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Taken from the JPL publication "Precursor Science for the Terrestrial Planet Finder" edited by P.R. Lawson, S.C. Unwin, and C.A. Beichman (JPL Pub 04-014, page 21, fig. 5, 5th Oct 2004)
Original Caption
Limiting sensitivity of techniques of planet finding. Shown in the above figure are the sensitivity limits of radial velocity surveys, astrometric surveys, microlensing surveys, and space-based transit techniques. The lines show 5-σ limits with 50 re-samples. The shaded areas show the expected progress towards the detection of Earth-like planets by 2006 and 2010. Planets in our Solar System are also indicated, as well as the highlighted target area of TPF science. The filled circles indicate the planets found by radial velocity surveys (blue), transit surveys (red), and microlensing surveys (yellow). The discovered extrasolar planets shown in this plot represent the reported findings up until 31 August 2004.
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ไฟล, extrasolar, planets, 2004, ไฟล, ประว, ไฟล, หน, าท, ภาพน, การใช, ไฟล, ามโครงการขนาดของต, วอย, างน, กเซล, ความละเอ, ยดอ, กเซล, กเซล, กเซล, กเซล, กเซล, ภาพท, ความละเอ, ยดส, งกว, 8206, กเซล, ขนาดไฟล, เมกะไบต, ชน, ดไมม, image, ปภาพหร, อไฟล, เส, ยงน, นฉบ, บอย, . ifl prawtiifl hnathimiphaphni karichiflkhamokhrngkarkhnadkhxngtwxyangni 383 599 phikesl khwamlaexiydxun 153 240 phikesl 307 480 phikesl 491 768 phikesl 655 1 024 phikesl 1 382 2 161 phikesl duphaphthimikhwamlaexiydsungkwa 8206 1 382 2 161 phikesl khnadifl 1 12 emkaibt chnidimm image png rupphaphhruxiflesiyngni tnchbbxyuthi khxmmxns raylaexiyddanlang epnkhxkhwamthiaesdngphlcak ifltnchbbinkhxmmxns khxmmxnsepnewbistinokhrngkarsahrbekbrwbrwmsuxesri thi khunsamarthchwyid phaphnimiphaphinrupaebbewketxr SVG hakphaph SVG thaihkaraesdngphldikwa hnathiichphaphnikhwrepliynipichphaph SVG aethn File Extrasolar Planets 2004 08 31 png File Extrasolar Planets 2004 08 31 svg sahrbkhxmulephimetimekiywkbphaphewketxr duthi karepliynipichphaph SVG inkhxmmxnsnxkcaknisamarthduephimetimekiywkb khxmulekiywkbkarrxngrbphaph SVG sahrbsxftaewrmiediywiki id inphasaxun Alemannisch nbsp Bahasa Indonesia nbsp Bahasa Melayu nbsp British English nbsp catala nbsp cestina nbsp dansk nbsp Deutsch nbsp eesti nbsp English nbsp espanol nbsp Esperanto nbsp euskara nbsp francais nbsp Frysk nbsp galego nbsp hrvatski nbsp Ido nbsp italiano nbsp lietuviu nbsp magyar nbsp Nederlands nbsp norsk bokmal nbsp norsk nynorsk nbsp occitan nbsp Plattduutsch nbsp polski nbsp portugues nbsp portugues do Brasil nbsp romană nbsp Scots nbsp sicilianu nbsp slovencina nbsp slovenscina nbsp suomi nbsp svenska nbsp Tiếng Việt nbsp Turkce nbsp veneto nbsp Ellhnika nbsp belaruskaya tarashkevica nbsp blgarski nbsp makedonski nbsp nohchijn nbsp russkij nbsp srpski srpski nbsp tatarcha tatarca nbsp ukrayinska nbsp ქართული nbsp հայերեն nbsp ব ল nbsp தம ழ nbsp മലയ ള nbsp ithy nbsp 한국어 nbsp 日本語 nbsp 简体中文 nbsp 繁體中文 nbsp עברית nbsp العربية nbsp فارسی nbsp nbsp Taken from the JPL publication Precursor Science for the Terrestrial Planet Finder edited by P R Lawson S C Unwin and C A Beichman JPL Pub 04 014 page 21 fig 5 5th Oct 2004 Original Caption Limiting sensitivity of techniques of planet finding Shown in the above figure are the sensitivity limits of radial velocity surveys astrometric surveys microlensing surveys and space based transit techniques The lines show 5 s limits with 50 re samples The shaded areas show the expected progress towards the detection of Earth like planets by 2006 and 2010 Planets in our Solar System are also indicated as well as the highlighted target area of TPF science The filled circles indicate the planets found by radial velocity surveys blue transit surveys red and microlensing surveys yellow The discovered extrasolar planets shown in this plot represent the reported findings up until 31 August 2004 NASA JPL Caltech sungepnphuthuxlikhsiththikhxngiflni xnuyatihnaiflniipichidinthukwtthuprasngkh rwmipthungkarthasa karnaiflniipichinkarsrangiflihm karichephuxkarkha aelakarichxun odymienguxnikhwa txngrabuchuxphuthuxlikhsiththikhxngiflnixyangehmaasmemuxnaiflniipich karaesdngthima Courtesy NASA JPL Caltech Attribution According to JPL s image use policy additional restriction is that no endorsement of any product or service by Caltech JPL or NASA is claimed or implied Caltech s disclaimer Caltech makes no representations or warranties with respect to ownership of copyrights in the images and does not represent others who may claim to be authors or owners of copyright of any of the images and makes no warranties as to the quality of the images Caltech shall not be responsible for any loss or expenses resulting from the use of the images and you release and hold Caltech harmless from all liability arising from such use Usage on the English Wikipedia On the English Wikipedia you can use the JPL Image template to display the copyright notice See w Wikipedia Using JPL images for details khabrryayodyyxithyephimkhabrryaythrrthdediywephuxkhyaykhwamwaiflnimixairixethmthiaesdngxyuiniflniprakxbdwysthanalikhsiththimilikhsiththisyyaxnuyatattribution only license nbsp xngkvs prawtiifl khlikwnthi ewlaephuxduiflthipraktinkhnann wnthi ewlarupyxkhnadphuichkhwamehn pccubn03 11 26 kumphaphnth 25491 382 2 161 1 12 emkaibt Fabio BettaniHot Jupiters along left edge including red dots discovered up to and including 31 August 2004 hnathimiphaphni hnatxipni oyngmathiphaphni dawphvhsbdirxn karichiflkhamokhrngkar wikixuntxipniichiflni karichbn ca wikipedia org Planeta extrasolar karichbn da wikipedia org Exoplanet karichbn de wikipedia org Hot Jupiter karichbn en wikipedia org User Nickshanks Gallery Portal Astronomy Featured August 2007 User Arnaud ramey GlamFiltered karichbn es wikipedia org Jupiter caliente karichbn hu wikipedia org Exobolygo Az exobolygok keresesenek modszerei Kivalasztasi effektus karichbn it wikipedia org Pianeta extrasolare Metodi di individuazione di pianeti extrasolari karichbn ko wikipedia org 외계 행성 뜨거운 목성 karichbn lb wikipedia org Hot Jupiter karichbn pl wikipedia org Metody poszukiwania planet pozaslonecznych karichbn vi wikipedia org Hanh tinh ngoai Hệ Mặt Trời karichbn zh wikipedia org 太陽系外行星 熱木星 ekhathungcak https th wikipedia org wiki ifl Extrasolar Planets 2004 08 31 png, wikipedia, วิกิ หนังสือ, หนังสือ, ห้องสมุด,