2002 - University of Maryland
sc_examII_fall_2002 - University of Maryland

... D. a few thousand miles away. E. at the Moon’s distance. 13. A planetary nebula, like the Ring Nebula shown in class, is A. evidence that planets exist around other stars. B. gas that is about to collapse and form planets. C. a giant molecular cloud that is about to form new stars. D. a very dense ...
Homework #1 Solutions
Homework #1 Solutions

... 1/2 1/R, and the escape velocity is 2 smaller than from the Earth . 7. We use Kepler’s third law to solve this problem. For our solar system, we can write this law as: P 2 = r3 , with the understanding that the orbital period P must be expressed in years and the orbital radius r in AU. We are given ...
Stars and Galaxies
Stars and Galaxies

... over time. The mass of a star controls its Evolution Lifespan Ultimate fate (how it dies) ...
Final Exam Review
Final Exam Review

... Depends on the wind speed between the train and the detector. ...
The Future Sun • Homework 5 is due Wed, 24 March at 6:30am
The Future Sun • Homework 5 is due Wed, 24 March at 6:30am

... Í Temperature (K) ...
< 1 ... 99 100 101 102 103 104 105 106 107 ... 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