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GO1_Distrubtion Of Matter In Space
GO1_Distrubtion Of Matter In Space

... • Gravity pulls gas and dust in a NEBULA together into a rotating sphere (composed of ~75% H and 23% He) • As more material is drawn into the spinning ball, the mass at its core increases causing the temperature to rise and possibly start to glow (called a pro-star) • As the process continues, heati ...
wk9 (part 1)
wk9 (part 1)

... spectral type (OBAFGKM) is directly related to their surface temperature ...
Apparent Magnitude
Apparent Magnitude

galaxies and stars - Valhalla High School
galaxies and stars - Valhalla High School

... faster it is moving. • It takes 2 million years for light from the Andromeda galaxy to reach earth. • Astronomers have classified most galaxies into three main categories: spiral, elliptical and irregular. ...
Teacher Sheet 1. What variables does the HR Diagram compare
Teacher Sheet 1. What variables does the HR Diagram compare

Study Guide: Unit 1, The Universe and its Stars, HS
Study Guide: Unit 1, The Universe and its Stars, HS

... 31) HS-ESS1-1 The final stage for a star which is as massive as the Sun is a ________. A) red giant B) black hole C) main-sequence star D) white dwarf 32) HS-ESS1-1 When a main-sequence star has exhausted the fuel in the inner region, it becomes a ________. A) black hole B) main-sequence star C) bla ...
Stars and Galaxies
Stars and Galaxies

Note Taking Guide #2: Characteristics of Stars Welcome back! As
Note Taking Guide #2: Characteristics of Stars Welcome back! As

Stellar evolution, II
Stellar evolution, II

29.2 Measuring the Stars - Mr. Tobin`s Earth Science Class
29.2 Measuring the Stars - Mr. Tobin`s Earth Science Class

... an observer’s position in space is always changing. • Distance to a star can be estimated using the star’s parallax (angle of change.) • Closer the star, the larger the shift. • Estimates are accurate up to 500 pc away. ...
Document
Document

... • You want to detect the faint star of an unresolved binary system comprising a B5V star and an M0V companion. What wavelength regime would you choose to try to detect the M0V star? What is the ratio of the flux from the B star to the flux from the M star at that wavelength? • You want to detect the ...
Lecture 14 - Center for Astrophysics and Space Astronomy CASA
Lecture 14 - Center for Astrophysics and Space Astronomy CASA

... White Dwarf Collapse As WD starts to collapse, the material falls through the gravitational field of the star. It heats very rapidly. In just a few seconds it reaches >100,000,000K. Carbon and Oxygen ignite and burn by fusion to even heavier elements. The whole star explodes in a frenzy of nuclear ...
The HR Diagram Interpreted (PowerPoint version)
The HR Diagram Interpreted (PowerPoint version)

... Is the Sun an ‘Average’ Star? It is (roughly) in the middle of the range, so it is certainly not unusual. But is it average? Analogy: is a human being an average-sized living creature? We are in the ‘mid-range’, between blue whales and bacteria, giraffes and mice,… But there are many more bacteria ...
The HR Diagram Interpreted: Properties of Stars
The HR Diagram Interpreted: Properties of Stars

Birth of Stars
Birth of Stars

downloadable pdf - University of Florida
downloadable pdf - University of Florida

1. absolute brightness -
1. absolute brightness -

Death of Stars
Death of Stars

... Birth Place of Stars: Dark and cold inter-stellar clouds These clouds are made of more hydrogen than helium. These clouds have very small amount of heavier elements. ...
Sample Math problems
Sample Math problems

The Future Sun
The Future Sun

... stars than Pleiades. b. Most stars are one the main sequence. c. Perseus has small range of luminosity d. Some clusters have giants. ...
Physics@Brock - Brock University
Physics@Brock - Brock University

Answers to Coursebook questions – Chapter E2
Answers to Coursebook questions – Chapter E2

... Initially the luminosity and surface temperature were lower than the values on the main sequence. So it had to be to the right of and lower than the present position. ...
Lecture 13: The stars are suns
Lecture 13: The stars are suns

Planetarium Activity 1 Learning to measure brightness and Limiting
Planetarium Activity 1 Learning to measure brightness and Limiting

Stars - Red, Blue, Old, New pt.3
Stars - Red, Blue, Old, New pt.3

... solar masses) will never be a supergiant. • Stars more massive than about 10 solar masses do get to be supergiants. • The massive stars fuse elements up to iron and they do it fast…timescales 1000s of years. ...
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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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