2-hydroxyimino-adipic acid diethyl ester

• 分子结构分类: 有机化合物 - 脂质和类脂质分子 - 脂肪酰基
• 英文名称: 2-hydroxyimino-adipic acid diethyl ester
• 英文别名: 2-Hydroxyimino-adipinsaeure-diaethylester
• 化学式: C₁₀H₁₇NO₅
• 分子量: 231.249
• InChiKey: YAHFIOCYVMMRAO-FLIBITNWSA-N

计算性质

• 辛醇/水分配系数(LogP)：
  1.11
• 重原子数：
  16.0
• 可旋转键数：
  7.0
• 环数：
  0.0
• sp3杂化的碳原子比例：
  0.7
• 拓扑面积：
  85.19
• 氢给体数：
  1.0
• 氢受体数：
  6.0

反应信息

• 作为反应物：
  描述：

  2-hydroxyimino-adipic acid diethyl ester 在 potassium carbonate 作用下， 生成 2-hydroxyimino-adipic acid
  参考文献：
  名称：

  Dieckmann, Chemische Berichte, 1900, vol. 33, p. 593

  摘要：

  DOI：
• 作为产物：
  描述：

  2-溴己二酸二乙酯 在 乙醇 、 sodium nitrite 作用下， 生成 2-hydroxyimino-adipic acid diethyl ester
  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

文献信息

• New Nitrogen Mustards for “Toxagenic” Anti-cancer Agents^1a,b
  作者：Orrie M. Friedman、Eliahu Boger

  DOI：10.1021/ja01599a036

  日期：1956.9
• Inoue; Sono, Nippon Nogeikagaku Kaishi, 1950, vol. 23, p. 396
  作者：Inoue、Sono

  DOI：——

  日期：——
• 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.
• Dieckmann, Chemische Berichte, 1900, vol. 33, p. 593
  作者：Dieckmann

  DOI：——

  日期：——