To view a still from this video go to: &lt;a href="<a rel="nofollow" class="external free" href="https://www.flickr.com/photos/gsfc/5637802618">https://www.flickr.com/photos/gsfc/5637802618</a>"&gt;www.flickr.com/photos/gsfc/5637802618&lt;/a&gt;
<p>To read more about this release go to: &lt;a href="<a rel="nofollow" class="external free" href="http://www.nasa.gov/mission_pages/hubble/science/hubble-rose.html">http://www.nasa.gov/mission_pages/hubble/science/hubble-rose.html</a>" rel="noreferrer nofollow"&gt;www.nasa.gov/mission_pages/hubble/science/hubble-rose.html&lt;/a&gt;
</p><p>This is a view looking high into a patch of the autumn sky containing the constellations Perseus, Andromeda, and Triangulum.
</p><p>We're zooming into a region of space nestled between the "demon star" Algol on the left, and the star Almaak on the right.
</p><p>Our view goes deeper and narrower into space. It is full of stars that are not visible to the naked eye.
</p><p>Up ahead is a remarkable spiral and S-shaped object that is 300 million light-years beyond our Milky Way.
</p><p>This is the interacting galaxy Arp 273.
</p><p>We'll first zoom into the smaller member of the pair. It is a nearly edge-on galaxy that shows distinct signs of intense star formation at its nucleus.
</p><p>This was perhaps triggered by the encounter with the companion galaxy above.
</p><p>It is gravitationally distorted into a rose-like shape by the tidal pull of the smaller companion galaxy.
</p><p>Video Credit: NASA, ESA, and Z. Levay, G. Bacon, and M. Estacion (STScI)
</p><p>Image Credit: A. Fujii; A. Block (Mount Lemmon SkyCenter, University of Arizona); Digitized Sky Survey (DSS), STScI/AURA, Palomar/Caltech; and the Hubble Heritage Team (STScI/AURA)
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