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March 26, 2014

Mtg: Reflecting on the Kepler Mission and TESS, NASA’s Next Exoplanet Mission to Find Earth’s Closest Cousins

by @ 10:01 am. Filed under ALL, Computers/Software, Electronics Design, Engineering Mgmt
 

WEDNESDAY April 23, 2014
OEB Signal Processing
Subject:
– survey, science results, habitable …
Speaker: Dr. Jon Jenkins, NASA Ames Research Center
Time: 11:45 AM – 1:00 PM
Cost: none; snacks/drinks served
Place: Lawrence Livermore National Laboratory, Livermore Valley Open Campus (off Greenville Road), Livermore
RSVP: from website; Walk-ins also welcome
Web: ewh.ieee.org/r6/oeb/SigProc/sigproc.html

Kepler vaulted into the heavens on March 7, 2009, initiating NASAâ??s search for Earth-size planets orbiting Sun-like stars in the habitable zone, where liquid water could exist on a rocky planetary surface. In the 4 years since Kepler began science operations, a flood of photometric data on upwards of 190,000 stars of unprecedented precision and continuity has provoked a watershed of 961+ confirmed or validated planets, 3845+ planetary candidates (most sub-Neptune in size and many comparable to or smaller).  The focus of the mission is shifting towards how to rapidly vet the 16,000+ threshold crossing events produced with each transiting planet search, and towards those studies that will allow us to understand what the data are saying about the prevalence of planets in the solar neighborhood and throughout the galaxy.  This talk will provide an overview of the science results from the Kepler Mission and the work ahead to derive the frequency of Earth-size planets in the habitable zone of solar-like stars from the treasure trove of Kepler data.
NASAâ??s quest for exoplanets continues with the Transiting Exoplanet Survey Satellite (TESS) mission, slated for launch in May 2017 by NASAâ??s Explorer Program.  TESS will conduct an all-sky transit survey to identify the 1000 best small exoplanets in the solar neighborhood for follow up observations and characterization.  TESSâ??s targets will include all F, G, K dwarfs from +4 to +12 magnitude and all M dwarfs known within ~200 light-years.  500,000 target stars will be observed over two years with ~500 square degrees observed continuously for a year in each hemisphere in the James Webb Space Telescope’s continuously viewable zones.  TESS discoveries will afford significant opportunities to measure the masses of the exoplanets and to characterize their atmospheres with JWST, ELTs and other exoplanet explorers.
Snacks and drinks are complementary and are provided by the IEEE/OEB Signal Processing Chapter.   This location is on US Government property and requires foreign national visitors to be properly documented in order to attend.  Please contact Ron Kane (kane2@llnl.gov) if you have questions.

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