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Stars
Stars

PPT
PPT

... • The overall range of stellar masses runs from 0.08 times the mass of the Sun to about 150 times the mass of the Sun. • Masses are only known for stars that form binary systems, but about half of all stars are in fact in binary systems! – 0.08 MSun is approximately 80 MJupiter ...
Astrophysics - Part 2
Astrophysics - Part 2

1 - Quia
1 - Quia

... 11. An "explosion" on the star that arcs its gases back onto the sun's surface is called a -. (2 points) A. solar flare B. solar prominence C. sunspot D. chromosphere 12. A light-year measures - (2 points) A. brightness B. distance C. radiation D. time 13. The layer of the sun with a red color is th ...
Time From the Perspective of a Particle Physicist
Time From the Perspective of a Particle Physicist

Astronomy Exam #4
Astronomy Exam #4

Lecture 19 - Stellar Lifecycles
Lecture 19 - Stellar Lifecycles

... • Once neutrons are formed the collapse stops, the surrounding gas is heated and explodes off the core. This is a supernova explosion. • The explosion is so energetic that it can outshine the combined light of a galaxy! • Heavy elements are formed in the material blown off the star. These elements a ...
Introduction - Willmann-Bell
Introduction - Willmann-Bell

Stellar Explosions
Stellar Explosions

... High Mass Stars can continue to fuse elements in its core right up to iron (after which the fusion reaction is energetically unfavored) As heavier elements are fused, the reactions go faster and the stage is over more quickly 20-solar-mass star will burn carbon for about 10,000 years, but its iron c ...
Parallax, Apparent Magnitude and Absolute Magnitude
Parallax, Apparent Magnitude and Absolute Magnitude

Planets beyond the solar system
Planets beyond the solar system

... the total light from the star. Since the planet is much smaller than the stars, the total light is reduced only by a few percent, even less for Earth-like planets. ...
Orion- The Swordsman of the Sky - A Winter Constellation from the
Orion- The Swordsman of the Sky - A Winter Constellation from the

Ch. S1 - Relativity Group
Ch. S1 - Relativity Group

1-1 H. Color Index: A color index is the difference of two color
1-1 H. Color Index: A color index is the difference of two color

AST1100 Lecture Notes
AST1100 Lecture Notes

Star evolution - El Camino College
Star evolution - El Camino College

... What should we observe as a result? CLICKER The light “gets stuck” and pushes the outer layers out. What happens to gas when you _______________? Color of outside? What kind of star do we have? What is the core made of? What is the structure? ...
Scientific Notation Worksheet
Scientific Notation Worksheet

... 43. Explain how astronomers can use the inverse square law to determine the Luminosity of a near-by star. Explain how astronomers would get the information they need to calculate Luminosity. ...
Assessment Schedule
Assessment Schedule

Chapter13
Chapter13

... dwarfs are found in the lower left corner of the HertzsprungRussell diagram. The more massive a white dwarf, the smaller it is! ...
Level 2 Science (90764) 2011 Assessment Schedule
Level 2 Science (90764) 2011 Assessment Schedule

... Explains gas clouds are the birth places for new stars. Supernova gives out clouds of gases and plasma exploding off its surface. AND These gas clouds are the birth places for new stars. AND After this process ceases, a black hole or a dense neutron star remains (detail provided about the formation) ...
Foundation 1 - Discovering Astronomy
Foundation 1 - Discovering Astronomy

... When core hydrogen fusion ceases, a main-sequence star becomes a giant • When hydrogen fusion ceases in the core, the star will collapse inward – this causes the layer just outside the core to become so hot and dense that hydrogen fusion will begin in this outer layer. • The energy produced by hydr ...
Lecture 6-1: Schematic Evolution of Stars as seen from the core
Lecture 6-1: Schematic Evolution of Stars as seen from the core

1 2 3 4 5 6 Orbital Distance (AU) Orbital Period (Years) 1 2 3 4 5 6 7
1 2 3 4 5 6 Orbital Distance (AU) Orbital Period (Years) 1 2 3 4 5 6 7

18. Formation of Stars.
18. Formation of Stars.

... Gravity and energy are the keys to understanding star formation & evolution. ◦ Gravity is constantly trying to pull matter toward the center of mass of a gas cloud or a star. ◦ Since stars do not have an infinite supply of energy, they must readjust their structure in response to the energy supply ...
HighRedshiftGalaxies
HighRedshiftGalaxies

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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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