diff --git a/public/ngc628_datasets.wtml b/public/ngc628_datasets.wtml
index 0ed3d64..244b2de 100644
--- a/public/ngc628_datasets.wtml
+++ b/public/ngc628_datasets.wtml
@@ -131,7 +131,7 @@
       </ImageSet>
     </ForegroundImageSet>
   </Place>
-  <Place
+  <!-- <Place
     Angle="0"
     AngularSize="0"
     Constellation="PSC"
@@ -172,14 +172,14 @@
         <ThumbnailUrl>http://wwtfiles.blob.core.windows.net/vamp/thumb-Wise-WISE2011-020b.jpg</ThumbnailUrl>
       </ImageSet>
     </ForegroundImageSet>
-  </Place>
-  <!-- <Place Angle="0"
+  </Place> -->
+  <Place Angle="0"
     AngularSize="0"
     Constellation="PSC"
     DataSetType="Sky"
     Dec="15.783830080030844"
     Magnitude="0"
-    Name="Infrared (Spitzer)"
+    Name="2023 Infrared (Spitzer)"
     Opacity="100"
     RA="1.6116031114664884"
     Rotation="0"
@@ -196,7 +196,7 @@
         ElevationModel="False"
         FileType=".png"
         Generic="False"
-        Name="Infrared (Spitzer)"
+        Name="2023 Infrared (Spitzer)"
         OffsetX="-5.2158523543506065e-05"
         OffsetY="-5.2158661456566194e-05"
         Projection="Tan"
@@ -222,7 +222,7 @@ In this image, infrared light at wavelengths of 3.6, 4.5, and 8.0 microns from S
         <ThumbnailUrl>https://raw.githubusercontent.com/johnarban/data_repo/main/spitzer_ngc628/thumb.jpg</ThumbnailUrl>
       </ImageSet>
     </ForegroundImageSet>
-  </Place> -->
+  </Place>
   <Place Angle="0"
     AngularSize="0"
     Constellation="PSC"
diff --git a/src/BubblingGalaxies.vue b/src/BubblingGalaxies.vue
index 70e10f8..3499390 100644
--- a/src/BubblingGalaxies.vue
+++ b/src/BubblingGalaxies.vue
@@ -604,6 +604,10 @@ const labelTitles: Record<PhantomImageNames | string, LabelInfo> = {
   "2011 Infrared Dust (WISE)": {
     title: "2011 Colder Infrared, WISE",
     content: "",
+  },
+  "2023 Infrared (Spitzer)": {
+    title: "2023 Infrared, Spitzer",
+    content: "",
   }
 };
 
diff --git a/src/components/ImageText.vue b/src/components/ImageText.vue
index 921a2e7..ac1d961 100644
--- a/src/components/ImageText.vue
+++ b/src/components/ImageText.vue
@@ -215,6 +215,55 @@
         <cite>Credit: KPNO/NOIRLab/NSF/AURA/Paul Mortfield and Deitmar Kupke/Flynn Haase</cite>
       </p>
     </article>
+
+
+
+    <article
+      v-if="which === '2023 Infrared (Spitzer)'"
+      class="image-text__text"
+    >
+      <h3 v-show="showHeading">
+        Previously On the Phantom Galaxy &ndash; <br /> 2023 Spitzer Infrared
+      </h3>
+
+      <p>
+        Messier 74, also known as the Phantom Galaxy, is seen here in infrared light which showcases its sweeping spiral
+        arms and star-forming regions. This image was created using archival data from NASA's Spitzer Space Telescope,
+        revealing dust clouds that, in visible light, appear dark.
+      </p>
+
+      <p>
+        Messier 74 is an archetype of the "grand design" spiral galaxy and is nearly face-on to our view, providing a
+        perfect view of its structure. In this infrared image, the light from stars appears blue, as stars are brightest
+        at shorter wavelengths of infrared light and less visible at longer wavelengths.
+      </p>
+
+      <p>
+        Filamentary dust clouds are a feature of spiral arms, and help to trace regions where gas reaches higher
+        densities
+        and can lead to the formation of stars. These clouds light up at longer wavelengths of light, appearing as pale
+        yellow filaments. Regions of newly-forming stars show up as bright red dots scattered along the arms, as they
+        glow
+        most brightly at the longest infrared wavelengths in this image.
+      </p>
+
+      <p>
+        The galaxy is located in the Pisces constellation and is situated about 30 million light-years away. It has a
+        visible diameter of approximately 10 arc minutes, which is about a third as wide as the full moon. However, its
+        low surface brightness makes it too faint to be seen with the naked eye and makes it a challenging target even
+        for small backyard telescopes.
+      </p>
+
+      <p>
+        In this image, infrared light at wavelengths of 3.6, 4.5, and 8.0 microns from Spitzer’s IRAC instrument is
+        displayed as blue, cyan, and green, respectively, while light from Spitzer’s MIPS instrument at 24 microns is
+        shown in red.
+      </p>
+
+      <p class="image-text__credit">
+        <cite>Image &amp; Text Credit: ASA/JPL-Caltech</cite>
+      </p>
+    </article>
   </div>
 </template>
 <script setup lang="ts">
diff --git a/src/types.ts b/src/types.ts
index b45eda6..0862449 100644
--- a/src/types.ts
+++ b/src/types.ts
@@ -3,6 +3,7 @@ export type PhantomImageNames =
   | 'Infrared Dust (JWST)'
   | 'Visible Light (Hubble)'
   | '2011 Infrared Dust (WISE)'
+  | '2023 Infrared (Spitzer)'
   | 'Optical (Kitt Peak)'
   | 'simulation'
   ;