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ANSWER.
ANSWER.

Chapter 30 Notes
Chapter 30 Notes

... mass is called a white dwarf and can shine for billions of years before it cools completely. Stars more massive than our sun do not become white dwarfs. Novas and Supernovas Nova- a star that suddenly becomes brighter. Some white dwarfs revolve around red giants. When this happens the white dwarf ma ...
Homework #1 - Rutgers Physics
Homework #1 - Rutgers Physics

Circumstellar interaction in supernovae
Circumstellar interaction in supernovae

... • First implosion (increasing density and temperature at the center) • Core very hard (nuclear matter density) • Implosion turns into explosion • Neutron star remnant at the centre. • Explosion with 1053 ergs energy • 99% in neutrinos and 1 % in ElectroMagnetic • Scatter all heavy material required ...
Birth of Stars
Birth of Stars

Beyond the Solar System Homework for Geology 8
Beyond the Solar System Homework for Geology 8

Astronomy 12 - hrsbstaff.ednet.ns.ca
Astronomy 12 - hrsbstaff.ednet.ns.ca

... death of such a massive star? What is important about the final product? E. Spectroscopy. Write a short essay describing how the spectrum of a star be used to:  determine chemical composition  surface temperature  magnetic field  density  radial velocity (how fast the star is moving towards Ear ...
docx - STAO
docx - STAO

... The effects of temperature and brightness may be discussed. Betelgeuse is 15 times bigger (in radius) than Rigel and it is closer by more than 100 ly. Why is Rigel brighter? The explanation is that Betelgeuse is a red supergiant star that has evolved off the main sequence. This means that it has bur ...
Teacher Demo: Bright Star or Close Star?
Teacher Demo: Bright Star or Close Star?

... The effects of temperature and brightness may be discussed. Betelgeuse is 15 times bigger (in radius) than Rigel and it is closer by more than 100 ly. Why is Rigel brighter? The explanation is that Betelgeuse is a red supergiant star that has evolved off the main sequence. This means that it has bur ...
The Galaxy–Dark Matter Connection
The Galaxy–Dark Matter Connection

... Method has been carefully tested using Mock Galaxy Redshift Surveys constructed with the Conditional Luminosity Function. Our sample: ~ 280,000 galaxies in ~ 50,000 groups. ...
1 Do Massive Stars Trigger New Waves of Star Formation
1 Do Massive Stars Trigger New Waves of Star Formation

Introduction to the HR Diagram
Introduction to the HR Diagram

... are "ballpark" numbers only - there is much to learn about the evolutionary history of stars.] The White Dwarf Branch: The white dwarf branch is located in the lower left corner of the H-R diagram. This branch consists of the end products of stellar evolution for mid-sized stars with an initial mass ...
Calculating the Age of a Planetary Nebula
Calculating the Age of a Planetary Nebula

Killer Skies
Killer Skies

Lecture 2
Lecture 2

Lecture 12, PPT version
Lecture 12, PPT version

... in nature, but it is extremely short-range. ...
Astronomy 114 – Summary of Important Concepts #2 1 Stars: key
Astronomy 114 – Summary of Important Concepts #2 1 Stars: key

... brighter by the factor you calculate using the inverse square law). If the star appears 100 times brighter its magnitude must decrease by 5. Thus when the star is at a distance of 10 parsecs it will appear to have a magnitude of 11 − 5 = 6. It has an absolute magnitude of 6. ...
ACTIVITIES for Grades 3-5 (Continued)
ACTIVITIES for Grades 3-5 (Continued)

... • What kinds of energy does the Sun provide for Earth? Answers may include: The Sun provides heat and light. Plants capture this energy through the process of photosynthesis, create sugars and starches, and store them for later use. • Where do a plant, a grasshopper, a chicken, and a human get their ...
Color and Temperature of Stars
Color and Temperature of Stars

... Universe. Nevertheless, our world and everything it contains—even life ...
ASTRONOMY 301 EXAMPLES OF TEST
ASTRONOMY 301 EXAMPLES OF TEST

Rogava_Course_-_First_lecture
Rogava_Course_-_First_lecture

... is a subgiant at a later evolutionary stage. ...
Name:
Name:

Beyond the Solar System Homework for Geology 8
Beyond the Solar System Homework for Geology 8

Name: Three Views Spectrum Simulation This simulation uses the
Name: Three Views Spectrum Simulation This simulation uses the

Stellar Evolution Guiding Questions Stars Evolve
Stellar Evolution Guiding Questions Stars Evolve

< 1 ... 47 48 49 50 51 52 53 54 55 ... 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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