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Blackbody Radiation
Blackbody Radiation

... White light is made up of all colors of light. To break the white light into its individual colors, we shine the light through a prism. Rain drops act as tiny prisms, and we see a rainbow when the Sun breaks through the rain clouds. The composition of light – called a spectrum – can be represented b ...
Review Quiz No. 22
Review Quiz No. 22

... the iron core of a very massive star collapses to form a white dwarf. the iron core of a very massive star collapses to form a neutron star. the iron core of a very massive star collapses to form a black hole. a neutron star is tidally disrupted by a ...
Stars_and_Galaxies
Stars_and_Galaxies

Variable and Binary Stars
Variable and Binary Stars

Unit 1
Unit 1

Postgraduate Seminar Series Small Angle Neutron scattering on the anisotropic superconductor CaC6.
Postgraduate Seminar Series Small Angle Neutron scattering on the anisotropic superconductor CaC6.

... of the system and will have evolved into a white dwarf (compact degenerate star), while the secondary is still a main sequence star (fusing hydrogen) and is transporting mass towards the primary. Due to friction this gas will expand to form an accretion disc around the white dwarf. At some point thi ...
Stars and Galaxies Section 1 Stars
Stars and Galaxies Section 1 Stars

Outline2a
Outline2a

... Due to the friction in the disk, matter flows onto the star. As the star’s mass increases, its core grows hotter. At this time, since the star is still surrounded by dust, it is invisible in the optical. But the heat from the star begins to warm the dust. ...
Study Guide: Use your notes and handouts to
Study Guide: Use your notes and handouts to

Evolution of Close Binary Systems
Evolution of Close Binary Systems

Slide 1
Slide 1

... The Lives of Stars Gestation, Birth, and Youth: 1. The womb: Stars are born in dense molecular clouds. --The interstellar medium must be dense enough so H atoms can collide and form H2 molecules. This also is facilitated on dust--for other molecules as well. It increases gravitation enough for stars ...
File
File

... Equinox for North America. Make sure to point Axis towards the North Star. ...
HR Diagram - Geneva 304
HR Diagram - Geneva 304

... 51. Compare and contrast stellar Population I with stellar Population II. Do the stars in the galactic cluster Pleiades belong to stellar Population I or II? ...
Stellar Evolution Simulation
Stellar Evolution Simulation

Star Classification Lab
Star Classification Lab

ASTR 300 Stars and Stellar Systems Spring 2011
ASTR 300 Stars and Stellar Systems Spring 2011

Solution - Caltech Astronomy
Solution - Caltech Astronomy

STARS AND CONSTELLATIONS
STARS AND CONSTELLATIONS

... - Last star in the Little Dipper handle - Pole star- called Polaris - Known to the Vikings as the Jewel Nailhead, to the Mongols as the Golden Peg, to the Chinese as the Emperor of Heavens, and to the American Indians as the Chief Star. The American Indians made and used star charts. - Polaris is a ...
Homework 3 available
Homework 3 available

... c. (10 points) Only the central 10% of the mass of the Sun is close enough to the core, i.e., hot and dense enough, for thermonuclear fusion to take place. With this in mind (and remembering that only 75% of the mass of the Sun is hydrogen) calculate how long the Sun can shine with its current lumin ...
22 Stellar Remnant/HR Diagram
22 Stellar Remnant/HR Diagram

... Guess why the classifications are so weird… Assigned a letter in alphabetical ...
Astronomers classify stars according to their physical characteristics
Astronomers classify stars according to their physical characteristics

... called its _apparent magnitude__ or brightness. •A star’s _apparent_ brightness depends upon how bright it _actually is and its _distance_ from Earth. •A star’s actual brightness (or _absolute magnitude) usually depends on the star’s _size_ and temperature__. •Because stars with _more mass ___ have ...
15compact2s
15compact2s

... If a stellar core has mass greater than the Chandrasehkar limit (1.4 Msun), electron degeneracy pressure cannot support it ...
Handout Life of Stars
Handout Life of Stars

... helium (the second simplest, with two protons and two neutrons in its nucleus). The nucleus of a helium atom actually weighs only 99.3% as much as the two protons and two neutrons that go to make it up, the remaining 0.7% being released as heat and light energy. This 0.7% coefficient, which is essen ...
THE SUN: OUR STAR
THE SUN: OUR STAR

class17
class17

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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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