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Catalog Page for PIA06939
<!DOCTYPE html PUBLIC "-//W3C//DTD XHTML 1.0 Transitional//EN" "http://www.w3.org/TR/xhtml1/DTD/xhtml1-transitional.dtd"> <html xmlns="http://www.w3.org/1999/xhtml"> <head> <title>Catalog Page for PIA06939</title> <link href="/css/main.css" rel="stylesheet" type="text/css" /> <!-- <link rel="alternate" type="application/rss+xml" title="Catalog Page for PIA06939" href="photojournal.jpl.nasa.gov:8443/rss/catalog/PIA06939"/> --> <!-- Google Analytics added 08-16-2013 --> <script id="_fed_an_js_tag" type="text/javascript" src="/js/federatedanalytics.all.min.js?agency=NASA&subagency=JPL-Photojournal"> </script> </head> <body> <!-- SiteCatalyst code version: H.20.3. Copyright 1997-2009 Omniture, Inc. 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NASA's Spitzer Space Telescope show that these catastrophes continue to occur around stars even after they have developed full-sized planets." /></a> </div> <img src="https://www.jpl.nasa.gov/images/spacer.gif" height="4px" /> </td> <td align="center"> <table border="0" width="auto"> <tr bgcolor=#eeeeee> <td align="right" bgcolor="#003366"><font size="-1" color="#ffffff"> Mission: </font></td> <td align="left"><strong> <A HREF="http://www.spitzer.caltech.edu/spitzer/" target="_blank">Spitzer Space Telescope</A> <br/> </strong></td> </tr> <tr bgcolor=#eeeeee> <td align="right" bgcolor="#003366"><font size="-1" color="#ffffff"> Instrument: </font></td> <td align="left"><strong> <A HREF="http://www.spitzer.caltech.edu/mission/398-The-Infrared-Array-Camera-IRAC-" target="_blank">IRAC</A> <br/> </strong></td> </tr> <tr bgcolor=#eeeeee> <td align="right" bgcolor="#003366"><font size="-1" color="#ffffff"> Product Size: </font></td> <td align="left"><strong>3000 x 2400 pixels (w x h)</strong> </td> </tr> <tr bgcolor=#eeeeee> <td align="right" bgcolor="#003366"><font size="-1" color="#ffffff"> Produced By: </font></td> <td align="left"><strong> California Institute of Technology <br/> </strong></td> </tr> <tr bgcolor=#eeeeee> <td align="right" bgcolor="#003366"> <font size="-1" color="#ffffff"> Full-Res TIFF: </font> </td> <td align="left"> <strong> <a href="/tiff/PIA06939.tif">PIA06939.tif</a> (4.159 MB) </strong> </td> </tr> <tr bgcolor=#eeeeee> <td align="right" bgcolor="#003366"> <font size="-1" color="#ffffff"> Full-Res JPEG: </font> </td> <td align="left"> <strong> <a href="/jpeg/PIA06939.jpg">PIA06939.jpg</a> (301.4 kB) </strong>  </td> </tr> </table> </td></tr> </table> <p> </p> <table border="0" width="960" style="font-family:Verdana, Arial, Helvetica, sans-serif;"> <tr><td bgcolor="#cccccc" align="center"> <font size="-2"> <b>Click on the image above to download a moderately sized image in JPEG format (possibly reduced in size from original)</b><br /> </font> </td></tr></table> <p> </p> <table border="0" width="960"> <tr><td bgcolor="#ffffff" align="left"> <dl> <dt> <b>Original Caption Released with Image: </b> </dt> <dd> <p><center><a href="https://photojournal.jpl.nasa.gov/figures/PIA06939_fig1.jpg"><img src="https://photojournal.jpl.nasa.gov/figures/PIA06939_fig1_thumb.jpg" alt="figure 1 for PIA06939"></a><br>Figure 1</center></p><center><table border="0"><tr><td align="center"><a href="https://photojournal.jpl.nasa.gov/figures/PIA06939_fig1_a.jpg"><img src="https://photojournal.jpl.nasa.gov/figures/PIA06939_fig1_a_thumb.jpg" alt="panel A of figure 1 for PIA06939"></a></td><td align="center"><a href="https://photojournal.jpl.nasa.gov/figures/PIA06939_fig1_b.jpg"><img src="https://photojournal.jpl.nasa.gov/figures/PIA06939_fig1_b_thumb.jpg" alt="panel B of figure 1 for PIA06939"><td align="center"><a href="https://photojournal.jpl.nasa.gov/figures/PIA06939_fig1_c.jpg"><img src="https://photojournal.jpl.nasa.gov/figures/PIA06939_fig1_c_thumb.jpg" alt="panel C of figure 1 for PIA06939"></a></td></tr><tr><td align="center">Panel A of Inset</td><td align="center"> Panel B of Inset </td><td align="center"> Panel C of Inset </td></tr></table></center></p><p>This artist's concept illustrates how planetary systems arise out of massive collisions between rocky bodies. New findings from NASA's Spitzer Space Telescope show that these catastrophes continue to occur around stars even after they have developed full-sized planets, when they are as old as one hundred million years. For reference, our own Sun, at 4.5 billion years old, is far past this late stage of planet formation.</p><p>In this image, a young star is shown circled by full-sized planets, and rings of dust beyond. These rings, also called "debris discs," arise when embryonic planets smash into each other. One of these collisions is illustrated in the inset of Figure 1. </p><p>Spitzer was able to see the dust generated by these collisions with its powerful infrared vision.<p> </dd> <dt> <b>Image Credit: </b></dt> <dd> NASA/JPL-Caltech</dd> <dt><br/><b>Image Addition Date: </b></dt> <dd> 2004-10-18</dd> </dl> </td></tr> </table> <!-- <hr width="960" align="center"></hr> --> </div> </div> </div> <!-- footer --> <div id="wrapper_bottom"> <script type="text/javascript" src="/js/footer.js"> </script> </div> <!-- end footer --> </body> </html>