Transcript 石黒 正晃
2009年3月1日鹿児島大学 皆既日食中の太陽近傍黄道光の観測 石黒正晃(国立天文台) 共同研究者: 上野宗孝、猿楽祐樹、臼井文彦、 Hong Seung Soo、Pyo Jeonghyun、Yang Hongu Poynting-Robertson効果によるダストの寿命 Mann et al. A&A Rv, 13, 3, 159-228 黄道光 b Pictoris (V=3.85 ) Kalas et al. 2005 Wyatt 2008 Chap 4. THE IPD CLOUD REVEALED TO AKARI 1) AKARI MAPS OF ZE BRIGHTNESS AKARI L18W ZE map after bands being removed ; 0o.5 x 0o.5 resolution The Sky Observed by AKARI S9W-band Leading direction Trailing direction The Sky Observed by AKARI L18W-band Leading direction Trailing direction Resonance Ring around the Sun at 1 AU 3) SEASONAL VARIATION OF POLE BRIGHTNESS Causes: symmetry plane tilt Earth eccentricity off-centering of IPD cloud Zodiacal Component Faint Stars Airglow mission CMB Cirrus 1.E-05 S k y B rig h tn ess (W m 1 ) -2 sr - 1.E-04 1.E-06 1.E-07 1.E-08 1.E-09 1.E-10 0.1 1 10 100 Wavelength (É m) 夜空の明るさ(Leinert et al. 1998) 1000 10000 明け方 真夜中 夕方 黄極(北) 黄道面 黄極(南) Intensity map of zodiacal light by WIZARD F() x constant Scattering phase function of the interplanetary dust Hong (1985). I0 phase angle: scattering angle: F()I0 Venus i=3.4° =77° Mars i=1.9° =50° Jupiter i=1.3° =101° Saturn i=2.5° =114° Giese, Kneissel and Rittich 1986 ST-7 ST-9 CCD format Resolution Field-of-view Readout time 756510 5.8'/pix (0.2R) 3349 (more than?) 11 sec 8.6'/pix (0.3R) 7373 11 sec? (4.6mm6.9mm) 512512 (10.2mm10.2mm) ST-7 + 8mm-fisheye ST-9 + 8mm-fisheye Predicted Morphology of the Zodiacal Light on July 22 b () 3.16106 S10 1.00106 S10 3.16105 S10 1.00105 S10 3.16104 S10 1.00104 S10 3.16103 S10 1.00103 S10 - () Spatial distribution: Kelsall el al. (1998) Scattering phase function: Hong (1985) • • • • Observation site: Predicted time for the total eclipse: Solar ecliptic longitude: Solar elevation: 135E, 28N 11:06:25-11:13:05 JST =11925m30s 75 Available Instruments • CCD – SBIG ST-9 – SBIG ST-7 2 Nishi-Harima observatory Amateurs' privately-owned • Lens – Nikon 8mm fish-eye – Nikon 16mm fish-eye – Nikon 24mm wide-field … • Filter – Johnson/Kron-Cousins (B,V,Rc,Ic), ECAS (b-z)