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The MAVEN Mission: Exploring Mars’ Climate History Sandra Cauffman, NASA/GSFC https://ntrs.nasa.gov/search.jsp?R=20150022427 2018-05-19T12:32:49+00:00Z

The MAVEN Mission: Exploring Mars’ Climate History · PDF fileThe MAVEN Mission: Exploring Mars’ Climate History Sandra Cauffman, NASA/GSFC 2018-01-19T11:54:32+00:00Z

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Page 1: The MAVEN Mission: Exploring Mars’ Climate History · PDF fileThe MAVEN Mission: Exploring Mars’ Climate History Sandra Cauffman, NASA/GSFC   2018-01-19T11:54:32+00:00Z

The MAVEN Mission: Exploring Mars’ Climate History

Sandra Cauffman, NASA/GSFC

https://ntrs.nasa.gov/search.jsp?R=20150022427 2018-05-19T12:32:49+00:00Z

Page 2: The MAVEN Mission: Exploring Mars’ Climate History · PDF fileThe MAVEN Mission: Exploring Mars’ Climate History Sandra Cauffman, NASA/GSFC   2018-01-19T11:54:32+00:00Z

The Science

Page 3: The MAVEN Mission: Exploring Mars’ Climate History · PDF fileThe MAVEN Mission: Exploring Mars’ Climate History Sandra Cauffman, NASA/GSFC   2018-01-19T11:54:32+00:00Z

Mars Earth

Page 4: The MAVEN Mission: Exploring Mars’ Climate History · PDF fileThe MAVEN Mission: Exploring Mars’ Climate History Sandra Cauffman, NASA/GSFC   2018-01-19T11:54:32+00:00Z
Page 5: The MAVEN Mission: Exploring Mars’ Climate History · PDF fileThe MAVEN Mission: Exploring Mars’ Climate History Sandra Cauffman, NASA/GSFC   2018-01-19T11:54:32+00:00Z

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?

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Evidence for Surface Water on Ancient Mars Where Did the Water Go? Where Did the CO2 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

Page 7: The MAVEN Mission: Exploring Mars’ Climate History · PDF fileThe MAVEN Mission: Exploring Mars’ Climate History Sandra Cauffman, NASA/GSFC   2018-01-19T11:54:32+00:00Z

MAVEN Will Allow Us to Understand Escape of Atmospheric Gases to Space

Page 8: The MAVEN Mission: Exploring Mars’ Climate History · PDF fileThe MAVEN Mission: Exploring Mars’ Climate History Sandra Cauffman, NASA/GSFC   2018-01-19T11:54:32+00:00Z

The Solar Wind is Able to Strip Off Gas from the Top of the Atmosphere

Page 9: The MAVEN Mission: Exploring Mars’ Climate History · PDF fileThe MAVEN Mission: Exploring Mars’ Climate History Sandra Cauffman, NASA/GSFC   2018-01-19T11:54:32+00:00Z

The Mission

Page 10: The MAVEN Mission: Exploring Mars’ Climate History · PDF fileThe MAVEN Mission: Exploring Mars’ Climate History Sandra Cauffman, NASA/GSFC   2018-01-19T11:54:32+00:00Z

The MAVEN Spacecraft •  Launch (Wet) Mass: 2455 kg at launch •  Spacecraft Dry Mass: 810 kg at launch •  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

SEP

Electra (behind)

Page 11: The MAVEN Mission: Exploring Mars’ Climate History · PDF fileThe MAVEN Mission: Exploring Mars’ Climate History Sandra Cauffman, NASA/GSFC   2018-01-19T11:54:32+00:00Z

The MAVEN Science Instruments:

Page 12: The MAVEN Mission: Exploring Mars’ Climate History · PDF fileThe MAVEN Mission: Exploring Mars’ Climate History Sandra Cauffman, NASA/GSFC   2018-01-19T11:54:32+00:00Z
Page 13: The MAVEN Mission: Exploring Mars’ Climate History · PDF fileThe MAVEN Mission: Exploring Mars’ Climate History Sandra Cauffman, NASA/GSFC   2018-01-19T11:54:32+00:00Z

Launched on 18 Nov. 2013,

first day of its 20-day launch

period Launch Vehicle:

Atlas – V 401

Ten-Month Type-II Ballistic Cruise to Mars

Orbit Insertion: 22 Sept 02:00, 2014 UTC. 33 minute rocket burn

MAVEN Mission Architecture

One Year of Science Operations

Page 14: The MAVEN Mission: Exploring Mars’ Climate History · PDF fileThe MAVEN Mission: Exploring Mars’ Climate History Sandra Cauffman, NASA/GSFC   2018-01-19T11:54:32+00:00Z

MAVEN’s Path To Mars

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Mars Orbit Insertion Preparations

• • • 

• • 

• 

Page 16: The MAVEN Mission: Exploring Mars’ Climate History · PDF fileThe MAVEN Mission: Exploring Mars’ Climate History Sandra Cauffman, NASA/GSFC   2018-01-19T11:54:32+00:00Z
Page 17: The MAVEN Mission: Exploring Mars’ Climate History · PDF fileThe MAVEN Mission: Exploring Mars’ Climate History Sandra Cauffman, NASA/GSFC   2018-01-19T11:54:32+00:00Z

The MAVEN Team that Got Us Here

Page 18: The MAVEN Mission: Exploring Mars’ Climate History · PDF fileThe MAVEN Mission: Exploring Mars’ Climate History Sandra Cauffman, NASA/GSFC   2018-01-19T11:54:32+00:00Z

The Comet

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Cosmic Serendipity

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The Problem

Page 21: The MAVEN Mission: Exploring Mars’ Climate History · PDF fileThe MAVEN Mission: Exploring Mars’ Climate History Sandra Cauffman, NASA/GSFC   2018-01-19T11:54:32+00:00Z

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HST Image of Siding Spring

What you see in this image is dust

Page 22: The MAVEN Mission: Exploring Mars’ Climate History · PDF fileThe MAVEN Mission: Exploring Mars’ Climate History Sandra Cauffman, NASA/GSFC   2018-01-19T11:54:32+00:00Z

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An image of comet Halley taken by the camera on ESA’s Giotto spacecraft. Giotto was hit by a large dust particle and took 30 minutes to recover.

Giotto Image of comet Halley

Page 23: The MAVEN Mission: Exploring Mars’ Climate History · PDF fileThe MAVEN Mission: Exploring Mars’ Climate History Sandra Cauffman, NASA/GSFC   2018-01-19T11:54:32+00:00Z

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Interplanetary Dust Particle

Page 24: The MAVEN Mission: Exploring Mars’ Climate History · PDF fileThe MAVEN Mission: Exploring Mars’ Climate History Sandra Cauffman, NASA/GSFC   2018-01-19T11:54:32+00:00Z

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Actually, Not So Bad

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IUVS Imaging of Comet Siding Spring

•  IUVS imaged CSS in scattered solar Lyman-alpha two days before closest approach to Mars

•  Reflects distribution of atomic H surrounding comet

•  H detected to distance of ~150,000 km (comparable to Mars miss distance of comet)

•  Gas cloud behaves differently from dust; dust comprises bulk of tail and is what is seen in visible images, so LyA images looks different from most telescopic images

Page 26: The MAVEN Mission: Exploring Mars’ Climate History · PDF fileThe MAVEN Mission: Exploring Mars’ Climate History Sandra Cauffman, NASA/GSFC   2018-01-19T11:54:32+00:00Z

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SIDING-SPRING

The Opportunity

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Strategy: Duck and Turn Off High Voltage

Page 28: The MAVEN Mission: Exploring Mars’ Climate History · PDF fileThe MAVEN Mission: Exploring Mars’ Climate History Sandra Cauffman, NASA/GSFC   2018-01-19T11:54:32+00:00Z

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Complications

Page 29: The MAVEN Mission: Exploring Mars’ Climate History · PDF fileThe MAVEN Mission: Exploring Mars’ Climate History Sandra Cauffman, NASA/GSFC   2018-01-19T11:54:32+00:00Z

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SIDING-SPRING

An Embarrassment of Riches

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Drama In The Control Room

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A Peak at Results: Dust After All

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IUVS False-Color Image of Mg+2 Distribution

•  Observed throughout periapsis pass of each orbit following comet passage •  Intensity of emissions decayed in hours to days, likely due to conversion of

Mg and Fe to other forms

Page 33: The MAVEN Mission: Exploring Mars’ Climate History · PDF fileThe MAVEN Mission: Exploring Mars’ Climate History Sandra Cauffman, NASA/GSFC   2018-01-19T11:54:32+00:00Z

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A Peak at Results: Dust After All

Page 34: The MAVEN Mission: Exploring Mars’ Climate History · PDF fileThe MAVEN Mission: Exploring Mars’ Climate History Sandra Cauffman, NASA/GSFC   2018-01-19T11:54:32+00:00Z

The Planet

Page 35: The MAVEN Mission: Exploring Mars’ Climate History · PDF fileThe MAVEN Mission: Exploring Mars’ Climate History Sandra Cauffman, NASA/GSFC   2018-01-19T11:54:32+00:00Z

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SEP Observes a Coronal Mass Ejection (CME) Arriving at Mars

Page 36: The MAVEN Mission: Exploring Mars’ Climate History · PDF fileThe MAVEN Mission: Exploring Mars’ Climate History Sandra Cauffman, NASA/GSFC   2018-01-19T11:54:32+00:00Z

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Magnetometer Measures Interactions With Solar Wind

| B |

•  Field draped over conducting ionosphere •  Lots of wave activity evident in sheath and associated with bow shock

September 23

Page 37: The MAVEN Mission: Exploring Mars’ Climate History · PDF fileThe MAVEN Mission: Exploring Mars’ Climate History Sandra Cauffman, NASA/GSFC   2018-01-19T11:54:32+00:00Z

Martian Dayglow: Determining the Upper Atmospheric Composition

FUV channel MUV channel In

tens

ity

H

O

CO2+

Inte

nsity

108 nm 190 nm 330nm 330nmn

l190 10

Page 38: The MAVEN Mission: Exploring Mars’ Climate History · PDF fileThe MAVEN Mission: Exploring Mars’ Climate History Sandra Cauffman, NASA/GSFC   2018-01-19T11:54:32+00:00Z

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IUVS Maps Changing Mars Ozone

Page 39: The MAVEN Mission: Exploring Mars’ Climate History · PDF fileThe MAVEN Mission: Exploring Mars’ Climate History Sandra Cauffman, NASA/GSFC   2018-01-19T11:54:32+00:00Z

39 MAVEN PSG, 12/5/2014

Atmospheric Density at Orbital Altitudes Shows Seasonal Trend

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IUVS Observations of Components of H2O and CO2 on Their Way to Escaping

Page 41: The MAVEN Mission: Exploring Mars’ Climate History · PDF fileThe MAVEN Mission: Exploring Mars’ Climate History Sandra Cauffman, NASA/GSFC   2018-01-19T11:54:32+00:00Z

Launch Year

MRO

Mars Express Coop

Odyssey

MER

2013 2016 2018 & Beyond 2011 2009 Operational / Recent

MAVEN

Mars Science Lab

NASA s Mars Exploration Program

Mars 2020

InSight

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MAVEN Impacts All Ages

MAVEN “Send your artwork to Mars” contest, 2013

LASP Clean Room Tour, 2012 Little Miss MAVEN, Halloween, 2014

Page 43: The MAVEN Mission: Exploring Mars’ Climate History · PDF fileThe MAVEN Mission: Exploring Mars’ Climate History Sandra Cauffman, NASA/GSFC   2018-01-19T11:54:32+00:00Z

•  MAVEN launched on schedule and under budget! •  It arrived at Mars in September and began its science

mission in November! •  Just beginning to get science results – stay tuned!

Go MAVEN! [Continue to follow us on Facebook and Twitter: MAVEN2MARS]

[Join MAVEN and Exploration Station – 1-5 p.m. today for hands-on exploration for the family.]