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      <title>electromagnetic spectrum  by Hailynn Denman</title>
      <link>https://padlet.com/hgdenman01/tgkgemgien8m</link>
      <description>Made with good vibes
hailynn denman</description>
      <language>en-us</language>
      <pubDate>2018-11-14 15:59:43 UTC</pubDate>
      <lastBuildDate>2025-10-07 16:11:34 UTC</lastBuildDate>
      <webMaster>hello@padlet.com</webMaster>
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         <title>what is electromagnetic spectrum</title>
         <author>hgdenman01</author>
         <link>https://padlet.com/hgdenman01/tgkgemgien8m/wish/304370079</link>
         <description><![CDATA[<div>Electromagnetic spectrum is the range of wavelengths or frequencies over which electromagnetic radiation extends.<br><br></div>]]></description>
         <enclosure url="" />
         <pubDate>2018-11-14 16:03:35 UTC</pubDate>
         <guid>https://padlet.com/hgdenman01/tgkgemgien8m/wish/304370079</guid>
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         <title>different waves</title>
         <author>hgdenman01</author>
         <link>https://padlet.com/hgdenman01/tgkgemgien8m/wish/304850091</link>
         <description><![CDATA[<div>This means that it is correct to talk about the energy of an X-ray or the <strong>wavelength</strong> of a <strong>microwave</strong> or the frequency of a <strong>radio wave</strong>. The electromagnetic spectrum includes, from longest <strong>wavelength</strong> to shortest: <strong>radio</strong> waves, microwaves, <strong>infrared</strong>, <strong>optical</strong>,<strong>ultraviolet</strong>, X-rays, and <strong>gamma</strong>-rays.</div>]]></description>
         <enclosure url="" />
         <pubDate>2018-11-15 15:30:33 UTC</pubDate>
         <guid>https://padlet.com/hgdenman01/tgkgemgien8m/wish/304850091</guid>
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         <title>em spectrum used to study space</title>
         <author>hgdenman01</author>
         <link>https://padlet.com/hgdenman01/tgkgemgien8m/wish/304854407</link>
         <description><![CDATA[<div>Astronomers use telescopes to see objects at wavelengths all across the electromagnetic spectrum. Some very hot stars emit <strong>light</strong> primarily at <strong>ultraviolet</strong> wavelengths. There are extremely hot objects that emit <strong>X-rays</strong> and even <strong>gamma rays</strong>. Some very cool stars shine mostly in the <strong>infrared light</strong>wavelengths</div>]]></description>
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         <pubDate>2018-11-15 15:37:34 UTC</pubDate>
         <guid>https://padlet.com/hgdenman01/tgkgemgien8m/wish/304854407</guid>
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      <item>
         <title>type of star is the sun</title>
         <author>hgdenman01</author>
         <link>https://padlet.com/hgdenman01/tgkgemgien8m/wish/304859846</link>
         <description><![CDATA[<div>The Sun is a as a G2V type star, a yellow dwarf and a main <strong>sequence star</strong>. Stars are classified by their spectra (the elements that they absorb) and their temperature. There are seven main types of stars.</div>]]></description>
         <enclosure url="" />
         <pubDate>2018-11-15 15:45:23 UTC</pubDate>
         <guid>https://padlet.com/hgdenman01/tgkgemgien8m/wish/304859846</guid>
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         <title>ems waves that come from the sun</title>
         <author>hgdenman01</author>
         <link>https://padlet.com/hgdenman01/tgkgemgien8m/wish/304861558</link>
         <description><![CDATA[<div>Radiation from the <strong>Sun</strong>. [/caption]Radiation from the <strong>Sun</strong>, which is more popularly known as <strong>sunlight</strong>, is a mixture of<strong>electromagnetic waves</strong> ranging from infrared (IR) to ultraviolet rays (UV). It of course includes visible light, which is in between IR and UV in the <strong>electromagnetic</strong> spectrum.Mar 19, 2010</div>]]></description>
         <enclosure url="" />
         <pubDate>2018-11-15 15:47:52 UTC</pubDate>
         <guid>https://padlet.com/hgdenman01/tgkgemgien8m/wish/304861558</guid>
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         <title>how does the sun effect us on earth</title>
         <author>hgdenman01</author>
         <link>https://padlet.com/hgdenman01/tgkgemgien8m/wish/304862730</link>
         <description><![CDATA[<div>Our Protective Atmosphere. Our <strong>Sun is</strong> a source of energy across the full spectrum, and its<strong>electromagnetic</strong> radiation bombards our atmosphere constantly. However, the <strong>Earth's</strong> atmosphere protects<strong>us</strong> from exposure to a range of higher energy <strong>waves</strong>that <strong>can</strong> be harmful to life.</div>]]></description>
         <enclosure url="" />
         <pubDate>2018-11-15 15:49:28 UTC</pubDate>
         <guid>https://padlet.com/hgdenman01/tgkgemgien8m/wish/304862730</guid>
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      <item>
         <title>what makes the sun differnt than the other stars</title>
         <author>hgdenman01</author>
         <link>https://padlet.com/hgdenman01/tgkgemgien8m/wish/304866190</link>
         <description><![CDATA[<div>Our <strong>Sun</strong> is a bright, hot ball of hydrogen and helium at the center of our solar system. It is 864,000 miles (1,392,000 km) in diameter, <strong>which makes</strong> it 109 times wider than Earth.Aug 15, 2018</div>]]></description>
         <enclosure url="" />
         <pubDate>2018-11-15 15:54:43 UTC</pubDate>
         <guid>https://padlet.com/hgdenman01/tgkgemgien8m/wish/304866190</guid>
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         <title>what is red shift</title>
         <author>hgdenman01</author>
         <link>https://padlet.com/hgdenman01/tgkgemgien8m/wish/304868112</link>
         <description><![CDATA[<div>In physics, redshift happens when light or other electromagnetic radiation from an object undergoes an increase in wavelength. "Redshifting" does not mean that the light is actually red, or actually becomes red.</div>]]></description>
         <enclosure url="" />
         <pubDate>2018-11-15 15:57:36 UTC</pubDate>
         <guid>https://padlet.com/hgdenman01/tgkgemgien8m/wish/304868112</guid>
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      <item>
         <title>blue shift</title>
         <author>hgdenman01</author>
         <link>https://padlet.com/hgdenman01/tgkgemgien8m/wish/305298829</link>
         <description><![CDATA[<div>A blueshift is any decrease in wavelength, with a corresponding increase in frequency, of an electromagnetic wave; the opposite effect is referred to as redshift. In visible light, this shifts the color from the red end of the spectrum to the blue end.</div>]]></description>
         <enclosure url="" />
         <pubDate>2018-11-16 15:31:48 UTC</pubDate>
         <guid>https://padlet.com/hgdenman01/tgkgemgien8m/wish/305298829</guid>
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         <title>how is em spectrum used to stars </title>
         <author>hgdenman01</author>
         <link>https://padlet.com/hgdenman01/tgkgemgien8m/wish/305300203</link>
         <description><![CDATA[<div>By using large infrared telescopes, astronomers have been able to peer through the dust lanes of the Milky Way into the core of our galaxy. The majority of <strong>stars</strong>emit most of their <strong>electromagnetic</strong> energy as visible light, the tiny portion of the <strong>spectrum</strong> to which our eyes are sensitive.</div>]]></description>
         <enclosure url="" />
         <pubDate>2018-11-16 15:34:35 UTC</pubDate>
         <guid>https://padlet.com/hgdenman01/tgkgemgien8m/wish/305300203</guid>
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         <title>how do em spectrum used to galaxys</title>
         <author>hgdenman01</author>
         <link>https://padlet.com/hgdenman01/tgkgemgien8m/wish/305300990</link>
         <description><![CDATA[<div><br></div><div>Meanwhile, the shorter wavelengths measure extremely energetic phenomena. Astronomers <strong>use </strong>the entire <strong>electromagnetic spectrum</strong> to observe a variety of things. ... By using large infrared telescopes, astronomers have been able to peer through the dust lanes of the Milky Way into the core of our <strong>galaxy</strong>.</div>]]></description>
         <enclosure url="" />
         <pubDate>2018-11-16 15:36:07 UTC</pubDate>
         <guid>https://padlet.com/hgdenman01/tgkgemgien8m/wish/305300990</guid>
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