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<title>Lovely English</title>
<link>http://lovelyenglish.blogfa.com/</link>
<description>Those who know nothing of foreign languages,  know noting of their own</description>
<language>fa</language>
<generator>blogfa.com</generator>
<lastBuildDate>Fri, 16 Oct 2009 06:02:18 GMT</lastBuildDate>
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<title>Nori ta Abadiyat (The Words I LOVE YOU</title>
<link>http://lovelyenglish.blogfa.com/post-48.aspx</link>
<description>&lt;P align=left&gt;&lt;FONT color=#00ccff size=3&gt;Hi friends&lt;/FONT&gt;&lt;/P&gt;
&lt;P align=left&gt;&lt;FONT color=#00ccff size=3&gt;I hope you are all well&lt;/FONT&gt;&lt;/P&gt;
&lt;P align=left&gt;&lt;FONT color=#00ccff size=3&gt;Can you hear the song which is playing in my weblog?That’s my favorite song,so I want to tell you some thing about it&lt;/FONT&gt;&lt;/P&gt;
&lt;P align=left&gt;&lt;FONT color=#00ccff size=3&gt;&lt;IMG alt=&quot;&quot; hspace=0 src=&quot;http://www.cjreport.com/files/mainimgs/Arian-De-burgh.jpg&quot; border=0&gt;&lt;/FONT&gt;&lt;/P&gt;
&lt;P align=left&gt;&lt;FONT color=#00ccff size=3&gt;I know that some of you aren’t persian &amp; don’t know anything about it so some parts of this song will be strange to you but you should know that english parts are kind of translations for persian parts&lt;/FONT&gt;&lt;/P&gt;
&lt;P align=left&gt;&lt;FONT color=#00ccff size=3&gt;Anyway, this song is a coprative song between The Arian Band &amp; Chris De Burg,my favorite singers&lt;/FONT&gt;&lt;/P&gt;
&lt;P align=left&gt;&lt;FONT color=#00ccff size=3&gt;&lt;IMG alt=&quot;&quot; hspace=0 src=&quot;http://www.arianmusic.com/en/images/stories/album/4.jpg&quot; border=0&gt;&lt;/FONT&gt;&lt;/P&gt;
&lt;P align=left&gt;&lt;FONT color=#00ccff size=3&gt;The Arian Band is a famous persian band that I hope you know cause have been having lots of tours all around the world&lt;/FONT&gt;&lt;/P&gt;
&lt;P align=left&gt;&lt;FONT color=#00ccff size=3&gt;&lt;IMG alt=&quot;&quot; hspace=0 src=&quot;http://assets.radiojavan.com/static/news/images/2007/11/14/831182df.jpeg&quot; border=0&gt;&lt;/FONT&gt;&lt;/P&gt;
&lt;P align=left&gt;&lt;FONT color=#00ccff size=3&gt; &lt;/FONT&gt;&lt;FONT color=#00ccff size=3&gt;About Chris De Burg I don’t think that there is need to say anything cause he is a really famous &amp; experienced Irish singer who sings English songs&lt;/FONT&gt;&lt;/P&gt;
&lt;P align=left&gt;&lt;FONT color=#00ccff size=3&gt;And about the song, this is a song about peace which recorded on 2008 for one of the albums of The Arian Band called “Without You With You” &amp; invites mankind to love eachother without paying attention to anything like nation,language,religion,… just because we all have the same destination &amp; the same God with diffirent names &lt;/FONT&gt;&lt;/P&gt;
&lt;P align=left&gt;&lt;FONT color=#00ccff size=3&gt;I think it’s better not to tell more cause it’s better to listen to this fantastic song&lt;/FONT&gt;&lt;/P&gt;
&lt;P align=left&gt;&lt;FONT color=#00ccff&gt;&lt;FONT size=3&gt;As in the song says we should express that we all love eachother so &lt;STRONG&gt;I LOVE YOU ALL&lt;/STRONG&gt;&lt;/FONT&gt;&lt;/FONT&gt;&lt;/P&gt;
&lt;P align=left&gt;&lt;FONT color=#00ccff size=3&gt;TAKE CARE&lt;/FONT&gt;&lt;/P&gt;
&lt;P align=left&gt;&lt;FONT color=#00ccff size=3&gt;BE SUCCESSFUL&lt;/FONT&gt;&lt;/P&gt;
&lt;P align=left&gt;&lt;FONT color=#00ccff&gt;&lt;FONT size=3&gt;     &lt;EM&gt;&lt;U&gt;&lt;FONT color=#0033ff&gt;Anonymous&lt;/FONT&gt;&lt;/U&gt;&lt;/EM&gt;&lt;/FONT&gt;&lt;/FONT&gt;&lt;/P&gt;
&lt;P align=left&gt;&lt;FONT color=#00ccff size=3&gt;p.s:If you want to to know more about this song you can visit the official site of The Arian Band : &lt;FONT color=#0000ff&gt;www.arianmusic.com&lt;/FONT&gt;&lt;/FONT&gt;&lt;/P&gt;
&lt;P align=left&gt;&lt;FONT color=#00ccff size=3&gt; &lt;/FONT&gt;&lt;/P&gt;</description>
<pubDate>Fri, 16 Oct 2009 06:02:18 GMT</pubDate>
<comments>http://commenting.blogfa.com/?blogid=lovelyenglish&amp;postid=48</comments>
<dc:creator>lovelyenglish</dc:creator>
<guid>http://lovelyenglish.blogfa.com/post-48.aspx</guid>
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<title>Hubble Servicing Mission 4 Early Release Observations</title>
<link>http://lovelyenglish.blogfa.com/post-47.aspx</link>
<description>&lt;P align=left&gt;&lt;STRONG&gt;&lt;FONT size=3&gt;&lt;FONT color=#00ff00&gt;&lt;SPAN class=inline-date&gt;September 9, 2009:&lt;/SPAN&gt; NASA&apos;s Hubble Space Telescope is back in business, ready to uncover new worlds, peer ever deeper into space, and even map the invisible backbone of the universe. The first &lt;FONT color=#00ff00&gt;snapshots&lt;/FONT&gt; from the refurbished Hubble showcase the 19-year old telescope&apos;s new vision&lt;/FONT&gt;&lt;/FONT&gt;&lt;/STRONG&gt;&lt;/P&gt;
&lt;P align=left&gt; &lt;IMG style=&quot;WIDTH: 336px; HEIGHT: 400px&quot; alt=&quot;&quot; hspace=0 src=&quot;http://imgsrc.hubblesite.org/hu/db/images/hs-2009-25-a-web.jpg&quot; align=middle border=0&gt;&lt;/P&gt;
&lt;P align=left&gt;&lt;STRONG&gt;&lt;FONT color=#00ff00 size=3&gt;Topping the list of exciting new views are colorful multi-wavelength pictures of far-flung galaxies, a densely packed star cluster, an eerie &quot;pillar of creation,&quot; and a &quot;butterfly&quot; nebula. With its new imaging camera, Hubble can view galaxies, star clusters, and other objects across a wide swath of the electromagnetic spectrum, from ultraviolet to near-infrared light. A new spectrograph slices across billions of light-years to map the filamentary structure of the universe and trace the distribution of elements that are fundamental to life. The telescope&apos;s new instruments also are more sensitive to light and can observe in ways that are significantly more efficient and require less observing time than previous generations of Hubble instruments. NASA astronauts installed the new instruments during the space shuttle servicing mission in May 2009. Besides adding the instruments, the astronauts also completed a dizzying list of other chores that included performing unprecedented repairs on two other science instruments&lt;/FONT&gt;&lt;/STRONG&gt;&lt;/P&gt;
&lt;P align=left&gt;&lt;STRONG&gt;&lt;FONT color=#00ff00 size=3&gt;Now that Hubble has reopened for business, it will tackle a whole range of observations. Looking closer to Earth, such observations will include taking a census of the population of Kuiper Belt objects residing at the fringe of our solar system, witnessing the birth of planets around other stars, and probing the composition and structure of the atmospheres of other worlds. Peering much farther away, astronomers have ambitious plans to use Hubble to make the deepest-ever portrait of the universe in near-infrared light. The resulting picture may reveal never-before-seen infant galaxies that existed when the universe was less than 500 million years old. Hubble also is now significantly more well-equipped to probe and further characterize the behavior of dark energy, a mysterious and little-understood repulsive force that is pushing the universe apart at an ever-faster rate&lt;/FONT&gt;&lt;/STRONG&gt;&lt;/P&gt;</description>
<pubDate>Mon, 28 Sep 2009 12:31:26 GMT</pubDate>
<comments>http://commenting.blogfa.com/?blogid=lovelyenglish&amp;postid=47</comments>
<dc:creator>lovelyenglish</dc:creator>
<guid>http://lovelyenglish.blogfa.com/post-47.aspx</guid>
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<title>Astronomers Find Hyperactive Galaxies in the Early Universe</title>
<link>http://lovelyenglish.blogfa.com/post-46.aspx</link>
<description>&lt;P align=left&gt;&lt;FONT size=3&gt;&lt;STRONG&gt;&lt;FONT face=&quot;arial, helvetica, sans-serif&quot;&gt;&lt;FONT color=#99cc00&gt; Even some galaxies may have been hyperactive youngsters. Looking almost 11 billion years into the past, astronomers have measured the motions of stars for the first time in a very distant galaxy. They are whirling at a speed of one million miles per hour—about twice the speed of our Sun through the Milky Way. Even stranger, the galaxies are a fraction the size of our Milky Way, and so may have evolved over billions of years into the full-grown galaxies seen around us today. Astronomers are puzzled by how galaxies like these formed. They may be what will eventually become the dense central regions of very large galaxies&lt;/FONT&gt;&lt;/FONT&gt;&lt;/STRONG&gt;&lt;/FONT&gt;&lt;/P&gt;
&lt;P align=left&gt;&lt;FONT size=3&gt;&lt;STRONG&gt;&lt;FONT face=&quot;arial, helvetica, sans-serif&quot;&gt;&lt;FONT color=#99cc00&gt;&lt;IMG border=0 hspace=0 alt=&quot;&quot; align=left src=&quot;http://imgsrc.hubblesite.org/hu/db/images/hs-2009-24-a-web.jpg&quot;&gt;. &lt;/FONT&gt;&lt;/FONT&gt;&lt;/STRONG&gt;&lt;/FONT&gt;&lt;/P&gt;
&lt;P align=left&gt;&lt;FONT color=#99cc00 size=3 face=&quot;arial, helvetica, sans-serif&quot;&gt;&lt;STRONG&gt;The galaxies were found by using the combined power of NASA’s Hubble Space Telescope and the 8-meter Gemini South telescope in Chile. Hubble shows that the galaxies are a fraction the size of most galaxies we see today. The Gemini telescope clocks their speed by using spectroscopy. To witness the formation of these extreme galaxies astronomers plan to observe galaxies even farther back in time with Hubble’s new Wide Field Camera 3&lt;/STRONG&gt;&lt;/FONT&gt;. &lt;/P&gt;</description>
<pubDate>Thu, 13 Aug 2009 12:49:05 GMT</pubDate>
<comments>http://commenting.blogfa.com/?blogid=lovelyenglish&amp;postid=46</comments>
<dc:creator>lovelyenglish</dc:creator>
<guid>http://lovelyenglish.blogfa.com/post-46.aspx</guid>
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<title>Rare Spherical Planetary Nebula Abell 39</title>
<link>http://lovelyenglish.blogfa.com/post-45.aspx</link>
<description>&lt;P align=left&gt;&lt;IMG alt=&quot;&quot; hspace=0 src=&quot;http://www.wolaver.org/Space/abell39nebula.jpg&quot; align=left border=0&gt;&lt;/P&gt;
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&lt;P align=justify&gt;&lt;FONT color=#ffff99 size=4&gt;&lt;STRONG&gt;The simple spherical geometry of &lt;/STRONG&gt;&lt;/FONT&gt;&lt;A href=&quot;http://www.wolaver.org/Space/planetarynebulae.htm&quot;&gt;&lt;FONT color=#ffff99 size=4&gt;&lt;STRONG&gt;planetary nebula&lt;/STRONG&gt;&lt;/FONT&gt;&lt;/A&gt;&lt;FONT color=#ffff99 size=4&gt;&lt;STRONG&gt; Abell 39 will help astronomers identify the source of very serious errors in measuring the chemical composition of dying stars&quot;The truly spherical nature of this beautiful nebula helps us eliminate a common confusion concerning the actual three-dimensional geometry of most nebulae,&quot; says George Jacoby, director of the Wisconsin-Indiana-Yale-NOAO (WIYN) Observatory and co-author of a study with Gary Ferland of University of Kentucky and Kirk Korista of Western Michigan University.The butterfly-like shape of many nebulae, and filaments or clumps of dense gas within them, cause starlight to penetrate the nebulae unevenly, depending on the density and thickness of the clumps, as well as the distance of the gas from the star. Only in rare cases can the nebula&apos;s geometry be deduced from indirect measurements in order to model the interactions.As reported today in San Diego at the 197th meeting of the American Astronomical Society, researchers found that the star that produced Abell 39 had only half the amount of oxygen found in the Sun. This result is not especially unusual, because the Sun has a relatively enriched composition of heavy elements. But for some stars, the same sorts of analyses have yielded compositions that can disagree with each other by a factor of three or more.&quot;Such discrepancies are totally unsatisfactory for developing a detailed picture of how chemical elements were built up over time in our galaxy and in other parts of the Universe,&quot; Jacoby explains.Abell 39 is the 39th entry in a catalog of large nebulae discovered by astronomer George Abell in 1966. This image of it was taken at the WIYN Observatory&apos;s 3.5-meter (138-inch) telescope, through a blue-green filter that isolates the light emitted by oxygen atoms in the nebula at a wavelength of 500.7 nanometers.Unfortunately, Abell 39 is so faint that Jacoby and collaborators were unable to measure all the critical information from the nebula that is needed to isolate the cause of the composition measurement discrepancies, even though they used the National Science Foundation&apos;s Mayall 4-meter telescope at Kitt Peak National Observatory to collect spectral details. Instead, they provide their predictions of what they expected to measure, in order to guide future observers with more sensitive equipment and larger telescopes.The nebula has a diameter of about five light-years, and the thickness of the spherical shell is about a third of a light-year. Positioned in the constellation Hercules, the nebula is located roughly 7,000 light-years from Earth. Careful viewing of the image shows that the &quot;central&quot; star is off-center to the right by a small amount (less than a tenth of a light-year.) The cause of this shift is unknown. Furthermore, the very faint glow barely visible around the brightest part of the nebula is evidence for a larger halo surrounding the main body. As a curiosity, several distant galaxies can be seen right through the nebula and just outside of it  &lt;/STRONG&gt;&lt;/FONT&gt;&lt;/P&gt;</description>
<pubDate>Mon, 20 Jul 2009 14:13:18 GMT</pubDate>
<comments>http://commenting.blogfa.com/?blogid=lovelyenglish&amp;postid=45</comments>
<dc:creator>lovelyenglish</dc:creator>
<guid>http://lovelyenglish.blogfa.com/post-45.aspx</guid>
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<title>Too long names</title>
<link>http://lovelyenglish.blogfa.com/post-44.aspx</link>
<description>&lt;P align=left&gt;&lt;FONT color=#0000ff&gt;&lt;FONT face=&quot;times new roman, times, serif&quot;&gt;&lt;FONT size=3&gt;Wales (country that is part of the United Kingdom), there is a village called &lt;FONT color=#009900&gt;Llanfairpwllgwyngyllgogerychwyrndrobwllllantysiliogogogoch (&lt;U&gt;58 letters&lt;/U&gt;)&lt;/FONT&gt;, which in English means &lt;FONT color=#009900&gt;&quot;Saint Mary&apos;s Church in the hollow of white hazel near a rapid whirlpool and the Church of Saint Tysilio near the red cave.&quot; &lt;/FONT&gt;The locals call it Llanfairpwll. Llanfairpwllgwyngyllgogerychwyrndrobwllllantysiliogogogoch.com is the longest single word .com domain name in the world. However in October 1999, it became possible to register domain names up to 67 characters in and finally, sadly even the &lt;U&gt;67 character&lt;/U&gt; allowance for a .com domain name is still insufficient for the town of &lt;FONT color=#660000&gt;&lt;B&gt;Tetaumatawhakatangihangakoauaotamateaurehaeaturipukapihima&lt;/B&gt;&lt;B&gt;ungahoronuku&lt;/B&gt;&lt;/FONT&gt;&lt;/FONT&gt;&lt;/FONT&gt;&lt;/FONT&gt;&lt;/P&gt;
&lt;P align=left&gt;&lt;FONT size=+0&gt;&lt;FONT face=&quot;times new roman, times, serif&quot;&gt;&lt;FONT color=#660000 size=3&gt;&lt;B&gt;pok&lt;/B&gt;&lt;/FONT&gt;&lt;/FONT&gt;&lt;/FONT&gt;&lt;FONT face=&quot;times new roman, times, serif&quot;&gt;&lt;FONT size=3&gt;&lt;B&gt;&lt;FONT color=#660000&gt;aiwhenuaakitanarahu&lt;/FONT&gt;&lt;/B&gt;&lt;FONT color=#0000ff&gt;&lt;B&gt; &lt;/B&gt;&lt;/FONT&gt;&lt;/FONT&gt;&lt;/FONT&gt;&lt;/P&gt;
&lt;P align=left&gt;&lt;FONT face=&quot;times new roman, times, serif&quot; color=#0000ff size=3&gt;Which translates into English as &lt;FONT color=#330000&gt;&quot;The brow of the hill where Tamatea, with the bony knees, who slid and climbed mountains, the great travelers, sat and played on the flute to his beloved&lt;BR&gt;&lt;/FONT&gt;This town is in New Zealand with &lt;/FONT&gt;&lt;A href=&quot;http://www.llanfairpwllgwyngyllgogerychwyrndrobwllllantysiliogogogoch.com/information-about-tetaumatawhakatang.htm&quot;&gt;&lt;FONT face=&quot;times new roman, times, serif&quot; color=#0000ff size=3&gt;a staggering 92 characters&lt;/FONT&gt;&lt;/A&gt;&lt;FONT face=&quot;times new roman, times, serif&quot; color=#0000ff size=3&gt; however even this seems positively tiny compared to the town of&lt;/FONT&gt;&lt;/P&gt;
&lt;P align=left&gt;&lt;B&gt;&lt;FONT face=&quot;times new roman, times, serif&quot; color=#ff3300 size=3&gt;Krungthepmahanakornamornratanakosinmahintarayutthayamahadilokphop&lt;/FONT&gt;&lt;/B&gt;&lt;B&gt;&lt;BR&gt;&lt;/B&gt;&lt;B&gt;&lt;FONT face=&quot;times new roman, times, serif&quot; color=#ff3300 size=3&gt;nopparatrajathaniburiromudomrajaniwesmahasatharn&lt;/FONT&gt;&lt;/B&gt;&lt;B&gt;&lt;BR&gt;&lt;/B&gt;&lt;B&gt;&lt;FONT face=&quot;times new roman, times, serif&quot; color=#ff3300 size=3&gt;amornphimarnavatarnsathitsakkattiyavisanukamprasit&lt;/FONT&gt;&lt;/B&gt;&lt;/P&gt;
&lt;P align=left&gt;&lt;FONT face=&quot;times new roman, times, serif&quot; color=#0000ff size=3&gt;In Thailand which is long so long that it doesn&apos;t even fit on one line! Meaning the &lt;FONT color=#ff3300&gt;&apos;City of Angels&apos;&lt;/FONT&gt; (a whopping 163 characters), is known to the locals as Krungthep Mahanakhon. However, it is not recognised by the Guinness Book of Records&lt;/FONT&gt;&lt;/P&gt;
&lt;P align=left&gt;&lt;FONT face=&quot;times new roman, times, serif&quot; color=#0000ff size=3&gt;However whilst the New Zealand place name is recognised by the Guinness Book of Record, the Thailand name is not&lt;/FONT&gt; &lt;/P&gt;</description>
<pubDate>Tue, 23 Jun 2009 09:46:18 GMT</pubDate>
<comments>http://commenting.blogfa.com/?blogid=lovelyenglish&amp;postid=44</comments>
<dc:creator>lovelyenglish</dc:creator>
<guid>http://lovelyenglish.blogfa.com/post-44.aspx</guid>
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<title>NGC 1333 </title>
<link>http://lovelyenglish.blogfa.com/post-43.aspx</link>
<description>&lt;/P&gt;
&lt;P&gt; &lt;IMG alt=&quot;&quot; hspace=0 src=&quot;http://antwrp.gsfc.nasa.gov/apod/image/0904/NGC1333_LRGB_leshin800.jpg&quot; align=left border=0&gt;&lt;/P&gt;
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&lt;P align=left&gt;&lt;FONT size=3&gt;&lt;B&gt;Explanation: &lt;/B&gt;NGC 1333 is seen in visible light as a &lt;/FONT&gt;&lt;A href=&quot;http://astronomy.swin.edu.au/cms/astro/cosmos/R/Reflection+Nebula&quot;&gt;&lt;FONT size=3&gt;reflection nebula&lt;/FONT&gt;&lt;/A&gt;&lt;FONT size=3&gt;, dominated by bluish hues characteristic of starlight reflected by dust. A mere 1,000 light-years distant toward the heroic constellation &lt;/FONT&gt;&lt;A href=&quot;http://www.hawastsoc.org/deepsky/per/index.html&quot;&gt;&lt;FONT size=3&gt;Perseus&lt;/FONT&gt;&lt;/A&gt;&lt;FONT size=3&gt;, it lies at the edge of a large, &lt;/FONT&gt;&lt;A href=&quot;http://loke.as.arizona.edu/~ckulesa/research/overview.html&quot;&gt;&lt;FONT size=3&gt;star-forming&lt;/FONT&gt;&lt;/A&gt;&lt;FONT size=3&gt; molecular cloud. &lt;/FONT&gt;&lt;A href=&quot;http://sleshin.startlogic.com/stargazergallery/main.php?g2_itemId=205&quot;&gt;&lt;FONT size=3&gt;This striking close-up&lt;/FONT&gt;&lt;/A&gt;&lt;FONT size=3&gt; view spans about 4 light-years at the estimated distance &lt;/FONT&gt;&lt;A href=&quot;http://www.robgendlerastropics.com/NGC1333text.html&quot;&gt;&lt;FONT size=3&gt;of NGC 1313&lt;/FONT&gt;&lt;/A&gt;&lt;FONT size=3&gt;. It shows details of the dusty region along with hints of contrasting emission in red &lt;/FONT&gt;&lt;A href=&quot;http://en.wikipedia.org/wiki/Herbig-Haro_object&quot;&gt;&lt;FONT size=3&gt;jets and glowing gas&lt;/FONT&gt;&lt;/A&gt;&lt;FONT size=3&gt; from recently formed stars. In fact, NGC 1333 contains hundreds of stars less than a million years old, &lt;/FONT&gt;&lt;A href=&quot;http://www.spitzer.caltech.edu/Media/releases/ssc2005-24/release.shtml&quot;&gt;&lt;FONT size=3&gt;most still hidden&lt;/FONT&gt;&lt;/A&gt;&lt;FONT size=3&gt; from optical telescopes by the &lt;/FONT&gt;&lt;A href=&quot;http://antwrp.gsfc.nasa.gov/apod/ap071129.html&quot;&gt;&lt;FONT size=3&gt;pervasive stardust&lt;/FONT&gt;&lt;/A&gt;&lt;FONT size=3&gt;. The chaotic environment may be similar to one in which our own Sun formed over 4.5 billion years ago&lt;/FONT&gt;&lt;/P&gt;</description>
<pubDate>Tue, 19 May 2009 14:06:18 GMT</pubDate>
<comments>http://commenting.blogfa.com/?blogid=lovelyenglish&amp;postid=43</comments>
<dc:creator>lovelyenglish</dc:creator>
<guid>http://lovelyenglish.blogfa.com/post-43.aspx</guid>
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<title>collocations of astronomy </title>
<link>http://lovelyenglish.blogfa.com/post-42.aspx</link>
<description>Hi my friends&lt;/P&gt;
&lt;P align=left&gt;From now I want to teach you some simple collocation of astronomy and then I will bring you a fantastic picture with some explanations&lt;/P&gt;
&lt;P align=left&gt;So the first collocation&lt;/P&gt;
&lt;P align=left&gt;Reflection Nebula&lt;/P&gt;
&lt;P&gt; &lt;IMG style=&quot;WIDTH: 300px; HEIGHT: 215px&quot; alt=&quot;&quot; hspace=0 src=&quot;http://astronomy.swin.edu.au/cms/imagedb/albums/userpics/reflectionnebula1.jpg&quot; align=left border=0&gt; &lt;/P&gt;
&lt;P align=left&gt;A reflection nebula is created when light from a star is scattered or reflected off a neighbouring &lt;A href=&quot;http://astronomy.swin.edu.au/cosmos/D/Dust+Grain&quot;&gt;dust&lt;/A&gt; cloud. The scattered light is slightly polarised and has a spectrum similar to that of the illuminating star, only bluer. This shift in colour arises because the typical size of &lt;A href=&quot;http://astronomy.swin.edu.au/cosmos/D/Dust+Grain&quot;&gt;dust&lt;/A&gt; grains in the cloud are comparable to the &lt;A href=&quot;http://astronomy.swin.edu.au/cosmos/W/Wavelength&quot;&gt;wavelength&lt;/A&gt; of blue light. The result is that blue light is scattered more efficiently than longer, red &lt;A href=&quot;http://astronomy.swin.edu.au/cosmos/W/Wavelength&quot;&gt;wavelengths&lt;/A&gt; giving the characteristic blue colour for these &lt;A href=&quot;http://astronomy.swin.edu.au/cosmos/N/Nebula&quot;&gt;nebulae&lt;/A&gt;&lt;IMG alt=&quot;&quot; hspace=0 src=&quot;http://astronomy.swin.edu.au/cms/imagedb/albums/userpics/reflectionnebula2.jpg&quot; align=right border=0&gt;&lt;/P&gt;
&lt;P align=left&gt;Reflection &lt;A class=autolink-term href=&quot;http://astronomy.swin.edu.au/cosmos/N/Nebula&quot;&gt;nebulae&lt;/A&gt; are usually less dense than &lt;A class=autolink-term href=&quot;http://astronomy.swin.edu.au/cosmos/D/Dark+Nebula&quot;&gt;dark nebulae&lt;/A&gt;, and have sizes that are determined by the source of illumination. Their extent is not defined by the size of the &lt;A class=autolink-term href=&quot;http://astronomy.swin.edu.au/cosmos/D/Dust+Grain&quot;&gt;dust&lt;/A&gt; cloud but rather the &lt;A class=autolink-term href=&quot;http://astronomy.swin.edu.au/cosmos/A/Area&quot;&gt;area&lt;/A&gt; over which their brightness remains above the point of detection.&lt;BR&gt;The nebulosity surrounding the &lt;A class=autolink-term href=&quot;http://astronomy.swin.edu.au/cosmos/S/Star&quot;&gt;stars&lt;/A&gt; in the Pleiades is perhaps the most well known example of a &lt;A class=autolink-term href=&quot;http://astronomy.swin.edu.au/cosmos/R/Reflection+Nebula&quot;&gt;reflection nebula&lt;/A&gt;&lt;/P&gt;
&lt;P align=left&gt; &lt;/P&gt;
&lt;DIV class=imageWrapper style=&quot;WIDTH: 244px; HEIGHT: 67px&quot;&gt;
&lt;DIV class=caption align=left&gt;The Pleiades is one of the most famous reflection &lt;A class=autolink-term href=&quot;http://astronomy.swin.edu.au/cosmos/N/Nebula&quot;&gt;nebulae&lt;/A&gt;.&lt;BR&gt;&lt;A href=&quot;http://www.aao.gov.au/images/captions/uks018.html&quot; target=_blank&gt;Credit&lt;/A&gt;: AAO/ROE/David Malin &lt;/DIV&gt;
&lt;DIV class=caption align=left&gt;ost famous reflection &lt;/DIV&gt;&lt;/DIV&gt;
&lt;P align=left&gt;
&lt;TABLE class=center style=&quot;MARGIN-LEFT: auto; MARGIN-RIGHT: auto&quot; cellSpacing=0&gt;
&lt;TBODY&gt;
&lt;TR&gt;
&lt;TD vAlign=top&gt;&lt;/TD&gt;&lt;/TR&gt;&lt;/TBODY&gt;&lt;/TABLE&gt;                                                                               &lt;/P&gt;</description>
<pubDate>Sat, 18 Apr 2009 09:03:28 GMT</pubDate>
<comments>http://commenting.blogfa.com/?blogid=lovelyenglish&amp;postid=42</comments>
<dc:creator>lovelyenglish</dc:creator>
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<item>
<title>Alfred Nobel </title>
<link>http://lovelyenglish.blogfa.com/post-41.aspx</link>
<description>&lt;P align=left&gt;&lt;FONT color=#003333 size=3&gt;&lt;STRONG&gt;childhood&lt;/STRONG&gt;&lt;/FONT&gt;&lt;/P&gt;
&lt;P align=left&gt;&lt;FONT color=#003333&gt;Alfred Nobel (1833-1896) was born in Stockholm, Sweden, on October 21, 1833. His family was descended from Olof Rudbeck, the best-known technical genius in Sweden in the 17th century, an era in which Sweden was a great power in northern Europe. Alfred&apos;s mother, born &lt;/FONT&gt;&lt;A href=&quot;http://nobelprize.org/alfred_nobel/biographical/articles/life-work/andriette.html&quot;&gt;&lt;FONT color=#003333&gt;Andriette Ahlsell&lt;/FONT&gt;&lt;/A&gt;&lt;FONT color=#003333&gt;, came from a wealthy family. His father &lt;/FONT&gt;&lt;A href=&quot;http://nobelprize.org/alfred_nobel/biographical/articles/life-work/immanuel.html&quot;&gt;&lt;FONT color=#003333&gt;Immanuel Nobel&lt;/FONT&gt;&lt;/A&gt;&lt;FONT color=#003333&gt; was an engineer and inventor who built bridges and buildings in Stockholm. In connection with his construction work Immanuel Nobel also experimented with different techniques for blasting rocks. Immanuel Nobel was also a pioneer in arms manufacture and in designing steam engines. Due to misfortunes in his construction work caused by the loss of some barges of building material, Immanuel Nobel was forced into bankruptcy the same year Alfred Nobel was born. Nobel was fluent in several languages, and wrote poetry and drama. Nobel was also very interested in social and peace-related issues, and held views that were considered radical during his time. In St. Petersburg, Immanuel&apos;s sons were given a first class education by private teachers. The training included natural sciences, languages and literature. By the age of 17 Alfred Nobel was fluent in Swedish, Russian, French, English and German. His primary interests were in English literature and poetry as well as in chemistry and physics. Alfred&apos;s father, who wanted his sons to join his enterprise as engineers, disliked Alfred&apos;s interest in poetry and found his son rather introverted&lt;/FONT&gt;&lt;/P&gt;
&lt;P align=left&gt;&lt;B&gt;&lt;FONT color=#003333&gt;Source: www.nobelprize.org&lt;/FONT&gt;&lt;/B&gt;&lt;/P&gt;</description>
<pubDate>Thu, 09 Apr 2009 15:59:18 GMT</pubDate>
<comments>http://commenting.blogfa.com/?blogid=lovelyenglish&amp;postid=41</comments>
<dc:creator>lovelyenglish</dc:creator>
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<item>
<title></title>
<link>http://lovelyenglish.blogfa.com/post-40.aspx</link>
<description>&lt;P align=left&gt;&lt;FONT color=#3300ff size=3&gt;Friendship is a chain of gold. Each link is a smile, a laugh, a tear, a grip of the &lt;/FONT&gt;&lt;FONT color=#3300ff size=3&gt;hand, a word of cheer&lt;/FONT&gt;&lt;/P&gt;
&lt;P align=left&gt;&lt;FONT color=#ff6600 size=3&gt;Friends are puzzle pieces. If one is lost, that special piece can never be replaced and puzzle will never be whole again&lt;/FONT&gt;&lt;/P&gt;
&lt;P align=left&gt;&lt;FONT color=#ff0066 size=3&gt;Love can never be taught for it is to be learned; love can never be bought for it is to be given; love can never be kept for it is to be free; love can never be old for it lives to last a lifetime&lt;/FONT&gt;&lt;/P&gt;</description>
<pubDate>Fri, 23 Jan 2009 09:06:35 GMT</pubDate>
<comments>http://commenting.blogfa.com/?blogid=lovelyenglish&amp;postid=40</comments>
<dc:creator>lovelyenglish</dc:creator>
<guid>http://lovelyenglish.blogfa.com/post-40.aspx</guid>
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<item>
<title>DAILY WORDS</title>
<link>http://lovelyenglish.blogfa.com/post-39.aspx</link>
<description>&lt;H1 style=&quot;MARGIN: 0cm 0cm 0pt&quot; align=left&gt;&lt;FONT face=&quot;Comic Sans MS&quot; size=7&gt;ABANDON&lt;/FONT&gt;&lt;/H1&gt;
&lt;P class=MsoNormal style=&quot;MARGIN: 0cm 0cm 0pt&quot; align=left&gt;&lt;SPAN style=&quot;FONT-SIZE: 26pt; COLOR: navy; FONT-FAMILY: &apos;Comic Sans MS&apos;&quot;&gt;Desert&lt;/SPAN&gt;&lt;SPAN style=&quot;FONT-SIZE: 26pt; FONT-FAMILY: &apos;Comic Sans MS&apos;&quot;&gt;, &lt;SPAN style=&quot;COLOR: blue&quot;&gt;leave without &lt;/SPAN&gt;&lt;/SPAN&gt;&lt;SPAN style=&quot;FONT-SIZE: 26pt; FONT-FAMILY: &apos;Comic Sans MS&apos;&quot;&gt;&lt;SPAN style=&quot;COLOR: blue&quot;&gt;planning to &lt;SPAN style=&quot;FONT-SIZE: 26pt; FONT-FAMILY: &apos;Comic Sans MS&apos;&quot;&gt;&lt;SPAN style=&quot;COLOR: #3366ff&quot;&gt;&lt;FONT color=#0000ff&gt;come back&lt;SPAN style=&quot;FONT-SIZE: 26pt; FONT-FAMILY: &apos;Comic Sans MS&apos;&quot;&gt;&lt;SPAN style=&quot;COLOR: #3366ff&quot;&gt;&lt;FONT color=#000000&gt;,&lt;/FONT&gt;&lt;/SPAN&gt;&lt;/SPAN&gt;&lt;SPAN style=&quot;FONT-SIZE: 26pt; FONT-FAMILY: &apos;Comic Sans MS&apos;&quot;&gt;&lt;SPAN style=&quot;COLOR: #3366ff&quot;&gt;quit&lt;/SPAN&gt;&lt;/SPAN&gt;&lt;/FONT&gt;&lt;/SPAN&gt;&lt;?xml:namespace prefix = o ns = &quot;urn:schemas-microsoft-com:office:office&quot; /&gt;&lt;o:p&gt;&lt;/o:p&gt;&lt;/SPAN&gt;&lt;/SPAN&gt; &lt;/SPAN&gt;&lt;/P&gt;
&lt;P class=MsoNormal style=&quot;MARGIN: 0cm 0cm 0pt&quot; align=left&gt;&lt;SPAN style=&quot;FONT-SIZE: 26pt; COLOR: red; FONT-FAMILY: &apos;Comic Sans MS&apos;&quot;&gt;A&lt;/SPAN&gt;&lt;SPAN style=&quot;FONT-SIZE: 26pt; FONT-FAMILY: &apos;Comic Sans MS&apos;&quot;&gt;: &lt;SPAN style=&quot;COLOR: green&quot;&gt;when Roy &lt;/SPAN&gt;abandoned&lt;SPAN style=&quot;COLOR: green&quot;&gt; &lt;/SPAN&gt;&lt;/SPAN&gt;&lt;SPAN style=&quot;FONT-SIZE: 26pt; FONT-FAMILY: &apos;Comic Sans MS&apos;&quot;&gt;&lt;SPAN style=&quot;COLOR: green&quot;&gt;his family, the police &lt;/SPAN&gt;&lt;/SPAN&gt;&lt;SPAN style=&quot;FONT-SIZE: 26pt; FONT-FAMILY: &apos;Comic Sans MS&apos;&quot;&gt;&lt;SPAN style=&quot;COLOR: green&quot;&gt;went looking for him&lt;/SPAN&gt;&lt;o:p&gt;&lt;/o:p&gt;&lt;/SPAN&gt;&lt;/P&gt;
&lt;P class=MsoNormal style=&quot;MARGIN: 0cm 0cm 0pt&quot; align=left&gt;&lt;SPAN style=&quot;FONT-SIZE: 26pt; COLOR: red; FONT-FAMILY: &apos;Comic Sans MS&apos;&quot;&gt;B&lt;/SPAN&gt;&lt;SPAN style=&quot;FONT-SIZE: 26pt; FONT-FAMILY: &apos;Comic Sans MS&apos;&quot;&gt;: &lt;SPAN style=&quot;COLOR: #339966&quot;&gt;the soldier couldn’t &lt;/SPAN&gt;abandon&lt;SPAN style=&quot;COLOR: #339966&quot;&gt; his friends who were hurt in battle&lt;/SPAN&gt;&lt;o:p&gt;&lt;/o:p&gt;&lt;/SPAN&gt;&lt;/P&gt;
&lt;P class=MsoNormal style=&quot;MARGIN: 0cm 0cm 0pt&quot; align=left&gt;&lt;SPAN style=&quot;FONT-SIZE: 26pt; COLOR: red; FONT-FAMILY: &apos;Comic Sans MS&apos;&quot;&gt;C&lt;/SPAN&gt;&lt;SPAN style=&quot;FONT-SIZE: 26pt; FONT-FAMILY: &apos;Comic Sans MS&apos;&quot;&gt;: &lt;SPAN style=&quot;COLOR: lime&quot;&gt;because rose was poor, she had to &lt;/SPAN&gt;abandon&lt;SPAN style=&quot;COLOR: lime&quot;&gt; her idea of going to college&lt;/SPAN&gt;&lt;o:p&gt;&lt;/o:p&gt;&lt;/SPAN&gt;&lt;/P&gt;
&lt;P class=MsoNormal style=&quot;MARGIN: 0cm 0cm 0pt&quot; align=left&gt;&lt;SPAN style=&quot;FONT-SIZE: 26pt; FONT-FAMILY: &apos;Comic Sans MS&apos;&quot;&gt;Keen&lt;o:p&gt;&lt;/o:p&gt;&lt;/SPAN&gt;&lt;/P&gt;
&lt;P class=MsoNormal style=&quot;MARGIN: 0cm 0cm 0pt&quot; align=left&gt;&lt;SPAN style=&quot;FONT-SIZE: 26pt; COLOR: navy; FONT-FAMILY: &apos;Comic Sans MS&apos;&quot;&gt;Sharp&lt;/SPAN&gt;&lt;SPAN style=&quot;FONT-SIZE: 26pt; FONT-FAMILY: &apos;Comic Sans MS&apos;&quot;&gt;, &lt;SPAN style=&quot;COLOR: blue&quot;&gt;eager&lt;/SPAN&gt;, &lt;SPAN style=&quot;COLOR: #3366ff&quot;&gt;intense&lt;/SPAN&gt;, &lt;SPAN style=&quot;COLOR: #00ccff&quot;&gt;sensitive&lt;/SPAN&gt;&lt;o:p&gt;&lt;/o:p&gt;&lt;/SPAN&gt;&lt;/P&gt;
&lt;P class=MsoNormal style=&quot;MARGIN: 0cm 0cm 0pt&quot; align=left&gt;&lt;SPAN style=&quot;FONT-SIZE: 26pt; COLOR: red; FONT-FAMILY: &apos;Comic Sans MS&apos;&quot;&gt;A&lt;/SPAN&gt;&lt;SPAN style=&quot;FONT-SIZE: 26pt; FONT-FAMILY: &apos;Comic Sans MS&apos;&quot;&gt;: &lt;SPAN style=&quot;COLOR: green&quot;&gt;the butcher’s &lt;/SPAN&gt;keen&lt;SPAN style=&quot;COLOR: green&quot;&gt; knife cut through the meat&lt;/SPAN&gt;&lt;SPAN style=&quot;mso-spacerun: yes&quot;&gt;  &lt;/SPAN&gt;&lt;o:p&gt;&lt;/o:p&gt;&lt;/SPAN&gt;&lt;/P&gt;
&lt;P class=MsoNormal style=&quot;MARGIN: 0cm 0cm 0pt&quot; align=left&gt;&lt;SPAN style=&quot;FONT-SIZE: 26pt; COLOR: red; FONT-FAMILY: &apos;Comic Sans MS&apos;&quot;&gt;B&lt;/SPAN&gt;&lt;SPAN style=&quot;FONT-SIZE: 26pt; FONT-FAMILY: &apos;Comic Sans MS&apos;&quot;&gt;: &lt;SPAN style=&quot;COLOR: #339966&quot;&gt;my dog has a &lt;/SPAN&gt;keen&lt;SPAN style=&quot;COLOR: #339966&quot;&gt; sense of smell&lt;/SPAN&gt;&lt;o:p&gt;&lt;/o:p&gt;&lt;/SPAN&gt;&lt;/P&gt;
&lt;P align=left&gt;&lt;SPAN style=&quot;FONT-SIZE: 26pt; COLOR: red; FONT-FAMILY: &apos;Comic Sans MS&apos;; mso-fareast-font-family: &apos;Times New Roman&apos;; mso-bidi-font-family: &apos;Times New Roman&apos;; mso-ansi-language: EN-US; mso-fareast-language: EN-US; mso-bidi-language: FA&quot;&gt;C&lt;/SPAN&gt;&lt;SPAN style=&quot;FONT-SIZE: 26pt; FONT-FAMILY: &apos;Comic Sans MS&apos;; mso-fareast-font-family: &apos;Times New Roman&apos;; mso-bidi-font-family: &apos;Times New Roman&apos;; mso-ansi-language: EN-US; mso-fareast-language: EN-US; mso-bidi-language: FA&quot;&gt;: &lt;SPAN style=&quot;COLOR: lime&quot;&gt;Bill’s &lt;/SPAN&gt;keen&lt;SPAN style=&quot;COLOR: lime&quot;&gt; mind pleased all his teachers&lt;/SPAN&gt;&lt;/SPAN&gt;&lt;/P&gt;</description>
<pubDate>Wed, 09 Jul 2008 12:09:18 GMT</pubDate>
<comments>http://commenting.blogfa.com/?blogid=lovelyenglish&amp;postid=39</comments>
<dc:creator>lovelyenglish</dc:creator>
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