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Featured articles - 23JP HOME SITE English - Click here French - Click here Spanish - Click here German - click here Italian - Click here Portuguese - Click here 現在のページコンテンツの追加情報 天文学の歴史 これは、現代の天文学の基礎に到達するのに役立つ要因の1つであり、理論的物理学データを実際の観測に適用することで現在私たちが理解しているその結果に到達しました。1915年にアルバートアインシュタインが相対性理論の一般理論を策定しました。しかし、アインシュタインは1916年に方程式を解いて、宇宙は固定されておらず、拡大または縮小していることを発見しました。アインシュタインは、宇宙が固定されているという信念を踏まえて、宇宙定数の方程式に追加し、1922年に科学者のアレクサンダーフリードマンが方程式の解を提示しました。フィールドのアインシュタイン。フリードマンルーメトリックロバートソンウォーカーメトリックとして知られている、膨張または収縮の対象となる宇宙について説明しています。 1910年、フェストスリーパー（および後にカールウィルヘルムウィルツ）は楕円銀河のスペクトルにおける赤方偏移の現象を説明しようとしましたが、これは後で地球から離れると解釈されますが、そのときの銀河の距離を決定することは困難でした。それらの方法の1つは、天体の物理的なサイズをその角度のサイズと比較することでしたが、物理的なサイズは実際のサイズになると想定されています。別の方法は、天体星雲の明るさを測定し、距離の2乗の逆法則に従って星雲の距離を計算できる固有の明るさを仮定することに基づいていました。これらの方法を適用することの難しさを考えると、星雲が実際に天の川の外にあったことを知ることは不可能でした。 1927年、ベルギーの司祭兼天文学者であるジョージルターは、フリードマン-ルンマー-ロバートソン-ウォーカーの方程式に基づいて、楕円星雲の円運動に基づいて、宇宙が「爆発」で始まり、ビッグバンと呼ばれたことを提案しました。 その後、1929年にエドウィンハッブルは楕円星雲で望遠鏡を使って観測を

Featured articles - 21VT HOME SITE English - Click here French - Click here Spanish - Click here German - click here Italian - Click here Portuguese - Click here Thông tin bổ sung cho nội dung trang hiện tại Lịch sử Thiên văn học Đó là một trong những yếu tố giúp đạt được những điều cơ bản của thiên văn học hiện đại và kết quả của nó mà chúng ta hiện đang hiểu bằng cách áp dụng dữ liệu vật lý lý thuyết với các quan sát thực tế. Albert Einstein đã xây dựng lý thuyết tương đối rộng vào năm 1915 sau Công nguyên. Nhưng vào năm 1916 sau Công Nguyên, Einstein đã phát hiện ra thông qua các phương trình của mình rằng vũ trụ không cố định và nó có thể giãn nở hoặc co lại. Với niềm tin vào thời điểm đó rằng vũ trụ là cố định, Einstein đã thêm vào phương trình hằng số vũ trụ, do đó dẫn đến một vũ trụ ổn định và ổn định trong không-thời gian. Einstein của trường, mô tả một vũ trụ được gọi là số liệu Friedman-Lumetric-Robertson-Walker có thể giãn nở hoặc co lại. Vào năm 1910 s

Featured articles - 20TL HOME SITE English - Click here French - Click here Spanish - Click here German - click here Italian - Click here Portuguese - Click here ప్రస్తుత పేజీ కంటెంట్ కోసం అదనపు సమాచారం ఖగోళ శాస్త్ర చరిత్ర ఆధునిక ఖగోళ శాస్త్రం మరియు దాని ఫలితాలను ఆచరణాత్మక పరిశీలనలతో సైద్ధాంతిక భౌతిక డేటాను వర్తింపజేయడం ద్వారా ప్రస్తుతం మనకు అర్థమయ్యే కారకాల్లో ఇది ఒకటి. ఆల్బర్ట్ ఐన్‌స్టీన్ క్రీ.శ 1915 లో సాపేక్ష సాపేక్ష సిద్ధాంతాన్ని రూపొందించారు. విశ్వం స్థిరంగా మరియు స్థిరంగా ఉందని శాస్త్రవేత్తలు విశ్వసించారు, ప్రారంభం లేదా ముగింపు లేదు. క్రీస్తుశకం 1916 లో, ఐన్స్టీన్ తన సమీకరణాల ద్వారా విశ్వం స్థిరంగా లేదని మరియు అది విస్తరిస్తుందని లేదా తగ్గిపోతుందని కనుగొన్నాడు. ఆ సమయంలో విశ్వం స్థిరంగా ఉందనే నమ్మకంతో, ఐన్స్టీన్ తన విశ్వోద్భవ స్థిరాంకం యొక్క సమీకరణాలకు జతచేశాడు, తద్వారా అంతరిక్ష సమయములో స్థిరమైన మరియు స్థిరమైన విశ్వం ఏర్పడింది, మరియు క్రీ.శ 1922 లో శాస్త్రవేత్త అలెగ్జాండర్ ఫ్రైడ్మాన్ సమీకరణాలకు పరిష్కారాలను సమర్పించాడు. ఫీల్డ్ యొక్క ఐన్స్టీన్, ఫ్రీడ్మాన్-లోమె

Featured articles - 19TH HOME SITE English - Click here French - Click here Spanish - Click here German - click here Italian - Click here Portuguese - Click here ข้อมูลเพิ่มเติมสำหรับเนื้อหาของเพจปัจจุบัน ประวัติศาสตร์ดาราศาสตร์ มันเป็นปัจจัยหนึ่งที่ช่วยในการเข้าถึงพื้นฐานของดาราศาสตร์สมัยใหม่และผลลัพธ์ของมันที่เราเข้าใจในปัจจุบันโดยการใช้ข้อมูลทางฟิสิกส์เชิงทฤษฎีกับการสังเกตในทางปฏิบัติ Albert Einstein ได้กำหนดทฤษฎีสัมพัทธภาพทั่วไปในปีค. ศ. 1915 นักวิทยาศาสตร์เชื่อว่าเอกภพมีความเสถียรและมั่นคงโดยไม่มีจุดเริ่มต้นหรือจุดจบ แต่ในปีค. ศ. 1916 ไอน์สไตน์ได้ค้นพบด้วยสมการของเขาว่าเอกภพไม่คงที่และทั้งขยายหรือหดตัวด้วยความเชื่อในเวลานั้นว่าเอกภพได้รับการแก้ไขแล้วไอน์สไตน์ได้เพิ่มสมการของค่าคงที่ของจักรวาลเพื่อส่งผลให้เอกภพมีเสถียรภาพและมีเสถียรภาพภายในห้วงเวลาและในปีพ. ศ. 2465 นักวิทยาศาสตร์ Alexander Friedman ได้นำเสนอวิธีแก้สมการ Einstein of the field อธิบายจักรวาลที่เรียกว่าเมตริก Friedman-Lumetric-Robertson-Walker ซึ่งอาจมีการขยายตัวหรือหดตัว ในปีค. ศ. 1910 Festo Slee