2008
DOI: 10.1016/j.jct.2007.06.013
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Isobaric specific heat capacity of {xH2O+(1−x)NH3} with x=(0.0000, 0.1566, 0.1597, 0.3030, 0.3048, 0.4956, 0.7061, and 0.8489) at T=(280, 300, 320, and 360)K over the pressure range from (0.1 to 15)MPa

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Cited by 7 publications
(4 citation statements)
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“…Data at higher pressure available in Fujita 112 and Hnedkovsky. 150 The fit covers the entire range 0 e w NH3 e 1.…”
Section: T H I S C O N T E N T Imentioning
confidence: 99%
“…Data at higher pressure available in Fujita 112 and Hnedkovsky. 150 The fit covers the entire range 0 e w NH3 e 1.…”
Section: T H I S C O N T E N T Imentioning
confidence: 99%
“…In previous publications [1][2][3][4][5], we reported measurements of (p, q, T, x), bubble point pressure, saturated liquid density, isobaric specific heat capacity, and the critical parameter for {xNH 3 + (1 À x)H 2 O} with x = (0.1016 to 1.0000) by a metal-bellows variable volumometer in the compressed liquid phase at T = (280 to 405) K at pressures up to p = 17 MPa. In continuation of our work, the results of the (p, q, T, x) property measurements for {xNH 3 + (1 À x)H 2 O} with x = (0.1048 to 1.0000) in the higher temperature and pressure regions at T = (450, 500) K, and at p = (10 to 200) MPa are presented in this paper.…”
Section: Introductionmentioning
confidence: 98%
“…Results from Chan and Giauque, Hildenbrand and Giauque, and Wrewsky and Kaigorodoff were the only caloric data sets considered. Other calorimetric studies were either conducted at room temperature, with very dilute mixtures, or with sparse results. , To date, there are no extensive studies of isobaric heat capacity in the binary water–ammonia system at low temperatures and mass fraction conditions relevant to outer solar system planetary studies (0–5 GPa, 100–300 K, 0–15 wt %) . The poor coverage of data at this space is primarily due to difficulty in measuring low ammonia mass fraction samples due to its high volatilization capacity at surface Earth conditions and a heavier focus on higher mass fraction solution properties for absorption refrigeration applications .…”
Section: Introductionmentioning
confidence: 99%
“…This work improves upon the current data set and also introduces novel data in the parameter space most relevant for outer solar system planetary bodies, shown as the shaded region and the shaded line along the melting curve. CG64—Chan and Giauque; 19 HG53—Hildenbrand and Giauque; 20 WK24—Wrewsky and Kaigorodoff; 22 C71—Chernen’kaya; 23 AW81—Allred and Woolley; 24 F08—Fujita et al; 25 and P22—Prieto-Ballesteros et al 26 …”
Section: Introductionmentioning
confidence: 99%