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Why not us interferometry to take a picture of Pluto?



The 2019 Stack Overflow Developer Survey Results Are InReason for disqualifying Pluto as a Planet?Planets and Pluto? Neptune?How long will it take Pluto to grow to planet size?VLT interferometry vs E-ELT?Can the expansion of spacetime be directly measured with laser interferometry (like GW can)Is Pluto a “proto-planet”?Why was the (small) Hubble better able to find KBO targets for New Horizons than large adaptive optics ground telescopes?Why does Jupiter atmosphere does not get thinner on edgesIs Optical VLBI theoretically feasible? If not why not?Why did the Event Horizon Telescope take so long to take a photo of a black hole?










2












$begingroup$


Interferometry is among the best ways (if not, the best way!) to have an image of a very distant object.



Recently a picture of the black hole at the center of M87 was released. It is the result of several data collected by the Event Horizon Telescope, a series of arrays all across our world, working as one like a giant Earth sized telescope. The picture is not really cutting edge and high definition however it is still very surprising and in a way detailed enough, considering the fact that M87 is 53.49 million light years away... and this is where I arrive to Pluto which is just around 6 to 7 billion kilometers from us.



If we used an interferometer, perhaps the same size as the EHT (or just a smaller one, the size of an entire continent), and point all the arrays at Pluto, then we should have a picture with a resolution that is at least higher as the Hubble Space Telescope, but likely not as high as the pictures from the New Horizons spacecraft which directly made a fly by of Pluto... right?



If so then why don't we use interferometry to take pictures of Pluto from Earth?










share|improve this question









$endgroup$
















    2












    $begingroup$


    Interferometry is among the best ways (if not, the best way!) to have an image of a very distant object.



    Recently a picture of the black hole at the center of M87 was released. It is the result of several data collected by the Event Horizon Telescope, a series of arrays all across our world, working as one like a giant Earth sized telescope. The picture is not really cutting edge and high definition however it is still very surprising and in a way detailed enough, considering the fact that M87 is 53.49 million light years away... and this is where I arrive to Pluto which is just around 6 to 7 billion kilometers from us.



    If we used an interferometer, perhaps the same size as the EHT (or just a smaller one, the size of an entire continent), and point all the arrays at Pluto, then we should have a picture with a resolution that is at least higher as the Hubble Space Telescope, but likely not as high as the pictures from the New Horizons spacecraft which directly made a fly by of Pluto... right?



    If so then why don't we use interferometry to take pictures of Pluto from Earth?










    share|improve this question









    $endgroup$














      2












      2








      2





      $begingroup$


      Interferometry is among the best ways (if not, the best way!) to have an image of a very distant object.



      Recently a picture of the black hole at the center of M87 was released. It is the result of several data collected by the Event Horizon Telescope, a series of arrays all across our world, working as one like a giant Earth sized telescope. The picture is not really cutting edge and high definition however it is still very surprising and in a way detailed enough, considering the fact that M87 is 53.49 million light years away... and this is where I arrive to Pluto which is just around 6 to 7 billion kilometers from us.



      If we used an interferometer, perhaps the same size as the EHT (or just a smaller one, the size of an entire continent), and point all the arrays at Pluto, then we should have a picture with a resolution that is at least higher as the Hubble Space Telescope, but likely not as high as the pictures from the New Horizons spacecraft which directly made a fly by of Pluto... right?



      If so then why don't we use interferometry to take pictures of Pluto from Earth?










      share|improve this question









      $endgroup$




      Interferometry is among the best ways (if not, the best way!) to have an image of a very distant object.



      Recently a picture of the black hole at the center of M87 was released. It is the result of several data collected by the Event Horizon Telescope, a series of arrays all across our world, working as one like a giant Earth sized telescope. The picture is not really cutting edge and high definition however it is still very surprising and in a way detailed enough, considering the fact that M87 is 53.49 million light years away... and this is where I arrive to Pluto which is just around 6 to 7 billion kilometers from us.



      If we used an interferometer, perhaps the same size as the EHT (or just a smaller one, the size of an entire continent), and point all the arrays at Pluto, then we should have a picture with a resolution that is at least higher as the Hubble Space Telescope, but likely not as high as the pictures from the New Horizons spacecraft which directly made a fly by of Pluto... right?



      If so then why don't we use interferometry to take pictures of Pluto from Earth?







      planet telescope interferometry






      share|improve this question













      share|improve this question











      share|improve this question




      share|improve this question










      asked 9 hours ago









      Victorbrine CassiniVictorbrine Cassini

      1262




      1262




















          1 Answer
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          5












          $begingroup$

          Radio interferometry can combine observations over very large baselines. But optical interferometry cannot. According to a list of interferometry instruments on wikipedia, the largest baseline for optical measurements is less than a kilometer. We can't take optical measurements with continent-sized instruments.



          Then if you drop down to radio where the instruments do have that capability, I think you'll find Pluto is quite dim (it's not a radio source, and there's no strong radio emissions that it can reflect to us). There's no radio signal from Pluto that can be imaged.



          From a page on optical interferometry:




          Interferometers are seen by most astronomers as very specialized
          instruments, as they are capable of a very limited range of
          observations. It is often said that an interferometer achieves the
          effect of a telescope the size of the distance between the apertures;
          this is only true in the limited sense of angular resolution. The
          combined effects of limited aperture area and atmospheric turbulence
          generally limit interferometers to observations of comparatively
          bright stars and active galactic nuclei.







          share|improve this answer











          $endgroup$












          • $begingroup$
            Might want to state Pluto is "dim" because it doesn't have many radio emissions (else one might infer you meant light).
            $endgroup$
            – Magic Octopus Urn
            8 hours ago











          Your Answer





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          1 Answer
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          1 Answer
          1






          active

          oldest

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          active

          oldest

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          active

          oldest

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          5












          $begingroup$

          Radio interferometry can combine observations over very large baselines. But optical interferometry cannot. According to a list of interferometry instruments on wikipedia, the largest baseline for optical measurements is less than a kilometer. We can't take optical measurements with continent-sized instruments.



          Then if you drop down to radio where the instruments do have that capability, I think you'll find Pluto is quite dim (it's not a radio source, and there's no strong radio emissions that it can reflect to us). There's no radio signal from Pluto that can be imaged.



          From a page on optical interferometry:




          Interferometers are seen by most astronomers as very specialized
          instruments, as they are capable of a very limited range of
          observations. It is often said that an interferometer achieves the
          effect of a telescope the size of the distance between the apertures;
          this is only true in the limited sense of angular resolution. The
          combined effects of limited aperture area and atmospheric turbulence
          generally limit interferometers to observations of comparatively
          bright stars and active galactic nuclei.







          share|improve this answer











          $endgroup$












          • $begingroup$
            Might want to state Pluto is "dim" because it doesn't have many radio emissions (else one might infer you meant light).
            $endgroup$
            – Magic Octopus Urn
            8 hours ago















          5












          $begingroup$

          Radio interferometry can combine observations over very large baselines. But optical interferometry cannot. According to a list of interferometry instruments on wikipedia, the largest baseline for optical measurements is less than a kilometer. We can't take optical measurements with continent-sized instruments.



          Then if you drop down to radio where the instruments do have that capability, I think you'll find Pluto is quite dim (it's not a radio source, and there's no strong radio emissions that it can reflect to us). There's no radio signal from Pluto that can be imaged.



          From a page on optical interferometry:




          Interferometers are seen by most astronomers as very specialized
          instruments, as they are capable of a very limited range of
          observations. It is often said that an interferometer achieves the
          effect of a telescope the size of the distance between the apertures;
          this is only true in the limited sense of angular resolution. The
          combined effects of limited aperture area and atmospheric turbulence
          generally limit interferometers to observations of comparatively
          bright stars and active galactic nuclei.







          share|improve this answer











          $endgroup$












          • $begingroup$
            Might want to state Pluto is "dim" because it doesn't have many radio emissions (else one might infer you meant light).
            $endgroup$
            – Magic Octopus Urn
            8 hours ago













          5












          5








          5





          $begingroup$

          Radio interferometry can combine observations over very large baselines. But optical interferometry cannot. According to a list of interferometry instruments on wikipedia, the largest baseline for optical measurements is less than a kilometer. We can't take optical measurements with continent-sized instruments.



          Then if you drop down to radio where the instruments do have that capability, I think you'll find Pluto is quite dim (it's not a radio source, and there's no strong radio emissions that it can reflect to us). There's no radio signal from Pluto that can be imaged.



          From a page on optical interferometry:




          Interferometers are seen by most astronomers as very specialized
          instruments, as they are capable of a very limited range of
          observations. It is often said that an interferometer achieves the
          effect of a telescope the size of the distance between the apertures;
          this is only true in the limited sense of angular resolution. The
          combined effects of limited aperture area and atmospheric turbulence
          generally limit interferometers to observations of comparatively
          bright stars and active galactic nuclei.







          share|improve this answer











          $endgroup$



          Radio interferometry can combine observations over very large baselines. But optical interferometry cannot. According to a list of interferometry instruments on wikipedia, the largest baseline for optical measurements is less than a kilometer. We can't take optical measurements with continent-sized instruments.



          Then if you drop down to radio where the instruments do have that capability, I think you'll find Pluto is quite dim (it's not a radio source, and there's no strong radio emissions that it can reflect to us). There's no radio signal from Pluto that can be imaged.



          From a page on optical interferometry:




          Interferometers are seen by most astronomers as very specialized
          instruments, as they are capable of a very limited range of
          observations. It is often said that an interferometer achieves the
          effect of a telescope the size of the distance between the apertures;
          this is only true in the limited sense of angular resolution. The
          combined effects of limited aperture area and atmospheric turbulence
          generally limit interferometers to observations of comparatively
          bright stars and active galactic nuclei.








          share|improve this answer














          share|improve this answer



          share|improve this answer








          edited 6 hours ago

























          answered 8 hours ago









          BowlOfRedBowlOfRed

          77637




          77637











          • $begingroup$
            Might want to state Pluto is "dim" because it doesn't have many radio emissions (else one might infer you meant light).
            $endgroup$
            – Magic Octopus Urn
            8 hours ago
















          • $begingroup$
            Might want to state Pluto is "dim" because it doesn't have many radio emissions (else one might infer you meant light).
            $endgroup$
            – Magic Octopus Urn
            8 hours ago















          $begingroup$
          Might want to state Pluto is "dim" because it doesn't have many radio emissions (else one might infer you meant light).
          $endgroup$
          – Magic Octopus Urn
          8 hours ago




          $begingroup$
          Might want to state Pluto is "dim" because it doesn't have many radio emissions (else one might infer you meant light).
          $endgroup$
          – Magic Octopus Urn
          8 hours ago

















          draft saved

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          Беларусь Змест Назва Гісторыя Геаграфія Сімволіка Дзяржаўны лад Палітычныя партыі Міжнароднае становішча і знешняя палітыка Адміністрацыйны падзел Насельніцтва Эканоміка Культура і грамадства Сацыяльная сфера Узброеныя сілы Заўвагі Літаратура Спасылкі НавігацыяHGЯOiТоп-2011 г. (па версіі ej.by)Топ-2013 г. (па версіі ej.by)Топ-2016 г. (па версіі ej.by)Топ-2017 г. (па версіі ej.by)Нацыянальны статыстычны камітэт Рэспублікі БеларусьШчыльнасць насельніцтва па краінахhttp://naviny.by/rubrics/society/2011/09/16/ic_articles_116_175144/А. Калечыц, У. Ксяндзоў. Спробы засялення краю неандэртальскім чалавекам.І ў Менску былі мамантыА. Калечыц, У. Ксяндзоў. Старажытны каменны век (палеаліт). Першапачатковае засяленне тэрыторыіГ. Штыхаў. Балты і славяне ў VI—VIII стст.М. Клімаў. Полацкае княства ў IX—XI стст.Г. Штыхаў, В. Ляўко. Палітычная гісторыя Полацкай зямліГ. Штыхаў. Дзяржаўны лад у землях-княствахГ. Штыхаў. Дзяржаўны лад у землях-княствахБеларускія землі ў складзе Вялікага Княства ЛітоўскагаЛюблінская унія 1569 г."The Early Stages of Independence"Zapomniane prawdy25 гадоў таму было аб'яўлена, што Язэп Пілсудскі — беларус (фота)Наша вадаДакументы ЧАЭС: Забруджванне тэрыторыі Беларусі « ЧАЭС Зона адчужэнняСведения о политических партиях, зарегистрированных в Республике Беларусь // Министерство юстиции Республики БеларусьСтатыстычны бюлетэнь „Полаўзроставая структура насельніцтва Рэспублікі Беларусь на 1 студзеня 2012 года і сярэднегадовая колькасць насельніцтва за 2011 год“Индекс человеческого развития Беларуси — не было бы нижеБеларусь занимает первое место в СНГ по индексу развития с учетом гендерного факцёраНацыянальны статыстычны камітэт Рэспублікі БеларусьКанстытуцыя РБ. Артыкул 17Трансфармацыйныя задачы БеларусіВыйсце з крызісу — далейшае рэфармаванне Беларускі рубель — сусветны лідар па дэвальвацыяхПра змену коштаў у кастрычніку 2011 г.Бядней за беларусаў у СНД толькі таджыкіСярэдні заробак у верасні дасягнуў 2,26 мільёна рублёўЭканомікаГаласуем за ТОП-100 беларускай прозыСучасныя беларускія мастакіАрхитектура Беларуси BELARUS.BYА. Каханоўскі. Культура Беларусі ўсярэдзіне XVII—XVIII ст.Анталогія беларускай народнай песні, гуказапісы спеваўБеларускія Музычныя IнструментыБеларускі рок, які мы страцілі. Топ-10 гуртоў«Мясцовы час» — нязгаслая легенда беларускай рок-музыкіСЯРГЕЙ БУДКІН. МЫ НЯ ЗНАЕМ СВАЁЙ МУЗЫКІМ. А. Каладзінскі. НАРОДНЫ ТЭАТРМагнацкія культурныя цэнтрыПублічная дыскусія «Беларуская новая пьеса: без беларускай мовы ці беларуская?»Беларускія драматургі па-ранейшаму лепш ставяцца за мяжой, чым на радзіме«Працэс незалежнага кіно пайшоў, і дзяржаву турбуе яго непадкантрольнасць»Беларускія філосафы ў пошуках прасторыВсе идём в библиотекуАрхіваванаАб Нацыянальнай праграме даследавання і выкарыстання касмічнай прасторы ў мірных мэтах на 2008—2012 гадыУ космас — разам.У суседнім з Барысаўскім раёне пабудуюць Камандна-вымяральны пунктСвяты і абрады беларусаў«Мірныя бульбашы з малой краіны» — 5 непраўдзівых стэрэатыпаў пра БеларусьМ. Раманюк. Беларускае народнае адзеннеУ Беларусі скарачаецца колькасць злачынстваўЛукашэнка незадаволены мінскімі ўладамі Крадзяжы складаюць у Мінску каля 70% злачынстваў Узровень злачыннасці ў Мінскай вобласці — адзін з самых высокіх у краіне Генпракуратура аналізуе стан са злачыннасцю ў Беларусі па каэфіцыенце злачыннасці У Беларусі стабілізавалася крымінагеннае становішча, лічыць генпракурорЗамежнікі сталі здзяйсняць у Беларусі больш злачынстваўМУС Беларусі турбуе рост рэцыдыўнай злачыннасціЯ з ЖЭСа. Дазволіце вас абкрасці! Рэйтынг усіх службаў і падраздзяленняў ГУУС Мінгарвыканкама вырасАб КДБ РБГісторыя Аператыўна-аналітычнага цэнтра РБГісторыя ДКФРТаможняagentura.ruБеларусьBelarus.by — Афіцыйны сайт Рэспублікі БеларусьСайт урада БеларусіRadzima.org — Збор архітэктурных помнікаў, гісторыя Беларусі«Глобус Беларуси»Гербы и флаги БеларусиАсаблівасці каменнага веку на БеларусіА. Калечыц, У. Ксяндзоў. Старажытны каменны век (палеаліт). Першапачатковае засяленне тэрыторыіУ. Ксяндзоў. Сярэдні каменны век (мезаліт). Засяленне краю плямёнамі паляўнічых, рыбакоў і збіральнікаўА. Калечыц, М. Чарняўскі. Плямёны на тэрыторыі Беларусі ў новым каменным веку (неаліце)А. Калечыц, У. Ксяндзоў, М. Чарняўскі. Гаспадарчыя заняткі ў каменным векуЭ. Зайкоўскі. Духоўная культура ў каменным векуАсаблівасці бронзавага веку на БеларусіФарміраванне супольнасцей ранняга перыяду бронзавага векуФотографии БеларусиРоля беларускіх зямель ва ўтварэнні і ўмацаванні ВКЛВ. Фадзеева. З гісторыі развіцця беларускай народнай вышыўкіDMOZGran catalanaБольшая российскаяBritannica (анлайн)Швейцарскі гістарычны15325917611952699xDA123282154079143-90000 0001 2171 2080n9112870100577502ge128882171858027501086026362074122714179пппппп