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in the constellation Triangulum, is another member of the Local Group There are several smaller irregular and elliptical galaxies as well All the galaxies in our cluster appear tilted at different angles in space When we look far into space, we find galaxies in every direction Along the spiral plane of our own Milky Way, it is almost impossible to see exterior objects because of the interstellar gas and dust that obscure the view The farther out we look, the more galaxies we find This is to be expected because larger and larger spheres of observation must encompass more and more rapidly increasing volumes of space Strangely enough, though, the distribution of the galaxies in the Cosmos is not altogether uniform Clusters of galaxies are the rule rather than the exception Our Local Group is a comparatively small cluster There are clusters with hundreds or even thousands of individual galaxies Just as stars can vary greatly in their character and the galaxies can exist in many different and unique forms, so the clusters are found in differing shapes, sizes, and constitutions The galaxies in some clusters are so close together that they collide often on a Cosmic time scale measured in millions upon millions of Earth years After an encounter with another galaxy, a spiral can lose its arms because of the gravitational and electromagnetic (EM) disturbance Some such spirals become irregular and disorganized One of the most dense known clusters of galaxies is found in the direction of the constellation Coma Berenices Near the center of this rich cluster, any galaxy can be expected to collide with another member several times during its life What would it be like if our Milky Way were currently in a collision with another galaxy Such an event occurs over a period of millions of years However, we certainly would be able to tell if it were happening There would be two sources of radio noise, not just one, coming from the galactic core, and the noise level would be much greater than we currently observe If we had the opportunity to view the invading galaxy, its nucleus would be visible with the unaided eye as a diffuse, glowing mass of starlight Clusters of galaxies extend as far as we can see with optical telescopes: up to several billion light-years Such distances must be inferred indirectly; how this is done will be shown a little later in this chapter.

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Near the horizon in the east-southeast sky is a group of stars whose outline looks like the main sail on a sailboat This constellation is Capricornus (often called Capricorn), the goat (Fig 2-17) This goat has the tail of a fish, according to the myths, and dwells at sea On its way to heaven after the death of the body, the human soul was believed to pass through this constellation; it is 180 degrees opposite in the celestial sphere from Cancer, through which souls were believed to enter this world

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Site maps are used as a data source for navigation controls such TreeViews, Menus, and SiteMapPaths (which provide bread crumbs). Used in conjunction with master pages, these allow for easy and universal navigation without having to place navigation controls on every page of the web site. Add a site map to the current web site by clicking on Website Add New Item . When the Add New Item dialog appears, select Site Map and accept the default name, Web.sitemap, as shown in Figure 6-19.

In the east-southeast sky, to the right and slightly above Capricornus, you will see a constellation whose outline resembles a teapot (Fig 2-18) This is Sagittarius, the centaur What, you might ask, is a centaur You ought to know if you have read mythology or seen a lot of movies or television; it is a creature with the lower body of a horse and the chest, head, and arms of a human being The centaur carries a bow and arrow with which to stun evil or obnoxious creatures Sagittarius lies in the direction of the densest part of the Milky Way, the spiral galaxy in which our Solar System resides

SQL Developer has a schema capture mechanism that can capture the source database schemas, either directly by connecting to the source (online) or indirectly by the use of source database-specific capture scripts (offline) The online method will capture the schema by reading the data dictionary of the source database The offline method will effectively do the same thing and can be used when you do not have the privileges or the network access to connect to the source system SQL Developer can generate source-specific capture scripts, which can be shipped to the source system and executed using appropriate credentials The output generated by these scripts can be shipped back and loaded into the SQL Developer repository to create the source model SQL Developer has built-in reports that will display a summary of all the conversions it has performed, and it is able to do this by querying the migration repository These reports can be run at the end of the conversion process to evaluate if there were any fallouts or warnings during the conversion Also, at each step during the conversion, the fallouts and warnings will be displayed in the SQL Developer window This will help you monitor the progress of the conversion and make appropriate decisions when encountering issues SQL Developer has built-in intelligence to handle a few types of fallouts When it finds an object type on the source database that is not named exactly the same in Oracle but it functions similarly, it will translate it to the Oracle-equivalent object A good example of this is when you have DB2 snapshot views on the source DB2 database The equivalent of DB2 snapshot views in Oracle is Materialized Views, and SQL Developer will automatically convert DB2 snapshots to Materialized Views Oracle SQL Developer for Data Migration Oracle SQL Developer is capable of creating extract and load scripts that can be utilized to perform the initial data migration The scripts generated by SQL Developer will incorporate the source-specific utilities for performing extracts and the Oracle-specific utilities for performing the loads In the absence of SQL Developer support for the type of the source database or the version, the data extract scripts need to be created manually The time and effort to create the scripts need to be factored into the migration process, and for the most part, this will be proportional to the number of source database objects being migrated However, SQL Developer.

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