宇宙の膨張の記事

$The ultimate fate of an expanding universe depends on the matter density Ω M {\displaystyle \Omega _{M}} and the dark energy density Ω Λ {\displaystyle \Omega _{\Lambda }} .$

宇宙の終焉ビッグバンから究極の運命まで

宇宙の終焉ビッグバン理論ダークエネルギービッグフリーズ

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Lyman Spitzer played a major role in the birth of the Hubble Space Telescope project.

ハッブル宇宙望遠鏡宇宙の深淵を照らす人類の眼

ハッブル宇宙望遠鏡NASA天文学宇宙観測

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$Except for the few stars in the foreground (which are bright and easily recognizable because only they have diffraction spikes), every speck of light in the composite photo is an individual galaxy, some of them as old as 13.2 billion years; the observable universe is estimated to contain more than 2 trillion galaxies.[1] From the Hubble eXtreme Deep Field.$

宇宙論宇宙の起源から究極の運命までを解き明かす科学と哲学

宇宙論ビッグバン理論物理宇宙論ダークマター

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KBCボイド天の川銀河が位置する巨大な宇宙の空白地帯

KBCボイドローカルホール宇宙論ハッブル定数

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