Sự Di Chuyển của Các Sao Chổi

Solar System Research - Tập 37 - Trang 165-174 - 2003
N. I. Perov1
1Yaroslavl State Pedagogical University, Yaroslavl, Russia

Tóm tắt

Dựa trên một trong những trường hợp đặc biệt của mô hình Hill trung bình hai lần cho phép tính đến tính hình cầu của cơ thể trung tâm, một phương trình tích phân được phát triển để xác định thời gian di chuyển của các hạt nhân sao chổi từ các kho chứa sao chổi khác nhau và một phương trình đại số bậc 14 để xác định các điều kiện ban đầu cho phép hạt nhân sao chổi (cái mà tại thời điểm ban đầu di chuyển trong quỹ đạo với độ lệch tâm tùy ý (0 < e < 1) và độ nghiêng (0° < i < 180°) nằm sâu bên trong lĩnh vực tương tác của cơ thể trung tâm) thoát ra khỏi lĩnh vực tương tác của cơ thể trung tâm hoặc tác động vào cơ thể trung tâm. Chúng tôi phân tích hình dạng của các ranh giới của các kho chứa sao chổi giả thuyết và phương pháp tìm kiếm các vùng có nồng độ cao của các hạt giữa các vì sao trong Hệ Mặt Trời.

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Tài liệu tham khảo

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