• 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
The life cycle of a star
The life cycle of a star

... When extremely large stars die, the resulting core is called a neutron star  An extremely dense star made of neutrons ...
spectral-type
spectral-type

Eclipsing Binaries
Eclipsing Binaries

... Many such measurements show us that mass increases on the Main Sequence as the temperature and luminosity increase. As theory predicts. Furthermore, Mass does not correlate with luminosity for giant, evolved stars. Giants might have a large mass, or they might have a small mass, but still they are v ...
The Life Cycle of a Star Webquest
The Life Cycle of a Star Webquest

... ______ The gas and dust compresses into a slowly rotating ball. ______ The gas ball begins to spin faster and cool. ______ A star begins to form from clouds of hydrogen gas and dust. ______ The ball separate into a core and spinning disks. 3. How long can a star stay a protostar? ___________________ ...
Problem Sheet for Introduction to Astrophysics
Problem Sheet for Introduction to Astrophysics

PHY299B Poster-Justin Hudson-v2
PHY299B Poster-Justin Hudson-v2

File - Mr. Goodyear Astronomy
File - Mr. Goodyear Astronomy

... hydrogen in core of star decreases and helium in core rises, the star starts to become unstable and equilibrium breaks down, gravity takes over – causing greater pressure on core and causes helium flash or fusion (new energy He C ) Star grows: increase energy overcomes gravity, star moves off the ma ...
Stars Notes
Stars Notes

... Sirius is the brightest star in our sky. It is about 9 light-years away from Earth and has a magnitude of 1.4 ...
Support worksheet – Topic 3 Questions
Support worksheet – Topic 3 Questions

... Suggest why the stellar parallax method is limited to distances of about 300 pc for Earth-based telescopes but can be extended to 1000 pc for satellite-based telescopes. ...
Stellar_Evol
Stellar_Evol

How Bright is that Star?
How Bright is that Star?

Astronomy 2
Astronomy 2

... The original mass of the star determines its temperature and the color. (Big – glows blue, medium – glows yellow-orange, small – glows red) Red Giants / Red Super-giants form as H2 fuel is used up and gravity overpowers released energy, center core contracts while outer layer expands (He2 + He2 → C ...
Sequence of Stars Notes
Sequence of Stars Notes

...  When a star uses up its supply of helium, it ...
1000
1000

... star and you notice that the star you are watching has moved about 15 degrees, how long have you been watching? ...
Chapter 28.3 Topic questions
Chapter 28.3 Topic questions

... 19. When all outer layers are blown away what is left? 20. What do we call a white dwarf when it carbon-oxygen core cools completely? 21. Stars that are ______________________ or _________________ times as massive as the sun have a different live cycle. 22. Does a massive star live as long as a mai ...
Stars_and_Galaxies
Stars_and_Galaxies

... north, there are constellations that appear to move in a circle around the north star, Polaris. These are circumpolar constellations. • They are visible year-round in each hemisphere ...
Lives of stars
Lives of stars

... brightness: binary system 1. How close the binary stars needs to be for any type of mass transfer to take place? Adetached, b-semi-detached, c- contact, dover contact. 2. In Which type of binary the atmospheric composition will be identical. A- detached, bsemi-detached, c- contact, d- over contact. ...
Study Guide
Study Guide

...  Explain the H-R diagram and the where each type of star lies on it. Classifies stars according to their absolute magnitude, temperature, and luminosity  State what part of its lifecycle our sun is in. Main sequence  State magnitudes of stars from the H-R diagram. White dwarfs, main sequence, gia ...
here - Lund Observatory
here - Lund Observatory

CONSTELLATION CANES VENATICI the two hunting dogs Canes
CONSTELLATION CANES VENATICI the two hunting dogs Canes

... the two hunting dogs Canes Venatici represents two dogs, two hounds, or two greyhounds, on a leash or brache (two hounds in leash are known as a brache, which is the same word as brace, meaning pair, and embrace). Here the leash is held by Bootes, the Herdsman or Bear Driver as they together pursue ...
RFS_multiple_choice_Dec8_Key
RFS_multiple_choice_Dec8_Key

... A. Messier objects: astronomical objects catalogued by Charles Messier B. They are all objects for which the first detailed study was carried out by the Mauna Kea Observatory in Hawaii C. Objects which lie within 5 degrees on either side of the ecliptic, and are hence occulted by the moon at some ti ...
Document
Document

Stars
Stars

... Mizar, 88 light years distant, is the middle star in the handle of the Big Dipper. It was the first binary star system to be imaged with a telescope. Spectroscopic observations show periodic Doppler shifts in the spectra of Mizar A and B, indicating that they are each binary stars. But they were too ...
3.6 spectral classes
3.6 spectral classes

Lesson 10 Red Shift
Lesson 10 Red Shift

... "visual spectrum." In the visual spectrum, wavelength corresponds to colour. In other words, violet and red each have a characteristic range of wavelengths. In the visible spectrum, violet has the shortest wavelengths and red as the longest. Normally when we look at white light, such as from the Sun ...
< 1 ... 111 112 113 114 115 116 117 118 119 ... 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