<div style="margin: 12px 0px; font-family: arial; color: #333333; background: #ffffff; border: solid 4px #e5e5e5; width: 100%; clear: left;"><div class="CM_CTB_Content_Wrap" style="margin: 0px; padding: 0px;background-color: #ffffff;"><div style="border-bottom: solid 1px #dcdcdc; white-space: nowrap; margin-bottom: 8px; background-color: #eeeeee ;background-image: url(http://www.clipmarks.com/images/source-bg.gif); background-repeat: repeat-x; height: 24px; line-height: 24px; vertical-align: middle; padding-bottom: 4px; color: #666666; font-size: 10px;" ><a href="http://clipmarks.com/clip-to-blog/" title="see clips that are hot right now"><img src="http://content.clipmarks.com/blog_embed/c552a420-cbe4-4c71-a8f2-3b9206bee77c/E7DA7633-F822-48C3-9069-CCDA147A2E3D/" alt="" width="19" height="19" border="0" style="vertical-align: middle; margin: 0px 4px; display: inline; border: none; float:none;" /></a>clipped from <a title="http://www.space.com/scienceastronomy/070717_st_rare_hjups.html" href="http://www.space.com/scienceastronomy/070717_st_rare_hjups.html" style="font-size: 11px;">www.space.com</a></div><blockquote style="text-align: left; padding: 0px 8px; margin: 4px 0px 8px 0px; background: transparent; border: none;" cite="http://www.space.com/scienceastronomy/070717_st_rare_hjups.html">The majority of extrasolar planets known were found using the <A href="http://www.space.com/searchforlife/seti_wobble_method_010523.html">radial velocity</A> method, which involves measuring the stellar wobbles caused by planets gravitationally tugging on their stars. Because this technique is best suited to detecting massive planets close to their stars (large planets located close to their stars create the biggest wobbles), astronomers were unsure whether more gas giants could be found at a greater distance from their stars via different detection methods.</blockquote><div style="height: 2px; font-size: 2px; background: #dcdcdc; border-bottom: solid 1px #f5f5f5; margin: 2px 4px;"></div><blockquote style="text-align: left; padding: 0px 8px; margin: 4px 0px 8px 0px; background: transparent; border: none;" cite="http://www.space.com/scienceastronomy/070717_st_rare_hjups.html">To answer this question, Biller and her colleagues conducted a three-year survey using telescopes in Arizona and Chile. The team looked specifically for gas giants residing relatively far from their parent stars. They surveyed 54 nearby, young stars where gas giant planets would still be forming. Theory predicts young Jupiters are brighter and thus easier to spot than older gas giants.</blockquote></div><div style="margin: 0px 6px 6px 4px;"><table style="font-size: 11px;border-spacing: 0px;padding: 0px;" cellpadding="0" cellspacing="0" width="100%"><tr><td style="background:transparent;border-width:0px;padding:0px;">&nbsp;</td><td align="right" style="background:transparent;border-width:0px;padding:0px;width:107px" width="107"><a href="http://clipmarks.com/share/E7DA7633-F822-48C3-9069-CCDA147A2E3D/blog/" title="blog or email this clip"><img src="http://content8.clipmarks.com/images/c2b-foot.png" border="0" alt="blog it" width="107" height="17" style="border-width:0px;padding:0px;margin:0px;" /></a></td></tr></table></div></div>

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