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About This Item
Linear Formula:
CH3CH3
CAS Number:
Molecular Weight:
30.07
Beilstein/REAXYS Number:
1730716
MDL number:
vapor density
1.05 (vs air)
vapor pressure
37.95 atm ( 21.1 °C)
autoignition temp.
881 °F
expl. lim.
13 %
concentration
10 ppm in nitrogen
bp
−88 °C (lit.)
mp
−172 °C (lit.)
density
0.362 g/mL at 20 °C (lit.)
SMILES string
CC
InChI
1S/C2H6/c1-2/h1-2H3
InChI key
OTMSDBZUPAUEDD-UHFFFAOYSA-N
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Application
For calibrating analytical instruments.
Packaging
Packaged in lightweight no-return cylinder
Recommended products
Control valve Z166995 or regulator Z167002 is recommended.
Certificates of Analysis (COA)
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Reika Kanya et al.
The Journal of chemical physics, 136(20), 204309-204309 (2012-06-07)
Two-body Coulomb explosion processes of ethane (CH(3)CH(3)) and its isotopomers (CD(3)CD(3) and CH(3)CD(3)) induced by an intense laser field (800 nm, 1.0 × 10(14) W/cm(2)) with three different pulse durations (40 fs, 80 fs, and 120 fs) are investigated by
Paul O Wennberg et al.
Environmental science & technology, 46(17), 9282-9289 (2012-08-03)
We use historical and new atmospheric trace gas observations to refine the estimated source of methane (CH(4)) emitted into California's South Coast Air Basin (the larger Los Angeles metropolitan region). Referenced to the California Air Resources Board (CARB) CO emissions
Ramiro F Quijano-Quiñones et al.
Molecules (Basel, Switzerland), 17(4), 4661-4671 (2012-04-24)
The energy change on each Occupied Molecular Orbital as a function of rotation about the C-C bond in ethane was studied using the B3LYP, mPWB95 functional and MP2 methods with different basis sets. Also, the effect of the ZPE on
Sonia Aguado et al.
Journal of the American Chemical Society, 134(36), 14635-14637 (2012-08-24)
Absolute ethylene/ethane separation is achieved by ethane exclusion on silver-exchanged zeolite A adsorbent. This molecular sieving type separation is attributed to the pore size of the adsorbent, which falls between ethylene and ethane kinetic diameters.
Isobel J Simpson et al.
Nature, 488(7412), 490-494 (2012-08-24)
After methane, ethane is the most abundant hydrocarbon in the remote atmosphere. It is a precursor to tropospheric ozone and it influences the atmosphere's oxidative capacity through its reaction with the hydroxyl radical, ethane's primary atmospheric sink. Here we present
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