Data Relay Systems for a Mars Human Base in Meridiani Planum L. Nikulásdóttir T. Velasco

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Data Relay Systems for a Mars Human Base in Meridiani Planum L. Nikulásdóttir T. Velasco

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Data Relay Systems for a Mars Human Base in Meridiani Planum L. Nikulásdóttir T. Velasco. Scope Requirements for the Communications Critical Parameters Case by Case Analysis Summary Optical Communications Conclusions. Scope. Scope of the Study: - PowerPoint PPT Presentation

Transcript of Data Relay Systems for a Mars Human Base in Meridiani Planum L. Nikulásdóttir T. Velasco

Page 1: Data Relay Systems for a Mars Human Base in Meridiani Planum L. Nikulásdóttir T. Velasco

Data Relay Systems for a Mars Human Base in Meridiani Planum

L. NikulásdóttirT. Velasco

Page 2: Data Relay Systems for a Mars Human Base in Meridiani Planum L. Nikulásdóttir T. Velasco

1. Scope2. Requirements for the Communications3. Critical Parameters4. Case by Case Analysis5. Summary6. Optical Communications7. Conclusions

Page 3: Data Relay Systems for a Mars Human Base in Meridiani Planum L. Nikulásdóttir T. Velasco

1. Scope

Scope of the Study: • Identify the Requirements and Criticalities for Communications

with the Mars Surface• Analyse the Main options for Mars-Earth Relay Satellite• Identify the best Strategy for a Mars Human Base in Meridiani

Planum Base

Meridiani Planum is located close to the Equator (1.9S; 354.5E)

Page 4: Data Relay Systems for a Mars Human Base in Meridiani Planum L. Nikulásdóttir T. Velasco

2. Requirements for the Communications

• Current Systems – not communication satellites• NASA Mission Mars Telecommunications Orbiter (2009)• Demanding Requirements for a Human Mission

Mars Odissey, source: NASA/JPL

Mars Telecommunications Orbiter, source: NASA/JPL

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2. Requirements for the Communications

• High Data Volume Communications

• High Data Rate Communications

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• “Continuous” Communications - occultations

2. Requirements for the Communications

• Reliability of the System

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• Missions Survey

2. Requirements for the Communications

Mission Year / Agency Data Rate to Earth

Mars Global Surveyor 1996 / NASA ~10kbps

Mars Odyssey 2001 / NASA ~14kbps

Mars Express 2003 / ESA ~97kbps

Mars Reconnaissance Orbiter 2005 / NASA ~200kbps

Mars Telecommunications Orbiter 2009 / NASA ~1Mbps

Data rates from Mars orbiting spacecraft to Earth. Values are estimated for the maximum distance Earth to Mars

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3. Critical Parameters for Communications

• Data Rates

• Link Visibility Mars Surface to Earth• Link Visibility Mars Surface to Relay Satellite• Link Visibility Relay Satellite to Earth• Technical Feasibility (by 2019) and Costs (v)

• Reliability/Redundancy

KdBJKdBTGdBNEdBLdBmEIRPbpsBR RXrequiredbPROPTX /6.198)/(/)(/)()()( ,0

orbincreq vvv vr

v MARSinc

2

Page 9: Data Relay Systems for a Mars Human Base in Meridiani Planum L. Nikulásdóttir T. Velasco

4. Case by Case Analysis

Low Mars Orbit

• Used for MER through Mars Odissey and MGS

• Typically 400km – Polar/Sun-synchronous

• Low Coverage (2%)• Low Data Volume• Constellations increase

performances

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4. Case by Case Analysis

Medium Mars Orbit

• Increases coverage time• MTO (2009)• Higher v for insertion

Page 11: Data Relay Systems for a Mars Human Base in Meridiani Planum L. Nikulásdóttir T. Velasco

4. Case by Case Analysis

High Elliptical Orbit

• Higher coverage• Continuous communication

possible with two satellites • Low v required for insertion

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4. Case by Case Analysis

Areostationary Orbit

• Equivalent to Geostationary orbit for Earth• Continuous coverage of the surface• Two satellites would provide continuous link with Earth• High v required• Needs orbit corrections

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4. Case by Case Analysis

Mars Moons

• Use of Phobos or Deimos orbiters• Performances are not very high

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4. Case by Case Analysis

Mars Occultation

• The Sun or Moon is between Mars and the Earth

• Occultation by the Moon is short (28 minutes)• Occultation by the Sun can happen each approx. 2 years, and can last

up to 3 weeks• Occultation by the Sun will not occur in 2019 nor 2021

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4. Case by Case Analysis

“Trojan” Orbit

• Satellite located in L4 or L5 Earth-Sun Lagrange points

• Not optimal performances, but solves the problem of occultation

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4. Case by Case Analysis

Lagrange Points

• Use L1 and L2 Sun-Mars • Good coverage• Low data rates (high

distance from Mars orbit)• High v needed

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5. Summary

Orbit Bit Rate Coverage Comments/Pro’s/Con’s

LMO low lowBig Constellation needed/ Low cost / Low performance

MMO high medConstellation needed / better performances / High cost

HEO high med/ high> two S/C needed / Low cost/ Performances are limited

Stationary very high high> two S/C needed / Best performances / Very high cost

Trojans med med For Mars occultations

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6. Optical Communications

• Limitation of the RF Systems• Limitation of the Bit Rates – increasing absorption• Laser Communications are the alternative• Technical Challenges: accurate pointing, cloud and dust

attenuation, components, etc• Mars Telecommunications Orbiter – Mars Laser

Communications Demonstration (MLCD)

MTO Laser communications, source: NASA/JPL

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7. Conclusions and Recommendations

• High Bit Rate and Continuous Coverage are Mandatory for a Human Mission on Mars

• Constellation of HEO or Areostationary seems to be the best solution. HEO is preferred for the low v needed for insertion

• Further Work to Optimise the Concept (Failure Recovery Modes)

• Development of Optical Communications would be big step forward

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The end

or… …The Beginning?