BEGIN:VCALENDAR PRODID:-//Microsoft Corporation//Outlook 14.0 MIMEDIR//EN VERSION:2.0 METHOD:PUBLISH X-MS-OLK-FORCEINSPECTOROPEN:TRUE BEGIN:VTIMEZONE TZID:Pacific Standard Time BEGIN:STANDARD DTSTART:16011104T020000 RRULE:FREQ=YEARLY;BYDAY=1SU;BYMONTH=11 TZOFFSETFROM:-0700 TZOFFSETTO:-0800 END:STANDARD BEGIN:DAYLIGHT DTSTART:16010311T020000 RRULE:FREQ=YEARLY;BYDAY=2SU;BYMONTH=3 TZOFFSETFROM:-0800 TZOFFSETTO:-0700 END:DAYLIGHT END:VTIMEZONE BEGIN:VEVENT CLASS:PUBLIC CREATED:20111208T235547Z DESCRIPTION:The Herschel Space Observatory\, launched on May 14\, 2009\, is designed to carry out astronomical observations at wavelengths from ~1mm to 100 microns. This region of the spectrum\, between radio waves and heat radiation\, is a unique probe of the “cool” universe\, that is\, of o bjects at temperatures between a few degrees and 100 degrees above absolut e zero. This includes material out of which new stars are forming in locat ions ranging from distant galaxies to nearby cold clouds of gas. To carry out these observations\, Herschel has the largest precision telescope laun ched for astronomy\, and three very sensitive instruments. Among many proj ects\, Herschel has followed the “water trail” – observing this mole cule in a wide range of sources ranging from giant molecular clouds to pro toplanetary disks around young stars to comets in the solar system. This t alk will present some of the highlights of Herschel observations and descr ibe how they are changing our picture of how new stars and planets form.\n Speaker:\nDr. Paul Goldsmith\nLocation:\nThursday\, Oct. 11\, 2012\, 7pm\n The von Kármán Auditorium at JPL\n4800 Oak Grove Drive\nPasadena\, CA\n › Directions \nWebcast:\nFo r the webcast on Thursday at 7 p.m. PST:\nLive video streaming\, with a re al-time web chat to take public questions\, will air on Ustream located he re. \n DTEND;TZID="Pacific Standard Time":20121011T200000 DTSTAMP:20111208T235547Z DTSTART;TZID="Pacific Standard Time":20121011T190000 LAST-MODIFIED:20111208T235547Z LOCATION:The von Kármán Auditorium at JPL PRIORITY:5 SEQUENCE:0 SUMMARY;LANGUAGE=en-us:Herschel Opens Up the Cool Universe TRANSP:OPAQUE UID:040000008200E00074C5B7101A82E00800000000F0A7B1D4C1B5CC01000000000000000 0100000001BCA74A8F80E184483FB978EAF0F7DB5 X-ALT-DESC;FMTTYPE=text/html:\n\n\n\n\n\n\n\n\n

The Herschel Spac e Observatory\, launched on May 14\, 2009\, is designed to carry out astro nomical observations at wavelengths from ~1mm to 100 microns. This region of the spectrum\, between radio waves and heat radiation\, is a unique pro be of the “cool” universe\, that is\, of objects at temperatures betwe en a few degrees and 100 degrees above absolute zero. This includes materi al out of which new stars are forming in locations ranging from distant ga laxies to nearby cold clouds of gas. To carry out these observations\, Her schel has the largest precision telescope launched for astronomy\, and thr ee very sensitive instruments. Among many projects\, Herschel has followed the “water trail” – observing this molecule in a wide range of sour ces ranging from giant molecular clouds to protoplanetary disks around you ng stars to comets in the solar system. This talk will present some of the highlights of Herschel observations and describe how they are changing ou r picture of how new stars and planets form.

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Speaker:

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Dr. Pa ul Goldsmith

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Location:< /P>\n\n

Thursday\, Oct. 11\, 2012\, 7pm
\nThe von Kármán Auditorium at JPL
\n4800 Oak Grove Drive
\nP asadena\, CA
\n› Directions< /SPAN>

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Webcast:

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For the webcast on Thursday at 7 p.m. PST:
\nLive video streaming\ , with a real-time web chat to take public questions\, will air on Ustream located here.< SPAN LANG="en-us">

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