Museum Alliance Sandra Cauffman MAVEN Deputy Project Manager NASA Goddard Space Flight Center October 30, 2013 Mars Atmosphere and Volatile EvolutioN (MAVEN)

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Presentation transcript:

Museum Alliance Sandra Cauffman MAVEN Deputy Project Manager NASA Goddard Space Flight Center October 30, 2013 Mars Atmosphere and Volatile EvolutioN (MAVEN) Mission 1

Why study Mars? 2

Overarching Question: Did Mars Ever Have Life? Mars appears to meet or have met all of the environmental requirements for the occurrence of life: Liquid water Access to the biogenic elements Source of energy to drive metabolism Did Mars ever have life? How did any life interact with its planetary environment? How has the habitability of Mars changed over time?

Climate Life Human Exploration Geology WATERWATER Theme For Exploring Mars: Follow The Water The Common Thread 4

Where Did The Water Go? Where Did The CO 2 Go? Volatiles can go into the crust Volatiles can be lost to space Carbonate deposits in a Martian meteorite Abundant evidence for ancient water Escaping ions detected from Mars Express

MAVEN Science Overview Possible scenario of Mars atmospheric evolution: Turn-off of the Martian magnetic field allowed turn-on of solar-EUV and solar-wind stripping of the atmosphere approximately 4.0 billion years ago, resulting in the present thin, cold atmosphere. Where did the water and early atmosphere go? H 2 O and CO 2 can go into the crust or be lost to space MAVEN will focus on volatile loss to space Ancient Valleys MAVEN will answer questions about the history of Martian volatiles and atmosphere and help us to understand the nature of planetary habitability 6

MAVEN Will Allow Us To Understand Escape Of Atmospheric Gases To Space MAVEN will determine the present state of the upper atmosphere and today’s rates of loss to space. Measurements will allow determination of the net integrated loss to space through time.

The MAVEN Spacecraft Launch (Wet) Mass: 2550 kg max Spacecraft Dry Mass: 903 kg max Power: 1135 W at Mars Aphelion MAG (2) “Gull-Wing” Solar Arrays LPW (2) SWEA Articulated Payload Platform (IUVS/STATIC/NGIMS) Fixed HGA SWIA SEP Electra (behind)

The MAVEN Spacecraft Same length as a school bus - wingtip to wingtip length of 37.5 ft. (11.43 meters) Same weight as a fully loaded, full-size SUV 5610 lbs. (2550 kg)

MAVEN Payload Solar Energetic Particles; Davin Larson, SSL SupraThermal and Thermal Ion Composition; Jim McFadden, SSL Solar Wind Electron Analyzer; David L. Mitchell, SSL Solar Wind Ion Analyzer; Jasper Halekas, SSL Langmuir Probe and Waves; Bob Ergun, LASP Magnetometer; Jack Connerney, GSFC Neutral Gas and Ion Mass Spectrometer; Paul Mahaffy, GSFC Imaging Ultraviolet Spectrometer; Nick Schneider, LASP Mass Spectrometry Instrument Particles and Fields Package Remote-Sensing Package Electra UHF Transceiver and Helix Antenna; Larry Epp, JPL Electra Relay Package

MAVEN Will Launch On An Atlas-V Launch is scheduled for November 18, 2013 Aboard an Atlas V Rocket from the Kennedy Space Center, Florida. If we miss launch window, next opportunity is 26 months later Watch on NASA TV, Time: 1:30 pm

20-Day Launch Period: November 18 – December 7, 2013 Ten-Month Ballistic Cruise to Mars Orbit Insertion: 22 Sept 2014 One Year of Science Operations MAVEN Mission Architecture

13 MAVEN Makes Measurements Throughout The Orbit And Measures All Regions Of Near-Mars Space IUVS Coronal Scans IUVS Coronal Scans STATIC Monitor Escape

Elliptical Orbit Allows Measurement of All Relevant Regions of Upper Atmosphere Nominal periapsis near 150 km. Five “deep-dip” campaigns with periapsis near 125 km. Provide complete coverage of entire upper atmosphere

MAVEN Orbit and Primary Science Mission Elliptical orbit to provide coverage of all altitudes The orbit precesses in both latitude and local solar time One-Earth-year mission allows thorough coverage of near-Mars space

Mission Operations at Lockheed Martin, Science Operations at CU/LASP Lockheed Martin Mission Support Area LASP MAVEN Science Operations Center

MAVEN Spacecraft Early In Assembly Integration of core structure with fuel tank

Nearly Complete Spacecraft In Lockheed Martin High-Bay Cleanroom

Observatory in Environmental Testing MAVEN in Acoustics MAVEN on Shaker – Sine Vibration

MAVEN Observatory Ready To Ship

MAVEN at KSC during the solar illlumination test

From Arrival At Cape To Launch Inspect, clean, and prepare spacecraft after shipping Re-install equipment that had been removed for shipping Re-install components that had been removed for minor rework or calibration Conduct System Verification Tests to ensure that everything works properly Install pyro devices Final spin balance test Load fuel Mate spacecraft to payload support structure that will attach to upper stage Install spacecraft into payload fairing Transport to Vertical Integration Facility (VIF) and mate with Atlas booster and Centaur upper stage Roll out to launch pad (day before launch) Fuel booster and upper stage (on launch pad on day of launch) Final countdown and launch Note: Launch is a major milestone in the project, but remember that the goal is the science!