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Astronomers have deduced certain things about the interiors of stars, including the Sun, just as they have been able to gather ideas about the interiors of the planets, including the Earth Different types of stars have different internal structures We also know that different types of stars have much different atmospheres The atmosphere surrounding a star can extend outward for millions of kilometers and is called the corona Computers have been used to construct model stars using programs that simulate events believed to take place in the depths of these fusion furnaces Known physical laws are applied to denote what happens inside a star with a given mass and material composition Stars are considered to have concentric layers or shells, each with a certain temperature, mass, and combination of elements The whole star is constructed by putting the shells together This can be done outward from the center toward the surface and then to the corona or inward from the corona to the surface and ultimately to the center Sometimes, when the two modeling schemes (inside-out versus outside-in) are both applied to objects having the same mass and material composition, the results are different In the depths of a large main-sequence star such as a blue supergiant, radiation and convection are believed to be mutually responsible for the transfer of energy from the core of the star into space Near the surface, radiation predominates Near the center, convection is thought to play a more important role because the matter deep inside stars is so dense that it is opaque to radiation This model of a large star is shown in Fig 13-5a In a much less massive main-sequence star, the reverse is believed to be the case A red-dwarf star apparently has a convective outer region and a more transparent core Radiation should predominate deep inside such a star This model of a red dwarf is shown in Fig 13-5b Both these models are largely speculative Computers can work only with the data that they get, and these data are based on educated guesswork Nature is not a computer program We can t be sure that the models we invent are perfect representations of what really goes on in the Universe In fact,.

Although this approach may not limit your ability to properly predict the extent of consolidation on a Database Machine, it has the advantage of a greater likelihood of ongoing success and happier users

Some meteorites cause fractures in the surface of the object on which they land These fractures can take the form of concentric rings around the

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It is the same as if you had coded HTML with inline styles, which is, in fact what ASP.NET sends to the browser based on the ASP.NET controls and their properties. You can also set or change style properties programmatically (as you can any control property). To see this, close the browser, then drag a Button control from the Standard section of the Toolbox onto the page. Using an If-Then-Else statement, change its Text property to toggle between two colors. Double-click the Button in Design view to open up the event handler for the Click event. Enter the highlighted code from Example 6-1.

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crater Jupiter s moon Callisto has a crater with these features In other cases, there is no particular pattern to the fracture lines; the surface apparently cracks along the weakest points in the crust Sometimes the fractures cover the whole surface of the object They can occur as canyons or as escarpments (cliffs) The impact of an especially massive meteorite or a small asteroid can produce volcanic activity all over the object it strikes, provided that there is hot lava inside the object that can rise up through the crust The maria, or seas, of the Moon are believed to have formed when lava from the interior spread

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over the surface following one or more violent meteorite landings The same thing is thought to have taken place on the Earth from time to time, but the features have been modified by weather erosion and by the constant shifting of the tectonic plates in the Earth s crust In the extreme, a catastrophic impact can shatter a moon or planet Nothing of this sort is thought to have taken place on any of the known planets or moons in the recent past, but in the early evolution of the Solar System, such events were commonplace Going all the way back to the formation of the Sun and planets from the rotating disk of gas and dust 46 billion years ago, major collisions were the rule and not the exception The ultimate longterm effect of meteorite landings is a sweeping up of space debris into major objects Thus, as time passes, catastrophes become less and less frequent

Protected Sub Button1_Click(ByVal sender As Object, _ ByVal e As System.EventArgs) Handles Button1.Click If TextBox1.ForeColor = Drawing.Color.Red Then TextBox1.ForeColor = Drawing.Color.Green Else TextBox1.ForeColor = Drawing.Color.Red End If End Sub

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