From: LARRY KLAES (ljk4_at_msn.com)
Date: Fri Oct 19 2007 - 08:47:35 PDT
>From: "AAS Press Officer Dr. Steve Maran" <Steve.Maran_at_aas.org>
>To: "AAS Press Officer Dr. Steve Maran" <steve.maran_at_aas.org>
>Subject: ESA: Names Candidate Missions for Cosmic Vision 2015-2025
>Date: Fri, 19 Oct 2007 11:33:09 -0400
>
THE FOLLOWING RELEASE WAS RECEIVED FROM THE EUROPEAN SPACE AGENCY'S "ESA WEB
PORTAL - SCIENCE," IN NOORDWIJK, THE NETHERLANDS AND IS FORWARDED FOR YOUR
INFORMATION. Steve Maran, American Astronomical Society
steve.maran_at_aas.org 1-202-328-2010 x116
Contact information at the end of the release
Article and images can be found at:
http://www.esa.int/esaSC/SEM1IQAMS7F_index_0.html
19 October 2007
Cosmic Vision 2015-2025: and the candidate missions are...
The first steps of the next great phase of European space science have been
taken! At its meeting held on 17-18 October 2007 in Paris, ESA's Space
Science Advisory Committee (SSAC) selected the new candidates for possible
future scientific missions.
"It has been an arduous process both inside ESA and in the community to get
these winning groups into what I suppose can be said to be the quarterfinals
of one of the ultimate competitions in world space science," said ESA's
Director of Science, David Southwood. "We can now get glimpses of the future
and it is going to be exciting!"
>From a list of 50 proposals submitted by the scientific community last
>summer, the candidates which have made it to the next phase of selection
>are:
Solar System
Laplace, studying the Jovian system
The Jovian System, with Jupiter and its moons, is a small planetary system
in its own right. Unique among the moons, Europa is believed to shelter an
ocean between its geodynamically active icy crust and its silicate mantle.
The proposed mission would answer questions on habitability of Europa and of
the Jovian system in relation to the formation of the Jovian satellites and
to the workings of the Jovian system itself. The mission will deploy three
orbiting platforms to perform coordinated observations of Europa, the Jovian
satellites, Jupiter's magnetosphere and its atmosphere and interior.
If finally approved, the mission would be implemented in collaboration with
NASA.
Tandem, a new mission to Saturn, Titan and Enceladus
Tandem has been proposed to explore two of Saturn's satellites (Titan and
Enceladus) in-situ and from orbit. Building on questions raised by Cassini,
the mission would investigate the Titan Enceladus systems, their origins,
interiors and evolution as well as their astrobiological potential. The
mission would carry two spacecraft - an orbiter and a carrier to deliver a
balloon and three probes onto Titan.
If approved, the mission would be implemented in collaboration with NASA.
It is expected that a first selection between Laplace or Tandem, i.e.
Jupiter or Saturn targets will be made in consultation with foreign partners
in the coming years.
Cross-scale, deeper study of near-earth space
Cross-Scale, proposed to employ 12 spacecraft, would make simultaneous
measurements of plasma - the gas of charged particles surrounding Earth - on
different scales at shocks, reconnection sites, and turbulent regions in
near-Earth space. It will address fundamental questions such as how shocks
accelerate and heat particles or how magnetic reconnection phenomena
generate or convert energy.
If approved, the mission would be implemented in collaboration with JAXA,
the Japanese Space and Exploration Agency.
Marco Polo, an asteroid sample-return mission
A sample-return mission to a near-earth object, Marco Polo would
characterise a near-earth object at multiple scales and return a sample. If
approved, the mission would study the origins and evolution of the Solar
System, the role of minor bodies in the process, origins and evolution of
Earth and of life itself. It would consist of a mother satellite which would
carry a lander, sampling devices, reentry capsule as well as instruments.
If approved, the mission would be implemented in collaboration with JAXA.
Astronomy
A dark energy mission
Two proposals have been received (Dune, the dark universe investigator and
SPACE, the new near-infrared all-sky cosmic explorer) addressing the study
of dark matter and dark energy - a hot topic in astronomy. While they
propose to use different techniques (Dune is proposed as a a wide-field
imager, while Space is proposed as a near-Infrared all-sky surveyor), they
address the same basic science goal. In the follow-up study phase a
trade-off will be performed leading to the definition in the spring of next
year of a proposal for a European dark energy mission to go forward in
competition.
Plato, the new planet finder
The proposed next-generation planet finder is a photometry mission that will
detect and characterise transiting exoplanets as well as measure the seismic
oscillations of their parent stars. It will be capable of observing rocky
exoplanets around brighter and better characterized stars than its
predecessors. Observations of the mission will be complemented by ground-
and space-based follow-up observations to derive the planet's masses and
study their atmospheres.
Spica, the next generation infrared observatory
Spica is a proposed medium- and far-infrared observatory with a
large-aperture cryogenic telescope. The mission would address planetary
formation, the way the solar system works and the origin of the universe. It
would perform wide field, high sensitivity photometric mapping at high
spatial resolution, spectral analysis as well as coronography of planets and
planetary disks.
Spica is proposed in collaboration with the Japanese Aerospace Exploration
Agency, JAXA, with ESA providing the telescope and a contribution to the
operations.
XEUS, X-ray Evolving Universe Spectroscopy
XEUS is a next-generation X-ray space observatory to study the fundamental
laws of the Universe and the origins of the universe. With unprecedented
sensitivity to the hot, million-degree universe, XEUS would explore key
areas of contemporary astrophysics: growth of supermassive black holes,
cosmic feedback and galaxy evolution, evolution of large-scale structures,
extreme gravity and matter under extreme conditions, the dynamical evolution
of cosmic plasmas and cosmic chemistry. XEUS would be stationed in a halo
orbit at L2, the second Lagrange point, with two satellites (one mirror
satellite and the other a detector satellite) that would fly in formation.
Various international partners have expressed interest in cooperation in
XEUS and discussions will start by the end of the year with the interested
agencies to ensure the earliest involvement in study work.
All the candidate missions are now competing in an assessment cycle which
ends in 2011. Before the end of the cycle, there will be an important
selection foreseen in 2009. At the end of this process, two missions will be
proposed for implementation to ESA's Science Programme Committee, with
launches planned for 2017 and 2018 respectively.
The selected missions fit well within the themes of ESA's Cosmic Vision
2015-2025 plan. The themes range from the conditions for life and planetary
formation, to the origin and formation of the Solar System, the fundamental
laws of our cosmos and the origin, structure and evolution of the Universe.
"The maturity of most of the proposals received demonstrates the excellence
of the scientific community in Europe. This made the task of the SSAC very
difficult but we believe that the set of selected missions will shape the
future of European space scence," said Tilman Spohn, chairperson of the SSAC
(German Aerospace Center, Berlin). "The next decade will indeed be very
exciting for the scientific exploration of space."
According to the chair of the Astronomy Working Group (AWG), Tommaso
Maccacaro, (INAF - Osservatorio Astronomico di Brera) "The chosen candidates
for astronomy missions show very promising and broad scientific return and
have received excellent recommendations also from external referees."
"Technical feasibility and potential for successful cooperation with other
agencies are two factors which are clearly evident in the Solar System
missions that have been chosen," added Nick Thomas at the Physikalisches
Institut, Universität Bern, chair of the Solar System Working Group.
For more information:
Sergio Volonte
ESA Head of Science Planning and Community Coordination Office
Email : Sergio.Volonte_at_esa.int
ESA PIO source:
Monica Talevi
Science Information Manager
ESA - Communication Dept.
Tel: +31 71 565 3223
Fax: +31 71 565 4101
Email: Monica.Talevi_at_esa.int
--------------------------------------------------------------------------
If you do not wish to receive press releases that are forwarded to the news
media by the American Astronomical Society, just reply accordingly to any
incoming press release, or write to steve.maran_at_aas.org. Requests for
referrals to experts on astronomy and space exploration should be sent to
the same address. Steve Maran, AAS Press Officer steve.maran_at_aas.org
Telephone 1-202-328-2010 X116
--- Message scanned for viruses and dangerous content by the AAS MailScanner, and is believed to be clean.
This archive was generated by hypermail 2.1.6 : Fri Oct 19 2007 - 08:53:15 PDT