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Các Chữ Ký Isotop Presolar Trong Thiên Thạch và Sao Chổi: Những Kiến Thức Mới Từ Nhiệm Vụ Rosetta Đến Sao Chổi 67P/Churyumov–Gerasimenko
Tóm tắt
Sao chổi được coi là những cơ thể hành tinh nguyên thủy nhất trong Hệ Mặt Trời của chúng ta, tức là chúng nên có sự bảo tồn tốt nhất các thành phần rắn của vật chất mà từ đó Hệ Mặt Trời của chúng ta hình thành. Nhiệm vụ Rosetta gần đây của ESA đến sao chổi 67P/Churyumov–Gerasimenko (67P/CG) đã cung cấp một kho dữ liệu đồng vị phong phú, mở rộng đáng kể các tập dữ liệu hiện có về thành phần đồng vị của sao chổi. Trong tài liệu này, chúng tôi xem xét kiến thức hiện tại của mình về các thành phần đồng vị của H, C, N, O, Si, S, Ar, và Xe trong các vật liệu nguyên thủy của Hệ Mặt Trời được nghiên cứu trong các phòng thí nghiệm trên trái đất và cách dữ liệu Rosetta thu được với các máy quang phổ khối ROSINA (Cảm biến Ion và Phân tích Trung tính của Tàu vũ trụ Rosetta) và COSIMA (Máy Chỉ Thị Khối Ion Thứ cấp của Sao chổi) phù hợp với bức tranh này. Dữ liệu đồng vị H, Si, S và Xe của sao chổi 67P/CG gợi ý rằng sao chổi này có thể đặc biệt nguyên thủy và có thể đã bảo tồn một lượng lớn vật chất trước sao chưa qua xử lý. Chúng tôi đề cập đến câu hỏi liệu thành phần Si bền của 67P/CG có chứa dấu vết đồng vị trước sao từ một siêu tân tinh (SN) loại II gần đó và thảo luận mức độ mà những bất thường đồng vị C và O bắt nguồn từ các hạt trước sao nên có thể quan sát được trong bụi từ 67P/CG. Cuối cùng, chúng tôi khám phá xem liệu dấu vết đồng vị của một đóng góp từ siêu tân tinh muộn có thể nhìn thấy trong thành phần dễ bay hơi của 67P/CG ở địa điểm hình thành 67P/CG trong tinh vân mặt trời hay không.
Từ khóa
#sao chổi #đồng vị #vật chất nguyên thủy #Rosetta #Churyumov-Gerasimenko #siêu tân tinh #hạt trước saoTài liệu tham khảo
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