{"id":99581,"date":"2025-10-26T22:11:17","date_gmt":"2025-10-26T22:11:17","guid":{"rendered":"https:\/\/www.newsbeep.com\/il\/99581\/"},"modified":"2025-10-26T22:11:17","modified_gmt":"2025-10-26T22:11:17","slug":"esa-focusing-on-ngc-3370","status":"publish","type":"post","link":"https:\/\/www.newsbeep.com\/il\/99581\/","title":{"rendered":"ESA &#8211; Focusing on NGC 3370"},"content":{"rendered":"<p>Today\u2019s ESA\/Hubble\u00a0Picture of the Week\u00a0features a galaxy that Hubble has captured multiple times over more than 20 years. The galaxy is called NGC 3370, and it is a\u00a0spiral galaxy\u00a0located nearly 90 million light-years away in the constellation\u00a0Leo\u00a0(The Lion).<\/p>\n<p>What is it about this galaxy that makes it a popular target for researchers? NGC 3370 is home to two kinds of objects that astronomers prize for their usefulness in determining distances to faraway galaxies: Cepheid variable\u00a0stars\u00a0and Type Ia\u00a0supernovae.<\/p>\n<p>Cepheid variable stars change in both size and temperature as they pulsate. As a result, the luminosity of these stars varies over a period of days to months. It does so in a way that reveals something important: the more luminous a Cepheid variable star is, the more slowly it pulsates. By measuring how long a Cepheid variable\u2019s brightness takes to complete one cycle, astronomers can determine how bright the star actually is. Paired with how bright the star appears from Earth, this information gives the distance to the star and its home galaxy.<\/p>\n<p>Type Ia supernovae provide a way to measure distances in a single explosive burst rather than through regular brightness variations. Type Ia supernovae happen when the dead core of a star ignites in a sudden flare of nuclear fusion. These explosions peak at very similar luminosities, and much like for a Cepheid variable star, knowing the intrinsic brightness of a supernova explosion allows for its distance to be measured. Observations of Cepheid variable stars and Type Ia supernovae are both critical for precisely measuring how fast our Universe is expanding.\u00a0<\/p>\n<p>A previous Hubble image of NGC 3370 was\u00a0<a href=\"https:\/\/esahubble.org\/images\/opo0324a\/\" rel=\"nofollow noopener\" target=\"_blank\">released in 2003<\/a>. The image released today zooms in on the galaxy, presenting a richly detailed view that incorporates\u00a0wavelengths of light\u00a0that were not included in the previous version. NGC 3370 is a member of the NGC 3370 group of galaxies along with other Hubble targets\u00a0<a href=\"https:\/\/esahubble.org\/images\/potw1712a\/\" rel=\"nofollow noopener\" target=\"_blank\">NGC 3447<\/a>\u00a0and\u00a0<a href=\"https:\/\/esahubble.org\/images\/potw1415a\/\" rel=\"nofollow noopener\" target=\"_blank\">NGC 3455<\/a>.<\/p>\n<p>[Image Description:\u00a0A spiral galaxy occupies most of the image. It is a slightly tilted disc of stars, yellow-white in the centre and blue in the outskirts, showing light from different stars in the galaxy. Its spiral arms curl outwards from the centre, speckled with blue star clusters. Dark reddish threads of dust swirl around the galaxy\u2019s centre. The backdrop is two medium-sized and many small, distant galaxies on a black background.]<\/p>\n","protected":false},"excerpt":{"rendered":"Today\u2019s ESA\/Hubble\u00a0Picture of the Week\u00a0features a galaxy that Hubble has captured multiple times over more than 20 years.&hellip;\n","protected":false},"author":2,"featured_media":99582,"comment_status":"","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[23],"tags":[85,46,141,145],"class_list":{"0":"post-99581","1":"post","2":"type-post","3":"status-publish","4":"format-standard","5":"has-post-thumbnail","7":"category-space","8":"tag-il","9":"tag-israel","10":"tag-science","11":"tag-space"},"_links":{"self":[{"href":"https:\/\/www.newsbeep.com\/il\/wp-json\/wp\/v2\/posts\/99581","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.newsbeep.com\/il\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.newsbeep.com\/il\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/il\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/il\/wp-json\/wp\/v2\/comments?post=99581"}],"version-history":[{"count":0,"href":"https:\/\/www.newsbeep.com\/il\/wp-json\/wp\/v2\/posts\/99581\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/il\/wp-json\/wp\/v2\/media\/99582"}],"wp:attachment":[{"href":"https:\/\/www.newsbeep.com\/il\/wp-json\/wp\/v2\/media?parent=99581"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.newsbeep.com\/il\/wp-json\/wp\/v2\/categories?post=99581"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.newsbeep.com\/il\/wp-json\/wp\/v2\/tags?post=99581"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}