AOGS Singapore 20.-24. June 2005 Paper ID: 58-PS-A0321 BepiColombo – Mission to Mercury Mission Overview Rita Schulz Johannes.

Slides:



Advertisements
Similar presentations
Space Weather Observations from the GOLD Mission Richard Eastes and the GOLD Team ( W. E. McClintock, A. G. Burns, S. C. Solomon, D. N. Anderson, L. Andersson,
Advertisements

MPO Scientific Aspects
Basics & Motivation Technique & Observations Fits & Measurements Summary & Outlook Atmospheric Wave Workshop ESTEC 11/10/2011 Tobias Stangier I st Physics.
Comparison of full-repeat and sub-cycle solutions in gravity recovery simulations of a GRACE-like mission Siavash Iran Pour, Nico Sneeuw, Matthias Weigelt,
A. Milillo, S. Orsini and A. Mura (INAF/Institute of Space Astrophysics and Planetology) And the SERENA Team.
Tilman Spohn Structure and Evolution of Terrestrial Planets.
The BepiColombo Mission
The first 80% of the History of Venus?. Some Geological Conclusions from Magellan Analysis -Volcanism and tectonism are the most abundant geological processes.
Geospace Electrodynamic Connections (GEC) Mission The GEC mission has been in the formulation phase as part of NASA’s Solar Terrestrial Probe program for.
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.
An insertion burn at local noon has the advantage that the spacecraft is kicked into a 11 resonant orbit, with an inexpensive recovery manoeuvre, if the.
PHEBUS Probing of Hermean Exosphere By Ultraviolet Spectroscopy PHEBUS Science Performance International Mercury Watch GroupObservatoire de Paris 5-6 April.
Prepared by: MORE Team MORE Relativity Meeting February 16-17, 2009 Rome Simulation of the solar conjunction experiment with BepiColombo.
Solar wind interaction with the comet Halley and Venus
Mercury, seen from Earth through a moderate telescope.
Mercury’s Atmosphere: A Surface-bound Exosphere Virginia Pasek PTYS 395.
Astronomy Picture of the Day. Question Which of the following provides the most useful information about the Earth's interior? A) drilling B) laser-ranging.
Three Worlds to Explore Look Up? (Astronomy) Look Down? (Geophysics) Look at Surface? (Geology)
Terrestrial Planets- Mercury & Venus 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);
“ PHOBOS - SOIL ” Phobos Sample Return Mission 1. goals, methods of study A.Zakharov, Russian academy of sciences Russian aviation.
The Atmosphere THE ATMOSPHERE. Definition: Atmosphere Air that surrounds the earth Composed of: – Nitrogen 78% – Oxygen 21% – Misc. Gases (water vapor,
Spacecraft Instruments. ► Spacecraft instrument selection begins with the mission description and the selected primary and secondary mission objectives.
Made by: Anuuke Vannavong. Facts Diameter (km) km Distance from Sun (km)- 57,900,000 Mass (kg)- 33 x 10 to the power of 22 (kg) Surface Gravity.
Computer Simulations in Solar System Physics Mats Holmström Swedish Institute of Space Physics (IRF) Forskarskolan i rymdteknik Göteborg 12 September 2005.
BepiColombo – Mission to Mercury MPO Payload Updates Mission &
Planet Project Venus By: Imani Tyakoff. Venus is the second planet from the Sun and is the second brightest object in the night sky after the Moon. Named.
1 Nori Laslo Johns Hopkins University Applied Physics Laboratory A NASA Discovery Mission.
Solar System Missions Division Solar Orbiter Next major Solar and Heliospheric mission ESA ILWS flagship Now with the Inner Heliospheric Sentinels.
Venus “lite” Currently in southwest sky after sunset, ( greatest elongation of 47 degrees was Nov 3 rd ), magnitude -4.3 Stays low, reaches inferior conjunction.
 The Venus Express Mission Håkan Svedhem Project Scientist ESAC, Spain 27 April 2010.
Coordinated Observations between MPO and MMO Harri Laakso ESA/ESTEC, Noordwijk.
Planetary Motion By Carol Greco. Why do planets move the around the sun the way they do? First you need to understand that scientists have discovered.
ASTRONOMY 340 FALL October 2007 Class #13.
9 May MESSENGER First Flyby Magnetospheric Results J. A. Slavin and the MESSENGER Team BepiColombo SERENA Team Meeting Santa Fe, New Mexico 11 May.
MAVEN MARS ATMOSPHERE AND VOLATILE EVOLUTION.
29 August, 2011 Beijing, China Space science missions related to ILWS in China
1 Mars Micro-satellite Mission Japanese micro-satellite mission to Mars to study the plasma environment and the solar wind interaction with a weakly-magnetized.
Lecture 33 The Solar System. The Inner Planets. The Solar System Overview Terrestrial Planets Chapter 16.1  16.8.
JAXA’s Exploration of the Solar System Beyond the Moon and Mars.
MMO-SWG #3[Mar ] BepiColombo Project & MMO Science Schedule H. Hayakawa, Y. Kasaba, M. Kato, T Mukai, and JAXA BepiColombo Project.
NASA Returns To Mercury in 2011 with MESSENGER. This is the first mission to Mercury since Mariner 10 in 1975 It will fully map the entire surface of.
Presented to Kepler Pre-Launch Educator Workshop January 31, 2009 Shari Asplund Discovery and New Frontiers Programs Education and Public Outreach Manager.
HNRS 227 Fall 2005 Chapter 13 The Solar System presented by Dr. Geller 27 October 2005.
The ionosphere of Mars never looked like this before Paul Withers Boston University Space Physics Group meeting, University of Michigan.
FAST LOW THRUST TRAJECTORIES FOR THE EXPLORATION OF THE SOLAR SYSTEM
Astronomy 405 Solar System and ISM Lecture 5 Mercury January 25, 2013.
Solar System: ground-based Inner solar system Mars Outer solar system –Dynamics of planetary atmospheres –Structure, dynamics and formation outer solar.
Earth-rise on Moon. The Moon A12 A14 A15 A17 A11 A16 L24 L20 L16 Apollo and Luna Landing Sites.
Gravimetry Geodesy Rotation
Exploring Jupiter with Radio Waves W. S. Kurth The University of Iowa Iowa City, IA.
Page 1 BepiColombo MMO Status Update For HEWG2014, June 2014.
1 MAVEN PFP ICDR May 23-25, 2011 Mars Atmosphere and Volatile EvolutioN (MAVEN) Mission Particles and Fields Science Critical Design Review May ,
Midterm Exam Material Covered –Chapter 1 to 6 Format of Exam –Multiple-Choice Questions: 40 to 50 questions –Facts –Concepts –Reasoning –Quantitative --
Bit of Administration …. Lab 2Lab 2 –New observation dates: March 22 - April 5 No need to duplicate observations in hand!No need to duplicate observations.
Mercury Monroe. Mercury, the winged footed, messenger of the Roman Gods.
Mars Express status and highlights IKI, Moscow 11 October 2010 Olivier Witasse, on behalf of the entire Mars Express project and scientific teams.
The Terrestrial Planets. Exploration of Mercury Mercury Half-Mapped.
ST9 TPWS OSS Science Needs Overview Robert M. Nelson Lead Scientist New Millennium Program Offcie California Institute of Technology, Jet Propulsion.
Lunar Surface Atmosphere Spectrometer (LSAS) Objectives: The instrument LSAS is designed to study the composition and structure of the Lunar atmosphere.
Mercury By: Edwin C. Devon S. Eduardo B.. Mercury Mercury is the smallest planet in our solar system, and it is closest to the sun, although it is the.
Juno Steve Levin Juno Project Scientist April 1, 2016.
What Juno about Jupiter?
A Global Hybrid Simulation Study of the Solar Wind Interaction with the Moon David Schriver ESS 265 – June 2, 2005.
Titan and Saturn reports June, TOST agenda.
By: Tiffany Pecorella Mercury is the first planet from the sun and looks a lot like Earth’s moon.
Adrian Martindale (on behalf of MIXS team) University of Leicester
BepiColombo Mission This mission will explore Mercury
Exploring the ionosphere of Mars
History of Earth.
Presentation transcript:

AOGS Singapore June 2005 Paper ID: 58-PS-A0321 BepiColombo – Mission to Mercury Mission Overview Rita Schulz Johannes Benkhoff

AOGS Singapore June 2005 Paper ID: 58-PS-A0321 Scientific Objectives

AOGS Singapore June 2005 Paper ID: 58-PS-A0321 Origin and evolution of a planet close to the parent star Mercury as a planet: Magnetosphere: Exosphere: Origin of Mercury’s magnetic field form, interior, geology, composition structure, dynamics, interaction with planet composition and dynamics Relativity and Gravitational Physics

AOGS Singapore June 2005 Paper ID: 58-PS-A0321 Interior:  mass, figure and moment of inertia  chemistry of the surface  surface heat flow  moment of inertia factor C/MR 2  ratio of moment of inertia factor of solid part of planet to total total moment of inertia  second degree tidal Love number k  map magnetic field, separation of internal/external sources

AOGS Singapore June 2005 Paper ID: 58-PS-A0321 Surface:  Map entire surface with a pixel size < 50 m  Characterize main features - pixel size < 10 m  Relate surface morphology to composition  Map global height distribution to 10 m accuracy on 100 km scale

AOGS Singapore June 2005 Paper ID: 58-PS-A0321 Mineralogical and Elemental Composition:  Global surface mapping  global abundance of key elements  spatially resolved measurements of elemental abundances  identify expected minerals  abundances of detected minerals  correlate composition and features  search and identify signatures of unexpected species

AOGS Singapore June 2005 Paper ID: 58-PS-A0321 Exosphere:  Composition and vertical structure  Dynamics  Search for Ionosphere  Surface release processes Search for noble gases, isotopes, molecules, atoms from crustal origin  day to night circulation  active and inactive regions (e.g. regolith, meteotites, etc.)  Exosphere/Magnetosphere exchange and transport processes

AOGS Singapore June 2005 Paper ID: 58-PS-A0321 Relativity and Gravitational Physics Test general relativity and alternative theories of gravity to a level better than by measuring the time delay and Doppler shift of radio waves, and the precession of Mercury’s perihelion Test the strong equivalence principle to a level better that 4 · Determine the gravitational oblateness of the Sun (J 2 ) to better than Set improved upper limits to the time variation of the gravitational “constant” G

AOGS Singapore June 2005 Paper ID: 58-PS-A0321 BepiColombo Elements

AOGS Singapore June 2005 Paper ID: 58-PS-A0321 Mercury Planetary Orbiter Mercury Magnetospheric Orbiter

AOGS Singapore June 2005 Paper ID: 58-PS-A0321 MMO & MPO on dedicated orbits MMO orbit optimized for study of magnetosphere MPO orbit optimized for study of planet itself  High-accuracy measurements of interior structure  Full coverage of planet surface at high resolution  Optimal coverage of polar area  Resolve ambiguities - exosphere - magnetosphere - magnetic field BepiColombo

AOGS Singapore June 2005 Paper ID: 58-PS-A0321 BepiColombo Mission Scenario

AOGS Singapore June 2005 Paper ID: 58-PS-A0321 MMO MPO CPM SEPM Launch on Soyuz 2-1B/Fregat-M (13 April 2012) Solar Electric Propulsion Chemical Propulsion Arrival: 4 April 2017

AOGS Singapore June 2005 Paper ID: 58-PS-A0321 Launch into high elliptical orbit Interplanetary cruise to Mercury Lunar fly-by and one-year Earth-to-Earth gravity assist 2 Venus and 2 Mercury gravity assists Intermediate Velocity Increment maneuvers by SEP Low-thrust cruise adopted as baseline: - Lower installed power mass for SEP - Longer thrust arcs (almost constant thrusting after Venus flybys)

AOGS Singapore June 2005 Paper ID: 58-PS-A0321 ITT release deferred ref. letter JvC 29 April 2005: –Cost estimates significantly higher than expected –Insufficient mass margin –Several risk items (S/A, SEP, HGA) Both study contractors are investigating recovery options, Main elements are: –Use conventional Chemical Propulsion –Launcher –Injection scenarios non-standard being studied –Technical optimisation wrt risk and cost reductions, towards more conventional design with potentially higher mass BepiColombo -- Project Status update

AOGS Singapore June 2005 Paper ID: 58-PS-A0321 Impact on MPO and Mission design: –Maintain MPO concept (and MMO) by both study contractors –P/L mass allocation unchanged, possible gains will be used to mitigate risks and costs, and to increase mass margins Programmatic impact: –Schedule margin for March 2012 mostly lost –AIV optimisation under investigation, –P/L delivery dates presently maintained BepiColombo - Project Status update

AOGS Singapore June 2005 Paper ID: 58-PS-A0321