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Chapter 26.4
Chapter 26.4

... about 5 billion years. (It is approaching us at 670,000 mi/hr). Eventually they may merge to form an elliptical galaxy. Because stars are so far apart – it may have no affect … then again – we could get ejected out of our “place” on the Orion arm due to collision. ...
Star Types - College of Engineering and Computer Science
Star Types - College of Engineering and Computer Science

... They have a bigger radius than the stars of the same temperature which gives them a higher luminosity. ...
The Galactic Super Star Cluster Westerlund 1
The Galactic Super Star Cluster Westerlund 1

... Whereas we would expect ~10 -3 of the kinetic energy of winds and supernovae to be dissipated in X-rays,or ~10 36 erg s-1, the luminosity of the diffuse X-ray emission is only 6x10 34 erg s-1 (0.58.0 keV). This represents a factor of 10 deficit in diffuse X-ray emission. Moreover, the diffuse flux i ...
Day-6
Day-6

... associated with it. Nadir: The point directly under your feet, opposite the zenith Altitude: A measure of the height of an object from the ground up. It is measured perpendicular to the horizon. The horizon is 0° altitude. The Zenith is 90° altitude. Azimuth: The point along the horizon –measured ea ...
The Mighty Hunter in the Winter Sky By Shannon Jackson
The Mighty Hunter in the Winter Sky By Shannon Jackson

... Five constellations are always in our northern sky. Other groupings appear seasonally, and then disappear as they fall below the horizon. There are five constellations, however, which seem to circle Polaris (po LAR us), also known as the North Star. The North Star always stays put while the other st ...
Leaving the Main Sequence
Leaving the Main Sequence

... 3. Red giant – Core begins to run out of hydrogen fuel, begins to contract and heats. Remaining hydrogen burns faster in the shell around core and generates extra energy, disrupting hydrostatic equilibrium and causing outer regions to expand and cool. Star turns red. – Core (helium) becomes a degene ...
An introduction to the HR diagram File
An introduction to the HR diagram File

... • These high mass stars finish their lives in massive supernova explosions • At the bottom right the stars are cool. These low mass stars are very long lived as they use their fuel so slowly. Very low mass M stars live many billions of years and will simply run out of fuel without dramatic events. ...
Astronomy Merit Badge Workshop
Astronomy Merit Badge Workshop

... see in the night sky. Pick out 10 constellations (at least 4 of which are in the Zodiac) and note them below. Alternatively, do an internet search for constellations visible from your area at this time of year, pick out 10, and note them below. *Do an Internet search for “Star Finder” of “Planispher ...
Introduction to Astronomy - Northumberland Astronomical Society
Introduction to Astronomy - Northumberland Astronomical Society

... Position Horizon and equatorial coordinate systems. Distance Astronomical Unit (AU), light-years and parsecs. Brightness The magnitude scale. We’ll also examine how our location on the Earth affects the stars and constellations we can see and how changes in the tilt of the Earth’s axis change the vi ...
Chapter 13 The Life of a Star The Life of a Star Mass Is the Key The
Chapter 13 The Life of a Star The Life of a Star Mass Is the Key The

... supernova explosion sweeping up interstellar material as it goes is called a supernova remnant – During a 1-100 year time frame, a supernova will expand from 0.03 ly to several light-years in diameter – Supernova remnants have a more ragged look compared to planetary and other nebulae ...
Chapter 13
Chapter 13

... Supernovae • In a few minutes, more energy is released than during the star’s entire life • It brightens to several billion times the luminosity of the Sun – a luminosity larger than all the stars in the Milky Way combined ...
Stars - MrCrabtreesScience
Stars - MrCrabtreesScience

... How Far? • Parallax – The apparent movement of an object seen at different viewpoints. – The more the object moves (the greater the parallax), the closer it is. – The Hipparcos satellite ...
slides
slides

... Q: Which is larger? A. K-type main sequence star B. K-type giant C. they are about the same ...
Coherence of starlight The nearest star (other than
Coherence of starlight The nearest star (other than

... Coherence of starlight The nearest star (other than our sun) to us is Proxima Centauri at a distance of 30 trillion kilometers, and it has an angular diameter of 2 millionth of a degree or 7 milliarseconds (1 milliarcsecond is 1 thousandth of an arcsecond which is one sixtieth of an arcminute which ...
this PDF file - University of Leicester Open Journals
this PDF file - University of Leicester Open Journals

... had predicted was finally directly observed. The star is too faint to be seen without a powerful telescope. The bright star we can see is called Sirius A and the companion star predicted by Bessel is Sirius B – a white dwarf, so called due to its small size and white hot glow. The existence of this ...
The Hertzsprung-Russell Diagram
The Hertzsprung-Russell Diagram

... Equal Radius Lines In general the hotter the star is the brighter it will be. Thus you would expect stars of the same size but different temperatures to form a diagonal line called an equal radius line. Equal Radius lines can be added to an H-R diagram ...
Stellar Structure - McMurry University
Stellar Structure - McMurry University

... The white dwarf can ignite the new matter and flare up as a nova. The white dwarf can accrete too much matter and detonate as a supernova type Ia. Either the white dwarf can ignite the new matter and flare up as a nova, or the white dwarf can accrete too much matter and detonate as a supernova type ...
Proxima
Proxima

... Centaurus is a Centaur, they are half man-half horse! Centaurus faces east because he defending himself against Lupus the goat another constellation nearby!  Centaurus is known as a “myth” constellation.  It’s the 9th largest constellation in the sky  Proxima is the 3rd star in Centaurus  Cont ...
Photometric analysis of the globular cluster NGC5466
Photometric analysis of the globular cluster NGC5466

... Star clusters are collections of stars kept together by their gravitational force. We can distinguish between open clusters and globular clusters. Open clusters do not have a regular shape and have from few tens to 103 stars, losely bound to each others, which are spread in a very large space; there ...
December 2015
December 2015

... has five NGC objects including an open star cluster. It looks like a red Christmas poinsettia. Hubble’s Variable Nebula (NGC 2261) changes as clouds periodically block its illuminating star There was a supernova in 2002 that brightened a million times from magnitude 15 to 6 leaving a impressive shel ...
Matariki-Maori New Year
Matariki-Maori New Year

Chapter 5 Galaxies and Star Systems
Chapter 5 Galaxies and Star Systems

... universe. It's sad that there is so much light pollution in most cities that many people have never seen the Milky Way. On a clear night away from lights the view is of a bright white river of stars. You don't need a telescope or even binoculars to see it. The view of the Milky Way is so bright beca ...
The Naked Eye Era
The Naked Eye Era

... Hipparchus’s sky survey, as incorporated into the work of Ptolemy and Ulugh Beg, saw few major refinements until Tycho Brahe (1546–1601) decided to devote his career to astrometry—the precise measurement of star positions. Tycho was inspired by two celestial events early in his career; the appearanc ...
Star - Astrophysics
Star - Astrophysics

... into a degenerate gas and then leads to helium burning. But because the degeneracy pressure does not increase and lead to expansion as the core heats further, the energy production becomes even stronger producing a brief ‘helium flash’. Helium core burning and hydrogen shell burning then continue, a ...
The Milky Way – A Classic Galaxy
The Milky Way – A Classic Galaxy

... Sequence Fitting for those in star clusters. First and best example: bright open cluster M23 has a Cepheid. As of 1999, 29 more clusters now known to have Cepheids. • Cepheid PL relation has much less noise if brightnesses measured in the Infrared, which is what is always done these days. • By “Ceph ...
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Lyra



Lyra (/ˈlaɪərə/; Latin for lyre, from Greek λύρα) is a small constellation. It is one of 48 listed by the 2nd century astronomer Ptolemy, and is one of the 88 constellations recognized by the International Astronomical Union. Lyra was often represented on star maps as a vulture or an eagle carrying a lyre, and hence sometimes referred to as Aquila Cadens or Vultur Cadens. Beginning at the north, Lyra is bordered by Draco, Hercules, Vulpecula, and Cygnus. Lyra is visible from the northern hemisphere from spring through autumn, and nearly overhead, in temperate latitudes, during the summer months. From the southern hemisphere, it is visible low in the northern sky during the winter months.The lucida or brightest star—and one of the brightest stars in the sky—is the white main sequence star Vega, a corner of the Summer Triangle. Beta Lyrae is the prototype of a class of stars known as Beta Lyrae variables, binary stars so close to each other that they become egg-shaped and material flows from one to the other. Epsilon Lyrae, known informally as the Double Double, is a complex multiple star system. Lyra also hosts the Ring Nebula, the second-discovered and best-known planetary nebula.
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