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Copyright 1995 Scientific American, Inc.
Copyright 1995 Scientific American, Inc.

... of them undergoes a supernoof Relativity. va explosion. The pair then Although this theory is acbecomes a massive x-ray bicepted today as the only vinary, so named for the emisable description of gravity, it sion that the neutron star has had only a few direct tests. produces as it strips the outer ...
TISHTRIYA - Earth`s second Sun
TISHTRIYA - Earth`s second Sun

... Although, to the naked eye, it looks like one Star it is composed of two Stars. In different research data there seems to be a wide inconsistency in the description of the size and brightness of each of the two stars. The larger and brighter of the two, Sirius A, averages 2-3 times the mass of our s ...
DSLR Photometry
DSLR Photometry

... Des says in theory it is advisable to also construct master flat field frames in order to remove the effects of the edge distortions of lens. Des has found, however, that the field of view of a DSLR is so wide that a flat field is not required, if you are using high quality lenses, provided the targ ...
Solar System Formation
Solar System Formation

... 756 sources corresponding to stars 504 dwarfs or subgiants 267 have 12 and 25 micron fluxes 36 have 12, 25, and 60 micron fluxes 12 are “Vega-like” with significant 60 micron fluxes 14% of A-type stars (N = 6) 3% of F-type stars (N = 4) < 1% of G/K-type stars (N = 2) detecting protostellar disks or ...
colour
colour

... . pressure → surface gravity → luminosity class . stellar rotation: in rapidly rotating stars, spectral lines are Doppler broadened by rotation . orbital velocities (due to periodic Doppler shifts) in binaries ...
STELLAR STRUCTURE AND EVOLUTION
STELLAR STRUCTURE AND EVOLUTION

... . pressure → surface gravity → luminosity class . stellar rotation: in rapidly rotating stars, spectral lines are Doppler broadened by rotation . orbital velocities (due to periodic Doppler shifts) in binaries ...
Globular Clusters - Lick Observatory
Globular Clusters - Lick Observatory

... Credited to: Scott Seagroves ...
Distances and Sizes - University of Iowa Astrophysics
Distances and Sizes - University of Iowa Astrophysics

... – from cosmic background radiation 1.41010 light years (1965) ...
Lect15-3-23-11-stars..
Lect15-3-23-11-stars..

... 2. Second, as the gas cloud continues to collapse, radiating into space essentially all of the heat generated from gravitational potential energy release, its surface temperature warms only slightly. However, as the collapse proceeds, the surface area of the cloud is diminished,, so that its luminos ...
Summary: Star Formation Near and Far
Summary: Star Formation Near and Far

... an accretion flow, but more work is needed to demonstrate this. What about the possibility of continuing fragmentation? In principle, one could imagine that a collapsing clump might fragment hierarchically into smaller and smaller objects until fragmentation is stopped by the increase of opacity at ...
Solutions
Solutions

... globular cluster, e.g. such as is found in Figure 16.17 in your text (and perhaps comparing that with the “cluster snapshot” diagrams on the previous page). (a) Because the red giant stars are the most luminous stars in globular clusters. Just as the stars we see most easily in the night sky with ou ...
Stellarium01 Starter Part A B Doc - ASTR101
Stellarium01 Starter Part A B Doc - ASTR101

... permanently located at a certain spot in the sky, in a particular constellation. There are many catalogs of Deep Sky Objects, most of which were published in the 18th or 19th centuries, including the NGC catalog (the New General Catalog), the Messier catalog (or the M Catalog named after French astr ...
Link again
Link again

... asteroid belt (the region between Mars and Jupiter). Chunks of ice called “comets” can be found in orbits beyond Pluto. Some comets have weird orbits that bring them close to the Earth or to the Sun and other planets. When they get close to the Sun, its heat turns some of the comet’s ice to vapor. T ...
Astronomy
Astronomy

... asteroid belt (the region between Mars and Jupiter). Chunks of ice called “comets” can be found in orbits beyond Pluto. Some comets have weird orbits that bring them close to the Earth or to the Sun and other planets. When they get close to the Sun, its heat turns some of the comet’s ice to vapor. T ...
Orion – The Hunter - Guild of Students
Orion – The Hunter - Guild of Students

... built to mirror the three stars of Orion's belt. Osiris was born in Thebes in Upper Egypt, the heavenly mirror-world that the Egyptians believed existed in the sky, to Nut and Geb. His grandfather Ra made him heir to the throne and so when his father Geb retired he took over as the fourth divine pha ...
Globular Clusters
Globular Clusters

... Way is low or even below the horizon in the Northern Hemisphere, so only a few bright globular clusters are easily visible from there, and the best ones often cannot be seen at all. Here in the southern hemisphere, the galactic centre is high in the winter sky, and we have a good view of all but 2 o ...
Document
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... winds heat and compress the disk causing agglomeration out to the snow line. The cores grow by collecting material infalling toward the star. They are in unstable orbits that can change radically or they can be ejected from the system. A core in a highly eccentric orbit that goes far into the disk c ...
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Document

... stellar remnants such as white dwarfs, neutron stars, black holes Students will learn the different types of supernovae observed and the physical theories of their production. ...
MSci Astrophysics 210PHY412
MSci Astrophysics 210PHY412

... stellar remnants such as white dwarfs, neutron stars, black holes Students will learn the different types of supernovae observed and the physical theories of their production. ...
There are 88 constellations in the sky around the Earth. 12 are the
There are 88 constellations in the sky around the Earth. 12 are the

Is there life outside of Earth? Activity 2: Moving Stars and Their Planets
Is there life outside of Earth? Activity 2: Moving Stars and Their Planets

... Q. Place a snapshot here of the first solution to the challenge above. A. Student answers will vary. The graph should look similar to the challenge graph. Q. Place a snapshot here of your solution to the challenge above. A. Student answers will vary. The graph should look similar to the challenge gr ...
PRESS 2001 Project Report - Hong Kong University of Science and
PRESS 2001 Project Report - Hong Kong University of Science and

white dwarfs, neutron stars, black hole
white dwarfs, neutron stars, black hole

... very big red giant), the core begins to yield to gravity and starts to shrink. As it shrinks, it grows hotter and denser, and a new series of nuclear reactions begin to occur, temporarily halting the collapse of the core. However, when the core becomes essentially just iron, it has nothing left to f ...
Lesson Plan G2 The Stars
Lesson Plan G2 The Stars

... good indicator of its distance. In Starry Night they will examine several different stars and they will see how some stars end their lives. ...
Article PDF - IOPscience
Article PDF - IOPscience

... RR Lyrae stars may be the best practical tracers of Galactic halo (sub-)structure and kinematics. The PanSTARRS1 (PS1) 3p survey offers multi-band, multi-epoch, precise photometry across much of the sky, but a robust identification of RR Lyrae stars in this data set poses a challenge, given PS1ʼs spa ...
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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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