• 中国出版政府奖提名奖

    中国百强科技报刊

    湖北出版政府奖

    中国高校百佳科技期刊

    中国最美期刊

    留言板

    尊敬的读者、作者、审稿人, 关于本刊的投稿、审稿、编辑和出版的任何问题, 您可以本页添加留言。我们将尽快给您答复。谢谢您的支持!

    姓名
    邮箱
    手机号码
    标题
    留言内容
    验证码

    撞击坑统计定年法及对月球虹湾地区的定年结果

    赵健楠 黄俊 肖龙 乔乐 王江 胡斯宇

    赵健楠, 黄俊, 肖龙, 乔乐, 王江, 胡斯宇, 2013. 撞击坑统计定年法及对月球虹湾地区的定年结果. 地球科学, 38(2): 351-361. doi: 10.3799/dqkx.2013.034
    引用本文: 赵健楠, 黄俊, 肖龙, 乔乐, 王江, 胡斯宇, 2013. 撞击坑统计定年法及对月球虹湾地区的定年结果. 地球科学, 38(2): 351-361. doi: 10.3799/dqkx.2013.034
    ZHAO Jian-nan, HUANG Jun, XIAO Long, QIAO Le, WANG Jiang, HU Si-yu, 2013. Crater Size-Frequency Distribution Measurements and Age Determination of Sinus Iridum. Earth Science, 38(2): 351-361. doi: 10.3799/dqkx.2013.034
    Citation: ZHAO Jian-nan, HUANG Jun, XIAO Long, QIAO Le, WANG Jiang, HU Si-yu, 2013. Crater Size-Frequency Distribution Measurements and Age Determination of Sinus Iridum. Earth Science, 38(2): 351-361. doi: 10.3799/dqkx.2013.034

    撞击坑统计定年法及对月球虹湾地区的定年结果

    doi: 10.3799/dqkx.2013.034
    基金项目: 

    国家自然科学基金项目 41072045

    国家基础科学人才培养专项基金项目 J0830520

    教育部高等学校博士学科点专项科研基金项目 20090145110001

    详细信息
      作者简介:

      赵健楠(1990-),男,博士研究生,主要从事行星地质学研究.E-mail:schwaitser@126.com

      通讯作者:

      肖龙,E-mail:longxiao@cug.edu.cn

    • 中图分类号: P691

    Crater Size-Frequency Distribution Measurements and Age Determination of Sinus Iridum

    • 摘要: 撞击作用是行星形成和表面重塑的重要地质过程,记录和揭示了行星的演化历史.撞击作用形成的撞击坑可用于研究天体表面地质单元形成的时间.依据内太阳系天体表面的撞击历史,总结了通过对撞击坑的直径和频率分布进行统计,计算天体表面模式年龄的原理和方法.在此基础上,利用美国“月球勘测轨道器(LRO)”广角相机获得的图像,对月球虹湾地区的撞击坑进行了直径-频率分布统计研究,获得其3个主要地质单元的绝对模式年龄分别为3.33 Ga、3.21 Ga和2.60 Ga,有效限定了本区主要地质事件发生的时间.

       

    • 图  1  NPF(1)与HPF(2)曲线对比(Ivanov, 2008, 有改动)

      图中D为撞击坑直径,R为利用公式(4)获得的R(D)值.图中曲线:1.NPF(Neukum et al., 2001);2.HPF(Hartmann,2005);3.饱和平衡曲线(Hartmann,1984)

      Fig.  1.  Comparison of NPF(1) and HPF(2)

      图  2  月球撞击年代曲线(据Hiesinger et al., 2000, 有简化)

      图中A代指Apollo,L代指Luna,横坐标T为月球表面绝对模式年龄,纵坐标Ncum(D>1 km)为单位面积上直径大于1 km的撞击坑总量

      Fig.  2.  Lunar Cratering Chronology Curve

      图  3  虹湾的位置及虹湾地区LRO广角相机图像

      a.虹湾在月球表面的位置,底图为LRO广角相机图像;b.虹湾LRO广角相机图像,图中点线区内为虹湾的范围,白色方框内为二次撞击坑集中分布区

      Fig.  3.  Location of Sinus Iridum and LRO Wide Angle Camera mosaic of Sinus Iridum

      图  4  虹湾地区地质单元划分与各地质单元定年结果

      a.虹湾地区地质单元划分与各单元绝对模式年龄.图中黑色虚线内为虹湾范围,黑色实线为各地质单元界限,白色虚线内为进行撞击坑直径-频率分布测量的区域,底图为利用Clementine不同波段比值合成的假彩色图像;b.地质单元A的定年结果;c.地质单元B1的定年结果;d.地质单元B2的定年结果;e.地质单元C的定年结果.图b~e中横坐标为撞击坑直径,纵坐标为累积撞击坑频率

      Fig.  4.  Geologic units in Sinus Iridum and their absolute model ages

      图  5  熔岩流覆盖对撞击坑直径-频率分布曲线的影响(据Neukum et al., 1976, 有改动)

      图中横坐标为撞击坑直径,纵坐标为累积撞击坑频率.t1表示t1时刻撞击坑直径-频率分布曲线;t2t2时刻撞击坑直径-频率分布曲线;D0t1时刻熔岩流所覆盖的撞击坑的直径上限

      Fig.  5.  Effects of lava flow on crater size-frequency distribution curve

      表  1  Neukum撞击坑产率函数的系数(Neukum et al., 2001)

      Table  1.   Coefficients in NPF (Neukum et al., 2001)

      ai 旧数值 新数值
      a0 -3.076 8 -3.087 6
      a1 -3.626 9 -3.557 528
      a2 +0.436 6 +0.781 027
      a3 +0.793 5 +1.021 521
      a4 +0.086 5 -0.156 012
      a5 -0.264 9 -0.444 058
      a6 -0.066 4 +0.019 977
      a7 +0.037 9 +0.086 850
      a8 +0.010 6 -0.005 874
      a9 -0.002 2 -0.006 809
      a10 -5.181 0-4 +8.251 0-4
      a11 +3.971 0-5 +5.541 0-5
      下载: 导出CSV

      表  2  各区域不同直径单元的累积撞击坑频率

      Table  2.   Ncum of different diameter units in each area

      区域 面积(km2) 各直径单元的累积撞击坑频率(km-2)
      0.5 km 0.6 km 0.7 km 0.8 km 0.9 km 1.0 km 1.2 km 1.5 km 2.0 km 2.5 km
      A 4 238.967 2.97e-2 2.17e-2 1.23e-2 8.73e-3 6.84e-3 5.43e-3 3.30e-3 7.08e-4 2.36e-4 0
      B1 7 418.919 3.48e-2 1.70e-2 1.05e-2 8.36e-3 5.26e-3 2.97e-3 1.89e-3 6.74e-4 4.04e-4 1.35e-4
      B2 3 855.643 3.55e-2 1.89e-2 1.14e-2 8.30e-3 5.19e-3 3.11e-3 1.82e-3 2.59e-4 2.59e-4 0
      C 6 288.833 2.56e-2 1.18e-2 8.11e-3 5.41e-3 3.98e-3 3.02e-3 1.59e-3 7.95e-4 3.18e-4 1.59e-4
      下载: 导出CSV

      表  3  各区域二次撞击坑剔除情况

      Table  3.   Number of eliminated secondary craters in each area

      区域 撞击坑总数 二次撞击坑数 有效撞击坑数
      A 165 39 126
      B1 319 61 258
      B2 173 36 137
      C 192 28 164
      下载: 导出CSV

      表  4  虹湾地区地质年龄(所属地层)对比(单位:Ga)

      Table  4.   Comparison of ages and stratigraphy for Sinus Iridum in billion years

      地质单元 年龄(本文) 所属地层 Hiesinger(2000) Schaber(1969)
      A 3.33 Im1 3.26 Im1/Im2
      B 3.21 Im2 3.01/3.39 Im1/Im2
      C 2.60 EIm 2.96 EIm
      Hiesinger(2000)的研究结果据Hiesinger et al.(2000)Schaber(1969)的研究结果据Schaber(1969).
      下载: 导出CSV
    • [1] Arvidson, R., Boyce, J., Chapman, C., et al., 1979. Standard Techniques for Presentation and Analysis of Crater Size-Frequency Data. Icarus, 37: 467-474. doi: 10.1016/0019-1035(79)90009-5
      [2] Boyce, J.M., Dial, A.L., 1975. Relative Ages of Flow Units in Mare Imbrium and Sinus Iridum. In: Merrill, R.B., ed., Proceedings of the Sixth Lunar Conference. Pergamon Press, New York, 2585-2595.
      [3] Boyce, J.M., Dial, A.L., Soderblom, L.A., 1974. Ages of the Lunar Nearside Light Plains and Maria. In: Gose, W.A., ed., Proceedings of the Fifth Lunar Conference. Pergamon Press, New York, 11-23.
      [4] Burgess, R., Turner, G., 1998. Laser Argon-40-Argon-39 Age Determinations of Luna 24 Mare Basalts. Meteoritics & Planetary Science, 33(4): 921-935. doi: 10.1111/j.1945-5100.1998.tb01697.x
      [5] Dundas, C.M., McEwen, A.S., 2007. Rays and Secondary Craters of Tycho. Icarus, 186: 31-40. doi: 10.1016/j.icarus.2006.08.011
      [6] Harland, D.M., 2008. Exploring the Moon: The Apollo Expiditions. Springer, Berlin, 363-371. doi: 10.1007/978-0-387-74641-8
      [7] Hartmann, W.K., 1966. Early Lunar Cratering. Icarus, 5: 406-418. doi: 10.1016/0019-1035(66)90054-6
      [8] Hartmann, W.K., 1977. Relative Crater Production Rates on Planets. Icarus, 31: 260-276. doi: 10.1016/0019-1035(77)90037-9
      [9] Hartmann, W.K., 1984. Does Crater 'Saturation Equilibrium' Occur in the Solar System? Icarus, 60: 56-74. doi: 10.1016/0019-1035(84)90138-6
      [10] Hartmann, W.K., 2005. Martian Cratering 8: Isochron Refinement and the Chronology of Mars. Icarus, 174: 294-320. doi: 10.1016/j.icarus.2004.11.023
      [11] Hartmann, W.K., 2007. Martian Cratering 9: Toward Resolution of the Controversy about Small Craters. Icarus, 189: 274-278. doi: 10.1016/j.icarus.2007.02.011
      [12] Hartmann, W.K., Gaskell, R.W., 1997. Planetary Cratering 2: Studies of Saturation Equilibrium. Meteoritics & Planetary Science, 32: 109-121. doi: 10.1111/j.1945-5100.1997.tb01246.x
      [13] Hartmann, W.K., Neukum, G., 2001. Cratering Chronology and the Evolution of Mars. Space Science Reviews, 96(1-4): 165-194. doi: 10.1023/A:1011945222010
      [14] Hiesinger, H., Head III, J.W., Wolf, U., et al., 2002. Lunar Mare Basalt Flow Units: Thicknesses Determined from Crater Size-Frequency Distributions. Geophysical Research Letters, 29(8): 89-81 - 89-84. doi: 10.1029/2002GL014847
      [15] Hiesinger, H., Head III, J.W., Wolf, U., et al., 2003. Ages and Stratigraphy of Mare Basalts in Oceanus Procellarum, Mare Nubium, Mare Cognitum, and Mare Insularum. Journal of Geophysical Research, 108(E7): 5065-5091. doi: 10.1029/2002JE001985
      [16] Hiesinger, H., Head III, J.W., Wolf, U., et al., 2010. Ages and Stratigraphy of Lunar Mare Basalts in Mare Frigoris and Other Nearside Maria Based on Crater Size-Frequency Distribution Measurements. Journal of Geophysical Research, 115(E3): E03003. doi: 10.1029/2009JE003380
      [17] Hiesinger, H., Jaumann, R., Neukum, G., et al., 2000. Ages of Mare Basalts on the Lunar Nearside. Journal of Geophysical Research, 105(E12): 29239-29275. doi: 10.1029/2000JE001244
      [18] Huang, J., Xiao, L., He, X.X., et al., 2011. Geological Characteristics and Model Ages of Marius Hills on the Moon. Journal of Earth Science, 22(5): 601-609. doi: 10.1007/s12583-011-0211-8
      [19] Ivanov, B.A., 2001. Mars/Moon Cratering Rate Ratio Estimates. Space Science Reviews, 96(1-4): 87-104. doi: 10.1023/A:1011941121102
      [20] Ivanov, B.A., 2008. Size-Frequency Distribution of Asteroids and Impact Craters: Estimates of Impact Rate. In: Adushkin, V.V., Nemchinov, I.V., eds., Catastrophic Events Caused Cosmic Objects. Springer Netherlands, Berlin, 91-116. doi: 10.1007/978-1-4020-6452-4_2
      [21] Ivanov, B.A., Neukum, G., Bottke, W., et al., 2002. The Comparison of Size-Frequency Distributions of Impact Craters and Asteroids and the Planetary Cratering Rate. In: Bottke, W.F., ed., Asteroids III. University of Arizona Press, Tucson, 89-101.
      [22] Li, L., 2011. Quantifying TiO2 Abundance of Lunar Soils: Partial Least Squares and Stepwise Multiple Regression Analysis for Determining Causal Effect. Journal of Earth Science, 22(5): 549-565. doi: 10.1007/s12583-011-0206-5
      [23] McEwen, A.S., Bierhaus, E.B., 2006. The Importance of Secondary Cratering to Age Constraints on Planetary Surfaces. Annual Review of Earth and Planetary Sciences, 34: 535-567. doi: 10.1146/annurev.earth.34.031405.125018
      [24] Michael, G.G., Neukum, G., 2010. Planetary Surface Dating from Crater Size-Frequency Distribution Measurements: Partial Resurfacing Events and Statistical Age Uncertainty. Earth and Planetary Science Letters, 294: 223-229. doi: 10.1016/j.epsl.2009.12.041
      [25] Nagumo, K., Nakamura, A.M., 2001. Reconsideration of Crater Size-Frequency Distribution on the Moon: Effect of Projectile Population and Secondary Craters. Advances in Space Research, 28: 1181-1186. doi: 10.1016/S0273-1177(01)00488-4
      [26] Neukum, G., Basilevsky, A.T., Kneissl, T., et al., 2010. The Geologic Evolution of Mars: Episodicity of Resurfacing Events and Ages from Cratering Analysis of Image Data and Correlation with Radiometric Ages of Martian Meteorites. Earth and Planetary Science Letters, 294: 204-222. doi: 10.1016/j.epsl.2009.09.006
      [27] Neukum, G., Ivanov, B.A., Hartmann, W.K., 2001. Cratering Records in the Inner Solar System in Relation to the Lunar Reference System. Space Science Reviews, 96(1-4): 55-86. doi: 10.1023/A:1011989004263
      [28] Neukum, G., Ivanov, B.A., 1994. Crater Size Distributions and Impact Probabilities on Earth from Lunar, Terrestrial-Planet, and Asteroid Cratering Data. In: Gehrels, T., Matthews, M.S., Schumann, A., eds., Hazards due to Comets and Asteroids. The University of Arizona Press, Tucson, 359.
      [29] Neukum, G., Horn, P., 1976. Effects of Lava Flows on Lunar Crater Populations. Earth, Moon, and Planets, 15(3-4): 205-222. doi: 10.1007/BF00562238
      [30] Neukum, G., König, B., 1976. Dating of Individual Lunar Craters. In: Merrill, R.B., ed., Proceedings of the Seventh Lunar Conference. Pergamon Press, New York, 2867-2881.
      [31] Neukum, G., König, B., Arkani-Hamed, J., 1975a. A Study of Lunar Impact Crater Size-Distributions. Earth, Moon, and Planets, 12(2): 201-229. doi: 10.1007/BF00577878
      [32] Neukum, G., König, B., Fechtig, H., et al., 1975b. Cratering in the Earth-Moon System: Consequences for Age Determination by Crater Counting. In: Merrill, R.B., ed., Proceedings of the Sixth Lunar Conference, New York, 2597-2620.
      [33] Neukum, G., Schneider, E., Mehl, A., et al., 1972. Lunar Craters and Exposure Ages Derived from Crater Statistics and Solar Flare Tracks. In: King, E.A., Heymann, D., Criswell, D.R., eds., Proceedings of the Third Lunar Science Conference. The MIT Press, Cambridge, MA, 2793-2810.
      [34] Öpik, E.J., 1960. The Frequency of Crater Diameters in Mare Imbrium. Astronomical Journal, 65: 55.
      [35] Pieters, C.M., Staid, M.I., Fischer, E.M., et al., 1994. A Sharper View of Impact Craters from Clementine Data. Science, 266(5192): 1844-1848. doi: 10.1126/science.266.5192.1844
      [36] Platz, T., Michael, G.G., Neukum, G., 2010. Confident Thickness Estimates for Planetary Surface Deposits from Concealed Crater Populations. Earth and Planetary Science Letters, 293: 388-395. doi: 10.1016/j.epsl.2010.03.012
      [37] Schaber, G.G., 1969. Geologic Map of the Sinus Iridum Quadrangle of the Moon. In: U.S. Geological Survey, ed., Geologic Atlas of the Moon. U.S. Geological Survey, Washington, D.C., I-602.
      [38] Shoemaker, E.M., 1965. Preliminary Analysis of the Fine Structure of the Lunar Surface in Mare Cognitum. In: Hess, W.N., Menz, D.H., O'Keefe, J.A., eds., The Nature of the Lunar Surface: Proceedings of the 1965 IAU-NASA Symposium. The Johns Hopkins Press, Baltimore, MD, 23.
      [39] Stöffler, D., Ryder, G., 2001. Stratigraphy and Isotope Ages of Lunar Geologic Units: Chronological Standard for the Inner Solar System. Space Science Reviews, 96(1-4): 9-54. doi: 10.1023/A:1011937020193
      [40] Xiao, Z.Y., Strom, R.G., 2012. Problems Determining Relative and Absolute Ages Using the Small Crater Population. Icarus, 220: 254-267. doi: 10.1016/j.icarus.2012.05.012
    • 加载中
    图(5) / 表(4)
    计量
    • 文章访问数:  3202
    • HTML全文浏览量:  198
    • PDF下载量:  311
    • 被引次数: 0
    出版历程
    • 刊出日期:  2013-03-01

    目录

      /

      返回文章
      返回