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about Stars
about Stars

... of B-V color, and are found on the left side of the diagram. Cooler stars are brighter in yellow light than in blue light, have larger values of B-V color, and are found on the right side of the diagram. ...
Chapter 8: Stars
Chapter 8: Stars

Astronomy - Test 3
Astronomy - Test 3

... E) Although such objects could occur, they would be so rare that we ignore them 26. Which of the following was not a method for making black holes that was discussed? A) Very high mass star supernova B) White dwarf supernova C) Accretion of matter onto a neutron star D) Merger of neutron stars E) Ac ...
Stellar Evolution
Stellar Evolution

Astronomy 114 – Summary of Important Concepts #2 1 Stars: key
Astronomy 114 – Summary of Important Concepts #2 1 Stars: key

... p = 0.1 arcseconds ...
Chapter 15 Surveying the Stars
Chapter 15 Surveying the Stars

... smaller radii: ...
Brightness and Distance
Brightness and Distance

Determining the Sizes & Distances of Stars Using the H
Determining the Sizes & Distances of Stars Using the H

... ● Giants: Giants are stars that have begun to evolve after finishing their time as a main sequence star. Their cores have filled with helium. There is not enough hydrogen left in the core so burning occurs in a shell surrounding the core, where more helium resides. In the process, the star grows in ...
Star Magnitude - ScienceEducationatNewPaltz
Star Magnitude - ScienceEducationatNewPaltz

... The First Magnitude Stars Table lists the brightest stars in the sky that are -1, 0 and 1 magnitude. Sirius is the brightest at -1.44 magnitude. These stars are referred to as First Magnitude stars since they are all 1 magnitude or brighter. Brightness of stars is assigned a number starting with the ...
The Magnitude Scale
The Magnitude Scale

... are not "exact", in that celestial objects are often measured to a precision or 0.1 or 0.01 magnitude; for example, Sirius shines at V = -1.47 (Yale Bright Star Catalogue), and the planet Venus varies in brightness generally from magnitude -4.5 to -3.7. Note that a comet of magnitude 5 will not be a ...
ASTR100 Class 01 - University of Maryland Department of
ASTR100 Class 01 - University of Maryland Department of

Lecture 5: Stars
Lecture 5: Stars

... We only know the absolute luminosity if we know the distance, but we only know the parallax distances out to about 100 pc (further to some bright stars). The problem is that if we see a star with a surface temperature of 3000K – is it a nearby red dwarf, or a distant red giant? Without more informat ...
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Study Island

... 3. A prediction is a forecast about what may happen in some future situation. An inference is an explanation based on observations and background knowledge. Based on these definitions, which of the following statements is a prediction? A. The stove was hot because the kitchen light was on too long. ...
Stars I - Astronomy Centre
Stars I - Astronomy Centre

... Seminar Quiz (Stars III) • Why, apart from the Sun, can we only measure reliable masses for stars in binary systems? • Sirius, the brightest star in the sky, has a parallax of 0.379 arcseconds. What is its distance in parsecs? In light years? • Sirius is 22 times more luminous than the Sun; Polaris ...
Astronomical Distance Determination
Astronomical Distance Determination

Star and Galaxies Chapter 13
Star and Galaxies Chapter 13

Name: pd: ______ Date: Constellation Scavenger Hunt! Google Sky
Name: pd: ______ Date: Constellation Scavenger Hunt! Google Sky

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The Solar Neighborhood

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Star and Galaxies Chapter 13 2013

... • Middle aged, absolute magnitude is about average • Shines yellow light • Takes 8 minutes for light to reach earth • It is unusual in fact it is found as a single star (normally stars are in groups of 2 (binary system) • Star clusters: group of stars that have a gravitation attraction to each other ...
Star Show FACILITATOR NOTES
Star Show FACILITATOR NOTES

... closely matches the Sun’s spectrum must have a temperature very close to the temperature at the Sun’s visible surface—well over 5000°C. Except for specialized lights used in photography, most real light filaments operate at a lower temperature (around 2500°C) which gives a more reddish-orange color ...
Introduction to the HR Diagram
Introduction to the HR Diagram

... carbon. Most of these stars go through a Mira variable instability strip with a periodic light curve of ~80 - 1000 days. Stars that have evolved to the giant branch are commonly referred to as red giants. Eventually these red giants will shrug off a planetary nebula and leave a white dwarf core remn ...
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The Zodiac - Alchemical.org
The Zodiac - Alchemical.org

... Sumerians had seen these stars as Enki, their river god. He was the ruler of the waters of the Euphrates. The Assyrians saw him as half fish, half man, Oannes, god of wisdom. The Egyptians associated the constellation with the Nile. The ancient Greeks first saw these stars as Pan, half man, half goa ...
Mr. Traeger`s Light and Stars PowerPoint
Mr. Traeger`s Light and Stars PowerPoint

... A cosmological red-shift indicates that stars and galaxies are moving away from us. As Mr. Auld pointed out, this means that our Universe is expanding, or moving outwards. ...
Lecture17
Lecture17

... How can this be? They emit less light per square meter than a blue main sequence star, but, they are much, much bigger (more square meters)! ...
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Auriga (constellation)



Auriga is one of the 48 constellations listed by the 2nd-century astronomer Ptolemy and remains one of the 88 modern constellations. Located north of the celestial equator, its name is the Latin word for ""charioteer"", associating it with various mythological charioteers, including Erichthonius and Myrtilus. Auriga is most prominent during winter evenings in the Northern Hemisphere, along with the five other constellations that have stars in the Winter Hexagon asterism. Because of its northern declination, Auriga is only visible in its entirety as far as 34° south; for observers farther south it lies partially or fully below the horizon. A large constellation, with an area of 657 square degrees, it is half the size of the largest constellation, Hydra.Its brightest star, Capella, is an unusual multiple star system among the brightest stars in the night sky. Beta Aurigae is an interesting variable star in the constellation; Epsilon Aurigae, a nearby eclipsing binary with an unusually long period, has been studied intensively. Because of its position near the winter Milky Way, Auriga has many bright open clusters in its borders, including M36, M37, and M38, popular targets for amateur astronomers. In addition, it has one prominent nebula, the Flaming Star Nebula, associated with the variable star AE Aurigae.In Chinese mythology, Auriga's stars were incorporated into several constellations, including the celestial emperors' chariots, made up of the modern constellation's brightest stars. Auriga is home to the radiant for the Aurigids, Zeta Aurigids, Delta Aurigids, and the hypothesized Iota Aurigids.
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