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every star in the cluster.
every star in the cluster.

... giants, continually forming from evolving stars near the turnoff. But there were originally many stars that were even more massive, that became red giants for a time, and that have moved on to a different final form. The cluster contains a huge number of ‘stellar remnants.’ [Details to follow!] ...
Stars: from Adolescence to Old Age
Stars: from Adolescence to Old Age

... dampen (diminish) the pulsations • But stars entering and leaving stage 6 can briefly (in terms of star lifetimes!) create conditions where the pressure and gravity are out of sync and the pulsations continue for a time • Larger, more luminous stars will pulsate with longer periods than the smaller, ...
1 Stars
1 Stars

... in whole or in sections must include the referral attribution link http://www.ck12.org/saythanks (placed in a visible location) in addition to the following terms. Except as otherwise noted, all CK-12 Content (including CK-12 Curriculum Material) is made available to Users in accordance with the Cre ...
Tutor Marked Assignment
Tutor Marked Assignment

... (a) Express the distances of the stars Sirius A and Antares in light years. ...
EF Eri: Its White Dwarf Primary and L Dwarf Secondary
EF Eri: Its White Dwarf Primary and L Dwarf Secondary

... magnetic field --> dwarf nova, classical nova, nova-like (IP). These binaries contain an accretion disk. • If the white dwarf has a ~10 to 250MG field --> Polar or AM Herculis type. These contain no accretion disk. ...
Unit 3 - Lesson 8.9 Life of Stars Challenge
Unit 3 - Lesson 8.9 Life of Stars Challenge

... unbalanced, the cloud collapses and breaks into small fragments. The smallest of these fragments contract further to form these pre-stars This catastrophic event is thought to be main source of elements heavier than hydrogen and helium A mass similar to that of the Sun, but only 1% of the Sun's diam ...
Stars, Galaxies, and the Universe Section 1
Stars, Galaxies, and the Universe Section 1

... rotational axis, so Polaris moves only slightly around the pole during one rotation of Earth. ...
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... it very different from BB ...
Glossary Topics - Home - DMNS Galaxy Guide Portal
Glossary Topics - Home - DMNS Galaxy Guide Portal

... 6. The ultimate fate of a star depends on its initial mass. The most massive stars (60 times the mass of the Sun or more) shed much of their mass during the main sequence phase as powerful stellar winds, including all of their hydrogen. In the cores of such massive stars most of the matter is conver ...
EarthComm_c1s9
EarthComm_c1s9

GenGeoAstroII_Stars
GenGeoAstroII_Stars

... (“Inverse square law”) ...
The Bigger Picture
The Bigger Picture

... motion of the centroid as it moves back and forth every six months. The lack of parallax apparent to the unaided eye was used as a proof that the Earth did not revolve around the Sun. ...
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Constellations

... Aquila represents the eagle of the roman god Jupiter in mythology. ...
Andromeda Check-List - Norman Lockyer Observatory
Andromeda Check-List - Norman Lockyer Observatory

Proper Motion
Proper Motion

... http://csep10.phys.utk.edu/astr162/lect/motion/pr oper.html ...
MS Word version
MS Word version

... Question 1: Complete the following table involving the horizon coordinate system. You should predict the answers and then use the simulator to check them. Remember that you can measure coordinates by dragging the active star to that location. ...
Devil physics The baddest class on campus IB Physics
Devil physics The baddest class on campus IB Physics

White Dwarfs
White Dwarfs

... a. These stars are fusing hydrogen at their surface. b. These stars have at least two active layers of fusion. c. These stars have multiple concentric layers of active fusion. d. We cannot see the interior stars that are below this temperature, as they are too dim. e. Planetary nebulae glow due to t ...
Chapter 1 Seeing the Light: The Art and Science of Astronomy
Chapter 1 Seeing the Light: The Art and Science of Astronomy

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1_Introduction

Three Coordinate Systems
Three Coordinate Systems

... Declination – angle from celestial equator (=0o), positive going north (north celestial pole = + 90o), negative going south (south celestial pole = - 90o) Right ascension (RA) – angle from celestial “prime meridian” – equivalent of celestial longitude RA – typically expressed as a time going east – ...
Variable star information
Variable star information

... outer layers expand and contract in a rhythmic manner. These stars are called pulsating variables because they periodically swell and shrink, as if they were breathing in and out. This pulsation causes periodic changes to the surface temperature, spectrum and brightness of these stars. There are dif ...
Constellations, Looking Far Away, and Stars/Stellar Evolution
Constellations, Looking Far Away, and Stars/Stellar Evolution

... D. Some Famous Star Patterns 1. Ursa Major: If you just looked at the pattern that makes up the asterism the Big Dipper, what would you ...
Amanda Boyle  Starstuff
Amanda Boyle Starstuff

... black holes and they drag everything down with themselves. But stellar collisions are not so common, at least to us because the universe operates in billions of years, and as a result our fleeting existence makes it difficult to speak with authority on these things. But we do understand the mainstr ...
Three Coordinate Systems
Three Coordinate Systems

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Boötes



Boötes /boʊˈoʊtiːz/ is a constellation in the northern sky, located between 0° and +60° declination, and 13 and 16 hours of right ascension on the celestial sphere. The name comes from the Greek Βοώτης, Boōtēs, meaning herdsman or plowman (literally, ox-driver; from βοῦς bous “cow”). The ""ö"" in the name is a diaeresis, not an umlaut, meaning that each 'o' is to be pronounced separately.One of the 48 constellations described by the 2nd century astronomer Ptolemy, Boötes is now one of the 88 modern constellations. It contains the fourth brightest star in the night sky, the orange-hued Arcturus. Boötes is home to many other bright stars, including eight above the fourth magnitude and an additional 21 above the fifth magnitude, making a total of 29 stars easily visible to the naked eye.
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