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The radius that an object must attain in order to become a black hole is directly proportional to the mass From elementary solid geometry, you will recall that the volume of an object is proportional to the cube of the radius If an object s mass is doubled, the size of its Schwarzchild radius doubles too However, its volume becomes eight times as great This means that the more massive a black hole happens to be, the less dense it is In fact, the density of a black hole is inversely proportional to the square of its mass (Fig 15-4) Suppose that before there were any stars in the Universe, but only hydrogen and helium gas, vast clouds congealed because of gravitation Suppose that this took place on a much bigger scale than the process of star formation If such a cloud were large enough, it could become a black hole before it attained a density anywhere near enough to start nuclear fusion The black hole would continue to pull matter in, becoming larger still and yet less dense As the atoms approached the event horizon, they would be accelerated to nearly the speed of light This would give them tremendous kinetic energy, and the result would be an object of brilliance greater than that of

Set Home.aspx as the startup page by right-clicking on it in the Solution Explorer and selecting Set As Start Page from the menu. Run the web site now and see the TreeView menu in action. Click on any of the menu items along the left of the web site and observe how it navigates from page to page. If you click on the Stores menu item, it will look almost exactly like Figure 6-18. The only difference is the bread crumbs are missing because you have not yet placed that control on the page. Menu items that contain subitems of their own, such as Home and Sales, display a small icon next to them. Clicking on this icon toggles between expanded and collapsed views of these subitems. This structure directly flows from the nesting of SiteMapNodes in the site map file.

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Refer to the text if necessary A good score is 8 correct Answers are in the back of the book 1 Major asteroid impacts on the planets (a) have never occurred in our Solar System (b) take place only on Jupiter and Saturn (c) were once commonplace in the Solar System (d) produce new comets 2 A comet might be expected to suddenly become brighter if (a) all the icy material in the nucleus has evaporated (b) the tail passes through the corona of the Sun (c) a solar flare occurs (d) its perihelion takes it outside the orbit of the Earth 3 A spherical swarm of millions or billions of distant comets that surrounds the Solar System is known as the (a) Van Allen belt (b) Oort cloud (c) primeval Solar System disk (d) tektite belt 4 A small asteroid or massive meteoroid that crashes into the Moon can produce (a) a comet shower (b) a new comet (c) a crater with rays (d) an Oort cloud around the Moon 5 The dirty snowball model for the structures of comets is sometimes credited to (a) Fred Whipple (b) Giuseppe Piazzi (c) Johann E Bode (d) Johann D Titius

The source system s ASM diskgroups must be configured with normal or high redundancy Application impact can be controlled such that the rebalance happens with minimal impact This can be adjusted with the POWER clause of the rebalance operation Since ASM on Exadata needs to access the legacy storage, the legacy storage must be exposed to the Database Machine using NFS or iSCSI If moving from a previous version of the Database Machine, then you should connect the two machines using the InfiniBand Network or the 10 Gigabit Ethernet Although the migration itself will incur zero downtime, in reality, there will be a slight downtime incurred in order to switch the database and ASM instances from the non-Exadata platform to the Database Machine

The TreeView control has many properties, methods, and events, which allow you to customize the look and feel of the TreeView. The easiest way to change the appearance of the TreeView is to view the page in Design view, click the TreeView s Smart Tag, and then click Auto Format , as shown in Figure 6-22.

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