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Goal: To understand how to find the brightness of stars and what
Goal: To understand how to find the brightness of stars and what

The Stars education kit - Student activities 5-10
The Stars education kit - Student activities 5-10

... Sirius is the brightest star in the night sky and is part of the constellation Canis Major. It is a blue-white supergiant star about 9 light years away. Alpha Centauri lies in the constellation of Centaurus. It is one of the bright Pointers that point to the Southern Cross. It is the third brightest ...
Magnitudes and Colours of Stars - Lincoln
Magnitudes and Colours of Stars - Lincoln

... In fact, as we will see in the next Module, stars behave very like practical examples of black bodies - theoretical objects with properties that have been determined by classical physicists. (We will leave the tricky question of how someone could describe a star as a black body to the next Module!) ...
Red Giants - Faculty Web Pages
Red Giants - Faculty Web Pages

Star Formation
Star Formation

... stars drift apart, becoming “stellar associations”, and then just individual stars • Globular clusters ~100x more massive than open clusters, and made during formation of the Galaxy. More on them in the chapter on the Milky Way Galaxy ...
Measuring Stars` Properties - Test 1 Study Guide
Measuring Stars` Properties - Test 1 Study Guide

Compact stars
Compact stars

... 3. Neutron stars The Crab Nebula is a supernova remnant containing the Crab Pulsar, a neutron star. Main article: Neutron star In certain binary stars containing a white dwarf, mass is transferred from the companion star onto the white dwarf, eventually pushing it over the Chandrasekhar limit. Elect ...
Stars - CBSD.org
Stars - CBSD.org

... Magnitudes • Hipparchus decided that all the brightest stars in the night sky were “first order magnitude” stars. • As they got dimmer, he classified them as “second magnitude,” “third magnitude,” and so on… • He got up to magnitude 6, after which stars are too dim to be seen without a telescope. • ...
The Solar Neighborhood
The Solar Neighborhood

... The globular star clusters are bright, and can be seen for a long distance. Their distances can be estimated accurately from their main sequence turnoffs, as well as by measuring the periods of variable stars that belong to each cluster. In the table below are listed several dozen Galactic globular ...
Death of Stars notes
Death of Stars notes

Pulsating Variable Stars and The Hertzsprung - Chandra X
Pulsating Variable Stars and The Hertzsprung - Chandra X

... brightness that a star appears to have (apparent magnitude) from our perspective here on Earth depends upon its distance from Earth and its actual intrinsic brightness, or absolute magnitude (MV). The behavior of stars that vary in magnitude (brightness) can be studied by measuring their changes in ...
Famous Constellations
Famous Constellations

... Orion, the Hunter, famous constellation named from Greek Mythology It is most easily recognized constellation https://img1.etsystatic.com/009/1/5742776/il_570xN.411934929_a84j.jpg Ursa Major is also famous and very important because it points to North Star Ursa Major means Big Bear in Latin http://3 ...
MS Word version
MS Word version

... demonstrating the Eclipsing Binary Simulator in a classroom situation. We provide these suggestions with appropriate questions (shown in bold italics) to pose to the class as an aid in promoting interactivity. We encourage instructors to adapt these suggestions to their particular educational goals ...
Life cycle of low mass stars
Life cycle of low mass stars

... 1. Scientists believe that their was a time when the density of matter was inconceivably high 2. All matter confined to a dense hot super-massive ball 3. 13.7 million years ago, a massive explosion occurred initiating the expansion of our universe. ...
Star Magnitude - ScienceEducationatNewPaltz
Star Magnitude - ScienceEducationatNewPaltz

... With the invention of the telescope and modern equipment to measure star magnitudes the scale has been extended in both directions. Dimmer stars are assigned magnitudes larger than 6 ( 6, 7, 8, 9, ... 30th ... etc.) The Hubble Space Telescope Deep Field image contains some galaxies as faint as 30th ...
Chapter 30 Notes
Chapter 30 Notes

... • Binary stars are pairs of stars that revolve around each other and are held together by gravity. The center of mass, or barycenter, is somewhere between the two stars. • In star systems that have more than two stars, two stars may revolve rapidly around a common barycenter, while a third star revo ...
Measuring the Properties of Stars (ch. 17)
Measuring the Properties of Stars (ch. 17)

Ch. 20
Ch. 20

... all the same age but have different masses. • Stars in binary systems can evolve quite differently due to interactions with each other. ...
What we can measure
What we can measure

ILÍDIO LOPES ()
ILÍDIO LOPES ()

DTU9ePPTChap13 - Faculty Lounge : Astronomy
DTU9ePPTChap13 - Faculty Lounge : Astronomy

Stars change over their life cycles.
Stars change over their life cycles.

... Betelgeuse (BEET-uhl-JOOZ) is more than 600 times greater in diameter than the Sun. If Betelgeuse replaced the Sun, it would fill space in our solar system well beyond Earth’s orbit. Because giant and supergiant stars have such huge surface areas to give off light, they are very bright. Betelgeuse i ...
Astrophysics notes
Astrophysics notes

... point sources such that they can be just barely distinguished as separate sources define the term ‘sensitivity’ of a telescope as the light-gathering power of the telescope (directly proportional to the square of the diameter of the objective) define the term parallax as the apparent shift in positi ...
File
File

... The more massive a star is, the shorter its stay on the main sequence. The most massive stars may be there for only a few million years. A star like the Sun, on the other hand, is not especially massive and will live on the main sequence for about ten billion years. Since it has taken over four bill ...
FREE Sample Here
FREE Sample Here

... appears to us when viewing the star from here on Earth. Apparent visual magnitude does not take into account any corrections for the star's distance, size, temperature, or the amount of dust between us and the star. It is simply the brightness as it appears to us in the night sky. ...
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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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