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SN 1604

SN 1604, přezdívaná též Keplerova supernova, je supernova, poslední, která byla v Mléčné dráze dobře pozorovatelná pouhým okem. Poprvé byla pozorována 9. října roku 1604. Jasnost supernovy se z původně nevýrazné hvězdy náhle zvýšila na −2,5 zdánlivé hvězdné velikosti, a tak byla pozorovatelná prostým okem celý rok. Důkladněji ji studoval Johannes Kepler…

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SN 1604

Nodes9
Edges8
Triples3
Avg. degree1.78
Density0.222222
Components1

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SN 1604

Top relations

related to Externí odkazy · 3
SN 1604 → Obrázky, SN, Wikimedia Commons

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Important terminology

1604 supernova pozorovatelná okem poprvé října sn přezdívaná též keplerova poslední mléčné dráze dobře pouhým pozorována roku jasnost supernovy původně

Entity relationships Subject–Predicate–Object triples

SubjectPredicateObjectConfidenceSrc
SN 1604related to Externí odkazyObrázky0.60section
SN 1604related to Externí odkazySN0.60section
SN 1604related to Externí odkazyWikimedia Commons0.60section

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    Min side: 3
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