LunarSmallBody 6 BAILET presID485 PresSlides docID1162

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G. Bailet 1 Master Students 2 : Romain Bossis, Maxime Carpentier, Florent Clouvel, Rémy Derollez, Barry Eich, Tarik Errabih, Thomas Hancock, Marcus Hott, Fernando Hübner, Emmanuel Jehanno, Jean-Michel Klein, Elena Kostaropoulou, Eliott Lindsay, Eve Pachoud, Quentin Paletta Etienne and Rouanet-Labé SIRONA - a low-cost plaYorm for lunar explora[on – Ch. O. Laux 1 1 Laboratoire EM2C, CNRS, CentraleSupélec, Université Paris-Saclay, France 2 CentraleSupélec, Université Paris-Saclay, France

Transcript of LunarSmallBody 6 BAILET presID485 PresSlides docID1162

SIRONA – June 14th 2018IPPW Presentation

G. Bailet1

Master Students2:Romain Bossis, Maxime Carpentier, Florent Clouvel, Rémy Derollez, Barry

Eich, Tarik Errabih, Thomas Hancock, Marcus Hott, Fernando Hübner, Emmanuel Jehanno, Jean-Michel Klein, Elena Kostaropoulou, Eliott Lindsay,

Eve Pachoud, Quentin Paletta Etienne and Rouanet-Labé

SIRONA- a low-cost plaYorm for lunar explora[on –

Ch. O. Laux1

1Laboratoire EM2C, CNRS, CentraleSupélec, Universite Paris-Saclay, France2CentraleSupélec, Universite Paris-Saclay, France

SIRONA – June 14th 2018IPPW Presentation2

Overview

Context

Mission Objectives

Mission Profile

Pla7orm Design

ASTERICS / OBELICS

Technological Blocks

Conclusion

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CS3 – Federa*ng Decades of Experience in the Space Field

• Brand new campus located at the south border of Paris, France

• A FabLab/MakerSpace and high level research facilities ranging fromAntenna testing to high enthalpy plasma torch

• 5 research labs and 7 departments of CentraleSupélec collaborating forthe projects of the Space Center (CS3)

• 2017-2018: 15 students

• On the horizon 2020: 30-40 professors/research engineers+ 120 students contributing to the CS3 projects

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Mission Objectives

Industrial Objec5ve (OBELICS)

Ø Op5mize Radia5on Shielding for future

human mission farther than LEO (CislunarSta9on, Lunar/Mar9an colonies…)

Ø Study the effect of Radia5ons on biological samples

Ø Gather long term data surpassing Apollo program that lasted a maximum of 7 days at a 9me

Scien5fic Objec5ve (ASTERICS)

Ø Test the hypothesis of the Lunar Cataclysm

Ø Demonstrate the capabili9es of a deployable telescope for Cube/SmallSats

Ø Improve database of LRO with addi9onal data and different lightning condi9ons

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Mission Profile

Cislunar Orbit < 6 months(using WB and manifolds)

Science Orbit > 6 months

Polar Orbit from PSLV

to reduce van Allen belt exposure

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Pla%orm design

SIRONAUndeployed configura<on

(le>: scaling reference)

SIRONADeployed configuration

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Pla%orm design

SIRONAUndeployed configura<on

SIRONADeployed configuration

(Saint-Emilion W ine Bottles are for scale purposes and are not intended to promote the amazing french products)

SIRONA – June 14th 2018IPPW Presentation

System description

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Pla3orm design

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Electrical Power System

Payload

ADCS

IMU

Star Tracker

Sun Sensors

Magnetotorquers

GPS Receiver

Reactionwheels

Battery

Power RegulaHonand Conversion

Communication

UplinkSband

DownlinkXband

Transceiver

UHF VHF antennaUHF VHF Transceiver

Petri Dish

Telescope

CMOS Magnetometer

Dosimeter

Science Card Propulsion System

Propellant tank

Main thrusters

PPT

Prop Power Unit

Thermal System

Heaters Thermal Sensors

Command and Data Handling

Flight Computer

Auxiliary boards

Data Interface

Radiation Protection

Information Flow Energy Flow

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Pla%orm design

SIRONA subsystems(front view)

SIRONA subsystems(back view)

BaFeries

Electric Power System (EPS)

TransceiverTx: X-bandRx: S-band

Command & Data Handling

On Board Computer

Ergol Tank &Propulsion

Management Unit

Electric Propulsion

Engine

Pulsed Plasma Thrusters

(Momentum Wheels desaturation)

AWtude DeterminaXon

and Control Unit(ADCS)

7 units available for payloads and system margins

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ASTERICS : Deployable TelescopeTime dependence of the Lunar cratering rate (Neukum 1983)

Ø Test the cataclysm hypothesis by providing high resoluLon images and detect all crater larger than 100 m of diameter

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ASTERICS : Deployable TelescopeNon deployable

CubeSat capabilities(simulated @ 200 km)

SIRONA capabilities(simulated @ 200 km)

Lunar Reconnaissance Orbiter (best data available, @50 km)

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ASTERICS : Deployable TelescopeNon deployable

CubeSat capabilities(simulated @ 200 km)

SIRONA capabilities(simulated @ 200 km)

Lunar Reconnaissance Orbiter (best data available, @50 km)

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ASTERICS : Deployable TelescopeDeployment strategy

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ASTERICS : Deployable TelescopeDeployment strategy

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ASTERICS : Deployable TelescopeDeployment strategy

• Ritchey-Chré@en architecture

• f/10 design

• Highly compact when stowed

• Scalable for any mission/plaKorm

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ASTERICS : Deployable TelescopeDeployment validation of ASTERICS’s concept

• Low mass/volume (x5 deployment factor, < 500 g)

• Passive deployment method (hot knife)

Ø Next step: Validate alignment (with piezo subtrate) on a Zero-g flight

See Tarik Errabih’s poster

SIRONA – June 14th 2018IPPW Presentation

OBELICS : Biological Experiment

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LED

SHIELDING

Photodiod

e

Phase change material

coil heater

filter for entering/exiting growth medium

OBELICS’ deployment Wells’ design

• Low mass/volume (tesKng with 10 to 100 wells, < 500 g)

• Passive deployment method (hot knife) allowing higher exposure to the radiaKon

• ValidaKon of the protocol this summer (with LPGP)

Ø Next step: Test of the payload in a relevant environment (alpha and proton accelerator at CEA)

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Technological Blocks

Cells arrangement and op7mized structure Radia7on Shielding using HDPE and Mylar (SPENVIS)

e=1 mm e=4 mm

Composite structure

Radiation shielding panels

Ø Next step: Test of the composite structure in a relevant environment(alpha and proton accelerator at CEA)

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Technological BlocksMomentum wheel desaturation with small plasma thrusters

Proof of concept Successful 1st

test campaign Final Concept

• Compact solu9on able for desatura9on of the wheels around on the 3 axis

• Extend life9me of the mission

• Increase volume/mass budgets compared to cold gas solu9ons

• Allows fine maneuvers if needed

Ø Next step: Reach TRL5 and test @ONERA (μN level performance tesKng)

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Technological BlocksPanel Array Drive Assembly

PADA integra:on on SIRONA PADA integra:on on SIRONA

• Allows fine pointing of the Sun (solar panels)

• Allows fine pointing of the Ground Station (S/X-band micro patch array antenna)

• Increase Power and Data budgets

• Use “free volume” for the assembly (no impact on the payload accommodation)

• Increase EPS and COMS redundancy

See Marcus Hott’s poster

Ø Next step: Refine the design for 3 to 27U and propose it to the CubeSat Missions

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Conclusion

Subsystems Mass (in g)

Structure 1700Radiation Shield 150

Thermal Components 150Solar Panels 900

Power Board (EPS) 110Solar Panel Motor 20

Battery 1000

Command and Data Handling 300

Antenna 1 (DOWNLINK) 64Antenna 2 (UPLINK) 65

Beacon UHF/VHF (for AMSATs) 85Transmitter 50

Receiver 50IMU 80

Star Trackers 200Sun Trackers 36GPS Receiver 45

Reaction wheels 1200PPT 300

Main Propulsion 4500Deployable Telescope 500Biological Experiment 385

Dosimeter 32

TOTAL 11922

• SIRONA is a feasible and realis]c low cost pla^orm for lunar explora]on Ø only 12kg (including ASTERICS and OBELICS)

• Industrial interest

Ø Qualifying radia]on shielding in relevant environment for future human missions

• Scien]fic interest Ø tes]ng the cataclysm hypothesis for research on

the solar system history

Large Volume/Mass available (8 kg) for otherexperiments or technology demonstra]on in lunarenvironment

Ø SIRONA is aiming to become a space bus for the lunar explora]on community providing with

• high downlink capabili]es • Trouble-free pla^orm integra]on and

maintenance for the hosted payload

Thank you for your attention

The research leading to these results has received funding andsupport from THALES ALENIA SPACE, EM2C andCENTRALESUPELEC

Special thanks:Jean-Loic Galle, Phillipe Lamotte and Christophe Valorge (TAS)Sébastien Ducruix, Noï Lavaud, Brigitte Llobel, NathalieRodrigues, Erika Jean-Bart, Jérôme Beaunier, Yannick Le teno,David Charalampous, Sébastien Turgis and Jean-Michel Dupays(EM2C)Filipa Lopes and Arnaud Bush (LGPM)Laurent Cabaret, Didier Coudray and Hanane Meliani (LaFabrique)Jean-Claude Vannier, Tanguy Phulpin, Mike Kirkpatrick andEmmanuel Odic (Geeps)Cécile Oriot and Sylvain Leclercq (Com’ CentraleSupélec)

The IPPW comity for accepting this oral presentation

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EPS - Electrical Power System

èLarge deployable solar panels. Direct them always towards the sun.èDevelopment of the PADA

0

200

-1000-500

0500 01000 200

Structural specification : SIRONA 12U 3 panels deployed.xls

y [ mm ]

z [

mm

]

x [ mm ]

12U CubeSat with large deployed solar panels

SIRONA – June 14th 2018IPPW Presentation

COMS - Communications

PARAMETER VALUESignal/GeneralDownlink Frequency Band X-Band

Uplink Frequency Band S-BandSignal Polarization Circular polarisation

Modulation Scheme QPSKMinimum elevation angle 15°

SIRONA TxPower 5.0W

Antenna Gain 25.0dBiAntenna type Micropatch-array

SIRONA RxAntenna Gain 1.0dBi

Summary of SIRONA’s parameters in the lunar phase

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First Stage Deployment

Final Deployed Configuration

Release Mechanism

Panels deployment by springs

Stops

ASTERICS : Deployable Telescope