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2-amino-decane-1,10-diol | 99868-67-4

中文名称
——
中文别名
——
英文名称
2-amino-decane-1,10-diol
英文别名
2-Amino-decan-1,10-diol;2-Aminodecane-1,10-diol;2-aminodecane-1,10-diol
2-amino-decane-1,10-diol化学式
CAS
99868-67-4
化学式
C10H23NO2
mdl
——
分子量
189.298
InChiKey
KZBGNJCVWFJJRR-UHFFFAOYSA-N
BEILSTEIN
——
EINECS
——
  • 物化性质
  • 计算性质
  • ADMET
  • 安全信息
  • SDS
  • 制备方法与用途
  • 上下游信息
  • 反应信息
  • 文献信息
  • 表征谱图
  • 同类化合物
  • 相关功能分类
  • 相关结构分类

计算性质

  • 辛醇/水分配系数(LogP):
    1
  • 重原子数:
    13
  • 可旋转键数:
    9
  • 环数:
    0.0
  • sp3杂化的碳原子比例:
    1.0
  • 拓扑面积:
    66.5
  • 氢给体数:
    3
  • 氢受体数:
    3

反应信息

  • 作为产物:
    描述:
    2-bromo-decanedioic acid dimethyl ester 在 lithium aluminium tetrahydride 、 乙醚乙醇 、 sodium nitrite 作用下, 生成 2-amino-decane-1,10-diol
    参考文献:
    名称:
    The irradiation history of the Ghubara (L5) regolith breccia
    摘要:
    Abstract— We measured cosmic‐ray products—noble gases, radionuclides, thermoluminescence, and nuclear tracks—and trace element contents and mineralogy of samples of three orthogonal and mutually intersecting cores (41–46 cm long) of a 101.6 kg Ghubara individual (1958,805) at The Natural History Museum, London. The xenoliths, like the host, have high concentrations of trapped solar gases and are heavily shocked. While contents of noble gases and degree of shock‐loading in this individual and three others differ somewhat, the data indicate that Ghubara is a two‐generation regolith breccia. Contents of cosmogenic 26Al and 10Be and low track densities indicate that the Ghubara individuals were located more than 15 cm below the surface of an 85 cm meteoroid. Because of its large size, Ghubara's cosmic‐ray exposure age is poorly defined to be 15–20 Ma from cosmogenic nuclides. Ghubara's terrestrial age, based on 14C data, is 2–3 ka. Not only is Ghubara the first known case of a two‐generation regolith breccia on the macroscale, it also has a complicated thermal and irradiation history.
    DOI:
    10.1111/j.1945-5100.2002.tb00819.x
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文献信息

  • ETHYLENICALLY UNSATURATED GROUP-CONTAINING ISOCYANATE COMPOUND AND PROCESS FOR PRODUCING THE SAME, AND REACTIVE MONOMER, REACTIVE (METH)ACRYLATE POLYMER AND ITS USE
    申请人:SHOWA DENKO K.K.
    公开号:EP1812381B1
    公开(公告)日:2011-02-16
  • Ethylenically Unsaturated Group-Containing Isocyanate Compound and Process for Producing the Same, and Reactive Monomer, Reactive (Meth) Acrylate Polymer and its Use
    申请人:Nozawa Kaneo
    公开号:US20080132597A1
    公开(公告)日:2008-06-05
    There are provided a novel ethylenically unsaturated group-containing isocyanate compound, a process for producing the same, and a reactive monomer produced from the isocyanate compound, a reactive polymer and its use. The ethylenically unsaturated group-containing isocyanate compound according to the present invention is represented by formula (I).
  • US7579066B2
    申请人:——
    公开号:US7579066B2
    公开(公告)日:2009-08-25
  • The irradiation history of the Ghubara (L5) regolith breccia
    作者:T. E. Ferko、M-S. Wang、D. J. Hillegonds、M. E. Lipschutz、R. Hutchison、L. Franke、P. Scherer、L. Schultz、P. H. Benoit、D. W. G. Sears、A. K. Singhvi、N. Bhandari
    DOI:10.1111/j.1945-5100.2002.tb00819.x
    日期:2002.3
    Abstract— We measured cosmic‐ray products—noble gases, radionuclides, thermoluminescence, and nuclear tracks—and trace element contents and mineralogy of samples of three orthogonal and mutually intersecting cores (41–46 cm long) of a 101.6 kg Ghubara individual (1958,805) at The Natural History Museum, London. The xenoliths, like the host, have high concentrations of trapped solar gases and are heavily shocked. While contents of noble gases and degree of shock‐loading in this individual and three others differ somewhat, the data indicate that Ghubara is a two‐generation regolith breccia. Contents of cosmogenic 26Al and 10Be and low track densities indicate that the Ghubara individuals were located more than 15 cm below the surface of an 85 cm meteoroid. Because of its large size, Ghubara's cosmic‐ray exposure age is poorly defined to be 15–20 Ma from cosmogenic nuclides. Ghubara's terrestrial age, based on 14C data, is 2–3 ka. Not only is Ghubara the first known case of a two‐generation regolith breccia on the macroscale, it also has a complicated thermal and irradiation history.
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