DSL$Mission$ConceptatLunar$Orbit - ASTRON · Space engineering solution • Launch into lunar orbit...

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DSL Mission Concept at Lunar Orbit Jingye Yan Na9onal Space Science Center (NSSC) Chinese Academy of Sciences (CAS) 1 20150202, ASTRON, The Netherland

Transcript of DSL$Mission$ConceptatLunar$Orbit - ASTRON · Space engineering solution • Launch into lunar orbit...

Page 1: DSL$Mission$ConceptatLunar$Orbit - ASTRON · Space engineering solution • Launch into lunar orbit by LM-2D or Vega plus an Launch upper stage • CCSDS Proximity-1 • SOIS Wireless

DSL  Mission  Concept  at  Lunar  Orbit

Jingye  Yan    

Na9onal  Space  Science  Center  (NSSC)  Chinese  Academy  of  Sciences  (CAS)  

1 2015-­‐02-­‐02,  ASTRON,  The  Netherland

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Payload  onboard  single  nano-­‐sat

2 Element  antenna

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Outline

•  Requirements •  Mission  concept  and  preliminary  design

•  Summary

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Qualita9ve  requirements

•  RFI  free/minimum  – Moon  shielding  is  beRer  than  mi9ga9on  

•  Long  baseline  for  high  resolu9on  – Long  distance  high  speed  communica9on  

•  Dense  UV  coverage  – Discover  unknowns  

•  S-­‐mission  

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Quan9ta9ve  requirements

•  Angular  resolu9on  •  Frequency  •  Spectral  resolu9on  •  Integra9on  9me  •  Polariza9on  

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Array  design  =  Op9mize  the  UV  coverage

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DSL  array  at  Lunar  orbit

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•  Linear  array  along  the  same  orbit  •  Dish  UV  coverage  every  half  orbit  •  Baseline’s  length  varies  from  orbit  to  orbit  

by  maneuver,  Full  UV  coverage  (Nyquist)  every  10  days  

•  UV  coverage  is  configurable  in  orbit  according  to  parEcular  scienEfic  goal  

•  Linear  array  simplifies  the  formaEon  maintenance  and  maneuver  

•  30%  of  the  life  Eme  is  RFI  FREE  

Example  array:  1    4    10    22    24    35    39    52    63    71    74    78    79  km  

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Snapshot

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u-­‐v-­‐w  filling  •  3-­‐D  u-­‐v  filling  a`er  a  full  precession  period  (360°);  •  In  DSL  case,  ~450  days  is  required  to  have  a  full  u-­‐v  filling  in  3-­‐D(0.76°  

precession  per  day);    

6°  precession  per  orbit  is  assumed  for  beRer  demonstra9on.  

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Moon  blockage

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Earth-­‐Moon  system  and  RFI  free

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•  30%  RFI  free  •  60%  coverage  (taking  into  

account  the  conjugate  points)  •  RFI  mi9ga9on  (if  works)  

improves  the  coverage

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RFI  free  +  precession

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RFI  free  +  Moon  blockage  +  precession

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Make  denser  coverage  in  UV  plane

Advantages:    ü   Easy  change  the  baseline  in  a  linear  array  ü   Dense  and  controllable  coverage    ü   Image  quality  is  improving  orbit  by  orbit  

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Mission concept

mother

daughter

control

Scientific data Status control

Wireless bus

communication

p  Linear formation flying

p  Central correlation/control

p  Downlink from the mother

Ground station

daughter

daughter

daughter

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Mission  concept  

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Baselines  change  from  100km  to  100m  within  5  days  needs  15g  cold  gas  for  12  satellites  maneuver  

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Satellite  

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Mission  Concept

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Target  orbit  analysis  

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Orbit  al9tude:  300km  Sun/Earth  free:  30%  

l Perfect  RFI  free  l 1  or  more  strong  sources  will  be  blocked  9me  to  9me,  enabling  diverse  comparisons  l Orbit  is  stable,  no  crash  will  be  happened  l Easier  to  avoid  satellites  collision  

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Antenna  field  of  view

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31.8° 1700km

1700km 300km

Moon

Earth

Sun

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Integrated  Electronic  Subsystem(IES)

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PowerDistributor

On-Board Computer

Mass Memory

Payload Interface

PowerSource

Attitude and Orbital

Control Sensor

Lock/unlock Controller

Thermalcontrol sensor Payload

InterSatelliteSynchronization&Communication

Transponder/Transmitter

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Communica9on,  Ranging  and  Time  Synchroniza9on

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1T

2t tΔ+τ 1r

1t tΔ−τ 2r

2T

ÖÕ¶ËA·¢ËÍ

ÖÕ¶ËB·¢ËÍ

ÖÕ¶ËA½ÓÊÕ

ÖÕ¶ËB½ÓÊÕ

Dual  One-­‐way  Ranging,DOR

Ta

Tb

Ra

Rb

Ranging Precision under Current Link Situation: 2cm

Time  Synchroniza9on

crrttTTD ⋅+−+−+⋅= )]()()[(21

212121 )]()()[(21

211221 rrttTTt −−−−−⋅=Δ

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Ajtude  control  and  baseline  determina9on

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•  Mother  sat  –  1  orbit  control  thruster,  12  ajtude  control  thrusters  and  4  momentum  wheels.  

•  Daughter  cubesat  –  1  bias  momentum  wheel  and  8  ajtude  control  thruster.    

baseline

baseline  determina9on  CCD  camera  of  0.01°angular  resolu9on

x

z

y

Bias momentum wheel

1A

1B

2A

2B

3A

3B

4A

4B

Ajtude  control  

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Radio  interferometry  

Rx2

Rx/Tx Mothership

Daughter Satellite

Rx1

One  main  and  two  sub  antennas  is  mounted  on  the  Mothership.  The  angle  of  arrival  (AOA)  is  measured  by  interferometry  between  antennas.

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Naviga9on

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INS

Ground remote measure

Star tracker

Mother satellite

Absolute position infomation

Attitude infomation

Relative distance meausre

Relative angle meausre

+

+

Relate position

Daughter satellite

DS Abs position

MS Abs positon

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Power  Subystem •  Power  subsystem  component  

–  Solar  panel  –  Lithium  Ion  baReries  –  power  management  and  distribu9on  system  

solar  panel  

power  management  

Lithium  Ion  batteries

Powerdistribution   output

The  block  diagram  of  power  subsystem

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Down  link  requirement

Assump9on:    correlate  30MHz  bandwidth  at  the  same  9me  (not  possible  for  ISL)  

•  13.2Mbps    •  6.6Mbps  (far  side  observa9on,  near  side  download)  •  High  gain  antenna  is  mandatory

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0

0

2

1 rfi-free= :

( )2

_( )

m

n ls

f f f

Tcff L

p Wdata rate Tf

τ ηπ

τ

=

⋅= ∑

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TT&C  Solu9on

TT&C

Transponder

TC

TM

USO

Crosslink(ISL) subsystem

PA

DUP LGA1

LGA2

BASE

SW

OBDH

PD

HGA

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In  orbit  calibra9on •  Rela9ve  amplitude  calibra9on  by  cosmic  background  

radia9on  •  Rela9ve  amplitude  and  phase  calibra9on  by  calibra9on  signal  

from  Mother  •  Absolute  amplitude  calibra9on  by  matched  load  and  cosmic  

background  •  Mothership  is  difficult  to  be  used  as  a  part  of  the  array

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High  speed  downlink  (op9onal)  Phased  array  antenna–  no  moving  parts  Reflector  antenna-­‐  light  and  easier

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Space engineering solution

•  Launch into lunar orbit by LM-2D or Vega plus an upper stage Launch

•  CCSDS Proximity-1 •  SOIS Wireless bus

•  Dual One-way Ranging,DOR Relative distance

•  Dual time comparison Time synchronization

•  Relative distance •  Relative spatial angle Relative positioning

•  Star tracker Attitude measurement

•  Space-borne radio synthetic aperture radiometer with 12 nano-satellites Payload

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Mission:  •  Orbit:                                                            300  km  •  Number  of  satellites:      13  (1  mother  +  12  daughters)  •  Mass:  300kg    

                                                                   Mother:  180kg                                                                                                      Daughters:  10kg*12  

•  Power:    15W*12  +  1200W    •  Downlink  rate:                            <20Mbps  (onboard  correlaEon);    

       >100  Mbps  (raw  data,  HGA)  •  Life  Eme:                                              3  years  

Payload  •  Frequency  range:  0.3  ÷  30  MHz  •  PolarizaEon:  Full-­‐pol  (circular  pol) •  Antenna:  Cross  dipole,  2.5  m  each  sEck  •  Baseline:          100  m  to  100  km      •  Angular  resoluEon:        6’@  1  MHz,    12”@30  MHz  •  VisibiliEes:                                          ≈  54K  (half  orbit),  59M  (20  days)    

Preliminary  specificaEons

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Mass  and  Power  consump9on •  Mother  satellite  mass  and  power  consump9on

Subsystem Subsystem Mass(kg)

Subsystem Power(W)

ADCS 3.87 6.6 Power 40.00 0.0 Propulsion 65.00 1100.0 Structure 50.00 0.0 Thermal 6.00 8.0 Communications 7.86 97.0 Payload 4.00 25.0 Data Handling 1.40 9.0 Total 178.13 1229.6

The mass of mother

satellite is 178.13kg, and

power is 1229.6W.

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Mass  and  Power  Consump9on •  Daughter  satellite  mass  and  power  consump9on

Subsystem Subsystem Mass(kg)

Subsystem Power(W)

ADCS 1.08 2.3 Power 1.55 0.0 Propulsion 0.60 2.0 Structure 2.00 0.0 Thermal 1.00 1.0 Communications 0.50 6.0 Payload 2.00 1.5 Data Handling 0.60 3.0 Total 9.33 15.8

The mass of daughter

satellite is 9.33kg, and

power is 15.8W.

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Summary

•  High  reliability  observa9on  with  Moon’s  shield  •  Longer  baseline  is  available  due  to  HGA  by  linear  array  

•  Denser,  univform  and  controllable  UVW  coverage  

•  High  performance  and  feasible  within  the  envelop  of  S-­‐mission  is  pre-­‐studied  

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