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HW #4 (due March 27)
HW #4 (due March 27)

... When astronomers look through their telescopes, they see billions of stars. What can they learn from their observations? In class, we’ve learned that the shape of the spectrum (especially, the wavelength at which it reaches its maximum intensity) can be used to determine a star’s temperature. In add ...
TYPES OF STARS
TYPES OF STARS

... When astronomers look through their telescopes, they see billions of stars. What can they learn from their observations? In class, we’ve learned that the shape of the spectrum (especially, the wavelength at which it reaches its maximum intensity) can be used to determine a star’s temperature. In add ...
6. 1 Star Distances 6. 2 Apparent Brightness, Intrinsic Brightness
6. 1 Star Distances 6. 2 Apparent Brightness, Intrinsic Brightness

Chapter 28 – Stars and Galaxies
Chapter 28 – Stars and Galaxies

... 1. The actual brightness of the star is luminosity 2. If two stars have the same surface temperature, the larger star would be more luminous 3. If the same size, hotter one would be brighter 4. Types of magnitude a. Absolute – as if all stars were same distance from earth b. Apparent – as they appea ...
Evan_Skillman_1
Evan_Skillman_1

... less than around 100 million years. ...
Stars - TeacherWeb
Stars - TeacherWeb

April - Bristol Astronomical Society
April - Bristol Astronomical Society

... Alpha (α) Corvi marks the beak of the crow, it is a F-class (F0) yellow dwarf star. Despite its alpha designation it only 5th in brightness at magnitude +4.00. The star’s proper name, Alchiba means ‘tent’ in Arabic and is thought to refer to the four stars that make up the main body of the crow. Bet ...
At the Heart of the Matter: The Blue White Dwarf in M 57. Paul Temple
At the Heart of the Matter: The Blue White Dwarf in M 57. Paul Temple

Microsoft Power Point version
Microsoft Power Point version

Teacher Subject Title Concept Context Tek/SE Verb
Teacher Subject Title Concept Context Tek/SE Verb

... Objects in the sky can be described and illustrated. We can observe objects in the sky, such as the Moon, Sun, and stars. — When is the best time to observe stars? — When is the best time to observe the Sun? The Sun is our nearest star. — What is the Sun? Objects in the sky can be described and illu ...
powerpoint - Physics @ IUPUI
powerpoint - Physics @ IUPUI

... • Will the spin get faster or slower? ...
The Life Cycle of Stars
The Life Cycle of Stars

The hierarchical structure of the Universe (go from little to large)
The hierarchical structure of the Universe (go from little to large)

Hertzsprung2 - courses.psu.edu
Hertzsprung2 - courses.psu.edu

... What is the luminosity (relative to the sun) of a star 3 times more massive than the sun? ...
Stellar Evolution 1 Star Formation 2 Nebulae
Stellar Evolution 1 Star Formation 2 Nebulae

... ˆ What are the basic properties of giant molecular clouds? ˆ How do clumps form in giant molecular clouds? ˆ How do clumps in giant molecular clouds evolve? What are the conditions for which this kind of evolution takes place? ˆ Where are protostars found on an H-R diagram? How do their locations on ...
Stars
Stars

Measuring Stars
Measuring Stars

PowerPoint
PowerPoint

Star Types
Star Types

... The H-R diagram “The stars are distant and unobtrusive, but bright and enduring as our fairest and most ...
Assessment 1 - Stars - Teacher Key
Assessment 1 - Stars - Teacher Key

15 - Edmodo
15 - Edmodo

Lifecycle of the stars.
Lifecycle of the stars.

...  Small proto star-a brown dwarf that was too small to generate enough heat to start fusion. ...
Hertzsprung-Russell Diagram
Hertzsprung-Russell Diagram

... The Main Sequence At one end, the stars are big, hot and bright. Due to their color and size they are called blue giants, and the very largest are blue supergiants. At the other end they are small, cool and dim and are known as red dwarfs. The sun is right in the middle. ...
Properties of stars
Properties of stars

Brightness + Magnitude of Stars
Brightness + Magnitude of Stars

< 1 ... 92 93 94 95 96 97 98 99 100 ... 132 >

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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