系外惑星大気
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- すずり よどぎみ
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1 transiting planet HDS
2 2
3 3
4 (Mayor & Queloz 1995) 4.2 4
5 (Charbonneau et al. 2000, Henry et al. 2000) HST HST Brown et al. (2001) 5
6 6
7 Radial velocity data Radial velocity data Radial velocity 7
8 Josh Obs (1.2m) November 24, 2003 transit H 8
9 newscenter/archive/ 2001/38/ g/cc
10 Radial velocity + transit HD G0V V 7.58 ( =47pc) 6000 HD209458b g/cc (< )
11 (15%) Additional absorption in Lyman emission line Geocorona, not planetary Vidal-Madjar et al. Nature 422(2003)
12 O I C II 2% H I 5% O I 10% C II 6% (upper) low-resolution HST spectra (lower) high-resolution HST spectra Si III HI Vidal-Madjar et al. (2004) astro-ph/
13 HD209458b ( ) ( ) Josh Winn (Harvard Univ.) Edwin Turner, Brenda Frye (Princeton Univ.) 13
14 HD209458b radial velocity Subaru/HDS previous velocity curve (Wittenmyer et al. 2003) Winn et al. (2004) PASJ, submitted. astro-ph/
15 HDS H Winn et al PASJ, in press (astro-ph/ ) Transit radial velocity (Rossiter-McLaughlin ) McLaughlin (Ohta, Taruya & Suto 2004) (S04B0015N) ( ) 15
16 HD Subaru/HDS spectrum two spectra taken 2.5hrs apart H Winn et al [ ] 16
17 HDS n,j : n j S 1 ( n,j ) S 2 ( n,j ) HDS S 2 S 1 n R( n,j )= S 1 ( n,j )/S 2 ( n,j ) R(n,j) 100 n n-1 n+1 R [S 1 ( n,j ) - S 2b ( n,j )] 2 S 2b ( n,j )=[c n+1 R(n+1,j)+c n-1 R(n-1,j)] S 2 ( n,j ) c n-1 1/2 j c n+1 S 1 c 0 λ S 2m ( n,j ) = c 0 S 2b ( n,j ) + λ ds 2b ( )/dλ 17
18 H H Na I (D2) Na I (D1) H H H H (Winn et al. 2004) H Transit 18 Transit
19 H (Winn et al. 2004)
20 H H <0.1% (Winn et al. 2004) L 15% (Vidal-Madjar et al. 2003) T ex < ( )eV ( ( 20
21 radial velocity 3m/s HD HD I 2 cell Subaru/HDS 21
22 Rossiter-McLaughlin (Rossiter 1924, McLaughlin 1924) 22
23 Spectroscopic transit signature (Rossiter-McLaughlin ) out of transit in transit HD radial velocity data Queloz et al. (2000) A&A 359, L13 ELODIE on 193cm telescope 23
24 Rossiter (Kopal 1990; Hosokawa 1953) (1953 Ohta et al. (2004) 24
25 radial velocity Subaru/HDS error-bar Subaru/HDS error-bar ε=0.64 ε=0 Limb darkening: B= 1- ε (1-cos θ) (Semi)-analytic template curves (Ohta, Taruya & Suto 2004) 25
26 50km/s 0.01% HDS
27 Biomarker (e.g., extrasolar plant) Habitable planet Extraterrestrial life 27
28 Biomarker red edge 28
29 extrasolar planet biomarker (extrasolar plant as a biomarker in extrasolar planets) Seager, Ford & Turner astro-ph/
30 @Lowell spiral nebulae Observatory 40(1917)304 Observations of Mars in 1924 made at the Lowell Observatory: II spectrum observations of Mars PASP 36(1924)261 30
31 Ford, Seager & Turner Nature 412 (2001)
32 red edge 2 Sunlight 32
33 Woolf & Smith ApJ 574(2002)430 The spectrum of earthshine: A Pale Blue Dot Observed from the Ground [ ] 33
34 characterization habitable planets? search for life 34
太陽系外惑星探査
http://hubblesite.org/newscenter/archive/2001/38/ Terra MODIS http://modarch.gsfc.nasa.gov/ http://www.nasa.gov/home/index.html / 2 Are we alone? Origins Where are they? (Fermi 1950) 3 4 0.5 arcsec 10pc
系外惑星大気
http://hubblesite.org/newscenter/archive/2001/38/ 2004 9 30 1781 1846 1930 50 2 3 radial velocity HDS 5m/s HD209458 HD209458+I 2 cell Subaru/HDS 4 (Mayor & Queloz 1995) 4.2 5 2 1.5% HST 4 orbits Brown
Revolution of our world-view We didn t know anything Invincible Photo taken by Y.Suto (Nov.4, 2004) post-nishinomiya-yukawa symposium, Kyoto Universit
Beyond a pale blue dot Yasushi Suto Department of Physics and Research Center for the Early Universe, the University of Tokyo November 12, 2015: The 2015 Kyoto Prize Workshop in Basic Sciences Formation
宇宙理論研究室ガイダンス
60 S.L.Glashow Glashow : Interaction Warner Books 4 4 1978 12 CMB 10-40 -40 CMB / The universe in a nutshell A H He C, O Ne, Mg Si Fe Sphere(0.1 cylinder (0. slab (0. Cylinder hole (0. Spherical hole
理論懇2014
Proposal for a project of high-precision stellar radial velocity work, Struve (1952)! But there seems to be no compelling reason why the hypothetical stellar planets should not, in some instances, be much
太陽系外惑星とバイオマーカー 物理学教室金曜ランチトーク 2010 年 6 月 11 日 須藤靖
太陽系外惑星とバイオマーカー 物理学教室金曜ランチトーク 2010 年 6 月 11 日 須藤靖 http://www-utap.phys.s.u-tokyo.ac.jp/~suto/mypresentation_2010j.html アイザック アシモフ著 夜来る 恐ろしい暗闇が訪れた 我々は宇宙の中心 我々は何も知らなかった イラスト : 羽馬有紗 2000 年に一度しか夜が来ない 地球 の人たち
4 太陽系外惑星の世界 (Credit: Zina Deretsky, アメリカ国立科学財団 )
4 太陽系外惑星の世界 (Credit: Zina Deretsky, アメリカ国立科学財団 ) もうひとつの宇宙の果て : 銀河系のど こかに生命を宿した惑星はあるのか? 宇宙の果てと太陽系外惑星 大望遠鏡は 暗い 天体を観測できる 本当は明るいのだが遠くにあり暗く見える天体 宇宙の果てにある銀河 すぐ近くにあるのだが本当に暗い天体 銀河内にある系外惑星 太陽系外惑星とは? 水金地火木土 ( 天海冥
SFN
THE STAR FORMATION NEWSLETTER No.291-14 March 2017 2017/04/28 16-20 16. X-Shooter spectroscopy of young stellar objects in Lupus. Atmospheric parameters, membership and activity diagnostics 17. The evolution
トランジット惑星系の主星自転 惑星軌道公転角 トランジット惑星系の自転公転射影角の分布 極軌道 Configuration of star-planet system 逆行 順行 理学講義棟 Z 年 1 月 29
トランジット惑星系の主星自転 惑星軌道公転角 トランジット惑星系の自転公転射影角の分布 極軌道 Configuration of star-planet system 逆行 順行 東京大学大学院理学系研究科物理学専攻須藤靖神戸大学地球惑星談話会 @ 理学講義棟 Z101 2015 年 1 月 29 日 16:00-17:00 太陽系外惑星発見の歴史年表 1995 年に我々は何も知ら なかった事を思い知る
★結果★ 藤沢市長杯 掲示用ヒート表
AA 35 Round 1 8 4 Round 2 28 16 SEMI FINAL H1 H5 H1 H1 Red 12802015 1 Red 12802109 1 1-1 Red 12802015 2 1-1 Red 12702346 White 12800232 2 White 12702406 3 3-1 White 12702346 1 3-1 White 12802109 Yellow
1 (1) (2)
1 2 (1) (2) (3) 3-78 - 1 (1) (2) - 79 - i) ii) iii) (3) (4) (5) (6) - 80 - (7) (8) (9) (10) 2 (1) (2) (3) (4) i) - 81 - ii) (a) (b) 3 (1) (2) - 82 - - 83 - - 84 - - 85 - - 86 - (1) (2) (3) (4) (5) (6)
- 2 -
- 2 - - 3 - (1) (2) (3) (1) - 4 - ~ - 5 - (2) - 6 - (1) (1) - 7 - - 8 - (i) (ii) (iii) (ii) (iii) (ii) 10 - 9 - (3) - 10 - (3) - 11 - - 12 - (1) - 13 - - 14 - (2) - 15 - - 16 - (3) - 17 - - 18 - (4) -
2 1980 8 4 4 4 4 4 3 4 2 4 4 2 4 6 0 0 6 4 2 4 1 2 2 1 4 4 4 2 3 3 3 4 3 4 4 4 4 2 5 5 2 4 4 4 0 3 3 0 9 10 10 9 1 1
1 1979 6 24 3 4 4 4 4 3 4 4 2 3 4 4 6 0 0 6 2 4 4 4 3 0 0 3 3 3 4 3 2 4 3? 4 3 4 3 4 4 4 4 3 3 4 4 4 4 2 1 1 2 15 4 4 15 0 1 2 1980 8 4 4 4 4 4 3 4 2 4 4 2 4 6 0 0 6 4 2 4 1 2 2 1 4 4 4 2 3 3 3 4 3 4 4
20 15 14.6 15.3 14.9 15.7 16.0 15.7 13.4 14.5 13.7 14.2 10 10 13 16 19 22 1 70,000 60,000 50,000 40,000 30,000 20,000 10,000 0 2,500 59,862 56,384 2,000 42,662 44,211 40,639 37,323 1,500 33,408 34,472
I? 3 1 3 1.1?................................. 3 1.2?............................... 3 1.3!................................... 3 2 4 2.1........................................ 4 2.2.......................................
ISLE 2010/08/17
ISLE 2010/08/17 Talk plan 1. ISLE 2. 3. 4. 2011A 2010/8/17 OAOUM 2010 ISLE 2010/8/17 OAOUM 2010 ISLE OASIS HAWAII (HgCdTe 1024 1024) 4.2 4.2 arcmin 2, 0.25 arcsec/pix (13 Filters) 2006B FWHM = 0.75 arcsec
atomic line spectrum emission line absorption line atom proton neutron nuclei electron Z atomic number A mass number neutral atom ion energy
1 22 22.1 atomic line spectrum emission line absorption line atom proton neutronnuclei electron Z atomic number A mass number neutral atom ion energy level ground stateexcited state ionized state 22.2
太陽系外惑星の光と影
太陽系外惑星の光と影 : 今日までそして明日から 東京大学大学院理学系研究科須藤靖 2007 年 11 月 24 日 @ 東京国際交流館 青空しか知らないと我々だけが 唯一の存在のように思ってしまう ( すばる観測所 田中壱氏撮影 ) 夜来たる 6 つの太陽をもつ惑星ラガッシュに二千年に一度の夜が訪れる 我々は何も知らなかった 満天の星空を見上げれば 我々以外の世界がないほうが不自然 ( すばる観測所
koji07-02.dvi
007 I II III 1,, 3, 4, 5, 6, 7 5 4 1 ε-n 1 ε-n ε-n ε-n. {a } =1 a ε N N a a N= a a
「諸雑公文書」整理の中間報告
30 10 3 from to 10 from to ( ) ( ) 20 20 20 20 20 35 8 39 11 41 10 41 9 41 7 43 13 41 11 42 7 42 11 41 7 42 10 4 4 8 4 30 10 ( ) ( ) 17 23 5 11 5 8 8 11 11 13 14 15 16 17 121 767 1,225 2.9 18.7 29.8 3.9
J_Lec_Re_total96
1 2 3 13 22 23 31 Blue Planet Prize 1996 1 Blue Planet Prize 1996 2 Blue Planet Prize 1996 3 Blue Planet Prize 1996 4 Blue Planet Prize 1996 5 Blue Planet Prize 1996 6 Blue Planet Prize 1996 7 Blue Planet
MW鹿児島
NGC1068 Dark Matter Halo baryon gas stars SMBH SMBH 1 SMBHs? (AGN) AGN Seyfertization Taniguchi 1987, ApJ, 317, L57 AGN The dead quasar problem (Rees 1990, Science, 247, 817) T AGN ~ 10 8 yrs AGN AGN
第32回新春波乗り大会2018
AA 32 Round 1 4 SEMI FINAL 2 20 8 FINAL H1 H1 H1 Red 12701793 1 1-1 Red 12701793 2 1-1 Red 11800623 White 12900058 4 3-1 White 12402115 4 2-1 White 12402209 Yellow 11603976 3 2-2 Yellow 12301534 3 1-2
1-1 - 2 3-2 - - 3 - i - 4 - ii - 5 - c - 6 - 4 1-7 - 2 1-8 - 2-9 - - 10 - - 11 - - 12 - - 13 - - 14 - - 15 - - 16 - - 17 - 3-18 - - 19 - - 20 - - 21 - - 22 - - 23 - iii i - 24 - - 25 - - 26 - 4-27 - 5
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kawaguchi2.pdf
Dusty Clumpy Torus (AGN) (BH) BH 3 BH 1 AGN () 1/3 (i) (ii) Kawaguchi(2003) 1/5 (iii) AGN : T. Kawaguchi & M. Mori, ApJL, 2010, 724, 183 187 T. Kawaguchi & M. Mori, ApJ, 2011, 737, 105 120 Toshihiro KAWAGUCHI
2 X-ray 6 gamma-ray 7 1 17.1 0:38m 0:77m nm 17.2 Hz Hz 1 E p E E = h = ch= (17.2) p = E=c = h=c = h= (17.3) continuum continuous spectrum line spectru
1 17 object 1 observation 17.1 X electromagnetic wave photon 1 = c (17.1) c =3 10 8 ms ;1 m mm = 10 ;3 m m =10 ;6 m nm = 10 ;9 m 1 Hz 17.1 spectrum radio 2 infrared 3 visual light optical light 4 ultraviolet
cm H.11.3 P.13 2 3-106-
H11.3 H.11.3 P.4-105- cm H.11.3 P.13 2 3-106- 2 H.11.3 P.47 H.11.3 P.27 i vl1 vl2-107- 3 h vl l1 l2 1 2 0 ii H.11.3 P.49 2 iii i 2 vl1 vl2-108- H.11.3 P.50 ii 2 H.11.3 P.52 cm -109- H.11.3 P.44 S S H.11.3
ρ ( ) sgv + ρwgv γ sv + γ wv γ s + γ w e e γ ρ g s s γ s ( ) + γ w( ) Vs + V Vs + V + e + e + e γ γ sa γ e e n( ) + e γ γ s ( n) + γ wn γ s, γ w γ γ +
σ P σ () n σ () n σ P ) σ ( σ P σ σ σ + u V e m w ρ w gv V V s m s ρ s gv s ρ ( ) sgv + ρwgv γ sv + γ wv γ s + γ w e e γ ρ g s s γ s ( ) + γ w( ) Vs + V Vs + V + e + e + e γ γ sa γ e e n( ) + e γ γ s (
森羅万象2018のコピー
PD Stellar Irradiation Mineral Atmosphere Na, K, SiO, O 2, O gas (MgO, Al, AlO, FeO etc ) https://www.nasa.gov/topics/universe/features/rocky_planet.html / (2018.5.9) Magma Ocean Ito et al. (2015) (HRE)
6 2 T γ T B (6.4) (6.1) [( d nm + 3 ] 2 nt B )a 3 + nt B da 3 = 0 (6.9) na 3 = T B V 3/2 = T B V γ 1 = const. or T B a 2 = const. (6.10) H 2 = 8π kc2
![6 2 T γ T B (6.4) (6.1) [( d nm + 3 ] 2 nt B )a 3 + nt B da 3 = 0 (6.9) na 3 = T B V 3/2 = T B V γ 1 = const. or T B a 2 = const. (6.10) H 2 = 8π kc2](/thumbs/92/109118076.jpg "6 2 T γ T B (6.4) (6.1) [( d nm + 3 ] 2 nt B )a 3 + nt B da 3 = 0 (6.9) na 3 = T B V 3/2 = T B V γ 1 = const. or T B a 2 = const. (6.10) H 2 = 8π kc2")
1 6 6.1 (??) (P = ρ rad /3) ρ rad T 4 d(ρv ) + PdV = 0 (6.1) dρ rad ρ rad + 4 da a = 0 (6.2) dt T + da a = 0 T 1 a (6.3) ( ) n ρ m = n (m + 12 ) m v2 = n (m + 32 ) T, P = nt (6.4) (6.1) d [(nm + 32 ] )a
B
B07557 0 0 (AGN) AGN AGN X X AGN AGN Geant4 AGN X X X (AGN) AGN AGN X AGN. AGN AGN Seyfert Seyfert Seyfert AGN 94 Carl Seyfert Seyfert Seyfert z < 0. Seyfert I II I 000 km/s 00 km/s II AGN (BLR) (NLR)
Akira MIZUTA(KEK) AM, Nagataki, Aoi (ApJ, , 2011) AM + (in prep)
Akira MIZUTA(KEK) AM, Nagataki, Aoi (ApJ, 732 26, 2011) AM + (in prep) 2011.12.28 GRB GRB. ex. GRB980425/SN1998bw, GRB030329/SN2003dh XRF060218/SN2006aj. GRB091127/SN2009nz XRF100316D/SN2010bh Spectrum
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August 26, 2005 1 1 1.1...................................... 1 1.2......................... 4 1.3....................... 5 1.4.............. 7 1.5.................... 8 1.6 GIM..........................
( ) Note Ω m = 1 Ω m : ( ) r-process α 1: 2 32T h(t 1/2 = y) 2 38U(t 1/2 = y) 2 35U(t 1/2 = 7.038
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掲示用ヒート表 第34回 藤沢市長杯 2017
34 8 4 2 Round 1 Round 2 SEMI FINAL 30 16 8 H1 H5 H1 H1 Red 12401821 2 Red 12601360 2 1-1 Red 12501915 1 1-1 Red 12501915 4 White 12900051 4 White 12600138 3 3-1 White 12802412 2 3-1 White 12801091 1 Yellow
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E-mail: khatano@fms.saitama-u.ac.jp Tel & Fax: 048-858-3535 Toxin Virus Bacterium Glycolipid Glycoprotein Vero toxin (Stx1 and Stx2) Side view Bottom view H H H H N H Grobotriaosyl Ceramide (Gb 3 : Galα1-4Galβ1-4Glcβ-Cer)
BH BH BH BH Typeset by FoilTEX 2
GR BH BH 2015.10.10 BH at 2015.09.07 NICT 2015.05.26 Typeset by FoilTEX 1 BH BH BH BH Typeset by FoilTEX 2 1. BH 1.1 1 Typeset by FoilTEX 3 1.2 2 A B A B t = 0 A: m a [kg] B: m b [kg] t = t f star free
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48 B 17 4 Annuals of Disas. Prev. Res. Inst., Kyoto Univ., No. 48 B, 2005 (CO 2 ) (2003) Sim-CYCLE(Ito and Oikawa, 2000) CO 2 CO 2 Figure 1 CO 2 0 (Denning et al., 1995) CO 2 (2004) Sim-CYCLE CO 2 CO 2
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1 211022 2 11150 211022384 3 1000 23% 77% 10% 10% 5% 20% 15% 40% 5% 3% 8% 16% 15% 42% 5% 6% 4 =1000 = 66 5 =1000 = 59 6 52%(42% 1000 7 56% 41% 40% 97% 3% 11%, 2% 3%, 41 7% 49% 30%, 18%, 40%, 83% =1000
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π, R { 2, 0, 3} , ( R),. R, [ 1, 1] = {x R 1 x 1} 1 0 1, [ 1, 1],, 1 0 1,, ( 1, 1) = {x R 1 < x < 1} [ 1, 1] 1 1, ( 1, 1), 1, 1, R A 1
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青空のムコウに別の世界はあるのか
太陽系外惑星 : 影から光へ 東京大学大学院理学系研究科物理学専攻須藤靖すばる望遠鏡 10 周年記念シンポジウム 2009 年 10 月 5 日 @ 一橋記念講堂 青空のムコウに別の世界はあるのか アイザック アシモフ著 夜来る 恐ろしい暗闇が訪れた 我々は宇宙の中心 我々は何も知らなかった イラスト : 羽馬有紗 2000 年に一度しか夜が来ない 地球 の人たち 自分たちの 地球 と宇宙との関係は?
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/ Total 8G48s1 2G48s8G x 6s 5. HK$1=12 1000 % HK$4,00048,000 175 7.5% HK$4,000-5,99948,000-71,000 129.4 5.6% HK$6,000-7,99972,00095,000 161.7 7.0% HK$8,000-9,99996,000-119,000 165.1 7.1% HK$10,000-14,999120,000-179,000
New version (2.15.1) of Specview is now available Dismiss Windows Specview.bat set spv= Specview set jhome= JAVA (C:\Program Files\Java\jre<version>\
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Specview VO 2012 2012/3/26 Specview Specview STSCI(Space Telescope SCience Institute) VO Specview Web page http://www.stsci.edu/resources/software hardware/specview http://specview.stsci.edu/javahelp/main.html
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dark matter density profiles
LSS & CDM 2 LSS & CDM 3 SPH simulation: movie SPH simulation in CDM : dark matter hot gas galaxy (Yoshikawa, Taruya, Jing & Suto 2001) LSS & CDM 4 Confronting elements of the CDM paradigm Global cosmological
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mr0511_01fix.indd
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プラネット広報誌 『 ＰＬＡＮＥＴvanvan 』 67号(2005年7月発行)
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スライド 1
TMT/ 可視高分散分光器等による 系外地球型惑星の大気吸収探索 国立天文台 太陽系外惑星探査プロジェクト室 成田憲保 背景 目次 系外惑星の大気吸収探索の方法論 ホットジュピターに対する先行研究 トランジットサーベイの現状 TMT で可能になるサイエンス ターゲットとなる吸収線と達成可能な精度 検討結果と好ましい観測ターゲットについて 補足 (cf. CoRoT-7b の場合 ) (cf. 月食を用いた地球大気吸収の模擬観測
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村上春樹 アフターダーク
もうひとつの地球の色は何色? 東京大学大学院理学系研究科物理学専攻須藤靖日本学術会議東北地区会議公開学術講演会サイエンストーク 宇宙ファミリー 2013 9 14 14:25-15:10@ 村上春樹 アフターダーク ハワイに流れ着いた 3 人の兄弟 n 果物がたわわに実り 真ん中には高い山がそびえるハワイのある美しい島に流れ着いた 3 人の兄弟 夢にでた神様が とてつもなく重く大きな岩が 3 つあるはず
Netcommunity SYSTEM X7000 IPコードレス電話機 取扱説明書
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K 2 X = 4 MWG(f), X P 2 F, υ 0 : X P 2 2,, {f λ : X λ P 1 } λ Λ NS(X λ ), (υ 0 ) λ : X λ P 2 ( 1) X 6, f λ K X + F, f ( 1), n, n 1 (cf [10]) X, f : X
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