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  1. ... the first stars.  See Feburary 24 2014 MIT News Faculty Profile written by Jennifer Chu.   * * * * * * * Robert A. ...

    Anonymous - 2017-03-16 13:57

  2. ... Fred Kavli A video interview from 2007 A 2012 profile Professor Jacqueline Hewitt, Director of MIT's Kavli Institute ...

    Debbie Meinbresse - 2013-11-22 19:35

  3. ... URL:  http://news.mit.edu/2013/faculty-profile-josh-winn-physics-0320 News Source:  MIT ... Faculty Solar system Students Profile Physics Kavli Institute Author:  ...

    siteadmin - 2017-01-18 09:53

  4. ... URL:  http://web.mit.edu/newsoffice/2013/faculty-profile-josh-winn-physics-0320.html News Source:  ... Faculty Kavli Institute Physics Profile Solar system Students Author:  Jennifer ...

    siteadmin - 2013-04-10 16:21

  5. ... force, and atmospheric density on its atmospheric pressure profile — the extent to which pressure changes throughout its atmosphere. ... could be derived from its atmospheric temperature, pressure profile, and density — parameters that, in principle, may be obtained from a ...

    Debbie Meinbresse - 2013-12-19 17:19

  6. ... of Astrophysical Journal Letters , expand the physical profile of 55 Cancri e. The planet orbits the star 55 Cancri, part of the ... Seager says that in addition to fleshing out the physical profile of 55 Cancri e, the group’s techniques may be adopted to characterize ...

    siteadmin - 2012-11-01 18:09

  7. ... of Astrophysical Journal Letters , expand the physical profile of 55 Cancri e. The planet orbits the star 55 Cancri, part of the ... Seager says that in addition to fleshing out the physical profile of 55 Cancri e, the group’s techniques may be adopted to characterize ...

    siteadmin - 2014-06-09 12:14

  8. ... of Astrophysical Journal Letters , expand the physical profile of 55 Cancri e. The planet orbits the star 55 Cancri, part of the ... Seager says that in addition to fleshing out the physical profile of 55 Cancri e, the group’s techniques may be adopted to characterize ...

    siteadmin - 2015-08-20 18:21

  9. ... for 8 AU before the heliopause crossing. The V2 flow profile is very different from that at V1; the average speed stays constant at ...

    Debbie Meinbresse - 2016-12-27 15:28

  10. ... The strong signal from SGR J1745-29 presents a complex pulse profile modulated with pulsed fraction 27% ± 3% in the 3-10 keV band. Two ...

    Debbie Meinbresse - 2013-07-12 20:13