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Bad White [126]
2 years ago
11

Which of the following compounds has the general formula X3Y2?Which of the following compounds has the general formula X3Y2?

Chemistry
1 answer:
prisoha [69]2 years ago
6 0

There are no above options to choose from so I am giving an example of a X3Y2 formula which is Magnesium nitride, the formula is Mg3N2.

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How many milligrams are in 2.5 kg?
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Answer:

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7 0
2 years ago
At 20 degrees Celsius, the density of air is 1.20 g/L. Nitrogen's density is 1.17 g/L. Oxygen's density is 1.33 g/L. Will balloo
Alinara [238K]

Explanation:

Since, density is the amount of mass present in per unit volume.

Mathematically,      Density = \frac{mass}{volume}

As density is directly proportional to mass of a substance. So, more is the density of a substance more will be its mass. And, when more is the mass of a substance then it is likely to sink at the bottom.

Here, it is given that density of oxygen is more than the density of nitrogen. Therefore, balloons filled with oxygen will sink in the air.

On the other hand, balloons filled with nitrogen will rise in the air.

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6 0
2 years ago
What will cause the particles of a solid to become arranged in a more random manner
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Question 13: Consider the strength of the Hβ absorption line in the spectra of stars of various surface temperatures. This is th
finlep [7]

Answer:

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Atoms possess distinct energy levels and these levels of energy are constant, that is, the temperature has no influence on it. However, temperature possesses an influence on the electron numbers found within these levels of energy. Therefore, to generate an absorption line of hydrogen in the electromagnetic spectrum's visible band, the electrons are required to be present in the second energy level, that is when it captivates a photon.  

Therefore, after captivating the photons the electrons jump from level 2 to level 4, which shows that there is an increase in the stellar surface temperature and at the same time one can witness a decline in the strength of the H-beta lines. In case, if the temperature of the surface increases too much, then one will witness no attachment of electron with the hydrogen atom and thus no H lines, and if the temperature of the surface becomes too low, then the electrons will stay in the ground state and no formation of H lines will take place in that condition too.  

Hence, to generate a very robust H line, after captivating photons the majority of the electrons are required to stay in the second energy level.  

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3 years ago
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