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Astronomical Toolkit
Astronomical Toolkit

a to z of astronomy
a to z of astronomy

... Two stars which are physically close together in space, held together gravitationally, and are orbiting their common centre of mass. They are to be distinguished from double stars which are two stars seen close together in the sky, but may be physically very distant from each other. BLACK BODY An im ...
Some Facts and Hypotheses regard
Some Facts and Hypotheses regard

Lesson 4 - Scientist in Residence Program
Lesson 4 - Scientist in Residence Program

... glass cools to show the difference between the bent pipette and the straight one. ...
Progenitor and environment of the peculiar red nova V838 Mon
Progenitor and environment of the peculiar red nova V838 Mon

2008F-ExtraSolarPlanets-Smith
2008F-ExtraSolarPlanets-Smith

... mass of Jupiter. The data shows that fainter stars can be seen with planets of smaller mass. Analyzing this information using the center of mass and Kepler’s Law shows why this is true. As the mass of the planet gets smaller and the mass of the moon is kept constant, the change in the center of mass ...
1 Exoplanets 2 Types of Exoplanets
1 Exoplanets 2 Types of Exoplanets

... systems from initial detection to flyby missions to even sending a lander to one of your choosing! You will work together in your group to make decisions regarding what you want to investigate, but then collectively decide as a class what will be investigated based on what is most frequently selecte ...
Lesson 6 - Magnitudes of Stars
Lesson 6 - Magnitudes of Stars

Measuring Stars` Properties - Test 1 Study Guide
Measuring Stars` Properties - Test 1 Study Guide

Summary: Star Formation Near and Far
Summary: Star Formation Near and Far

DP11 Foundations of Astronomy
DP11 Foundations of Astronomy

... at about a third of the rate predicted by theory. This was a problem for a long time, and many theories were advanced to explain it. Was the Sun's core cooler than expected? Could there be a lot of neutrinos with energies too low to be detected? The answer turns out to be that there are three differ ...
Chapter 12: Measuring the Properties of Stars
Chapter 12: Measuring the Properties of Stars

... 3. The extent of line broadening allows us to classify stars in different luminosity classes, denoted by roman numerals I, II, III, IV and V; supergiants (I), bright giants (II), giants (III), subgiants (IV), and main sequence stars (V). 4. The classification of stars in luminosity classes allows sp ...
What Is A Spectrum?
What Is A Spectrum?

Celestial Distances
Celestial Distances

... Astronomers take this number as another unit (besides the light year) for astronomical distances, called the parsec (abbreviated pc) In other words, 1 parsec is the distance to a star that has a parallax of 1 second of arc Thus, 1 pc = 206,265 AU = 3.26 LY 22 March 2005 ...
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Slide 1

... A very massive star collapsed to form a neutron star and not a black hole as expected, according to new results from NASA's Chandra X-ray Observatory. This discovery shows that nature has a harder time making black holes than previously thought. ...
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Signs of the Zodiac: Capricorn

ASTR1102-002 Potentially useful facts and mathematical relations
ASTR1102-002 Potentially useful facts and mathematical relations

NuSeti-2015 - Department of Physics and Astronomy
NuSeti-2015 - Department of Physics and Astronomy

... ideal carrier. (open problem: how to make Z-clocks!) We imagine that an ETI is doing just that at distances of order of kiloparsecs in the galaxy for its own spread out outposts… We expect to see neutrinos of energy of about 45.5 GeV. To get a few events per year in a KM3 detector, we estimate power ...
Stars PowerPoint
Stars PowerPoint

... sized star, of middle age, at 4.6 byo and 150 million km from earth. -It’s diameter is 1.35 million km-we could fit 1,000,000 Earths inside. ...
RTFS Test - 2017 BCS Cobra
RTFS Test - 2017 BCS Cobra

Stars and Constellations
Stars and Constellations

... with a lower number indicating a higher magnitude. A star with a magnitude of 5.5 is less bright than a star with a magnitude of -2.7. There are two types of magnitude - apparent and actual. The brightness of a star it appears from Earth is called apparent magnitude. Apparent magnitude measures a st ...
Star Formation
Star Formation

AST1100 Lecture Notes
AST1100 Lecture Notes

DO NOW - PBworks
DO NOW - PBworks

< 1 ... 30 31 32 33 34 35 36 37 38 ... 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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