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Krupp (1999) broadly defines the interdisciplinary field
Krupp (1999) broadly defines the interdisciplinary field

... fainter than magnitude 3. The spatial relation of the one exception (a magnitude 2.9 star, 7O away) is such that it conceivably could be represented by a cupule on the other side of the crack. (The next nearest bright stars in the sky are in the constellation Scorpius.) Sagittarius does not present ...
Exploring Stars - Discovery Education
Exploring Stars - Discovery Education

... 1. Talk about the life of a star. A good way to introduce this topic is to show Exploring Stars. After watching the program, talk about the different types of stars found in the universe. What are stars? What are they made of? How is a red star different from a blue star? Discuss and review the life ...
Chapter 5 Galaxies and Star Systems
Chapter 5 Galaxies and Star Systems

... Our sun is the one star in our solar system. As you move past our solar system, billions of other stars make up our galaxy. Most stars are members of groups of two or more stars, called star systems. Binary stars are pairs of stars. Scientists detect binary stars by observing the brightness and moti ...
Analysis of Two Pulsating X-ray Sources
Analysis of Two Pulsating X-ray Sources

... The acceleration due to gravity (g) on the surface of a star (according to Newton’s Universal Law of Gravitation) is given by g = (GM)/R2 where G = 6.67 X 10-11 Nm2/kg2, M=star’s mass and R = star’s radius Centripetal acceleration (ac) of an object on the surface of a star at its equator is given by ...
E1 Introduction to the universe
E1 Introduction to the universe

... scales of luminosity and/or absolute magnitude, spectral class and/or surface temperature Students should be aware that the scale is not linear. Students should know that the mass of main sequence stars determines their position on the HR diagram. ...
August Newsletter
August Newsletter

... Corona Australis, the Southern Crown is an old constellation and is believed to represent the crown worn by the centaur Sagittarius. It was one of the original 48 constellations named by the astronomer Ptolemy. In ancient times it was pictured as a hand full of arrows held by the centaur, Centaurus. ...
Celestial Distances - Wayne State University
Celestial Distances - Wayne State University

Surveying the Stars
Surveying the Stars

star - TeacherWeb
star - TeacherWeb

about Stars
about Stars

... • Astronomers quantify the “color” of a star by using the difference in brightness between the brightness in the B and V spectral regions • The B-V color is related to the slope of the ...
Chapter 30 Notes
Chapter 30 Notes

... Black hole- an object so massive (not always big but having a lot of mass) and dense that even light cannot escape its gravity. Some massive stars produce leftovers too massive to become stable neutron stars. These leftovers contract and the force of the contraction leaves a black hole. Star Groups ...
Friday, April 25 - Otterbein University
Friday, April 25 - Otterbein University

... distance ladder out as far as we can see Cepheids – about 50 million ly • In 1920 Hubble used this technique to measure the distance to Andromeda (about 2 million ly) • Works best for periodic variables ...
Luminosity - U of L Class Index
Luminosity - U of L Class Index

... • The light curve of this pulsating variable star shows that its brightness alternately rises and falls over a 50-day period ...
Interpreting the HR diagram of stellar clusters
Interpreting the HR diagram of stellar clusters

... In fact, it seems that stars are usually born in big groups, as members of a cluster of stars. All the stars in the cluster form at about the same time. So, if we look at a cluster, we see a bunch of stars which are all roughly the same age. However, the stars do not all have the same mass: most ten ...
Stars, Constellations, and Quasars
Stars, Constellations, and Quasars

Astrophysics E1. This question is about stars.
Astrophysics E1. This question is about stars.

... E2. This question is about cosmology. (a) The diagram below represents a spherical region of space based on Newton’s model of the universe. Earth is at the centre of the region. The dark line represents a very thin spherical shell of space distance R from Earth. With reference to the diagram and New ...
H R Diagram Online Activity
H R Diagram Online Activity

OBAFGKM(LT) extra credit due today. Mid
OBAFGKM(LT) extra credit due today. Mid

Classifying the Spectra of Stars:
Classifying the Spectra of Stars:

... noticeable. Band heads are very "thick" absorption lines that break up the spectrum. ...
HW #02 Solutions
HW #02 Solutions

... 10. If our Sun has a surface temperature of 5840 K, how many times hotter than the Sun is the hottest Otype star? How many times cooler than the Sun is the coolest M-type star? The hottest O-type star has a temperature of about 50,000 K and this is approximately 10 times hotter than the Sun (5,800 K ...
STAR FORMATION (Ch. 19) - University of Texas Astronomy Home
STAR FORMATION (Ch. 19) - University of Texas Astronomy Home

... disks, and progressing to evolved massive stars in the young starburst cluster.To the upper right of center is the evolved blue supergiant called Sher 25. The star has a unique circumstellar ring of glowing gas that is a galactic twin to the famous ring around the supernova 1987A--see the image of S ...
Introduction to Astrotheology
Introduction to Astrotheology

Document
Document

apparent magnitude - Harding University
apparent magnitude - Harding University

... they orbit one another.  A visual binary is an orbiting pair of stars that can be resolved (normally with a telescope) as two stars.  If one uses large telescopes, about 10% of the stars in the sky are visual binaries. ...
The Milky Way - Houston Community College System
The Milky Way - Houston Community College System

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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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