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Vision and Voyages for Planetary Science in the - Solar System ...

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Mars Sample Return Orbiter <strong>and</strong> Earth Entry Vehicle<br />

MSR Orbiter an <strong>and</strong> Earth Entry Vehicle<br />

SOURCE: NASA Mission Study (transmitted from Lisa May, NASA <strong>Planetary</strong> <strong>Science</strong><br />

Division)<br />

Scientific Objectives<br />

• Detect, rendezvous, <strong>and</strong> capture Orbit<strong>in</strong>g Sample placed<br />

<strong>in</strong> orbit by Mars Ascent Vehicle<br />

• Transfer <strong>the</strong> Orbit<strong>in</strong>g Sample to an Earth Entry Vehicle<br />

(EEV)<br />

• Return <strong>the</strong> EEV to Earth<br />

• Provide a communications relay between Earth <strong>and</strong> <strong>the</strong><br />

Mars Sample Return L<strong>and</strong>er<br />

• Build Sample Process<strong>in</strong>g Facility<br />

• Key science <strong>the</strong>mes:<br />

– None<br />

Key Parameters<br />

• Payload<br />

– Optical Navigation Camera Assembly<br />

– Sample Capture <strong>and</strong> Transfer <strong>System</strong><br />

– Earth Entry Vehicle<br />

• One x 4.3 m Ultraflex solar array (1.25 kW @1AU<br />

Beg<strong>in</strong>n<strong>in</strong>g of Life) plus one unpopulated 4.3 m panel <strong>for</strong><br />

aerobrak<strong>in</strong>g<br />

• Launch Mass: 3270 kg<br />

• Launch Date: 2022 (on Atlas V 551)<br />

• Orbit: 500 km circular Mars orbit (with<strong>in</strong> ± 30 deg<br />

<strong>in</strong>cl<strong>in</strong>ation) followed by sample retrieval <strong>and</strong> Earth return<br />

Key Challenges<br />

• Sample Detection, Rendezvous, <strong>and</strong> Capture<br />

– More autonomy required than Orbital Express mission<br />

– M<strong>in</strong>imal <strong>in</strong>strumentation <strong>for</strong> rendezvous <strong>and</strong> capture<br />

• Orbiter Instrument <strong>and</strong> Communications Package<br />

Growth<br />

– Growth anticipated <strong>for</strong> onboard <strong>in</strong>strumentation<br />

– Low (10 kbps) telemetry rate unlikely to support<br />

<strong>in</strong>strument growth<br />

• Sample Transfer to EEV <strong>and</strong> Back Contam<strong>in</strong>ation<br />

– Lack of def<strong>in</strong>ition <strong>for</strong> sample transfer <strong>and</strong> encapsulation<br />

– <strong>Planetary</strong> protection methodologies to prevent back<br />

contam<strong>in</strong>ation need fur<strong>the</strong>r development<br />

• New Earth Entry Vehicle Design<br />

– Very high reliability required <strong>for</strong> new EEV design<br />

– Heritage carbon phenolic manufactur<strong>in</strong>g process needs<br />

to be rediscovered<br />

Key Cost Element Comparison<br />

Cost Risk Analysis S‐Curve<br />

PREPUBLICATION COPY—SUBJECT TO FURTHER EDITORIAL CORRECTION<br />

C-12

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