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Nebulae.The Lagoon and Dumbbell Nebulae
Nebulae.The Lagoon and Dumbbell Nebulae

... These layers expand in space, forming a temporary wrap around the star.). M27 Dumbbell is found by Charles Messier on the 12 of July 1764. He describes it as a nebula without a star that has oval shape. The name comes from John Herschel, an English astronomer, who observed the nebula in 1828 and com ...
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... Students should determine how this may or may not differ from how an astronomer might relate a certain temperature range and colors. Answer: An object acting like a blackbody radiator (like a star) will emit more light towards the blue end of the visible spectrum when at a higher temperature, and wi ...
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... molecules, and dust grains, which we call the interstellar medium (ISM). As quoted from D. Osterbrock (1984), “The interstellar medium is anything not in stars”. While this is true by definition, it disregards that the ISM and stars are intimately linked. Stellar feedback through ultraviolet (UV) ra ...
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... disrupted. Masses larger than 1.20 solar may remain acceptable if allowance is made for a faster evolution of complex life than was the case on Earth. Yet, besides these well-accepted notions, quite a few other considerations have recently been increasingly considered as playing fundamental roles fo ...
Process of Science: PreMainSequence Stellar Life Tracks on the HR
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... radioactive decay of unstable isotopes A newly forming star has no energy source, because it does not shine at all until it becomes a true main­sequence star. gravitational contraction nuclear fusion of hydrogen into helium ...
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... ____stars____ named after ____an animal____, ____a person____ or ___ an object ____. B. In modern astronomy, a constellation is defined as a specific ____area____ of the sky as determined by the International Astronomical Union (IAU). C. The celestial sphere is divided into __88___ contiguous region ...
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... Context. High-precision determinations of abundances of elements in the atmospheres of the Sun and solar twin stars indicate that the Sun has an unusual low ratio between refractory and volatile elements. This has led to the suggestion that the relation between abundance ratios, [X/Fe], and elementa ...
Chapter 17--Star Stuff
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... potassium ions moderate communications of the nervous system. What does all this biology have to do with astronomy? The profound answer, recognized only in the second half of the twentieth century, is that life is based on elements created by stars. We’ve already discussed in general terms how the e ...
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... generations of stars generated the elements that make up our planet and the chemical elements required for life. It is not an understatement to say that we exist because stars exist. The Observing Stellar Evolution Observing Program will be of interest to beginning observers as well as more experien ...
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... visible with good binoculars towards the constellation of Sagittarius. The energetic processes of star formation create not only the colors but the chaos. ...
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... simulations of elliptical galaxies, with an SPH code, by including the contribution from SN Ia and SN II, also accounting for stellar lifetimes. Valdarnini (2003) performed an extended set of cluster simulations and showed that profiles of the iron abundance are steeper than the observed ones. A sim ...
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... However, Laplace did not consider comets to be part of the Solar System as some travelled in highly eccentric orbits, and while they moved into the Sun’s domain they also moved far beyond the planetary sphere. ...
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... Knowing the age of a star is only the first step to understanding stellar evolution and completely describing how stars change with time. In short, different stars take different amounts of time to form, and to fully grasp the formation process, physical properties of the star must be determined. A ...
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Theoretical astronomy

Theoretical astronomy is the use of the analytical models of physics and chemistry to describe astronomical objects and astronomical phenomena.Ptolemy's Almagest, although a brilliant treatise on theoretical astronomy combined with a practical handbook for computation, nevertheless includes many compromises to reconcile discordant observations. Theoretical astronomy is usually assumed to have begun with Johannes Kepler (1571–1630), and Kepler's laws. It is co-equal with observation. The general history of astronomy deals with the history of the descriptive and theoretical astronomy of the Solar System, from the late sixteenth century to the end of the nineteenth century. The major categories of works on the history of modern astronomy include general histories, national and institutional histories, instrumentation, descriptive astronomy, theoretical astronomy, positional astronomy, and astrophysics. Astronomy was early to adopt computational techniques to model stellar and galactic formation and celestial mechanics. From the point of view of theoretical astronomy, not only must the mathematical expression be reasonably accurate but it should preferably exist in a form which is amenable to further mathematical analysis when used in specific problems. Most of theoretical astronomy uses Newtonian theory of gravitation, considering that the effects of general relativity are weak for most celestial objects. The obvious fact is that theoretical astronomy cannot (and does not try) to predict the position, size and temperature of every star in the heavens. Theoretical astronomy by and large has concentrated upon analyzing the apparently complex but periodic motions of celestial objects.
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