You need to use the equation PV = nRT
The only “trick” in these problems is you need to use the correct UNITS. Especially for the “R” value.
If you get the units (eg temps in Celsius or Kelvin) corresponding to the correct “matching” units of the other variables.
You need to convert the temp into Kelvin first
D - density: 1 g/cm³
m - mass: 2,89g
V - volume: ?
----------------------------
d = m/V
V = m/d
V = 2,89/1
V = 2,89cm³
:•)
Answer:
Its C how contributions by many different cultures throughout history have advanced our understanding of the solar system.
Explanation:
Answer:
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Explanation:
