Question: A star too small and cold to shine has been found by S. Kulkarni, K. Matthews, B.R. Oppenheimer, and T. Nakajima (Science 270, 1478 (1995)).
(a) From available thermodynamic data, test the stability of methane at temperatures above 1000 K.
(b) What is Amax for this star?
(c) What is the energy density of the star relative to that of the Sun (6000 K)?
(d) To determine whether the star will shine, estimate the fraction of the energy density of the star in the visible region of the spectrum.
Step by Step Solution
3.46 Rating (166 Votes )
There are 3 Steps involved in it
a CH4 g Cgraphite 2Hg AG AG CH4 5072 kJ mol 5072 kJ mol AH AfH CH4 7481 kJ mol 7481 kJ mol at T at F 25C We want to find the temperature at which AG T ... View full answer
Get step-by-step solutions from verified subject matter experts
Document Format (1 attachment)
57-C-PC-S (32).docx
120 KBs Word File
