188-00-1 Usage
Chemical structure
1,2,3,4,5,6,10,11-Tetrabenzanthanthrene is a polycyclic aromatic hydrocarbon (PAH) with four benzene rings fused in a linear arrangement.
Stability
Highly stable compound due to its fused aromatic ring structure.
Polarity
Non-polar in nature, which contributes to its solubility in organic solvents.
Solubility
Insoluble in water, but soluble in organic solvents such as benzene, toluene, and xylene.
Applications
Used in organic synthesis and materials science as a building block for various derivatives and functional materials.
Reactivity
Its unique molecular structure makes it a valuable tool for studying the reactivity and properties of PAHs.
Environmental impact
Potential environmental pollutant due to its persistence and resistance to degradation.
Health risks
Classified as a carcinogen, which means it has the potential to cause cancer in humans.
Safety precautions
Use and handling should be carried out with caution and in accordance with safety regulations to minimize exposure and environmental contamination.
Check Digit Verification of cas no
The CAS Registry Mumber 188-00-1 includes 6 digits separated into 3 groups by hyphens. The first part of the number,starting from the left, has 3 digits, 1,8 and 8 respectively; the second part has 2 digits, 0 and 0 respectively.
Calculate Digit Verification of CAS Registry Number 188-00:
(5*1)+(4*8)+(3*8)+(2*0)+(1*0)=61
61 % 10 = 1
So 188-00-1 is a valid CAS Registry Number.
InChI:InChI=1/C36H18/c1-3-10-21-19(8-1)23-12-5-14-25-27-16-7-17-28-26-15-6-13-24-20-9-2-4-11-22(20)30-18-29(21)34(31(23)25)36(33(27)28)35(30)32(24)26/h1-18H
188-00-1Relevant academic research and scientific papers
HEXA-PERI-BENZOCORONENE, A CANDIDATE FOR THE ORIGIN OF THE DIFFUSE INTERSTELLAR VISIBLE ABSORPTION BANDS ?
Hendel, W.,Khan, Z. H.,Schmidt, W.
, p. 1127 - 1134 (2007/10/02)
Large polycyclic aromatic hydrocarbons (PAH's) have recently been suggested to be abundant in the interstellar medium surrounding carbon rich stars.To aid in the identification of the species responsible for the astronomical UV and IR data, a new synthesis is reported for hexa-peri-benzocoronene and its dimethyl derivative.The UV, fluorescence, phosphorescence, photoelectron and IR spectra of this extremely stable hydrocarbon are presented and compared with the available astronomical spectra.Experiments useful to check the PAH hypothesis are suggested.
