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sunmoon - University of Glasgow
sunmoon - University of Glasgow

HW7-3
HW7-3

... (261) P 1: In the Figure 12-2, how much of the sun’s mass is hotter than 13,000,000 K? About 7.3%. Probably a bit more. L2L 1: In the photograph of the Pleiades on page 255, there are no bright red stars. Use the H-R diagram to explain why the brightest stars are blue. Have there ever been bright re ...
The Evening Sky Map
The Evening Sky Map

... Conjunction – An alignment of two celestial bodies such that they present the least angular separation as viewed from Earth. Constellation – A defined area of the sky containing a star pattern. Diffuse Nebula – A cloud of gas illuminated by nearby stars. Double Star – Two stars that appear close to ...
HighRedshiftGalaxies
HighRedshiftGalaxies

... In addition to the scatter arising from extinction (accounted for via individual Balmer emission line decrements), somebody suggests that some fraction of their UV-selected population must be suffering star formation which is erratic in its time history. In such a situation, different diagnostics wi ...
Galaxy clusters - University of Iowa Astrophysics
Galaxy clusters - University of Iowa Astrophysics

... • From this, the amount of X-ray emitting gas can be calculated to be 2×1014 M • The mass of X-ray emitting gas is greater than the mass in all the stars in all the galaxies in the cluster and about 10% of the total mass. ...
etlife_exoplanets - University of Glasgow
etlife_exoplanets - University of Glasgow

... We can tell that planets are there by the effect they have on their star. ...
2.1 Introduction
2.1 Introduction

... at the same time each year (or in practice if we correct for the effects of the Earth’s orbit around the Sun), we find that its position in a reference frame based on very distant objects such as quasars is not the same from year to year (see Figure 2.2). This is proper motion, reflecting the fact t ...
STAAR Science Tutorial 35 TEK 8.8B: The Sun
STAAR Science Tutorial 35 TEK 8.8B: The Sun

Astrophysics Outline—Option E
Astrophysics Outline—Option E

... E.3.10 Explain how stellar distance may be determined using apparent brightness and luminosity. E.3.11 State that the method of spectroscopic parallax is limited to measuring stellar distances less than about 10 Mpc. E.3.12 Solve problems involving stellar distances, apparent brightness and luminosi ...
Absolute Magnitudes of Supernovae
Absolute Magnitudes of Supernovae

... Summary Using the Hubble Law, determine the absolute magnitudes of Type Ia supernovae occurring in distant galaxies. Background - During a three-week period in 1997, the Hubble Space Telescope was used to observe a supernova - an exploding star in a distant galaxy. These exploding stars appear sudde ...
MIDTERM #1 AST209 - The Cosmos Feb 10, 2012 50 minutes
MIDTERM #1 AST209 - The Cosmos Feb 10, 2012 50 minutes

... A) radio, infrared, visible light, ultraviolet, X rays, gamma rays B) infrared, visible light, ultraviolet, X rays, gamma rays, radio C) radio, X rays, visible light, ultraviolet, infrared, gamma rays D) gamma rays, X rays, visible light, ultraviolet, infrared, radio E) visible light, infrared, X ra ...
Astronomy
Astronomy

Lecture 42
Lecture 42

... stars, of which the star T-Tauri (now known to be a binary pair) is the type example. During this phase, a visible star begins to emerge from its cocoon of gas and dust, but it remains surrounded by its circumstellar disk. The luminosity is due entirely to continued accretion and gravitational colla ...
• Constellations is a group of visible stars hat form a pattern when
• Constellations is a group of visible stars hat form a pattern when

Spectropolarimetric view of the lower atmosphere of
Spectropolarimetric view of the lower atmosphere of

... II - Sciences et techniques, IN2P3 – Université de Montpellier II Place Eugène Bataillon - CC 72 34095 Montpellier Cédex 05, France ...
Star Cycle2013
Star Cycle2013

... energy than you started with! So instead of generating pressure to hold up the outer layers, the iron fusion actually takes it out of the core. Thus, there is nothing left to combat gravity from the outer layers. ...
Sermon Notes
Sermon Notes

... Deceiver; Rakis – The Bound (the Arabic meaning is “Bound as with a chain”) Revelation 20:1 – 2 And I saw an angel come down from heaven, having the key of the bottomless pit and a great chain in his hand. And he laid hold on the dragon, that old serpent, which is the Devil, and Satan, and bound him ...
Topic Outline - Physics Rocks!
Topic Outline - Physics Rocks!

... E.3.11 State that the method of spectroscopic parallax is limited to measuring stellar distances ...
Issue 118 - Apr 2014
Issue 118 - Apr 2014

... [Editor's Note: The May 13 public meeting at the Florida Museum features Dr. Mario Motto as our guest speaker. A former president of the American Association of Variable Star Observers, Dr. Motto will talk about variable stars.] Variable stars are stars that change brightness. Some important types o ...
20 – N10/4/PHYSI/SP3/ENG/TZ0/XX Option E
20 – N10/4/PHYSI/SP3/ENG/TZ0/XX Option E

... (iii) State why the method of parallax can only be used for stars at a distance of less than a few hundred parsecs from Earth. ...
Astronomy
Astronomy

... C) It has hydrogen burning to helium D) It has helium burning to carbon and oxygen E) It has carbon and oxygen burning to heavier elements 29. How does the number of sunspots change over time? A) It rises and falls in an approximate eleven year cycle B) It rises and falls about every month at the r ...
Document
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... B) Measure the relative fraction of main sequence stars to dead stars, such as white dwarfs C) Make a Hertzsprung-Russell diagram for the cluster, and see where it “turns off” from the main sequence D) Measure the velocity of the stars and see how much the cluster has spread over time E) Measure the ...
MS Word
MS Word

... that B0 stars are the hottest and M9 stars are the coolest. Thus the left side of an H-R diagram is for the hottest stars while the right side is for the coolest. Now look at the other axis. This is absolute magnitude (denoted by a capital M). This is the brightness a star would have if it was 10 pa ...
Westerlund 1 : A Super-Star Cluster within the Milky Way
Westerlund 1 : A Super-Star Cluster within the Milky Way

constellation - Bucks-Mont Astronomical Association
constellation - Bucks-Mont Astronomical Association

... When you think about the new stars forming in the Milky Way, you probably think of the giant starforming regions like the Orion Nebula, containing thousands of new stars with light so bright it's visible to the naked eye. At over 400 parsecs (1,300 light years) distant, it's one of the most spectacu ...
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Perseus (constellation)



Perseus, named after the Greek mythological hero Perseus, is a constellation in the northern sky. It was one of 48 listed by the 2nd-century astronomer Ptolemy and among the 88 modern constellations defined by the International Astronomical Union (IAU). It is located in the northern celestial hemisphere near several other constellations named after legends surrounding Perseus, including Andromeda to the west and Cassiopeia to the north. Perseus is also bordered by Aries and Taurus to the south, Auriga to the east, Camelopardalis to the north, and Triangulum to the west.The galactic plane of the Milky Way passes through Perseus but is mostly obscured by molecular clouds. The constellation's brightest star is the yellow-white supergiant Alpha Persei (also called Mirfak), which shines at magnitude 1.79. It and many of the surrounding stars are members of an open cluster known as the Alpha Persei Cluster. The best-known star, however, is Algol (Beta Persei), linked with ominous legends because of its variability, which is noticeable to the naked eye. Rather than being an intrinsically variable star, it is an eclipsing binary. Other notable star systems in Perseus include X Persei, a binary system containing a neutron star, and GK Persei, a nova that peaked at magnitude 0.2 in 1901. The Double Cluster, comprising two open clusters quite near each other in the sky, was known to the ancient Chinese. The constellation gives its name to the Perseus Cluster (Abell 426), a massive galaxy cluster located 250 million light-years from Earth. It hosts the radiant of the annual Perseids meteor shower—one of the most prominent meteor showers in the sky.
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