Image:Voyager 1 & 2 positions in 2005.


	Image:Voyager 1 & 2 positions in 2005.

BitDrifter

8-25-2006 6:56 PM

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tags:

nasa, space, voyager, voyager 1, voyager 2, image, images, solar system

BitDrifter says:

Also shows where they are in relation to the Termination Shock, Heliosphere, Heliosheath, Heliopause and the Bow Shock.

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<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://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/039da527-fcd0-4f07-8a8a-826e37143fbc/BB22F512-3241-44D4-8F4F-7C1412AA9373/" 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://en.wikipedia.org/w/index.php?title=Image:Voyager_1_entering_heliosheath_region.jpg&oldid=45523487" href="http://en.wikipedia.org/w/index.php?title=Image:Voyager_1_entering_heliosheath_region.jpg&oldid=45523487" style="font-size: 11px;">en.wikipedia.org</a></div><blockquote style="text-align: left; padding: 0px 8px; margin: 4px 0px 8px 0px; background: transparent; border: none;" cite="http://en.wikipedia.org/w/index.php?title=Image:Voyager_1_entering_heliosheath_region.jpg&oldid=45523487"><div align="center"><img src="http://content8.clipmarks.com/blog_cache/en.wikipedia.org/img/76285CEC-FE12-4D72-8863-185A685E574F" alt="" /></div></blockquote><div style="border-bottom: solid 1px #dcdcdc; white-space: nowrap; margin-bottom: 8px; background-color: #eeeeee ;background-image: url(http://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://content9.clipmarks.com/images/clip-icon.gif" 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://en.wikipedia.org/w/index.php?title=Termination_shock&oldid=71712061" href="http://en.wikipedia.org/w/index.php?title=Termination_shock&oldid=71712061" style="font-size: 11px;">en.wikipedia.org</a></div><blockquote style="text-align: left; padding: 0px 8px; margin: 4px 0px 8px 0px; background: transparent; border: none;" cite="http://en.wikipedia.org/w/index.php?title=Termination_shock&oldid=71712061"><P>In <A title="Space%20physics" href="http://en.wikipedia.org/wiki/Space_physics">space physics</A>, the <B>termination shock</B> is the boundary marking one of the outer limits of the sun's influence. It is where the bubble of <A title="Solar%20wind" href="http://en.wikipedia.org/wiki/Solar_wind">solar wind</A> particles slows down to <A title="Subsonic" href="http://en.wikipedia.org/wiki/Subsonic">subsonic</A> speed (with respect to the star) due to interactions with the local <A title="Interstellar%20medium" href="http://en.wikipedia.org/wiki/Interstellar_medium">interstellar medium</A>. This causes <A title="Physical%20compression" href="http://en.wikipedia.org/wiki/Physical_compression">compression</A>, <A title="Heating" href="http://en.wikipedia.org/wiki/Heating">heating</A>, and a change in the <A title="Magnetic%20field" href="http://en.wikipedia.org/wiki/Magnetic_field">magnetic field</A>. The termination shock is believed to be 75-90 <A title="Astronomical%20unit" href="http://en.wikipedia.org/wiki/Astronomical_unit">astronomical units</A><A title="http://antwrp.gsfc.nasa.gov/apod/ap020624.html" class="external%20autonumber" href="http://antwrp.gsfc.nasa.gov/apod/ap020624.html">[1]</A> from the Sun. The termination shock boundary fluctuates in its distance from the sun as a result of fluctuations in <A title="Solar%20flare" href="http://en.wikipedia.org/wiki/Solar_flare">solar flare</A> activity, i.e. changes in the ejections of gas and dust from the sun.</P></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://en.wikipedia.org/w/index.php?title=Termination_shock&oldid=71712061"><P>Going outward from the sun, the termination shock is followed by the <A title="Heliopause" href="http://en.wikipedia.org/wiki/Heliopause">Heliopause</A> where solar wind particles are stopped by the interstellar medium, then the <A title="Bow%20Shock" href="http://en.wikipedia.org/wiki/Bow_Shock">Bow Shock</A> past which particles from the interstellar medium are no longer excited.</P></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/BB22F512-3241-44D4-8F4F-7C1412AA9373/blog/" title="blog or email this clip"><img src="http://content6.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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