{"id":568,"date":"2019-03-05T16:09:50","date_gmt":"2019-03-05T16:09:50","guid":{"rendered":"https:\/\/192.243.19.131\/wordpress\/?page_id=562"},"modified":"2019-08-29T09:55:25","modified_gmt":"2019-08-29T07:55:25","slug":"radio-astronomy","status":"publish","type":"page","link":"https:\/\/www.mdscc.nasa.gov\/index.php\/en\/radio-astronomy\/","title":{"rendered":"Radio Astronomy"},"content":{"rendered":"\n<div class=\"wp-block-columns has-2-columns is-layout-flex wp-container-core-columns-is-layout-8f761849 wp-block-columns-is-layout-flex\">\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\">\n<div class=\"wp-block-columns has-2-columns is-layout-flex wp-container-core-columns-is-layout-8f761849 wp-block-columns-is-layout-flex\">\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\">\n<figure class=\"wp-block-image is-resized\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/www.mdscc.nasa.gov\/wp-content\/uploads\/2019\/07\/gamma-e1563541985243-MOD.jpg\" alt=\"\" width=\"251\" height=\"188\"\/><\/figure>\n<\/div>\n\n\n\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\">\n<figure class=\"wp-block-image is-resized\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/www.mdscc.nasa.gov\/wp-content\/uploads\/2019\/07\/electromagnetic_radiation-e1563541957616-MOD.jpg\" alt=\"\" width=\"252\" height=\"189\"\/><\/figure>\n<\/div>\n<\/div>\n\n\n\n<p class=\"wp-block-paragraph\"><\/p>\n<\/div>\n\n\n\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\">\n<div class=\"wp-block-columns has-2-columns is-layout-flex wp-container-core-columns-is-layout-8f761849 wp-block-columns-is-layout-flex\">\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\">\n<figure class=\"wp-block-image is-resized\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/www.mdscc.nasa.gov\/wp-content\/uploads\/2019\/07\/Magallanes-e1563541920634.jpg\" alt=\"\" width=\"251\" height=\"188\"\/><\/figure>\n<\/div>\n\n\n\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\">\n<figure class=\"wp-block-image is-resized\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/www.mdscc.nasa.gov\/wp-content\/uploads\/2019\/07\/1.jpg\" alt=\"\" width=\"245\" height=\"184\"\/><\/figure>\n\n\n\n<p class=\"wp-block-paragraph\"><\/p>\n<\/div>\n<\/div>\n\n\n\n<p class=\"wp-block-paragraph\"><\/p>\n<\/div>\n<\/div>\n\n\n\n<p class=\"wp-block-paragraph\">Radio astronomy is a subfield of <a href=\"https:\/\/en.wikipedia.org\/wiki\/Astronomy\">astronomy <\/a>that studies <a href=\"https:\/\/en.wikipedia.org\/wiki\/Astronomical_object\">celestial objects<\/a> at <a href=\"https:\/\/en.wikipedia.org\/wiki\/Radio_frequency\">radio frequencies<\/a>. The initial detection of radio waves from an astronomical object was made in the 1930s, when <a href=\"https:\/\/en.wikipedia.org\/wiki\/Karl_Guthe_Jansky\">Karl Jansky<\/a> observed radiation coming from the <a href=\"https:\/\/en.wikipedia.org\/wiki\/Milky_Way\">Milky Way<\/a>. Subsequent observations have identified a number of different sources of radio emission. These include <a href=\"https:\/\/en.wikipedia.org\/wiki\/Star\">stars <\/a>and <a href=\"https:\/\/en.wikipedia.org\/wiki\/Galaxy\">galaxies<\/a>, as well as entirely new classes of objects, such as <a href=\"https:\/\/en.wikipedia.org\/wiki\/Radio_galaxy\">radio galaxies<\/a>, <a href=\"https:\/\/en.wikipedia.org\/wiki\/Quasar\">quasars<\/a>, <a href=\"https:\/\/en.wikipedia.org\/wiki\/Pulsar\">pulsars<\/a>, and <a href=\"https:\/\/en.wikipedia.org\/wiki\/Astrophysical_maser\">masers<\/a>. The discovery of the<a href=\"https:\/\/en.wikipedia.org\/wiki\/Cosmic_microwave_background\"> cosmic microwave background radiation<\/a>, which provided compelling evidence for the <a href=\"https:\/\/en.wikipedia.org\/wiki\/Big_Bang\">Big Bang<\/a>, was made through radio astronomy.<\/p>\n\n\n\n<p class=\"wp-block-paragraph\">Radio astronomy is conducted using large <a href=\"https:\/\/en.wikipedia.org\/wiki\/Antenna_(radio)\">radio antennas<\/a> referred to as <a href=\"https:\/\/en.wikipedia.org\/wiki\/Radio_telescope\">radio telescopes<\/a>, that are either used singularly, or with multiple linked telescopes utilizing the techniques of <a href=\"https:\/\/en.wikipedia.org\/wiki\/Astronomical_interferometer\">radio interferometry<\/a> and <a href=\"https:\/\/en.wikipedia.org\/wiki\/Aperture_synthesis\">aperture synthesis<\/a>. The use of interferometry allows radio astronomy to achieve high <a href=\"https:\/\/en.wikipedia.org\/wiki\/Angular_resolution\">angular resolution<\/a>, as the resolving power of an interferometer is set by the distance between its components, rather than the size of its components.<\/p>\n\n\n\n<p class=\"wp-block-paragraph\">               <\/p>\n","protected":false},"excerpt":{"rendered":"<p>Radio astronomy is a subfield of astronomy that studies celestial objects at radio frequencies. The initial detection of radio waves from an astronomical object was made in the 1930s, when Karl Jansky observed radiation coming from the Milky Way. Subsequent observations have identified a number of different sources of radio emission. These include stars and &#8230; <a title=\"Radio Astronomy\" class=\"read-more\" href=\"https:\/\/www.mdscc.nasa.gov\/index.php\/en\/radio-astronomy\/\" aria-label=\"Leer m\u00e1s sobre Radio Astronomy\">Leer m\u00e1s<\/a><\/p>\n","protected":false},"author":1,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-568","page","type-page","status-publish"],"aioseo_notices":[],"aioseo_head":"\n\t\t<!-- All in One SEO 4.9.8 - aioseo.com -->\n\t<meta name=\"description\" content=\"Radio astronomy is a subfield of astronomy that studies celestial objects at radio frequencies. The initial detection of radio waves from an astronomical object was made in the 1930s, when Karl Jansky observed radiation coming from the Milky Way. Subsequent observations have identified a number of different sources of radio emission. These include stars and\" \/>\n\t<meta name=\"robots\" content=\"max-image-preview:large\" \/>\n\t<link rel=\"canonical\" href=\"https:\/\/www.mdscc.nasa.gov\/index.php\/en\/radio-astronomy\/\" \/>\n\t<meta name=\"generator\" content=\"All in One SEO (AIOSEO) 4.9.8\" \/>\n\t\t<meta property=\"og:locale\" content=\"es_ES\" \/>\n\t\t<meta property=\"og:site_name\" content=\"Madrid Deep Space Communications Complex                                                         - DEEP SPACE NETWORK\" \/>\n\t\t<meta property=\"og:type\" content=\"article\" \/>\n\t\t<meta property=\"og:title\" content=\"Radio Astronomy - Madrid Deep Space Communications Complex\" \/>\n\t\t<meta property=\"og:description\" content=\"Radio astronomy is a subfield of astronomy that studies celestial objects at radio frequencies. The initial detection of radio waves from an astronomical object was made in the 1930s, when Karl Jansky observed radiation coming from the Milky Way. 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