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href='http://www.blogger.com/comment.g?blogID=2526373410357936790&amp;postID=2560342805837536692' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/2526373410357936790/posts/default/2560342805837536692'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/2526373410357936790/posts/default/2560342805837536692'/><link rel='alternate' type='text/html' href='http://bejolly.blogspot.com/2007/07/get-freee-plasma-tv.html' title='Get freee plasma TV'/><author><name>online</name><uri>http://www.blogger.com/profile/02319735062177097136</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-2526373410357936790.post-7106271990791962858</id><published>2007-02-06T01:25:00.000-08:00</published><updated>2007-02-06T01:26:12.926-08:00</updated><title type='text'></title><content type='html'>&lt;h2&gt;&lt;span class="mw-headline"&gt;Beauty&lt;/span&gt;&lt;/h2&gt; &lt;div class="thumb tright"&gt; &lt;div class="thumbinner" style="width: 162px;"&gt;&lt;a href="http://en.wikipedia.org/wiki/Image:Salmonlarvakils.jpg" class="internal" title="Salmon fry hatching.  The root of the Latin   &amp;quot;natura&amp;quot; {&amp;quot;nature&amp;quot;) is &amp;quot;natus,&amp;quot; from &amp;quot;nasci&amp;quot; (&amp;quot;to be born&amp;quot;)."&gt;&lt;img src="http://upload.wikimedia.org/wikipedia/commons/thumb/e/e2/Salmonlarvakils.jpg/160px-Salmonlarvakils.jpg" alt="Salmon fry hatching.  The root of the Latin   &amp;quot;natura&amp;quot; {&amp;quot;nature&amp;quot;) is &amp;quot;natus,&amp;quot; from &amp;quot;nasci&amp;quot; (&amp;quot;to be born&amp;quot;)." longdesc="/wiki/Image:Salmonlarvakils.jpg" class="thumbimage" height="233" width="160" /&gt;&lt;/a&gt; &lt;div class="thumbcaption"&gt; &lt;div class="magnify" style="float: right;"&gt;&lt;a href="http://en.wikipedia.org/wiki/Image:Salmonlarvakils.jpg" class="internal" title="Enlarge"&gt;&lt;img src="http://en.wikipedia.org/skins-1.5/common/images/magnify-clip.png" alt="" height="11" width="15" /&gt;&lt;/a&gt;&lt;/div&gt; &lt;a href="http://en.wikipedia.org/wiki/Salmon" title="Salmon"&gt;Salmon&lt;/a&gt; &lt;a href="http://en.wikipedia.org/wiki/Fry" title="Fry"&gt;fry&lt;/a&gt; hatching. The root of the &lt;a href="http://en.wikipedia.org/wiki/Latin" title="Latin"&gt;Latin&lt;/a&gt; "&lt;i&gt;natura&lt;/i&gt;" {"nature") is "&lt;i&gt;natus&lt;/i&gt;," from "&lt;i&gt;nasci&lt;/i&gt;" ("to be born").&lt;sup id="_ref-54" class="reference"&gt;&lt;a href="http://en.wikipedia.org/wiki/Nature#_note-54" title=""&gt;[57]&lt;/a&gt;&lt;/sup&gt;&lt;/div&gt; &lt;/div&gt; &lt;/div&gt; &lt;p&gt;Beauty in nature is a common theme in modern life and in art, and books emphasizing beauty in nature fill large sections of libraries and bookstores. That nature has been depicted and celebrated by so much &lt;a href="http://en.wikipedia.org/wiki/Art" title="Art"&gt;art&lt;/a&gt;, &lt;a href="http://en.wikipedia.org/wiki/Photography" title="Photography"&gt;photography&lt;/a&gt;, &lt;a href="http://en.wikipedia.org/wiki/Poetry" title="Poetry"&gt;poetry&lt;/a&gt; and other literature shows the strength with which many people associate nature and beauty. Why this association exists, and what the association consists of, is studied by the branch of philosophy called &lt;a href="http://en.wikipedia.org/wiki/Aesthetics" title="Aesthetics"&gt;aesthetics&lt;/a&gt;. Beyond certain basic characteristics that many philosophers agree about to explain what is seen as beautiful, the opinions are virtually endless.&lt;span class="reference"&gt;&lt;sup id="ref_Fnone"&gt;&lt;a href="http://en.wikipedia.org/wiki/Nature#endnote_Fnone" title=""&gt;[f]&lt;/a&gt;&lt;/sup&gt;&lt;/span&gt;&lt;/p&gt; &lt;p&gt;Many scientists, who study nature in more specific and organized ways, also share the conviction that nature is beautiful; the French mathematician, &lt;a href="http://en.wikipedia.org/wiki/Henri_Poincar%C3%A9" title="Henri Poincaré"&gt;Jules Henri Poincaré&lt;/a&gt; (1854-1912) said:&lt;/p&gt; &lt;blockquote&gt; &lt;p&gt;The scientist does not study nature because it is useful; he studies it because he delights in it, and he delights in it because it is beautiful.&lt;br /&gt;If nature were not beautiful, it would not be worth knowing, and if nature were not worth knowing, life would not be worth living. Of course I do not here speak of that beauty which strikes the senses, the beauty of qualities and of appearance; not that I undervalue such beauty, far from it, but it has nothing to do with science; I mean that profounder beauty which comes from the harmonious order of the parts and which a pure intelligence can grasp.&lt;sup id="_ref-55" class="reference"&gt;&lt;a href="http://en.wikipedia.org/wiki/Nature#_note-55" title=""&gt;[58]&lt;/a&gt;&lt;/sup&gt;&lt;/p&gt; &lt;/blockquote&gt; &lt;p&gt;A common classical idea of beautiful art involves the word &lt;a href="http://en.wikipedia.org/wiki/Mimesis" title="Mimesis"&gt;mimesis&lt;/a&gt;, the imitation of nature. Also in the realm of ideas about beauty in nature is that the perfect is implied through symmetry, equal division, and other perfect mathematical &lt;a href="http://en.wikipedia.org/wiki/Forms" title="Forms"&gt;forms&lt;/a&gt; and notions.&lt;/p&gt; &lt;div class="thumb tleft"&gt; &lt;div class="thumbinner" style="width: 162px;"&gt;&lt;a href="http://en.wikipedia.org/wiki/Image:HAtomOrbitals.png" class="internal" title="The first few hydrogen atom electron orbitals shown as cross-sections with color-coded probability density"&gt;&lt;img src="http://upload.wikimedia.org/wikipedia/commons/thumb/c/cf/HAtomOrbitals.png/160px-HAtomOrbitals.png" alt="The first few hydrogen atom electron orbitals shown as cross-sections with color-coded probability density" longdesc="/wiki/Image:HAtomOrbitals.png" class="thumbimage" height="160" width="160" /&gt;&lt;/a&gt; &lt;div class="thumbcaption"&gt; &lt;div class="magnify" style="float: right;"&gt;&lt;a href="http://en.wikipedia.org/wiki/Image:HAtomOrbitals.png" class="internal" title="Enlarge"&gt;&lt;img src="http://en.wikipedia.org/skins-1.5/common/images/magnify-clip.png" alt="" height="11" width="15" /&gt;&lt;/a&gt;&lt;/div&gt; The first few &lt;a href="http://en.wikipedia.org/wiki/Hydrogen_atom" title="Hydrogen atom"&gt;hydrogen atom&lt;/a&gt; &lt;a href="http://en.wikipedia.org/wiki/Electron_orbital" title="Electron orbital"&gt;electron orbitals&lt;/a&gt; shown as cross-sections with color-coded probability density&lt;/div&gt; &lt;/div&gt; &lt;/div&gt; &lt;p&gt;&lt;a name="Matter_and_energy" id="Matter_and_energy"&gt;&lt;/a&gt;&lt;/p&gt; &lt;h2&gt;&lt;span class="editsection"&gt;&lt;a href="http://en.wikipedia.org/w/index.php?title=Nature&amp;action=edit&amp;amp;section=12" title="Edit section: Matter and energy"&gt;&lt;/a&gt;&lt;/span&gt; &lt;span class="mw-headline"&gt;Matter and energy&lt;/span&gt;&lt;/h2&gt; &lt;dl&gt;&lt;dd&gt; &lt;div class="noprint"&gt;&lt;i&gt;Main articles: &lt;a href="http://en.wikipedia.org/wiki/Matter" title="Matter"&gt;Matter&lt;/a&gt; and &lt;a href="http://en.wikipedia.org/wiki/Energy" title="Energy"&gt;Energy&lt;/a&gt;&lt;/i&gt;&lt;/div&gt; &lt;/dd&gt;&lt;/dl&gt; &lt;p&gt;Some fields of &lt;a href="http://en.wikipedia.org/wiki/Science" title="Science"&gt;science&lt;/a&gt; see nature as matter in motion, obeying certain laws of nature which science seeks to understand. For this reason the most fundamental science is generally understood to be "&lt;a href="http://en.wikipedia.org/wiki/Physics" title="Physics"&gt;physics&lt;/a&gt;"—the name for which is still recognizable as meaning that it is the study of nature.&lt;/p&gt; &lt;p&gt;Matter is commonly defined as the substance of which physical objects are composed. It constitutes the &lt;a href="http://en.wikipedia.org/wiki/Observable_universe" title="Observable universe"&gt;observable universe&lt;/a&gt;. According to the theory of &lt;a href="http://en.wikipedia.org/wiki/Special_relativity" title="Special relativity"&gt;special relativity&lt;/a&gt;, there is no unchangeable distinction between matter and &lt;a href="http://en.wikipedia.org/wiki/Energy" title="Energy"&gt;energy&lt;/a&gt;, because matter can be converted to energy (see &lt;a href="http://en.wikipedia.org/wiki/Annihilation" title="Annihilation"&gt;annihilation&lt;/a&gt;), and vice versa (see &lt;a href="http://en.wikipedia.org/wiki/Matter_creation" title="Matter creation"&gt;matter creation&lt;/a&gt;). The visible components of the universe are now believed to compose only 4 percent of the total mass. The remainder is believed to consist of 23 percent cold &lt;a href="http://en.wikipedia.org/wiki/Dark_matter" title="Dark matter"&gt;dark matter&lt;/a&gt; and 73 percent &lt;a href="http://en.wikipedia.org/wiki/Dark_energy" title="Dark energy"&gt;dark energy&lt;/a&gt;.&lt;sup id="_ref-56" class="reference"&gt;&lt;a href="http://en.wikipedia.org/wiki/Nature#_note-56" title=""&gt;[59]&lt;/a&gt;&lt;/sup&gt; The exact nature of these components is still unknown and is currently under intensive investigation by physicists.&lt;/p&gt; &lt;p&gt;The behavior of matter and energy throughout the &lt;a href="http://en.wikipedia.org/wiki/Observable_universe" title="Observable universe"&gt;observable universe&lt;/a&gt; appears to follow well-defined &lt;a href="http://en.wikipedia.org/wiki/Physical_law" title="Physical law"&gt;physical laws&lt;/a&gt;. These laws have been employed to produce &lt;a href="http://en.wikipedia.org/wiki/Physical_cosmology" title="Physical cosmology"&gt;cosmological&lt;/a&gt; models that successfully explain the structure and the evolution of the universe we can observe. The mathematical expressions of the laws of physics employ a set of twenty &lt;a href="http://en.wikipedia.org/wiki/Physical_constant" title="Physical constant"&gt;physical constants&lt;/a&gt;&lt;sup id="_ref-57" class="reference"&gt;&lt;a href="http://en.wikipedia.org/wiki/Nature#_note-57" title=""&gt;[60]&lt;/a&gt;&lt;/sup&gt; that appear to be static across the observable universe.&lt;sup id="_ref-58" class="reference"&gt;&lt;a href="http://en.wikipedia.org/wiki/Nature#_note-58" title=""&gt;[61]&lt;/a&gt;&lt;/sup&gt; The values of these constants have been carefully measured, but the reason for their specific values remains a mystery.&lt;/p&gt; &lt;dl&gt;&lt;dd&gt;&lt;span class="boilerplate seealso"&gt;&lt;i&gt;See also: &lt;a href="http://en.wikipedia.org/wiki/Chemistry" title="Chemistry"&gt;Chemistry&lt;/a&gt; and &lt;a href="http://en.wikipedia.org/wiki/Physics" title="Physics"&gt;Physics&lt;/a&gt;&lt;/i&gt;&lt;/span&gt;&lt;/dd&gt;&lt;/dl&gt; &lt;p&gt;&lt;a name="Nature_beyond_Earth" id="Nature_beyond_Earth"&gt;&lt;/a&gt;&lt;/p&gt; &lt;h2&gt;&lt;span class="editsection"&gt;&lt;/span&gt; &lt;span class="mw-headline"&gt;Nature beyond Earth&lt;/span&gt;&lt;/h2&gt; &lt;dl&gt;&lt;dd&gt; &lt;div class="noprint"&gt;&lt;i&gt;Main articles: &lt;a href="http://en.wikipedia.org/wiki/Outer_space" title="Outer space"&gt;Outer space&lt;/a&gt; and &lt;a href="http://en.wikipedia.org/wiki/Universe" title="Universe"&gt;Universe&lt;/a&gt;&lt;/i&gt;&lt;/div&gt; &lt;/dd&gt;&lt;/dl&gt; &lt;div class="thumb tright"&gt; &lt;div class="thumbinner" style="width: 282px;"&gt;&lt;a href="http://en.wikipedia.org/wiki/Image:NGC_4414_%28NASA-med%29.jpg" class="internal" title="NGC 4414, a typical spiral galaxy in the constellation Coma Berenices, is about 56,000 light years in diameter and approximately 60 million light years distant."&gt;&lt;img src="http://upload.wikimedia.org/wikipedia/commons/thumb/c/c3/NGC_4414_%28NASA-med%29.jpg/280px-NGC_4414_%28NASA-med%29.jpg" alt="NGC 4414, a typical spiral galaxy in the constellation Coma Berenices, is about 56,000 light years in diameter and approximately 60 million light years distant." longdesc="/wiki/Image:NGC_4414_%28NASA-med%29.jpg" class="thumbimage" height="231" width="280" /&gt;&lt;/a&gt; &lt;div class="thumbcaption"&gt; &lt;div class="magnify" style="float: right;"&gt;&lt;a href="http://en.wikipedia.org/wiki/Image:NGC_4414_%28NASA-med%29.jpg" class="internal" title="Enlarge"&gt;&lt;img src="http://en.wikipedia.org/skins-1.5/common/images/magnify-clip.png" alt="" height="11" width="15" /&gt;&lt;/a&gt;&lt;/div&gt; &lt;b&gt;&lt;a href="http://en.wikipedia.org/wiki/NGC_4414" title="NGC 4414"&gt;NGC 4414&lt;/a&gt;&lt;/b&gt;, a typical spiral galaxy in the constellation &lt;a href="http://en.wikipedia.org/wiki/Coma_Berenices" title="Coma Berenices"&gt;Coma Berenices&lt;/a&gt;, is about 56,000 light years in diameter and approximately 60 million light years distant.&lt;/div&gt; &lt;/div&gt; &lt;/div&gt; &lt;div class="thumb tright"&gt; &lt;div class="thumbinner" style="width: 282px;"&gt;&lt;a href="http://en.wikipedia.org/wiki/Image:Universe.jpg" class="internal" title="The deepest visible-light image of the universe, the Hubble Ultra Deep Field. Image Credit: NASA, ESA, S. Beckwith (STScI) and the HUDF team."&gt;&lt;img src="http://upload.wikimedia.org/wikipedia/commons/thumb/6/61/Universe.jpg/280px-Universe.jpg" alt="The deepest visible-light image of the universe, the Hubble Ultra Deep Field. Image Credit: NASA, ESA, S. Beckwith (STScI) and the HUDF team." longdesc="/wiki/Image:Universe.jpg" class="thumbimage" height="279" width="280" /&gt;&lt;/a&gt; &lt;div class="thumbcaption"&gt; &lt;div class="magnify" style="float: right;"&gt;&lt;a href="http://en.wikipedia.org/wiki/Image:Universe.jpg" class="internal" title="Enlarge"&gt;&lt;img src="http://en.wikipedia.org/skins-1.5/common/images/magnify-clip.png" alt="" height="11" width="15" /&gt;&lt;/a&gt;&lt;/div&gt; The deepest visible-light image of the &lt;a href="http://en.wikipedia.org/wiki/Universe" title="Universe"&gt;universe&lt;/a&gt;, the &lt;a href="http://en.wikipedia.org/wiki/Hubble_Ultra_Deep_Field" title="Hubble Ultra Deep Field"&gt;Hubble Ultra Deep Field&lt;/a&gt;. Image Credit: NASA, ESA, S. Beckwith (STScI) and the HUDF team.&lt;/div&gt; &lt;/div&gt; &lt;/div&gt; &lt;p&gt;&lt;b&gt;Outer space&lt;/b&gt;, also simply called &lt;i&gt;space&lt;/i&gt;, refers to the relatively empty regions of the &lt;a href="http://en.wikipedia.org/wiki/Universe" title="Universe"&gt;universe&lt;/a&gt; outside the &lt;a href="http://en.wikipedia.org/wiki/Celestial_body%27s_atmosphere" title="Celestial body's atmosphere"&gt;atmospheres&lt;/a&gt; of celestial bodies. &lt;i&gt;Outer&lt;/i&gt; space is used to distinguish it from &lt;a href="http://en.wikipedia.org/wiki/Airspace" title="Airspace"&gt;airspace&lt;/a&gt; (and terrestrial locations). There is no discrete boundary between the &lt;a href="http://en.wikipedia.org/wiki/Earth%27s_atmosphere" title="Earth's atmosphere"&gt;Earth's atmosphere&lt;/a&gt; and space, as the atmosphere gradually attenuates with increasing altitude. Outer space within the &lt;a href="http://en.wikipedia.org/wiki/Solar_system" title="Solar system"&gt;solar system&lt;/a&gt; is called &lt;a href="http://en.wikipedia.org/wiki/Interplanetary_space" title="Interplanetary space"&gt;interplanetary space&lt;/a&gt;, which passes over into &lt;a href="http://en.wikipedia.org/wiki/Interstellar_medium" title="Interstellar medium"&gt;interstellar space&lt;/a&gt; at what is known as the &lt;a href="http://en.wikipedia.org/wiki/Heliopause" title="Heliopause"&gt;heliopause&lt;/a&gt;.&lt;sup id="_ref-59" class="reference"&gt;&lt;a href="http://en.wikipedia.org/wiki/Nature#_note-59" title=""&gt;[62]&lt;/a&gt;&lt;/sup&gt;&lt;/p&gt;&lt;div class="blogger-post-footer"&gt;&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/2526373410357936790-7106271990791962858?l=bejolly.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://bejolly.blogspot.com/feeds/7106271990791962858/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=2526373410357936790&amp;postID=7106271990791962858' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/2526373410357936790/posts/default/7106271990791962858'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/2526373410357936790/posts/default/7106271990791962858'/><link rel='alternate' type='text/html' href='http://bejolly.blogspot.com/2007/02/beauty-salmon-fry-hatching.html' title=''/><author><name>online</name><uri>http://www.blogger.com/profile/02319735062177097136</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry></feed>
