{"id":11852,"date":"2020-11-02T09:00:00","date_gmt":"2020-11-02T11:00:00","guid":{"rendered":"https:\/\/mindthegraph.com\/blog\/?p=11852"},"modified":"2023-05-22T11:05:20","modified_gmt":"2023-05-22T14:05:20","slug":"nobel-prize-the-first-black-hole-picture","status":"publish","type":"post","link":"https:\/\/mindthegraph.com\/blog\/lv\/nobel-prize-the-first-black-hole-picture\/","title":{"rendered":"Nobela pr\u0113mija un pirmais meln\u0101 cauruma att\u0113ls"},"content":{"rendered":"

J\u016bs, iesp\u0113jams, dzird\u0113j\u0101t zi\u0146as par zin\u0101tnieka public\u0113to pirmo meln\u0101 cauruma att\u0113lu. \u0160is att\u0113ls bija p\u0101rsteidzo\u0161a zi\u0146a ne tikai astronomijas nozarei, bet ar\u012b visai pasaulei. \u0160is att\u0113ls bija pirmais solis ce\u013c\u0101 uz jaun\u0101m inform\u0101cijas durv\u012bm. Visums ar katru jaunu inform\u0101ciju k\u013c\u016bst arvien apgaismot\u0101ks, un pateicoties tam m\u0113s sp\u0113jam lab\u0101k izprast visus nosl\u0113pumus \u0101rpus m\u016bsu plan\u0113tas.<\/p>\n

Nesen m\u0113s redz\u0113j\u0101m, k\u0101 divpadsmit laure\u0101tiem tika pie\u0161\u0137irta 2020. gada Nobela pr\u0113mija un k\u0101 viens no vi\u0146iem ar saviem p\u0113t\u012bjumiem un atkl\u0101jumiem sniedza iev\u0113rojamu ieguld\u012bjumu cilv\u0113ces lab\u0101. Vi\u0146i visi ir apbr\u012bnojami p\u0113tnieki, un m\u0113s labpr\u0101t \u0161eit past\u0101st\u012btu par katru no vi\u0146iem, bet \u0161odien, lai lab\u0101k izskaidrotu un izprastu pirm\u0101 meln\u0101 cauruma att\u0113la kontekstu, m\u0113s run\u0101sim par Nobela pr\u0113mijas fizik\u0101 laure\u0101tu Rod\u017eera Penroza, Reinharda Genzela un Andrea G\u0113za darbu.<\/p>\n

K\u0101 teikts Nobela pr\u0113mijas ofici\u0101laj\u0101 t\u012bmek\u013ca vietn\u0113, laure\u0101ti tika apbalvoti \"par atkl\u0101jumu, ka melno caurumu veido\u0161an\u0101s ir visp\u0101r\u0113j\u0101s relativit\u0101tes teorijas dro\u0161s paredz\u0113jums\" un \"par supermas\u012bva kompakta objekta atkl\u0101\u0161anu m\u016bsu galaktikas centr\u0101\". Penrouzs ar iespaid\u012bg\u0101m matem\u0101tisk\u0101m metod\u0113m pier\u0101d\u012bja, ka melnie caurumi ir saist\u012bti ar Ein\u0161teina relativit\u0101tes teoriju, savuk\u0101rt Reinharda Genzela un Andrea G\u0113za darbs neapstr\u012bdami pier\u0101d\u012bja, ka m\u016bsu Piena Ce\u013ca galaktikas centr\u0101 patie\u0161\u0101m atrodas melnais caurums, kas \u0161odien paz\u012bstams ar nosaukumu Sagittarius A*.<\/p>\n

\"Nobela<\/a><\/p>\n

Lai piln\u012bb\u0101 izprastu \u0161o t\u0113mu, mums ir j\u0101zina da\u017ei pamatj\u0113dzieni par melnajiem caurumiem, piem\u0113ram, \"Kas ir melnais caurums?\"; \"No k\u0101 tie sast\u0101v?\"; \"No k\u0101 tie sast\u0101v? Kur m\u0113s t\u0101du varam atrast?\"<\/p>\n

Pirmais, kas mums j\u0101zina, ir j\u0113dziens, kas tiek bie\u017ei izmantots daudz\u0101s astronomijas t\u0113m\u0101s, proti, j\u0113dziens par to, kas ir telpiskais laiks. Laiks-att\u0101lums ir \u010detru dimensiju daudzst\u016bris, tr\u012bs telpas dimensijas un viena laika dimensija; koordin\u0101tu sist\u0113m\u0101 m\u0113s redzam (x,y,z,t). Interesants fakts ir tas, ka vienu punktu \u0161aj\u0101 koordin\u0101tu sist\u0113m\u0101 sauc par notikumu. \u0145emot to v\u0113r\u0101, m\u0113s varam ieg\u016bt meln\u0101 cauruma defin\u012bciju.<\/p>\n

Melnais caurums ir telpisk\u0101 laika apgabals<\/strong> kur gravit\u0101cija ir tik \u013coti, bet tik \u013coti sp\u0113c\u012bga, ka no t\u0101s nevar izlauzties neviena g\u0101ze, putek\u013ci, da\u013ci\u0146a vai pat gaisma! T\u0101s visas tiek sp\u0113c\u012bgi pievilktas ar gravit\u0101cijas sp\u0113ku melnaj\u0101 caurum\u0101 un paz\u016bd, dodoties uz vietu, kas zin\u0101tniekiem v\u0113l \u0161odien ir nezin\u0101ma. Interesant\u0101kais ir tas, ka, ja pat gaisma nesp\u0113j atbr\u012bvoties no \u0161\u012b sp\u0113ka, nav iesp\u0113jams redz\u0113t melno caurumu vai pat zin\u0101t, kur t\u0101ds ir. Tas ir t\u0101pat k\u0101 m\u0113\u0123in\u0101t ieraudz\u012bt melnu objektu meln\u0101 fon\u0101, j\u016bs to nevarat saskat\u012bt, vai ar\u012b, ja j\u016bs to sp\u0113jat, tas ir \u013coti gr\u016bti. T\u0101tad, k\u0101 zin\u0101tnieki to dara?<\/p>\n

\"\"<\/a><\/p>\n

Teor\u0113tiski melnie caurumi parasti veidojas, kad sabr\u016bk \u013coti mas\u012bva zvaigzne, kas ir daudz smag\u0101ka par Sauli, t\u0101s dz\u012bves beig\u0101s. Masa ir \u013coti svar\u012bgs faktors, lai izlemtu, vai mirus\u012b zvaigzne p\u0101rv\u0113rt\u012bsies par melno caurumu vai neitronu zvaigzni. Saska\u0146\u0101 ar visp\u0101r\u0113jo relativit\u0101tes teoriju \u0161\u012b supermas\u012bv\u0101 zvaigzne gravit\u0101cijas d\u0113\u013c tiek saspiesta \u013coti maz\u0101 telp\u0101, un, lai veidotu melno caurumu, \u0161\u012b kompakt\u0101 masa var deform\u0113t telpisko laiku.<\/p>\n

\u0160\u012b telpisko laiku deform\u0101cija rada gravit\u0101cijas pa\u0101trin\u0101juma sp\u0113ku, kas v\u0113rsts uz bl\u012bv\u0101s masas \u0137erme\u0146a centru. \u0160\u012b sp\u0113ka d\u0113\u013c g\u0101ze un da\u013ci\u0146as, kas atrodas tuvu melnajam caurumam vai t\u0101 tuvum\u0101, s\u0101k palielin\u0101t rot\u0101cijas \u0101trumu un tiek piespiedu k\u0101rt\u0101 ievilktas melnaj\u0101 caurum\u0101. \u0160o par\u0101d\u012bbu sauc par Akr\u0113cijas disks<\/strong>.<\/p>\n

\u0160is gravit\u0101cijas un berzes sp\u0113ks liek vis\u0101m g\u0101z\u0113m un da\u013ci\u0146\u0101m ar elektrisko l\u0101di\u0146u rad\u012bt ne tikai temperat\u016bras paaugstin\u0101\u0161anos, bet ar\u012b da\u017e\u0101du frekven\u010du elektromagn\u0113tisko starojumu, piem\u0113ram, infrasarkano vai rentgena starojumu. Pateicoties \u0161ai p\u0101rsteidzo\u0161ajai \u012bpa\u0161\u012bbai, melno caurumu var \"redz\u0113t\". Tas ir labi, bet neatvieglo zin\u0101tnieka darbu simtprocent\u012bgi, jums ir frekvence, ko varat izsekot, bet j\u016bs joproj\u0101m nevarat teikt \"o, skatieties, tur, debes\u012bs, ir melnais caurums\". Meln\u0101 cauruma gaismu m\u0113s nevaram piel\u012bdzin\u0101t parastas zvaigznes gaismai; t\u0101s \u013coti at\u0161\u0137iras viena no otras. Ta\u010du lab\u0101 zi\u0146a ir t\u0101, ka melnais objekts no s\u0101kuma tagad ir nedaudz izgaismots melnaj\u0101 fon\u0101.<\/p>\n

Pirmaj\u0101 meln\u0101 cauruma att\u0113l\u0101 redzams akr\u0113cijas disks. Melnais caurums \u0161aj\u0101 gad\u012bjum\u0101 ir 6,5 miljonus rei\u017eu smag\u0101ks par m\u016bsu Sauli un atrodas Messier 87 galaktik\u0101, 53 miljonus gaismas gadu no Zemes. Att\u0113lu bija iesp\u0113jams ieg\u016bt, izmantojot asto\u0146u da\u017e\u0101du teleskopu vis\u0101 pasaul\u0113, notikumu apv\u0101r\u0161\u0146a teleskopa un da\u017eu citu kosmosa teleskopu misiju laika darbu, kop\u0101 tie 2017. gada apr\u012bl\u012b vienlaic\u012bgi uz\u0146\u0113ma datus no M87. Katrs no tiem uz\u0146\u0113ma at\u0161\u0137ir\u012bgus datus no meln\u0101 cauruma, p\u0113c tam viss tika salikts kop\u0101, veidojot att\u0113lu. Tas var izklaus\u012bties k\u0101 vienk\u0101r\u0161a un viena so\u013ca lieta, ta\u010du zin\u0101tniekam bija smagi j\u0101str\u0101d\u0101, lai piln\u012bb\u0101 izprastu visus datus un to, k\u0101 ar tiem r\u012bkoties, k\u0101du algoritmu izmantot un k\u0101 to izmantot.<\/p>\n

1997. gad\u0101 public\u0113taj\u0101 rakst\u0101 Genzels par\u0101d\u012bja, ka piecu da\u017e\u0101du gadu (no 1992. l\u012bdz 1996. gadam) v\u0101k\u0161anas dati fiks\u0113 \u0101tri kust\u012bgas zvaigznes tie\u0161\u0101 Sgr A* tuvum\u0101 un ka \u0161o zvaig\u017e\u0146u vid\u016b atrodas \u013coti liela un smaga tum\u0161\u0101 masa. \"Pie \u0161\u0101da bl\u012bvuma nav stabilas norm\u0101lu zvaig\u017e\u0146u, zvaig\u017e\u0146u atlieku vai zemzvaig\u017e\u0146u vien\u012bbu konfigur\u0101cijas,\" teikts rakst\u0101 (GENZEL et al., 1997). Secinot, \"Piena Ce\u013ca kodol\u0101 j\u0101b\u016bt mas\u012bvam melnajam caurumam\".<\/p>\n

Cit\u0101 1998. gad\u0101 public\u0113taj\u0101 \u017d\u0113za (Ghez) rakst\u0101 divu gadu p\u0113t\u012bjum\u0101 tika atkl\u0101ts t\u0101ds pats kust\u012bgu s\u0101kumu modelis taj\u0101 pa\u0161\u0101 viet\u0101, k\u0101 teikts rakst\u0101: \"gan zvaig\u017e\u0146u virsmas bl\u012bvuma, gan \u0101truma dispersijas maksimumi atbilst meln\u0101 cauruma kandid\u0101ta (tolaik v\u0113l kandid\u0101ta) Sgr A* st\u0101voklim\" (GHEZ et al., 1998). P\u0113t\u012bjum\u0101 izmantotie att\u0113li tika ieg\u016bti, izmantojot tuv\u0101 infrasarkan\u0101 starojuma vi\u013c\u0146u garumu, proti, t\u0101du frekvenci, k\u0101du izstaro akr\u0113cijas disks.<\/p>\n

\u0160eit ir \u012bss saraksts ar \u0161iem rakstiem:<\/p>\n

GENZEL, R. et al. On the nature of the dark mass in the center of the Milky Way. <\/span>Karalisk\u0101s Astronomijas biedr\u012bbas ikm\u0113ne\u0161a pazi\u0146ojumi (Monthly Notices of the Royal Astronomical Society)<\/b>, t. 291, n. 1, p. 219-234, 11 \u0101r\u0101. 1997.<\/span><\/p>\n

GHEZ, A. M. et al. High Proper-Motion Stars in the Vicinity of Sagittarius A\\ast: Pier\u0101d\u012bjumi par supermas\u012bvu melno caurumu m\u016bsu galaktikas centr\u0101. <\/span>Astrofizikas \u017eurn\u0101ls<\/b>, t. 509, n. 2, p. 678-686, 1998. gada decembris.<\/span><\/p>\n

GHEZ, A. M. et al. Measuring Distance and Properties of the Milky Way's Central Supermassive Black Hole with Stellar Orbits. <\/span>Astrofizikas \u017eurn\u0101ls<\/b>, v. 689, n. 2, p. 1044-1062, dez. 2008.<\/span><\/p>\n

\"\"<\/a><\/p>\n

Vai Visums nav tik skaists?<\/p>\n

Tas viss jau ir neticami, bet ir v\u0113l daudz ko dar\u012bt, k\u0101 teica Nobela fizikas komitejas priek\u0161s\u0113d\u0113t\u0101js Deivids Havilands \"...\u0161ie eksotiskie objekti joproj\u0101m rada daudz jaut\u0101jumu, kas prasa atbildes un motiv\u0113 turpm\u0101kos p\u0113t\u012bjumus. Ne tikai jaut\u0101jumi par to iek\u0161\u0113jo uzb\u016bvi, bet ar\u012b jaut\u0101jumi par to, k\u0101 p\u0101rbaud\u012bt m\u016bsu gravit\u0101cijas teoriju ekstr\u0113mos apst\u0101k\u013cos meln\u0101 cauruma tie\u0161\u0101 tuvum\u0101\". Un m\u0113s b\u016bsim \u0161eit, tom\u0113r ar nepaciet\u012bbu gaid\u0101m n\u0101kamo p\u0101rtraukumu! Tikm\u0113r m\u0113s pateicamies \u0161\u012b gada laure\u0101tiem Roger Penrose, Reinhard Genzel<\/strong> un Andrea Ghez<\/strong>, j\u016bs esat lieliski!<\/p>\n

Ja ar\u012b j\u016bs v\u0113laties izlas\u012bt par Rod\u017eera Penroza darbu, \u0161eit ir da\u017ei raksti, kuros aprakst\u012bts vi\u0146a darbs. Viens no tiem tika public\u0113ts kop\u0101 ar le\u0123end\u0101ro St\u012bvens Hokings<\/a>. \u0160os rakstus varat apskat\u012bt ar\u012b \u0161eit:<\/p>\n

HAWKING, S.; PENROSE, R. The Nature of Space and Time. American Journal of Physics<\/strong>, v. 65, n. 7, p. 676-676, 1997. gada 1. j\u016blijs.<\/p>\n

EHLERS, J.; RINDLER, W.; PENROSE, R. Ener\u0123ijas saglab\u0101\u0161ana k\u0101 relat\u012bv\u0101s meh\u0101nikas pamats. II. American Journal of Physics, t. 33, n. 12, p. 995-997, 1 dez. 1965.<\/p>\n

NEWMAN, E.; PENROSE, R. Pieeja gravit\u0101cijas starojumam ar griezuma koeficientu metodi. Journal of Mathematical Physics, t. 3, n. 3, p. 566-578, 1962. gada 1. maijs.<\/p>\n

PENROSE, R.; RINDLER, W. Ener\u0123ijas saglab\u0101\u0161ana k\u0101 relat\u012bv\u0101s meh\u0101nikas pamats. American Journal of Physics, t. 33, n. 1, p. 55-59, 1965. gada 1. janv\u0101ris.<\/p>\n

\"\"<\/a><\/p>\n

Ja jums ir projekts vai prezent\u0101cija par jebkuru astronomijas jomu, varat izmantot Mind the Graph, lai padar\u012btu saturu efekt\u012bv\u0101ku, didaktisk\u0101ku un jautr\u0101ku! M\u0113s zin\u0101m, ka ir gr\u016bti ieg\u016bt labus att\u0113lus par \u0161o t\u0113mu, t\u0101p\u0113c m\u0113s esam \u0161eit, lai jums pal\u012bdz\u0113tu, j\u016bs varat p\u0101rbaud\u012bt m\u016bsu saturu par astronomiju. <\/span>tie\u0161i \u0161eit<\/span><\/a>.<\/span><\/p>\n

Mind the Graph j\u016bs atrad\u012bsiet visu nepiecie\u0161amo, un, ja jums nav, m\u0113s varam jums pal\u012bdz\u0113t!<\/span><\/p>\n

Uzlabosim komunik\u0101ciju zin\u0101tn\u0113 kop\u0101! Vai esat gatavs izm\u0113\u0123in\u0101t?<\/span><\/p>","protected":false},"excerpt":{"rendered":"","protected":false},"author":4,"featured_media":11862,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":[],"categories":[959,28],"tags":[554,250],"yoast_head":"\nThe Nobel Prize and The First Black Hole Picture - Mind the Graph Blog<\/title>\n<meta name=\"description\" content=\"Read this blog to know how three scientists are awarded the Nobel Prize 2020 in Physics for their contribution to the Black Hole.\" \/>\n<meta name=\"robots\" content=\"index, follow, max-snippet:-1, max-image-preview:large, max-video-preview:-1\" \/>\n<link rel=\"canonical\" href=\"https:\/\/mindthegraph.com\/blog\/lv\/nobel-prize-the-first-black-hole-picture\/\" \/>\n<meta property=\"og:locale\" content=\"lv_LV\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"The Nobel Prize and The First Black Hole Picture - Mind the Graph Blog\" \/>\n<meta property=\"og:description\" content=\"Read this blog to know how three scientists are awarded the Nobel Prize 2020 in Physics for their contribution to the Black Hole.\" \/>\n<meta property=\"og:url\" content=\"https:\/\/mindthegraph.com\/blog\/lv\/nobel-prize-the-first-black-hole-picture\/\" \/>\n<meta property=\"og:site_name\" content=\"Mind the Graph Blog\" \/>\n<meta property=\"article:published_time\" content=\"2020-11-02T11:00:00+00:00\" \/>\n<meta property=\"article:modified_time\" content=\"2023-05-22T14:05:20+00:00\" \/>\n<meta property=\"og:image\" content=\"https:\/\/mindthegraph.com\/blog\/wp-content\/uploads\/2020\/11\/the-nobel-prize-and-the-first-black-hole-picture.png\" \/>\n\t<meta property=\"og:image:width\" content=\"1110\" \/>\n\t<meta property=\"og:image:height\" content=\"600\" \/>\n\t<meta property=\"og:image:type\" content=\"image\/png\" \/>\n<meta name=\"author\" content=\"Fabricio Pamplona\" \/>\n<meta name=\"twitter:card\" content=\"summary_large_image\" \/>\n<meta name=\"twitter:label1\" content=\"Written by\" \/>\n\t<meta name=\"twitter:data1\" content=\"Fabricio Pamplona\" \/>\n\t<meta name=\"twitter:label2\" content=\"Est. reading time\" \/>\n\t<meta name=\"twitter:data2\" content=\"7 minutes\" \/>\n<!-- \/ Yoast SEO plugin. -->","yoast_head_json":{"title":"The Nobel Prize and The First Black Hole Picture - 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a tool used by over 400K users in 60 countries. He has a Ph.D. and solid scientific background in Psychopharmacology and experience as a Guest Researcher at the Max Planck Institute of Psychiatry (Germany) and Researcher in D'Or Institute for Research and Education (IDOR, Brazil). Fabricio holds over 2500 citations in Google Scholar. He has 10 years of experience in small innovative businesses, with relevant experience in product design and innovation management. Connect with him on LinkedIn - Fabricio Pamplona.","sameAs":["http:\/\/mindthegraph.com","https:\/\/www.linkedin.com\/in\/fabriciopamplona"],"url":"https:\/\/mindthegraph.com\/blog\/lv\/author\/fabricio\/"}]}},"_links":{"self":[{"href":"https:\/\/mindthegraph.com\/blog\/lv\/wp-json\/wp\/v2\/posts\/11852"}],"collection":[{"href":"https:\/\/mindthegraph.com\/blog\/lv\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/mindthegraph.com\/blog\/lv\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/mindthegraph.com\/blog\/lv\/wp-json\/wp\/v2\/users\/4"}],"replies":[{"embeddable":true,"href":"https:\/\/mindthegraph.com\/blog\/lv\/wp-json\/wp\/v2\/comments?post=11852"}],"version-history":[{"count":3,"href":"https:\/\/mindthegraph.com\/blog\/lv\/wp-json\/wp\/v2\/posts\/11852\/revisions"}],"predecessor-version":[{"id":27975,"href":"https:\/\/mindthegraph.com\/blog\/lv\/wp-json\/wp\/v2\/posts\/11852\/revisions\/27975"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/mindthegraph.com\/blog\/lv\/wp-json\/wp\/v2\/media\/11862"}],"wp:attachment":[{"href":"https:\/\/mindthegraph.com\/blog\/lv\/wp-json\/wp\/v2\/media?parent=11852"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/mindthegraph.com\/blog\/lv\/wp-json\/wp\/v2\/categories?post=11852"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/mindthegraph.com\/blog\/lv\/wp-json\/wp\/v2\/tags?post=11852"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}