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author | toma <toma@283d02a7-25f6-0310-bc7c-ecb5cbfe19da> | 2009-11-25 17:56:58 +0000 |
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committer | toma <toma@283d02a7-25f6-0310-bc7c-ecb5cbfe19da> | 2009-11-25 17:56:58 +0000 |
commit | ce599e4f9f94b4eb00c1b5edb85bce5431ab3df2 (patch) | |
tree | d3bb9f5d25a2dc09ca81adecf39621d871534297 /doc/kstars/spiralgalaxies.docbook | |
download | tdeedu-ce599e4f9f94b4eb00c1b5edb85bce5431ab3df2.tar.gz tdeedu-ce599e4f9f94b4eb00c1b5edb85bce5431ab3df2.zip |
Copy the KDE 3.5 branch to branches/trinity for new KDE 3.5 features.
BUG:215923
git-svn-id: svn://anonsvn.kde.org/home/kde/branches/trinity/kdeedu@1054174 283d02a7-25f6-0310-bc7c-ecb5cbfe19da
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diff --git a/doc/kstars/spiralgalaxies.docbook b/doc/kstars/spiralgalaxies.docbook new file mode 100644 index 00000000..01bcf1a8 --- /dev/null +++ b/doc/kstars/spiralgalaxies.docbook @@ -0,0 +1,91 @@ +<sect1 id="ai-spiralgal"> + +<sect1info> +<author> +<firstname>Mike</firstname> +<surname>Choatie</surname> +</author> +</sect1info> + +<title>Spiral Galaxies</title> +<indexterm><primary>Spiral Galaxies</primary> +</indexterm> + +<para> +Spiral galaxies are huge collections of billions of stars, most of +which are flattened into a disk shape, with a bright, spherical bulge +of stars at its center. Within the disk, there are +typically bright arms where the youngest, brightest stars are +found. These arms wind out from the center in a spiral pattern, giving +the galaxies their name. Spiral galaxies look a bit like hurricanes, +or like water flowing down a drain. They are some of the most beautiful +objects in the sky. +</para> +<para> +Galaxies are classified using a <quote>tuning fork diagram</quote>. +The end of the fork classifies <link linkend="ai-ellipgal">elliptical +galaxies</link> on a scale from the roundest, which is an E0, to +those that appear most flattened, which is rated as E7. The +<quote>tines</quote> of the tuning fork are where the two types of +spiral galaxies are classified: normal spirals, and +<quote>barred</quote> spirals. A barred spiral is one whose nuclear +bulge is stretched out into a line, so it literally looks like it has +a <quote>bar</quote> of stars in its center. +</para><para> +Both types of spiral galaxies are sub-classified according to the +prominence of their central <quote>bulge</quote> of stars, their overall +surface brightness, and how tightly their spiral arms are wound. These +characteristics are related, so that an Sa galaxy has a large central bulge, +a high surface brightness, and tightly-wound spiral arms. An Sb galaxy +has a smaller bulge, a dimmer disk, and looser arms than an Sa, and so on +through Sc and Sd. Barred galaxies use the same classification scheme, +indicated by types SBa, SBb, SBc, and SBd. +</para><para> +There is another class of galaxy called S0, which is morphologically a +transitional type between true spirals and ellipticals. Its spiral arms are +so tightly wound as to be indistinguishable; S0 galaxies have disks with a +uniform brightness. They also have an extremely dominant bulge. +</para><para> +The Milky Way galaxy, which is home to earth and all of the stars in our +sky, is a Spiral Galaxy, and is believed to be a barred spiral. The name +<quote>Milky Way</quote> refers to a band of very faint stars in the sky. +This band is the result of looking in the plane of our galaxy's disk from +our perspective inside it. +</para><para> +Spiral galaxies are very dynamic entities. They are hotbeds of star +formation, and contain many young stars in their disks. Their central +bulges tend to be made of older stars, and their diffuse halos are +made of the very oldest stars in the Universe. Star formation is active +in the disks because that is where the gas and dust are most concentrated; +gas and dust are the building blocks of star formation. +</para><para> +Modern telescopes have revealed that many Spiral galaxies harbor +supermassive black holes at their centers, with masses that can exceed +that of a billion Suns. Both elliptical and spiral galaxies are known +to contain these exotic objects; in fact many astronomers now believe +that <emphasis>all</emphasis> large galaxies contain a supermassive +black hole in their nucleus. Our own Milky Way is known to harbor +a black hole in its core with a mass millions of times bigger than a +star's mass. +</para> + +<tip> +<para> +There are many fine examples of spiral galaxies to be found in +&kstars;, and many have beautiful images available in their +<link linkend="popup-menu">popup menu</link>. You can find them +by using the <link linkend="findobjects">Find Object</link> window. +Here is a list of some spiral galaxies with nice images available: +<itemizedlist> +<listitem><para>M 64, the Black-Eye Galaxy (type Sa)</para></listitem> +<listitem><para>M 31, the Andromeda Galaxy (type Sb)</para></listitem> +<listitem><para>M 81, Bode's Galaxy (type Sb)</para></listitem> +<listitem><para>M 51, the Whirlpool Galaxy (type Sc)</para></listitem> +<listitem><para>NGC 300 (type Sd) [use DSS image link]</para></listitem> +<listitem><para>M 83 (type SBa)</para></listitem> +<listitem><para>NGC 1530 (type SBb)</para></listitem> +<listitem><para>NGC 1073 (type SBc)</para></listitem> +</itemizedlist> +</para> +</tip> +</sect1> |