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Problems_blackbody_spectra_hr
Problems_blackbody_spectra_hr

Star signs and horoscopes
Star signs and horoscopes

... is the part of the sky in which the Sun appears to move across the heavens (of course it is actually the Earth that moves). The zodiac is divided into 12 equal parts, each of which has its own star sign. Then explain that long ago, people thought there was a special meaning behind the movements and ...
Announcements Evolution of High-Mass Stars: Red Supergiants
Announcements Evolution of High-Mass Stars: Red Supergiants

Astronomy Study Guide
Astronomy Study Guide

... Apparent brightness—the brightness of a star as seen from Earth Absolute brightness—a star’s brightness as if it were a standard distance from Earth Constellation—an imaginary pattern of stars (example—Orion) Hertzsprung - Russell diagram (H-R diagram)—a graph of stars showing surface temperature on ...
Star Fromation and ISM
Star Fromation and ISM

... in the globular cluster is due to its extreme age – those stars have already used up their fuel and have moved off the main sequence. ...
Practice Questions for Exam 3
Practice Questions for Exam 3

... C. The Sun initially began generating energy through nuclear fusion as it formed, but today it generates energy primarily through the sunspot cycle. D. As the Sun was forming, gravitational contraction increased the Sun's temperature until the core become hot enough for nuclear fusion, which ever si ...
Student Exploration Sheet: Growing Plants
Student Exploration Sheet: Growing Plants

... If a star is moving away from an observer, spectral lines are redshifted, or shifted toward the red end of the spectrum. An approaching star is blueshifted. ...
Constituents of the Milky Way
Constituents of the Milky Way

Participant Handout - Math Machines Home
Participant Handout - Math Machines Home

... a very large “red giant,” with a diameter about 600 times that of our Sun. (If our Sun were that large, it would engulf the Earth and extend well beyond the orbit of Mars.) The actual power of a star (the quantity of light it emits per second) is called its “luminosity” and can be measured either in ...
CASPEC Observations of the Most Metal-Deficient Main
CASPEC Observations of the Most Metal-Deficient Main

... these stars may originate from lower initial masses. This raises the question: how small can the mass of a B[e] star in the MCs be? If future surveys confirm the presence of low mass B[e] stars in the MCs, this will have important implications for current models of massive star evolution in the Clou ...
Papervision3D star (sun) tutorial and source - 02
Papervision3D star (sun) tutorial and source - 02

Newfoundland Sky in Summer
Newfoundland Sky in Summer

... out in space. If we are viewing the stars on a moonlit night we may get the impression that the moon i s much larger than any of the stars. However, this is not so. The moon seems larger because it is much closer to us than even the nearest of the stars. ...
Nebulae
Nebulae

... Jets: Clumps of glowing gas are sometimes found along these jets and at their ends ...
Journey to the Stars: Activities for Grades 9-12
Journey to the Stars: Activities for Grades 9-12

Evolution of a Protostar
Evolution of a Protostar

The Stars - Department of Physics and Astronomy
The Stars - Department of Physics and Astronomy

... chemical testing of actual samples of stellar matter electromagnetic radiation spacecraft in orbit around distant stars both B and C above no data is used ...
Reach for the Stars – Div. B
Reach for the Stars – Div. B

... Lagoon Nebula(catalogued as Messier 8 or M8, and as NGC 6523) is a giant interstellar cloud in theconstellation Sagittarius. It is classified as an emission nebula and as a H II region. • The Lagoon Nebula was discovered by Giovanni Hodierna before 1654 and is one of only two star-forming nebulae fa ...
The Hertzsprung-Russell Diagram
The Hertzsprung-Russell Diagram

... expect stars of the same size but different temperatures to form a diagonal line called an equal radius line. Equal Radius lines can be added to an H-R diagram ...
Introduction: The Night Sky
Introduction: The Night Sky

Astronomy and Space Science
Astronomy and Space Science

... A: • Use the center of the vision to observe detail and color for bright object. • Use averted vision to detect/observe dim objects. More: • The color receptors, called cones, are distributed densely and mainly near the center of vision. • The more sensitive rods can only detect light intensity, and ...
Module 6: “The Message of Starlight Assignment 9: Parallax, stellar
Module 6: “The Message of Starlight Assignment 9: Parallax, stellar

Study Guide
Study Guide

Slides from Lecture04
Slides from Lecture04

Stars and Nebulae
Stars and Nebulae

G-stars - Gemini Astronomie
G-stars - Gemini Astronomie

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Corona Borealis

Corona Borealis /kɵˈroʊnə bɒriˈælɨs/ is a small constellation in the Northern Celestial Hemisphere. It is one of the 48 constellations listed by the 2nd-century astronomer Ptolemy, and remains one of the 88 modern constellations. Its brightest stars form a semicircular arc. Its Latin name, inspired by its shape, means ""northern crown"". In classical mythology Corona Borealis generally represented the crown given by the god Dionysus to the Cretan princess Ariadne and set by him in the heavens. Other cultures likened the pattern to a circle of elders, an eagle's nest, a bear's den, or even a smokehole. Ptolemy also listed a southern counterpart, Corona Australis, with a similar pattern. The brightest star is the magnitude 2.2 Alpha Coronae Borealis. The yellow supergiant R Coronae Borealis is the prototype of a rare class of giant stars—the R Coronae Borealis variables—that are extremely hydrogen deficient, and thought to result from the merger of two white dwarfs. T Coronae Borealis, also known as the Blaze Star, is another unusual type of variable star known as a recurrent nova. Normally of magnitude 10, it last flared up to magnitude 2 in 1946. ADS 9731 and Sigma Coronae Borealis are multiple star systems with six and five components respectively. Five star systems have been found to have Jupiter-sized exoplanets. Abell 2065 is a highly concentrated galaxy cluster one billion light-years from our Solar System containing more than 400 members, and is itself part of the larger Corona Borealis Supercluster.
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