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at Harvard University named Annie Cannon compiled a record of the spectra of nearly half a million stars This became known as the Henry Draper Catalogue There are seven main categories of stars, classified according to the type of spectrum they have The main categories have been given the names O, B, A, F, G, K, and M Each of these seven classes is divided into subcategories from 0 through 9 Thus a type A9 star is followed by a type F0 star, which is followed by F1, F2, F3, and so on In all, there are 70 different spectral types of stars What do these letters and numbers actually mean It turns out that the spectrum of a star tells us the surface temperature Type O stars are the hottest and appear bluish to the eye Type M stars have the lowest surface temperatures, and they appear orange or ruddy Within a particular alphabetic subdivision, the number 0 represents the highest temperature, and the number 9 represents the lowest The hottest possible star would be symbolized O0 (the letter O followed by the numeral 0); the

Where you want to consolidate two significantly different I/O-intensive database instances onto the same physical storage cell, you can leverage an interdatabase plan on the Oracle Exadata Database Machine storage cells directly In this example, you can consider an OLTP database instance that is highly sensitive to the latency of physical I/O requests You will also consider a data warehousing database instance called DW that issues larger I/O requests but is more sensitive to throughput In order to consolidate these two very different databases onto the same physical Oracle Exadata Database Machine storage cell, you must be able to prevent the DW from slowing down the OLTP database, yet allow the DW to open up on the storage cells when the OLTP database is no longer performing physical I/Os (because it is being satisfied from main memory or from the secondary flash memory area) Directly activating an interdatabase plan on the storage cells themselves will provide a solution to this common historic problem

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coolest would be M9 On this scale, our Sun is a type G2 star This means that it is medium cool Of course, hot and cool are relative terms; even an M9 star is scorching hot by Earthly standards The surface temperature of a star is related to its absolute visual magnitude This relationship was found in the early 1900s by a Danish astronomer named Ejnar Hertzsprung and an American named Henry Russell These two scientists, working independently, graphed the absolute magnitudes of some nearby stars as a function of spectral classification They found that, in general, as the surface temperature increases, so does the absolute brightness This is not surprising, but it does not tell the whole story Temperature is not the only variable in star classification Size matters too Our Sun is a rather small star The largest stars are called giants The smallest are called dwarfs Some relatively cool stars are bright because they are huge: the red giants Some hot stars are dim because they are tiny: the white dwarfs

CellCLI> ALTER IORMPLAN dbPlan=( (name=OLTP,level=1,allocation=80), (name=DW,level=2,allocation=80), (name=other,level=3,allocation=100))

When the spectral type of a star is graphed along with its absolute magnitude, the star is represented by a single point on a coordinate plane Figure 13-3 shows what Hertzsprung and Russell found Such graphs are used by astronomers to this day and are called, appropriately enough, HertzsprungRussell (H-R) diagrams On the horizontal axis, the highest temperature is toward the left, and the coolest is toward the right On the vertical axis, the brightest absolute visual magnitude is toward the top, and the dimmest is toward the bottom Our Sun is shown by the large dot Stars denoted in the upper right part of the H-R diagram are red giants Blue giants are in the upper left corner, at the top of the main sequence The smallest and coolest stars, the red and orange dwarfs, are at the lower right end of the main sequence White dwarfs appear at the bottom and are not on the main sequence There are also supergiants that do not fall onto the main sequence; these are shown at the top middle So what exactly is this main sequence As Hertzsprung and Russell plotted their diagrams, they noticed an interesting correlation Most stars fall along a curve running diagonally from the upper left to the lower right This became known as the main sequence because it contains the majority of stars When astronomers began investigating the relationship between the location of a star in the galaxy and its position on the H-R diagram, some fascinating discoveries were made Hot, massive stars seem to be concentrated

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