• Study Resource
  • Explore Categories
    • Arts & Humanities
    • Business
    • Engineering & Technology
    • Foreign Language
    • History
    • Math
    • Science
    • Social Science

    Top subcategories

    • Advanced Math
    • Algebra
    • Basic Math
    • Calculus
    • Geometry
    • Linear Algebra
    • Pre-Algebra
    • Pre-Calculus
    • Statistics And Probability
    • Trigonometry
    • other →

    Top subcategories

    • Astronomy
    • Astrophysics
    • Biology
    • Chemistry
    • Earth Science
    • Environmental Science
    • Health Science
    • Physics
    • other →

    Top subcategories

    • Anthropology
    • Law
    • Political Science
    • Psychology
    • Sociology
    • other →

    Top subcategories

    • Accounting
    • Economics
    • Finance
    • Management
    • other →

    Top subcategories

    • Aerospace Engineering
    • Bioengineering
    • Chemical Engineering
    • Civil Engineering
    • Computer Science
    • Electrical Engineering
    • Industrial Engineering
    • Mechanical Engineering
    • Web Design
    • other →

    Top subcategories

    • Architecture
    • Communications
    • English
    • Gender Studies
    • Music
    • Performing Arts
    • Philosophy
    • Religious Studies
    • Writing
    • other →

    Top subcategories

    • Ancient History
    • European History
    • US History
    • World History
    • other →

    Top subcategories

    • Croatian
    • Czech
    • Finnish
    • Greek
    • Hindi
    • Japanese
    • Korean
    • Persian
    • Swedish
    • Turkish
    • other →
 
Profile Documents Logout
Upload
Supernovae - Cloudfront.net
Supernovae - Cloudfront.net

Astronomy – Studying the Stars & Space
Astronomy – Studying the Stars & Space

... and dense that even use their hydrogen quickly and may light cannot escape explode in a huge its gravity bright flash • Gas or dust that sink • Can be brighter than into black hole from a an entire galaxy for star form x-ray light several days which may indicate a • A collapsed star can black holes’ ...
properties of stars 2012
properties of stars 2012

... A PULSATING variable is a star that is swelling and shrinking. As it swells, the same energy is spread over a larger area, the star cools and appears dimmer. (also, star cols because less pressure allows energy to escape) As it shrinks, it heats up (Gay-Lussac’s law--more pressure = higher temperatu ...
Stars and H
Stars and H

... blown away ...
Star Study Guide Chapter 21 Test
Star Study Guide Chapter 21 Test

... shows the relationship between absolute brightness and surface temperature of a star ...
February - Bristol Astronomical Society
February - Bristol Astronomical Society

“Do you have a good caption for the pop-eyed, thin
“Do you have a good caption for the pop-eyed, thin

EMS, HR, Star Lives classwork/homework
EMS, HR, Star Lives classwork/homework

The Hertzsprung – Russell Diagram Star Data Table
The Hertzsprung – Russell Diagram Star Data Table

... Danish astronomer Ejnar Hertzsprung and American astronomer Henry Russell discovered a  relationship between the ​ brightness of a star​  and the ​ surface temperature ​ of a star.  The graph of  a star’s absolute magnitude versus its temperature is called an ​ ...
December 2014 - Coconino Astronomical Society
December 2014 - Coconino Astronomical Society

22 Stellar Remnant/HR Diagram
22 Stellar Remnant/HR Diagram

... Spectroscopic Parallax? We can now get the temperature (within a few 10’s of a degree)  Find a MS star at that Temp  Find the Luminosity/absolute magnitude  Gives a distance! ...
The Life of a Star
The Life of a Star

... • ….are in the second and longest stage. • As long as they have hydrogen atoms to fuse into helium atoms they just keep on releasing lots of energy. ...
Characteristics of Stars Stars Analyzing Starlight Star Characteristics
Characteristics of Stars Stars Analyzing Starlight Star Characteristics

24-2 Characteristics of Stars
24-2 Characteristics of Stars

... 24-2 Characteristics of Stars ...
Star Life Cycle Worksheet Directions: Write in the correct stages of a
Star Life Cycle Worksheet Directions: Write in the correct stages of a

... 1. ___________ are clouds of dust and gas from which a star first forms. They are pulled together by gravity into a spinning disc. The center of the disc becomes a star while the rest can become a system of planets. 2. _________ come from giant or massive stars. They grow to as much as three times t ...
Review Game
Review Game

Sample exam 2
Sample exam 2

... d. move from spectral type M to spectral type G e. not change luminosity class or spectral type Essay questions — choose three of the following questions; circle the numbers of the ones chosen, so I know which ones to grade. Please answer each question in sentence/paragraph format or a drawing, depe ...
Stars Part 2 - westscidept
Stars Part 2 - westscidept

... • Absolute magnitude is a measure of how bright a star would be if the star were 32.6 light-years away from Earth. • The absolute magnitude of the sun is +4.8. But because the sun is so close to Earth, its apparent magnitude is -26.8, which makes it the brightest object in the sky. ...
Place in Space
Place in Space

01-ChapterRadiation
01-ChapterRadiation

... Negative values for the color index (B-V) correspond to blue stars. ...
Stars from Afar
Stars from Afar

... A spectrograph (spek truh graf) breaks the light from an object into colors and photographs the resulting spectrum. Astronomers use spectrographs to get information about stars, including their chemical compositions and temperatures. ...
Due Date: Thursday, November 16, 2006
Due Date: Thursday, November 16, 2006

... The most significant difference between a high-mass star and the Sun will be their lifetime! Look at the HR diagram in Figure 11.1. The lifetime of Spica (10 Msun) is only about 10 million years. The lifetime of Achernar (6 Msun) is only 100 million years…so when we really should not expect the Sun ...
- ALMA Observatory
- ALMA Observatory

... Have you ever pulled a loose thread on your sweater, only to find that it has no end? Astronomers have observed a similar phenomenon in space! Two stars orbit around each other, in what is called a binary ...
Can We Make A Star?
Can We Make A Star?

... move so that the gasses will react with each other • Then we just sit way back and wait until the gasses explode into a fireball ...
How Is a Star`s Color Related to Its Temperature?
How Is a Star`s Color Related to Its Temperature?

< 1 ... 118 119 120 121 122 123 124 125 126 ... 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.
  • studyres.com © 2026
  • DMCA
  • Privacy
  • Terms
  • Report