English
| 正體中文 |
简体中文
|
全文筆數/總筆數 : 94201/94201 (100%)
造訪人次 : 81536405 線上人數 : 2347
RC Version 7.0 © Powered By DSPACE, MIT. Enhanced by
NTU Library IR team.
搜尋範圍
全部NCUIR
理學院
天文研究所
--期刊論文
查詢小技巧:
您可在西文檢索詞彙前後加上"雙引號",以獲取較精準的檢索結果
若欲以作者姓名搜尋,建議至進階搜尋限定作者欄位,可獲得較完整資料
進階搜尋
主頁
‧
登入
‧
上傳
‧
說明
‧
關於NCUIR
‧
管理
NCU Institutional Repository
>
理學院
>
天文研究所
>
期刊論文
>
Item 987654321/101756
資料載入中.....
書目資料匯出
Endnote RIS 格式資料匯出
Bibtex 格式資料匯出
引文資訊
資料載入中.....
資料載入中.....
請使用永久網址來引用或連結此文件:
https://ir.lib.ncu.edu.tw/handle/987654321/101756
題名:
Boulders on asteroid toutatis as observed by chang e-2
作者:
葉永烜
;
Jiang, Yun
;
Ji, Jianghui
;
Huang, Jiangchuan
;
Marchi, Simone
;
Li, Yuan
;
Ip, Wing-Huen
貢獻者:
理學院天文研究所
關鍵詞:
639/33/445
;
704/445/848
;
Asteroids
;
Frequency distribution
;
Geology
;
Humanities and Social Sciences
;
Morphology
;
multidisciplinary
;
Preservation
;
Science
;
Spacecraft
;
Spatial distribution
日期:
2015-11-02
上傳時間:
2026-04-21 14:43:11 (UTC+8)
出版者:
Nature Publishing Group;London: Springer Science and Business Media LLC
摘要:
摘要: AbstractBoulders are ubiquitously found on the surfaces of small rocky bodies in the inner solar system and their spatial and size distributions give insight into the geological evolution and collisional history of the parent bodies. Using images acquired by the Chang’e-2 spacecraft, more than 200 boulders have been identified over the imaged area of the near-Earth asteroid Toutatis. The cumulative boulder size frequency distribution (SFD) shows a steep slope of −4.4 ± 0.1, which is indicative of a high degree of fragmentation. Similar to Itokawa, Toutatis probably has a rubble-pile structure, as most boulders on its surface cannot solely be explained by impact cratering. The significantly steeper slope for Toutatis’ boulder SFD compared to Itokawa may imply a different preservation state or diverse formation scenarios. In addition, the cumulative crater SFD has been used to estimate a surface crater retention age of approximately 1.6 ± 0.3 Gyr.
其他題名: Sci Rep
出版者: London: Springer Science and Business Media LLC
出版日期: 2015-11-02
出處: Scientific Reports, 2015-11, Vol.5 (1), p.16029-16029, Article 16029
資源來源: Publicly available content database
版權: The Author(s) 2015
版權: Copyright Nature Publishing Group Nov 2015
版權: Copyright © 2015, Macmillan Publishers Limited 2015 Macmillan Publishers Limited
識別號: ISSN: 2045-2322
識別號: EISSN: 2045-2322
識別號: DOI: 10.1038/srep16029
識別號: PMID: 26522880
顯示於類別:
[天文研究所] 期刊論文
文件中的檔案:
檔案
描述
大小
格式
瀏覽次數
index.html
0Kb
HTML
11
檢視/開啟
在NCUIR中所有的資料項目都受到原著作權保護.
社群 sharing
::: Copyright National Central University. | 國立中央大學圖書館版權所有 |
收藏本站
|
設為首頁
| 最佳瀏覽畫面: 1024*768 | 建站日期:8-24-2009 :::
DSpace Software
Copyright © 2002-2004
MIT
&
Hewlett-Packard
/
Enhanced by
NTU Library IR team
Copyright ©
-
隱私權政策聲明