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    Karanlık madde

    Astrofiziksel Kavram
    evrimagaci.org sitesinden görsel
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    Yazeka

    Arama sonuçlarına dayanarak oluşturuldu

    Karanlık madde, astrofizikte elektromanyetik dalgalarla etkileşime girmeyen, varlığı yalnızca diğer maddeler üzerindeki kütleçekimsel etkisiyle belirlenen varsayımsal bir maddedir. Evrenin büyük bölümünü oluşturduğu düşünülen bu madde, galaksilerin dönme hızları ve kütle dağılımını açıklamak için gereklidir.123

    Kütleçekim etkisi ile gözlemlenebilen karanlık madde, gökada kümelerinde ve evrende gözle görülebilen maddelerden çok daha fazla miktarda bulunur. Varlığı, ışığın bükülmesi (kütleçekimsel merceklenme) gibi dolaylı yöntemlerle kanıtlanmıştır.1423

    tr.wikipedia.org1
    evrimagaci.org2
    evrenatlasi.com.tr3
    bilimgenc.tubitak.gov.tr4

    İlgili gündem

    Evrenin büyük bir kısmını oluşturan karanlık maddenin yer çekiminden etkilendiği doğrulandı. Ancak bilim insanları, keşfedilirse evreni inceleme şeklimizi değiştirecek beşinci bir temel kuvvetin var olma ihtimalinin, düşük de olsa, hâlâ mevcut olduğunu ve yeni verileri beklediklerini açıkladı.
    chip.com.tr5 Kasım
    Cenevre Üniversitesi öncülüğünde yürütülen yeni bir çalışma, karanlık maddenin de aynı normal madde gibi klasik fizik kurallarına uygun davrandığını verilerle ortaya koydu.
    donanimhaber.com4 Kasım
    Evrenin sonsuza kadar genişlemeyeceği, aksine milyarlarca yıl içinde kendi üzerine çökebileceği yönündeki yeni teori yaklaşık 20 milyar yıllık bir son kullanma tarihine işaret ediyor. Detaylar haberde...
    anlatilaninotesi.com.tr8 Ekim

    Astronomi hipotezleri

    Çokluevren
    Solucan
    deliği
    Kütleçekimsel
    tekillik
    Hawking
    radyasyonu
    Panspermia
    Dünya
    dışı yaşam
    Heat
    death of the universe
    Drake
    denklemi
    Yanıt, yapay zeka tarafından internetteki kaynaklara dayanarak oluşturulmuştur. Hatalar içerebilir.
    Yazeka hakkındatr.wikipedia.org
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