[Baps] BU seminar today (Thursday) - Kurt Retherford
Withers, Paul
withers at bu.edu
Thu Sep 20 09:50:23 EDT 2018
Apologies for the late notice.
Future seminars and logistics described at:
http://www.bu.edu/csp/edoutreach/seminar/
Paul
-------- Forwarded Message --------
Subject: [Announce] CSP Seminar - Retherford (9/20)
Date: Thu, 20 Sep 2018 13:24:33 +0000
From: Gordon, Mary <megordon at bu.edu>
To: announce at skynet.bu.edu <announce at skynet.bu.edu>,
csp_seminar at skynet.bu.edu <csp_seminar at skynet.bu.edu>
_Thursday, 9/20 @ 4:00pm _
CAS 502
**
*Speaker:*
Kurt Retherford
/Southwest Research Institute/
*Title:*
Europa-UVS, JUICE-UVS, and Hubble Observations of Galilean Satellite
Atmospheres
**
*Abstract: *
The Galilean satellites display a diverse range of activity and coupling
of their tenuous (mostly exospheric) atmospheres to the plasma
environment of Jupiter. UV remote sensing observations of these
atmospheres inform our understanding of Io’s volcanism and feeding of
plasma into the Jupiter system, Europa’s water vapor plumes and
habitability, Ganymede’s internal magnetic field and ocean, and
Callisto’s atmospheric composition and volatile transport. NASA's
Europa Clipper mission plans for ~44 Europa flybys and focuses its
science goals to investigate potential habitable regions within Europa's
subsurface, answering questions such as could the source of water vapor
plumes connect directly with the liquid ocean? The European Space
Agency’s Jupiter Icy Moons Explorer (JUICE) mission objectives include
this same habitability goal for Europa, planning 2 Europa flybys.
Moreover, JUICE investigates the entire Jupiter system and ultimately
orbits Ganymede to investigate its subsurface ocean and habitability,
among numerous other goals. I’ll describe our group’s Europa
Ultraviolet Spectrograph (Europa-UVS) and JUICE-UVS instrument
developments at SwRI and planned observations, which utilize far-UV
emissions, reflectance, and transmission techniques to constrain the
composition and structure of satellite atmospheres, surfaces, and plasma
environments. Our long series of Hubble Space Telescope (HST)
observations of the Galilean satellites inform these mission plans; I
will summarize results from recent HST observations by several groups.
//
/Light refreshments will be served prior to the seminar at 3:45pm in CAS
500. /
Mary Gordon
Fiscal Coordinator | Boston University
Center for Space Physics | Institute for Astrophysical Research
725 Commonwealth Avenue, Room 506 | Boston, Massachusetts 02215
Tel: 617-353-5992 | Fax: 617-353-6463
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