找回密码
 立即注册
查看: 8474|回复: 5

月球陨石高清大图(1)

[复制链接]
发表于 2019-11-13 10:18:41 | 显示全部楼层 |阅读模式
国际认证过的。就不标名字啦。
image002 (1).jpg
image002 (2).jpg
image002 (4).jpg
image002 (5).jpg
image002 (6).jpg
image002 (7).jpg
image002 (11).jpg
image002 (12).jpg
image002 (13).jpg
image002 (15).jpg
image002 (16).jpg
image002 (17).jpg
image002 (18).jpg
image002 (19).jpg
image002 (21).jpg
image002 (22).jpg
image002 (23).jpg
image002 (24).jpg
image002 (25).jpg
image002 (26).jpg
image002 (27).jpg
image002 (28).jpg
image002 (29).jpg
image002 (30).jpg
image002 (31).jpg
image002 (32).jpg
image002 (33).jpg
image002 (34).jpg
image002 (36).jpg
image002 (37).jpg
image002 (38).jpg
image002 (39).jpg
image002 (40).jpg
发表于 2019-11-13 17:50:38 | 显示全部楼层
没有名称及文字说明学习意义不大
 楼主| 发表于 2019-11-14 08:52:15 | 显示全部楼层
梦回的流星 发表于 2019-11-13 17:50
没有名称及文字说明学习意义不大

以后有空补上。这里每个图保证都是认证过的,国际数据库里的图。

美国wustl大学代为维护的数据库里的。

发表于 2019-11-14 09:54:29 | 显示全部楼层
第一张不是陨石吧?
 楼主| 发表于 2019-11-14 13:52:25 | 显示全部楼层

第一块月陨的名字是:Jiddat al Harasis 838 in Oman


这里所有的月陨图片都是经过国际陨石命名委员会认证过的。欢迎监督。
 楼主| 发表于 2019-11-14 13:53:25 | 显示全部楼层

第一块月陨的说明:

Jiddat al Harasis 838
Al Wusta, Oman
Find: 2003 Feb 28
Mass: 34.36 g
Classification: Lunar meteorite
History: One stone of 34.36 g was discovered about 28 km south of Al Ghaftain on a desert expedition on Feb. 28, 2003.
Physical characteristics: (R. Bartoschewitz, Bart) The meteorite lacks an obvious fusion crust but has the frosted, ablated exterior typical of Omani lunar stones. The interior is black-gray with many white, brown, and gray inclusions. Terrestrial weathering is negligible.
Petrography: (R. Bartoschewitz, Bart; P. Appel, B. Mader, Kiel) Fragmental breccia composed of a variety of lithic clasts and mineral fragments of plagioclase, augite, pigeonite, poor-Ca pyroxene, and olivine set in a fine-grained matrix. Lithic clasts include anorthosite, fragmental breccia, gabbro, norite, basalt, pyroxenite, and regolith (chondritic and lunar metal; HASP spherule) set in a fine-grained dark gray matrix, and with Ni-iron, troilite, pyrrhotite, pentlandite, ilmenite, chromite, zirconolite, baddeleyite, and zircon.
Geochemistry:(R. Bartoschewitz, Bart., P. Appel and B. Mader, Kiel) Fa39.7 (mg# = 74-53, Fe/Mn = 90, n=3); low-Ca pyroxene Fs56Wo3 (mg# = 51-32); pigeonite Fs36Wo11 (mg# = 36-58, n=13); subcalcic augite Fs32Wo17 (n=1); augite Fs22Wo33 (mg# = 52-44, n=7); ferro-augite Fs41Wo27 (mg# = 29-33, n=9; Fe/Mn = 55); An93Or1 (An63-97, n=63). Kamacite Ni 5-76, Co 12-5 (mg/g, n=3); taenite Ni 192, Co 15 (mg/g); awaruite Ni 636, Co 18 (mg/g); pyrrhotite; troilite; pentlandite Ni 331, Co 11 (mg/g). Bulk composition (R. Korotev, WUSL): FeO 4.9, K2O 0.3 wt%; Sc 8.99, Ni 229, Zr 138, La 9.8, Ce 24.5, Nd 14.9, Sm 4.43, Eu 0.986, Ta 0.447, Ir 0.0094, Au 0,0074, Th 2.3, U 0.64 (all in ppm).
Classification: Lunar (mingled regolith breccia). Classified as a mingled regolith breccia rather than a feldspathic fragmental breccia based as well on the presence of mare and KREEPy material as of HASP and chondritic metal.
Specimens: A total of 6.9 g is on deposit at Kiel. Thin section and 3.5 g at Bart. The main mass is held by the finder.   

您需要登录后才可以回帖 登录 | 立即注册

本版积分规则

QQ|Archiver|手机版|中陨网✪国陨网 ( 冀ICP备10012798号-1 )点击这里给我发消息

GMT+8, 2024-5-20 19:36 , Processed in 0.070000 second(s), 20 queries .

Powered by Discuz! X3.5

© 2001-2024 Discuz! Team.

快速回复 返回顶部 返回列表