IPGP Mage activities. 27/04/20042004 EUG MAGE Meeting Team n Planetology team in Saint Maur des Fossés u P. Lognonné, M.Wieczoreck, J. Gagnepain-Beyneix.

Slides:



Advertisements
Similar presentations
What are the three Chemical layers of the Earth?
Advertisements

Tilman Spohn Structure and Evolution of Terrestrial Planets.
The first 80% of the History of Venus?. Some Geological Conclusions from Magellan Analysis -Volcanism and tectonism are the most abundant geological processes.
MAGE mid-term meeting Strasbourg – 2004, September 23 rd MAGE mid-term report CETP research activities.
Mercury’s origin and evolution:- Likely evidence from surface composition David A Rothery 1, J Carpenter 2, G Fraser 2 & the MIXS team 1 Dept of Earth.
Connecting Planetary Interiors and Surfaces Shaping Planetary Surfaces.
Lecture 6: Earth as a Planet 1.The Young Earth 2.Earth as a planet: interior 3.Plate tectonics 4.Atmosphere.
Earth: the home planet Earth’s Interior Earth’s Layered Structure Earth’s interior consists of layers Earth’s interior consists of layers Layers are.
Planetary Geology. Layering of Terrestrial Worlds The process of differentiation separates materials with different densities Dense metals fall.
Review 2 Astronomy 150, April 27 th Moon’s Formation Giant-Impact theory –A Mars-sized object hits the Earth and the Moon is created from the debris.
Physics 202: Introduction to Astronomy – Lecture 9 Carsten Denker Physics Department Center for Solar–Terrestrial Research.
The Lunar Interior A Presentation by Kyle Stephens October 2, 2008.
The Earth’s Structure. The Earth’s Lithosphere S and P Waves S and P waves travel at different speeds Both waves travel through sold material Only P.
Geophysics & Meteorology on the surface of Mars P.Lognonné, T.Spohn, F.Forget IPGP, DLR, IPSL.
The Solar System.
An active Seismic experiment on Bepi-Colombo Lognonné, P, Garcia. R (IPGP, France) P.; Gudkova, T.(IPE, Russia) ; Giardini, D., Lombardi D. (ETHZ, Switzerland);
Chapter 7 Earth and The Terrestrial Worlds Principles of Comparative Planetology Comparative Planetology is the study of the solar system through examining.
The Earth and Its Moon The Earth Solid inner core, liquid outer core atmosphere - 50km thick magnetosphere - charged particles caught in Earth’s magnetic.
Terrestrial Planets Earthlike Worlds of Rocks and Metals.
Inner Planetary Geology I. Terrestrial Planets  The Terrestrial Planets cooled from molten masses  Acquired structure during cooling  Made primarily.
ASTRONOMY 340 FALL September 2007 Class #8.
Layers of the Earth.
Class 1: Plate Tectonics Review Today’s topics:  Earth’s compositional layers  Plate tectonics: theory & actions.
Lecture 5 6/8/07 AST1001.
Magellan's Venus pictures show several examples of faults and fractures suggesting movement of the planet's crust and the existence of Venus quakes. If.
Report of work at ROB within the MAGE European Training Network Véronique Dehant.
1 The Earth-Moon System The Earth’s Atmosphere Unique among terrestrial planets in its composition –78% Nitrogen (N 2 ) –21% Oxygen (O 2 ) –0.9% Argon.
August 19 & 20 Welcome Task Pick up your lab notebook and a textbook “Inside Earth” Copy all words and define: Crust Mantle Inner Core Outer Core Lithosphere.
How can we study quakes on other planets? Cannot do it entirely from earth Need to send people or landers to the planet Apollo Mission sent astronauts.
The Earth-Moon System The Earth’s Atmosphere
ASTR-1010 Planetary Astronomy Day Announcements Smartworks Chapter 6: Due Today, March 22. Smartworks Chapter 7: Due Friday, March st Quarter.
The Moon Chapter 10. The Earth Moon System Primary Surface Features.
Chapter 5 Earth and its Moon. The Earth Table 5-1 Some Properties of Earth and the Moon.
© 2007 Pearson Prentice Hall This work is protected by United States copyright laws and is provided solely for the use of instructors in teaching their.
Dynamical modeling of Mars deep interior Sylvaine Ferrachat Institut für Planetologie Westfälische Wilhelms-Universität Münster.
Copyright © 2010 Pearson Education, Inc. Lecture Outline Chapter 5 Earth and Its Moon.
The Earth Classify stuff –Composition: Crust, mantle, outer core, inner core –Physical Properties Atmosphere, biosphere, lithosphere, asthenosphere, mesosphere,
PLANETARY GEOLOGY. Discuss the factors that affected the geologic processes and formations of the planets Outline the information in the 6 slides Use.
Exploring Mars: The Inside Story Walter S. Kiefer Lunar and Planetary Institute.
Astronomy 1010 Planetary Astronomy Fall_2015 Day-28.
Standard 2 Objective 1 Study Notes Plate Tectonics 1.
How can we study quakes on other planets? Cannot do it entirely from earth Need to send people or landers to the planet Apollo Mission sent astronauts.
Earth’s Interior Jeopardy
Chapter 8 The Earth. How do we know that planet Earth really revolves and rotates? What is Aberration and what does it prove about the Earth? What is.
MAGE postdoc presentation - MAGE midterm meeting Peter van Thienen D épartement de Géophysique Spatiale et Planétaire, Institut de Physique du Globe de.
© 2007 Pearson Prentice Hall This work is protected by United States copyright laws and is provided solely for the use of instructors in teaching their.
Chapter 6: Terrestrial Planets -The Moon. Earth’s interior is revealed by seismology, the study of earthquakes. Layers are revealed: A layered object:
Explored through mines and wells Temperature and pressure increases with depth Earthquake (Seismic) Waves scientists are able to tell the density and.
Pop Quiz! 1.__ 2.__ 3.__ 4.__ 5.__ 6.__ 7.__ 8.__ Inner Core Mantle Mesosphere Outer Core Asthenosphere Ocean Crust Lithosphere Continental Crust.
ASTR-1010 Planetary Astronomy Day Announcements Smartworks Chapter 7: Due Friday, March st Quarter Observing Nights: Tues & Thurs, March.
© 2017 Pearson Education, Inc.
EXPLORING EARTH’S INTERIOR
Note that the following lectures include animations and PowerPoint effects such as fly ins and transitions that require you to be in PowerPoint's Slide.
Connecting Planetary Interiors and Surfaces
Planetary Discovery in the era of Spacecraft Exploration Xi Zhang
Ch. 8: Earth as a Planet.
The Moon Chapter 10.
5.3 Atmospheres Troposphere is where convection takes place – responsible for weather.
Earth and The Terrestrial Worlds
Do Now: What is your favorite layered food?
Basic Stats, Motion and Moons
The Fiery Earth Earth’s Interior.
List and explain what scientist learned from drilling in the sea floor
What are the three Chemical layers of the Earth?
Plate Tectonics Chapter 12.2.
Review…. Density of Earth Lab What planet is the most dense? What planet is the least dense? **Name some earth systems that are driven by density differences.
Planetary Geology: dominant processes
Introduction to Earth Structure
Earth’s Interior.
Presentation transcript:

IPGP Mage activities

27/04/ EUG MAGE Meeting Team n Planetology team in Saint Maur des Fossés u P. Lognonné, M.Wieczoreck, J. Gagnepain-Beyneix u Other scientists in IPGP Jussieu ( B.Bourdon, S.Labrosse, primitive Mars), C.Jaupart’s team ( convection), Seismo lab, etc n 2 MAGE post-docs u Amir Khan ( 4/2003->8/2004) u Peter van Thienen (3/2004-2/2006) n 2 PhD Students u H. Chenet ( -> 12/2003) ( Moon seismology ) u V.Belleguic (->12/2004) ( Mars Gravimetry and Topography ) u M. Le Feuvre ( 9/2004 -> ) ( Moon and Mars Chronology ) u Ana Rita Baptista ( 1/2005 -> ) ( Mars magnetosphere and radiative environement )

27/04/ EUG MAGE Meeting Planetary Cores M. Wieczorek, A. Khan, S.Labrosse et P. Lognonné n Science Objectives u Planetary Formation processes u Present size, state and mineralogy n Data: LLR, Sismo Apollo, Gravimetry LP n Some results: u Moon: confirmation of a liquid core, estimation of the temperature u Mars: detailed analysis and theory of tidal signals

27/04/ EUG MAGE Meeting Crust and Martian lithosphere M. Wieczoreck, V. Belleguic, P. van Thienen et P. Lognonné n Science objectives u Crustal formation,evolution, impact and volcanic comparative tectonics u Propagation of seismic waves in the Martian crust. n Data: MGS ( gravimetry, altimetry) n results: u Crustal thickness. Estimation of the fraction of primary crust in the southern hemisphere u Estimation of the thickness of the elastic lithosphere and of the density of volcanoes

27/04/ EUG MAGE Meeting Lunar crust and Mantle A.Khan, J. Gagnepain, P. Lognonné, H.Chenet ( ISAS, Japan) n Science objectives: u Crustal thickness u Mineralogical and temperature composition of the mantle. n Data: Apollo, LP ( gravimetry, altimetry) n Results: u New estimate of the crustal thickness u Better agreement with geochemistry u New estimate of the U content in the mantle.

27/04/ EUG MAGE Meeting Mineralogical and temperature results Seismic velocities

27/04/ EUG MAGE Meeting New research orientations n Primitive Mars and Mars evolution u more in P. van Thienen presentation u Effect of atmosphere and volatiles on long term convection n Determination of a new cratering chronology for the Moon and Mars(Le Feuvre and Wieczoreck) n Magnetosphere, magnetic crust and radiation ( collaboration with CETP and Portugal) …. In addition to MAGE activities