The complex interactions of three stars in the Orion B molecular cloud complex [ http://www.seds.org/messier/more/oricloud.html ] have resulted in the ejection of particles along a 12 light-year [ http://www.treasure-troves.com/astro/Light-Year.html ] long jet. One of the stars in the HH111 [ http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=1999A%26A...352L..83R ] system has apparently also been ejected leaving two stars tightly bound in a binary [ http://antwrp.gsfc.nasa.gov/apod/ap991219.html ] orbit. The spectacular jet [ http://antwrp.gsfc.nasa.gov/apod/ap971124.html ] emanates from one of these two stars. The complete system is quite complex and involves another less-luminous jet and disks of rapidly rotation gas. In the top part of this Hubble Space Telescope image [ http://oposite.stsci.edu/pubinfo/pr/2000/05/pr-photos.html ] taken in visible light, successive bubbles are seen to move along the jet. At the bottom in infrared light [ http://www.eecs.umich.edu/mathscience/funexperiments/agesubject/lessons/newton/infrared.html ], a torus [ http://www.bangor.ac.uk/SculMath/image/torus.htm ] of dark dust [ http://antwrp.gsfc.nasa.gov/apod/ap990509.html ] and gas from which the stars formed millions of years ago can be seen. Protons [ http://www.neutron.anl.gov/proton.htm ] and electrons [ http://www.aip.org/history/electron/ ] zip along near 500 kilometers per second in the HH111 [ http://adsbit.harvard.edu/cgi-bin/nph-iarticle_query?1992ApJ...392..145R ] jet, which is about 1500 light-years away.