N3 - Institut für Physik

Transcrição

EUROPLANET
Koordinierte Planetologie in Europa
Helmut O. Rucker
Summer University “Graz in Space 2006”
Sept 8, 2006
I3/CA Europlanet - EC Contract 001637 - http://europlanet.cesr.fr/
Planetary Missions in Europe
(2000 to 2017)
January 14, 2005 : A European probe lands on Titan
Titan : multi-scale study of a new world
Courtesy: Cassini-Huygens teams
Participants
Technische Univ. München
Institüt für Weltraumforschung
Austrian Academy of Sciences
IRSP
International Research School
of Planetary Sciences
Prague Observatory
Royal Observatory Blegium
Astronomical
Institute of the
Romanian Academy
g
lin
el r y
od o
M the
M La
e a bo
s u ra
re to
m ry
en
ts
Education
ESA
Venus
Rosetta
Bepi
Smart
1
Mars
Express
Planetary
Express
Colombo
Missions
Ground-based
observations
Public
EuroPlaNet Structure and Activities
N1: EuroPlaNet Management
Blanc, Dougherty, Guidice, Witasse
40 laboratories/institutions
(i.e. 60 institutes) from
17 EU countries
13 associate participants worldwide
Dutuit, Szego
N6
Meetings
Chanteur, Flamini
Krupp, Matti
Discipline
Discipline
Working
Working
Groups
Groups
N3
Rucker, Miller
N4
Zarnecki, Lebreton
Ground-based
Ground-based
Observation
Observation
Coordination
Coordination
Outreach
Outreach
Strategy
Strategy
N5
Personnel
Exchange
Srama, Serote
N2
Activity N7:
N4:
N5:
Developing
Personnel
andexchange
an
development
outreach strategy
of
N2:Design
Discipline
working
groups
N3:
Co-ordinated
space/earthDeveloping
Supporting
akey
pan-European
exchanges
outreach
of personnel
plan that
the
IDIS
Establishment
of
“discipline
working
groups”
in
based
observations
Activity
N6:
Meetings,
conferences
Creation
will
between
help research
to
of associate
ansynergies
Integrated
groups
the European
and
the
Distributed
Citi-zens
aim
to to
the
different
science
areas
ofwith
planetary
sciences
Developing
between
in-situ
Organisation
of
EuroPlaNet
meetings
during
the
establish
Information
Planetary
a of
Service
Exploration
long-term
(IDIS)
working
program
and
itsactivities
relation
further
with
the aim
tothecover
all
major
fields
exploration
planetary
systems
andofin
the project.
Europe
between
evolution
the
into
groups.
space
a European
agencies,
Virtual
research
Planetary
institutes,
planetary(incl.
sciences.
telescope
observations
from
the ground
or
Universities
Observatory.
Earth orbit. and science museums).
N7
IDIS
EuroPlaNet and modern
Planetary Science
N6
SPACE-BASED observations
N3
N5: Personal Exchange
N2
N2
processing
N6
N6
EARTH-BASED observations
N3
N2
Data
Inference)
N2
N6
N6
data
Lab Measurements
N2
N2
Scientific
results
N6
(scientific
Theoretical
interpretations
N2
bases,
algorithms
N6
N6
N7: IDIS
Numerical simulation
N2
N5: Personal Exchange
Outreach
products
N4
N3: Coordination of Ground-based
and Space Observations
N3
N3 Scientific
Scientific Focus
Focus Points
Points
• Space Mission complementary observations
- Ground-based observations of radio and IR emissions to
compliment space missions in-situ and remote measurements
IRTF campaign of H3+ observations
on Saturn (UCL)
Cassini/RPWS observations of
SKR (Univ.Iowa, Meudon (F),
IWF/OEAW (A))
NASA/IRTF
Subaru
Keck
Mauna Kea
Hawaii
August 2004
N3
N3 Scientific
Scientific Focus
Focus Points
Points
• Space Mission complementary observations
- Ground-based observations of radio and IR emissions to
compliment space missions in-situ and remote measurements
IRTF campaign of H3+ observations
on Saturn (UCL)
Cassini/RPWS observations of
SKR (Univ.Iowa, Meudon (F),
IWF/OEAW (A))
Pre-SOI science:
J. Clarke
Cassini and HST join in studying the dynamics
of the Saturnian aurora
W. Kurth
F. Crary
E. Bunce
Remote / in-situ
P uv
P dyn
P skr
Die Aurora – ein faszinierendes Phänomen
an den magnetischen Polen
der Planeten mit einem Magnetfeld
Earth
Dynamic Explorer )
UV - 130 nm
(Courtesy . L. Frank)I3/CA
Jupiter
HST-STIS
UV - 150 nm
Europlanet
- EC Contract
001637 (R. Prangé
& L Pallier)
Saturn
HST-STIS
UV - 130 nm
http://europlanet.cesr.fr/
(R. Prangé & L Pallier)
Planetary Aurorae
1st Workshop on
“Saturn’s Aurorae: Magnetospheric Generation and Energy Considerations“
November 25-26, 2005
IWF-OEAW, Graz
Follow-up workshop: 2nd Strategic Workshop on
„Comparative Aurorae“
Nov 22 – 23, 2006, UCL London
(LOC/SOC: Steve Miller, Helmut O. Rucker et al.)
Nördliche Polkappe ist einige km dick,
vielleicht das größte Wasserreservoir auf Mars.
Die Atmosphäre von Mars
Trotz der dünnen Atmosphäre von Mars gibt es Sandstürme
und Dünen auf Mars.
N3
/exospheres and
N3 strategic
strategic WS
WS on
on Atmospheres
Atmospheres/exospheres
and their
their
dynamics
/composition on
dynamics/composition
on Venus
Venus and
and Mars
Mars
•WS am 2. April 2006 in
Wien
•16 Teilnehmer
•Thema: erdgebundene
Beobachtungen der Dynamik
und Chemie in den oberen
Atmosphären von Venus und
Mars
N3
N3 strategic
strategic WS
WS on
on Coordinated
Coordinated Observation
Observation of
of
SMART
-1 low
SMART-1
low altitude
altitude operation
operation and
and impact
impact
• 3 WS im Jahr 2006 (2 am
IWF Graz)
• Thema: Beobachtungen von
SMART-1 in der letzten
Phase der Mission (auch
durch Amateure)
Smart-1 lunar impact
Impact with 2 km/s
Impact in volcanic plane „Lake of Excellence“,
Sept 3, 2006 (05:42 UT)
Exoplanet status September 2, 2005
¾ 164 exoplanetary
systems
¾ 20 multiple planetary
systems
¾ total: 204 exoplanets
COROT
launch 2006
smallest size
2 Earth-radii
COROT will enhance
the number and statistics
of exoplanets < 0.5 AU
to a large extent
New Horizon Pluto Express
Launch
Jan 19, 2006
Jupiter flyby
Feb 28, 2007
Pluto closest approach
July 14, 2015
New Horizon Pluto Express
Coordinated Jupiter multiwavelengths observations
during NH Pluto Express Jupiter flyby Feb 28, 2007
Cassini (from Saturn system)
Rosetta
Ulysses
HST (from Earth orbit)
Web sites
http://europlanet.cesr.fr/
http://europlanet.oeaw.ac.at

N3 - Institut für Physik

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