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2,4,4,5,5,5-hexafluoro-3-oxo-valeric acid ethyl ester | 1513-61-7

中文名称
——
中文别名
——
英文名称
2,4,4,5,5,5-hexafluoro-3-oxo-valeric acid ethyl ester
英文别名
2,4,4,5,5,5-Hexafluor-3-oxo-valeriansaeure-aethylester;Ethyl 2,4,4,5,5,5-hexafluoro-3-oxopentanoate
2,4,4,5,5,5-hexafluoro-3-oxo-valeric acid ethyl ester化学式
CAS
1513-61-7
化学式
C7H6F6O3
mdl
——
分子量
252.113
InChiKey
OZJJJJWONGATBX-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):
    1.65
  • 重原子数:
    16.0
  • 可旋转键数:
    4.0
  • 环数:
    0.0
  • sp3杂化的碳原子比例:
    0.71
  • 拓扑面积:
    43.37
  • 氢给体数:
    0.0
  • 氢受体数:
    3.0

反应信息

  • 作为反应物:
    参考文献:
    名称:
    Source regions and timescales for the delivery of water to the Earth
    摘要:
    Abstract—In the primordial solar system, the most plausible sources of the water accreted by the Earth were in the outer asteroid belt, in the giant planet regions, and in the Kuiper Belt. We investigate the implications on the origin of Earth's water of dynamical models of primordial evolution of solar system bodies and check them with respect to chemical constraints. We find that it is plausible that the Earth accreted water all along its formation, from the early phases when the solar nebula was still present to the late stages of gas‐free sweepup of scattered planetesimals. Asteroids and the comets from the Jupiter‐Saturn region were the first water deliverers, when the Earth was less than half its present mass. The bulk of the water presently on Earth was carried by a few planetary embryos, originally formed in the outer asteroid belt and accreted by the Earth at the final stage of its formation. Finally, a late veneer, accounting for at most 10% of the present water mass, occurred due to comets from the Uranus‐Neptune region and from the Kuiper Belt. The net result of accretion from these several reservoirs is that the water on Earth had essentially the D/H ratio typical of the water condensed in the outer asteroid belt. This is in agreement with the observation that the D/H ratio in the oceans is very close to the mean value of the D/H ratio of the water inclusions in carbonaceous chondrites.
    DOI:
    10.1111/j.1945-5100.2000.tb01518.x
  • 作为产物:
    描述:
    参考文献:
    名称:
    Source regions and timescales for the delivery of water to the Earth
    摘要:
    Abstract—In the primordial solar system, the most plausible sources of the water accreted by the Earth were in the outer asteroid belt, in the giant planet regions, and in the Kuiper Belt. We investigate the implications on the origin of Earth's water of dynamical models of primordial evolution of solar system bodies and check them with respect to chemical constraints. We find that it is plausible that the Earth accreted water all along its formation, from the early phases when the solar nebula was still present to the late stages of gas‐free sweepup of scattered planetesimals. Asteroids and the comets from the Jupiter‐Saturn region were the first water deliverers, when the Earth was less than half its present mass. The bulk of the water presently on Earth was carried by a few planetary embryos, originally formed in the outer asteroid belt and accreted by the Earth at the final stage of its formation. Finally, a late veneer, accounting for at most 10% of the present water mass, occurred due to comets from the Uranus‐Neptune region and from the Kuiper Belt. The net result of accretion from these several reservoirs is that the water on Earth had essentially the D/H ratio typical of the water condensed in the outer asteroid belt. This is in agreement with the observation that the D/H ratio in the oceans is very close to the mean value of the D/H ratio of the water inclusions in carbonaceous chondrites.
    DOI:
    10.1111/j.1945-5100.2000.tb01518.x
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文献信息

  • Cascade Knoevenagel and aza-Wittig reactions for the synthesis of substituted quinolines and quinolin-4-ols
    作者:Xiaofeng Zhang、Xiaoming Ma、Weiqi Qiu、Jason Evans、Wei Zhang
    DOI:10.1039/c8gc03180k
    日期:——
    A [4 + 2] annulation involving cascade Knoevenagel, aza-Wittig and dehydrofluorination reactions is developed for the synthesis of substituted quinolin-4-ols including analogs bearing CF2H, CF3, and C2F5 groups. This simple and highly efficient method is also applicable for the synthesis of substituted quinolines. A number of reported biologically active compounds can be readily prepared by this one-pot
    开发了一种包括级联Knoevenagel,aza-Wittig和脱氟化氢反应的[4 + 2]环合反应,用于合成取代的喹啉-4-醇,包括带有CF 2 H,CF 3和C 2 F 5基团的类似物。这种简单而高效的方法也适用于取代喹啉的合成。通过一锅法合成可以容易地制备许多报道的生物活性化合物。新反应过程的绿色化学指标分析提供了令人满意的结果。
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马来酰基乙酸 顺-3-己烯-1-丙酮酸 青霉酸 钠氟草酰乙酸二乙酯 醚化物 酮霉素 辛酸,2,4-二羰基-,乙基酯 草酸乙酯钠盐 草酰乙酸二乙酯钠盐 草酰乙酸二乙酯 草酰乙酸 草酰丙酸二乙酯 苯乙酰丙二酸二乙酯 苯丁酸,b-羰基-,2-丙烯基酯 聚氧化乙烯 羟基-(3-羟基-2,3-二氧代丙基)-氧代鏻 磷酸二氢2-{(E)-2-[4-(二乙胺基)-2-甲基苯基]乙烯基}-1,3,3-三甲基-3H-吲哚正离子 碘化镝 硬脂酰乙酸乙酯 甲氧基乙酸乙酯 甲氧基乙酰乙酸酯 甲基氧代琥珀酸二甲盐 甲基4-环己基-3-氧代丁酸酯 甲基4-氯-3-氧代戊酸酯 甲基4-氧代癸酸酯 甲基4-氧代月桂酸酯 甲基4-(甲氧基-甲基磷酰)-2,2,4-三甲基-3-氧代戊酸酯 甲基3-羰基-2-丙酰戊酸酯 甲基3-氧代十五烷酸酯 甲基2-氟-3-氧戊酯 甲基2-氟-3-氧代己酸酯 甲基2-氟-3-氧代丁酸酯 甲基2-乙酰基环丙烷羧酸酯 甲基2-乙酰基-4-甲基-4-戊烯酸酯 甲基2-乙酰基-2-丙-2-烯基戊-4-烯酸酯 甲基2,5-二氟-3-氧代戊酸酯 甲基2,4-二氟-3-氧代戊酸酯 甲基2,4-二氟-3-氧代丁酸酯 甲基1-异丁酰基环戊烷羧酸酯 甲基1-乙酰基环戊烷羧酸酯 甲基1-乙酰基环丙烷羧酸酯 甲基1-乙酰基-2-乙基环丙烷羧酸酯 甲基(2Z,4E,6E)-2-乙酰基-7-(二甲基氨基)-2,4,6-庚三烯酸酯 甲基(2S)-2-甲基-4-氧代戊酸酯 甲基(1S,2R)-2-乙酰基环丙烷羧酸酯 甲基(1R,2R)-2-乙酰基环丙烷羧酸酯 瑞舒伐他汀杂质 瑞舒伐他汀杂质 环氧乙烷基甲基乙酰乙酸酯 环戊戊烯酸,Β-氧代,乙酯