International VLBI tracking of SELENE N.Kawano, H.Hanada and K.Matsumoto NAOJ.

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International VLBI track ing of SELENE N.Kawano, H.Hanada and K.Matsum oto NAOJ

Transcript of International VLBI tracking of SELENE N.Kawano, H.Hanada and K.Matsumoto NAOJ.

Page 1: International VLBI tracking of SELENE N.Kawano, H.Hanada and K.Matsumoto NAOJ.

International VLBI tracking of SELENE

N.Kawano, H.Hanada and K.MatsumotoNAOJ

Page 2: International VLBI tracking of SELENE N.Kawano, H.Hanada and K.Matsumoto NAOJ.

Main Sat.

V-star

R-starConcept of SELENE

By T. Iwata

( JAXA)

Page 3: International VLBI tracking of SELENE N.Kawano, H.Hanada and K.Matsumoto NAOJ.

VLBI satellite (Vstar)

Solar Cell

Spin Stabilizer

Co-linear antenna

Page 4: International VLBI tracking of SELENE N.Kawano, H.Hanada and K.Matsumoto NAOJ.

Existence of core ? Internal structure ?

Given by Gusev and Kawano

Page 5: International VLBI tracking of SELENE N.Kawano, H.Hanada and K.Matsumoto NAOJ.

RSAT/VRAD

Relay satellite100km×2400km

Lunar orbiter100km±25km

JAXA/ISAS UDSC

JAXA new GN VRAD satellite100km×800km

radio source

transponder

transponder

radio source

NAOJ VERA foreign sites

Quasar

Gravity field of lunar limb (VRAD) far-side (RSAT)

TLM/CMD

From T.iwata

Page 6: International VLBI tracking of SELENE N.Kawano, H.Hanada and K.Matsumoto NAOJ.

Doppler data coverage of main satellite

●2-way Doppler●4-way Doppler

Near-sideFar-side

By K.Matsumoto

Page 7: International VLBI tracking of SELENE N.Kawano, H.Hanada and K.Matsumoto NAOJ.

VLBI obs. is effective in “Face-on”

Edge-on

Face-on

Gravity

Line of sight

Page 8: International VLBI tracking of SELENE N.Kawano, H.Hanada and K.Matsumoto NAOJ.

Improvement by VLBI

Spherical harmonics

By Rstar. By VLBI

Page 9: International VLBI tracking of SELENE N.Kawano, H.Hanada and K.Matsumoto NAOJ.

VERA Network for SELENE

Baseline~2000km

Page 10: International VLBI tracking of SELENE N.Kawano, H.Hanada and K.Matsumoto NAOJ.

0 1 day

Sep. 2007       Aug.2008

0   30 days

8 hours

Nominal VLBI observation for SELENE

Regular obs.

~12days

~12days/month x 12

Total: ~1200 hours

El>15deg.

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International VLBI Network

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MizusawaUrumqiWettzell

Time (day) From August 1215 20 25 30 35 40

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deg)

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0 1 day

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Sep. 2007       Aug.2008

0   30 days

4 hours x4

3~4 days x 2

4 hours

1 month x 2 , “Face-on”

Intensive international VLBI observation

Extended obs.

~12days

~12days/month x 2

Total: 64 hours Total: ~100 hours

Core obs. Extended Obs.

Page 14: International VLBI tracking of SELENE N.Kawano, H.Hanada and K.Matsumoto NAOJ.

Center frequency 2212 MHz 2218 MHz 2287 MHz 8456 MHz

Band width CW CW CW CW

Sample rate 200 ksps 200 ksps 200 ksps 200 ksps

Recording Hard disc

EIRP 24 mW 24 mW 24 mW 250 mW(Rstar)

38 mW(Vstar)

Polarization RHCP RHCP RHCP RHCP

Specifications of signals from Vstar and Rstar

Page 15: International VLBI tracking of SELENE N.Kawano, H.Hanada and K.Matsumoto NAOJ.

Orbits of three satellites Main orbiter Perilune Apolune Inclination Period

Main orbiter 100 km 100 km 90 deg. ~120 min.

Vstar 100 km 800km 90 deg. ~153 min.

Rstar 100 km 2400 km 90 deg. ~240 min.

Page 16: International VLBI tracking of SELENE N.Kawano, H.Hanada and K.Matsumoto NAOJ.

Thank you for your attention.