lambda_handler: Update feeds

apod.json

@@ -1,6 +1,21 @@
 {
     "version": "https://jsonfeed.org/version/1.1",
     "items": [
+        {
+            "id": "https://apod.nasa.gov/apod/ap240724.html",
+            "url": "https://apod.nasa.gov/apod/ap240724.html",
+            "title": "Exaggerated Moon",
+            "content_html": "<p class=\"summary\" hidden=\"hidden\">Our Moon doesn't really have craters this big. Earth's Moon, Luna, also doesn't naturally show this spikey texture, and its colors are more subtle. But this digital creation is based on reality. The featured image is a digital composite of a good Moon image and surface height data taken from NASA's Lunar Orbiter Laser Altimeter (LOLA) mission -- and then exaggerated for educational understanding. The digital enhancements, for example, accentuate lunar highlands and show more clearly craters that illustrate the tremendous bombardment our Moon has been through during its 4.6-billion-year history. The dark areas, called maria, have fewer craters and were once seas of molten lava. Additionally, the image colors, although based on the moon's real composition, are changed and exaggerated. Here, a blue hue indicates a region that is iron rich, while orange indicates a slight excess of aluminum. Although the Moon has shown the same side to the Earth for billions of years, modern technology is allowing humanity to learn much more about it -- and how it affects the Earth.</p><figure><a href=\"image/2407/ExaggeratedMoon_Ibatulin_2610.jpg\"> <img src=\"image/2407/ExaggeratedMoon_Ibatulin_960.jpg\" alt=\"Earth's Moon is shown with the heights of surface features all greatly exaggerated. Also, the colors of the Moon have been exaggerated so areas of blue and red are more easily seen. Please see the explanation for more detailed information.\" style=\"max-width:100%\"></a> <figcaption><p><b> Credit: </b> Data: <a href=\"https://www.nasa.gov/\">NASA</a>, <a href=\"https://science.nasa.gov/mission/lro/lola/\">Lunar Orbiter Laser Altimeter</a>; Image &amp; Processing: <a href=\"https://www.instagram.com/_ibatullin_ildar_/\">Ildar Ibatullin</a> </p></figcaption></figure><p> <b> Explanation: </b> Our Moon doesn't really have craters this big. <a href=\"https://science.nasa.gov/moon/\">Earth's Moon</a>, Luna, also doesn't naturally show this spikey texture, and its colors are more subtle. But this digital creation is based on reality. The <a href=\"https://www.instagram.com/p/C9VolwSsvhk/\">featured image</a> is a digital composite of a good Moon image and surface height data taken from NASA's <a href=\"https://science.nasa.gov/mission/lro/lola/\">Lunar Orbiter Laser Altimeter</a> (LOLA) mission -- and then exaggerated for <a href=\"https://images-wixmp-ed30a86b8c4ca887773594c2.wixmp.com/f/fc529a49-3f59-4502-a7c3-5ac4c3c5a032/d5q4hbz-5b803f71-04b3-47a3-a27c-8f49425d3d8c.jpg?token=eyJ0eXAiOiJKV1QiLCJhbGciOiJIUzI1NiJ9.eyJzdWIiOiJ1cm46YXBwOjdlMGQxODg5ODIyNjQzNzNhNWYwZDQxNWVhMGQyNmUwIiwiaXNzIjoidXJuOmFwcDo3ZTBkMTg4OTgyMjY0MzczYTVmMGQ0MTVlYTBkMjZlMCIsIm9iaiI6W1t7InBhdGgiOiJcL2ZcL2ZjNTI5YTQ5LTNmNTktNDUwMi1hN2MzLTVhYzRjM2M1YTAzMlwvZDVxNGhiei01YjgwM2Y3MS0wNGIzLTQ3YTMtYTI3Yy04ZjQ5NDI1ZDNkOGMuanBnIn1dXSwiYXVkIjpbInVybjpzZXJ2aWNlOmZpbGUuZG93bmxvYWQiXX0.zOT8uNXcb5eNG6mmR7iiEuPGjUE8u35YDhheTEmE8lM\">educational understanding</a>. The digital enhancements, for example, accentuate <a href=\"https://www.lpi.usra.edu/exploration/education/hsResearch/presentations/2017-2018/Henry-M-Jackson-Moon-a.pdf\">lunar highlands</a> and show more clearly craters that illustrate the <a href=\"https://en.wikipedia.org/wiki/Late_Heavy_Bombardment\">tremendous bombardment</a> our Moon has been through during its <a href=\"https://science.nasa.gov/moon/composition/#otp_lunar_origins\">4.6-billion-year history</a>. The <a href=\"https://en.wikipedia.org/wiki/Lunar_mare#/media/File:Moon_names.svg\">dark areas</a>, called <a href=\"https://en.wikipedia.org/wiki/Lunar_mare\">maria</a>, have fewer <a href=\"https://youtu.be/HTukFx17Ryg\">craters</a> and were once seas of <a href=\"https://youtu.be/wiRdr5LzbwY\">molten lava</a>. Additionally, the image <a href=\"ap210831.html\">colors</a>, although based on the moon's real composition, are changed and exaggerated. Here, a blue hue indicates a region that is <a href=\"https://astrobiology.nasa.gov/news/a-story-of-iron-in-ancient-sediments/\">iron rich</a>, while orange indicates a slight excess of <a href=\"https://youtu.be/ZVkpQKRgHvU\">aluminum</a>. Although the <a href=\"https://spaceplace.nasa.gov/all-about-the-moon/en/\">Moon</a> has shown the same side to the Earth for billions of years, <a href=\"ap140113.html\">modern technology</a> is allowing humanity to learn <a href=\"ap190717.html\">much more</a> about it -- and how it <a href=\"https://www.iop.org/explore-physics/moon/how-does-moon-affect-earth\">affects the Earth</a>. </p><footer class=\"footnote\"> <hr><b> Authors &amp; editors: </b> <a href=\"http://www.phy.mtu.edu/faculty/Nemiroff.html\">Robert Nemiroff</a> (<a href=\"http://www.phy.mtu.edu/\">MTU</a>) &amp; <a href=\"https://antwrp.gsfc.nasa.gov/htmltest/jbonnell/www/bonnell.html\">Jerry Bonnell</a> (<a href=\"http://www.astro.umd.edu/\">UMCP</a>)<br> <b>NASA Official: </b> Amber Straughn <a href=\"lib/about_apod.html#srapply\">Specific rights apply</a>. <a href=\"https://www.nasa.gov/about/highlights/HP_Privacy.html\">NASA Web Privacy</a>, <a href=\"https://www.nasa.gov/general/accessibility/\">Accessibility</a>, <a href=\"https://www.nasa.gov/privacy/\">Notices</a>; <br> <b>A service of:</b> <a href=\"https://astrophysics.gsfc.nasa.gov/\">ASD</a> at <a href=\"https://www.nasa.gov/\">NASA</a> / <a href=\"https://www.nasa.gov/centers/goddard/\">GSFC</a>, <br> <a href=\"https://science.nasa.gov/learners\">NASA Science Activation</a> &amp; <a href=\"http://www.mtu.edu/\">Michigan Tech. U.</a><br> </footer>",
+            "date_published": "2024-07-24T12:00:00Z",
+            "date_modified": "2024-07-24T09:00:21+00:00Z",
+            "image": "https://apod.nasa.gov/apod/image/2407/ExaggeratedMoon_Ibatulin_960.jpg",
+            "tags": [
+                "Moon",
+                "surface",
+                "craters"
+            ],
+            "summary": "Our Moon doesn't really have craters this big. Earth's Moon, Luna, also doesn't naturally show this spikey texture, and its colors are more subtle. But this digital creation is based on reality. The featured image is a digital composite of a good Moon image and surface height data taken from NASA's Lunar Orbiter Laser Altimeter (LOLA) mission -- and then exaggerated for educational understanding. The digital enhancements, for example, accentuate lunar highlands and show more clearly craters that illustrate the tremendous bombardment our Moon has been through during its 4.6-billion-year history. The dark areas, called maria, have fewer craters and were once seas of molten lava. Additionally, the image colors, although based on the moon's real composition, are changed and exaggerated. Here, a blue hue indicates a region that is iron rich, while orange indicates a slight excess of aluminum. Although the Moon has shown the same side to the Earth for billions of years, modern technology is allowing humanity to learn much more about it -- and how it affects the Earth."
+        },
         {
             "id": "https://apod.nasa.gov/apod/ap240723.html",
             "url": "https://apod.nasa.gov/apod/ap240723.html",
@@ -440,21 +455,6 @@
                 "globular cluster"
             ],
             "summary": "What is that strange brown ribbon on the sky? When observing the star cluster NGC 4372, observers frequently take note of an unusual dark streak nearby running about three degrees in length. The streak, actually a long molecular cloud, has become known as the Dark Doodad Nebula. (Doodad is slang for a thingy or a whatchamacallit.) Pictured here, the Dark Doodad Nebula sweeps across the center of a rich and colorful starfield. Its dark color comes from a high concentration of interstellar dust that preferentially scatters visible light. The globular star cluster NGC 4372 is visible as the fuzzy white spot on the far left, while the bright blue star gamma Muscae is seen to the cluster's upper right. The Dark Doodad Nebula can be found with strong binoculars toward the southern constellation of the Fly (Musca)."
-        },
-        {
-            "id": "https://apod.nasa.gov/apod/ap240624.html",
-            "url": "https://apod.nasa.gov/apod/ap240624.html",
-            "title": "JADES-GS-z14-0: A New Farthest Object",
-            "content_html": "<p class=\"summary\" hidden=\"hidden\">What if we could see back to the beginning of the universe? We could see galaxies forming. But what did galaxies look like back then? These questions took a step forward recently with the release of the analysis of a James Webb Space Telescope (JWST) image that included the most distant object yet discovered. Most galaxies formed at about 3 billion years after the Big Bang, but some formed earlier. Pictured in the inset box is JADES-GS-z14-0, a faint smudge of a galaxy that formed only 300 million years after the universe started. In technical terms, this galaxy lies at the record redshift of z=14.32, and so existed when the universe was only one fiftieth of the its present age. Practically all of the objects in the featured photograph are galaxies.</p><figure><a href=\"image/2406/MostDistantGalaxy_Webb_960.jpg\"> <img src=\"image/2406/MostDistantGalaxy_Webb_960.jpg\" alt=\"A dark field is shown filled with smudges that are distant galaxies. One smudge is expanded in an inset box. This box shows a reddish elongated object. Please see the explanation for more detailed information.\" style=\"max-width:100%\"></a> <figcaption><p><b> Image Credit: </b> <a href=\"https://www.nasa.gov/\">NASA</a>, <a href=\"https://www.esa.int/\">ESA</a>, <a href=\"https://www.asc-csa.gc.ca/eng/\">CSA</a>, <a href=\"https://www.stsci.edu/\">STScI</a>, <a href=\"https://www.astro.ucsc.edu/faculty/index.php?uid=brant\">B. Robertson</a> (<a href=\"https://www.astro.ucsc.edu/\">UC Santa Cruz</a>), B. Johnson (CfA), S. Tacchella (Cambridge), P. Cargile (CfA) </p></figcaption></figure><p> <b> Explanation: </b> What if we could see back to the beginning of the universe? We could see galaxies forming. But what did <a href=\"ap210802.html\">galaxies look like</a> back then? These questions took a step forward recently with the <a href=\"https://arxiv.org/abs/2405.18485\">release of the analysis</a> of a <a href=\"https://webb.nasa.gov/content/about/index.html\">James Webb Space Telescope</a> (JWST) image that included the most distant object yet discovered. Most <a href=\"https://science.nasa.gov/universe/galaxies/evolution/\">galaxies formed</a> at about 3 billion years after the <a href=\"https://en.wikipedia.org/wiki/Big_Bang\">Big Bang</a>, but some formed earlier. <a href=\"https://webbtelescope.org/contents/early-highlights/nasas-james-webb-space-telescope-finds-most-distant-known-galaxy\">Pictured</a> in the inset box is <a href=\"https://jades-survey.github.io/\">JADES</a>-<a href=\"https://esawebb.org/images/jades4/\">GS-z14-0</a>, a faint smudge of <a href=\"ap230531.html\">a galaxy that formed</a> only 300 million years after the <a href=\"ap231231.html\">universe started</a>. In technical terms, this galaxy lies at the record <a href=\"ap130408.html\">redshift</a> of z=14.32, and so existed when the <a href=\"https://imagine.gsfc.nasa.gov/science/featured_science/tenyear/age.html\">universe</a> was only one fiftieth of the its present age. <a href=\"https://encrypted-tbn0.gstatic.com/images?q=tbn:ANd9GcQCn05AuCb0JVqZCnh5FzGXDqXOtri0W2cwEw&amp;s\">Practically all</a> of the objects in the <a href=\"https://webbtelescope.org/contents/media/images/01HZ083EXXCJNE64ERAH2ER2FM\">featured photograph</a> are galaxies. </p><footer class=\"footnote\"> <hr><b> Authors &amp; editors: </b> <a href=\"http://www.phy.mtu.edu/faculty/Nemiroff.html\">Robert Nemiroff</a> (<a href=\"http://www.phy.mtu.edu/\">MTU</a>) &amp; <a href=\"https://antwrp.gsfc.nasa.gov/htmltest/jbonnell/www/bonnell.html\">Jerry Bonnell</a> (<a href=\"http://www.astro.umd.edu/\">UMCP</a>)<br> <b>NASA Official: </b> Amber Straughn <a href=\"lib/about_apod.html#srapply\">Specific rights apply</a>. <a href=\"https://www.nasa.gov/about/highlights/HP_Privacy.html\">NASA Web Privacy</a>, <a href=\"https://www.nasa.gov/general/accessibility/\">Accessibility</a>, <a href=\"https://www.nasa.gov/privacy/\">Notices</a>; <br> <b>A service of:</b> <a href=\"https://astrophysics.gsfc.nasa.gov/\">ASD</a> at <a href=\"https://www.nasa.gov/\">NASA</a> / <a href=\"https://www.nasa.gov/centers/goddard/\">GSFC</a>, <br> <a href=\"https://science.nasa.gov/learners\">NASA Science Activation</a> &amp; <a href=\"http://www.mtu.edu/\">Michigan Tech. U.</a><br> </footer>",
-            "date_published": "2024-06-24T12:00:00Z",
-            "date_modified": "2024-06-24T09:00:03+00:00Z",
-            "image": "https://apod.nasa.gov/apod/image/2406/MostDistantGalaxy_Webb_960.jpg",
-            "tags": [
-                "star formation",
-                "early universe",
-                "JWST"
-            ],
-            "summary": "What if we could see back to the beginning of the universe? We could see galaxies forming. But what did galaxies look like back then? These questions took a step forward recently with the release of the analysis of a James Webb Space Telescope (JWST) image that included the most distant object yet discovered. Most galaxies formed at about 3 billion years after the Big Bang, but some formed earlier. Pictured in the inset box is JADES-GS-z14-0, a faint smudge of a galaxy that formed only 300 million years after the universe started. In technical terms, this galaxy lies at the record redshift of z=14.32, and so existed when the universe was only one fiftieth of the its present age. Practically all of the objects in the featured photograph are galaxies."
         }
     ],
     "title": "Astronomy Picture of the Day",

arloandjanis.xml

@@ -6,8 +6,23 @@
     </author>
     <link href="https://meissnem.github.io/feeds/arloandjanis.xml" rel="self" />
     <link href="https://www.gocomics.com/arloandjanis" rel="alternate" type="text/html" />
-    <updated>2024-07-23T04:00:30.092893-05:00</updated>
+    <updated>2024-07-24T04:00:47.916344-05:00</updated>
     <id>https://www.gocomics.com/arloandjanis</id>
+    <entry>
+        <title type="text">Arlo and Janis - July 24, 2024</title>
+        <link href="https://www.gocomics.com/arloandjanis/2024/07/24" />
+        <id>https://www.gocomics.com/arloandjanis/2024/07/24</id>
+        <author>
+            <name>Jimmy Johnson</name>
+        </author>
+        <published>2024-07-24T05:00:00-05:00</published>
+        <updated>2024-07-24T05:00:00-05:00</updated>
+        <content type="xhtml">
+            <figure xmlns="http://www.w3.org/1999/xhtml">
+                <img src="https://assets.amuniversal.com/c46c8ea025aa013d612b005056a9545d" />
+            </figure>
+        </content>
+    </entry>
     <entry>
         <title type="text">Arlo and Janis - July 23, 2024</title>
         <link href="https://www.gocomics.com/arloandjanis/2024/07/23" />

babyblues.xml

@@ -6,8 +6,23 @@
     </author>
     <link href="https://meissnem.github.io/feeds/babyblues.xml" rel="self" />
     <link href="https://www.gocomics.com/babyblues" rel="alternate" type="text/html" />
-    <updated>2024-07-23T04:00:31.917846-05:00</updated>
+    <updated>2024-07-24T04:00:49.652145-05:00</updated>
     <id>https://www.gocomics.com/babyblues</id>
+    <entry>
+        <title type="text">Baby Blues - July 24, 2024</title>
+        <link href="https://www.gocomics.com/babyblues/2024/07/24" />
+        <id>https://www.gocomics.com/babyblues/2024/07/24</id>
+        <author>
+            <name>Rick Kirkman and Jerry Scott</name>
+        </author>
+        <published>2024-07-24T05:00:00-05:00</published>
+        <updated>2024-07-24T05:00:00-05:00</updated>
+        <content type="xhtml">
+            <figure xmlns="http://www.w3.org/1999/xhtml">
+                <img src="https://assets.amuniversal.com/62d05b3025d8013d6147005056a9545d" />
+            </figure>
+        </content>
+    </entry>
     <entry>
         <title type="text">Baby Blues - July 23, 2024</title>
         <link href="https://www.gocomics.com/babyblues/2024/07/23" />

calvinandhobbes.xml

@@ -6,8 +6,24 @@
     </author>
     <link href="https://meissnem.github.io/feeds/calvinandhobbes.xml" rel="self" />
     <link href="https://www.gocomics.com/calvinandhobbes" rel="alternate" type="text/html" />
-    <updated>2024-07-23T04:00:33.695215-05:00</updated>
+    <updated>2024-07-24T04:00:51.462909-05:00</updated>
     <id>https://www.gocomics.com/calvinandhobbes</id>
+    <entry>
+        <title type="text">Calvin and Hobbes - July 25, 1989</title>
+        <link href="https://www.gocomics.com/calvinandhobbes/1989/07/25" />
+        <id>https://www.gocomics.com/calvinandhobbes/1989/07/25</id>
+        <author>
+            <name>Bill Watterson</name>
+        </author>
+        <published>2024-07-25T05:00:00-05:00</published>
+        <updated>2024-07-25T05:00:00-05:00</updated>
+        <content type="xhtml">
+            <figure xmlns="http://www.w3.org/1999/xhtml">
+                <img src="https://assets.amuniversal.com/ebe76ab0deca013171a6005056a9545d" />
+                <figcaption>Originally published July 25, 1989</figcaption>
+            </figure>
+        </content>
+    </entry>
     <entry>
         <title type="text">Calvin and Hobbes - July 24, 1989</title>
         <link href="https://www.gocomics.com/calvinandhobbes/1989/07/24" />

crankshaft.xml

@@ -6,8 +6,23 @@
     </author>
     <link href="https://meissnem.github.io/feeds/crankshaft.xml" rel="self" />
     <link href="https://www.gocomics.com/crankshaft" rel="alternate" type="text/html" />
-    <updated>2024-07-23T04:00:35.070745-05:00</updated>
+    <updated>2024-07-24T04:00:52.732107-05:00</updated>
     <id>https://www.gocomics.com/crankshaft</id>
+    <entry>
+        <title type="text">Crankshaft - July 24, 2024</title>
+        <link href="https://www.gocomics.com/crankshaft/2024/07/24" />
+        <id>https://www.gocomics.com/crankshaft/2024/07/24</id>
+        <author>
+            <name>Tom Batiuk and Dan Davis</name>
+        </author>
+        <published>2024-07-24T05:00:00-05:00</published>
+        <updated>2024-07-24T05:00:00-05:00</updated>
+        <content type="xhtml">
+            <figure xmlns="http://www.w3.org/1999/xhtml">
+                <img src="https://assets.amuniversal.com/61f2efe0250f013d60fd005056a9545d" />
+            </figure>
+        </content>
+    </entry>
     <entry>
         <title type="text">Crankshaft - July 23, 2024</title>
         <link href="https://www.gocomics.com/crankshaft/2024/07/23" />

fminus.xml

@@ -6,8 +6,23 @@
     </author>
     <link href="https://meissnem.github.io/feeds/fminus.xml" rel="self" />
     <link href="https://www.gocomics.com/fminus" rel="alternate" type="text/html" />
-    <updated>2024-07-23T04:00:36.916402-05:00</updated>
+    <updated>2024-07-24T04:00:54.510215-05:00</updated>
     <id>https://www.gocomics.com/fminus</id>
+    <entry>
+        <title type="text">F Minus - July 24, 2024</title>
+        <link href="https://www.gocomics.com/fminus/2024/07/24" />
+        <id>https://www.gocomics.com/fminus/2024/07/24</id>
+        <author>
+            <name>Tony Carrillo</name>
+        </author>
+        <published>2024-07-24T05:00:00-05:00</published>
+        <updated>2024-07-24T05:00:00-05:00</updated>
+        <content type="xhtml">
+            <figure xmlns="http://www.w3.org/1999/xhtml">
+                <img src="https://assets.amuniversal.com/022552e022b0013d6091005056a9545d" />
+            </figure>
+        </content>
+    </entry>
     <entry>
         <title type="text">F Minus - July 23, 2024</title>
         <link href="https://www.gocomics.com/fminus/2024/07/23" />